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| SDSS J231437.53+015414.2 , the SIMBAD biblio (7 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST15:13:29 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
| 2020ApJ...898..142K | 553 | D | X C | 13 | 36 | 43 | Extremely metal-poor representatives explored by the Subaru Survey (EMPRESS). I. A successful machine-learning selection of metal-poor galaxies and the discovery of a galaxy with M* < 106 M☉ and 0.016 Z☉. | KOJIMA T., OUCHI M., RAUCH M., et al. | |
| 2021ApJ...913...22K | 685 | D | X C | 16 | 19 | 17 | EMPRESS. II. Highly Fe-enriched metal-poor galaxies with ∼1.0 (Fe/O)☉ and 0.02 (O/H)☉: possible traces of supermassive >300 M☉) stars in early galaxies. | KOJIMA T., OUCHI M., RAUCH M., et al. | |
| 2021ApJ...918...54I | 3026 | D | X C | 72 | 23 | 17 | EMPRESS. III. Morphology, stellar population, and dynamics of extremely metal-poor galaxies (EMPGs): are EMPGs local analogs of high-z young galaxies? | ISOBE Y., OUCHI M., KOJIMA T., et al. | |
| 2022ApJ...925..111I | 17 | D | 1 | 22 | 17 | EMPRESS. IV. Extremely Metal-poor Galaxies Including Very Low-mass Primordial Systems with M* = 104-105M☉ and 2%-3% (O/H): High (Fe/O) Suggestive of Metal Enrichment by Hypernovae/Pair-instability Supernovae. | ISOBE Y., OUCHI M., SUZUKI A., et al. | ||
| 2022ApJ...929..134X | 44 | X | 1 | 13 | 13 | EMPRESS. VI. Outflows Investigated in Low-mass Galaxies with M* = 104-107M☉: Weak Feedback in Low-mass Galaxies?. | XU Y., OUCHI M., RAUCH M., et al. | ||
| 2024ApJ...962...50W | 421 | D | X C | 9 | 21 | ~ | EMPRESS. XIII. Chemical Enrichment of Young Galaxies Near and Far at z ∼ 0 and 4-10: Fe/O, Ar/O, S/O, and N/O Measurements with a Comparison of Chemical Evolution Models. | WATANABE K., OUCHI M., NAKAJIMA K., et al. | |
| 2024ApJ...974..310L | 45 | X | 1 | 26 | ~ | Hydrodynamics and Nucleosynthesis of Jet-driven Supernovae. II. Comparisons with Abundances of Extremely Metal-poor Galaxies and Constraints on Supernova Progenitors. | LEUNG S.-C. and NOMOTO K. |
