The ASTRI gamma-ray air-Cherenkov experiment: status of the project

Not scheduled
20m
Itaca Hall (Sorrento)

Itaca Hall

Sorrento

Ulisse Deluxe Hostel Via del Mare, 22 - 80067 Sorrento – Napoli – Italy
Oral Gamma Ray Astronomy

Speaker

Giovanni Pareschi (INAF - Osservatorio Astronomico di Brera)

Description

The ASTRI Mini-Array is a next-generation ground-based gamma-ray experiment being built at the Observatorio del Teide (Tenerife, Canary Islands). It aims to explore the largely uncharted 0.5–300 TeV energy range with exceptional angular and spectral performance. The array includes nine identical 4-meter class imaging atmospheric Cherenkov telescopes (IACTs), each featuring the dual-mirror aplanatic Schwarzschild–Couder optical design and equipped with compact silicon photomultiplier (SiPM) cameras. These cameras use innovative peak-finder front-end electronics to provide a wide field of view (≥ 10°) and high collection efficiency. During 2024–2025, the first telescope (ASTRI-1) completed its commissioning and started regular data collection, including a dedicated observation campaign of the Crab Nebula—the standard candle of very-high-energy gamma-ray astronomy—for about 200 hours with detection of the source under various observing conditions (zenith angles, moonlight levels, wobble-mode offsets). Here, we report the completion of the mini-array, with all nine telescopes installed and some already equipped with focal-plane cameras. This enabled us to make the first observations in a stereoscopic configuration, demonstrating the design's effectiveness and the system's readiness for full-array operations and providing the first scientific data. We outline the scientific potential of the ASTRI Mini-Array once fully operational: the broad field of view and excellent angular resolution will enable morphological and spectral studies of both point-like and extended gamma-ray sources (e.g. supernova remnants, pulsar wind nebulae, PeVatrons), monitor blazars at very high energies, follow up transient events, and investigate cosmic-ray origins and fundamental physics. The ASTRI Mini-Array is poised to become one of the most sensitive instruments in the Northern Hemisphere at multi-TeV energies, bridging the observational gap between current IACTs and extensive air-shower arrays while offering unprecedented precision and versatility.

Author

Giovanni Pareschi (INAF - Osservatorio Astronomico di Brera)

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