Position modeling for the AXAF High Resolution Camera (HRC)

Details Position modeling for the AXAF High Resolution Camera (HRC) Position modeling for the AXAF High Resolution Camera (HRC)

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989spie.1159..460c&link_type=abstract

IN: EUV, X-ray, and gamma-ray instrumentation for astronomy and atomic physics; Proceedings of the Meeting, San Diego, CA, Aug.

Astronomy and Astrophysics

Astrophysics

High Resolution, X Ray Astrophysics Facility, Algorithms, Imaging Techniques, Microchannel Plates, Models, Position Errors

Scientific paper

The High Resolution Camera (HRC) is one of four instruments selected to fly on the NASA Advanced X-ray Astrophysics Facility Murray and Chappell (1988). The HRC is designed to detect single X-ray photon events in the soft X-ray energy range from 0.1 to 10.0 KeV. The measured spatial resolution (FWHM) is 25 micron over a 100 sq cm detecting area. This paper investigates the accuracy and limitations of the position algorithm used with the coarse/fine resistive wire readout system.

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