RA Range: 09:38, 12:53

Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): 1.2 2CLR 1.5 0.1 60

Pre-imaging run?	No!	Chilean run?	No!	Special calibrations?	No!
Time critical?	No!	ToO?	No!	Carry-over run?	No!

 
  
This is a MOS programme on very massive clusters and groups
of galaxies. The users want to study the dynamical ages, the mass
fractions of various matter components, the galaxy populations, the
heavy elements abundances, the supernova rates, the entropy structure
of the intracluster medium and the large scale structure environments
of these systems. 7 different MOS masks are used.

Note that the users have supplied a full-field and an enlargement for each
of the 7 MOS masks.

 
 

Run status page 169.A-0595E

README of this run:

169.A-0595E.README