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Walker 90/V590 Monocerotis
Brigham Young University BYU ScholarsArchive Faculty Publications 2008-05-17 The enigmatic young object: Walker 90/V590 Monocerotis M. D. Joner [email protected] M. R. Perez B. McCollum M. E. van dend Ancker Follow this and additional works at: https://scholarsarchive.byu.edu/facpub Part of the Astrophysics and Astronomy Commons, and the Physics Commons BYU ScholarsArchive Citation Joner, M. D.; Perez, M. R.; McCollum, B.; and van dend Ancker, M. E., "The enigmatic young object: Walker 90/V590 Monocerotis" (2008). Faculty Publications. 189. https://scholarsarchive.byu.edu/facpub/189 This Peer-Reviewed Article is brought to you for free and open access by BYU ScholarsArchive. It has been accepted for inclusion in Faculty Publications by an authorized administrator of BYU ScholarsArchive. For more information, please contact [email protected], [email protected]. A&A 486, 533–544 (2008) Astronomy DOI: 10.1051/0004-6361:200809933 & c ESO 2008 Astrophysics The enigmatic young object: Walker 90/V590 Monocerotis, M. R. Pérez1, B. McCollum2,M.E.vandenAncker3, and M. D. Joner4 1 Los Alamos National Laboratory, PO Box 1663, ISR-1, MS B244, Los Alamos, NM 87545, USA e-mail: [email protected] 2 Caltech, SIRTF Science Center, MS, 314-6, Pasadena, CA 91125, USA e-mail: [email protected] 3 European Southern Observatory, Karl-Schwarzschild-Strasse 2, 85748, Garching bei München, Germany e-mail: [email protected] 4 Brigham Young University, Dept. of Physics and Astronomy – ESC – N488, Provo, Utah 84602, USA e-mail: [email protected] Received 8 April 2008 / Accepted 17 May 2008 ABSTRACT Aims. -
David Charbonneau Refereed Publications As of May 2015
David Charbonneau Refereed Publications as of May 2015 160. Low False Positive Rate of Kepler Candidates Estimated From A Combination Of Spitzer And Follow-Up Observations Désert, Jean-Michel; Charbonneau, David; Torres, Guillermo; Fressin, François; Ballard, Sarah; Bryson, Stephen T.; Knutson, Heather A.; Batalha, Natalie M.; Borucki, William J.; Brown, Timothy M.; Deming, Drake; Ford, Eric B.; Fortney, Jonathan J.; Gilliland, Ronald L.; Latham, David W.; Seager, Sara The Astrophysical Journal, Volume 804, Issue 1, article id. 59 (2015). 159. The Mass of Kepler-93b and The Composition of Terrestrial Planets Dressing, Courtney D.; Charbonneau, David; Dumusque, Xavier; Gettel, Sara; Pepe, Francesco; Collier Cameron, Andrew; Latham, David W.; Molinari, Emilio; Udry, Stéphane; Affer, Laura; Bonomo, Aldo S.; Buchhave, Lars A.; Cosentino, Rosario; Figueira, Pedro; Fiorenzano, Aldo F. M.; Harutyunyan, Avet; Haywood, Raphaëlle D.; Johnson, John Asher; Lopez-Morales, Mercedes; Lovis, Christophe; Malavolta, Luca; Mayor, Michel; Micela, Giusi; Motalebi, Fatemeh; Nascimbeni, Valerio; Phillips, David F.; Piotto, Giampaolo; Pollacco, Don; Queloz, Didier; Rice, Ken; Sasselov, Dimitar; Ségransan, Damien; Sozzetti, Alessandro; Szentgyorgyi, Andrew; Watson, Chris The Astrophysical Journal, Volume 800, Issue 2, article id. 135 (2015). 158. An Empirical Calibration to Estimate Cool Dwarf Fundamental Parameters from H-band Spectra Newton, Elisabeth R.; Charbonneau, David; Irwin, Jonathan; Mann, Andrew W. The Astrophysical Journal, Volume 800, Issue 2, article -
The Minor Planet Bulletin
THE MINOR PLANET BULLETIN OF THE MINOR PLANETS SECTION OF THE BULLETIN ASSOCIATION OF LUNAR AND PLANETARY OBSERVERS VOLUME 36, NUMBER 3, A.D. 2009 JULY-SEPTEMBER 77. PHOTOMETRIC MEASUREMENTS OF 343 OSTARA Our data can be obtained from http://www.uwec.edu/physics/ AND OTHER ASTEROIDS AT HOBBS OBSERVATORY asteroid/. Lyle Ford, George Stecher, Kayla Lorenzen, and Cole Cook Acknowledgements Department of Physics and Astronomy University of Wisconsin-Eau Claire We thank the Theodore Dunham Fund for Astrophysics, the Eau Claire, WI 54702-4004 National Science Foundation (award number 0519006), the [email protected] University of Wisconsin-Eau Claire Office of Research and Sponsored Programs, and the University of Wisconsin-Eau Claire (Received: 2009 Feb 11) Blugold Fellow and McNair programs for financial support. References We observed 343 Ostara on 2008 October 4 and obtained R and V standard magnitudes. The period was Binzel, R.P. (1987). “A Photoelectric Survey of 130 Asteroids”, found to be significantly greater than the previously Icarus 72, 135-208. reported value of 6.42 hours. Measurements of 2660 Wasserman and (17010) 1999 CQ72 made on 2008 Stecher, G.J., Ford, L.A., and Elbert, J.D. (1999). “Equipping a March 25 are also reported. 0.6 Meter Alt-Azimuth Telescope for Photometry”, IAPPP Comm, 76, 68-74. We made R band and V band photometric measurements of 343 Warner, B.D. (2006). A Practical Guide to Lightcurve Photometry Ostara on 2008 October 4 using the 0.6 m “Air Force” Telescope and Analysis. Springer, New York, NY. located at Hobbs Observatory (MPC code 750) near Fall Creek, Wisconsin. -
