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We present results from a high-sensitivity (60 $\mu$Jy), large-scale (2.26square degree) survey obtained with the Karl G. Jansky Very Large Array as partof the Gould's Belt Survey program. We detected 374 and 354 sources at 4.5 and7.5 GHz, respectively. Of these, 148 are associated with previously known YoungStellar Objects (YSOs). Another 86 sources previously unclassified at eitheroptical or infrared wavelengths exhibit radio properties that are consistentwith those of young stars. The overall properties of our sources at radiowavelengths such as their variability and radio to X-ray luminosity relationare consistent with previous results from the Gould's Belt Survey. Ourdetections provide target lists for followup VLBA radio observations todetermine their distances as YSOs are located in regions of high nebulosity andextinction, making it difficult to measure optical parallaxes.

The Gould's Belt Very Large Array Survey III. The Orion region