| discov_num | notes | refcode |
| TOK 409 | HIP 79576 has a variable RV (GCS). The 79mas separation implies an | |
| orbital period of ~5yr. This is the high-PM star LTT 6467 with a low | ||
| metallicity [Fe/H]=-0.78. Ivanov et al. (2013 A&A 560, 21) found no | ||
| CPM companions. | Tok2015c |
| refcode | metd | author | reference |
| Tok2015c | orb+j | Tokovinin, A., Mason, B.D., Hartkopf, W.I., Mendez, R.A., & Horch, E.P. | 2015AJ....150...50T |
| Tok2015c | +St | AJ 150, 50, 2015 (some measures corrected in Tok2017b) | 2017AJ....154..110T |
| coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
| 16142-5047 | TOK 409 | 2014 | 1 | 145 | 0.1 | 8.70 | 12.00 | G8V | 161409.91-504701.7 | ||
| 16142-5047 | TOK 409 | 2015 | 2 | 185 | 0.0 | 8.70 | 12.00 | G8V | 161409.91-504701.7 | ||
| 16142-5047 | TOK 409 | 2018 | 6 | 159 | 0.0 | 8.70 | 12.00 | G8V | N | 161409.92-504704.8 |