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Table 1.
Seven most probable alignments before 2035.5, ordered chronologically.
| Lens DR2 id | Lens G | Source DR2 id | Source G | P(d < 1RE) | fmax | Tmax |
|---|---|---|---|---|---|---|
| 4116504399886241792a | 13.86 | 4116504399831319424b | 18.85 | 19.95 |  |
2020 Jul 3–22 |
| 2042703905028908928c | 14.70 | 2042703900727995008 | 18.60 | 76.77 |  |
2025 Jul 20–27 |
| 2030898139472914688 | 15.62 | 2030898105088410112 | 19.92 | 49.29 |  |
2025 Sep 1–16 |
| 5903487940560263936d | 14.63 | 5903487940560263808 | 17.86 | 44.60 |  |
2026 May 25–Jun 7 |
| 318399257231042304e,f | 17.27 | 318399257231042048 | 17.94 | 35.85 |  |
2028 Jul 10–27 |
| 5918299904067162240g | 14.91 | 5918299908365843840 | 13.90 | 45.93 |  |
2030 Mar 31–Apr 2 |
| 3425318817510655360h | 16.15 | 3425318813215052288 | 19.35 | 27.96 |  |
2034 Sep 7–19 |
Notes. We give Gaia DR2 identifiers for the lens and the source, the probability of passage within one Einstein radius P(d < 1RE), the median and 68% confidence intervals for the peak net magnification (including dilution by the lens), and the epoch of peak magnification. Alternative identifiers for the lenses are given in the footnotes (marked ‘?’ where not certain). Further details for these and all 30 pairs are given in the appendix.
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