! Started logfile: /scr/pima/rdv96_uvs/J2258-2758_S_uvs.log on Sat Dec 21 00:26:12 2013
obs /scr/pima/rdv96_uvs/J2258-2758_S_uva.fits
! Reading UV FITS file: /scr/pima/rdv96_uvs/J2258-2758_S_uva.fits
! AN table 1: 6 integrations on 3 of 3 possible baselines.
! AN table 2: 2 integrations on 10 of 10 possible baselines.
! AN table 3: 2 integrations on 28 of 28 possible baselines.
! AN table 4: 2 integrations on 28 of 28 possible baselines.
! AN table 5: 2 integrations on 36 of 36 possible baselines.
! AN table 6: 2 integrations on 28 of 28 possible baselines.
! AN table 7: 2 integrations on 15 of 15 possible baselines.
! AN table 8: 11 integrations on 3 of 3 possible baselines.
! Apparent sampling: 0.970674 visibilities/baseline/integration-bin.
! Found source: J2258-2758
! 
! There are 4 IFs, and a total of 4 channels:
! 
!  IF  Channel    Frequency  Freq offset  Number of   Overall IF
!       origin    at origin  per channel   channels    bandwidth
!  ------------------------------------------------------------- (Hz)
!  01        1  2.23299e+09        8e+06          1        8e+06
!  02        2  2.26299e+09        8e+06          1        8e+06
!  03        3  2.35299e+09        8e+06          1        8e+06
!  04        4  2.37299e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 0 lines of history.
! 
! Reading 1324 visibilities.
select RR
! Selecting polarization: RR,  channels: 1..4
! Reading IF 1 channels: 1..1
! Reading IF 2 channels: 2..2
! Reading IF 3 channels: 3..3
! Reading IF 4 channels: 4..4
print "field_size =",field_size
! field_size = 1024 
print "field_cell =",field_cell
! field_cell = 0.4 
print "taper_size =",taper_size
! taper_size = 20 
![@/home/lpetrov/bin/rdv_muppet /scr/pima/rdv96_uvs/J2258-2758_S]
integer clean_niter
clean_niter = 100
float clean_gain
clean_gain = 0.03
float dynam
dynam = 6.0
float soltime1
soltime1 = 800000
float soltime2
soltime2 = 15
float soltime3
soltime3 = 1
float thresh
thresh = 0.5
float win_mult
win_mult = 1.8
float old_peak
float new_peak
float flux_cutoff
selfant "",false
! 1:HH       self-cal  status=correctable  weight=1
! 1:WF       self-cal  status=correctable  weight=1
! 1:WZ       self-cal  status=correctable  weight=1
! 2:FD       self-cal  status=correctable  weight=1
! 2:HH       self-cal  status=correctable  weight=1
! 2:HN       self-cal  status=correctable  weight=1
! 2:SC       self-cal  status=correctable  weight=1
! 2:WF       self-cal  status=correctable  weight=1
! 3:FD       self-cal  status=correctable  weight=1
! 3:HH       self-cal  status=correctable  weight=1
! 3:HN       self-cal  status=correctable  weight=1
! 3:LA       self-cal  status=correctable  weight=1
! 3:NL       self-cal  status=correctable  weight=1
! 3:PT       self-cal  status=correctable  weight=1
! 3:SC       self-cal  status=correctable  weight=1
! 3:WF       self-cal  status=correctable  weight=1
! 4:FD       self-cal  status=correctable  weight=1
! 4:HN       self-cal  status=correctable  weight=1
! 4:KP       self-cal  status=correctable  weight=1
! 4:LA       self-cal  status=correctable  weight=1
! 4:NL       self-cal  status=correctable  weight=1
! 4:PT       self-cal  status=correctable  weight=1
! 4:SC       self-cal  status=correctable  weight=1
! 4:WF       self-cal  status=correctable  weight=1
! 5:FD       self-cal  status=correctable  weight=1
! 5:HN       self-cal  status=correctable  weight=1
! 5:KP       self-cal  status=correctable  weight=1
! 5:LA       self-cal  status=correctable  weight=1
! 5:NL       self-cal  status=correctable  weight=1
! 5:OV       self-cal  status=correctable  weight=1
! 5:PT       self-cal  status=correctable  weight=1
! 5:SC       self-cal  status=correctable  weight=1
! 5:WF       self-cal  status=correctable  weight=1
! 6:BR       self-cal  status=correctable  weight=1
! 6:FD       self-cal  status=correctable  weight=1
! 6:KP       self-cal  status=correctable  weight=1
! 6:LA       self-cal  status=correctable  weight=1
! 6:MK       self-cal  status=correctable  weight=1
! 6:NL       self-cal  status=correctable  weight=1
! 6:OV       self-cal  status=correctable  weight=1
! 6:PT       self-cal  status=correctable  weight=1
! 7:FD       self-cal  status=correctable  weight=1
! 7:KP       self-cal  status=correctable  weight=1
! 7:LA       self-cal  status=correctable  weight=1
! 7:MK       self-cal  status=correctable  weight=1
! 7:OV       self-cal  status=correctable  weight=1
! 7:PT       self-cal  status=correctable  weight=1
! 8:HH       self-cal  status=correctable  weight=1
! 8:MA       self-cal  status=correctable  weight=1
! 8:WZ       self-cal  status=correctable  weight=1
system "rm /tmp/ff.ff"
mapsize field_size, field_cell
! Map grid = 1024x1024 pixels with 0.400x0.400 milli-arcsec cellsize.
