MINIMO: a Search for Mini Proper Motion Stars in the Southern Sky

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5-3-2007

MINIMO: A Search for Mini Proper Motion Stars in the Southern Sky

Charlie Thomas Finch

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This Thesis is brought to you for free and open access by the Department of Physics and Astronomy at ScholarWorks @ Georgia State University. It has been accepted for inclusion in Physics and Astronomy Theses by an authorized administrator of ScholarWorks @ Georgia State University. For more information, please contact [email protected]. MINIMO: A SEARCH FOR MINI PROPER MOTION STARS IN THE SOUTHERN SKY

by Charlie T. Finch

Under the Direction of Todd J. Henry

Abstract

I report 1684 new proper motion systems in the southern sky (declinations −90◦ to −47◦) with 000.50 yr−1 > µ ≥ 000.18 yr−1. This effort is a continuation of the SuperCOSMOS-RECONS (SCR) proper motion search to lower proper motions than reported in Hambly et al. (2004); Henry et al. (2004); Subasavage et al. (2005a,b). Distance estimates are presented for the new systems, assuming that all stars are on the main sequence. I find that 34 systems are within 25 pc, including three systems — SCR 0838-5855, SCR 1826-6542, and SCR 0630-7643AB — anticipated to be within 10 pc. These mini-motion (MINIMO) discoveries constitute a more than ten-fold increase in new systems found in the same region of sky searched for systems with µ ≥ 000.50 yr−1, suggesting a happy hunting ground for new nearby slower proper motion systems in the region just north (declinations −47◦ to 0◦), much of which has not been rigorously searched during previous efforts.

Index Words: Stars: Proper Motion, Solar Neighborhood, Distances, Statistics, Sur- veys, Astrometry MINIMO: A SEARCH FOR MINI PROPER MOTION STARS IN THE SOUTHERN SKY

Charlie T. Finch

A Thesis Presented in Partial Fulﬁllment of Requirements for the Degree of Master of Science in the College of Arts and Sciences Georgia State University

2007 Copyright by Charlie T. Finch 2007 MINIMO: A SEARCH FOR MINI PROPER MOTION STARS IN THE SOUTHERN SKY

Charlie T. Finch

Major Professor: Todd J. Henry Committee: Douglas R. Gies Harold A. McAlister

Electronic Version Approved:

Oﬃce of Graduate Studies College of Arts & Sciences Georgia State University May 2007 iv – 0 – Dedication

This thesis is dedicated in loving memory of my grandfather Charlie Clyde Smith, to whom I not only inherited my name but also my good looks. I miss you... v – 0 – Acknowledgments

Probably the hardest part of a thesis is trying to acknowledge everyone who has contributed to and made this part of my life more enjoyable during the process. It is a pleasure to show my gratitude to the many people who have made this thesis possible.

My family has always been a great support throughout my life and without them I could have never made it to where I am today. I would like to thank my parents for their encouragement and support, both emotional and monetary, and their uncanny ability to put up with me. I also would like to thank my grandfather for whom this thesis is dedicated for always believing in me and everything that I do. My thanks also go out to the rest of my family who have been the backbone of my support. Many thanks go out to all my friends who have supported me in all my decisions and have always been there for me. In particular, I would like to thank Nicole Geiger, without her friendship and support I would have never ﬁnished my degree. To my girlfriend Amelia Griﬃth, I would like to say thank you for putting up with my long nights of working and for your encouragement. I need to thank Georgia State University for giving me the opportunity to explore the research opportunities available at this institution. I give my gratitude to Dr. Douglas Gies and Dr. Harold McAlister for agreeing to serve on my thesis committee and thoroughly reading through my thesis for suggestions. To my supervisor Dr. Todd Henry, I give many thanks for giving me the opportunity to prove that this thesis was not beyond my reach and without whom this thesis would have not been possible. vi

Without the support, encouragement and friendship from the many faculty and staﬀ at the Georgia State Physics and Astronomy department, time spent on this thesis would not have been as manageable. I am honored to have had the opportunity to work with them and thank them for everything they have contributed. Finally I would like to thank Nigel C. Hambly, John P. Subasavage and Jao Wei-Chun for their many contributions that have made this search possible. vii – 0 – Contents

Acknowledgments ...... v

Tables ...... ix Figures ...... x Abbreviations and Acronyms ...... xii

1 Introduction ...... 1 1.1 Early Discoveries ...... 2 1.1.1 Barnard’s Star ...... 2 1.1.2 Kapteyn’s Star ...... 3 1.1.3 Groombridge 1830 ...... 4 1.2 Proper Motion Surveys ...... 5 1.2.1 Why Are They Important? ...... 5 1.2.2 Historical Beginnings ...... 6 1.2.3 Luyten & Giclas ...... 7 1.2.4 Surveys Relevant to This Search ...... 8 1.3 Goals and Motivation ...... 10 2 Search Criteria ...... 12

3 Comparison to Previous Proper-Motion Surveys ...... 20 4 Data ...... 22 5 Photometric and Spectroscopic Observations of the Nearby Sample 28 5.1 Photometry ...... 28 5.2 Spectroscopy ...... 32

6 Analysis ...... 35 6.1 Color-Magnitude Diagram ...... 35 6.2 Reduced Proper Motion Diagram ...... 37 viii

6.3 New Common Proper Motion Systems ...... 40 6.4 Comments on Individual MINIMO Systems ...... 46 7 Discussion ...... 47 References ...... 52

Appendix ...... 56 ix – 0 – Tables

2.1 Discovery Statistics for Entire SCR Sample ...... 19

3.1 Number of NLTT-Type Objects Discovered South of Declination −47◦ 21

4.1 Characteristics of New SCR Systems Estimated to be Nearer than 25 Parsecs and New White Dwarf Candidates with 000.50 yr−1 > µ ≥ 000.18 yr−1 from −90◦ < δ ≤ −47◦ ...... 25

5.1 Photometry, Spectral Types and CCD Distance Estimates for MIN- IMO Systems Estimated to be Nearer than 25 pc with 000.50 yr−1 > µ ≥ 000.18 yr−1 from −90◦ < δ ≤ −47◦ ...... 31

6.1 Common Proper Motion Systems ...... 42

7.1 Distance Estimate Statistics for SCR Systems ...... 50 x – 0 – Figures

2.1 Plate coverage of the sky included in the MINIMO search. White boxes indicate plates that were excluded, primarily due to crowding in the Galactic Plane, LMC, and SMC, or because of an insuﬃcient spread in plate epochs. Plates 179, 227, and 228 are included because they were searched for objects with 000.50 yr−1 > µ ≥ 000.40 yr−1 but not for objects with 000.40 yr−1 > µ ≥ 000.18 yr−1...... 17 2.2 Hit Rate percentage of true proper motion objects (real proper motion objects / total candidates extracted) for the entire SCR sample having µ ≥ 000.18 yr−1 south of −47◦. Horizontal bars show the proper motion bins adopted, while vertical lines delineate the three individual SCR samples — MOTION, SLOWMO and MINIMO...... 18

4.1 Comparison of NLTT, Hipparcos, and SCR proper motions and position angles. The solid lines indicate perfect agreement. Note that proper motion data for NLTT is quantized south of −45◦...... 27

5.1 Spectral plots of new SCR discoveries estimated to be within 25 pc. Note that spectra of SCR 0630-7643AB, SCR 1240-8116, and SCR 1245-5506 were taken with a 200 slit width and may have minor ﬂux calibration problems...... 34

6.1 Color-apparent magnitude diagram for SCR systems (open circles) and known systems (small points) with 000.50 yr−1 > µ ≥ 000.18 yr−1 from ◦ ◦ −90 < δ ≤ −47 . Data points below our search cutoﬀ of R59F = 16.5 are CPM companions noticed during the blinking process...... 36 6.2 Reduced proper motion diagram for SCR systems (open circles) and known systems (small points) with 000.50 yr−1 > µ ≥ 000.18 yr−1 from −90◦ < δ ≤ −47◦. The arbitrary dotted line separates the white dwarfs from the subdwarfs. Triangles denote previously known white dwarfs. 39 xi

6.3 Comparison of proper motions for components in multiple systems. Proper motions from the automated SCR search are denoted by ﬁlled circles and proper motions manually obtained through SuperCOSMOS are denoted by open circles. The solid line indicates perfect agreement between the two and the dashed lines represent conservative limits of 000.20 yr−1 based on our uncertanties...... 44 6.4 Comparison of position angles for components in multiple systems. Position angles from the automated SCR search are denoted by ﬁlled circles and position angles manually obtained through SuperCOSMOS are denoted by open circles. The solid line indicates perfect agreement between the two and the dashed lines represent conservative limits of 5.0 degrees based on our uncertainties...... 45

7.1 Sky distribution of SCR systems with µ ≥ 000.18 yr−1. Open circles denote SCR discoveries from this search and small ﬁlled circles indicate SCR discoveries from past papers. The curve represents the Galactic plane...... 49 7.2 Histogram showing the number of new proper motion discoveries in 000.01 yr−1 bins for the entire MINIMO sample (light shade) and the number of those objects having distance estimates within 50 pc (dark shade)...... 51 xii – 0 – Abbreviations and Acronyms

APS Automated Plate Scanner

CCD Charge-Coupled Device

CDC Control Data Corporation CPM Common Proper Motion

CTIO Cerro Tololo Inter-American Observatory ESO European Southern Observatory FWHM Full-Width Half-Maximum GSC Guide Star Catalog

HPM High Proper Motion HST Hubble Space Telescope IRAF Image Reduction and Analysis Facility LEHPM Liverpool-Edinburgh High Proper Motion LHS Luyten Half Second

LMC Large Magellanic Cloud

MINIMO Mini Proper Motion MOTION Fast Proper Motion NLTT New Luyten Two-Tenths

NOMAD Naval Observatory Merged Astrometric Dataset RPM Reduced Proper Motion

SCR SuperCOSMOS-RECONS SD Subdwarf

SIM Space Interferometry Mission xiii

SIPS Southern Infrared Proper Motion Survey SLOWMO Slow Proper Motion

SMC Small Magellanic Cloud

SSS SuperCOSMOS Sky Survey

TSN The Solar Neighborhood UKST UK Schmidt Telescope

USNO US Naval Observatory WD White Dwarf YPC Yale Parallax Catalogue 2MASS Two Micron All Sky Survey 1 – 1 – Introduction

Proper motion is the measure of a celestial object’s angular motion perpendicular to the observer’s line of sight, resulting in an apparent change in position when compared to more distant celestial objects. This motion is a projection onto the celestial sphere of a star’s true motion in space relative to the Sun. To measure a star’s actual velocity through space relative to the Sun, we have to measure the tangential velocity (across our line of sight) and radial velocity (toward or away from us). The radial velocity can be determined by measuring the Doppler shift in the object’s observed spectral lines.

The standard relation between the tangential velocity (Vtan) and proper motion is

Vtan = 4.74µd.

Therefore the observed proper motion (µ) in arc seconds per year is inversely related to the distance (d) in parsecs, meaning that if two objects exhibit the same tangential velocity, the closer one will reveal a higher proper motion. This is why high proper motions can be a good indicator for detecting nearby stars. Using this assumption, the closer a star is to the observer, the faster the star’s relative motion will be when compared to far away stars, which seem to move slowly or not at all over relatively short timescales. Hence, for asteroids, comets, and planets, proper motion can be observed in as little as a few hours. However, this is only a piece of the equation. Slower proper motions do not always mean larger distances. A star’s motion in space is rarely perpendicular to the observer’s line of sight, so proper motions are observed to be slower, or not observed at all, and could hide some nearby gems. 2

1.1 Early Discoveries

From the mid-eighteen hundreds to the mid nineteen hundreds, three discoveries were made of stars moving faster than 700.0 yr−1. These high proper motion stars have held the test of time and, as of this writing, still have the three fastest proper motions of any known star.

1.1.1 Barnard’s Star

In 1916, Edward Emerson Barnard noticed by comparing photographic plates taken in 1894 and 1916 that he had found a small star with large proper motion (Barnard 1916). Even today, as of writing this thesis (17 February 2007), Barnard’s Star has the largest proper motion of any known star. Named after the discoverer, with µ = 1000.35 yr−1 and parallax of 000.54553 ± 000.00029 from an average of Hipparcos, Yale Parallax Catalogue (YPC) and Hubble Space Telescope (HST) data, Barnard’s star is the second closest star system after the Alpha Centauri system, at 1.83 pc as listed by the RECONS one hundred nearest star systems. This red dwarf, with a visual magnitude of 9.54 mag and spectral type M4.0 V (Kirkpatrick et al. 1991) is not visible to the naked eye. The small dim star has a mass estimated to be 17 percent the mass of the Sun, using relations from Henry & McCarthy (1993) and Henry et al. (1999), and has 0.35 percent of the Sun’s bolometric luminosity (Dawson & De Robertis 2004). It has been given the variable star designation V2500 Ophiuchus after a 1998 ﬂare that has been investigated by Paulson et al. (2006). Barnard’s Star has been studied for almost a century and is considered a Tier 1 target star for the Space Interferometer Mission (SIM), which will search for planets around parent stars. Peter van de Kamp in 1969 published his initial data pointing to a companion planet revolving around Barnard’s Star (van de Kamp 1969). Later, 3

Gatewood & Eichhorn (1973) looked at photographic plates taken with the 20-inch refractor at Wesleyan University’s Van Vleck Observatory and the 30-inch refractor at Allegheny Observatory in Pittsburg and found no evidence of any wobble in proper motion. Investigations by Hershey (1973) have shown that van de Kamp might have been looking at bad data due to an adjustment of the objective lens and change in emulsion of the Sproul 24-inch refractor.

1.1.2 Kapteyn’s Star

With µ = 800.67 yr−1 and parallax of 000.25527 ± 000.00086 from an average of Hipparcos, YPC and HST data, Kapteyn’s Star is the second fastest proper motion star and the twenty ﬁfth closest star system, at 3.92 pc as listed by the RECONS one hundred nearest star systems. Discovered in 1897 by Jacobus Cornelius Kapteyn and Robert

Innes, Kapteyn’s Star had the largest proper motion of any star at the time, but later was pushed aside with the discovery of Barnard’s Star in 1916. Kapteyn discovered, while looking at photographic plates at the Cape Observatory in South Africa, that one star was not at its documented position on the photographic plates (Kruesi 2006). Robert Innes, who was an assistant at the observatory looked for the star and found a star matching the description but slightly east of where it should have been (Kruesi 2006). Originally catalogued as Cordoba Zone 5 hours 243 for its position in the sky, it was later re-named after Kapteyn’s death to Kapteyn’s Star, probably because he was the ﬁrst to notice it changing position from photographic plates. With a visual magnitude of 8.84 mag, this M1.5 subdwarf and halo star (Gizis 1997) is not visible to the naked eye. With such a close proximity to the Sun, Kapteyn’s Star has been chosen, like Barnard’s Star, as a Tier 1 target star for SIM, which will search for planets around parent stars. Its mass has been estimated to be 39 percent that of the Sun using relations from Henry & McCarthy (1993); Henry et al. (1999). Kapteyn’s 4

Star is likely the closest halo star (Krawchuk et al. 2000).

1.1.3 Groombridge 1830

Groombridge 1830 has µ = 700.06 yr−1 with a parallax of 000.10978 ± 000.00070 from an average of Hipparcos, YPC and HST, at 9.11 pc Groombridge 1830 is the third fastest proper motion star. Discovered in 1842 by Friedrich Wilhelm August Arge- lander after he noticed the exceptionally large proper motion, Groombridge 1830 was previously listed in Stephen Groombridge’s “A Catalog of Circumpolar Stars, Re- duced to January 1, 1810”. With a visual magnitude of 6.45 mag, this Population II subdwarf of spectral type G8 (Smith et al. 1992) is on the edge of naked eye visibility. Groombridge 1830, an old halo star, is about 0.6 the mass of the Sun and one-tenth of the solar metallicity, with an eﬀective temperature of 5170 K (Smith et al. 1992).

Groombridge 1830 had many flare observations that were thought at the time to possibly be coming from a companion star. This proposed companion, was not detected on any photographic plates, and it was later theorized that the flarewas an exceptionally large mass ejection, now known as a superflare, coming from the primary star itself (Schaefer et al. 2000). These flares can reach energies 100 to 10 million times that of typical solar flares, making it unlikely for any habitable Earth- like planet. Typical solar flares have energies on the order of 1029 ergs, although the flares recorded on Groombridge 1830 by Schaefer et al. (2000) reach 1035 ergs for a duration of 18 minutes. 5

1.2 Proper Motion Surveys

1.2.1 Why Are They Important?

Stars with the same motion in space typically originate from the same star forming cloud; this is particularly the case if found in the same region of the sky. Proper motion studies can be used to locate clusters, determine cluster membership and identify moving groups. This determination of membership is necessary to study the spatial distributions of cluster members, study the morphology of the color-magnitude diagram, and investigate the luminosity and mass functions (Jones 1997). Furthermore, accurate proper motions with radial velocities can be used to determine the space motions of stars, cluster members or a cluster as a whole. These motions can also be used to identify unusual stars that travel in orbits that are peculiar when compared to “normal” background stars. As mentioned earlier, high proper motions can also be used to identify nearby stars, because they tend to move faster than background stars that are farther away. Close dim stars with low luminosities are typically white dwarfs if bluish and brown dwarfs or M-stars if reddish. These stars can be difficult to identify, but make up the majority of stars discovered through proper motion surveys and in fact, the majority of all stellar objects in the universe. Using proper motions, one can construct a Reduced Proper Motion (RPM) diagram that can be useful in picking out white dwarf and subdwarf targets. The RPM diagram takes into account that stars with smaller distances have larger proper motions. As mentioned earlier, this is not always the case, but as can be seen in § 6.2 gives a slight advantage over a color-magnitude diagram for separating the luminosity classes. In my view, the importance of these catalogues is of no question, whether it be to further our understanding of galactic structure or merely to find fixed point 6 sources to set up a reference frame of stars. This ideal that Science is a body of cumulative data that builds upon itself, feeding on knowledge and learning from past endeavors, makes all scientific accomplishments worth sharing with the world.

1.2.2 Historical Beginnings

Edmund Halley in 1718 noticed that Sirius, Aldebaran, Betelgeux, and Arcturus were not in the observed locations charted on ancient Greek charts by Ptolemy nearly 1600 years earlier (Campbell 1913). This led him to deduce that these stars were in fact moving, which ultimately led to the discovery of proper motion (Luyten 1979). By the 1800’s, proper motion study was one of the most popular astronomical topics being researched around the world. This discovery has led to the publication of many proper motion catalogues. In chronological order and in no way complete I have done my best to list some of these historical catalogues below. In 1892, Jermain Gildersleeve Porter published “A catalogue of stars with proper motion of half a second and upwards” (Porter 1892) containing 301 entries. This catalogue, as far as I can tell, is a subset of “A catalogue of 1340 proper motion stars” (Porter 1892). Porter’s catalogue is a list of high proper motions determined from a variety of sources. Fourteen years later, Hermann Kobold published a catalogue of proper motion stars with stars having proper motions greater than 000.5 yr−1 (C. 1906) and this catalog was the standard until 1914. In 1915, a comprehensive “List of Stars with Proper Motions Exceeding 000.5 yr−1” containing 533 objects was published by van Maanen (1915). A supplement was published a few months later, which mostly contained absolute proper motions (from meridian circle observations). This supplement deleted 20 and added another 18 stars to the list (Luyten 1979). In 1919 Bossert published a catalogue of 5671 stars (Bossert & Schulhof 1919), which like the catalogues of Porter and van Maanen is a list of stars with high proper 7 motions determined by a variety of sources. Max Wolf in 1919 also published his catalogue “Katalog von 1053 staerker bewegten Fixsternen” (Wolf 1919) where he examined around 75 regions 7 x 7 degrees square in the northern hemisphere using the Bruce 16 inch telescope (Giclas 1958). The Ross Survey (Ross 1925) published by Frank E. Ross contained objects found by comparing 238 northern ﬁelds with photographic plates taken by Professor E. E. Barnard about 20 years earlier using the Bruce photographic doublet of the Yerkes Observatory (Ross 1925). These ﬁelds covered 170 square degrees with only the central 50 square degrees considered useable by Ross (Giclas 1958). Comparison of the photographic plates was done with the

ZEISS Stereocomparator using the blink attachment with proper motions relative to one comparison star (Ross 1925).

1.2.3 Luyten & Giclas

The pioneering surveys of (Giclas et al. 1971, 1978) and (Luyten 1979, 1980)1 have provided most of the proper motion systems catalogued, even as massive computer searches of digitized photographic plates have become possible. After the Bruce proper motion survey (Luyten 1938), which listed 28,535 stars south of declination -50◦ was completed in 1937, Luyten published his catalogue of stars with motions larger than 000.5 yr−1 (Luyten 1955). The famous Luyten Half Second Catalogue (LHS) (Luyten 1979) contains previously discovered proper motion stars as well as new motions from the Palomar Sky Survey. Luyten used the POSS I E plates and his own Luyten Red E plates for his northern survey. The comprehensive New Luyten Two-Tenths Catalogue (NLTT) contains 58,693 proper motion objects with µ ≥ 000.18 yr−1 and is in essence an extension of the LHS catalogue to lower proper motions. Luyten, realizing the extraordinary amount of time it would take to

1VizieR Online Data Catalogue, I/98A (Luyten 1995) 8 manually blink 936 plates, had engineers from Control Data Corporation build the ﬁrst computer controlled measuring engine known as the CDC/Luyten machine, and it was used to produce both the LHS and NLTT catalogues (Humphreys et al. 1997).

The CDC/Luyten machine has been modernized and refurbished, and is now called the Automated Plate Scanner (APS). Henry L. Giclas started work on his proper motion survey in 1957 working at the Lowell Observatory and stopped in 1975. Working with the 13-inch photographic telescope, Giclas compared earlier plates from around 1928 taken during the Pluto search with plates he continuously took as the survey progressed to look for stars that had moved from one epoch to the next. This gave Giclas an epoch spread of about 28 years at the start of his search to about 47 years by the end. Like Luyten, he realized that manually blinking all the plates would take a lifetime, so he used a projection blink comparator instrument that was modiﬁed after receiving it from the builders to have better quality condensing lenses, slow motion controls and an adjustable position angle circle (Giclas 1958). The Lowell Proper Motion Survey 8991 - Northern Stars with µ ≥ 000.27 yr−1, is a summary of many papers published from 1958 to 1970 (Giclas et al. 1971). The Lowell Proper Motion Survey - Southern Hemisphere lists of 2758 stars with µ ≥ 000.20 yr−1, and provides a summary of many papers published from 1958 to 1978 (Giclas et al. 1978).

1.2.4 Surveys Relevant to This Search

Many new high proper motion surveys have been carried out using new techniques, with each one complementing the work of Giclas and Luyten. In chronological order, surveys that sampled the sky south of declination −47◦ (the region relevant to the survey reported here) include (1) seven papers covering various portions of the southern sky by Wroblewski and collaborators who used photographic plates (Wroblewski & 9

Torres 1994), (2) UKST survey plates of 40 survey ﬁelds by Scholz and collaborators

(Scholz et al. 2000, 2002), (3) a survey of the South Galactic Cap down to R59F = 19.8 (Oppenheimer et al. 2001), (4) the machine-selected catalogue of 11289 objects from SuperCOSMOS R-band material generated by Pokorny et al. (2004), (5) the second US Naval Observatory (USNO) CCD Astrograph Catalog released in 2003 July (Zacharias et al. 2004a), (6) our own SuperCOSMOS-RECONS (SCR) proper motion search of the entire southern sky (Hambly et al. 2004; Henry et al. 2004; Subasavage et al. 2005a,b), which uses plates with all four emulsions, (7) the Naval Observatory Merged Astrometric Dataset (NOMAD) contains astrometric and photometric data for over 1 billion stars derived from the Hipparcos, Tycho-2, UCAC2, and USNO- B catalogs (Zacharias et al. 2004b), (8) the southern infrared proper motion survey

(SIPS) (Deacon et al. 2005), which uses a combination of Two Micron All Sky Survey (2MASS) data and SuperCOSMOS I band images, and (9) Lépine’sSUPERBLINK survey of a portion of the southern sky (Lépine2005). The Calan-ESO survey (Ruiz et al. 2001), which identified proper motions in 14 ESO areas of the southern sky, did not reach as far south as declination −47◦ (but one of the three ESO regions in Ruiz et al. (1993) did reach south of −47◦, yielding 39 objects). In addition, Lépine’s continuing SUPERBLINK survey will provide a vast database of proper-motion systems down to 000.15 yr−1. He has already published the northern portion of the survey, which yielded 61,977 objects (Lépine& Shara 2005).

Previously, the SCR survey focused on the faster proper motions in hopes of ﬁnd- ing new nearby stars. In this new edition of the investigation of the solar neighborhood, we continue the search for nearby stars by focusing our eﬀorts on mini-motion (MINIMO) systems with proper motions between 000.50 yr−1 and 000.18 yr−1. The like- lihood that a slow proper motion system is nearby is far lower than a fast proper motion system. Nonetheless, the much larger number of slow proper motion systems 10 discovered provides an extensive dataset for Galactic structure analyses, yields many candidates for followup work, and reveals a few nearby gems that move little relative to the Sun.

The goal since the beginning of the SCR search has been to complete a comprehensive proper-motion survey of the neglected southern sky. Adding results reported here, we have searched the sky from the south celestial pole to declination −47◦ for objects with 1000.00 yr−1 ≥ µ ≥ 000.18 yr−1, where the lower cutoﬀ was chosen to match that for the NLTT survey.

1.3 Goals and Motivation

My motivation for writing this thesis has changed slightly from when I ﬁrst began. As I mentioned earlier, I have no doubt that proper motion surveys are of great importance to the astronomical community. This however, was something that became more apparent as my work progressed. My main focus when starting this survey was to learn more about proper motion surveys, complete the SCR survey of the southern sky and of course, to obtain my Master’s degree. What I quickly found out was that

I would not be able to complete the MINIMO survey of the entire southern sky and that I would lear more from this project than expected. What has truly attracted me to this work is the combination of observational and data reduction methods required for this project. The techniques I have learned have provided me with a wealth of experience and information that I will use throughout my professional career. The photometric, spectroscopic and astrometric techniques that I have learned, have fueled my interest in parallax work. This survey has brought with it a better understanding of close faint stars with low luminosities, which happen to make up the majority of stellar objects in the universe. My goal, which was to 11 complete the SCR survey, has in return expanded my knowledge of nearby stars and helped me obtain fundamental skills associated with photometry, spectroscopy, and astrometry. 12 – 2 – Search Criteria

I introduce clear nomenclature here in an effort to sort three categories of systems revealed during the SCR proper motion search. MOTION systems have µ ≥ 100.00 yr−1 (Hambly et al. 2004). The 100.00 yr−1 cutoff is convenient and has been studied in detail by Jao (2004). SLOWMO systems have 100.00 yr−1 > µ ≥ 000.50 yr−1 (Subasavage et al. 2005a,b) . The 000.50 yr−1 cutoff has been selected to match the famous Luyten Half Second (LHS) sample. MINIMO systems reported here have 000.50 yr−1 > µ ≥ 000.18 yr−1, where the lower cutoff is designed to match that of the NLTT catalogue. Papers XII and XV (Subasavage et al. 2005a,b) include some MINIMO stars because in those papers we pushed to µ = 000.40 yr−1 to ensure that we picked up any “LHS equivalent” systems with µ ∼ 000.50 yr−1. Those papers also split the southern sky into two portions: Subasavage et al. (2005a) covered the sky from declinations −90◦ to −47◦, while Subasavage et al. (2005b) stretched north to the celestial equator. For this search, I match the boundaries in Subasavage et al. (2005a) and report all

MINIMO systems in the range 000.50 yr−1 > µ ≥ 000.18 yr−1 south of declination −47◦. This phase of the SCR search uses techniques identical to our earlier efforts, sim- ply with a lower proper motion cutoff. Identical methodology allows us to assess completeness comprehensively and compare statistics from the various search phases. Additional phases of the search can be found in Papers VIII (Hambly et al. 2004), X (Henry et al. 2004), XII (Subasavage et al. 2005a), and XV (Subasavage et al. 2005b), in The Solar Neighborhood series of papers by RECONS (hereafter TSN). The SCR search utilizes four of the Schmidt survey photographic plates available in each ESO/SRC survey field, which provide astrometric and photometric information 13

in the BJ , ESO-R, R59F and IIVN photographic passbands. Two distinct epochs in the R band come from the ESO (first epoch; also known as ESO-R) and UK (second epoch; also known as AAO-R) Schmidt telescope surveys. Sources must be detected on at least three plates and are required to have R59F brighter than magnitude 16.5. After object detection and parameterization (see Hambly et al. 2001b), coordinates are given to each detection making use of a grid of reference stars with known coordinates distributed over the plates, as described in Hambly et al. (2001a). Then the default SuperCOSMOS Sky Survey (SSS) matching of objects on multiple plates is used to extract proper motion objects (a full description can be found in Hambly et al. (2001a)). The matching is set to exclude all images that appear on all four plates having an astrometric solution that indicates a proper motion less than the cut off for this search at 000.18 yr−1 and a goodness-of-fit parameter of χ2 < 1.0 (Hambly et al. 2004). Each image either not matched or having inconsistent astrometric solu- tions due to incorrect matching is then processed one at a time using every possible combination to find a pair out to the upper limit of the SCR search, 000.50 yr−1 for this MINIMO survey. Proper motions so determined are relative to the mean reference frame defined for all stars on the plates, because all stars are used to map out small scale systematic errors in positions due to the photographic and measurement processes (see for example Hambly et al. (2001a)). Photographic plates scanned and folded into the SuperCOSMOS database are

6◦ × 6◦ with a 0.5◦ overlap of adjacent fields on each side, providing ∼25 square degrees of unique sky coverage for each field. Two hundred and three fields have been included in the MINIMO search, yielding a total coverage of ∼5075 square degrees, corresponding to 13.4% of the entire sky. In this region a total of 7410 candidate objects were detected, more than four times the amount of candidates found in TSN paper XII. Fields shown as whitespaces in Figure 2.1 were omitted 14 because of crowding near the Magellanic Clouds or Galactic Plane, or because those plate regions had epoch spreads inadequate for reliable proper motion measurements. It is worth noting that three plates (179, 227, and 228) were omitted for 000.40 yr−1 > µ

≥ 000.18 yr−1 because longer plate epoch separations are required to reliably determine slower proper motions, but were included for 000.50 yr−1 > µ ≥ 000.40 yr−1. The total region of 40 plates omitted amounts to 2.4% of the entire sky. A three stage sifting method was used to remove false detections. These steps included first a color check of the two R color plate (ESO-R, R59F ) magnitudes - they were considered to be consistent in identifying the same object if they differed by less than one magnitude. Then a second color check was used to determine if B - R and B - I were either both positive or both negative indicating the colors of a real object. The final stage of the sifting process was to check the ellipticity quality flag; if two or more ellipticities were found to be greater than 0.3 the source was deemed to be a false detection. If an object passed all three checks then it advanced to a check of databases for previous identifications. Coordinates of these objects were cross-checked using both VizieR and SIMBAD to identify previously known objects. In VizieR, a ten arcminute radius was used to match SCR detections with both the NLTT and The Liverpool-Edinburgh High Proper Motion (LEHPM) catalogues. If the coordinates of an SCR object were within a few arcminutes of a catalogue object, and the proper motion and magnitude matched, then the target object was labeled as previously known. As a final discovery verification, all potentially new objects are checked against SIMBAD to determine if they had been previously reported as proper motion objects. One class of known objects, GSC objects from the Hubble Space Telescope (HST) Guide Star Catalogue, was not considered previously “found”, as those stars were merely selected as pointing reference points for HST, not as sci- entifically noteworthy sources. Some near matches were found to be common proper 15 motion (CPM) companions to previously known proper motion objects. All of these new companions were visually inspected for accuracy and are discussed in §6.3. If the object was not found to be previously known, a visual blink inspection was done to confirm its veracity. Images were downloaded from SuperCOSMOS using wget, a free software package that can download large packets of files using a con- structed URL, pointing to the RA and DEC needed with given parameters. For the blinking process, a box size of 10 arcminutes was used to download images from the UKST blue and red surveys, which gave a sufficient epoch spread (an average of about 14 years) to confirm proper motion and wide enough area of sky to detect companions. Visual inspections are carried out by blinking the BJ and R59F SuperCOSMOS digitized plate images, using a program developed by John Subasavage. Thus, all objects reported here have been confirmed by eye, but some small number of real objects may have been discarded because visual inspections were not carried out for sources that did not pass the three checks. In keeping with previous discovery statistics, I compare the successful hit rates (real proper motion objects / total candidates extracted) for the MOTION, SLOWMO, and MINIMO samples in the portion of the sky covered by all three, from declinations −90◦ to −47◦ (not including individual plate regions that were discarded in any search). The hit rates are 6.6% for MOTION systems, 78.6% for SLOWMO systems, and 78.1% for MINIMO systems. These hit rates take into account new, known, duplicate, and “garbage” (not real) objects. In Figure 2.2, I show a plot of proper motion vs. percent successful hit rate for the entire SCR sample having µ ≥ 000.18 yr−1 south of declination −47◦. The SCR search has a sweet spot near µ ∼ 000.45 yr−1, where the success rate in picking up proper motion objects is 93%. This high success rate deteriorates toward faster and slower proper motion regimes, where the SCR search is more susceptible to false detections. Causes include mistaken object 16 movement from one plate to another when there are slight shifts between the plates, focus abnormalities, spurious objects created via plate defects, and bright star halos. In Table 2.1, SCR objects in the various papers have been categorized into the MO-

TION, SLOWMO, and MINIMO samples and discovery statistics are shown for the entire SCR sample. 17

Figure. 2.1 Plate coverage of the sky included in the MINIMO search. White boxes indicate plates that were excluded, primarily due to crowding in the Galactic Plane, LMC, and SMC, or because of an insuﬃcient spread in plate epochs. Plates 179, 227, and 228 are included because they were searched for objects with 000.50 yr−1 > µ ≥ 000.40 yr−1 but not for objects with 000.40 yr−1 > µ ≥ 000.18 yr−1. 18

100

% Hit Rate 40

MINIMO SLOWMO MOTION 20

0 0 0.2 0.4 0.6 0.8 1 1.2 1.4 1.6 1.8 2 2.2 2.4 2.6 2.8 3 proper motion (arcsec yr-1)

Figure. 2.2 Hit Rate percentage of true proper motion objects (real proper motion objects / total candidates extracted) for the entire SCR sample having µ ≥ 000.18 yr−1 south of −47◦. Horizontal bars show the proper motion bins adopted, while vertical lines delineate the three individual SCR samples — MOTION, SLOWMO and MINIMO. 19

Table 2.1. Discovery Statistics for Entire SCR Samplea

MOTIONb SLOWMOc MINIMOd New Discoveries 9 142 1879 Knowns 171 1159 5581 Duplicates 15 91 864 Garbage 1989 344 3613 Total Hits 2184 1736 11937

aEntire SCR Sample, including all previous SCR proper motion papers bMOTION sample; µ ≥ 100.00 yr−1 cSLOWMO sample; 100.00 yr−1 > µ ≥ 000.50 yr−1 dMINIMO sample; 000.50 yr−1 > µ ≥ 000.18 yr−1 20 – 3 – Comparison to Previous Proper-Motion Surveys

The NLTT catalogue lists 58693 objects with µ ≥ 000.18 yr−1. Of these, 2457 objects meet the search criteria of this paper, are within the ﬁelds searched, and have estimated red magnitudes of 16.5 or brighter. I recover 1966 of the 2457 NLTT objects, resulting in an 80% recovery rate. Several factors contribute to the 20% of unrecov- ered stars. Our proper motions are accurate to ∼000.02 yr−1 and our magnitudes to

∼0.3 mag. Proper motions and magnitudes in the NLTT in some cases differ from ours, which causes us to drop some objects that were included in the NLTT. On rare occasions we also miss stars that are lost on recent plates due to mergers where two object are now occupying the same space on the photographic plate, but were uncorrupted during previous efforts. Our SCR search has trouble picking up brighter sources due to halo effects present on the photographic plates. The brightest NLTT source I obtain in my search is at R59F ∼ 5.4 mag while the brightest NLTT source in this portion of the sky is R ∼ 1.6 mag. Here I compare the results from the entire

SCR survey to date for declinations −90◦ to −47◦ to the proper motion surveys listed in Table 3.11. The numbers listed reﬂect only the total number of entries in each work — I have not conﬁrmed that all sources by other groups are both real and original.

1For samples that were reported in 1950 coordinates, I have not computed 2000 coordinates or slid stars because of proper motion over 50 years. The number of objects that may have slipped out of the sample by moving north of −47◦ is expected to be small, and a comparable number of replacement objects likely have slipped south. 21 b a ◦ 47 − Total # of Publications References 1 − 18 yr . 00 0 ≥ > µ 1 − 50 yr . 00 0 1 − 50 yr . 00 0 ≥ > µ 1 − 00 yr . 00 1 1 − 00 yr . 00 1 ≥ µ Table 3.1. Number of NLTT-Type Objects Discovered South of Declination Survey References include (1) Luyten (1979, 1980); (2,3,4,5,6) Hambly et al. (2004); Henry et al. (2004); Subasavage et al. (2005a,b), this paper; (7,8,9) Wroblewski Numbers listed indicate objects reported as “new” in the survey publications. Pokorny did not diﬀerentiate between new and previously known objects, so a b NLTTSuperCOSMOS-RECONSWroblewski and collaboratorsSUPERBLINKScholz and collaboratorsRuiz and collaboratorsSIPSOppenheimer et al.Pokorny 3 5 et al. 2 0 1 56 1 28 70 mixed 7 11 2 43 261 mixed 4 1742 488 20 55 37 3529 29 1817 mixed 519 2 68 5 4 3846 mixed 0 39 73 2, 3, 4, 2 7, 7 5, 8, 6 2 9 1 1 1 27 11, 12 16, 1 17 1 13 10 1 15 14 & Torres (1989, 1991,(2001); 1994); (16,17) (10) Pokorny L´epine(2005); et (11,12) al. Scholz (2003, et 2004) al. (2000, 2002); (13) Ruiz et al. (1993); (14) Deacon et al. (2005); (15) Oppenheimer et al. the entry is labled as mixed. 22 – 4 – Data

In the Appendix I list the 1684 new MINIMO systems reported in this survey covering declinations −90◦ to −47◦ with 000.50 yr−1 > µ ≥ 000.18 yr−1. In Table 4.1, I highlight the 34 systems for which we estimate distances of less than 25 pc, and 17 additional white dwarf candidates. As in previous SCR search papers, in the Appendix and

Table 4.1 I list SCR names, coordinates, relative proper motions, plate magnitudes from SuperCOSMOS, infrared photometry from 2MASS, the R59F −J color, a distance estimate, and notes. All coordinates are for epoch and equinox J2000.0 and are computed using the Two Micron All Sky Survey (2MASS) coordinates and adjusted to epoch 2000.0 using the SCR proper motions and position angles. Proper motions are extracted using the

J and R59F combination of plates to produce a uniform survey with the highest possible accuracy, as described in Hambly et al. (2001a), where a full description can be found. In brief, these two plates have a good time baseline between the ﬁrst and second epoch and reach to J ∼ 22.5 and R59F ∼ 21.0 giving the best plate pairing.

For this search, R59F brighter than 16.5 mag was chosen, because those magnitudes are easily reachable with the 0.9-m Cassegrain telescope at the Cerro Tololo Inter- American Observatory (CTIO) in Chile. From our search algorithm, the average proper motion errors are ∼000.010 yr−1. I show in Figure 4.1 that our proper motion and position angle measurements are consistent with those in NLTT and Hipparcos by examining 298 MINIMO stars that had data in both catalogues.1 The results indicate that the SCR proper motions and position angles have average deviations

1NLTT proper motion data are quantized south of DEC −45◦, hence the structure of the points at low proper motions. 23 of ∼000.020 yr−1 and ∼3.9◦ compared to Hipparcos motions, and ∼000.025 yr−1 and ∼6.8◦ compared to NLTT. I also show that the NLTT and Hipparcos proper motions and position angles show average deviations in proper motions of ∼000.019 yr−1 and

∼5.1◦ when compared to each other. Comparison of the three outlying data points in position angle in the SCR vs. NLTT and Hipparcos vs. NLTT plots indicates that these NLTT measurements are incorrect. The consistency between SCR and Hipparcos is particularly encouraging because Hipparcos only observed stars brighter than V ∼ 12, and these are the stars with the poorest measured proper motions in the SCR survey.

