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THE 1000 BRIGHTEST HIPASS GALAXIES: H I PROPERTIES B
The Astronomical Journal, 128:16–46, 2004 July A # 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A. THE 1000 BRIGHTEST HIPASS GALAXIES: H i PROPERTIES B. S. Koribalski,1 L. Staveley-Smith,1 V. A. Kilborn,1, 2 S. D. Ryder,3 R. C. Kraan-Korteweg,4 E. V. Ryan-Weber,1, 5 R. D. Ekers,1 H. Jerjen,6 P. A. Henning,7 M. E. Putman,8 M. A. Zwaan,5, 9 W. J. G. de Blok,1,10 M. R. Calabretta,1 M. J. Disney,10 R. F. Minchin,10 R. Bhathal,11 P. J. Boyce,10 M. J. Drinkwater,12 K. C. Freeman,6 B. K. Gibson,2 A. J. Green,13 R. F. Haynes,1 S. Juraszek,13 M. J. Kesteven,1 P. M. Knezek,14 S. Mader,1 M. Marquarding,1 M. Meyer,5 J. R. Mould,15 T. Oosterloo,16 J. O’Brien,1,6 R. M. Price,7 E. M. Sadler,13 A. Schro¨der,17 I. M. Stewart,17 F. Stootman,11 M. Waugh,1, 5 B. E. Warren,1, 6 R. L. Webster,5 and A. E. Wright1 Received 2002 October 30; accepted 2004 April 7 ABSTRACT We present the HIPASS Bright Galaxy Catalog (BGC), which contains the 1000 H i brightest galaxies in the southern sky as obtained from the H i Parkes All-Sky Survey (HIPASS). The selection of the brightest sources is basedontheirHi peak flux density (Speak k116 mJy) as measured from the spatially integrated HIPASS spectrum. 7 ; 10 The derived H i masses range from 10 to 4 10 M . -
The Extragalactic Distance Scale
The Extragalactic Distance Scale Published in "Stellar astrophysics for the local group" : VIII Canary Islands Winter School of Astrophysics. Edited by A. Aparicio, A. Herrero, and F. Sanchez. Cambridge ; New York : Cambridge University Press, 1998 Calibration of the Extragalactic Distance Scale By BARRY F. MADORE1, WENDY L. FREEDMAN2 1NASA/IPAC Extragalactic Database, Infrared Processing & Analysis Center, California Institute of Technology, Jet Propulsion Laboratory, Pasadena, CA 91125, USA 2Observatories, Carnegie Institution of Washington, 813 Santa Barbara St., Pasadena CA 91101, USA The calibration and use of Cepheids as primary distance indicators is reviewed in the context of the extragalactic distance scale. Comparison is made with the independently calibrated Population II distance scale and found to be consistent at the 10% level. The combined use of ground-based facilities and the Hubble Space Telescope now allow for the application of the Cepheid Period-Luminosity relation out to distances in excess of 20 Mpc. Calibration of secondary distance indicators and the direct determination of distances to galaxies in the field as well as in the Virgo and Fornax clusters allows for multiple paths to the determination of the absolute rate of the expansion of the Universe parameterized by the Hubble constant. At this point in the reduction and analysis of Key Project galaxies H0 = 72km/ sec/Mpc ± 2 (random) ± 12 [systematic]. Table of Contents INTRODUCTION TO THE LECTURES CEPHEIDS BRIEF SUMMARY OF THE OBSERVED PROPERTIES OF CEPHEID -
10. Scientific Programme 10.1
10. SCIENTIFIC PROGRAMME 10.1. OVERVIEW (a) Invited Discourses Plenary Hall B 18:00-19:30 ID1 “The Zoo of Galaxies” Karen Masters, University of Portsmouth, UK Monday, 20 August ID2 “Supernovae, the Accelerating Cosmos, and Dark Energy” Brian Schmidt, ANU, Australia Wednesday, 22 August ID3 “The Herschel View of Star Formation” Philippe André, CEA Saclay, France Wednesday, 29 August ID4 “Past, Present and Future of Chinese Astronomy” Cheng Fang, Nanjing University, China Nanjing Thursday, 30 August (b) Plenary Symposium Review Talks Plenary Hall B (B) 8:30-10:00 Or Rooms 309A+B (3) IAUS 288 Astrophysics from Antarctica John Storey (3) Mon. 20 IAUS 289 The Cosmic Distance Scale: Past, Present and Future Wendy Freedman (3) Mon. 27 IAUS 290 Probing General Relativity using Accreting Black Holes Andy Fabian (B) Wed. 22 IAUS 291 Pulsars are Cool – seriously Scott Ransom (3) Thu. 23 Magnetars: neutron stars with magnetic storms Nanda Rea (3) Thu. 23 Probing