Poster presented at the XXXII International Astronomical Union General Assembly

[ Marek Nikołajuk, XXXII IAU, 6-15 August 2024 in Cape Town ] Marek Nikołajuk, member of the SST-1M consortium, presented a poster at the International Astronomical Union General Assembly held in Cape Town, South Africa. The presentation showcased an overview of the telescope and camera design, as well as preliminary results derived from the commissioning data and data analysis. The event provided an opportunity to highlight that the SST-1M mini-array has demonstrated its remarkable potential for conducting detailed astronomical observations. Despite operating under commissioning conditions at the Ondřejov Observatory, the array has already achieved significant results. These achievements pave the...

Observation of Astrophysical Sources with SST-1M Telescopes – First Results

[ Jakub Jurysek (Institute of Physics of Czech Academy of Sciences), Gamma 2024 – Milano, 2.-6. September 2024 ] The Single-Mirror Small Size Cherenkov Telescope (SST-1M) was developed by a consortium of institutes in Switzerland, Poland, and the Czech Republic. The SST-1M design is based on the DaviesCotton concept, featuring a 4-meter mirror and an innovative SiPM-based camera. It is most sensitive to gamma rays in the TeV and multi-TeV energy bands. Since 2021, two SST-1M prototypes have been commissioned at the Ondřejov Observatory in the Czech Republic, where their performance in both mono and stereo observation modes is being tested....

Commissioning and Operation of the SST-1M Stereoscopic Imaging Atmospheric Cherenkov Telescopes

[ Matthieu Heller (University of Geneva), Gamma 2024 – Milano, 2.-6. September 2024 ] The small-size single mirror telescopes, SST-1Ms, are two Cherenkov telescope prototypes developed by a consortium of Czech, Polish, and Swiss institutions. Featuring a 9.42 m² multi-segment mirror and a 5.6 m focal length, the SST-1Ms offer a broad 9-degree field of view and have proven capable of detecting gamma rays with energies starting from several hundred GeV. The innovative cameras incorporate a compact photo-detector plane with 1296 hexagonal silicon photomultiplier pixels and a fully digital readout and trigger system utilizing 250 MSps FADCs. Currently undergoing commissioning at...

Commissioning and Preliminary Observation Results of SST-1M presented at TeVPA conference in Chicago

[ Thomas Tavernier (FZU, Prague, Czech Republic), TeVPa 2024 – Chicago, 27. 8. 2024 ] SST-1M is a single-mirror small size Cherenkov telescope prototype developed by a consortium among institutes in Switzerland, Poland, and the Czech Republic. With a 4 meter mirror and a 5.6 m focal length, SST-1Ms have a broad 9 degree field of view and aim to detect gamma rays spanning the energy range of 1 to 300 TeV. The DigiCam camera incorporates a compact Photo-Detector Plane comprising 1296 hexagonal silicon photomultiplier pixels and a fully digital readout and trigger system using a 250 MHz ADC. Two SST-1M...

Poster presented on CTAO Science Symposium

[ Bastien Lacave, CTAO Science Symposium, 15-18 April 2024 in Bologna ] Current status and recent results of the SST-1M telescopes were presented at the CTAO Science Symposium in Bologna. Bastien Lacave, member of the SST-1M consortium, presented poster to the general audience, emhasizing achievemts reached with the telescopes operation in stereo mode and future prospects for scientific observations. [ View the poster ] [ CTAO Science Symposium 2024 – website ] Photo: archive of the Astronomical Institute of the Academy of Sciences of the Czech Republic.

Design, Performance, and Commissioning Results of a SST-1M Telescope

Thomas Tavernier (FZU, Prague, Czech Republic), TeVPa 2023 – Napoli, 12. 9. 2023 SST-1M is a single-mirror Small Size Telescope prototype developed by a consortium of institutes from Poland, Switzerland and the Czech Republic. The design of the SST-1M follows the Davies-Cotton design, with a 9.42m2 multi-segment mirror. With a wide field of view of 9 degrees, SST-1M is designed to detect gamma rays in the energy range between 1 and 300 TeV. The two SST-1Ms that have been built are equipped with the DigiCam camera, which features a fully digital readout and trigger system using 250 MHz ADC, and a compact...

Analysis of commissioning data from SST-1M : APrototype of Single-Mirror Small Size Telescope

Thomas Tavernier (on behalf of SST-1M Group), ICRC 2023, Nagoya, Japan, 26. 7. – 3. 8. 2023 SST-1M is a prototype of a single-mirror Small Size Telescope developed by a consortium of institutes from Poland, Switzerland and the Czech Republic. With a wide field of view of 9 degrees, SST-1Ms are designed to detect gamma-rays in the energy range between 1 and 300 TeV. The design of the SST-1M follows the Davies-Cotton concept, with a 9.42m2 multi-segment mirror. SST-1M is equipped with DigiCam camera, which features a fully digital readout and trigger system using 250 MHz ADC, and a compact...

Mono and stereo performance of the two SST-1M telescope prototypes

Jakub Jurysek (on behalf of SST-1M Group), ICRC 2023, Nagoya, Japan, 26. 7. – 3. 8. 2023 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,...