March 13th 2006: On sky tests
in tiptilt mode
On-sky tests with faint guide stars and fully functioning L3
wavefront sensor. Earlier problems with the bias gradient were solved.
Report
on observations (Jure Skvarc)
Final report on L3 WFS hardware
May 20th : First Light with
the L3 WFS
The Naomi loop was closed using the L3 WFS in mode 1. Oasis was used in
imaging mode and recorded a drop in image FWHM from 0.55 to 0.25" when
the loop was closed on a Mag11 guide star. Movie
here (made using program written by Bojan
Dintinjana from the Crni Vrh Observatory)
Firstlight Image
The L3 WFS head
L3 on
ISIS : Progress
Potential of L3 : Photon Counting
