Difference between revisions of "GAL02"

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== Proposal ==
 
== Proposal ==
 
Proposal: [[Media:GAL02_López-Oramas.pdf|Target of Opportunity observations of Galactic Transient sources]] <br>
 
Proposal: [[Media:GAL02_López-Oramas.pdf|Target of Opportunity observations of Galactic Transient sources]] <br>
PI: Alicia Lòpez-Oramas (alicia.lopez@iac.es)  <br>
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PI: Alicia López-Oramas (alicia.lopez@iac.es)  <br>
  
 
   Source: SN2023ixf  
 
   Source: SN2023ixf  
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=== Observational settings/limits ===
 
=== Observational settings/limits ===
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'''SN2023ixf'''
  
 
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)

Latest revision as of 10:06, 12 June 2023

Proposal[edit]

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[edit]

SN2023ixf

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)