Image Details
Caption: Figure 13.
Comparison between BAGLE and VBMicrolensing’s amplifications for a simulated FSPL event without a parallax. The amplification (top) and residuals with respect to the BAGLE model (bottom) are shown over time. The heliocentric SSB model parameters for this event are t0,⊙ = 55775 MJD, u0,⊙ = 0.044, tE,⊙ = 206 days, bsff = 1, and ρ* = 0.177 θE
© 2026. The Author(s). Published by the American Astronomical Society.