Planetary transits of TrES-2 and TrES-3

We used the Optical System for Imaging and low Resolution Integrated Spectroscopy (OSIRIS) tunable filter imager on the GTC to acquire high-precision, narrow-band photometry of the transits of the giant exoplanets, TrES-2b and TrES-3b. We obtained near-simultaneous observations in two near-infrared wavelengths (790.2 and 794.4nm).

We provide normalized flux ratios for each target, where the flux ratio is defined as the target flux divided by the total combined flux from several non-variable reference stars. The flux ratios have been normalized against the baseline (out-of-transit) flux ratio for each target. We provide normalized flux ratios for each target, where the flux ratio is defined as the target flux divided by the total combined flux from several non-variable reference stars.