FIRSST: direct detection spectrometer instrument
Space Telescopes and Instrumentation: Optical, Infrared, and Millimeter Wave, pp. 16
Abstract
The Direct Detection Spectrometer Instrument (DDSI) is one of two instruments designed for the Far-IR Spectroscopy Space Telescope (FIRSST) recently proposed to NASA in response to the Astrophysics Probe Explorer call. The DDSI consists of two modules: HR delivering spectra at R~20,000 to 100,000 in three select bands (HR1-3) across 56-184μm, and LR providing broadband spectral coverage at R~100 in four bands (LR1-4) across 35-260 µm. The dispersive element of the HR bands is a compact optical resonator known as a virtually imaged phase array. All DDSI bands use microwave kinetic inductance detector (MKID) arrays cooled to 120mK. The total DDSI MKID pixel count is 2612 pixels.
Authors 13
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Affiliation as printed
NASA Goddard Space Flight Ctr. (United States)
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Affiliation as printed
Cornell Univ. (United States)
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Affiliation as printed
Cornell Univ. (United States)
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Affiliation as printed
NASA Goddard Space Flight Ctr. (United States)
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Affiliation as printed
NASA Goddard Space Flight Ctr. (United States)
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Space Research Organisation Netherlands
Affiliation as printed
SRON Netherlands Institute for Space Research (Netherlands)
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Affiliation as printed
Ball Aerospace (United States)
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Affiliation as printed
Ball Aerospace (United States)
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Affiliation as printed
Ball Aerospace (United States)
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Affiliation as printed
Ball Aerospace (United States)
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Affiliation as printed
Ball Aerospace (United States)
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Rochester Institute of Technology
Affiliation as printed
Rochester Institute of Technology (United States)
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