Optical counterpart and radio contour plots of C2625. The header contains: i) The source name used in the present project; ii) the rms noise value at which the VLA contours start; iii) The VLBA+GBT naturally-weighted image S/N; iv) The VLBA naturally-weighted image S/N; v) The VLA peak flux density (in μJy); vi) The VLBA+GBT peak flux density (in μJy); vii) The VLBA peak flux density (in μJy). Left panel: HST image of the optical counterpart (background greyscale image) (Koekemoer et al. 2007; Massey et al. 2010). The white contours represent the VLA contours of the source, starting at four times the rms noise level of the VLA image and increasing by a factor of two. The blue circle represents the VLBA detection position. Middle panel: green contours represent the VLBA+GBT contours of the source, starting at three times the rms noise level of the naturally-weighted image and increasing by a factor of . Right panel: green contours represent the VLBA detection contours, starting at three times the rms noise level of the naturally-weighted image and increasing by a factor of .