| discov_num | notes | refcode |
| STT 266 | Scardia et al. say the quadrant is unambiguous for their 2004 theta | Sca2005a |
| value of 178.1; this does not agree with other determinations of | ||
| magnitude difference, however. |
| refcode | metd | author | reference |
| Izm2019 | orb u | Izmailov, I.S. | 2019AstL...45...30I |
| Izm2019 | Ast. Lett. 45, 30, 2019 | ||
| Izm2019 | (Orbital elements from weighted solutions used when available (Table 2), | ||
| Izm2019 | unweighted elements (Table 1) used for remaining 29 systems.) | ||
| Sca2005a | S j | Scardia, M., Prieur, J.-L., Sala, M., Ghigo, M., Koechlin, L., Aristidi, E., | 2005MNRAS.357.1255S |
| Sca2005a | +C | & Mazzoleni, F. | |
| Sca2005a | +orb | MNRAS 357, 1255, 2005 | |
| Sca2005a | (theta corrections from Prieur, private communication) |
| idgroup | discov | author |
| 1 | STT | Struve, O. |
| coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
| 13284+1543 | STT 266 | 2006 | 208 | 357 | 2.0 | 7.97 | 8.42 | F5 | N D | 132826.68+154230.5 | |
| 13284+1543 | STT 266 | 2007 | 210 | 358 | 2.0 | 7.97 | 8.42 | F5 | N D | 132826.68+154230.5 | |
| 13284+1543 | STT 266 | 2010 | 212 | 357 | 2.0 | 7.97 | 8.42 | F5 | N D | 132826.68+154230.5 | |
| 13284+1543 | STT 266 | 2011 | 213 | 357 | 2.0 | 7.97 | 8.42 | F5 | NOD | 132826.68+154230.5 | |
| 13284+1543 | STT 266 | 2013 | 214 | 358 | 2.0 | 7.97 | 8.42 | F5 | NOD | 132826.68+154230.5 | |
| 13284+1543 | STT 266 | 2016 | 210 | 357 | 2.0 | 7.97 | 8.42 | F5 | NO | 132826.68+154230.5 | |
| 13284+1543 | STT 266 | 2017 | 211 | 358 | 2.0 | 7.97 | 8.42 | F5 | NO | 132826.68+154230.5 | |
| 13284+1543 | STT 266 | 2018 | 214 | 358 | 2.0 | 7.97 | 8.42 | F5 | NO | 132826.68+154230.5 | |
| 13284+1543 | STT 266 | 2020 | 218 | 355 | 1.9 | 7.97 | 8.42 | F5 | NO | 132826.68+154230.5 |