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This paper describes the new QuickFind method in LcTools for finding signalsand associated TTVs (Transit Timing Variations) in light curves from NASA spacemissions. QuickFind is adept at finding medium to large sized signals(generally those with S/N ratios above 15) extremely fast, significantlyreducing overall processing time for a light curve as compared to the BLSdetection method. For example, on the lead author's computer, QuickFind wasable to detect both KOI signals for star 10937029 in a 14 quarter Kepler lightcurve spanning 1,459 days in roughly 2 seconds whereas BLS took about 155seconds to find both signals making QuickFind in this example about 77 timesfaster than BLS. This paper focuses on the user interfaces, data processingalgorithm, and performance tests for the QuickFind method in LcTools.

LcTools II: The QuickFind Method for Finding Signals and Associated TTVs in Light Curves from NASA Space Missions