Mono and stereo performance of the two SST-1M telescope prototypes
J. Jurysek, T. Tavernier, V. Novotn\'y, M. Heller, D. Mandat, M. Pech,, C. Alispach, A. Araudo, V. Beshley, J. Blazek, J. Borkowski, S. Boula, T., Bulik, F. Cadoux, S. Casanova, A. Christov, L. Chytka, D. della Volpe, Y., Favre, L. Gibaud, T. Gieras, P. Hamal, M. Hrabovsky
TL;DR
This paper evaluates the performance of SST-1M telescopes in mono and stereo modes for gamma-ray observations, introducing a data analysis pipeline and assessing capabilities during commissioning.
Contribution
It presents a new data analysis pipeline and provides performance results of SST-1M telescopes in mono and stereo configurations during commissioning.
Findings
Performance metrics for mono and stereo observations
Validation of the sst1mpipe data analysis pipeline
Assessment of telescopes' capabilities in different observation modes
Abstract
The Single-Mirror Small-Sized Telescope, or SST-1M, was originally developed as a prototype of a small-sized telescope for CTA, designed to form an array for observations of gamma-ray-induced atmospheric showers for energies above 3 TeV. A pair of SST-1M telescopes is currently being commissioned at the Ondrejov Observatory in the Czech Republic, and the telescope capabilities for mono and stereo observations are being tested in better astronomical conditions. The final location for the telescopes will be decided based on these tests. In this contribution, we present a data analysis pipeline called sst1mpipe, and the performance of the telescopes when working independently and in a stereo regime.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Gamma-ray bursts and supernovae · Particle Detector Development and Performance