Recent advances in superconducting nanowire single-photon detector technology for exoplanet transit spectroscopy in the mid-infrared

被引:43
|
作者
Wollman, Emma E. [1 ]
Verma, Varun B. [2 ]
Walter, Alexander B. [1 ]
Chiles, Jeff [2 ]
Korzh, Boris [1 ]
Allmaras, Jason P. [1 ]
Zhai, Yao [2 ,3 ]
Lita, Adriana E. [2 ]
McCaughan, Adam N. [2 ]
Schmidt, Ekkehart [1 ]
Frasca, Simone [1 ,4 ]
Mirin, Richard P. [2 ]
Nam, Sae Woo [2 ]
Shaw, Matthew D. [1 ]
机构
[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[2] NIST, Boulder, CO 80305 USA
[3] Univ Colorado, Dept Phys, Boulder, CO 80309 USA
[4] Ecole Polytech Fed Lausanne, Adv Quantum Architecture Lab, Neuchatel, Switzerland
基金
美国国家航空航天局;
关键词
superconducting nanowire single-photon detectors; superconducting detectors; single-photon detectors; infrared; detectors; space telescope;
D O I
10.1117/1.JATIS.7.1.011004
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The Origins Space Telescope mission concept includes an exoplanet transit spectrometer that requires detector arrays with ultrahigh pixel-to-pixel stability. Superconducting nanowire single-photon detectors, or SNSPDs, have the potential to meet these stringent stability requirements due to their digital-like output. Traditionally used for applications at near-IR telecom wavelengths, SNSPDs have demonstrated near-unity detection efficiencies, ultralow dark-count rates, and high dynamic ranges. Until recently, however, SNSPD operation at the mid-infrared (mid-IR) wavelengths of interest for Origins had not been demonstrated, and SNSPD formats were limited to small arrays and active areas. Recent advances in SNSPD fabrication techniques have pushed SNSPD sensitivity to wavelengths beyond 7 mu m and have enabled millimeter-scale active areas and kilopixel arrays. We report here on this progress and the outlook toward developing arrays of ultrastable superconducting nanowire single-photon detectors for mid-IR astronomy applications. (C) The Authors. Published by SPIE under a Creative Commons Attribution 4.0 Unported License.
引用
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页数:10
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