Hafnium Films and Magnetic Shielding for TIME, A mm-Wavelength Spectrometer Array
TIME is a mm-wavelength grating spectrometer array that will map fluctuations of the 157.7- μ m 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, f...
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Published in: | Journal of low temperature physics Vol. 193; no. 5-6; pp. 893 - 900 |
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Main Authors: | , , , , , , , , , , , , , , , , , , , , , , |
Format: | Journal Article |
Language: | English |
Published: |
New York
Springer US
01-12-2018
Springer Nature B.V |
Subjects: | |
Online Access: | Get full text |
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Summary: | TIME is a mm-wavelength grating spectrometer array that will map fluctuations of the 157.7-
μ
m
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
μ
m 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
. |
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ISSN: | 0022-2291 1573-7357 |
DOI: | 10.1007/s10909-018-1906-3 |