RA Range: ~12h - 19h

Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): 2.0, 3THN, 1.8, 1.0, 30

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

 
 
  This program aims at obtaining UVES red spectra of 17 stars in 
the globular cluster NGC 6752 and two metal--poor field stars for 
comparison. One rapidly rotating B star (HR 6788) should be observed 
on each night some of the cluster stars are observed, although P.I. 
submitted only 5 such OBs: if possible, preference should be given 
to observing more than one science target per night. 

  No special scheduling requirement. The instrumental setup is always 
the RED arm centered at 580nm and image slicer #3. All OBs have 3 
(concatenated) exposures, for a total of up to 1h30min (not really 
justified). User has been warned that OBs will not be repeated if 
constraints are not fulfilled in last 30min of exposure. The expected 
S/N per exposure around 5120A should be of the order of ~80-100. 

 
 

Run status page 67.D-0145A

README of this run:

67.D-0145A.README