EGAL07
Revision as of 13:42, 14 June 2023 by Davidsanchez (talk | contribs) (→Observational settings/limits)
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.
