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IBIS/PICsIT in-flight performances

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arxiv astro-ph/0309224 v1 pith:FMMGHQIT submitted 2003-09-08 astro-ph

classification astro-ph
keywords picsitenergyarcminibisimagingin-flighton-boardperformances
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PICsIT (Pixellated Imaging CaeSium Iodide Telescope) is the high energy detector of the IBIS telescope on-board the INTEGRAL satellite. PICsIT operates in the gamma-ray energy range between 175 keV and 10 MeV, with a typical energy resolution of 10% at 1 MeV, and an angular resolution of 12 arcmin within a \~100 square degree field of view, with the possibility to locate intense point sources in the MeV region at the few arcmin level. PICsIT is based upon a modular array of 4096 independent CsI(Tl) pixels, ~0.70 cm^2 in cross-section and 3 cm thick. In this work, the PICsIT on-board data handling and science operative modes are described. This work presents the in-flight performances in terms of background count spectra, sensitivity limit, and imaging capabilities.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Probing Heavy Axion-like Particles from Massive Stars with X-rays and Gamma Rays

    hep-ph 2024-12 conditional novelty 5.0 of 10

    Decay photons from heavy ALPs produced in Wolf-Rayet stars can be probed by INTEGRAL SPI down to gaγ ~ 4e-11 GeV^-1 for ma ~ 10-100 keV, modestly extending existing limits.

  2. Hard X-ray and gamma-ray detectors

    astro-ph.IM 2024-11 unverdicted

    A review chapter surveying detector technologies and telescope configurations for hard X-ray and gamma-ray space astronomy, with no new experimental or theoretical results.

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