| discov_num | notes | refcode |
| I 7 | The 94-yr orbit by Heintz (1995) plus the HIP parallax gives | Hei1995 |
| impossibly small mass-sum. Probably both a and P are much larger (no | ||
| orbit for another century), but motion should be followed. | ||
| Malkov et al. (2012) derive dynamical, photometric, and spectroscopic | ||
| masses of 0.43 +/- 0.23, 1.54, and 0.76 Msun, respectively. | Mlk2012 |
| refcode | metd | author | reference |
| Hei1995 | Ma j | Heintz, W.D. | 1995ApJS...99..693H |
| Hei1995 | +Po | ApJS 99, 693, 1995 | |
| Hei1995 | +orb | ||
| Mlk2012 | not - | Malkov, O.Yu., Tamazian, V.S., Docobo, J.A., & Chulkov, D.A. | 2012A&A...546A..69M |
| Mlk2012 | A&A 546, A69, 2012 | ||
| 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 |
| idgroup | discov | author |
| 1 | I | Innes, R.T.A. |
| 5 | I | MNRAS 57, 533, 1897 (data also in I__1897b, |
| 5 | I | I__1897c) |
| coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
| 07175-4659 | I 7 | 2001 | 60 | 26 | 0.8 | 7.10 | 8.35 | K3V | NOD | 071729.56-465845.4 | |
| 07175-4659 | I 7 | 2009 | 61 | 205 | 0.8 | 7.10 | 8.35 | K3V | NOD | 071729.56-465845.4 | |
| 07175-4659 | I 7 | 2010 | 64 | 205 | 0.7 | 7.10 | 8.35 | K3V | NOD | 071729.56-465845.4 | |
| 07175-4659 | I 7 | 2012 | 65 | 203 | 0.7 | 7.10 | 8.35 | K3V | NO | 071729.56-465845.4 | |
| 07175-4659 | I 7 | 2014 | 66 | 202 | 0.7 | 7.10 | 8.35 | K3V | NO | 071729.56-465845.4 | |
| 07175-4659 | I 7 | 2018 | 69 | 201 | 0.6 | 7.10 | 8.35 | K3V | NO | 071729.56-465845.4 | |
| 07175-4659 | I 7 | 2021 | 70 | 199 | 0.6 | 7.10 | 8.35 | K3V | NO | 071729.56-465845.4 |