M I R a C 3 User’S Manual

Total Page:16

File Type:pdf, Size:1020Kb

M I R a C 3 User’S Manual M I R A C 3 USER’S MANUAL Steward Observatory, University of Arizona Harvard Smithsonian Center for Astrophysics William F. Hoffmann Joseph L. Hora Manual Version mrcman91.99w.wpd May 22, 1999 Program Version 7.22 May 3, 1999 readme.txt May 22, 1999 This readme.txt file dexcribing the MIRAC3 Users Manual, and the gzip postscript MIRAC manual files can be found in kepler.as.arizona.edu anonymous pub/mirac The current version of the MIRAC Users Manual, mrcman91.99w.wpd, was completed May 22, 1999. This version has been updated for the hardware and software changes in MIRAC3 and includes corrections and additional material on standard stars, filters, and operation and troubleshooting the camera. Send comments to [email protected] The following gzip compressed Postscript files contain the manual. The postscript files are printed with a binding offset for double sided printing. File Chapters Pages Compressed Uncompressed mr01x02.ps.gz Contents - 2 Title - 12 319562 1494992 mr03x10.ps.gz 3 - 10 13 - 78 610574 2786308 mr11x13.ps.gz 11 - 13 79 - 102 264316 2531688 mra01x10.ps.gz A1 - A10 103 - 142 678263 3958165 mra11x13.ps.gz A11 - A13 143 - 178 122065 518709 mra14x15.ps.gz A14 - A15 179 - 204 2409854 6116263 mra16x19.ps.gz A16 - A19 205 - 226 215722 1586640 mra20x24.ps.gz A20 - A24 227 - 249 107361 403727 readme.txt MIRAC Manual Organization The MIRAC User’s Manual provides information and check lists for shipping, setup, preparation, observation, data reduction and maintainance. The asterisk (*) indicates subjects most useful to review before an observing run. Subject Chapters Appendices Organization of the manual and performance of MIRAC * 1 - 2 Preparation for an observing run * 3 - 4 * A1 - A5 Setting up and shutting down for a run and for a night of observing 5 - 6 Observing with the camera * 7 - 10 A6 Quick look display and processing 11 - 13 Post observing data reduction A7 - A10 MIRAC files and menus A11 - A12 Shipping and setup A13 - A15 Trouble shooting and service A16 - A19 Unix commands, tape backup, weather, and address information A20 - A24 5/23/99 Contents i Table of Contents List of Figures.............................................................vii List of Tables ............................................................ viii 1. Organization of MIRAC User’s Manual ........................................1 2. Overview and Performance..................................................3 2.1 MIRAC3 on the World Wide Web .....................................3 2.2 General Description of MIRAC3.......................................3 2.3 Magnification and Pixel Scale.........................................6 2.4 Filter Selections ...................................................7 2.5 HF-16 Array and MIRAC System Properties..............................7 2.6 Background, Sensitivity, and Noise.....................................9 2.7 Telescope and Sky Emissivity........................................11 3. Observing Run Arrangements...............................................13 3.1 Observing Proposals...............................................13 3.2 Observatory Arrangements...........................................14 3.2.1 Kitt Peak Arrangements.....................................14 3.2.2 Mt Hopkins Arrangements...................................14 3.2.3 Hawaii Mauna Kea Arrangements..............................14 3.3 IRTF Requirements List ............................................15 3.4 Cryogenics Cost...................................................17 4. Software Preparation.....................................................19 4.1 Object Lists and Air Mass Charts .....................................19 4.2 Offset and Command Files ..........................................19 4.3 Establishing an Individual Guest Account...............................20 5. Start and End of Run Setup and Shutdown Check Lists ...........................21 5.1 Preparation of MIRAC after Shipping or Storage .........................21 5.2 Start of Run Setup Tasks ...........................................21 5.3 End of Run Shutdown Tasks.........................................26 5.3.1 Initial Control Room End of Run Tasks .........................26 5.3.2 Telescope Chamber End of Run Tasks..........................26 5.4 Complete Shut Down and Packing ....................................30 6. Nightly Startup and Shutdown Check