The broad-lined Type Ic supernova 2003jd

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dc.contributor.authorValenti, S
dc.contributor.authorBenetti, Stefano
dc.contributor.authorCappellaro, Enrico
dc.contributor.authorPatat, Ferdinando
dc.contributor.authorMazzali, Paolo A
dc.contributor.authorTuratto, Massimo
dc.contributor.authorHurley, K C
dc.contributor.authorMaeda, Keiichi
dc.contributor.authorGal-Yam, Avishay
dc.contributor.authorFoley, Ryan
dc.contributor.authorFilippenko, Alexei
dc.contributor.authorSalvo, Maria
dc.contributor.authorSchmidt, Brian
dc.date.accessioned2015-12-08T22:44:56Z
dc.date.issued2008
dc.date.updated2015-12-08T10:49:21Z
dc.description.abstractThe results of a worldwide coordinated observational campaign on the broad-lined Type Ic supernova (SN Ic) 2003jd are presented. In total, 74 photometric data points and 26 spectra were collected using 11 different telescopes. SN 2003jd is one of the most luminous SN Ic ever observed. A comparison with other Type Ic supernovae (SNe Ic) confirms that SN 2003jd represents an intermediate case between broad-line events (2002ap, 2006aj) and highly energetic SNe (1997ef, 1998bw, 2003dh, 2003lw), with an ejected mass of Mej = 3.0 ± 1 M⊙ and a kinetic energy of Ek(tot) = 7+3-2 × 1051 erg. SN 2003jd is similar to SN 1998bw in terms of overall luminosity, but it is closer to SNe 2006aj and 2002ap in terms of light-curve shape and spectral evolution. The comparison with other SNe Ic suggests that the V-band light curves of SNe Ic can be partially homogenized by introducing a time-stretch factor. Finally, because of the similarity of SN 2003jd to the SN 2006aj/XRF 060218 event, we discuss the possible connection of SN 2003jd with a gamma-ray burst (GRB). Journal compilation
dc.description.sponsorshipThis work was supported by grant no. 2006022731 of the PRIN of Italian Ministry of University and Sci. Research. AG-Y acknowledges partial support by NASA through Hubble Fellowship grant HST-HF-01158.01-A awarded by STScI, which is operated by AURA, Inc., for NASA, under contract NAS 5-26555. AVF’s group at the University of California, Berkeley, is supported by National Science Foundation (NSF) grant AST-0607485 and by the TABASGO Foundation. KAIT was made possible by generous donations from Sun Microsystems, Inc., the Hewlett-Packard Company, AutoScope Corporation, Lick Observatory, the NSF, the University of California and the Sylvia & Jim Katzman Foundation. KH is grateful for IPN support under the following grants and contracts: JPL 958056 (Ulysses), MIT SC-A-293291 (HETE), NAG5-13080 (RHESSI), NAG5-12614 (INTEGRAL) and NAG5-11451 (HETE and Mars Odyssey).
dc.format16 pages
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/1885/37619
dc.provenancehttp://www.sherpa.ac.uk/romeo/issn/0035-8711/ Author can archive publisher's version/PDF. Publisher's version/PDF on Institutional repositories or Central repositories, with all rights reserved (Sherpa/Romeo as of 16/10/2018).
dc.publisherBlackwell Publishing Ltd
dc.rights© 2007 The Authors. Journal compilation. © 2007 RAS. https://academic.oup.com/journals/pages/access_purchase/rights_and_permissions/self_archiving_policy_p This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2007 S. Valenti S. Benetti E. Cappellaro F. Patat P. Mazzali M. Turatto K. Hurley K. Maeda A. Gal-Yam R. J. Foley A. V. Filippenko A. Pastorello P. Challis F. Frontera A. Harutyunyan M. Iye K. Kawabata R. P. Kirshner W. Li Y. M. Lipkin T. Matheson K. Nomoto E. O. Ofek Y. Ohyama E. Pian D. Poznanski M. Salvo D. N. Sauer B. P. Schmidt A. Soderberg L. Zampieri. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. (Publisher journal website as of 16/10/2018)
dc.sourceMonthly Notices of the Royal Astronomical Society
dc.subjectKeywords: Supernovae: general; Supernovae: individual: 1996aq; Supernovae: individual: 2003jd
dc.titleThe broad-lined Type Ic supernova 2003jd
dc.typeJournal article
dcterms.accessRightsOpen Access
local.bibliographicCitation.issue4
local.bibliographicCitation.lastpage1500
local.bibliographicCitation.startpage1485
local.contributor.affiliationValenti, S, INAF-Osservatorio Astronomico di Capadimonte
local.contributor.affiliationBenetti, Stefano, INAF-Osservatorio Astronomico di Padova
local.contributor.affiliationCappellaro, Enrico, INAF Osservatorio Astronomico di Padova,
local.contributor.affiliationPatat, Ferdinando, European Southern Observatory
local.contributor.affiliationMazzali, Paolo A, INAF-Osservatorio Astronomico di Trieste
local.contributor.affiliationTuratto, Massimo, INAF-Osservatorio Astronomico di Padova
local.contributor.affiliationHurley, K C, University of California
local.contributor.affiliationMaeda, Keiichi, University of Tokyo
local.contributor.affiliationGal-Yam, Avishay, California Institute of Technology
local.contributor.affiliationFoley, Ryan, University of California
local.contributor.affiliationFilippenko, Alexei, University of California
local.contributor.affiliationSalvo, Maria, College of Physical and Mathematical Sciences, The Australian National University
local.contributor.affiliationSchmidt, Brian, College of Physical and Mathematical Sciences, The Australian National University
local.contributor.authoremailu9500253@anu.edu.au
local.contributor.authoruidSalvo, Maria, u3925878
local.contributor.authoruidSchmidt, Brian, u9500253
local.description.notesImported from ARIES
local.identifier.absfor020103 - Cosmology and Extragalactic Astronomy
local.identifier.ariespublicationu4362859xPUB151
local.identifier.citationvolume383
local.identifier.doi10.1111/j.1365-2966.2007.12647.x
local.identifier.essn1365-2966
local.identifier.scopusID2-s2.0-38349140082
local.identifier.thomsonID000252446900017
local.identifier.uidSubmittedByu4362859
local.type.statusPublished Version

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