  We present VLA HI imaging of four LSB galaxies which were thought to strongly
deviate from the TF relation based on Arecibo single-dish observations. We do
not detect three of the four targeted LSB galaxies in HI down to a 4-sigma
limit of 0.08Jy km/s. We find that two of the four of these LSBs have bright
galaxies which have contaminated the Arecibo signal. A further examination of
the Arecibo sample shows that five out of the six galaxies that were found to
deviate from TF have nearby bright galaxies and we conclude that possibly all
but one of the non-TF galaxies are contaminated by HI from nearby galaxies. The
sixth galaxy was not detected by us. A new observation by Arecibo did not
confirm the earlier detection. The integrated profiles of the bright galaxies
are consistent with the Arecibo results both in velocity range and amplitude,
which indicates that most of the extreme deviators from the TF relation must
have been affected by bright companions in this earlier HI survey. A more
recent determination of the sidelobe structure of the Arecibo beam supports our
conclusion and shows that the degree of sidelobe contamination was much larger
than could have been initially predicted. Hence, we have corrected the results
found in O'Neil et al. (2000) and have reconstructed the TF relation. These new
observations then show a) a reconstructed TF relation that has relatively large
scatter at all values of rotational velocity (possibly indicating the true
range in disk galaxy properties) and b) the presence of at least some red, gas
poor, LSB disks that indeed may be in an advanced evolutionary state as the
faded remnants of their former high surface brightness actively star forming
state.
