Post-AGB candidates with emission lines in an Hα image of the LMC (Kennicutt et al. 1995). The circle denotes the object with the [O iii] features at 4959 and 5007 Å in emission, they are in absorption for the two sources indicated with a square and are not present in the spectra of the two stars denoted with a diamond. The three crosses indicate the position of the other objects with an emission-line spectrum that did not cover the [O iii] feature.