  We review the status of the EXOTIME project (EXOplanet search with the TIming
MEthod). The two main goals of EXOTIME are to search for sub-stellar companions
to sdB stars in wide orbits, and to measure the secular variation of the
pulsation periods, which are related to the evolutionary change of the stellar
structure. Now, after four years of dense monitoring, we start to see some
results and present the brown dwarf and exoplanet candidates V1636 Ori b and DW
Lyn b.