startmod
! Applying default point source starting model.
! Performing phase self-cal
! Adding 1 model components to the UV plane model.
! The established model now contains 1 components and 1 Jy
! 
! Correcting IF 1.
!  A total of 6 telescope corrections were flagged in sub-array 1.
!  A total of 33 telescope corrections were flagged in sub-array 8.
! 
! Correcting IF 2.
!  A total of 6 telescope corrections were flagged in sub-array 1.
!  A total of 2 telescope corrections were flagged in sub-array 2.
!  A total of 33 telescope corrections were flagged in sub-array 8.
! 
! Correcting IF 3.
!  A total of 6 telescope corrections were flagged in sub-array 1.
!  A total of 2 telescope corrections were flagged in sub-array 2.
!  A total of 33 telescope corrections were flagged in sub-array 8.
! 
! Correcting IF 4.
!  A total of 6 telescope corrections were flagged in sub-array 1.
!  A total of 33 telescope corrections were flagged in sub-array 8.
! 
! Fit before self-cal, rms=1.809515Jy  sigma=25.635052
! Fit after  self-cal, rms=0.849659Jy  sigma=10.236045
! clrmod: Cleared the established, tentative and continuum models.
! Redundant starting model cleared.
print "=== Flag out IVS stations"
! === Flag out IVS stations 
integer lun
string  cfg_file
lun = outfile ( "/tmp/ff.ff" ) 
do i=1,nsub
  do j=1,ntel(i)
    fprintf lun, "%s\n", telname(j,i)
    end do
  end do
close ( lun )
system "/home/lpetrov/bin/dimap_flag_process.csh /tmp/ff.ff"
![@/tmp/ff.ff \]
flag 1:HH
! Flagging baselines of antenna 1:HH in the currently selected channels.
flag 1:WF
! Flagging baselines of antenna 1:WF in the currently selected channels.
flag 1:WZ
! Flagging baselines of antenna 1:WZ in the currently selected channels.
flag 2:HH
! Flagging baselines of antenna 2:HH in the currently selected channels.
flag 2:WF
! Flagging baselines of antenna 2:WF in the currently selected channels.
flag 3:HH
! Flagging baselines of antenna 3:HH in the currently selected channels.
flag 3:WF
! Flagging baselines of antenna 3:WF in the currently selected channels.
flag 4:WF
! Flagging baselines of antenna 4:WF in the currently selected channels.
flag 5:WF
! Flagging baselines of antenna 5:WF in the currently selected channels.
flag 8:HH
! Flagging baselines of antenna 8:HH in the currently selected channels.
flag 8:MA
! Flagging baselines of antenna 8:MA in the currently selected channels.
flag 8:WZ
! Flagging baselines of antenna 8:WZ in the currently selected channels.
![Exited script file: /tmp/ff.ff]
uvw 2,-1
! Uniform weighting binwidth: 2 (pixels).
