Notes. Column (1) gives the ID of the source from the VLA radio catalogue, Cols. (2) and (3) represent the coordinates of the source. Position errors in arcseconds, as calculated using the AIPS task SAD, are shown in Cols. (4) and (5). Peak surface brightness and its error are given in Cols. (6) and (7) in units of μJy beam^-1, followed by total flux density in Col. (8) and its error in Col. (9), both given in μJy. A flag denoting a resolved source is stated in column (Res = 1 it the source is resolved, 0 otherwise) (10), while a flag for a source located on a sidelobe is given in Col. (11). Sources found on a sidelobe by visual inspection were flagged with Sidelobe = 1. A flag indicating a source composed of multiple components is stated in Col. (12) (Multi = 1 if the source is multicomponent, 0 if single component). The major axis FWHM of the deconvolved Gaussian component and its error are given in Cols. (13) and (14) in arcseconds, respectively. Column (15) gives the minor axis FWHM of the fitted Gaussian with its error in Col. (16) in arcseconds. The position angle of the major axis of the fit Gaussian and its error are shown in (17) and (18) in degrees, respectively. In total, 25 sources are considered resolved, eight have been flagged as multicomponent and 11 as positioned on a sidelobe. The full catalogue is available as a queryable database table XXL_VLA_15 via the XXL Master Catalogue browser http://cosmosdb.iasf-milano.inaf.it/XXL. A copy is also available at the CDS.