Calibration and Performance Validation of the SST-1M Telescopes Using Crab Nebula Observations

SST-1M is a prototype single mirror Small Sized Cherenkov Telescope designed for very high energy (VHE) gamma-ray astronomy. With a 4 meter primary mirror and a 5.6 meter focal length, it provides a wide 9 degree optical field of view, optimized for detecting VHE gamma-rays from 1 TeV to several hundred TeV. Its focal plane is equipped with DigiCam, a fully digital trigger and readout camera made of 1296 silicon photomultiplier (SiPM) pixels. The use of SiPM sensors enables observation under high night sky background (NSB) conditions, significantly enhancing the instrument's duty cycle and allowing observations under moonlight. Currently, two SST-1M telescopes are deployed at the Ondřejov Observatory in the Czech Republic, operating in stereo, at 510 m altitude, to observe astrophysical sources. This contribution presents the SiPM calibration procedure and performance validation of the instrument, based on updated results from Crab Nebula observations.

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Publication Details

Published
2025-09-24
DOI
https://doi.org/10.22323/1.501.0861
Primary Topic
Adaptive optics and wavefront sensing
Type
article
Field-Weighted Citation Impact
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Calibration and Performance Validation of the SST-1M Telescopes Using Crab Nebula Observations

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Adaptive optics and wavefront sensing
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Calibration and Performance Validation of the SST-1M Telescopes Using Crab Nebula Observations

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article en

Abstract

SST-1M is a prototype single mirror Small Sized Cherenkov Telescope designed for very high energy (VHE) gamma-ray astronomy. With a 4 meter primary mirror and a 5.6 meter focal length, it provides a wide 9 degree optical field of view, optimized for detecting VHE gamma-rays from 1 TeV to several hundred TeV. Its focal plane is equipped with DigiCam, a fully digital trigger and readout camera made of 1296 silicon photomultiplier (SiPM) pixels. The use of SiPM sensors enables observation under high night sky background (NSB) conditions, significantly enhancing the instrument's duty cycle and allowing observations under moonlight. Currently, two SST-1M telescopes are deployed at the Ondřejov Observatory in the Czech Republic, operating in stereo, at 510 m altitude, to observe astrophysical sources. This contribution presents the SiPM calibration procedure and performance validation of the instrument, based on updated results from Crab Nebula observations.

European Commission, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung, Ministerstvo Školství, Mládeže a Tělovýchovy, Grantová Agentura České Republiky, Université de Genève
Openalex Percentile: Top 79%
Adaptive optics and wavefront sensing
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