| discov_num | notes | refcode |
| STF2052 | AB: NLTT 42901/42900 | Chm2004 |
| AB: Malkov et al. (2012) derive dynamical, photometric, and | ||
| spectroscopic masses 1.63 +/- 0.88, 1.67, and 0.79 Msun, respectively. | Mlk2012 |
| refcode | metd | author | reference |
| Chm2004 | E - | Chaname, J. & Gould, A. | 2004ApJ...601..289C |
| Chm2004 | ApJ 601, 289, 2004 | ||
| Chm2004 | (Photometry, coordinates, and astrometry from rNLTT. Astrometry from early | ||
| Chm2004 | versions of 2MASS and UCAC, with date given only as "circa 2000". Measures | ||
| Chm2004 | identical to discovery observations - predominantly close pairs - were assumed | ||
| Chm2004 | not new observations, so not included in WDS. Similar concerns when primary and | ||
| Chm2004 | secondary magnitudes or proper motions were the same.) | ||
| Izm2019 | orb u | Izmailov, I.S. | 2019AstL...45...30I |
| Izm2019 | Ast. Lett. 45, 30, 2019 | ||
| Izm2019 | |||
| Izm2019 | |||
| Mlk2012 | not - | Malkov, O.Yu., Tamazian, V.S., Docobo, J.A., & Chulkov, D.A. | 2012A&A...546A..69M |
| Mlk2012 | A&A 546, A69, 2012 |
| discov | author |
| CHM | Chaname, J. & Gould, A. |
| IZM | Izmailov, I.S., Khovricheva, M.L., Khovrichev, M. Yu., Kiyaeva, O.V., Khrutskaya, |
| IZM | E.V., Romanenko, L.G., Grosheva, E.A., Maslennikov, K.L. & Kalinichenko, O.A. |
| coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | dm_number | notes | coord_arcsec_2000 |
| 16289+1825 | STF2052 | AB | 2007 | 528 | 121 | 2.2 | 7.69 | 7.91 | K1V | +18 3182 | OD | 162852.67+182450.6 |
| 16289+1825 | STF2052 | AB | 2009 | 531 | 121 | 2.3 | 7.69 | 7.91 | K1V | +18 3182 | OD | 162852.67+182450.6 |
| 16289+1825 | STF2052 | AB | 2010 | 542 | 120 | 2.3 | 7.69 | 7.91 | K1V | +18 3182 | NOD | 162852.67+182450.6 |
| 16289+1825 | STF2052 | AB | 2012 | 552 | 120 | 2.2 | 7.69 | 7.91 | K1V | +18 3182 | NOD | 162852.67+182450.6 |
| 16289+1825 | STF2052 | AB | 2013 | 553 | 121 | 2.3 | 7.69 | 7.91 | K1V | +18 3182 | NOD | 162852.67+182450.6 |
| 16289+1825 | STF2052 | AB | 2014 | 527 | 121 | 2.3 | 7.69 | 7.91 | K1V | +18 3182 | NOD | 162852.67+182450.6 |
| 16289+1825 | STF2052 | AB | 2015 | 529 | 119 | 2.4 | 7.69 | 7.91 | K1V | +18 3182 | NOD | 162852.67+182450.6 |
| 16289+1825 | STF2052 | AB | 2016 | 541 | 121 | 2.4 | 7.69 | 7.91 | K1V | +18 3182 | NO | 162852.67+182450.6 |
| 16289+1825 | STF2052 | AB | 2017 | 542 | 118 | 2.3 | 7.69 | 7.91 | K1V | +18 3182 | NO | 162852.67+182450.6 |
| 16289+1825 | STF2052 | AB | 2018 | 546 | 119 | 2.5 | 7.69 | 7.91 | K1V | +18 3182 | NO | 162852.67+182450.6 |
| 16289+1825 | STF2052 | AB | 2019 | 554 | 118 | 2.5 | 7.69 | 7.91 | K1V | +18 3182 | NO | 162852.67+182450.6 |
| 16289+1825 | STF2052 | AB | 2020 | 556 | 118 | 2.5 | 7.69 | 7.91 | K1V | +18 3182 | NO | 162852.67+182450.6 |
| 16289+1825 | STF2052 | AB | 2022 | 569 | 117 | 2.5 | 7.69 | 7.91 | K3V+K3V | +18 3182 | NO | 162852.67+182450.6 |