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| NAME EWS 2012-BLG-0026c , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST06:30:06 |
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| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2013ApJ...762L..28H | 82 | T | 1 | 5 | 58 | The second multiple-planet system discovered by microlensing: OGLE-2012-BLG-0026Lb, c–A pair of jovian planets beyond the snow line. | HAN C., UDALSKI A., CHOI J.-Y., et al. | ||
| 2013ApJ...768..126G | 38 | X | 1 | 12 | 8 | OGLE-2011-BLG-0417: a radial velocity testbed for microlensing. | GOULD A., SHIN I.-G., HAN C., et al. | ||
| 2014MNRAS.439..604S | 39 | X | 1 | 15 | 29 | MOA-2011-BLG-322Lb: a `second generation survey' microlensing planet. | SHVARTZVALD Y., MAOZ D., KASPI S., et al. | ||
| 2014ApJ...788...73Z | 15 | D | 1 | 28 | 24 | Predictions for microlensing planetary events from core accretion theory. | ZHU W., PENNY M., MAO S., et al. | ||
| 2016ApJ...824...83B | 42 | X | 1 | 5 | 32 | Revisiting the microlensing event OGLE 2012-BLG-0026: a solar mass star with two cold giant planets. | BEAULIEU J.-P., BENNETT D.P., BATISTA V., et al. | ||
| 2017AJ....153..143M | 79 | C | 1 | 53 | 15 | OGLE-2016 a high-mass planet from a high-magnification pure-survey microlensing event. | MROZ P., HAN C., UDALSKI A., et al. | ||
| 2018MNRAS.473..345W | 16 | D | 1 | 69 | 1 | Transit visibility zones of the Solar system planets. | WELLS R., POPPENHAEGER K., WATSON C.A., 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. | ||
| 2019ApJ...878L..29M | 41 | X | 1 | 20 | ~ | A pair of planets likely in mean-motion resonance from gravitational microlensing. | MADSEN S. and ZHU W. | ||
| 2019AJ....158..114H | 41 | X | 1 | 29 | ~ | OGLE-2018-BLG-1011Lb,c: microlensing planetary system with two giant planets orbiting a low-mass star. | HAN C., BENNETT D.P., UDALSKI A., et al. |
