12 October 1996 Hard x-ray telescope mission
Author Affiliations +
Abstract
The Hard X-Ray Telescope was selected for study as a possible new intermediate size mission for the early 21st century. Its principal attributes are: (1) multiwavelength observing with a system of focussing telescopes that collectively observe from the UV to over 1 MeV, (2) much higher sensitivity and much better angular resolution in the 10 - 100 keV band, and (3) higher sensitivity for detecting gamma ray lines of known energy in the 100 keV to 1 MeV band. This paper emphasizes the mission aspects of the concept study such as the payload configuration and launch vehicle. An engineering team at the Marshall Space Center is participating in these two key aspects of the study.
© (1996) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Paul Gorenstein, D. M. Worrall, Karsten Dan Joensen, Suzanne E. Romaine, Martin C. Weisskopf, Brian D. Ramsey, James W. Bilbro, Richard A. Kroeger, Neil A. Gehrels, Ann M. Parsons, Robert K. Smither, Finn Erland Christensen, Oberto Citterio, Peter von Ballmoos, "Hard x-ray telescope mission", Proc. SPIE 2807, Space Telescopes and Instruments IV, (12 October 1996); doi: 10.1117/12.255094; http://dx.doi.org/10.1117/12.255094
PROCEEDINGS
12 PAGES


SHARE
KEYWORDS
Sensors

Space telescopes

Crystals

X-ray telescopes

Mirrors

Telescopes

Hard x-rays

RELATED CONTENT

BOMBOLO: A 3-arms optical imager for SOAR Observatory
Proceedings of SPIE (July 24 2014)
Laser-driven polyplanar optic display
Proceedings of SPIE (May 04 1998)
SPIRE: a bolometer instrument for FIRST
Proceedings of SPIE (July 31 1998)
A relay imaging probe to check focus map of Earth...
Proceedings of SPIE (October 28 2014)

Back to Top