Cosmological Evolution of the Hard X‐Ray Active Galactic Nucleus Luminosity Function and the Origin of the Hard X‐Ray Background
Institute of Space and Astronautical Science · National Astronomical Observatory of Japan · +2 more institutions
Abstract
We investigate the cosmological evolution of the hard X-ray luminosity function (HXLF) of active galactic nuclei (AGNs) in the 2-10 keV luminosity range of 10 41.5 -10 46.5 ergs s 1 as a function of redshift up to 3. From a combination of surveys conducted at photon energies above 2 keV with HEAO 1, ASCA, and Chandra, we construct a highly complete (>96%) sample consisting of 247 AGNs over the wide flux range of 10 10 to 3:8 10 15 ergs cm 2 s 1 (2-10 keV).For our purpose, we develop an extensive method of calculating the intrinsic (before absorption) HXLF and the absorption (N H ) function.This utilizes the maximum likelihood method, fully correcting for observational biases with consideration of the X-ray…
Citation impact
- FWCI
- 43.41
- Percentile
- 100%
- References
- 92
Authors
4Topics & keywords
- Physics
- Astrophysics
- Redshift
- Active galactic nucleus
- Luminosity function
- Luminosity
- Population
- Flux (metallurgy)