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Calibration and performance of the photon sensor response of FACT -- The First G-APD Cherenkov telescope

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arxiv 1403.5747 v2 pith:7PEDLEJF submitted 2014-03-23 astro-ph.IM physics.ins-det

classification astro-ph.IMphysics.ins-det
keywords cherenkovperformancebeendetectorsfirstphotodemonstratingfact
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The First G-APD Cherenkov Telescope (FACT) is the first in-operation test of the performance of silicon photo detectors in Cherenkov Astronomy. For more than two years it is operated on La Palma, Canary Islands (Spain), for the purpose of long-term monitoring of astrophysical sources. For this, the performance of the photo detectors is crucial and therefore has been studied in great detail. Special care has been taken for their temperature and voltage dependence implementing a correction method to keep their properties stable. Several measurements have been carried out to monitor the performance. The measurements and their results are shown, demonstrating the stability of the gain below the percent level. The resulting stability of the whole system is discussed, nicely demonstrating that silicon photo detectors are perfectly suited for the usage in Cherenkov telescopes, especially for long-term monitoring purpose.

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Cited by 3 Pith papers

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

  1. Development and Quality Control of PMT Modules for the Large-Sized Telescopes of the Cherenkov Telescope Array Observatory

    astro-ph.IM 2025-02 conditional novelty 5.0 of 10

    All four CTAO Large-Sized Telescope cameras are now equipped with qualified seven-PMT modules that meet the observatory performance requirements, with a rejection rate below one percent during quality control.

  2. Atmospheric Cherenkov Telescopes as a Potential Veto Array for Neutrino Astronomy

    astro-ph.IM 2019-08 conditional novelty 5.0 of 10

    A roughly 250-telescope IACT veto array could reject atmospheric neutrinos above 15-30 TeV and increase IceCube event rates from overhead sources by factors of 3 to 13.

  3. Active Galactic Nuclei as high-energy neutrino sources

    astro-ph.HE 2026-06 unverdicted novelty 2.5 of 10

    Review summarizing correlations between astrophysical neutrinos and gamma-ray/radio AGN, specific source associations, proposed production mechanisms, and future prospects.

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