Image Details
Caption: Figure 11.
Comparison between BAGLE, VBMicrolensing, and pyLIMA for a simulated PSPL + parallax event’s normalized separation, u(t). The normalized source–lens separation over time is shown (top) along with the residuals (bottom). We use the same microlensing parameters as in Figure 10: t0,⊙ = 55775 MJD, u0,⊙ = 1, tE,⊙ = 100 days, πE,E = 0.2, πE,N = 0.1, bsff = 1, and magS = 19.
© 2026. The Author(s). Published by the American Astronomical Society.