WE PROPOSE TO OBSERVE WITH THE VLA 46 FERMI/4FGL UNASSOCIATED SOURCES THAT ARE CLASSIFIED AS PULSAR-LIKE BASED ON THEIR GAMMARAY PROPERTIES. WE WILL APPLY AN IMAGE-BASED METHOD THAT USES TWO RADIO CRITERIA: COMPACTNESS AND SPECTRAL INDEX IN ORDER TO IDENTIFY PROMISING PULSAR CANDIDATES FOR FOLLOW-UP PULSATION SEARCHES.