1 1/4/18 Dr. Stefi Alison Baum Dean, Faculty of Science Professor, Dept
RESUME – DR. STEFI BAUM, 1/4/18 Dr. Stefi Alison Baum Dean, Faculty of Science Professor, Dept. of Physics and Astronomy University of Manitoba Winnipeg, MB, Canada Email [email protected] cell phone 204-297-0698 EDUCATION B.A. Physics, cum laude June 1980 Harvard University, Cambridge, MA Co-Captain Varsity Women’s Lacrosse and Co-Captain Varsity Women’s Soccer PhD Astronomy Dec 1987 University of Maryland, College Park, MD POST-DEGREE EDUCATION Center for Higher Education Research and Development • The Senior University Administrators Course, Niagara-on-the-Lake, 2015 University of Wisconsin-Madison, Fluno Center, Executive Education, 2013 • Fundraising and Development for Nonprofits Harvard University, Graduate School of Education, 2012 • Performance Assessment in Higher Education Peabody Fellow, Vanderbilt Peabody Professional Institute, 2011 • Higher Education Management Pardee RAND Graduate School, 2009, New Security Challenges Harvard-MIT-Tufts Program on Negotiation, Executive Ed Series, 2007 • Program on Negotiation for Senior Executives • Dealing with Difficult People and Difficult Situations American Council on Education, 2005, Chairing the Academic Department MIT-Sloan Executive Series, 2002, 2003, 2005: • System Dynamics for Senior Managers • Managing Technical Professionals and Organizations • The Innovative Organization United States Foreign Service Institute, 2004, Global Issues Coursera Courses Completed - 2013 • Leading Innovative Change in Organizations, Vanderbilt University • Synapses, Neurons and Brains, Hebrew University of Jerusalem • What a Plant Knows, Tel Aviv University, (audit) • Epigenetic Control of Gene Expression, University of Melborne, (audit) • A Brief History of Humankind, Hebrew University (audit) • Surviving Disruptive Technologies, University of Maryland, (audit) 1 EXPERTISE Over 25 years of leadership in highly interdisciplinary research and educational environments, including higher education, not for profits, and government agencies. -
The Impact of the Astro2010 Recommendations on Variable Star Science
The Impact of the Astro2010 Recommendations on Variable Star Science Corresponding Authors Lucianne M. Walkowicz Department of Astronomy, University of California Berkeley [email protected] phone: (510) 642–6931 Andrew C. Becker Department of Astronomy, University of Washington [email protected] phone: (206) 685–0542 Authors Scott F. Anderson, Department of Astronomy, University of Washington Joshua S. Bloom, Department of Astronomy, University of California Berkeley Leonid Georgiev, Universidad Autonoma de Mexico Josh Grindlay, Harvard–Smithsonian Center for Astrophysics Steve Howell, National Optical Astronomy Observatory Knox Long, Space Telescope Science Institute Anjum Mukadam, Department of Astronomy, University of Washington Andrej Prsa,ˇ Villanova University Joshua Pepper, Villanova University Arne Rau, California Institute of Technology Branimir Sesar, Department of Astronomy, University of Washington Nicole Silvestri, Department of Astronomy, University of Washington Nathan Smith, Department of Astronomy, University of California Berkeley Keivan Stassun, Vanderbilt University Paula Szkody, Department of Astronomy, University of Washington Science Frontier Panels: Stars and Stellar Evolution (SSE) February 16, 2009 Abstract The next decade of survey astronomy has the potential to transform our knowledge of variable stars. Stellar variability underpins our knowledge of the cosmological distance ladder, and provides direct tests of stellar formation and evolution theory. Variable stars can also be used to probe the fundamental physics of gravity and degenerate material in ways that are otherwise impossible in the laboratory. The computational and engineering advances of the past decade have made large–scale, time–domain surveys an immediate reality. Some surveys proposed for the next decade promise to gather more data than in the prior cumulative history of astronomy. -
