Poster + Paper
31 August 2022 Testing magnetic interference between TES detectors and the telescope environment for future CMB satellite missions
Author Affiliations +
Conference Poster
Abstract
The two most common components of several upcoming CMB experiments are large arrays of superconductive TES (Transition-Edge Sensor) detectors and polarization modulator units, e.g. continuously-rotating Half-Wave Plates (HWP). A high detector count is necessary to increase the instrument raw sensitivity, however past experiments have shown that systematic effects are becoming one of the main limiting factors to reach the sensitivity required to detect primordial B-modes. Therefore, polarization modulators have become popular in recent years to mitigate several systematic effects. Polarization modulators based on HWP technologies require a rotating mechanism to spin the plate and modulate the incoming polarized signal. In order to minimize heat dissipation from the rotating mechanism, which is a stringent requirement particularly for a space mission like LiteBIRD, we can employ a superconductive magnetic bearing to levitate the rotor and achieve contactless rotation. A disadvantage of this technique is the associated magnetic fields generated by those systems. In this paper we investigate the effects on a TES detector prototype and find no detectable Tc variations due to an applied constant (DC) magnetic field, and a non-zero TES response to varying (AC) magnetic fields. We quantify a worst-case TES responsivity to the applied AC magnetic field of ∼ 105 pA/G, and give a preliminary interpretation of the pick-up mechanism.
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Tommaso Ghigna, Thuong D. Hoang, Takashi Hasebe, Yurika Hoshino, Nobuhiko Katayama, Kunimoto Komatsu, Adrian Lee, Tomotake Matsumura, Yuki Sakurai, Shinya Sugiyama, Aritoki Suzuki, Christopher Raum, Ryota Takaku, and Benjamin Westbrook "Testing magnetic interference between TES detectors and the telescope environment for future CMB satellite missions", Proc. SPIE 12190, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI, 121902N (31 August 2022); https://doi.org/10.1117/12.2630091
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KEYWORDS
Sensors

Polarization

Telescopes

Bolometers

Satellites

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