Changes between Version 10 and Version 11 of docs/CommissioningPlan/P3.5

Timestamp:

04/22/22 20:45:59 (3 years ago)

Author:

kradhakrishnan

Comment:

--

docs/CommissioningPlan/P3.5

@@ -1 @@
- == P3.5        PSF Alignment == 
+ == P3.5        Verify the ADC rotation on sky == 
  
 - **Phase**             :       3  
 - **Status**            :       Draft    
-- **Category**  :       Nighttime testing (functionality and operability) (C5) + Nighttime calibration (C6)
-- **Recurrence**        :       before every observing target (CI, LSS), starting from commissioning.
-- **Duration**  :       2 hours
+- **Category**  :       Nighttime testing (functionality and operability) (C5)
+- **Recurrence**        :       once at commissioning
+- **Duration**  :       4 hours
 
 **Description**
-- Alignment of the PSF with occulter (or slit) in coronagraphic mode. 
+- Evaluate the performance of the SHARK-NIR ADC.
 
 **Prerequisites**
-- Bad pixel map, Background or Dark, Flat-field, detector RON 
+- Atmospheric conditions: photometric.
+- Authorize SHARK-NIR on the SX side.
+- Photometric stars as targets for every filter.
+- AO is working.
+- Target(s) at different Zenith distances?
 
 **Procedure**
-The internal deformable mirror's position (TTM_DM) is optimized to have the PSF image on the intermediate focal plane centered with the occulter. We compare the PSF image, formed on the SCICAM, with the image of the occulter obtained on the SCICAM using the calibration flat-field source. 
+- Check the working of the ADC using different targets in varying zenith distances and observing using different science filters?
 
 **Templates**
-- SHARKNIR_gen_tec_PSFAlignment (not realased)
 
 **Success criteria**
-- the expected accuracy of 0.2 pixels (DV: need to check if we can reach this). 
+- xxx
 
 **Notes**
-- Same as activity 8.3 in AD4
-- 7 cases, 30 mins per case.
 
 **LBTO support**