Share Email Print

Proceedings Paper

The ASTRI SST-2M prototype for the next generation of Cherenkov telescopes: structure and mirrors
Author(s): Rodolfo Canestrari; Enrico Cascone; Paolo Conconi; Mauro Fiorini; Enrico Giro; Nicola La Palombara; Luigi Lessio; Giovanni Pareschi; Gabriele Rodeghiero; Giorgia Sironi; Luca Stringhetti; Giorgio Toso; Gino Tosti; Francesco Martelli; Giancarlo Parodi; Pierfrancesco Rossettini; Raffaele Tomelleri
Format Member Price Non-Member Price
PDF $14.40 $18.00
cover GOOD NEWS! Your organization subscribes to the SPIE Digital Library. You may be able to download this paper for free. Check Access

Paper Abstract

The next generation of Imaging Atmospheric Cherenkov Telescope will explore the uppermost end of the Very High Energy domain up to about few hundreds of TeV with unprecedented sensitivity, angular resolution and imaging quality.

To this end, the Italian National Institute of Astrophysics (INAF) is currently developing a scientific and technological telescope prototype for the implementation of the Cherenkov Telescope Array (CTA) observatory. The Italian ASTRI program foresees the full design, development, installation and calibration of a Small Size 4-meter class Telescope, adopting an aplanatic, wide-field, double-reflection optical layout in a Schwarzschild-Couder configuration.

In this paper we discuss about the technological solutions adopted for the telescope and for the mirrors. In particular we focus on the structural and electro-mechanical design of the telescope, now under fabrication. The results on the optical performance derived from mirror prototypes are here described, too.

Paper Details

Date Published: 26 September 2013
PDF: 13 pages
Proc. SPIE 8861, Optics for EUV, X-Ray, and Gamma-Ray Astronomy VI, 886102 (26 September 2013); doi: 10.1117/12.2024379
Show Author Affiliations
Rodolfo Canestrari, INAF - Osservatorio Astronomico di Brera (Italy)
Enrico Cascone, INAF - Osservatorio Astronomico di Capodimonte (Italy)
Paolo Conconi, INAF - Osservatorio Astronomico di Brera (Italy)
Mauro Fiorini, INAF - IASF Milano (Italy)
Enrico Giro, INAF - Osservatorio Astronomico di Padova (Italy)
Nicola La Palombara, INAF - IASF Milano (Italy)
Luigi Lessio, INAF - Osservatorio Astronomico di Padova (Italy)
Giovanni Pareschi, INAF - Osservatorio Astronomico di Brera (Italy)
Gabriele Rodeghiero, INAF - Osservatorio Astronomico di Padova (Italy)
Giorgia Sironi, INAF - Osservatorio Astronomico di Brera (Italy)
Luca Stringhetti, INAF - IASF Milano (Italy)
Giorgio Toso, INAF - IASF Milano (Italy)
Gino Tosti, Univ. degli Studi di Perugia (Italy)
Francesco Martelli, BCV Progetti S.r.l. (Italy)
Giancarlo Parodi, BCV Progetti S.r.l. (Italy)
Pierfrancesco Rossettini, Tomelleri S.r.l. (Italy)
Raffaele Tomelleri, Tomelleri S.r.l. (Italy)

Published in SPIE Proceedings Vol. 8861:
Optics for EUV, X-Ray, and Gamma-Ray Astronomy VI
Stephen L. O'Dell; Giovanni Pareschi, Editor(s)

© SPIE. Terms of Use
Back to Top