History of CSV/BeamMapMeasurementAnalysisSBRx (No. 10)

• History
• View the source.
• CSV/BeamMapMeasurementAnalysisSBRx has been deleted.
  • 1 (2016-07-26 (Tue) 16:52:15)
  • 2 (2016-07-26 (Tue) 17:21:19)
  • 3 (2016-08-05 (Fri) 12:17:10)
  • 4 (2016-08-14 (Sun) 16:00:39)
  • 5 (2016-08-15 (Mon) 13:43:56)
  • 6 (2016-08-16 (Tue) 13:17:54)
  • 7 (2016-08-16 (Tue) 21:10:29)
  • 8 (2016-08-24 (Wed) 13:52:16)
  • 9 (2016-08-28 (Sun) 17:47:12)
  • 10 (2016-09-02 (Fri) 11:18:15)
  • 11 (2016-09-02 (Fri) 17:24:11)
  • 12 (2017-03-13 (Mon) 15:09:05)

Commissioning and Science Verification

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

Revision history

• 2016-07-26 - Kamazaki,T. - created
• 2016-09-02 - Kamazaki,T. - added two obs. tables for fine maps

Table of contents

• Beam map>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 (preferable, but can skip)
    

   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	str05d3.start	5' x 5', 10" spacing	quick map for a large area
   		str02d3.start	2' x 2', 10" spacing	quick map for a small area
   		stb2xd3.start	2' x 2', 4" spacing, x-scan	fine map
   		stb2yd3.start	2' x 2', 4" spacing, y-scan
   	BAND8	str05b8.start	5' x 5', 8" spacing	quick map for a large area
   		str05b8.start	2' x 2', 8"spacing	quick map for a small area
   		stb2xb8.start	2' x 2', 4" spacing, x-scan	fine map
   		stb2yb8.start	2' x 2', 4" spacing, y-scan

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> -link
   e.g.)
   asteXX@aste-ms1: ~/analysis/bin/cont_rsync.sh sbrf16 str02b8 2016-08-15 -link
   ...

   • cont_rsync.sh -link automatically create symbolic links with old file names to new CONT files
   • The symbolic links can be also created by cont_link.sh, if you miss to put the -link option

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

3. 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.
4. Read the exported FITS on ds9 for further processing