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| KMT-2018-BLG-1976 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST09:44:38 |
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More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2021A&A...650A..89H | 1756 | A | D | S X C | 41 | 22 | 12 | Three microlensing planets with no caustic-crossing features. | HAN C., UDALSKI A., KIM D., et al. |
| 2021A&A...655A..21H | 42 | X | 1 | 22 | 8 | Three faint-source microlensing planets detected via the resonant-caustic channel. | HAN C., UDALSKI A., KIM D., et al. | ||
| 2022A&A...658A..62H | 43 | X | 1 | 40 | ~ | KMT-2018-BLG-1988Lb: Microlensing super-Earth orbiting a low-mass disk dwarf. | HAN C., GOULD A., ALBROW M.D., 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..782Z | 85 | C | 1 | 31 | 15 | A ubiquitous unifying degeneracy in two-body microlensing systems. | ZHANG K., GAUDI B.S. and BLOOM J.S. | ||
| 2022AJ....164..262J | 145 | D | X | 4 | 45 | 11 | Systematic KMTNet Planetary Anomaly Search. VI. Complete Sample of 2018 Sub-prime-field Planets. | JUNG Y.K., ZANG W., HAN C., et al. | |
| 2024A&A...683A.115H | 45 | X | 1 | 21 | ~ | Three sub-Jovian-mass microlensing planets: MOA-2022-BLG-563Lb, KMT-2023-BLG-0469Lb, and KMT-2023-BLG-0735Lb. | HAN C., JUNG Y.K., BOND I.A., et al. | ||
| 2024A&A...687A.225H | 45 | X | 1 | 24 | ~ | Four microlensing giant planets detected through signals produced by minor-image perturbations. | HAN C., BOND I.A., LEE C.-U., et al. | ||
| 2024A&A...689A.209H | 45 | X | 1 | 31 | ~ | KMT-2021-BLG-2609Lb and KMT-2022-BLG-0303Lb: Microlensing planets identified through signals produced by major-image perturbations. | HAN C., ALBROW M.D., LEE C.-U., et al. | ||
| 2025A&A...694A..90H | 93 | X | 2 | 30 | ~ | MOA-2022-BLG-033Lb, KMT-2023-BLG-0119Lb, and KMT-2023-BLG-1896Lb: Three low mass-ratio microlensing planets detected through dip signals. | HAN C., BOND I.A., JUNG Y.K., et al. |
