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| SDSS J161226.17+042146.6 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.25CEST06:04:01 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| 2012ApJ...744..195C | 16 | D | 1 | 35 | 134 | Carbon-enhanced metal-poor stars in the inner and outer halo components of the Milky Way. | CAROLLO D., BEERS T.C., BOVY J., et al. | ||
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...765..156C
|
16 | D | 1 | 26 | 2 | The CH(G) index as a new criterion for selecting red giant stars. | CHEN Y.Q., ZHAO G., CARRELL K., et al. | ||
| 2013AJ....146..132L | 17 | D | 1 | 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 | 1 | 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. | ||
|
2014ApJ...794...60T
|
16 | D | 1 | 17948 | 6 | Red giant stars from the Sloan Digital Sky Survey. II. Distances. | TAN K., CHEN Y., CARRELL K., et al. | ||
|
2014ApJ...797...21P
|
16 | D | 1 | 606 | 226 | Carbon-enhanced metal-poor star frequencies in the galaxy: corrections for the effect of evolutionary status on carbon abundances. | PLACCO V.M., FREBEL A., 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. | ||
|
2022ApJS..259...60R
|
18 | D | 1 | 139 | 22 | SEGUE-2: Old Milky Way Stars Near and Far. | ROCKOSI C.M., SUN LEE Y., MORRISON H.L., et al. |
