The VLA-COSMOS 3 GHz Large Project: Continuum data and source catalog release

Abstract

We present the VLA-COSMOS 3 GHz Large Project based on 384 hours of observations with the Karl G. Jansky Very Large Array (VLA) at 3 GHz (10 cm) toward the two square degree Cosmic Evolution Survey (COSMOS) field. The final mosaic reaches a median rms of 2.3 uJy/beam over the two square degrees at an angular resolution of 0.75". To fully account for the spectral shape and resolution variations across the broad (2 GHz) band, we image all data with a multiscale, multifrequency synthesis algorithm. We present a catalog of 10,830 radio sources down to 5 sigma, out of which 67 are combined from multiple components. Comparing the positions of our 3 GHz sources with those from the Very Long Baseline Array (VLBA)-COSMOS survey, we estimate that the astrometry is accurate to 0.01" at the bright end (signal-to-noise ratio, S/N_3GHz > 20). Survival analysis on our data combined with the VLA-COSMOS 1.4~GHz Joint Project catalog yields an expected median radio spectral index of alpha=-0.7. We compute completeness corrections via Monte Carlo simulations to derive the corrected 3 GHz source counts. Our counts are in agreement with previously derived 3 GHz counts based on single-pointing (0.087 square degrees) VLA data. In summary, the VLA-COSMOS 3 GHz Large Project simultaneously provides the largest and deepest radio continuum survey at high (0.75") angular resolution to date, bridging the gap between last-generation and next-generation surveys.

arXiv comment19 pages, 18 figures, 5 tables, accepted for publication in A&A

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• Revealing the differences in the SMBH accretion rate distributions of starburst and non-starburst galaxies
• The VLA-COSMOS 3 GHz Large Project: Average radio spectral energy distribution of active galactic nuclei
• The Seahorse Nebula: New views of the filamentary infrared dark cloud G304.74+01.32 from SABOCA, Herschel, and WISE
• Molecular Gas Excitation of the Massive Dusty Starburst CRLE and the Main-Sequence Galaxy HZ10 at z=5.7 in the COSMOS Field
• Going deeper into the dark with COSMOS-Web: JWST unveils the total contribution of Radio-Selected NIRfaint galaxies to the cosmic Star Formation Rate Density
• A Systematic Search for Reddest Far-infrared and Sub-millimeter Galaxies: revealing dust-embedded starbursts at high redshifts
• The XXL Survey. XLI. Radio AGN luminosity functions based on the GMRT $610\mathrm{MHz}$ continuum observations
• How are Red and Blue Quasars Different? The Radio Properties
• The MeerKAT Absorption Line Survey: Homogeneous continuum catalogues towards a measurement of the cosmic radio dipole
• Effect of the environment on star formation activity and stellar mass for star-forming galaxies in the COSMOS field
• COSMOS-Web galaxy groups: Evolution of red sequence and quiescent galaxy fraction
• Revealing the hidden cosmic feast: A z=4.3 galaxy group hosting two optically dark, efficiently star-forming galaxies
• Behind the dust veil: A panchromatic view of an optically dark galaxy at z=4.82
• The ALPINE-ALMA [CII] Survey: Unveiling the baryon evolution in the ISM of $z\sim 5$ star-forming galaxies
• Radio-Optical Galaxy Shape and Shear Correlations in the COSMOS Field using 3 GHz VLA Observations
• What is the origin of the stacked radio emission in radio-undetected quasars?: Insights from a radio-infrared image stacking analysis
• Feedback Factory: Multiple faint radio-jets detected in a cluster at z=2
• Intrinsic alignments of the extended radio continuum emission of galaxies in the EAGLE simulations
• UNIONS Optical Identifications for VLASS Radio Sources in the Euclid Sky (UNVEIL) I. A Catalog of ~146,000 Radio Galaxies up to z~5
• The Radio Spectral Energy Distribution and Star Formation Calibration in MIGHTEE-COSMOS Highly Star-Forming Galaxies at 1.5 < z < 3.5
• The ViCTORIA project: description of a multi-frequency radio survey of the Virgo galaxy cluster
• An ultra-high-resolution map of (dark) matter
• Shapes of galaxies hosting radio-loud AGNs with z \leq 1
• A Ly-alpha nebula at z~3.3
• The ALPINE-ALMA [CII] survey: The infrared-radio correlation and AGN fraction of star-forming galaxies at z $\sim$ 4.4-5.9
• Pulsar B1237+25 Aberration/Retardation Analysis from Decimeter to Decameter Wavelength: Challenge to "Radius-to-Frequency Mapping"
• The Jet Paths of Radio AGN and their Cluster Weather
• The superMIGHTEE project: MeerKAT and GMRT Together to Unveil the Deep Radio Sky
• SEMPER I. Radio Predictions for Star-Forming Galaxies at $0<z<5$
• A High-resolution Far-infrared Survey to Probe Black Hole-Galaxy Co-evolution
• A PAH deficit in the starburst core of a distant spiral galaxy
• Exploring the X-ray-radio connection for AGN via measurements of the multi-dimensional luminosity function
• ULTIMATE-deblending I. A 50-band Ultraviolet to Mid-infrared Photometric Catalog Combining Space- and Ground-based Data in the JWST/PRIMER survey
• The Radio Galaxy Environment Reference Survey (RAGERS): a submillimetre study of the environments of massive radio-quiet galaxies at $z=1-3$
• Deblending the MIGHTEE-COSMOS survey with XID+: The resolved radio source counts to $S_{1.4}\approx 5\mu$Jy
• The evolution of the radio luminosity function of group galaxies in COSMOS
• ALMA measures molecular gas reservoirs comparable to field galaxies in a low-mass galaxy cluster at z=1.3
• Hosts and environments: a (large-scale) radio history of AGN and star-forming galaxies
• An empirical model of the extragalactic radio background
• Properties of Polarized Radio Sources in the Wide Chandra Deep Field South from 2 to 4GHz
• A multiwavelength study of an early galaxy group merger in COSMOS revealed by two tailed radio galaxies at z = 0.35
• Something Bright at the Edge of Everything: A Uniquely JWST-Dark Radio Source in COSMOS
• RadioLensfit: an HPC Tool for Accurate Galaxy Shape Measurement with SKA
• The NIKA2 cosmological legacy survey at 2 mm: catalogs, colors, redshift distributions, and implications for deep surveys
• MIGHTEE: total intensity radio continuum imaging and the COSMOS / XMM-LSS Early Science fields
• An exploration of in-band spectral index techniques for extended radio sources with EMU