Wide Area X-ray Surveys for AGN and Starburst Galaxies

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

7 pages, 5 figures. Conference proceedings in "Classification and Discovery in Large Astronomical Surveys", 2008, C.A.L. Baile

Scientific paper

10.1063/1.3059018

While often the point sources in X-ray surveys are dominated by AGN, with the high sensitivity of modern X-ray telescopes such as Chandra and XMM-Newton normal/starburst galaxies are also being detected in large numbers. We have made use of Bayesian statistics for both the selection of galaxies from deep X-ray surveys and in the analysis of the luminosity functions for galaxies. These techniques can be used to similarly select galaxies from wide-area X-ray surveys and to analyze their luminosity function. The prospects for detecting galaxies and AGN from a proposed ``wide-deep'' XMM-Newton survey and from future wide-area X-ray survey missions (such as WFXT and eRosita) are also discussed.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Wide Area X-ray Surveys for AGN and Starburst Galaxies does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Wide Area X-ray Surveys for AGN and Starburst Galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Wide Area X-ray Surveys for AGN and Starburst Galaxies will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-667499

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.