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


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Timestamp:
02/04/21 15:18:40 (4 years ago)
Author:
kradhakrishnan
Comment:

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  • docs/CommissioningPlan/P4.5

    v4 v5  
    1 == 4.5 Long-slit spectrograph mode testing      ==
     1== 4.5  Disk: Coronagraphic imaging of stellar jets ==
    22•       **Phase**               :       4 
    33•       **Status**              :       Draft   
    4 •       **Category**            :       Nighttime testing for functionality, operability, and performance (C5 + C7)
     4•       **Category**            :       Science verification / Early science (C8)
    55•       **Recurrence**  :       once after the completion of nighttime testing and performance check
    6 •       **Duration**            :       2 night(s)
     6•       **Duration**            :       1 night(s)
    77**Description**
    8 •       Dedicated to check the complete procedure and running of the OB scripts through SHINS for all the combinations of this observing mode.
     8•       Disk: Coronagraphic imaging of stellar jets
    99**Prerequisites**
    1010•       Authorize SHARK-NIR on the SX side.
    11 •       Atmospheric conditions: ?
    12 •       Atmospheric conditions: ?
     11•       Atmospheric conditions: CLEAR
    1312•       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:
     13•       Cloud Cover             : no clouds
     14•       Astronomical Seeing     : 0.8" or better
     15•       Sky Background  : Any
     16•       Water Vapor             : low
     17•       Timing Windows  : no major limitation as the observation will be done in filed stabilized mode
     18•       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?
     19•       Observing Filters       : NB_FeII, NB_HeI and NB_PaB both using single and dual band imaging
     20•       Detector Mode, DIT: according to the target brightness
     21•       Daytime Calibration Data required: dark/background, flat
     22•       Nighttime Calibration Data required: no night calibration needed
    2423
    2524**Procedure**
    26 •       ?
     25•       Observing of the target in field stabilized mode. No coronagraph used in this case to image the inner part of the system.
    2726**Notes**
    2827
    … …  
    3130
    3231**Associated SHARK-NIR personnel**
     32
    3333       
    34 
    3534**Date performed and by whom**