Changes between Version 4 and Version 5 of Instructions


Ignore:
Timestamp:
10/30/09 10:13:17 (15 years ago)
Author:
NaomiMcClureGriffiths
Comment:

--

Legend:

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  • Instructions

    v4 v5  
    1919 1. Load the rpfits file into "parkespol" format.
    2020{{{
    21 pload 1934.rpf
     21pload 2006-11-20_0915_1934-638DEC1.rpf
    2222#
    23 # This will create a directory 1934/ and
     23# This will create a directory 2006-11-20_0915_1934-638DEC1/ and
    2424# with contents
    2525# -rw-r--r--   1 mcc381  atculg  2355200 Feb  1 22:23 data.rpf
     
    3131 1. Perform the bandpass calibration
    3232{{{
    33 bpass 1934
     33bpass 2006-11-20_0915_1934-638DEC1
    3434}}}
    3535
     
    6161}}}
    6262
     63Be careful not to perform this procedure more than twice.  If you need to back up in the process remove the scan.dat, phasefit.dat and polparams.dat files from within the calibrator directory.
    6364
    6465=== Reduce the astronomical data ===
    65  1. Load the rpfits file
     66 1. Load the rpfits file (called source.rpf in this example).
    6667{{{
    6768pload source.rpf
     
    6970 1. Copy the bandpass tables and polarisation corrections
    7071{{{
    71 gcopy source 1934 3c138
     72gcopy source 2006-11-20_0915_1934-638DEC1 2006-11-20_1401_3c138_Cal_DEC
    7273}}}
    73  1. Apply the calibrations and write results as a single-dish FITS file.
     74 1. Apply the calibrations and write results as a single-dish FITS file called output.sdfits in this example.
    7475{{{
    75 calscans.pl list
     76calscans.pl list ouput.sdfits
    7677}}}
    7778where list is a list of the data files to be calibrated.