69D0390A.html

Last update of this page: Thu Apr 24 17:45:05 2003
Last update of the USG file: Jul 17 09:43:05 2002

Major Instrument Modes: UVES Dic1_390+564

RA Range: 01h

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

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

Special Remarks:
OBs need to be well distributed between May and end of the period (cf README)

 
 
 Simple spectroscopic program divided in 4 parts (one part per target), 
aiming at taking long-term time series of Luminous Blue Variable stars in 
the SMC and LMC to study in depth the structure of the stellar wind and 
its variability. Each part (A,B,C,D) consists of identical OBs including 
a short exposure (to get H_Alpha without saturation) and a longer exposure, 
that may saturate (no problem for this). PI has provided an useful and 
informative 'book keeping sheet' (file: 69.D-0390A.002.ps). 

 Requirements: observations should start as soon as possible (as early as 
May for the SMC target, and July for the LMC targets). It is important 
that observations are well distributed until the end of the period. Weekly 
frequency is optimal - cf corresponding README file for more info.

Information about the progress of this run:

Run status page 69.D-0390A

README of this run:

69.D-0390A.README