other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
SDSS J085136.67+101803.1 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST09:50:09 |
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 |
---|---|---|---|---|---|---|---|---|---|
2013AJ....145...13A | 16 | D | 1 | 151 | 146 | High-resolution spectroscopy of extremely metal-poor stars from SDSS/SEGUE. I. Atmospheric parameters and chemical compositions. | AOKI W., BEERS T.C., LEE Y.S., et al. | ||
2013ApJ...762...25N | 16 | D | 1 | 74 | 50 | The most metal-poor stars. I. Discovery, data, and atmospheric parameters. | NORRIS J.E., BESSELL M.S., YONG D., et al. | ||
2013ApJ...762...26Y | 16 | D | 4 | 198 | 263 | The most metal-poor stars. II. Chemical abundances of 190 metal-poor stars including 10 new stars with [Fe/H] ≤ -3.5. | YONG D., NORRIS J.E., BESSELL M.S., et al. | ||
2013AJ....146..132L | 95 | D | C | 2 | 39 | 128 | Carbon-enhanced metal-poor stars in SDSS/SEGUE. I. Carbon abundance estimation and frequency of CEMP stars. | LEE Y.S., BEERS T.C., MASSERON T., et al. | |
2014ApJ...788..180C | 16 | D | 2 | 329 | 52 | Carbon-enhanced metal-poor stars: CEMP-s and CEMP-no subclasses in the halo system of the Milky Way. | CAROLLO D., FREEMAN K., BEERS T.C., et al. | ||
2016A&A...591A.118S | 16 | D | 1 | 31406 | 141 | The PASTEL catalogue: 2016 version. | SOUBIRAN C., LE CAMPION J.-F., BROUILLET N., et al. | ||
2019MNRAS.486.2169K | 17 | D | 1 | 25030 | 80 | White dwarf and subdwarf stars in the Sloan Digital Sky Survey Data Release 14. | KEPLER S.O., PELISOLI I., KOESTER D., et al. | ||
2021A&A...651A..79B | 17 | D | 2 | 57451 | 21 | TOPoS. VI. The metal-weak tail of the metallicity distribution functions of the Milky Way and the Gaia-Sausage-Enceladus structure. | BONIFACIO P., MONACO L., SALVADORI S., et al. |