MOA 2012-BLG-288 , the SIMBAD biblio

MOA 2012-BLG-288 , the SIMBAD biblio (15 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.06.11CEST19:41:43


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Title First 3 Authors
2013A&A...549A.147B viz 19       D               2 61 387 Chemical evolution of the Galactic Bulge as traced by microlensed dwarf and subgiant stars. V. Evidence for a wide age distribution and a complex MDF. BENSBY T., YEE J.C., FELTZING S., et al.
2015A&A...577A..72V 16       D               1 58 11 On the age of Galactic bulge microlensed dwarf and subgiant stars. VALLE G., DELL'OMODARME M., PRADA MORONI P.G., et al.
2015ApJ...809...74F 358           X C       8 13 35 OGLE-2012-BLG-0563Lb: a saturn-mass planet around an M dwarf with the mass constrained by Subaru AO imaging. FUKUI A., GOULD A., SUMI T., et al.
2016ApJ...830..150P 136       D     X         4 38 33 Is the galactic bulge devoid of planets? PENNY M.T., HENDERSON C.B. and CLANTON C.
2016ApJ...833..145S 18       D               1 64 176 The exoplanet mass-ratio function from the MOA-II survey: discovery of a break and likely peak at a Neptune mass. SUZUKI D., BENNETT D.P., SUMI T., et al.
2017A&A...605A..89B viz 17       D               1 91 141 Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. VI. Age and abundance structure of the stellar populations in the central sub-kpc of the Milky Way. BENSBY T., FELTZING S., GOULD A., et al.
2018AJ....156..104P 82             C       1 12 4 An ice giant exoplanet interpretation of the anomaly in microlensing event OGLE-2011-BLG-0173. POLESKI R., GAUDI B.S., UDALSKI A., et al.
2020ApJ...890...23L viz 17       D               1 4935 35 Current population statistics do not favor photoevaporation over core-powered mass loss as the dominant cause of the exoplanet radius gap. LOYD R.O.P., SHKOLNIK E.L., SCHNEIDER A.C., et al.
2020A&A...634A.130B viz 17       D               1 95 ~ Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. VII. Lithium. BENSBY T., FELTZING S., YEE J.C., et al.
2020AJ....159..268K 1107     A D     X C       26 12 ~ Bayesian approach for determining microlens system properties with high-angular-resolution follow-up imaging. KOSHIMOTO N., BENNETT D.P. and SUZUKI D.
2021A&A...655A.117B viz 17       D               1 93 4 Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. VIII. Carbon and oxygen. BENSBY T., GOULD A., ASPLUND M., et al.
2022A&A...657A..29L 18       D               1 127 5 Sulfur abundances in the Galactic bulge and disk. LUCERTINI F., MONACO L., CAFFAU E., et al.
2022NatAs...6..121C 18       D               1 115 8 Microlensing mass measurement from images of rotating gravitational arcs. CASSAN A., RANC C., ABSIL O., et al.
2022A&A...663A...4S viz 18       D               1 14206 7 Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys. SOUBIRAN C., BROUILLET N. and CASAMIQUELA L.
2023ApJ...946...28J 19       D               1 96 12 The Ages of Galactic Bulge Stars with Realistic Uncertainties. JOYCE M., JOHNSON C.I., MARCHETTI T., et al.

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