| discov_num | notes | refcode |
| FIN 329 | Malkov et al. (2012) derive dynamical, photometric, and spectroscopic | |
| masses of 05.99 +/- 37.68, 3.70, and 1.88 Msun, respectively. | Mlk2012 | |
| Docobo & Andrade (2013) derive a dynamical parallax of 8.36 +/- 0.17 | ||
| mas and component masses 2.32 +/- 0.18 and 2.09 +/- 0.16 Msun (for | ||
| spectral type A2.5V) or 8.74 +/- 0.17 mas, 2.04 +/- 0.15 and 1.82 +/- | ||
| 0.14 Msun (for A6IV). See paper for extensive notes on this system. | Doc2013d |
| refcode | metd | author | reference |
| Doc2013d | orb - | Docobo, J.A. & Andrade, M. | 2013MNRAS.428..321D |
| Doc2013d | MNRAS 428, 321, 2013 | ||
| Mlk2012 | not - | Malkov, O.Yu., Tamazian, V.S., Docobo, J.A., & Chulkov, D.A. | 2012A&A...546A..69M |
| Mlk2012 | A&A 546, A69, 2012 | ||
| Tok2020g | orb - | Tokovinin, A. | 2020IAUDS.201....1A |
| Tok2020g | Inf. Circ. 201, 1, 2020 | ||
| Tok2021f | orb - | Tokovinin, A. | 2021IAUDS.204....1T |
| Tok2021f | Inf. Circ. 204, 1, 2021 |
| idgroup | discov | author |
| 1 | FIN | Finsen, W.S. |
| coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
| 21158-5316 | FIN 329 | 1991 | 20 | 64 | 0.1 | 6.33 | 6.80 | A6IV | NO | 211545.84-531547.0 | |
| 21158-5316 | FIN 329 | 2008 | 23 | 64 | 0.1 | 6.33 | 6.80 | A6IV | NO | 211545.84-531547.0 | |
| 21158-5316 | FIN 329 | 2009 | 25 | 57 | 0.1 | 6.33 | 6.80 | A6IV | NOD | 211545.84-531547.0 | |
| 21158-5316 | FIN 329 | 2014 | 26 | 335 | 0.1 | 6.33 | 6.80 | A6IV | NO | 211545.84-531547.0 | |
| 21158-5316 | FIN 329 | 2015 | 27 | 136 | 0.1 | 6.33 | 6.80 | A6IV | NO | 211545.84-531547.0 | |
| 21158-5316 | FIN 329 | 2017 | 29 | 111 | 0.1 | 6.33 | 6.80 | A6IV | NO | 211545.84-531547.0 | |
| 21158-5316 | FIN 329 | 2018 | 30 | 105 | 0.1 | 6.33 | 6.80 | A6IV | NO | 211545.84-531547.0 | |
| 21158-5316 | FIN 329 | 2020 | 31 | 92 | 0.2 | 6.33 | 6.80 | A6IV | NO | 211545.84-531547.0 |