New Associations of Gamma-Ray Sources from the Fermi Second Source
  Catalog
  We present the results of an all-sky radio survey between 5 and 9 GHz of the
fields surrounding all unassociated gamma-ray objects listed in the Fermi Large
Area Telescope Second Source Catalog (2FGL). The goal of these observations is
to find all new gamma-ray AGN associations with radio sources >10 mJy at 8 GHz.
We observed with the Very Large Array and the Australia Telescope Compact Array
the areas around unassociated sources, providing localizations of weak radio
point sources found in 2FGL fields at arcmin scales. Then we followed-up a
subset of those with the Very Long Baseline and the Long Baseline Arrays to
confirm detections of radio emission on parsec-scales. We quantified
association probabilities based on known statistics of source counts and
assuming a uniform distribution of background sources. In total we found 865
radio sources at arcsec scales as candidates for association and detected 95 of
170 selected for follow-up observations at milliarcsecond resolution. Based on
this we obtained firm associations for 76 previously unknown gamma-ray AGN.
Comparison of these new AGN associations with the predictions from using the
WISE color-color diagram shows that half of the associations are missed. We
found that 129 out of 588 observed gamma-ray sources at arcmin scales not a
single radio continuum source was detected above our sensitivity limit within
the 3-sigma gamma-ray localization. These "empty" fields were found to be
particularly concentrated at low Galactic latitudes. The nature of these
Galactic gamma-ray emitters is not yet determined.
