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We present deep ($\sim 17~\mu$Jy) radio continuum observations of the Serpensmolecular cloud, the Serpens south cluster, and the W40 region obtained usingthe Very Large Array in its A configuration. We detect a total of 146 sources,29 of which are young stellar objects (YSOs), 2 are BV stars and 5 more areassociated with phenomena related to YSOs. Based on their radio variability andspectral index, we propose that about 16 of the remaining 110 unclassifiedsources are also YSOs. For approximately 65% of the known YSOs detected here asradio sources, the emission is most likely non-thermal, and related to stellarcoronal activity. As also recently observed in Ophiuchus, our sample of YSOswith X-ray counterparts lies below the fiducial G\"udel & Benz relation.Finally, we analyze the proper motions of 9 sources in the W40 region. Thisallows us to better constrain the membership of the radio sources in theregion.

The Gould's Belt Very Large Array Survey II: The Serpens region