2MASS J14001456+1435527 , the SIMBAD biblio

2MASS J14001456+1435527 , the SIMBAD biblio (19 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST17:05:25

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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
2008ApJ...689L.113N 1 25 51 The abundance spread in the Bootes I dwarf spheroidal galaxy. NORRIS J.E., GILMORE G., WYSE R.F.G., et al.
2009A&A...508L...1F 188     A D     X         6 15 40 Evidence of enrichment by individual SN from elemental abundance ratios in the very metal-poor dSph galaxy Bootes I. FELTZING S., ERIKSSON K., KLEYNA J., et al.
2010ApJ...723.1632N viz 15       D               1 282 153 Chemical enrichment in the faintest galaxies: the carbon and iron abundance spreads in the Bootes I dwarf spheroidal galaxy and the Segue 1 system. NORRIS J.E., WYSE R.F.G., GILMORE G., et al.
2013ApJ...763...61G viz 555       D     X C       14 13 72 Elemental abundances and their implications for the chemical enrichment of the Bootes I ultrafaint galaxy. GILMORE G., NORRIS J.E., MONACO L., et al.
2014MNRAS.439..788H viz 944       D     X C F     23 129 2 Photometric metallicities in Bootes I. HUGHES J., WALLERSTEIN G., DOTTER A., et al.
2014A&A...562A.146I viz 634       D     X C       16 19 33 Chemical compositions of six metal-poor stars in the ultra-faint dwarf spheroidal galaxy Bootes I. ISHIGAKI M.N., AOKI W., ARIMOTO N., et al.
2014MNRAS.440.2665R viz 39           X         1 21 19 Detailed abundance analysis of the brightest star in Segue 2, the least massive galaxy. ROEDERER I.U. and KIRBY E.N.
2015MNRAS.446.4220R 328       D     X C       8 19 13 Chemical enrichment in very low metallicity environments: Bootes I. ROMANO D., BELLAZZINI M., STARKENBURG E., et al.
2016ApJ...826..110F viz 826     A D S   X C       20 59 26 The chemical evolution of the Bootes I ultra-faint dwarf galaxy. FREBEL A., NORRIS J.E., GILMORE G., et al.
2017A&A...604A.129M viz 56       D     X         2 73 18 The formation of the Milky Way halo and its dwarf satellites: a NLTE-1D abundance analysis. I. Homogeneous set of atmospheric parameters. MASHONKINA L., JABLONKA P., PAKHOMOV Y., et al.
2017A&A...608A..89M viz 119           X         3 75 50 The formation of the Milky Way halo and its dwarf satellites: a NLTE-1D abundance analysis. II. Early chemical enrichment. MASHONKINA L., JABLONKA P., SITNOVA T., et al.
2018ApJ...863...89S viz 16       D               1 1159 133 Gaia proper motions and orbits of the ultra-faint Milky Way satellites. SIMON J.D.
2019A&A...631A..43M viz 16       D               1 48 ~ Influence of inelastic collisions with hydrogen atoms on the non-local thermodynamic equilibrium line formation for Fe I and Fe II in the 1D model atmospheres of late-type stars. MASHONKINA L., SITNOVA T., YAKOVLEVA S.A., et al.
2020AJ....160..120J viz 16       D               1 365763 238 APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al.
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.
2022AJ....163..152S viz 17       D               1 583193 11 APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. SPRAGUE D., CULHANE C., KOUNKEL M., et al.
2022ApJS..259...35A viz 17       D               1 611005 320 The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. ABDURRO'UF, ACCETTA K., AERTS C., et al.
2025ApJ...987..121R 280           X C       5 11 ~ Hidden Population III Descendants in Ultrafaint Dwarf Galaxies. ROSSI M., SALVADORI S., SKULADOTTIR A., et al.
2026ApJ...998..117S 20       D               1 609 ~ The Apache Point Observatory Extra-galactic Evolution Experiment (APOeGEE): Chemical Abundance Trends for Seven Dwarf Spheroidal Galaxies in the APOGEE Survey. SHETRONE M., BEATON R.L., HAYES C.R., et al.

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