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The INTEGRAL observatory has discovered a variety of hard X-ray sources inthe Galactic plane since its launch. Using GMRT, we have made repeatedobservations of these sources to search for the radio counterparts of seventeenof them at low frequencies. The source positions were taken from the variousATEL and IAUC reporting their discovery. Possible radio counterparts for sevenof these sources namely, IGR J06074+2205, IGR J15479-4529, IGR J16479-4514, IGRJ17091-3624, IGR J18027-1455, IGR J18539+0727 and IGR J21247+5058 were detectedwithin 3$\sigma$ of the position uncertainty derived from the INTEGRALobservations. The offset in the radio position was calculated using thepositions mentioned in the ATEL. We have also analyzed the available NVSSimages for a few of these fields at 1.4 GHz along with our observations. Inthis paper we present the radio images and the best fit positions for thepositive detections. The X-ray variability for few of the sources within thetime scales of 100 s to 1 ks as seen in the RXTE/PCA light curves suggeststheir Galactic origin and possible binary nature. We discuss briefly thecharacteristics of these sources from the available information at differentwave bands.Comment: 14 pages, 10 figures,accepted in A&

GMRT observations of the field of INTEGRAL X-ray sources - I