Changes between Version 2 and Version 3 of Instructions


Ignore:
Timestamp:
10/30/09 10:08:20 (15 years ago)
Author:
NaomiMcClureGriffiths
Comment:

--

Legend:

Unmodified
Added
Removed
Modified

  • Instructions

    v2 v3  
    1111 1. freqtab.dat lists the centre frequencies (in MHz) of channels in the final output data.
    1212 1. feed.dat is used to transform raw data to Stokes vectors (in the telescope frame). It defines the transformation in terms of reordering and sign changes.
    13  1. 0637Flux.dat tabulates the frequency dependence of the flux and polarization characteristics of the polarized calibrator (3c138, B0637-75, ...).
     13 1. 3c138Flux.dat tabulates the frequency dependence of the flux and polarization characteristics of the polarized calibrator (3c138, B0637-75, ...).
    1414
    15 These files should be in the working directory.  Copies will be assigned to each data file being processed.
     15These files should be in the working directory.  Copies of the first two will be assigned to each data file being processed.
     16The 3c138Flux.dat (or 0637Flux.dat) file will remain in the working directory and is found by the srcnam call in psolve. 
    1617
    1718=== Reduce the bandpass calibrator data ===