Changes between Version 3 and Version 4 of docs/CommissioningPlan/P3.0


Ignore:
Timestamp:
01/14/22 18:38:11 (3 years ago)
Author:
kradhakrishnan
Comment:

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  • docs/CommissioningPlan/P3.0

    v3 v4  
    11== P3.0 Large spatial scale instrument and telescope flat field ==
    2 •       **Phase**               :       3 
    3 •       **Status**              :       Draft   
    4 •       **Category**            :       Nighttime testing (functionality and operability) (C5) + Nighttime calibration (C6)
    5 •       **Recurrence**  :       before every night observations (valid for all observing modes). 2/day for CI (BB filter only).
    6 •       **Duration**            :       2 hours
     2
     3- **Phase**             :       3 
     4- **Status**            :       Draft   
     5- **Category**  :       Nighttime testing (functionality and operability) (C5) + Nighttime calibration (C6)
     6- **Recurrence**        :       before every night observations (valid for all observing modes). 2/day for CI (BB filter only).
     7- **Duration**  :       2 hours
     8
    79**Description**
    8 •       Flat field taken during twilight
     10- Flat field is taken during twilight
     11
    912**Prerequisites**
    10 •       Authorize SHARK-NIR on the SX side.
    11 •       Atmospheric conditions: AO working conditions.
    12 •       Bad pixel map, Background or Dark.
     13- Authorize SHARK-NIR on the SX side.
     14- Atmospheric conditions: AO working conditions.
     15- Bad pixel map, Background, or Dark.
     16
    1317**Procedure**
    14 •       This calibration is performed by sky observation combined with pointing scan in order to record a flat (that include telescope large scale transmission variations) on the detector.
    15 •       Single integration times for a given setup, using various flux levels with natural light with no coronagraph.
     18- This calibration is performed by sky observation combined with a pointing scan to record a flat (including telescope large scale transmission variations) on the detector.
     19- Single integration times for a given setup, using various flux levels with natural light with no coronagraph.
     20
     21**Templates**
     22
    1623**Success criteria**
    17 •       Width of flux distribution: 3.10-2 
     24- Width of flux distribution: 3.10-2 
     25
    1826**Notes**
    19 •       Same as activity 7.5 in AD4
     27- Same as activity 7.5 in AD4
     28
    2029**LBTO support**
    21 •       Dome open during twilight
    22 
    23 **Associated SHARK-NIR personnel**
     30- Dome open during twilight
    2431
    2532**Date performed and by whom**