MOA 2013-BLG-260 , the SIMBAD biblio

MOA 2013-BLG-260 , the SIMBAD biblio (45 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST07:21:52


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Title First 3 Authors
2014Sci...345...46G 10 4 82 A terrestrial planet in a ∼1-AU orbit around one member of a ∼15-AU binary. GOULD A., UDALSKI A., SHIN I.-G., et al.
2014ApJ...795...42P 41           X         1 12 50 Triple microlens OGLE-2008-BLG-092L: binary stellar system with a circumprimary Uranus-type planet. POLESKI R., SKOWRON J., UDALSKI A., et al.
2015ApJ...809...74F 40           X         1 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...812...47U 41           X         1 5 25 A venus-mass planet orbiting a brown dwarf: a missing link between planets and moons. UDALSKI A., JUNG Y.K., HAN C., et al.
2016MNRAS.457.4089S viz 173       D     X   F     4 31 60 The frequency of snowline-region planets from four years of OGLE-MOA-Wise second-generation microlensing. SHVARTZVALD Y., MAOZ D., UDALSKI A., et al.
2016ApJ...825....8H 40           X         1 4 15 A new nonplanetary interpretation of the microlensing event OGLE-2013-BLG-0723. HAN C., BENNETT D.P., 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 79           X         2 7 ~ Planetary caustic perturbations of a close-separation planet on microlensing. RYU Y.-H., KIM H.-S., CHUNG S.-J., et al.
2016ApJ...830..150P 252       D     X         7 38 33 Is the galactic bulge devoid of planets? PENNY M.T., HENDERSON C.B. and CLANTON C.
2016AJ....152..112M viz 39           X         1 14 11 Very low-mass stellar and substellar companions to solar-like stars from MARVELS. VI. A giant planet and a brown dwarf candidate in a close binary system HD 87646. MA B., GE J., WOLSZCZAN A., et al.
2016AJ....152..125B 42           X         1 11 68 The first circumbinary planet found by microlensing: OGLE-2007-BLG-349L(AB)c. BENNETT D.P., RHIE S.H., UDALSKI A., et al.
2016ApJ...833..145S 40           X         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.
2017MNRAS.466.1555B 40           X         1 28 11 Dynamics and habitability in circumstellar planetary systems of known binary stars. BAZSO A., PILAT-LOHINGER E., EGGL S., et al.
2017A&A...604A.103P 40         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.
2017MNRAS.469.2434B 40           X         1 16 24 The lowest mass ratio planetary microlens: OGLE 2016-BLG-1195Lb. BOND I.A., BENNETT D.P., SUMI T., et al.
2017AJ....154..223H 79           X         2 11 13 OGLE-2016-BLG-0613LABb: a microlensing planet in a binary system. HAN C., UDALSKI A., GOULD A., et al.
2018AJ....156..113B 120           X         3 21 9 A planetary microlensing event with an unusually red source star: MOA-2011-BLG-291. BENNETT D.P., UDALSKI A., BOND I.A., et al.
2019MNRAS.483.3465F 16       D               1 15 3 Dynamical origin of S-type planets in close binary stars. FRAGIONE G.
2019AJ....157...72J 16       D               1 32 7 KMT-2017-BLG-0165Lb: a super-Neptune-mass planet orbiting a Sun-like host star. JUNG Y.K., GOULD A., ZANG W., et al.
2018AcA....68....1U 486           X         12 13 53 OGLE-2017-BLG-1434Lb: eighth q<1×10–4 mass-ratio microlens planet confirms turnover in planet mass-ratio function. UDALSKI A., RYU Y.-H., SAJADIAN S., et al.
2019ApJ...880...72D 41           X         1 8 ~ Triple-lens gravitational microlensing: critical curves for arbitrary spatial configuration. DANEK K. and HEYROVSKY D.
2020AJ....159...48H 82           X         2 15 ~ OGLE-2018-BLG-1700L: microlensing planet in binary stellar system. HAN C., LEE C.-U., UDALSKI A., 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....159..268K 41           X         1 12 ~ Bayesian approach for determining microlens system properties with high-angular-resolution follow-up imaging. KOSHIMOTO N., BENNETT D.P. and SUZUKI D.
