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A Census of the Deep Radio Sky with the VLA I: 10GHz Survey of the GOODS-N field

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arxiv 2406.13801 v1 pith:SCCHJLYA submitted 2024-06-19 astro-ph.GA

classification astro-ph.GA
keywords radiocatalogfielddeepgoods-nmosaicsurveyarcsec
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

We present the first high-resolution, high-frequency radio continuum survey that fully maps an extragalactic deep field: the 10GHz survey of the Great Observatories Origins Deep Survey-North (GOODS-N) field. This is a Large Program of the Karl G. Jansky Very Large Array that allocated 380 hours of observations using the X-band ($8-12$GHz) receivers, leading to a 10GHz mosaic of the GOODS-field with an average rms noise $\sigma_{\rm n}=671\,\rm nJy\,beam^{-1}$ and angular resolution $\theta_{1/2}=0.22$arcsec across 297$\rm arcmin^2$. To maximize the brightness sensitivity we also produce a low-resolution mosaic with $\theta_{1/2}=1.0$arcsec and $\sigma_{\rm n}=968\,\rm nJy\,beam^{-1}$, from which we derive our master catalog containing 256 radio sources detected with peak signal-to-noise ratio $\geq 5$. Radio source size and flux density estimates from the high-resolution mosaic are provided in the master catalog as well. The total fraction of spurious sources in the catalog is 0.75%. Monte Carlo simulations are performed to derive completeness corrections of the catalog. We find that the 10GHz radio source counts in the GOODS-N field agree, in general, with predictions from numerical simulations/models and expectations from 1.4 and 3GHz radio counts.

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Cited by 1 Pith paper

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  1. The Zero-Age Massive Stellar Population of W49A from VLA Observations

    astro-ph.GA 2026-08 conditional novelty 6.0 of 10

    The high-mass stellar population of W49A, traced by 101 H II regions, shows a steep mass function slope (Gamma > 2.5) compared to the standard Salpeter slope of 1.35, implying a deficit of the most massive stars.

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