MOA 2011-BLG-262 , the SIMBAD biblio

MOA 2011-BLG-262 , the SIMBAD biblio (28 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST08:54:41

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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
2014ApJ...784...28K 39           X         1 39 74 The hunt for exomoons with Kepler (HEK). IV. A search for moons around eight M dwarfs. KIPPING D.M., NESVORNY D., BUCHHAVE L.A., et al.
2014ApJ...785..155B 575     A     X C       14 6 120
MOA-2011-BLG-262Lb: a sub-Earth-mass moon orbiting a gas giant primary or a high velocity planetary system in the galactic bulge. 		BENNETT D.P., BATISTA V., BOND I.A., et al.
2014ApJ...785..156S 410 T   A     X C       9 2 1 New method to measure proper motions of microlensed sources: application to candidate free-floating-planet event
MOA-2011-BLG-262. 		SKOWRON J., UDALSKI A., SZYMANSKI M.K., et al.
2014ApJ...794...71H 15       D               1 24 11 Candidate gravitational microlensing events for future direct lens imaging. HENDERSON C.B., PARK H., SUMI T., et al.
2015ApJ...804...41D 43           X         1 1 8 Viscoelastic models of tidally heated exomoons. DOBOS V. and TURNER E.L.
2015ApJ...809...74F 79           X         2 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.
2015ApJ...814L..11Y 39           X         1 5 8 Lens masses and distances from microlens parallax and flux. YEE J.C.
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 56       D     X         2 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.
2017AJ....154....3K 41           X         1 7 24 MOA-2016-BLG-227Lb: a massive planet characterized by combining light-curve analysis and Keck AO imaging. KOSHIMOTO N., SHVARTZVALD Y., BENNETT D.P., et al.
2017AJ....154...35N 40           X         1 12 4 MOA-2012-BLG-505Lb: a super-Earth-mass planet that probably resides in the Galactic bulge. NAGAKANE M., SUMI T., KOSHIMOTO N., et al.
2017AJ....154...59B 40           X         1 30 10 The star blended with the MOA-2008-BLG-310 source is not the exoplanet host star. BHATTACHARYA A., BENNETT D.P., ANDERSON J., et al.
2017AJ....154...68B 79           X         2 11 2 MOA data reveal a new mass, distance, and relative proper motion for planetary system OGLE-2015-BLG-0954L. BENNETT D.P., BOND I.A., ABE F., et al.
2018AJ....156..136M 41           X         1 4 4 MOA-2015-BLG-337: a planetary system with a low-mass brown dwarf/planetary boundary host, or a brown dwarf binary. MIYAZAKI S., SUMI T., BENNETT D.P., 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.
2021AJ....162...17K viz 17       D               1 54 ~ KMT-2019-BLG-0371 and the limits of Bayesian analysis. KIM Y.H., CHUNG S.-J., YEE J.C., et al.
2021ApJ...918L...8K 42           X         1 13 11 No large dependence of planet frequency on Galactocentric distance. KOSHIMOTO N., BENNETT D.P., SUZUKI D., et al.
2021AJ....162...96R viz 184       D     X         5 15 ~ Shortest microlensing event with a bound planet: KMT-2016-BLG-2605. RYU Y.-H., HWANG K.-H., GOULD A., et al.
2021AJ....162..267S viz 84           X         2 6 ~ Using source proper motion to validate terrestrial parallax: OGLE-2019-BLG-1058. SHIN I.-G., YEE J.C., HWANG K.-H., 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.
2022A&A...664A..33H 85             C       1 36 6 Four sub-Jovian-mass planets detected by high-cadence microlensing surveys. HAN C., KIM D., GOULD A., et al.
2022MNRAS.516.1894Y 43           X         1 17 8 KMT-2021-BLG-0171Lb and KMT-2021-BLG-1689Lb: two microlensing planets in the KMTNet high-cadence fields with followup observations. YANG H., ZANG W., GOULD A., et al.
2024ApJ...967...77N 45           X         1 8 ~ Measurement of Dependence of Microlensing Planet Frequency on the Host Star Mass and Galactocentric Distance by Using a Galactic Model. NUNOTA K., KOSHIMOTO N., SUZUKI D., et al.
2024AJ....168..175H viz 45           X         1 11 ~ RV Measurements of Directly Imaged Brown Dwarf GQ Lup B to Search for Exosatellites. HORSTMAN K., RUFFIO J.-B., BATYGIN K., et al.
2024A&A...692A.106H 18       D               1 16 ~ KMT-2024-BLG-1044L: A sub-Uranus microlensing planet around a host at the star-brown dwarf mass boundary. HAN C., RYU Y.-H., LEE C.-U., et al.
2025AJ....169..131T 1400     A D S   X C F     28 14 ~ A Candidate High-velocity Exoplanet System in the Galactic Bulge. TERRY S.K., BEAULIEU J.-P., BENNETT D.P., et al.
2025AJ....170..339S 65       D     X         2 52 ~ Binary-lens Microlensing Degeneracy: Impact on Planetary Sensitivity and Mass-ratio Function. SHANG Y., YANG H., ZHANG J., et al.

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