Signals from the Noise: Image Stacking for Quasars in the FIRST Survey
arXiv:astro-ph/0607335 · doi:10.1086/507700
Abstract
We present a technique to explore the radio sky into the nanoJansky regime by employing image stacking using the FIRST survey. We first discuss the non-intuitive relationship between the mean and median values of a distribution that is dominated by noise, followed by an analysis of the systematic effects present in FIRST's 20cm VLA snapshot images. Image stacking allows us to recover the properties of source populations with fluxes a factor of 30 or more below the rms noise level. Mean estimates of radio flux density, luminosity, etc., are derivable for any source class having arcsecond positional accuracy. We use this technique to compute the mean radio properties for 41,295 quasars from the SDSS DR3 catalog. There is a tight correlation between optical and radio luminosity, with the radio luminosity increasing as the 0.85 power of optical luminosity. This implies declining radio-loudness with optical luminosity: the most luminous objects (M=-28.5) have average radio-to-optical ratios 3 times lower than the least luminous objects (M=-20). There is also a striking correlation between optical color and radio loudness: quasars that are either redder or bluer than the norm are brighter radio sources, with objects 0.8 magnitudes redder than the SDSS composite spectrum having radio-loudness ratios that are higher by a factor of 10. We explore the longstanding question of whether a radio-loud/radio-quiet dichotomy exists in quasars, finding that optical selection effects probably dominate the distribution function of radio loudness, which has at most a modest (~20%) inflection between the radio-loud and radio-quiet ends of the distribution. We also find, surprisingly, that broad absorption line quasars have higher mean radio flux densities, with the greatest disparity arising in the rare low-ionization BAL subclass.
17 pages, 19 figures, accepted by ApJ; corrected error in absolute magnitudes
Cited by in corpus (25)
- An Observational Determination of the Bolometric Quasar Luminosity Function
- The Influence of Magnetic Field Geometry on the Evolution of Black Hole Accretion Flows: Similar Disks, Drastically Different Jets
- Evidence for Quasar Activity Triggered by Galaxy Mergers in HST Observations of Dust-reddened Quasars
- The Radio-Loud Fraction of Quasars is a Strong Function of Redshift and Optical Luminosity
- On the origin of radio emission in radio quiet quasars
- The Coincidence of Nuclear Star Clusters and Active Galactic Nuclei
- The Co-Formation of Spheroids and Quasars Traced in their Clustering
- New Insights on the QSO Radio-Loud/Radio-Quiet Dichotomy: SDSS Spectra in the Context of the 4D Eigenvector1 Parameter Space
- A Full Year's Chandra Exposure on SDSS Quasars from the Chandra Multiwavelength Project
- Star formation rates in Lyman break galaxies: radio stacking of LBGs in the COSMOS field and the sub-Jy radio source population
- On the origin of radio core emission in radio-quiet quasars
- Dependence of the BALQSO fraction on Radio Luminosity
- Black hole spin and radio loudness in a LCDM universe
- Radio Properties of Low Redshift Broad Line Active Galactic Nuclei
- The Young and the Dustless: Interpreting Radio Observations of UltraViolet Luminous Galaxies
- Radio source stacking and the infrared / radio correlation at microJy flux densities
- Radio Detection of Radio-Quiet Galaxies
- Deep 610-MHz Giant Metrewave Radio Telescope observations of the Spitzer extragalactic First Look Survey field - III. The radio properties of Infrared-Faint Radio Sources
- Radio AGN in 13,240 galaxy clusters from the Sloan Digital Sky Survey
- The Radio Luminosity Function and Galaxy Evolution in the Coma Cluster
- FIRST-based survey of Compact Steep Spectrum sources, V. Milliarcsecond-scale morphology of CSS objects
- Star-Formation in Low Radio Luminosity AGN from the Sloan Digital Sky Survey
- The NIR to UV continuum of radio loud vs. radio quiet quasars
- Radio-loudness of Active Galaxies and the Black Hole Evolution
- Active Galaxies in the Sloan Digital Sky Survey II: galaxy and activity evolution