67D0106A.html


Last update of this page: Thu Apr 24 17:45:02 2003
Last update of the USG file: Jul 17 09:42:33 2002

Major Instrument Modes: UVES Dic2_437+860

RA Range: 10h - 23h

Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): 1.5, 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!


Special Remarks:


 

  High-res (R=60.000) observations of the sulphur lines at 869, 923,
and 1046 nm in halo stars. Depending of the radial velocity shift of 
the star, the SI lines may be blended by telluric H2O lines. Hence, 
it is important that the given OBs for fast rotating early B-type 
stars are executed. 

  Expected S/N at the wavelengths of interest are 300, 250, and 100, 
respectively. Hence, it is important that a sufficient number of 
day-time flat-field calibration frames are taken. Constraints 
relaxed wrt Phase1, because of use of I.S. #1. Airmasses were 
specified by user already as tight as possible. 

==> Please, check updated README file for observing strategy 
of the only telluric standard star (HR8858) to be used for the 
remaining 10 program stars, and for target priorities. 
Preferentially, the program stars should be grouped together on 
a few nights. 


 


Information about the progress of this run:

Run status page 67.D-0106A

README of this run:

67.D-0106A.README