  We present a multi-epoch radio study of the Taurus-Auriga star-forming
complex made with the Karl G. Jansky Very Large Array at frequencies of 4.5 GHz
and 7.5 GHz. We detect a total of 610 sources, 59 of which are related to young
stellar objects and 18 to field stars. The properties of 56\% of the young
stars are compatible with non-thermal radio emission. We also show that the
radio emission of more evolved young stellar objects tends to be more
non-thermal in origin and, in general, that their radio properties are
compatible with those found in other star forming regions. By comparing our
results with previously reported X-ray observations, we notice that young
stellar objects in Taurus-Auriga follow a G\"{u}del-Benz relation with
$\kappa$=0.03, as we previously suggested for other regions of star formation.
In general, young stellar objects in Taurus-Auriga and in all the previous
studied regions seem to follow this relation with a dispersion of $\sim1$ dex.
Finally, we propose that most of the remaining sources are related with
extragalactic objects but provide a list of 46 unidentified radio sources whose
radio properties are compatible with a YSO nature.
