Presentation
14 December 2020 The Origins Survey Spectrometer (OSS) for the Origins Space Telescope
Author Affiliations +
Abstract
OSS on Origins is designed to decode the cosmic history of nucleosynthesis, star formation, and supermassive black hole growth with wide-area spatial-spectral 3-D surveys in the 30 to 670 micron band. Six wideband grating modules combine to cover the full band at R=300, each couples a long slit with at least 30 beams on the sky. Two high-resolution modes are provided: one incorporates an interferometer in front of the gratings providing R of more than 40,000 at 112 microns, the other adds an etalon for R>300,000 at 112 microns. The full system design is presented, including optics, detector arrays, readouts, and the thermal design.
Conference Presentation
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Charles M. Bradford, Bruce Cameron, Bradley Moore, James A. Corsetti, Edward Amatucci, Michael J. DiPirro, David T. Leisawitz, and Margaret Meixner "The Origins Survey Spectrometer (OSS) for the Origins Space Telescope", Proc. SPIE 11443, Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave, 114436V (14 December 2020); https://doi.org/10.1117/12.2562949
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KEYWORDS
Spectroscopy

Sensors

Space telescopes

Fourier transforms

Spectral resolution

Collimation

Fabry–Perot interferometers

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