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| OGLE-2006-BLG-284 , the SIMBAD biblio (14 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST19:01:01 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| 2010AcA....60..197J | 63 | 12 | Binary lenses in OGLE-III EWS database. Seasons 2006-2008. | JAROSZYNSKI M., SKOWRON J., UDALSKI A., et al. | |||||
| 2020AJ....160...72B | 354 | T A | X C | 7 | 15 | ~ |
A gas giant planet in the OGLE-2006-BLG-284L stellar binary system. |
BENNETT D.P., UDALSKI A., BOND I.A., 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..270H 
|
43 | X | 1 | 8 | 11 | KMT-2019-BLG-1715: planetary microlensing event with three lens masses and two source stars. | HAN C., UDALSKI A., KIM D., et al. | ||
|
2021AJ....162..203H
|
125 | X C | 2 | 12 | 3 | OGLE-2019-BLG-0304: competing interpretations between a planet-binary model and a binary-source + binary-lens model. | HAN C., UDALSKI A., LEE C.-U., et al. | ||
| 2022MNRAS.516.1704K | 85 | X | 2 | 20 | 5 | OGLE-2019-BLG-1470LABc: Another microlensing giant planet in a binary system? | KUANG R., ZANG W., JUNG Y.K., et al. | ||
| 2023A&A...670A.172H | 17 | D | 1 | 23 | 1 | OGLE-2018-BLG-0584 and KMT-2018-BLG-2119: Two microlensing events with two lens masses and two source stars. | HAN C., UDALSKI A., JUNG Y.K., et al. | ||
| 2023MNRAS.520.4540K | 17 | D | 1 | 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 | 44 | X | 1 | 24 | 1 | KMT-2021-BLG-1122L: The first microlensing triple stellar system. | HAN C., JUNG Y.K., GOULD A., et al. | ||
| 2023A&A...678A.101H | 44 | X | 1 | 21 | ~ | KMT-2021-BLG-1547Lb: Giant microlensing planet detected through a signal deformed due to source binarity. | HAN C., ZANG W., JUNG Y.K., et al. | ||
| 2024A&A...692A.221H | 18 | D | 1 | 31 | ~ | KMT-2021-BLG-0284, KMT-2022-BLG-2480, and KMT-2024-BLG-0412: Three microlensing events involving two lens masses and two source stars. | HAN C., UDALSKI A., BOND I.A., et al. | ||
| 2025AJ....170...75C | 47 | X | 1 | 19 | ~ | KMT-2022-BLG-0086: Another Binary-lens Binary-source Microlensing Event. | CHUNG S.-J., HWANG K.-H., YEE J.C., et al. | ||
| 2025A&A...700A.181H | 93 | X | 2 | 23 | ~ | KMT-2024-BLG-0404L: A triple microlensing system consisting of a star, a brown dwarf, and a planet. | HAN C., UDALSKI A., LEE C.-U., et al. | ||
| 2025PASP..137j4501H | 47 | X | 1 | 34 | ~ | Three Binary-source Binary-lens Microlensing Events from the 2024 Microlensing Campaign. | HAN C., LEE C.-U., UDALSKI A., et al. |
