  The GLOSTAR survey studies star formation with the VLA and the Effelsberg
100m telescope in the Galactic plane (-2d<l<60d; |b|<1d) and the Cygnus X
region with unprecedented sensitivity in both flux density (~50uJy/beam) and
the capability of detecting emission with angular scales in the range from 1"
to the largest radio structures in the Galaxy.
  We provide a complete GLOSTAR-VLA D-configuration radio source catalog for
the covered part of the Galactic disk. A catalog for the pilot region
(28d<l<36d) has been published in a previous paper and here we present the
complementary catalog for the area within 2d<l<28d, 36d<l<60d and |b|<1d.
  Observations were taken with the VLA in a 4-8GHz band to image 100
degrees$^2$ of the inner Galactic disk at a reference frequency of 5.8GHz,
using 260h of telescope time. We determined spectral indices inside the
observed band and in the frequency range 1.4-5.8GHz by complementing our
results with those from the THOR survey (1-2GHz).
  The final images have an angular resolution of 18" and an average sensitivity
of 123uJy/beam. The sensitivity is better (~60uJy/beam) in areas free of
extended emission. The Galactic disk catalog presented in this work, consists
of 11211 radio sources. Of these, 1965 are known large-scale structure sources
such as star-forming region complexes, well-known SNRs, SNR candidates or parts
thereof. The remaining 9227 are discrete individual sources. Source parameters,
namely flux densities, sizes, spectral indices, and classifications are
reported. We identify 769 HII region candidates, 359 are newly classified as
such. The mean value of spectral indices of 225 HII regions is 0.14$\pm$0.02,
consistent with most of them emitting optically thin thermal radio emission.
Combining our results with the previously published catalog of the pilot
region, the final GLOSTAR-VLA D-configuration catalog contains 12981 radio
sources.