Gravitation with Pulsars Michael Kremer (3) Thu. 23 IAUS 292 From Gas to Stars over Cosmic Time Mordacai-Mark Mac Low (B) Tue. 21 IAUS 293 The Kepler Mission: NASA’s ExoEarth Census Natalie Batalha (3) Tue. 28 IAUS 294 The Origin and Evolution of Cosmic Magnetism Bryan Gaensler (B) Wed. 29 IAUS 295 Black Holes in Galaxies John Kormendy (B) Thu. 30 (c) Symposia - Week 1 IAUS 288 Astrophysics from Antartica IAUS 290 Accretion on all scales IAUS 291 Neutron Stars and Pulsars IAUS 292 Molecular gas, Dust, and Star Formation in Galaxies (d) Symposia –Week 2 IAUS 289 Advancing the Physics of Cosmic -
NATIONAL ACADEMIES of SCIENCES and ENGINEERING NATIONAL RESEARCH COUNCIL of the UNITED STATES of AMERICA
NATIONAL ACADEMIES OF SCIENCES AND ENGINEERING NATIONAL RESEARCH COUNCIL of the UNITED STATES OF AMERICA UNITED STATES NATIONAL COMMITTEE International Union of Radio Science National Radio Science Meeting 4-8 January 2000 Sponsored by USNC/URSI University of Colorado Boulder, Colorado U.S.A. United States National Committee INTERNATIONAL UNION OF RADIO SCIENCE PROGRAM AND ABSTRACTS National Radio Science Meeting 4-8 January 2000 Sponsored by USNC/URSI NOTE: Programs and Abstracts of the USNC/URSI Meetings are available from: USNC/URSI National Academy of Sciences 2101 Constitution Avenue, N.W. Washington, DC 20418 at $5 for 1983-1999 meetings. The full papers are not published in any collected format; requests for them should be addressed to the authors who may have them published on their own initiative. Please note that these meetings are national. They are not organized by the International Union, nor are the programs available from the International Secretariat. ii MEMBERSHIP United States National Committee INTERNATIONAL UNION OF RADIO SCIENCE Chair: Gary Brown* Secretary & Chair-Elect: Umran S. !nan* Immediate Past Chair: Susan K. Avery* Members Representing Societies, Groups, and Institutes: American Astronomical Society Thomas G. Phillips American Geophysical Union Donald T. Farley American Meteorological Society vacant IEEE Antennas and Propagation Society Linda P.B. Katehi IEEE Geosciences and Remote Sensing Society Roger Lang IEEE Microwave Theory and Techniques Society Arthur A. Oliner Members-at-Large: Amalia Barrios J. Richard Fisher Melinda Picket-May Ronald Pogorzelski W. Ross Stone Richard Ziolkowski Chairs of the USNC/URSI Commissions: Commission A Moto Kanda Commission B Piergiorgio L. E. Uslenghi Commission C Alfred 0. -
Astrostatistics
CHANCEVol. 32, No. 3, 2019 Using Data to Advance Science, Education, and Society Special Issue on ASTROSTATISTICS Including... Statistics for Stellar Systems: From Globular Clusters to Clusters of Galaxies ARIMA for the Stars: How Statistics Finds Exoplanets 09332480(2019)32(3) EXCLUSIVE BENEFITS FOR ALL ASA MEMBERS! SAVE 30% on Book Purchases with discount code ASA18. Visit the new ASA Membership page to unlock savings on the latest books, access exclusive content and review our latest journal articles! With a growing recognition of the importance of statistical reasoning across many different aspects of everyday life and in our data-rich world, the American Statistical Society and CRC Press have partnered to develop the ASA-CRC Series on Statistical Reasoning in Science and Society. This exciting book series features: • Concepts presented while assuming minimal background in Mathematics and Statistics. • A broad audience including professionals across many fields, the general public and courses in high schools and colleges. • Topics include Statistics in wide-ranging aspects of professional and everyday life, including the media, science, health, society, politics, law, education, sports, finance, climate, and national security. DATA VISUALIZATION Charts, Maps, and Interactive Graphs Robert Grant, BayersCamp This book provides an introduction to the general principles of data visualization, with a focus on practical considerations for people who want to understand them or start making their own. It does not cover tools, which are varied and constantly changing, but focusses on the thought process of choosing the right format and design to best serve the data and the message. September 2018 • 210 pp • Pb: 9781138707603: $29.95 $23.96 • www.crcpress.com/9781138707603 VISUALIZING BASEBALL Jim Albert, Bowling Green State University, Ohio, USA A collection of graphs will be used to explore the game of baseball. -
