We present CCD photometry and proper motion studies of the two open star cl
usters NGC 1960 (M 36) and NGC2194. Fitting isochrones to the colour magnit
ude diagrams, for NGC 1960 we found an age of t = 16 Myr and a distance of
roughly d = 1300 pc and for NGC 2194 t = 550 Myr and d = 2900 pc, respectiv
ely. We combined membership determination by proper motions and statistical
field star subtraction to derive the initial mass function of the clusters
and found slopes of Gamma = -1.23 +/- 0.17 for NGC 1960 and Gamma = -1.33
+/- 0.29 for NGC 2194. Compared to other IMF stud ies of the intermediate m
ass range, these values indicate shallow mass functions.