  Searching for transits provides a very promising technique for finding
close-in extra-solar planets. Transiting planets present the advantage of
allowing one to determine physical properties such as mass and radius
unambiguously. The EXPLORE (EXtra-solar PLanet Occultation REsearch) project is
a transit search project carried out using wide-field CCD imaging cameras on
4-m class telescopes, and 8-10m class telescopes for radial velocity
verification of the photometric candidates. We describe some of the
considerations that go into the design of the EXPLORE transit search to
maximize the discovery rate and minimize contaminating objects that mimic
transiting planets. We show that high precision photometry (2 to 10 millimag)
and high time sampling (few minutes) are crucial for sifting out contaminating
signatures, such as grazing binaries. We have completed two searches using the
8k MOSAIC camera at the CTIO4m and the CFH12k camera at CFHT, with runs
covering 11 and 16 nights, respectively. We obtained preliminary light curves
for approximately 47,000 stars with better than ~1% photometric precision. A
number of light curves with flat-bottomed eclipses consistent with being
produced by transiting planets has been discovered. Preliminary results from
follow-up spectroscopic observations using the VLT UVES spectrograph and the
Keck HIRES spectrograph obtained for a number of the candidates are presented.
Data from four of these can be interpreted consistently as possible planet
candidates, although further data are still required for definitive
confirmations.
