低温工学
Online ISSN : 1880-0408
Print ISSN : 0389-2441
ISSN-L : 0389-2441
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超伝導センサーMKIDによる天文観測
―電波天文と宇宙背景放射―
本多 俊介 末野 慶徳田中 智永辻井 未来沓間 弘樹服部 誠鈴木 惇也美馬 覚田島 治大谷 知行村山 洋佑李 豪純石崎 悠治永井 誠久野 成夫
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2024 年 59 巻 1 号 p. 34-42

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The cutting-edge superconducting detector, Microwave Kinetic Inductance Detector(MKID) has been popular in the field of astronomical radio observations such as Cosmic Microwave Background(CMB), star-forming regions, and galaxy surveying. MKID is a resonator-based superconducting detector which has the scalability to exceed O(1,000) pixels in one readout line. The photon-noise-limited sensitivity can be achieved with the hybrid-type MKID which consists of two superconducting materials. The hybrid-type MKID arrays are utilized in “GroundBIRD” and “Tsukuba-KID camera” projects which are led by Japanese teams. Each project observed astronomical objects by the commissioning with developed MKID arrays and will start the science observations in the near future.

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