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SN 2005Cs in M51 – II
Mon. Not. R. Astron. Soc. 394, 2266–2282 (2009) doi:10.1111/j.1365-2966.2009.14505.x SN 2005cs in M51 – II. Complete evolution in the optical and the near-infrared A. Pastorello,1 S. Valenti,1 L. Zampieri,2 H. Navasardyan,2 S. Taubenberger,3 S. J. Smartt,1 A. A. Arkharov,4 O. Barnbantner,¨ 5 H. Barwig,5 S. Benetti,2 P. Birtwhistle,6 M. T. Botticella,1 E. Cappellaro,2 M. Del Principe,7 F. Di Mille,8 G. Di Rico,7 M. Dolci,7 N. Elias-Rosa,9 N. V. Efimova,4,10 M. Fiedler,11 A. Harutyunyan,2,12 P. A. Hoflich,¨ 13 W. Kloehr,14 V. M. Larionov,4,10,15 V. Lorenzi,12 J. R. Maund,16,17 N. Napoleone,18 M. Ragni,7 M. Richmond,19 C. Ries,5 S. Spiro,1,18,20 S. Temporin,21 M. Turatto22 and J. C. Wheeler17 1Astrophysics Research Centre, School of Mathematics and Physics, Queen’s University Belfast, Belfast BT7 1NN 2INAF Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, 35122 Padova, Italy 3Max-Planck-Institut fur¨ Astrophysik, Karl-Schwarzschild-Str. 1, 85741 Garching bei Munchen,¨ Germany 4Central Astronomical Observatory of Pulkovo, 196140 St Petersburg, Russia 5Universitats-Sternwarte¨ Munchen,¨ Scheinerstr. 1, 81679 Munchen,¨ Germany 6Great Shefford Observatory, Phlox Cottage, Wantage Road, Great Shefford RG17 7DA 7INAF Osservatorio Astronomico di Collurania, via M. Maggini, 64100 Teramo, Italy 8Dipartmento of Astronomia, Universita´ di Padova, Vicolo dell’Osservatorio 2, 35122 Padova, Italy 9Spitzer Science Center, California Institute of Technology, 1200 East California Blvd., Pasadena, CA 91125, USA 10Astronomical Institute of St Petersburg University, St Petersburg, Petrodvorets, Universitetsky pr. -
Distance Estimate and Progenitor Characteristics of SN 2005Cs In
Mon. Not. R. Astron. Soc. 000, 1–7 (2006) Printed 9 July 2018 (MN LATEX style file v2.2) Distance estimate and progenitor characteristics of SN 2005cs in M51 K. Tak´ats1⋆ and J. Vink´o1† 1Department of Optics and Quantum Electronics, University of Szeged, D´om t´er 9., Szeged, Hungary Accepted; Received; in original form ABSTRACT Distance to the Whirlpool Galaxy (M51, NGC 5194) is estimated using published pho- tometry and spectroscopy of the Type II-P supernova SN 2005cs. Both the Expanding Photosphere Method (EPM) and the Standard Candle Method (SCM), suitable for SNe II-P, were applied. The average distance (7.1 ± 1.2 Mpc) is in good agreement with earlier SBF- and PNLF-based distances, but slightly longer than the distance obtained by Baron et al. (1996) for SN 1994I via the Spectral Fitting Expanding At- mosphere Method (SEAM). Since SN 2005cs exhibited low expansion velocity during the plateau phase, similarly to SN 1999br, the constants of SCM were re-calibrated including the data of SN 2005cs as well. The new relation is better constrained in the −1 low velocity regime (vph(50) ∼ 1500−2000km s ), that may result in better distance estimates for such SNe. The physical parameters of SN 2005cs and its progenitor is re-evaluated based on the updated distance. All the available data support the low- mass (∼ 9 M⊙) progenitor scenario proposed previously by its direct detection with the Hubble Space Telescope (Maund et al. 2005; Li et al. 2006). Key words: stars: evolution – supernovae: individual (SN 2005cs) – galaxies: indi- vidual (M51) 1 INTRODUCTION Both teams have detected the possible progenitor, but only in the I band, which led to the conclusion that the progeni- The Type II-P SN 2005cs in M51 was discovered by Kloehr arXiv:astro-ph/0608430v1 21 Aug 2006 tor was probably a red giant. -