Waiting with Baboons
CAREER VIEW NATURE|Vol 455|30 October 2008 MOVERS NETWORKS & SUPPORT Colin Lonsdale, director, Haystack Observatory, Massachusetts Institute of Technology, Sustenance for sustainability Westford, Massachusetts Scientists who seek intensely curiosity-driven research to short- interdisciplinary study could be term goals. Within the next 2 years, 2006–08: Assistant director, the beneficiaries of increasing they plan to recruit at least 10 Haystack Observatory, interest in the emerging field of faculty members, 10–20 graduate Massachusetts Institute of sustainability research, with new students and up to 5 postdocs to Technology university programmes offering tackle technical issues surrounding 1986–2008: Research novel opportunities. Portland State alternative energy sources, scientist, Haystack University in Oregon and Cornell sustainable urban communities Observatory, Massachusetts University in Ithaca, New York, are the and developing the metrics of Institute of Technology most recent entrants to the field. They sustainability. He also hopes to set 1983–86: Research follow the example set by institutions up a visiting faculty programme associate, Pennsylvania State such as the School of Sustainability at to forge national and international University, University Park, Arizona State University in Tempe. connections. Pennsylvania Broadly defined, sustainability Cornell’s Institute for Computational bridges disciplines to determine how Sustainability involves scientists from Colin Lonsdale says radio astronomy is experiencing a to meet the -
Scientific Problems Addressed by the Spektr-UV Space Project (World Space Observatory—Ultraviolet)
ISSN 1063-7729, Astronomy Reports, 2016, Vol. 60, No. 1, pp. 1–42. c Pleiades Publishing, Ltd., 2016. Original Russian Text c A.A. Boyarchuk, B.M. Shustov, I.S. Savanov, M.E. Sachkov, D.V. Bisikalo, L.I. Mashonkina, D.Z. Wiebe, V.I. Shematovich, Yu.A. Shchekinov, T.A. Ryabchikova, N.N. Chugai, P.B. Ivanov, N.V. Voshchinnikov, A.I. Gomez de Castro, S.A. Lamzin, N. Piskunov, T. Ayres, K.G. Strassmeier, S. Jeffrey, S.K. Zwintz, D. Shulyak, J.-C. G´erard, B. Hubert, L. Fossati, H. Lammer, K. Werner, A.G. Zhilkin, P.V. Kaigorodov, S.G. Sichevskii, S. Ustamuich, E.N. Kanev, E.Yu. Kil’pio, 2016, published in Astronomicheskii Zhurnal, 2016, Vol. 93, No. 1, pp. 3–48. Scientific Problems Addressed by the Spektr-UV Space Project (World Space Observatory—Ultraviolet) A. A. Boyarchuk1, B.M.Shustov1*, I. S. Savanov1, M.E.Sachkov1, D. V. Bisikalo1, L. I. Mashonkina1, D.Z.Wiebe1,V.I.Shematovich1,Yu.A.Shchekinov2, T. A. Ryabchikova1, N.N.Chugai1, P.B.Ivanov3, N.V.Voshchinnikov4, A. I. Gomez de Castro5,S.A.Lamzin6,N.Piskunov7,T.Ayres8, K. G. Strassmeier9, S. Jeffrey10,S.K.Zwintz11, D. Shulyak12,J.-C.Gerard´ 13,B.Hubert13, L. Fossati14, H. Lammer14,K.Werner15,A.G.Zhilkin1,P.V.Kaigorodov1, S. G. Sichevskii1,S.Ustamuich5,E.N.Kanev1, and E. Yu. Kil’pio1 1Institute of Astronomy, Russian Academy of Sciences, ul. Pyatnitskaya 48, Moscow, 119017 Russia 2Southern Federal University, Rostov-on-Don, 344006 Russia 3Astro Space Center, Lebedev Physical Institute, Russian Academy of Sciences, Moscow, Russia 4St. -
Making a Sky Atlas
