22 October 1999 HERO program: high-energy replicated optics for a hard-x-ray balloon payload
Author Affiliations +
We are developing high-energy replicated optics for a balloon-borne hard-x-ray telescope. When completed, the telescope will have around 130 cm2 of effective collecting area at 60 keV, and an angular resolution of <EQ 30 arc seconds, half power diameter. With an array of gas scintillation proportional counters in the focal plane the payload will provide unprecedented sensitivity for pointed observations in the hard-x-ray band. We present an overview of the HERO program, together with test data from the first mirror shell. The overall sensitivity of the full payload is given for planned long- and ultra-long-duration balloon flights.
© (1999) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Brian D. Ramsey, Brian D. Ramsey, Darell E. Engelhaupt, Darell E. Engelhaupt, Chet O. Speegle, Chet O. Speegle, Stephen L. O'Dell, Stephen L. O'Dell, Robert A. Austin, Robert A. Austin, Jeffery J. Kolodziejczak, Jeffery J. Kolodziejczak, Martin C. Weisskopf, Martin C. Weisskopf, } "HERO program: high-energy replicated optics for a hard-x-ray balloon payload", Proc. SPIE 3765, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy X, (22 October 1999); doi: 10.1117/12.366569; https://doi.org/10.1117/12.366569


XUV Wide Field Camera for ROSAT
Proceedings of SPIE (July 27 1989)
The x-ray telescope ROSITA on its way to orbit
Proceedings of SPIE (October 10 2004)
The development of hard x-ray optics at MSFC
Proceedings of SPIE (January 28 2004)
Development of a thin substrate for x-ray telescope
Proceedings of SPIE (November 13 2001)
The XUV Wide Field Camera on ROSAT
Proceedings of SPIE (July 13 1986)

Back to Top