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A promising method for detecting earth-sized exoplanets is the timinganalysis of a known transit. The technique allows a search for variations ineither the transit duration or the center induced by the perturbation of athird body, e.g. a second planet or an exomoon. By applying this method, theTASTE (The Asiago Search for Transit Timing variations of Exoplanets) projectwill collect high-precision, short-cadence light curves for a selected sampleof transits by using imaging differential photometry at the Asiago 1.82mtelescope. The first light curves show that our project can achieve acompetitive timing accuracy, as well as a significant improvement of theorbital parameters. We derived refined ephemerides for HAT-P-3b and HAT-P-14bwith a timing accuracy of 11 and 25 s, respectively.

TASTE: The Asiago Search for Transit timing variations of Exoplanets. I. Overview and improved parameters for HAT-P-3b and HAT-P-14b