Note Text --- --- - ------------------------------------------------------------------------------ a Radio emission is resolved, providing a likely explanation for the somewhat a large radio-optical separation. b The morphology of the extended radio emission is consistent with that of the b optical. In the case of spiral galaxies this indicates that the radio b emission traces the galaxy disk, whereas for elliptical galaxies the center b of the galaxy appears to be where the radio emission originates. c Source appears to be the host of a radio double. The indicated separation is c for distance from optical source to midpoint of the radio counterparts listed c in the last two columns. d Source separation is greater than 3". See Figure 5. e Optical position for bright clump within larger galaxy. f Galaxy appears to be one member of a galaxy pair. Many of the possible f companions may be found in Table 3. g Radio emission is unresolved, but lies within the optical extent of the galaxy h Optical source not in SDSS catalog due to proximity to bright source, usually h the diffraction spike of a saturated star. The position represents the h coordinates of the peak of the object as measured directly in the h SDSS r band image. i Although the radio-optical separation is acceptable for the r magnitude of the i potential counterpart, visual inspection of the overlaid radio contours i strongly suggested the sources are unassociated. j The radio source was assigned to a galaxy with a smaller separation j (see Table 3). k Same comment as "a" plus the radio source is detected at less than 5{sigma}. l The radio morphology is that of a radio double source, and this optical l counterpart appears to be a chance superposition of a galaxy with one of the l lobes. The optical counterpart for the radio emission would be expected to l lie in between the lobes, and not coincident with one. m Visually appears offset. The radio emission also appears to be a lobe of a m separate FR2 type source, and hence not associated with this galaxy. n This radio source was assigned to a brighter galaxy with radio-optical n separation greater than 3''. It may be seen in Figure 5.