Competition between Increasing and Decreasing Effects of the Afterpulsing Rate of PMTs during Night-Sky Observations

Fuente: arXiv
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Main Authors: Kiyomoto, Takuto, Nagayoshi, Tsutomu, Sakurai, Shunsuke, Takahashi, Mitsunari, Yamamoto, Tokonatsu, Donini, Alice, Inome, Yusuke, Kobayashi, Yukiho, Mazin, Daniel, Mirzoyan, Razmik, Nozaki, Seiya, Ohoka, Hideyuki, Okumura, Akira, Saito, Takayuki, Takeishi, Ryuji, Teshima, Masahiro
Format: Preprint
Published: 2025
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author Kiyomoto, Takuto
Nagayoshi, Tsutomu
Sakurai, Shunsuke
Takahashi, Mitsunari
Yamamoto, Tokonatsu
Donini, Alice
Inome, Yusuke
Kobayashi, Yukiho
Mazin, Daniel
Mirzoyan, Razmik
Nozaki, Seiya
Ohoka, Hideyuki
Okumura, Akira
Saito, Takayuki
Takeishi, Ryuji
Teshima, Masahiro
author_facet Kiyomoto, Takuto
Nagayoshi, Tsutomu
Sakurai, Shunsuke
Takahashi, Mitsunari
Yamamoto, Tokonatsu
Donini, Alice
Inome, Yusuke
Kobayashi, Yukiho
Mazin, Daniel
Mirzoyan, Razmik
Nozaki, Seiya
Ohoka, Hideyuki
Okumura, Akira
Saito, Takayuki
Takeishi, Ryuji
Teshima, Masahiro
contents Photomultiplier tubes (PMTs) have been widely used in imaging atmospheric Cherenkov telescopes (IACTs). The Large-Sized Telescopes (LSTs) of the Cherenkov Telescope Array Observatory (CTAO), the latest-generation IACTs, are optimized for challenging observations of low-energy gamma rays, specifically in the 20 to 150 GeV range. To this end, PMTs with an exceptionally low afterpulsing probability have been developed and installed. However, the afterpulsing rate increases over time due to the infiltration of atmospheric molecules, particularly helium, into the tube. Interestingly, we found that the afterpulsing rate decreases when PMTs are operated at high voltage and exposed to light -- a condition naturally met during IACT observations. To evaluate the latest instrument response, after five years of operation, we removed several PMTs from the first LST, which is currently the only operational telescope among the CTAO instruments. Our laboratory measurements showed no increase in afterpulsing compared to pre-installation values. This suggests that the decrease in afterpulsing during operation offsets the increase, thereby maintaining the long-term performance of the PMTs.
format Preprint
id arxiv_https___arxiv_org_abs_2502_02423
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Competition between Increasing and Decreasing Effects of the Afterpulsing Rate of PMTs during Night-Sky Observations
Kiyomoto, Takuto
Nagayoshi, Tsutomu
Sakurai, Shunsuke
Takahashi, Mitsunari
Yamamoto, Tokonatsu
Donini, Alice
Inome, Yusuke
Kobayashi, Yukiho
Mazin, Daniel
Mirzoyan, Razmik
Nozaki, Seiya
Ohoka, Hideyuki
Okumura, Akira
Saito, Takayuki
Takeishi, Ryuji
Teshima, Masahiro
Instrumentation and Methods for Astrophysics
Photomultiplier tubes (PMTs) have been widely used in imaging atmospheric Cherenkov telescopes (IACTs). The Large-Sized Telescopes (LSTs) of the Cherenkov Telescope Array Observatory (CTAO), the latest-generation IACTs, are optimized for challenging observations of low-energy gamma rays, specifically in the 20 to 150 GeV range. To this end, PMTs with an exceptionally low afterpulsing probability have been developed and installed. However, the afterpulsing rate increases over time due to the infiltration of atmospheric molecules, particularly helium, into the tube. Interestingly, we found that the afterpulsing rate decreases when PMTs are operated at high voltage and exposed to light -- a condition naturally met during IACT observations. To evaluate the latest instrument response, after five years of operation, we removed several PMTs from the first LST, which is currently the only operational telescope among the CTAO instruments. Our laboratory measurements showed no increase in afterpulsing compared to pre-installation values. This suggests that the decrease in afterpulsing during operation offsets the increase, thereby maintaining the long-term performance of the PMTs.
title Competition between Increasing and Decreasing Effects of the Afterpulsing Rate of PMTs during Night-Sky Observations
topic Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2502.02423