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Aims. We used VLT/VIMOS images in the V band to obtain light curves of
the extrasolar planetary transits OGLE-TR-111 and OGLE-TR-113 and the
candidate planetary transits: OGLE-TR-82, OGLE-TR-86, OGLE-TR-91,
OGLE-TR-106, OGLE-TR-109, OGLE-TR-110, OGLE-TR-159, OGLE-TR-167,
OGLE-TR-170, OGLE-TR-171.
Methods. Using difference imaging photometry, we were able to achieve
millimagnitude errors in the individual data points.
We present the analysis of the data and the light curves by measuring
transit amplitudes and ephemerides and by calculating geometrical
parameters for some of the systems.
Results. We observed nine OGLE objects at the predicted transit moments. Two other
transits were shifted in time by a few hours. For another seven objects
we expected to observe transits during the VIMOS run, but they were not
detected.
Conclusions. The stars OGLE-TR-111 and OGLE-TR-113 are probably the only OGLE objects
in the observed sample to host planets, with the other objects being very
likely eclipsing binaries or multiple systems. In this paper we also
report on four new transiting candidates which we have found in the data
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