Design and performance of a high-throughput cryogenic detector system

Elmer H. Sharp; Dominic J. Benford; Dale J. Fixsen; Stephen F. Maher; Catherine T. Marx; Johannes G. Staguhn; Edward J. Wollack

doi:10.1117/12.790058

21 July 2008 Design and performance of a high-throughput cryogenic detector system

Elmer H. Sharp, Dominic J. Benford, Dale J. Fixsen, Stephen F. Maher, Catherine T. Marx, Johannes G. Staguhn, Edward J. Wollack

Author Affiliations +

Proceedings Volume 7020, Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV; 70202L (2008) https://doi.org/10.1117/12.790058
Event: SPIE Astronomical Telescopes + Instrumentation, 2008, Marseille, France

Abstract

The Goddard IRAM Superconducting Millimeter Observer (GISMO) is a new superconducting bolometer array camera for the IRAM 30 Meter Telescope on Pico Veleta, Spain. GISMO uses a 3He/4He cooler mounted to a liquid He/LN2 cryostat to cool the bolometer array and SQUID electronics to an operating temperature of 260mK. The bolometer array is based on the backshort-under-grid architecture and features 128 2mm square absorbing pixels. A 101mm diameter anti-reflection coated silicon lens is used to define the beam. A single cold pupil stop prevents warm radiation from reaching the array, but no other stops are used. In the beam, filters and a cold baffling and stray light suppression system were used to define the bandpass and prevent out-of-band radiation to a very high level, including out-of-band radiation leaking through the metal-mesh filters from extreme angles. We present a detailed description of this optical design and its performance. A comprehensive report of the electronics and cryogenic integration are also included.

Citation Download Citation

Elmer H. Sharp, Dominic J. Benford, Dale J. Fixsen, Stephen F. Maher, Catherine T. Marx, Johannes G. Staguhn, and Edward J. Wollack "Design and performance of a high-throughput cryogenic detector system", Proc. SPIE 7020, Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV, 70202L (21 July 2008); https://doi.org/10.1117/12.790058

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