Stripe 82 X: Archival XMM Newton- And Chandra-selected AGN In SDSS Stripe 82

Other

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

Multiwavelength surveys have proved very powerful tools for studying galaxies, AGN, and clusters. A "wedding cake" (i.e., tiered) strategy of depth and area samples a wide range of luminosity and redshift, essential for disentangling evolution- and mass-based effects. The study of AGN requires X-rays, and deep X-ray surveys have been a critical part of highly productive multiwavelength surveys like GOODS, COSMOS, Lockman, AEGIS, MUSYC, and Bootes. Most of these surveys cover too small an area to sample rare objects like high luminosity or high redshift AGN, however, so larger surveys are needed to those regimes. Using archival XMM and Chandra data in Stripe 82, along with SDSS spectra and other multiwavelength data for cross-matched sources, we present AGN number counts and the redshift and luminosity distributions. These data constrain the luminosity function and evolution of X-ray-selected AGN in areas of parameter space that have been poorly sampled to date.

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

Stripe 82 X: Archival XMM Newton- And Chandra-selected AGN In SDSS Stripe 82 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 Stripe 82 X: Archival XMM Newton- And Chandra-selected AGN In SDSS Stripe 82, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stripe 82 X: Archival XMM Newton- And Chandra-selected AGN In SDSS Stripe 82 will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1576890

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