68D0637A.html

Last update of this page: Thu Apr 24 17:45:05 2003
Last update of the USG file: Jul 17 09:42:47 2002

Major Instrument Modes: WFI with VI filters

RA Range: 9h - 16.4h

Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): 1.3 2CLR-1PHO 2.0 0.5 30.

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

Special Remarks:

 
 
The program is going to study the stellar mass function in the
already identified tidal tails in a sample of 3 Galactic Globular
Clusters. The OBs containing the clusters have to be observed under
photometric conditions.

  ! Time-critical ??:
If possible the fields of each cluster should be observed on the
same night.

The Standard Calibrations are required.

Information about the progress of this run:

Run status page 68.D-0637A

README of this run:

68.D-0637A.README