An Optical/Near-Infrared Study of Radio-Loud Quasar Environments II. Imaging Results
arXiv:astro-ph/9806151 · doi:10.1086/306349
Abstract
We use optical and near-IR imaging to examine the properties of the significant excess population of K>=19 galaxies found in the fields of 31 z=1-2 radio-loud quasars by Hall, Green & Cohen (1998). The excess occurs on two spatial scales: a component at <40'' from the quasars significant compared to the galaxy surface density at >40'' in the same fields, and a component roughly uniform to ~100'' significant compared to the galaxy surface density seen in random-field surveys in the literature. The r-K color distributions of the excess galaxy populations are indistinguishable and are significantly redder than the color distribution of the field population. The excess galaxies are consistent with being predominantly early-type galaxies at the quasar redshifts, and there is no evidence that they are associated with intervening MgII absorption systems. The average excess within 0.5 Mpc (~65'') of the quasars corresponds to Abell richness class ~0 compared to the galaxy surface density at >0.5 Mpc from the quasars, and to Abell richness class ~1.5 compared to that from the literature. We discuss the spectral energy distributions (SEDs) of galaxies in fields with data in several passbands. Most candidate quasar-associated galaxies are consistent with being 2-3 Gyr old early-types at the quasar redshifts of z~1.5. However, some objects have SEDs consistent with being 4-5 Gyr old at z~1.5, and a number of others are consistent with ~2 Gyr old but dust-reddened galaxies at the quasar redshifts. These potentially different galaxy types suggest there may be considerable dispersion in the properties of early-type cluster galaxies at z~1.5. There is also a population of galaxies whose SEDs are best modelled by background galaxies at z>2.5.
Accepted to ApJ; 54 pages including 30 figures; 2 color GIF files available separately; also available from http://www.astro.utoronto.ca/~hall/thesis.html
References in corpus (17)
- A Large Structure of Galaxies At Redshift z~3 and its Cosmological Implications
- The Evolution of Early-Type Galaxies in Distant Clusters
- The Age Of Globular Clusters In Light Of Hipparcos: Resolving the Age Problem?
- Hubble Space Telescope imaging of the CFRS and LDSS redshift surveys II: Structural parameter and the evolution of disk galaxies to z=1
- Optical-IR Spectral Energy Distributions of z>2 Lyman Break Galaxies
- HST imaging of CFRS and LDSS galaxies - I: Morphological Properties
- HST, radio and infrared observations of 28 3CR radio galaxies at redshift z ~ 1: I. Old stellar populations in central cluster galaxies
- Galaxy-Galaxy Lensing in the Hubble Deep Field: The Halo Tully-Fisher Relation at Intermediate Redshift
- An IR-Selected Galaxy Cluster at z=1.27
- A maximum-likelihood method for improving faint source flux and color estimates
- The Norris Survey of the Corona Borealis Supercluster: III. Structure and Mass of the Supercluster
- Deep WFPC2 and Ground-based Imaging of a Complete Sample of 3C Quasars and Galaxies
- The ESO K'-band Galaxy Survey - Galaxy Counts
- Morphology and Surface Brightness Evolution of z\sim1.1 Radio Galaxies
- Infrared emission-line galaxies associated with damped Lyman-alpha and strong metal absorber redshifts
- The Clustering of K\sim 20 Galaxies on 17 Radio Galaxy Fields
- On the Dust Extinction in High-z Galaxies and the Case of Extremely Red Objects
Cited by in corpus (51)
- The Evolution of X-ray Clusters of Galaxies
- Binary Quasars in the Sloan Digital Sky Survey: Evidence for Excess Clustering on Small Scales
- An X-ray Selected Galaxy Cluster at z=1.26
