This directory contains the source code of a few miriad adapted for WSRT data.
To install these programs, the easiest way is to put them in the miriad source
tree and update the miriad installation. 


The following sources are available:


calstoke.for 

Computes fluxes for a few standard sources. Fluxes and ranges have been
adapted for 3C48 and 3C147 to suit the WSRT better. This is a library routine
that should go in the subs directory. You should recompile mfcal. You may
consider not implementing this function since it will affect ALL miriad
programs that compute fluxes for these two calibrators.


ivcFits.*
Read WSRT uvfits files and includes the Tsys values in the miriad uvfile. If
you want to apply Tsys coprrections to the data (which you probably should at
least at 21 cm), you should read the data with this program instead of with
the standard miriad fits reader.

uvfil.*
This does a Hanning smoothing on uvfiles. Note that the calibration tables
(including the bandpass) are NOT copied to the output file. The bandpass would
not be valid anymore after the Hanning smoothing. Better to apply this program
on calibrated data.


In the directory linux there are executables of the programs, compiled under
linux SuSe 8.3.