High Cadence Near Infrared Timing Observations of Extrasolar Planets: I. GJ 436b and XO-1b

Currently the only technique sensitive to Earth mass planets around nearby stars (that are too close for microlensing) is the monitoring of the transit time variations of the transiting extrasolar planets. We search for additional planets in the systems of the hot Neptune GJ 436b, and the hot-Jupiter XO-1b, using high cadence observations in the J and Ks bands. New high-precision transit timing measurements are reported: GJ 436b Tc = 2454238.47898 pm 0.00046 HJD; XO-1b Tc(A) = 2454218.83331 pm 0.00114 HJD, Tc(B) = 2454222.77539 pm 0.00036 HJD, Tc(C) = 2454222.77597 pm 0.00039 HJD, Tc(D) = 2454226.71769 pm 0.00034 HJD, and they were used to derive new ephemeris. We also determined depths for these transits. No statistically significant timing deviations were detected. We demonstrate that the high cadence ground based near-infrared observations are successful in constraining the mean transit time to ~30 sec., and are a viable alternative to space missions.