Fabrication of Low-Noise TES Arrays for the SAFARI Instrument on SPICA

Journal article (2016)

Authors

Marcel Ridder SRON–Netherlands Institute for Space Research
P. Khosropanah SRON–Netherlands Institute for Space Research
R. A. Hijmering SRON–Netherlands Institute for Space Research
T. Suzuki SRON–Netherlands Institute for Space Research, Japan Aerospace Exploration Agency
M.P. Bruijn SRON–Netherlands Institute for Space Research
H. F C Hoevers SRON–Netherlands Institute for Space Research
Jian Rong Gao Kavli institute of nanoscience Delft, SRON–Netherlands Institute for Space Research, QN/Gao Lab
M.R. Zuiddam Kavli institute of nanoscience Delft, QN/Kavli Nanolab Delft
Research Group
QN/Gao Lab
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Published Date

01-07-2016

Language

English

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Research Group

QN/Gao Lab

Abstract

Ultra-low-noise transition edge sensors (TES) with noise equivalent power lower than 2 × 10- 19 W/Hz1 / 2 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 μ 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.

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