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Proceedings Paper

Concept study for a compact homodyne astrophysics spectrometer for exoplanets (CHASE)
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Paper Abstract

In this concept study, we are targeting to build a new instrument to sequentially observe exoplanet atmospheres and their parent’s stellar spectra over a significant time in NUV and FUV. The Compact Homodyne Astrophysics Spectrometer for Exoplanets (CHASE) offers integrated spectra over a wide field-of-view (FOV~40arcsec) in high spectral resolution (R>105) in a miniaturized architecture using no (or a small < 1m) primary mirror. CHASE’s wide FOV is compatible with the relaxed pointing requirements of current CubeSats and SmallSats which makes it readily qualifiable for space in a compact format and have the potential to enable major scientific breakthroughs.

Paper Details

Date Published: 18 July 2016
PDF: 9 pages
Proc. SPIE 9905, Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray, 990534 (18 July 2016); doi: 10.1117/12.2233242
Show Author Affiliations
Sona Hosseini, Jet Propulsion Lab. (United States)
Chris Webster, Jet Propulsion Lab. (United States)
Debra Fischer, Yale Univ. (United States)
Evgenya Shkolnik, Arizona State Univ. (United States)
Shouleh Nikzad, Jet Propulsion Lab. (United States)
Gautam Vasisht, Jet Propulsion Lab. (United States)
Wesley Traub, Jet Propulsion Lab. (United States)

Published in SPIE Proceedings Vol. 9905:
Space Telescopes and Instrumentation 2016: Ultraviolet to Gamma Ray
Jan-Willem A. den Herder; Tadayuki Takahashi; Marshall Bautz, Editor(s)

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