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Snake River Skies the Newsletter of the Magic Valley Astronomical Society
Snake River Skies The Newsletter of the Magic Valley Astronomical Society www.mvastro.org Membership Meeting MVAS President’s Message June 2018 Saturday, June 9th 2018 7:00pm at the Toward the end of last month I gave two presentations to two very different groups. Herrett Center for Arts & Science College of Southern Idaho. One was at the Sawtooth Botanical Gardens in their central meeting room and covered the spring constellations plus some simple setups for astrophotography. Public Star Party Follows at the The other was for the Sun Valley Company and was a telescope viewing session Centennial Observatory given on the lawn near the outdoor pavilion. The composition of the two groups couldn’t be more different and yet their queries and interests were almost identical. Club Officers Both audiences were genuinely curious about the universe and their questions covered a wide range of topics. How old is the moon? What is a star made of? Tim Frazier, President How many exoplanets are there? And, of course, the big one: Is there life out [email protected] there? Robert Mayer, Vice President The SBG’s observing session was rained out but the skies did clear for the Sun [email protected] Valley presentation. As the SV guests viewed the moon and Jupiter, I answered their questions and pointed out how one of Jupiter’s moons was disappearing Gary Leavitt, Secretary behind the planet and how the mountains on our moon were casting shadows into [email protected] the craters. Regardless of their age, everyone was surprised at the details they 208-731-7476 could see and many expressed their amazement at what was “out there”. -
Observing List
day month year Epoch 2000 local clock time: 22.00 Observing List for 20 4 2019 RA DEC alt az Constellation object mag A mag B Separation description hr min deg min 27 293 Auriga M36 Pinwheel Cluster open cluster of a dozen or so young stars (30million years old) 5 36.1 34 8 29 289 Auriga M37 January Salt and Pepper Cluster rich, open cluster of 150 stars, very fine 5 52.4 32 33 27 295 Auriga M38 Starfish Cluster large open cluster 220 million years old 5 28.7 35 50 36 303 Auriga IC2149 planetary nebula, stellar to small disk, slightly elongated 5 56.5 46 6.3 30 307 Auriga Capella 0.1 alignment star 5 16.6 46 0 40 290 Auriga UU Aurigae Magnitude 5.1-7.0 carbon star (AL# 36) 6 36.5 38 27 33 293 Auriga 37 Theta Aurigae 2.6 7.1 3.6 white & bluish stars 5 59.7 37 13 23 294 Auriga 14 Aurigae 5.1 7.4 14.6 pale yellow and blue 5 15.4 32 31 57 56 Bootes 17, Kappa Bootis 4.6 6.6 13.4 bright white primary & bluish secondary 14 13.5 51 47 56 57 Bootes 21, Iota Bootis 4.9 7.5 38.5 wide yellow & blue pair 14 16.2 51 22 38 102 Bootes 29, Pi Bootis 4.9 5.8 5.6 fine bright white pair 14 40.7 16 25 43 90 Bootes 36, Epsilon Bootis (Izar) (*311) (HIP72105) 2.9 4.9 2.8 golden & greenish-blue 14 45 27 4 37 97 Bootes 37, Xi Bootis 4.7 7 6.6 beautiful yellow & reddish orange pair 14 51.4 19 6 41 72 Bootes 51, Mu Bootis 4.3 7 108.3 primary of yellow & close orange BC pair 15 24.5 37 23 41 78 Bootes Delta Bootis 3.5 8.7 105 wide yellow & blue pair 15 15.5 33 19 44 104 Bootes Arcturus -0.11 alignment star 14 15.6 19 10.4 43 124 Bootes NGC5248 galaxy with bright -
Observing List
