MOA 2010-BLG-73 , the SIMBAD biblio

MOA 2010-BLG-73 , the SIMBAD biblio (15 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST20:37:58


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Title First 3 Authors
2013ApJ...763...67S 999 T   A     X C       24 9 30

MOA-2010-BLG-073L
: an m-dwarf with a substellar companion at the Planet/Brown dwarf boundary.
STREET R.A., CHOI J.-Y., TSAPRAS Y., et al.
2013ApJ...763..141G 78           X         2 12 16 MOA-2010-BLG-523: "Failed planet" = RS CVn star. GOULD A., YEE J.C., BOND I.A., et al.
2014ApJ...794...71H 39           X         1 24 11 Candidate gravitational microlensing events for future direct lens imaging. HENDERSON C.B., PARK H., SUMI T., et al.
2015A&A...580A.125R 79           X         2 20 10 MOA-2007-BLG-197: Exploring the brown dwarf desert. RANC C., CASSAN A., ALBROW M.D., 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.
2017A&A...604A.103P 41         O X         1 14 10 A companion on the planet/brown dwarf mass boundary on a wide orbit discovered by gravitational microlensing. POLESKI R., UDALSKI A., BOND I.A., et al.
2018AJ....156..236Z 82             C       1 20 5 KMT-2016-BLG-1397b: KMTNET-only discovery of a microlens giant planet. ZANG W., HWANG K.-H., KIM H.-W., et al.
2018ApJS..239...14J viz 16       D               1 1561 6 Revised exoplanet radii and habitability using Gaia data release 2. JOHNS D., MARTI C., HUFF M., 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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