Lists.....................................31 6.1 Nightly Startup Tasks..............................................31 6.2 Nightly Shutdown Tasks............................................35 7. Observing Procedures and Check Lists........................................39 ii MIRAC User’s Manual 7.1 Check List for each Set of Observations ................................39 7.2 Check List for a Nights Observations ..................................40 7.3 Wavelengths, Frame Times, Frame/Filter Link Files and Filter Change Times ....40 7.4 Macro Aids......................................................42 7.5 Command Files...................................................43 7.6 Offset Files......................................................46 7.7 Focus Settings....................................................47 7.8 Acquisition of Star and Focus........................................48 7.9 Final Telescope Focusing ...........................................49 7.10 Autoguiding at IRTF..............................................49 7.11 Autoguiding at UKIRT............................................49 7.12 Observing Times.................................................49 7.13 Calculating Image Scale ...........................................50 7.14 Printing Images..................................................50 8. Short Form Instructions for Running MIRAC Using the MIRAC Program.............53 8.1 General Notes ....................................................53 8.2 Starting MIRAC...................................................53 8.3 Observing with MIRAC.............................................55 8.4 Shutting Down MIRAC.............................................56 9. Using the MIRAC Program ................................................59 9.1 Running the MIRAC Program on a PC Stand-Alone .......................59 9.2 Directory Structure................................................59 9.3 Data File Name Conventions.........................................60 9.4 Main Screen Display...............................................60 9.5 Using MIRAC Menus and Functions...................................64 9.6 Selecting Display Modes and Options..................................66 9.7 Setting Camera Parameters and Taking Data.............................66 9.8 Filter Wheel Initialization and Motion..................................67 9.9 Observing Modes and Options........................................67 9.9.1 Source Frames and Off-source Beam Switch......................68 9.9.1.1 Grab.............................................68 9.9.1.2 Chop ............................................68 9.9.1.3 Chop-Nod ........................................68 9.9.1.4 Nod (2 beam)......................................70 9.9.1.5 Nod (4 beam)......................................70 9.9.2 Fast Data Mode ...........................................71 9.9.3 Ultra Fast Mode...........................................71 9.10 Telescope Control................................................72 9.10.1 Nod Control by Logic Level.................................72 9.10.2 RS-232 Control of the Telescope .............................72 9.10.3 Ethernet Control of the Telescope.............................73 9.10.4 Offset Modes and Taking Data...............................74 5/23/99 Contents iii 10. Mask, Gain, and Flat Field Maps............................................75 10.1 Mask Map......................................................75 10.2 Gain Map Generation .............................................76 10.3 Preparing a Flat Field .............................................76 10.4 Using the Mask, Gain, and Flat Field maps .............................77 10.5 Principles of Mid-Infrared Flat Fielding................................77 11. Reading Stored Data and Data Processing ....................................79 11.1 Methods of Loading Data..........................................79 11.1.1 Current Observation.......................................79 11.1.2 Accumulated Observation...................................80 11.1.3 Replay Mode ............................................80 11.1.4 Operation...............................................80 11.1.5 Mosaic.................................................81 11.1.6 Multiple Image Display.....................................82 11.1.7 Processed Images.........................................83 11.1.8 Noise..................................................83 11.2 Display Modes ..................................................83 11.2.1 Grayscale...............................................84 11.2.2 Contour ................................................84 11.2.3 Slice...................................................85 11.2.4 Frequency...............................................86 11.2.5 Histogram...............................................86 11.2.6 Radial Plot..............................................87 11.2.7 Plot Command Line Options.................................88 11.2.7.1 Setup...........................................88 11.2.7.2 Redraw .........................................89 11.2.7.3 Fit .............................................89
Recommended publications
  • Searches After Gravitational-Waves Using Arizona Observatories (SAGUARO): System Overview and First Results from Advanced LIGO/Virgo’S Third Observing Run
    Draft version July 19, 2019 Typeset using LATEX twocolumn style in AASTeX62 Searches After Gravitational-waves Using ARizona Observatories (SAGUARO): System Overview and First Results from Advanced LIGO/Virgo's Third Observing Run M. J. Lundquist,1 K. Paterson,2 W. Fong,2 D. J. Sand,1 J. E. Andrews,1 I. Shivaei,1, 3 P. N. Daly,1 S. Valenti,4 S. Yang,4, 5, 6 E. Christensen,7 A. R. Gibbs,7 F. Shelly,7 S. Wyatt,1 O. Kuhn,8 R. C. Amaro,1 I. Arcavi,9 P. Behroozi,1 N. Butler,10 L. Chomiuk,11 A. Corsi,12 M. R. Drout,13, 14 E. Egami,1 X. Fan,1 R. J. Foley,15 B. Frye,1 P. Gabor,16 E. M. Green,1 C. J. Grier,1 F. Guzman,17, 1 E. Hamden,1 D. A. Howell,18 B. T. Jannuzi,1 P. Kelly,19 P. Milne,1 M. Moe,1 A. Nugent,2 E. Olszewski,1 E. Palazzi,20 V. Paschalidis,1 D. Psaltis,1 D. Reichart,21 A. Rest,22, 23 A. Rossi,20 G. Schroeder,2 P. S. Smith,1 N. Smith,1 K. Spekkens,24 J. Strader,11 D. P. Stark,1 D. Trilling,25 C. Veillet,1, 8 M. Wagner,26, 8 B. Weiner,1, 27 J. C. Wheeler,28 G. G. Williams,1, 27 and A. Zabludoff1 1Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721-0065, USA 2Center for Interdisciplinary Exploration and Research in Astrophysics and Department of Physics and Astronomy, Northwestern University, 2145 Sheridan Road, Evanston, IL 60208-3112, USA 3Hubble Fellow 4Department of Physics, University of California, 1 Shields Avenue, Davis, CA 95616-5270, USA 5Department of Physics and Astronomy Galileo Galilei, University of Padova, Vicolo dell'Osservatorio, 3, I-35122 Padova, Italy 6INAF Osservatorio Astronomico
    [Show full text]
  • A Bibliography of Navajo and Native American Teaching Materials = Dine K'eeji Naaltsoos Bee Nida'nitinigii
    DOCUMENT RESUME ED 232 801 RC 014 198 AUTHOR McCarty, T. L., Comp.; And Others TITLE A Bibliography of Navajo and Native AmericanTeaching Materials = Dine K'eeji Naaltsoos BeeNida'nitinigii. Revised Edition. INSTITUTION Rough Rock Demonstration School,AZ. Navajo Curriculum Center. SPONS AGENCY Office of Indian Education (ED), Washington,D.C. REPORT NO ISBN-0-936008-15-6 PUB DATE Jun 83 NOTE 106p. AVAILABLE FROMNavajo Curriculum Center, RoughRock Demonstration School, Star Route 1, Rough Rock AZ86503 ($7.50; 5 or more, 15% discount). PUB TYPE Reference Materials- Bibliographies (131) EDRS PRICE MF01 Plus Postage. PC Not Availablefrom EDRS. DESCRIPTORS American Indian Culture; *AmericanIndian Education; American Indian History; American IndianLiterature; American Indians; Annotated Bibliographies; Audiovisual Aids; Bilingual InstructionalMaterials; Cultural Background; *Cultural Education;Elementary Secondary Education; *InstructionalMaterials; Mathematics; Music; Native LanguageInstruction; *Navajo; Periodicals; Physical Education;Publishing Industry; *Resource Materials; SocialStudies; SupplemerCzary Reading Materials IDENTIFIERS *Navajo (Nation) ABSTRACT A revised annotated bibliography of Navajoand Native American teaching materials publishedbetween 1910 and 1982 (most from 1970 to 1982), compiledas part of the Title IV-B Navajo Materials Development Project, listsresources for teachers of Navajo and other Native American students.Most citations are of written materials, although some posters,non-textual materials and catalogs of audio-visual aidsare described. The first two sections divide text materials by grade level and by language:148 written primarily in Navajo (Section I), and 193 bilingual(Navajo-English) or primarily in English (Section II).Both sections cite: fiction and non-fiction; Navajo-based texts in socialstudies, history, mathematics, physical education, musicand art; and teacher's guides to accompany texts.
