EWS 2013-BLG-102 , the SIMBAD biblio

EWS 2013-BLG-102 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST08:32:19


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Title First 3 Authors
2015ApJ...798..123J 344 T   A     X C       7 6 28

OGLE-2013-BLG-0102L
A,B: microlensing binary with components at star/brown dwarf and brown dwarf/planet boundaries.
JUNG Y.K., UDALSKI A., SUMI T., et al.
2015A&A...584A.128L 40           X         1 23 12 An eclipsing double-line spectroscopic binary at the stellar/substellar boundary in the Upper Scorpius OB association. LODIEU N., ALONSO R., GONZALEZ HERNANDEZ J.I., et al.
2016ApJ...822...75H 16       D               1 17 9 OGLE-2014-BLG-0257L: a microlensing brown dwarf orbiting a low-mass M dwarf. HAN C., JUNG Y.K., UDALSKI A., et al.
2016ApJ...827L..22T 16       D               2 44 4 An opportunistic search for extraterrestrial intelligence (SETI) with the murchison widefield array. TINGAY S.J., TREMBLAY C., WALSH A., et al.
2016ApJ...829...43R 40           X         1 7 ~ Planetary caustic perturbations of a close-separation planet on microlensing. RYU Y.-H., KIM H.-S., CHUNG S.-J., et al.
2019ApJ...871..179C 17       D               1 21 3 Spitzer microlensing of MOA-2016-BLG-231L: a counter-rotating brown dwarf binary in the Galactic disk. CHUNG S.-J., GOULD A., SKOWRON J., et al.
2020AJ....159...68B 43           X         1 26 ~ Keck observations confirm a super-Jupiter planet orbiting M dwarf OGLE-2005-BLG-071L. BENNETT D.P., BHATTACHARYA A., BEAULIEU J.-P., 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.
2021A&A...650A..89H 87             C       1 22 12 Three microlensing planets with no caustic-crossing features. HAN C., UDALSKI A., KIM D., 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.
2022MNRAS.514.5952Z 45           X         1 20 11 OGLE-2018-BLG-0799Lb: a q ∼ 2.7 x 10–3 planet with Spitzer parallax. ZANG W., SHVARTZVALD Y., UDALSKI A., et al.

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