Appendix A Making a Sky Atlas Although a number of very advanced sky atlases are now available in print, none is likely to be ideal for any given task. Published atlases will probably have too few or too many guide stars, too few or too many deep-sky objects plotted in them, wrong- size charts, etc. I found that with MegaStar I could design and make, specifically for my survey, a “just right” personalized atlas. My atlas consists of 108 charts, each about twenty square degrees in size, with guide stars down to magnitude 8.9. I used only the northernmost 78 charts, since I observed the sky only down to –35°. On the charts I plotted only the objects I wanted to observe. In addition I made enlargements of small, overcrowded areas (“quad charts”) as well as separate large-scale charts for the Virgo Galaxy Cluster, the latter with guide stars down to magnitude 11.4. I put the charts in plastic sheet protectors in a three-ring binder, taking them out and plac- ing them on my telescope mount’s clipboard as needed. To find an object I would use the 35 mm finder (except in the Virgo Cluster, where I used the 60 mm as the finder) to point the ensemble of telescopes at the indicated spot among the guide stars. If the object was not seen in the 35 mm, as it usually was not, I would then look in the larger telescopes. If the object was not immediately visible even in the primary telescope – a not uncommon occur- rence due to inexact initial pointing – I would then scan around for it. -
Ngc Catalogue Ngc Catalogue
NGC CATALOGUE NGC CATALOGUE 1 NGC CATALOGUE Object # Common Name Type Constellation Magnitude RA Dec NGC 1 - Galaxy Pegasus 12.9 00:07:16 27:42:32 NGC 2 - Galaxy Pegasus 14.2 00:07:17 27:40:43 NGC 3 - Galaxy Pisces 13.3 00:07:17 08:18:05 NGC 4 - Galaxy Pisces 15.8 00:07:24 08:22:26 NGC 5 - Galaxy Andromeda 13.3 00:07:49 35:21:46 NGC 6 NGC 20 Galaxy Andromeda 13.1 00:09:33 33:18:32 NGC 7 - Galaxy Sculptor 13.9 00:08:21 -29:54:59 NGC 8 - Double Star Pegasus - 00:08:45 23:50:19 NGC 9 - Galaxy Pegasus 13.5 00:08:54 23:49:04 NGC 10 - Galaxy Sculptor 12.5 00:08:34 -33:51:28 NGC 11 - Galaxy Andromeda 13.7 00:08:42 37:26:53 NGC 12 - Galaxy Pisces 13.1 00:08:45 04:36:44 NGC 13 - Galaxy Andromeda 13.2 00:08:48 33:25:59 NGC 14 - Galaxy Pegasus 12.1 00:08:46 15:48:57 NGC 15 - Galaxy Pegasus 13.8 00:09:02 21:37:30 NGC 16 - Galaxy Pegasus 12.0 00:09:04 27:43:48 NGC 17 NGC 34 Galaxy Cetus 14.4 00:11:07 -12:06:28 NGC 18 - Double Star Pegasus - 00:09:23 27:43:56 NGC 19 - Galaxy Andromeda 13.3 00:10:41 32:58:58 NGC 20 See NGC 6 Galaxy Andromeda 13.1 00:09:33 33:18:32 NGC 21 NGC 29 Galaxy Andromeda 12.7 00:10:47 33:21:07 NGC 22 - Galaxy Pegasus 13.6 00:09:48 27:49:58 NGC 23 - Galaxy Pegasus 12.0 00:09:53 25:55:26 NGC 24 - Galaxy Sculptor 11.6 00:09:56 -24:57:52 NGC 25 - Galaxy Phoenix 13.0 00:09:59 -57:01:13 NGC 26 - Galaxy Pegasus 12.9 00:10:26 25:49:56 NGC 27 - Galaxy Andromeda 13.5 00:10:33 28:59:49 NGC 28 - Galaxy Phoenix 13.8 00:10:25 -56:59:20 NGC 29 See NGC 21 Galaxy Andromeda 12.7 00:10:47 33:21:07 NGC 30 - Double Star Pegasus - 00:10:51 21:58:39 -
Radio Astronomy Institute"-Radioscience Laboratory, Stanford Univefsity - Frank D
Up 1h~ {~Ji()}Oec41.,! t;7/JI~,.rt5 vel ,J-~cpt:fT ~)11. I ~ SqP1~ /? /lA.f "'6~n~ ~ 6V"C~Mk';, .-.If?t)J M4fer Z,I/ lCJop.r - ~.t'1 ..r I'e-t ".r . !l4'C~1/ ,-1"1/}'/ , 70. f!ql'~ ~ N.~ - 1. .. I. r--/,./r ~ ~ J ! "c ~r~1H ,-~/~ POT- SHors NO · IISI Don't take the -Pr'esent m oment too sertousld;J gt ~"n' be h ere for to~. :TABLE b: SCORECARD ;1Lt. ,A. ,Never /yery REPORT Numbel' of Number i* Operation Number in operation Number eventually Number 'eventually unlikely Identifiable ~ 15 yr *fter report ,;;; 15 yr after report built with built with Items with mostly federal with mostly other ' mostly federal mostly other Requested funding , fundingCs tate, funding funding ptiyate, foreign) Whitford 13 6 0 0 , 1 6 Greenstein 21 5 (+1 similar) 2' 4 1 8 Fie ld 21 3 (+2 similar) 2 3 2 9 Baheall 29 11 6 5 () 7 McKee-Taylor 23 8 1 5 3 6 TOTAL 106 33 (::t, 3 similar) 11 17 7 36 /" PANEL ON ASTRONOMICAL FACILITIES A. E. W bittw:d.. Chairman, Lick ObsefvatofY, University of California R. N. lJrqcewell, Radio Astronomy Institute"-Radioscience Laboratory, Stanford Univefsity - Frank D. Drake, Department of Astronomy, Cornell Univefsity Frederick T. Haddock, Jr., Radio Astronomy Observatory, University of Michigan ,..-----William Liller, Department of Astronomy, Harvard University W. W. Morgan, Yerkes Observatory, University of Chicago Bruce H. Rule, California Institute of Technology · ·-~\llan R. Sandage, Mt. Wilson and Palomar Observatories, California Institute of Technology, Carnegie Institution of Washington Whit£ODd - publ . -
