In addition to the list of UBV photometries of 955 galactic foreground
stars in the direction to the Large Magellanic Cloud published by Goc
hermann et al. (1993a), a supplement of 545 stars is presented, which
have been measured with the same photometric accuracy. Moreover, less
reliable photometries of 379 further foreground stars are listed in a
separate table. The homogeneous data base of more than 1500 high accur
acy photometries represented by these stars has been used to construct
a reddening distribution map of the galactic foreground towards the L
MC by Oestreicher et al. (1995).