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Proceedings Paper

SuperMOS: a new class of low resolution multiobject spectrographs
Author(s): Benjamin A. Mazin; Danica Marsden; Kieran O'Brien
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Paper Abstract

Microwave Kinetic Inductance Detector (MKID) arrays, recently demonstrated at the Palomar 200 inch telescope, are a new superconducting detector technology that has great potential for astrophysics. We propose a new type of instrument, a Superconducting Multi-Object Spectrograph (SuperMOS), that uses MKIDs in conjunction with a focal plane mask. We present the design and science goals of a SuperMOS designed for LSST follow-up named Giga-z. Housing a 100,000 pixel MKID array with energy resolution R=50{100 and a 0.35-1.35 μm bandwidth, it will be capable of measuring 2 billion spectra and determining redshifts over 20,000 square degrees in 3 years down to mi ≈ 24.5 on a dedicated 4-meter telescope. Compared to LSST alone, Giga-z should improve the redshift precision by a factor of three with a much lower catastrophic failure rate.

Paper Details

Date Published: 5 October 2012
PDF: 14 pages
Proc. SPIE 8446, Ground-based and Airborne Instrumentation for Astronomy IV, 84460O (5 October 2012); doi: 10.1117/12.926398
Show Author Affiliations
Benjamin A. Mazin, Univ. of California, Santa Barbara (United States)
Danica Marsden, Univ. of California, Santa Barbara (United States)
Kieran O'Brien, Univ. of California, Santa Barbara (United States)


Published in SPIE Proceedings Vol. 8446:
Ground-based and Airborne Instrumentation for Astronomy IV
Ian S. McLean; Suzanne K. Ramsay; Hideki Takami, Editor(s)

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