The SPICA-SAFARI detector system: TES detector arrays with frequency-division multiplexed SQUID readout

B.D. Jackson, P.A.J. de Korte, J. van Der Kuur, P.D. Mauskopf, J. Beyer, M.P. Bruijn, A. Cros, J.-R. Gao, D. Griffin, R. Den Hartog, Mikko Kiviranta, G. de Lange, B.-J. van Leeuwen, C. Macculi, L. Ravera, N. Trappe, H. van Weers, S. Withington

    Research output: Contribution to journalArticleScientificpeer-review

    68 Citations (Scopus)

    Abstract

    The SAFARI instrument is a far-infrared imaging Fourier transform spectrometer for JAXA's SPICA mission. Taking advantage of the low emission of SPICA's 5 K telescope, SAFARI will provide sky background-limited, Nyquist-sampled spectroscopic imaging of a 2 ' × 2 ' field-of-view over 34-210 μm, creating significant new possibilities for far-infrared astronomy. SAFARI's aggressive science goals drive the development of a unique detector system combining large-format Transition Edge Sensor arrays and frequency division multiplexed SQUID readout with a high 160x multiplexing factor. The detectors and their cold readout electronics are packaged into 3 focal plane arrays that will be integrated into SAFARI's focal plane unit. Here we present the preliminary system design and current development status of the SAFARI detector system.
    Original languageEnglish
    Pages (from-to)12-21
    JournalIEEE Transactions on Terahertz Science and Technology
    Volume2
    Issue number1
    DOIs
    Publication statusPublished - 2012
    MoE publication typeA1 Journal article-refereed

    Funding

    This work was supported in part by the European Space Agency under ESA TRP Contracts 22559/09/NL/CP and 22559/09/NL/CP.

    Keywords

    • Astrophysics
    • bolometers
    • frequency-division multiplexing
    • superconducting devices
    • system-level design

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