Photographic magnitudes are given in the Appendix and Table 4.1 for three plate emulsions: BJ , R59F , and IIVN . Plate magnitude errors are typically less than 0.3 mag for sources fainter than 15th mag, with errors increasing for brighter objects because of systematic errors (Hambly et al. 2001b). Plate color errors are typically only 0.07 mag. 2MASS JHKs photometry and a representative color, R59F −J, generated using two of the most reliable photometric measurements, are given. All JHKs infrared photometry is extracted from 2MASS via VizieR and these magnitudes were spot- checked by eye for accuracy. 2MASS magnitude errors are 0.03 mag or less in most cases. This holds true unless J > 15, H > 14.5 or Ks > 14, for which the errors are typically 0.05 mag or greater. The six-band photometry is used to generate 12 colors that are utilized to compute distance estimates, as described in Hambly et al. (2004). All estimates assume that the objects are single, main sequence stars. The accuracy of the technique is 26%, deﬁned as the mean of the absolute values of the diﬀerences between distances for stars with trigonometric parallaxes and distances estimated via the relations. In cases where objects are too blue for the relations, no distance is listed. In a few cases the BJ and/or

IIVN plate magnitudes are not determined (likely causes include confusing sources and 24 plate defects) making the distance estimate less reliable. Seventeen white dwarf and 191 subdwarf candidates have erroneous distances (listed in brackets) from the suite of relations because they are not main sequence stars; more accurate estimates are given in the notes for the white dwarfs. Overall, I find three systems within 10 pc, 31 between 10 and 25 pc, and 408 between 25 and 50 pc. Some of the common proper motion (CPM) candidates were not revealed during the SCR search because of confusion with another source, or because the companion was fainter than our magnitude cutoff; these were however, noticed during the blinking process. In these cases the objects are investigated using SIMBAD and VizieR to check for previous identification. If the object was not previously known, I used Su- perCOSMOS and 2MASS magnitudes to find the six colors used to compute distance estimates, and proper motion data from SuperCOSMOS to compute proper motions and position angles (see § 6.3). 25 a a a (pc) Est Dist Notes J − from F 1 59 − R s 18 yr . 00 0 ≥ > µ 1 − JHK 11.84 11.23 10.91 4.49 24.6 50 yr 25pc . 00 ··· IVN < ◦ I 47 F 59 R ≤ − J < δ ◦ 90 ) − ◦ SCR Red Dwarf candidates )( 00 µ θ B (J2000) (J2000) ( Parsecs and New White Dwarf Candidates with 0 Table 4.1. Characteristics of New SCR Systems Estimated to be Nearer than 25 Name RA DEC SCR 2241-6119A 22 41 44.36 -61 19 31.2 0.184 124.0 15.64 13.65 11.70 10.20 9.61 9.35 3.44 23.2 SCR 0635-6722SCR 0838-5855SCR 1147-5504SCR 1217-7810 06SCR 35 1220-8302 48.81 08SCR 38 1224-5339 02.24 11SCR 47 1240-8116 -67 52.49 22 12SCR 58.5 17 1245-5506 -58 26.93 55 12SCR 58.7 20 1347-7610 -55 03.71 04 12SCR 0.383 11.9 24 1420-7516 -78 24.44 10 12SCR 0.320 45.9 40 1441-7338 -83 55.99 340.0 02 12SCR 0.192 29.2 45 1448-5735 -53 52.53 188.9 39 13SCR 0.212 08.8 47 1456-7239 -81 12.21 56.80 011.3 16 14SCR 0.243 30.9 20 1738-5942 -55 18.44 36.84 056.6 06 14SCR 0.189 50.2 41 1820-6225 -76 14.95 9.83 14.42 244.2 10 14SCR 0.492 20.0 16.11 48 1826-6542 17.54 39.82 251.9 -75 14SCR 0.412 16 12.23 56 1853-7537 -73 17.03 5.9 02.29 279.8 38 17SCR 0.194 8.66 12.43 41.4 15.69 38 1856-4704 -57 16.93 41.02 107.0 35 18SCR 10.25 17.7 14.93 20 1926-8216 -72 15.15 0.195 49.35 089.7 39 18 10.30SCR 0.207 13.14 41.4 14.77 26 1932-5005 -59 8.54 14.84 46.83 42 18SCR 0.202 12.79 9.67 24.4 13.11 53 1959-6236 243.7 -62 12.39 26.61 029.0 25 18 11.19SCR 9.70 0.207 12.30 52.7 12.82 56 2016-7531 -65 38.40 188.8 7.95 42 19 10.97SCR 0.280 14.22 11.25 39.9 10.26 26 2042-5737 -75 18.27 9.08 10.64 48.64 225.0 37 19 10.50SCR 0.190 10.34 39.8 32 9.26 2230-5244 -47 12.47 10.39 48.64 148.2 04 19 12.68 0.311 7.69 9.73 58.3 16.14 59 10.35 8.88 -82 16.50 33.55 164.8 16 20SCR 8.81 9.93 0.304 8.99 47.6 10.59 16 2335-6433A 10.07 -50 16.57 11.25 10.44 178.9 05 20 0.252 13.04 38.9 14.22 42 -62 13.35 9.16 46.44 168.7 8.62 36 22 0.195 5.80 12.46 13.4 14.20 30 9.64 -75 18.68 8.42 27.95 131.3 4.49 9.44 31 1.29 11.19 23 0.257 11.99 04.5 11.17 35 -57 12.20 2.56 172.5 18.43 3.96 37 8.89 0.189 11.92 8.01 9.14 15.3 16.43 -52 16.29 10.60 157.5 44 10.62 8.12 0.253 8.90 29.1 8.43 12.22 -64 9.85 288.7 10.38 33 0.264 4.26 12.91 13.92 42.4 10.26 16.86 7.77 8.55 10.05 081.3 8.4 0.369 10.00 24.5 22.7 17.47 8.63 3.38 142.6 9.13 10.56 9.83 9.09 0.196 11.64 24.1 14.50 25.0 17.06 3.83 9.74 125.7 8.43 10.20 15.35 15.06 4.95 103.1 10.29 9.96 11.99 8.48 1.64 14.74 9.58 8.34 19.01 18.1 12.67 9.04 3.23 13.22 11.79 10.75 9.74 12.24 19.1 16.34 9.54 3.60 8.29 1.45 7.73 11.06 11.55 11.4 8.42 9.97 10.11 10.46 3.82 19.0 9.44 10.49 22.5 7.49 9.97 9.84 21.3 8.30 9.86 5.86 9.01 2.04 10.22 24.9 18.2 9.52 3.63 9.50 20.8 8.63 1.51 3.75 0.96 4.29 9.03 22.4 9.2 8.02 4.28 21.4 7.86 20.0 3.25 24.4 17.3 24.3 16.2 1.33 22.7 24.5 SCR 0100-7904SCR 0135-6127SCR 0138-5353SCR 0211-6108 01SCR 00 0232-8458 56.08 01SCR 35 0246-7024 53.66 01SCR 38 0527-7231 -79 20.51 04 02SCR 25.2 11 0630-7643AB -61 35.42 27 02 11.1 32 -53 50.12 53 02 0.379 06 26.1 46 -61 30 02.25 08 05 46.61 0.255 53.8 27 -84 06.99 215.3 58 0.297 09.5 -70 -76 256.8 24 0.234 43 06.3 -72 08.9 13.69 071.0 31 0.220 20.0 15.61 060.8 0.259 0.483 11.69 15.70 141.9 0.368 13.67 11.68 113.2 356.8 13.69 9.98 12.31 018.3 11.80 15.71 9.73 15.77 11.73 10.17 16.01 8.79 10.05 13.32 13.56 10.27 9.23 13.96 9.87 9.53 10.71 8.16 10.73 9.69 11.76 8.67 8.99 9.83 9.24 8.89 7.88 10.33 9.42 8.15 8.34 9.32 8.27 9.76 3.61 8.07 2.89 8.18 9.01 3.42 7.92 9.47 1.06 1.17 20.8 3.49 14.9 4.67 3.63 24.2 22.9 24.9 20.0 22.6 6.9 26 8.1pc 4.4pc 11.9pc 10.4pc 6.9pc 5.6pc 12.2pc 9.7pc ± ± 6.0 pc 7.6pc 4.4pc 5.9 pc ± ± ± ± ± ± 6.0pc 5.8pc 7.0pc 9.8pc 7.7pc ± ± ± ± ± ± ± ± ± 40.5 22.2 59.3 52.2 34.5 28.0 60.7 48.7 29.8 38.2 22.2 29.3 29.9 28.9 34.8 49.1 38.6 a b c c d e a c f c e f c c f c e f c a b c d c c e a b c d c f c f c a b c c ··· ··· ··· ··· (pc) Est Dist Notes J − F 59 R s JHK ······························ IVN I F 59 R SCR WD Candidates J Table 4.1 (cont’d) ) ◦ )( 00 µ θ B (J2000) (J2000) ( Name RA DEC Not detected during automated search but noticed by eye during theNot blinking in process 2MASS Common proper motion; see Table 6.1 WD candidate with unreliable distance estimate [in brackets]; more reliable WDAll distance colors estimate are in too notes blue for distance relations WD confirmed via spectroscopy; results already published or will be published in a future paper by John P. Subasavage a b c d e f SCR 0018-6851 00 18 08.56 -68 51 19.4 0.220 091.6 16.55 16.46 16.48 16.62 16.13 17.18 -0.16 SCR 0004-6120B 00 04 45.41 -61 23 40.0 0.171 127.6 16.86 16.76 16.53 16.43 15.93 16.47 0.32 [1216.2] SCR 0104-5742BSCR 0150-7207 01SCR 04 0245-6038 12.14SCR 0252-7522 01 -57 50SCR 42 38.49 0311-6215 02 48.6 45SCR 27.77 0355-5611 02 -72 52 0.239 07SCR 45.71 16.8 0429-5423B -60 03 38 11SCR 58.2 21.33 0840-7826 091.1 03 -75 0.334 55 04SCR 22 31.89 29 0857-6032 44.5 05.93 0.196 -62 16.19SCR 15 223.9 1257-5554B 15.7 08 -56 0.496 40SCR 11 -54 049.6 29.00 1821-5951 28.2 23 15.89 08 16.18 03.6 12 57 0.416SCR 57 08.21 063.5 2016-7945 32.85 17.15 -78 0.279 15.78 26SCR 0.170 15.71 083.3 46.0 2020-7806 18 -60 17.09 21 -55 32 16.36SCR 59.54 54 029.1 45.4 15.67 2032-4948B 48.9 20 15.24 15.68 0.399 39.7 16SCR 16.32 49.74 2354-6023 20 -59 16.07 17.36 0.217 15.56 20 20 51 0.413 15.65 52.98 010.3 32 16.05 48.5 17.91 41.74 -79 16.17 45 15.83 333.3 16.46 15.75 53.0 293.3 23 15.64 -78 16.06 0.365 16.13 54 06 -49 17.08 15.77 50.63 18.7 48 15.47 15.20 16.11 57.2 0.434 15.05 15.42 15.82 194.9 16.13 16.97 15.76 -60 0.276 15.66 23 15.37 0.22 0.270 16.05 128.4 13.89 16.0 17.49 15.77 16.31 15.33 209.2 15.45 182.4 15.53 16.74 0.230 11.97 0.06 16.31 16.50 15.62 16.03 0.52 17.15 15.44 15.94 16.09 098.6 [872.1] 15.57 15.72 0.55 16.09 16.77 16.20 15.75 16.31 -0.08 15.47 15.20 16.11 0.41 15.78 [821.9] 16.73 16.06 15.10 15.00 [675.9] 15.92 16.62 15.02 15.93 0.20 14.90 -0.56 15.59 15.87 [755.9] 14.64 15.87 15.68 15.88 15.77 1.11 [763.9] 0.99 16.31 0.16 0.14 [588.9] 0.18 [482.5] [834.9] [900.1] [1127.8] 27

0.5 360

330 0.46 300 0.42 270 ) -1 0.38 240

210 0.34 180 0.3 150 Hipparcos star 0.26 T 120 Hipparcos (arcsec yr P -1 90 ' = 3.9 o 0.22 ' = 0".020 yr 60 0.18 30

0.14 0 0.14 0.18 0.22 0.26 0.3 0.34 0.38 0.42 0.46 0.5 0 30 60 90 120 150 180 210 240 270 300 330 360 P SCR (arcsec yr-1) T SCR star 0.5 360

330 0.46 300 0.42 270 )

-1 0.38 240

210 0.34 180

0.3 NLTT T 150

NLTT (arcsec yr 0.26 120 P

-1 90 ' = 6.8 o 0.22 ' = 0".025 yr 60 0.18 30

0.14 0 0.14 0.18 0.22 0.26 0.3 0.34 0.38 0.42 0.46 0.5 0 30 60 90 120 150 180 210 240 270 300 330 360 P SCR (arcsec yr-1) T SCR star 0.5 360

330 0.46 300 0.42 270 )

-1 0.38 240

210 0.34 180

0.3 NLTT T 150

NLTT (arcsec yr 0.26 120 P

-1 90 ' o 0.22 ' = 0".019 yr = 5.1 60 0.18 30

0.14 0 0.14 0.18 0.22 0.26 0.3 0.34 0.38 0.42 0.46 0.5 0 30 60 90 120 150 180 210 240 270 300 330 360 P Hipparcos (arcsec yr-1) T Hipparcos star

Figure. 4.1 Comparison of NLTT, Hipparcos, and SCR proper motions and position angles. The solid lines indicate perfect agreement. Note that proper motion data for NLTT is quantized south of −45◦. 28 – 5 – Photometric and Spectroscopic Observations of the Nearby Sample

The nearby systems are of special interest, so we obtained photometric and spectroscopic observations to better limit and understand the nature of these objects. In all we obtained photometry for sixteen and spectra for twelve of the thirty-four 25 pc MINIMO sample.

5.1 Photometry

All but two nights of VJ ,RC , and IC photometry observations were made with the Tek 2 VRI ﬁlter set using the CTIO 0.9 meter telescope equipped with a 2048 x 2048 Tektronix CCD camera, yielding a 000.401 pixel−1 plate scale (Jao et al. 2003). Two nights in 2005 August were taken with a standard Kitt Peak VRI ﬁlter set using the

CTIO 1.0 meter telescope equipped with a OSU 4K x 4K CCD camera, yielding a 20 x 20 arcminute ﬁeld of view and a 000.289 pixel−1 plate scale. Results for systems within 25 pc according to their plate and 2MASS magnitudes are listed in Table 5.1. All VRI values were obtained between 2003 October and 2006 November. I also list the number of observations, 2MASS JHKS photometry, spectral type, photometric CCD distance estimates, and notes. For the VRI photometry, bias and dome ﬂats were taken at the beginning of each night and used to calibrate the science frames during reductions. Science stars were observed between 1.11 and 1.75 airmasses with a range of exposure times depending on the brightness of the star. Typically, at least eight standard stars from Graham (1982), Bessel (1990), and Landolt (1992) were observed between 1.0 and 2.0 airmasses 29

each night to calibrate the VJ RC IC system and to calculate extinction corrections. All the data were reduced using the Image Reduction and Analysis Facility (IRAF) following the CTIOPI Photometry Reduction User Guide written by Wei-Chun Jao.

The initial bias subtraction, flat fielding and overscan are done with a customized IRAF package called redpi (Jao et al. 2005). After this initial processing of the raw data, each image is checked by eye for cosmic rays, crowding around the science star, and to obtain the average Full Width at Half Max (FWHM), which changes from night to night. The next step is to tag the standard stars with a circular aperture of 1400 in diameter to match Landolt’s (1992) observations of standard stars. Once all the standard stars have been tagged, a sky annulus of 2000 in radius with a 300 width is used to determine the background counts (Jao et al. 2003). Instrumental magnitudes are extracted using the IRAF task apercorr and grouped into a master file. The transformation equations from Wei-Chun Jao’s Photometry Reduction User Guide used to obtain apparent magnitudes are

V = mV + a1 + a2X + a3(mV − mI ) + a4(mV − mI )X,

R = mR + b1 + b2X + b3(mR − mI ) + b4(mR − mI )X,

I = mI + c1 + c2X + c3(mR − mI ) + c4(mR − mI )X.

Where V, R, and I are apparent magnitudes for standard stars, mVRI are instrumental magnitudes from IRAF, a1234, b1234, and c1234 are transformation coefficients and X is airmass. The IRAF task fitparam is then used to obtain transformation coefficients that were used for the science star photometry. The science stars are then checked for cosmic rays and tagged using the same method as above with a circular aperture of 1400 in diameter. A few stars had other 30 sources within this aperture, so an aperture correction was used with an appropriate circular aperture of 700- 800 in diameter to minimize stray light. Instrumental magnitudes were then obtained as above using the IRAF task apercorr. The final VJ ,RC , and IC magnitudes are extracted by applying the transformation equations using a custom Perl task written by Wei-Chun Jao similar to the IRAF task evalfit. Errors in optical photometry have been analyzed in Henry et al. (2004), where a full discussion can be found. I adopt the same error of ±0.03 mag in each band, and the results are listed in Table 5.1.

For CCD distance estimates, VRI photometry from CTIO observations and JHKs infrared photometry extracted from 2MASS are used to generate 12 colors that are utilized to compute estimates as described in Henry et al. (2004). Brieﬂy, ﬁfth-order

fits are used for the 12 colors with any higher order not improving the fits in any meaningful way. All estimates assume that the objects are single, main sequence stars. The reliability of these distance estimates has been investigated in Henry et al. (2004), where a sample of 140 stars used to generate the fits were run back through the relations, yielding an accuracy of 15.3% for this technique. Henry et al. (2004) also show that for the reddest dwarfs the accuracy is remarkably better at 9.3%. CCD distance estimates are more accurate than plate estimates determined from the SSS BRI and 2MASS infrared magnitudes, which have errors of 26% in estimated distances. In Table 5.1, I list CCD distance estimates for 16 of the 34 systems with distances within 25 pc according to their plate and 2MASS magnitudes. Of these 16 CCD distances, six have estimates that are greater than 25 pc with only three of the six greater than 30 pc. These are, however, still approximate until parallax data is obtained for final distance determinations. 31 from a a b b 1 a b c − 18 yr . 00 ··· ··· ··· ··· 0 ≥ ········································································ ···································· Dist SpT Notes > µ 1 s − 50 yr . 00 ◦ 47 JHK 9.14 8.559.13 8.43 8.489.04 8.29 8.429.97 8.30 9.52 9.03 9.67 9.08 8.81 8.629.44 8.01 8.90 7.77 8.63 10.6210.38 10.05 9.83 9.74 9.58 10.7511.06 10.1110.46 10.49 9.84 11.84 9.86 10.22 10.20 11.23 9.50 9.61 10.91 9.35 10.29 9.74 9.44 11.1910.97 10.6410.50 10.39 10.35 9.93 10.07 9.64 ≤ − # < δ Obs (pc) ◦ 90 C I − C R J V ························································································································ ························ ···························································· ············ Name Published in (Subasavage et al. 2005a) Common proper motion see Table 6.1 First published in (Henry et al. 2004) a b c SCR 1456-7239 SCR 1738-5942 SCR 1820-6225 SCR 1826-6542SCR 1926-8216 17.34SCR 1932-5005 SCR 1959-6236 15.27SCR 2016-7531 SCR 2042-5737 12.96SCR 2230-5244 SCR 2241-6119A SCR 3 2335-6433A 10.56 11.20 10.42 9.96 9.64 9.54 9.2 1 8.63 8.02 7.86 35.8 SCR 1448-5735 SCR 1853-7537SCR 1856-4704 11.22 10.31 9.43 1 8.34 7.73 7.49 25.0 SCR 1217-7810 SCR 1220-8302 SCR 1224-5339 SCR 1240-8116SCR 1245-5506SCR 1347-7610 SCR 1420-7516 14.10SCR 1441-7338 13.66 12.88 12.31 11.28 17.04 10.61 15.32 1 2 13.27 9.73 8.99 1 9.16 8.42 11.19 8.89 10.60 8.12 19.3 10.26 11.3 M4.0V 16.6 M4.0V SCR 0635-6722SCR 0838-5855SCR 1147-5504 11.54 17.19 10.62 15.07 9.64 12.78 2 3 8.54 10.30 9.70 7.95 9.26 7.69 25.8 7.9 M1.0V M6.0V SCR 0100-7904SCR 0135-6127SCR 0138-5353SCR 0211-6108 12.45SCR 0232-8458 14.28SCR 0246-7024 11.42 14.35SCR 0527-7231 13.10 10.40SCR 10.08 0630-7643AB 13.21 11.47 11.57 14.84 9.84 14.82 11.70 10.65 14.71 1 13.43 1 13.08 9.37 13.49 9.90 1 11.60 10.99 8.79 11.88 10.05 1 1 10.27 1 8.16 4 9.53 2 9.69 8.67 8.99 7.88 9.83 9.24 8.89 10.33 9.42 8.15 18.7 8.34 25.2 9.32 9.76 8.27 29.7 M2.5V 8.07 M3.5V 8.18 9.01 9.47 7.92 M3.5V 58.5 43.2 14.2 24.9 5.4 K3.0V M0.0V M4.5V M3.5V M5.0V Systems Estimated to be Nearer than 25 pc with 0 Table 5.1. Photometry, Spectral Types and CCD Distance Estimates for MINIMO 32

5.2 Spectroscopy

All spectroscopic observations were made with the CTIO 1.5m telescope equipped with a Ritchey-Chr´etienSpectrograph and a Loral 1200 x 800 CCD camera. The results listed in Table 5.1 are from observations taken between 2003 December and

2006 December. Grating number 32 was used covering wavelengths from 6000 to 9500 A˚ with a resolution of 8.6 A.˚ Bias and dome flats were taken at the beginning of each night and used to calibrate the science frames in the reductions. Observations were taken at an airmass of less than 2.0 with a slit width of 600 at various exposure times ranging from 10 - 1800 seconds. Three targets (SCR 0630-7643, SCR 1240- 8116, and SCR 1245-5506) were observed before 2006 with a 200 slit width and may have flux calibration problems. Two exposures were taken of each object to help in the removal of cosmic rays and were then combined into a single spectrum of each object. After each science exposure, a He-Ne-Ar comparison lamp exposure was taken for wavelength calibration. Standard stars (white dwarf or main sequence) were observed to enable flux calibration. The spectra are plotted in Figure 5.1, and they are normalized at 7500A˚ with the addition of an integer to fit on the plot. All the data were reduced using IRAF with bias subtraction and flat fielding done using the standard IRAF tasks. Reduction was done following the steps in a User Guide to Spectroscopy Reduction, which I wrote after learning how to reduce spectra from Thom Beaulieu. After the initial processing of the raw data, the next step is to check the background fit by using the IRAF task background. Once this is done we can extract the apertures using the IRAF task apsum on spectra of the science stars, flux standards, and comparison lamp spectra. This procedure extracts a comparison lamp image for every science/flux standard image using the same extraction parameters. The IRAF task identify is used to identify known features within the 33 spectra. Sensitivity functions were created for each standard using the IRAF task sensfunc and then used with the IRAF task calibrate to apply extinction and flux calibrations to all the images. The final step is to clean the images by clipping cosmic rays and bad columns using IRAF task splot. Spectral types listed in Table 5.1 were assigned using an updated version of the ALLSTAR program, which is described in Henry et al. (2002). This program matches spectra from a list of standard spectra in the RECONS database. 34

HĮ K I Na I Ca II 13

12 SCR 0838-5855 (M6.0V) 11 SCR 0630-7643 (M5.0V) 10 SCR 0246-7024 (M4.5V)

9 SCR 1240-8116 (M4.0V)

8 SCR 1245-5506 ) + Integer + ) (M4.0V) O

7 SCR 0527-7231 (M3.5V)

6 SCR 0135-6127 (M3.5V)

5 SCR 0138-5353 (M3.5V)

NormalizedFlux(F 4 SCR 0100-7904 (M2.5V)

SCR 0635-6722 3 (M1.0V)

SCR 0232-8458 2 (M0.0V) SCR 0211-6108 (K3.0V) 1

0 6100 6600 7100 7600 8100 8600 9100 Wavelength (Å)

Figure. 5.1 Spectral plots of new SCR discoveries estimated to be within 25 pc. Note that spectra of SCR 0630-7643AB, SCR 1240-8116, and SCR 1245-5506 were taken with a 200 slit width and may have minor ﬂux calibration problems. 35 – 6 – Analysis

6.1 Color-Magnitude Diagram

Plotted in Figure 6.1 is a color magnitude diagram comparing the new SCR objects (open circles) to the known objects (small points) from this MINIMO phase of the search. As in TSN Papers XII and XV, the bulk of the new discoveries are fainter and redder than the known stars, including three objects, SCR 0838-5855, SCR 1826-6542, and SCR 2241-6119B with R59F − J > 5.5. Unlike the sources extracted in previous eﬀorts, there are more new discoveries featured in this search that are brighter and bluer than before. In fact, there are nine new discoveries with R59F brighter than

10th magnitude that had not been identiﬁed previously. The point at R59F = 8.14 is SCR 1914-7109, which is too blue for us to estimate a distance using the plate- 2MASS relations. CCD photometry and spectroscopy observations would clarify its true nature. As in comparable plots in previous papers, several white dwarf candidates are clearly separated from the bulk of the sample. The subdwarf population is less well- deﬁned, but a population of subdwarfs can be detected below the concentration of main sequence stars. 36

SCR Discoveries 6

Known 8

59F 12 R

20 -2 -1 0 1 2 3 4 5 6

R59F - J

Figure. 6.1 Color-apparent magnitude diagram for SCR systems (open circles) and known systems (small points) with 000.50 yr−1 > µ ≥ 000.18 yr−1 from −90◦ < δ ≤ ◦ −47 . Data points below our search cutoﬀ of R59F = 16.5 are CPM companions noticed during the blinking process. 37

6.2 Reduced Proper Motion Diagram

Shown in Figure 6.2 is the reduced proper motion (RPM) diagram for objects found in this search, similar to the RPM diagrams shown in TSN Papers XII and XV. The RPM diagram relies on the statistical (inverse) relationship between proper motion and distance: objects that have larger distances generally have smaller proper motions. As such, it can be used to separate white dwarfs and (less clearly) subdwarfs from main-sequence stars. While this assumption is not always valid, it is a fairly reliable indicator of luminosity class for most stars. As in previous papers related to the SCR search, the relation used to determine HR is

HR = R59F + 5 + 5 log µ.

A comparison of Figures 6.1 and 6.2 shows that the RPM diagram is slightly better than the color magnitude diagram at separating the three samples, in particular the split between subdwarf and main sequence stars. There is a clear break separating the white dwarfs from the rest of the sample. The arbitrary dashed line between the subdwarfs and white dwarfs is the same as used in TSN Paper XV, although the proper motions are smaller. In this region of the diagram, I ﬁnd 15 new white dwarf candidates: SCR 0004-6120B, SCR 0018-6851, SCR 0104-5742B, SCR 0150-7207, SCR 0245-6038, SCR 0252-7522, SCR 0311-6215, SCR 0355-5611, SCR 0840-7826, SCR 0857-6032, SCR 1821-5951, SCR 2016-7945, SCR 2020-7806, SCR 2032-4948B, and SCR 2354-6023. Two additional candidates, SCR 0429-5423B and SCR 1257-5554B were noticed while blinking to have the colors consistent with a white dwarf, bringing the total number of white dwarf candidates for this search to 17, but both lack the 2MASS data to plot in the RPM diagram. One object SCR 1800-5112B is a close double with blended photometry in SuperCOSMOS, 38 which puts it inside the white dwarf regime of the RPM diagram. The infrared colors however are not consistent with a white dwarf, and therefore is not considered a white dwarf candidate. Of the 17 candidates, three (SCR 0104-5742B, SCR 0150-7207 and

SCR 1821-5951) have been spectroscopically confirmed (results to be presented in a future publication). Three more (SCR 0252-7522, SCR 0311-6215 and SCR 2016- 7945) have been spectroscopically confirmed in a earlier publication (Subasavage et al. 2005a). Each is listed in Table 4.1 with a bracketed erroneous distance estimate assuming the object is a main sequence star. I include a distance estimate based on the assumption of the source being a main sequence member because large distances can be used to flag possible white dwarfs. All the white dwarfs have distances for main sequence luminosities beyond 400 pc except SCR 0018-6851, SCR 0150-7207,

SCR 0311-6215, SCR 0429-5423B, SCR 0857-6032, and SCR 1257-5554B, which have blended SuperCOSMOS photometry, no 2MASS data, or are too blue for the relations. In the notes I give more accurate distance estimates assuming the objects are single white dwarfs by comparing the candidates to a sample of 47 white dwarfs of known

distance to calibrate the R59F − J color vs. MR59F relation (valid for −0.25 < R59F − J < 1.6) developed by John Subasavage. Errors in the distances are estimated to be 13%. This brings the total number of white dwarf candidates to 31 for the SCR survey. To be consistent with TSN Paper XV, subdwarf candidates are selected to have

R59F − J > 1.0 and HR > 4.0 mag above the dashed line separating the white dwarfs from the subdwarfs. As with the white dwarf cutoﬀ line, the subdwarf cutoﬀ used is arbitrary, yet provides a fairly accurate distinction between the subdwarfs and main sequence classes. Although some contamination of the sample is expected, we count a total of 191 new subdwarf candidates from this search. This brings the total number of SCR subdwarf candidates to date to 238. 39

SCR Discoveries 6 Confirmed Known WD Known 8

R 12 H

20 -2 -1 0 1 2 3 4 5 6

R59F - J

Figure. 6.2 Reduced proper motion diagram for SCR systems (open circles) and known systems (small points) with 000.50 yr−1 > µ ≥ 000.18 yr−1 from −90◦ < δ ≤ −47◦. The arbitrary dotted line separates the white dwarfs from the subdwarfs. Triangles denote previously known white dwarfs. 40

6.3 New Common Proper Motion Systems

In this search I found a total of 57 new likely CPM systems, including 55 doubles and two triples (i.e. 59 companions). All primaries, companions and their proper motions are recorded in Table 6.1, where the separations and position angles of the companions relative to the primary stars are also listed. Twenty-three pairs of objects were discovered via the automated search and were subsequently noticed to have common proper motion. Twenty-six additional new SCR companions not revealed during the automated search were noticed during the blinking process. Ten previously known objects were noticed by eye to have common proper motions to SCR stars discovered during the automated search. In Figures 6.3 and 6.4, I compare the proper motions and position angles for the 55 pairs having complete sets of µ and θ. Because of blending in four systems,

SuperCOSMOS data could not be obtained for the potential companion, and they were too close to obtain accurate manual measurements. Values obtained through the systematic SCR trawl are shown with ﬁlled circles, while open circles are used if a companion was noticed during the blinking process of the SuperCOSMOS scans. Data were then retrieved manually from SuperCOSMOS for the noticed companions.

Usually, such companions are fainter than the search cutoﬀ of R59F = 16.5. As is typical with proper motion surveys, the position angles of the proper motions are better determined than the proper motions themselves, which are particularly volatile at these relatively low values. Hence, the position angles are given greater weight when deciding whether or not two sources really are part of the same system. The average scatter for the proper motions and position angles are ∼000.020 yr−1 and ∼ 5.0◦, respectively, which is consistent with comparisons of SCR data to NLTT and Hipparcos, as discussed previously. Distance estimates for multiple components 41 within a factor of two are considered to be consistent, given the errors of the distance estimating relations. Distances in parentheses are deemed unreliable due to either lack of BRI photometry, used fewer than six relations, I photometry suspect or because the primary is likely an unresolved double. If the distance estimate appears in brackets it is unreliable because the star is a possible white dwarf or subdwarf candidate. 42 8.1pc 11.9pc 6.9pc ± ± ± notes see Subasavage et al. (2005b) WD candidate at 40.5 Hipparcos distance at 100.70pc Hipparcos distance at 93.63pc Hipparcos distance at 47.46pc Hipparcos distance of 77.94pc WD candidate at 59.3 Hipparcos distance at 30.61pc WD candidate atHipparcos 34.5 distance at 46.46pc Hipparcos distance atHipparcos 56.31pc distance at 39.84pc b bc b de a b bc a b b a b c b a b b b a b b a b c bd a b c b d a bc be bc c bc b c a c bd ) θ ◦ )( 00 5.8 359.3 0.90 34.0 discussed in Henry et al. (2004) 10.4 16.3 138.0 115.4 316.2 59.6 ··· ··· ··· ··· Distance Separation ) (pc) ( ◦ )( 00 µ θ ········· ··············· ······························ SCR 1800-5112B 0.317 220.3 178.3 4.6 123.7 SCR 0927-6239C 0.197 309.0 SCR 1348-5536B 0.204SCR 0436-8233B 112.1 236.9 0.233 51.1 46.9 48.6 310.9 SCR 2155-7330B 108.9 0.459 338.7 202.0 31.5 364.2 133.5 Table 6.1. Common Proper Motion Systems ··· ··· ··· ··· Distance Secondary/Tertiary ) (pc) ( ◦ )( 00 µ θ ( Primary SCR 0454-8045ASCR 0611-7302ASCR 0.195 0630-7643A 0.188 14.2 0.483SCR 208.1 0757-7444ASCR 356.8 0853-7705ASCR 0.197 0921-7523A 43.0SCR 0.211 65.7 1117-7226A 50.9 0.291SCR 7.0 1229-5738A 306.7 0.188SCR 1246-5328A SCR 321.1 SCR 0454-8045B 0.197SCR 0611-7302B 1257-5554A 275.8 (99.4) 0.188SCR SCR 52.6 256.6 1800-5112A 0630-7643B 0.410 62.2SCR 0.191 1804-5541A SCR 29.0 0.190 0757-7444B 72.2 0.289SCR 290.1 1809-6154A SCR 92.7 0.222 0853-7705BSCR 13.5 211.4 226.5 1816-6615A SCR 0.218 0921-7523BSCR 45.3 NLTT 194.4 0.180 1902-7550A 26927 39.1 0.209 253.2 SCR 0.225 69.4 1229-5738B 56.5 0.303 48.0 207.1 (47.2) 0.286 SCR 1246-5328B 293.2 SCR 168.8 159.3 1257-5554B 316.3 [448.4] 0.189 SCR 158.5 1804-5541B 0.204 101.9 76.2 0.183 SCR 262.7 14.4 75.9 1809-6154B SCR 0.413 80.4 1816-6615B 273.7 25.3 0.198 293.3 109.8 46.1 LEHPM 10.4 1248-2 0.201 189.1 201.7 52.0 224.1 82.1 259.8 14.0 163.4 311.4 10.8 0.286 99.5 163.9 28.8 309.5 168.5 19.5 215.0 18.9 111.7 19.3 30.5 298.8 302.6 269.7 20.3 129.4 SCR 0745-4814A 0.200 174.9 31.4 SCR 0745-4814B 0.201 176.0 25.7 43.7 220.5 SCR 0017-5036ASCR 0025-5254A 0.204SCR 0055-5529A 0.196SCR 112.1 0156-6402A 0.234SCR 101.2 0156-6702A 0.197SCR (83.6) 0205-6122A 53.6 0.183SCR 0206-6609A 85.6 44.4 0.184SCR NLTT 0246-4935A 57.4 00918 0.181SCR 88.9 192.8 0353-6844A 0.247 140.4SCR SCR 0429-5423A 0025-5254B 80.6 0.232 29.7 [74.6] 72.3 SCR 0.188 0055-5529B SCR 0156-6402B 38.0 101.4 0.110 49.4 SCR SCR 0205-6122B 0156-6702B 40.0 107.1 0.212 0.217 53.2 SCR 0206-6609B 54.4 52.6 0.177 SCR 86.2 80.0 0246-4935B SCR 0353-6844B 0.220 47.4 SCR 0429-5423B 82.1 0.243 75.9 0.238 286.8 45.2 58.0 0.170 38.1 124.5 280.5 330.7 39.7 (31.4) 19.3 59.3 107.4 261.8 8.2 79.8 92.6 13.5 145.3 226.4 HD 158866NLTT 01733NLTT 03566NLTT 13852NLTT 15903 0.235 0.250NLTT 20147 0.257NLTT 188.4 21827 115.3 0.233 87.5 0.223NLTT (13.1) 26256 46.3 0.222 36.1NLTT 36394 17.9 0.231NLTT 342.8 SCR 45592 27.9 1746-8211B 312.1NLTT SCR 49033 0.194 0032-5528BNLTT 36.4 (40.4) 49299 0.238 SCRNLTT 283.9 0104-5742B 0.228 52323 53.9 0.174PPM 238.9 365916 0.221 SCR SCR 0843-5007B 184.9 0.270 0551-8116BSCR 178.9 (12.5) 0004-6120A 0.295 115.2 0.239 SCR (36.9) 159.1 0927-6239B 0.466 0.180 100.1 14.5 (23.3) SCR 0.225 91.1 0.259 0.233 1104-7856B 204.3 70.3 SCR 129.0 1411-7525B 28.8 338.8 0.204 135.1 (22.9) 19.5 SCR 1755-7241B [872.1] 0.203 312.2 35.8 (33.0) 76.5 0.250 SCR 74.1 SCR 2019-4701B 2029-5757B 283.1 349.6 56.5 0.199 242.1 110.6 41.6 SCR SCR 2237-6238B 0004-6120B 175.2 101.1 290.8 0.265 0.314 71.4 111.5 24.0 206.6 158.1 107.8 99.6 0.191 0.171 60.3 200.9 260.4 127.4 127.6 52.5 79.0 64.3 21.8 266.1 [1216.2] 92.0 102.2 167.7 69.6 275.5 111.7 67.9 179.6 273.7 118.8 102.8 205.5 86.9 107.6 HD 120056 0.164 230.1 43 9.7pc ± notes without I A atWD 81pc candidate and at B 48.7 at 128pc a b b b b c b b g h h b b b f b d ) θ ◦ )( 00 Distance Separation ) (pc) ( ◦ )( 00 µ θ ··············· Table 6.1 (cont’d) SCR 2057-6358C 0.130 138.7 46.7 261.5 121.6 Distance Secondary/Tertiary ) (pc) ( ◦ )( 00 µ θ ( Primary Companion not detected during automated search but noticed to be aWhite common dwarf proper candidate motion with companion unreliable during distance visual when inspection listed [in brackets] Distance estimate unreliable (in parentheses), because primary is likely an unresolved double Subdwarf candidate with unreliable distance listed [in brackets] Distance estimate unreliable when listed (in parentheses); if distance not given BRI plate photometry not available Fewer than 6 relations, therefore distance estimate unreliable (in parentheses); HipparcosNo distance 2MASS given photometry in available notes for when companion available I photometry suspect, therefore distance unreliable (in parentheses) a b c d e f g h SCR 2036-6454ASCR 2057-6358A 0.197 0.187SCR 146.0 2100-5804ASCR 139.9 2112-5428A 0.186SCR 2218-5310A 72.7 0.209SCR [102.0] 117.6 2241-6119A 0.190SCR 2255-5120A 95.3 0.184SCR SCR SCR 2333-7923A 2057-6358B 2036-6454B 95.3 80.5 0.335SCR 124.0 2335-6433A 0.394SCR 35.6 227.1 2353-8204A (61.1) 0.196 0.190 101.4 SCR 2100-5804B 23.2 0.216 103.1 153.3 SCR 69.7 SCR 2112-5428B [183.1] 2218-5310B 66.9 0.181 SCR (24.5) 2241-6119B 88.2 SCR SCR 2333-7923B 2255-5120B 116.1 0.152 0.191 (26.8) SCR 2335-6433B 117.0 0.162 95.9 147.0 0.388 SCR 0.263 2353-8204B 117.6 35.3 0.196 100.0 13.5 228.9 96.6 0.209 99.1 27.8 [216.2] 16.4 112.6 72.5 68.4 15.3 57.5 35.2 300.7 11.2 9.6 54.2 17.4 60.6 142.1 123.0 22.4 359.3 211.2 34.5 25.9 181.9 SCR 1912-4910ASCR 1917-4915A 0.229 0.216 187.7 200.3 35.8 48.2 SCR 1912-4910B LEHPM 3221-2 0.254 185.5 0.212 200.8 42.3 81.8 20.9 44.0 262.8 131.6 SCR 1953-5037ASCR 1958-8000A 0.181SCR 2032-4948A 0.183 144.3 0.265 149.1 179.0 31.6 (61.3) 75.3 SCR SCR 1953-5037B 1958-8000B SCR 2032-4948B 0.171 0.192 142.9 145.8 0.270 (133.4) 182.4 45.0 [900.1] 6.7 82.5 8.8 258.7 188.8 213.1 44

0.5

0.46

0.42 )

-1 0.38

0.34

0.3

0.26 CPM starCPM (arcsec yr 0.22 P

0.18

0.14

0.1 0.1 0.14 0.18 0.22 0.26 0.3 0.34 0.38 0.42 0.46 0.5 P SCR star (arcsec yr-1)

Figure. 6.3 Comparison of proper motions for components in multiple systems. Proper motions from the automated SCR search are denoted by ﬁlled circles and proper motions manually obtained through SuperCOSMOS are denoted by open circles. The solid line indicates perfect agreement between the two and the dashed lines represent conservative limits of 000.20 yr−1 based on our uncertanties. 45

360

330

300

270

240

210

180 CPM star CPM 150 T

120

0 0 30 60 90 120 150 180 210 240 270 300 330 360 T SCR star

Figure. 6.4 Comparison of position angles for components in multiple systems. Posi- tion angles from the automated SCR search are denoted by ﬁlled circles and position angles manually obtained through SuperCOSMOS are denoted by open circles. The solid line indicates perfect agreement between the two and the dashed lines represent conservative limits of 5.0 degrees based on our uncertainties. 46

6.4 Comments on Individual MINIMO Systems

SCR 0630-7643AB was discussed in Henry et al. (2004). It is a new nearby

00 (∼7 pc) binary with separation 1.0 and brightness diﬀerence of ∼0.25 mag at IC .

SCR 0838-5855 has R59F = 16.11 and R59F − J = 5.80. This is likely to be a late M dwarf at an estimated distance of only 8.4 pc. This is a high priority target on our CTIOPI parallax program (Jao et al. 2005; Henry et al. 2006). SCR 0927-6239BC are possible CPM companions to NLTT 21827. The B component has a separation of 20000.9 at position angle 92.0◦ from the primary. The C component is not in 2MASS and has a separation of 31600.2 at a position angle of 59.6◦ from the primary. See Table 6.1. SCR 1257-5554AB was discussed in Subasavage et al. (2005a) as a probable red dwarf/white dwarf pair.

SCR 1441-7338 has R59F = 16.14 and R59F − J = 4.95 with a distance estimate of 19.0 pc.

SCR 1826-6542 has R59F = 16.43 and R59F − J = 5.86. This is likely to be a late M dwarf at an estimated distance of only 9.2 pc. It is the reddest object found in the MINIMO search. SCR 1914-7109 is the brightest object found in the MINIMO search, with

R59F = 8.14 and R59F − J = −0.54. It is too blue for us to estimate a distance using the plate-2MASS relations. SCR 2057-6358ABC is a possible triple system with the A and B components separated by less than 200., and having blended SuperCOSMOS photometry, but which are separated in 2MASS. Both the B and C components were noticed by eye during the blinking process. The C component has a separation of 26100.5 at position angle 121.6◦ from the primary. See Table 6.1. 47 – 7 – Discussion

Including all papers pertaining to the SCR proper motion survey, we have discovered 1967 new systems (2030 objects) with µ ≥ 000.18 yr−1 between declinations −90◦ and 0◦. Systems reported in previous papers are represented by filled circles in the sky map of SCR systems in Figure 7.1; systems in this search are represented by open circles. The 1684 systems in this search comprise 86% of the entire SCR sample and bring the total number of systems south of −47◦ to 1761 (1817 objects). From this search, there are 17 likely white dwarfs and 191 subdwarf candidates. Six of the white dwarfs (but none of the subdwarfs) have been spectroscopically confirmed, while the rest remain to be targeted in future spectroscopic efforts to confirm their luminosity classes. Discovery statistics for the entire SCR sample, separated by distance horizons, are given in Table 7.1. In order to be consistent with previous SCR papers, new common proper motion candidates that are companions to known objects and probable white dwarfs (because their distance estimates require a different set of relations) are not included. For all proper motion bins except the last, we have searched the entire southern sky; for the last bin only −47◦ to −90◦ has been searched. In the complete sample of new SCR systems to date, 7 are estimated to be within 10 pc, and 67 additional systems lie between 10 and 25 pc. Of the 1684 systems reported in this search, three are estimated to be within 10 pc, with an additional 31 between 10 and 25 pc. This illustrates that even in this relatively slow proper motion regime there are nearby stars hidden in the solar neighborhood. Should they prove to be within 10 48 pc, the three nearest stars reported in this search would rank as the 10th (000.311 yr−1 SCR 1826-6542), 11th (000.320 yr−1 for SCR 0838-5855), and 33rd (000.483 yr−1 SCR 0630-7643AB) slowest systems in the RECONS sample of 248 systems within 10 pc

(Henry et al. 2006). Plotted in Figure 7.2 is a histogram showing the number of new proper motion discoveries found in 000.01 yr−1 bins for the entire MINIMO sample (light shade). From this we can see that if the SCR survey were to look at slower proper motions, a substantial number of new discoveries objects could be found. While no turnover is seen here, at some point I suspect that the SCR search would have difficulty measuring stars with very low proper motions because of errors in the proper motion calculations and insufficient epoch spread from plate to plate. I also look at the number of new discoveries within each 000.01 yr−1 bin that have an estimated distance within 50 pc denoted by the darker shade in Figure 7.2. From this we see that the number of objects found within 50 pc gets greater toward the slower proper motion realm where a larger number of objects have been found. The greatest percent of objects (objects within 50 pc / total objects in bin) out of each bin having distance estimates within 50 pc come from proper motions which are greater than 000.29 yr−1. Although the counts of new 10 pc candidates are small in each of the SCR proper motion samples, the largest number of candidates between 10 and 25 pc is found in the slowest sample from this MINIMO survey, even though only a portion of the southern sky has been searched. I anticipate that continuing searches for MINIMO systems in the southern sky will be a promising endeavor for finding additional nearby stars. 49

0 Dec (Degrees) -30

-60

-90 24 18 12 6 0 RA (Hours)

Figure. 7.1 Sky distribution of SCR systems with µ ≥ 000.18 yr−1. Open circles denote SCR discoveries from this search and small ﬁlled circles indicate SCR discoveries from past papers. The curve represents the Galactic plane. 50

Table 7.1. Distance Estimate Statistics for SCR Systemsa

Proper motion d ≤ 10 pc 10 pc < d ≤ 25 pc d > 25 pc µ ≥ 100.00 yr−1 2 + 0 0 + 0 6 + 0 100.00 yr−1 > µ ≥ 000.80 yr−1 0 + 0 3 + 0 3 + 0 000.80 yr−1 > µ ≥ 000.60 yr−1 1 + 0 11 + 0 48 + 0 000.60 yr−1 > µ ≥ 000.40 yr−1 1 + 1 22 + 2 113 + 71 000.40 yr−1 > µ ≥ 000.18 yr−1 0 + 2 0 + 29 0 + 1545 Total 4 + 3 36 + 31 170 + 1617

aEntire SCR sample excluding white dwarf candidates and new common proper motion companions noticed by eye; the ﬁrst number is from previous SCR eﬀorts and the second number is from this search 51

325

300

275

250

225

200

175

150

# pm objects pm # 125

100

0.2 0.3 0.4 0.5 0.18 0.19 0.21 0.22 0.23 0.24 0.25 0.26 0.27 0.28 0.29 0.31 0.32 0.33 0.34 0.35 0.36 0.37 0.38 0.39 0.41 0.42 0.43 0.44 0.45 0.46 0.47 0.48 0.49 proper motion (arcsec yr-1)

Figure. 7.2 Histogram showing the number of new proper motion discoveries in 000.01 yr−1 bins for the entire MINIMO sample (light shade) and the number of those objects having distance estimates within 50 pc (dark shade). 52 – 7 – References

Barnard, E. E. 1916, AJ, 29, 181

Bessel, M. S. 1990, A&AS, 83, 357

Bossert, J., & Schulhof, L. 1919, Annales de l’Observatoire de Paris, 29, A1 Campbell, W. W. 1913, New Haven, Yale university press; [etc., etc.] 1913.,

C., G. C. 1906, Science, 24, 270 Dawson, P. C., & De Robertis, M. M. 2004, AJ, 127, 2909 Deacon, N. R., Hambly, N. C., & Cooke, J. A. 2005, A&A, 435, 363 Gatewood, G., & Eichhorn, H. 1973, AJ, 78, 769

Giclas, H. L. 1958, Lowell Observatory Bulletin, 4, 1 Giclas, H. L., Burnham, R., & Thomas, N. G. 1971, Flagstaﬀ, Arizona: Lowell Ob- servatory, 1971 Giclas, H. L., Burnham, R., & Thomas, N. G. 1978, Lowell Observatory Bulletin, 8, 89

Gizis, J. E. 1997, AJ, 113, 806

Graham, J. A. 1982, PASP, 94, 244 Hambly, N. C., Davenhall, A. C., Irwin, M. J., & MacGillivray, H. T. 2001c, MNRAS, 326, 1315

Hambly, N. C., Henry, T. J., Subasavage, J. P., Brown, M. A., & Jao, W. 2004, AJ, 128, 437 Hambly, N. C., Irwin, M. J., & MacGillivray, H. T. 2001b, MNRAS, 326, 1295 Henry, T. J., Franz, O. G., Wasserman, L. H., Benedict, G. F., Shelus, P. J., Ianna,

P. A., Kirkpatrick, J. D., & McCarthy, D. W., Jr. 1999, ApJ, 512, 864 53

Henry, T. J., & McCarthy, D. W., Jr. 1993, AJ, 106, 773 Henry, T. J., Jao, W.-C., Subasavage, J. P., Beaulieu, T. D., Ianna, P. A., Costa, E., & M´endez,R. A. 2006, AJ, 132, 2360 (Paper XVII)

Henry, T. J., Subasavage, J. P., Brown, M. A., Beaulieu, T. D., Jao, W.-C., & Hambly, N. C. 2004, AJ, 128, 2460 (Paper X) Henry, T. J., Walkowicz, L. M., Barto, T. C., & Golimowski, D. A. 2002, AJ, 123, 2002

Hershey, J. L. 1973, AJ, 78, 421 Humphreys, R. M., Cornuelle, C., Larsen, J., Aldering, G., & Cabanela, J. 1997, ASP

Conf. Ser. 127: Proper Motions and Galactic Astronomy, 127, 41

Jao, W.-C. 2004, Ph.D. Thesis

Jao, W.-C., Henry, T. J., Subasavage, J. P., Bean, J. L., Costa, E., Ianna, P. A., & M´endez,R. A. 2003, AJ, 125, 332

Jao, W.-C., Henry, T. J., Subasavage, J. P., Brown, M. A., Ianna, P. A., Bartlett, J. L., Costa, E., & M´endez,R. A. 2005, AJ, 129, 1954 Jones, B. 1997, Memorie della Societa Astronomica Italiana, 68, 833 Kirkpatrick, J. D., Henry, T. J., & McCarthy, D. W., Jr. 1991, ApJS, 77, 417

Krawchuk, C. A. P., Dawson, P. C., & De Robertis, M. M. 2000, AJ, 119, 1956 Kruesi, Liz 2006, Astronomy, Online extras Landolt, A. U. 1992, AJ, 104, 340

L´epine,S., & Shara, M. M. 2005, AJ, 129, 1483

L´epine,S. 2005, AJ, 130, 1247

Luyten, W. J. 1938, Minneapolis, University of Minnesota Press, 1938-60., Luyten, W. J. 1955, Luyten’s Five Tenths. (1955), 0

Luyten, W. J. 1979, LHS Catalogue (Minneapolis: Univ. of Minnesota Press) 54

Luyten, W. J. 1980, Proper Motion Survey with the 48-inch Telescope, Univ. Min- nesota, 55, 1 (1980), 55, 1 Luyten, W. J. 1995, VizieR Online Data Catalog, 1098, 0 van Maanen, A. 1915, ApJ, 41, 187

Oppenheimer, B. R., Hambly, N. C., Digby, A. P., Hodgkin, S. T., & Saumon, D. 2001, Science, 292, 698

Paulson, D. B., Allred, J. C., Anderson, R. B., Hawley, S. L., Cochran, W. D., & Yelda, S. 2006, PASP, 118, 227 Pokorny, R. S., Jones, H. R. A., & Hambly, N. C. 2003, A&A, 397, 575 Pokorny, R. S., Jones, H. R. A., Hambly, N. C., & Pinﬁeld, D. J. 2004, A&A, 421, 763

Porter, J. 1892, Publications of the Cincinnati Observatory, 12, 1

Porter, J. G. 1892, AJ, 12, 25 Ross, F. E. 1925, AJ, 36, 96 Ruiz, M. T., Takamiya, M. Y., Mendez, R., Maza, J., & Wishnjewsky, M. 1993, AJ, 106, 2575 Ruiz, M. T., Wischnjewsky, M., Rojo, P. M., & Gonzalez, L. E. 2001, ApJS, 133, 119

Schaefer, B. E., King, J. R., & Deliyannis, C. P. 2000, ApJ, 529, 1026 Scholz, R.-D., Irwin, M., Ibata, R., Jahreiß, H., & Malkov, O. Y. 2000, A&A, 353, 958

Scholz, R.-D., Szokoly, G. P., Andersen, M., Ibata, R., & Irwin, M. J. 2002, ApJ, 565, 539