    [Show full text]
  • Golder Ranch Fire District Governing Board Meeting Public Notice and Agenda Regular Session
    GOLDER RANCH FIRE DISTRICT GOVERNING BOARD MEETING PUBLIC NOTICE AND AGENDA REGULAR SESSION Tuesday, November 13, 2018 0900 hrs 3885 East Golder Ranch Drive, Tucson, Arizona Pursuant to ARS § 38-431.02, ARS § 38-431.03 and ARS § 38-431.05, the Golder Ranch Fire District Governing Board will meet in Regular Session that begins at approximately 9:00 a.m. on Tuesday, November 13, 2018. The meeting will be held at the Fire District Administration Board Room, which is located at 3885 East Golder Ranch Drive, Tucson, Arizona. Members of the GRFD Governing Board will attend either in person or by telephone conference call. The order of the Agenda may be altered or changed by direction of the Board. The Board may vote to go into Executive Session, which are not open to the public, on any agenda item pursuant to ARS § 38-431.03(A )(3) for discussion and consultation for legal advice with the Fire District Attorney on the matter(s) as set forth in the agenda item. The following topics and any reasonable variables related thereto will be subject to discussion and possible action. 1. CALL TO ORDER/ROLL CALL 2. SALUTE AND PLEDGE OF ALLEGIANCE 3. FIRE BOARD REPORTS 4. CALL TO THE PUBLIC This is the time for the public to comment. Members of the Board may not discuss items that are not on the agenda. Therefore, action taken as a result of public comment will be limited to directing staff to study the matter or scheduling the matter for further consideration and decision at a later date.
    [Show full text]
  • Download Date 30/09/2021 08:32:26
    Light Variations of the Seyfert Galaxy NGC 4151. III. Long Term Photographic B Variations and Infrared K Data Item Type text Authors Pacholczyk, A. G. Citation APJ 163: 449-54 (1971) Publisher Steward Observatory, The University of Arizona (Tucson, Arizona) Rights Copyright © All Rights Reserved. Download date 30/09/2021 08:32:26 Link to Item http://hdl.handle.net/10150/627204 ii i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i ii i i i i i i i i i i i i i i i i i i i i i ii i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i i ., P I'' E IN OF THE ¡rn A r V . V ' I JS.y OB V V I O THE UNIVERSITY OF ARIZONA TUCSON, ARIZONA ,, , , , , , , , , , , , , , , , , , , , , , , , , , , Z , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , LIGHT VARIATIONS OF THE SEYFERT GALAXY NGC 4151.
    [Show full text]
  • A CONNECTION to STONY METEORITES? MD Hicks1, BJ Buratti1, DL Rabinowitz1, P
    Lunar and Planetary Science XXX 1719.pdf THE DEEP SPACE 1 MISSION TARGET 1992 KD: A CONNECTION TO STONY METEORITES? M. D. Hicks1, B. J. Buratti1, D. L. Rabinowitz1, P. R. Weissman1, A. Doressoundiram1, U. Fink2. 1Jet Propulsion Laboratory, Palomar Observatory-Caltech, MS 183-501, 4800 Oak Grove Drive, Pasadena CA 91109, [email protected]. 2Lunar and Planetary Laboratory, University of Arizona, Tucson AZ 85721. Introduction: Deep Space 1, the first in NASA's New through Johnson BV, Kron R and Gunn I filters (0.44, 0.54, Millennium program, was successfully launched on Oct 24 0.62, 0.80 micron). Each set of observations began with 1998 and currently scheduled to rendezvous with the near- imaging standard star fields [1] obtained over a wide range Earth asteroid 1992 KD in July of 1999. We took advantage of airmasses and stellar types though all filters. 1992 KD of the asteroid's apparition in late 1998 to obtain BVRI filter was considered a viable target once its airmass rose above photometry at a number of telescopes in order to character- 2.0. We cycled though the filters: a typical sequence would ize the physical properties of the object; its size, colors and be R-I-R-V-R-B-R. In this way, we could correct for light- rotational state. We found that the object is significantly curve effects in the color ratios. Often we were forced to smaller than originally predicted, with evidence of a high pause our observations to allow the object to move through amplitude lightcurve with a relatively long period.