European VLBI Network Newsletter Number 5 May 2003 EVN User JIVE Newsletter Publications Meetings Proposals Homepage Support Homepage Archive
European VLBI Network: Newsletter 5 - May 2003 Página 1 de 10 European VLBI Network Newsletter Number 5 May 2003 EVN User JIVE Newsletter Publications Meetings Proposals Homepage Support Homepage Archive Contents 1. Call for Proposals - Deadline 1 June 2003 2. Report from the Chairman of the CBD of the EVN 3. HRH Prince Charles Rededicates the Lovell Telescope 4. Problems with the Effelsberg Track 5. EVN Achieves e-VLBI 1 Gbps Fringes 6. Report on the 2nd e-VLBI Workshop held at JIVE, Dwingeloo, 15-16 May 2003 7. The First Step Towards a Deep Extragalactic VLBI-Optical Survey (DEVOS) 8. High-sensitivity Observations of Radio Supernovae in Arp 220 1. Call for Proposals - Deadline 1 June 2003 Observing proposals are invited for the EVN, a VLBI network of radio telescopes in Europe and beyond operated by an international Consortium of institutes (http://www.evlbi.org). The EVN is open to all astronomers, and encourages use of the Network by astronomers not specialised in the VLBI technique. The Joint Institute for VLBI in Europe, JIVE (http://www.jive.nl), can provide support and advice on project preparation, scheduling, correlation and analysis. See htmlhttp://www.evlbi.org/support/evn_support.html. Complete a coversheet (now available in LaTeX format) and attach a scientific justification (maximum 2 pages). Up to 2 additional pages with diagrams may be included; the total, including cover sheet, should not exceed 6 pages. See http://www.evlbi.org/proposals/prop.html. The detailed "Call for Proposals" has further information on Global VLBI, EVN+MERLIN and guidelines for proposal submission: see http://www.obs.u-bordeaux1.fr/vlbi/EVN/call-long.html. -
The Messier Objects
Warren H. Finlay Concise Catalog of Deep-Sky Objects Astrophysical Information for 550 Galaxies, Clusters and Nebulae Second Edition The Patrick Moore The Patrick Moore Practical Astronomy Series For further volumes: http://www.springer.com/series/3192 Concise Catalog of Deep-Sky Objects Astrophysical Information for 550 Galaxies, Clusters and Nebulae Warren H. Finlay Second Edition Warren H. Finlay Edmonton , AB , Canada ISSN 1431-9756 ISSN 2197-6562 (electronic) ISBN 978-3-319-03169-9 ISBN 978-3-319-03170-5 (eBook) DOI 10.1007/978-3-319-03170-5 Springer Cham Heidelberg New York Dordrecht London Library of Congress Control Number: 2014938104 © Springer International Publishing Switzerland 2003, 2014 This work is subject to copyright. All rights are reserved by the Publisher, whether the whole or part of the material is concerned, specifi cally the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microfi lms or in any other physical way, and transmission or information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed. Exempted from this legal reservation are brief excerpts in connection with reviews or scholarly analysis or material supplied specifi cally for the purpose of being entered and executed on a computer system, for exclusive use by the purchaser of the work. Duplication of this publication or parts thereof is permitted only under the provisions of the Copyright Law of the Publisher’s location, in its current version, and permission for use must always be obtained from Springer. Permissions for use may be obtained through RightsLink at the Copyright Clearance Center.