day month year Epoch 2000 local clock time: 22.00 Observing List for 18 5 2019 RA DEC alt az Constellation object mag A mag B Separation description hr min deg min 10 305 Auriga M37 January Salt and Pepper Cluster rich, open cluster of 150 stars, very fine 5 52.4 32 33 20 315 Auriga IC2149 planetary nebula, stellar to small disk, slightly elongated 5 56.5 46 6.3 15 319 Auriga Capella 0.1 alignment star 5 16.6 46 0 21 303 Auriga UU Aurigae Magnitude 5.1-7.0 carbon star (AL# 36) 6 36.5 38 27 15 307 Auriga 37 Theta Aurigae 2.6 7.1 3.6 white & bluish stars 5 59.7 37 13 74 45 Bootes 17, Kappa Bootis 4.6 6.6 13.4 bright white primary & bluish secondary 14 13.5 51 47 73 47 Bootes 21, Iota Bootis 4.9 7.5 38.5 wide yellow & blue pair 14 16.2 51 22 57 131 Bootes 29, Pi Bootis 4.9 5.8 5.6 fine bright white pair 14 40.7 16 25 64 115 Bootes 36, Epsilon Bootis (Izar) (*311) (HIP72105) 2.9 4.9 2.8 golden & greenish-blue 14 45 27 4 57 124 Bootes 37, Xi Bootis 4.7 7 6.6 beautiful yellow & reddish orange pair 14 51.4 19 6 62 86 Bootes 51, Mu Bootis 4.3 7 108.3 primary of yellow & close orange BC pair 15 24.5 37 23 62 96 Bootes Delta Bootis 3.5 8.7 105 wide yellow & blue pair 15 15.5 33 19 62 138 Bootes Arcturus -0.11 alignment star 14 15.6 19 10.4 56 162 Bootes NGC5248 galaxy with bright stellar nucleus and oval halo 13 37.5 8 53 72 56 Bootes NGC5676 elongated galaxy with slightly brighter center 14 32.8 49 28 72 59 Bootes NGC5689 galaxy, elongated streak with prominent oval core 14 35.5 48 45 16 330 Camelopardalis 1 Camelopardalis 5.7 6.8 10.3 white & -
Novice Handbook
THE I RISH F EDERATION O F A STRONOMICAL S OCIETIES PRESENT THE NOVICE ASTRONOMER OBSERVING CHALLENGES HANDBOOK A Self-contained Handbook and Logbook for the Novice Astronomer, as part of the IFAS Observing Certificates Programme AUTUMN 2004 THE OBSERVING CERTIFICATES WORKING GROUP WORKING UNDER THE IRISH FEDERATION OF ASTRONOMICAL SOCIETIES Shane Culleton Irish Astronomical Society South Dublin Astronomical Society John Flannery Irish Astronomical Society South Dublin Astronomical Society Seanie Morris Tullamore Astronomical Society Ronan Newman Galway Astronomy Club Michael O’Connell Shannonside Astronomy Club Tullamore Astronomical Society Albert White Irish Astronomical Society South Dublin Astronomical Society OBSERVING PROGRAMME REGULATIONS 1. To take part in the Observing Certificates Programme you must be a member of one of the member clubs or societies of the IFAS. Check out the list of clubs and links to their websites at the IFAS webpage, www.irishastronomy.org , or on page 4 of this handbook. 2. Observations must be made after September 18 th 2004 (the launch date), AND after the date of purchase of this handbook. 3. You must either post or hand this Handbook to the Observations Secretary who will then verify your recordings. Your Handbook must be received at least 21 days before the star party at which you wish to receive your certificate ( Connaught in January, COSMOS in March, Whirlpool in September). 4. Duplicate observations must be made for each Observing Challenge. If, for example, you observe M31, the Andromeda Galaxy for the Messier Objects Observing Challenge , you cannot use the same observation for the Binocular Sky Observation Challenge . Please remember that the people involved in this project are volunteers who are giving their time freely to run and maintain this programme. -
Biological Damage of Uv Radiation in Environments Of
BIOLOGICAL DAMAGE OF UV RADIATION IN ENVIRONMENTS OF F-TYPE STARS by SATOKO SATO Presented to the Faculty of the Graduate School of The University of Texas at Arlington in Partial Fulfillment of the Requirements for the Degree of DOCTOR OF PHILOSOPHY THE UNIVERSITY OF TEXAS AT ARLINGTON May 2014 Copyright c by Satoko Sato 2014 All Rights Reserved I dedicate this to my daughter Akari Y. Sato. Acknowledgements First of all, I would like to thank my supervising professor Dr. Manfred Cuntz. His advice on my research and academic life has always been invaluable. I would have given up the Ph.D. bound program without his encouragement and generous support as the supervising professor during a few difficult times in my life. I would like to thank Dr. Wei Chen, Dr. Yue Deng, Dr. Zdzislaw E. Musielak, and Dr. Sangwook Park for their interest in my research and for their time to serve in my committee. Next, I would like to acknowledge my research collaborators at University of