A ThermalKinetic Inductance Detectors Pixel Design for Cosmic Microwave Background Observations at 90/150 GHz bands

Fuente: arXiv
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Auteurs principaux: Chai, Ye, Shu, Shibo, Li, Yongping, Sun, Jiamin, Liu, Zhouhui, Xu, Yu, Yan, Daikang, Li, Zhengwei, Liu, Yang, Wang, Yiwen, Guo, Weijie, Cao, Juexian, Liu, Congzhan
Format: Preprint
Publié: 2024
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author Chai, Ye
Shu, Shibo
Li, Yongping
Sun, Jiamin
Liu, Zhouhui
Xu, Yu
Yan, Daikang
Li, Zhengwei
Liu, Yang
Wang, Yiwen
Guo, Weijie
Cao, Juexian
Liu, Congzhan
author_facet Chai, Ye
Shu, Shibo
Li, Yongping
Sun, Jiamin
Liu, Zhouhui
Xu, Yu
Yan, Daikang
Li, Zhengwei
Liu, Yang
Wang, Yiwen
Guo, Weijie
Cao, Juexian
Liu, Congzhan
contents The highly sensitive millimeter-wave telescope is an important tool for accurate measurement of Cosmic Microwave Background (CMB) radiation, and its core component is a detector array located in a cryogenic focal plane. The feasibility of utilizing thermal kinetic inductance detectors (TKIDs) for CMB observations has been demonstrated. We propose a pixel design of TKIDs for observing CMB through atmospheric windows for observations in the 90/150 GHz bands. Assuming lossless dielectric, the coupling efficiency of a single pixel is around 90%. This pixel design will be utilized for future large-scale TKIDs array designs for CMB observations.
format Preprint
id arxiv_https___arxiv_org_abs_2401_14995
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle A ThermalKinetic Inductance Detectors Pixel Design for Cosmic Microwave Background Observations at 90/150 GHz bands
Chai, Ye
Shu, Shibo
Li, Yongping
Sun, Jiamin
Liu, Zhouhui
Xu, Yu
Yan, Daikang
Li, Zhengwei
Liu, Yang
Wang, Yiwen
Guo, Weijie
Cao, Juexian
Liu, Congzhan
Instrumentation and Methods for Astrophysics
The highly sensitive millimeter-wave telescope is an important tool for accurate measurement of Cosmic Microwave Background (CMB) radiation, and its core component is a detector array located in a cryogenic focal plane. The feasibility of utilizing thermal kinetic inductance detectors (TKIDs) for CMB observations has been demonstrated. We propose a pixel design of TKIDs for observing CMB through atmospheric windows for observations in the 90/150 GHz bands. Assuming lossless dielectric, the coupling efficiency of a single pixel is around 90%. This pixel design will be utilized for future large-scale TKIDs array designs for CMB observations.
title A ThermalKinetic Inductance Detectors Pixel Design for Cosmic Microwave Background Observations at 90/150 GHz bands
topic Instrumentation and Methods for Astrophysics
url https://arxiv.org/abs/2401.14995