    [Show full text]
  • Alessondra Springmann
    .......................................................................................... Alessondra Springmann PhD Candidate 1629 E University Blvd Lunar & Planetary Laboratory Tucson, AZ 85721 Department of Planetary Sciences [email protected] University of Arizona http://www.lpl.arizona.edu/ sondy e .......................................................................................... Education University of Arizona Tucson, AZ PhD Candidate, Lunar & Planetary Laboratory August 2014– Future Investigators in NASA Earth and Space Sciences and Technology (FINESST) Fellowship Recipient September 2020– Massachusetts Institute of Technology Cambridge, MA Master of Science in Earth and Planetary Science Received June 2011 Wellesley College Wellesley, MA Bachelor of Arts in Astrophysics Received June 2007 Additional Training Instituto de Astrofísica de Canarias Winter School on Planetary Exploration 2016 NASA Jet Propulsion Laboratory Planetary Science Summer School 2008 Peer-Reviewed Publications 10. Steckloff, J. K., J. Debes, A. Steele, B. Johnson, E. R. Adams, S. A. Jacobson, and A. Springmann 2021. The Sublimative Control of Dusty Debris Disk Formation Around White Dwarf Stars. ApJ Letters, submitted 9. Kareta, T., J. Andrews, J. W. Noonan, W. M. Harris, N. Smith, P. O’Brien, B. N. L. Sharkey, V. Reddy, A. Springmann, C. Lejoly, K. Volk, A. Conrad, and C. Veillet 2020. Carbon Chain Depletion of 2I/Borisov. Astrophysical Journal Letters 8. Springmann, A., D. S. Lauretta, B. Klaue, Y. S. Goreva, J. D. Blum, A. Andronikov, and J. K. Steckloff 2019. Thermal alteration of labile elements in carbonaceous chon- drites. Icarus 324, 104 – 119 7. Noonan, J. W., V. Reddy, W. M. Harris, W. F. Bottke, J. A. Sanchez, R. Furfaro, Z. Brown, R. Fernandes, T. Kareta, C. Lejoly, R. Teja Nallapu, H. K. Niazi, L. R. Slick, L.
    [Show full text]
  • ARIZONA PUBLIC MEDIA (A Division of the University of Arizona) YEARS
    ARIZONA PUBLIC MEDIA (A Division of the University of Arizona) YEARS ENDED JUNE 30, 2020 AND 2019 ARIZONA PUBLIC MEDIA (A Division of the University of Arizona) YEARS ENDED JUNE 30, 2020 AND 2019 CONTENTS Page Message from the General Manager 1 Independent auditors' report 2 ‐ 3 Management's discussion and analysis 4 ‐ 10 Financial statements: Statements of net position 12 Statements of revenues, expenses and changes in net position 13 Statements of cash flows 14 ‐ 15 Notes to financial statements 16 ‐ 40 Required supplementary information: Schedule of AZPM's proportionate share of the net pension liability ‐ Arizona State Retirement System 42 Schedule of pension contributions ‐ Arizona State Retirement System 43 Schedule of AZPM's proportionate share of the total OPEB liability ‐ Arizona Department of Administration 44 Supplementary information to the financial statements: Statement of functional expenses by station ‐ 2020 46 Statement of functional expenses by station ‐ 2019 47 A Message from the Chief Executive Officer During FY 2019‐2020, Arizona Public Media enjoyed exceptional audience growth on every platform: television, radio, and online, including exponential growth for AZPM Passport, its video‐on‐demand member benefit. Such growth can be attributed to AZPM’s commitment to creating and providing quality programming. AZPM staff members were honored with 8 individual Emmy® Awards for four projects, including a win for the special documentary project The Arizonans, and the second consecutive win for Arizona 360. Arizona Illustrated earned nods in two categories: arts/entertainment and societal concerns. AZPM also received two regional Edward R. Murrow Awards for journalistic excellence in the categories of multimedia and feature reporting.
