The Rockets for Extended-source X-ray Spectroscopy Instrument Design

Author:

Miles Drew M.ORCID,McEntaffer Randall L.ORCID,Tutt James H.ORCID,Baker Logan,McCurdy RossORCID,Myers Bailey,O’Meara Bridget,Weston Joseph

Abstract

Abstract The Rockets for Extended-source X-ray Spectroscopy (tREXS) are a series of suborbital rocket payloads designed to collect spectral emission from extended astronomical sources of soft X-rays. The tREXS spectrograph uses mechanical beam-shaping modules and reflection gratings to passively focus and then disperse incident X-rays to an array of Teledyne/e2v CIS 113 CMOS X-ray sensors. Designed to achieve a moderate spectral resolution, R ⪆ 50, from ≈15 to 40 Å over a large field of view (>10 deg2), the tREXS instrument is sensitive to line emission from key ion species over the soft-X-ray band. Here we present the complete end-to-end design of the tREXS spectrograph and discuss its significance and expected performance, using simulated observations of the Cygnus Loop supernova remnant and an enhanced region in the soft X-ray background.

Funder

NASA ∣ Science Mission Directorate

NASA ∣ Space Technology Mission Directorate

Publisher

American Astronomical Society

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