activity
19941998
most citedThe ROSAT-HRI X-Ray Survey of the Cygnus Loop

77 citations · 92 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph1998★ 3 cited

A search for soft X-ray emission associated with prominent high-velocity-cloud complexes

J. Kerp, W. B. Burton, R. Egger +5

We correlate the ROSAT 1/4 keV all-sky survey with the Leiden/Dwingeloo HI survey, looking for soft X-ray signatures of prominent high-velocity-cloud (HVC) complexes. We study the…

astro-ph1997★ 77 cited

The ROSAT-HRI X-Ray Survey of the Cygnus Loop

N. A. Levenson, J. R. Graham, B. Aschenbach +13

We describe and report progress on the joint U.S. and German campaign to map the X-ray emission from the entire Cygnus Loop supernova remnant with the ROSAT High Resolution Imager.…

astro-ph1996★ 2 cited

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★ 1 cited

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-ph1996

A Large-Area Cross-Correlation Study of High Galactic Latutude Soft and Hard X-ray Skies

Takamitsu Miyaji, Guenther Hasinger, Roland Egger +2

We have made cross-correlation analyses of (2 -- 15 keV) HEAO A2 and 1 keV ROSAT PSPC All-Sky Survey maps over a selected area ( 4000 deg) with high galactic latitude (b>…

astro-ph1995★ 9 cited

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…