The ROSAT autocorrelation function of the X ray background

Details The ROSAT autocorrelation function of the X ray background The ROSAT autocorrelation function of the X ray background

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992xrea.conf..368g&link_type=abstract

In MPI für Extraterrestrische Physik, X Ray Emission from Active Galactic Nuclei and the Cosmic X Ray Background p 368-372 (SEE

Astronomy and Astrophysics

Astronomy

1

Autocorrelation, Background Radiation, Cosmic X Rays, Rosat Mission, X Ray Astronomy, X Ray Spectra, Active Galactic Nuclei, Starburst Galaxies

Scientific paper

The Autocorrelation Function (ACF) of the x-ray background on arcminute angular scales using about 30 ksec Rosat exposures were derived. No significant signal was detected with the ACF being consistent with zero at all angular scales. The constraints that the upper limit on the ACF places on the contribution of active galactic nuclei and starbursts on the 0.5 to 2 keV background are discussed.

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