Changes between Version 7 and Version 8 of docs/CommissioningPlan/P4.6

Timestamp:

02/02/21 10:08:47 (4 years ago)

Author:

kradhakrishnan

Comment:

--

docs/CommissioningPlan/P4.6

@@ -6 +6 @@
 •       **Duration**            :       10 night(s)
 **Description**
-•       
+•       Exo-planet: Giant planets and brown dwarfs in SFR, stellar associations, & young open clusters
 **Prerequisites**
 •       Authorize SHARK-NIR on the SX side.
@@ -23 +23 @@
 
 **Procedure**
-•       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 
-        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 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 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. 
+•       After pre-set and acquisition of the target, we will run a 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.
+* 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 ADI. This part should be at least 1:20-1:30 hours long.  
+* At the end of the observation, the centering and flux calibration templates are executed with the same modalities adopted at the beginning of the observations. 
 **Notes**