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SDSS J002314.00+030758.0 , the SIMBAD biblio (21 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST06:43:18 |
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...854L..34A | 933 | T A | X C | 21 | 7 | 21 |
J0023+0307 a mega metal-poor dwarf star from SDSS/BOSS. |
AGUADO D.S., ALLENDE PRIETO C., GONZALEZ HERNANDEZ J.I., et al. | |
2018MNRAS.480.1043N | 82 | X | 2 | 2 | ~ | Condition for low-mass star formation in shock-compressed metal-poor clouds. | NAKAUCHI D., OMUKAI K. and SCHNEIDER R. | ||
2018A&A...619A..10F | 230 | A | S X C | 4 | 11 | 3 | Chemical analysis of very metal-poor turn-off stars from SDSS-DR12. | FRANCOIS P., CAFFAU E., WANAJO S., et al. | |
2019ApJ...871..146F | 3009 | T K A | D | S X C F | 69 | 33 | 17 |
Chemical abundance signature of J0023+0307 a second-generation main-sequence star with [Fe/H] < -6. |
FREBEL A., JI A.P., EZZEDDINE R., et al. |
2019MNRAS.484.2166S | 101 | D | F | 5 | 45 | 69 | Tracing the formation of the Milky Way through ultra metal-poor stars. | SESTITO F., LONGEARD N., MARTIN N.F., et al. | |
2019ApJ...874L..21A | 1353 | T K A | D | X C | 31 | 3 | 45 |
Back to the lithium plateau with the [Fe/H] < -6 star J0023+0307. |
AGUADO D.S., GONZALEZ HERNANDEZ J.I., ALLENDE PRIETO C., et al. |
2019ApJ...879...37N | 17 | D | 1 | 74 | 7 | The most metal-poor stars. V. The CEMP-no stars in 3D and non-LTE. | NORRIS J.E. and YONG D. | ||
2019MNRAS.488L.109N | 50 | X | 1 | 6 | 52 | The lowest detected stellar Fe abundance: the halo star SMSS J160540.18-144323.1. | NORDLANDER T., BESSELL M.S., DA COSTA G.S., et al. | ||
2019A&A...628A.111G | 42 | X | 1 | 9 | ~ | The 6Li/7Li isotopic ratio in the metal-poor binary CS22876-032. | GONZALEZ HERNANDEZ J.I., BONIFACIO P., CAFFAU E., et al. | ||
2019MNRAS.489.5900D | 42 | X | 1 | 205 | 44 | The SkyMapper DR1.1 search for extremely metal-poor stars. | DA COSTA G.S., BESSELL M.S., MACKEY A.D., et al. | ||
2020A&A...633A.129B | 17 | D | 1 | 15 | ~ | ESPRESSO highlights the binary nature of the ultra-metal-poor giant HE 0107-5240. | BONIFACIO P., MOLARO P., ADIBEKYAN V., et al. | ||
2020ApJ...889L..13G | 451 | A | X C | 10 | 10 | ~ | The extreme CNO-enhanced composition of the primitive iron-poor dwarf star J0815+4729. | GONZALEZ HERNANDEZ J.I., AGUADO D.S., ALLENDE PRIETO C., et al. | |
2020A&A...638A..58M | 43 | X | 1 | 3 | ~ | Improving spectroscopic lithium abundances. Fitting functions for 3D non-LTE corrections in FGK stars of different metallicity. | MOTT A., STEFFEN M., CAFFAU E., et al. | ||
2020A&A...642A..25F | 85 | C | 1 | 11 | ~ | Detailed abundances in a sample of very metal-poor stars. | FRANCOIS P., WANAJO S., CAFFAU E., et al. | ||
2021AJ....161..197C | 17 | D | 1 | 19 | ~ | Searching for low-mass Population III stars disguised as white dwarfs. | CHANDRA V. and SCHLAUFMAN K.C. | ||
2021MNRAS.504.1183S | 44 | X | 1 | 38 | 4 | The formation of the milky way halo and its dwarf satellites: a NLTE-1D abundance analysis. IV. Segue 1, Triangulum II, and Coma Berenices UFDs. | SITNOVA T.M., MASHONKINA L.I., TATARNIKOV A.M., et al. | ||
2021MNRAS.508.3068L | 45 | X | 1 | 5 | 7 | The Pristine survey - XIV. Chemical analysis of two ultra-metal-poor stars. | LARDO C., MASHONKINA L., JABLONKA P., et al. | ||
2022A&A...668A..86A | 332 | D | S X | 7 | 21 | 8 | ESPRESSO observations of HE 0107-5240 and other CEMP-no stars with [Fe/H] ≤ -4.5. | AGUADO D.S., MOLARO P., CAFFAU E., et al. | |
2023MNRAS.522.1358N | 513 | S X C | 9 | 19 | 1 | A critique of the Spite Plateau and the astration of primordial lithium. | NORRIS J.E., YONG D., FREBEL A., et al. | ||
2023MNRAS.525.4700L | 47 | X | 1 | 11 | ~ | Evolution of low mass population III stars from the pre-main sequence to the white dwarf cooling track. | LAWLOR T.M. and MacDONALD J. | ||
2023A&A...679A..72M | 65 | D | X | 2 | 56 | ~ | The 12C/13C isotopic ratio at the dawn of chemical evolution. | MOLARO P., AGUADO D.S., CAFFAU E., et al. |