Peter,
Interesting...
If you use PHD V2.6 (or AA6 slit guiding) you can record and register the position of the fibre in the guide camera FOV.
You can then "nudge" the target star to this X-Y position.
How does the other end of the fibre join to the rest of the spectrograph?
As Bojan indicates there's a fibre f ratio degradation.....a f7 into the fibre comes out at around f5....
(See Astronomical Spectroscopy for Amateurs, p 210)
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