Smith, G., Lambert, D. L., & Ruck, M. J. 1992, A&A, 263, 249 Subasavage, J. P., Henry, T. J., Hambly, N. C., Brown, M. A., & Jao, W. C. 2005, AJ, 129, 413 (Paper XII) 55

Subasavage, J. P., Henry, T. J., Hambly, N. C., Brown, M. A., Jao, W. C., & Finch, C. T. 2005, AJ, 130, 1658 (Paper XV) van de Kamp, P. 1969, AJ, 74, 238

Wolf, M. 1919, Veroeﬀentlichungen der Badischen Sternwarte zu Heidelberg, 7, 195

Wroblewski, H., & Torres, C. 1989, A&AS, 78, 231 Wroblewski, H., & Torres, C. 1991, A&AS, 91, 129

Wroblewski, H., & Torres, C. 1994, A&AS, 105, 179 Zacharias, N., Monet, D. G., Levine, S. E., Urban, S. E., Gaume, R., & Wycoff, G. L. 2004, Bulletin of the American Astronomical Society, 36, 1418 Zacharias, N., Urban, S. E., Zacharias, M. I., Wycoff, G. L., Hall, D. M., Monet, D. G., & Rafferty, T. J. 2004, AJ, 127, 3043 56

Appendix 57 a b c a d d d b d ··· (pc) Est Dist Notes 18 . 00 J 0 − ≥ F 59 R > µ 1 s − 50 yr . 00 JHK ◦ 47 IVN I ≤ − F < δ 59 R ◦ 90 J − from ) ◦ 1 − yr )( 00 µ θ B (J2000) (J2000) ( Table Appendix. Characteristics of New SCR Systems with 0 Name RA DEC SCR 0004-6120ASCR 0005-4707SCR 00 0005-5747 04 56.20SCR 0005-6152 00SCR 05 0006-6009 -61 10.27 00 20SCR 05 58.0 0006-7740 43.09 00SCR -47 05 0007-7015 07 31.98 0.180SCR 00 34.6 -57 0008-8731 06 47 49.72SCR 00 30.5 0008-4916 06 -61 129.0 24.03 0.210 52 00SCR 48.7 07 0008-5843 -60 07.43 0.239 09 00SCR 13.63 35.2 08 -77 087.9 0009-6021 42.35 40 00 0.283SCR 59.2 08 -70 150.8 0009-6257 20.84 15 0.184 11.28 00 16.02 53.6SCR -87 08 161.1 0009-7305 31 15.37 0.221 00 17.74 00.0SCR -49 09 096.2 0011-7558 16 14.87 34.26 0.210 00 00.6 18.40SCR 9.94 09 -58 128.3 0011-5823 15.61 43.82 0.183 43 00SCR 31.7 14.81 -60 185.5 09 0012-5753 14.24 0.270 21 16.25 48.15SCR 00 17.66 29.4 -62 107.2 0013-5218 13.27 11 9.66 57 0.224 12.72 17.84SCR 00 15.52 27.1 11.51 103.1 0014-8000 11 -73 15.16 15.39 51.90 0.200 05SCR 00 17.44 11.97 37.5 0014-6205 12 123.7 -75 11.61 9.08 13.49 06.97 0.225 10.90SCR 58 00 17.92 0015-6957 14.36 01.7 13 -58 084.1 14.19 15.52 12.32 11.49SCR 23 00 0.276 16.40 0015-7638 45.7 14 11.17 -57 101.8 10.64 12.53 15.93 21.15SCR 53 00 13.70 0.184 8.81 17.25 0016-5911 38.8 14 13.17 -52 11.25 13.84 117.6 44.15SCR 18 00 14.54 0.220 10.55 18.22 0016-5220 11.0 15 11.72 -80 13.87 52.50 13.69 097.4SCR 00 00 14.97 0.221 12.63 0016-5938 10.1 15 12.74 18.10 -62 55.92 089.7 13.45 10.36SCR 05 00 16.09 0.203 11.11 0017-5448 56.7 16 12.74 -69 15.93 19.32 166.9 12.43SCR 57 00 12.68 0.183 12.11 0017-5036A 16.04 20.5 16 -76 17.63 3.36 12.91 04.62 114.6 10.95SCR 38 00 14.09 0.240 1.62 12.15 0017-5350 40.3 16 13.73 -59 17.45 3.64 11.69 30.07 147.6 11.87SCR 11 00 00 0.302 15.31 0018-6122 09.6 12.33 17 15.42 17 -52 12.17 12.78 45.04 1.89 103.6 59.74 11.92 20 0.183SCR 11.67 01.5 15.20 11.18 0018-6851 -59 16.08 108.5 1.55 14.58 38 00 0.214 12.15 12.95 42.0 17 10.69 12.20 -54 12.15 40.2 -50 31.97 138.2 2.22 48 00 11.55 36 0.197 35.8 10.90 12.51 11.5 18 14.02 39.1 [324.9] 14.58 53.2 14.04 23.87 073.8 1.77 11.82 0.180 00 11.94 11.03 10.24 -53 17.31 18 10.93 105.6 2.78 50 08.56 11.42 0.194 0.204 11.87 31.5 12.54 13.87 -61 17.23 11.24 098.0 3.19 76.5 22 158.3 03.3 15.23 10.52 18.29 9.83 -68 10.83 212.8 8.79 112.1 11.15 0.253 1.64 51 10.91 15.10 10.95 19.4 12.61 96.1 0.194 3.28 13.68 101.2 16.28 10.56 14.56 14.42 10.59 190.9 9.32 3.32 9.03 13.33 0.220 10.51 9.89 [167.0] 082.1 87.4 12.74 14.26 13.02 1.46 12.38 10.37 17.27 12.34 091.6 10.05 9.20 2.18 19.29 8.42 12.19 9.24 13.15 51.4 12.27 10.59 14.95 3.60 11.76 16.55 [380.3] 79.9 16.44 3.78 12.02 9.88 12.59 8.18 12.15 12.22 12.68 9.01 11.52 16.47 15.10 2.87 12.35 65.9 11.57 11.58 9.30 11.45 0.86 16.48 45.5 13.86 11.51 35.7 11.36 10.86 16.63 9.23 2.50 13.28 1.21 2.65 2.76 10.58 50.2 16.14 26.6 3.13 12.98 17.19 123.1 0.88 0.16 27.9 0.63 28.0 85.3 109.9 3.50 2.58 133.4 -0.16 83.6 45.5 a 38.4 151.7 SCR 0000-5029SCR 0001-7015SCR 0003-6021SCR 00 0004-5740 00 44.10SCR 00 0004-6709 01 56.59 00SCR 03 0004-6120B -50 59.01 29 00 24.8 04 -70 26.79 15 00 00 08.4 04 -60 04 35.59 21 0.402 45.41 58.1 -57 40 0.202 02.7 -67 091.8 -61 09 0.249 23 37.9 40.0 141.1 0.181 15.55 145.1 0.188 0.171 18.22 091.2 13.43 17.84 091.6 127.6 16.20 16.00 11.65 15.68 18.54 16.87 14.64 13.87 11.21 12.92 16.35 16.76 13.36 12.36 10.72 11.68 14.21 16.54 12.79 11.47 10.48 11.08 12.62 16.44 12.66 10.87 10.75 12.00 15.94 10.65 11.74 16.48 2.22 2.84 4.00 2.41 3.73 68.2 0.33 142.5 35.3 [1216.2] 66.0 58.4 SCR 0020-7412SCR 0021-6152SCR 0022-6047 00SCR 20 0022-5843 49.53 00SCR 21 0022-5251 27.98 00SCR 22 -74 0023-6641 48.33 12 00SCR 39.1 -61 22 0023-5606 52 41.01SCR 00 34.0 -60 0023-5926 22 47 16.15 0.236 00 09.7 23 -58 07.28 0.196 43 00 10.4 23 -52 093.5 53.91 0.218 51 00 31.4 23 -66 091.1 08.45 41 0.265 17.82 07.9 -56 100.5 06 0.197 17.84 17.4 -59 155.9 26 15.74 0.310 13.13 21.4 214.1 15.73 0.183 17.72 094.5 13.67 11.79 0.214 13.43 099.6 13.69 16.04 17.56 12.78 108.9 11.00 11.54 17.13 12.10 15.28 15.52 12.25 13.92 10.34 10.78 15.00 11.46 14.31 12.01 13.65 12.25 10.32 9.81 11.19 13.13 13.75 12.09 11.59 12.00 9.78 13.58 9.68 11.50 10.77 11.37 2.97 11.26 9.59 10.14 3.63 11.17 10.05 1.72 1.45 101.9 47.8 3.42 1.22 [301.6] 3.00 54.9 1.48 55.7 55.3 64.4 59.4 58 d d a a c d d a d d d (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 0024-8029SCR 0025-5254ASCR 0025-6049 00SCR 00 24 0025-5254B 25 41.50 55.49SCR 0026-4807SCR 00 00 0027-6422 25 -80 25 -52 32.66 29SCR 40.00 54 51.5 0028-6322 00.2SCR 00 0028-7029 26 -60 -52 26.71SCR 49 00 0.194 49 0.196 0029-5339 49.8 27 50.0 40.98SCR 00 0030-6329 28 -48 105.1 59.36SCR 101.2 07 00 0.292 0.110 0031-7926 36.3 28 -64 50.64 22 00SCR 20.1 29 18.58 0031-6308 -63 11.82 50.79 099.5 22 107.1 00 0.184 08.6 30SCR -70 19.98 0032-6112 29 00 0.187 15.84 36.1 31 10.51SCR -53 16.55 18.46 10.83 085.9 0032-5541 39 0.190 00 55.7SCR -63 31 082.4 0032-5528B 29 48.08 0.193 15.09 10.06 03.8 14.47 00SCR 15.59 -79 15.58 177.3 32 0033-5958 26 0.180 09.86 45.6SCR 00 18.47 00 -63 215.5 0033-6025 13.98 32 0.226 32 08 12.72 13.67 02.12 13.91 41.10 50.6 14.40 9.86SCR 145.6 -61 0.185 0033-4739 16.48 12 00 17.02 13.43SCR 060.5 21.0 33 11.56 -55 12.69 0033-6317 -55 12.54 0.198 13.21 08.74 41 00 14.70 28SCR 074.7 49.1 33 9.44 51.3 0035-6215 15.07 14.82 08.39 13.17 18.17 0.296 10.94 00SCR 12.06 11.69 181.7 -59 33 0036-5822 12.60 12.69 58 10.98 12.51 0.188SCR 0.221 00 18.5 13.84 -60 0037-4900 12.87 33 190.8 16.00 9.34 10.73 25 11.87 02.32 11.05 16.53SCR 00 38.2 11.87 0038-5012 11.53 35 -47 109.5 115.2 06.63 0.248 13.29 39SCR 00 9.59 11.53 17.25 34.4 0039-5521 14.33 36 -63 10.87 14.89 55.56 0.211 11.32SCR 17 00 10.96 18.05 0039-5347 50.1 37 17.58 1.86 -62 103.8 13.05 15.14 10.96SCR 15 00 15.26 0.281 13.09 0042-5916 53.8 38 -58 070.5 14.09 11.27 8.60 51.82 10.29SCR 22 00 15.80 0.341 15.48 17.58 0044-6546 03.8 39 0.65 -49 2.91 10.67 2.90 111.6 11.25 12.55 14.51SCR 00 00 0.303 [230.6] 16.70 0045-6314 13.43 27.9 39 -50 10.15 09.72 072.9SCR 12 8.62 00 13.84 15.55 13.32 0.301 0047-6513 10.0 42 17.76 -55 1.97 12.27 13.55 52.25 126.6 21 00 12.88 14.67 0.181SCR 26.7 44 0047-4905 -53 15.68 2.64 12.68 21.76 12.27 057.8 47 00 13.70 0.204SCR 15.82 8.06 25.1 12.96 45 44.4 -59 16.66 1.34 55.2 0048-5343 80.0 08.08 12.77 247.1 16 00 12.95 0.209SCR 58.8 47 13.79 12.12 -65 11.72 17.55 3.29 0048-5807 12.10 57.85 111.0 46 0.193 12.85 00 15.18SCR 27.4 14.80 -63 17.61 1.73 87.7 47 0048-6110 7.91 11.93 103.4 14 185.1 35.04 0.193 11.88SCR 00 11.93 11.47 44.9 15.40 11.63 -65 15.57 2.91 0049-6034 48 097.9 14.20 13 109.8 59.33 0.217SCR 00 12.81 25.5 15.52 11.31 13.42 0049-5150 48 -49 222.4 10.41 48.05 0.183 05 11.35SCR 00 13.50 13.81 48.7 18.46 43.9 0049-5045 13.62 48 1.46 -53 063.6 11.51 12.61 0.196 11.07 43 00 13.66 11.50SCR 15.00 66.9 27.5 49 0049-4831 -58 129.1 111.1 12.20 17.39 1.71 07 00 13.17 0.259 9.80 16.41 13.45SCR 16.02 34.5 0.97 49 10.96 -61 103.8 0050-4734 12.36 47.60 3.12 10 00 10.33 3.21 12.83 0.279SCR [227.8] 15.79 30.6 49 11.59 -60 0050-6349 12.36 100.0 02.62 34 14.42 14.42 0.328 00 10.71SCR 16.29 03.7 9.57 11.85 [234.5] -51 49 0051-6510 085.4 3.45 50 11.64 07.74 14.77 0.392 11.35SCR 00 9.88 02.3 11.77 15.59 -50 0051-6027 50 13.25 122.1 2.75 45 13.10 14.31 16.14 0.210 11.59SCR 00 15.0 26.2 16.50 0052-6155 50 10.91 -48 134.2 84.1 14.23 70.3 41.61 0.184 1.62 31 11.64SCR 00 13.83 12.72 53.7 17.80 0052-4834 51 9.25 12.13 -47 087.3 12.49 14.74 0.262 34 00 14.40 10.34 15.94 28.5 51 13.93 -63 077.3 59.6 42.16 3.29 13.28 12.48 49 00 0.201 15.66 3.38 11.58 18.58 55.4 52 11.48 [291.7] -65 203.3 70.2 9.06 09.93 3.20 10.11 10 00 13.00 13.65 0.232 13.46 17.91 12.2 52 -60 12.82 177.9 23.90 3.16 11.42 27 13.77 16.41 0.200 10.88 17.54 10.8 -61 12.17 113.7 1.45 13.46 55 11.72 15.81 0.286 22.8 12.23 17.63 -48 12.53 194.1 10.68 49.1 34 14.66 15.30 0.194 26.9 31.5 11.58 17.24 10.50 044.2 3.16 63.2 13.93 0.220 12.15 15.74 11.98 16.33 13.23 1.62 130.1 1.92 75.1 13.55 0.187 11.38 125.2 15.11 16.84 12.67 086.9 2.29 9.99 14.96 11.71 14.30 12.66 13.90 12.57 066.3 0.84 12.84 114.2 14.74 12.10 14.82 2.83 14.16 12.40 12.58 10.94 9.72 12.04 18.32 41.5 61.4 11.83 1.01 11.85 12.94 108.9 12.63 13.55 11.48 2.23 11.81 293.0 16.27 11.28 9.84 11.91 3.13 10.86 13.45 10.91 [153.3] 58.0 14.49 11.03 11.31 3.18 9.53 3.15 10.70 9.98 13.38 3.14 99.7 11.06 2.73 78.6 8.87 12.84 9.35 1.58 103.2 30.6 3.28 12.63 8.65 83.6 9.12 2.82 [305.2] 97.7 2.84 55.6 2.89 58.0 1.41 2.65 66.7 137.6 31.9 28.8 SCR 0024-7644 00 24 25.41 -76 44 31.1 0.201 067.3 17.76 15.80 15.04 14.39 13.79 13.63 1.41 [343.7] 59 d d a c a d d a b d d d (pc) Est Dist Notes J ······ − F 59 R s JHK 14.65 14.07 13.86 IVN I F 59 ······ R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 0055-6645SCR 0055-5057SCR 0055-5529B 00SCR 55 0055-4957 30.11SCR 00 00 0055-5529A 55 55 06.13SCR 10.46 0055-6014 -66 45SCR 00 00 05.1 0056-6106 55 55 -50 -55 28.12 10.49SCR 57 29 0056-5326 02.0 35.0SCR 00 0.312 0058-4721 55 -49 -55 53.67SCR 57 00 29 0.279 0.212 0058-6545 34.3 56 41.1 120.6 06.06 00SCR 56 0058-5137 -60 43.28 286.0 14 00 0.380 0.234SCR 52.6 57.2 58 18.34 -61 0059-6531 23.33 06 00SCR 02.1 58 -53 17.11 0059-4731 38.75 104.2 053.6 26 0.210 00SCR 16.30 21.02 19.1 -47 58 0059-5253 21 18.26 0.186SCR 00 18.5 14.82 -65 18.10 0100-7904 17.64 59 076.8 45 12.14 0.377 15.15SCR 00 49.5 0100-6503 59 -51 239.4 56.63 0.209 37SCR 00 12.64 15.69 15.17 54.8 18.04 0101-5852 59 -65 077.6 14.10 00.29 0.213 31 01SCR 16.73 34.3 00 0104-4809 -47 140.4 11.94 56.08 31 01 13.09 0.334 14.07 16.01SCR 17.38 36.2 13.51 00 -52 065.7 0104-5249 05.69 53 01 14.55 0.204 14.39 34.6 01SCR 11.43 -79 11.90 179.5 12.56 13.97 0104-5742B 04 14.13 15.32 0.216 13.35 01 16.61 25.2SCR -65 04 190.2 0104-8152 03 12.47 12.06 12.53 0.368 11.19 01 52.6 11.37 17.23SCR 11.93 -58 01 04 12.66 045.8 0105-6646 52 14.08 04 14.72 53.60 0.379 24.7 12.14SCR 17.69 11.22 -48 093.1 0107-4950 11.81 0.183 09 10.99 11.71 15.30 12.11SCR 09.5 01 16.28 12.94 -52 215.3 0107-5837 13.34 04 0.236 -57 49 15.55 06.31 10.66 01 16.93 42 29.5 11.61SCR 200.6 05 48.6 2.20 0107-4825 14.25 11.82 0.246 13.98 11.84 12.41 01 13.70 12.28SCR 184.2 07 -81 2.88 10.42 0109-4707 14.29 15.08 33.94 0.229 11.08 52 01 18.12 0.239SCR 13.49 52.6 07 142.0 -66 12.23 0110-4911 12.31 11.70 22.38 11.69 46 15.34 01SCR [250.9] 20.4 13.26 -49 070.9 3.78 10.91 07 0110-4957 2.61 13.20 16.05 091.1 50 40.60 12.90 0.208 16.72 01 34.7 11.83SCR -58 11.42 09 13.70 0111-5713 37 22.75 0.182 12.66 01 16.35 9.98 49.4 11.95SCR 3.35 70.9 16.20 14.56 10 -48 12.68 013.0 0112-4826 14.65 08.88 0.201 11.26 25 01SCR 51.3 3.33 12.95 10 -47 095.4 12.47 0112-7939 13.97 27.33 0.222 11.44 07 13.39 15.90 01SCR 15.40 2.39 41.8 8.80 50.8 88.9 -49 083.4 13.29 11.04 11 0112-7805 11 14.00 0.222 12.72SCR 01 15.74 0.92 18.8 -49 084.9 11.16 0112-4905 12.51 12 12.97 57 15.79 14.08 09.53 0.269SCR 01 18.18 2.44 75.8 13.06 35.7 0112-4956 12 8.17 -57 171.0 12.19 13.33 23.47 0.191 13SCR 01 16.58 39.6 11.27 1.81 30.4 12.67 0113-4810 140.8 12 15.67 -48 185.8 13.45 12.49 16.20 14.72 0.184SCR 26 01 17.07 2.30 12.08 0114-5138 11.0 104.8 12 -79 196.8 11.41 7.88 14.54 56.80 10.66SCR 39 01 0.180 15.57 16.67 2.15 0116-4951 13.1 12 12.52 12.40 -78 147.7 14.31 24.91SCR [212.5] 05 01 95.7 15.25 0.181 18.24 3.12 0117-5054 28.6 13 11.05 -49 10.42 12.73 093.7 42.08SCR 15.76 05 01 14.44 0.323 12.02 16.60 0118-6006 28.8 14 13.27 -49 158.2 16.26 132.5 14.64SCR 56 01 16.08 0.224 10.39 2.66 0118-5958 35.1 16 12.03 17.05 -48 26.56 066.3 11.87SCR 10 01 12.69 14.59 0.202 12.69 0.98 86.1 0119-6842 22.7 17 -51 16.27 14.08 2.90 00.25 046.0 10.14 38 01 13.74 0.253SCR 11.42 65.6 15.33 17.4 18 1.59 0122-5752 -49 17.16 12.01 04.52 066.4 12.40 51 01 12.50 0.299SCR 12.7 13.55 18 14.03 -50 17.23 2.69 0122-5734 157.3 12.41 00.45 122.8 11.17 0.23 54 01 0.299 14.59 02.4 19 15.14 11.49 -60 18.19 172.8 11.72 44.46 163.6 06 0.206 13.40 01 [194.4] 12.29 00.5 15.41 11.80 -59 16.28 22 14.9 078.3 1.56 13.55 58 14.76 0.187 11.26 01 12.89 49.6 16.07 11.18 -68 18.23 [872.1] 22 080.3 2.28 42 11.32 36.73 0.228 11.50 13.80 45.6 13.91 17.53 48.8 12.92 -57 069.2 2.94 11.18 0.207 52 10.94 13.87 16.08 12.6 17.41 10.68 -57 074.8 2.51 12.26 0.215 34 12.29 135.9 15.21 12.71 16.08 29.4 10.62 117.0 12.77 1.17 14.38 0.204 15.18 10.44 17.05 11.68 101.1 51.8 11.75 2.43 13.36 121.3 13.72 0.207 10.34 12.04 12.18 13.54 121.8 3.67 13.52 14.99 11.47 18.25 11.26 [292.6] 82.2 12.21 063.7 2.87 11.47 11.64 11.94 12.99 18.00 12.55 13.32 15.70 1.78 11.02 11.67 18.60 10.89 87.3 11.32 2.71 12.79 16.10 12.00 12.63 55.1 13.20 3.96 11.39 16.45 10.27 11.03 [193.6] 65.9 3.14 15.35 11.77 12.06 11.77 3.31 14.19 10.58 9.99 14.72 2.16 11.88 50.7 11.24 12.96 2.54 10.53 29.3 14.23 2.99 10.91 73.4 12.44 2.64 82.2 14.00 85.1 12.13 169.8 2.83 2.35 0.62 69.6 3.93 99.8 1.39 122.9 39.8 3.48 75.8 [413.2] 36.2 83.1 SCR 0054-6107 00 54 48.19 -61 07 45.9 0.200 160.5 16.63 15.29 14.70 14.04 13.55 13.38 1.25 [284.6] 60 d d d d d d ··· (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 15.36 14.56 13.91 13.44 13.21 1.45 [279.1] R J ··· ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 0128-7614SCR 0128-4858 01SCR 28 0128-6100 28.50SCR 01 0128-7104 28 31.75 01SCR -76 28 0129-6928 14 11.34 01 32.0SCR 28 -48 0129-5940 50.62 58 01 37.7 -61 29SCR 0.220 00 15.93 0130-6239 41.9 01 -71SCR 29 04 0.251 0130-6020 13.01 52.6 067.6SCR -69 01 0.229 0131-5011 28 30 17.1 31.21SCR 109.5 01 -59 0.452 0131-6804 17.38 30 40 56.47SCR 062.0 26.4 01 0132-5824 31 0.236 -62 17.79 01.67SCR 39 088.8 01 15.26 0132-5941 01.0 31 -60 13.05 0.361 01.07SCR 20 01 078.6 0133-7200 57.4 32 15.80 -50 17.59 36.49SCR 11 01 0.185 14.08 0133-6513 01.0 32 105.8 11.89 -68 03.23SCR 17.93 04 01 0.306 0134-8033 15.15 33.8 33 15.44 -58 098.7 12.99 13.18SCR 24 01 0.197 0135-6127 52.9 11.38 33 -59 15.77 27.80SCR 129.0 41 01 14.15 0.204 0135-5943 53.2 13.23 34 17.19 -72 12.56 50.58 116.4 00 01SCR 0.259 11.25 04.1 35 0135-8323 -65 17.22 14.85 13.58 53.66 165.1 13 01 0.235 12.63SCR 12.42 14.94 59.6 35 0136-7607 -80 16.74 46.69 118.2 10.71 33 0.433SCR 01 14.00 36.1 15.14 13.42 0136-7115 -61 18.54 35 148.5 12.12 27 45.42 0.326SCR 13.66 01 11.1 14.76 0137-8240 -59 15.50 10.65 36 172.2 43 13.52 09.43 0.210SCR 01 12.61 14.5 16.35 0137-7428 16.82 11.88 36 -83 064.7 13.24 38.23 0.255SCR 23 01 12.69 13.35 0138-6638 53.6 16.91 37 13.34 -76 065.3 11.66 46.90 0.412SCR 07 01 14.69 2.08 14.84 0138-7855 17.17 11.2 12.70 37 -71 256.8 11.38 22.18SCR 15 01 11.41 0.201 14.63 1.65 0138-5353 16.78 36.1 38 11.05 -82 081.5 13.49 44.04SCR 40 01 12.83 14.99 0.208 12.49 0139-7536 15.62 0.64 11.3 38 10.81 -74 10.55 083.5 53.97SCR 28 01 12.16 14.79 0.184 10.81 0139-6013 17.35 2.81 43.8 169.2 38 12.96 -66 12.05 20.51SCR 053.6 [291.7] 38 01 12.86 13.67 0.186 10.53 0140-6852 08.7 39 10.01 18.24 1.77 -78 11.36 27.90SCR 131.1 55 01 13.07 15.24 0.217 12.72 0140-5906 18.1 39 11.52 -53 15.70 12.27 59.94SCR 066.1 53 01 11.81 0.182 0140-6812 81.8 16.15 26.1 40 10.78 -75 18.62 103.3 11.65 19.51 9.74SCR 086.4 36 01 13.00 0.202 1.70 11.26 [290.5] 0140-7929 14.0 40 13.96 11.80 -60 18.17 10.06 43.93 225.6 13 01 0.297 3.48 15.43 10.49 52.5 40 16.45 11.11 -68 14.60 12.01 35.24 075.4 52 01 0.279 3.38 11.50 12.29 01.4 40 16.19 -59 18.30 32.83 [196.3] 071.0 14.09 06 9.53 0.202 2.86 10.84 14.24 12.4 13.50 11.51 -68 14.87 060.3 12 11.36 0.255 14.37 57.6 16.12 -79 15.70 13.51 2.81 047.4 29 13.20 0.228 2.79 11.24 46.7 13.11 55.3 12.78 9.24 14.67 10.74 087.5 12.70 0.340 3.27 42.1 14.37 13.70 13.26 18.12 139.9 12.63 055.3 12.72 0.183 2.72 11.20 12.79 10.50 18.09 12.14 155.2 13.57 3.14 11.74 16.11 12.36 17.01 12.35 37.5 061.3 79.4 10.92 15.89 11.84 18.89 9.92 13.00 10.28 3.23 42.9 14.40 14.94 3.62 12.34 17.39 89.3 14.06 16.50 2.06 12.81 9.87 9.35 12.67 53.4 13.79 9.69 15.35 2.60 13.16 14.85 3.25 12.16 9.24 12.16 [246.3] 63.7 13.25 9.11 20.8 3.49 9.42 12.68 13.73 0.78 11.86 11.57 11.60 8.97 2.55 12.45 61.0 13.20 101.6 11.30 11.04 12.99 71.4 172.3 2.86 10.74 3.42 169.6 3.45 2.92 2.73 2.78 26.7 2.77 24.2 3.76 74.1 135.2 25.3 74.1 159.9 38.1 SCR 0122-6400SCR 0123-6802SCR 01 0123-6320 22 21.31SCR 01 0125-6146 23 59.06SCR 01 0125-6359 23 -64 48.67SCR 00 01 0125-5814 33.0 25 -68 03.32SCR 02 01 0126-6614 27.9 25 -63 09.06SCR 20 01 0.423 0127-5213 53.8 25 -61 57.89SCR 46 01 0.225 0127-5927 02.4 26 -63 37.25SCR 113.9 59 01 0.353 0127-7655 12.3 27 -58 30.83SCR 081.0 14 01 0.184 0127-6211 37.9 27 -66 15.13 42.14SCR 078.5 14 01 0.291 0127-6103 16.0 27 -52 18.32 50.49 100.7 13 01SCR 0.183 16.9 27 13.22 0128-5031 -59 18.11 08.32 237.5 27 01 0.235 18.3 27 16.17 -76 14.10 23.34 087.8 55 0.180 01 12.48 11.8 15.77 -62 16.02 28 090.2 11 09.23 0.352 14.23 30.8 12.60 -61 16.12 061.4 03 12.52 0.187 13.51 43.0 13.71 16.97 -50 138.7 12.60 0.193 31 11.94 13.90 22.9 17.09 11.93 076.2 12.39 0.283 11.55 14.49 16.86 12.00 083.6 12.03 12.28 0.374 15.07 11.80 16.41 11.76 163.9 11.23 12.32 14.79 11.74 17.62 11.47 11.51 076.9 13.47 14.36 11.48 16.25 10.64 11.89 12.67 15.29 11.40 10.91 16.98 12.25 12.96 14.20 10.40 11.33 12.00 13.29 0.70 10.69 14.60 11.67 11.92 11.81 3.57 11.06 11.47 12.62 3.39 14.06 11.41 11.31 11.06 0.57 11.23 12.09 175.8 12.91 2.47 11.10 10.51 2.39 11.81 63.2 12.38 2.60 10.25 60.6 2.82 12.20 2.79 56.2 2.44 66.8 2.67 71.1 3.13 79.1 77.3 1.69 80.3 99.9 [159.8] 42.9 61 d b d a d a a c a c d a a c d a c ··· (pc) Est Dist Notes J ······ − F 59 R s JHK 11.34 10.71 10.49 IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B ··············· (J2000) (J2000) ( Name RA DEC SCR 0141-6728SCR 0142-7952SCR 0143-6405SCR 01 0145-6135 41 36.96SCR 01 0146-7140 42 59.82SCR 01 0148-6007 43 -67 29.50SCR 28 01 0148-5013 52.1 45 -79 26.89SCR 52 01 0149-8038 17.9 46 -64 43.19 05 01 0.195SCR 35.6 48 0150-7207 -61 06.85 35 01 0.206 03.6 48 -71 49.22 073.3 40 01 0.323 12.8 49 -60 43.63 033.8 07 0.194 01 12.9 -50 15.81 50 115.1 13 38.49 0.220 21.3 -80 16.84 059.7 38 0.228 28.1 13.50 17.29 -72 087.4 0.196 07 14.90 16.8 16.89 095.1 0.464 12.19 15.56 16.69 034.2 13.67 0.334 14.91 13.07 080.5 11.37 13.53 14.63 15.73 12.44 223.9 13.26 11.85 18.41 10.79 12.74 12.41 13.62 11.86 16.19 11.86 11.28 16.35 10.56 12.25 12.08 12.04 11.65 15.72 11.16 10.47 13.83 12.00 11.53 10.68 15.24 10.93 10.01 11.67 11.28 10.08 15.65 2.14 11.11 9.93 2.46 15.64 9.89 2.82 10.72 3.05 15.42 2.54 68.2 104.6 117.3 1.38 2.94 4.68 55.6 87.3 0.06 58.6 36.4 25.2 SCR 0141-4947SCR 0141-7126 01 41 05.53 01 41 23.03 -49 47 08.5 -71 26 10.2 0.297 0.211 050.4 122.8 15.21 16.76 13.32 14.91 12.03 13.86 11.07 13.59 10.44 13.03 10.24 12.86 2.25 1.32 [245.5] 60.0 SCR 0150-7741SCR 0152-7816SCR 0152-6640SCR 01 0152-7649 50 27.55SCR 01 0153-5000 52 58.39SCR 01 0154-6235 52 -77 03.06SCR 41 01 0154-6244 16.3 52 -78 09.23SCR 16 01 0154-6654 27.5 53 -66 24.18 40 01 0.212SCR 21.9 54 0155-7114 -76 31.22 49 01 0.189SCR 41.3 54 -50 0156-6402A 46.31 112.9 00 01 0.221 04.3 54SCR -62 39.13 0156-7326 071.7 35 0.189 01 01 08.9SCR -62 18.07 55 56 081.3 0156-7157 44 59.23 0.182 52.90 29.0SCR -66 16.62 052.0 0156-6702A 54 0.228 42.7 16.04 01SCR 17.03 -71 025.4 56 0156-6702B -64 0.181 14 09.20 02 14.70SCR 40.2 01 17.83 01 02.3 043.8 0156-6402B 56 56 0.207 14.85 14.83 40.33 26.08SCR 14.78 01 084.2 0157-5950 -73 56 13.47 0.266 15.84 26 0.197SCR 29.33 18.42 01 240.9 02.5 0159-6933 13.31 56 -71 -67 12.83 12.45SCR 10.61 57 11.24 02 0159-6324 12.6 12.19 36.2 074.5 085.6 -67 14.13 16.26SCR 01 16.79 0.224 02 12.77 0200-6747 57 11.57 32.8 -64 10.95 10.12 00.99SCR 01 02 0.211 11.52 0.183 17.34 0200-6243 17.49 59 12.96 42.1 14.05 137.5 14.65 58.80 12.61SCR 01 10.96 0.177 0200-5955 59 -59 20.90 098.4 11.37SCR 057.4 50 02 15.34 9.93 12.36 15.51 0.217 9.79 0201-7106 42.6 00 12.47 18.22 -69 12.76 14.04 10.69SCR 33 047.4 02 0201-5810 47.7 00 -63 14.47 13.55 40.86 14.07 12.15SCR 24 086.2 02 14.18 0.239 11.91 0201-5739 16.02 54.8 00 9.30 11.53 -67 9.65 21.94 02.78SCR 47 02 0.211 0202-5343 24.6 01 12.26 11.37 -62 14.00 18.99 13.09 59.63 069.2 2.73 11.67 43 02 0.215SCR 10.98 15.06 39.3 01 19.21 0203-8415 -59 9.03 43.81 084.5 2.51 55 02 9.28 0.237SCR 11.33 10.22 50.0 13.52 01 16.75 12.46 -71 17.40 0204-5938 38.82 092.1 3.26 10.69 14.07 06 02 0.205SCR 01.3 02 16.23 -58 18.51 0205-5428 46.74 108.3 2.89 10 11.30 0.183 13.26 02SCR 12.27 145.0 14.1 9.17 15.53 14.73 -57 15.86 03 0205-6122A 13.47 9.44 126.4 39 45.62 0.249 13.81SCR 02 36.1 16.20 -53 17.55 0205-6122B 04 10.71 072.4 3.79 88.9 43 09.09 0.210 13.13SCR 02 14.00 02 57.2 14.14 13.28 16.23 0206-6729 05 2.52 -84 05 039.2 13.22 44.9 8.75 41.70 0.202 15 56.20 14.09 110.0 15.29 02SCR 10.55 57.5 17.78 05 0206-5742 -59 084.4 12.60 3.12 12.56 0.205 56.20 38 13.03 14.13SCR 17.70 12.80 58.3 -54 075.4 0206-6609B -61 13.05 1.33 28 2.42 02 13.70 0.240 22 0.48 15.75 8.59 17.30 12.34 09.4 06 40.0 12.04 179.4 57.1 -61 12.26 53.05 13.21 22 15.47 0.214 02 14.98 02 28.0 12.45 40.0 06 12.90 098.0 07 13.84 26.18 15.23 0.216 1.95 0.184 11.82 13.90 17.51 11.67 [294.5] -67 49.3 12.42 024.2 29 13.55 13.05 0.96 12.26 34.9 140.4 12.34 16.08 12.36 -57 076.5 192.8 -66 13.55 41.8 15.43 42 11.46 5.40 09 11.82 34.8 19.24 12.85 55.0 [257.9] 11.49 0.243 1.93 12.11 15.04 3.63 11.71 18.64 15.12 11.98 13.92 11.63 0.313 16.28 12.28 0.220 10.14 190.7 14.50 2.97 11.45 84.4 16.47 11.37 13.52 12.90 184.6 3.14 12.02 075.9 15.19 45.2 16.54 13.47 9.47 29.7 1.88 11.13 14.95 82.1 11.47 12.36 18.46 20.29 13.32 2.39 14.28 12.91 14.06 11.40 1.70 12.13 94.3 9.25 16.48 12.72 18.31 3.39 98.5 12.25 12.86 121.3 13.52 10.79 2.62 15.66 12.46 128.7 16.23 11.45 3.25 13.34 10.53 132.1 14.20 14.29 10.87 2.53 60.9 2.90 113.1 13.64 13.68 1.57 10.64 55.8 2.95 13.46 13.53 2.41 2.13 126.3 [208.2] 27.9 2.83 97.7 230.9 74.6 2.28 4.02 [257.3] 54.8 124.5 62 a d d d d d d d ··· (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 0206-5439SCR 0207-5720SCR 0207-5235 02SCR 06 0208-6505 22.73 02SCR 07 0208-6801 04.74 02SCR -54 07 0208-5355 39 19.51SCR 02 58.0 -57 0208-5329 08 20 36.76SCR 02 08.9 0208-6127 08 -52 47.23 0.202 35SCR 02 39.9 0208-5730 08 -65 46.70 0.202SCR 05 02 0209-5436 16.6 08 -68 083.6 42.06SCR 01 02 0.250 0209-6001 16.5 08 -53 139.5 21.96SCR 55 02 0.229 16.23 0210-7316 21.7 08 -53 164.8 39.03 29 02 0.200SCR 13.25 33.4 09 0210-6304 -61 00.42 095.5 27 02 14.31 0.280SCR 44.8 09 18.59 -57 0210-6252 56.53 024.5 30 02 12.43 0.253SCR 43.2 10 -54 16.23 0211-6108 43.70 053.1 36 13.45 0.188 02SCR 16.40 07.4 -60 18.45 10 0212-6938 082.5 01 11.69 31.84 0.392SCR 02 32.4 14.22 -73 17.80 0212-7238 10 12.69 078.4 16 43.98 0.223 15.21SCR 02 19.9 16.33 13.16 0212-6811 11 10.89 -63 117.4 35.42 0.187 04SCR 02 12.34 15.73 12.10 35.3 16.63 0212-5032 12 -62 062.5 14.19 11.41 0.277SCR 52 02 14.16 10.73 10.60 17.97 0213-6400 30.0 12 -61 234.4 11.54 13.74 11.93 08 02 13.76 0.324 14.77 17.84 53.8 13.65 12 -69 048.1 12.62 24.89 10.51 38 02 10.17 15.94 0.456 18.20 13.5 12 10.85 -72 12.77 161.4 24.86 38 02 13.29 15.89 0.234 13.37 16.69 32.0 13 12.08 -68 05.14 050.0 11 14.41 16.17 0.274 10.66 9.47 48.7 12.26 15.93 -50 12.25 060.8 32 14.52 14.52 0.250 11.81 50.1 -64 17.23 12.53 069.6 1.63 00 14.20 0.197 11.99 14.33 06.4 11.70 11.69 8.79 13.65 227.3 1.55 12.56 0.198SCR 14.95 12.04 15.01 0216-5257 12.36 090.1 0.202 2.22 13.63 11.43SCR 13.11 16.13 0217-5255 11.43 050.7 9.73 8.61 2.68 11.81SCR 12.91 152.7 13.14 11.78 17.19 0217-7234 118.4 13.12 3.71 12.92SCR 02 14.01 10.81 15.57 0217-5233 16 [246.7] 81.3 11.85 32.03 2.95 11.47SCR 02 11.85 15.10 9.23 12.31 0219-5026 12.57 17 34.30 10.58SCR 02 12.33 13.44 0219-5610 17 11.29 -52 11.21 44.06 2.51SCR 60.1 57 02 13.65 10.60 12.39 0219-7102 46.7 17 -52 8.67 11.37 1.26 42.62 3.41SCR 63.8 55 02 11.50 11.01 100.9 0219-8343 18.9 19 10.60 -72 12.67 12.24 2.25 34 02 10.10 0.193SCR 34.6 19 10.75 0220-6904 -52 10.52 03.25 3.81 8.15 33 02 0.204 10.37 40.5 19SCR 12.14 -50 10.06 50.81 0220-6358 234.2 3.08 95.4 26 02 0.192 10.52 10.4 19SCR -56 33.6 37.98 101.5 74.3 0220-5226 10 9.93 0.346 1.21 02 11.91 8.07 210.3 28.2 -71 16.20 20SCR 044.4 02 15.07 9.57 0.188 0220-5345 3.10 51.1 02 -83 17.29SCR 039.2 51.2 20 43 0.297 0220-6240 54.84 51.0 14.11 9.64 02 15.03 -69 [197.9] 061.3 47.0 20SCR 0.275 04 1.93 15.07 06.85 9.40 0220-7841 03.5 16.71 02 041.9 -63 0.256SCR 2.64 20 11.99 13.09 58 0221-6223 15.67 03.12 041.0 17.5 02SCR -52 2.43 56.8 13.14 1.06 20 0.319 14.55 0221-6418 26 16.52 30.95 040.3 23.5 10.62 02SCR 11.87 -53 13.61 20 0222-6336 16.92 0.291 45 43.68 12.05 076.9 24.3 02 71.4 12.61 14.45 2.92 -62 17.50 21 0.329 40 55.12 11.03 02 56.0 52.1 11.48 098.6 9.96 14.78 0.54 119.4 21 -78 11.46 17.96 0.196 23.55 11.44 41 02 12.35 22.9 15.64 095.7 51.4 22 -62 10.47 06.67 0.192 10.90 17.08 23 13.45 11.17 28.2 15.75 102.9 9.68 -64 10.85 11.22 18 16.58 0.308 13.82 33.2 10.25 47.8 -63 086.3 10.31 15.18 12.82 36 0.197 18.39 14.67 10.56 16.7 10.67 093.3 14.32 12.30 0.267 14.35 10.06 12.13 14.01 097.3 16.30 13.97 0.297 10.41 18.02 11.77 13.09 075.3 12.44 3.03 11.92 13.06 3.50 16.82 13.35 080.9 15.30 2.06 11.56 16.29 12.10 17.24 11.49 12.53 3.11 14.91 13.18 17.46 14.74 11.61 15.58 2.71 15.33 11.01 12.32 13.13 3.22 62.6 14.25 15.35 25.6 11.37 14.69 13.20 1.96 64.7 10.42 12.24 13.99 13.46 3.34 45.9 14.10 12.06 10.25 45.9 1.78 11.72 12.25 42.5 13.93 137.0 11.50 2.12 11.49 11.66 2.22 [261.3] 70.9 11.25 1.56 11.42 [166.9] 1.43 1.60 [408.3] 98.6 2.67 3.27 [365.0] 72.5 3.10 93.3 63.6 69.5 SCR 0206-6609A 02 06 56.20 -66 09 50.0 0.181 080.6 17.68 15.65 13.80 12.80 12.21 11.95SCR 0213-5353SCR 0213-6118SCR 0214-5350SCR 2.85 02 0214-7137 13 39.87SCR 02 0214-6202 13 04.35 02SCR 14 0215-6840 -53 53.78 53 02 14.6 101.4 14 -61 53.23 18 02 29.3 14 -53 11.08 50 0.217 02 17.5 -71 15 37 06.40 0.208 36.9 -62 070.7 02 0.216 57.5 -68 098.2 0.185 40 34.2 17.97 194.6 0.214 17.87 038.1 0.300 15.95 16.26 076.3 15.86 18.01 084.9 14.02 14.04 17.45 13.69 15.94 17.62 13.16 12.01 15.33 12.16 14.22 15.49 12.59 11.09 13.74 11.59 12.92 14.56 12.39 10.55 12.58 11.26 12.30 13.76 10.20 11.96 12.05 13.26 11.75 2.79 13.06 3.69 2.96 3.03 131.2 2.75 49.9 1.73 42.3 94.7 [257.2] 93.2 63 d d d d d d d d (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 15.60 13.67 12.58 12.03 11.75 3.03 83.4 R J ··· ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 0222-5238SCR 0222-6408SCR 02 0222-5758 22 45.75SCR 02 0223-8806 22 10.37 02SCR 22 0223-8227 -52 31.55 38 02SCR 11.0 23 0224-6433 -64 10.29 08SCR 02 28.4 0224-5728 -57 23 58 05.03 0.187 02SCR 26.7 -88 24 0224-6446 06 10.97 0.189 02 52.5SCR 24 -82 0224-5659 099.3 13.41 0.303 27 02 59.1SCR -64 098.3 24 0224-5424 0.188 33 39.00 02 13.82 01.7 -57 196.0SCR 24 28 0.204 0224-5608 03.42 15.39 15.5 02 225.6SCR -64 24 11.40 0.448 0224-6946 46 16.70 12.17 15.6 076.3 02 -56SCR 13.25 0.182 24 59 15.93 0225-7548 18.98 28.5 107.3 02 10.47SCR -54 14.54 24 0.317 0225-5628 24 18.32 54.00 023.7 35.2 11.58SCR 14.04 02 -56 0.194 0226-5348 25 16.26 08 59.11 12.44SCR 197.9 41.3 02 16.49 9.73 0227-4736 -69 13.19 25 0.215 10.89 46 12.34 26.55SCR 087.7 02 53.1 13.96 0228-6248 26 -75 11.60 18.12 0.217 52.55 48 02 15.64SCR 146.4 11.32 10.26 49.9 27 0228-5952 9.13 11.51 -56 18.32 00.97 0.194 28 02 11.79SCR 11.06 55.8 28 16.08 162.0 0228-5641 -53 14.40 13.92 16.98 48 10.02 0.367 10.16SCR 02 10.89 45.1 16.11 0228-6801 -47 085.4 28 10.94 8.89 36 10.80 11.47 0.231SCR 16.55 02 14.58 48.0 13.83 0228-5325 -62 28 15.23 090.0 48 10.66 40.21 0.183SCR 02 14.79 04.5 13.92 9.85 0229-7237 10.43 28 -59 142.2 14.47 13.71 49.03 0.240SCR 52 13.66 02 16.55 0229-7614 20.7 14.43 28 -56 220.4 12.42 18.91 0.229 12.35SCR 41 02 10.12 0229-7028 15.63 30.1 29 13.19 9.25 -68 078.5 13.69 2.36 59.71SCR 01 02 14.95 0.181 13.77 0229-6656 17.91 52.2 29 1.67 -53 060.8 11.78 10.97 2.94 53.09SCR 25 02 13.51 0.190 12.96 0230-6328 13.05 56.0 29 -72 2.54 096.5 13.28 07.52SCR 9.02 14.17 37 02 15.80 0.232 0231-5834 15.84 11.48 05.1 