  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.