Find Your Telescope. Your Find Find Yourself
FIND YOUR TELESCOPE. FIND YOURSELF. FIND ® 2008 PRODUCT CATALOG WWW.MEADE.COM TABLE OF CONTENTS TELESCOPE SECTIONS ETX ® Series 2 LightBridge ™ (Truss-Tube Dobsonians) 20 LXD75 ™ Series 30 LX90-ACF ™ Series 50 LX200-ACF ™ Series 62 LX400-ACF ™ Series 78 Max Mount™ 88 Series 5000 ™ ED APO Refractors 100 A and DS-2000 Series 108 EXHIBITS 1 - AutoStar® 13 2 - AutoAlign ™ with SmartFinder™ 15 3 - Optical Systems 45 FIND YOUR TELESCOPE. 4 - Aperture 57 5 - UHTC™ 68 FIND YOURSEL F. 6 - Slew Speed 69 7 - AutoStar® II 86 8 - Oversized Primary Mirrors 87 9 - Advanced Pointing and Tracking 92 10 - Electronic Focus and Collimation 93 ACCESSORIES Imagers (LPI,™ DSI, DSI II) 116 Series 5000 ™ Eyepieces 130 Series 4000 ™ Eyepieces 132 Series 4000 ™ Filters 134 Accessory Kits 136 Imaging Accessories 138 Miscellaneous Accessories 140 Meade Optical Advantage 128 Meade 4M Community 124 Astrophotography Index/Information 145 ©2007 MEADE INSTRUMENTS CORPORATION .01 RECRUIT .02 ENTHUSIAST .03 HOT ShOT .04 FANatIC Starting out right Going big on a budget Budding astrophotographer Going deeper .05 MASTER .06 GURU .07 SPECIALIST .08 ECONOMIST Expert astronomer Dedicated astronomer Wide field views & images On a budget F IND Y OURSEL F F IND YOUR TELESCOPE ® ™ ™ .01 ETX .02 LIGHTBRIDGE™ .03 LXD75 .04 LX90-ACF PG. 2-19 PG. 20-29 PG.30-43 PG. 50-61 ™ ™ ™ .05 LX200-ACF .06 LX400-ACF .07 SERIES 5000™ ED APO .08 A/DS-2000 SERIES PG. 78-99 PG. 100-105 PG. 108-115 PG. 62-76 F IND Y OURSEL F Astronomy is for everyone. That’s not to say everyone will become a serious comet hunter or astrophotographer. -
Direct Identification of Core-‐Collapse SN Progenitors
Direct Identification of Core-Collapse SN Progenitors Schuyler D. Van Dyk (IPAC/Caltech) Main collaborators: Nancy Elias –Rosa, Alex Filippenko, Weidong Li Core-Collapse SNe: Classification Thermonuclear SNe Core Collapse SNe NO Hydrogen Hydrogen NO II/Ib Si II lines hybrid Light curve differences Si II lines Linear Plateau Ia He IIb II-L II-P NO YES H lines Narrow disappear H lines dominate in ~few IIn at all epochs Ic Ib weeks, reappear in nebular (hypernovae, phase Envelope Stripping (adapted froM Ic-bl, SN-GRB) Turatto 2003) Progenitor ID Paucity2 Core-Collapse SNe: Classification 56Ni/56Co decay (Van Dyk & Matheson 2012) Mass of 56Ni depends on Mass of core 3 Core-Collapse SNe: Classification SN II-L 2009kr in NGC 1832 (Elias-Rosa et al. 2010) 4 Core-Collapse SNe: Classification SN IIb 2008ax in NGC 4490 SN IIb 1993J in M81 (Chornock et al. 2011) (Richmond et al. 1996) 5 Core-Collapse SNe: Rates Li et al. (2010) Lick Observatory SN Search 6 Direct Identification of SN Progenitors SN 1978K (IIn) SN 2008bk (II-P) SN 1987A (II pec) SN 2008cn (II-P ?) SN 1993J (IIb) SN 2009hd (II-L ?) SN 1999ev (II-P) SN 2009kr (II-L) SN 2003gd (II-P) SN 2009md (II-P) SN 2004A (II-P) SN 2010jl (IIn) ? SN 2004et (II-P) SN 2011dh (IIb) SN 2005cs (II-P) SN 2012A (II-P) SN 2005gl (IIn) SN 2012aw (II-P) SN 2008ax (IIb) 7 SN II-P Progenitors The Most coMMon core-collapse SNe high-lum II-P “normal” II-P low-lum II-P Inserra et al. -
