OUTPUT FILES
  
  tempo.lis 
  
     ASCII format.  Lists input parameters, input data (TOAs,
     frequencies, weights), pre-fit and post-fit residuals,
     best-fit parameters and uncertaities, statistics, and a
     crude covariance matrix.
  
  resid2.tmp 
  
     Residuals, etc.  Binary format.  
     Each record contains eight real*8 values:
       --TOA (MJD, referenced to solar system barycenter)
       --Postfit residual (pulse phase, from 0 to 1)
       --Postfit residual (seconds)
       --Orbital phase (where applicable)
       --Observing frequency (in barycenter frame)
       --Weight of point in the fit
       --Timing uncertainty (according to input file)
       --Prefit residual (pulse phase)
  
  matrix.tmp 
  
      Covariance matrix.  Binary format with variable length
      records.  The n'th record contains:
       --integer m (see below)
       --integer j (parameter index)
       --char*4  parameter name
       --real*8  generalized covariance of parameter
       --real*8  uncertainty of parameter
       --real*8(m) normalized covarinaces:
                   a(j,k)/sig(j)sig(k),k=1..m
  
  <psrname>.par 
  
      ASCII format.  Control parameters and name, final value, fit 
      flag and error for pulsar parameters. Can be used as an input 
      parameter file for TEMPO and other programs.
  
  gro.1, gro.2
  
      Timing parameters in "GRO" format.  ASCII.  Produced in "GRO" 
      mode only. gro.2 contains binary parameters where applicable.
      Note: for TEMPO V11.0, the name of barycentric ephemeris and the
      full pulsar name are appended to the gro.1 output line.
  
  gro.99
  
      Rotation parameters translated to epoch at middle of data set.  
      ASCII format.  Produced in "GRO" mode only.

  polyco.dat

      Pulsar ephemerides.  See "prediction mode (tz)" section.