Wide Field Multiband Imaging of Low Redshift Quasar Environments
arXiv:1504.03401 · doi:10.1088/0004-637X/800/2/93
Abstract
We present photometry of the large scale environments of a sample of twelve broad line AGN with from deep images in the SDSS , , , and filters taken with the 90Prime prime focus camera on the Steward Observatory Bok Telescope. We measure galaxy clustering around these AGN using two standard techniques: correlation amplitude (B) and the two point correlation function. We find average correlation amplitudes for the 10 radio quiet objects in the sample equal to (918, 144114, -3956, 295260) Mpc in (, , , ), all consistent with the expectation from galaxy clustering. Using a ratio of the galaxy-quasar cross-correlation function to the galaxy autocorrelation function, we calculate the relative bias of galaxies and AGN, . The bias in the band, is larger compared to that calculated in the other bands, but it does not correlate with AGN luminosity, black hole mass, or AGN activity via the luminosity of the [OIII] emission line. Thus ongoing nuclear accretion activity is not reflected in the large scale environments from 10 h kpc to 0.5 h Mpc and may indicate a non-merger mode of AGN activity and/or a significant delay between galaxy mergers and nuclear activity in this sample of mostly radio quiet quasars.
arXiv comment23 pages, 17 figures; Accepted for publication in the Astrophysical Journal; Table 2 available as a machine readable table in online article
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