Development of Ultra-Low-Noise TES Bolometer Arrays

被引:29
作者
Suzuki, T. [1 ,2 ]
Khosropanah, P. [2 ]
Ridder, M. L. [2 ]
Hijmering, R. A. [2 ]
Gao, J. R. [2 ,3 ]
Akamatsu, H. [2 ]
Gottardi, L. [2 ]
van der Kuur, J. [2 ]
Jackson, B. D. [2 ]
机构
[1] Inst Space & Astronaut Sci ISAS JAXA, Chuo Ku, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2525210, Japan
[2] SRON Netherlands Inst Space Res, Sorbonnelaan 2, NL-3584 CA Utrecht, Netherlands
[3] Delft Univ Technol, Kavli Inst NanoSci, Delft, Netherlands
关键词
Transition edge sensor; TES; Far-infrared spectrometer; SiN membrane; Cryogenic detectors; THz detectors; Deep reactive-ion etching; DRIE;
D O I
10.1007/s10909-015-1401-z
中图分类号
O59 [应用物理学];
学科分类号
摘要
SRON is developing ultra-low-noise transition edge sensors (TESs) based on a superconducting Ti/Au bilayer on a suspended SiN island with SiN legs for SAFARI aboard SPICA. We have two major concerns about realizing TESs with an ultra-low NEP of : achieving lower thermal conductance and no excess noise with respect to the phonon noise. To realize TESs with phonon-noise-limited NEPs, we need to make thinner () and narrower () SiN legs. With deep reactive-ion etching, three types of TESs were fabricated in combination with different SiN island sizes and the presence or absence of an optical absorber. Those TESs have a thin ), narrow (0.5-0.7 ), and long (340-460 ) SiN legs and show of and of . These TESs were characterized under AC bias using our frequency-division multiplexing readout (1-3 MHz) system. TESs without the absorber show NEPs as low as with a reasonable response speed (), which achieved the phonon noise limit. For TESs with the absorber, we confirmed a higher ) than that of TESs without the absorber likely due to stray light. The lowest NEP can make the new version of SAFARI with a grating spectrometer feasible.
引用
收藏
页码:52 / 59
页数:8
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