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SPI: The spectrometer aboard INTEGRAL

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SPI: The spectrometer aboard INTEGRAL

dc.contributor.author	Vedrenne, G.
dc.contributor.author	Roques, J. P.
dc.contributor.author	Schönfelder, V.
dc.contributor.author	Mandrou, P.
dc.contributor.author	Lichti, G.
dc.contributor.author	von Kienlin, A.
dc.contributor.author	Cordier, B.
dc.contributor.author	Schanne, S.
dc.contributor.author	Knödlseder, J.
dc.contributor.author	Skinner, G.
dc.contributor.author	Jean, P.
dc.contributor.author	Sánchez Martínez, Filomeno
dc.contributor.author	Caraveo, P.
dc.contributor.author	Teegarden, B.
dc.contributor.author	von Ballmoos, P.
dc.contributor.author	Bouchet, L.
dc.contributor.author	Paul, P.
dc.contributor.author	Matteson, J.
dc.contributor.author	Boggs, S.
dc.contributor.author	Wunderer, C.
dc.contributor.author	Leleux, P.
dc.contributor.author	Weidenspointner, G.
dc.contributor.author	Durouchoux, Ph.
dc.contributor.author	Diehl, R.
dc.contributor.author	Strong, A.
dc.contributor.author	Cassé, M.
dc.contributor.author	Clair, M. A.
dc.contributor.author	André, Y.
dc.date.accessioned	2010-07-13T08:14:22Z
dc.date.available	2010-07-13T08:14:22Z
dc.date.issued	2003
dc.identifier.citation	VEDRENNE, G. ; Vedrenne, G. ; Roques, J.-P ; Schönfelder, V. ; Mandrou, P. ; Lichti, G.G. ; von Kienlin, A. ; Cordier, B. ; Schanne, S. ; Knödlseder, J. ; Skinner, G. ; Jean, P. ; Sanchez Martinez, Filomeno ; Caraveo, P. ; Teegarden, B. ; von Ballmoos, P. ; Bouchet, L. ; Paul, P. ; Matteson, J. ; Boggs, S. ; Wunderer, C. ; Leleux, P. ; Weidenspointner, G. ; Durouchoux, Ph. ; Diehl, R. ; Strong, A. ; Cassé, M. ; Clair, M.A. ; André, Y., 2003, SPI: The spectrometer aboard INTEGRAL, Astronomy and Astrophysics, vol. 411, no. 1, p. L63-L70	en
dc.identifier.uri	http://hdl.handle.net/10550/16002
dc.description.abstract	SPI is a high spectral resolution gamma-ray telescope on board the ESA mission INTEGRAL (International Gamma Ray Astrophysics Laboratory). It consists of an array of 19 closely packed germanium detectors surrounded by an active anticoincidence shield of BGO. The imaging capabilities of the instrument are obtained with a tungsten coded aperture mask located 1.7 m from the Ge array. The fully coded field-of-view is 16º, the partially coded field of view amounts to 31º, and the angular resolution is 2.5º. The energy range extends from 20 keV to 8 MeV with a typical energy resolution of 2.5 keV at 1.3 MeV. Here we present the general concept of the instrument followed by a brief description of each of the main subsystems. INTEGRAL was successfully launched in October 2002 and SPI is functioning extremely well.	en
dc.language.iso	en	en
dc.subject	Detector ; Spectrograph ; Techniques ; Spectroscopic	en
dc.title	SPI: The spectrometer aboard INTEGRAL	en
dc.type	journal article	es_ES
dc.subject.unesco	UNESCO::ASTRONOMÍA Y ASTROFÍSICA	en
dc.subject.unesco	UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Astronomía óptica	en
dc.identifier.doi	10.1051/0004-6361:20031482	en
dc.type.hasVersion	VoR	es_ES
dc.identifier.url	http://www.aanda.org/articles/aa/pdf/2003/43/aaINTEGRAL67.pdf	en