| discov_num | notes | refcode |
| JNN 77 | Due to the small separation (~0.42") of the companion detected in the | |
| AstraLux images, it is likely a physical companion, although common | ||
| proper motion has not yet been tested. | Jnn2012 | |
| Bowler et al. (2015) confirm the physical nature and detect orbital | ||
| motion. Riaz et al. (2006 AJ 132, 866) identify the pair as | ||
| chromospherically active. | Bwl2015 |
| refcode | metd | author | reference |
| Bwl2015 | Ac j | Bowler, B.P., Liu, M.C., Shkolnik, E.L., & Tamura, M. | 2015ApJS..216....7B |
| Bwl2015 | ApJS 216, 7, 2015 | ||
| Jnn2012 | Cl j | Janson, M., Hormuth, F., Bergfors, C., Brandner, W., Hippler, S., Daemgen, S., | 2012ApJ...754...44J |
| Jnn2012 | +E2 | Kudryavtseva, N., Schmalzl, E., Schnupp, C., & Henning, T. | |
| Jnn2012 | ApJ 754, 44, 2012 (some recalibrated measures published in Jnn2014b) | 2014ApJS..214...17J |
| coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
| 12064-1315 | JNN 77 | 2010 | 1 | 65 | 0.4 | 12.90 | 15.40 | M3.5 M5.5 | 120622.14-131456.0 | ||
| 12064-1315 | JNN 77 | 2012 | 2 | 54 | 0.4 | 12.90 | 15.40 | M3.5 M5.5 | NV | 120622.14-131456.0 |