29 10.73 -76 04.55SCR 105.1 2.09 14 02 12.48 12.40 0.190 0232-8458 10.6 30 17.87 13.08 -70 13.30 50.1 21.60SCR 075.3 28 02 14.23 3.02 13.53 0.274 10.18 0232-5850 11.6 31 -66 36.2 12.89 57.9 11.81 29.21 12.22SCR 097.8 56 02 0.193 0233-6513 15.81 45.1 12.74 32 -63 17.90 [308.3] 66.0 13.27 50.12SCR 055.0 28 02 11.28 0.253 2.37 0233-8536 40.5 32 10.99 11.33 9.95 -58 18.21 00.89SCR 1.47 068.2 34 02 0.181 12.57 14.99 0234-6227 3.76 44.5 33 15.71 12.76 -84 18.38 10.43 35.95SCR 089.8 58 02 39.9 0.243 11.07 0234-6036 10.50 09.5 33 16.04 1.46 -58 16.16 48.37 103.3 [201.5] 14.33 50 02SCR 0.257 12.52 13.48 19.3 34 16.14 0235-7043 -65 16.08 06.17 1.41 088.2 13 02 10.03 9.86 0.220SCR 14.16 20.7 34 14.09 0235-6000 -85 14.11 13.91 09.15 190.0 40.5 36 12.44 0.203 02 [268.4] 14.09 51.7 SCR 22.9 14.11 1.69 -62 16.48 35 0237-6049 141.9 27 14.37 12.96 0.206 1.65 02 12.53 07.1 9.47 13.06 13.69SCR 9.57 [177.5] -60 18.48 35 11.90 0237-6747 126.9 36 12.63 33.08 0.204 1.70 12.23 59.1 14.23SCR 02 12.31 -70 12.37 0238-7142 067.4 37 11.68 0.182 43 2.54 12.63 55.84 16.39SCR 11.64 13.6 02 16.80 9.37 12.04 [194.6] 0238-6952 -60 062.0 37 11.56 0.249 00 12.43 10.17 42.19SCR 12.12 59.6 02 18.12 21.9 11.04 0238-5257 074.9 38 12.56 -60 14.43 0.220 14.78 49.17SCR 49 11.81 02 15.52 104.2 10.93 0239-7207 050.9 17.5 38 11.95 -67 15.95 34.60 0.272 1.48 3.10SCR 10.84 47 02 18.09 151.5 12.21 0239-6015 9.88 32.2 38 13.27 107.4 -71 12.73 13.49 58.85SCR 10.75 42 02 17.37 0.213 11.37 0240-6043 03.4 39 -69 046.8 13.97 16.11 44.57SCR 3.27 12.13 52 02 0.213 0.96 12.74 16.85 0241-7305 29.9 39 12.18 [358.5] -52 9.00 11.59 158.7 15.14 44.30 3.08 11.10 57 02 0.281 13.50 32.7 40 12.89 -72 14.41 16.59 29.5 086.3 3.51 12.56 07 02 14.70 0.202 11.67 53.8 41 10.65 18.05 -60 13.34 24.47 061.9 2.40 15 8.34 11.50 0.193 12.35 55.3 13.11 -60 16.00 042.8 2.55 13.79 11.43 73.1 43 0.199 42.6 10.08 15.89 09.7 12.65 -73 17.69 214.1 0.51 12.09 95.5 05 10.76 0.185 12.59 00.3 8.18 13.77 16.91 13.23 039.2 2.28 67.0 0.269 12.19 14.52 15.54 9.82 16.56 10.48 066.5 3.12 12.31 72.1 0.190 12.22 12.74 14.76 15.53 097.4 11.92 67.9 13.87 13.57 164.1 14.76 18.07 064.3 2.60 11.70 9.81 12.47 13.26 13.37 15.17 13.39 3.06 84.1 12.48 13.05 121.5 1.17 15.93 16.92 11.12 12.66 11.99 12.86 13.14 9.70 2.84 11.91 3.01 12.08 14.00 14.80 10.96 12.12 2.49 92.8 11.34 11.09 11.64 11.50 97.6 13.16 1.47 12.80 24.9 11.89 10.81 10.86 113.7 11.29 38.7 12.56 11.64 117.0 2.02 1.02 10.58 10.31 [205.2] 2.06 12.26 11.02 3.07 10.05 [245.4] 2.10 10.75 57.7 2.68 2.03 86.6 2.77 78.3 133.4 2.00 3.15 85.1 74.7 118.8 57.1 49.3 64 d d d b a a c d d b d ··· 31.4 (pc) Est Dist Notes J ··· − F 59 R s JHK IVN 18.83 12.33 11.70 11.41 I F 59 ··· R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 0241-7719SCR 0242-5935SCR 0242-6051 02 41SCR 29.53 0242-8138 02SCR 42 0243-6044 26.39 02SCR -77 42 0243-6746 19 14.17 56.1 02SCR -59 42 0243-7249 35 22.48SCR 01.6 02 -60 0244-7217 43 0.187 51 09.21 02 39.2SCR 43 -81 0245-6038 0.466 51.46 38 02SCR 059.3 53.6 43 -60 0246-7024 13.37 0.260 44 02SCR 24.9 44 185.2 -67 0246-4935A 43.32 46 17.47 0.201 02SCR 48.0 -72 183.0 45 0246-4935B 49 27.77 0.190 16.03 02 02 51.6 -72 46 105.0 46 15.45 17 02.25 0.251 23.44 18.10 02.6 02 -60 46 178.8 15.01 0.198 38 23.96 17.73 58.2 13.46 -70 085.6 -49 15.85 0.188 24 35 18.23 06.3 03.2 051.2 14.03 -49 15.91 0.196 35 12.19 15.24 09.9 084.5 13.71 16.08 0.259 0.247 15.55 13.55 049.6 11.61 15.08 13.07 0.233 18.85 12.84 113.2 072.3 13.93 12.99 13.58 17.16 11.40 13.87 11.44 16.50 12.30 51.2 15.71 14.66 13.16 12.78 11.97 16.36 13.29 11.20 12.05 13.94 19.11 13.33 12.68 11.96 11.07 13.14 16.07 10.61 12.65 12.38 10.71 10.17 10.39 3.26 15.83 10.38 12.08 1.46 10.25 10.18 9.84 15.47 3.01 11.85 2.04 15.67 9.63 [228.8] 66.1 9.33 2.91 1.87 9.36 [247.0] 98.2 2.51 9.02 3.84 123.0 0.53 70.3 51.5 1.71 [821.9] 61.1 3.49 40.0 20.0 SCR 0241-6459 02 41 09.78 -64 59 41.2 0.353 178.5 16.44 14.71 13.94 12.96 12.43 12.27 1.75 [171.2] SCR 0246-5531SCR 0246-5724SCR 0246-7322 02SCR 46 0247-6136 15.01 02SCR 46 0247-5818 46.71 02SCR -55 46 0247-5729 31 54.02SCR 02 18.9 -57 0247-5538 47 24 39.88SCR 02 47.5 0247-7403 47 -73 58.07 0.199 22SCR 02 44.8 0248-7134 47 -61 14.61 0.189SCR 36 02 0248-6834 18.3 47 -58 128.6 37.98 18 02 0.272SCR 20.9 47 0248-4908 -57 195.2 07.51 29 02 0.202SCR 13.02 21.5 48 -55 0248-7318 077.3 04.81 38 02 0.217SCR 13.45 26.1 48 -74 0248-7529 23.30 087.1 03 11.87 0.216 02SCR 47.6 15.99 -71 48 0249-6914 049.3 34 07.87 11.50 0.188SCR 02 32.9 -68 16.60 0249-6640 48 187.7 34 11.42 47.50 0.241SCR 02 14.66 48.4 18.43 0249-6904 48 -49 055.0 10.89 46.56 0.207 08SCR 02 14.32 52.8 16.56 0250-6919 49 11.17 -73 172.9 13.15 0.211 14.13SCR 18 02 16.20 16.72 0251-4718 51.9 49 10.45 -75 027.7 37.48 29 02 12.79 0.212 14.16SCR 10.73 17.15 53.1 49 0252-7522 -69 045.6 13.55 00.94 14 02 14.41 14.73 0.217SCR 15.99 18.1 50 -66 0252-7148 12.20 094.1 9.85 20.08 10.67 40 02 11.78 14.98 0.186SCR 17.98 24.1 13.06 51 -69 0253-7349 13.29 32.11 077.6 04 13.00 13.85 0.252 02SCR 57.7 11.70 17.63 -69 52 0254-7051 11.20 100.7 19 13.00 45.71 15.81 0.195 12.89 9.73 02 59.8SCR 12.67 -47 18.07 52 11.89 0255-7242 067.2 18 12.10 22.35 0.264 11.44 02 15.85 52.4 10.62SCR 14.31 53 12.46 -75 050.2 0255-7924 13.75 46.00 0.180 22 12.43 02 15.85 11.33SCR 44.5 15.64 54 11.59 -71 069.4 0.70 0256-5436 42.15 0.208 15.02 10.36 48 12.00 11.86 02SCR 17.31 46.1 12.77 -73 036.3 55 0256-6745 11.06 49 13.33 05.55 0.496 13.48 11.05SCR 02 18.00 22.8 -70 124.4 0258-5048 14.39 55 1.10 1.05 11.62 51 10.30 15.31 18.39 0.245 12.24SCR 02 17.52 45.4 0259-7508 56 12.34 -72 063.5 2.13 10.80 11.66 15.96 59.00 0.196 42SCR 02 16.96 13.87 42.0 81.8 0303-7436 56 10.39 -79 036.7 2.92 11.93 13.60 15.53 48.30 0.213SCR 24 02 11.74 17.09 [222.7] 0303-7209 55.6 58 11.14 -54 065.8 2.96 13.78 14.78 41.85 13.65SCR 36 02 0.439 18.64 0304-5720 43.3 59 12.49 54.2 -67 063.1 2.84 13.79 9.72 26.08 11.47 45 03 105.7 16.32 0.185 10.56 15.62 49.5 03 12.62 -50 2.52 12.41 051.7 13.84 48 03 116.6 16.44 0.243 11.97 18.65 34.7 03 12.84 -75 2.27 44.06 025.9 16.17 10.25 08 03 13.30 0.190 9.53 12.09 33.7 04 12.00 17.52 -74 3.04 45.1 28.36 055.4 11.74 36 14.62 16.47 0.201 12.26 47.7 -72 18.25 68.1 15.77 1.46 167.3 11.84 09 11.15 0.215 11.37 15.43 59.6 -57 15.80 99.2 13.41 195.8 3.51 12.00 20 14.21 0.331 08.0 15.76 16.21 18.32 76.2 10.55 063.2 11.17 0.430 14.26 13.33 12.90 [346.5] 18.16 91.7 13.03 072.4 2.34 0.196 15.33 1.61 14.20 16.19 10.00 15.46 085.9 2.82 13.73 12.59 12.05 16.00 12.41 18.75 090.2 3.34 60.5 12.62 14.30 13.85 18.77 13.23 9.72 2.69 11.58 12.17 14.21 16.44 12.59 12.11 2.78 56.3 13.38 48.5 12.61 16.38 13.00 10.97 95.9 13.19 0.55 13.85 12.17 11.87 12.89 79.8 12.26 3.03 14.11 112.1 10.76 12.66 12.20 11.77 12.62 11.64 2.75 [675.9] 73.6 12.71 3.45 12.41 11.59 11.73 1.70 11.48 122.2 12.23 3.60 11.29 11.49 1.76 11.94 37.0 [254.3] 83.8 2.81 11.47 2.81 1.59 70.6 4.24 83.0 143.0 3.67 126.2 0.44 125.0 38.1 67.7 65 d b d d d ··· (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 0304-7930SCR 0304-7949SCR 03 0304-7157 04 30.27SCR 03 0305-7143 04 50.50 03SCR 04 0305-6725 -79 50.61 30 03SCR 01.4 05 0306-5334 -79 00.99 49SCR 03 57.7 0308-7451 -71 05 57 37.04 0.193SCR 03 58.2 0310-6953 -71 06 43 38.29 0.185 03SCR 06.9 08 0311-6215 -67 087.5 09.99 0.196 25 03SCR 16.4 10 0312-7531 -53 065.2 59.01 0.215 34SCR 03 16.57 56.5 0312-7408 -74 346.6 11 51 21.33 0.182SCR 03 18.23 17.2 0314-7838 -69 063.6 12 53 47.13SCR 14.45 0.238 03 14.94 42.9 0315-5635 12 -62 147.2 45.89SCR 16.12 0.336 15 03 16.89 0319-6718 15.7 14 -75 194.6 12.79 03.61SCR 12.87 0.268 31 03 0319-6918 17.16 01.4 15 -74 085.0 14.21 13.79SCR 14.59 08 03 0.416 0319-7926 33.8 18.70 19 11.83 -78 067.2 11.19 52.45 38 03SCR 15.36 0.193 55.4 15.81 19 0320-6736 12.67 -56 12.98 31.43 083.3 35 03 0.217SCR 16.33 11.24 20.4 17.59 19 10.18 0322-6842 -67 26.49 214.4 18 14.38 0.307SCR 13.46 03 12.12 36.9 12.19 0322-7913 -69 15.68 20 110.3 18 10.97 59.36 14.56 0.220SCR 15.61 03 40.8 0323-8059 -79 16.37 22 13.59 036.6 9.55 26 11.86 11.63 59.54 0.194 11.68 03SCR 49.3 16.05 18.31 22 0324-6757 -67 13.19 167.5 14.09 36.57 0.311 36 03 14.17SCR 13.00 12.5 17.53 23 11.03 0325-6931 -68 055.4 11.41 16.61 0.185 9.33 42 16.13 16.26SCR 03 12.67 16.51 08.2 12.69 0325-7018 -79 057.2 24 12.88 13 12.12 08.97 0.253 15.51SCR 10.57 03 18.43 35.0 0326-6918 -80 045.4 2.62 25 16.13 59 14.91 12.36 14.35 11.47 0.211SCR 12.19 03 15.94 02.4 0326-6812 3.45 25 11.33 -67 077.7 13.61 10.31 16.33 32.85 0.188SCR 57 03 17.54 16.31 0326-7034 29.7 26 13.83 -69 066.7 12.50 11.91 13.86 50.96 0.192SCR 31 03 10.77 18.11 0326-6034 15.1 2.40 26 12.17 -70 044.6 2.69 14.35 15.53 40.42SCR 16.50 18 03 0.196 13.29 0328-5508 16.41 58.1 69.8 26 11.28 -69 144.6 1.77 12.06 24.38SCR 10.57 18 03 16.35 0.294 11.68 0331-5312 12.08 06.1 72.4 26 12.80 -68 3.14 13.68 064.9 37.93SCR 13.07 12 03 14.53 0.183 10.69 0331-8251 17.85 20.2 28 10.97 -70 2.43 45.93SCR 038.5 15.37 11.39 34 03 10.64 0.248 12.17 0331-6919 [235.1] 34.0 92.9 31 12.47 14.33 -60 31.9 2.92 52.09SCR 029.8 10.41 34 03 12.85 15.76 0.189 10.35 0332-7456 32.1 31 -0.08 -55 16.12 14.52 41.85SCR 052.0 11.93 08 03 10.45 0.223 11.84 0332-4848 13.34 40.3 31 -53 16.42 99.6 11.86 16.29SCR 062.4 2.83 10.15 12 03 14.22 0.231 0335-6403 07.6 14.00 32 14.16 -82 16.17 56.0 58.02SCR 027.8 2.43 11.57 51 03 0.228 12.79 0336-6653 9.78 10.2 32 14.36 11.34 -69 17.08 97.6 12.88 53.17 030.0 3.34 19 03SCR 0.186 13.78 12.28 30.3 35 14.27 0338-7102 -74 16.96 55.46 068.5 3.08 12.33 56 03 0.447SCR 11.12 12.75 44.8 36 15.04 12.41 0340-6541 -48 16.03 9.37 53.44 081.5 3.53 54.0 48 11.11 0.223SCR 03 12.79 203.4 54.0 14.78 0340-6724 -64 17.57 38 11.92 050.8 2.89 03 29.72 11.46 0.182SCR 12.18 03 13.18 35.2 13.94 0340-6528 -66 17.60 40 10.57 031.3 3.07 63.6 53 11.85 9.24 29.65 0.187SCR 03 12.95 37.7 15.44 11.82 0341-6252 18.24 40 -71 10.86 027.9 43.4 11.99 59.31 0.183 1.82SCR 02 03 12.38 15.60 10.28 0341-5326 54.1 17.16 40 11.22 -65 107.6 71.1 11.51 17.87 0.185SCR 2.66 41 03 14.01 16.43 10.61 0342-6000 15.39 02.0 41 11.38 -67 036.7 42.7 10.95 40.82SCR 24 03 13.96 0.180 15.28 11.02 0344-7214 18.19 23.3 41 10.93 [346.5] -65 094.8 76.0 12.85 21.44SCR 2.88 28 03 14.65 13.16 0.183 11.14 0346-7019 16.50 40.7 42 10.39 -62 12.84 0.86 146.3 21.41 52 03 13.54 15.61 0.180 1.01 10.67 17.85 19.0 44 12.27 -53 13.20 20.63 081.9 79.2 26 03 11.24 14.38 0.185 3.05 10.12 20.9 46 12.32 17.38 -60 12.31 17.95 136.3 00 13.84 15.83 0.260 2.90 12.01 112.5 06.3 12.69 -72 12.04 10.77 [135.1] 032.2 14 12.24 0.364 2.43 12.10 15.85 41.3 11.74 -70 18.27 12.72 38.4 037.6 19 13.60 0.189 3.05 12.46 11.9 10.95 10.18 15.53 11.70 035.6 0.249 3.27 15.12 11.51 43.8 16.40 12.12 15.59 12.33 108.8 0.277 2.99 52.0 10.28 13.31 11.12 18.67 9.95 048.9 14.11 2.59 11.84 80.7 14.75 13.51 11.82 16.72 048.9 10.75 2.76 10.89 63.2 11.84 16.30 16.51 13.50 13.63 3.23 11.56 44.4 11.80 14.64 16.25 10.39 11.35 2.97 39.8 13.82 14.29 13.38 112.7 13.06 11.49 13.61 14.33 10.26 115.7 10.76 2.39 12.25 2.89 12.34 12.81 115.1 10.86 12.88 2.68 12.71 10.50 11.68 11.72 3.49 80.9 10.65 12.29 11.07 1.74 11.37 11.07 47.9 83.3 0.20 12.12 10.51 67.8 2.77 10.82 [270.5] 65.4 1.97 10.28 2.02 4.05 93.2 161.6 1.76 2.57 71.7 3.25 77.1 42.8 164.6 65.4 39.5 66 d d a a d d d b d d d d d d d (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 0347-8145SCR 0348-6759SCR 0350-8642 03SCR 47 0351-7143 25.56 03SCR 48 0352-6824 41.23 03SCR 50 -81 0353-7232 45.82 45 03SCR 20.3 -67 51 0353-6844A 59 46.89SCR 03 10.7 -86 0353-6844B 52 42 0.202 34.31SCR 03 03 21.9 0354-7109 53 -71 53 14.60 0.189 43 40.90SCR 03 12.7 0354-5243 170.1 53 -68 0.184 39.10 24SCR 08.7 0354-6848 -72 122.4 -68 32 03 0.392 44 16.76 10.3 54SCR 22.1 039.5 -68 21.53 0354-7043 03 44 0.200 18.26 54 31.4SCR 122.8 13.19 15.09 0.286 0354-6043 0.232 03 15.99 -71 54SCR 135.8 09 59.45 16.38 0355-5204 0.238 06.6 03 18.15 -52 094.6 14.37 54 038.0 43SCR 14.05 57.26 00.9 0355-5611 17.10 -68 03 038.1 14.52 0.198SCR 48 54 15.97 0357-7343 32.7 16.49 33.17 13.45 16.96 03 12.59 -70 0.205SCR 55 15.17 43 0357-5110 27.50 17.09 13.14 023.2 44.6 03 15.37 0.269SCR -60 12.85 14.42 14.76 55 11.36 0358-7058 43 023.2 31.89 57.4 03 14.03SCR -52 12.56 14.92 17.53 57 0.217 0358-7527 04 14.52 34.34 040.2 12.68 03 15.9 13.02 12.68SCR 10.64 15.69 57 -56 0359-7155 0.182 50.27 12.90 11 12.35 088.6 15.25 12.94 03 28.2SCR 14.02 -73 18.68 58 0.215 11.86 0359-6732 11.68 43 10.47 15.84 13.66 03 24.9 081.4SCR -51 12.30 58 17.77 0400-5443 11.87 10 0.279 13.44 02.86 13.92 03 39.9 16.03SCR 205.1 11.29 11.09 59 -70 0401-6754 12.71 09.87 0.212 58 18.10 12.07 03SCR 42.2 11.30 15.88 029.1 12.54 -75 1.64 59 0401-7328 0.244 27 17.57 15.81 11.07 48.19 10.83SCR 04 55.0 12.11 -71 188.3 0402-4812 3.24 00 16.13 55 0.181 17.69 11.02 17.37SCR 11.99 04 15.08 13.2 166.7 0403-5309 2.69 01 14.90 -67 15.41 28.47 0.184 32SCR 11.51 04 17.58 [202.6] 47.1 15.14 0403-4916 01 156.4 -54 1.45 11.75 16.47 14.36 01.90 0.310SCR 43 04 16.24 14.31 0404-6832 07.0 13.01 02 -67 053.2 2.27 11.32 105.5 15.64 02.39 54 04 0.244 14.58SCR 18.40 16.7 03 13.85 0404-5322 -73 075.9 16.11 2.55 3.09 14.13 46.16 14.03 28 04 0.184 11.81SCR 14.37 [381.7] 32.1 53.5 03 -48 0404-6732 14.04 131.3 14.07 53.62 3.05 12 04 16.36 0.268SCR 13.62 15.91 16.05 36.7 04 -53 0406-7240 12.25 54.35 089.8 11.21 09 136.2 12.46 0.212 04SCR 05.0 12.70 18.88 13.95 -49 04 0407-6925 2.71 220.0 15.70 16 02.17 15.54 13.68 0.247SCR 04 28.4 11.41 -68 14.42 10.91 0408-6756 1.55 76.0 04 53.2 019.1 32 10.88 31.26 0.184 12.05SCR 04 16.25 18.5 15.64 0408-6750 14.82 06 -53 15.44 59.3 163.3 1.12 11.73 48.91 0.191 10.86 22SCR 04 12.55 47.8 18.21 0409-6251 07 10.69 -67 188.6 11.76 57.70 0.270 15.68 1.52 32 04 14.20 13.30SCR 15.76 47.4 95.3 08 11.00 0409-6654 -72 035.1 10.59 118.7 42.24 40 04 11.56 0.185 16.32 10.12 1.56SCR 18.08 [398.5] 34.9 08 -69 042.6 0409-7923 14.96 39.74 14.07 25 04 11.51 13.68 0.185 10.47 13.46 3.60 59.1 09SCR -67 [336.5] 10.96 058.4 30.85 0411-6859 56 14.72 15.87 0.209 04 15.07 23.8 14.33 0.41SCR 9.75 -67 09 10.81 192.7 10.23 [393.4] 0411-6833 50 12.10 13.04 11.44 0.247 04 59.6 10.32 18.28 -62 2.94 09 13.22SCR 045.4 51 14.00 12.74 55.86 0.196 14.09 0412-6844 05.1 10.25 04 14.00 2.72 11.51 -66 029.5 11SCR 0.260 54 10.16 [755.9] 44.3 16.30 28.15 0413-6911 12.60 08.4 04 17.88 9.97 12.86 1.54 -79 039.9 10.87 11 0.197SCR 10.01 23 11.73 52.76 10.99 0414-6810 18.63 46.0 04 062.4 -68SCR 15.46 12.32 12 0.368 15.92 12.32 59 1.77 0415-6918 18.43 87.4 16.39 10.40 026.5 16.9 2.68 9.67 04SCR -68 10.73 10.59 16.39 0.247 13 [403.4] 0416-6648 33 15.63 57.5 55.38 14.73 32.6 081.7 1.29 04 12.05 14.04 -68 16.25 13.82 14 0.283 44 58.90 10.36 9.87 349.2 04.2 04 1.59 14.54 9.06 13.48 15 -69 14.11 0.265 16.96 22.54 12.63 11 04 2.49 14.49 112.1 11.77 43.8 55.4 16 -68 [408.5] 16.96 49.0 0.313 44.47 13.42 10 3.10 11.66 9.77 14.04 9.57 090.2 33.9 15.04 8.83 -69 12.07 13.33 17.45 18 2.18 0.192 10.63 06.0 060.0 14.78 -66 12.91 11.68 48 18.82 3.01 66.9 0.302 13.70 11.89 18.8 9.53 12.82 15.22 047.2 10.76 46.4 0.214 17.23 12.59 13.06 106.8 11.18 16.45 093.9 13.21 0.307 12.54 18.42 10.14 14.25 094.3 77.4 14.99 12.22 1.57 2.33 10.95 1.77 16.71 14.16 12.67 179.3 95.9 16.21 13.55 17.96 11.69 14.16 9.97 3.28 14.52 12.85 12.48 1.37 16.14 [415.5] 13.04 15.30 2.97 15.84 11.40 13.56 12.39 40.5 12.58 2.92 13.93 36.1 12.78 14.52 13.94 1.80 13.09 12.07 11.98 12.23 83.0 53.1 13.97 125.3 1.01 12.94 12.93 1.82 126.3 11.45 12.01 13.81 2.56 12.48 92.9 11.21 11.43 1.67 [196.8] 12.22 3.60 62.5 11.21 1.43 [226.2] 88.0 1.69 2.55 [252.9] 74.7 2.90 [363.2] 1.93 82.5 115.1 101.4 67 a a bc e d a d a (pc) Est Dist Notes J − F 59 R s JHK ··············· IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 0417-5710SCR 0418-7249SCR 0418-6226SCR 04 0422-6706 17 15.74SCR 04 0422-6606 18 30.31SCR 04 0422-7507 18 -57 08.02SCR 10 04 0422-7048 25.7 22 -72 09.04SCR 49 04 0424-6302 47.1 22 -62 05.82SCR 26 04 0.204 0424-4700 54.4 22 -67 45.60SCR 06 04 0.199 0424-6942 00.4 22 -66 06.67 055.1SCR 06 04 0.201 0424-6839 23.3 24 -75 48.19 024.8SCR 07 04 0.230 0425-6521 42.9 24 -70 16.57 58.60 006.5SCR 48 04 0.337 0426-6245 45.9 24 -63 14.76 00.11 070.5SCR 02 04 0.200 0428-6432 09.6 24 14.59 -47 18.61 18.75 037.6SCR 00 04 0.199 0429-5423A 04.2 25 12.83 -69 17.41 39.34 056.3 42 04 0.192SCR 12.86 18.9 26 16.30 0429-5423B -68 15.96 28.36 174.8 39 04 04 0.203SCR 11.70 24.1 28 15.07 29 0429-5037 -65 17.84 25.49 030.3 05.93 21 11.81 0.184SCR 14.30 04 56.4 13.92 0430-7050 -62 16.19 29 181.8 45 10.88 0.328SCR 05.93 13.06 18.3 15.87 0430-6621 -64 16.24 -54 11.19 178.0 32 13.36 23 0.335SCR 04 11.86 17.4 13.92 03.6 0430-4740 18.31 29 10.26 060.2 -54 57.13 12.24 0.256SCR 04 13.69 23 14.17 10.95 0431-6301 12.45 30 03.6 12.80 066.9 33.82 11.50 0.312 0.188 04 12.36SCR 16.16 10.07 17.37 30 0431-6316 -50 11.70 083.1 12.53 12.02 37 04 11.83 11.00SCR 0.170 12.52 15.7 18.53 30 -70 10.96 0432-6852 016.1 049.4 29.07 11.60 50 04 13.78 15.26SCR 11.38 08.0 16.90 31 -66 11.40 0433-7843 47.63 11.09 21 0.188 16.28 04SCR 39.7 10.68 52.5 17.95 15.03 -47 11.09 31 0434-7457 9.91 12.75 40 59.18 13.79 0.234 14.82SCR 2.79 04 11.10 59.2 -63 10.51 0435-7215 32 170.8 01 14.21 04.44 0.195 16.01SCR 12.94 04 1.95 10.84 17.91 19.1 12.16 0436-8233B 33 -63 12.96 027.0 9.98 13.15 23.40 0.182 16SCR 2.94 04 10.28 24.9 15.81 0437-7554 34 13.22 -68 011.6 14.11 21.54 0.312 11.35 17.09SCR 52 04 2.82 11.91 04 12.42 17.29 0437-7553 58.0 35 12.67 36 -78 088.6 39.75SCR 06.17 43 2.42 66.1 0.198 9.36 13.62 12.65 17.02 0439-7133 17.0 13.36 -74 019.9 10.84 16.97 SCR 57 3.86 04 12.21 61.1 15.27 0.198 12.08 15.64 0440-5909 41.5 121.9 37 -72 -82 295.2 25.49SCR 15 04 2.32 12.02 12.39 33 15.11 0.214 12.84 16.90 0440-7319 10.21 59.6 37 9.21 14.2 57.57 034.2SCR 3.08 04 13.59 11.87 75.5 13.58 0.187 0442-5626 39 17.99 -75 11.20 08.00 159.1 54 04 13.21 3.41 12.56 69.3 14.84 0.249SCR 0.233 13.9 40 0442-5034 -75 15.48 9.97 12.66 02.41 152.3 53 04 12.53 42.8 SCR 16.12 18.5 40 10.57 -71 16.36 0444-7329 12.65 00.03 010.7 33 051.1 2.30 04 12.66 74.2 0.343SCR 50.0 42 13.34 12.09 -59 16.56 0445-7744 12.01 23.75 09 3.06 43.9 0.387 04 15.11 10.32SCR 28.7 14.15 1.01 12.08 -73 18.12 42 0445-6524 15.73 11.85 027.5 19 2.15 77.9 56.10 0.196 11.84SCR 04 12.17 38.0 14.88 11.44 -56 0445-8039 44 027.5 14.37 26 2.65 44.88 0.187 11.81SCR 04 12.08 36.3 144.2 16.01 11.24 13.43 15.75 0447-6510 2.10 45 -50 066.3 11.63 11.01 0.194 34 11.28SCR 04 14.04 110.0 50.0 17.64 0448-7204 13.83 45 -73 013.3 11.27 09.94 0.306 11.01SCR 29 04 14.37 130.3 13.84 11.66 48.3 17.70 0448-6450 36.0 45 10.96 -77 057.0 13.12 56.11 2.42SCR 44 04 0.247 153.9 15.73 13.55 15.65 0452-8036 04.0 47 10.68 -65 051.8 13.29 42.90 10.93 2.62SCR 24 04 12.10 15.72 0.227 10.82 15.26 0453-4959 37.3 54.4 48 12.57 -80 028.4 22.36 2.46SCR 39 04 13.78 13.65 0.241 10.43 16.27 0454-8045B 58.8 48 12.72 -65 10.34 10.87 28.69 086.5 1.57 10 04 13.76 13.32 0.295 12.35 45.9 52 18.13 -72 12.31 19.08 044.6 2.99 55.3 04 04 12.02 14.15 04 0.187 12.46 107.8 10.11 07.4 53 10.30 54 -64 15.98 12.54 56.30 025.9 41.30 50 11.82 0.265 1.75 117.0 16.29 06.5 11.75 -80 16.56 11.31 172.1 36 12.08 0.189 1.71 10.07 116.1 23.3 14.12 12.01 -49 18.21 -80 10.58 048.7 59 45 0.180 2.88 15.43 11.50 14.2 14.24 10.69 37.9 15.23 11.33 [324.0] 034.0 62.7 0.220 1.76 11.76 13.11 16.41 16.25 063.2 14.76 9.99 0.270 2.71 10.44 0.195 12.44 2.50 13.27 10.72 16.43 056.0 12.22 90.3 13.86 14.23 14.94 14.28 086.0 014.2 11.68 2.97 10.46 48.8 12.07 13.84 9.72 15.65 176.1 11.65 12.61 3.42 12.41 12.84 14.07 16.10 133.5 18.74 11.12 11.61 3.18 12.36 48.6 13.69 11.45 12.03 11.76 2.34 11.72 13.58 10.88 16.48 11.01 11.64 41.5 12.19 11.71 11.16 11.57 2.82 65.1 11.72 14.09 2.74 10.82 11.07 11.61 82.5 1.53 10.87 10.94 11.05 12.64 62.7 1.90 10.82 11.05 2.56 10.75 10.49 12.02 [417.4] 51.5 38.0 3.80 10.81 1.67 10.26 11.75 118.8 2.47 2.20 67.4 1.27 63.6 2.08 93.5 2.53 73.0 3.84 71.7 91.3 83.7 49.6 43.0 68 a d d (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 14.89 13.12 12.33 11.85 11.57 2.56 96.9 R J ··· ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 0458-7530SCR 0501-8013SCR 0502-7952 04SCR 58 0505-5633 54.34 05SCR 01 0505-8343 51.22 05SCR -75 02 0507-7940 30 00.27SCR 05 22.9 -80 0507-7655 05 13 05.50SCR 05 38.8 0509-8101 05 -79 04.39 0.193 52SCR 05 19.9 0511-7421 07 -56 56.46 0.336SCR 33 05 0513-4948 14.0 07 -83 021.5 14.62SCR 43 05 0.237 0514-6148 39.7 09 -79 305.0 54.89SCR 40 05 0.349 14.34 0514-6015 01.9 11 -76 145.2 34.94SCR 55 05 0.183 15.72 0515-7500 55.3 13 -81 21.72 172.6SCR 01 05 12.60 0.262 0518-4759 57.6 14 16.55 -74 49.96 022.6SCR 21 05 13.60 0.186 0519-8037 49.9 14 -49 17.11 49.28 021.5SCR 48 05 11.85 0.223 0519-5136 14.71 42.1 15 -61 15.49 33.22 061.3SCR 48 05 11.98 0.291 0519-8325 37.4 18 14.75 -60 16.95 10.81 19.56 031.4 15 05 0.206SCR 14.06 44.5 19 13.50 0522-7333 -75 18.52 11.01 31.90 019.9 00 05 0.182SCR 12.51 49.2 19 14.93 10.14 -47 17.85 0523-8140 14.62 343.7 13.03 59 05 0.211SCR 12.50 12.3 19 16.39 10.47 -80 18.23 0523-7249 34.76 355.5 37 11.77 0.334 05 10.04SCR 13.02 18.7 15.78 -51 17.76 22 0524-5604 12.46 063.9 36 53.50 11.90 0.187 10.21SCR 05 14.91 20.3 16.29 -83 16.65 0525-7425 23 11.20 100.8 25 11.94 32.21 0.259SCR 05 13.71 30.0 15.92 12.28 17.16 0526-8257 23 -73 11.22 235.6 13.04 36.82 0.209 33SCR 05 14.18 14.74 10.92 28.3 16.06 0527-4928 24 11.37 -81 000.4 12.44 38.67 0.193SCR 40 05 13.95 15.21 11.11 16.58 0527-7231 09.8 25 12.47 -72 166.3 12.45 45.52 1.79SCR 49 05 12.67 0.222 14.26 11.11 17.03 0529-6157 14.5 26 11.92 -56 035.2 12.75 53.16 2.59SCR 04 05 13.72 13.89 0.181 12.15 18.44 0529-7330 05.5 27 11.89 -74 11.46 016.9 37.36SCR 25 05 12.51 15.18 0.251 1.67 11.68 15.88 0532-7405 26.0 27 12.23 -82 12.69 06.99 097.1SCR 57 05 12.47 16.47 0.251 2.98 11.63 0535-6019 23.5 29 10.83 17.27 -49 11.24 06.80 012.7SCR 61.7 28 05 12.97 13.78 0.417 1.61 11.99 0535-5103 16.7 29 12.15 -72 16.34 11.41 59.33 [162.9] 349.2SCR 50.4 31 05 15.11 0.283 2.98 10.60 0537-5612 15.73 20.0 32 10.67 -61 17.54 11.76 41.45 040.2SCR 57 05 11.82 0.236 3.35 11.96 0537-7817 14.7 35 14.36 10.93 -73 16.76 13.83 11.52 016.0SCR 30 05 0.368 3.35 14.45 10.48 57.8 0537-7421 36.0 35 16.19 11.13 -74 14.81 107.2 11.10 57.51 169.3SCR 05 05 0.195 3.84 10.71 13.25 0537-5730 58.2 37 14.92 13.26 -60 17.09 53.75 018.3SCR 13.63 19 05 0.269 3.18 10.85 65.3 14.06 0540-7700 00.9 37 12.89 10.47 -51 17.37 34.24 035.1SCR 03 05 12.56 0.198 3.28 12.99 84.0 13.15 0541-8013 48.7 37 15.13 -56 16.01 13.10 17.45 013.4SCR 12 05 12.44 0.189 2.52 10.24 73.1 11.35 0545-6210 17.3 37 15.45 -78 16.90 11.92 22.47 029.9SCR 17 05 12.43 0.218 3.02 56.6 13.13 0547-8034 27.8 40 13.97 12.86 -74 17.92 11.81 30.11 350.7SCR 21 05 10.03 0.402 2.48 95.4 13.45 0547-4804 26.6 41 14.66 11.79 -57 15.75 11.88 54.01 003.8SCR 30 05 12.12 0.217 3.42 45.7 11.77 0548-7800 53.0 45 16.06 11.56 -77 12.50 121.0 45.05 122.7 SCR 00 05 12.32 0.201 2.64 12.05 0548-5956 57.4 9.42 47 13.89 11.64 -80 18.56 11.48 55.31 041.2SCR 13 05 10.34 0.214 2.68 50.4 14.38 0550-7637 47.5 47 11.04 -62 11.74 53.02 138.9SCR 10 05 11.08 0.314 60.5 12.43 0550-6118 53.0 48 16.26 2.10 11.22 -80 17.65 9.21 09.73 024.8 34 05 12.66 0.331 48.8 10.36 03.9 9.76 48 1.80 11.52 -48 17.29 178.8 10.47 25.32 061.8 04 05 11.26 0.183 13.66 53.6 50 15.59 3.75 -78 11.39 12.10 56.67 007.8 00 05 10.03 0.215 [223.4] 49.2 25.8 50 15.60 2.49 10.24 -59 17.09 9.47 10.64 13.90 035.2 56 12.05 0.279 13.75 39.3 10.08 11.85 -76 17.24 331.7 140.4 37 0.215 13.84 13.1 9.47 15.38 3.02 10.43 -61 13.14 2.86 11.42 158.5 18 12.47 0.232 48.9 14.97 3.14 64.9 15.73 347.2 9.38 108.4 12.14 0.217 13.47 11.63 11.13 15.62 9.33 11.95 010.4 0.183 13.30 13.84 3.58 13.08 3.63 11.60 048.2 11.48 9.17 10.95 14.21 3.40 11.71 67.7 18.03 28.7 041.3 12.16 11.99 11.06 2.63 11.31 76.2 15.82 10.95 10.41 11.91 15.95 17.28 8.68 11.54 10.98 13.89 4.20 10.69 33.7 1.01 22.6 9.88 11.52 14.31 9.81 15.29 11.33 77.3 10.40 8.60 12.26 3.12 56.4 10.98 13.34 9.40 13.69 3.46 10.12 9.69 10.71 10.74 36.1 47.6 12.84 12.83 3.89 8.76 10.11 2.82 12.61 81.1 12.25 0.91 61.0 8.52 9.83 2.87 12.08 1.22 2.69 38.0 72.8 35.2 2.61 44.8 56.9 1.67 3.18 2.45 73.3 154.9 129.9 32.0 32.6 SCR 0454-8045A 04 54 40.35 -80 45 52.1 0.191 013.5 18.60 16.45 14.12 12.35 11.73 11.41 4.10 56.5 69 a d d a a d a d (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 0551-8116B 05 51 54.70 -81 16 08.4 0.233 019.5 17.74 15.74 13.70 12.17 11.64 11.37 3.57 56.5 SCR 0551-7604SCR 0551-7602SCR 0551-7510SCR 0551-7620 05SCR 51 0553-5821 28.71 05SCR 51 0554-5750 59.42 05SCR 51 -76 0556-7249 26.43 04 05SCR 47.4 51 -76 0556-7330 45.93 02 05SCR 49.0 53 -75 0557-6049 58.16 10 05 0.258SCR 51.6 54 -76 0600-5024 59.43 20 0.277 05SCR 56.3 -58 56 0601-7909 069.4 21 54.79 0.188 05SCR 35.0 -57 56 0602-5039 039.1 50 57.15 0.184 05 55.6SCR 17.10 57 -72 044.2 0602-7253 00.69 0.188 49 06 05.9 18.31SCR 00 -73 074.4 0606-7551 03.95 0.208 30 06 15.15 18.32SCR 59.4 01 -60 332.6 0608-7904 17.09 49 06 0.383 16.23 16.23SCR 19.8 02 -50 031.1 0608-7458 53.22 24 13.41 16.20 0.384 06 15.56SCR 20.9 -79 02 0610-5155 355.3 09 14.48 41.76 14.03 0.212 06 17.50SCR 31.4 -50 06 11.62 0610-6231 096.3 39 14.84 13.34 04.20 0.254 06SCR 00.0 16.55 08 12.55 0611-7302A -72 164.6 12.68 15.57 22.43 0.202 53 06SCR 11.14 10.6 16.25 08 13.19 0611-7302B -75 356.4 11.79 11.95 0.225 51 06 15.07SCR 12.02 18.20 24.2 10 11.10 0613-6312 -79 185.9 14.16 53.59 10.87 04 06 0.327SCR 06 14.36 12.74 14.71 44.6 10 10.93 0615-5807 11 -74 168.5 42.17 18.74 14.29 11.73 58SCR 16.21 06 0.180 10.50 16.56 59.4 13.31 0615-7615 11 -51 026.5 12.45 35.53 55 12.35SCR 12.51 0.295 10.37 16.99 04.3 0616-5827 -62 -73 13.08 021.4 10.27 31 06 14.05SCR 02 14.63 0.258 12.74 32.9 13 0616-6523 01.9 18.20 -73 10.76 59.54 139.6 10.11 06 10.24SCR 00 14.82 0.216 12.61 15 0617-5641 51.3 11.90 12.81 05.00 335.2 3.53 12.55 06 12.53SCR 0.242 0.188 16.31 15 0618-6704 10.25 -63 15.57 10.10 15.26 100.4 3.68 12 06 13.47SCR 12.46 0.190 27.8 16 10.67 0620-5655 12.27 -58 18.16 11.28 28.96 349.7 3.01 208.1 07 06SCR 16.28 43.3 16 13.37 0621-6131 -76 14.83 12.95 00.55 9.99 2.93 15 211.4 06SCR 9.46 0.235 11.97 10.03 54.6 17 16.46 0621-5022 10.70 -58 16.97 14.86 48.31 2.42 46.4 14.52 27 06SCR 0.410 11.55 20.3 18 13.64 0622-4956 12.35 -65 15.50 25.95 003.4 2.26 61.6 23 06SCR 0.373 10.47 13.91 117.1 57.4 20 14.89 9.21 0624-6539 13.17 -56 9.95 14.04 05.87 314.6 41 06 10.40SCR 0.181 1.99 12.19 12.84 00.2 21 0625-7705 13.36 -67 16.59 38.51 070.8 42.2 04 06 12.03SCR 0.255 12.73 11.92 00.4 21 13.81 0628-6921 -56 16.62 27.17 3.61 322.8 50.7 55 06 9.53 12.69SCR 0.183 3.41 175.8 32.8 9.81 22 14.51 12.11 0628-4757 -61 18.00 11.44 36.14 [166.8] 336.1 31 06 11.70 11.10 0.436SCR 22.2 24 14.45 -50 17.80 0629-6938 12.22 34.77 302.8 22 06 0.344 11.32 3.35 12.63SCR 9.44 46.7 25 16.15 2.42 11.12 -49 17.85 9.59 0630-7643AB 11.13 12.19 10.48 031.4 56 06 0.190 1.87 12.43SCR 29.1 28 15.75 12.14 -65 16.63 0630-5433 12.59 30.4 347.2 10.70 39 06 11.77 0.248 82.0 14.29SCR 25.6 28 15.77 1.79 06 10.86 -77 10.25 14.59 0630-7812 11.94 089.4 30 05 11.48 0.184 06 13.70 46.61SCR 22.8 14.73 -69 16.07 29 10.48 0631-6613 11.21 159.1 21 56.41 13.22 0.190 42.2 13.55SCR 34.7 12.66 33.5 -47 16.04 163.3 0632-6821 10.98 002.9 57 12.39 -76 0.269 [308.4] 06 13.16SCR 0.73 52.3 13.95 43 4.44 11.00 18.23 30 2.98 0632-6547 -69 12.74 120.8 08.9 12.47 35.71 0.186 38 06 10.74 13.71 0.96 10.70SCR 13.4 17.40 30 11.88 080.1 0632-6455 11.84 27.54 0.223 06 12.69 15.99 3.19 12.46 2.07 16.23 0.483 31 11.92 -54 150.0 10.39 38.62 33 06 12.00 0.473 15.16 11.62 17.98 2.04 43.7 32 11.24 -78 336.2 11.34 31.49 12 06 13.87 356.8 47.6 14.03 11.64 36.3 15.28 57.0 32 31.2 -66 176.2 11.04 153.6 36.22 13 12.45 9.87 15.98 0.231 06 2.74 11.04 16.47 33.5 10.72 -68 32 12.70 15.77 21 13.31 22.14 14.22 0.180 2.97 53.2 65.7 26.9 10.50 18.13 -65 11.20 126.4 47 14.59 14.08 0.237 2.93 10.48 69.4 27.9 9.60 12.19 13.56 11.70 -64 000.3 13.73 0.243 55 3.36 10.25 16.22 10.62 32.4 18.06 13.43 014.1 12.45 0.202 3.29 11.90 69.6 11.10 10.73 18.01 13.30 032.8 14.75 2.89 10.29 54.4 0.229 16.01 12.90 17.01 132.2 11.87 182.8 10.86 16.05 12.87 16.26 8.89 13.66 131.3 2.62 12.68 70.8 13.55 14.82 2.27 11.34 17.26 2.68 12.75 73.1 14.54 14.21 13.13 17.87 12.18 3.30 8.27 11.08 66.6 12.63 15.07 13.38 3.97 12.41 12.90 15.83 11.63 11.63 2.33 54.0 13.04 45.7 7.92 12.79 11.25 2.55 47.6 14.89 11.35 11.07 12.11 0.92 79.9 12.54 10.70 2.21 28.8 14.26 10.76 11.49 71.6 2.56 10.42 163.4 13.72 11.21 4.67 207.5 3.84 13.49 [183.8] 84.6 2.67 3.19 2.96 6.9 2.96 50.7 144.0 1.58 49.5 47.6 [318.5] 66.2 70 d d d d d d d d ··· (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 0632-6257SCR 0633-7405SCR 06 0633-6823 32 31.52SCR 06 0635-7021 33 45.91SCR 06 0635-5717 33 -62 