Difference between revisions of "GAL02"
| Line 3: | Line 3: | ||
PI: Alicia Lòpez-Oramas (alicia.lopez@iac.es) <br> | PI: Alicia Lòpez-Oramas (alicia.lopez@iac.es) <br> | ||
| − | Source: | + | Source: SN2023ixf |
| − | RA (J2000) | + | RA (J2000) 14:03:38.56 <br> |
| − | DEC (J2000) | + | DEC (J2000) 54:18:42.02 <br> |
=== Observational settings/limits === | === 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). | ||
Revision as of 10:04, 12 June 2023
Proposal
Proposal: Target of Opportunity observations of Galactic Transient sources
PI: Alicia Lòpez-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).
