71.A-0165(B)

PI:Fiore/ Savaglio/ Fontana/ Marconi/ Stella/ Antonelli/ Di Paola/ Stratta/ Chincarini/ Ghisellini/ Saracco/ Lazzati/ Covino/ Zerbi/ Tagliaferri/ Campana/ Perna/ Vietri/ Frontera/ Mereghetti/ Meurs

71A0165B.html

Last update of this page: Tue Oct 21 17:45:08 2003
Last update of the USG file: Mar 10 14:39:44 2003

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!

 

 ToO program of a GRB optical afterglow. UVES observations will be activated 
only after a FORS1 image has been taken (cf 71.A-0165A.README) and the 
optical afterglow is brighter than R=19.5 mag. Activation email will come 
from PI and/or by Dr. Angelo Antonelli (angelo@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 can be executed alternating 
Dic1 and Dic2 OBs, or just following the numbers in the OB names.

 
 

Run status page 71.A-0165B

README of this run:

71.A-0165B.README