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| SMSS J022410.38-534659.9 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST10:43:38 |
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 |
|---|---|---|---|---|---|---|---|---|---|
2015ApJ...807..171J 
|
16 | D | 1 | 131 | 106 | High-resolution spectroscopic study of extremely metal-poor star candidates from the SkyMapper survey. | JACOBSON H.R., KELLER S., FREBEL A., et al. | ||
|
2016ApJ...833...20Y
|
16 | D | 1 | 304 | 147 | Observational constraints on first-star nucleosynthesis. I. Evidence for multiple progenitors of CEMP-no stars. | YOON J., BEERS T.C., PLACCO V.M., et al. | ||
|
2018ApJ...857...46I
|
16 | D | 1 | 205 | 88 | The initial mass function of the first stars inferred from extremely metal-poor stars. | ISHIGAKI M.N., TOMINAGA N., KOBAYASHI C., et al. | ||
|
2018ApJ...857..111T
|
17 | D | 1 | 73 | 76 | Stellar yields of rotating first stars. II. Pair-instability supernovae and comparison with observations. | TAKAHASHI K., YOSHIDA T. and UMEDA H. | ||
| 2019A&A...632A..62C | 81 | C | 1 | 261 | ~ | Inferring the velocity of early massive stars from the abundances of extremely metal-poor stars. | CHOPLIN A., TOMINAGA N. and ISHIGAKI M.N. | ||
|
2021MNRAS.503.2539C
|
17 | D | 1 | 478 | 34 | Exploring the Galaxy's halo and very metal-weak thick disc with SkyMapper and Gaia DR2. | CORDONI G., DA COSTA G.S., YONG D., et al. | ||
|
2023ApJ...947...23Z
|
17 | D | 1 | 647 | 14 | Chemodynamically Tagged Groups of CEMP Stars in the Halo of the Milky Way. I. Untangling the Origins of CEMP-s and CEMP-no Stars. | ZEPEDA J., BEERS T.C., PLACCO V.M., et al. | ||
| 2023MNRAS.524..577O | 17 | D | 1 | 24 | ~ | The SkyMapper search for extremely metal-poor stars in the Large Magellanic Cloud. | OH W.S., NORDLANDER T., DA COSTA G.S., et al. |
