Phase-folded light curves of nine candidates that orbit M-dwarfs from the WTS 19 h field. As it was done for the candidates around F-G-K-stars, we overplot the best-fitting single eclipse with green solid lines, whereas the light curves with two eclipses are shown with the best-fitting trapeziod model, using red-solid lines. The objects with two eclipses are reported in Sect. 7.2 as MEB candidates. Objects 19a1-02980 and 19a1-10878 were found by our selection criteria during the process of transiting planet detection, whereas the system 19c4-06354 was separately detected by an additional analysis carried out on the AP and DI light curves.