2020AJ....160...72B 41           X         1 15 ~ A gas giant planet in the OGLE-2006-BLG-284L stellar binary system. BENNETT D.P., UDALSKI A., BOND I.A., et al.
2020AJ....160...74H viz 41           X         1 29 ~ OGLE-2017-BLG-0406: Spitzer microlens parallax reveals Saturn-mass planet orbiting M-dwarf host in the inner Galactic disk. HIRAO Y., BENNETT D.P., RYU Y.-H., et al.
2020AJ....160..183R 41           X         1 23 ~ OGLE-2018-BLG-0532Lb: cold Neptune with possible jovian sibling. RYU Y.-H., UDALSKI A., YEE J.C., et al.
2020ApJ...903..141S 41           X         1 24 ~ Statistical properties of habitable zones in stellar binary systems. SIMONETTI P., VLADILO G., SILVA L., et al.
2021MNRAS.503.6143K 42           X         1 13 ~ Light-curve calculations for triple microlensing systems. KUANG R., MAO S., WANG T., et al.
2021AJ....161..270H viz 43           X         1 8 11 KMT-2019-BLG-1715: planetary microlensing event with three lens masses and two source stars. HAN C., UDALSKI A., KIM D., et al.
2021AJ....161..279B 84           X         2 13 ~ OGLE-2017-BLG-1434Lb: confirmation of a cold super-Earth using Keck adaptive optics. BLACKMAN J.W., BEAULIEU J.-P., COLE A.A., et al.
2021AJ....161..293J viz 85             C       1 27 27 OGLE-2018-BLG-0567Lb and OGLE-2018-BLG-0962Lb: two microlensing planets through the planetary-caustic channel. JUNG Y.K., HAN C., UDALSKI A., et al.
2021A&A...649A..91H 59       D     X         2 26 ~ KMT-2019-BLG-0797: Binary-lensing event occurring on a binary stellar system. HAN C., LEE C.-U., RYU Y.-H., et al.
2021AJ....162..203H viz 84             C       1 12 3 OGLE-2019-BLG-0304: competing interpretations between a planet-binary model and a binary-source + binary-lens model. HAN C., UDALSKI A., LEE C.-U., et al.
2021A&A...655A..24H 209           X         5 11 4 KMT-2021-BLG-0322: Severe degeneracy between triple-lens and higher-order binary-lens interpretations. HAN C., GOULD A., HIRAO Y., 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.
2022MNRAS.514.5952Z 43           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.
2022MNRAS.516.1704K 85           X         2 20 5 OGLE-2019-BLG-1470LABc: Another microlensing giant planet in a binary system? KUANG R., ZANG W., JUNG Y.K., et al.
2023MNRAS.520.4540K 17       D               1 23 ~ Simulations of triple microlensing events I: detectability of a scaled Sun-Jupiter-Saturn system. KUANG R., ZANG W., MAO S., et al.
2023A&A...672A...8H 44           X         1 24 1 KMT-2021-BLG-1122L: The first microlensing triple stellar system. HAN C., JUNG Y.K., GOULD A., et al.
2023A&A...675A.114C 87               F     1 25 ~ Chasing extreme planetary architectures I. HD 196885 Ab, a super-Jupiter dancing with two stars? CHAUVIN G., VIDELA M., BEUST H., et al.
2023ApJ...956...29Q 17       D               1 40 ~ Prospects for Cryovolcanic Activity on Cold Ocean Planets. QUICK L.C., ROBERGE A., TOVAR MENDOZA G., et al.
2025PASP..137f4401Q 47           X         1 7 ~ Systematic Search for FFPs in KMTNet Full-frame Images. I. Photometry Pipeline. QIAN Q., YANG H., ZANG W., et al.
2025AJ....170...75C 47           X         1 19 ~ KMT-2022-BLG-0086: Another Binary-lens Binary-source Microlensing Event. CHUNG S.-J., HWANG K.-H., YEE J.C., et al.
2025A&A...700A.181H 47           X         1 23 ~ KMT-2024-BLG-0404L: A triple microlensing system consisting of a star, a brown dwarf, and a planet. HAN C., UDALSKI A., LEE C.-U., et al.

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