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| MOA 2012-BLG-527 , the SIMBAD biblio (28 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST10:15:22 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2016ApJ...833..145S | 213 | D | X | 6 | 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....153....1K | 281 | X C | 6 | 3 | 22 | OGLE-2012-BLG-0950Lb: the first planet mass measurement from only microlens parallax and lens flux. | KOSHIMOTO N., UDALSKI A., BEAULIEU J.P., 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. | ||
| 2018AJ....156..226H | 281 | X | 7 | 17 | 4 | MOA-2016-BLG-319Lb: microlensing planet subject to rare minor-image perturbation degeneracy in determining planet parameters. | HAN C., BOND I.A., GOULD A., et al. | ||
| 2018AJ....156..236Z | 40 | X | 1 | 20 | 5 | KMT-2016-BLG-1397b: KMTNET-only discovery of a microlens giant planet. | ZANG W., HWANG K.-H., KIM H.-W., et al. | ||
| 2018AJ....156..289B | 428 | A | X | 11 | 7 | 26 |
WFIRST exoplanet mass-measurement method finds a planetary mass of 39 ± 8 M⊕ for OGLE-2012-BLG-0950Lb. |
BHATTACHARYA A., BEAULIEU J.-P., BENNETT D.P., et al. | |
| 2018ApJ...869L..34S | 75 | X | 1 | 2 | 70 | Microlensing results challenge the core accretion runaway growth scenario for gas giants. | SUZUKI D., BENNETT D.P., IDA S., et al. | ||
| 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. | ||
| 2019ApJ...872..175J | 81 | X | 2 | 6 | 2 | OGLE-2016-BLG-0156: microlensing event with pronounced microlens-parallax effects yielding a precise lens mass measurement. | JUNG Y.K., HAN C., BOND I.A., et al. | ||
| 2019AJ....157..232R | 41 | X | 1 | 22 | 1 | OGLE-2015-BLG-1670Lb: a cold Neptune beyond the snow line in the provisional WFIRST microlensing survey Field. | RANC C., BENNETT D.P., HIRAO Y., et al. | ||
|
2019ApJS..244...29M |
16 | D | 1 | 5755 | 55 | Microlensing optical depth and event rate toward the Galactic bulge from 8 yr of OGLE-IV observations. | MROZ P., UDALSKI A., SKOWRON J., et al. | ||
| 2020AJ....159...68B | 41 | X | 1 | 26 | ~ | Keck observations confirm a super-Jupiter planet orbiting M dwarf OGLE-2005-BLG-071L. | BENNETT D.P., BHATTACHARYA A., BEAULIEU J.-P., 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....159..256H |
43 | X | 1 | 7 | 18 | OGLE-2018-BLG-0677Lb: a super-earth near the Galactic bulge. | HERRERA-MARTIN A., ALBROW M.D., UDALSKI A., et al. | ||
| 2020AJ....159..268K | 1729 | A | D | X C | 42 | 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..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. | ||
|
2021AJ....161...54T |
42 | X | 1 | 7 | ~ | MOA-2009-BLG-319Lb: a sub-Saturn planet inside the predicted mass desert. | TERRY S.K., BHATTACHARYA A., BENNETT D.P., et al. | ||
|
2021A&A...649A..90H |
84 | C | 1 | 22 | ~ | KMT-2018-BLG-1025Lb: microlensing super-Earth planet orbiting a low-mass star. | HAN C., UDALSKI A., LEE C.-U., et al. | ||
| 2021AJ....162...60B | 42 | X | 1 | 9 | ~ | MOA-2007-BLG-400 a super-Jupiter-mass planet orbiting a Galactic bulge K-dwarf revealed by Keck adaptive optics imaging. | BHATTACHARYA A., BENNETT D.P., BEAULIEU J.P., 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. | ||
| 2021RAA....21..239Z | 43 | X | 1 | 17 | 27 | An Earth-mass planet in a time of COVID-19: KMT-2020-BLG-0414Lb. | ZANG W., HAN C., KONDO I., 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.515..928Z | 170 | X C | 3 | 24 | 19 | Systematic KMTNet planetary anomaly search. IV. Complete sample of 2019 prime-field. | ZANG W., YANG H., HAN C., et al. | ||
|
2023AJ....165..103Z |
44 | X | 1 | 45 | 8 | Systematic KMTNet Planetary Anomaly Search. VII. Complete Sample of q < 10–4 Planets from the First 4 yr Survey. | ZANG W., JUNG Y.K., YANG H., 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. | ||
| 2023AJ....166..145G | 87 | X | 2 | 18 | ~ | OGLE-2016-BLG-1195 AO: Lens, Companion to Lens or Source, or None of the Above? | GOULD A., SHVARTZVALD Y., ZHANG J., 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. | ||
| 2024AJ....168..152J | 287 | D | X C F | 5 | 16 | ~ | KMT-2023-BLG-2669: Ninth Free-floating Planet Candidate with θE Measurements. | JUNG Y.K., HWANG K.-H., YANG H., et al. |