|
other query modes : |
Identifier query |
Coordinate query |
Criteria query |
Reference query |
Basic query |
Script submission |
TAP |
Output options |
Object types |
Help |
| OGLE-2018-BLG-0567 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST23:31:50 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
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 |
|---|---|---|---|---|---|---|---|---|---|
2021AJ....161..293J 
|
1213 | A | D | X C | 29 | 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. |
|
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. | ||
| 2022AJ....164..262J | 60 | D | X | 2 | 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 | 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...699A..91H | 47 | X | 1 | 29 | ~ | MOA-2022-BLG-091Lb and KMT-2024-BLG-1209Lb: Microlensing planets detected through weak caustic-crossing signals. | HAN C., LEE C.-U., UDALSKI A., et al. |
