SDSS J134338.67+484426.6 , the SIMBAD biblio

SDSS J134338.67+484426.6 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST01:24:45


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Title First 3 Authors
2016MNRAS.458.2648S 1812 T   A D     X C       45 1 5 Abundance analysis of
SDSS J134338.67+484426.6: an extremely metal-poor star from the MARVELS pre-survey.
SUSMITHA RANI A., SIVARANI T., BEERS T.C., et al.
2016A&A...593A..28F viz 94       D     X         3 108 4 Deep SDSS optical spectroscopy of distant halo stars. III. Chemical analysis of extremely metal-poor stars. FERNANDEZ-ALVAR E., ALLENDE PRIETO C., BEERS T.C., et al.
2017A&A...605A..40A viz 79           X         2 19 15 WHT follow-up observations of extremely metal-poor stars identified from SDSS and LAMOST. AGUADO D.S., GONZALEZ HERNANDEZ J.I., ALLENDE PRIETO C., et al.
2021ApJ...913...11L viz 17       D               1 1901 19 Targeting bright metal-poor stars in the disk and halo systems of the Galaxy. LIMBERG G., SANTUCCI R.M., ROSSI S., et al.
2021ApJ...923..183L viz 17       D               1 147 ~ Fuzzy cluster analysis: application to determining metallicities for very metal-poor stars. LI H.
2022ApJ...926...26S viz 17       D               2 6507 18 Dynamically Tagged Groups of Metal-poor Stars from the Best and Brightest Survey. SHANK D., BEERS T.C., PLACCO V.M., et al.
2022ApJ...928..173O 272       D     X         7 4 ~ Accurate Metallicities for Very Metal-poor Stars from the Ca II Infrared Triplet. OSORIO Y., AGUADO D.S., ALLENDE PRIETO C., et al.
2022A&A...663A...4S viz 17       D               1 14206 7 Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys. SOUBIRAN C., BROUILLET N. and CASAMIQUELA L.
2023ApJS..266...14T viz 17       D               1 21501 ~ A New Catalog of Am-type Chemically Peculiar Stars Based on LAMOST. TIAN X.-M., WANG Z.-H., ZHU L.-Y., et al.
2025ApJ...992..215I 19       D               4 21 ~ Potassium Abundances in Extremely Metal Poor Stars: Implications for Nucleosynthesis in the Final Stages of Massive Star Evolution. ISHIGAKI M.N., TOMINAGA N., AOKI W., et al.

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