Add a vetter that takes a light curve and tce and determine the difference between the depths of the odd and the even transits. It should return both depths and the errors. Usually a cut is made when significant depth differences are seen.
The astropy BLS code actually is one path forward for this test.
Add a vetter that takes a light curve and tce and determine the difference between the depths of the odd and the even transits. It should return both depths and the errors. Usually a cut is made when significant depth differences are seen.
The astropy BLS code actually is one path forward for this test.