    [Show full text]
  • 2017-18 Overview
    2017-18 OVERVIEW Page 0 ORGANIZATIONAL PROFILE AZPM is a member-supported, non-profit public media organization that serves all of Southern Arizona. AZPM offers three public television program services and three radio program services. AZPM produces award-winning content from its studios on the campus of the University of Arizona (UA) and is provided as a community service and educational resource. AZPM is an operating unit of the University, but, since its inception in 1959, maintains editorial independence from the institution. The Arizona Board of Regents holds the FCC license for AZPM’s broadcast stations. See Appendices I and II for more information about the history of AZPM as well as details regarding the public media funding model. Television KUAT and KUAS television stations are Public Broadcasting Service (PBS) affiliates and are broadcast via two digital transmitters that cover a broad portion of southeastern Arizona. Both stations provide a constant stream of PBS high- definition (HD) programming 24-hours a day, seven days a week on PBS 6 (Channels 6.1 and 27.1). They are also the only two locally owned and operated television stations in Tucson. AZPM offers two additional discrete standard definition program services, PBS 6 PLUS on KUAT, and PBS Kids on KUAS. AZPM also manages and operates the UA Channel on YouTube, which features a diverse mix of PBS titles, community programs, as well as University of Arizona-related lectures and events. Radio AZPM has two radio stations, KUAZ-AM/FM and KUAT-FM. Via three full-power transmitters and five translators, these stations reach listeners throughout Southern Arizona.
    [Show full text]
  • Oral Histories in Meteoritics and Planetary Science – Xxxx: Dale
    Oral Histories in Meteoritics and Planetary Science – XX: Dale P. Cruikshank by Derek W. G. Sears Planetary Science and Astrobiology Division NASA Ames Research Center, Mountain View California. SUPPLEMENTAL INFORMATION Recollections of Gerard Kuiper DS: Okay, so we have recorded your oral history, let’s spend some time recollecting your interactions with Gerard Kuiper. You described how you met him at Yerkes Observatory as an undergraduate and how you went to graduate school after he moved to the University of Arizona DC: Alan Binder and I applied to graduate school in Arizona and did our graduate training there. At about the same time, Bill Hartmann came to Tucson as a graduate student from Penn State, Elliott Moore and Tobias Owen also came as students from the University of Chicago. Several astronomers and atmospheric physicists also came to Tucson in those first years; Joseph Chamberlain, Donald Hunten, and Lloyd Wallace came to Arizona and joined the staff at the Kitt Peak National Observatory. The National Observatory had decided to locate in Tucson and build its observatory at Kitt Peak some 40 miles outside of town. By the time Kuiper got there Kitt Peak National Observatory was becoming quite a significant national establishment, and that provided a strong draw to the area. The Kitt Peak offices were located on the edge of the University of Arizona campus, just across the street from the University's Steward Observatory. When Kuiper left Yerkes several people involved in his lunar studies enterprise went with him, including David Arthur and Ewen Whitaker. Eventually Tom Gehrels, formerly associated with Kuiper at the University of Chicago, joined the group in Tucson.
