| discov_num | notes | refcode |
| RST3352 | ups Phe. Variable RV suspected. The lines are poor and show a scatter | |
| of 40km/s without apparent relation to the visual motion. | ||
| Malkov et al. (2012) derive dynamical, photometric, and spectroscopic | ||
| masses of 3.16 +/- 0.34, 2.78, and 2.09 Msun, respectively. | Mlk2012 |
| refcode | metd | author | reference |
| DRs2012 | A j | De Rosa, R.J., Patience, J., Vigan, A., Wilson, P.A., Schnieder, A., | 2012MNRAS.422.2765D |
| DRs2012 | McConnell, N.J., Wiktorowicz, S.J., Marois, C., Song, I., Macintosh, B., | ||
| DRs2012 | Graham, J.R., Bessell, M.S., Doyon, R., & Lai, O. | ||
| DRs2012 | MNRAS 422, 2765, 2012 | ||
| DRs2012 | (includes re-reduction of some data originally published in DRs2011) | 2011MNRAS.415..854D | |
| Mlk2012 | not - | Malkov, O.Yu., Tamazian, V.S., Docobo, J.A., & Chulkov, D.A. | 2012A&A...546A..69M |
| Mlk2012 | A&A 546, A69, 2012 |
| idgroup | discov | author |
| 1 | RST | Rossiter, R.A. |
| coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
| 01078-4129 | RST3352 | 2001 | 35 | 337 | 0.2 | 5.54 | 6.88 | A3IV | NOD | 010747.83-412913.0 | |
| 01078-4129 | RST3352 | 2008 | 38 | 141 | 0.1 | 5.54 | 6.88 | A3IV | NOD | 010747.83-412913.0 | |
| 01078-4129 | RST3352 | 2009 | 40 | 336 | 0.1 | 5.54 | 6.88 | A3IV | NOD | 010747.83-412913.0 | |
| 01078-4129 | RST3352 | 2014 | 45 | 270 | 0.1 | 5.54 | 6.88 | A3IV | NO | 010747.83-412913.0 | |
| 01078-4129 | RST3352 | 2018 | 46 | 300 | 0.3 | 5.54 | 6.88 | A3IV | NO | 010747.83-412913.0 | |
| 01078-4129 | RST3352 | 2020 | 47 | 308 | 0.3 | 5.54 | 6.88 | A3IV | NO | 010747.83-412913.0 |