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| UCAC4 464-129364 , the SIMBAD biblio (19 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST17:12:24 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2018ApJ...858...92H |
16 | D | 1 | 115 | 108 | The r-process alliance: first release from the southern search for r-process-enhanced stars in the galactic halo. | HANSEN T.T., HOLMBECK E.M., BEERS T.C., et al. | ||
|
2018MNRAS.478.4513B |
16 | D | 1 | 342691 | 271 | The GALAH Survey: second data release. | BUDER S., ASPLUND M., DUONG L., et al. | ||
|
2019ApJ...870..122P |
16 | D | 1 | 859 | 1 | The r-process Alliance: spectroscopic follow-up of low-metallicity star candidates from the Best & Brightest Survey. | PLACCO V.M., SANTUCCI R.M., BEERS T.C., et al. | ||
|
2019ApJ...882...27M |
1462 | A | D | S X C | 35 | 9 | ~ | Metal-poor stars observed with the automated Planet Finder telescope. II. Chemodynamical analysis of six low-metallicity stars in the halo system of the Milky Way. | MARDINI M.K., PLACCO V.M., TAANI A., et al. |
|
2020MNRAS.497L...7S |
16 | D | 1 | 5378 | 47 | The Pristine survey - X. A large population of low-metallicity stars permeates the Galactic disc. | SESTITO F., MARTIN N.F., STARKENBURG E., et al. | ||
|
2021MNRAS.506..150B |
17 | D | 1 | 588596 | 276 | The GALAH+ survey: Third data release. | BUDER S., SHARMA S., KOS J., et al. | ||
|
2021ApJ...923..183L |
17 | D | 1 | 147 | ~ | Fuzzy cluster analysis: application to determining metallicities for very metal-poor stars. | LI H. | ||
|
2022ApJ...926...26S |
17 | D | 1 | 6507 | 18 | Dynamically Tagged Groups of Metal-poor Stars from the Best and Brightest Survey. | SHANK D., BEERS T.C., PLACCO V.M., et al. | ||
| 2022ApJ...930...47H | 17 | D | 2 | 72 | 6 | The GALAH Survey: A New Sample of Extremely Metal-poor Stars Using a Machine-learning Classification Algorithm. | HUGHES A.C.N., SPITLER L.R., ZUCKER D.B., et al. | ||
|
2022ApJ...931..146A |
17 | D | 1 | 423 | 7 | Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. I. Survey Design, Follow-up Program, and Binary Frequency. | AOKI W., LI H., MATSUNO T., et al. | ||
|
2022ApJ...931..147L |
17 | D | 1 | 397 | 21 | Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances. | LI H., AOKI W., MATSUNO T., et al. | ||
|
2023ApJ...943...23S |
17 | D | 1 | 1792 | 5 | The R-Process Alliance: Chemodynamically Tagged Groups. II. An Extended Sample of Halo r-process-enhanced Stars. | SHANK D., BEERS T.C., PLACCO V.M., et al. | ||
|
2023AJ....165..145L |
17 | D | 1 | 180 | 1 | LOTUS: A (Non-) LTE Optimization Tool for Uniform Derivation of Stellar Atmospheric Parameters. | LI Y. and EZZEDDINE R. | ||
| 2023RAA....23g5019S | 17 | D | 1 | 95 | ~ | Sodium Abundances in Very Metal-poor Stars. | SHEN Y.-F., ALEXEEVA S.A., ZHAO G., et al. | ||
|
2024A&A...683L..11V |
18 | D | 1 | 1441 | ~ | Gaia's brightest very metal-poor (VMP) stars Metallicity catalogue of a thousand VMP stars from Gaia's radial velocity spectrometer spectra. | VISWANATHAN A., STARKENBURG E., MATSUNO T., et al. | ||
| 2024ApJ...966..174Z | 45 | X | 1 | 19 | ~ | Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. III. Dynamically Tagged Groups and Chemodynamical Properties. | ZHANG R., MATSUNO T., LI H., et al. | ||
|
2024A&A...685A..59M |
90 | C | 1 | 3 | ~ | Improving metallicity estimates for very metal-poor stars in the Gaia DR3 GSP-Spec catalog. | MATSUNO T., STARKENBURG E., BALBINOT E., et al. | ||
| 2024A&A...692A.130B | 18 | D | 1 | 100 | ~ | Cosmological insights into the early accretion of r-process-enhanced stars II. Dynamical identification of lost members of Reticulum II. | BERCZIK P., ISHCHENKO M., SOBODAR O., et al. | ||
| 2026ApJ...998..139A | 20 | D | 1 | 104 | ~ | A Systematic NLTE Study of Very Metal-poor Stars with Metallicity down to -4.3 dex. VI. Light Neutron-capture Elements and the Sr-Na Correlation as a Signature of Spinstar Nucleosynthesis in the Early Galaxy. | ALEXEEVA S., YAN H., ZHAO G., et al. |