Difference between revisions of "TRAN02"
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| − | + | Coordinates differ case to case. They will be computed and given by the Transient Handler (TH). <br> | |
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=== Observational settings/limits === | === Observational settings/limits === | ||
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| + | The observational limits are part of the TH algorithm that defines if the source is observable or not. If the source fulfil these parameters it will consider observable: | ||
| + | |||
| + | *Max Zenith: 70deg (preferred <60deg) | ||
| + | |||
| + | *Wobbles: standard | ||
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| + | *Night Sky: dark/twilight | ||
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| + | Joint observation with MAGIC is preferable, when possible. | ||
Revision as of 07:24, 10 July 2023
Proposal
Proposal: TRANS02:Gamma-ray burst observations
PI: Alice Donini (alice.donini@inaf.it)
Source:
Coordinates differ case to case. They will be computed and given by the Transient Handler (TH).
Observational settings/limits
The observational limits are part of the TH algorithm that defines if the source is observable or not. If the source fulfil these parameters it will consider observable:
- Max Zenith: 70deg (preferred <60deg)
- Wobbles: standard
- Night Sky: dark/twilight
Joint observation with MAGIC is preferable, when possible.
