Changes between Version 1 and Version 2 of NightOperations/SciencePlans/20181122


Ignore:
Timestamp:
Nov 21, 2018 7:53:39 PM (5 years ago)
Author:
shetrone
Comment:

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  • NightOperations/SciencePlans/20181122

    v1 v2  
    4141
    4242Note if these values for the integral and principle values are clearly wrong or bad then try smaller values ki=0.05 and kp=0.95.
     43
     44=== Testing of the ACAM position ===
     45
     46Purpose:  We want to see if the ACAM position changes with respect to the IHMP over time.  We want this data when ever we get an unusually high or low temperature.   It would be good to vary the Az as well.
     47
     48Determine the Center of the BIB:
     49  *  Select a 14th mag star in a reasonably rich field with shuffle for the BIB
     50  *  Setup on the very center of the BIB field of view and save an image note any differences from the wiki center position.
     51  *  Guide on one of the guide probes
     52  *  Put in the ACAM and save an shallow image with the target star not saturated.
     53  *  Report on the position of the BIB in the night report and on [wiki:NightOperations/Commissioning/Results]
     54  *  Save a deeper image which should show more than a dozen stars.
     55
     56Determine the Center of LRS2-B
     57  *  Select a 14th mag star in a reasonably rich field with shuffle for the LRS2-B
     58  *  Setup on LRS2-B and start guiding on one of the guiders
     59  *  Take LRS2-B spectrum, probably 60 seconds. 
     60  *  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"
     61{{{syscmd -T 'Guider1_offset_fiducial ( dx_asec=-0.01,dy_asec=0.55,compensate="false")'}}}
     62  *  Confirm the star is at the center of the IFU by taking a spectrum.
     63  *  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.
     64  *  Report on the position of the LRS2-B in the night report and on [wiki:NightOperations/Commissioning/Results]
     65  *  Take a deeper image so that there are large number of stars.
     66
     67Determine the Center of LRS2-R
     68  *  Select a 14th mag=== Testing of the ACAM position === star in a reasonably rich field with shuffle for the LRS2-R
     69  *  Setup on LRS2-R and start guiding on one of the guiders
     70  *  Take LRS2-R spectrum, probably 60 seconds. 
     71  *  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"
     72  *  Confirm the star is at the center of the IFU by taking a spectrum.
     73  *  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.
     74  *  Report on the position of the LRS2-R in the night report and on [wiki:NightOperations/Commissioning/Results]
     75  *  Take a deeper image so that there are large number of stars.
     76
     77Determine the Center of the HPFACQ IFU on the ACQ:
     78  *  Select a 9-10th mag star with shuffle for the regular setup (600)
     79  *  Setup on the very center of the HPFACQ field of view and save an image.
     80  *  Guide on one of the guide probes and make sure that the star is still at the center of the HPFACQ
     81  *  Put in the ACAM and save an shallow image with the target star not saturated.
     82  *  Report on the position of the HPFACQ regular setup in the night report, on the markers wiki page and on [wiki:NightOperations/Commissioning/Results]
     83
    4384
    4485