Changes between Version 143 and Version 144 of HetProcedures/RA/hpf


Ignore:
Timestamp:
Nov 6, 2018 12:36:15 PM (6 years ago)
Author:
shetrone
Comment:

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  • HetProcedures/RA/hpf

    v143 v144  
    309309
    310310==== Evening ====
     311
     312The evening 'A' calibration sequence includes the LFC and Etalon
     313frames (and flats) that are necessary to start the nightly drift
     314calibration.  The 'C' calibrations contain the UNe lamps, which are
     315only present as an emergency backup source in case the LFC is offline.
     316Taking the 'A' sequence is critical; skipping the 'C' sequence if you
     317are crunched for time is OK, although that sequence has been timed to
     318fit within a typical stack time.
     319
     320
     321
     322
     323
    311324* The RA performing Ops in the afternoon will typically start the eveening HPS cal set. This will take about 1h10m to complete.
    312325{{{
     
    334347[hpf@hpfserver CalScripts] /home/hpf/Scripts/InstConfig/CalScripts/hpf_TurnOn.sh UNeS
    335348}}}
     349
     350We have added an additional script (hpf_takeLFCHRCalExposure.sh)
     351that will take a LFC exposure through the calibration fiber (~2 minutes
     352to complete).  This should not interfere with any other telescope
     353operations, as it is entirely internal to HPF.  If you find yourself in
     354a situation similar to last night, you can run this stand alone script
     355a few times while a different primary operation is happening (e.g. LRS
     356or VIRUS exposure, slew, or other telescope setup).  That will at least
     357provide a few LFC reference points to tie the drift calculation to.
     358
     359The script accepts an optional argument - N - where N is the number of
     360ramps you wish to take. e.g.  {{{ ./hpf_takeLFCHRCalExposure.sh 3 }}}
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