Detection rate
\citet{2003ApJ...583..334H} detected the [O I] 6300 Ang line in emission in a little more than half of the objects and all our candidates are on that list.
Discussion
We begin the discussion by looking at the two sources where the jet was clearly detected.
DF Tau
DF Tau is a
\citet{2004ApJ...609..261H} observed the jet of DF Tau with low-resolution slitless spectroscopy with STIS. They see jet and counterjet at a position angle of 127 degrees, but the binary is not resolved and it remains unclear if we see one jet from both components each or if both are launched from the same component of the binary. For our observations , the PA of the slit was XXX TAB XXX thus,
Notes that still need to be worked into the text:
Acknowledgments
Support for this work was provided for AVU and HMG by NASA through grant GO-13766.010 from the Space Telescope Science Institute.