Difference between revisions of "GAL08 C2"
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We will plan our observations according to the orbital configurations (observations will be coordinated with the schedulers) and possible external triggers. | We will plan our observations according to the orbital configurations (observations will be coordinated with the schedulers) and possible external triggers. | ||
| − | The configurations expected | + | The orbital configurations are expected to happen on: |
phase Orbital phenomenon MJD Date | phase Orbital phenomenon MJD Date | ||
Latest revision as of 14:05, 15 May 2024
Contents
Proposal[edit]
Proposal: GAL08:The periastron passage of the colliding wind binary WR140: the first CWB VHE emitter in the Northern hemisphere?
PI: Alicia López-Oramas (alicia.lopez@iac.es)
Source information[edit]
Source: WR140
RA (J2000): 305.117 deg
Dec (J2000): 43.8544 deg
Observational settings/limits[edit]
Min Zenith [deg] = 5
Max Zenith [deg] = 60
Night Sky Background = Dark
Wobbles = Standard
Scheduling[edit]
From the proposal:
We will plan our observations according to the orbital configurations (observations will be coordinated with the schedulers) and possible external triggers.
The orbital configurations are expected to happen on:
phase Orbital phenomenon MJD Date ============================================================== 0.9551 conjunction: WC star behind 60506 2024.54 July 15 0.9965 quadrature 60626 2024.86 Nov 12 0.000 periastron passage 60637 2024.89 Nov 23 0.0032 conjunction: O star behind 60645 2024.91 Dec 1 0.0393 quadrature 60751 2025.21 Mar 17
Instructions for shifters[edit]
None.
