Physics Of Eclipsing Binaries. II. Towards the Increased Model Fidelity
Andrej Pr\v{s}a, Kyle E. Conroy, Martin Horvat, Herbert Pablo, Angela, Kochoska, Steven Bloemen, Joseph Giammarco, Kelly M. Hambleton, Pieter, Degroote

TL;DR
This paper discusses advancements in modeling eclipsing binary stars by improving physical accuracy and computational methods, addressing previous limitations in reproducing observed data.
Contribution
It introduces new modeling techniques and algorithms in PHOEBE to enhance the fidelity of eclipsing binary star simulations.
Findings
Improved surface discretization with triangulation.
Enhanced treatment of limb darkening and reflection.
Better modeling of light time travel and orbital effects.
Abstract
The precision of photometric and spectroscopic observations has been systematically improved in the last decade, mostly thanks to space-borne photometric missions and ground-based spectrographs dedicated to finding exoplanets. The field of eclipsing binary stars strongly benefited from this development. Eclipsing binaries serve as critical tools for determining fundamental stellar properties (masses, radii, temperatures and luminosities), yet the models are not capable of reproducing observed data well either because of the missing physics or because of insufficient precision. This led to a predicament where radiative and dynamical effects, insofar buried in noise, started showing up routinely in the data, but were not accounted for in the models. PHOEBE (PHysics Of Eclipsing BinariEs; http://phoebe-project.org) is an open source modeling code for computing theoretical light and radial…
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