Ultra-low noise TES bolometer arrays for SAFARI instrument on SPICA

Conference Paper (2016)
Author(s)

P Khosropanah (SRON–Netherlands Institute for Space Research)

T. Suzuki (Nagoya University)

M. L. Ridder (SRON–Netherlands Institute for Space Research)

R. A. Hijmering (SRON–Netherlands Institute for Space Research)

H. Akamatsu (SRON–Netherlands Institute for Space Research)

L Gottardi (SRON–Netherlands Institute for Space Research)

J. Van Der Kuur (SRON–Netherlands Institute for Space Research)

J. R. Gao (SRON–Netherlands Institute for Space Research, TU Delft - QN/Gao Lab)

B. D. Jackson (SRON–Netherlands Institute for Space Research)

Research Group
QN/Gao Lab
DOI related publication
https://doi.org/10.1117/12.2233472
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Publication Year
2016
Language
English
Research Group
QN/Gao Lab
Volume number
9914
Article number
99140B
ISBN (electronic)
978-151060207-6
Event
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII (2016-06-28 - 2016-07-01), Edinburgh, United Kingdom
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Abstract

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 the SAFARI instrument aboard the SPICA mission. We successfully fabricated TESs with very narrow (0.5-0.7 μm) and thin (0.25 μm) SiN legs on different sizes of SiN islands using deep reactiveion etching process. The pixel size is 840x840 μm2 and there are variety of designs with and without optical absorbers. For TESs without absorbers, we measured electrical NEPs as low as <1x10-19 W/√Hz with response time of 0.3 ms and reached the phonon noise limit. Using TESs with absorbers, we quantified the darkness of our setup and confirmed a photon noise level of 2x10-19 W/√Hz.

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