! Started logfile: /scr/pima/rdv96_uvs/J2337-0230_S_uvs.log on Sat Dec 21 00:26:18 2013
obs /scr/pima/rdv96_uvs/J2337-0230_S_uva.fits
! Reading UV FITS file: /scr/pima/rdv96_uvs/J2337-0230_S_uva.fits
! AN table 1: 7 integrations on 3 of 3 possible baselines.
! AN table 2: 33 integrations on 6 of 6 possible baselines.
! AN table 3: 3 integrations on 36 of 36 possible baselines.
! AN table 4: 5 integrations on 55 of 55 possible baselines.
! AN table 5: 60 integrations on 3 of 3 possible baselines.
! AN table 6: 15 integrations on 6 of 6 possible baselines.
! Apparent sampling: 0.676606 visibilities/baseline/integration-bin.
! Found source: J2337-0230
! 
! 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 2360 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/J2337-0230_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:HN       self-cal  status=correctable  weight=1
! 1:WZ       self-cal  status=correctable  weight=1
! 2:HH       self-cal  status=correctable  weight=1
! 2:NY       self-cal  status=correctable  weight=1
! 2:WF       self-cal  status=correctable  weight=1
! 2:WZ       self-cal  status=correctable  weight=1
! 3:BR       self-cal  status=correctable  weight=1
! 3:FD       self-cal  status=correctable  weight=1
! 3:HN       self-cal  status=correctable  weight=1
! 3:KP       self-cal  status=correctable  weight=1
! 3:LA       self-cal  status=correctable  weight=1
! 3:NL       self-cal  status=correctable  weight=1
! 3:OV       self-cal  status=correctable  weight=1
! 3:PT       self-cal  status=correctable  weight=1
! 3:WZ       self-cal  status=correctable  weight=1
! 4:BR       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:MK       self-cal  status=correctable  weight=1
! 4:NL       self-cal  status=correctable  weight=1
! 4:OV       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:HH       self-cal  status=correctable  weight=1
! 5:MA       self-cal  status=correctable  weight=1
! 5:WZ       self-cal  status=correctable  weight=1
! 6:HH       self-cal  status=correctable  weight=1
! 6:MA       self-cal  status=correctable  weight=1
! 6:SC       self-cal  status=correctable  weight=1
! 6: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 44 telescope corrections were flagged in sub-array 2.
!  A total of 22 telescope corrections were flagged in sub-array 4.
!  A total of 180 telescope corrections were flagged in sub-array 5.
!  A total of 60 telescope corrections were flagged in sub-array 6.
! 
! Correcting IF 2.
!  A total of 44 telescope corrections were flagged in sub-array 2.
!  A total of 22 telescope corrections were flagged in sub-array 4.
!  A total of 180 telescope corrections were flagged in sub-array 5.
!  A total of 60 telescope corrections were flagged in sub-array 6.
! 
! Correcting IF 3.
!  A total of 44 telescope corrections were flagged in sub-array 2.
!  A total of 22 telescope corrections were flagged in sub-array 4.
!  A total of 180 telescope corrections were flagged in sub-array 5.
!  A total of 60 telescope corrections were flagged in sub-array 6.
! 
! Correcting IF 4.
!  A total of 44 telescope corrections were flagged in sub-array 2.
!  A total of 22 telescope corrections were flagged in sub-array 4.
!  A total of 180 telescope corrections were flagged in sub-array 5.
!  A total of 60 telescope corrections were flagged in sub-array 6.
! 
