Since January 1997, we have monitored 15 GRB fields, detecting 6 optical/IR afterglows. For GRB 970508, we derive a power-law decay exponent alpha = -1.19 (R-band). The luminosity of the host galaxy L relative to the characteristic luminosity L^{star} is in the range 0.06--0.15, i.e. a dwarf galaxy. For GRB 980326, we derive a power-law decay exponent alpha = -1.7, taking into account the new upper limit for the host as R > 27.3 provided by Bloom and Kulkarni (1998). This implies one of the fastest GRB optical decays ever measured. The fact that only about 50% of optical transients have been found within the gamma/X-ray error boxes, suggest that either considerable intrinsic absorption is present or that some optical transients display a very fast decline. We also propose that the secondary maximum detected on 17 Apr 1998 could be explained in the context of the SN-like light curves 2-3 weeks after the GRB, as recently suggested by Woosley (1999).Comment: Accepted for publication in Astronomy and Astrophysics Supplement Series (special issue on "Gamma-ray bursts in the afterglow era"). 2 pages and 2 postscript figure