Changes between Version 4 and Version 5 of docs/CommissioningPlan/P4.4

Timestamp:

02/04/21 15:16:05 (4 years ago)

Author:

kradhakrishnan

Comment:

--

docs/CommissioningPlan/P4.4

@@ -1 @@
-== 4.4  Coronagraphic imaging + pupil stabilization mode testing == 
+== 4.4  Disk: Coronagraphic imaging of stellar jets == 
 •       **Phase**               :       4  
 •       **Status**              :       Draft    
-•       **Category**            :       Nighttime testing for functionality, operability, and performance (C5 + C7)
-•       **Recurrence**  :       once
-•       **Duration**            :       3 night(s)
+•       **Category**            :       Science verification / Early science (C8)
+•       **Recurrence**  :       once after the completion of nighttime testing and performance check
+•       **Duration**            :       1 night(s)
 **Description**
-•       Dedicated to check the complete procedure and running of the OB scripts through SHINS for all the combinations of this observing mode.
+•       Disk: Coronagraphic imaging of stellar jets
 **Prerequisites**
 •       Authorize SHARK-NIR on the SX side.
-•       Atmospheric conditions: ?
-•       Atmospheric conditions: ?
+•       Atmospheric conditions: CLEAR
 •       Bad pixel map, Background or Dark, Flat-field, distortion map 
-•       Cloud Cover             : 
-•       Astronomical Seeing     : 
-•       Sky Background  : Any / Bright
-•       Water Vapor             : Any
-•       Timing Windows  : 
-•       Observing Targets       : 
-•       Observing Filters       : 
-•       Detector Mode, DIT:
-•       Daytime Calibration Data required: 
-•       Nighttime Calibration Data required: 
+•       Cloud Cover             : no clouds
+•       Astronomical Seeing     : 0.8" or better
+•       Sky Background  : Any
+•       Water Vapor             : low
+•       Timing Windows  : no major limitation as the observation will be done in filed stabilized mode
+•       Observing Targets       : TBD. We will consider stars with H mag in the range 4-12 (typical 7-9), R will have a similar distribution. Stars with known jets?
+•       Observing Filters       : NB_FeII, NB_HeI and NB_PaB both using single and dual band imaging
+•       Detector Mode, DIT: according to the target brightness
+•       Daytime Calibration Data required: dark/background, flat
+•       Nighttime Calibration Data required: no night calibration needed
 
 **Procedure**
-•       ?
+•       Observing of the target in field stabilized mode. No coronagraph used in this case to image the inner part of the system.
 **Notes**