- ... clusters
- Based on observations with the 2.2 m MPI ESO telescope.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...
)
-
Note that #853 really designates a number ID, and not a wavelength
(see also http://www.ls.eso.org/lasilla/sciops/2p2/E2p2M/WFI/filters/).
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
- ...
available
- At WFI@2.2m 60 h have already been approved
to us for 2006.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.
.