The Radio/Optical Catalog of the SSA13 Field
arXiv:astro-ph/0607058 · doi:10.1086/508169
Abstract
We present a 1.4-GHz catalog of 810 radio sources (560 sources in the complete sample) with 1.8" resolution found within a 17' radius in the SSA13 field (RA=13h12m,DEC=42d38'). The radio image from the VLA has an rms noise level of 4.82 microJy/beam at the field center, and Subaru optical images in r-band (6300A) and z-band (9200A) have a three-sigma detection magnitude of 26.1 and 24.9, respectively. 88% of the radio sources are identified with an optical counterpart, and there is significantly more reddening for objects fainter than 24-mag. The radio and optical parameters are tabulated, and source morphologies are displayed by radio contours overlaying optical false-color images. The radio structures show a wealth of complexity and these are classified into a small number of categories. About one-third of the radio sources are larger than 1.2" and their orientation is often similar to that of the associated galaxy or binary-galaxy system. The density of sources in the SSA13 field above 75 microJy is 0.40 per square arcmin, with a slope of -2.43 in the differential counts. The radio spectral index may steepen for sources below 75 microJy. We estimate that at most 40% of the microJansky radio sources are dominated by AGN processes.
arXiv comment50 pages, 14 figures of which fig 6 contains 33 parts. In press, Astrophysical Journal, Suppl
References in corpus (13)
- The VLBA Calibrator Survey - VCS1
- The Nature of Radio Emission from Distant Galaxies: The 1.4 GHz Observations
- Radio Emission from Galaxies In The Hubble Deep Field
- High Resolution Studies of Radio Sources in the Hubble Deep and Flanking Fields
- Starburst in the Ultra-luminous Galaxy Arp 220 - Constraints from Observations of Radio Recombination Lines and Continuum
- A Deep VLA survey at 20cm of the ISO ELAIS survey regions
- The Micro-Jansky Sky at 8.4 GHz
- The Evolution of the Ultraluminous Infrared Galaxy Population from Redshift 0 to 1.5
- The Phoenix Deep Survey: spectroscopic catalog
- AGN and starbursts at high redshift: High resolution EVN radio observations of the Hubble Deep Field
- Deep VLBI Imaging of Faint Radio Sources in the NOAO Bootes Field
- Deep Radio Continuum Studies with the SKA: Evolution of Radio AGN Populations
- The Phoenix Deep Survey: Optical and near infrared imaging catalogs
Cited by in corpus (56)
- The VLA-COSMOS Survey: II. Source Catalog of the Large Project
- Radio and Millimeter Continuum Surveys and their Astrophysical Implications
- LOFAR 150-MHz observations of the Boötes field: Catalogue and Source Counts
- The LOFAR Two Meter Sky Survey: Deep Fields, I -- Direction-dependent calibration and imaging
- HI intensity mapping : a single dish approach
- Cosmic evolution of submillimeter galaxies and their contribution to stellar mass assembly
- The VLA-COSMOS Survey. IV. Deep Data and Joint Catalog
- The Stellar Mass Content of Submillimeter-Selected Galaxies
- Precision Astrometry with the Very Long Baseline Array: Parallaxes and Proper Motions for 14 Pulsars
- The Star Formation History of the Universe as Revealed by Deep Radio Observations
- An excess of dusty starbursts related to the Spiderweb galaxy
- The star-formation history of K-selected galaxies
- A new method to separate star forming from AGN galaxies at intermediate redshift: The submillijansky radio population in the VLA-COSMOS survey
- The Deep SWIRE Field I. 20cm Continuum Radio Observations: A Crowded Sky
- VLA 1.4GHz observations of the GOODS-North Field: Data Reduction and Analysis
- The VLA-COSMOS Survey: III. Further Catalog Analysis and the Radio Source Counts
- Precise Identifications of Submillimeter Galaxies: Measuring the History of Massive Star-Forming Galaxies to z>5
