Changes between Version 2 and Version 3 of NightOperations/SciencePlans/20181122


Ignore:
Timestamp:
Nov 21, 2018 7:54:54 PM (5 years ago)
Author:
shetrone
Comment:

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  • NightOperations/SciencePlans/20181122

    v2 v3  
    9797  *  mark this as an engineering target and charge the time to engineering time of type ENG18-2-004
    9898
    99   *  Do a total of 10 sets to complete the test (this can be the same flux standard but on different tracks (E/W or different nights).
    10099
    101 == Low Priority On Sky Engineering Tests ==
    102 
    103 === Testing of the ACAM position ===
    104 
    105 Purpose:  We want to see if the ACAM position changes with respect to the IHMP over time.  We want this data every night and when ever we get an unusually high or low temperature.   It would be good to vary the Az as well.
    106 
    107 Determine the Center of the BIB:
    108   *  Select a 14th mag star in a reasonably rich field with shuffle for the BIB
    109   *  Setup on the very center of the BIB field of view and save an image note any differences from the wiki center position.
    110   *  Guide on one of the guide probes
    111   *  Put in the ACAM and save an shallow image with the target star not saturated.
    112   *  Report on the position of the BIB in the night report and on [wiki:NightOperations/Commissioning/Results]
    113   *  Save a deeper image which should show more than a dozen stars.
    114 
    115 Determine the Center of LRS2-B
    116   *  Select a 14th mag star in a reasonably rich field with shuffle for the LRS2-B
    117   *  Setup on LRS2-B and start guiding on one of the guiders
    118   *  Take LRS2-B spectrum, probably 60 seconds. 
    119   *  Adjust the position so that the star is at the center of LRS2-B IFU using lmap until the offsets are less than 0.3"
    120 {{{syscmd -T 'Guider1_offset_fiducial ( dx_asec=-0.01,dy_asec=0.55,compensate="false")'}}}
    121   *  Confirm the star is at the center of the IFU by taking a spectrum.
    122   *  Once it is as the center of the IFU put in the ACAM and take a shallow image so that the star is not saturated.
    123   *  Report on the position of the LRS2-B in the night report and on [wiki:NightOperations/Commissioning/Results]
    124   *  Take a deeper image so that there are large number of stars.
    125 
    126 Determine the Center of LRS2-R
    127   *  Select a 14th mag=== Testing of the ACAM position === star in a reasonably rich field with shuffle for the LRS2-R
    128   *  Setup on LRS2-R and start guiding on one of the guiders
    129   *  Take LRS2-R spectrum, probably 60 seconds. 
    130   *  Adjust the position so that the star is at the center of LRS2-R IFU using lmap until the offsets are less than 0.3"
    131   *  Confirm the star is at the center of the IFU by taking a spectrum.
    132   *  Once it is as the center of the IFU put in the ACAM and take a shallow image so that the star is not saturated.
    133   *  Report on the position of the LRS2-R in the night report and on [wiki:NightOperations/Commissioning/Results]
    134   *  Take a deeper image so that there are large number of stars.
    135 
    136 
    137  
    138  
    139100
    140101== Closed dome engineering: ==