Changes between Version 3 and Version 4 of docs/CommissioningPlan/SDC2

Timestamp:

01/24/22 11:44:30 (3 years ago)

Author:

kradhakrishnan

Comment:

--

docs/CommissioningPlan/SDC2

@@ -15 +15 @@
 - Use the calibration flat-field source.
 - This calibration is performed illuminating the detector uniformly using the instrument FF lamp, for each filter. 
-- It is expected that the detector FF depends on filters, final accumulated charge in the pixels. Thus, a series of exposures will be taken at different count levels (realized via ND filters and/or DIT) for each filter setup. In this case, the template takes the background frames automatically. Comparing different count rates at constant DIT will also yield a linearity map of the detector. 
+- It is expected that the detector FF depends on filters, the final accumulated charge in the pixels. Thus, a series of exposures will be taken at different count levels (realized via ND filters and/or DIT) for each filter setup. In this case, the template takes the background frames automatically. Comparing different count rates at constant DIT will also yield a linearity map of the detector. 
 
 **Templates**
+- SHARKNIR_gen_cal_InstrumentFlatField (not released)
 
 **Success criteria**