TYC 22-581-1 , the SIMBAD biblio

TYC 22-581-1 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST16:43:08


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Title First 3 Authors
2015ApJ...798..110L viz 212       D     X         6 15 35 Spectroscopic analysis of metal-poor stars from LAMOST: early results. LI H.-N., ZHAO G., CHRISTLIEB N., et al.
2016ApJS..224....2H viz 16       D               1 31769 226 The K2 ecliptic plane input catalog (EPIC) and stellar classifications of 138,600 targets in campaigns 1-8. HUBER D., BRYSON S.T., HAAS M.R., et al.
2019ApJ...882...40J viz 16       D               1 210 41 The lanthanide fraction distribution in metal-poor stars: a test of neutron star mergers as the dominant r-process site. JI A.P., DROUT M.R. and HANSEN T.T.
2019MNRAS.490.5647M viz 16       D               1 1738 ~ Searching for correlations in Gaia DR2 unbound star trajectories. MONTANARI F., BARRADO D. and GARCIA-BELLIDO J.
2020ApJS..251...15Z viz 16       D               1 20886 38 Phase II of the LAMOST-Kepler/K2 survey. I. Time series of medium-resolution Spectroscopic observations. ZONG W., FU J.-N., DE CAT P., et al.
2021RAA....21...36C 100       D       C       2 17 ~ Searching for r-process-enhanced stars in the LAMOST survey I: the method. CHEN T.-Y., SHI J.-R., BEERS T.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               1 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.
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.
2025ApJS..280...19Q 47           X         1 2 ~ Phase II of the LAMOST-Kepler/K2 Survey. II. Time Domain of Medium-resolution Spectroscopic Observations from 2018 to 2023. QIN M., FU J.-N., ZONG W., et al.

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