2006/02/17 by A. T. Steffen, Iskra Strateva, I. Strateva +9 · 17 citations
Physics and Astronomy · #Active galactic nucleus #Astronomy #Astrophysical Phenomena and Observations #Astrophysics #Galaxies: Formation, Evolution, Phenomena #Galaxy #Gamma-ray bursts and supernovae #Luminosity #Physics #Population #Quasar #Redshift #Redshift survey #Sky #Universe #astro-ph
paper · pdf · doi:10.1086/503627
published as Astron.J.131:2826-2842,2006 · 16 pages, 10 figures, emulateapj. Accepted for publication in AJ
arxiv created 2006/02/17 · openalex publication_date 2006/06/01 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/06
We present partial-correlation analyses that examine the strengths of the relationships between l 2500 Å , l 2 keV , α OX , and redshift for optically selected active galactic nuclei (AGNs). We extend the work of Strateva and coworkers, which analyzed optically selected AGNs from the Sloan Digital Sky Survey (SDSS), by including 52 moderate-luminosity, optically selected AGNs from the COMBO-17 survey with corresponding deep (≈250 ks to 1 Ms) X-ray observations from the Extended Chandra Deep Field-South. The COMBO-17 survey extends ∼3 mag deeper than the SDSS and probes the moderate-luminosity AGNs that numerically dominate the AGN population in the universe. We also include recently published observations of 19 high-redshift, optically selected AGNs and 46 luminous, low-redshift AGNs from the Bright Quasar Survey. The full sample used in our analysis consists of 333 AGNs, extending out to z ∼ 6, with 293 (88%) having X-ray detections. The sample spans five decades in UV luminosity and four decades in X-ray luminosity. We confirm that α OX is strongly anticorrelated with l 2500 Å (13.6 σ), the highest significance found for this relation to date, and find evidence suggesting that the slope of this relation may be dependent on l 2500 Å . We find that no significant correlation exists between α OX and redshift (1.3 σ) and constrain the maximum evolution of AGN UV-to-X-ray flux ratios to be less than 30% (1 σ) out to z = 5. Using our sample's high X-ray detection fraction, we also find a significant anticorrelation (3.0 σ) between α OX and l 2 keV . We make comparisons to earlier studies on this topic and discuss implications for X-ray and optical AGN luminosity functions.