Changes between Version 1 and Version 2 of docs/CommissioningPlan/P3.12


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Timestamp:
01/19/21 17:30:52 (4 years ago)
Author:
kradhakrishnan
Comment:

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  • docs/CommissioningPlan/P3.12

    v1 v2  
    1  == P3.12       Checking field-stabilized mode/bearing rotation service ==
     1 == P3.12       Star center Fourier mode images ==
    22•       **Phase**               :       3 
    33•       **Status**              :       Draft   
    4 •       **Category**            :       Nighttime testing (functionality and operability) (C4)
    5 •       **Recurrence**  :       once at commissioning
    6 •       **Duration**            :       40 minutes
     4•       **Category**            :       Nighttime calibration (C5)
     5•       **Recurrence**  :       on every target, starting from commissioning.
     6•       **Duration**            :       1 hour
    77**Description**
    8 •       The field stabilized mode or in other words, the working of the bearing tracking service will be tested.
     8•       This calibration is performed to calibrate the target star center with respect to the detector in order to provide a reference input for frame derotation and quadrant combination.
    99**Prerequisites**
     10•       Authorize SHARK-NIR on the SX side.
    1011•       Atmospheric conditions: AO working conditions.
    11 •       Authorize SHARK-NIR on the SX side.
    12 •       Targets (star cluster) near zenith and horizon (say airmass of 2).
     12•       Bad pixel map, Dark
    1313**Procedure**
    14 •       Select the target near airmass 2. There should be stars spread across the entire SCICAM, preferably close to the edges as well.
    15 •       Start the bearing tracking services (field-stabilized mode).
    16 •       Take short-exposure images for a duration of ##minutes.
    17 •       Check if the positions of these stars.
    18 •       Repeat the same for the target close to the zenith.
    19 •       The above may be repeated for a target where the rotation of the bearing is in the opposite direction as of the above tested one.
     14•       DM produce a pattern offset with four spots symmetric with respect to the star + AO closed-loop + coronagraph
     15•       The required specifications of the corresponding image are a grid of at least 2x2 regularly spaced focal plane image peaks within 5 and 15 lambda/D with FWHM < 45 mas and separation precision < 6 mas.
     16•       DM offset applied on target acquisition to produce a waffle image. Find the center of the four first-order diffraction peaks (cross geometry) to deduce the pixel corresponding to the center field.
    2017**Success criteria**
    21 •       The bearing tracking service works well and the field is stabilized within the precision needed.
     18•       Accuracy of 3 mas (goal 1 mas)
    2219**Notes**
     20•       Same as activity 7.8 in AD4
    2321**LBTO support**
    24 •       Support from LBTI/LBTO?
     22•       SOUL-AO support
    2523**Associated SHARK-NIR personnel**
    26 •       JF, LM, MdP
     24
    2725**Date performed and by whom**