- Joint Cosmological Formation of QSOs and Bulge-dominated Galaxies
- Extended Lyman alpha emission around bright quasars
- The Habitat Segregation between Lyman Break Galaxies and Lyman alpha Emitters around a QSO at z~5
- The cluster environments of powerful radio-loud and radio-quiet AGN
- Clustering of galaxies around radio quasars at 0.5 < z < 0.8
- The HELLAS2XMM survey. V. Near-Infrared observations of X-ray sources with extreme X/O ratios
- Red galaxy overdensities and the varied cluster environments of powerful radio sources with z~1.6
- High redshift FRII radio sources: large-scale X-ray environment
- The CORALS Survey II: Clues to Galaxy Clustering Around QSOs from z_abs ~ z_em Damped Lyman Alpha Systems
- Properties of galaxies in SDSS Quasar environments at z < 0.2
- Radio-quiet quasar environments at 0.5 < z < 0.8
- An H-alpha search for over-dense regions at z=2.23
- Galaxy Population in a Cluster of Galaxies around the Radio Galaxy 3C 324 at z=1.2
- Extremely Red Objects in the Field of QSO 1213-0017: A Galaxy Concentration at z=1.31
- Environment of MAMBO galaxies in the COSMOS field
- Overdensities of Extremely Red Objects in the Fields of High-Redshift Radio-Loud Quasars
- Very Red and Extremely Red Galaxies in the Fields of z ~ 1.5 Radio-Loud Quasars
- An Optical/Near-Infrared Study of Radio-Loud Quasar Environments I. Methods and z=1-2 Observations
- A Study of High-redshift AGN Feedback in SZ Cluster Samples
- Cluster of galaxies around seven radio-loud QSOs at 1<z<1.6: K-band images
- An excess of damped Lyman alpha galaxies near QSOs
- Searching High Redshift Large-Scale Structures: Photometry of Four Fields Around Quasar Pairs at z~1
- Near-Infrared Observations of the Environments of Radio Quiet QSOs at z >~ 1
- A Rich Cluster of Galaxies Near the Quasar B2 1335+28 at z=1.1: Color Distribution and Star-Formation Properties
- The density of extremely red objects around high-z radio-loud AGN
- The cluster environments of radio-loud quasars at 0.6 < z < 1.1
- Radio galaxy selected clusters at high redshift and associated ERO overdensities
- The Galaxy Environment of a Quasar at z=1.226: A Possible Cluster Merger
- Number Counts of Bright Extremely Red Objects: Evolved Massive Galaxies at z~1
- The candidate cluster and protocluster catalog (CCPC) of spectroscopically identified structures spanning
- The environments of hyperluminous infrared galaxies at 0.44<z<1.55
- Search for Galaxy Clustering around a Quasar Pair at z=4.25 found in the Sloan Digital Sky Survey
- Tunable-filter imaging of quasar fields at z~1. I. A cluster around MRC B0450-221
- The Spitzer Extragalactic Representative Volume Survey (SERVS): The Environments of High-z SDSS Quasi-Stellar-Objects
- The Clustering of AGN and Galaxies at Intermediate Redshift
- The DRaGONS Survey: A Search for High Redshift Radio Galaxies And Heavily Obscured AGNs
- Properties of Extremely Red Objects in an Overdense Region
- Tunable-filter imaging of quasar fields at z ~ 1. II. The star-forming galaxy environments of radio-loud quasars
- The X-ray luminous cluster underlying the z = 1.04 quasar PKS1229-021
- B3 0003+387: AGN Marked Large-Scale Structure at z=1.47?
- Morphologies in a Cluster of Extremely Red Galaxies with Old Stellar Populations at z=1.34
- An Overdensity of Extremely Red Objects Around Faint Mid-IR galaxies
- Red Companions to a z=2.15 Radio Loud Quasar
- Evolution of Lyman Break Galaxies Beyond Redshift Four
- Three candidate clusters around high redshift radio-loud sources: MG1 J04426+0202, 3C 068.2, MS 1426.9+1052
- Triplets of Quasars at high redshift I: Photometric data
- The distant red galaxy neighbour population of 1 < z < 2 QSOs and optically obscured sources
- Clustering around radio galaxies at z~1.5