A Comparative Study of Type II-P and II-L Supernova Rise Times As Exemplified by the Case of Lsq13cuw⋆
A&A 582, A3 (2015) Astronomy DOI: 10.1051/0004-6361/201525868 & c ESO 2015 Astrophysics A comparative study of Type II-P and II-L supernova rise times as exemplified by the case of LSQ13cuw E. E. E. Gall1,J.Polshaw1,R.Kotak1, A. Jerkstrand1, B. Leibundgut2, D. Rabinowitz3, J. Sollerman5, M. Sullivan6, S. J. Smartt1, J. P. Anderson7, S. Benetti8,C.Baltay9,U.Feindt10,11, M. Fraser4, S. González-Gaitán12,13 ,C.Inserra1, K. Maguire2, R. McKinnon9,S.Valenti14,15, and D. Young1 1 Astrophysics Research Centre, School of Mathematics and Physics, Queen’s University Belfast, Belfast BT7 1NN, UK e-mail: [email protected] 2 ESO, Karl-Schwarzschild-Strasse 2, 85748 Garching, Germany 3 Center for Astronomy and Astrophysics, Yale University, New Haven, CT 06520, USA 4 Institute of Astronomy, University of Cambridge, Madingley Road, Cambridge, CB3 0HA, UK 5 Department of Astronomy, The Oskar Klein Centre, Stockholm University, AlbaNova, 10691 Stockholm, Sweden 6 School of Physics and Astronomy, University of Southampton, Southampton, SO17 1BJ, UK 7 European Southern Observatory, Alonso de Cordova 3107, Vitacura, Casilla 19001, Santiago, Chile 8 INAF Osservatorio Astronomico di Padova, Vicolo dell’Osservatorio 5, 35122 Padova, Italy 9 Department of Physics, Yale University, New Haven, CT 06250-8121, USA 10 Institut für Physik, Humboldt-Universität zu Berlin, Newtonstr. 15, 12489 Berlin, Germany 11 Physikalisches Institut, Universität Bonn, Nußallee 12, 53115 Bonn, Germany 12 Millennium Institute of Astrophysics, Casilla 36-D, Santiago, Chile 13 Departamento -
HET Publication Report HET Board Meeting 3/4 December 2020 Zoom Land
HET Publication Report HET Board Meeting 3/4 December 2020 Zoom Land 1 Executive Summary • There are now 420 peer-reviewed HET publications – Fifteen papers published in 2019 – As of 27 November, nineteen published papers in 2020 • HET papers have 29363 citations – Average of 70, median of 39 citations per paper – H-number of 90 – 81 papers have ≥ 100 citations; 175 have ≥ 50 cites • Wide angle surveys account for 26% of papers and 35% of citations. • Synoptic (e.g., planet searches) and Target of Opportunity (e.g., supernovae and γ-ray bursts) programs have produced 47% of the papers and 47% of the citations, respectively. • Listing of the HET papers (with ADS links) is given at http://personal.psu.edu/dps7/hetpapers.html 2 HET Program Classification Code TypeofProgram Examples 1 ToO Supernovae,Gamma-rayBursts 2 Synoptic Exoplanets,EclipsingBinaries 3 OneorTwoObjects HaloofNGC821 4 Narrow-angle HDF,VirgoCluster 5 Wide-angle BlazarSurvey 6 HETTechnical HETQueue 7 HETDEXTheory DarkEnergywithBAO 8 Other HETOptics Programs also broken down into “Dark Time”, “Light Time”, and “Other”. 3 Peer-reviewed Publications • There are now 420 journal papers that either use HET data or (nine cases) use the HET as the motivation for the paper (e.g., technical papers, theoretical studies). • Except for 2005, approximately 22 HET papers were published each year since 2002 through the shutdown. A record 44 papers were published in 2012. • In 2020 a total of fifteen HET papers appeared; nineteen have been published to date in 2020. • Each HET partner has published at least 14 papers using HET data. • Nineteen papers have been published from NOAO time. -
