The prototype Schwarzschild Couder Telescope: A Medium-Sized Telescope for the Cherenkov Telescope Array

The Schwarzschild-Couder Telescope (SCT) is a dual-mirror telescope designed for the Cherenkov Telescope Array Observatory (CTAO) to observe very-high-energy gamma rays (20 GeV to 300 TeV). It features a dualmirror system and a high-resolution camera with an 8° field of view (FoV) for enhanced angular resolution and background rejection. A prototype (pSCT) is operational at the Fred Lawrence Whipple Observatory (FLWO) in Arizona, with a 2.7° FoV SiPM array. The pSCT recently detected the Crab Nebula with 8.6 standard deviations of significance. The focal plane is currently being upgraded to improve sensors and expand the FoV from 2.7° to 8°. An overview of the pSCT project, its results, and the camera upgrade will be presented.

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Publication Details

Journal
Springer Link (Chiba Institute of Technology)
Published
2025-03-06
DOI
https://doi.org/10.1051/epjconf/202531912002/pdf
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
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article

The prototype Schwarzschild Couder Telescope: A Medium-Sized Telescope for the Cherenkov Telescope Array

Francesca Romana Pantaleo
Springer Link (Chiba Institute of Technology)
Astrophysics and Cosmic Phenomena
article

The prototype Schwarzschild Couder Telescope: A Medium-Sized Telescope for the Cherenkov Telescope Array

Francesca Romana Pantaleo
article en

Abstract

The Schwarzschild-Couder Telescope (SCT) is a dual-mirror telescope designed for the Cherenkov Telescope Array Observatory (CTAO) to observe very-high-energy gamma rays (20 GeV to 300 TeV). It features a dualmirror system and a high-resolution camera with an 8° field of view (FoV) for enhanced angular resolution and background rejection. A prototype (pSCT) is operational at the Fred Lawrence Whipple Observatory (FLWO) in Arizona, with a 2.7° FoV SiPM array. The pSCT recently detected the Crab Nebula with 8.6 standard deviations of significance. The focal plane is currently being upgraded to improve sensors and expand the FoV from 2.7° to 8°. An overview of the pSCT project, its results, and the camera upgrade will be presented.

Springer Link (Chiba Institute of Technology)
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Astrophysics and Cosmic Phenomena
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