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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
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.
Keywords
cosmic microwave background
gain calibrator
detector calibration
transition edge sensor
Published Date
2024-01-27
Publication Title
Journal of Astronomical Telescopes, Instruments, and Systems
Volume
volume10
Issue
issue1
Publisher
Society of Photo-optical Instrumentation Engineers
Start Page
018003
ISSN
2329-4124
Content Type
Journal Article
language
English
OAI-PMH Set
岡山大学
File Version
publisher
DOI
Web of Science KeyUT
License
http://creativecommons.org/licenses/by/4.0/
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
Funder Name
Japan Society for the Promotion of Science
Ozaki Exchange Program 2019
SOKENDAI
Ministry of Education, Culture, Sports, Science and Technology
助成番号
JP19J10652
18H01240
19KK0079
19K14734
22H04945
22K20371