SN 2005Cs and SN 2006Bp
Using Quantitative Spectroscopic Analysis to Determine the Properties and Distances of Type II Plateau Supernovae: SN 2005cs and SN 2006bp The Harvard community has made this article openly available. Please share how this access benefits you. Your story matters Citation Dessart, Luc, Stéphane Blondin, Peter J. Brown, Malcolm Hicken, D. John Hillier, Stephen T. Holland, Stefan Immler, et al. 2008. “Using Quantitative Spectroscopic Analysis to Determine the Properties and Distances of Type II Plateau Supernovae: SN 2005cs and SN 2006bp.” The Astrophysical Journal 675 (1): 644–69. https:// doi.org/10.1086/526451. Citable link http://nrs.harvard.edu/urn-3:HUL.InstRepos:41399737 Terms of Use This article was downloaded from Harvard University’s DASH repository, and is made available under the terms and conditions applicable to Open Access Policy Articles, as set forth at http:// nrs.harvard.edu/urn-3:HUL.InstRepos:dash.current.terms-of- use#OAP Draft version October 28, 2018 Preprint typeset using LATEX style emulateapj v. 10/09/06 USING QUANTITATIVE SPECTROSCOPIC ANALYSIS TO DETERMINE THE PROPERTIES AND DISTANCES OF TYPE II-PLATEAU SUPERNOVAE: SNe 2005cs AND 2006bp Luc Dessart1,2, Stephane´ Blondin3, Peter J. Brown4, Malcolm Hicken 3, D. John Hillier 5, Stephen T. Holland6,7, Stefan Immler6,7, Robert P. Kirshner3, Peter Milne1, Maryam Modjaz3, & Peter W. A. Roming4 Draft version October 28, 2018 ABSTRACT We analyze the Type II Plateau supernovae (SN II-P) 2005cs and 2006bp with the non-LTE model atmosphere code CMFGEN. We fit 13 spectra in the first month for SN 2005cs and 18 for SN 2006bp. -
Extragalactic Astronomy
Astrophysics and Space Science Library 435 Mauro D’Onofrio Roberto Rampazzo Simone Zaggia Editors From the Realm of the Nebulae to Populations of Galaxies Dialogues on a Century of Research From the Realm of the Nebulae to Populations of Galaxies Astrophysics and Space Science Library EDITORIAL BOARD Chairman W. B. BURTON, National Radio Astronomy Observatory, Charlottesville, Virginia, U.S.A. ([email protected]); University of Leiden, The Netherlands ([email protected]) F. BERTOLA, University of Padua, Italy C. J. CESARSKY, Commission for Atomic Energy, Saclay, France P. EHRENFREUND, Leiden University, The Netherlands O. ENGVOLD, University of Oslo, Norway A. HECK, Strasbourg Astronomical Observatory, France E. P. J. VAN DEN HEUVEL, University of Amsterdam, The Netherlands V. M. KASPI, McGill University, Montreal, Canada J. M. E. KUIJPERS, University of Nijmegen, The Netherlands H. VAN DER LAAN, University of Utrecht, The Netherlands P. G. MURDIN, Institute of Astronomy, Cambridge, UK B. V. SO M OV, Astronomical Institute, Moscow State University, Russia R. A. SUNYAEV, Space Research Institute, Moscow, Russia More information about this series at http://www.springer.com/series/5664 Mauro D’Onofrio • Roberto Rampazzo • Simone Zaggia Editors From the Realm of the Nebulae to Populations of Galaxies Dialogues on a Century of Research 123 Editors Mauro D’Onofrio Roberto Rampazzo Department of Physics and Astronomy INAF–Osservatorio Astronomico University of Padova di Padova Italy Padova, Italy Simone Zaggia INAF–Osservatorio Astronomico di Padova Padova, Italy ISSN 0067-0057 ISSN 2214-7985 (electronic) Astrophysics and Space Science Library ISBN 978-3-319-31004-6 ISBN 978-3-319-31006-0 (eBook) DOI 10.1007/978-3-319-31006-0 Library of Congress Control Number: 2016946611 © Springer International Publishing Switzerland 2016 This work is subject to copyright. -
