Changes between Version 4 and Version 5 of docs/CommissioningPlan/P4.9


Ignore:
Timestamp:
02/02/21 10:21:47 (4 years ago)
Author:
kradhakrishnan
Comment:

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  • docs/CommissioningPlan/P4.9

    v4 v5  
    22•       **Phase**               :       4 
    33•       **Status**              :       Draft   
    4 •       **Category**            :       Science verification / Early science (C7)
     4•       **Category**            :       Science verification / Early science (C8)
    55•       **Recurrence**  :       once after the completion of nighttime testing and performance check
    66•       **Duration**            :       1 night(s)
    … …  
    2323
    2424**Procedure**
    25 •       After pre-set and acquisition of the target we will run on flux calibration template with the star off-centered from the coronagraph (short templete - few minutes). To this a centering
    26         observation follows with the Fourier mode on the DM allowing the creation of four satellite spots (around 5% of the target brightness). Also this template is short. We then perform the scientific coronagraphic
    27         observation using pupil stabilized observing mode. This observation should be taken during the passage of the star to the meridian to maximize the rotation of the FOV and allow to implement ADI. This part should
    28         be long at least 1:20-1:30 hours. The observation is closed running again centering and flux calibration with the same modalities adopted at the beginning of the observations.
     25•       After pre-set and acquisition of the target we will run on flux calibration template with the star off-centered from the coronagraph (short template - few minutes). After this, a centering observation follows with the Fourier mode on the DM allowing the creation of four satellite spots (around 5% of the target brightness). Also, this template is short.
     26* We then perform the scientific coronagraphic observation using pupil stabilized observing mode. This observation should be taken during the passage of the star to the meridian to maximize the rotation of the FOV and allowing to implement the ADI. This part should be at least 1:20-1:30 hours long.
     27* The observation is closed running again the centering and flux calibration templates with the same modalities adopted at the beginning of the observations.
    2928
    3029**Notes**