Difference between revisions of "GAL01"

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   '''Zenith:''' 60-75 deg (if the source is used as backup source, other zenith angles could be also useful for systematics studies). <br>
 
   '''Zenith:''' 60-75 deg (if the source is used as backup source, other zenith angles could be also useful for systematics studies). <br>
   '''Moon:''' 2-3 Moon level <br>
+
   '''Moon:''' Dark (eventually 2-3 dark NSB Moon level) <br>

Latest revision as of 08:07, 14 June 2023

Proposal[edit]

Proposal: GAL01:Large Zenith Angle observation of the hadronic PeVatron candidate in the Boomerang SNR (G106.3+2.7) with LST-1
PI: Franca Cassol (cassol@cppm.in2p3.fr)

Coordinates[edit]

  We aim to measure both the tail and the head of the Boomerang SNR. For that the wobbles are back to back in a point that not 
  correspond to the two source targets, that we call "Center of wobbles". 
Wobbles coordinates: W1 : RA: 337.488 deg, Dec: 60.701 deg W2 : RA: 336.160 deg, Dec: 61.134 deg
Center of wobbles: RA (J2000) = 336.829 deg DEC (J2000) = 60.919 deg
Wobble distance = 0.3885 deg
Wobble angles: W1 = 146 deg W2 = W1+180 deg = 326 deg

Observational settings/limits[edit]

  Zenith: 60-75 deg (if the source is used as backup source, other zenith angles could be also useful for systematics studies). 
Moon: Dark (eventually 2-3 dark NSB Moon level)