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| OGLE-2019-BLG-0954 , the SIMBAD biblio (11 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST12:46:58 |
| 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 | 84 | A | D | S X C | 1 | 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..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. | ||
|
2022AJ....163...43H |
17 | D | 2 | 59 | 29 | Systematic KMTNet planetary anomaly search. II. Six new q < 2 x 10–4 mass-ratio planets. | HWANG K.-H., ZANG W., GOULD A., et al. | ||
| 2022MNRAS.515..928Z | 145 | D | X | 4 | 24 | 19 | Systematic KMTNet planetary anomaly search. IV. Complete sample of 2019 prime-field. | ZANG W., YANG H., HAN C., et al. | |
| 2022A&A...666A.132H | 43 | X | 1 | 41 | 3 | KMT-2017-BLG-0673Lb and KMT-2019-BLG-0414Lb: Two microlensing planets detected in peripheral fields of KMTNet survey. | HAN C., LEE C.-U., GOULD 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 | 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. | ||
| 2025ApJ...995L..55Z | 19 | D | 1 | 18 | ~ | The Brown-dwarf Desert Persists as a Mass-ratio Desert around Low-mass Stars. | ZHANG K. |