The SPI spectrometer on INTEGRAL features a camera system with 19 Ge detector modules, imaging photons through a tungsten coded mask. Background is reduced by an anticoincidence detector system surrounding these. The specifics of this instrument lead to data correction and analysis methods which are described here. Raw data for science analysis are detector event messages and spectra for different categories of detector hits and pulse shapes. Preprocessing combines calibrated spectra from these, which are then interpreted using the imaging and spectral response function for measured spectra where parts of the detector plane are occulted by the mask. Background dominates the overall signal, tailored background estimates and models a...
International audienceContext. The INTEGRAL/SPI, X/γ-ray spectrometer (20 keV–8 MeV) is an instrumen...
The International Gamma-ray Astrophysics Laboratory (INTEGRAL) is conceived as the next logical step...
SPI, the Spectrometer on board the ESA INTEGRAL satellite, to be launched in October 2002, will stud...
SPI is a high spectral resolution gamma-ray telescope on board the ESA mission INTEGRAL (Internatio...
Context. The coded-mask spectrometer-telescope SPI on board the INTErnational Gamma-Ray Astrophysics...
Context. The space based γ-ray observatory INTEGRAL of the European Space Agency (ESA) includes the ...
INTEGRAL's main instruments employ coded apertures to obtain directional information on the incomin...
A key tool in the package of software available for the analysis of data from the SPI spectrometer o...
International audienceContext. The space based γ-ray observatory INTEGRAL of the European Space Agen...
Context. The INTEGRAL/SPI, X/γ-ray spectrometer (20 keV–8 MeV) is an instrument for which recovering...
In its space environment the INTEGRAL observatory is subject to an intense irradiation by energetic ...
International audienceContext. The INTEGRAL/SPI, X/γ-ray spectrometer (20 keV–8 MeV) is an instrumen...
The International Gamma-ray Astrophysics Laboratory (INTEGRAL) is conceived as the next logical step...
SPI, the Spectrometer on board the ESA INTEGRAL satellite, to be launched in October 2002, will stud...
SPI is a high spectral resolution gamma-ray telescope on board the ESA mission INTEGRAL (Internatio...
Context. The coded-mask spectrometer-telescope SPI on board the INTErnational Gamma-Ray Astrophysics...
Context. The space based γ-ray observatory INTEGRAL of the European Space Agency (ESA) includes the ...
INTEGRAL's main instruments employ coded apertures to obtain directional information on the incomin...
A key tool in the package of software available for the analysis of data from the SPI spectrometer o...
International audienceContext. The space based γ-ray observatory INTEGRAL of the European Space Agen...
Context. The INTEGRAL/SPI, X/γ-ray spectrometer (20 keV–8 MeV) is an instrument for which recovering...
In its space environment the INTEGRAL observatory is subject to an intense irradiation by energetic ...
International audienceContext. The INTEGRAL/SPI, X/γ-ray spectrometer (20 keV–8 MeV) is an instrumen...
The International Gamma-ray Astrophysics Laboratory (INTEGRAL) is conceived as the next logical step...
SPI, the Spectrometer on board the ESA INTEGRAL satellite, to be launched in October 2002, will stud...