  The main goal of this study is to screen the PENELLOPE/UVES targets for
outflow activity and find microjets via spectro-astrometry in, e.g., the
[OI]$\lambda$6300 line. In total, 34 T\,Tauri stars of the PENELLOPE survey
have been observed with the high resolution slit spectrograph UVES in three
different slit positions rotated by $120^\text{o}$. Our spectro-astrometric
analysis in the [OI]$\lambda$6300 wind line reveals two newly discovered
microjets associated with Sz\,103 and XX\,Cha. Both microjets have an extent of
about $0.04$ arcseconds, that is, $<10\,\text{au}$, and we confined their
orientation by the three slit observations. Furthermore, we confirm the binary
nature of VW\,Cha and CVSO\,109. We present (further) evidence that DK\,Tau\,B
and CVSO\,104\,A are spectroscopic binaries. Sz\,115 is tentatively a
spectroscopic binary. The origin of the LVC, that is, MHD winds versus
photoevaporative winds, of the Sz\,103 and XX\,Cha microjets remains unclear.
