2001/01/08 by D. Gotz, Dario Götz, D. I. Cremonesi +4
Physics and Astronomy · #Astronomy and Astrophysical Research #Astrophysics (astro-ph) #FOS: Physical sciences #Particle Detector Development and Performance #Superconducting and THz Device Technology #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0101099
4 pages, latex, 8 figures, Paper presented at the 4th INTEGRAL Workshop, Alicante 4-8 September 2000, to be published by ESA-SP
arxiv created 2001/01/08 · openalex publication_date 2001/01/08 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We have used the IBIS Simulator to produce preliminary response matrices for the ISGRI and PICsIT detectors in order to help understanding their scientific performances before the calibration results are available. The derived matrices, in a format compatible with the XSPEC spectral analysis package, have been tested by fitting simple models and then used to analyze simulations of astrophysical sources with more complex spectra.