    [Show full text]
  • Searches After Gravitational Waves Using Arizona Observatories (SAGUARO): System Overview and First Results from Advanced LIGO/Virgo’S Third Observing Run
    The Astrophysical Journal Letters, 881:L26 (13pp), 2019 August 20 https://doi.org/10.3847/2041-8213/ab32f2 © 2019. The American Astronomical Society. All rights reserved. Searches after Gravitational Waves Using ARizona Observatories (SAGUARO): System Overview and First Results from Advanced LIGO/Virgo’s Third Observing Run M. J. Lundquist1 , K. Paterson2 , W. Fong2 , D. J. Sand1 , J. E. Andrews1 , I. Shivaei1,29 , P. N. Daly1, S. Valenti3 , S. Yang3,4,5 , E. Christensen6, A. R. Gibbs6 , F. Shelly6, S. Wyatt1, O. Eskandari2,7, O. Kuhn8, R. C. Amaro1 , I. Arcavi9 , P. Behroozi1 , N. Butler10 , L. Chomiuk11 , A. Corsi12 , M. R. Drout13,14, E. Egami1, X. Fan1 , R. J. Foley15, B. Frye1, P. Gabor16, E. M. Green1, C. J. Grier1 , F. Guzman1,17 , E. Hamden1, D. A. Howell18 , B. T. Jannuzi1 , P. Kelly19 , P. Milne1 , M. Moe1, A. Nugent2 , E. Olszewski1, E. Palazzi20 , V. Paschalidis1, D. Psaltis1, D. Reichart21 , A. Rest22,23 , A. Rossi20 , G. Schroeder2 , P. S. Smith1, N. Smith1, K. Spekkens24 , J. Strader11 , D. P. Stark1, D. Trilling25 , C. Veillet1,8, M. Wagner8,26, B. Weiner1,27 , J. C. Wheeler28 , G. G. Williams1,27 , and A. Zabludoff1 1 Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721-0065, USA 2 Center for Interdisciplinary Exploration and Research in Astrophysics and Department of Physics and Astronomy, Northwestern University, 2145 Sheridan Road, Evanston, IL 60208-3112, USA 3 Department of Physics, University of California, 1 Shields Avenue, Davis, CA 95616-5270, USA 4 Department of Physics and Astronomy
    [Show full text]
  • New Tools for the Optimized Follow-Up of Imminent Impactors
    universe Article New Tools for the Optimized Follow-Up of Imminent Impactors Maddalena Mochi 1 and Giacomo Tommei 2,* 1 Department of Physics, University of Pisa, 56127 Pisa, Italy; [email protected] 2 Department of Mathematics, University of Pisa, 56127 Pisa, Italy * Correspondence: [email protected] Abstract: The solar system is populated with, other than planets, a wide variety of minor bodies, the majority of which are represented by asteroids. Most of their orbits are comprised of those between Mars and Jupiter, thus forming a population named Main Belt. However, some asteroids can run on trajectories that come close to, or even intersect, the orbit of the Earth. These objects are known as Near Earth Asteroids (NEAs) or Near Earth Objects (NEOs) and may entail a risk of collision with our planet. Predicting the occurrence of such collisions as early as possible is the task of Impact Monitoring (IM). Dedicated algorithms are in charge of orbit determination and risk assessment for any detected NEO, but their efficiency is limited in cases in which the object has been observed for a short period of time, as is the case with newly discovered asteroids and, more worryingly, imminent impactors: objects due to hit the Earth, detected only a few days or hours in advance of impacts. This timespan might be too short to take any effective safety countermeasure. For this reason, a necessary improvement of current observation capabilities is underway through the construction of dedicated telescopes, e.g., the NEO Survey Telescope (NEOSTEL), also known as “Fly-Eye”. Thanks to these developments, the number of discovered NEOs and, consequently, imminent impactors detected per year, is expected to increase, thus requiring an improvement of the methods and algorithms used to handle such cases.
    [Show full text]
  • The Comet's Tale
    THE COMET’S TALE Newsletter of the Comet Section of the British Astronomical Association Number 27, 2007 December Discovery of a New Comet in Andromeda We have had very little decent weather for observing in rather over than under the mark, but I consider the London of late, but I make a practice of never missing milky state of the sky somewhat reduced apparent an opportunity. Sunday, November 6th, was far from diameter, and that probably 5' is exact. The position in clear, and did not improve as the night deepened, so declination is very close also, as both comet and star after looking at Jupiter and a few double stars and travelled accurately on wire. As regards R.A., the finding the seeing unsatisfactory, I made up my mind to difference did not exceed 1m 10s I am sure, but it may close observing at 11.30pm. have been 1s less. On Monday morning I wrote the Astronomer Royal, but as I omitted to say I saw the Andromeda nebula at the same time, he very naturally at first thought I had blundered. My friend Mr Kidd, with whom I have corresponded for years, and to whom I am indebted for much counsel and kindness, also suspected a mistake, but on Monday evening he saw the comet with the naked eye, as did also Mr Bartlett of Bramley. I wrote again to Greenwich, and being now satisfied of the reality of the discovery, they took measures to spread necessary information. Mr Maw accepted the matter at once and wrote to congratulate me.
    [Show full text]