SN 2002lt and GRB 021211: a SN/GRB Connection at z = 1

Simple item page
dc.creatorDella Valle, M.
dc.creatorMalesani, D.
dc.creatorBenetti, S.
dc.creatorTesta, V.
dc.creatorHamuy, M.
dc.creatorAntonelli, L. A.
dc.creatorChincarini, G.
dc.creatorCocozza, G.
dc.creatorCovino, S.
dc.creatorD'Avanzo, P.
dc.creatorFugazza, D.
dc.creatorGhisellini, G.
dc.creatorGilmozzi, R.
dc.creatorLazzati, D.
dc.creatorMason, E.
dc.creatorMazzali, P.
dc.creatorStella, L.
dc.date2003-12-10
dc.date.accessioned2026-07-07T10:27:09Z
dc.date.available2026-07-07T10:27:09Z
dc.descriptionWe present spectroscopic and photometric observations of the afterglow of GRB 021211 and the discovery of its associated supernova, SN 2002lt. The spectrum shows a broad feature (FWHM = 150 A), around 3770 A (in the rest-frame of the GRB), which we interpret as Ca H+K blueshifted by 14400 km/s. Potential sources of contamination due to the host galaxy and/or residuals of telluric absorption have been analyzed and ruled out. Overall, the spectrum shows a suggestive resemblance with the one of the prototypical type-Ic SN 1994I. This might indicate that GRBs are produced also by standard type-Ic supernovae.
dc.description6 pages, 5 color figures. Proceedings of the 2003 GRB Conference (Santa Fe, NM, 2003 Sep 8-12). Needs aipprocs LaTeX class
dc.identifierhttps://arxiv.org/abs/astro-ph/0312264
dc.identifierhttp://arxiv.org/abs/astro-ph/0312264
dc.identifierAIPConf.Proc.727:403-407,2004
dc.identifierdoi:10.1063/1.1810874
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/177068
dc.subjectAstrophysics
dc.titleSN 2002lt and GRB 021211: a SN/GRB Connection at z = 1
dc.typetext

Files

Collections

arXiv