072.D-0414(A)

PI:Hubrig/ Castelli/ Mathys/ Savanov/ Ritter

Rank Class: C

072D0414A.html

Last update of this page: Fri Apr 2 13:45:57 2004
Last update of the USG file: Aug 18 09:03:12 2003

Major Instrument Modes: UVES-DIC1

RA Range: 07:30, 09:36, 15:27, 19:53

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

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

Special Remarks:
NO_REMARKS

 
 
This is a simple UVES programme aimed at detecting spectral variations
in 4 bright variable stars. In general, the PI requests that
individual targets are NOT observed twice (or more) during the same
night. On the contrary, the OBs for a given target must be spread on
as many nights as possible.

Some other requirements apply to single targets:

1) HD 188041: this star has a long period. The PI recommends to execute
the first two OBs in October 2003 and the last two ones in March 2004;

2) HD 137909: this star can be observed in March 2004 only.

Information about the progress of this run:

Run status page 072.D-0414A

README of this run:

072.D-0414A.README

Finding charts for this run:

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