69A0516B.html

Last update of this page: Thu Apr 24 17:45:05 2003
Last update of the USG file: Jul 17 09:42:51 2002

Major Instrument Modes: UVES Dic1_346+580, Dic2_437+860

RA Range: ToO

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?	Yes!	Carry-over run?	No!

Special Remarks:
ToO program on GRB afterglows. To be triggered only after FORS2 observations are taken and analyzed. Please follow README file.

 
 

 ToO program of a GRB optical afterglow. UVES observations will be 
activated after a FORS2 image has been taken (cf 69.A-0516A.README) and 
only if the optical afterglow is brighter than R = 19.5 mag. Program will 
be activated by the PI and/or by Dr. Angelo Antonelli 
(angelo@coma.mporzio.astro.it).

 Observing strategy: OB GRB_TOO1 should be the first to be executed, 
followed by OB GRB_TOO2. The rest of the OBs should be executed alternating 
Dic1 and Dic2 OBs, or just following the numbers in the OB names.
 NOTE: user modified binning mode (from 1x1 to 2x2) on 9.4.02

Information about the progress of this run:

Run status page 69.A-0516B

README of this run:

69.A-0516B.README