Calibration and performance of the readout system based on switched capacitor arrays for the Large-Sized Telescope of the Cherenkov Telescope Array

• Published in: arXiv.org
• Main Authors: Nozaki, Seiya, Awai, Kyosuke, Bamba, Aya, Juan Abel Barrio, Bernardos, Maria Isabel, Blanch, Oscar, Boix, Joan, Cassol, Franca, Choushi, Yuki, Delgado, Carlos, Diaz, Carlos, Fouque, Nadia, Freixas, Lluis, Gliwny, Pawel, Gunji, Shunichi, Hadasch, Daniela, Hoffmann, Dirk, Houles, Julien, Inome, Yusuke, Iwamura, Yuki, Jouvin, Léa, Katagiri, Hideaki, Kawamura, Kiomei, Kerszberg, Daniel, Konno, Yusuke, Kubo, Hidetoshi, Kushida, Junko, Kobayashi, Yukiho, López-Coto, Rubén, Martinez, Gustavo, Masuda, Shu, Mazin, Daniel, Moralejo, Abelardo, Moretti, Elena, Nagayoshi, Tsutomu, Nakamori, Takeshi, Nishijima, Kyoshi, Nogami, Yuto, Nogués, Leyre, Ohoka, Hideyuki, Oka, Tomohiko, Okazaki, Nao, Okumura, Akira, Orito, Reiko, Panazol, Jean-Luc, Paoletti, Riccardo, Pio, Cristobal, Polo, Miguel, Prast, Julie, Saito, Takayuki, Sakurai, Shunsuke, Sitarek, Julian, Sunada, Yuji, Suzuki, Megumi, Takahashi, Mitsunari, Tamura, Kenji, Tanaka, Manobu, Tejedor, Luis Angel, Terada, Yukikatsu, Teshima, Masahiro, Tsukamoto, Yusuke, Yamamoto, Tokonatsu
• Format: Paper Journal Article
• Language: English
• Published: Ithaca Cornell University Library, arXiv.org 13.03.2022
• Subjects: Arrays; Calibration; Cameras; Capacitors; Diameters; Focal plane; Gamma rays; Ground-based observation; Night sky; Photomultiplier tubes; Physics - Instrumentation and Methods for Astrophysics; Read out systems; Waveforms
• ISSN: 2331-8422
• DOI: 10.48550/arxiv.2203.06582

The Cherenkov Telescope Array (CTA) is the next-generation ground-based very-high-energy gamma-ray observatory. The Large-Sized Telescope (LST) of CTA is designed to detect gamma rays between 20 GeV and a few TeV with a 23-meter diameter mirror. We have developed the focal plane camera of the first LST, which has 1855 photomultiplier tubes (PMTs) and the readout system which samples a PMT waveform at GHz with switched capacitor arrays, Domino Ring Sampler ver4 (DRS4). To measure the precise pulse charge and arrival time of Cherenkov signals, we developed a method to calibrate the output voltage of DRS4 and the sampling time interval, as well as an analysis method to correct the spike noise of DRS4. Since the first LST was inaugurated in 2018, we have performed the commissioning tests and calibrated the camera. We characterised the camera in terms of the charge pedestal under various conditions of the night sky background, the charge resolution of each pixel, the charge uniformity of the whole camera, and the time resolutions with a test pulse and calibration laser.