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Commissioning and Science Verification

Beam map>Measurement and analysis for single-beam receivers†

Revision history

• 2016-07-26 - Kamazaki,T. - created.

Table of contents

• Beam map>Measurement and analysis for single-beam receivers
  • Measurement
  • Analysis

Measurement†

1. Start COSMOS3
2. Login to COSMOS3 manager GUI with Group=asteXX and Project=sbrfXX
3. Tune receivers
4. Adjust pointing (preferable, but can skip)
5. Run either of the following observation tables according to available planets
    

   Jupiter	DASH345	jpr5d3.start
   	BAND8	jpr5b8.start
   Saturn	DASH345	str5d3.start
   	BAND8	str5b8.start

Analysis†

1. Login to an analysis computer with account=asteXX
2. Confirm that continuum data is transferred and is located at ~/sbrfXX/continuum/data

   aste16@aste-ms1> ls ~/sbrfXX/continuum/data/CONT.(obs. table).*.LCK
   ...

3. Run cont

   aste16@aste-ms1> ~/analysis/bin/cont.sh

   1. Map Analysis>CFITS
      1. Select a LCK file in the .LCK File List button
      2. Set parameters
         Normally, it is enough to use default values as shown below.
         &ref(): File not found: "cfits_v6.png" at page "CSV/BeamMapMeasurementAnalysisSBRx";
      3. Push the EXEC button to create a image FITS file
   2. Map Analysis>CMAP
      1. Select the image FITS file created in the previous step

• Endian conversion is UNNECESSARY for continuum data taken on Linux COSMOS3.
• LCK endian and FITS endian buttons are NOT available.

e.g.)
aste16@aste-ms1> ls ~/test/continuum/data/CONT.jpzd3.*.LCK
/home/aste16/test/continuum/data/CONT.jpzd3.aste16.linux16.201602050910.LCK@
/home/aste16/test/continuum/data/CONT.jpzd3.aste16.linux16.201602050922.LCK@
aste16@aste-ms1> ~/analysis/bin/lck_sbrefz.py ~/test/continuum/data/CONT.jpzd3.aste16.linux16.201602050910.LCK 
*** it is assumed that dummy scan duration is "10.0" seconds
# Plot fit results
* -> ddz [sample] = 186.326212
* -> ddz [mm]     = -0.018781

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