The EXOTIME monitoring program discovers substellar companion candidates around the rapidly pulsating subdwarf B stars V1636 Ori and DW Lyn

The EXOTIME monitoring program has discovered sub-stellar companion candidates around the rapidly pulsating subdwarf B stars V1636 Ori and DW Lyn using the timing method. Here we motivate our continuing search, and refer to descriptions of the photometric data collected, the data analysis and the characteristics of the O-C diagrams obtained. We also discuss our on-going efforts to consolidate the candidate discoveries with additional simulations and confirm them with independent methods.