Optics for EUV, X-Ray, and Gamma-Ray Astronomy VIII 2017
DOI: 10.1117/12.2276767
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The ASTRI SST-2M prototype for the Cherenkov Telescope Array: status after the commissioning phase of the telescope

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Cited by 2 publications
(3 citation statements)
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“…Since its inauguration in 2014, an extensive set of tests was performed, to characterize and subsequently monitor the performance of the ASTRI-Horn telescope [10].…”
Section: Comissioning and Validation Of The Astri-horn Telescopementioning
confidence: 99%
“…Since its inauguration in 2014, an extensive set of tests was performed, to characterize and subsequently monitor the performance of the ASTRI-Horn telescope [10].…”
Section: Comissioning and Validation Of The Astri-horn Telescopementioning
confidence: 99%
“…As the southern site chosen for CTA has no volcanos in the immediate environment and no aggressive atmosphere, the rate of degradation should be in line with CTA requirements. The electromechanical structure has been intensively studied and its parameters have been optimized to achieve the maximum performance as thoroughly described in [6]. As part of regularly scheduled activity, an observational campaign to monitor the tracking and pointing performance as well as the astrometric precision of the telescope between November 2017 and January 2018 has been carried out.…”
Section: The Commissioning Of the Astri-horn Telescopementioning
confidence: 99%
“…While LSTs provide sensitivity at the lowest energies (20 < E < 150 GeV), SSTs are optimised to the highest VHE energies (5 < E < 300 GeV; [3]). There are currently three different SST prototypes under development within the CTA Collaboration, i.e., the single-mirror SST [4] and the dual-mirror (2M) telescopes GCT [5] and ASTRI [6]. The latter is conducted by the Italian National Institute for Astrophysics (INAF) since 2011 with the aim to design and develop within the CTA framework an end-to-end prototype of the SST in 2M configuration.…”
Section: Introductionmentioning
confidence: 99%