Version 1 (modified by 15 years ago) (diff) | ,
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CABB Reduction Example
Data was taken by J Stevens (JBS) and M Voronkov (MV) on the night of 2009-04-01. This experiment is described http://svn.atnf.csiro.au/trac/operations/wiki/NFO/Development/CABB/Logs/001,here.
This data is a set of 3-point mosaics on calibrators around 0823-500 and 1934-638. This reduction is to test:
- bandpass stability on calibrators
- mosaic reduction with CABB data
- can we detect polarisation on 1514-241?
- check for decorrelation at offset pointings
Loading the data
For this example I will load only the data from 2009-04-01_1407 onwards as the RA half-power point problem was resolved and the observations include a possibly polarised source 1514-241.
The files we are using are:
4.5G 2009-04-02 11:14 2009-04-01_1407.C999 4.7G 2009-04-02 11:15 2009-04-01_1543.C999 2.8G 2009-04-02 11:17 2009-04-01_1723.C999 1.9G 2009-04-02 11:17 2009-04-01_1822.C999 3.1G 2009-04-02 11:18 2009-04-01_1938.C999
for a total of 17G.
First atlod:
atlod% inp Task: atlod in = *.C999 out = firstnight_1934.uv ifsel = 1,2 restfreq = options = nfiles = nscans =
Attachments (10)
- firstnight_firstlook.2.png (15.8 KB) - added by 15 years ago.
- firstnight_firstlook.png (15.8 KB) - added by 15 years ago.
- firstnight_aftertimeflag.png (28.1 KB) - added by 15 years ago.
- firstnight_1934_beforecal.png (12.1 KB) - added by 15 years ago.
- firstnight_1934p_beforecal.png (7.1 KB) - added by 15 years ago.
- firstnight_1934b_beforecal.png (18.1 KB) - added by 15 years ago.
- firstnight_1934_aftercal1.png (10.6 KB) - added by 15 years ago.
- firstnight_1934b_aftercal1.png (20.5 KB) - added by 15 years ago.
- firstnight_1934p_aftercal1.png (9.2 KB) - added by 15 years ago.
- firstnight_1934ri_aftercal1.png (20.9 KB) - added by 15 years ago.
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