Consequences of parameterization choice on eclipsing binary light curve solutions
Eclipsing Binaries (EBs) are known to be the source of most ac- curate stellar parameters, which are important for testing theories of stellar evolution. With improved quality and quantity of observations using space tele- scopes like TESS, there is an urgent need for accuracy in modeling to obtain precise parameters. We use the soon to be released PHOEBE 2.3 EB modeling package to test the robust
