Image Details
Caption: Figure 16.
The impact of changing the lens parallax in BAGLE models for PSPL photometry (top) and astrometry (bottom). Five models are shown (different colors) with similar lightcurves, but with different lens distances and lens masses ML ∝ 10 M⊙(0.2/πrel). The remaining model parameters include β = 0.5, XS,0,⊙ = [0.00, 0.50] mas, μL,⊙ = [0, 0] mas yr−1, μS,⊙ = [0, 2] mas yr−1, dS = 8 kpc, bSFF = 1, magS = 19, t0 = 57200 MJD, α = 262﹩\mathop{.}\limits^{\unicode{x000b0}}﹩5, and δ = −30°.
© 2026. The Author(s). Published by the American Astronomical Society.