072.B-0412(A)

PI:Saviane/ Aparicio/ Rosenberg/ Piotto

Rank Class: A

072B0412A.html

Last update of this page: Sun Feb 29 17:45:15 2004
Last update of the USG file: Oct 8 12:28:36 2003

Major Instrument Modes: WFI with standard V and I filters

RA Range: 3.7h - 5.1h

Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance):
1.2 1PHO-2CLR 5.0 0.3 90

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

Special Remarks:
NO_REMARKS

 
 
The program consists of simple imaging in 2 filters, of 7 different fields.
One field is centered on the cluster NGC 1841, four more flank the central
field in the N, S, E, and W directions. One field is centered on the LMC
halo, and finally there is a control field away from both the LMC and the
cluster.

Since PI wants to look for variable stars, with periods of few hours,
it is important that one observations of one field is well separated in time
from the previous one.

If the fields are observed during 1 night, then the best strategy would be
to observe each of them once, and then repeat the cycle three times.

If the fields are observed in different nights, pls. observe several
different fields before going back to the first one in the series.

PCa requested for those OBs which will be observed with 1PHO
conditions.

Information about the progress of this run:

Run status page 072.B-0412A

README of this run:

072.B-0412A.README

Finding charts for this run:

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