Fabrication of Low-Noise TES Arrays for the SAFARI Instrument on SPICA
Fabrication of Low-Noise TES Arrays for the SAFARI Instrument on SPICA
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DOI:
10.1007/s10909-015-1381-z
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发表时间:
2016-07-01
影响因子:
2
通讯作者:
Zuiddam, M. R.
中科院分区:
文献类型:
--
作者:
Ridder, M. L.;Khosropanah, P.;Zuiddam, M. R.
Ultra-low-noise transition edge sensors (TES) with noise equivalent power lower than 2 10 W/Hz have been fabricated by SRON, which meet the sensitivity requirements for the far-infrared SAFARI instrument on space infrared telescope for cosmology and astrophysics. Our TES detector is based on a titanium/gold (Ti/Au) thermistor on a silicon nitride (SiN) island. The island is thermally linked with SiN legs to a silicon support structure at the bath temperature. The SiN legs are very thin (250 nm), narrow (500 nm), and long (above 300 m); these dimensions are needed in leg-isolated bolometers to achieve the required level of sensitivity. In this paper, we describe the latest fabrication process for our TES bolometers with improved sensitivity.