SPI instrumental background characteristics
Boggs, S.; Knödlseder, J.; von Kienlin, A.; Schanne, S.; Cordier, B.; Schönfelder, V.; Diehl, R.; Mandrou, P.; Teegarden, B. J.; Jean, P.; Lonjou, V.; von Ballmoos, P.; Lichti, G. G.; Roques, J. P.; Kalemci, E.; Caraveo, P.; Kiener, J.; Weidenspointner, G.; Vedrenne, G.; Attié, D.; Skinner, G. K.; Gros, M.; Wunderer, C.; Paul, Ph.; Leleux, P.
France, Germany, United States, Italy, Belgium
Abstract
In its space environment the INTEGRAL observatory is subject to an intense irradiation by energetic cosmic-ray particles that leads, via nuclear interactions with the telescope and spacecraft materials, to an important background of false events. In this paper we present the characteristics of the instrumental background that is observed in the spectrometer SPI (SPectrometer of INTEGRAL). We explain the tuning that has been performed on the parameters of the anticoincidence system in order to optimise the telescope sensitivity over the full energy range. Temporal variations of the instrumental background are discussed and methods are proposed that allow for their modelling in first order.
Based on observations with INTEGRAL, an ESA project with instruments and science data centre funded by ESA member states (especially the PI countries: Denmark, France, Germany, Italy, Switzerland, Spain), Czech Republic and Poland, and with the participation of Russia and the USA.