Difference between revisions of "GAL01"

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   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  
 
   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". <br>
 
   correspond to the two source targets, that we call "Center of wobbles". <br>
 
 
   '''Wobbles coordinates:'''
 
   '''Wobbles coordinates:'''
 
     W1 : RA: 337.488 deg, Dec: 60.701 deg
 
     W1 : RA: 337.488 deg, Dec: 60.701 deg
     W2 : RA: 336.160 deg, Dec: 61.134 deg
+
     W2 : RA: 336.160 deg, Dec: 61.134 deg <br>
 
   '''Center of wobbles:'''
 
   '''Center of wobbles:'''
 
     RA (J2000)  = 336.829 deg
 
     RA (J2000)  = 336.829 deg
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=== Observational settings/limits ===
 
=== Observational settings/limits ===
  
'''Zenith:''' target is 60-75 deg (if the source is used as backup source, other zenith angles could be also useful for systematics studies).  
+
  '''Zenith:''' 60-75 deg (if the source is used as backup source, other zenith angles could be also useful for systematics studies). <br>
 
+
  '''Moon:''' Dark (eventually 2-3 dark NSB Moon level) <br>
'''Moon:''' 2-3 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)