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Table 1.

Our quality cuts applied to the raw target list of high-proper-motion stars, background sources, and events.

Application Criteria
Lenses μtot > 150 mas yr−1
Lenses ϖ/σϖ >  8
Lenses ϖ/μtot <  0.3 yr
Lenses
Sources (Sou_ϖ + 0.029 mas)/Sou_σϖ >  −3
Sources
Sources |μtot − Sou_μtot|  <  0.7 ⋅ |μtot|
Sources Sou_ϖ <  ϖ
Events δθ+ >  0.1 mas

Notes. These quantetites based on the position (ra,  dec), the total proper motion (μtot), the parallax (ϖ), the number of photometric observations in G (nobs) by Gaia, the G flux (G_flux), the corresponding errors (σ) as well as the expected shift of the brightest image (δθ+). Parameters from the background source are indicated with a Sou_prefix.

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