Guanajuato, Cecilia M. Guerra Olvera, Dr. Dennis Jack, and Dr. Klaus-Peter Schr¨oder,for providing me the data of F-type evolutionary tracks and UV spectra. I would also like to express my deep gratitude to my parents, Hideki and Kumiko Yakushigawa, for their enormous support in many ways in my entire life, and to my sister, Tomoko Yakushigawa, for her constant encouragement to me. I am grateful to my husband, Makito Sato, and my daughter, Akari Y. Sato. Their presence always gives me strength. I am thankful to my parents-in-law, Hisao and Tsuguho Sato, and my grand-parents-in-law, Kanji and Ayako Momoi, for their financial support and prayers. -
Mapping Stellar Kinematics Across the Galactic Bar: HST Measurements Of
Mon. Not. R. Astron. Soc. 000, 000–000 (2006) Printed 24 October 2018 (MN LATEX style file v2.2) Mapping stellar kinematics across the Galactic bar: HST measurements of proper motions in 35 fields. ⋆ S. Koz lowski1†, P. R. Wo´zniak2, S. Mao1, M. C. Smith3, T. Sumi4, W. T. Vestrand2 andL. Wyrzykowski5 1 Jodrell Bank Observatory, The University of Manchester, Macclesfield, Cheshire SK11 9DL, UK 2 Los Alamos National Laboratory, MS-D466, Los Alamos, NM 87545, USA 3 Kapteyn Institute, PO Box 800, 9700 AV Groningen, the Netherlands 4 Princeton University Observatory, Princeton, NJ 08544, USA 5 Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge CB3 OHA, UK Accepted 2006 April 26. Received 2006 April 26; in original form 2006 March 22 ABSTRACT We present a proper motion mini-survey of 35 fields in the vicinity of Baade window, (l,b) = (1◦, −4◦), sampling roughly a 5 × 2.5 deg region of the Galactic bar. Our second epoch observations collected with the ACS/HRC instrument on board the Hubble Space Telescope were combined with the archival WFPC2/PC images. The resulting time baselines are in the range of 4–8 years. Precise proper motions of 15,863 stars were determined in the reference frame defined by the mean motion of stars with magnitudes between IF 814W = 16.5 − 21.5 along the line of sight. We clearly detect −1 small gradients in proper motion dispersions (σl, σb) ∼ (3.0, 2.5) mas yr , and in the amount of anisotropy (σl/σb ∼ 1.2). Both the longitude dispersion σl and its ratio to the vertical motion σb increase toward the Galactic plane. -
Eric Agol – Bibliography
Eric Agol | Curriculum Vitae Department of Astronomy, Box 351580, University of Washington, Seattle, WA 98195-1580 Ó (206) 543-7106 • Q [email protected] • faculty.washington.edu/agol/ Professor of Astronomy, Adjunct Professor of Physics. Previous Employment University of Washington Seattle + Professor 2017 – present Department of Astronomy; Adjunct in Physics. University of Washington Seattle + Associate Professor 2009 –2017 University of Washington Seattle + Assistant Professor 2003 – 2009 Caltech Pasadena + Chandra Fellow 2000 – 2003 Johns Hopkins University Baltimore + Postdoctoral Fellow 1997 – 2000 Education Academic Qualifications................................................... ........................................... University of California Santa Barbara + PhD, Department of Physics, Astrophysics 1992–1997 University of California Berkeley + BA, Physics and Mathematics 1988–1992 Dissertation................................................... ................................................... ......... + ‘The Effects of Magnetic Fields, Absorption, and Relativity on the Polarization of Accretion Disks around Supermassive Black Holes.’ Advisor: Omer Blaes. Selected Research Accomplishments: + Created grid of models for Quasars (Hubeny, Agol et al. 2000; Agol 1997). + Computed optically-thin general-relativistic ray-tracing model, and proposed experiment for imaging the shadow of the Galactic Center black hole (Falcke, Melia & Agol 2000), which culminated in the Event Horizon Telescope. + Derived fast, analytic transit model for -
December 1997
