# Low redshift AGN in the Hamburg/ESO Survey: I. The local AGN luminosity function

## TL;DR

This paper determines the local luminosity function of optically selected type 1 AGN using the Hamburg/ESO Survey, revealing a double power law shape and evidence for luminosity-dependent evolution consistent with AGN downsizing.

## Contribution

It provides the first comprehensive local AGN luminosity function spanning over four orders of magnitude, combining HES and SDSS data, and compares optical and X-ray luminosity functions.

## Key findings

- The AGN luminosity function follows a double power law with slopes -2.0 and -2.8.
- There is a smooth transition between Seyfert 1 and more luminous AGN.
- Evidence supports luminosity-dependent evolution, consistent with AGN downsizing.

## Abstract

We present a determination of the local (z=0) luminosity function of optically selected type 1 (broad-line) Active Galactic Nuclei. Our primary resource is the Hamburg/ESO Survey (HES), which provides a well-defined sample of more than 300 optically bright AGN with redshifts z<0.3 and blue magnitudes B<17.5. AGN luminosities were estimated in two ways, always taking care to minimise photometric biases due to host galaxy light contamination. Firstly, we measured broad-band B_J (blue) magnitudes of the objects over small apertures of the size of the seeing disk. Secondly, we extracted H alpha and H beta broad emission line luminosities from the spectra which should be entirely free of any starlight contribution. The resulting AGN luminosity function (AGNLF) is consistent with a single power law, also when considering the effects of number density evolution within the narrow redshift range. We compared our AGNLF with the H alpha luminosity function of lower luminosity Seyfert 1 galaxies by Hao et al. (2005) and found a smooth transition between both, with excellent agreement in the overlapping region. From the combination of HES and SDSS samples we constructed a single local AGNLF spanning more than 4 orders of magnitude in luminosity. It shows only mild curvature which can be well described as a double power law with slope indices of -2.0 for the faint end and -2.8 for the bright end. We predicted the local AGNLF in the soft X-ray domain and compared this to recent literature data. We also compared the local AGNLF with results obtained at higher redshifts and find strong evidence for luminosity-dependent evolution, in the sense that AGN with luminosities around M_B~-19 are as common in the local universe as they were at z=1.5, supporting the 'AGN downsizing' picture (abridged).