1999A&A...341..943D

For observed galactic microlensing events only one fit is usually presented, though, especially for a binary lens, several fits may be possible. This has been shown for the MACHO LMC#1 event (Dominik & Hirshfeld, 1996A&A...313..841D). Here I discuss the strong binary lens events OGLE#7 and DUO#2. It is shown that several models with a large variety of parameters are in accordance with the photometric data. For most of the fits, 1-σ-bounds on the fit parameters are given. The variation of the parameters within these bounds is in some cases considerable. It is likely that other binary lens events which will occur will have properties similar to the discussed events.