Changes between Version 16 and Version 17 of docs/CommissioningPlan/P1.7

Timestamp:

04/22/22 17:31:53 (3 years ago)

Author:

kradhakrishnan

Comment:

--

docs/CommissioningPlan/P1.7

@@ -1 @@
-== P1.7 Motor/light sources functional verification and filter artifacts/defects verification == 
+
+== P1.7 Science detector calibrations == 
 
 - **Phase**             :       1  
 - **Status**            :       Draft    
-- **Category**  :       Unpack, Assemble, and Verification (C1)
-- **Recurrence**        :       once
-- **Duration**  :       1.5 days
+- **Category**  :       Daytime testing (functionality and operability) (C3) + Daytime calibration (C4)
+- **Recurrence**        :       starting from commissioining. daily/weekly/monthly/yearly depending on individual activities.
+- **Duration**  :       0.5 day
 
 **Description**
-- Checking the working of motors and light sources within SHARK-NIR using optical feedback. Finding the filter defects/artefacts using an internal calibration source (flat-field) within the instrument.
+- Calibration and testing of the SHARK-NIR science detector.
 
 **Prerequisites**
 - SHARK-NIR connected to LBT network.
-- Electronics racks on.
-- DM best shape uploaded (shape minimizing internal aberrations)
+- Electronics cabinets on.
 - The cryostat should be running and cooled down.
+- Internal alignment of the SHARK-NIR is verified.
 
 **Procedure**
-- When the services are up and running, after the motors are sent to home positions, each of the individual motors is individually tested for their different named/nominal positions. 
-- The light sources within SHARK-NIR are used simultaneously to check the working of the motors looking at the optical feedback.
-- Check the CRED-2 and ALPAO-DM SW using optical feedback.
-- Take the images of all the filters using the internal calibration source (flat-field) within the instrument to locate/find out the filter defects/artefacts, if any. You may take short- and long-exposures to get better contrast of the features if required.
-- Check the filter wheel position monitoring script detailed in [wiki:/docs/Commissioning/SNM1 SNM1]. Save the data in the repository.
+- Check bias calibration & master dark scripts and then perform the following daytime calibration procedures below.
+
+||**Code**||**Activity**||**Location to perform this test**||
+||SDC1||[wiki:/docs/CommissioningPlan/SDC1 Instrumental background for science]||Padova / LBT cleanroom / LBT Platform||
+||SDC2||[wiki:/docs/CommissioningPlan/SDC2 Instrument flat field, detector linearity and bad pixels]||Padova / LBT cleanroom||
+||SDC3||[wiki:/docs/CommissioningPlan/SDC3 Wavelength calibration]||Padova / LBT cleanroom||
+||SDC4||[wiki:/docs/CommissioningPlan/SDC4 Thermal background]||Padova / LBT cleanroom / LBT Platform||
+||SDC5||[wiki:/docs/CommissioningPlan/SDC5 Detector gain]||Padova / LBT cleanroom / LBT Platform||
+||SDC6||[wiki:/docs/CommissioningPlan/SDC6 Detector persistence]||Padova / LBT cleanroom / LBT Platform||
+||SDC7||[wiki:/docs/CommissioningPlan/SDC7 Spectral resolution]||Padova / LBT cleanroom||
+||SDC8||[wiki:/docs/CommissioningPlan/SDC8 Ghost calibration]||Padova||
+
+- Check the working of all the detector read-out modes and windowing possibilities. Note that this will be checked rigorously in the Padova laboratory. 
 
 **Templates**
-- SHARKNIR_ci_mon_LyotMaskPos (not released)
-- SHARKNIR_di_mon_MaskRepeatability (not released)
+- SHARKNIR_cal_InstrumentBackground (not released)
+- SHARKNIR_gen_cal_InstrumentFlatField (not released)
+- SHARKNIR_lss_cal_Wavelenght (not released)
+- SHARKNIR_gen_mon_ThermalBackground (not released)
+- SHARKNIR_di_mon_DetectorGain (not released)
+- SHARKNIR_ci_mon_DetectorPersistence (not released)
+- SHARKNIR_lss_mon_SpectraResolution (not released)
+- SHARKNIR_cal_mon_Ghost (not released)
 
 **Success criteria**
-- All the motors can reach the named positions / nominal positions.
-- All the light sources are working and confirmed through optical feedback at the SCICAM.
-- Filter wheel position monitoring script is run successfully and data is saved in the repository.
-- CRED-2 AND ALPAO-DM working normally.
-- All the filter images are saved.
+- SCICAM linearity as expected.
+- SCICAM bad pixels mask created.
+- SCICAM  bias and flat scripts working.
+- All individual activity (in the table) success criteria are met.
 
 **Notes**
+- Save all the intermediate images to check the SHARK-NIR Data Reduction pipeline.
 
 **LBTO support**