! Started logfile: /scr/pima/rdv96_uvs/J1939-1525_S_uvs.log on Sat Dec 21 00:25:36 2013
obs /scr/pima/rdv96_uvs/J1939-1525_S_uva.fits
! Reading UV FITS file: /scr/pima/rdv96_uvs/J1939-1525_S_uva.fits
! AN table 1: 11 integrations on 55 of 55 possible baselines.
! AN table 2: 2 integrations on 28 of 28 possible baselines.
! AN table 3: 48 integrations on 3 of 3 possible baselines.
! AN table 4: 3 integrations on 3 of 3 possible baselines.
! AN table 5: 19 integrations on 6 of 6 possible baselines.
! AN table 6: 4 integrations on 15 of 15 possible baselines.
! AN table 7: 19 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.474227 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J1939-1525
! 
! 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 3496 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/J1939-1525_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:BR       self-cal  status=correctable  weight=1
! 1:FD       self-cal  status=correctable  weight=1
! 1:HH       self-cal  status=correctable  weight=1
! 1:HN       self-cal  status=correctable  weight=1
! 1:KP       self-cal  status=correctable  weight=1
! 1:LA       self-cal  status=correctable  weight=1
! 1:NL       self-cal  status=correctable  weight=1
! 1:OV       self-cal  status=correctable  weight=1
! 1:PT       self-cal  status=correctable  weight=1
! 1:SC       self-cal  status=correctable  weight=1
! 1:WF       self-cal  status=correctable  weight=1
! 2:BR       self-cal  status=correctable  weight=1
! 2:FD       self-cal  status=correctable  weight=1
! 2:KP       self-cal  status=correctable  weight=1
! 2:LA       self-cal  status=correctable  weight=1
! 2:MK       self-cal  status=correctable  weight=1
! 2:NL       self-cal  status=correctable  weight=1
! 2:OV       self-cal  status=correctable  weight=1
! 2:PT       self-cal  status=correctable  weight=1
! 3:HH       self-cal  status=correctable  weight=1
! 3:MA       self-cal  status=correctable  weight=1
! 3:WZ       self-cal  status=correctable  weight=1
! 4:HN       self-cal  status=correctable  weight=1
! 4:SC       self-cal  status=correctable  weight=1
! 4:WF       self-cal  status=correctable  weight=1
! 5:HH       self-cal  status=correctable  weight=1
! 5:MA       self-cal  status=correctable  weight=1
! 5:WF       self-cal  status=correctable  weight=1
! 5:WZ       self-cal  status=correctable  weight=1
! 6:FD       self-cal  status=correctable  weight=1
! 6:HN       self-cal  status=correctable  weight=1
! 6:LA       self-cal  status=correctable  weight=1
! 6:NL       self-cal  status=correctable  weight=1
! 6:SC       self-cal  status=correctable  weight=1
! 6:WF       self-cal  status=correctable  weight=1
! 7:FD       self-cal  status=correctable  weight=1
! 7:HH       self-cal  status=correctable  weight=1
! 7:HN       self-cal  status=correctable  weight=1
! 7:KP       self-cal  status=correctable  weight=1
! 7:LA       self-cal  status=correctable  weight=1
! 7:MA       self-cal  status=correctable  weight=1
! 7:NL       self-cal  status=correctable  weight=1
! 7:SC       self-cal  status=correctable  weight=1
! 7:WF       self-cal  status=correctable  weight=1
! 7: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 67 telescope corrections were flagged in sub-array 1.
!  A total of 144 telescope corrections were flagged in sub-array 3.
!  A total of 76 telescope corrections were flagged in sub-array 5.
!  A total of 125 telescope corrections were flagged in sub-array 7.
! 
! Correcting IF 2.
!  A total of 67 telescope corrections were flagged in sub-array 1.
!  A total of 144 telescope corrections were flagged in sub-array 3.
!  A total of 76 telescope corrections were flagged in sub-array 5.
!  A total of 125 telescope corrections were flagged in sub-array 7.
! 
! Correcting IF 3.
!  A total of 67 telescope corrections were flagged in sub-array 1.
!  A total of 144 telescope corrections were flagged in sub-array 3.
!  A total of 76 telescope corrections were flagged in sub-array 5.
!  A total of 125 telescope corrections were flagged in sub-array 7.
! 
! Correcting IF 4.
!  A total of 67 telescope corrections were flagged in sub-array 1.
!  A total of 144 telescope corrections were flagged in sub-array 3.
!  A total of 76 telescope corrections were flagged in sub-array 5.
!  A total of 125 telescope corrections were flagged in sub-array 7.
! 
