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Commissioning and Science Verification

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

Revision history

• 2016-07-26 - created by Kamazaki,T.

Table of contents

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

Measurement†

1. Start COSMOS3 and tune a receiver to be used
2. Login to COSMOS3 manager GUI with Group=asteXX (e.g. aste16) and Project=sbrfXX (e.g. sbrf16)
3. Adjust pointing (preferable, but can skip)
4. Run either of the following observation tables according to a planet and a receiver band
    

   Saturn	DASH345	str05d3.start	5' x 5', 10" spacing
   		str02d3.start	2' x 2', 10" spacing
   	BAND8	str05b8.start	5' x 5', 8" spacing
   		str05b8.start	2' x 2', 8"spacing

Analysis†

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

   asteXX@aste-ms1: rsync -e ssh -avz astecntl@aste-1c:/cosmos3/aste/bklog/contlck/curr/CONT.<obs. table>.<group>.<project>.<date>.LCK ~/sbrfXX/continuum/data
   e.g.)
   asteXX@aste-ms1: rsync -e ssh -avz astecntl@aste-1c:/cosmos3/aste/bklog/contlck/curr/CONT.str02d3.aste16.sbrf16.20160815*.LCK
   ~/sbrfXX/continuum/data/
   ...

3. Create symbolic links with old file names to new CONT files

   asteXX@aste-ms1> ~/analysis/bin/cont_link.sh ~/sbrfXX/continuum/data/CONT.*.LCK

4. Run cont

   asteXX@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.