Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..951k&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 951-956 (SEE N90-258
Astronomy and Astrophysics
Astrophysics
1
Active Galactic Nuclei, Computerized Simulation, High Resolution, Spectral Resolution, X Ray Spectra, Background Radiation, European Space Programs, Galactic Radiation, Nasa Space Programs, Performance Prediction, X Ray Astrophysics Facility, X Ray Spectroscopy
Scientific paper
The improvements in spectral resolution and sensitivity in soft X-rays detection by NASA's Advanced X-ray Astrophysics Facility (AXAF) and ESA's X-ray Multi-Mirror Mission (XMM) are underlined. Spectral simulations with 0.05A resolution are performed to investigate the diagnostic capabilities of the XMM reflection grating spectrometer for Active Galactic Nuclei (AGN) spectra. Observations of resolved emission lines and absorption edges in soft X-rays allow a better interpretation of the origins of the different spectral components.
Brinkman Albert C.
Kaastra Jelle S.
Mewe Rolf
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