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| OGLE-2014-BLG-1722 , the SIMBAD biblio (17 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST03:07:17 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2018AJ....155..263S | 666 | A | X C | 16 | 16 | 8 | A likely detection of a two-planet system in a low-magnification microlensing event. | SUZUKI D., BENNETT D.P., UDALSKI A., et al. | |
| 2019ApJ...878L..29M | 81 | C | 1 | 20 | ~ | A pair of planets likely in mean-motion resonance from gravitational microlensing. | MADSEN S. and ZHU W. | ||
| 2019ApJ...880...72D | 41 | X | 1 | 8 | ~ | Triple-lens gravitational microlensing: critical curves for arbitrary spatial configuration. | DANEK K. and HEYROVSKY D. | ||
| 2019AJ....158..114H | 122 | X | 3 | 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. | ||
| 2020AJ....159...48H | 123 | X C | 2 | 15 | ~ | OGLE-2018-BLG-1700L: microlensing planet in binary stellar system. | HAN C., LEE C.-U., UDALSKI A., et al. | ||
|
2020ApJ...890...23L |
16 | D | 2 | 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...17H | 41 | X | 1 | 10 | ~ | One planet or two planets? The ultra-sensitive extreme-magnification microlensing event KMT-2019-BLG-1953. | HAN C., KIM D., JUNG Y.K., et al. | ||
| 2021MNRAS.503.6143K | 42 | X | 1 | 13 | ~ | Light-curve calculations for triple microlensing systems. | KUANG R., MAO S., WANG T., et al. | ||
|
2021AJ....161..293J |
85 | C | 1 | 27 | 27 | OGLE-2018-BLG-0567Lb and OGLE-2018-BLG-0962Lb: two microlensing planets through the planetary-caustic channel. | JUNG Y.K., HAN C., UDALSKI A., et al. | ||
| 2021A&A...649A..91H | 59 | D | X | 2 | 26 | ~ | KMT-2019-BLG-0797: Binary-lensing event occurring on a binary stellar system. | HAN C., LEE C.-U., RYU Y.-H., 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. | ||
| 2022A&A...658A..93H | 43 | X | 1 | 31 | 10 | OGLE-2019-BLG-0468Lb,c: Two microlensing giant planets around a G-type star. | HAN C., UDALSKI A., LEE C.-U., 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. | ||
| 2022A&A...662A..70H | 43 | X | 1 | 16 | 9 | KMT-2021-BLG-1077L: The fifth confirmed multiplanetary system detected by microlensing. | HAN C., GOULD A., BOND I.A., et al. | ||
| 2023MNRAS.520.4540K | 61 | D | X | 2 | 23 | ~ | Simulations of triple microlensing events I: detectability of a scaled Sun-Jupiter-Saturn system. | KUANG R., ZANG W., MAO S., et al. | |
| 2023A&A...672A...8H | 87 | C | 1 | 24 | 1 | KMT-2021-BLG-1122L: The first microlensing triple stellar system. | HAN C., JUNG Y.K., GOULD A., et al. | ||
| 2025A&A...694A.219B | 47 | X | 1 | 6 | ~ | VBMicroLensing: Three algorithms for multiple lensing with contour integration. | BOZZA V., SAGGESE V., COVONE G., et al. |