IPAC, located on the Caltech campus, is not under direct threat from local fires at this time, though it is subject to the effects of strong winds and poor air quality. Many members of the IPAC community have been impacted by these events, and IPAC will follow Caltech guidance on closures and safe operations. For more information, visit Caltech’s Emergency Updates page at http://www.caltech.edu/emergency.
Asteroidscomets

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

September 2024 • 2024ApJ...972...89J

Authors • Jiménez-Andrade, Eric F. • Murphy, Eric J. • Momjian, Emmanuel • Condon, James J. • Chary, Ranga-Ram • Taylor, Russ • Dickinson, Mark

Abstract • We present the first high-resolution, high-frequency radio continuum survey that fully maps an extragalactic deep field: the 10 GHz 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 (VLA) that allocated 380 hr of observations using the X-band (8–12 GHz) receivers, leading to a 10 GHz mosaic of the GOODS-N field with an average rms noise σ n = 671 nJy beam‑1 and angular resolution θ 1/2 = 0.″22 across 297 arcmin2. To maximize the brightness sensitivity we also produce a low-resolution mosaic with θ 1/2 = 1.″0 and σ n = 968 nJy beam‑1, from which we derive our master catalog containing 256 radio sources detected with peak signal-to-noise ratio ≥ 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 10 GHz radio source counts in the GOODS-N field agree, in general, with predictions from numerical simulations/models and expectations from 1.4 and 3 GHz radio counts. * https://science.nrao.edu/science/surveys/vla-x-gn/home

Links


IPAC Authors
(alphabetical)