Difference between revisions of "GAL01"
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PI: Franca Cassol (cassol@cppm.in2p3.fr) <br> | PI: Franca Cassol (cassol@cppm.in2p3.fr) <br> | ||
| − | + | === Coordinates === | |
| − | + | 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> | |
| + | '''Wobbles coordinates:''' | ||
| + | W1 : RA: 337.488 deg, Dec: 60.701 deg | ||
| + | W2 : RA: 336.160 deg, Dec: 61.134 deg <br> | ||
| + | '''Center of wobbles:''' | ||
| + | RA (J2000) = 336.829 deg | ||
| + | DEC (J2000) = 60.919 deg <br> | ||
| + | '''Wobble distance''' = 0.3885 deg <br> | ||
| + | '''Wobble angles:''' | ||
| + | W1 = 146 deg | ||
| + | W2 = W1+180 deg = 326 deg | ||
=== Observational settings/limits === | === Observational settings/limits === | ||
| + | |||
| + | '''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> | ||
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)
