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| UCAC4 469-115243 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST03:09:12 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
| 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 | 20623 | 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. | ||
|
2019ApJ...877...60B
|
16 | D | 1 | 658 | 26 | The elusive majority of young moving groups. I. Young binaries and lithium-rich stars in the solar neighborhood. | BOWLER B.P., HINKLEY S., ZIEGLER C., et al. | ||
|
2020AJ....160..120J
|
16 | D | 1 | 365763 | 238 | APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. | JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al. | ||
|
2021AJ....162..184K
|
17 | D | 1 | 8106 | 31 | Double-lined spectroscopic binaries in the APOGEE DR16 and DR17 data. | KOUNKEL M., COVEY K.R., STASSUN K.G., et al. | ||
|
2022AJ....163..152S
|
17 | D | 1 | 583193 | 11 | APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. | SPRAGUE D., CULHANE C., KOUNKEL M., et al. | ||
|
2022ApJS..259...35A
|
17 | D | 1 | 611005 | 320 | The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. | ABDURRO'UF, ACCETTA K., AERTS C., et al. | ||
|
2023AJ....165..267H
|
17 | D | 1 | 64663 | 1 | Bioverse: A Comprehensive Assessment of the Capabilities of Extremely Large Telescopes to Probe Earth-like O2 Levels in Nearby Transiting Habitable-zone Exoplanets. | HARDEGREE-ULLMAN K.K., APAI D., BERGSTEN G.J., et al. | ||
|
2024MNRAS.533..395L
|
18 | D | 1 | 1559 | ~ | Atmospheric parameters and chemical abundances within 100 pc: a sample of G, K, and M main-sequence stars. | LOPEZ-VALDIVIA R., ADAME L., ZAGALA LAGUNAS E., et al. |
