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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 15.

Fitting output for a mock photometric dataset generated using BSPL_PhotAstrom_noPar_EllOrbs_Param1 and the parameters displayed in Table 6. We see correlated residuals in the linear fit, unlike the circular and elliptical fits. (Left) Best fit with linear orbital motion. (Center) Best fit with circular orbital motion. (Right) Best fit with elliptical orbital motion.

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