Dr. Lynn Cominsky Dr. Kevin Mclin SSU E/PO Group
Supernova Educator Guide Dr. Lynn Cominsky Dr. Kevin McLin SSU E/PO Group Saturday, November 1, 2008 NASA E/PO Group at SSU ~10 people working collaboratively to educate the public about current and future NASA high-energy missions. XMM-Newton Fermi Gamma-ray Space Telescope Led by Professor Lynn Cominsky Fermi and XMM • XMM-Newton • NASA/ESA X-ray telescope • Observes black holes, pulsars, AGN, etc • Launched December 20, 1999 (recently had some communication problems, but okay now). • Fermi Gamma-ray Space Telescope • First imaging gamma ray telescope • Observes black holes, pulsars, AGN, GRB, etc, but at higher energies than x-ray telescopes • Launched June 11, 2008 Image: R. Jay GeBany Find the Supernova The picture on the right shows SN 2005cs, a supernova that was discovered on June 28, 2005 in the galaxy M51. The supernova is the bright “star” just below the galaxy’s core, near the middle of the spiral arm. This figure is from a packet of materials on supernova that was developed for the Night Sky Network. It shows the star-gas cycle. On the left is a schematic of the life cycle for low mass stars (below a few times the mass of the Sun). They evolve through their hydrogen burning phase to become red giants (when they burn helium to carbon). When these stars run out of helium, they are done. They become planetary nebula and leave behind a white dwarf compact remnant. Stellar material blown of during the red giant and planetary nebula phases can be incorporated back into gas clouds, which can then form new stars. -
A 'Catchers Tale' the 'Leviathan Lord'
The ‘Leviathan Lord’ of Birr Castle The ‘Leviathan Lord’ of Birr Castle William Parsons, 3rd Earl of Rosse A ‘Catchers Tale’ Featuring Featuringthe Forgotten the Forgotten LivesLives of theof Men the and Men Women and who FirstWomen who First PhotographedPhotographed the Heavens the Heavens Stefan Hughes Contents 1. The ‘Catchers Tales’ 1 1.1 Introduction 2 1.2 Birr Castle Today 4 1.3 The ‘Great Telescope Builder’ 5 2. The Life and Work of William Parsons 6 2.1 ‘Great Telescopes’ 7 2.2 Lord Oxmantown 8 2.3 Mary Field of Heaton Hall 10 2.4 Parsonstown 17 2.5 Mirror, Mirror on the Estate... 23 2.6 The ‘Leviathan’ 30 2.7 ‘The Problem of the Nebulae’ 36 2.8 ‘Spirals’ 44 2.9 Photography at Birr 50 2.10 Homage 54 2.11 After... 58 3. Appendices 64 A: William Parsons: Family Pedigree 65 B: Mary Field: Family Pedigree 69 C: Glossary of Terms & Personalities 73 4. End Piece 80 Notes & Bibliography 81 Acknowledgements 91 Index 92 The Author 97 i 1. The ‘Catchers Tales’ Catchers of the Light William Parsons 3rd Earl of Rosse The Forgotten Lives of the Men and Women who First Photographed the Heavens Their True Tales of Adventure, Adversity & Triumph Stefan Hughes1 1.1 Introduction The ‘Catchers Tales’, each feature a single life of one of the men and women who first photographed the heavens. Their lives are ones full of adventure, adversity and triumph - which would test the abilities of even the best author or screenwriter to recreate as a work of fiction. -