No. 90 – December 1997 T E L E S C O P E S A N D I N S T R U M E N T A T I O N A Deep Field with the Upgraded NTT S. D’ODORICO, ESO This colour deep image has been prepared from 4 deep images through the filters B, V, r and i obtained with the SUSI CCD imager at the ESO NTT. The image covers a 2.2 × 2.2 arcmin “emp- ty” field centred about 2 arcminutes south of the z = 4.7 QSO BR 1202- 0725. The four images result from the co-addition of dithered short integra- tions for a total of 52,800, 23,400, 23,400 and 16,200 seconds in the four bands, and the co-added images have average FWHMs of 0.84, 0.80, 0.80 and 0.68 arcsec respectively. The data were obtained for a scientif- ic programme approved for the ESO Period 58 and aimed at the study of the photometric redshift distribution of the faint galaxies and of gravitational lens- ing effects in the field. The P.I. of the proposal is Sandro D’Odorico and the Co-P.I. are J. Bergeron, H.M. Adorf, S. Charlot, D. Clements, S. Cristiani, L. da Costa, E. Egami, A. Fontana, B. Fort, L. Gautret, E. Giallongo, R. Gilmozzi, R.N. Hook, B. Leibundgut, Y. Mellier, P. Petitjean, A. Renzini, S. Savaglio, P. Shaver, S. Seitz and L. Yan. The pro- gramme was executed in service mode by the NTT team in February through April 1997 in photometric nights with seeing better than 1 arcsec. -
Observing List for Niabi
day month year Epoch 2000 local clock time: 23.98 Observing List for Niabi 16 3 2019 RA DEC alt az Constellation object mag A mag B Separation description hr min deg min 30 291 Auriga M36 open cluster of a dozen or so young stars (30million years old) 5 36.1 34 8 32 287 Auriga M37 rich, open cluster of 150 stars, very fine 5 52.4 32 33 30 293 Auriga M38 large open cluster 220 million years old 5 28.7 35 50 39 301 Auriga IC2149 planetary nebula, stellar to small disk, slightly elongated 5 56.5 46 6.3 33 305 Auriga Capella 0.1 alignment star 5 16.6 46 0 43 288 Auriga UU Aurigae Magnitude 5.1-7.0 carbon star (AL# 36) 6 36.5 38 27 36 291 Auriga 37 Theta Aurigae 2.6 7.1 3.6 white & bluish stars 5 59.7 37 13 25 292 Auriga 14 Aurigae 5.1 7.4 14.6 pale yellow and blue 5 15.4 32 31 54 56 Bootes 17, Kappa Bootis 4.6 6.6 13.4 bright white primary & bluish secondary 14 13.5 51 47 54 56 Bootes 21, Iota Bootis 4.9 7.5 38.5 wide yellow & blue pair 14 16.2 51 22 35 99 Bootes 29, Pi Bootis 4.9 5.8 5.6 fine bright white pair 14 40.7 16 25 40 87 Bootes 36, Epsilon Bootis (Izar) (*311) (HIP72105) 2.9 4.9 2.8 golden & greenish-blue 14 45 27 4 34 94 Bootes 37, Xi Bootis 4.7 7 6.6 beautiful yellow & reddish orange pair 14 51.4 19 6 38 70 Bootes 51, Mu Bootis 4.3 7 108.3 primary of yellow & close orange BC pair 15 24.5 37 23 38 76 Bootes Delta Bootis 3.5 8.7 105 wide yellow & blue pair 15 15.5 33 19 41 101 Bootes Arcturus -0.11 alignment star 14 15.6 19 10.4 41 119 Bootes NGC5248 galaxy with bright stellar nucleus and oval halo 13 37.5 8 53 51 59 Bootes NGC5676 -
A Data Viewer for R
Paul Murrell A Data Viewer for R A Data Viewer for R Paul Murrell The University of Auckland July 30 2009 Paul Murrell A Data Viewer for R Overview Motivation: STATS 220 Problem statement: Students do not understand what they cannot see. What doesn’t work: View() A solution: The rdataviewer package and the tcltkViewer() function. What else?: Novel navigation interface, zooming, extensible for other data sources. Paul Murrell A Data Viewer for R STATS 220 Data Technologies HTML (and CSS), XML (and DTDs), SQL (and databases), and R (and regular expressions) Online text book that nobody reads Computer lab each week (worth 0.5%) + three Assignments 5 labs + one assignment on R Emphasis on creating and modifying data structures Attempt to use real data Paul Murrell A Data Viewer for R Example Lab Question Read the file lab10.txt into R as a character vector. You should end up with a symbol habitats that prints like this (this shows just the first 10 values; there