Difference between revisions of "EGAL07"
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=== Observational settings/limits === | === Observational settings/limits === | ||
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| + | 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. | ||
Latest revision as of 13:42, 14 June 2023
Proposal[edit]
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[edit]
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.
