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Commissioning and Science Verification

Subref z-position offsets>Measurement and analysis for single-beam receivers†

Revision history

• 2016-07-26 - created by Kamazaki,T.

Table of contents

• Subref z-position offsets>Measurement and analysis for single-beam receivers
  • Measurement
  • Analysis

Measurement†

1. Start COSMOS3 and tune the receiver to be used
2. Login to COSMOS3 manager GUI with Group=asteXX (e.g. aste16) and Project=sbrfXX (e.g. sbrf16)
3. Run CONT qlook (qlookc) from cos3launcher
4. Adjust pointing using either of the following observation tables
    

   Saturn	DASH345	stx5d3.start
   	BAND8	stx5b8.start

    
   • Auto-pointing is available toward bright planets
   • Turn on auto-pointing on the CONT qlook if necessary
5. Run either of the following observation tables according to a planet and a receiver
    

   Saturn	DASH345	stsbd3z.start
   	BAND8	stsbb8z.start

Analysis†

1. Login to an analysis computer (e.g. aste-ms1/aste-mx3) with account=asteXX (e.g. aste16)
2. Rsync CONT data from the ASTE site

   asteXX@aste-ms1: ~/analysis/bin/cont_rsync.sh <project> <obs. table> <time>
   e.g.)
   asteXX@aste-ms1: ~/analysis/bin/cont_rsync.sh sbrf16 stsbb8z 201608150
   ...

3. Run lck_sbrfz.py

   aste16@aste-ms1> ~/analysis/bin/lck_sbrefz.py ~/sbrfXX/continuum/data/CONT. ... .LCK

• Example

  aste16@aste-ms1> ~/analysis/bin/lck_sbrefz.py -c 1 ~/test/continuum/data/CONT.jpzd3.aste16.linux16.201602050910.LCK 
  *** the following parameters are assumed
  ***   dummy scan duration = 10.0 seconds
  ***   start dz =  -3.0 seconds
  ***   stop  dz = +13.0 seconds
  # Plot fit results
  * -> ddz [sample] = 186.326212
  * -> ddz [mm]     = -0.018781

  &ref(): File not found: "example_sbrefz.png" at page "CSV/SubrefZPositionMeasurementAnalysisSBRx";