Here you will find information about how to obtain the light curve data you need, how to read the data files in python, and how to smooth the light curve data to Keplers long cadence (~30 minutes). 
If you have any questions please contact me, Beatriz Campos Estrada (current email: beatriz.estrada@nbi.ku.dk). I am able to obtain more white light curves for these types of planets if having access to the appropriate optical data. If you are interested in any of the materials which I have tested but are not available in this folder, let me know and I will make the data available to you. I can also easily model the secondary eclipses if needed.

The data available are the light curves of the simulations presented in Campos Estrada+ 2024. Inside the folder 'data' you will find folder which are named in following manner:
mineralname_planetname
For example, if you are looking for light curves of KIC 1255b (Kepler-1520b), with dust composed of Corundum (Al2O3), you will be able to find these on the folder Al2O3_KIC1255b.
The files within each folder are named as follow: if the model has an initial dust grain size of 1.0 micron, a mass-loss rate of 2.0, and a spherical outflow geometry, then the naming will be:
s1.0_mdot2.0_sph_txxx
So 's' is for the initial dust grain size, mdot for the mass-loss rate, and the 'sph' for the geometry. If you want the 'day-side' geometry it will be named as 'day'. The final t and following number indicate in which orbit the simulation was. We started at the 0th orbit - some of the models we have ran up to the 4th orbit, some to the 5th, some to the 7th. Either way, all the light curves presented here are converged except for the exceptional case of Mg2SiO4 (this is explained in the paper).

Please follow the light_curve.py script under this folder to read the light curve data - including the smoothing of the data to Keplers long cadence.