- The VLA-COSMOS Perspective on the IR-Radio Relation. I. New Constraints on Selection Biases and the Non-Evolution of the IR/Radio Properties of Star Forming and AGN Galaxies at Intermediate and High Redshift
- Far-infrared and Molecular CO Emission From the Host Galaxies of Faint Quasars at z~6
- The VLA Survey of the Chandra Deep Field South: I. Overview of the Radio Data
- Millimeter and Radio Observations of z~6 Quasars
- The LOFAR Two-metre Sky Survey Deep Fields Data Release 1: V. Survey description, source classifications and host galaxy properties
- The discovery of a highly accreting, radio-loud quasar at z=6.82
- Simulations for single-dish intensity mapping experiments
- The Lockman Hole Project: new constraints on the sub-mJy source counts from a wide-area 1.4 GHz mosaic
- Sources of the Radio Background Considered
- Predictions for Herschel from LambdaCDM: unveiling the cosmic star formation history
- Sample variance, source clustering and their influence on the counts of faint radio sources
- Contribution to the Diffuse Radio Background from Extragalactic Radio Sources
- An Accurate Position for HDF 850.1: The Brightest Submillimeter Source in the Hubble Deep Field-North
- ATLAS 1.4 GHz Data Release 2 -- II. Properties of the faint polarized sky
- Molecular Gas in Submillimetre-Faint, Star-Forming Ultraluminous Galaxies at z>1
- The Deep SWIRE Field. IV. First properties of the sub-mJy galaxy population: redshift distribution, AGN activity and star formation
- The Deep SWIRE Field II. 90cm Continuum Observations and 20cm-90cm Spectra
- MIGHTEE: Deep 1.4 GHz Source Counts and the Sky Temperature Contribution of Star Forming Galaxies and Active Galactic Nuclei
- An Extremely Deep Wide-Field Near-Infrared Survey: Bright Galaxy Counts and Local Large Scale Structure
- The star-formation history of mass-selected galaxies from the VIDEO survey
- Photometric Catalogue of Quasars and Other Point Sources in the Sloan Digital Sky Survey
- A deep radio survey of the AKARI North Ecliptic Pole Field - WSRT 20 cm Radio survey description, observations and data reduction
- A deep ATCA 20cm radio survey of the AKARI Deep Field South near the South Ecliptic Pole
- Associating Fast Radio Bursts with Extragalactic Radio Sources: General Methodology and a Search for a Counterpart to FRB 170107
- Unveiling Far-Infrared Counterparts of Bright Submillimeter Galaxies Using PACS Imaging
- The cosmic radio background from 150 MHz--8.4 GHz, and its division into AGN and star-forming galaxy flux
- Radio and millimeter properties of Ly emitters in the COSMOS field: limits on radio AGN, submm galaxies, and dust obscuration
- A deep 1.4 GHz survey of the J1030 equatorial field: a new window on radio source populations across cosmic time
- VLBA+GBT observations of the COSMOS field and radio source counts at 1.4 GHz
- The Contribution of Active Galactic Nuclei to the Microjansky Radio Population
- Deep observations of the Super-CLASS super-cluster at 325 MHz with the GMRT: the low-frequency source catalogue
- GMRT 610-MHz observations of the faint radio source population - and what these tell us about the higher-radio-frequency sky
- The XXL Survey : XXVI. Optical and near-infrared identifications of the ATCA 2.1 GHz radio sources in the XXL-S Field
- Are Active Galactic Nuclei the Solution to the Excess Cosmic Radio Background at 1.4 GHz?
- Observability of the virialization phase of spheroidal galaxies with radio arrays
- Searching for obscured AGN in z 2 submillimetre galaxies
- A first quantification of the effects of absorption for HI Intensity Mapping experiments
- The FIRST radio survey: Panchromatic properties of FIRST radio sources identified in the Bootes and Cetus fields
- Kiloparsec-scale imaging of the CO(1-0)-traced cold molecular gas reservoir in a z~3.4 submillimeter galaxy