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