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
Main Authors: Hunacek, J., Bock, J., Bradford, C. M., Butler, V., Chang, T.-C., Cheng, Y.-T., Cooray, A., Crites, A., Frez, C., Hailey-Dunsheath, S., Hoscheit, B., Kim, D. W., Li, C.-T., Marrone, D., Moncelsi, L., Shirokoff, E., Steinbach, B., Sun, G., Trumper, I., Turner, A., Uzgil, B., Weber, A., Zemcov, M.
Format: Journal Article
Language:English
Published: New York Springer US 01-12-2018
Springer Nature B.V
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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 .
ISSN:0022-2291
1573-7357
DOI:10.1007/s10909-018-1906-3