A census of the deep radio sky with the vla. i. 10 ghz survey of the goods-n field

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 that allocated 380 hours of observations using the X-band (8 − 12 GHz) receivers, leading to a 10 GHz mosaic of the GOODS-field with an average rms noise σn = 671 nJy beam−1 and angular resolution θ1/2 = 0. ′′22 across 297 arcmin2 . To maximize the brightness sensitivity we also produce a low-resolution mosaic with θ1/2 = 1. ′′0 and σn = 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.