We identify four candidates for extended emission in the [O I] line: UY Aur and DF Tau.  

DF Tau

The PVD for DF Tau is shown in figure \ref{553567} using the stellar radial velocity from \citet{2006AstL...32..759G}.
Flux of jet at 6302 A is 1.78184e-14 erg/(s*cm^2), calculated within 0.2 contour.
Flux of jet at 6365 A is 9.10147e-14   erg/(s*cm^2)  

UY Aur

Flux of jet at 6302 A is 2.30746e-15 erg/(s*cm^2)  
Flux of jet at 6365 A is 6.69094e-15 erg/(s*cm^2*A*arcsec^2)