  We present high precision K-band photometry of the transit and secondary
eclipse of extrasolar planet OGLE-TR-113, using the SOFI near-infrared
instrument on ESO's NTT. Data were taken in 5 second exposures over two periods
of 3-4 hours, using random jitter position offsets. In this way, a relative
photometric precision of ~1% per frame was achieved, avoiding systematic
effects that seem to become dominant at precisions exceeding this level, and
resulting in an overall accuracy of 0.1% per ~10 minutes. The observations of
the transit show a flat bottom light-curve indicative of a significantly lower
stellar limb-darkening at near-infrared than at optical wavelengths. The
observations of the secondary eclipse result in a 3 sigma detection of emission
from the exoplanet at 0.17+-0.05%. However, residual systematic errors make
this detection rather tentative.
