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Hafnium Films and Magnetic Shielding for TIME, A mm-Wavelength Spectrometer Array

Authors :
Jonathon Hunacek
A. C. Weber
Lorenzo Moncelsi
Isaac Trumper
Yun-Ting Cheng
Guochao Sun
Charles M. Bradford
Asantha Cooray
Dae Wook Kim
V. Butler
M. Zemcov
J. J. Bock
Tzu-Ching Chang
Bryan Steinbach
Erik Shirokoff
Clifford Frez
S. Hailey-Dunsheath
Benjamin L. Hoscheit
B. Uzgil
Chao-Te Li
Daniel P. Marrone
A. T. Crites
A. D. Turner
Source :
Journal of Low Temperature Physics. 193:893-900
Publication Year :
2018
Publisher :
Springer Science and Business Media LLC, 2018.

Abstract

TIME is a mm-wavelength grating spectrometer array that will map fluctuations of the 157.7-μm emission line of singly ionized carbon ([CII]) during the epoch of reionization (redshift z ∼5–9). Sixty transition-edge sensor (TES) bolometers populate the output arc of each of the 32 spectrometers, for a total of 1920 detectors. Each bolometer consists of gold absorber on a ∼ 3 × 3 mm silicon nitride micro-mesh suspended near the corners by 1 × 1 × 500 μm silicon nitride legs targeting a photon-noise-dominated NEP ∼1×10^(-17)W/√Hz. Hafnium films are explored as a lower-T_c alternative to Ti (500 mK) for TIME TESs, allowing thicker support legs for improved yield. Hf T_c is shown to vary between 250 and 450 mK when varying the resident Ar pressure during deposition. Magnetic shielding designs and simulations are presented for the TIME first-stage SQUIDs. Total axial field suppression is predicted to be 5×10^7.

Details

ISSN :
15737357 and 00222291
Volume :
193
Database :
OpenAIRE
Journal :
Journal of Low Temperature Physics
Accession number :
edsair.doi...........c175e208e37c6564dca24601baaa73fb
Full Text :
https://doi.org/10.1007/s10909-018-1906-3