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5. Concluding remarks

The X-ray catalogue derived from the medium deep ROSAT Survey in HS 47.5/22 contains in total 574
X-ray sources with likelihoods tex2html_wrap_inline1821 and broad band fluxes tex2html_wrap_inline2147.

The analyses of both individual pointings and merged data were proven to be necessary to find all the X-ray sources in the field. As a completeness test for the catalogue, the tex2html_wrap_inline2149-curve was created and compared with the literature (Molthagen 1996). We found that for sources with tex2html_wrap_inline2151, our catalogue is of comparable completeness with previous works down to a broad band flux tex2html_wrap_inline2153; details of this and other results (e.g. variability) will be given elsewhere (Molthagen, in preparation).

Acknowledgements

We wish to thank the HQS group for their readiness to share experience and software, and especially for giving access to their data prior to publication. KM wishes to thank N. Bade for his help with the follow-up observations, and the MPE Garching for the possibility to perform the merging of the X-ray pointings, and analysis thereof, in Garching. We acknowledge that C. Feldt performed and reduced the 100m RT 21cm line observations.
This work has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.
Part of this work was supported by a grant from the BMFT (DARA FKZ 50OR9308).



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