37.96SCR 57 06 0635-6722 37.5 35 -74 28.01SCR 05 06 0635-7042 59.4 35 -68 22.66 23 06 0.216SCR 50.8 35 0635-7356 -70 48.81 21 06 0.196SCR 24.7 35 0636-6915 -57 036.2 10.90 17 0.297SCR 06 49.2 0639-6934 -67 35 001.6 22 27.14 0.184SCR 06 58.5 15.79 0639-6939 -70 36 004.6 42 45.99 0.193SCR 06 58.6 0642-4933 17.34 39 -73 202.3 22.30 0.383SCR 56 06 14.27 0643-6627 52.8 16.22 39 -69 355.3 08.43 0.319SCR 15 06 15.50 0644-5833 17.12 46.7 42 -69 340.0 03.29SCR 13.49 34 06 0.327 14.04 0644-4820 13.59 12.5 43 -69 015.1 23.77SCR 39 06 13.65 15.13 0.394 0645-6453 12.21 31.5 44 -49 13.18 014.4 20.77SCR 33 06 12.10 11.51 0.258 0646-6632 18.50 56.3 44 -66 12.39 58.47SCR 358.8 27 06 13.09 0.251 0647-6014 01.1 12.56 45 17.37 -58 9.84 11.16 17.24SCR 023.5 33 06 10.04 16.49 0.189 0647-8023 02.6 46 11.82 -48 18.29 11.76 10.32SCR 021.2 20 06 0.322 12.42 0648-5400 15.73 13.2 47 10.60 -64 13.68 39.84SCR 217.2 53 06 14.07 0.328 11.53 8.67 0648-6339 9.59 14.5 47 16.17 11.08 -66 14.60 32.16SCR 124.8 32 06 0.185 14.83 10.31 0651-6534 16.6 48 11.25 -60 16.73 12.44 42.51SCR 325.5 14 06 0.200 10.83 0651-6852 14.21 32.4 48 12.40 -80 8.54 17.44 8.99 40.63 337.4 13.91 23 06SCR 0.207 10.11 33.5 51 14.31 0651-5653 11.91 -54 17.78 10.14 340.5 00 06 12.85 0.204 1.09SCR 10.59 03.1 51 15.29 0651-6352 -63 17.44 13.32 48.81 186.3 7.96 39 8.72 0.316 06 3.12 11.63 12.18 44.4 15.76 -65 12.97 51 9.55 12.33 189.9 34 23.64 10.09 0.227 2.88 06 13.37 06.9 15.31 13.16 -68 16.41 51 [199.1] 004.8 52 11.13 54.41 0.264 3.37 13.54 7.69 37.5 10.92 12.08 16.18 -56 315.4 8.94 12.72 0.223 53 13.30 9.49 14.17 45.6 15.89 10.56 -63 354.2 12.28 0.186 76.8 52 14.05SCR 16.54 44.1 12.24 0654-5755 015.0 9.72 12.09 1.93 4.06 46.1 12.18 0.284 8.73 13.99SCR 10.29 18.77 9.25 11.67 0656-6415 341.4 46.8 12.17 14.47 0.193 1.81SCR 11.98 06 14.58 11.49 0656-7534 54 11.52 328.4 9.82 12.04 1.30 16.43 54.09 3.32 11.40 06 17.46SCR 56 11.63 0657-7219 139.4 12.65 13.50 04.11 11.20 06SCR 10.92 16.67 56 11.04 32.5 [252.1] 0657-7057 -57 52.2 13.94 15.48 00.99 55 9.17 11.08 06 13.95SCR 55.4 11.69 -64 57 12.92 1.70 0658-6038 3.18 10.65 15 14.74 06.32 2.31 10.46 06 05.1 12.48SCR -75 14.04 22.7 57 0659-5622 2.57 10.86 86.7 34 12.94 52.20 0.184 11.16 06.9 8.98 12.71SCR 06 -72 0700-5849 3.48 13.76 10.20 58 0.193 11.99 19 57.68 12.76SCR 24.0 06 0701-7710 -70 339.3 3.21 10.93 12.38 59 0.209 12.25 57 40.76SCR 07 12.80 32.6 33.4 0705-6348 167.6 11.69 38.3 00 -60 36.0 12.17 118.6 0.240 02.11SCR 38 07 17.28 12.40 0705-6730 000.3 24.5 2.66 12.16 01 -56 12.17 40.54 0.255 22 07 13.50SCR 2.42 11.89 59.2 47.4 05 0706-7606 126.7 -58 1.10 15.11 23.74 12.04 49 07 17.52 0.190 2.95 59.1 SCR 08.2 05 11.99 -77 152.2 0706-6507 11.96 41.28 10 0.238 07 16.10 2.78 24.6SCR -63 11.96 06 13.41 174.2 15.59 0707-7203 48 26.69 0.197 16.43 3.95 59.0 22.4SCR 07 -67 11.24 0707-6733 187.6 06 30 13.86 0.194 0.79 74.1 52.13 55.1 12.91 17.11 07 13.51 -76 41.7 011.9 07 14.39 0.270 06 2.72 44.9 58.68 11.07 25.3 07 15.80 356.2 13.47 07 -65 0.192 12.30 66.5 15.60 19.93 11.98 07 1.94 13.71 152.0 26.7 12.51 -72 10.48 54.1 0.289 13.48 03 17.94 0.53 12.40 162.6 017.1 12.04 31.4 -67 11.41 14.93 12.08 33 18.05 0.224 103.2 11.56 10.34 45.6 003.9 [147.2] 11.19 11.76 16.03 16.22 0.243 11.14 14.40 10.79 151.2 15.78 11.03 0.218 17.62 10.35 11.58 14.71 14.34 004.5 13.86 10.81 17.16 10.74 13.64 342.2 15.44 2.20 13.12 18.33 12.49 9.77 13.70 10.14 0.89 15.54 12.34 12.30 15.38 12.57 3.61 16.50 11.63 9.49 11.74 14.89 10.62 1.46 9.94 14.42 134.7 12.35 10.97 15.10 2.84 11.43 14.00 78.3 13.87 1.20 10.75 9.86 13.73 [126.5] 50.2 13.45 13.74 13.19 3.14 9.57 13.34 1.27 [357.2] 59.6 2.91 12.99 3.43 9.02 2.71 1.02 28.0 120.1 64.2 8.88 1.54 57.8 2.76 [250.4] 63.5 [269.2] 176.9 1.05 38.3 SCR 0651-8005SCR 0653-7657SCR 06 0654-5344 51 14.75 06SCR 53 0654-7358 33.51 06 54 -80 10.14 05 06 58.0 -76 54 57 06.30 00.0 -53 44 0.186 09.0 -73 0.202 58 03.6 124.7 0.194 092.3 0.467 16.96 162.8 18.45 020.2 15.21 15.68 16.49 18.18 13.23 13.70 14.81 16.23 11.81 12.34 13.01 15.10 11.30 12.10 12.53 13.98 11.07 11.50 12.23 13.47 11.30 13.28 3.40 3.48 1.60 2.25 57.3 88.0 116.4 [246.7] 71 d d (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 0708-7009SCR 0708-4715SCR 07 0708-4709 08 25.67 07SCR 08 0708-6706 57.82 07SCR 08 0709-5333 -70 32.04 09SCR 07 09.0 0710-5320 -47 08 15 52.28 07SCR 26.4 -47 09 0710-5441 09 31.74 0.268 07 30.6SCR 10 -67 0711-6336 29.04 0.209 06SCR 07 31.4 0712-6706 -53 017.5 10 0.402 33 03.73SCR 07 51.8 0714-8401 -53 134.3 11 20 0.246 28.67SCR 07 16.39 11.7 0714-8420 115.0 12 -54 04.69 0.287SCR 41 07 17.22 0714-7140 11.0 14 246.2 -63 14.50 50.04 0.211SCR 36 07 14.49 0716-5302 52.6 14 -67 100.6 15.18 23.83SCR 06 07 0.324 17.03 0717-5709 01.4 14 -84 327.5 12.54 12.48 26.18SCR 01 07 0.225 0717-7503 16.90 08.0 16 -84 13.12 143.0 29.38SCR 20 07 15.82 0.202 0718-5638 18.32 07.5 17 11.40 -71 11.58 10.92SCR 000.3 40 07 14.70 0.182 0718-4738 37.8 17 12.26 16.99 -53 36.58SCR 008.0 15.26 02 07 15.81 0.245 10.87 0719-5050 07.8 18 11.44 -57 17.48 56.25SCR 023.8 09 07 13.00 0.199 11.75 0720-7719 15.13 36.9 18 -75 16.48 14.71 22.82SCR 349.3 10.64 03 07 13.41 0.238 10.90 0721-5809 41.6 19 15.21 -56 16.81 12.46 35.35SCR 336.9 11.46 38 07 0.204 14.08 0723-4921 18.9 14.65 20 14.49 -47 16.25 12.27 53.31SCR 335.5 10.76 38 07 0.331 0724-6212 13.21 36.7 21 14.96 11.95 -50 18.06 56.23SCR 354.3 13.80 50 07 0.325 14.47 0724-5949 12.69 52.4 23 14.10 11.67 -77 15.99 42.22SCR 353.4 19 07 12.18 0.304 11.69 0725-6043 13.23 12.3 24 16.01 -58 17.80 13.19 55.01SCR 331.0 3.10 09 07 11.55 0.216 11.40 0726-4810 12.56 39.6 24 14.43 -49 17.35 11.60 51.92SCR 350.9 2.92 21 07 12.18 0.211 0726-5419 13.73 16.7 25 15.76 13.05 -62 17.62 10.90 31.55SCR 107.3 1.04 12 07 11.57 0.230 0726-4954 11.64 27.1 26 15.16 11.35 -59 18.75 11.62 27.19SCR 095.4 49 07 11.72 0.191 1.11 0727-6145 13.63 57.3 26 15.59 10.70 -60 16.00 11.00 26.43SCR 306.7 52.2 43 07 10.84 0.188 2.24 0727-6032 12.71 46.2 26 16.43 11.40 -48 18.09 11.09 39.48SCR 350.7 81.1 10 07 12.54 0.217 3.54 0727-5912 13.26 20.0 27 13.74 10.78 -54 17.99 10.30 09.95SCR [479.6] 334.7 93.6 19 07 11.67 0.217 0727-6056 14.09 26.9 27 16.05 1.33 10.77 -49 17.15 11.97 07.59SCR 082.0 54 07 12.27 0.335 0728-5946 10.88 58.4 27 16.03 3.04 10.00 -61 16.35 115.6 11.09 11.02SCR 280.3 45 07 12.67 0.200 0729-4804 13.98 06.9 27 15.10 2.94 11.67 -60 16.91 11.66 41.21SCR 000.0 32 07 10.33 0.260 [267.4] 54.0 0730-6335 13.84 21.8 28 14.07 2.78 10.80 -59 17.33 12.13 40.40SCR 009.2 12 07 13.11 0.277 0731-4807 13.60 33.8 29 15.19 2.52 11.45 -60 17.78 21.66SCR 308.0 56 07 12.43 0.271 0731-5748 11.94 52.2 9.74 30 15.16 4.29 11.84 68.1 -59 17.66 12.64 52.89SCR 150.4 46 07 12.52 0.202 0732-5908 13.44 46.3 31 15.75 3.59 54.3 -48 17.90 11.88 08.08SCR 312.0 04 07 10.93 0.219 0732-7213 12.96 27.3 31 15.42 3.22 12.42 85.5 -63 18.28 9.48 11.97 30.89SCR 358.6 35 07 12.13 0.238 0732-6028 13.98 20.0 32 15.90 3.50 11.62 66.4 -48 17.42 10.36 43.90SCR 342.2 07 07 11.72 0.304 0733-5357 14.53 33.3 32 16.29 3.32 11.73 29.8 -57 16.18 11.61 13.72SCR 145.2 48 07 12.69 0.348 0733-5514 13.63 38.9 32 15.51 3.76 10.10 35.6 -59 12.61 11.20 58.86SCR 047.1 08 07 13.17 0.235 0734-5653 14.47 16.8 33 14.22 11.39 76.0 -72 17.47 12.21 06.88SCR 124.0 13 07 12.28 0.188 0734-6032 13.67 43.1 33 10.71 2.94 10.90 45.0 -60 13.95 3.42 12.66 52.39SCR 317.6 28 07 12.98 0.202 0735-5551 12.50 53.9 34 15.53 3.60 11.98 67.3 -53 16.31 11.81 03.92 345.6 57 07 12.38 0.343 28.0 34 11.54 2.58 12.42 61.4 -55 17.72 12.41 51.27 340.7 9.98 14 07 11.53 0.338 13.73 51.2 35 14.00 3.14 11.50 -56 18.26 11.89 24.04 104.7 128.1 53 0.190 10.20 17.6 15.59 3.07 12.15 -60 17.85 10.06 26.6 10.92 350.5 32 12.25 0.192 11.82 50.0 16.28 3.44 11.65 63.8 -55 17.65 332.4 102.9 51 10.02 0.215 13.00 12.3 15.88 3.06 10.69 17.62 11.60 155.9 9.48 10.80 0.228 14.27 15.46 2.25 36.8 17.44 318.0 11.32 0.206 14.15 9.44 15.70 3.62 11.38 77.4 16.53 10.22 000.0 12.86 14.30 9.37 15.58 3.31 47.8 17.44 10.77 307.6 12.79 14.04 14.61 3.13 95.9 17.25 9.19 12.26 155.4 12.96 9.98 13.60 15.22 2.70 10.41 15.75 12.21 12.59 12.74 15.25 12.06 60.8 12.42 12.25 13.67 13.86 3.28 11.92 89.7 11.99 11.51 13.09 0.65 12.25 81.8 11.64 12.42 11.99 11.73 61.5 1.52 10.90 11.64 3.20 4.27 11.35 11.79 11.18 3.42 10.60 63.5 11.08 57.4 3.09 11.57 10.60 2.51 10.78 43.3 33.7 3.11 10.39 26.1 3.33 83.0 3.10 88.9 130.9 2.80 3.61 81.3 2.69 63.0 49.0 81.6 42.3 55.7 72 e d a c a d a c a d (pc) Est Dist Notes J − F 59 R s JHK ··············· IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 0735-8148SCR 0736-7615SCR 0736-5320SCR 07 0736-4844 35 03.82SCR 07 0738-5120 36 06.13SCR 07 0739-4814 36 -81 52.24SCR 48 07 0740-6418 49.6 36 -76 57.47SCR 15 07 0740-5532 30.6 38 -53 47.92SCR 20 07 0.195 0740-7212 36.4 39 -48 46.92SCR 44 07 0.226 0741-7045 53.1 40 -51 32.95 320.2SCR 20 07 0.196 0742-5612 04.7 40 -48 59.64 341.0SCR 14 07 0.283 0742-5555 50.1 40 -64 17.23 00.80 126.5 18 07 0.185SCR 11.0 41 0742-7814 -55 17.74 03.24 020.0 32 07 0.192SCR 12.1 42 15.39 -72 16.39 0743-6038 26.10 341.1 12 07 0.181SCR 27.8 42 15.60 -70 16.11 0744-5553 02.04 323.3 45 0.218 07SCR 14.30 02.4 14.42 -56 16.46 42 0744-5005 351.1 12 10.63 0.481SCR 07 13.12 13.9 14.05 -55 17.95 0744-6941 43 343.1 55 12.92 06.21 0.216SCR 07 12.95 46.8 14.26 18.17 0745-4814B 44 -78 003.7 11.98 21.11 0.221 14SCR 07 11.94 15.93 56.2 18.21 0745-4814A 44 12.33 -60 327.1 11.93 33.71 0.285SCR 38 07 11.89 16.37 07 17.24 0747-7844 36.4 44 11.35 45 -55 334.9 11.15 35.17SCR 29.37 53 14.15 0.279 07 16.31 12.10 17.86 0748-5352 11.2 11.36 45 -50 062.0 10.73 32.21SCR 05 15.49 15.27 0.207 11.07 14.18 0748-4712 51.3 10.56 -69 -48 13.01 090.7SCR 41 07 14.94 15 15.83 0.187 11.14 17.59 0749-4955 58.0 47 10.22 29.7 -48 55.87 318.3SCR 07 13.30 14 12.11 0.222 10.35 0750-6641 48 56.5 12.40 18.22 13.91 16.92 351.6SCR 07 13.69 15.51 0.441 0.201 0750-5526 48 -78 16.09 11.76 13.28 9.97 323.4SCR 44 07 11.33 0.200 2.47 12.16 0751-6703 16.10 43.0 49 13.32 -53 14.72 12.09 29.43 001.2 52 176.0 07 13.63SCR 3.61 34.5 50 14.07 11.26 0752-5618 -47 17.43 10.61 07.08 174.9 12 07 0.191 2.49 15.48 13.13SCR 46.5 50 12.77 11.57 -49 17.14 0752-4709 19.26 12.35 27.88 55 07 0.181 2.90 10.99SCR 12.11 05.5 51 15.58 -66 129.1 0752-6130 18.00 18.84 358.7 14.50 41 9.93 0.259 07 11.25SCR 11.66 11.3 15.04 11.88 17.05 -55 52 0753-6438 3.54 118.9 26 15.18 11.25 0.257 2.92SCR 47.7 07 13.24 46.4 15.80 -67 10.89 0755-8714 13.97 52 311.6 03 10.83 30.88 0.258 11.61SCR 82.6 07 13.38 34.4 13.92 9.77 11.90 0756-5434 52 -56 10.64 150.9 12.04 19.42 0.236 18 2.40SCR 48.4 07 13.14 10.45 13.92 01.4 15.88 0757-5828 53 10.21 -47 000.3 12.17 43.19 0.185 11.99 3.51SCR 09 07 10.41 10.40 16.64 107.7 0757-7444B 47.0 55 11.53 30.5 -61 150.1 11.57 41.28 3.74SCR 30 07 0.201 13.99 10.04 17.52 0757-7444A 54.0 56 11.69 -64 064.1 11.38 9.62 48.70SCR 38 07 14.74 07 0.207 11.28 16.54 215.6 0758-4906 24.5 57 57 11.03 -87 9.57 134.0 22.40 3.16SCR 06.96 14 12.33 07 15.41 0.245 1.50 11.41 12.33 0758-5524 11.06 40.3 57 -54 328.1 08.94SCR 49.8 34 9.67 12.34 14.43 0.195 1.61 10.74 0758-7023 57.1 18.00 -58 -74 11.62 335.5SCR 49.2 28 9.37 07 13.53 44 11.19 0.279 2.82 0759-5504 42.5 58 46.8 17.51 -74 10.93 06.06 336.1SCR 07 12.74 44 0.446 1.94 0759-5816 9.28 16.26 58 53.7 11.07 17.89 12.02 33.95 [374.2] 344.1SCR 76.6 07 10.63 0.223 58.5 3.55 0.180 0759-6640 8.80 58 15.13 10.25 -49 14.67 11.59 19.98 324.2SCR 06 07 0.197 15.39 2.87 10.83 0800-6516 5.06 36.5 59 15.80 11.54 -55 16.88 9.20 16.02 135.7 24 048.0 07SCR 50.7 4.24 12.91 9.82 31.7 59 12.51 11.02 0801-5706 -70 17.85 8.67 21.12 9.96 050.9 14.48 23 07 0.180 11.31SCR 60.3 13.19 43.3 59 14.97 -55 18.28 0801-5524 18.65 08.66 04 08 11.74 0.197 10.76 59.3 11.51 05.3 00 15.90 -58 14.00 13.93 9.48 06.75 005.6 16 11.70 0.285 08 78.7 12.92 25.7 48.3 16.35 16.31 -66 01 11.16 136.2 40 45.09 10.62 0.211 2.37 08 13.55 31.4 52.0 13.66 12.18 -65 17.20 0.78 01 11.07 316.5 16 11.78 9.39 49.91 0.200 14.28 37.7 14.45 10.82 18.12 1.04 -57 3.81 325.9 11.85 0.182 06 3.39 11.31 9.99 15.32 10.72 00.9 17.71 11.19 -55 162.8 12.78 0.278 13.58 2.84 24 16.09 18.04 55.2 11.27 154.0 11.44 77.6 13.72 0.227 15.82 10.94 16.21 52.2 9.77 12.26 170.0 13.05 14.30 15.97 0.365 1.77 10.97 14.29 35.2 26.3 10.77 12.70 1.38 001.4 59.2 13.76 14.60 3.39 12.00 16.91 12.86 12.87 358.1 57.4 14.53 13.35 4.10 10.66 12.16 18.27 12.35 [318.4] 12.99 14.93 12.31 16.60 13.14 12.75 3.19 11.93 16.39 1.89 11.73 11.83 44.9 13.41 4.05 12.07 44.1 14.74 12.58 12.07 3.57 15.64 11.48 32.2 2.73 11.23 12.27 12.35 0.75 13.23 11.69 14.44 11.02 56.4 52.3 11.75 12.31 2.62 11.60 38.1 13.82 158.5 3.23 11.48 77.3 11.76 3.46 99.4 13.61 2.84 11.56 115.9 2.77 1.28 90.0 2.66 62.9 120.3 1.95 74.1 2.43 122.6 [307.9] 90.4 105.9 73 d d d d (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 0802-4704SCR 0802-6514SCR 08 0802-6924 02 21.25SCR 08 0803-8146 02 59.51SCR 08 0805-7843 02 -47 21.46SCR 04 08 0806-6439 31.7 03 -65 42.37SCR 14 08 0806-7057 39.4 05 -69 05.10SCR 24 08 0.302 0807-7013 31.1 06 -81 00.38SCR 46 08 0.184 0807-6734 22.7 06 -78 37.38SCR 303.4 43 08 0.255 0808-7157 37.0 07 -64 48.58SCR 339.1 39 08 0.182 0809-6136 21.7 07 -70 16.06 48.01SCR 346.7 57 08 0.184 0810-7002 30.3 08 -70 16.72 14.27SCR 338.2 13 08 0.199 0812-6402 39.2 09 14.00 -67 17.96 47.54SCR 159.4 34 08 0.252 0813-4932 35.4 10 14.66 -71 15.74 02.72SCR 110.5 57 08 0.192 0813-7836 11.98 17.7 12 16.19 -61 12.34 23.34SCR 332.9 36 08 0.323 0814-4806 13.55 36.3 13 14.06 -70 16.78 54.88SCR 279.4 02 08 11.45 0.270 0814-6917 14.26 12.9 13 10.51 -64 16.37 16.27SCR 096.2 02 08 12.36 0.217 0815-7632 12.79 23.8 14 14.74 -49 15.82 10.81 54.56 313.2 32 08 12.91SCR 0.192 10.09 32.1 14 14.37 0815-5737 -78 15.43 11.80 38.83 341.9 36 08 11.22 0.409SCR 12.81 42.1 15 13.77 10.59 0815-4710 -48 16.77 12.39 33.04 130.9 06 0.294SCR 08 12.96 19.5 13.43 11.58 0816-5103 -69 15.75 15 9.67 10.62 340.0 17 57.14 11.26 0.199SCR 08 11.93 44.8 14.39 12.16 0816-6804 -76 17.67 15 153.0 32 11.84 00.37 0.377SCR 08 12.08 26.6 13.75 10.32 0817-5600 17.07 16 -57 10.69 144.1 9.16 10.78 34.92 0.234SCR 37 08 12.56 15.82 0817-4714 36.4 16.88 16 11.23 -47 326.8 10.82 43.77 0.238SCR 10 08 11.96 15.22 2.56 10.43 0818-6326 16.20 50.1 17 10.20 -51 348.0 11.22 25.20SCR 03 08 13.81 0.181 9.02 15.31 2.29 11.00 0819-6734 15.10 16.6 17 10.23 -68 334.6 10.86 52.35SCR 04 08 13.25 14.15 0.186 3.28 0820-8003 16.87 16.1 18 10.63 -56 12.51 146.4 29.76 9.98SCR 00 08 13.68 12.74 0.305 2.84 10.00 0822-7225 15.53 45.4 19 10.23 -47 11.79 52.39SCR 156.5 14 08 12.41 15.04 0.227 10.35 61.7 0823-6957 53.4 20 11.98 15.77 -63 106.5 11.97 03.38SCR 337.0 26 08 11.03 13.62 0.194 3.48 10.00 0823-6558 25.3 22 11.32 -67 18.26 11.50 41.73SCR 049.4 34 08 13.55 0.84 0.260 2.53 11.75 99.5 0823-5545 14.65 00.3 23 11.45 -80 17.61 10.33 02.11SCR 339.2 03 08 12.27 0.223 11.03 49.8 0823-5908 14.8 23 16.24 10.90 -72 16.47 12.52 45.87 2.99SCR 332.6 25 08 0.188 2.61 14.03 11.25 0823-7056 01.7 23 15.88 -69 14.50 11.17 56.79SCR 319.0 57 08 9.74 0.211 3.16 10.64 37.4 0824-5351 14.78 02.2 23 14.42 11.97 -65 17.30 07.67 311.5 13.61 58 08SCR 37.1 0.269 2.89 74.3 13.68 04.6 23 12.95 0824-4701 10.55 -55 17.78 06.76 299.1 45 08 13.97 0.202SCR 3.31 11.73 12.76 23.4 24 15.28 9.51 0824-6721 -59 18.31 13.15 25.32 38.3 336.2 08 12.20 0.214SCR 08 3.43 10.34 45.4 12.26 33.2 15.79 0828-6511 -70 14.96 24 13.40 302.9 56 02.09 11.87 0.187SCR 3.33 38.2 08 12.80 46.9 16.26 13.08 0828-4927 -53 16.16 24 11.65 319.6 51 11.31 03.21 0.196SCR 2.65 40.2 08 14.14 44.4 12.77 13.15 0832-6900 16.66 28 -47 11.37 324.9 11.82 17.92 0.207SCR 01 79.9 08 14.29 14.09 11.40 0832-5823 50.0 16.56 28 10.68 -67 337.4 12.67 31.20 0.188 2.51 54.3 21 08 11.79SCR 14.45 2.41 11.12 13.91 50.4 32 0833-5338 11.25 -65 172.0 12.54 12.66 2.45 65.8 11 08 11.97 0.187 14.48SCR 10.58 12.65 21.3 32 12.19 0834-6212 -49 135.0 11.06 13.24 60.1 27 12.54 12.35 0.403 1.05 08 10.94 15.42SCR 29.7 11.96 -69 33 10.70 0834-6825 345.7 00 12.90 11.34 10.83 0.185 2.27 11.94 08 16.26 110.5 48.3SCR 10.47 -58 34 11.20 0834-5808 288.9 23 11.65 13.27 07.95 0.311 37.7 3.68 11.71 40.7 10.11 08 16.00 11.52 -53 [241.3] 325.6 57.5 34 14.26 0.228 38 2.55 10.25 19.75 10.58 37.6 08 17.54 9.88 10.86 -62 348.6 11.56 34 0.258 1.64 12 14.25 47.35 10.92 16.56 225.4 08.3 9.85 062.4 12.88 -68 3.46 10.33 0.212 15.29 10.21 25 17.39 10.56 328.6 01.3 9.56 -58 13.29 3.12 10.69 58.8 14.55 0.251 08 18.51 11.75 31.7 132.6 3.72 10.07 80.5 13.13 15.86 18.54 0.237 12.96 9.98 326.8 1.71 76.9 12.76 8.92 16.12 11.16 0.197 18.54 11.55 50.7 13.63 107.7 16.40 12.45 3.39 16.17 11.72 3.25 10.91 91.3 13.87 9.73 271.7 16.43 8.76 10.95 12.75 18.49 2.97 59.8 14.10 12.28 14.19 11.08 12.83 17.59 1.49 69.2 15.39 10.69 12.23 16.49 12.59 10.89 12.95 12.34 30.1 15.52 38.0 14.19 12.04 12.05 15.45 2.51 52.5 12.20 2.71 12.08 1.27 13.62 13.71 63.1 1.29 11.75 14.36 11.70 3.74 11.98 13.48 13.87 2.84 11.44 [190.3] 71.8 11.42 37.8 3.10 37.3 13.66 3.29 11.15 3.82 36.0 62.5 2.24 111.3 1.98 87.1 2.12 [263.8] 59.0 3.54 115.5 [305.2] 50.2 74 b a d a d a d (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 0834-5529SCR 0835-7447SCR 0836-5434SCR 08 0837-5020 34 03.60SCR 08 0838-5855 35 45.48SCR 08 0839-6507 36 -55 56.45SCR 29 08 0840-7344 53.2 37 -74 31.39 47 08SCR 36.3 38 0840-7826 -54 02.24 34 08 0.196SCR 30.9 39 -50 0842-5737 53.47 20 08 0.228SCR 10.3 40 -58 0843-5154 51.26 291.7 55 0.217 08SCR 58.7 -65 40 0843-5007B 118.7 07 29.00 0.186SCR 08 39.1 -73 14.74 0843-5209 42 318.3 44 30.10 0.320SCR 08 22.5 08 17.59 0843-7005 43 -78 43 184.9 11.05 0.215 26SCR 15.84 12.62 46.0 18.16 0843-6330 -57 188.9 0.207SCR 37 08 15.83 14.82 0843-7831 25.4 43 -51 357.4 -50 38.82SCR 54 08 10.92 0.399 07 16.17 18.44 0844-7120 03.5 43 24.8 154.0 05.16SCR 08 13.91 12.73 0.188 15.14 0845-7645 43 -52 10.26 010.3 01.06SCR 09 08 13.87 16.11 0.402 0.225 16.79 0845-6041 27.4 43 -70 12.46 58.71 301.9SCR 05 08 11.06 13.16 0846-7455 38.5 44 16.06 -63 12.05 54.59 310.7SCR 30 338.8 08 12.44 9.62 15.00 0.482 0846-4933 37.9 45 11.85 -78 16.45 11.28 09.00SCR 31 08 11.75 0.184 0847-5749 15.83 50.3 45 11.46 -71 16.09 16.64 10.31 26.61 307.3SCR 20 08 13.64 0.385 11.58 0847-5346 42.9 46 14.34 9.40 10.64 -76 10.85 47.08 328.5 45 08 0.195SCR 15.77 11.17 08.3 46 13.94 14.85 0847-7928 -60 16.41 12.58 40.07 135.6 41 08 9.71 0.201 10.34SCR 12.52 11.7 47 10.23 -74 17.86 0847-7346 22.86 325.3 15.62 55 08 0.194SCR 12.36 21.0 47 14.29 12.81 11.97 -49 17.19 0848-6018 17.22 311.3 33 11.49 0.201 08 10.04SCR 49.9 15.81 9.27 -57 11.75 47 0849-7657 15.57 002.3 49 16.19 11.76 0.305 11.93 3.37 11.83SCR 08 12.57 00.5 15.04 2.37 -53 15.11 0849-5903 47 10.95 316.5 46 56.02 0.180 4.12SCR 08 14.00 07.9 10.09 15.48 17.21 0850-4934 48 -79 11.21 287.1 11.41 11.87 25.36 0.183 28 1.45SCR 08 12.92 13.08 10.68 34.1 14.56 0851-6638 49 -73 107.8 12.73 51.94 0.263SCR 46 08 15.16 10.96 15.18 0852-4948 11.15 32.2 49 11.38 -60 317.5 9.50 11.60 46.41 2.31SCR 70.4 18 08 11.04 0.210 12.47 5.80 37.6 17.61 0852-4912 57.3 50 12.09 -76 293.3 24.91 2.42SCR 39.7 57 08 13.44 13.11 0.184 11.11 18.35 0852-6624 07.4 51 11.02 -59 10.25 299.4 41.68SCR 75.3 03 9.26 08 11.21 15.86 0.232 0.21 11.88 17.45 0852-6344 33.7 52 -49 12.12 06.43 339.5SCR 34 08 11.56 16.28 0.334 2.85 10.74 0853-7323 23.9 52 17.46 -66 10.06 14.32 323.7SCR 53.0 38 08 14.37 9.57 15.29 0.267 2.18 119.9 0853-7705B 8.82 2.92 38.4 52 11.56 -49 17.40 10.60 8.4 21.42 [763.9] 305.5 48 08 14.21 0.469SCR 15.73 00.3 52 0853-5213 -49 18.30 12.85 35.02 280.7 12 08 13.38 9.45 08 0.191 2.42 11.29SCR 11.4 53 15.36 9.30 10.00 54 -66 17.57 0853-7705A 8.64 12.94 36.15 295.5 32.74 24 0.305 3.08 14.89SCR 56.3 30.5 16.19 12.28 -63 18.34 0854-5406 11.85 114.8 44 0.183 08 3.44SCR 84.5 13.65 74.1 08 40.8 15.58 9.21 12.35 -73 17.41 53 0854-6138 -77 53 9.73 318.4 13.90 23 22.74 06 0.232 26.75 12.04SCR 13.95 12.9 16.23 11.32 27.8 16.46 0854-7036 151.1 12.40 0.240 12.07 84.1 08 13.30 15.59SCR 17.61 13.35 54 -52 0854-6640 011.9 -77 12.78 10.76 0.191 13 3.04 11.05 86.6 0.225 08 14.31 05 14.42 2.83SCR 25.1 16.34 0.82 54 50.6 11.87 153.0 0854-5051 11.68 32.11 43.2 08 13.46 15.76 13.24SCR 16.29 54 12.16 -54 315.0 0854-7246 293.2 13.19 47.92 06 12.50 0.217 14.35 2.41 0.211 08 11.61SCR 16.25 08.0 11.12 2.51 -61 54 0855-4932 12.22 3.00 38 13.28 59.15 14.26 11.91 08 15.93 10.4 17.61 12.62 -70 54 11.46 129.2 3.34 67.6 306.7 36 12.84 14.43 14.54 0.349 29.8 10.77 08 15.0 32.1 11.77 54 12.10 -66 3.44 13.28 13.96 54.53 0.193 40 12.38 16.13 08 10.84 15.72 12.8 15.99 55 12.07 -50 323.7 12.35 35.37 0.186 1.83 33.4 11.51 51 102.9 11.57 41.5 30.0 12.44 -72 286.4 12.15 14.03 2.96 10.61 46 14.73 0.199 11.46 14.06 16.69 52.3 11.08 -49 134.0 84.5 3.41 11.28 32 0.240 11.78 17.35 43.2 10.78 [269.0] 12.51 49.8 114.6 3.90 13.77 11.26 12.32 14.34 0.214 10.58 16.11 178.4 3.04 11.60 15.20 0.258 10.24 12.01 16.15 13.16 11.24 321.2 3.37 10.26 82.8 13.02 13.98 17.97 315.1 2.96 76.7 13.00 11.75 14.56 12.68 9.94 10.71 17.16 11.88 3.66 36.6 12.20 112.5 16.19 15.87 12.08 2.28 12.54 13.76 10.43 15.31 11.30 11.25 1.82 72.2 13.89 14.05 11.57 3.35 52.0 13.04 11.09 13.73 10.63 56.3 3.62 12.54 11.30 12.45 3.19 12.44 94.2 12.35 10.41 126.2 11.97 11.47 1.56 2.82 12.33 11.78 39.6 11.73 10.90 76.2 2.46 11.60 34.8 [203.2] 3.12 10.72 2.73 52.6 1.53 75.3 3.65 68.3 2.96 [180.8] 51.4 2.57 68.9 85.0 68.2 75 b d d d d a a d d ··· (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 0856-6342SCR 0857-7001SCR 0857-4859 08SCR 56 0857-6032 16.84 08 57 20.03 08 57 -63 45.31 42 08 47.4 -70 57 01 08.21 05.7 -48 59 0.190 28.3 -60 0.184 32 45.4 302.0 0.233 124.9 0.217 16.52 181.1 17.44 333.3 14.31 16.96 15.49 15.21 12.54 15.60 13.64 15.38 11.56 13.36 12.49 15.46 11.00 11.77 11.96 15.94 10.72 11.17 11.71 16.20 10.96 15.78 2.75 3.00 3.83 -0.56 58.3 87.9 48.4 SCR 0858-5857SCR 0858-7707SCR 0858-6743SCR 08 0858-7041 58 01.63SCR 08 0859-5445 58 12.98SCR 08 0859-7517 58 -58 02.38SCR 57 08 0904-6233 25.3 58 -77 48.35SCR 07 08 0904-4851 38.8 59 -67 43.67SCR 43 08 0.272 0905-5509 49.3 59 -70 51.95SCR 41 09 0.226 0905-7534 54.1 04 -54 12.83 301.4SCR 45 09 0.207 0905-7936 00.2 04 -75 47.84 124.8SCR 17 09 0.206 0907-5627 30.3 05 -62 16.44 33.33 344.5SCR 33 09 0.342 0907-6600 24.3 05 -48 18.15 33.46 334.2SCR 51 09 0.291 0907-4810 24.0 05 14.42 -55 17.94 33.75 345.1 09 09 0.185SCR 01.6 07 16.29 0908-7506 -75 16.35 12.71 330.7 34 09 0.185SCR 12.53 12.2 07 15.88 -79 17.85 0908-5336 03.05 342.3 36 09 0.243 14.78 29.2 07 14.16SCR -56 14.64 45.41 0908-6649 313.7 27 11.56 0.182 09 13.69 37.3 16.02SCR -66 14.80 08 305.8 0909-6311 00 01.94 13.57 0.259 09 12.19 47.9 12.66SCR -48 17.58 08 11.00 340.3 0910-5643 10 12.15 34.46 0.215 13.85 41.2 12.58 09SCR 18.37 -75 13.03 337.0 08 0910-7645 11.03 0.186 06 10.96 14.05 15.80 10.75SCR 25.5 09 17.98 11.57 -53 304.6 0912-6917 09 12.28 0.187 36 12.50 16.49 19.02 12.81SCR 09 17.73 21.1 10.47 076.6 0912-5444 10 -66 13.54 0.239 16.10 48.06 49 11.28SCR 09 12.93 9.86 11.77 309.7 40.7 0913-6918 10 11.92 -63 14.35 15.90 12.91 0.315 10.20SCR 11 09 17.68 0914-7304 25.5 12 11.49 318.0 -56 14.78 10.82 38.97 11.53SCR 43 09 15.12 0.232 11.34 0915-4737 22.3 12 9.24 12.58 -76 021.5 14.42 15.73 06.02 2.86SCR 45 09 0.286 10.94 18.09 0915-5246 46.2 13 13.61 -69 10.13 022.3 13.05 32.37 2.72 11.18 17 09 0.220SCR 12.04 17.88 07.9 14 13.15 0917-5836 -54 13.22 9.03 53.85 330.8 3.73 10.60 44 09 16.26 0.271 13.05SCR 04.1 15 17.43 -69 0919-6246 11.93 36.93 358.5 3.13 11.81 18 09 9.79 15.70 0.245 12.63 19.0 15 11.67SCR -73 18.32 07.86 0919-6112 349.3 3.75 15.51 12.86 59.0 04 0.288 09 166.0 15.22 19.3 10.88SCR -47 15.49 17 110.6 12.38 0920-6216 37 13.51 23.69 0.180 11.11 09 41.1 9.22 16.25SCR -52 16.50 14.47 19 230.8 0.67 49.4 0920-7557 46 32.16 0.182 10.25 14.01 48.9 13.14 09SCR 16.57 12.94 2.79 -58 314.1 4.31 10.81 38.9 19 0920-6054 0.186 36 14.78 44.98 13.84 14.49SCR 25.1 09 16.71 9.09 -62 319.4 3.90 10.04 59.7 0921-7523B 13.41 20 0.207 46 10.71 14.12 13.73 12.39SCR 09 16.88 04.9 121.9 2.49 0921-7523A 20 13.56 -61 13.56 12.80 0.276 14.44 27.75 12SCR 09 16.00 12.79 09 333.4 44.6 2.76 93.2 0921-5524 20 10.62 21 -62 12.22 12.02 14.83 48.42 0.299SCR 20.88 16 12.72 09 27.0 13.06 29.7 0923-5348 19.9 11.59 281.2 21 -75 11.59 13.84 12.58 23.73 57 18.53 0.204SCR 10.00 4.06 61.4 24.8 11.09 0923-7648 -60 322.3 -75 12.55 185.6 11.85 12.81 54 09 23 0.202 1.03 11.03 16.31SCR 2.16 33.0 21 11.39 09.9 0924-7422 -75 11.87 135.1 169.2 16.45 55.10 09 23 0.262 10.51SCR 17.64 23 11.38 18.8 1.80 9.77 0925-7609 11.42 47.45 315.8 10.83 14.04 0.185 10.90 09 0.286 10.50SCR 18.29 -55 2.76 23 14.66 0926-6416 272.5 10.24 24 41.75 15.45 10.88 0.291 09 35.9 46.5 11.33 -53 18.03 24 1.82 132.0 12.92 10.60 48 316.3 31.20 43.4 [315.1] 09 54.2 15.99 21.4 13.72 16.03 25 -76 9.87 2.69 10.64 321.1 13.10 59.21 0.240 10.98 48 15.68 09 45.7 12.94 12.72 17.94 -74 26 121.9 0.219 13.11 14.97 22 18.08 13.96 2.52 [195.5] 17.16 06.6 12.19 -76 329.0 2.90 10.95 9.61 09 12.94 0.368 12.17 10.84 16.14 24.1 142.5 3.04 12.91 13.96 -64 11.82 162.1 0.181 11.65 16 15.14 15.39 22.6 3.05 11.54 289.2 12.00 0.181 14.11 14.81 13.43 3.45 9.81 11.12 182.1 11.43 13.11 13.46 40.9 0.249 10.96 18.04 59.7 054.0 12.65 13.26 13.27 10.55 16.30 0.52 39.9 11.97 3.34 9.76 11.55 306.6 10.65 16.38 17.62 12.10 2.73 51.7 12.41 10.26 14.08 11.39 44.3 11.66 17.68 1.32 15.81 9.19 11.92 15.51 12.79 3.26 11.17 12.02 11.16 95.3 15.77 26.3 14.60 165.2 2.03 13.92 12.23 [163.6] 8.95 11.17 4.14 10.91 15.12 14.14 12.61 2.83 12.08 10.58 [251.3] 68.0 14.39 3.49 13.99 12.08 3.17 10.28 13.86 30.8 11.83 1.09 1.80 47.7 13.67 0.48 80.4 62.2 1.78 2.91 39.9 93.0 2.90 193.7 [326.7] 1.37 44.6 [340.1] 92.4 76 a c a c d d ··· (pc) Est Dist Notes J − F 59 R s JHK ··············· IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 0927-6239CSCR 0927-6239BSCR 09 0928-5906 27 20.99SCR 09 0929-5857 27 10.53SCR 0930-5325 -62SCR 09 37 0930-5107 28 04.1 -62 34.74SCR 09 39 0930-8341 29 50.9 28.11SCR 09 0.197 0930-5056 30 -59 21.91SCR 06 09 0.204 0931-5558 01.5 30 -58 08.98SCR 57 309.0 09 0932-6152 20.5 30 -53 56.74SCR 25 312.2 09 0.200 0932-4838 02.1 30 -51 18.17 04.06SCR 07 09 0.248 0933-5055 22.0 31 -83 17.74 18.97 302.5SCR 41 09 0.190 0934-5717 39.0 32 17.81 -50 45.81 115.8SCR 56 09 0.204 0938-5552 45.4 32 15.62 -55 14.28 09.07 299.2SCR 58 09 0.242 0943-4833 14.4 33 17.58 -61 17.35 48.14 171.2SCR 52 09 0.230 0946-4813 10.9 34 12.44 13.38 -48 17.16 52.93 140.4SCR 38 09 0.184 0946-6129 30.3 38 15.33 -50 17.93 09.31 167.1SCR 55 09 0.186 11.85 10.62 0946-5157 52.9 43 14.80 -57 15.58 18.20 132.8 17 09 0.228 14.03 54.2 46 16.17 -55 15.32 02.64 146.2 11.23 52 09 10.81 0.203 12.62 57.2 46 12.62 -48 14.57 34.37 279.3 33 09 13.25 0.334 15.11 49.9 46 13.41 -48 15.00 10.98 10.16 41.27 293.1 13 11.78 0.251 12.93 16.8 11.83 -61 17.23 12.72 328.7 29 13.33 0.216 11.90 40.2 13.02 10.00 -51 16.23 11.22 315.9 57 10.84 0.191 41.6 15.48 12.49 16.73 12.76 285.4 9.93 10.66 0.183 11.45 14.41 10.99 14.06 10.27 153.5 0.210 13.58 14.43 12.57 15.31 3.76 10.04 10.08 231.3 10.98 12.77 11.28 10.02 17.03 119.4 11.54 12.01 13.27 1.63 17.59 10.35 9.48 11.60 9.86 14.92 2.08 13.41 11.01 9.73 11.67 11.30 15.39 3.03 10.10 41.6 11.06 12.96 9.14 12.46 2.84 10.70 11.06 10.18 9.66 13.21 1.78 10.82 58.0 180.1 11.39 11.99 10.82 12.27 2.76 9.56 58.6 9.03 10.81 140.2 11.96 2.04 11.71 1.79 3.94 10.57 45.6 9.27 11.62 8.81 2.81 11.42 41.0 2.76 11.57 60.0 34.5 36.9 3.53 64.7 3.10 1.62 3.12 61.4 0.50 38.4 26.0 33.0 69.8 SCR 0947-7053SCR 0951-7224 09 47 23.50 09 51 44.73 -70 53 35.0 -72 24 20.2 0.268 0.212 345.8 324.1 16.82 18.56 14.73 16.11 13.12 16.04 12.10 14.61 11.58 13.96 11.35 13.68 2.63 1.50 [303.2] 85.0 SCR 0952-6542SCR 0956-8518SCR 0956-6724SCR 09 0957-4716 52 09.94SCR 09 1002-4912 56 14.01SCR 09 1005-4943 56 -65 31.12SCR 42 09 1007-5210 57.1 57 -85 21.32SCR 18 10 1007-8033 01.5 02 -67 08.06SCR 24 10 0.257 1011-8106 58.4 05 -47 47.90SCR 16 10 0.478 1012-4801 54.2 07 -49 24.94 284.4SCR 12 10 0.353 1024-6424 49.1 07 -49 56.03 319.2SCR 43 10 0.251 1027-8148 21.3 11 -52 18.19 12.38 310.1SCR 10 10 0.257 1028-7920 09.2 12 -80 17.10 30.58 293.4SCR 33 10 0.289 1029-6251 15.4 24 16.03 -81 18.15 20.04 265.6SCR 06 10 0.206 1031-6428 41.9 27 15.13 -48 17.98 17.56 297.6SCR 01 10 0.181 13.45 1036-8236 55.3 28 15.91 -64 15.09 31.61 154.5SCR 24 10 0.450 13.97 1036-6702 43.2 29 15.26 -81 16.01 48.04 332.7SCR 48 10 12.47 0.208 13.40 1036-8034 14.7 31 13.08 -79 16.76 34.68 112.4SCR 20 10 12.49 0.283 13.11 1037-8057 47.6 36 14.37 -62 17.24 11.91 16.17 312.1SCR 51 10 11.77 0.222 11.48 1037-7404 43.8 36 15.29 -64 16.54 11.94 26.85 312.4SCR 28 10 12.10 0.212 12.83 1040-6231 21.1 36 15.41 11.60 -82 17.37 11.18 10.10 271.9SCR 36 10 10.94 0.367 13.82 1041-6349 18.9 37 14.50 11.73 -67 18.45 11.58 06.03 291.2SCR 02 10 