EGAL07

Proposal

Proposal: EGAL07:Target of Opportunity observations on AGN with LST-1
PI: David Sanchez (david.sanchez@lapp.in2p3.fr)

  Source:

    RA (J2000)   

    DEC (J2000)  

Observational settings/limits

ToO observation are triggered by the PI/co-PI or, in the future by flare advocate using the ToO form. This trigger will give the position of the source and the requested time

Trigger Channels :

Fermi pipelines : FLaapLUC and FFASA

Optical channel

Triggers :

• For a trigger, at least 2 hours of observation per night will be asked with as zenith angle as low as possible. This can go up to a full night. • The continuation of the ToO will be based on RTA results and a Next Day Analysis but also on the information provided by the other trigger channels.