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| MOA 2011-BLG-291 , the SIMBAD biblio (6 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST16:37:09 |
| 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 | 135 | D | X | 4 | 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. | |
| 2018AJ....156..113B | 787 | T A | X C | 18 | 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.488.3308L | 41 | X | 1 | 5 | 2 | OGLE-2017-BLG-1186: first application of asteroseismology and Gaussian processes to microlensing. | LI S.-S., ZANG W., 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. | ||
|
2021AJ....162...17K |
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. | ||
| 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. |