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Observatory Galactic Science with the ASTRI-Mini Array during the observatory phase of the project

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Author(s):
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D'Ai, Antonino ; Amato, E. ; Burtovoi, A. ; Compagnino, A. A. ; Fiori, M. ; Giuliani, A. ; La Palombara, N. ; Paizis, A. ; Piano, G. ; Saturni, F. G. ; Tutone, A.
Total Authors: 11
Document type: Journal article
Source: 2022 25TH INTERNATIONAL CONFERENCE ON INFORMATION FUSION (FUSION 2022); v. N/A, p. 8-pg., 2022-01-01.
Abstract

The ASTRI-Mini Array will be composed of nine imaging atmospheric Cherenkov telescopes at the Teide Observatory site. The array will observe in the 0.5-200 TeV range with an angular resolution of a few arc-minutes and an energy resolution of about 10%. The deployment of the first cameras will begin in 2022, and in the first four operational years the ASTRI Collaboration has developed a core-science programme focused on a limited number of key science targets. Additionally, thanks to a field-of-view of about 6 degree radius, ASTRI-MA will collect data from many other field sources that will constitute the base of a long-term Galactic observatory programme. In this contribution, I will overview the main themes for this extended observatory science programme for the different astrophysical Galactic environments. (AU)

FAPESP's process: 13/10559-5 - Investigation of high energy and plasma astrophysics phenomena: theory, numerical simulations, observations, and instrument development for the Cherenkov Telescope Array (CTA)
Grantee:Elisabete Maria de Gouveia Dal Pino
Support Opportunities: Special Projects