Precise Determination of the Bright End of the Local Galaxy X-Ray Luminosity Function

Details Precise Determination of the Bright End of the Local Galaxy X-Ray Luminosity Function Precise Determination of the Bright End of the Local Galaxy X-Ray Luminosity Function

Sep 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002cxo..prop.1092p&link_type=abstract

Chandra Proposal ID #04700038

Mathematics

Logic

Chandra Proposal Id #04700038

Scientific paper

The X-ray luminosity function (XLF) of local galaxies and of local AGN was derived from the ROSAT Bright Survey (RBS). Both XLFs are relatively uncertain in the range of 41.0

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