Poster + Paper
26 August 2024 Production via thermal slumping of large glass monolithic secondary mirrors (1.8 m diameter) for Schwarzschild-Couder air-Cherenkov gamma-ray telescopes
G. Sironi, L. Proserpio, R. Millul, G. Tagliaferri, L. Lessio, S. Scuderi, C. Torricelli, A. Torricelli, G. Valsecchi, G. Pareschi
Author Affiliations +
Conference Poster
Abstract
The standard design for 4-meter diameter class Imaging Atmospheric Cherenkov Telescopes (IACTs) used in groundbased gamma-ray astronomy is the dual-mirror Schwarzschild-Couder-like configuration. This design has been adopted for the telescopes in the ASTRI-Horn and ASTRI Mini-Array experiments (1 + 9 telescopes) and the construction of the 37 telescopes in the Small Size Telescope (SST) sub-array of the Cherenkov Telescope Array Observatory (CTAO) in Chile. The design provides an aplanatic optical response across a field of view wider than 10 degrees and is suitable for compact cameras using small pixels such as SiPM sensors. The telescopes feature secondary mirrors with a diameter of 1.8 meters, made of monolithic glass using a hot-slumping replication process. The paper discusses the manufacturing and characterization results of the prototype mirrors.
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
G. Sironi, L. Proserpio, R. Millul, G. Tagliaferri, L. Lessio, S. Scuderi, C. Torricelli, A. Torricelli, G. Valsecchi, and G. Pareschi "Production via thermal slumping of large glass monolithic secondary mirrors (1.8 m diameter) for Schwarzschild-Couder air-Cherenkov gamma-ray telescopes", Proc. SPIE 13100, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation VI, 131003H (26 August 2024); https://doi.org/10.1117/12.3019743
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KEYWORDS
Mirrors

Telescopes

Glasses

Manufacturing

Atmospheric Cherenkov telescopes

Prototyping

Gamma ray astronomy

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