! Fit before self-cal, rms=1.116991Jy  sigma=5.959113
! Fit after  self-cal, rms=0.522675Jy  sigma=2.500740
! 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 3:HH
! Flagging baselines of antenna 3:HH in the currently selected channels.
flag 3:MA
! Flagging baselines of antenna 3:MA in the currently selected channels.
flag 3:WZ
! Flagging baselines of antenna 3:WZ in the currently selected channels.
flag 4:WF
! Flagging baselines of antenna 4:WF in the currently selected channels.
flag 5:HH
! Flagging baselines of antenna 5:HH in the currently selected channels.
flag 5:MA
! Flagging baselines of antenna 5:MA in the currently selected channels.
flag 5:WF
! Flagging baselines of antenna 5:WF in the currently selected channels.
flag 5:WZ
! Flagging baselines of antenna 5:WZ in the currently selected channels.
flag 6:WF
! Flagging baselines of antenna 6:WF in the currently selected channels.
flag 7:HH
! Flagging baselines of antenna 7:HH in the currently selected channels.
flag 7:MA
! Flagging baselines of antenna 7:MA in the currently selected channels.
flag 7:WF
! Flagging baselines of antenna 7:WF in the currently selected channels.
flag 7:WZ
! Flagging baselines of antenna 7: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=4.083 mas, bmaj=9.683 mas, bpa=-6.2 degrees
! Estimated noise=3.81191 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 = 0.441271 Jy
! Component: 100  -  total flux cleaned = 0.537508 Jy
! Total flux subtracted in 100 components = 0.537508 Jy
! Clean residual min=-0.015528 max=0.026868 Jy/beam
! Clean residual mean=0.000022 rms=0.004599 Jy/beam
! Combined flux in latest and established models = 0.537508 Jy
! Performing phase self-cal
! Adding 2 model components to the UV plane model.
! The established model now contains 2 components and 0.537508 Jy
! 
! Correcting IF 1.
!  A total of 13 telescope corrections were flagged in sub-array 1.
!  A total of 9 telescope corrections were flagged in sub-array 4.
!  A total of 4 telescope corrections were flagged in sub-array 6.
!  A total of 20 telescope corrections were flagged in sub-array 7.
! 
! Correcting IF 2.
!  A total of 13 telescope corrections were flagged in sub-array 1.
!  A total of 9 telescope corrections were flagged in sub-array 4.
!  A total of 4 telescope corrections were flagged in sub-array 6.
!  A total of 20 telescope corrections were flagged in sub-array 7.
! 
! Correcting IF 3.
!  A total of 13 telescope corrections were flagged in sub-array 1.
!  A total of 9 telescope corrections were flagged in sub-array 4.
!  A total of 4 telescope corrections were flagged in sub-array 6.
!  A total of 20 telescope corrections were flagged in sub-array 7.
! 
! Correcting IF 4.
!  A total of 13 telescope corrections were flagged in sub-array 1.
!  A total of 9 telescope corrections were flagged in sub-array 4.
!  A total of 4 telescope corrections were flagged in sub-array 6.
!  A total of 20 telescope corrections were flagged in sub-array 7.
! 
! Fit before self-cal, rms=0.128148Jy  sigma=0.818437
! Fit after  self-cal, rms=0.127575Jy  sigma=0.818069
! Inverting map and beam 
! Estimated beam: bmin=4.072 mas, bmaj=9.768 mas, bpa=-6.061 degrees
! Estimated noise=3.81481 mJy/beam.
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0258095 Jy
! Component: 100  -  total flux cleaned = 0.0387074 Jy
! Total flux subtracted in 100 components = 0.0387074 Jy
! Clean residual min=-0.016804 max=0.016174 Jy/beam
! Clean residual mean=-0.000012 rms=0.004009 Jy/beam
! Combined flux in latest and established models = 0.576216 Jy
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 19 components and 0.576216 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.119547Jy  sigma=0.760067
! Fit after  self-cal, rms=0.119521Jy  sigma=0.759868
! 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=5.066 mas, bmaj=10.95 mas, bpa=-7.715 degrees
! Estimated noise=2.9037 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 = 0.0175965 Jy
! Component: 100  -  total flux cleaned = 0.0276468 Jy
! Component: 150  -  total flux cleaned = 0.0338561 Jy
! Component: 200  -  total flux cleaned = 0.0377225 Jy
! Total flux subtracted in 200 components = 0.0377225 Jy
! Clean residual min=-0.012767 max=0.015211 Jy/beam
! Clean residual mean=-0.000090 rms=0.003946 Jy/beam
! Combined flux in latest and established models = 0.613938 Jy
! Performing phase self-cal
! Adding 22 model components to the UV plane model.
! The established model now contains 38 components and 0.613938 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.116899Jy  sigma=0.741213
! Fit after  self-cal, rms=0.116885Jy  sigma=0.741059
! 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:
!   BR        1.11     FD        0.98     HH        1.00*    HN        0.97     
!   KP        1.02     LA        1.17     NL        0.99     OV        1.03     
!   PT        1.09     SC        0.98     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.02     FD        0.99     KP        1.01     LA        1.16     
!   MK        0.98     NL        1.01     OV        1.02     PT        1.07     
! 
