Notes. Column 1: map name; Col. 2: Hyper source number; Col. 3: reference wavelength of the source; Cols. 4 and 5: source peak flux expressed in MJy/sr and Jy respectively; Cols. 6 and 7: source flux and source flux error. The source flux is corrected for the aperture size but not for colour corrections. The flux error is estimated from the sky rms multiplied by the square root of the number of pixels in the area over which the source flux is integrated; Cols. 8 and 9: rms of the sky evaluated in the rectangular region used to model the background before and after the background subtraction respectively; Col. 10: polynomial order used to model the background; Cols. 11 and 12: FWHM minor and FWHM major of the source. They correspond to the aperture radii used to evaluate the flux; Col. 13: Source Position Angle; Col. 14: goodness of the 2D Gaussian fit. Status can be equal to [0, − 1, − 2] as described in Sect. 3; Cols. 15−18: source centroids Galactic and equatorial coordinates. Issues related to the proprietary nature of these data require that the coordinates can not be presented here. However the positions are in complete agreement with Cutex and getsources positions and will be soon released by the HGBS consortium; Col. 19: number of sources identified as companions and deblended; Col. 20: distance from the source centroids in the wavelength used to identify the source and the source counterparts at the other wavelengths; Col. 21: number of source counterparts at each wavelength. It is usually equal to 1 but it can be higher if the source is resolved in more than one counterparts in the high resolution maps.