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=3.789 mas, bmaj=12.52 mas, bpa=-5.414 degrees
! Estimated noise=2.07064 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (0, 0).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 1.03375 Jy
! Component: 100  -  total flux cleaned = 1.30535 Jy
! Total flux subtracted in 100 components = 1.30535 Jy
! Clean residual min=-0.043769 max=0.119310 Jy/beam
! Clean residual mean=0.002169 rms=0.016176 Jy/beam
! Combined flux in latest and established models = 1.30535 Jy
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 17 components and 1.30535 Jy
! 
! Correcting IF 1.
!  A total of 12 telescope corrections were flagged in sub-array 1.
!  A total of 4 telescope corrections were flagged in sub-array 2.
!  A total of 4 telescope corrections were flagged in sub-array 3.
!  A total of 2 telescope corrections were flagged in sub-array 4.
!  A total of 2 telescope corrections were flagged in sub-array 5.
! 
! Correcting IF 2.
!  A total of 12 telescope corrections were flagged in sub-array 1.
!  A total of 2 telescope corrections were flagged in sub-array 2.
!  A total of 4 telescope corrections were flagged in sub-array 3.
!  A total of 2 telescope corrections were flagged in sub-array 4.
!  A total of 2 telescope corrections were flagged in sub-array 5.
! 
! Correcting IF 3.
!  A total of 12 telescope corrections were flagged in sub-array 1.
!  A total of 2 telescope corrections were flagged in sub-array 2.
!  A total of 4 telescope corrections were flagged in sub-array 3.
!  A total of 2 telescope corrections were flagged in sub-array 4.
!  A total of 2 telescope corrections were flagged in sub-array 5.
! 
! Correcting IF 4.
!  A total of 12 telescope corrections were flagged in sub-array 1.
!  A total of 4 telescope corrections were flagged in sub-array 2.
!  A total of 4 telescope corrections were flagged in sub-array 3.
!  A total of 2 telescope corrections were flagged in sub-array 4.
!  A total of 2 telescope corrections were flagged in sub-array 5.
! 
! Fit before self-cal, rms=0.323528Jy  sigma=5.902435
! Fit after  self-cal, rms=0.320961Jy  sigma=5.883390
! Inverting map and beam 
! Estimated beam: bmin=3.789 mas, bmaj=12.52 mas, bpa=-5.414 degrees
! Estimated noise=2.07064 mJy/beam.
! Added new window around map position (-3.6, -4.4).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.134373 Jy
! Component: 100  -  total flux cleaned = 0.206652 Jy
! Total flux subtracted in 100 components = 0.206652 Jy
! Clean residual min=-0.034211 max=0.046513 Jy/beam
! Clean residual mean=0.000584 rms=0.009632 Jy/beam
! Combined flux in latest and established models = 1.512 Jy
! Performing phase self-cal
! Adding 24 model components to the UV plane model.
! The established model now contains 38 components and 1.512 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.253969Jy  sigma=4.418654
! Fit after  self-cal, rms=0.252336Jy  sigma=4.400823
! Inverting map 
print "=== Finished uniform weighting clean ==="
! === Finished uniform weighting clean === 
uvw 0,-1
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
win_mult = win_mult * 1.6
clean_niter = clean_niter * 2
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=4.659 mas, bmaj=14.88 mas, bpa=-4.014 degrees
! Estimated noise=1.55221 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0651217 Jy
! Component: 100  -  total flux cleaned = 0.0971009 Jy
! Component: 150  -  total flux cleaned = 0.115699 Jy
! Component: 200  -  total flux cleaned = 0.127025 Jy
! Total flux subtracted in 200 components = 0.127025 Jy
! Clean residual min=-0.028162 max=0.025743 Jy/beam
! Clean residual mean=-0.000196 rms=0.007773 Jy/beam
! Combined flux in latest and established models = 1.63903 Jy
! Performing phase self-cal
! Adding 63 model components to the UV plane model.
