Changes between Version 64 and Version 65 of NightOperations/Commissioning/pFPA


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Timestamp:
Oct 15, 2023 8:54:29 AM (7 months ago)
Author:
stevenj
Comment:

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  • NightOperations/Commissioning/pFPA

    v64 v65  
    103103These twilight tests are in additional to the regular evening twilights for all science instruments.
    104104
     105=== Acquire twilights for both guiders in all filters === #gctwi
     106  * Start this about 5-7min before sunset
     107  * Try exposure times like 0.01s with very short cycle times
     108  * Cycle through all filters: B, g‘, r‘, i‘, (Clear - optional)
     109  * Adjust exposure times of both GCs to obtain two sets of twilights:
     110     * 20 "bright" images at 40-50k counts
     111     * 20 "faint" images at 5-10k counts
     112  * Full instructions are here: [wiki:HetProcedures/RA/probecals] and include how to take the images, how to process them into flats, and how to install them (either temporarily or permanently) into TCS.
     113
    105114=== Acquire WFS twilights (high flux and low flux) === #wftwi
     115  * Start this about 3-5min before sunset.
    106116  * Be sure that "Store images" is selected.
    107   * Adjust exposure times of both WFS to obtain two sets of twilights: one with peak flux values around ~3000 counts and one with peak flux values at 40-50k counts (saturation is 65k).
    108   * '''Verify that the spot positions are unchanged''' from flats taken previously (i.e., daily during OPS with dome lights on). If the spots have moved, contact Hanshin to get help updating the PAS pipeline that processes the wavefront sensor images.
    109 
    110 === Acquire HPFACQ twilights (high flux and low flux) === #hpfacqtwi
     117  * Adjust exposure times of both WFS to obtain two sets of twilights:
     118     * ~20 flats with one with peak flux values around ~3-5k counts
     119     * ~20 flats with peak flux values at 40-50k counts (saturation is 65k).
     120  * Try exposure times like *0.01s* with very short cycle times.
     121  * '''Verify again that the spot positions are unchanged''' from flats taken previously (i.e., daily during OPS with dome lights on). If the spots have moved, contact Hanshin to get help updating the PAS pipeline that processes the wavefront sensor images.
     122
     123=== Acquire HPFACQ camera twilights (high flux and low flux) === #hpfacqtwi
     124  * Start this about 3-5min before sunset
    111125  * Be sure that "Store images" is selected.
    112   * Adjust exposure times of the HPF ACQ camera to obtain two sets of twilights: one with peak flux values around ~200 counts and one with peak flux values at ~3000 counts (saturation is 4095 counts).
    113 
    114 === Acquire twilights for both guiders in all filters === #gctwi
    115   * Full instructions are here: [wiki:HetProcedures/RA/probecals] and include how to take the images, how to process them into flats, and how to install them (either temporarily or permanently) into TCS.
     126  * Adjust exposure times of the HPF ACQ camera to obtain two sets of twilights:
     127     * ~20 flats with one with peak flux values around ~200 counts
     128     * ~20 flats with peak flux values at ~3k counts (saturation is 4095).
     129  * Try exposure times like *0.01s* with very short cycle times.
     130  * These are not being used yet but will be invaluable for future comparisons
     131
    116132
    117133