SPI energy calibration

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dc.creatorLonjou, V.
dc.creatorKnodlseder, J.
dc.creatorRoques, J. P.
dc.creatorSkinner, G. K.
dc.creatorvon Ballmoos, P.
dc.creatorJean, P.
dc.creatorPaul, P.
dc.creatorWeidenspointner, G.
dc.creatorWunderer, C.
dc.creatorSchanne, S.
dc.date2005-04-14
dc.date.accessioned2026-07-07T02:17:27Z
dc.date.available2026-07-07T02:17:27Z
dc.descriptionThe status of the SPI energy calibration after the first year of INTEGRAL operations is reported. We have studied the gain variations and we have demonstrated that the most important parameter is the germanium detector temperature. This study permits us to determine the limits of our calibration method and the frequency of calibrations needed.
dc.description3 pages, 7 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0504325
dc.identifierhttp://arxiv.org/abs/astro-ph/0504325
dc.identifierProc. 5th INTEGRAL Workshop, ESA SP-552, 713, 2004
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9179
dc.subjectAstrophysics
dc.titleSPI energy calibration
dc.typetext

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