  The photometric data collected during 2001 season OGLE-III planetary/low
luminosity object transit campaign were reanalyzed with the new transit search
technique -- the BLS method by Kovacs, Zucker and Mazeh. In addition to all
presented in our original paper transits, additional 13 objects with transiting
low-luminosity companions were discovered. We present here a supplement to our
original catalog -- the photometric data, light curves and finding charts of
all 13 new objects.
  The model fits to the transit light curves indicate that a few new objects
may be Jupiter-sized (R<1.6 R_Jup). OGLE-TR-56 is a particularly interesting
case. Its transit has only 13 mmag depth, short duration and a period of
1.21190 days. Model fit indicates that the companion may be Saturn-sized if the
passage were central. Spectroscopic follow-up observations are encouraged for
final classification of the transiting objects as planets, brown dwarfs or late
M-type dwarf stars.
  We also provide the most recent ephemerides of other most promising planetary
transits: OGLE-TR-10 and OGLE-TR-40 based on observations collected in June
2002.
  All photometric data are available to the astronomical community from the
OGLE Internet archive.
