One of the observers noted that when following a source for an
extended period of time the source drifts in the order of 10 pixels
(
1.5 arcsec) per hour. Examination of the data showed that the
drift is mostly in the vertical direction with respect to the
telescope. The fact that the drift is similar in V and I excludes
differential diffraction affects, while the straight tracks for the
drifts makes it unlikely to be a problem in the tracking or
guiding. The most likely cause is flexure of the camera with respect
to the 45 degree pick-off mirror. Checking the mirror fixation itself
does not show any slack, but it might be that the whole probe moves.