2026-06-27T12:27:19Zhttps://docta.ucm.es/rest/oai/requestoai:docta.ucm.es:20.500.14352/76192023-08-28T10:19:12Zcom_20.500.14352_14col_20.500.14352_15
Docta Complutense
author
Hoang, Kim Dinh
author
Hassan, Tarek
author
Angel Tejedor, Luis
author
Barrio Uña, Juan Abel
author
López Moya, Marcos
author
Fink, David
author
Will, Martin
author
Contreras González, José Luis
2023-06-17T08:56:34Z
2023-06-17T08:56:34Z
2020-08-28
2329-4124
10.1117/1.JATIS.6.3.036002
https://hdl.handle.net/20.500.14352/7619
https://doi.org/10.1117/1.JATIS.6.3.036002
https://www.spiedigitallibrary.org/
The MAGIC telescopes are a system of two imaging atmospheric Cherenkov telescopes designed to observe very-high-energy y rays. MAGIC utilizes a large reflective surface and photodetectors with ultrafast time response to capture Cherenkov photons. These features, together with the dedicated system installed in the central photomultiplier tube of their camera, so-called central pixel system (CPS), turn MAGIC into a suitable telescope to study high-speed optical astronomy in the millisecond (ms) regime. We report on the status of the CPS currently mounted in the MAGIC-II camera, its performance and calibration to demonstrate the sensitivity of MAGIC-II to ms optical pulses, for both transient and periodic signals, and discuss its potential over several science cases. (C) The Authors. Published by SPIE under a Creative Commons Attribution 4.0 Unported License.
eng
Atribución 3.0 España
MAGIC-II's central pixel system for simultaneous optical and gamma-ray observation
journal article
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https://docta.ucm.es/bitstreams/a43eb0e5-090d-4ff7-8ce4-a875d5d7aceb/download
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ContrerasJL35libre+CC.pdf
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ContrerasJL35libre+CC.pdf.txt