SDSS J211558.32-173445.0 , the SIMBAD biblio

SDSS J211558.32-173445.0 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST07:59:26


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Title First 3 Authors
2020ApJ...898..142K 347       D     X C       8 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 560       D     X C       13 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.
2022ApJ...925..111I 102       D     X         3 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.
2023ApJ...951..102I 627       D     X C       14 18 4 EMPRESS. IX. Extremely Metal-poor Galaxies are Very Gas-rich Dispersion-dominated Systems: Will the James Webb Space Telescope Witness Gaseous Turbulent High-z Primordial Galaxies? ISOBE Y., OUCHI M., NAKAJIMA K., et al.
2024ApJ...961...49X 152       D     X         4 29 ~ EMPRESS. XII. Statistics on the Dynamics and Gas Mass Fraction of Extremely Metal-poor Galaxies. XU Y., OUCHI M., ISOBE Y., et al.
2024ApJ...962...50W 18       D               1 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.
2024A&A...686A.186C 18       D               1 41 ~ Trading oxygen for iron I. The [O/Fe]-specific star formation rate relation of galaxies. CHRUSLINSKA M., PAKMOR R., MATTHEE J., et al.
2024ApJ...974..266Y 376       D     X         9 6 ~ Strong He I Emission Lines in High N/O Galaxies at z ∼ 6 Identified in JWST Spectra: High He/H Abundance Ratios or High Electron Densities? YANAGISAWA H., OUCHI M., WATANABE K., et al.
2024ApJ...974..310L 18       D               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.
2025ApJ...988...46F 19       D               1 23 ~ Probing Chemical Enrichment in Extremely Metal-poor Galaxies. FUKUSHIMA K., NAGAMINE K., MATSUMOTO A., et al.

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