! Fit before self-cal, rms=1.081740Jy  sigma=5.814337
! Fit after  self-cal, rms=0.599991Jy  sigma=2.799367
! 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: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:NY
! Flagging baselines of antenna 2:NY in the currently selected channels.
flag 2:WF
! Flagging baselines of antenna 2:WF in the currently selected channels.
flag 2:WZ
! Flagging baselines of antenna 2:WZ 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:WZ
! Flagging baselines of antenna 5:WZ in the currently selected channels.
flag 6:HH
! Flagging baselines of antenna 6:HH in the currently selected channels.
flag 6:MA
! Flagging baselines of antenna 6:MA in the currently selected channels.
flag 6:WZ
! Flagging baselines of antenna 6: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=3.312 mas, bmaj=7.861 mas, bpa=-1.578 degrees
! Estimated noise=4.138 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 = 0.38654 Jy
! Component: 100  -  total flux cleaned = 0.474616 Jy
! Total flux subtracted in 100 components = 0.474616 Jy
! Clean residual min=-0.015445 max=0.030909 Jy/beam
! Clean residual mean=0.000061 rms=0.005292 Jy/beam
! Combined flux in latest and established models = 0.474616 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 9 components and 0.474616 Jy
! 
! Correcting IF 1.
!  A total of 21 telescope corrections were flagged in sub-array 1.
!  A total of 88 telescope corrections were flagged in sub-array 2.
!  A total of 3 telescope corrections were flagged in sub-array 3.
!  A total of 3 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 2.
!  A total of 21 telescope corrections were flagged in sub-array 1.
!  A total of 88 telescope corrections were flagged in sub-array 2.
!  A total of 3 telescope corrections were flagged in sub-array 3.
!  A total of 3 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 3.
!  A total of 21 telescope corrections were flagged in sub-array 1.
!  A total of 88 telescope corrections were flagged in sub-array 2.
!  A total of 3 telescope corrections were flagged in sub-array 3.
!  A total of 3 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 4.
!  A total of 21 telescope corrections were flagged in sub-array 1.
!  A total of 88 telescope corrections were flagged in sub-array 2.
!  A total of 3 telescope corrections were flagged in sub-array 3.
!  A total of 3 telescope corrections were flagged in sub-array 4.
! 
! Fit before self-cal, rms=0.106049Jy  sigma=0.811089
! Fit after  self-cal, rms=0.106072Jy  sigma=0.810915
! Inverting map and beam 
! Estimated beam: bmin=3.312 mas, bmaj=7.861 mas, bpa=-1.578 degrees
! Estimated noise=4.138 mJy/beam.
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=4.05 mas, bmaj=9.259 mas, bpa=-3.567 degrees
! Estimated noise=3.43228 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 = 0.0424036 Jy
! Component: 100  -  total flux cleaned = 0.0632777 Jy
! Component: 150  -  total flux cleaned = 0.0750675 Jy
! Component: 200  -  total flux cleaned = 0.0819954 Jy
! Total flux subtracted in 200 components = 0.0819954 Jy
! Clean residual min=-0.013050 max=0.020717 Jy/beam
! Clean residual mean=-0.000104 rms=0.003888 Jy/beam
! Combined flux in latest and established models = 0.556611 Jy
! Performing phase self-cal
! Adding 39 model components to the UV plane model.
! The established model now contains 44 components and 0.556611 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.092076Jy  sigma=0.670987
! Fit after  self-cal, rms=0.091768Jy  sigma=0.669148
! 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*    HN        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   HH        0.00*    NY        0.00*    WF        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.05     FD        1.00     HN        1.03     KP        1.01     
!   LA        1.18     NL        1.04     OV        0.99     PT        1.02     
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.02     FD        0.93     HN        1.03     KP        1.00     
!   LA        1.19     MK        0.97     NL        1.03     OV        0.97     
!   PT        1.06     SC        0.98     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 6:
!   HH        0.00*    MA        0.00*    SC        0.00*    WZ        0.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   HH        0.00*    HN        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   HH        0.00*    NY        0.00*    WF        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.04     FD        1.03     HN        1.07     KP        1.03     
!   LA        1.05     NL        1.07     OV        1.02     PT        0.98     
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.07     FD        1.02     HN        1.04     KP        1.01     
!   LA        1.08     MK        1.03     NL        1.06     OV        1.00     
!   PT        0.99     SC        1.08     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 6:
!   HH        0.00*    MA        0.00*    SC        0.00*    WZ        0.00*    
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   HH        0.00*    HN        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   HH        0.00*    NY        0.00*    WF        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.02     FD        1.06     HN        1.05     KP        0.91     
!   LA        0.99     NL        1.10     OV        1.09     PT        1.02     
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.07     FD        1.02     HN        1.03     KP        0.89     
!   LA        1.03     MK        1.03     NL        1.12     OV        1.00     
!   PT        1.04     SC        0.96     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 6:
!   HH        0.00*    MA        0.00*    SC        0.00*    WZ        0.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   HH        0.00*    HN        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   HH        0.00*    NY        0.00*    WF        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.03     FD        1.07     HN        0.92     KP        0.83     
!   LA        0.81     NL        1.00     OV        0.86     PT        0.93     
!   WZ        1.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.01     FD        0.95     HN        0.92     KP        0.81     
!   LA        0.86     MK        1.16     NL        1.06     OV        0.87     
!   PT        0.91     SC        1.03     WF        1.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   HH        0.00*    MA        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 6:
!   HH        0.00*    MA        0.00*    SC        0.00*    WZ        0.00*    
! 