12.06 0.255 13.85 1046-5141 45.3 37 14.90 10.82 -80 17.79 10.36 38.37 265.0 34 10 12.61 0.180SCR 12.53 49.0 40 16.40 11.27 -80 1047-4815 16.74 11.49 08.41 280.0 57 10 12.63 0.251 12.19 19.5 41 15.72 10.12 -74 14.49 12.00 08.54 298.6 04 10 10.81 0.201 14.45 22.8 46 14.75 3.56 11.26 -62 16.18 12.11 31.94 035.2 31 11.35 0.234 10 13.81 30.8 12.60 2.64 11.79 -63 17.25 47 10.24 308.6 49 49.08 12.81 0.205 12.91 44.2 14.23 4.14 11.85 -51 16.75 10.80 287.4 41 12.12 0.250 11.31 46.7 15.24 3.17 18.34 -48 12.19 304.8 11.29 0.313 9.92 15 12.88 14.87 2.14 10.51 64.3 10.9 16.64 11.58 321.4 100.7 10.29 0.365 12.80 16.36 2.31 11.96 17.55 10.73 225.1 11.45 13.45 0.215 14.79 2.68 11.31 32.3 18.36 304.2 11.43 15.18 9.73 15.72 2.78 10.44 58.3 16.40 10.87 12.22 153.9 13.12 14.73 59.0 15.68 10.88 14.05 3.69 13.93 14.58 3.55 10.60 99.7 9.50 11.71 18.04 111.6 11.76 13.18 13.61 3.60 10.58 13.45 104.7 12.07 12.97 3.59 11.44 16.03 11.20 11.78 11.63 3.46 13.23 11.46 11.92 26.6 15.03 10.94 38.4 11.19 10.63 2.78 11.18 70.9 2.31 11.54 14.01 3.81 10.87 53.0 10.04 2.65 11.12 38.1 13.41 2.31 9.73 3.04 55.5 13.29 42.2 3.65 35.9 2.95 90.5 227.7 2.67 60.6 2.98 50.0 2.02 43.1 81.0 [262.1] 34.0 77 d a a (pc) Est Dist Notes J − F 59 R s JHK 12.11 11.50 11.21 4.11 40.1 ··· IVN I F 59 13.47 12.23 10.53 9.95 9.67 2.94 29.1 R J ··· ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 1050-6825SCR 1050-6247SCR 1053-6926 10SCR 50 1054-5159 48.73SCR 10 1054-8135 50 21.42SCR 10 1055-8130 53 -68 08.35 25SCR 10 12.8 1056-7555 54 -62 16.38 47SCR 10 35.9 1056-6945 54 -69 00.77SCR 26 10 0.209 1100-4959 31.7 55 -51 03.61 59SCR 10 0.296 03.5 1100-5233 56 -81 301.6 15.85SCR 35 10 0.212 1101-6314 33.6 56 -81 30.83 293.3SCR 30 11 0.408 1101-6342 59.8 00 18.04 -75 13.51 323.0 55SCR 11 0.234 06.1 1104-4836 00 -69 16.49 28.84 306.1SCR 45 11 0.303 16.23 1104-7856B 40.0 01 -49 17.21 54.40 307.1 59SCR 11 0.285 07.0 1104-8352 01 15.38 -52 17.31 14.36 002.4SCR 33 11 11 0.220 15.62 1105-4836 34.4 04 14.78 04 -63 16.05 45.92 305.2 39.95SCR 14 0.194 13.06 1106-6514 44.7 15.37 -63 15.98 261.1 14.58 42SCR 11 0.198 12.63 55.5 1107-7916 04 13.98 -48 17.27 -78 50.97 271.3SCR 36 11 12.23 56 0.293 13.37 1108-6513 03.0 05 14.31 21.5 12.32 13.90 07.96 279.9SCR 11 11.31 0.275 12.29 1108-4933 06 15.46 -83 17.29 11.67 44.40 279.8SCR 52 11 11.71 0.377 0.203 12.69 1109-6510 24.6 07 10.74 13.69 -48 16.53 10.65 42.08 296.6SCR 36 11 11.31 13.70 1110-4737 18.6 08 15.19 11.32 -65 15.41 11.10 03.62 300.7 14SCR 283.1 11 11.36 0.440 26.7 1110-7327 08 14.46 10.36 -79 17.10 10.69 00.77 9.89SCR 16 11 11.75 0.225 13.58 1111-7845 26.9 09 13.19 10.87 -65 16.82 17.86 10.87 11.27 256.7 13SCR 11 0.203 12.53 12.7 1115-7806 10 14.92 10.50 -49 11.24 22.85 273.0SCR 33 11 12.33 0.266 9.28 11.28 1117-7226B 40.6 10 14.61 1.65 10.57 16.32 -65 49.85 310.8 10SCR 11 11.22 0.398 13.22 07.1 1117-5023 11 3.15 10.97 -47 12.21 11.77 33.08 290.1 37SCR 11 10.83 11 0.181 12.67 07.7 1118-6400 15 14.84 3.46 17 -73 18.62 8.59 10.68 06.51 129.9 36.66SCR 27 11.65 0.252 [284.0] 1118-5143 27.2 10.79 3.66 11.51 -78 16.25 10.25 308.6 45SCR 11 11.55 0.283 13.06 45.8 1118-4721 17 16.46 2.67 10.41 -78 17.95 -72 11.04 58.61 147.7SCR 06 8.56 11 26 0.199 10.00 1120-8408 55.3 18 14.48 13.5 2.95 10.01 83.4 18.43 10.98 36.85 272.0 12.46SCR 11 0.201 15.20 1121-8057 18 16.22 3.71 10.82 33.2 -50 15.21 15.05 053.9SCR 23 11 0.269 0.188 13.30 1121-5742 35.1 18 16.33 10.76 42.7 -64 12.46 12.18 9.79 27.20 297.7SCR 00 11 13.40 1121-7111 28.6 20 12.80 2.86 55.7 -51 16.50 20.10 294.6 43SCR 275.8 11 11.71 0.333 14.70 22.2 1123-7459 21 11.03 3.24 56.1 -47 15.91 12.70 27.90SCR 21 1.45 11 9.28 0.252 11.54 1123-4819 57.0 21 14.87 2.36 46.0 -84 17.86 17.98 11.15 52.74 302.5 08SCR 11 13.14 0.253 10.47 01.6 1124-7602 21 14.19 3.27 12.44 -80 17.26 274.5SCR 57 11 10.22 0.322 13.09 9.19 1125-7349 03.2 23 16.24 3.06 10.91 80.5 15.99 -57 17.57 3.26 12.54 12.91 264.2SCR 42 11 10.00 0.304 13.30 1126-7655 13.9 23 41.8 -71 16.77 03.78 275.1 11SCR 11 32.2 11.33 0.247 15.49 40.6 1126-4706 9.65 24 14.94 13.94 12.33 50.0 -74 17.04 45.14 274.0SCR 59 11 11.56 0.191 1127-4857 46.5 9.53 25 14.84 47.0 -48 16.37 10.74 03.17 295.4 19SCR 11 13.60 101.1 0.196 12.66 13.02 51.3 1127-7816 26 15.07 3.06 52.0 -76 16.76 9.42 11.04 09.16 290.9SCR 02 11 0.309 13.21 1.00 1127-4807 34.3 26 15.62 2.77 10.46 -73 15.52 9.46 12.86 33.96 088.8 11.98SCR 49 11 11.78 0.189 13.58 1127-4808 17.9 27 15.03 10.81 -76 15.21 02.85 264.6 55 11 11.60 0.220 15.18 09.6 27 13.92 3.20 12.71 -47 17.91 11.73 11.22 16.78 279.8 105.6 06 11 12.26 0.292 13.44 38.9 27 12.47 -48 17.04 11.14 22.29 318.8 57 11 14.45 0.185 11.92 36.6 45.3 27 15.89 10.95 67.5 -78 18.10 2.58 11.67 36.51 249.3 16 11.84 0.191 10.98 40.1 15.24 3.54 10.84 -48 17.79 1.04 14.37 294.9 07 10.48 0.194 13.84 57.8 16.06 2.62 11.47 99.7 -48 17.90 11.37 192.8 08 10.29 0.196 13.46 55.9 16.19 2.64 14.35 17.54 3.33 248.4 13.02 0.200 13.91 9.84 15.62 11.07 18.30 32.3 192.4 11.56 0.183 15.28 9.71 15.80 3.16 39.9 18.74 45.0 12.49 103.8 13.33 14.04 16.21 3.24 69.1 17.97 9.60 10.94 260.2 149.1 13.79 14.39 16.46 2.82 12.29 15.83 72.2 9.47 12.78 11.84 14.19 15.93 1.16 10.69 17.03 13.17 12.54 13.68 13.78 3.19 12.54 49.3 11.27 12.61 13.44 14.66 12.98 52.8 11.96 12.57 11.68 10.99 82.8 3.43 12.04 442.5 11.69 12.65 2.87 11.71 2.19 11.94 11.23 3.67 11.79 62.4 11.14 12.04 2.74 11.67 10.64 2.40 10.86 28.4 11.46 123.0 3.79 10.32 37.7 3.26 11.20 39.8 145.5 3.60 204.6 3.89 4.24 39.9 2.55 78.7 2.63 65.9 56.3 33.3 55.0 75.6 78 d d d ··· (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 1129-4711SCR 1129-7532SCR 11 1130-7525 29 42.16SCR 11 1130-8122 29 32.31SCR 11 1130-4852 30 -47 06.81SCR 11 11 1131-7508 22.7 30 -75 39.01SCR 32 11 1133-5249 22.1 30 -75 21.78SCR 25 11 0.219 1134-5033 52.5 31 -81 51.40SCR 22 11 0.336 1135-5605 57.3 33 -48 40.91SCR 246.9 52 11 0.218 1135-8701 55.9 34 -75 29.84SCR 089.1 08 11 0.247 1137-5157 54.9 35 -52 17.10 41.91SCR 101.0 49 11 0.183 1138-5359 54.6 35 -50 16.65 54.23SCR 296.5 33 11 0.214 1140-5447 40.1 37 15.11 -56 16.79 38.37SCR 286.1 05 11 0.322 1140-5510 17.7 38 14.88 -87 18.03 07.76SCR 298.3 01 11 0.298 1140-6943 13.04 40.4 40 15.22 -51 17.49 15.98SCR 267.2 57 11 0.297 1141-8337 13.07 32.3 40 16.23 -53 17.80 37.74SCR 257.7 59 11 11.82 0.255 1143-7526 13.69 10.1 40 15.38 -54 17.53 25.94SCR 273.4 47 11 11.42 0.203 1143-7704 14.13 13.9 41 16.34 -55 15.59 11.27 07.63SCR 267.0 10 11 12.00 0.302 1145-5412 12.99 34.9 43 15.55 -69 17.56 10.93 09.88SCR 246.9 43 11 12.80 0.196 1146-4841 14.80 45.8 43 13.27 11.03 -83 14.82 11.48 07.94SCR 295.7 37 11 12.24 0.251 1147-5504 12.71 38.0 45 15.53 10.64 -75 15.20 12.30 52.06SCR 332.8 26 11 12.85 0.280 1148-7639 10.53 00.5 46 12.93 11.18 -77 15.92 11.64 03.48SCR 253.1 04 11 11.43 0.193 1149-5629 13.70 52.3 47 12.86 12.06 -54 14.31 12.28 52.49SCR 269.3 12 11 10.44 0.186 1151-5700 11.93 56.1 48 13.66 11.39 -48 16.47 10.95 03.27SCR 289.7 41 11 12.68 0.229 1152-7947 10.95 37.6 49 12.46 3.29 12.00 -55 17.19 43.94SCR 108.5 04 11 10.78 0.192 1153-5430 11.51 11.9 9.91 51 14.32 3.46 10.68 -76 13.05 12.14 31.85SCR 001.4 39 11 10.77 0.279 1155-7904 11.56 12.5 52 15.54 3.22 -56 16.18 10.15 34.57SCR 181.3 29 11 11.17 0.192 1156-6922 11.79 27.8 53 11.56 3.43 11.93 -57 16.60 9.60 10.19 22.59SCR 166.0 00 11 11.49 0.230 1158-4934 13.40 23.5 54 14.48 3.14 56.0 -79 12.14 10.58 59.92SCR 011.3 47 11 11.01 0.228 9.93 1158-6950 11.08 23.5 56 15.01 3.49 44.8 -54 16.32 10.93 51.45SCR 275.8 30 11 11.93 0.226 9.95 1200-5659 13.14 07.5 58 10.63 4.11 10.33 65.9 -79 14.96 10.47 59.25SCR 330.7 04 11 0.252 1202-5449 14.12 12.9 58 13.83 10.86 89.2 -69 18.07 9.75 11.35 58.09SCR 284.5 22 12 11.08 0.304 1202-4723 52.3 00 12.23 2.85 10.22 70.6 -49 17.73 2.82 04.61SCR 268.6 9.82 34 12 12.50 0.401 1203-8559 11.36 13.4 02 16.24 11.12 86.6 -69 13.58 10.50 18.96SCR 255.7 50 12 9.24 0.201 2.14 1203-6836 10.25 33.9 02 15.79 35.5 -56 17.64 10.03 12.00 28.02 297.3 59 12 10.79 0.252 2.10 13.92 40.0 03 11.46 2.49 10.26 -54 15.39 15.97 292.5 102.5 49 12 0.297 14.32 9.06 29.1 03 15.82 0.98 11.76 -47 18.17 9.67 34.4 10.21 35.63 228.2 23 9.52 12.26 0.206SCR 10.41 56.0 13.16 3.31 1205-4916 -85 12.71 270.7 59 12.98 0.209SCR 53.2 13.81 25.8 16.23 3.62 1207-5530 -68 15.89 11.65 292.7 36 9.08 10.20 0.319 9.95SCR 52.3 12 11.01 9.37 30.4 10.34 54.9 1208-5436 15.61 05 12.46 235.3 11.96 26.07 0.182 12 14.99SCR 14.14 3.40 11.40 98.8 15.35 07 1208-5737 213.2 10.21 32.54 0.207 12 1.81 8.81 9.58 13.51SCR 2.51 12.20 38.9 17.48 08 11.38 1208-7037 -49 301.1 9.63 13.29 49.12 16 12.47 13.34 12 53.5 16.11SCR 41.5 -55 274.5 08 1209-5002 30 11.79 49.92 9.58 15.19 11.10 12 16.55 56.0SCR 9.44 12.65 -54 08 12.01 3.05 1211-5712 36 9.64 11.80 0.60 13.82 22.85 0.185 38.3 12.33 16.8 12 114.7 11.21 -57 09 13.05 31.9 14.65 0.255 37 3.98 12.43 16.45 9.28 11.37 23.9 12 11.38 -70 096.4 11.69 11 2.56 11.10 0.203 2.81 37 9.07 22.76 10.57 35.5 11.98 082.0 13.39 -50 11.12 0.186 10.86 02 16.50 10.76 35.9 295.6 49.1 10.63 57.1 -57 3.86 10.42 0.373 1.26 11.47 12 14.85 8.88 12.47 24.3 266.4 10.60 49.0 14.34 10.17 16.64 118.2 0.350 10.72 24.1 263.5 2.94 11.24 12.71 2.95 11.85 0.281 15.67 12.46 264.4 14.40 10.36 9.94 16.82 2.13 11.65 44.8 11.94 50.3 253.8 14.42 11.92 14.67 2.30 10.33 12.63 119.5 0.70 15.12 11.49 17.83 1.96 27.4 13.89 11.32 12.65 11.97 3.22 12.60 10.94 15.63 96.5 13.29 11.09 11.35 11.40 3.06 2.18 62.8 11.33 10.72 44.1 13.80 12.76 0.38 78.6 11.22 11.29 10.73 61.7 12.78 12.73 10.70 117.8 10.48 35.4 12.26 2.42 10.52 1.23 12.04 2.44 1.13 81.2 3.79 92.4 1.36 [206.2] 84.6 2.85 37.2 [81.8] 104.5 SCR 1204-5148SCR 1204-4929 12 04 38.61 12 04 14.79 -51 48 15.6 -49 29 28.2 0.208 0.221 279.8 307.9 15.89 16.32 13.76 14.26 11.89 13.17 11.46 12.85 10.88 12.27 10.63 12.05 2.30 1.41 [165.2] 69.3 79 a a c (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 1229-5738BSCR 1231-4803SCR 12 1231-7020 29SCR 04.12 1232-7014SCR 12 1233-5401 31 -57 28.42SCR 12 38 1233-7722 31 50.1 45.57SCR 12 1236-4713 32 -48 25.63SCR 03 12 0.189 1237-4940 35.6 33 -70 04.31SCR 20 12 1238-5159 45.6 33 -70 37.98SCR 14 262.7 12 0.260 1238-5327 29.4 36 -54 25.90SCR 01 12 0.237 1239-4759 13.3 37 -77 17.59 07.09 233.7SCR 22 12 0.237 1240-4904 19.9 38 -47 40.91 306.1SCR 13 12 0.188 1240-8209 14.4 38 15.53 -49 18.31 13.72 282.0 40 12 0.226 51.2 39 -51 16.73 51.37 127.5 59 12 0.256 18.3 40 16.25 14.08 -53 15.58 56.79 181.5 27 12 0.206 54.5 40 14.40 -47 13.96 50.93 270.0 59 0.198 12.79 13.99 07.7 13.58 -49 17.78 255.1 04 0.361 12.86 01.9 12.08 -82 16.96 097.7 12.25 09 12.12 0.401 11.45 03.4 16.08 16.90 260.5 11.84 0.199 11.53 14.97 16.26 12.03 11.50 268.5 10.46 0.486 14.37 14.97 15.13 11.27 269.4 11.13 13.15 14.21 11.19 17.26 272.4 12.17 13.63 9.81 12.86 11.00 18.30 10.61 12.19 12.24 15.25 16.18 11.66 12.73 11.36 16.22 10.44 2.74 9.59 11.64 11.98 12.92 14.55 11.37 12.15 10.63 14.35 4.14 11.40 11.46 11.57 12.29 2.56 11.93 10.04 12.95 109.8 11.16 11.08 10.85 0.95 3.13 12.45 9.80 3.91 10.79 38.8 10.19 2.78 12.21 69.5 2.24 9.93 2.23 71.4 30.6 52.0 2.23 3.68 83.3 131.9 3.27 92.4 3.70 46.6 42.7 95.4 29.2 SCR 1211-7328SCR 1211-6849SCR 1212-6736SCR 12 1213-4820 11 48.47SCR 12 1215-8218 11 39.71SCR 12 1216-5622 12 -73 40.09SCR 28 12 1217-5437 28.8 13 -68 07.13SCR 49 12 1217-5530 30.2 15 -67 11.40SCR 36 12 0.184 1217-5545 06.8 16 -48 52.72SCR 20 12 0.489 1217-7810 07.9 17 -82 32.05 280.4SCR 18 12 0.196 1218-5345 29.8 17 -56 42.94 293.4SCR 22 12 0.480 1218-4950 24.6 17 -54 17.10 50.67 291.2SCR 37 12 0.195 1218-5132 31.6 17 -55 16.90 26.93 268.0SCR 30 12 0.208 1220-5346 30.8 18 15.46 -55 16.52 52.34 261.7SCR 45 12 0.237 1220-8302 39.6 18 14.73 -78 16.51 14.09 251.2SCR 10 12 0.189 13.50 1220-4814 45.9 18 14.48 -53 15.73 01.06 070.4SCR 45 12 0.196 12.42 1221-5723 08.9 20 14.24 -49 15.84 17.18 290.2SCR 50 12 12.01 0.212 12.53 1221-5516 03.1 20 13.97 -51 17.80 03.71 290.6SCR 32 12 11.38 0.225 11.95 1221-5237 18.4 20 14.02 -53 18.17 11.47 27.79 056.6SCR 46 12 11.91 0.198 12.10 1221-7609 00.2 21 15.74 -83 17.40 10.90 27.87 288.9SCR 02 12 11.24 0.204 12.52 1221-5722 29.2 21 16.49 11.20 -48 17.55 11.30 16.08 290.0SCR 14 12 11.10 0.254 14.48 1222-4937 42.5 21 15.46 10.62 -57 14.51 10.72 45.47 264.3SCR 23 12 11.84 0.243 15.05 1223-7043 11.3 21 15.69 11.07 -55 16.70 10.56 39.93 272.1SCR 16 12 13.55 0.200 14.38 1224-4708 26.8 21 13.05 10.45 -52 16.48 11.21 28.22 244.2SCR 37 12 14.04 0.197 13.15 1224-5339 25.4 22 14.72 10.34 -76 16.14 13.03 44.23 128.3SCR 09 12 13.49 0.264 12.18 1224-5027 51.4 23 14.54 3.45 11.02 -57 17.03 13.50 12.78 273.8SCR 22 12 11.20 0.186 12.86 1224-5341 56.0 24 15.60 3.35 12.81 -49 18.06 12.83 31.01 256.8SCR 37 12 12.06 0.350 13.20 1224-8205 12.4 24 14.94 2.57 13.25 -70 15.84 10.64 24.44 276.2SCR 43 12 11.42 0.194 13.97 1225-5323 56.6 24 16.07 3.00 12.70 -47 16.90 11.57 54.47 264.7SCR 08 12 12.11 0.190 12.80 1227-5155 06.6 24 13.89 2.86 10.36 60.1 -53 18.66 10.80 08.47 274.1SCR 39 12 12.93 0.264 14.36 1229-5738A 08.8 24 14.56 2.18 11.44 45.3 -50 15.91 11.50 39.81 257.8 27 12 10.97 0.357 11.52 22.9 25 16.46 2.19 10.54 77.0 -53 17.21 12.40 14.20 288.4 41 12 12.81 12 0.189 13.66 47.6 27 14.03 29 2.44 11.30 47.9 -82 16.93 10.39 24.09 186.6 04.89 05 10.65 0.187 14.63 53.3 15.05 1.97 12.15 51.9 -53 18.24 12.32 251.9 23 12.72 0.379 12.24 54.0 15.15 4.49 10.07 89.9 -51 17.36 -57 273.3 199.4 55 13.11 38 0.273 12.33 23.0 9.99 16.04 41.3 0.99 12.07 16.93 12.22 268.2 235.2 10.66 0.265 12.91 15.59 3.30 17.73 12.56 183.2 202.7 11.23 0.217 0.197 14.86 14.78 2.43 11.97 17.72 9.71 10.12 277.2 12.15 13.56 15.77 2.67 12.30 24.5 16.42 10.62 279.8 131.0 256.6 13.22 12.30 15.76 3.96 17.63 11.62 12.40 9.85 14.23 14.37 3.26 10.31 42.7 16.92 15.36 12.59 10.51 14.75 15.68 11.36 90.5 11.95 115.0 12.80 12.22 15.09 13.57 1.84 12.34 3.25 13.07 13.77 9.93 3.36 11.66 25.0 12.27 10.69 13.05 12.86 90.6 12.56 12.59 3.37 3.82 12.03 9.65 10.06 145.5 11.88 11.74 3.01 12.37 31.0 12.04 2.82 91.0 11.33 11.06 9.81 3.20 11.80 31.3 11.11 31.4 10.92 2.98 80.1 4.27 113.4 2.69 84.4 3.69 3.10 100.9 3.21 1.84 18.1 133.5 25.4 87.6 62.7 92.7 80 d a a a a bc e d d d (pc) Est Dist Notes J − F 59 R s JHK ··············· IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 1240-8116SCR 1241-4717SCR 1241-5627SCR 12 1242-4810 40 55.99 12SCR 41 1244-7449 33.15 12SCR 41 -81 1245-5025 12.72 16 12SCR 30.9 42 -47 1245-5506 14.00 17 12SCR 05.8 -56 44 1246-5328B 27 30.38 0.492SCR 12 30.6 -48 1246-5328A 45 10 52.20 0.428SCR 12 50.3 12 1247-7712 45 -74 46 279.8 52.53 0.279 49SCR 03.73 12 06.9 1247-5524 46 -50 257.9 0.268 05.64SCR 25 15.15 1250-5734 07.3 -55 251.6 -53SCR 06 12 0.229 28 16.51 1252-4956 50.2 47 21.8 249.7 -53 24.98SCR 12 28 13.11 0.187 17.36 1254-5301 47 31.2 267.4 22.38SCR 12 14.38 0.412 0.183 17.76 1254-5609 50 -77 18.48 136.9SCR 12 12 11.25 15.64 0.188 1256-5410 29.4 52 18.15 -55 59.55 107.0SCR 24 025.3 12 13.42 15.65 1257-4701 50.2 54 -57 18.39 35.61SCR 029.0 34 12 13.85 0.255 1257-5554A 16.37 9.73 22.5 54 -49 14.84 16.05 12.77 17.22 56 12 13.21 0.367SCR 51.5 56 16.41 1257-5554B -53 14.06 12.33 01.97 280.0 01 12 12 0.215SCR 15.57 33.2 57 12.82 12.21 57 14.32 1257-5655 -56 9.16 11.61 54.01 269.8 32.85 09 0.204SCR 14.45 12 51.6 11.75 11.94 1258-4850 -54 17.77 57 258.6 14.45 10 0.193SCR 32.85 12.05 10.34 07.5 12.73 11.08 1259-5611 -47 17.32 -55 253.3 01 13.03 54 8.89 0.233SCR 12 11.44 10.97 11.4 16.34 48.9 1300-6229 17.26 57 13.80 283.0 -55 32.84 0.207SCR 11.81 12 10.77 54 15.70 1301-6009 18.35 58 8.99 48.9 12.54 259.7 34.22 10.15 0.191SCR 0.410 12 14.64 15.19 13.65 1301-8212 17.82 59 -56 271.3 11.27 16.36SCR 55 13 14.43 16.35 0.413 12.29 1302-7806 42.7 18.17 00 -48 287.9 290.1 8.42 51.87 12.65SCR 50 13 1.61 13.84 15.96 9.54 1304-5259 49.4 18.20 01 11.02 -56 07.60 12.88 3.38 11 293.3 3.30 13 14.24 0.311SCR 16.29 09.4 17.37 01 14.83 1304-5730 -62 12.07 55.89 12.49 29 13 4.04 14.43 0.184 8.12 16.24SCR 29.6 02 -60 12.33 9.36 1305-7554 15.05 18.58 12.68 277.2 09 13 14.29 0.301 15.54 1.92SCR 13.46 11.81 14.1 166.2 04 -82 11.91 1306-7445 30.79 12.67 267.0 12 13.98 0.214 13SCR 3.37 12.13 19.1 13.89 -78 12.10 17.61 04 1308-5421 12.36 19.1 272.1 06 68.4 39.66 13.66 0.269 11.45SCR 13 11.70 03.0 2.51 -52 12.15 16.78 1311-4756 05 11.90 241.9 [321.0] 59 34.5 48.78 0.221SCR 13 11.80 08.6 15.36 11.97 11.82 18.08 1315-5015 06 -57 12.76 242.6 10.48 54.79 0.210 3.83 30SCR 13 11.94 14.86 11.32 21.6 16.29 1.80 1315-5453 08 -75 239.6 44.23 0.244SCR 54 3.69 13 13.42 11.61 97.0 16.05 12.16 12.75 1315-7240 49.7 11 -74 108.1 41.44SCR 9.89 45 2.83 13 13.36 11.08 0.185 14.79 82.1 16.54 1318-5104 51.3 15 -54 096.6 12.20 43.83 21 13 2.70 13.71 11.96 11.28 0.253SCR 17.44 38.9 15 1319-6200 -47 12.30 276.4 49.91 11.4 56 3.67 13 13.60 14.61 0.221SCR 16.97 9.66 45.3 40.4 15 11.66 -50 1319-7537 12.26 35.50 193.2 15 13 11.23 3.29 73.4 15.84 0.204SCR 20.0 120.2 18 11.75 18.45 -54 1319-5952 11.63 33.49 264.8 53 3.93 13.22 15.31 0.227 13 11.40 27.6SCR 11.60 -72 15.25 19 10.13 1320-7542 284.5 40 4.34 14.05 94.2 04.51 0.207 11.51 13 16.39 58.4 11.00SCR -51 17.73 19 12.12 232.1 1321-5736 04 2.79 13.49 64.8 20.06 0.204 11.35 13 58.6 13.47SCR 17.98 19 12.31 -62 270.0 1322-8121 86.0 9.78 45.12 0.203 00 15.71 10.79 2.98 15.73 11.51 13SCR 19.0 18.24 12.32 -75 258.7 20 1323-5504 55.3 0.200 37 12.21 47.57 16.09 11.75SCR 13 17.54 27.4 -59 217.4 1324-5114 14.48 35.2 21 3.16 11.30 52 13.71 0.286 110.8 16.24 43.62 9.73 11.83 13 11.50 30.1 235.6 22 11.40 -75 2.56 11.50 14.56 15.70 15.45 0.251 42 13 17.90 13.86 51.0 23 12.72 017.8 -57 3.79 11.60 14.33 39.1 10.21 24.46 0.232 36 13 18.30 10.82 52.3 24 13.39 -81 227.6 3.16 14.32 16.04 25.01 13.79 21 0.434 12.16 18.21 06.6 12.85 -55 267.1 66.0 16.38 10.60 04 0.219 12.85 17.77 9.79 15.6 12.79 -51 2.49 96.1 13.89 249.3 1.15 11.88 14 16.41 0.182 12.33 18.09 00.5 3.53 49.7 14.50 243.0 12.64 15.24 0.370 12.23 12.57 17.87 2.99 56.0 9.55 258.3 15.63 12.01 15.98 0.184 12.79 14.31 1.91 218.9 11.96 13.64 12.00 15.82 15.51 88.2 14.13 45.4 309.9 2.07 14.32 9.09 12.25 12.92 15.89 66.0 12.75 3.01 11.73 14.71 13.49 13.80 [337.3] 17.62 90.6 12.63 2.70 12.01 11.96 9.00 13.83 12.19 3.39 13.93 13.30 12.64 15.18 12.04 2.92 77.3 11.35 11.87 12.60 13.32 93.3 11.13 11.82 14.29 154.3 10.78 3.46 11.72 13.26 10.57 3.59 82.0 13.37 101.1 0.66 10.61 11.14 2.28 10.30 12.80 2.49 10.95 72.7 3.35 12.64 [239.2] 76.3 37.7 1.89 1.57 103.6 2.67 [270.8] 73.2 2.11 1.81 81.8 53.4 86.1 196.8 81 d d d d d d d a d d (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 1324-6036 13 24 25.68 -60 36 25.0 0.315 273.8 16.93 14.48 13.66 12.72 12.12 11.90 1.75 [139.6] SCR 1326-7554SCR 1328-5317SCR 1329-6014 13SCR 26 1331-5138 02.50SCR 13 1332-5517 28 44.53SCR 13 1332-5422 29 -75 14.02 54 13SCR 15.1 31 -53 1333-5055 06.81 17 13SCR 52.0 32 -60 1335-6115 04.27 14 13 0.186SCR 25.6 32 -51 1336-5701 06.31 38 0.256 13 02.5SCR -55 33 262.4 1338-5356 17 37.80 0.240 13 04.6 -54SCR 35 242.5 22 1338-5518 34.24 0.484 13 22.8 18.25 36 -50SCR 276.0 30.28 0.185 55 1339-5914 13 28.0 17.49 -61 294.9SCR 38 0.243 15 1339-7101 16.42 34.08 13 15.82 50.9 -57 058.5SCR 38 01 1339-5507 0.203 15.61 34.21 16.06 07.8 13 231.3 -53SCR 15.56 39 14.27 0.185 56 1339-5119 16.16 06.87 07.5 13 250.8 -55SCR 13.75 39 14.10 0.294 18 1340-7155 15.92 02.35 13 14.73 35.1 253.5SCR 13.53 39 -59 14.43 1341-5621 0.280 50.37 14 17.04 12.18 13 265.9SCR 17.7 11.94 14.35 -71 39 1341-6153 14.06 0.200 01 17.49 22.57 12.50SCR 13 54.3 12.66 268.6 -55 1342-5714 40 15.36 11.62 07 17.39 0.246 59.99 10.98SCR 13 54.8 12.58 13.93 243.9 1343-6938 41 -51 15.74 11.91 08.88 0.231 11.23 19 17.82 13SCR 50.6 14.70 11.34 41 261.6 15.69 -71 10.50 1343-5210 35.67 0.354 11.28 55 13 17.88SCR 11.77 13.4 13.66 42 -56 143.6 10.64 1344-4948 16.15 32.13 21 13 0.391 13.89 16.63SCR 10.26 04.1 14.04 43 -61 249.6 10.68 1346-5408 16.41 00.01 53 0.193 12.29 13SCR 15.17 10.41 56.6 -57 15.26 43 1346-7834 232.5 13.30 14 15.48 56.05 0.204 12.17 1.69SCR 13 16.92 10.48 49.5 -69 1347-7610 14.63 44 254.3 11.69 38 12.95 14.53 0.183SCR 13 3.44 14.06 21.2 18.32 13.09 1348-7052 46 -52 216.2 11.62 14.78 15.34 02.71 0.211 10SCR 13 1.77 12.97 56.4 16.75 11.44 1348-5536B 46 -49 254.0 [374.8] 11.64 13.52 00.41 0.266SCR 48 13 3.12 16.41 16.25 11.40 13.52 1349-4829 33.9 47 -54 224.6 13.60 56.80 12.41 08SCR 13 3.20 0.355 14.99 13 16.03 14.4 1349-5109 48 10.88 13.33 48 -78 257.3 15.82 15.62 27.46SCR 34 3.08 60.1 13.01 14.39 0.186 11.83 1352-7100 22.3 128.2 11.92 -76 12.20 280.2 10SCR 13 12.84 14.09 0.185 10.29 1.47 16.85 20.0 1353-6756 49 -70 14.54 -55 16.37 12.95 283.2SCR 52 13 13.18 44.4 36 10.47 0.224 11.46 3.45 1354-5538 13.9 49 22.8 17.77 12.00 44.45 230.6 10.09SCR 13 12.51 45.1 15.02 0.194 3.52 1355-5623 14.16 52 -48 17.99 11.75 59.82 022.1 11.18 [241.3] 29SCR 13 51.4 0.210 0.204 16.00 36.6 1355-4707 53 11.44 2.09 -51 16.83 9.67 11.05 45.15 089.7SCR 09 13 12.41 13.96 1355-5537 47.2 54 15.72 11.18 -71 16.71 3.44 53.29 211.0 00SCR 236.9 13 0.195 15.37 11.17 64.9 44.6 1358-5615 55 15.33 10.43 -67 12.40 11.64 15.66 1.97SCR 56 9.59 13 0.236 10.97 [271.2] 13.66 62.1 1358-5459 00.5 55 14.98 -55 13.63 17.07 40.13 165.7 2.07 13.93 38 13 0.342SCR 10.21 14.31 11.6 55 10.27 11.08 -56 1358-7428 02.93 245.7 3.42 23 13 12.42 0.182SCR 13.12 9.15 21.0 58 11.46 [210.2] 14.52 -47 17.97 99.0 1359-5212 13.44 16.45 251.8 07 13 12.88 0.188 1.87 10.82SCR 37.4 58 -55 16.84 1401-5311 11.82 13.74 248.2 8.88 37 12.16 0.329 13 2.99 11.31 40.0 16.05 13.40 13.36SCR -56 18.12 58 9.03 12.29 224.1 1404-5434 57.2 15 06.48 0.197 2.64 13 05.1 14.88 11.60 -54SCR 16.73 59 11.62 [381.8] 254.3 62.0 59 1404-5131 10.76 17.58 0.233 11.92 3.04 8.62 14 14.20 10.7 16.15 12.06SCR 11.53 01 -74 239.6 1404-5310 25.12 0.210 28 13.05 14.74 14 11.41 24.8 16.88 10.17 -52 255.8 11.27 04 12.89 0.214 3.38 72.7 12 13.99 11.17 10.45 14 15.89 8.01 55.4 -53 300.9 04 11.67 72.0 11 12.52 0.389 15.02 26.82 2.06 10.05 14 16.60 11.04 0.89 17.5 12.37 245.7 04 12.43 -54 41.4 10.16 14.04 15.19 0.304 34 3.30 17.86 11.06 16.6 7.77 11.67 259.2 -51 12.47 14.93 0.198 2.45 12.14 31 16.82 11.87 17.9 [253.4] -53 264.3 52.9 11.79 16.10 2.82 10.85 10 0.283 9.83 11.12 16.49 20.8 11.13 255.6 13.20 14.53 11.66 44.1 0.184 16.86 11.30 14.16 264.6 0.69 10.86 67.3 13.51 2.61 0.187 10.53 18.19 134.7 9.48 11.66 13.62 260.8 15.04 10.69 1.65 12.56 17.79 249.2 3.16 13.31 10.27 87.3 16.45 11.11 12.39 18.25 9.39 3.21 10.49 13.45 12.03 15.93 16.69 12.21 3.72 10.88 56.2 15.25 63.8 11.78 16.36 12.19 3.07 11.76 15.26 100.3 22.5 11.61 14.94 13.32 11.63 14.27 11.67 3.89 52.0 13.76 11.41 13.61 12.68 0.62 2.74 61.4 12.58 11.38 13.23 3.28 58.2 12.08 12.47 11.99 3.55 13.10 11.42 2.13 31.0 11.69 44.8 58.1 1.30 11.25 55.2 2.85 72.3 3.13 110.0 [108.6] 2.17 3.78 81.3 2.86 116.6 [232.6] 59.4 74.9 82 d d a d d d d (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 1404-8228SCR 1406-4908SCR 1407-7042 14SCR 04 1407-7248 17.68 14SCR 06 1409-5337 07.46SCR 14 -82 1409-7343 07 28 26.39SCR 14 39.1 1410-7402 07 -49 01.17 08 14SCR 41.5 09 -70 1410-7534 49.48 0.205 42 14SCR 21.7 09 -72 1411-7525B 52.18 48 14 0.277SCR 59.7 10 -53 199.3 1412-4954 11.12 37 0.204 14SCR 25.9 14 -73 10 1412-8307 213.5 11 43 21.88 0.241 51.41SCR 17.31 36.3 -74 1413-4902 137.4 02 0.450SCR 14 00.4 16.54 1417-5018 12 -75 242.9 -75 15.35 43.86 0.211 34SCR 14 25 47.0 17.47 1419-4847 12 05.4 212.4 41.92 0.215SCR 14 15.25 16.07 1420-7516 13 -49 269.1 13.35 19.82SCR 54 14 0.203 15.64 0.250 16.45 1420-5106 32.2 17 -83 183.9 56.29 14.61 07SCR 14 14.09 16.53 45.0 1423-7122 19 11.90 -49 177.5 14.26SCR 02 242.1 14 13.25 14.33 0.420 17.03 1424-8503 40.8 20 -50 13.60 36.84SCR 18 14 12.70 14.71 0.277 11.41 1424-8124 22.5 20 17.97 -48 17.90 12.00 21.66 212.9 47SCR 14 13.06 15.18 0.335 33.2 1426-5330 13.08 23 -75 11.85 58.92 241.3 11.12SCR 16 14 12.63 0.200 16.21 1426-8655 05.9 24 11.52 16.43 -51 15.85 11.72 51.43 259.2 06 14 13.27 0.197 12.89SCR 51.3 24 11.20 -71 1426-4715 16.16 11.41 44.98 226.7 22 14 0.195 15.56 11.28 57.7 26 13.82 14.54 11.24SCR -85 17.41 11.95 29.58 245.4 1426-4946 03 14 0.489 11.04 05.5 26 14.09 10.88 -81SCR 17.35 08.79 243.7 14.33 24 1427-7335 0.213 13.10 14 10.95 12.25 12.0 15.44 11.40 -53SCR 17.33 26 130.4 3.45 30 1429-7412 05.28 0.205 10.66 12.51 26.9 15.26 14 -86SCR 14.23 13.73 213.7 12.57 26 55 1430-5331 11.66 0.250 1.66 11.22 13.83 02.67 41.5 15.32SCR 14 14.64 -47 241.2 1431-4904 27 11.90 0.297 15 3.64 13.67 12.68 27.58 13.54SCR 51.4 14 12.57 12.32 11.12 239.2 1432-7154 29 12.53 -49 0.301 2.24 13.34 13.01 31.49 46SCR 14 16.80 11.38 [208.4] 251.4 51.9 54.3 1433-7138 30 12.24 -73 2.61 10.45 0.288 10.71 51.02 10.88 35 14 17.60 12.01SCR 232.4 39.9 31 12.05 -74 1433-6905 3.31 11.57 14.76 05.07 11.14 12 14 17.14 0.194 11.68SCR 16.2 32 256.5 -53 3.23 57.7 1434-5003 10.42 15.70 29.85 11.78 31 14 18.18 9.44 0.183 11.49 11.9 33 10.46SCR -49 85.8 12.48 251.0 15.66 41.79 1.88 1434-7433 11.40 04 3.33 0.326 14 17.51 22.6 10.21 -71SCR 70.2 33 13.42 16.01 253.9 11.21 54 1435-5717 42.36 0.365 14 13.6 8.91 11.23 17.14 -71SCR 49.1 13.92 34 9.92 237.8 2.16 38 1438-4707 15.64 09.30 0.201 42.6 11.54 14 [286.9] SCR 15.04 64.5 13.90 -69 9.65 268.0 2.19 34 1438-8102 0.229 10.61 05 15.73 34.69 12.14 111.5 SCR 53.4 14 17.10 8.63 -50 222.7 14.56 2.91 1438-5327 35 0.182 9.70 10.95 03 12.98 20.21 12.58SCR 14 17.98 34.5 310.6 3.02 10.33 1440-5745 38 -74 9.60 11.64 15.18 0.201 15.41 54.54 33SCR 14 18.06 13.63 202.0 39.4 3.27 10.66 83.9 1440-5059 38 -57 11.99 11.87 16.14 50.42 0.195SCR 17 14 17.80 11.36 92.9 13.78 1440-7456 27.6 38 242.5 -47 13.24 13.00 15.99 02.18 07SCR 14 13.62 0.218 11.69 93.3 28.5 1440-5601 40 11.17 -81 220.9 14.25 16.23 02.06SCR 02 14 13.11 0.229 3.24 16.14 70.7 1440-5020 26.4 40 12.00 12.85 2.55 -53 13.86 250.3 11.69 12.58 27SCR 14 0.194 10.52 16.66 3.54 59.8 35.0 1440-5159 40 11.94 0.50 -57 14.36 57.42 12.90 271.1SCR 45 14 15.13 0.193 11.51 4.16 1441-7003 17.8 40 12.17 16.79 -50 11.19 42.43 189.5 10.38SCR 59 14 14.45 0.196 11.42 3.52 1441-7338 23.1 40 13.09 -74 16.07 16.72 125.9 14.58 11.29 56 14 0.208 21.3 11.67 3.42 15.25 20.3 40 10.46 44.5 -56 13.00 32.67 211.4 11.07 01 14 12.92 0.221 12.56 35.3 33.4 41 14.47 2.01 49.7 -50 13.75 13.71 25.89 238.6 11.39 20 14 0.210 14.68 31.4 36.3 41 11.02 -51 17.45 11.63 9.84 14.42 1.96 234.6 12.31 59 0.205 13.18 65.0 46.0 13.18 11.72 -70 14.00 225.3 1.81 13.53 03 0.185 [216.6] 10.40 66.8 00.8 16.09 11.02 -73 18.30 261.0 3.41 38 11.26 0.192 13.15 9.72 11.22 41.4 12.14 [166.9] 17.36 12.91 244.6 4.19 0.183 10.81 13.85 16.25 18.15 9.89 10.59 162.1 3.82 0.207 11.54 15.18 12.78 18.12 9.94 256.7 3.13 72.5 11.79 13.93 16.26 10.42 15.91 029.0 65.7 9.24 10.23 13.55 16.21 17.61 11.27 38.5 9.34 12.16 1.43 1.23 14.94 13.94 18.28 50.8 12.22 2.82 14.32 117.8 9.11 9.62 15.62 11.00 11.59 12.81 12.70 9.11 16.15 1.72 11.64 [253.4] 12.85 14.77 3.21 11.28 9.51 12.33 11.37 53.1 13.05 11.44 12.31 13.67 [184.9] 57.4 11.99 10.82 11.20 1.13 4.30 12.07 13.00 1.78 10.55 44.9 10.61 4.09 12.83 1.90 2.97 10.27 41.7 3.45 40.3 37.9 3.36 2.57 42.0 43.9 1.95 73.3 4.95 81.0 87.6 59.7 212.1 19.0 83 d d d (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 1442-5112SCR 1443-5555SCR 14 1443-5502 42 10.13SCR 14 1445-5046 43 21.36SCR 14 1445-6913 43 -51 26.04SCR 12 14 1446-4718 56.4 45 -55 23.96SCR 55 14 1446-7119 44.1 45 -55 19.02SCR 02 14 0.182 1448-5735 53.2 46 -50 34.24SCR 46 14 0.181 1449-5456 06.0 46 -69 22.07SCR 235.1 13 14 0.477 1450-7047 17.1 48 -47 39.82SCR 162.3 18 14 0.435 1450-5651 47.3 49 -71 16.38 49.03SCR 277.5 19 14 0.228 1451-5407 59.9 50 -57 16.46 12.68SCR 244.1 35 14 0.191 1451-5115 17.7 50 14.33 -54 15.08 41.74SCR 018.8 56 14 0.199 1451-5039 59.7 51 14.32 -70 17.09 39.66 246.3 47 14SCR 0.202 12.53 47.9 51 13.22 1452-7055 -56 17.12 21.76 219.9 51 14 0.252SCR 13.45 48.0 51 15.51 1452-7147 -54 16.49 30.65 188.8 07 11.14 0.187SCR 14 11.56 44.9 15.56 1454-4940 -51 16.26 52 157.7 15 11.98 12.17 0.322SCR 14 13.63 54.6 14.58 1454-7347 -50 12.47 52 10.58 250.3 39 10.28 45.04 0.182SCR 14 13.65 57.3 14.00 1455-6926 17.67 54 -70 11.64 252.4 12.02 16.15 0.201SCR 55 14 12.87 10.60 10.27 1455-4846 29.6 14.45 54 -71 217.4 12.59 00.73 0.192SCR 47 14 13.06 9.70 15.82 11.43 1455-8150 15.85 37.9 55 11.49 -49 271.5 12.02 04.04SCR 40 14 12.46 0.196 13.66 1456-7239 16.57 06.2 55 12.07 -73 162.2 12.34 27.37SCR 47 14 15.23 14.09 0.219 11.29 1457-8409 14.75 44.5 55 9.48 11.40 -69 216.8 04.97SCR 26 14 12.95 14.84 0.295 11.78 1457-4843 16.41 9.15 27.4 56 11.72 -48 13.33 02.29SCR 319.9 46 14 12.71 12.84 0.202 3.19 11.22 1457-5012 29.6 57 17.22 -81 12.86 44.19SCR 232.9 50 14 13.90 14.53 0.200 2.15 11.56 1459-7007 32.9 57 12.57 -72 18.52 8.56 10.80 33.90SCR 229.7 39 14 11.49 0.331 1500-5606 15.37 41.4 57 12.34 -84 15.12 12.12 41.45SCR 275.1 09 14 12.32 0.265 3.49 12.33 1501-4723 16.8 59 16.49 