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UPM J1710-5300 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.05.14CEST07:05:19 |
Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
---|---|---|---|---|---|---|---|---|---|
2009ApJS..184..138H | 15 | D | 2 | 20664 | 68 | XID II: statistical cross-association of ROSAT bright source catalog X-ray sources with 2MASS point source catalog near-infrared sources. | HAAKONSEN C.B. and RUTLEDGE R.E. | ||
2010AJ....140..844F | 15 | D | 1 | 485 | 14 | UCAC3 proper motion survey. I. Discovery of new proper motion stars in UCAC3 with 0.40"/yr > µ ≥ 0.18"/yr between declinations -90° and -47°. | FINCH C.T., ZACHARIAS N. and HENRY T.J. | ||
2014ApJ...788...81M | 16 | D | 2 | 351 | 123 | BANYAN. III. Radial velocity, rotation, and X-ray emission of low-mass star candidates in nearby young kinematic groups. | MALO L., ARTIGAU E., DOYON R., et al. | ||
2014AJ....148..119F | 16 | D | 1 | 1765 | 12 | UCAC4 nearby star survey: a search for our stellar neighbors. | FINCH C.T., ZACHARIAS N., SUBASAVAGE J.P., et al. | ||
2015AJ....149....5W | 16 | D | 1 | 1773 | 104 | The solar neighborhood. XXXV. Distances to 1404 M dwarf systems within 25 pc in the southern sky. | WINTERS J.G., HAMBLY N.C., JAO W.-C., et al. | ||
2016ApJS..224...36K | 16 | D | 1 | 45305 | 70 | The AllWISE motion survey, part 2. | KIRKPATRICK J.D., KELLOGG K., SCHNEIDER A.C., et al. | ||
2018AJ....156...49R | 222 | D | X C | 5 | 136 | 2 | The solar neighborhood. XLIII. Discovery of new nearby stars with µ<0.18"/yr (TINYMO sample). | RIEDEL A.R., SILVERSTEIN M.L., HENRY T.J., et al. | |
2019AJ....157..216W | 84 | S | 1 | 177 | 120 | The solar neighborhood. XLV. The stellar multiplicity rate of M dwarfs within 25 pc. | WINTERS J.G., HENRY T.J., JAO W.-C., et al. | ||
2020AJ....160..215V | 17 | D | 1 | 605 | 16 | The solar neighborhood. XLVI. Revealing new M dwarf binaries and their orbital architectures. | VRIJMOET E.H., HENRY T.J., JAO W.-C., et al. |