A differentiable N-body code for transit timing and dynamical modelling - II. Photodynamics

Building on ericagol/NbodyGradient.jl, this team combines transit models from rodluger/Limbdark.jl to create full photodynamic models.

Package: langfzac/Photodynamics.jl

These models can then be used to model multi-planetary transit light curves. See their paper published in MNRAS below for more:

Langford, Z., & Agol, E. (2025). A differentiable N-body code for transit timing and dynamical modelling - II. Photodynamics. Monthly Notices of the Royal Astronomical Society, 540(1), 106-127. [ADS]

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