Spectroscopy of AGNs with Xspect/Sodart in 1993

Details Spectroscopy of AGNs with Xspect/Sodart in 1993 Spectroscopy of AGNs with Xspect/Sodart in 1993

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296.1077w&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 2: AGN and the X Ray Background p 1077-1079 (SEE N90-2

Computer Science

Performance

Active Galactic Nuclei, Performance Prediction, Spectral Resolution, X Ray Spectroscopy, X Ray Telescopes, Design Analysis, Iron, Line Spectra, Mission Planning, Proportional Counters, Spectrometers, U.S.S.R. Space Program

Scientific paper

The Xspect/Sodart telescope system on board the Soviet mission Spectrum-X scheduled for launch in 1993 is designed for high throughput at 7 keV. One of the two telescopes will be equipped with an objective crystal spectrometer with a spectral resolution of about 5 eV at the 6.7 keV iron line. The prime broad band spectrometer is a solid state pixel detector with resolution of 150 eV which allows good iron line detection for a large number of Active Galactic Nuclei (AGN). Position sensitive gas detectors are included.

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