MOA 2014-BLG-307 , the SIMBAD biblio

MOA 2014-BLG-307 , the SIMBAD biblio (28 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST21:58:30


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Title First 3 Authors
2015ApJ...799..237U 848 T   A S   X C       19 8 101 Spitzer as a microlens parallax satellite: mass measurement for the

OGLE-2014-BLG-0124L
planet and its host star.
UDALSKI A., YEE J.C., GOULD A., et al.
2015ApJ...804...20C 118           X C       2 30 68 Pathway to the galactic distribution of planets: combined Spitzer and ground-based microlens parallax measurements of 21 single-lens events. CALCHI NOVATI S., GOULD A., UDALSKI A., et al.
2015ApJ...805....8Z 119           X         3 6 34 Spitzer as a microlens parallax satellite: mass and distance measurements of the binary lens system OGLE-2014-BLG-1050L. ZHU W., UDALSKI A., GOULD A., et al.
2015ApJ...814L..11Y 156           X C       3 5 8 Lens masses and distances from microlens parallax and flux. YEE J.C.
2015ApJ...814..129Z 843     A S   X C       20 4 8 Planet sensitivity from combined ground- and space-based microlensing observations. ZHU W., GOULD A., BEICHMAN C., et al.
2016ApJ...819...93S 42           X         1 9 66 Spitzer parallax of OGLE-2015-BLG-0966: a cold Neptune in the galactic disk. STREET R.A., UDALSKI A., CALCHI NOVATI S., 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...824..109C 39           X         1 5 9 Microlensing parallax for observers in heliocentric motion. CALCHI NOVATI S. and SCARPETTA G.
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 94       D       C       3 38 33 Is the galactic bulge devoid of planets? PENNY M.T., HENDERSON C.B. and CLANTON C.
2017ApJ...834...82H 40           X         1 7 8 OGLE-2015-BLG-0196: ground-based gravitational microlens parallax confirmed by space-based observation. HAN C., UDALSKI A., GOULD A., et al.
2017ApJ...845..129W 16       D               1 12 8 Ground-based parallax confirmed by Spitzer: binary microlensing event MOA-2015-BLG-020. WANG T., ZHU W., MAO S., et al.
2018AJ....155...40R 97       D       C       2 17 21 OGLE-2016-BLG-1190Lb: the first Spitzer bulge planet lies near the planet/brown-dwarf boundary. RYU Y.-H., YEE J.C., UDALSKI A., et al.
2018ApJ...853...70U 41           X         1 7 7 OGLE-2014-BLG-0289: precise characterization of a quintuple-peak gravitational microlensing event. UDALSKI A., HAN C., BOZZA V., et al.
2018AJ....155...78B 594     A S   X C       13 2 17 Combining Spitzer parallax and Keck II adaptive optics imaging to measure the mass of a solar-like star orbited by a cold gaseous planet discovered by microlensing. BEAULIEU J.-P., BATISTA V., BENNETT D.P., et al.
2018ApJ...859...82H 40           X         1 7 4 OGLE-2017-BLG-0329L: a microlensing binary characterized with dramatically enhanced precision using data from space-based observations. HAN C., CALCHI NOVATI S., UDALSKI A., et al.
2018AJ....155..261C 80             C       1 15 8 Spitzer opens new path to break classic degeneracy for Jupiter-mass microlensing planet OGLE-2017-BLG-1140Lb. CALCHI NOVATI S., SKOWRON J., JUNG Y.K., et al.
2018ApJ...860...25W 81           X         2 3 4 OGLE-2017-BLG-1130: the first binary gravitational microlens detected from Spitzer only. WANG T., CALCHI NOVATI S., UDALSKI A., et al.
2018ApJ...863...22J 40           X         1 11 4 OGLE-2017-BLG-0537: a microlensing event with a resolvable lens in <=5 years from high-resolution follow-up observations. JUNG Y.K., HAN C., UDALSKI A., et al.
2019ApJ...873...30S 16       D               2 19 3 OGLE-2014-BLG-0962 and a comparison of Galactic model priors to microlensing data. SHAN Y., YEE J.C., UDALSKI A., et al.
2019AJ....157..121C 42           X         1 13 16 Spitzer microlensing parallax for OGLE-2016-BLG-1067: a sub-Jupiter orbiting an M dwarf in the disk. CALCHI NOVATI S., SUZUKI D., 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....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.
2021MNRAS.506.2482H viz 17       D               1 1962 ~ A microlensing search of 700 million VVV light curves. HUSSEINIOVA A., McGILL P., SMITH L.C., 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.
2024AJ....167...88R 45           X         1 32 ~ Systematic KMTNet Planetary Anomaly Search. X. Complete Sample of 2017 Prime-field Planets. RYU Y.-H., UDALSKI A., YEE J.C., et al.
2025ApJ...994..144M 280       S   X C       4 1 ~ microJAX: A Differentiable Framework for Microlensing Modeling with GPU-accelerated Image-centered Ray Shooting. MIYAZAKI S. and KAWAHARA H.

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