| discov_num | notes | refcode |
| KUI 53 | A is also a spectroscopic binary with a period of 5244d which is not | Grf2014c |
| either of these visual pairs. With the proper motion similarity of | ||
| the A and B components this could be a physical quadruple. | ||
| AB: A is SB1, P=10.812y. CfA: P(Aa,Ab)=5241d = 14.35y | Tok2014d | |
| LEP 38 | AC: SHY 219. Bayesian analysis by Shaya & Olling (2011) indicates only | Shy2011 |
| ~50% probability pair is physical. |
| refcode | metd | author | reference |
| Grf2014c | not - | Griffin, R.F. | 2014Obs...134..245G |
| Grf2014c | Observatory 134, 245, 2014 | ||
| Shy2011 | - | Shaya, E.J. & Olling, R. | 2011ApJS..192....2S |
| Shy2011 | ApJS 192, 2, 2011 | ||
| Shy2011 | (Statistical analysis of probability that wide Hipparcos pairs are physical. Pairs | ||
| Shy2011 | added to WDS only if probability 90% or greater.) | ||
| Tok2014d | E2 - | Tokovinin, A. | 2014AJ....147...86T |
| Tok2014d | AJ 147, 86, 2014 |
| idgroup | discov | author |
| 1 | KUI | Kuiper, G.P., Schilt, van den Bos, W., and van Gent |
| 63 | LEP | Lepine, S., Wallace, D., Shara, M., Moffat, A., & Niemela, V. |
| coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
| 11003+4255 | KUI 53 | AB | 1998 | 2 | 151 | 37.3 | 6.02 | 11.70 | F9V | D | 110020.76+425443.3 |
| 11003+4255 | KUI 53 | AB | 2002 | 3 | 151 | 36.7 | 6.02 | 11.70 | F9V | N D | 110020.76+425443.3 |
| 11003+4255 | KUI 53 | AB | 2015 | 4 | 151 | 37.2 | 6.03 | 11.70 | F9V | N | 110020.67+425442.2 |
| 11003+4255 | KUI 53 | AB | 2016 | 9 | 151 | 37.2 | 6.03 | 11.70 | F9V | N | 110020.67+425442.2 |