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| KMT-2022-BLG-0475 , the SIMBAD biblio (6 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST20:27:31 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
| 2023A&A...676A..97H | 131 | A | D | S X C | 2 | 5 | ~ |
KMT-2022-BLG-0475Lb and KMT-2022-BLG-1480Lb: Microlensing ice giants detected via the non-caustic-crossing channel. |
HAN C., LEE C.-U., BOND I.A., 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 | 47 | X | 1 | 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. | ||
| 2025A&A...696A..94D | 19 | D | 1 | 44 | ~ | Earth-like planet predictor: A machine learning approach. | DAVOULT J., ELTSCHINGER R. and ALIBERT Y. |
