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Proceedings Paper

The survey and time-domain astrophysical research explorer (STAR-X) (Conference Presentation)
Author(s): William W. Zhang

Paper Abstract

STAR-X was proposed in December 2016 as a MIDEX mission for launch in 2023. It is an X-ray telescope with the following characteristics: (1) large field of view; (2) excellent uniform PSF in the entire FOV; and (3) large effective area. STAR-X will catch and study transients, including those resulting from mergers of compact objects, supernova explosions, tidal disruptions, and gamma ray bursts. STAR-X will also conduct surveys to study the growth of compact objects, including stellar mass black holes in the Milky Way and nearby galaxies as well as distant, high-redshift supermassive black holes. The capabilities of STAR-X also enable the study of hot, low surface brightness diffuse emission from galaxy clusters and supernova remnants. STAR-X is facilitated by a spacecraft bus capable of autonomous and fast slewing to targets of opportunity. In this paper we will describe the STAR-X mission design, technology, and major science objectives and its synergy with other major observatories in the 2020s, including eROSITA, JWST, WFIRST, and Athena.

Paper Details

Date Published: 19 September 2017
Proc. SPIE 10397, UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XX, 103970O (19 September 2017); doi: 10.1117/12.2270862
Show Author Affiliations
William W. Zhang, NASA Goddard Space Flight Ctr. (United States)

Published in SPIE Proceedings Vol. 10397:
UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XX
Oswald H. Siegmund, Editor(s)

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