[KCB2015] Reti 18 , the SIMBAD biblio

[KCB2015] Reti 18 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST09:38:16

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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
2015ApJ...808...95S viz 16       D               1 72 135 Stellar kinematics and metallicities in the ultra-faint dwarf galaxy Reticulum II. SIMON J.D., DRLICA-WAGNER A., LI T.S., et al.
2015ApJ...808..108W viz 16       D               1 47 60 Magellan/M2FS spectroscopy of the Reticulum 2 dwarf spheroidal galaxy. WALKER M.G., MATEO M., OLSZEWSKI E.W., et al.
2015ApJ...811...62K 17       D               1 52 132 Kinematics and chemistry of recently discovered Reticulum 2 and Horologium 1 dwarf galaxies. KOPOSOV S.E., CASEY A.R., BELOKUROV V., et al.
2016AJ....151...82R viz 608       D     X C       15 24 128 Detailed chemical abundances in the r-process-rich ultra-faint dwarf galaxy Reticulum 2. ROEDERER I.U., MATEO M., BAILEY III J.I., et al.
2016Natur.531..610J 22       D               1 20 279 r-process enrichment from a single event in an ancient dwarf galaxy. JI A.P., FREBEL A., CHITI A., et al.
2016ApJ...826..110F viz 39           X         1 59 26 The chemical evolution of the Bootes I ultra-faint dwarf galaxy. FREBEL A., NORRIS J.E., GILMORE G., et al.
2016ApJ...830...93J viz 254       D     X         7 26 135 Complete element abundances of nine stars in the r-process galaxy Reticulum II. JI A.P., FREBEL A., SIMON J.D., et al.
2017ApJ...838...44H viz 79             C       1 49 92 An r-process enhanced star in the dwarf galaxy Tucana III. HANSEN T.T., SIMON J.D., MARSHALL J.L., et al.
2018ApJ...856..138J 42           X         1 13 27 From actinides to zinc: using the full abundance pattern of the brightest star in Reticulum II to distinguish between different r-process sites. JI A.P. and FREBEL A.
2018ApJ...863...89S viz 16       D               1 1159 133 Gaia proper motions and orbits of the ultra-faint Milky Way satellites. SIMON J.D.
2018A&A...620A.155M viz 16       D               1 292 22 With and without spectroscopy: Gaia DR2 proper motions of seven ultra-faint dwarf galaxies. MASSARI D. and HELMI A.
2019ApJ...875...77P viz 16       D               1 430 71 Proper motions of Milky Way ultra-faint satellites With Gaia DR2 X DES DR1. PACE A.B. and LI T.S.
2020A&A...636A.111A 16       D               1 44 ~ Chemical abundance analysis of extremely metal-poor stars in the Sextans dwarf spheroidal galaxy. AOKI M., AOKI W. and FRANCOIS P.
2020AJ....160..124M 16       D               2 174 54 Revised and new proper motions for confirmed and candidate Milky Way dwarf galaxies. McCONNACHIE A.W. and VENN K.A.
2020A&A...641A.127R viz 99       D   O X         3 401 41 Neutron-capture elements in dwarf galaxies. III. A homogenized analysis of 13 dwarf spheroidal and ultra-faint galaxies. REICHERT M., HANSEN C.J., HANKE M., et al.
2023AJ....165..100J viz 17       D               1 139 10 Metal Mixing in the r-process Enhanced Ultrafaint Dwarf Galaxy Reticulum II. JI A.P., SIMON J.D., ROEDERER I.U., et al.
2023A&A...676A.129H viz 17       D               1 114943 ~ The Gaia-ESO Survey: Homogenisation of stellar parameters and elemental abundances. HOURIHANE A., FRANCOIS P., WORLEY C.C., et al.
2023ApJ...955...17H 2150       D     X C       49 19 ~ GHOST Commissioning Science Results: Identifying a New Chemically Peculiar Star in Reticulum II. HAYES C.R., VENN K.A., WALLER F., et al.
2024ApJ...970L..30X 18       D               1 81 ~ Discovery of an Extremely r-process-enhanced Thin-disk Star with [Eu/H] = +0.78. XIE X.-J., SHI J., YAN H.-L., et al.
2024A&A...692A.228C viz 18       D               1 49864 ~ Inferring stellar parameters and their uncertainties from high-resolution spectroscopy using invertible neural networks. CANDEBAT N., SACCO G.G., MAGRINI L., et al.
2025RAA....25h5015A 47           X         1 14 ~ The Abundance Origin of a Highly r-process Enhanced r-II Star: LAMOST J020623.21+494127.9. ASHRAF M.Z., CUI W. and LI H.

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