Fast and easy exoplanet transit light curve modelling.
Programs to obtain planet parameters from phase-folded light curves from the Kepler satellite, run with QMUL
Fast and Efficient Processing of PAM Data
This software generates a light curve caused by the mutual motions of stars in a binary system. Depending on stars, orbits parameters and locus the light curve changes the shape and amplitude.
Utility for detecting exoplanet transits within SuperWASP logs
Light curve analysis pipeline for exoplanet detection using Kepler data, integrating photometric preprocessing, DTW-based similarity learning, and 2D CNN classification
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