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Modeling Binary Lenses and Sources with the BAGLE Python Package

  • Authors: T. Dex Bhadra, J. R. Lu, Natasha S. Abrams, Andrew Scharf, Edward Broadberry, Casey Lam, Macy J. Huston

T. Dex Bhadra et al 2026 The Astrophysical Journal 1002 .

  • Provider: AAS Journals

Caption: Figure 18.

PSBL geometry, where blue is the binary axis and orange is the source moving by with relative proper motion μrel. We are transforming from L to ﹩{L}^{{\prime} }﹩, where ﹩{L}^{{\prime} }﹩ is farther along in the direction of ﹩\hat{s}﹩ by d. The source’s point of closest approach to L is S at a distance u0 at time t0. The source’s point of closest approach to ﹩{L}^{{\prime} }﹩ is ﹩{S}^{{\prime} }﹩ at a distance ﹩{u}_{0}^{{\prime} }﹩ at time ﹩{t}_{0}^{{\prime} }﹩.

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