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19952005
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astro-ph2005

Signs of WHIM in the soft X-ray background

A. M. Soltan, M. J. Freyberg, G. Hasinger

Small angular scale structure of the soft X-ray background correlated with the galaxy distribution is investigated. An extensive data sample from the ROSAT and XMM-Newton archives…

astro-ph2000

Testing the origin of the gamma-ray background

Andrzej M. Soltan, Radoslaw Marcinkowski

Fluctuations of the gamma-ray background (GRB) are investigated. It is assumed that the GRB is produced by discrete sources. Two basic classes of objects as dominant contributors t…

astro-ph1996

Search for correlations between COBE DMR and ROSAT PSPC All-Sky survey data

R. Kneissl, R. Egger, G. Hasinger +2

Results from a cross-correlation analysis between the COBE DMR 4 year, and ROSAT PSPC All-Sky Survey data are presented. Statistical comparisons between microwave and X-ray maps ca…

astro-ph1996

The large scale structure of the soft X-ray background. II: Galaxies

Andrzej M. Soltan, Guenther Hasinger, Roland Egger +2

The intensity of the soft X-Ray background is correlated with the distribution of galaxies. To demonstrate this, magnitude limited galaxy samples extracted from bright galaxy catal…

astro-ph1995

The large scale structure of the soft X-ray background. I: Clusters of galaxies

Andrzej M. Soltan, Guenther Hasinger, Roland Egger +2

Large-scale fluctuations of the X-ray background are investigated using the ROSAT All-Sky Survey. The autocorrelation function of the extragalactic background at 1 keV is determine…