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?	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 the notification (if possible
within the first week after explosion). The PI will activate the 
program. 

  The total time of the submitted OBs exceeds the allocation by the OPC, 
because PI has submitted 2 sequences of OBs, one for a SNIa and one for a 
SNII. Each of them complies with the OPC allocated time. The final choice 
of which sequence will be observed clearly depends on which type of 
supernova will trigger the program. 

  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. Once activated, please follow observing sequence as described in 
detail in the README file. 


 

Run status page 68.D-0143A

README of this run:

68.D-0143A.README