Difference between revisions of "GAL08 C2"

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(Scheduling)
 
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From the proposal:
 
From the proposal:
  
  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 are:
+
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

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.