Gamma-Ray Burst Detection with INTEGRAL/SPI

Simple item page
dc.creatorvon Kienlin, Andreas
dc.creatorArend, Nikolas
dc.creatorLichti, Giselher
dc.creatorStrong, Andrew
dc.creatorConnell, Paul
dc.date2004-07-05
dc.date.accessioned2026-07-07T02:13:44Z
dc.date.available2026-07-07T02:13:44Z
dc.descriptionThe spectrometer SPI, one of the two main instruments of the INTEGRAL spacecraft, has strong capabilities in the field of Gamma-Ray Burst (GRB) detections. In its 16 deg field of view (FoV) SPI is able to trigger and to localize GRBs with an accuracy for strong bursts better than 1 deg. The expected GRB detection rate is about one per month.
dc.description4 pages, 1 figure, to appear in "Gamma-ray bursts in the afterglow era", 3rd workshop, Rome 17-20 Sept. 2002
dc.identifierhttps://arxiv.org/abs/astro-ph/0407082
dc.identifierhttp://arxiv.org/abs/astro-ph/0407082
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/7912
dc.subjectAstrophysics
dc.titleGamma-Ray Burst Detection with INTEGRAL/SPI
dc.typetext

Files

Collections

arXiv