are 192 values in total): > head(habitats, 10) [1] "upwd1201" "upwd0502" "upwd0702" [4] "upwd1002" "upwd1102" "upwd0203" [7] "upwd0503" "upwd0803" "upwd0104" [10] "upwd0704" Paul Murrell A Data Viewer for R The file lab10.txt upwd1201 upwd0502 upwd0702 upwd1002 upwd1102 upwd0203 upwd0503 upwd0803 upwd0104 upwd0704 upwd0804 upwd1204 upwd0805 upwd1005 upwd0106 dnwd1201 dnwd0502 dnwd0702 dnwd1002 dnwd1102 dnwd1202 dnwd0103 dnwd0203 dnwd0303 dnwd0403 dnwd0503 dnwd0803 dnwd0104 dnwd0704 dnwd0804 dnwd1204 dnwd0805 dnwd1005 dnwd0106 uppl0502 uppl0702 uppl1002 uppl1102 uppl0203 uppl0503 -
A Review of the History, Theory and Observations Of
A REVIEW OF THE HISTORY, THEORY AND OBSERVATIONS OF GRAVITATIONAL MICROLENSING UP UNTIL THE PRESENT DAY A thesis submitted in fulfilment of the requirements for the Degree of Master of Science in Astronomy in the University of Canterbury by T. McClelland University of Canterbury 2008 TABLE OF CONTENTS ABSTRACT CHAPTERS 1 The Early History of Lensing Theory ...............................................................................................................................4 Newtonian Mechanics General Relativity 1960 developments Detection 2 Lens Theory and Lensing Phenomena .............................................................................................................................40 The Deflection of Light by Massive Objects Newtonian Mechanics General Relativistic Mechanics Gravitational Lensing Lens Equation Einstein Rings Gravitational Microlensing Quasar Microlensing Light curve variations and implications Parallax Caustic Curves 3 Modern Techniques and their Applications .............................................................................................................................66 Inverse Ray Technique Inverse Polygon Mapping Difference Imaging Astrometry 4 Applications .............................................................................................................................70 Dark Matter Binary Systems Extrasolar Planets Black Holes Stellar Mass Stellar Atmospheres Quasar Abnormalities Understanding Galactic Structure 5 Systematic Observational Networks .............................................................................................................................84 -
NSL3 Variant Map for 2300AD
2300AD Star Map based on Near Star List III Human Homeworld / Colony Homeworld -60 to -30 ly A Blue Human Outpost Trade Route - Chinese Arm -30 to -10 ly F White Kafer Homeworld / Colony Major Trade Route - Chinese Arm Other Route - Chinese Trade Route - American Arm -10 to +10 ly G Yellow Kafer Outpost Major Trade Route - American Arm Other Route - America Trade Route- French Arm +10 to +30 ly K Orange Ylii Homeworld / Colony Major Trade Route- French Arm Other Route- French A M Red Alien Homeworld / Colony +30 to +60 ly -60.0 -59.5 -59.0 -58.5 -58.0 -57.5 -57.0 -56.5 -56.0 -55.5 -55.0 -54.5 -54.0 -53.5 -53.0 -52.5 -52.0 -51.5 -51.0 -50.5 -50.0 -49.5 -49.0 -48.5 -48.0 -47.5 -47.0 -46.5 -46.0 -45.5 -45.0 -44.5 -44.0 -43.5 -43.0 -42.5 -42.0 -41.5 -41.0 -40.5 -40.0 -39.5 -39.0 -38.5 -38.0 -37.5 -37.0 -36.5 -36.0 -35.5 60.0 59.5 59.0 58.5 DM-13 2420 58.0 57.5 DM+22 1921 57.0 56.5 56.0 55.5 55.0 54.5 54.0 DM+21 1949 AC-1 409-15 53.5 53.0 52.5 52.0 51.5 51.0 DM+7 1997 50.5 50.0 49.5 DM+12 1888 Ross 686 49.0 48.5 DM-5 2603 48.0 47.5 47.0 46.5 46.0 DM-5 2778 45.5 45.0 44.5 DM+1 2277 44.0 DM-42 4577 43.5 43.0 42.5 42.0 41.5 DM+8 2131 DM-20 2936 41.0 DM+5 2143 DM-5 2802 40.5 DM+34 1949 40.0 39.5 39.0 38.5 38.0 37.5 Ross 84 37.0 DM-8 2689 36.5 36.0 AC+27 24424 35.5 DM+40 2208 35.0 DM-44 5200 34.5 Theta Antilae 34.0 DM+27 1775 2300AD Star Map based on Near Star List III Human Homeworld / Colony Homeworld -60 to -30 ly A Blue Human Outpost Trade Route - Chinese Arm -30 to -10 ly F White Kafer Homeworld / Colony Major Trade Route - Chinese Arm Other