西蒙斯阵列宇宙微波背景实验 POLARBEAR-2a 接收器系统增益校准系统的设计与性能

IF 1.7 3区 工程技术 Q2 ENGINEERING, AEROSPACE
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, Takayuki Tomaru
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引用次数: 0

摘要

我们为 POLARBEAR-2a 提出了一种先进的系统,用于用斩波热源校准探测器增益响应率,POLARBEAR-2a 是宇宙微波背景(CMB)偏振测量实验:西蒙斯阵列的第一个接收系统。探测器之间的校准误差导致的强度-偏振泄漏是偏振敏感实验系统误差的一个重要来源。为了抑制这种系统不确定性,POLARBEAR-2a 通过在每期科学观测前后观测一个斩波热源来校准探测器的增益响应度。该系统包括一个高温陶瓷加热器和一个用于调制辐射信号的光学斩波器。我们讨论了增益校准的实验要求和校准 POLARBEAR-2a 的系统设计。我们在接收机系统早期调试期间对系统性能进行了评估。这套校准系统对未来新一代的 CMB 地面偏振观测大有可为。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Design and performance of a gain calibration system for the POLARBEAR-2a receiver system at the Simons Array cosmic microwave background experiment
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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来源期刊
CiteScore
4.40
自引率
13.00%
发文量
119
期刊介绍: The Journal of Astronomical Telescopes, Instruments, and Systems publishes peer-reviewed papers reporting on original research in the development, testing, and application of telescopes, instrumentation, techniques, and systems for ground- and space-based astronomy.
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