RA Range: TBD (ToO)

Constraint set (Typical seeing, Transparency,Airmass, FLI, Moon distance): (example: 0.4 1PHO 1.5 0.30 100 - copy from ORID.SUM file)

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

 
 
  This is a ToO program which 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 6.5 days after explosion). 

  The total time of the submitted OBs exceeds the allocation by the 
OPC. This is because it is not known yet if target will be SNIa or SNII. 
Only one branch of OBs (those for SNII or those for SNIa) will need 
to be executed. Each single branch complies with the allocated time. 

  P.I. has also provided OBs for a flux standard star that will be 
selected nearby the SN event and that needs to be observed at the same 
phases (these OBs are wrongly addressed by the P.I. as "calibration" blocks 
in the README file). 

  Once program is activated (by P.I.), please follow observing sequence 
as summarized in README file (sequence depends on if the supernova is 
of type II or Ia). 



 

Run status page 67.D-0227A

README of this run:

67.D-0227A.README