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Author |
Kaneko, Daisuke
High Energy Accelerator Research Organization, International Center for Quantum-field Measurement Systems for Studies of the Universe and Particles
Takatori, Sayuri
Okayama University, Research Institute for Interdisciplinary Science
Hasegawa, Masaya
High Energy Accelerator Research Organization, International Center for Quantum-field Measurement Systems for Studies of the Universe and Particles
Hazumi, Masashi
High Energy Accelerator Research Organization, International Center for Quantum-field Measurement Systems for Studies of the Universe and Particles
Inoue, Yuki
National Central University, Center for High Energy and High Field Physics, Department of Physics
Jeong, Oliver
University of California, Department of Physics
Katayama, Nobuhiko
University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe
Lee, Adrian T.
University of California, Department of Physics
Matsuda, Frederick
Japan Aerospace Exploration Agency, Institute of Space and Astronautical Science
Nishino, Haruki
The University of Tokyo, Graduate School of Science, Research Center for the Early Universe
Siritanasak, Praween
National Astronomical Research Institute of Thailand
Suzuki, Aritoki
Lawrence Berkeley National Laboratory, Physics Division
Takakura, Satoru
Kyoto University, Department of Physics, Faculty of Science
Tomaru, Takayuki
National Astronomical Observatory of Japan, Gravitational Wave Project Office
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Abstract | We present an advanced system for calibrating the detector gain responsivity with a chopped thermal source for POLARBEAR-2a, which is the first receiver system of a cosmic microwave background (CMB) polarimetry experiment: the Simons Array. Intensity-to-polarization leakage due to calibration errors between detectors can be a significant source of systematic error for a polarization-sensitive experiment. To suppress this systematic uncertainty, POLARBEAR-2a calibrates the detector gain responsivities by observing a chopped thermal source before and after each period of science observations. The system includes a high-temperature ceramic heater that emits blackbody radiation covering a wide frequency range and an optical chopper to modulate the radiation signal. We discuss the experimental requirements of gain calibration and system design to calibrate POLARBEAR-2a. We evaluate the performance of our system during the early commissioning of the receiver system. This calibration system is promising for the future generation of CMB ground-based polarization observations.
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Keywords | cosmic microwave background
gain calibrator
detector calibration
transition edge sensor
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Published Date | 2024-01-27
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Publication Title |
Journal of Astronomical Telescopes, Instruments, and Systems
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Volume | volume10
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Issue | issue1
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Publisher | Society of Photo-optical Instrumentation Engineers
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Start Page | 018003
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ISSN | 2329-4124
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Content Type |
Journal Article
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language |
English
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OAI-PMH Set |
岡山大学
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Copyright Holders | © The Authors.
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File Version | publisher
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DOI | |
Web of Science KeyUT | |
Related Url | isVersionOf https://doi.org/10.1117/1.jatis.10.1.018003
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License | http://creativecommons.org/licenses/by/4.0/
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Citation | Daisuke Kaneko, Sayuri Takatori, Masaya Hasegawa, Masashi Hazumi, Yuki Inoue, Oliver Jeong, Nobuhiko Katayama, Adrian T. Lee, Frederick Matsuda, Haruki Nishino, Praween Siritanasak, Aritoki Suzuki, Satoru Takakura, and Takayuki Tomaru "Design and performance of a gain calibration system for the POLARBEAR-2a receiver system at the Simons Array cosmic microwave background experiment," Journal of Astronomical Telescopes, Instruments, and Systems 10(1), 018003 (27 January 2024). https://doi.org/10.1117/1.JATIS.10.1.018003
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Funder Name |
Japan Society for the Promotion of Science
Ozaki Exchange Program 2019
SOKENDAI
Ministry of Education, Culture, Sports, Science and Technology
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助成番号 | JP19J10652
18H01240
19KK0079
19K14734
22H04945
22K20371
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