Difference between revisions of "GAL02"
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Standard wobble, observations at the lowest zenith angle preferred. In case of a 2 sigma hint in RTA (or if a 2 sigma hint in MAGIC online Analysis MOLA, when doing piggyback observations), please extend the observations as much as possible (up to ZA<60). | Standard wobble, observations at the lowest zenith angle preferred. In case of a 2 sigma hint in RTA (or if a 2 sigma hint in MAGIC online Analysis MOLA, when doing piggyback observations), please extend the observations as much as possible (up to ZA<60). | ||
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| + | Contact persons for Supernovae: Alicia López-Oramas (alicia.lopez@iac.es) and Alessandro Carosi (alessandro.carosi@inaf.it) | ||
Revision as of 10:05, 12 June 2023
Proposal
Proposal: Target of Opportunity observations of Galactic Transient sources
PI: Alicia López-Oramas (alicia.lopez@iac.es)
Source: SN2023ixf
RA (J2000) 14:03:38.56
DEC (J2000) 54:18:42.02
Observational settings/limits
Standard wobble, observations at the lowest zenith angle preferred. In case of a 2 sigma hint in RTA (or if a 2 sigma hint in MAGIC online Analysis MOLA, when doing piggyback observations), please extend the observations as much as possible (up to ZA<60).
Contact persons for Supernovae: Alicia López-Oramas (alicia.lopez@iac.es) and Alessandro Carosi (alessandro.carosi@inaf.it)
