| discov_num | notes | refcode |
| JNN 93 | The B component seen in the AstraLux images appears to be a very close | |
| binary itself due to a PSF extension visible in five separate epochs. | ||
| However, we count the system as a regular binary here since we do not | ||
| get a converging fit for the closer pair. | Jnn2012 |
| refcode | metd | author | reference |
| 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 |
| 13295+5142 | JNN 93 | 2009 | 6 | 304 | 1.8 | 12.40 | 15.40 | K7 M2 | 132932.12+514211.3 | ||
| 13295+5142 | JNN 93 | 2016 | 8 | 304 | 1.8 | 12.40 | 15.40 | K7+M2 | NU | 132932.12+514211.3 |