RA Range: 0.7h - 1.5h

Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): 1.5 2CLR 3.0 0.3 120

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

 
 
The purpose of these observations is to search for asteroids in the
Lagrangian points of the outer planets. The strategy is to image a total
of 3 mosaics, consisting of 12 subframes each, and then to re-observe them,
ideally the next night, in order to discover objects which moved, and
to obtain position measurements for the determination of a prliminary orbit.

To increase the detection probability they have chosen to observe at times
when the Lagrangian points of several planets overlap. Obviously these
situations change, so the observations specified herein are only valid
for the period around February 2003.

For details of suggested strategy, please, see README "Description of
observations" section.

Standard Calibrations were requested for V filter.

 

Run status page 70.C-0135A

README of this run:

70.C-0135A.README