RA Range: 6.7h - one field

Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): 2.0 3THN 2.0 1.0 75

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

 
 
This is a imaging programme for studying the long-term behavior of the
variable stars in the young cluster NGC 2264. This program requires
appropriate time sampling, i.e. ideally 2 exposures per month.

This run is for March 2003!!!

Program requested for standard calibrations for B,V and I filters.

Time Critical Aspects:
In order to get a useful time sampling for long-term variability properties
of the young stars the sequences Mar_I+V_1 and Mar_I+V_2 must be executed
between one and three weeks apart of each other.
It would be most ideal if the OB Mar_I+B is carried out in the same night as
one of the other OBs (Mar_I+V_1 or Mar_I+V_2) but it is also acceptable
to execute the OB Mar_I+B in a different night in March 2003.

For more details, please, see README file.

 

Run status page 70.C-0394E

README of this run:

70.C-0394E.README