Paper
16 September 1994 Calibration program for the Advanced X-ray Astrophysics Facility (AXAF) high-resolution camera
Author Affiliations +
Abstract
The High Resolution Camera, or HRC, is a set of microchannel plate based detectors designed to fly aboard the Advanced X-Ray Astrophysics Facility (AXAF), a major NASA space observatory. It will undergo a series of calibration tests before launch in September 1998. The overall calibration is planned in three phases: tests performed before delivery, end-to-end testing at Marshall Space Flight Center, and post launch calibration observations. In this paper, we examine the planned calibration program for the HRC, focusing on laboratory and synchrotron tests to be made before delivery.
© (1994) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Kathryn A. Flanagan, Marco Barbera, Stephen S. Murray, and Martin V. Zombeck "Calibration program for the Advanced X-ray Astrophysics Facility (AXAF) high-resolution camera", Proc. SPIE 2280, EUV, X-Ray, and Gamma-Ray Instrumentation for Astronomy V, (16 September 1994); https://doi.org/10.1117/12.186816
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KEYWORDS
Calibration

Sensors

Quantum efficiency

X-rays

Microchannel plates

Mirrors

Astrophysics

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