Changes between Version 12 and Version 13 of docs/CommissioningPlan/P3.12

Timestamp:

01/14/22 17:46:57 (3 years ago)

Author:

kradhakrishnan

Comment:

--

docs/CommissioningPlan/P3.12

@@ -1 @@
- == P3.12       Star center Fourier mode images == 
-•       **Phase**               :       3  
-•       **Status**              :       Draft    
-•       **Category**            :       Nighttime testing (functionality and operability) (C5) + Nighttime calibration (C6)
-•       **Recurrence**  :       on every target, starting from commissioning.
-•       **Duration**            :       2 days
+ == P2.7        Star center Fourier mode images == 
+ 
+- **Phase**             :       2  
+- **Status**            :       Draft    
+- **Category**  :       Daytime testing (functionality and operability) (C3) + Daytime calibration (C4)
+- **Recurrence**        :       once after instrument installation at telescope platform
+- **Duration**  :       2 days
+
 **Description**
-•       This calibration is performed to calibrate the target star center with respect to the detector in order to provide a reference input for frame derotation and quadrant combination. 
+- This calibration is performed to calibrate the target star center with respect to the detector in order to provide a reference input for frame derotation and quadrant combination. 
+
 **Prerequisites**
-•       Authorize SHARK-NIR on the SX side.
-•       Atmospheric conditions: AO working conditions.
-•       Bad pixel map, Dark 
+- Authorize SHARK-NIR on the SX side.
+- Atmospheric conditions: AO working conditions.
+- Bad pixel map, Dark 
+
 **Procedure**
-•       DM produce a pattern offset with four spots symmetric with respect to the star + AO closed-loop + coronagraph
-•       The required specifications of the corresponding image are a grid of at least 2x2 regularly spaced focal plane image peaks within 5 and 15 lambda/D with FWHM < 45 mas and separation precision < 6 mas.
-•       DM offset applied on target acquisition to produce a waffle image. Find the center of the four first-order diffraction peaks (cross geometry) to deduce the pixel corresponding to the center field.
+- DM produce a pattern offset with four spots symmetric with respect to the star + AO closed-loop + coronagraph
+- The required specifications of the corresponding image are a grid of at least 2x2 regularly spaced focal plane image peaks within 5 and 15 lambda/D with FWHM < 45 mas and separation precision < 6 mas.
+- DM offset applied on target acquisition to produce a waffle image. Find the center of the four first-order diffraction peaks (cross geometry) to deduce the pixel corresponding to the center field.
+
+**Templates** 
+
 **Success criteria**
-•       Accuracy of 3 mas (goal 1 mas) 
+- Accuracy of 3 mas (goal 1 mas) 
+
 **Notes**
-•       Same as activity 7.8 in AD4
+- Same as activity 7.8 in AD4
+
 **LBTO support**
-•       AO support
-**Associated SHARK-NIR personnel**
+- AO support
 
 **Date performed and by whom**
-
-** Comments**