! The established model now contains 95 components and 1.63903 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.240118Jy  sigma=4.100320
! Fit after  self-cal, rms=0.239421Jy  sigma=4.092885
! Inverting map 
print "=== Finished natural weighting clean for VLBI sites ==="
! === Finished natural weighting clean for VLBI sites === 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Telescope amplitude corrections in sub-array 1:
!   HH        0.00*    WF        0.00*    WZ        0.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   FD        0.00*    HH        0.00*    HN        0.00*    SC        0.00*    
!   WF        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   FD        1.00     HH        1.00*    HN        1.11     LA        1.21     
!   NL        1.17     PT        1.11     SC        0.95     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   FD        1.01     HN        1.05     KP        1.02     LA        1.22     
!   NL        1.03     PT        1.04     SC        0.97     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   FD        1.01     HN        1.04     KP        1.03     LA        1.20     
!   NL        0.99     OV        1.04     PT        1.05     SC        0.96     
!   WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 6:
!   BR        1.01     FD        0.98     KP        1.04     LA        1.20     
!   MK        0.98     NL        1.05     OV        1.01     PT        1.09     
! 
!  Telescope amplitude corrections in sub-array 7:
!   FD        1.01     KP        1.07     LA        1.23     MK        1.01     
!   OV        0.98     PT        1.08     
! 
!  Telescope amplitude corrections in sub-array 8:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   HH        0.00*    WF        0.00*    WZ        0.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   FD        0.00*    HH        0.00*    HN        0.00*    SC        0.00*    
!   WF        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   FD        1.08     HH        1.00*    HN        1.14     LA        1.08     
!   NL        1.26     PT        1.06     SC        1.01     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   FD        1.06     HN        1.05     KP        1.04     LA        1.11     
!   NL        1.07     PT        1.05     SC        1.05     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   FD        1.07     HN        1.09     KP        1.03     LA        1.08     
!   NL        1.01     OV        1.05     PT        1.05     SC        1.06     
!   WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 6:
!   BR        1.04     FD        1.04     KP        1.02     LA        1.06     
!   MK        1.01     NL        1.08     OV        1.05     PT        1.04     
! 
!  Telescope amplitude corrections in sub-array 7:
!   FD        1.07     KP        1.06     LA        1.07     MK        1.02     
!   OV        1.04     PT        1.05     
! 
!  Telescope amplitude corrections in sub-array 8:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   HH        0.00*    WF        0.00*    WZ        0.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   FD        0.00*    HH        0.00*    HN        0.00*    SC        0.00*    
!   WF        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   FD        1.05     HH        1.00*    HN        1.09     LA        0.97     
!   NL        1.28     PT        1.08     SC        0.90     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   FD        1.05     HN        1.01     KP        0.89     LA        0.96     
!   NL        1.07     PT        1.05     SC        0.93     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   FD        1.06     HN        1.02     KP        0.88     LA        0.96     
!   NL        1.01     OV        1.03     PT        1.04     SC        0.93     
!   WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 6:
!   BR        1.02     FD        1.05     KP        0.88     LA        0.96     
!   MK        0.96     NL        1.11     OV        1.00     PT        1.03     
! 
!  Telescope amplitude corrections in sub-array 7:
!   FD        1.07     KP        0.91     LA        0.98     MK        1.00     
!   OV        1.01     PT        1.05     
! 
!  Telescope amplitude corrections in sub-array 8:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   HH        0.00*    WF        0.00*    WZ        0.00*    
! 
!  A total of 6 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   FD        0.00*    HH        0.00*    HN        0.00*    SC        0.00*    
!   WF        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   FD        1.07     HH        1.00*    HN        0.95     LA        0.82     
!   NL        1.21     PT        0.94     SC        0.90     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   FD        1.05     HN        0.89     KP        0.83     LA        0.83     
!   NL        0.98     PT        0.91     SC        0.95     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   FD        1.04     HN        0.91     KP        0.80     LA        0.79     
!   NL        0.93     OV        0.87     PT        0.92     SC        0.96     
!   WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 6:
!   BR        0.96     FD        1.02     KP        0.80     LA        0.80     
!   MK        1.06     NL        1.04     OV        0.85     PT        0.91     
! 
!  Telescope amplitude corrections in sub-array 7:
!   FD        1.07     KP        0.82     LA        0.82     MK        1.11     
!   OV        0.86     PT        0.91     
! 
!  Telescope amplitude corrections in sub-array 8:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
! 