2.94 10.18 -48 17.73 10.83 23.94SCR 265.9 43 15 8.43 0.207 14.51 2.97 12.20 39.3 1502-7214 29.1 00 13.29 11.47 -50 17.27 103.7 11.31 33.52SCR 005.7 12 15 0.362 2.56 1507-4931 15.12 34.4 01 15.51 10.21 -70 16.52 54.28 9.98SCR 225.0 13.68 07 15 0.183 1.67 11.23 1507-6803 11.18 20.4 02 15.35 10.73 -56 15.96 14.16SCR 216.0 06 15 14.11 0.221 10.06 63.1 1507-4740 13.57 49.4 07 14.74 32.3 -47 16.50 100.5 13.16 09.55SCR 076.3 23 15 10.59 0.202 2.50 10.45 1508-6816 13.83 14.2 07 14.26 -72 17.02 13.58 21.25 227.0 14 15 12.25SCR 1.45 0.270 0.80 84.6 12.54 03.0 07 14.22 12.95 1508-8302 -49 13.10 127.6 10.01 03.83 039.0 31 15 12.99 0.196SCR 13.47 05.3 08 14.81 13.39 1510-5454 -68 15.17 11.70 59.03 3.29 216.8 03 11.91 0.300SCR 15 2.72 11.99 34.7 10.76 1510-5141 -47 15.53 111.7 08 12.43 178.2 40 33.10 12.32 0.195 9.74SCR 2.00 15 13.58 41.6 13.64 11.45 1513-4945 -68 15.00 195.7 10 11.36 214.6 16 10.62 18.2 15.50 0.181SCR 3.23 15 10.18 41.7 13.50 12.19 1514-5017 12.58 10 -83 11.76 173.6 12.58 56.56 0.202 02 15 11.83SCR 13.32 1.69 11.15 54.7 16.91 13 1517-8208 10.06 34.7 -54 230.4 10.03 40.66 0.191 77.9 54 15 11.67SCR 2.38 11.58 17.66 05.2 14 12.05 1522-4725 -51 246.0 9.86 11.51 05.38 60.5 41 12.19 0.324 14.75SCR 15 16.87 35.6 1522-8409 -49 231.0 17 10.75 2.71 9.74 [243.6] 45.3 45 50.25 9.38 15.68 0.281SCR 3.25 11.81 15 15.55 00.7 10.89 1522-7024 -50 22 10.67 246.9 17 12.74 16.07 08.68 0.329SCR 2.36 9.32 15 18.09 35.2 10.05 1530-6823 243.6 22 -82 220.3 12.99 13.51 19.95 0.230SCR 08 2.83 10.68 15 9.25 10.05 18.17 1531-6937 56.2 22 11.63 -47 276.1 13.90 16.01 28.02 0.263 1.94 25 15 9.52 16.49 08.3 30 11.90 9.83 41.6 -84 238.2 11.98 02.21 64.9 09 15 16.21 0.200 11.10 13.95 143.3 13.2 31 13.14 3.60 9.82 -70 266.7 13.96 04.37 2.23 24 15.23 0.199 11.33 17.55 41.4 11.25 -68 8.91 235.7 14.66 10.83 77.9 23 11.32 0.217 12.55 16.58 122.6 30.7 12.87 -69 255.1 2.13 11.02 37 13.40 15.91 0.307 0.73 10.68 34.6 15.49 13.77 087.7 12.30 8.66 15.15 0.323 12.36 119.7 2.75 24.9 16.97 9.59 11.33 204.5 10.43 13.53 0.219 14.50 13.27 2.65 13.15 229.1 12.10 13.22 14.82 10.74 17.68 12.87 304.1 3.12 81.2 9.39 13.08 44.4 14.05 11.20 17.69 12.20 3.78 10.46 13.40 15.93 12.27 38.9 17.00 2.93 13.20 0.34 10.03 8.84 15.63 11.63 42.8 2.26 12.69 12.02 14.04 14.70 12.68 3.14 53.3 11.45 13.53 9.56 8.58 12.12 46.3 12.64 2.44 12.35 149.1 12.57 33.8 11.97 3.91 11.92 12.07 64.7 8.92 11.21 11.36 [212.2] 97.4 3.04 11.84 10.71 2.95 8.71 11.10 1.93 37.4 1.30 10.44 2.13 108.6 [194.0] 89.5 3.29 28.0 1.64 3.66 132.9 3.49 83.9 35.4 46.3 37.8 84 d d d (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 1532-6950SCR 1537-6928SCR 15 1542-4731 32 05.13SCR 15 1546-4733 37 55.84 15SCR 42 1547-7106 -69 41.40 50 15SCR 23.7 46 1550-4718 -69 44.18 28SCR 15 50.7 1552-7052 -47 47 31 07.97 0.299SCR 15 54.4 1552-8108 -47 50 33 55.19 0.247SCR 15 29.8 1555-4733 52 -71 249.3 46.86 0.263SCR 06 15 1558-7045 14.2 52 -47 226.9 38.55 0.181SCR 18 15 16.21 1601-8428 48.6 55 -70 230.6 54.65SCR 52 15 0.379 1609-6854 18.10 01.9 58 -81 230.7 48.36SCR 08 16 14.77 0.413 1611-7526 18.18 44.9 01 -47 240.2 42.12SCR 33 16 15.95 0.468 1615-7035 17.64 35.0 09 -70 42.32SCR 247.6 14.06 45 16 16.36 0.194 1616-8403 30.1 11 17.54 -84 11.47SCR 216.0 28 16 13.82 15.95 0.196 1618-7516 10.7 15 -68 16.12 13.24 38.80SCR 236.0 54 16 14.86 0.187 1618-8212 15.53 40.7 16 -75 16.32 12.26 56.37SCR 246.7 26 16 13.88 0.273 1620-7553 30.0 12.69 18 14.23 -70 15.41 13.22 39.61SCR 229.2 35 16 0.255 14.59 1621-7709 16.0 18 14.18 11.71 -84 15.70 12.14 32.89SCR 208.6 03 16 0.181 12.63 1622-7220 13.22 55.7 20 13.64 12.60 -75 16.37 44.08 218.7 13.72 16 16SCR 0.223 11.51 11.92 09.4 21 14.13 1627-7337 11.51 -82 18.06 57.68 182.6 12 16 11.79 0.205SCR 12.39 12.17 08.7 22 14.07 1631-7925 -75 16.52 13.05 59.49 213.7 53 10.80 0.236SCR 16 11.23 13.21 43.1 16.05 1633-6834 -77 17.99 27 11.19 086.2 09 37.11 11.57 0.236SCR 16 12.24 34.0 14.44 12.87 1633-7004 -72 18.41 31 10.28 210.1 20 11.34 47.23 0.244 1.53SCR 16 14.30 02.0 16.20 10.98 1634-6320 16.63 33 -73 10.93 234.5 11.29 01.69 0.258SCR 37 3.69 16 12.64 16.49 10.06 1636-7806 06.3 16.77 33 10.79 -79 199.1 13.08 46.54 0.203SCR 3.14 25 16 14.86 14.45 10.73 1637-7437 16.40 48.2 34 10.75 [208.3] -68 216.0 11.92 38.77SCR 3.81 34 16 14.67 0.439 14.73 10.56 1637-6232 18.35 09.4 36 12.67 -70 197.3 13.99 47.81SCR 04 16 12.51 14.35 0.320 1.81 10.48 1637-6826 17.38 30.9 37 11.42 -63 13.49 235.8 08.06SCR 55.8 20 16 12.62 16.11 0.207 2.44 12.37 1641-7520 18.45 110.7 01.5 37 13.42 -78 11.42 22.62SCR 194.6 06 16 12.46 15.16 0.183 3.38 11.24 1643-6327 34.2 37 12.95 15.71 -74 11.97 44.59SCR [226.8] 239.6 49.5 37 16 14.08 16.47 0.204 2.07 13.22 1646-6434 19.0 41 10.90 -62 16.91 11.21 17.72SCR 215.8 32 16 12.80 0.182 2.79 12.74 1646-6419 13.88 41.3 43 11.43 -68 16.87 13.03 54.73SCR 305.9 26 16 14.72 0.225 2.78 10.57 77.2 1647-6557 54.6 46 14.94 10.57 -75 17.30 11.71 21.36SCR 212.3 20 16 0.281 2.97 13.26 11.22 34.4 1648-7238 43.9 46 15.43 12.49 -63 17.41 13.19 12.79SCR 198.3 27 16 0.185 2.51 10.33 81.7 1648-6252 12.77 35.5 47 15.11 11.14 -64 17.93 51.98SCR 199.5 12.65 34 16 0.193 2.21 12.29 58.7 1649-7643 13.40 16.6 48 15.30 12.60 -64 16.73 17.41SCR 199.7 19 16 11.45 0.245 3.00 10.83 50.8 1649-7036 13.88 31.1 48 15.86 -65 16.94 122.0 12.01 57.49SCR 186.8 57 16 12.05 0.256 3.03 12.33 1651-8229 14.35 55.5 49 14.55 -72 17.61 10.90 26.05SCR 223.3 38 16 12.88 0.215 2.77 87.2 1652-7609 13.87 18.8 49 15.06 11.94 -62 15.80 248.3 11.44 05.92SCR 205.3 52 16 13.38 0.210 3.14 1652-6931 12.85 17.9 51 15.58 10.65 -76 16.39 141.7 12.32 13.61SCR 206.7 43 16 12.44 0.332 3.08 1652-7444 13.09 20.5 52 13.79 11.19 -70 17.22 12.81 49.72SCR 190.9 36 16 11.84 0.184 3.45 48.6 1652-6655 14.16 36.7 52 14.09 12.13 -82 18.33 11.88 04.90SCR 192.7 29 16 11.89 0.279 3.28 78.4 1653-7237 11.96 45.6 52 14.78 12.64 -76 16.63 11.26 46.53 185.3 09 16 13.08 0.225 41.0 12.21 12.5 52 16.00 1.23 11.64 -69 18.40 105.7 11.36 47.31 205.6 31 16 11.05 0.193 12.95 14.2 53 14.47 3.49 11.04 -74 13.30 12.48 45.84 165.8 44 11.23 0.283 45.6 14.48 11.1 16.25 3.38 11.17 -66 16.24 10.42 169.8 55 11.79 0.205 [151.7] 98.4 12.76 21.8 11.72 2.23 12.30 -72 17.15 10.65 206.4 37 13.28 0.298 14.36 18.5 14.16 1.92 10.18 13.80 11.17 195.4 11.74 0.185 10.89 15.49 3.42 10.43 43.1 15.73 12.67 218.7 12.76 0.203 12.51 11.84 2.72 10.93 63.8 18.48 11.23 224.4 139.2 10.33 13.50 13.57 3.17 12.38 15.46 12.25 053.8 198.1 11.71 10.97 16.38 2.51 11.00 16.90 12.17 11.49 9.76 13.39 2.73 11.99 67.6 18.47 11.16 10.25 14.31 15.03 2.86 68.9 11.56 10.59 12.06 16.38 2.99 10.96 65.3 9.61 137.5 12.95 13.24 9.61 2.73 11.30 10.01 11.10 14.42 2.73 47.1 12.34 12.20 3.49 48.0 9.46 10.55 12.93 9.77 12.11 54.0 11.69 119.4 2.45 10.29 1.39 12.34 3.32 11.42 68.9 12.10 75.5 1.59 2.98 3.43 77.2 53.7 2.29 65.4 2.83 3.45 49.8 34.8 82.0 59.4 84.4 80.7 85 d d d d d (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 1654-5737SCR 1654-6439SCR 16 1655-6239 54 40.26SCR 16 1655-6650 54 12.98SCR 16 1655-6432 55 -57 47.41SCR 37 16 1656-4708 41.2 55 -64 46.31SCR 39 16 1658-6731 59.3 55 -62 26.52SCR 39 16 0.186 1700-7930 27.6 56 -66 07.57SCR 50 16 0.181 1700-6653 47.9 58 -64 198.2 02.99 32 17SCR 0.185 59.0 00 1700-7452 -47 27.60 200.9 08 17 0.235SCR 16.6 00 17.52 1700-6950 -67 01.37 236.5 31 0.203SCR 17 15.8 1701-6212 -79 16.80 00 255.7 30 16.10 0.183SCR 17 15.71 19.7 1701-6742 -66 16.53 00 238.8 53 12.83 0.222SCR 17 12.1 14.70 1702-7106 18.25 01 -74 212.5 11.67 0.264SCR 52 15.10 17 14.93 1702-7628 41.7 17.56 01 -69 189.6 15.91 0.194SCR 50 17 13.28 16.36 1703-5922 13.16 51.8 02 -62 188.3 14.16 25.58SCR 12 17 13.86 0.193 15.42 1705-6349 15.38 34.0 02 -67 228.7 12.37 09.93SCR 42 17 14.07 11.00 0.258 1705-7115 16.85 52.3 13.57 03 -71 13.02 299.9 56.54SCR 06 17 13.74 13.34 0.196 1706-6330 15.52 24.4 05 11.80 -76 12.82 34.41SCR 197.4 28 17 10.17 14.66 0.219 13.46 1707-6521 21.0 05 12.41 17.04 -59 12.69 26.19SCR 199.3 22 17 11.81 13.53 0.212 11.56 1707-6354 47.9 06 12.31 -63 18.07 38.01SCR 173.3 49 17 13.09 0.218 12.25 1709-6636 15.46 9.59 46.4 07 12.13 -71 18.20 10.80 31.02SCR 194.7 15 17 12.67 0.227 12.03 1709-7154 56.7 07 16.03 -63 17.04 11.98 23.44SCR 216.0 30 17 0.256 14.54 11.92 1712-7108 22.5 09 15.86 10.19 -65 17.81 8.94 12.02 06.12SCR 157.4 21 17 0.282 1.56 1714-7008 14.61 57.5 09 14.89 11.43 -63 16.95 32.15SCR 152.0 13.72 54 17 0.201 2.33 1714-7129 14.00 59.8 12 15.76 11.47 -66 19.29 38.42 9.97SCR 189.0 36 17 13.36 8.75 0.217 1.91 11.21 1715-7414 13.01 48.5 14 14.64 -71 17.12 13.25 02.13SCR [276.9] 166.8 54 17 13.19 0.238 3.54 11.28 1715-5821 13.88 58.8 14 16.43 -71 16.78 12.84 29.15SCR 262.0 08 17 11.86 0.322 2.73 1715-6712 12.64 04.9 15 15.06 13.01 -70 14.35 104.0 12.66 46.38SCR 169.6 08 17 12.73 0.241 1717-6916 14.44 23.5 15 14.81 12.64 -71 14.69 161.9 11.29 11.13SCR 203.1 29 17 11.58 0.227 1718-6036 13.23 31.7 15 12.35 12.47 -74 17.79 12.04 14.95 2.54SCR 194.4 14 17 13.36 1.42 0.206 2.67 82.2 1720-6547 12.88 39.8 17 13.15 11.00 -58 18.46 103.8 10.98 52.67 236.0 21 17 12.13SCR 0.210 1.50 11.20 45.4 18 15.36 1721-7341 11.90 -67 17.17 12.81 06.96 209.3 12 17 11.59 0.389SCR 12.43 53.7 20 16.47 1.74 10.72 1721-7004 -69 15.67 11.65 05.72 177.3 16 10.66 0.222SCR 17 13.45 43.3 15.20 2.67 12.55 1722-5638 -60 17.80 21 10.99 46.3 175.3 36 42.99 11.86 37.0 0.287SCR 75.9 17 14.16 23.3 13.56 2.67 11.42 1724-5637 -65 16.89 114.8 21 10.01 202.0 47 12.16 26.19 0.466 [245.0] 17 13.24SCR 22.2 15.62 3.03 10.74 16.05 22 1724-6102 -73 11.28 217.8 12.82 30.78 0.213 41 17 12.18 16.27SCR 3.02 01.0 15.90 24 11.58 1725-5417 -70 320.9 152.1 11.99 36.41 0.206 9.85 04 13.36 13.90SCR 17 3.06 11.14 17.51 46.8 12.27 1725-7358 -56 196.7 135.7 24 11.28 38 14.20 44.53 0.194 14.91SCR 3.07 11.33 17 17.45 01.9 11.45 1726-7404 -56 181.8 25 11.88 37 12.07 15.38 39.14 0.274SCR 2.94 12.07 58.9 17 13.40 03.2 10.72 1727-5851 25 13.01 -61 318.6 12.95 15.03 11.47 0.185SCR 02 3.23 11.16 89.6 17 15.63 11.31 1727-7410 25.6 26 11.17 -54 184.6 13.33 12.28 43.50 0.421SCR 10.52 49.6 17 17 12.36 16.43 1727-5439 105.7 49.6 27 12.10 1.69 -73 202.3 12.86 13.53 15.09 1.29 11.05 58 17 0.199 10.59 14.30 53.6 27 12.48 -74 154.5 11.72 11.43 3.20 12.13 79.1 04 17 15.02 0.226 11.45 15.04 33.5 27 11.48 -58 11.81 206.3 08.58 3.65 10.40 49.3 51 12.00 0.181 11.87 15.17 24.3 11.57 -74 198.3 3.21 14.18 11.28 10 13.38 0.214 10.94 109.7 34.6 10.95 17.45 59.0 -54 185.2 2.27 11.65 39 11.16 13.11 0.188 11.20 41.1 11.64 13.40 193.4 3.74 10.66 59.5 11.80 0.253 10.41 15.56 17.86 10.96 153.7 3.26 11.11 77.8 11.42 0.251 12.83 10.58 15.76 10.83 212.7 2.72 10.19 61.2 14.72 15.69 10.32 17.36 10.39 136.3 2.81 66.5 12.73 10.04 13.66 10.23 18.13 2.91 43.8 14.17 10.16 13.62 123.3 15.02 14.00 3.55 9.85 10.03 12.50 16.21 9.60 13.66 0.70 51.9 12.44 13.09 11.51 2.59 92.9 11.75 14.80 13.38 9.63 11.88 86.0 9.10 11.91 1.62 10.58 11.09 38.3 13.58 1.04 102.1 11.68 11.33 2.55 9.02 10.91 9.95 13.05 [214.0] 50.8 11.12 1.40 2.72 12.88 9.37 68.8 51.2 3.26 [309.4] 0.98 9.22 1.91 37.2 3.11 2.63 74.3 36.9 88.9 1.56 58.1 177.1 43.7 SCR 1653-6442 16 53 11.65 -64 42 15.7 0.185 213.6 17.24 15.70 14.85 13.89 13.29 13.17 1.81 [243.7] 86 d d d d d d d a a (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 1727-7053SCR 1728-5720SCR 1729-6906SCR 17 1730-6934 27 14.06 17SCR 28 1730-7501 54.83 17SCR 29 -70 1730-5609 29.72 53 17SCR 50.8 30 -57 1730-6932 21.60 20 17 43.9SCR -69 30 1731-5538 06 04.75 0.203 17 12.3 -69SCR 30 34 1732-5643 27.68 0.188 17 00.6SCR 30 -75 140.0 1732-5908 56.07 0.197 01 17SCR 10.2 -56 185.0 31 1732-5831 0.321 09 16.01SCR 17 16.00 29.6 -69 238.3 1732-7219 32 32 0.268 28.39SCR 17 11.65 35.3 191.8 1733-7445 32 -55 13.87 13.00 0.345 38SCR 17 17.06 40.2 1734-8202 32 196.1 -56 10.77 54.29 0.199 43SCR 17 16.19 29.4 1734-5926 32 -59 220.1 12.46 15.09 04.61SCR 08 17 0.181 13.88 1734-5542 31.4 33 -58 214.2 10.30 14.21 20.39 31SCR 17 0.208 14.50 39.6 1734-5605 34 11.56 -72 14.06 169.7 31.53SCR 19 17 12.96 0.208 16.40 1736-5901 42.0 34 -74 12.24 20.25 223.2 45 17 9.89 13.30 0.192 10.95SCR 21.9 34 13.17 17.30 -82 1737-6831 57.45 177.8 12.23 02 17 14.23 0.327SCR 16.4 34 11.04 -59 16.89 1738-5607 34.07 178.0 10.73 26 17 11.49 0.222 12.61SCR 15.89 38.4 36 9.40 -55 17.23 11.94 1738-7600 21.35 214.2 42 13.02 0.252 10.52 17SCR 31.6 14.82 -56 16.20 37 1738-5942 11.20 179.1 12.46 05 22.68 0.193 15.18SCR 17 45.4 11.56 14.95 -59 17.73 1739-7027 38 12.12 9.35 236.2 10.25 01 03.17 0.264 17 13.59 50.6 14.15 10.48SCR 15.68 38 -68 178.3 1739-8222 14.57 25.08 0.240 11.44 31 17 12.92 15.66 11.54 57.5 17.62 38SCR -56 192.1 2.32 13.01 41.02 0.185 1740-5646 10.37 07 17 12.30 13.71 18.69 15.1 14.02 39 -76 317.3SCR 11.45 27.00 11.37 00 1742-6923 13.71 0.182 15.77 17 17.00 28.8 12.48 -59 177.1SCR 1.93 39 11.11 42 1742-7239 12.11 45.36 16.37 0.271 13.88 15.29 24.4 0.89 10.86 17 -70SCR 3.17 12.39 187.9 40 27 1742-6817 13.77 14.75 0.218 12.28 18.45 46.96 05.3 10.56 17 70.4 11.20 -82SCR 1.02 203.1 13.85 42 13.15 0.280 22 1743-6234 10.61 56.17 11.83 17.96 02.2 17 12.14 186.6SCR 2.11 12.54 186.6 42 -56 16.45 0.282 10.35 1743-5943 28.55 10.57 46 17 16.69 12.06 148.2 58.0 2.11 11.55 42SCR -69 11.61 16.22 0.465 48.55 43.4 11.63 1744-6238 [129.2] 23 17.27 41.4 11.46 17 195.9 07.0 14.61 1.32 -72SCR 10.39 43 14.49 11.50 39 1744-7043 16.57 48.96 0.448 10.89 17 19.7 211.8 -68SCR 1.80 15.38 11.38 43 15.37 10.86 17 1745-7357 16.69 38.83 0.197 12.96 66.2 22.5 17SCR 3.50 11.18 12.61 103.2 -62 229.5 14.21 10.24 44 1746-8211B 0.199 34 17.05 [386.8] 18.63 14.36SCR 35.4 17 3.04 10.57 13.77 14.62 -59 194.3 12.43 1747-6031 44 0.243 43 48.60 11.92 18.47SCR 17 3.27 10.03 31.4 11.93 17 148.1 1748-5628 177.1 45 15.03 -62 13.71 46 0.196 05.64 12.70 38 21.54SCR 17.21 2.51 12.13 12.90 212.3 06.7 1748-7211 -70 11.35 15.90 0.365 10.38SCR 43 17 12.14 3.64 38.2 13.53 14.21 1751-6104 15.0 47 188.9 -73 12.09 -82 15.66 47.93 11.66SCR 57 17 18.19 4.32 45.1 0.296 11 11.12 1752-4742 24.7 48 56.6 196.3 14.44 10.27 10.67SCR 17 3.29 72.0 12.89 0.325 9.83 15.72 11.89 1753-7403 48 -60 11.10 13.76 182.5 16.11 51.79SCR 31 17 2.26 57.5 0.184 0.228 17.71 13.83 1754-5954 41.6 51 -56 12.37 05.52 237.5 28SCR 17 3.49 57.6 14.26 10.85 9.69 09.5 1755-7241B 52 12.59 18.39 9.58 -72 14.41 17.48 191.2SCR 11 184.9 17 35.2 13.33 15.92 0.216 1.85 1757-5646 53.0 53 12.19 -61 16.04 32.61 13.66SCR 04 17 42.6 0.206 17 12.02 2.57 16.31 1757-5821 06.8 54 13.32 55 -47 14.25 8.96 13.42 09.12 13.19 214.0 32.16 42 14.27 52.3 0.428 2.67 24.1 14.01 -74 12.98 207.9 11.76 [309.7] 03 17 82.3 0.188 12.77 15.40 46.4 57 12.13 11.36 -59 17.13 -72 12.81 34.86 191.0 54 17 8.37 41 0.310 12.24 2.95 32.7 12.46 57 21.4 3.83 18.13 16.15 177.9 12.55 14.21 0.181 10.86 77.2 15.05 12.29 2.14 -56 16.99 108.8 179.0 46 11.19 9.65 0.187 12.38 0.199 23.3 8.25 15.92 -58 18.50 13.66 2.07 194.6 21 10.00 12.03 12.89 50.6 14.85 18.43 10.65 238.9 3.08 175.2 0.270 [151.6] 14.03 57.7 8.55 16.19 13.51 20.8 16.28 11.51 0.190 12.87 9.38 16.19 10.43 [232.9] 18.00 15.60 159.9 2.79 12.98 14.61 14.04 7.99 10.98 199.6 11.57 1.29 13.64 1.32 16.22 13.54 18.24 9.15 12.48 94.1 13.35 3.11 11.80 10.75 16.78 10.99 12.47 7.71 14.34 137.8 16.00 12.10 2.10 12.26 12.76 [179.6] 10.56 15.34 2.82 10.74 11.96 12.89 11.18 14.37 27.0 12.57 [279.5] 98.9 13.55 9.96 11.66 2.14 12.34 10.62 13.48 3.55 12.21 2.81 2.94 12.08 51.9 10.38 9.70 12.91 3.28 11.58 2.83 12.71 36.4 3.72 11.31 43.2 111.8 14.5 3.33 46.8 2.36 3.48 126.7 2.51 60.9 3.13 91.4 60.3 26.1 160.9 74.2 87 a c a a c a a d a a a c d d b (pc) Est Dist Notes J ······ ······ − F 59 R s JHK 12.58 12.08 11.85 15.30 14.15 14.62 IVN I F 59 R J ········· ) ◦ Table Appendix (cont’d) )( 00 µ θ B ··············· (J2000) (J2000) ( Name RA DEC SCR 1759-5105SCR 1800-5112A 17 18 59 00 12.11 29.91 -51 -51 05 12 03.6 12.7 0.230 0.289 257.6 226.5 16.13 14.09 13.00 12.22 11.68 11.49 1.87 121.1 SCR 1800-5112BSCR 1800-4925SCR 18 1800-6441 00 29.91SCR 1801-4724SCR 18 1801-5855 00 -51 42.76SCR 18 12 1801-7000 00 12.7 59.80SCR 18 1802-5338 01 -49 41.62SCR 25 18 0.317 1804-5541B 40.8 01 -64 24.68SCR 41 18 1804-8007 51.3 01 -47 28.85 220.3SCR 24 18 18 0.212 1804-5541A 24.1 02 04 -58 46.98SCR 29.22 55 0.208 1806-5436 36.6 -70 14.23 167.2SCR 00 18 18 0.185 1806-4923 49.4 04 04 -53 -55 21.58 203.1 31.10SCR 38 41 0.227 1807-5359 14.9 13.67 06.3 17.23 141.5 18 0.240SCR 06 1809-6154A -80 18.30 -55 18.44 221.1 07 18 41 0.200SCR 0.198 11.46 13.4 06 15.20 16.5 16.95 1809-6154B 14.98 160.7 18SCR 18 07 16.32 -54 18.59 1810-6401 09 06.47 179.5 36 201.7 13.42 05.35 0.193 0.222SCR 13.17 04.8 14.72 18 -49 15.10 1810-5527 09 23SCR 02.62 14.40 58.1 16.47 -53 14.01 1810-7144 19.36 12.90 -61 180.2 194.4 59 12.25 0.212SCR 54 18 12.98 53.2 13.00 1811-5510 14.5 10 -61 12.97 37.96 0.194SCR 18 15.20 54 12.71 17.66 12.69 14.06 1811-6144 11.94 10 11.71 14.6 198.9 11.91 49.77 0.190SCR 18 10.97 0.218 1813-7325 10 12.46 -64 143.6 13.71 12.57SCR 01 18 12.00 12.32 15.70 10.81 11.43 0.201 16.82 1813-4905 01.4 11 11.36 -55 191.3 10.01 34.95 253.2SCR 27 18 12.24 14.45 1814-7133 03.7 11 13.14 -71 11.48 46.87 14.13SCR 44 259.8 18 10.97 10.24 14.66 0.181 11.18 17.18 1814-4848 56.1 13 -55 16.82 45.56SCR 10 18 9.41 12.49 0.189 12.93 0.25 1816-6615A 37.8 13 10.90 -61 13.67 17.28 48.99 179.2SCR 44 18 12.50 15.08 0.248 1816-6615B 9.86 33.7 14 13.93 9.96 -73 57.74 186.3SCR 25 18 11.68 18 0.482 2.95 10.77 1817-7527 13.43 03.8 14 9.16 16 15.48 -49 13.25 11.54 05.39 197.7 09.08SCR 05 [178.3] 13.08 18 0.219 3.35 13.54 1817-5026 42.3 16 -71 17.13 9.22 12.05 9.56 197.9 09.08 33 0.197SCR 2.81 06.5 11.29 14.25 10.90 1817-5825 -48 17.38 -66 12.00 190.6 48 18 12.84 15 0.251 2.77SCR 59.5 17 14.95 14.4 11.51 17.39 1818-5455 -66 50.22 176.2 18 9.02 15 0.271 9.49 13.14 10.64SCR 77.9 10.29 17 15.43 11.35 14.4 17.58 1818-7504 12.32 22.63 133.6 0.259 0.209 18 1.23 11.29SCR 95.4 12.99 3.54 15.16 2.99 -75 17.48 17 1819-5912 164.7 12.57 27 27.34 11.09SCR 71.0 18 13.61 13.6 15.45 12.09 -50 16.73 159.6 1819-5014 9.66 18 178.0 207.1 26 11.95 05.38SCR 18 12.87 57.3 15.51 16.72 1819-5414 12.43 18 -58 12.46 15.94 0.235 25SCR 18 13.25 14.64 59.4 18.26 1820-5317 18.08 19 163.4 11.31 -54 9.03 11.62 2.46 11.11 0.198 0.85 3.12SCR 93.8 55 18 13.45 14.89 26.1 1820-5553 18.7 19 11.94 -75 221.0 12.06 16.92 0.44 04 18 12.34 0.269 16.13SCR 16.14 11.09 30.2 19 11.06 1820-6357 -59 183.2 12.32 11.28 3.08 12 18 13.32 8.87 0.292 1.10 11.69SCR 17.17 06.5 20 11.50 -50 1820-6225 11.25 221.3 06.49 14 18 13.94 15.71 0.207 10.78SCR 18.19 2.34 11.5 20 11.74 -54 1821-6532 12.34 32.1 46.62 47.2 170.7 48.0 14 15.37 0.244 18 11.24SCR 134.0 14.6 10.74 17.98 -53 20 1821-5549 12.99 15.21 174.0 [159.3] 17 40.59 16.22 0.182 11.49SCR 18 09.9 11.86 -55 17.00 1821-5622 20 199.1 59.8 53 14.39 49.35 0.330 3.00 10.46 18 16.07 07.7SCR 12.47 14.14 17.69 21 163.9 -63 1821-5951 206.6 14.43 1.63 11.00 0.211 57 2.96 11.65 18 14.79 18.6 15.35 21 13.07 -62 186.4 45.90 0.213 3.54 15.46 12.22 25 14.52 18 15.76 17.81 52.7 21 13.23 -65 185.9 07.25 3.39 32 12.47 0.197 12.64 12.58 18 15.73 17.4 -55 149.5 21 14.45 3.19 61.2 49 13.41 59.54 15.40 0.190 12.72 18.31 17.0 -56 11.23 37.7 236.2 3.39 12.37 88.2 22 11.71 14.28 0.204 17.43 39.0 13.91 12.31 -59 164.8 2.55 12.51 42.5 13.45 16.25 0.424 51 10.68 17.99 48.5 11.69 198.6 3.14 57.4 0.92 12.34 15.36 0.391 13.70 11.75 13.35 12.19 181.0 72.0 13.82 10.44 16.09 0.365 11.04 18.08 11.34 228.4 41.4 13.37 11.48 107.8 11.18 11.65 16.97 12.47 2.30 194.9 15.17 10.89 102.9 448.4 16.15 10.79 16.01 12.27 2.99 11.34 14.63 11.82 17.49 8.44 14.08 1.62 10.59 15.03 13.91 11.71 3.55 11.55 12.61 161.3 16.32 13.49 13.69 3.45 11.41 9.14 11.98 128.4 [317.8] 11.56 0.94 13.32 15.73 13.14 10.94 3.21 8.49 10.99 2.94 36.6 15.20 12.92 10.42 3.78 65.8 10.73 8.30 15.01 3.09 99.7 10.18 60.2 2.00 14.91 60.7 54.8 2.46 [269.5] 71.0 3.07 2.04 2.97 1.12 189.1 50.1 22.4 [588.9] 43.1 88 d d a (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 1828-5558SCR 1828-5050SCR 1831-4932SCR 18 1831-5912 28 08.78SCR 18 1832-5804 28 16.45SCR 18 1834-5000 31 -55 43.21SCR 58 18 1836-5219 05.6 31 -50 25.20SCR 50 18 1836-6727 14.4 32 -49 24.18SCR 32 18 0.202 1836-4756 06.3 34 -59 48.67SCR 12 18 0.252 1837-6057 18.7 36 -58 12.71 172.1SCR 04 18 0.209 1838-6514 30.6 36 -50 34.04 190.9SCR 00 18 0.214 1840-7152 05.9 36 -52 16.19 27.12 173.0SCR 19 18 0.216 1840-4900 08.1 37 -67 17.99 21.26 179.6SCR 27 18 0.227 1843-5154 33.6 38 14.12 -47 16.42 34.92 172.3SCR 56 18 0.277 1844-6032 53.3 40 15.89 -60 14.78 41.99 191.8SCR 57 18 0.186 12.31 1844-6225 05.6 40 14.59 -65 18.12 48.17 177.5SCR 14 18 0.316 13.79 1849-6705 26.1 43 12.80 -71 17.25 58.65 195.0SCR 52 18 11.22 0.294 12.91 1850-4905 17.8 44 16.13 -49 18.11 34.32 185.0SCR 00 18 12.70 0.196 11.25 1850-6257 20.9 44 15.10 -51 11.34 10.62 32.51 201.8SCR 54 18 12.24 0.205 14.82 1851-6156 49.4 49 15.96 -60 16.90 12.21 47.96 193.6 32 18 10.60 0.278SCR 12.90 08.5 50 10.46 10.40 1852-7345 -62 16.83 11.65 53.70 197.6 25 18 13.77 0.182SCR 13.82 58.2 50 14.90 12.00 -67 17.93 1853-4725 54.73 171.4 05 18 11.99 0.373SCR 10.09 54.1 9.95 51 14.76 11.44 -49 17.08 1853-7537 13.20 55.36 162.3 05 12.37 0.211 18SCR 12.75 02.4 15.91 -62 18.40 52 1855-6425 11.45 168.3 57 25.46 0.186SCR 18 12.94 24.8 14.88 13.07 -61 15.91 1856-4704 9.75 53 9.71 11.77 298.9 56 11.85 09.43 0.192SCR 18 13.75 56.2 16.44 2.91 11.16 18.56 1857-5841 53 -73 143.3 11.87 26.61 0.221 45SCR 18 13.08 13.59 3.19 11.48 24.2 16.80 1859-5211 55 11.37 -47 175.2 9.44 12.09 24.41 0.328SCR 25 18 14.92 16.48 2.35 18.38 1859-5432 03.2 56 11.30 -75 202.8 12.09 38.40SCR 37 18 12.03 0.212 14.98 11.11 18.26 1859-8233 39.8 57 11.52 -64 245.2 13.77 53.27SCR 25 18 14.15 9.35 16.27 0.244 2.36 11.04 47.9 18.33 1902-7550A 29.4 59 2.20 11.48 -47 11.41 178.6 48.21SCR 04 18 13.02 16.27 0.304 3.11 11.29 92.1 14.09 1903-7419 58.3 59 13.30 -58 103.9 12.32 47.91 232.1SCR 41 18 15.02 19 16.14 0.257 3.59 11.30 1903-5412 54.6 59 10.80 02 14.78 -52 11.36 13.64 168.7 50.53 11 14.48 12.10 0.252 13.04 10.6 11.75 -54 18.18 211.9 13.66 187.7 32 19 13.97 0.185 3.05 10.60 13.95 21.0 03 47.2 10.77 -82 12.20 -75 13.17 50.62 131.3 33 19 10.30 50 0.71 0.198 2.90 11.43 63.2 51.0 03 15.58 55.2 13.13 18.37 12.34 28.43 138.7 0.233 3.82 13.37 10.49 56.1 12.68 -74 16.29 171.1 19 9.85 0.204 0.303 2.80 12.89 14.15 9.50 07.7 16.09 11.82 -54 17.91 168.2 12.81 12 2.67 12.42 67.0 11.0 13.93 15.29 164.5 168.8 12.98 44.0 0.203 2.18 11.56 65.0 13.79 15.90 9.09 12.93 12.45 8.88 0.223 4.16 48.4 11.65 13.09 11.18 16.41 12.45 169.3 12.31 3.62 74.7 14.31 11.74 12.39 187.9 165.3 8.34 10.29 8.69 2.61 11.66 10.28 14.51 12.30 17.94 11.74 13.02 3.10 68.3 10.94 17.75 10.86 3.79 43.5 7.73 12.85 9.75 16.21 11.44 12.45 9.91 10.40 37.4 15.53 169.9 10.20 11.83 14.50 1.14 12.17 7.50 115.9 9.45 2.61 9.25 13.21 9.79 2.59 11.28 13.14 9.98 54.0 11.54 [182.3] 3.78 11.07 8.91 9.68 12.59 10.95 120.5 25.4 2.89 12.43 1.51 3.63 8.85 10.67 2.23 50.2 2.68 1.35 109.1 20.0 21.4 3.07 1.04 50.5 3.98 75.9 55.6 123.9 32.8 32.1 SCR 1821-5544SCR 1822-5349SCR 1822-5114SCR 18 1823-5849 21 38.13SCR 18 1824-8428 22 06.36SCR 18 1825-5749 22 -55 17.25SCR 44 18 1825-5745 53.4 23 -53 42.25SCR 49 18 1825-5607 00.4 24 -51 27.87SCR 14 18 0.243 1825-7152 21.0 25 -58 12.48SCR 49 18 0.208 1825-5640 27.7 25 -84 55.97 181.8SCR 28 18 0.267 1826-6542 40.6 25 -57 53.04 183.2 49 18 0.239SCR 03.6 25 1827-5732 -57 15.25 24.60 191.9 45 18 0.193 01.6 25 -56 15.54 03.64 192.9 07 18 0.263 13.9 26 13.29 -71 16.52 46.83 177.5 52 0.323 18 34.7 13.93 -56 18.60 27 210.6 40 18.34 0.307 11.89 59.9 14.46 -65 14.82 006.0 42 0.226 13.53 39.9 16.36 17.28 -57 173.9 11.21 0.260 32 12.42 12.97 26.5 15.07 160.5 13.23 0.311 14.11 15.12 15.88 10.57 212.5 11.54 11.38 0.285 12.91 14.62 12.80 178.9 12.50 12.95 13.79 10.39 15.38 10.98 10.16 212.4 11.18 12.57 12.75 18.68 11.87 11.49 11.90 13.35 10.76 19.07 10.23 11.40 9.52 16.44 11.61 10.89 10.86 11.67 16.48 10.76 12.91 9.68 2.08 10.64 9.29 10.20 10.76 0.71 15.82 10.17 10.57 2.92 9.40 10.16 9.97 14.88 3.86 9.95 9.96 67.9 210.9 14.26 9.91 3.63 2.81 58.1 14.15 9.55 51.8 2.67 2.93 1.82 37.5 30.7 2.60 1.60 5.87 33.1 38.1 59.9 44.1 [392.1] 9.2 89 d a a a d d d d d ··· (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 1908-5407SCR 1908-4713SCR 1911-5018SCR 19 1912-5034 08 09.01SCR 19 1912-4910A 08 55.41SCR 19 1912-4910B 11 -54 21.14SCR 07 19 19 1913-5800 41.3 12 12 -47 45.02 23.97SCR 13 19 1914-7836 56.4 12 -50SCR 21.86 18 0.310 1914-6028 45.8 -50 -49SCR 34 19 10 0.189 1914-7109 34.4 13 51.4 -49 03.80 161.9 19 10 0.328 14 54.0 06.62 262.4 19 0.447 0.229 14 -58 17.44 55.28 187.8 00 19 0.254 31.6 14 -78 18.22 34.09 233.7 187.7 36 00.7 15.57 -60 16.08SCR 28 185.5 0.209 1919-4833 00.2 16.29 -71 18.23 15.57SCR 09 0.187 13.62 1919-6953 47.9 14.00 16.24 354.1SCR 0.220 14.42 1920-5130 16.02 13.71 287.8SCR 19 12.34 0.214 11.96 1924-5302 19 14.33 17.49 48.89 247.7SCR 19 13.19 13.69 1925-7310 11.68 19 17.21 11.83 57.49 168.7SCR 19 10.87 1925-7844 20 15.13 12.32 -48 16.73 12.66 32.56 33 19 12.18 10.67SCR 08.1 24 15.62 11.58 1926-8744 -69 10.49 10.26 12.86 53 19 11.17 12.77 56.2 25 14.65SCR 12.43 -51 11.67 19.53 1926-5218 10.06 30 19 0.201 14.90 07.2 25SCR -53 31.91 10.56 1926-6146 02 8.14 11.59 0.230 9.98 19 13.53 54.0 11.35SCR -73 26 265.3 1926-8216 10 39.60 13.56 0.184 9.79 02.9 19SCR -78 10.31 11.01 168.6 26 1927-5808 44 12.61 0.180 48.70 42.2 3.23SCR 8.66 19 16.03 -87 12.94 207.4 1928-8549 26 0.205 44 30.23 3.10 10.72 04.6 19 17.41SCR 12.04 249.9 26 -52 0.288 1928-7714 14.03 48.64 18 12.80 19 16.09 176.3 8.69 18.2 27SCR 3.13 -61 0.396 15.22 00.59 1930-6258 3.84 11.87 46 19 17.16 159.3 33.0 28SCR -82 3.04 13.00 14.12 51.67 76.2 1930-7638 16 16.39 3.16 0.494 19 117.7 47.6 233.7SCR -58 28 8.34 13.38 15.22 1931-5840 08 17.13 49.61 0.203 30.0 12.05 19 -85 13.09SCR 191.2 14.41 3.54 30 49 0.195 1931-8502 18.23 30.34 22.5 12.03 35.6 19 13.48 -77 15.46SCR 155.3 2.05 48.3 8.25 30 0.181 11.49 14 1932-5209 09.03 12.13 16.97 37.5 19 35.8 12.73SCR 172.5 2.04 31 16.01 42.3 -62 0.225 11.43 1932-5005 21.57 12.60 58 18.05 14.32 19SCR 203.5 39.1 11.30 -76 11.54 31 1934-5140 15.22 0.386 11.48 38 12.22 30.28SCR 115.9 19 14.73 11.17 40.4 46.1 -58 12.08 1934-6343 204.8 32 16.11 12.80 40 17.67 0.185 28.03SCR 19 11.35 37.1 184.8 10.90 14.39 1935-6319 135.1 32 -85 10.01 -0.54 18.08 13.66 48.64 0.210 02SCR 19 11.84 12.25 45.9 1936-8616 14.28 34 204.3 15.70 -52 09.33 0.402 17.36SCR 09 19 10.64 13.54 1936-4736 18.9 10.20 34 13.15 16.05 -50 269.2 50.02 05 19 1.98 12.03 0.285 12.69 16.87 38.9 14.13 35 -51 135.7 15.57 12.96 10.05 40 19 3.20 0.198 12.95 16.65 42.1 14.20 36 -63 9.04 171.5 46.69 12.23 43 19 1.99 15.30 0.257 12.60 16.82 47.3 36 12.86 -63 14.94 32.09 158.1 19 2.62 14.92 0.233 12.75 07.8 106.5 18.60 -86 11.92 157.5 11.99 14.78 16 2.93 8.43 14.69 0.201 13.63 02.3 -47 17.42 127.2 12.25 36 13.40 2.66 57.5 0.184 16.50 08.5 108.3 16.87 11.79 13.49 138.8 13.32 13.03 0.180 2.35 111.1 15.45 8.31 14.76 12.01 12.41 138.0 0.264 15.40 12.98 14.51 1.68 12.12 12.18 12.89 094.8 53.6 14.12 121.1 12.97 11.78 13.03 3.42 153.2 [194.7] 14.11 12.79 11.99 10.83 11.66 18.67 12.94 11.57 [229.7] 11.96 11.99 18.16 3.10 13.60 10.75 11.43 10.11 16.42 0.96 3.30 12.41 12.09 11.50 16.31 13.33 80.0 10.11 1.93 14.04 12.21 9.58 11.55 10.88 1.81 14.95 83.5 12.57 9.85 2.51 17.3 11.07 [207.5] 86.1 10.46 9.14 13.71 2.51 11.99 [178.8] 2.39 10.38 13.13 9.07 2.51 11.75 103.1 12.91 3.76 [228.5] 91.7 0.89 135.0 1.12 1.24 3.85 113.9 24.4 2.60 70.7 42.5 57.2 180.2 SCR 1903-5313SCR 1903-7846SCR 1904-5732SCR 19 1906-5857 03 34.49SCR 19 1907-7924 03 34.36 19SCR 04 1908-6129 -53 37.22 13 19 10.8 06 -78 07.83 46 19 31.0 07 -57 53.45 32 0.230 19 17.3 -58 08 57 36.82 0.290 58.7 -79 175.4 24 0.200 02.5 -61 149.8 0.189 29 32.6 17.01 158.2 0.271 17.07 278.0 0.199 14.66 17.57 038.7 15.21 17.48 200.3 13.13 15.47 15.53SCR 14.08 15.52 1914-8241 17.29 12.15SCR 13.54 13.59 1915-5046 12.74SCR 14.08 1917-5221 15.56 11.50 12.31SCR 19 11.77 1917-4915A 14 12.18 13.00 12.83 19 14.70 11.28 15 11.73 10.36 47.43 19 19 11.94 17 12.52 17 -82 54.71 38.29 13.77 41 11.44 50.8 -50 46 9.82 12.27 17.7 -52 -49 13.17 21 15 0.196 46.7 54.2 0.209 2.52 13.05 9.56 200.4 0.258 0.216 2.47 178.3 3.16 15.91 323.4 200.3 2.53 16.62 79.1 13.97 16.70 120.5 15.10 14.60 1.79 3.23 68.4 12.18 14.54 12.84 139.8 12.75 10.77 [240.9] 13.18 11.45 11.51 28.9 10.15 11.82 10.71 10.88 11.25 10.05 9.88 10.62 11.07 9.82 3.20 3.09 2.72 2.13 33.0 48.5 68.9 48.2 90 d a c a d a a c (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 1936-4957SCR 1937-4842SCR 1937-5147SCR 19 1937-5800 36 32.66SCR 19 1938-7829 37 37.45SCR 19 1938-5048 37 -49 32.28SCR 57 19 1939-6757 55.5 37 -48 51.70SCR 42 19 1940-6349 30.9 38 -51 54.67SCR 47 19 0.224 1940-5205 46.4 38 -58 03.48SCR 00 19 0.189 1940-6330 51.0 39 -78 22.59 