MOA 2010-BLG-477 , the SIMBAD biblio

MOA 2010-BLG-477 , the SIMBAD biblio (18 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST02:05:17


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Title First 3 Authors
2012ApJ...754...73B 614           X C       15 5 41 MOA 2010-BLG-477Lb: constraining the mass of a microlensing planet from microlensing parallax, orbital motion, and detection of blended light. BACHELET E., SHIN I.-G., HAN C., et al.
2013A&A...552A.119S viz 15       D               1 1487 118 Magnetic energy fluxes in sub-Alfvenic planet star and moon planet interactions. SAUR J., GRAMBUSCH T., DULING S., et al.
2013MNRAS.431.2975A 38           X         1 6 6 Extending the planetary mass function to Earth mass by microlensing at moderately high magnification. ABE F., AIREY C., BARNARD E., et al.
2014A&A...562A.108S viz 15       D               1 196 44 Search for 150 MHz radio emission from extrasolar planets in the TIFR GMRT Sky Survey. SIROTHIA S.K., LECAVELIER DES ETANGS A., GOPAL-KRISHNA, et al.
2014ApJ...794...71H 54       D     X         2 24 11 Candidate gravitational microlensing events for future direct lens imaging. HENDERSON C.B., PARK H., SUMI T., et al.
2015ApJ...802..108S 195     A D     X         6 12 1 Constraint on additional planets in planetary systems discovered through the channel of high-magnification gravitational microlensing events. SHIN I.-G., HAN C., CHOI J.-Y., 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...830..150P 16       D               1 38 33 Is the galactic bulge devoid of planets? PENNY M.T., HENDERSON C.B. and CLANTON C.
2016ApJ...833..145S 17       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.
2020ApJ...890...23L viz 16       D               1 4936 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.
2020AJ....160..183R 82           X         2 23 ~ OGLE-2018-BLG-0532Lb: cold Neptune with possible jovian sibling. RYU Y.-H., UDALSKI A., YEE J.C., et al.
2021Natur.598..272B 470           X C       10 3 31 A Jovian analogue orbiting a white dwarf star. BLACKMAN J.W., BEAULIEU J.P., BENNETT D.P., et al.
2022NatAs...6..121C 17       D               1 115 8 Microlensing mass measurement from images of rotating gravitational arcs. CASSAN A., RANC C., ABSIL O., et al.
2023MNRAS.522.6055Z 44           X         1 16 1 KMT-2022-BLG-0440Lb: A new q < 10–4 microlensing planet with the central-resonant caustic degeneracy broken. ZHANG J., ZANG W., JUNG Y.K., et al.
2023ApJ...950..128O 44           X         1 4 2 Giant Planet Engulfment by Evolved Giant Stars: Light Curves, Asteroseismology, and Survivability. O'CONNOR C.E., BILDSTEN L., CANTIELLO M., et al.
2024AJ....167..154K viz 45           X         1 12 ~ OGLE-2014-BLG-0221Lb: A Jupiter Mass Ratio Companion Orbiting Either a Late-type Star or a Stellar Remnant. KIRIKAWA R., SUMI T., BENNETT D.P., et al.
2024AJ....168...15B 45           X         1 23 ~ Keck and Hubble Observations Show that MOA-2008-BLG-379Lb is a Super-Jupiter Orbiting an M Dwarf. BENNETT D.P., BHATTACHARYA A., BEAULIEU J.-P., et al.
2025AJ....170..310V 47           X         1 6 ~ MOA-2010-BLG-328: Keck and HST Expose the Limits of Occams Razor in Microlensing. VANDOROU A., BENNETT D.P., BEAULIEU J.-P., et al.

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