! Fit before self-cal, rms=0.239421Jy  sigma=4.092885
! Fit after  self-cal, rms=0.083515Jy  sigma=1.106299
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=4.651 mas, bmaj=15.16 mas, bpa=-3.557 degrees
! Estimated noise=1.55401 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (-12.4, -7.6).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0114048 Jy
! Component: 100  -  total flux cleaned = 0.0122165 Jy
! Component: 150  -  total flux cleaned = 0.0119049 Jy
! Component: 200  -  total flux cleaned = 0.0119145 Jy
! Total flux subtracted in 200 components = 0.0119145 Jy
! Clean residual min=-0.008897 max=0.007577 Jy/beam
! Clean residual mean=-0.000232 rms=0.002137 Jy/beam
! Combined flux in latest and established models = 1.65094 Jy
! Performing phase self-cal
! Adding 32 model components to the UV plane model.
! The established model now contains 127 components and 1.65094 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.079193Jy  sigma=1.044684
! Fit after  self-cal, rms=0.078773Jy  sigma=1.038082
! Inverting map 
selfcal true, true, soltime1
! Performing amp+phase self-cal over 800000 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.078773Jy  sigma=1.038082
! Fit after  self-cal, rms=0.078408Jy  sigma=1.033675
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=4.648 mas, bmaj=15.17 mas, bpa=-3.5 degrees
! Estimated noise=1.55384 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00432624 Jy
! Component: 100  -  total flux cleaned = 0.00460001 Jy
! Component: 150  -  total flux cleaned = 0.00481064 Jy
! Component: 200  -  total flux cleaned = 0.00500118 Jy
! Total flux subtracted in 200 components = 0.00500118 Jy
! Clean residual min=-0.008308 max=0.006882 Jy/beam
! Clean residual mean=-0.000110 rms=0.001900 Jy/beam
! Combined flux in latest and established models = 1.65594 Jy
selfcal
! Performing phase self-cal
! Adding 47 model components to the UV plane model.
! The established model now contains 167 components and 1.65594 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.076576Jy  sigma=1.010299
! Fit after  self-cal, rms=0.076366Jy  sigma=1.008155
flux_cutoff = imstat(rms) * dynam
! Inverting map 
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00143768 Jy
! Component: 100  -  total flux cleaned = 0.00125712 Jy
! Component: 150  -  total flux cleaned = 0.00125647 Jy
! Component: 200  -  total flux cleaned = 0.00110711 Jy
! Total flux subtracted in 200 components = 0.00110711 Jy
! Clean residual min=-0.007910 max=0.006035 Jy/beam
! Clean residual mean=-0.000130 rms=0.001817 Jy/beam
! Combined flux in latest and established models = 1.65705 Jy
! Performing phase self-cal
! Adding 33 model components to the UV plane model.
! The established model now contains 188 components and 1.65705 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.075416Jy  sigma=0.998327
! Fit after  self-cal, rms=0.075306Jy  sigma=0.997437
! Inverting map 
selfcal true, true, soltime2
! Performing amp+phase self-cal over 15 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.075306Jy  sigma=0.997437
! Fit after  self-cal, rms=0.075047Jy  sigma=0.994767
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=4.648 mas, bmaj=15.18 mas, bpa=-3.464 degrees
! Estimated noise=1.5533 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000193615 Jy
! Component: 100  -  total flux cleaned = 0.000128654 Jy
! Component: 150  -  total flux cleaned = 0.00026828 Jy
! Component: 200  -  total flux cleaned = 0.000265729 Jy
! Total flux subtracted in 200 components = 0.000265729 Jy
! Clean residual min=-0.007443 max=0.005713 Jy/beam
! Clean residual mean=-0.000033 rms=0.001713 Jy/beam
! Combined flux in latest and established models = 1.65732 Jy
selfcal
! Performing phase self-cal
! Adding 41 model components to the UV plane model.
! The established model now contains 205 components and 1.65732 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.074309Jy  sigma=0.986058
! Fit after  self-cal, rms=0.074218Jy  sigma=0.985220
flux_cutoff = imstat(rms) * dynam
! Inverting map 
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000614112 Jy
! Component: 100  -  total flux cleaned = 0.000608501 Jy
! Component: 150  -  total flux cleaned = 0.000494558 Jy
! Component: 200  -  total flux cleaned = 0.000496386 Jy
! Total flux subtracted in 200 components = 0.000496386 Jy
! Clean residual min=-0.007359 max=0.005499 Jy/beam
! Clean residual mean=-0.000042 rms=0.001673 Jy/beam
! Combined flux in latest and established models = 1.65781 Jy
! Performing phase self-cal
! Adding 33 model components to the UV plane model.