172.6SCR 29 19 0.183 1941-4752 20.0 40 -50 14.52 180.6SCR 48 19 0.193 1942-7431 39.7 40 -67 16.76 16.59 138.4SCR 57 19 0.192 1942-4921 35.1 40 -63 15.71 30.12 164.1SCR 49 19 0.244 1942-4854 14.4 41 14.51 -52 13.36 00.48 163.8SCR 05 19 0.186 1943-7716 32.0 42 13.67 -63 11.40 33.42 261.0SCR 30 19 0.186 11.97 1944-4751 53.5 42 11.99 -47 17.16 57.98 201.6SCR 52 19 0.187 12.69 1944-7700 08.3 42 10.11 -74 17.90 15.47 225.6SCR 31 19 10.81 0.250 11.29 1946-7713 08.3 43 15.44 -49 18.41 47.99 152.2SCR 21 19 11.91 0.227 1947-7329 15.8 44 15.91 -48 17.44 10.21 00.44 187.1 9.38SCR 54 19 10.98 0.202 13.59 1947-7646 59.6 44 16.42 -77 18.32 11.27 24.15 151.9SCR 16 19 0.308 14.11 1948-5914 08.5 46 15.60 -47 18.62 10.44 53.00 155.8SCR 51 19 11.80 0.233 9.94 9.47 14.89 1948-7604 10.3 47 16.29 11.11 -77 18.23 03.52 241.9SCR 00 19 12.79 0.215 14.58 1949-7110 22.4 47 16.20 10.40 -77 18.06 11.19 14.69 156.0SCR 13 19 13.58 0.263 14.31 1953-7220 46.2 48 16.14 -73 16.14 9.00 12.29 58.76 156.8SCR 29 19 13.45 0.187 13.54 1953-5037B 53.9 48 16.08 10.96 -76 17.20 13.13 10.94 269.4SCR 46 19 13.06 0.241 13.95 1953-5037A 55.3 49 13.85 12.03 -59 18.06 12.84 46.01 179.4SCR 14 8.86 19 11.74 19 0.214 3.70 14.55 1954-8552 23.2 53 15.29 1.76 12.83 53 -76 18.46 12.53 35.96 179.1SCR 41.06 04 12.40 19 0.235 11.83 1954-5216 55.5 16.07 53 1.01 12.63 -71 17.52 11.13 148.3 42.39SCR 10 13.25 0.415 13.21 1954-6737 41.2 16.32 12.30 -72 16.46 -50 11.84 133.8SCR 20 19 10.76 39 0.261 14.28 1955-6228 03.8 54 15.49 16.0 3.64 10.82 17.19 -50 12.69 43.50 151.7SCR 102.9 19 12.14 37 0.205 27.2 14.10 1956-8228 54 14.76 54.5 3.12 11.57 17.58 10.19 32.27 309.9SCR 0.64 19 12.69 0.200 0.171 13.97 1956-6052 54 15.19 2.84 12.53 79.8 -85 16.59 11.56 53.97 135.3SCR 52 19 12.42 0.181 13.55 1957-7032 29.0 55 15.78 2.16 -52 18.47 12.14 32.61 137.9 16 142.9 19 12.70SCR 9.95 13.12 39.1 56 14.63 3.22 11.32 47.1 1958-5609 -67 16.30 11.88 41.41 144.3 37 19 12.27 0.230SCR 13.35 45.0 56 16.28 4.46 11.92 95.7 -62 12.18 1958-8000A 19.52 12.13 40.10 156.7 28 19 47.5 11.98 0.193SCR 12.39 21.9 57 14.33 3.73 11.64 -82 1958-8000B 16.11 11.70 14.55 166.4 186.8 28 11.39 0.194 19SCR 14.13 19 12.2 10.95 2.83 11.87 17.40 -60 58 1959-6236 11.34 58 174.4 102.4 52 31.26 11.11 0.256 46.70SCR 13.23 55.8 19 13.91 11.48 -70 17.37 1959-5549 10.78 58 183.7 32 12.40 0.185 3.09SCR 44.18 10.70 05.2 14.90 3.14 11.12 27.5 17.92 2000-6734 -56 10.57 160.6 -80 12.46 0.335 09SCR 19 00 11.94 15.53 3.38 10.49 56.2 10.6 18.39 2002-6356 59 44.5 11.83 237.9 135.6 -80 33.55 0.279 12.85 19 00 15.58 3.90 10.27 15.73 9.93 59 11.87 45.8 169.5 10.72 58.76 20 13.69 0.494 16.36 0.183 2.78 11.53 13.35 00 -62 202.1 12.24 41.99 34.8 36 20 13.98 13.64 2.49 11.67 69.1 0.192 17.38 13.4 02 10.12 -55 9.40 12.41 161.9 42.83 149.1 49 15.03 12.13 3.21 78.9 18.51 11.90 29.6 -67 12.71 34 145.8 11.93 15.49 0.189 4.39 53.9 32.5 11.84 17.59 -63 15.28 13.77 9.85 56 11.54 9.26 16.21 0.413 3.52 99.2 02.0 12.11 19.54 10.84 288.7 14.07 0.220 3.88 11.66 99.8 15.55 13.25 13.58 10.81 169.9 13.93 0.213 1.87 11.84 59.0 10.26 17.85 17.48 12.98 173.9 14.40 13.04 27.0 4.55 13.50 10.22 16.18 12.71 167.5 35.9 15.36 16.28 12.44 11.81 9.99 3.19 13.29 1.03 11.41 10.15 50.3 13.95 12.20 16.40 131.3 14.05 3.12 12.18 12.68 10.31 12.76 10.81 2.88 11.86 11.82 45.0 14.51 13.60 11.07 2.59 12.52 10.62 9.79 31.6 10.46 35.8 12.87 13.28 10.49 2.81 1.32 82.7 11.99 2.52 87.2 9.55 9.87 10.23 189.0 3.50 11.45 2.26 2.17 9.04 9.62 41.1 64.9 11.17 134.3 3.80 8.90 [169.0] 70.8 4.29 61.3 133.4 3.49 2.52 24.3 0.76 25.0 84.6 36.0 SCR 1936-8104SCR 1936-4826SCR 1936-4816 19SCR 36 1936-5535 16.09 19 36 31.54 19 36 -81 33.29 04 19 11.1 -48 36 26 01.80 26.4 -48 16 0.206 53.5 -55 0.343 35 51.5 173.9 0.311 230.8 0.189 17.55 073.3 17.13 147.9 16.14 17.23 15.11 17.46 14.46 15.05 13.39 14.90 12.43 12.55 12.31 14.53 11.83 11.05 11.81 13.64 11.58 10.47 11.59 12.96 10.18 12.84 3.71 2.80 3.99 1.26 65.7 90.4 [228.8] 26.3 91 d b d a b a a a b c a a ··· (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 2007-7409SCR 2008-7322 20 07 21.62SCR 2013-5847 20 08 -74 56.52SCR 09 2016-7531 51.1 20 13 -73 39.23 22 0.183 48.9 20SCR 16 -58 2017-6711 11.25 210.7 47 0.280 15.8 -75 14.28 187.9 31 0.193 20 04.5 17 54.18 13.52SCR 18.11 161.1 2019-4701B 0.253 -67 11 13.09 16.18 18.18 25.4 20 081.3 19 36.15SCR 12.63 2023-8211 14.64 16.32 0.182 17.07 -47 01 12.34SCR 13.48 54.3 172.4 2025-5115 14.28 14.75 20 23 12.30 20.69 12.89SCR 0.265 17.87 12.67 2028-5958 12.25 20 25 -82 12.70 158.1 15.92 09.74 12.07SCR 11 10.47 2029-7910 05.3 20 28 17.41 -51 11.80 14.12 54.13SCR 15 0.190 2029-5757B 03.1 9.86 0.89 20 15.17 29 12.81 -59 45.54 123.0SCR 58 20 0.228 2031-7807 03.5 29 2.70 9.51 46.25 12.88 12.29 -79 17.97 132.6SCR 10 167.6 0.189 2032-4948A 06.2 3.65 -57 11.89 12.02 20 57 31 16.26 52.8 18.04 33.08 139.5 155.7 20 0.287 32 11.28 42.24SCR 0.314 14.39 16.15 -78 17.81 2033-5748 4.28 135.5 07 11.00 11.1 67.0 -49 107.8 12.39 48SCR 14.60 16.00 49.8 17.61 2036-7021 3.12 0.273 20 33 17.45 11.84 13.45 47.93 0.265SCR 14.47 15.61 2036-6454B 16.2 162.0 20 11.58 15.34 36 12.92 -57 179.0 13.13 30.47SCR 48 13.85 3.28 20 16.45 2036-6454A 12.5 37 95.7 02.50 13.54 12.78 17.42 12.55 -70 12.23 21 20 14.75 0.187 08.5 36 -64 12.38 57.21 54 15.39 12.39 11.68 42.7 213.6 13.22 52.5 0.188 3.87 11.79 -64 54 13.33 11.42 0.190 53.3 17.04 11.62 138.0 2.70 11.56 12.25 153.3 0.197 15.12 11.07 18.63 2.87 57.6 11.75 17.67 146.0 10.87 13.49 16.45 166.8 3.38 11.50 15.68 14.96 12.35 14.22 2.96 128.8 13.82 12.54 11.73 12.68 12.68 3.12 62.1 11.40 11.56 12.05 3.14 79.0 12.06 11.14 11.88 11.80 10.44 58.2 75.3 2.77 10.28 3.77 3.00 89.2 1.41 62.6 88.2 72.7 SCR 2002-5824SCR 2004-5408 20 02 53.97SCR 2005-8916 20 04 -58 10.06 24 17.1 20 -54 05 08 30.14 0.216 21.9 -89 136.3 0.186 16 51.9 11.66 150.2 0.219 10.35 18.49 217.2 16.43 17.16 9.61 14.67 15.25 9.28 13.05 14.40 8.81 12.51 13.44 12.30 8.69 12.84 12.69 3.38 1.07 1.80 93.1 35.3 [213.7] SCR 2006-6259SCR 2008-8239 20 06 16.57SCR 2009-6005 20 08 -62 36.82SCR 59 2015-7050 50.5 20 09 -82 23.35 39 0.199SCR 16.7 2016-7945 20SCR 15 -60 2017-5715 30.61 129.7 05 0.286 43.6 20SCR -70 13.53 16 2017-6438 145.0 50 49.74 0.414 20 47.5 17 23.47 12.03SCR 15.32 -79 154.3 2018-4836 0.279 45 20 53.0 17 -57 11.01 15 10.98 13.55 18.17 09.0SCR 174.1 2020-7806 0.434 20SCR -64 18 10.24 2021-7411 38 11.91 15.87 13.66 0.250 18.31 48.8 128.4 20SCR 10.72 -48 170.9 20 2023-5922 13.71 9.60 16.08 0.189 36 52.98 16.74 20 51.7 21 16.88 10.03SCR 17.71 12.10 134.7 2027-4812 14.08 -78 16.09 0.410 9.45 06 20 18.7 23 -74 15.70 39.05 11.58SCR 11 12.94 13.08 9.84 2029-6404 29.5 147.2 15.75 20 0.276 27 -59 11.26 14.50 11.76 08.28 12.55SCR 22 0.234 17.38 2029-6342 15.10 22.5 209.2 20 29 13.27 -48 12.35 11.12 54.29 1.79 093.9SCR 12 15.02 15.19 0.230 2030-7950 05.6 16.03 20 12.75 2.83 29 11.23 -64 18.44 57.21 14.64 192.1SCR 04 13.33 0.228 2032-8000 16.09 08.3 3.77 12.52 20 10.85 30 16.35 -63 18.19 12.08 15.94 46.2 120.6 42 0.213SCR 16.12 46.4 2032-4948B 3.00 10.76 20SCR 39.7 14.43 32 16.33 11.61 -79 14.16 2033-6411 27.40 154.2 15.92 50 0.213 20 53.0 46.4 32 0.99 12.92 41.74 11.37SCR 14.43 12.15 -80 12.73 2034-4850 15.60 248.7 2.44 00 113.2 0.292 20 24.0 33 12.36 -49 12.97 48.40SCR 11.07 48 11.62 15.68 [482.5] 17.98 2036-5131 57.2 134.6 0.53 0.185 20 12.05 34 12.47 -64 10.60 26.74SCR 11 10.82 158.4 15.98 0.270 17.70 2036-6210 14.4 130.7 3.11 20 12.22 36 -48 10.76 07.32 182.4 50 13.70 9.94 15.86 0.284 16.16 36.6 20 0.17 36 10.24 -51 17.15 12.31 56.42 203.4 31 13.82 14.51 0.299 3.44 36.6 9.74 69.0 10.11 16.77 11.72 -62 18.05 12.25 [834.9] 236.1 10 13.02 0.195 3.36 53.5 11.44 16.73 15.98 11.64 16.51 11.39 202.8 0.226 79.5 16.63 11.40 14.10 14.29 1.55 10.76 15.38 098.0 0.86 96.1 15.87 12.89 10.58 12.03 13.38 13.37 3.67 15.88 12.37 11.07 11.96 12.32 57.5 3.61 72.7 12.14 10.47 11.43 11.50 3.12 55.8 10.22 10.80 11.03 0.15 57.3 10.60 10.37 3.09 50.6 [900.1] 10.25 3.22 100.8 1.95 1.29 38.2 77.8 72.6 SCR 2018-6606 20 18 28.70 -66 06 44.5 0.462 191.3 17.72 15.75 14.70 13.67 13.14 12.99 2.08 [228.0] SCR 2003-6217SCR 2005-6548 20 03 39.83 20 05 -62 40.70 17 34.2 -65 48 0.245 46.6 175.9 0.209 18.25 159.8 16.35 18.03 14.73 16.16 13.24 14.22 12.69 12.79 12.49 12.26 11.99 3.11 3.38 118.7 84.9 92 d d a a c a c a c a d a c a (pc) Est Dist Notes J ······ − F 59 R s JHK 12.33 11.75 11.66 IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B ··············· (J2000) (J2000) ( Name RA DEC SCR 2037-6347SCR 2038-7618SCR 2039-7912 20SCR 37 2039-5242 37.61 20SCR 38 2040-6422 32.80 20SCR 39 -63 2040-7923 59.56 47 20SCR 28.2 -76 39 2042-5737 18 28.10SCR 20 42.1 -79 2042-7500 40 12 24.88 0.264SCR 20 24.7 2043-6347 40 -52 24.37 0.260 42SCR 20 38.0 2043-7552 42 -64 139.0 46.44 0.217SCR 22 20 2043-6220 16.7 42 -79 171.7 12.24SCR 23 20 0.193 17.61 2043-7826 51.5 43 -57 183.2 07.07SCR 37 20 0.188 16.31 2044-7848 15.3 43 -75 191.6 59.31SCR 00 20 15.50 0.283 17.47 2044-6316 57.5 43 -63 25.72 150.6SCR 47 20 14.39 0.264 2047-6537 04.9 43 18.14 -75 45.90 023.8SCR 52 20 13.42 15.79 0.210 2047-5823 45.5 44 -62 15.32 48.07 142.6SCR 20 20 12.64 0.254 2049-7200 16.39 52.9 44 -78 16.39 12.11 13.84 284.9SCR 26 20 14.14 0.184 2050-7849 56.3 47 13.53 -78 15.07 11.68 11.82 134.2SCR 48 20 0.204 15.66 2050-8051 34.7 47 14.52 11.49 -63 16.20 12.34 35.83 118.7 16 20 0.391SCR 12.61 46.9 49 13.22 11.13 2052-6607 -65 17.52 59.68 191.6 14.51 37 20 0.312 11.22SCR 13.04 34.8 50 14.23 11.79 -58 12.02 2052-5202 39.71 147.5 23 20 12.13 0.232 10.90SCR 11.56 46.7 50 15.14 -72 12.20 2053-6017 13.94 11.75 135.8 00 11.38 0.184 20 11.56SCR 12.22 44.4 10.06 -78 18.04 52 2055-6525 11.46 118.6 49 39.29 0.224SCR 20 12.81 31.9 10.72 13.76 -80 17.59 2057-6358A 9.97 52 10.87 122.7 51 11.15 30.81 0.294SCR 20 51.5 16.09 11.39 18.04 2057-6358B 53 -66 167.1 9.35 11.62 11.66 0.206 07 3.38SCR 20 20 15.77 10.66 20.6 17.94 2057-6358C 55 10.65 57 -52 215.1 9.88 9.53 11.60 0.180 56.20 2.71SCR 02 14.29 16.14 20 15.43 2058-5550 55.2 11.13 57 -60 194.1 3.45SCR 56.20 17 8.83 13.95 0.249 20 15.96 10.39 17.39 2059-5646 27.4 58 -65 154.2 -63 12.34SCR 30.06 25 9.84 14.31 58 9.03 13.55 0.219 1.88 10.83 17.95 2059-6201 26.2 42.2 -63 12.23 232.6SCR 55.2 20 14.28 58 15.52 0.198 1.40 13.70 2059-6218 8.23 58 11.74 42.2 -64 13.13 18.39 139.7SCR 69.1 20 12.12 00 16.18 0.257 0.187 3.13 2100-5804B 9.27 59 11.71 59.4 18.17 13.19 41.24 [343.6] 159.5SCR 69.2 20 13.22 12.62 11.50 2100-5804A 59 12.60 -55 17.45 8.02 10.52 16.17 136.6SCR 139.9 50 20 14.28 21 3.08 11.51 0.130 2101-6624 16.05 00.9 59 12.65 00 -56 15.16 123.2 9.14 11.76 10.29 33.15 46 12.00 3.25 21SCR 3.53 12.37 05.2 15.46 00 2104-5229 -62 16.33 16.77 12.50 34.93 01 138.7 9.93 0.252 14.91 12.46SCR 51.2 21.4 13.95 11.17 -62 2105-8530 -58 11.19 18 21 04 0.200SCR 13.49 39.0 01 14.32 11.96 15.28 09.1 2106-7822 -58 18.48 15.50 047.9 14.07 04 0.209 21 3.75 11.01SCR 46.8 13.34 9.67 17.5 10.69 04 2110-7459 1.22 152.8 00.58 12.12 22.7 0.187 3.54 11.72SCR 43.6 0.181 21 12.80 13.46 16.38 -66 18.12 2111-4707 0.88 13.56 05 131.3 24 12.29 51.15 0.186 3.01 10.60SCR 21 02.8 16.98 2112-5428B 06 -52 11.50 163.7 116.1 11.89 12.77 26.35 29 2.77SCR 21 14.37 16.06 13.33 43.5 18.29 2112-7525 10 11.74 -85 117.6 51.32 0.180SCR 54.5 30 21 15.09 21 11.24 14.44 2112-5428A 57.2 26.6 11 19.41 11.26 12 12.11 -78 24.61 12.40 3.76SCR 64.2 56.65 22 13.93 0.400 16.21 3.03 11.64 119.9 2112-7231 16.83 03.0 44.0 -74 113.4 3.68SCR 59 21 13.32 21 13.51 0.209 11.06 17.49 11.54 136.5 2114-5515 12.3 12 12 -47 11.77 -54 12.52 233.7 36.51 55.12 1.42SCR 07 14.26 28 0.328 14.81 14.58 2118-4721 02.6 06.8 12.09 110.7 21 12.93 15.79 0.328 1.98 11.48 12 11.98 17.59 -75 -54 12.44 50.73 181.2 46.2 25 21 28 13.53 12.72 0.188 32.9 3.34 0.152 18.4 14 14.3 11.42 15.10 12.18 54.59 14.07 136.2 66.4 21 1.66 11.75 15.41 18 11.85 -72 18.05 12.13 10.27 [270.9] 195.5 79.1 31 117.0 11.64 0.193 0.209 2.43 11.18 2.51 44.4 12.74 11.79 -55 13.52 14.15 15 14.42 11.58 07.6 16.24 11.53 -47 16.04 17.08 10.57 148.0 095.3 21 0.306 11.80 57.8 11.53 3.97 13.28 07.0 12.16 116.3 13.43 0.203 11.33 14.01 13.70 15.27 16.01 13.37 102.0 130.5 11.21 9.90 0.269 3.54 80.4 10.95 12.94 104.2 12.08 3.00 11.87 14.03 13.49 11.32 18.04 10.61 143.0 10.10 3.77 46.7 12.76 9.75 12.75 11.56 11.11 10.15 1.32 12.59 3.42 10.57 16.05 10.39 16.53 68.3 2.68 9.54 11.49 11.27 10.49 12.10 66.0 13.93 14.64 9.54 9.61 54.3 10.85 10.25 138.2 147.0 9.27 11.47 12.46 12.49 1.98 2.15 9.32 10.38 8.99 80.5 1.53 11.25 11.93 11.55 4.16 [207.2] 9.91 8.80 11.74 11.05 49.2 2.59 2.06 10.81 75.6 9.76 5.12 1.94 43.3 1.71 3.59 49.0 40.8 13.5 105.7 3.09 1.11 35.6 68.0 58.6 54.4 93 d d d a d d (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 2124-6311SCR 2125-5350SCR 21 2126-5246 24 49.49SCR 21 2130-7733 25 42.47 21SCR 26 2131-8038 -63 45.33 11 21SCR 35.2 30 2131-7119 -53 02.90 50SCR 21 33.2 2134-8027 -52 31 46 17.09 0.190SCR 21 38.7 2134-5400 -77 31 33 04.50 0.224SCR 21 23.9 2136-7819 34 -80 157.2 57.74 0.207SCR 38 21 2136-5153 37.2 34 -71 144.0 59.45 0.186SCR 19 21 2140-7417 12.33 43.2 36 -80 118.8 41.34SCR 27 21 0.302 2142-8125 17.77 02.4 36 -54 128.6 53.25SCR 00 21 10.64 0.198 2142-6412 16.26 21.5 40 -78 167.0 45.94SCR 19 21 15.93 0.187 2144-5539 15.73 11.5 42 -51 23.58SCR 167.5 53 21 10.08 14.24 0.197 2151-6154 52.6 42 15.90 -74 35.22 143.5 17 21 14.16SCR 14.12 0.311 19.2 44 2151-8604 -81 16.07 12.85 150.9 25 21 12.17 0.187SCR 14.60 9.35 43.4 51 2152-5448 -64 14.35 12.89 59.01 135.8 12 12.48 0.366SCR 21 56.9 14.24 2153-6122 -55 18.16 51 10.79 224.8 39 37.35 0.309SCR 13.81 21 40.8 13.47 12.33 2153-7422 -61 18.37 52 8.67 10.98 110.1 54 10.66 0.248SCR 21 12.82 07.4 16.18 10.19 2154-5502 17.62 53 -86 162.8 12.67 04.06 0.209SCR 04 12.12 21 12.91 16.39 10.41 2154-4754 33.3 18.43 53 -54 107.7 12.16 8.62 33.81 0.362SCR 48 21 14.37 15.60 2154-7346 18.07 28.3 12.08 54 9.93 -61 140.9 12.09 15.40SCR 10.18 22 21 14.99 0.454 16.25 2154-5345 17.70 11.4 54 11.60 -74 160.8 12.91 02.53SCR 22 21 14.24 16.20 0.292 11.94 2155-7330 18.23 23.4 54 11.71 -55 13.39 192.7 08.98SCR 02 21 14.09 15.67 0.248 11.38 2158-7809 18.05 05.4 54 12.33 -47 13.03 42.09SCR 081.1 3.03 54 21 14.64 16.34 0.209 11.64 2159-7505 02.3 55 12.91 16.56 -73 12.40 1.30 47.49SCR 120.8 46 21 13.33 15.80 0.194 12.10 2200-7342 13.0 58 12.47 3.45 -53 18.09 13.47 20.16SCR 102.6 3.14 45 21 15.01 0.190 12.68 2200-5051 14.48 27.3 59 11.85 -73 17.73 12.12 52.26SCR 132.3 30 22 14.04 0.378 1.93 12.30 2200-7602 105.6 24.3 00 15.88 13.00 -78 17.62 13.85 26.01SCR 069.3 09 22 0.184 13.57 2.09 11.59 2201-8012 08.9 00 15.48 11.54 -75 17.75 12.97 31.6 21.47 160.7 05 22SCR 0.459 1.38 12.79 13.93 26.4 00 15.63 2201-6154 13.26 30.2 -73 16.46 08.96 [130.8] 122.6 42.7 12.74 42 22 0.267SCR 3.27 11.26 12.99 08.4 01 15.26 12.45 2202-7339 -50 16.85 43.56 202.0 51 12.53 0.321SCR 22 3.00 13.12 13.41 22.4 14.32 2203-4949 -76 16.49 110.4 01 12.23 117.2 02 54.38 11.64 0.182 2.57 12.25 22 13.71SCR 49.2 14.84 -80 15.77 125.4 02 2204-7401 11.93 132.3 12 12.04 03.55 0.260 3.84 22 12.00 46.2 14.53 12.03SCR 17.52 03 -61 11.07 2205-7839 134.4 12.35 13.65 0.254 54 2.72 89.9 12.86 13.97SCR 22 11.69 48.3 16.85 134.9 11.47 2207-7149 -73 125.8 04 10.71 0.346 3.56 39 12.91 59.09 15.84SCR 10.78 22 15.84 134.8 34.3 11.77 2207-8418 -49 089.2 05 11.60 2.49 49 11.85 0.186 14.98 11.83SCR 11.18 22 17.69 07.5 10.13 2210-6429 220.9 07 12.04 -74 2.84 52.9 13.68 13.98 37.61 0.204SCR 01 11.52 22 16.24 167.3 11.17 2211-5024 42.3 07 10.59 178.4 -78 12.67 15.83 44.89 0.185 1.74SCR 39 22 16.44 11.48 2212-4706 44.8 10 11.98 9.84 -71 114.6 54.5 12.74 14.40 32.57 3.35 10.88 49 22 209.0 0.268 10.05 14.55 28.3 11 11.27 -84 127.5 13.96 14.68 45.98 3.84 11.25 18 22 115.1 0.204 11.43 17.63 54.0 12 11.83 [160.5] -64 12.99 130.1 17.72 3.59 29 13.09 0.188 10.69 18.10 48.2 12.59 9.78 -50 13.82 129.1 2.91 11.16 24 15.60 0.185 11.16 31.7 11.86 17.21 -47 126.5 12.39 10.41 68.3 06 16.20 0.222 12.10 15.2 12.50 3.61 16.62 150.8 3.24 11.05 37.1 13.83 0.194 11.30 15.54 13.85 12.03 113.7 2.50 11.85 51.7 14.71 0.184 11.95 14.73 17.64 12.52 116.4 11.09 72.3 14.72 11.48 12.08 3.38 18.16 13.24 168.5 3.86 11.74 12.56 15.59 11.96 26.9 16.12 3.71 54.6 13.79 11.34 11.17 16.08 12.74 18.31 2.15 87.9 11.33 11.70 14.28 14.14 13.13 3.24 10.46 12.53 14.38 16.24 31.5 10.74 2.53 48.4 13.14 13.04 13.02 2.18 35.2 13.50 14.24 9.78 10.46 12.59 90.4 11.65 1.05 12.98 86.1 12.29 3.08 12.43 9.61 10.99 81.1 2.96 124.6 12.73 11.65 [119.1] 1.76 10.83 3.40 11.38 81.2 131.1 [236.9] 2.46 1.62 2.59 2.48 41.1 3.95 150.7 51.0 165.6 69.1 45.4 SCR 2120-7551SCR 2123-7110SCR 21 2123-4832 20 24.91 21SCR 23 2124-5417 15.89 21 23 -75 10.91 51 21 28.6 -71 24 10 00.70 00.4 -48 32 0.185 50.9 -54 0.194 17 26.3 134.5 0.188 096.4 0.271 17.70 177.7 12.17 182.7 15.54 14.01 11.48 16.83 13.16 12.28 11.14 14.79 11.67 11.32 10.41 13.87 11.06 11.09 12.96 9.99 10.74 10.50 12.38 10.37 9.95 12.21 3.88 1.19 1.07 1.83 35.4 [168.2] 78.4 52.2 94 a a d d d d a d a a c d d a (pc) Est Dist Notes J − F 59 R s JHK 11.85 11.24 10.91 4.50 24.6 ··· IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 2218-5310BSCR 2219-5359 22SCR 18 2221-7346 46.17SCR 2222-6146 22 19SCR -53 55.35 2223-7405 10 22 53.8SCR 21 2224-7242 36.44 22SCR -53 22 2224-5014 59 0.191 40.59 01.7SCR 22 -73 2226-5246 23 46 14.46SCR 51.0 22 2228-6952 095.9 24 -61 0.194 51.58 46SCR 22 16.4 2228-5843 24 -74 0.245 27.72SCR 05 22 17.37 109.0 2228-7334 42.8 26 -72 58.56SCR 42 22 0.207 2228-6645 00.0 28 189.7 -50 22.64SCR 15.15 14 22 17.76 0.245 2230-7825 08.6 28 -52 172.3 24.87 46 22 0.189SCR 16.81 12.9 28 2230-7442 -69 15.57 19.43 13.44 119.9 52 22 0.210SCR 18.8 28 18.39 -58 2230-5244 34.59 250.1 43 22 15.09 0.182SCR 49.2 30 -73 12.53 15.75 2230-5743 13.63 07.37 256.7 34 0.209 22SCR 16.32 50.7 -66 15.80 30 2233-5858 147.8 14.28 45 19.24 0.192 22 11.94 54.9 13.81 12.44SCR -78 17.99 30 2234-5313 129.5 25 27.95 0.245 15.48 22 08.8 13.80SCR 16.03 13.59 30 -74 165.2 2235-7718 11.70 20.20 0.182 11.84 42 22 12.25 15.83SCR 28.8 15.83 33 -52 150.3 2235-6620 14.51 32.94 0.184 44 11.79 13.02 14.02 22SCR 18.31 29.1 -57 115.0 11.58 34 2237-6238B 11.30 43 14.13 27.19 0.211 13.66SCR 22 14.50 30.0 14.01 -58 207.2 2237-7039 35 10.46 12.89 58 12.26 16.45 33.91 0.369 22 17.01 13.6 22SCR 10.65 35 13.19 -53 155.0 37 2238-4936 12.52 12.36 23.52 0.186 13.74 13 56.38 17.28SCR 39.3 2.62 10.83 -77 125.7 2241-6333 14.44 9.87 14.87 0.191 10.45 18 22 12.70 17.65SCR 05.9 37 12.17 -66 150.6 2241-4943 -62 10.77 15.39 49.60 20 0.219 38 10.26 22SCR 19.02 3.13 25.4 13.63 01.8 292.5 38 2241-6119A 13.23 12.46 15.84 01.57 0.225 9.57 11.50SCR 22 11.84 1.50 -70 2241-6119B 14.15 41 125.9 10.02 39 9.89 16.34 53.42 0.206 13.13SCR 0.191 22 16.42 22 53.0 12.16 96.6 2242-5554 41 -49 41 1.81 114.3 14.91 11.35 10.65 38.57 36 44.36SCR 22 12.87 17.96 56.0 2242-5103 41 -63 097.2 2.51 12.94 127.4 14.33 0.181 11.58SCR [242.5] 43.67 33 72.4 9.32 17.47 2242-7919 14.03 27.8 -49 -61 12.29SCR 43 22 15.82 0.241 19 [342.6] 16.04 9.96 2247-8852 27.2 42 15.66 31.2 119.3 2.64 11.34 -61 12.68 47.38 3.34 22 13.47 19 15.51 0.197SCR 42 9.06 39.4 2247-5003 3.19 12.08 128.3 10.90 15.32 22 13.80 0.210 0.184 13.67 17.68 42 10.93SCR -55 1.49 58.9 9.58 32.13 13.30 2249-6324 104.7 54 22 13.39 0.162 02.2 47 18.26SCR -51 2.82 14.53 35.26 229.1 2252-6905 124.0 03 12.71 140.9 15.70 12.14 10.41 22 28.0SCR -79 17.68 47 12.15 26.9 2254-7211 19 117.6 9.07 04.22 0.225 16.05 53.3 13.99 22SCR -88 13.03 2.71 35.6 15.64 12.32 11.37 10.13 49 2254-8712 52 13.83 121.2 0.182 47.14 37.6 15.59 2.47 11.53SCR 22 2.52 20.65 -50 135.0 2254-7325 177.2 52 0.182 13.77 03 15.16 8.98 11.09 19.20 11.75 13.65SCR 47.2 22 10.76 12.49 1.81 225.8 2255-5120A 54 -63 0.197 11.26 13.60 06.09 24 18.21 22 16.73 130.5 37.9 14.47 54 -69 11.57 0.180 10.60 11.70 21.28 11.90 05 22 12.78 79.3 22 119.4 9.86 47.7 125.4 54 12.52 55 -72 14.76 24.22 15.77 30.9 43.88 [281.9] 11 15.49 0.454 13.82 3.40 27.6 118.3 10.21 -87 11.65 10.98 12 16.45 0.261 11.93 51.8 1.29 -73 12.64 -51 9.59 12.78 1.07 174.0 13.45 13.75 25 20 0.284 17.24 58.4 05.6 3.36 14.92 102.1 9.61 11.74 0.401 12.05 9.44 11.47 18.26 1.49 12.04 2.30 131.7 8.94 15.77 0.233 0.335 [349.8] 33.3 16.83 13.92 115.6 11.68 10.93 9.35 16.27 11.17 17.16 3.21 9.20 40.4 085.1 14.81 227.1 8.71 14.83 13.08 16.11 59.2 1.58 10.66 134.6 10.58 15.49 15.11 16.84 14.34 16.12 69.6 3.08 8.66 12.43 12.39 14.13 10.32 14.69 12.92 13.80 14.82 13.88 [359.2] 75.2 12.34 5.57 10.93 3.44 12.29 8.36 14.04 11.61 13.60 12.89 12.42 1.50 10.31 3.28 83.3 11.10 13.95 11.03 11.75 11.49 10.02 10.53 2.29 27.8 23.2 10.76 11.24 11.00 1.85 1.78 34.7 10.29 47.0 1.42 10.97 10.75 1.58 60.0 172.3 3.89 [337.2] 29.2 3.50 [393.6] 3.03 3.07 2.38 26.0 43.9 44.1 60.1 69.7 SCR 2212-7337SCR 2212-5946SCR 2215-7039SCR 22 2215-7025 12 05.45SCR 22 2216-4907 12 03.38SCR 22 2218-5310A 15 -73 54.47 37 22 17.2 15 -59 02.91 46 22 22 51.1 16 18 -70 19.11 43.77 39 0.419 09.4 -70 25 0.186 56.4 -49 -53 122.9 07 10 0.200 53.2 26.0 196.7 0.199 17.43 131.3 0.183 0.190 17.07 138.3 15.31 18.49 111.5 095.3 15.06 16.05 12.89 16.32 15.36 12.19 13.53 14.05 11.39 14.94 13.54 11.07 12.71 12.26 10.85 13.61 12.21 10.19 12.16 11.29 10.48 13.04 10.85 10.24 11.93 10.66 12.80 10.20 9.73 10.39 10.02 3.92 9.61 2.35 2.70 2.76 2.69 31.5 126.1 0.83 152.9 51.1 45.4 61.1 95 a c d d d d d d d a d a d d a a d d (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC SCR 2258-5449SCR 2302-5630SCR 2303-5251SCR 22 2304-6855 58 09.45SCR 23 2304-6750 02 36.09SCR 23 2305-7116 03 -54 54.47 49 23SCR 32.3 04 2305-7729 -56 24.63 30 23SCR 43.5 04 -52 2310-6108 49.96 51 23 0.261SCR 08.3 05 -68 2311-5434 22.68 55 0.217 23SCR 11.6 -67 05 2312-7941 131.8 50 01.93 0.202 23 10.5SCR -71 10 2314-5024 138.8 16 39.06 0.234 23 17.0 16.69 11SCR -77 131.5 34.18 0.199 2317-5140 29 23 12.8 18.26 12 -61 085.7SCR 26.27 0.183 08 14.56 2318-5527 23 16.02 02.8 -54 138.7 14SCR 34 56.58 0.429 16.37 2318-7300 11.95 39.9 23 -79 135.0SCR 17 41 12.97 13.92 0.182 2319-7137 12.73 08.91 32.3 -50 193.7 23 14.65SCR 10.09 0.217 24 18 12.67 2320-4941 54.6 29.01 11.59 076.5 23 12.44 -51 10.98 0.279SCR 18 40 17.31 2323-5345 40.09 13.12 156.4 19.6 23 10.93SCR 19 0.252 -55 11.04 2325-8057 13.86 9.29 21.61 11.30 27 113.1 10.43 23 10.8 15.73SCR -73 12.65 20 15.75 0.446 2327-8000 00 07.73 10.41 148.0 23 10.80 48.9 11.72 -71 10.63 16.65 23SCR 37 0.197 8.80 18.95 2329-8758 23 14.89 12.38 37.9 9.72 192.1 13.82 25 -49 17.13SCR 52.91 0.196 41 10.42 10.52 9.62 2333-7923A 14.68 23 33.9 139.0 -53 27 13.81 0.249SCR 17.04 45 33.50 11.72 8.29 2333-6203 06.0 15.13 9.17 23 -80 135.2 23 29 57 0.191SCR 12.95 15.90 33 04.03 40.7 9.99 2333-7923B 13.30 9.04 100.1 47.61 15.01 -80 10.61 2.97 0.209SCR 00 17.81 14.18 8.14 2334-4926 10.9 223.1 11.80 9.02 23 3.25 14.27 -87 0.201 13.17 23 18.29 33SCR -79 58 13.71 33 25.66 2334-4832 9.28 8.89 205.4 23 06.6 2.62 13.19 51.01 15.93 9.93 49.3 0.200SCR 17.38 11.21 2335-6946 106.9 13.62 16.12 23 12.82SCR -62 17.01 34 0.429 12.60 -79 2335-6433B 03 14.17 54.8 0.394 32.11 106.4 9.09 23 54.1 11.00 15.37 108.2 23SCR 9.71 16.55 55.4 12.84 34 2335-4736 13.64 12.25 51.58 111.6 15.15SCR 1.28 23 12.40 23 13.15 101.4 -49 15.76 1.26 2335-6433A 35 52.9 0.188 35 26 14.48 1.92 37.29 0.388 12.22 14.45SCR 19.95 22.0 12.68 12.04 1.31 2336-5007 -48 15.79 14.08 32SCR 12.64 16.74 23 23 14.42 103.3 48.9 2336-7614 35 13.59 35 -69 100.0 12.10 -64 12.09 24.77 0.207 18.43SCR 12.09 46 33 2336-4918 01.3 [238.6] 14.48 22.3 12.77 1.72 12.40 2.88 14.91SCR 28.2 23 17.50 13.76 3.22 0.182 13.02 2336-4741 38.8 17.38 36 10.85 -47 111.6 -64 11.82 20.85SCR 36 23 1.94 33 0.186 0.196 12.17 13.44 2336-5231 35.7 20.1 36 42.4 13.85 13.40 158.0 15.47 01.58SCR 12.83 23 15.42 10.26 15.02 2.19 2337-5857 36 -50 51.67 096.8 07 099.1 23 12.01 12.70 0.227SCR 0.196 11.0 36 13.23 12.89 15.41 2337-5630 -76 1.43 39.9 14.08 [177.9] 65.4 22.29 14 23 30.8 14.34 12.86SCR 20.5 36 -49 16.91 9.98 2337-4937 2.78 16.55 12.11 19.51 088.2 103.1 18 23 [139.4] 0.254 12.61 12.81 13.81 35.9 37 13.17SCR -47 3.44 13.49 34.98 2338-4937 41 11.79 0.204 23 [155.2] 43.7 14.85SCR 11.96 14.49 -52 18.15 37 11.80 137.7 12.39 1.78 2338-5055 31 51.88 0.196 12.66 13.17 23 57.6 12.96SCR -58 37 11.31 107.7 2339-6753 57 2.39 136.1 41.85 0.195 12.89 16.7 16.01 12.57 23SCR 16.30 -56 210.1 12.43 38 2339-6006 12.68 9.97 0.216 30 12.77 37.60 10.65SCR 38.7 23 18.08 3.60 [227.7] 74.2 -49 226.0 2340-6209 38 11.43 0.231 11.60 1.02 37 14.18 14.27 53.05SCR 23 17.36 45.2 12.14 088.4 2340-4812 39 -49 10.50 0.254 129.2 16.03 02.34 37 1.78 23 17.51 9.02 10.76 117.3 1.68 39.1 11.02 39 12.97 -50 12.62 15.35 26.57 0.198 11.95 55 23 16.11 [215.4] 58.9 40 113.8 -67 14.27 15.22 02.60 10.52 53 23 11.60 29.2 0.251 10.76 12.41 2.30 8.64 49.1 40 11.65 -60 105.2 [144.5] 1.93 13.48 13.83 53.04 06 [183.1] 0.335 17.88 59.5 13.06 -62 13.26 106.4 12.12 09 0.260 11.04 16.79 39.4 9.83 12.37 -48 1.54 12.04 8.02 096.2 12 15.87 0.203 12.53 [216.2] 42.2 12.24 18.43 162.5 1.13 151.2 10.86 14.97 0.189 11.85 11.22 16.54 107.8 14.92 3.42 12.29 8.84 2.89 7.86 0.211 11.65 16.45 13.86 084.4 11.64 13.34 10.64 14.50 [146.8] 11.43 80.9 14.28 194.9 3.05 11.39 15.67 8.89 12.19 18.64 12.38 10.41 12.40 13.68 18.54 2.63 38.9 14.83 9.93 57.5 11.41 16.19 11.82 8.29 2.97 11.35 1.33 13.53 16.34 14.25 2.98 97.9 10.91 11.62 14.38 8.78 10.70 2.99 8.12 14.46 14.00 10.26 2.62 68.0 13.61 113.5 10.51 9.15 13.21 24.5 10.14 13.05 85.7 1.59 12.72 70.5 2.60 8.53 12.76 53.4 0.94 1.62 12.42 [326.2] 3.15 8.47 1.28 102.6 [405.1] 29.6 2.58 3.13 45.8 69.3 0.77 154.4 109.0 33.6 SCR 2255-5120B 22 55 43.86 -51 19 48.2 0.263 228.9 19.43 17.38 15.86 13.72 13.27 12.96 3.66 112.6 96 d d d d d a a b d (pc) Est Dist Notes J − F 59 R s JHK IVN I F 59 R J ) ◦ Table Appendix (cont’d) )( 00 µ θ B (J2000) (J2000) ( Name RA DEC White dwarf candidate picked from RPM diagram or noticed by colors,Subdwarf plate candidate distance picked [in from bracket] RPM is diagram; incorrect; plate see distance Table [in 4.1 bracket] is incorrect Common proper motion companion; see Table 6.1 Not detected during automated search but noticed bye eye during theSource blinking not process in 2MASS a b c d e SCR 2343-4816SCR 2344-4810SCR 2344-5132 23 43SCR 26.39 2344-6358 23 44 15.87SCR 2344-7227 23 -48 44 16SCR 57.32 18.1 2345-5132 -48 23SCR 10 44 2345-5207 03.1 09.02 -51 0.189 23SCR 32 44 2347-6144 11.3 08.08SCR 23 0.193 -63 2349-7719 45 58 139.1 01.72SCR 35.3 23 2350-5942 45 0.202 -72 13.81 097.0 27SCR 23 48.2 2351-4813 17.27 47 -51 0.262 58.53SCR 32 23 143.8 2353-5853 09.3 49 -52 16.99 58.14SCR 07 23 0.204 15.00 2353-8205B 18.3 50 150.3 -61 32.79 18.15SCR 44 23 0.241 2353-8204A 02.8 51 15.34 -77 127.4 02.65 19 23 13.28 23 0.252SCR 17.28 27.4 53 53 2354-6023 -59 16.33 34.91 069.0 49.43 42 23 0.181SCR 14.59 00.2 53 17.68 -48 2354-7216 12.24 089.3 49.99 13 15.48 0.181SCR 49.1 -58 18.39 15.44 2354-5027 -82 117.2 53 13.88 05 0.366 23SCR 15.77 00.5 01.2 11.69 16.60 54 2355-7308 -82 152.1 14.18 50.63 04 0.278SCR 23 14.48 16.26 26.7 13.98 2355-4916 54 13.35 110.8 12.83 0.189 14.99SCR 0.209 23 11.42 14.43 13.17 2356-5818 13.42 54 -60 090.9 13.94 07.83 23 0.216SCR 23 14.69 13.12 13.17 16.0 17.93 2358-6206 55 -72 106.9 14.13 068.4 37.44SCR 16 23 12.93 12.77 11.20 18.36 2358-5811 20.3 55 13.72 -50 066.9 13.36 03.99SCR 27 23 12.66 0.230 15.78 16.05 2359-5957 24.1 13.60 56 14.99 -73 12.00 31.13 12.61SCR 08 23 10.27 16.36 0.189 2359-7403 11.90 44.0 58 12.78 -49 12.54 098.6 28.78 16 23 13.88 2.75 13.78 0.255 13.41SCR 13.06 49.5 58 11.39 2359-4845 -58 10.39 57.54 102.7 18 23 14.54 0.181 10.40 1.46 12.54 25.9 59 12.27 16.31 -62 12.66 17.88 083.7 06 23 12.26 0.252 11.56 11.27 01.9 59 1.85 -58 17.74 13.08 52.41 118.5 11 9.78 0.190 23 12.19 16.06 37.6 12.17 -59 15.79 59 9.26 11.35 2.06 206.7 10.85 [271.8] 57 79.3 23.46 0.382 00.5 15.70 12.52 -74 17.20 092.3 03 0.182 1.65 15.94 11.91 [343.8] 17.7 13.84 9.64 10.77 18.50 10.23 -48 191.2 8.97 0.197 45 2.90 12.29 14.16 15.16 [194.3] 37.7 13.65 095.5 15.88 0.191 2.42 10.51 12.32 16.44 16.50 [303.1] 098.7 9.99 13.08 0.58 13.82 0.189 8.33 11.71 18.12 15.78 122.2 11.41 14.07 14.35 16.03 125.5 12.56 12.98 194.7 3.12 10.73 16.09 16.31 0.81 15.71 8.09 10.81 12.53 3.27 87.3 12.78 13.97 12.35 168.5 12.38 17.71 10.17 2.43 14.10 13.60 10.64 12.04 2.21 11.94 12.67 12.17 16.08 12.65 88.5 12.82 9.56 59.6 11.76 11.37 11.89 98.1 0.19 15.28 1.42 12.06 12.06 59.3 2.62 11.17 9.40 11.32 54.2 14.45 2.43 11.78 [1127.8] 11.47 2.18 11.12 13.90 3.90 11.30 26.8 137.2 13.65 2.42 67.7 1.55 146.8 3.44 2.08 59.5 1.55 84.2 1.63 47.7 70.8 94.5 118.2 [321.7] SCR 2340-4727SCR 2342-6217 23 40 07.33 23 42 03.46 -47 27 54.1 -62 17 25.1 0.189 0.203 109.9 202.1 14.59 16.95 12.86 15.23 12.14 14.61 11.69 13.80 11.04 13.19 10.94 13.10 1.16 1.43 100.0 [245.5]