RA Range: ToO

Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): 1.8, THK, 3.0, 1.0, 30

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

 
 
 ToO program that attempts to detect narrow emission lines at the earliest 
observable phases of a supernova. The observations should be taken as soon 
as possible after notification (if possible within the first week after 
explosion). Lundqvist (PI), Leibundgut or Sollerman can activate the program. 

 Total time of submitted OBs exceeds the allocation time, but PI has 
submitted 2 sequences of OBs, one for a SNIa and one for a SNII. Only 
one has to be executed, depending on nature of event. 

  P.I. has also provided dummy OBs for a flux standard star (to be chosen 
by PSO among the list of UVES spec-phot. standard stars depending on time 
of observation). Once activated, please follow observing sequence as 
described in detail in the README file. 
 

 

Run status page 69.D-0244A

README of this run:

69.D-0244A.README