June 2013 BRAS Newsletter
www.brastro.org June 2013 What's in this issue: PRESIDENT'S MESSAGE .............................................................................................................................. 2 NOTES FROM THE VICE PRESIDENT ........................................................................................................... 3 MESSAGE FROM THE HRPO ...................................................................................................................... 4 OBSERVING NOTES ..................................................................................................................................... 6 MAY ASTRONOMICAL EVENTS .................................................................................................................... 9 PRESIDENT'S MESSAGE Greetings Everyone, Summer is here and with it the humidity and bugs, but I hope that won't stop you from getting out to see some of the great summer time objects in the sky. Also, Saturn is looking quite striking as the rings are now tilted at a nice angle allowing us to see the Casini Division and shadows on and from the planet. Don't miss it! I've been asked by BREC to make sure our club members are all aware of the Park Rules listed on BREC's website. Many of the rules are actually ordinances enacted by the city of Baton Rouge (e.g., No smoking permitted in public areas, No alcohol brought onto or sold on BREC property, No Gambling, No Firearms or Weapons, etc.) Please make sure you observe all of the Park Rules while at the HRPO and provide good examples for the general public. (Many of which are from outside East Baton Rouge Parish and are likely unaware of some of the policies.) For a full list of BREC's Park Rules, you may visit their Park Rules section of their website at http://brec.org/index.cfm/page/555/n/75 I'm sorry I had to miss the outing to LIGO, but it will be good to see some folks again at our meeting on Monday, June 10th. -
The Astronomy Theory, Observations and Methods (ATOM) Journal
Robotic Telescopes, Student Research and Education (RTSRE) Proceedings Conference Proceedings, Hilo, Hawaii, USA, Jul 23-27, 2018 Fitzgerald, M., Bartlett, S., Salimpour, S., Eds. Vol. 2, No. 1, (2019) ISBN 978-0-6483996-1-2 / doi : 10.32374/rtsre.2019.003 / CC BY-NC-ND license Peer Reviewed Article. rtsre.org/ojs Rationale for a New Journal: the Astronomy Theory, Observations and Methods (ATOM) Journal Michael Fitzgerald1* Abstract In this article, the rationale behind the creation of a new journal, Astronomy Theory, Observa- tions and Methods (ATOM) journal, currently hosted at rtsre.org is provided. It aims to fill a niche in the community for papers on any general topic in astronomy that may not find their place in top tier astronomical journals. The article outlines the thinking behind why there is a gap to be filled with regards to current scholarly metrics and the nature of other journals of similar scope and impact. The journal aims to be accessible to new and novice scientific authors, as well as those more established, through accessible developmental peer review and an explicit aim to avoid using publication metrics as a barrier to publication selection. The scope, which accepts more broader articles than most, of the journal and considerations on behalf of a potential author are also outlined. Keywords Scientific publishing — Amateur Astronomy — Student Research — Scientometrics 1School of Education, Edith Cowan University *Corresponding author: psyfi[email protected] journal, such as MNRAS, ApJ, AJ or AA, PASP or PASA. The “race to the top” for mainstream astron- Introduction omy journals means that the journals in the middle Part of the rationale for many astronomy student to top range of impact factor, such as those men- research projects (e.g. -
Introductory Guide for Authors This Guide Is for Early-Career Researchers Who Are Beginning to Write Papers for Publication
