Radio-quiet objects in the 2QZ survey
Abstract
Co-addition of blank-field FIRST data at the location of over 8000 QSOs in the 2QZ survey has yielded statistical detections of radio quiet QSOs with median flux levels of 20-40microJy. We show that the total radio flux of radio-quiet QSOs in the 2QZ is consistent with a smooth extrapolation of the 2QZ radio-loud QSO number-flux distribution based on the slope of the relation flattening near the FIRST flux limit. However, we are unable to distinguish a smooth extrapolation of the luminosity function to faint levels from a bimodal luminosity function with a break close to or below the FIRST radio detection limit. We also demonstrate that the redshift dependence of the median radio-to-optical spectral index for these radio quiet QSOs is consistent with that obtained for individual radio-loud 2QZ QSOs detected by FIRST.
Cite
@article{arxiv.astro-ph/0502401,
title = {Radio-quiet objects in the 2QZ survey},
author = {M. Wals and B. J. Boyle and S. M. Croom and L. Miller and R. Smith and T. Shanks and P. Outram},
journal= {arXiv preprint arXiv:astro-ph/0502401},
year = {2011}
}
Comments
MNRAS accepted, 5 pages, 5 figures