X/gamma-ray measurements of the faint GRB 020321

Simple item page
dc.creatorZand, J. J. M. in 't
dc.creatorKuiper, L.
dc.creatorHeise, J.
dc.creatorAmati, L.
dc.creatorCosta, E.
dc.creatorFeroci, M.
dc.creatorFrontera, F.
dc.creatorGandolfi, G.
dc.creatorNicastro, L.
dc.creatorPiro, L.
dc.creatorRodriguez-Pascual, P.
dc.creatorSantos-Lleo, M.
dc.creatorSchartel, N.
dc.date2003-05-20
dc.date.accessioned2026-07-07T02:08:32Z
dc.date.available2026-07-07T02:08:32Z
dc.descriptionGRB 020321 is a faint GRB that received wide follow-up attention in X-rays (BeppoSAX/NFI, Chandra/ACIS-S, XMM-Newton), radio (ATCA) and optical (ESO, HST). We identify a weak X-ray afterglow by a combined study of the Chandra and XMM-Newton observations. Its decay index of 1.2 is typical for GRB afterglows. Inside the 4"-accurate error box there is a weak optical counterpart candidate with a much shallower decay index.
dc.description5 pages, 3 figures, to be published in Proc. "GRBs in the afterglow era: 3rd Rome workshop (2002)", eds. L. Piro, F. Frontera, N. Masetti, M. Feroci
dc.identifierhttps://arxiv.org/abs/astro-ph/0305359
dc.identifierhttp://arxiv.org/abs/astro-ph/0305359
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6088
dc.subjectAstrophysics
dc.titleX/gamma-ray measurements of the faint GRB 020321
dc.typetext

Files

Collections

arXiv