Introductory guide for authors This guide is for early-career researchers who are beginning to write papers for publication. publishingsupport.iopscience.org publishingsupport.iopscience.org This guide is for early-career researchers who are beginning to write papers for publication. Academic publishing is rapidly changing, with new technologies and publication models giving authors much more choice over where and how to publish their work. Whether you are writing up the results of a PhD chapter or submitting your first paper, knowing how to prepare your work for publication is essential. This guide will provide an overview of academic publishing and advice on how to make the most of the process for sharing your research. For more information and to download a digital version of this guide go to publishingsupport.iopscience.org. c o n t e n t s Page Choosing where to submit your paper 4 Writing and formatting 6 Peer-review process 8 Revising and responding to referee reports 10 Acceptance and publication 12 Promoting your published work 13 Copyright and ethical integrity 14 Frequently asked questions 15 Publishing glossary 16 IOP publications 18 Introductory guide for authors 3 publishingsupport.iopscience.org Choosing where to submit your paper It can be tempting to begin writing a paper before giving much thought to where it might be published. However, choosing a journal to target before you begin to prepare your paper will enable you to tailor your writing to the journal’s audience and format your paper according to its specific guidelines, which you may find on the journal’s website. -
Profile Variability of the Hα and Hβ Broad Emission Lines in NGC 5548
Astronomy & Astrophysics manuscript no. (will be inserted by hand later) Profile variability of the Hα and Hβ broad emission lines in NGC 5548 A.I. Shapovalova1,5, V.T. Doroshenko2,7, N.G. Bochkarev2, A.N. Burenkov1,5, L. Carrasco3, V.H. Chavushyan3, S. Collin4, J.R. Vald´es3, N. Borisov1, A.-M. Dumont4, V.V. Vlasuyk1, I. Chillingarian2, I.S. Fioktistova1, and O.M. Martinez6 1 Special Astrophysical Observatory of the Russian AS, Nizhnij Arkhyz, Karachaevo-Cherkesia, 369167, Russia 2 Sternberg Astronomical Institute, University of Moscow, Universitetskij Prospect 13, Moscow 119899, Russia 3 Instituto Nacional de Astrof´isica, Optica y Electr´onica, INAOE, Apartado Postal 51 y 216, 7200, Puebla, Pue., M´exico 4 LUTH, Observatoire de Paris, Section de Meudon, Place Janssen, 92195, Meudon France 5 Isaac Newton Institute of Chile, SAO Branch, Russia 6 Benem´erita Universidad Aut´onoma de Puebla, Facultad de Ciencias F´ısico-Matem´aticas, Apdo. Postal 1152, C.P. 72000, Puebla, Pue. M´exico 7 Isaac Newton Institute of Chile, Crimean Branch, Ukraine Received: 10 November 2003 / Accepted: 26 April 2004 Abstract. Between 1996 and 2002, we have carried out a spectral monitoring program for the Seyfert galaxy NGC 5548 with the 6 m and 1 m telescopes of SAO (Russia) and with the 2.1 m telescope of Guillermo Haro Observatory (GHO) at Cananea, M´exico. High quality spectra with S/N> 50 in the continuum near Hα and Hβ were obtained, covering the spectral range ∼(4000 – 7500) A˚ with a (4.5 to 15) A-resolution.˚ We found that both the flux in the lines and the continuum gradually decreased, reaching minimum values during May-June 2002. -
Meeting Program
A A S MEETING PROGRAM 211TH MEETING OF THE AMERICAN ASTRONOMICAL SOCIETY WITH THE HIGH ENERGY ASTROPHYSICS DIVISION (HEAD) AND THE HISTORICAL ASTRONOMY DIVISION (HAD) 7-11 JANUARY 2008 AUSTIN, TX All scientific session will be held at the: Austin Convention Center COUNCIL .......................... 2 500 East Cesar Chavez St. Austin, TX 78701 EXHIBITS ........................... 4 FURTHER IN GRATITUDE INFORMATION ............... 6 AAS Paper Sorters SCHEDULE ....................... 7 Rachel Akeson, David Bartlett, Elizabeth Barton, SUNDAY ........................17 Joan Centrella, Jun Cui, Susana Deustua, Tapasi Ghosh, Jennifer Grier, Joe Hahn, Hugh Harris, MONDAY .......................21 Chryssa Kouveliotou, John Martin, Kevin Marvel, Kristen Menou, Brian Patten, Robert Quimby, Chris Springob, Joe Tenn, Dirk Terrell, Dave TUESDAY .......................25 Thompson, Liese van Zee, and Amy Winebarger WEDNESDAY ................77 We would like to thank the THURSDAY ................. 