! The established model now contains 217 components and 1.65781 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.073769Jy  sigma=0.980518
! Fit after  self-cal, rms=0.073715Jy  sigma=0.980055
! Inverting map 
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 20 mega-wavelengths.
win_mult = win_mult * 1.2
selfcal true, true, soltime2
! Performing amp+phase self-cal over 15 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.073715Jy  sigma=0.980055
! Fit after  self-cal, rms=0.073539Jy  sigma=0.978729
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=8.84 mas, bmaj=18.86 mas, bpa=0.3121 degrees
! Estimated noise=1.62511 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000662852 Jy
! Component: 100  -  total flux cleaned = -5.51179e-06 Jy
! Component: 150  -  total flux cleaned = 8.17361e-05 Jy
! Component: 200  -  total flux cleaned = 0.000161726 Jy
! Total flux subtracted in 200 components = 0.000161726 Jy
! Clean residual min=-0.005312 max=0.005050 Jy/beam
! Clean residual mean=-0.000050 rms=0.001682 Jy/beam
! Combined flux in latest and established models = 1.65797 Jy
selfcal
! Performing phase self-cal
! Adding 34 model components to the UV plane model.
! The established model now contains 244 components and 1.65798 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.073189Jy  sigma=0.975078
! Fit after  self-cal, rms=0.073133Jy  sigma=0.974621
flux_cutoff = imstat(rms) * dynam
! Inverting map 
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00041444 Jy
! Component: 100  -  total flux cleaned = 0.000570607 Jy
! Component: 150  -  total flux cleaned = 0.000640411 Jy
! Component: 200  -  total flux cleaned = 0.000641435 Jy
! Total flux subtracted in 200 components = 0.000641435 Jy
! Clean residual min=-0.005235 max=0.004988 Jy/beam
! Clean residual mean=-0.000068 rms=0.001670 Jy/beam
! Combined flux in latest and established models = 1.65862 Jy
! Performing phase self-cal
! Adding 22 model components to the UV plane model.
! The established model now contains 256 components and 1.65862 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.072926Jy  sigma=0.972677
! Fit after  self-cal, rms=0.072894Jy  sigma=0.972411
! Inverting map 
uvtaper 0,0
! No UV-taper is currently set.
win_mult = win_mult / 1.2
print "=== Finished amplitude self-cal for VLBA stations ==="
! === Finished amplitude self-cal for VLBA stations === 
unflag *
! Unflagging all baselines in the currently selected channels.
uncalib false, false, true
! uncal: All telescope correction flags have been un-done.
integer lun
lun = outfile ( "/tmp/ff.ff" )
do i=1,nsub
  do j=1,ntel(i)
    fprintf lun, "%s\n", telname(j,i)
    end do
  end do
close ( lun )
system "/home/lpetrov/bin/dimap_selfant_process.csh /tmp/ff.ff"
![@/tmp/ff.ff]
1:HH
! Syntax error in line:
! 1:HH
! ^
! Found constant: 1.000 
! Where a command or assignment expression was expected.
![Exited script file: /tmp/ff.ff]
![Exited script file: /home/lpetrov/bin/rdv_muppet]
! 
wmap "/scr/pima/rdv96_uvs/J2258-2758_S\_map.fits"
! Inverting map and beam 
! Estimated beam: bmin=3.158 mas, bmaj=6.463 mas, bpa=23.08 degrees
! Estimated noise=1.53391 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 3.158 x 6.463 at 23.08 degrees (North through East)
! Clean map  min=-0.043309  max=1.2613 Jy/beam
! Writing clean map to FITS file: /scr/pima/rdv96_uvs/J2258-2758_S_map.fits
float peak_flux
peak_flux = peak(flux,max)
invert
! Inverting map 
float image_peak
image_peak = int(10000*peak_flux)/10000
float image_rms
image_rms  = int(100000*imstat(rms))/100000
print "========================================="
! ========================================= 
print "The image peak= ", image_peak, " rms= ", image_rms, " Jy"
! The image peak=  1.2613  rms=  0.01398  Jy 
quit
! Quitting program
! Log file /scr/pima/rdv96_uvs/J2258-2758_S_uvs.log closed on Sat Dec 21 00:26:14 2013