!  Telescope amplitude corrections in sub-array 3:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   HN        0.00*    SC        0.00*    WF        0.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   HH        0.00*    MA        0.00*    WF        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 6:
!   FD        1.09     HN        1.06     LA        1.23     NL        1.01     
!   SC        0.89     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 7:
!   FD        0.93     HH        1.00*    HN        1.05     KP        0.89     
!   LA        1.06     MA        1.00*    NL        1.01     SC        0.96     
!   WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.09     FD        1.10     HH        1.00*    HN        1.08     
!   KP        1.04     LA        1.07     NL        1.01     OV        1.05     
!   PT        1.02     SC        1.05     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.03     FD        1.07     KP        1.07     LA        1.07     
!   MK        1.04     NL        1.08     OV        1.03     PT        1.04     
! 
!  Telescope amplitude corrections in sub-array 3:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   HN        0.00*    SC        0.00*    WF        0.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   HH        0.00*    MA        0.00*    WF        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 6:
!   FD        1.05     HN        1.15     LA        1.11     NL        1.07     
!   SC        1.04     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 7:
!   FD        1.06     HH        1.00*    HN        1.04     KP        1.01     
!   LA        1.05     MA        1.00*    NL        1.04     SC        1.00     
!   WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.21     FD        1.05     HH        1.00*    HN        0.99     
!   KP        0.92     LA        0.95     NL        1.07     OV        1.05     
!   PT        1.05     SC        0.96     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.04     FD        1.07     KP        0.90     LA        0.98     
!   MK        1.05     NL        1.07     OV        1.02     PT        1.05     
! 
!  Telescope amplitude corrections in sub-array 3:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   HN        0.00*    SC        0.00*    WF        0.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   HH        0.00*    MA        0.00*    WF        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 6:
!   FD        1.09     HN        1.07     LA        0.95     NL        1.05     
!   SC        0.90     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 7:
!   FD        1.07     HH        1.00*    HN        1.02     KP        0.87     
!   LA        0.94     MA        1.00*    NL        1.02     SC        0.91     
!   WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.04     FD        1.08     HH        1.00*    HN        0.88     
!   KP        0.82     LA        0.81     NL        1.01     OV        0.88     
!   PT        0.92     SC        1.02     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.01     FD        1.06     KP        0.84     LA        0.83     
!   MK        1.14     NL        1.01     OV        0.88     PT        0.94     
! 
!  Telescope amplitude corrections in sub-array 3:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   HN        0.00*    SC        0.00*    WF        0.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   HH        0.00*    MA        0.00*    WF        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 6:
!   FD        1.09     HN        0.97     LA        0.78     NL        1.05     
!   SC        0.97     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 7:
!   FD        1.05     HH        1.00*    HN        0.90     KP        0.81     
!   LA        0.81     MA        1.00*    NL        0.95     SC        0.99     
!   WF        1.00*    WZ        1.00*    
! 
! 
! Fit before self-cal, rms=0.116885Jy  sigma=0.741059
! Fit after  self-cal, rms=0.080499Jy  sigma=0.496974
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=5.064 mas, bmaj=10.96 mas, bpa=-7.789 degrees
! Estimated noise=2.89411 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 = 0.00175179 Jy
! Component: 100  -  total flux cleaned = 0.00167193 Jy
! Component: 150  -  total flux cleaned = 0.00160856 Jy
! Component: 200  -  total flux cleaned = 0.00160713 Jy
! Total flux subtracted in 200 components = 0.00160713 Jy
! Clean residual min=-0.004860 max=0.005057 Jy/beam
! Clean residual mean=-0.000016 rms=0.001295 Jy/beam
! Combined flux in latest and established models = 0.615545 Jy
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 50 components and 0.615545 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.080323Jy  sigma=0.495874
! Fit after  self-cal, rms=0.080416Jy  sigma=0.495627
! 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=0.080416Jy  sigma=0.495627
! Fit after  self-cal, rms=0.080446Jy  sigma=0.495472
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=5.057 mas, bmaj=10.95 mas, bpa=-7.802 degrees
! Estimated noise=2.89627 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000935332 Jy
! Component: 100  -  total flux cleaned = 0.00105567 Jy