! 
! Fit before self-cal, rms=0.091768Jy  sigma=0.669148
! Fit after  self-cal, rms=0.064370Jy  sigma=0.438708
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=4.077 mas, bmaj=9.359 mas, bpa=-3.374 degrees
! Estimated noise=3.42755 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 (16, 20.8).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0145446 Jy
! Component: 100  -  total flux cleaned = 0.0226087 Jy
! Component: 150  -  total flux cleaned = 0.0275874 Jy
! Component: 200  -  total flux cleaned = 0.029396 Jy
! Total flux subtracted in 200 components = 0.029396 Jy
! Clean residual min=-0.005403 max=0.007062 Jy/beam
! Clean residual mean=-0.000036 rms=0.001638 Jy/beam
! Combined flux in latest and established models = 0.586007 Jy
! Performing phase self-cal
! Adding 36 model components to the UV plane model.
! The established model now contains 80 components and 0.586007 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.061074Jy  sigma=0.410742
! Fit after  self-cal, rms=0.060960Jy  sigma=0.409518
! 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=0.060960Jy  sigma=0.409518
! Fit after  self-cal, rms=0.060847Jy  sigma=0.408416
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=4.081 mas, bmaj=9.364 mas, bpa=-3.346 degrees
! Estimated noise=3.42244 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00160477 Jy
! Component: 100  -  total flux cleaned = 0.00223343 Jy
! Component: 150  -  total flux cleaned = 0.00233473 Jy
! Component: 200  -  total flux cleaned = 0.00242663 Jy
! Total flux subtracted in 200 components = 0.00242663 Jy
! Clean residual min=-0.004653 max=0.006204 Jy/beam
! Clean residual mean=-0.000028 rms=0.001476 Jy/beam
! Combined flux in latest and established models = 0.588434 Jy
selfcal
! Performing phase self-cal
! Adding 26 model components to the UV plane model.
! The established model now contains 97 components and 0.588434 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.060389Jy  sigma=0.405039
! Fit after  self-cal, rms=0.060350Jy  sigma=0.404755
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)
! Added new window around map position (6, 8.4).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0051523 Jy
! Component: 100  -  total flux cleaned = 0.00567929 Jy
! Component: 150  -  total flux cleaned = 0.00536364 Jy
! Component: 200  -  total flux cleaned = 0.00498449 Jy
! Total flux subtracted in 200 components = 0.00498449 Jy
! Clean residual min=-0.004729 max=0.005210 Jy/beam
! Clean residual mean=-0.000026 rms=0.001334 Jy/beam
! Combined flux in latest and established models = 0.593418 Jy
! Performing phase self-cal
! Adding 31 model components to the UV plane model.
