Co-moving space density of x-ray-selected active galactic nuclei
Jun, 20044 pages
Published in:
- Astrophys.J. 624 (2005) 630-637
e-Print:
- astro-ph/0406330 [astro-ph]
DOI:
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Abstract: (arXiv)
For measurement of the AGN luminosity function and its evolution, X-ray selection samples all types of AGN and provides reduced obscuration bias in comparison with UV-excess or optical surveys. The apparent decline in optically-selected quasars above z~3 may be strongly affected by such a bias. The Chandra Multiwavelength Project (ChaMP) is characterizing serendipitously detected X-ray sources in a large number of fields with archival Chandra imaging. We present a preliminary measure of the co-moving space density using a sample of 311 AGN found in 23 ChaMP fields (~1.8 deg^2) supplemented with 57 X-ray bright AGN from the CDF-N and CDF-S. Within our X-ray flux (f(0.3-8.0 keV) > 4x10^-15 erg cm^-2 s^-1) and optical magnitude (r' < 22.5) limits, our sample includes 14 broad emission line AGN at z > 3. Using this X-ray selected sample, we detect a turnover in the co-moving space density of luminous type 1 AGN (log Lx > 44.5: units erg s^-1: measured in the 0.3-8.0 keV band and corrected for Galactic absorption) at z > 2.5. Our X-ray sample is the first to show a behavior similar to the well established evolution of the optical quasar luminosity function. A larger sample of high redshift AGN and with a greater fraction of identified sources, either spectroscopic or photometric, at faint optical magnitudes (r' > 22.5) are required to remove the remaining uncertainty in our measure of the X-ray luminosity function. We confirm that for z < 1, lower luminosity AGN (log Lx < 44.5) are more prevalent by more than an order of magnitude than those with high luminosity. We have combined the Chandra sample with AGN from the ROSAT surveys to present a measure of the space density of luminous type 1 AGN in the soft X-ray band (0.5-2.0 keV) which confirms the broad band turnover described above.- galaxies: active
- quasars: general
- surveys
- X-rays: galaxies
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