X-ray luminosity functions of different morphological and X-ray type AGN populations

TL;DR

This paper presents X-ray luminosity functions of AGN across different morphological and X-ray types, revealing luminosity evolution up to redshift 1.4, with type-1 sources dominating at higher luminosities.

Contribution

It provides detailed luminosity functions for various AGN populations and confirms luminosity evolution without density evolution up to z<1.4.

Findings

Strong luminosity evolution observed in all bands.

No evidence of density evolution in tested bands.

Type-1 AGN are more numerous at higher luminosities.

Abstract

Luminosity functions are one of the most important observational clues when studying galaxy evolution over cosmic time. In this paper we present the X-ray luminosity functions of X-ray detected AGN in the SXDS and GWS fields. The limiting fluxes of our samples are 9.0x10^(-15) and 4.8x10^(-16) erg/cm^2/sec^(-1) in the 0.5 - 7.0 keV band in the two fields, respectively. We carried out analysis in three X-ray bands and in two redshift intervals up to z < 1.4. Moreover, we derive the luminosity functions for different optical morphologies and X-ray types. We confirm strong luminosity evolution in all three bands, finding the most luminous objects at higher redshift. However, no signs of density evolution are found in any tested X-ray band. We obtain similar results for compact and early-type objects. Finally, we observe the `Steffen effect', where X-ray type-1 sources are more numerous at higher luminosities in comparison with type-2 sources.