SONYC - Substellar Objects in Nearby Young Clusters - is a survey program to investigate the frequency and properties of substellar objects with masses down to a few times that of Jupiter in nearby star-forming regions. In two papers of the SONYC series we have obtained follow-up spectroscopy for a large number of candidate very low ma ss (VLM) members of the ~1Myr old cluster rho Ophiuchi. For more details on the survey, see the associated paper (Muzic et al., 2012ApJ...744..134M). Here we publish the two catalogues of photometric candidate members from which the spectroscopic samples were extracted (see Geers et al. 2011ApJ...726...23G and Muzic et al. 2012ApJ...744..134M for more details on these catalogues). We include a table containing all the spectroscopically confirmed VLM members of the cluster observed within the SONYC campaign. We also attach and a table with all the objects that have been rejected as VLM members based on our spectroscopic follow-up. The majority of these latter objects are expected to be background contaminants, although some of them could also be embedded cluster members with spectral types earlier than M.

Cone search capability for table J/ApJ/744/134/ijk_cand (iJKs candidate catalogue (photometry only))

Cone search capability for table J/ApJ/744/134/jks_cand (JKs-Spitzer candidate catalog (photometry only))

Cone search capability for table J/ApJ/744/134/members (Spectroscopically confirmed very low mass members of rho Ophiuchi from Papers II and V)

Cone search capability for table J/ApJ/744/134/excluded (Objects ruled out by spectroscopy as very low mass members of rho Ophiuchi from Papers II and V (duplicates removed))