IBIS/PICsIT Data and Analysis

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dc.creatorStephen, J. B.
dc.creatorFoschini, L.
dc.creatorGianotti, F.
dc.creatorCaroli, E.
dc.creatorMalaguti, G.
dc.creatorDi Cocco, G.
dc.creatorBassani, L.
dc.creatorCiocca, C.
dc.creatorLabanti, C.
dc.creatorMauri, A.
dc.creatorRossi, E.
dc.creatorSchiavone, F.
dc.creatorSpizzichino, A.
dc.creatorTraci, A.
dc.creatorTrifoglio, M.
dc.date2002-05-03
dc.date.accessioned2026-07-07T02:03:33Z
dc.date.available2026-07-07T02:03:33Z
dc.descriptionThe imager IBIS on board INTEGRAL is composed of two detector planes: ISGRI (15 keV - 1 MeV) and PICsIT (170 keV - 10 MeV). Here we describe the data structure of PICsIT and the instrument specific software, including the standard scientific analysis. Some examples of shadowgrams and spectra are shown, by using data collected during the End-to-End Tests of January 2002.
dc.description6 pages, 6 figures. Proceedings of the 22nd Moriond Astrophysics Meeting - The Gamma-ray Universe (Les Arcs, France, 9-16 March 2002). To be published
dc.identifierhttps://arxiv.org/abs/astro-ph/0205048
dc.identifierhttp://arxiv.org/abs/astro-ph/0205048
dc.identifierEdited by A. Goldwurm, D.N. Neumann, J. Tran Thanh Van, The Gioi Publishers, Vietnam (2002), p. 441.
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4421
dc.subjectAstrophysics
dc.titleIBIS/PICsIT Data and Analysis
dc.typetext

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