RA Range: 0.6 - 18h

Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): 2.0, THN, 5.0, 1.0, 30

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

 
 
 Program for precision RV monitoring of 10 different M dwarfs using the 
UVES iodine cell. Since the time variability of these objects is unknown: 
a) execution of OBs should be distributed in time throughout the period; 
b) distribution of nights should be as irregular as possible for a given star;
c) sometimes, for stars for which 6 OBs are available, OBs should be 
executed on consecutive nights. However, on any given night not more than 
1 OB per star should be executed. 

 No special requirement, since the R_600+iodine cell setting is now 
standard. Flatfields with and without the iodine cell need to be taken 
for all nights of observations.

 
 

Run status page 68.C-0415A

README of this run:

68.C-0415A.README