! The established model now contains 127 components and 0.593418 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.059599Jy  sigma=0.400531
! Fit after  self-cal, rms=0.059523Jy  sigma=0.400129
! 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=0.059523Jy  sigma=0.400129
! Fit after  self-cal, rms=0.059436Jy  sigma=0.399522
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=4.082 mas, bmaj=9.353 mas, bpa=-3.262 degrees
! Estimated noise=3.42077 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00241682 Jy
! Component: 100  -  total flux cleaned = 0.00215366 Jy
! Component: 150  -  total flux cleaned = 0.00174856 Jy
! Component: 200  -  total flux cleaned = 0.00145441 Jy
! Total flux subtracted in 200 components = 0.00145441 Jy
! Clean residual min=-0.004709 max=0.005184 Jy/beam
! Clean residual mean=-0.000023 rms=0.001245 Jy/beam
! Combined flux in latest and established models = 0.594873 Jy
selfcal
! Performing phase self-cal
! Adding 36 model components to the UV plane model.
! The established model now contains 153 components and 0.594873 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.059093Jy  sigma=0.397722
! Fit after  self-cal, rms=0.059053Jy  sigma=0.397529
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)
! Added new window around map position (78.8, -61.2).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00393233 Jy
! Component: 100  -  total flux cleaned = 0.00430801 Jy
! Component: 150  -  total flux cleaned = 0.00438962 Jy
! Component: 200  -  total flux cleaned = 0.00446214 Jy
! Total flux subtracted in 200 components = 0.00446214 Jy
! Clean residual min=-0.004551 max=0.004708 Jy/beam
! Clean residual mean=-0.000015 rms=0.001153 Jy/beam
! Combined flux in latest and established models = 0.599335 Jy
! Performing phase self-cal
! Adding 25 model components to the UV plane model.
! The established model now contains 170 components and 0.599335 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.058625Jy  sigma=0.394766
! Fit after  self-cal, rms=0.058606Jy  sigma=0.394665
! 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=0.058606Jy  sigma=0.394665
! Fit after  self-cal, rms=0.058576Jy  sigma=0.394388
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=8.44 mas, bmaj=14.61 mas, bpa=-14.67 degrees
! Estimated noise=3.79592 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 8.11421e-05 Jy
! Component: 100  -  total flux cleaned = -0.000474214 Jy
! Component: 150  -  total flux cleaned = -0.000666572 Jy
! Component: 200  -  total flux cleaned = -0.000835212 Jy
! Total flux subtracted in 200 components = -0.000835212 Jy
! Clean residual min=-0.003810 max=0.004367 Jy/beam
! Clean residual mean=-0.000019 rms=0.001196 Jy/beam
! Combined flux in latest and established models = 0.5985 Jy
selfcal
! Performing phase self-cal
! Adding 24 model components to the UV plane model.
! The established model now contains 193 components and 0.5985 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.058519Jy  sigma=0.393523
! Fit after  self-cal, rms=0.058492Jy  sigma=0.393389
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 = 0.000215961 Jy
! Component: 100  -  total flux cleaned = 8.03497e-07 Jy
! Component: 150  -  total flux cleaned = -9.61804e-05 Jy
! Component: 200  -  total flux cleaned = -0.000224815 Jy
! Total flux subtracted in 200 components = -0.000224815 Jy
! Clean residual min=-0.003832 max=0.004235 Jy/beam
! Clean residual mean=-0.000019 rms=0.001158 Jy/beam
! Combined flux in latest and established models = 0.598275 Jy
! Performing phase self-cal
! Adding 28 model components to the UV plane model.
! The established model now contains 210 components and 0.598275 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.058472Jy  sigma=0.393009
! Fit after  self-cal, rms=0.058457Jy  sigma=0.392946
! 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/J2337-0230_S\_map.fits"
! Inverting map and beam 
! Estimated beam: bmin=2.704 mas, bmaj=3.591 mas, bpa=36.69 degrees
! Estimated noise=3.62537 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 2.704 x 3.591 at 36.69 degrees (North through East)
! Clean map  min=-0.029346  max=0.43621 Jy/beam
! Writing clean map to FITS file: /scr/pima/rdv96_uvs/J2337-0230_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=  0.4362  rms=  0.00538  Jy 
quit
! Quitting program
! Log file /scr/pima/rdv96_uvs/J2337-0230_S_uvs.log closed on Sat Dec 21 00:26:21 2013