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

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    2017-ltd-jhunacek.pdf
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    Description:
    Final Accepted Manuscript
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    Author
    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.
    Show allShow less
    Affiliation
    Univ Arizona
    Issue Date
    2018-04-06
    Keywords
    Spectrometers
    Bolometers
    Transition-edge sensors
    Hafnium
    Magnetic shielding
    
    Metadata
    Show full item record
    Publisher
    SPRINGER/PLENUM PUBLISHERS
    Citation
    Hunacek, J., Bock, J., Bradford, C.M. et al. J Low Temp Phys (2018) 193: 893. https://doi.org/10.1007/s10909-018-1906-3
    Journal
    JOURNAL OF LOW TEMPERATURE PHYSICS
    Rights
    © Springer Science+Business Media, LLC, part of Springer Nature 2018.
    Collection Information
    This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.
    Abstract
    TIME is a mm-wavelength grating spectrometer array that will map fluctuations of the 157.7-mm emission line of singly ionized carbon ([CII]) during the epoch of reionization (redshift z similar to 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 similar to 3 x 3 mm silicon nitride micro-mesh suspended near the corners by 1 x 1 x 500 mu m silicon nitride legs targeting a photon-noise-dominated NEP similar to 1 x 10-(17) W/root 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 x 10(7).
    Note
    12 month embargo; published online: 6 April 2018
    ISSN
    0022-2291
    1573-7357
    DOI
    10.1007/s10909-018-1906-3
    Version
    Final accepted manuscript
    Sponsors
    National Science Foundation Graduate Research Fellowship [DGE-1144469]; National Science Foundation Astronomy and Astrophysics Postdoctoral Fellowship [1602677]
    Additional Links
    http://link.springer.com/10.1007/s10909-018-1906-3
    ae974a485f413a2113503eed53cd6c53
    10.1007/s10909-018-1906-3
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    UA Faculty Publications

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