2005 Astronomy Magazine Index
2005 Astronomy Magazine Index Subject index flyby of Titan, 2:72–77 Einstein, Albert, 2:30–53 Cassiopeia (constellation), 11:20 See also relativity, theory of Numbers Cassiopeia A (supernova), stellar handwritten manuscript found, 3C 58 (star remnant), pulsar in, 3:24 remains inside, 9:22 12:26 3-inch telescopes, 12:84–89 Cat's Eye Nebula, dying star in, 1:24 Einstein rings, 11:27 87 Sylvia (asteroid), two moons of, Celestron's ExploraScope telescope, Elysium Planitia (on Mars), 5:30 12:33 2:92–94 Enceladus (Saturn's moon), 11:32 2003 UB313, 10:27, 11:68–69 Cepheid luminosities, 1:72 atmosphere of water vapor, 6:22 2004, review of, 1:31–40 Chasma Boreale (on Mars), 7:28 Cassini flyby, 7:62–65, 10:32 25143 (asteroid), 11:27 chonrites, and gamma-ray bursts, 5:30 Eros (asteroid), 11:28 coins, celestial images on, 3:72–73 Eso Chasma (on Mars), 7:28 color filters, 6:67 Espenak, Fred, 2:86–89 A Comet Hale-Bopp, 7:76–79 extrasolar comets, 9:30 Aeolis (on Mars), 3:28 comets extrasolar planets Alba Patera (Martian volcano), 2:28 from beyond solar system, 12:82 first image of, 4:20, 8:26 Aldrin, Buzz, 5:40–45 dust trails of, 12:72–73 first light from, who captured, 7:30 Altair (star), 9:20 evolution of, 9:46–51 newly discovered low-mass planets, Amalthea (Jupiter's moon), 9:28 extrasolar, 9:30 1:68–71 amateur telescopes. See telescopes, Conselice, Christopher, 1:20 smallest, 9:26 amateur constellations whether have diamond layers, 5:26 Andromeda Galaxy (M31), 10:84–89 See also names of specific extraterrestrial life, 4:28–34 disk of stars surrounding, 7:28 constellations eyepieces, telescope. -
Identification of the Red Supergiant Progenitor of Supernova 2005Cs
Identification of the Red Supergiant Progenitor of Supernova 2005cs: Do the Progenitors of Type II-P Supernovae Have Low Mass? Weidong Li1, Schuyler D. Van Dyk2, Alexei V. Filippenko1, Jean-Charles Cuillandre3, Saurabh Jha1, Joshua S. Bloom1, Adam G. Riess4, & Mario Livio4 Received ; accepted arXiv:astro-ph/0507394v1 18 Jul 2005 1Department of Astronomy, University of California, Berkeley, CA 94720-3411; email (wli, alex, sjha, jbloom)@astro.berkeley.edu 2Spitzer Science Center, California Institute of Technology, Mailcode 220-6, Pasadena, CA 91125; email [email protected] 3Canada-France-Hawaii Telescope Corporation, 65-1238 Mamalahoa Hwy, Kamuela, HI 96743; email [email protected] 4Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218; email (ariess, mlivio)@stsci.edu –2– ABSTRACT The stars that end their lives as supernovae (SNe) have been directly observed in only a handful of cases, due mainly to the extreme difficulty in identifying them in images obtained prior to the SN explosions. Here we report the identification of the progenitor for the recent Type II-plateau (core-collapse) SN 2005cs in pre-explosion archival images of the Whirlpool Galaxy (M51) obtained with the Hubble Space Telescope (HST) Advanced Camera for Surveys (ACS). From high-quality ground-based images of the SN from the Canada-France-Hawaii Telescope, we precisely determine the position of the SN and are able to isolate the SN progenitor to within 0′′.04 in the HST ACS optical images. We further pinpoint the SN location to within 0′′.005 from HST ACS ultraviolet images of the SN, confirming our progenitor identification.