67A0505B.html

Last update of this page: Thu Apr 24 17:45:02 2003
Last update of the USG file: Jul 17 09:42:31 2002

Major Instrument Modes: UVES DIC1_346+580; DIC2_437+860

RA Range: 00h (ToO)

Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): 2.0, CLR, 5.0,1.0,30

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

Special Remarks:

 
 
  This is a ToO observation of a GRB optical afterglow. Once program 
is activated, first a FORS2 image needs to be taken (see  
67.A-0505(A).README). UVES observations of the optical afterglow may 
follow IF the optical afterglow is brighter than 19 mag.

  The PI (Dr. Fabrizio Fiore) and the Co-I (Dr. Angelo Antonelli) are 
the ones allowed to activate the program. If started, please observe 
first OB=GRB_TOO1 (Dic1), then OB=GRB_TOO3 (Dic2), and then the others,
alternating Dic1 and Dic2 OBs (details given in README file).

Information about the progress of this run:

Run status page 67.A-0505B

README of this run:

67.A-0505B.README