! Component: 150  -  total flux cleaned = 0.00105708 Jy
! Component: 200  -  total flux cleaned = 0.00101737 Jy
! Total flux subtracted in 200 components = 0.00101737 Jy
! Clean residual min=-0.004826 max=0.004763 Jy/beam
! Clean residual mean=-0.000012 rms=0.001272 Jy/beam
! Combined flux in latest and established models = 0.616563 Jy
selfcal
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 54 components and 0.616563 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.080370Jy  sigma=0.495017
! Fit after  self-cal, rms=0.080363Jy  sigma=0.494990
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 = -0.000155472 Jy
! Component: 100  -  total flux cleaned = -0.000152117 Jy
! Component: 150  -  total flux cleaned = -0.000182987 Jy
! Component: 200  -  total flux cleaned = -0.000181906 Jy
! Total flux subtracted in 200 components = -0.000181906 Jy
! Clean residual min=-0.004816 max=0.004691 Jy/beam
! Clean residual mean=-0.000012 rms=0.001264 Jy/beam
! Combined flux in latest and established models = 0.616381 Jy
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 61 components and 0.616381 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.080332Jy  sigma=0.494809
! Fit after  self-cal, rms=0.080326Jy  sigma=0.494790
! 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=0.080326Jy  sigma=0.494790
! Fit after  self-cal, rms=0.080349Jy  sigma=0.494723
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=5.053 mas, bmaj=10.95 mas, bpa=-7.803 degrees
! Estimated noise=2.89754 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000421281 Jy
! Component: 100  -  total flux cleaned = 0.000494377 Jy
! Component: 150  -  total flux cleaned = 0.00049741 Jy
! Component: 200  -  total flux cleaned = 0.000497387 Jy
! Total flux subtracted in 200 components = 0.000497387 Jy
! Clean residual min=-0.004765 max=0.004451 Jy/beam
! Clean residual mean=-0.000008 rms=0.001255 Jy/beam
! Combined flux in latest and established models = 0.616878 Jy
selfcal
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 65 components and 0.616878 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.080321Jy  sigma=0.494564
! Fit after  self-cal, rms=0.080316Jy  sigma=0.494548
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 = -0.000102294 Jy
! Component: 100  -  total flux cleaned = -5.56825e-05 Jy
! Component: 150  -  total flux cleaned = -5.63961e-05 Jy
! Component: 200  -  total flux cleaned = -5.67461e-05 Jy
! Total flux subtracted in 200 components = -5.67461e-05 Jy
! Clean residual min=-0.004740 max=0.004409 Jy/beam
! Clean residual mean=-0.000008 rms=0.001251 Jy/beam
! Combined flux in latest and established models = 0.616821 Jy
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 69 components and 0.616821 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.080303Jy  sigma=0.494469
! Fit after  self-cal, rms=0.080299Jy  sigma=0.494459
! 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=0.080299Jy  sigma=0.494459
! Fit after  self-cal, rms=0.080304Jy  sigma=0.494440
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=8.032 mas, bmaj=13.33 mas, bpa=-12.29 degrees
! Estimated noise=3.19779 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000245386 Jy
! Component: 100  -  total flux cleaned = 0.000328299 Jy
! Component: 150  -  total flux cleaned = 0.000382177 Jy
! Component: 200  -  total flux cleaned = 0.000445417 Jy
! Total flux subtracted in 200 components = 0.000445417 Jy
! Clean residual min=-0.005070 max=0.004915 Jy/beam
! Clean residual mean=-0.000008 rms=0.001459 Jy/beam
! Combined flux in latest and established models = 0.617267 Jy
selfcal
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 80 components and 0.617267 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.080298Jy  sigma=0.494441
! Fit after  self-cal, rms=0.080297Jy  sigma=0.494433
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 = 4.11886e-05 Jy
! Component: 100  -  total flux cleaned = 6.93849e-05 Jy
! Component: 150  -  total flux cleaned = 8.07464e-05 Jy
! Component: 200  -  total flux cleaned = 0.000104075 Jy
! Total flux subtracted in 200 components = 0.000104075 Jy
! Clean residual min=-0.005068 max=0.004790 Jy/beam
! Clean residual mean=-0.000008 rms=0.001457 Jy/beam
! Combined flux in latest and established models = 0.617371 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 84 components and 0.617371 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.080295Jy  sigma=0.494429
! Fit after  self-cal, rms=0.080295Jy  sigma=0.494426
! 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:BR
! Syntax error in line:
! 1:BR
! ^
! 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/J1939-1525_S\_map.fits"
! Inverting map and beam 
! Estimated beam: bmin=3.17 mas, bmaj=5.19 mas, bpa=16.37 degrees
! Estimated noise=2.94002 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 3.17 x 5.19 at 16.37 degrees (North through East)
! Clean map  min=-0.029539  max=0.51546 Jy/beam
! Writing clean map to FITS file: /scr/pima/rdv96_uvs/J1939-1525_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=  0.5154  rms=  0.00478  Jy 
quit
! Quitting program
! Log file /scr/pima/rdv96_uvs/J1939-1525_S_uvs.log closed on Sat Dec 21 00:25:38 2013