High resolution X-ray spectroscopy with the low energy transmission grating of AXAF.

Details High resolution X-ray spectroscopy with the low energy transmission grating of AXAF. High resolution X-ray spectroscopy with the low energy transmission grating of AXAF.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996rftu.proc..677b&link_type=abstract

International Conference on X-ray Astronomy and Astrophysics: Röntgenstrahlung from the Universe, p. 677 - 678

Astronomy and Astrophysics

Astronomy

X-Ray Astronomy: Space Missions, X-Ray Astronomy: Space Instrumentation

Scientific paper

The Advanced X-ray Astrophysics Facility (AXAF) is the third in the series of great observatories in the NASA programme after the Hubble Space Telescope and the Gamma Ray Observatory, and will be launched in a highly eccentric orbit, in 1998. The AXAF payload contains a Wolter-type I high resolution mirror assembly (HRMA) two insertable grating systems, the high energy transmission grating (HETG) and the low energy transmission grating (LETG) and two imaging detector systems. The LETG is being developed in a collaborative effort between SRON and MPE.

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