| discov_num | notes | refcode |
| RST4917 | 1995.1024: Quadrant determined by speckle imaging analysis. | Hor1996 |
| 1997.1229: A smaller annulus was used in the power spectrum fit due to | ||
| the faintness of the source. As a consequence, the separation and | ||
| position angle uncertainties may be larger than other measures. | Hor1997 |
| refcode | metd | author | reference |
| Hor1996 | S j | Horch, E.P. Dinescu, D.I., Girard, T.M., van Altena, W.F., Lopez, C., & Franz, O. | 1996AJ....111.1681H |
| Hor1996 | AJ 111, 1681, 1996 (see also 1997 Inf. Circ. 131, 1 re: HR 4143) | 1997IAUDS.131....1H | |
| Hor1997 | S j | Horch, E.P., Ninkov, Z., & Slawson, R. | 1997AJ....114.2117H |
| Hor1997 | AJ 114, 2117, 1997 |
| 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 |
| 09398-5008 | RST4917 | 1997 | 14 | 44 | 0.6 | 7.37 | 9.31 | F0IV/V | N | 093945.88-500817.1 | |
| 09398-5008 | RST4917 | 2015 | 15 | 47 | 0.7 | 7.37 | 9.31 | F0IV/V | N | 093945.88-500817.1 |