Bragg crystal spectroscopy and the Advanced X-ray Astrophysics Facility (AXAF)

Details Bragg crystal spectroscopy and the Advanced X-ray Astrophysics Facility (AXAF) Bragg crystal spectroscopy and the Advanced X-ray Astrophysics Facility (AXAF)

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988spie..982..245m&link_type=abstract

IN: X-ray instrumentation in astronomy II; Proceedings of the Meeting, San Diego, CA, Aug. 15-17, 1988 (A89-40276 17-35). Bellin

Astronomy and Astrophysics

Astrophysics

2

Astronomical Spectroscopy, X Ray Astronomy, X Ray Astrophysics Facility, X Ray Spectroscopy, Bragg Angle, Grazing Incidence, Solar Spectra, Stellar Spectra, X Ray Sources

Scientific paper

Some of the Bragg spectrometers which have been proposed in the last 15 years are reviewed, with special emphasis on two classes of spectrometers which are used in combination with grazing incidence telescopes: objective crystal spectrometers and focal plane crystal spectrometers. The Bragg crystal spectrometer on AXAF is described, including the design goals, the contributors to the rocking curve width, minimization of the Bragg angle, and the sensitivity.

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