| discov_num | notes | refcode |
| BEU 5 | Rectilinear solution by Miles & Mason (2016) and | Msn2016b |
| Mason et al. (2018). Despite linear solution, based on proper motion | Msn2018a | |
| and parallax appears to be physical. |
| refcode | metd | author | reference |
| Msn2016b | orb - | Miles, K.N. & Mason, B.D. | 2016IAUDS.190....1M |
| Msn2016b | +lin | Inf. Circ. 190, 1, 2016 | |
| Msn2018a | Su+ j | Mason, B.D., Hartkopf, W.I., Miles, K.N., Subasavage, J.P., Raghavan, D. & | 2018AJ....155..215M |
| Msn2018a | +orb+ | Henry, T.J. | . |
| Msn2018a | +lin | AJ 155, 215, 2018 |
| idgroup | discov | author |
| 1 | BEU | Beuzit, J.-L., Segransan, D., Forveille, T., Udry, S., Delfosse, X., Mayor, M., |
| 1 | BEU | Perrier, C., Hainaut, M.-C., et al. |
| coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
| 04073-2429 | BEU 5 | 2002 | 1 | 72 | 0.6 | 12.40 | M3.5 | D | 040720.51-242913.7 | ||
| 04073-2429 | BEU 5 | 2006 | 2 | 80 | 0.8 | 12.40 | M3.5 | D | 040720.51-242913.7 | ||
| 04073-2429 | BEU 5 | 2010 | 4 | 89 | 1.0 | 12.40 | M3.5 | D | 040720.51-242913.7 | ||
| 04073-2429 | BEU 5 | 2014 | 5 | 94 | 1.2 | 12.30 | 12.60 | M3.5 | R | 040720.51-242913.7 | |
| 04073-2429 | BEU 5 | 2016 | 6 | 96 | 1.2 | 12.30 | 12.60 | M3.5 | L R | 040720.51-242913.7 | |
| 04073-2429 | BEU 5 | 2019 | 8 | 99 | 1.3 | 12.30 | 12.60 | M3.5 | LTR | 040720.51-242913.7 | |
| 04073-2429 | BEU 5 | 2021 | 10 | 100 | 1.4 | 12.30 | 12.60 | M3.5 | LTR | 040720.51-242913.7 |