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| UCAC4 551-007718 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST06:32:52 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2010AJ....139.1338F |
15 | D | 1 | 590 | 31 | Ultraviolet-selected field and pre-main-sequence stars toward Taurus and upper Scorpius. | FINDEISEN K. and HILLENBRAND L. | ||
|
2010MNRAS.408..475H |
15 | D | 2 | 1926 | 134 | A large sample of photometric rotation periods for FGK Pleiades stars. | HARTMAN J.D., BAKOS G.A., KOVACS G., et al. | ||
|
2016ApJS..224....2H |
16 | D | 1 | 31769 | 226 | The K2 ecliptic plane input catalog (EPIC) and stellar classifications of 138,600 targets in campaigns 1-8. | HUBER D., BRYSON S.T., HAAS M.R., et al. | ||
|
2019AJ....158..122K |
16 | D | 1 | 290057 | 150 | Untangling the Galaxy. I. Local structure and star formation history of the Milky Way. | KOUNKEL M. and COVEY K. | ||
|
2020MNRAS.495.1252Z |
16 | D | 1 | 1120 | 18 | Magnetic activity based on LAMOST medium-resolution spectra and the Kepler survey. | ZHANG L.-Y., LONG L., SHI J., et al. | ||
|
2020ApJ...903...96G |
16 | D | 1 | 588 | 27 | The µ Tau Association: a 60 Myr old coeval group at 150 pc from the Sun. | GAGNE J., DAVID T.J., MAMAJEK E.E., 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. | ||
|
2022MNRAS.514.4781X |
17 | D | 2 | 801 | ~ | Investigation of stellar magnetic activity using variational autoencoder based on low-resolution spectroscopic survey. | XIANG Y., GU S. and CAO D. | ||
|
2024AJ....167..210V |
18 | D | 1 | 7289 | ~ | The Occurrence of Small, Short-period Planets Younger than 200 Myr with TESS. | VACH S., ZHOU G., HUANG C.X., et al. |