Changes between Version 1 and Version 2 of docs/CommissioningPlan/P3.23


Ignore:
Timestamp:
02/04/21 14:50:45 (4 years ago)
Author:
kradhakrishnan
Comment:

--

Legend:

Unmodified
Added
Removed
Modified

  • docs/CommissioningPlan/P3.23

    v1 v2  
    1  == P3.23       Wavelength calibration ==
    2 •       **Phase**               :       3 
     1== 3.23 Coronagraphic imaging + pupil stabilization mode testing ==
     2•       **Phase**               :       4 
    33•       **Status**              :       Draft   
    4 •       **Category**            :       Daytime calibration (C3)
    5 •       **Recurrence**  :       every night when LSS observing mode is used.
    6 •       **Duration**            :       10 minutes
     4•       **Category**            :       Nighttime testing for functionality, operability, and performance (C5 + C7)
     5•       **Recurrence**  :       once
     6•       **Duration**            :       3 night(s)
    77**Description**
    8 •       Determine the central wavelength of each pixel for the long split spectroscopy observing mode.
     8•       Dedicated to check the complete procedure and running of the OB scripts through SHINS for all the combinations of this observing mode.
    99**Prerequisites**
    1010•       Authorize SHARK-NIR on the SX side.
    11 •       Atmospheric conditions: AO working conditions.
     11•       Atmospheric conditions: ?
     12•       Atmospheric conditions: ?
    1213•       Bad pixel map, Background or Dark, Flat-field, distortion map
     14•       Cloud Cover             :
     15•       Astronomical Seeing     :
     16•       Sky Background  : Any / Bright
     17•       Water Vapor             : Any
     18•       Timing Windows  :
     19•       Observing Targets       :
     20•       Observing Filters       :
     21•       Detector Mode, DIT:
     22•       Daytime Calibration Data required:
     23•       Nighttime Calibration Data required:
     24
    1325**Procedure**
    14 •       This calibration is performed illuminating the slit with the spectral calibration lamps with at least 5 known emission lines; background exposures with lamps switched off required.
    15 **Success criteria**
    16 •       LRS: 10 nm (goal 5 nm), MRS: 1 nm.
     26•       ?
    1727**Notes**
    18 •       Same as activity 7.10 in AD4
     28
    1929**LBTO support**
    20 •       Support from LBTI/LBTO?
     30•       SOUL-AO support
     31
    2132**Associated SHARK-NIR personnel**
    22 •       JF, LM, MdP
     33
     34       
    2335**Date performed and by whom**