Fig. 19. (a) histogram of the velocity shifts between the two way (sky
fibre - star fibre). The line is a Gaussian with
=2.3 m
s-1. Note that a correction is done to suppress a slight mismatch
between the two optical paths:
Vr(sky) =
Vr(star)-.04\
Vr(star)+0.6 (
Vr is the velocity
variation of the spectrograph in units of m s-1). (b) histogram
of the variation of the spectrograph monitor by the star-way during the
measurements.