KFPA and Pipeline Data Reduction Guide
Note that much of the content of this documentation is out of date. Please refer to the GBT Pipeline documentation instead!!!
The KFPA was developed simultaneously with a data reduction pipeline.
Here we describe tools to check the status of an observation and run completed blocks of observations
through the pipeline to produce images. Finally we describe methods for combining blocks of calibrated
observations into images of complete regions.
Data Reduction Guide
The latest release of the data reduction guide is available as a PDF:
The remainder of this page expands on this guide and includes executable commands.
The observer is advised to make a short observation of a target source known to have
strong lines. Typically only a few seconds (30) are required for detection
of NH3 lines of sources like
W3OH or TMC-1.
The observer should then check the system temperatures of all beams/polarizations using
the GBTIDL command:
- showtsys,Scan-Number - Display the system temperatures for all beams, polarizations and frequency bands.
- getsigref,OnScan,OffScan - Display the sig-ref calibrated observations of your target source. The target source should be selected for strong lines in the frequency range of interest. Check all beams, polarizations and frequency bands for smooth spectral shapes. If the spectrometer is not setup properly use the CLEO spectrometer "reset-parameters" option to re-configure the spectrometer.
Pipeline with parameters tuned for Science requirements
The gbtpipeline automates many steps in the calibration and reduction steps.
To simplify the very first try of the Pipeline for NH3 1-1 and 2-2 line observations, we've created a script
demoW51 to run through a complete observation reduction and imaging process.
The total reduction and imaging process takes approximately 10 minutes and yields a number of images. Two Integrated line images are produced and displayed. The pipeline must run on a 64 bit machine (eg arcturus.gb.nrao.edu, thales.gb.nrao.edu or euclid.gb.nrao.edu)
To use this script in the Green Bank Linux environment type the following:
mkdir /home/scratch/$USER/pipeline
cd /home/scratch/$USER/pipeline
cp /home/gbtpipeline/release/contrib/demoW51 .
./demoW51
The commands above create a scratch directory, then copy a demo script to that directory and finally executes the script.
After completing the calibration and mapping, the script uses the casaviewer to display the integrated line intensity
images and the temperature map.
The pipeline executable is located at
- /opt/local/bin/gbtpipeline
Without arguments, the gbtpipeline starts up the appropriate version
for the NRAO computer the observer is currently using.
The development version is also available as
- /opt/local/bin/gbtpipeline-test
Pipeline parameter file options
The
gbtpipeline command takes a large number of command line options. These values may also be input via a
pipeline parameter file. To see the latest
gbtpipeline options, run the command without any arguments.
Time sequence of KFPA On-Off Moon observations
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Plot of Cal factors based on Lunar obs. at 18.5, 21.5, 23.7 and 25.5 GHz.
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2011 October 23
Observations made during KFPA commissioning time on. Made a sequence of observations to confirm repeatability of
observations. Three repetitions of observations of 23.7 GHz; Scans 1,2, 3,4 and 14,15. One observation each
at 18.5, 21.5 and 25.5 GHz with all beams and polarizations:
GBTIDL -> mooncalget,'TKFPA_83',1,2
...
#IF 1L 1R 2L 2R 3L 3R 4L 4R 5L 5R 6L 6R 7L 7R MHz Az(d) El(d) Scan
0 165.8 162.6 161.0 166.5 161.6 161.7 211.7 218.9 157.8 190.4 212.2 283.3 150.6 136.6 23705.606 225.8 41.7 1
1 151.4 150.6 22344.399 225.9 41.7 1
Calibration Factors
--gain-factors-left 1.046,1.077,1.073,0.819,1.099,0.817,1.152
--gain-factors-right 1.066,1.042,1.073,0.792,0.911,0.612,1.269
...
GBTIDL -> mooncalget,'TKFPA_83',3,4
#IF 1L 1R 2L 2R 3L 3R 4L 4R 5L 5R 6L 6R 7L 7R MHz Az(d) El(d) Scan
0 165.6 162.5 159.9 166.2 161.1 159.2 210.2 217.8 158.5 190.1 212.2 285.1 150.7 136.2 23705.605 226.6 41.3 3
1 150.8 150.6 22344.398 226.7 41.3 3
Calibration Factors
--gain-factors-left 1.046,1.083,1.075,0.824,1.092,0.816,1.149
--gain-factors-right 1.066,1.042,1.087,0.795,0.911,0.607,1.272
...
GBTIDL -> mooncalget,'TKFPA_83',10,11
...
#IF 1L 1R 2L 2R 3L 3R 4L 4R 5L 5R 6L 6R 7L 7R MHz Az(d) El(d) Scan
0 146.0 144.1 159.8 156.4 150.1 139.6 239.2 240.8 166.8 196.4 202.7 220.5 201.1 373.9 18500.984 229.6 39.6 10
1 161.5 160.2 19400.984 229.6 39.6 10
...
Calibration Factors
--gain-factors-left 1.294,1.182,1.258,0.790,1.132,0.932,0.939
--gain-factors-right 1.310,1.208,1.352,0.784,0.961,0.856,0.505
...
GBTIDL -> mooncalget,'TKFPA_83',12,13
...
#IF 1L 1R 2L 2R 3L 3R 4L 4R 5L 5R 6L 6R 7L 7R MHz Az(d) El(d) Scan
0 159.2 143.1 163.4 149.0 156.0 148.8 191.0 198.7 171.2 179.9 198.9 234.8 171.4 177.6 21501.144 230.5 39.1 12
1 153.3 154.2 22401.144 230.6 39.1 12
...
Calibration Factors
--gain-factors-left 1.089,1.061,1.112,0.908,1.012,0.872,1.011
--gain-factors-right 1.211,1.164,1.165,0.872,0.963,0.738,0.976
...
GBTIDL -> mooncalget,'TKFPA_83',14,15
...
#IF 1L 1R 2L 2R 3L 3R 4L 4R 5L 5R 6L 6R 7L 7R MHz Az(d) El(d) Scan
0 163.9 161.0 159.4 163.4 160.1 159.0 209.1 216.5 156.9 187.9 210.6 281.9 149.4 134.9 23705.601 231.4 38.6 14
1 149.5 149.1 22344.394 231.4 38.6 14
...
Calibration Factors
--gain-factors-left 1.045,1.075,1.070,0.819,1.092,0.814,1.147
--gain-factors-right 1.064,1.048,1.078,0.791,0.912,0.608,1.270
...
GBTIDL -> mooncalget,'TKFPA_83',16,17
...
#IF 1L 1R 2L 2R 3L 3R 4L 4R 5L 5R 6L 6R 7L 7R MHz Az(d) El(d) Scan
0 166.4 169.1 159.4 159.7 164.3 171.5 215.7 227.7 166.3 195.1 213.4 271.2 150.2 94.9 25501.356 232.1 38.1 16
1 172.7 189.7 26401.356 232.2 38.1 16
...
Calibration Factors
--gain-factors-left 1.031,1.076,1.044,0.796,1.032,0.804,1.142
--gain-factors-right 1.015,1.074,1.001,0.753,0.880,0.633,1.808
--
GlenLangston - 2011-09-07