143 following sponsors: FRIDAY ......................... 203 Elsevier Northrop Grumman SATURDAY .................. 241 Lockheed Martin The TABASGO Foundation AUTHOR INDEX ........ 242 AAS COUNCIL J. Craig Wheeler Univ. of Texas President (6/2006-6/2008) John P. Huchra Harvard-Smithsonian, President-Elect CfA (6/2007-6/2008) Paul Vanden Bout NRAO Vice-President (6/2005-6/2008) Robert W. O’Connell Univ. of Virginia Vice-President (6/2006-6/2009) Lee W. Hartman Univ. of Michigan Vice-President (6/2007-6/2010) John Graham CIW Secretary (6/2004-6/2010) OFFICERS Hervey (Peter) STScI Treasurer Stockman (6/2005-6/2008) Timothy F. Slater Univ. of Arizona Education Officer (6/2006-6/2009) Mike A’Hearn Univ. of Maryland Pub. Board Chair (6/2005-6/2008) Kevin Marvel AAS Executive Officer (6/2006-Present) Gary J. Ferland Univ. of Kentucky (6/2007-6/2008) Suzanne Hawley Univ. -
The Soft X-Ray Variability and Spectrum of 1H0419-577From A
The Soft X-ray Variability and Spectrum of 1H0419-577from a long EUVE Observation H. L. Marshall 1 Eureka Scientific, Inc., 2452 Delmer St, Suite 100, Oakland, CA, 94602 J. P. Halpern Columbia University K. Leighly Columbia University Received ; accepted 1Mailing address: 5 Whipple Rd., Lexington, MA 02173. 2 ABSTRACT The active galaxy associatedwith the hard X-ray source1H0419-577was observedwith EUVE for about 25 days to obtain a long, contiguouslight curve and an EUV spectrum. An EUV sourcewas detectedwhich was about asbright asthe AGN and was later identified asan AM Her type system(Halpern et al. 1999). The AGN showedvariations as large as a factor of two over 5-10day time scalesand occasionallyvaried by 20-30%in < 0.5day. The spectrum is dominated by a continuum that is poorly fit by a simple powerlaw. There are possibleemissionlines without positive identifications but the lines are likely to be spurious. Subject headings: quasars - Individual: LB1727 -3- 1. Introduction There were less than 10 active galactic nuclei (AGN) detected in the EUVE all-sky survey that were bright enough to be considered detected unambiguously (Marshall, Fruscione, & Carone 1995). Of these, only a few have brbad lines and are bright enough to be detected well using the EUVE spectrometer. There has been significant controversy regarding the extreme ultraviolet (EUV) spectra of the few AGN that have been observed. While there are claims of possible emission lines in some active galaxies (NGC 5548: Kaastra et al. (1995); Mrk 478 and Ton S180 Hwang, C.-Y. &: Bowyer, S. 1997), there is also evidence that the AGN spectra are dominated by continua and that any lines must very weak (Mrk 478: Marshall et al. -
Esa Cosmic Vision – “The Four Themes”
ESA COSMIC VISION –“THE FOUR THEMES” Planets and Life ‐ The Solar System ‐ Fundamental laws ‐ The UiUniverse EUROPEAN ULTRAVIOLET‐VISIBLE OBSERVATORY Thierry Appourchaux –IAS France; Martin Barstow – University of Leicester UK; Mathieu Barthelemy ‐ IPAG, France; Fréderic Baudin “Building galaxies, stars, planets –IAS, France; Stefano Benetti –OAPD‐ INAF, Italy; Pere Blay ‐ Universidad de Valencia, Spain; Noah Brosch ‐ Tel Aviv University, and the ingredients for life between Israel; Enma Bunce ‐ University of Leicester, UK; Domitilla de Martino – OAC‐INAF, Italy; Ana Ines Gomez de Castro – the stars” Universidad Complutense de Madrid, Spain; Jean‐Michel Deharveng –Observatoire Astronomique Marseille‐Provence, France; Roger Ferlet ‐ Institute d'Astrophysique de Paris, France; Kevin France ‐ University of Colorado, USA; Miriam García –IAC, Spp;ain; Boris Gaensicke ‐University of Warwick, UK; Cecile Gry ‐ Observatoire Astronomique Marseille‐Provence, France; Lynne Hillenbrand – Caltech, USA; Eric Josselin ‐ University of Montpellier, France; Carolina Kehrig – Instituto de Astrofísica de Andalucía, Spain; Laurent Lamy ‐ LESIA, France; Jon Lapington – University of Leicester, UK; Alain Lecavelier des Etangs – Institute d'Astrophysique de Paris, France; Frank LePetit – Observatoire Paris‐Meudom, France; Javier Lopez Santiago ‐ Universidad Complutense de Madrid, Spain; Bruno Milliard‐ Observatoire Astronomique Marseille‐Provence, France; Richard Monier ‐ Université de Nice, France; Giampiero Naletto – University of Padova, Italy;Yael Nazé ‐ Liège