Free access article
A&A 411, L71-L79 (2003)
DOI: 10.1051/0004-6361:20031302
Letter
INTEGRAL/SPI ground calibration
D. Attié1, B. Cordier1, M. Gros1, Ph. Laurent1, S. Schanne1, G. Tauzin1, P. von Ballmoos2, L. Bouchet2, P. Jean2, J. Knödlseder2, P. Mandrou2, Ph. Paul2, J.-P. Roques2, G. Skinner2, G. Vedrenne2, R. Georgii3, A. von Kienlin3, G. Lichti3, V. Schönfelder3, A. Strong3, C. Wunderer3, C. Shrader4, S. Sturner4, B. Teegarden4, G. Weidenspointner4, J. Kiener5, M.-G. Porquet5, V. Tatischeff5, S. Crespin6, S. Joly6, Y. André7, F. Sanchez8 and P. Leleux91 DSM/DAPNIA/Service d'Astrophysique, CEA Saclay, 91191 Gif-sur-Yvette, France,
2 Centre d'Études Spatiales des Rayonnements, 9 avenue du Colonel Roche, 31028 Toulouse, France
3 Max-Planck-Institut für extraterrestrische Physik, Giessenbachstraße, 85748 Garching, Germany
4 NASA/Goddard Space Flight Center, code 661, Greenbelt, MD 20771, USA
5 Centre de Spectrométrie Nucléaire et de Spectrométrie de Masse, IN2P3-CNRS, 91405 Orsay Campus, France
6 CEA Bruyères-le-Châtel, BP 12, 91680 Bruyères-le-Châtel, France
7 CNES/Centre Spatial de Toulouse, 18 avenue E. Belin, 31401 Toulouse, France
8 Universitat de Valencia, IFIC, Dr Moliner 50, 46100 Burjassot, Valencia, Spain
9 Univ. of Louvain, chemin du Cyclotron, 1348 Louvain-La-Neuve, Belgium
(Received 14 July 2003 / Accepted 26 August 2003)
Abstract
Three calibration campaigns of the spectrometer SPI have
been performed before launch in order to determine the instrument
characteristics, such as the effective detection area, the
spectral resolution and the angular resolution. Absolute
determination of the effective area has been obtained from
simulations and measurements. At 1 MeV, the effective area is 65 cm
2 for a point source on the optical axis, the spectral
resolution ~2.3 keV. The angular resolution is better than
2.5° and the source separation capability about 1°. Some
temperature dependant parameters will require permanent in-flight
calibration.
Key words: instrumentation: detectors -- instrumentation: spectrographs -- space vehicles: instruments -- gamma rays: observations
Offprint request: D. Attié, David.Attie@cea.fr
© ESO 2003



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