! Started logfile: /d2/scr/pima/rdv96_uvs/J2101+0341_X_uvs.log on Fri Dec 20 23:46:50 2013
obs /d2/scr/pima/rdv96_uvs/J2101+0341_X_uva.fits
! Reading UV FITS file: /d2/scr/pima/rdv96_uvs/J2101+0341_X_uva.fits
! AN table 1: 8 integrations on 45 of 45 possible baselines.
! AN table 2: 2 integrations on 55 of 55 possible baselines.
! AN table 3: 32 integrations on 6 of 6 possible baselines.
! AN table 4: 2 integrations on 1 of 1 possible baselines.
! AN table 5: 9 integrations on 15 of 15 possible baselines.
! AN table 6: 9 integrations on 28 of 28 possible baselines.
! AN table 7: 18 integrations on 55 of 55 possible baselines.
! Apparent sampling: 0.836355 visibilities/baseline/integration-bin.
! Found source: J2101+0341
! 
! 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  8.40599e+09        8e+06          1        8e+06
!  02        2  8.47599e+09        8e+06          1        8e+06
!  03        3  8.79099e+09        8e+06          1        8e+06
!  04        4  8.89599e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 0 lines of history.
! 
! Reading 6828 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 = 0.2 
print "taper_size =",taper_size
! taper_size = 70 
![@/home/lpetrov/bin/rdv_muppet /d2/scr/pima/rdv96_uvs/J2101+0341_X]
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: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:NY       self-cal  status=correctable  weight=1
! 1:PT       self-cal  status=correctable  weight=1
! 1:WF       self-cal  status=correctable  weight=1
! 1:WZ       self-cal  status=correctable  weight=1
! 2:BR       self-cal  status=correctable  weight=1
! 2:FD       self-cal  status=correctable  weight=1
! 2:HN       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
! 2:SC       self-cal  status=correctable  weight=1
! 2:WF       self-cal  status=correctable  weight=1
! 3:HH       self-cal  status=correctable  weight=1
! 3:MA       self-cal  status=correctable  weight=1
! 3:NY       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
! 5:HH       self-cal  status=correctable  weight=1
! 5:HN       self-cal  status=correctable  weight=1
! 5:MA       self-cal  status=correctable  weight=1
! 5:SC       self-cal  status=correctable  weight=1
! 5:WF       self-cal  status=correctable  weight=1
! 5:WZ       self-cal  status=correctable  weight=1
! 6:HH       self-cal  status=correctable  weight=1
! 6:HN       self-cal  status=correctable  weight=1
! 6:MA       self-cal  status=correctable  weight=1
! 6:NL       self-cal  status=correctable  weight=1
! 6:NY       self-cal  status=correctable  weight=1
! 6:SC       self-cal  status=correctable  weight=1
! 6:WF       self-cal  status=correctable  weight=1
! 6:WZ       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:PT       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 0.200x0.200 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 20 telescope corrections were flagged in sub-array 1.
!  A total of 4 telescope corrections were flagged in sub-array 3.
!  A total of 4 telescope corrections were flagged in sub-array 4.
!  A total of 13 telescope corrections were flagged in sub-array 5.
!  A total of 18 telescope corrections were flagged in sub-array 6.
!  A total of 4 telescope corrections were flagged in sub-array 7.
! 
! Correcting IF 2.
!  A total of 20 telescope corrections were flagged in sub-array 1.
!  A total of 4 telescope corrections were flagged in sub-array 3.
!  A total of 4 telescope corrections were flagged in sub-array 4.
!  A total of 13 telescope corrections were flagged in sub-array 5.
!  A total of 18 telescope corrections were flagged in sub-array 6.
!  A total of 4 telescope corrections were flagged in sub-array 7.
! 
! Correcting IF 3.
!  A total of 32 telescope corrections were flagged in sub-array 1.
!  A total of 44 telescope corrections were flagged in sub-array 3.
!  A total of 4 telescope corrections were flagged in sub-array 4.
!  A total of 13 telescope corrections were flagged in sub-array 5.
!  A total of 26 telescope corrections were flagged in sub-array 6.
!  A total of 4 telescope corrections were flagged in sub-array 7.
! 
! Correcting IF 4.
!  A total of 32 telescope corrections were flagged in sub-array 1.
!  A total of 44 telescope corrections were flagged in sub-array 3.
!  A total of 4 telescope corrections were flagged in sub-array 4.
!  A total of 13 telescope corrections were flagged in sub-array 5.
!  A total of 26 telescope corrections were flagged in sub-array 6.
!  A total of 4 telescope corrections were flagged in sub-array 7.
! 
! Fit before self-cal, rms=1.248783Jy  sigma=8.432418
! Fit after  self-cal, rms=0.422041Jy  sigma=1.783006
! 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 \]
![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 
! Your choice of large map pixels excluded 8.66% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
! Estimated beam: bmin=0.5981 mas, bmaj=0.9996 mas, bpa=8.47 degrees
! Estimated noise=2.24446 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 = 0.554445 Jy
! Component: 100  -  total flux cleaned = 0.711839 Jy
! Total flux subtracted in 100 components = 0.711839 Jy
! Clean residual min=-0.025875 max=0.063224 Jy/beam
! Clean residual mean=0.000351 rms=0.005686 Jy/beam
! Combined flux in latest and established models = 0.711839 Jy
! Performing phase self-cal
! Adding 5 model components to the UV plane model.
! The established model now contains 5 components and 0.711839 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.236115Jy  sigma=1.180583
! Fit after  self-cal, rms=0.235717Jy  sigma=1.179528
! Inverting map 
! Your choice of large map pixels excluded 8.66% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0648713 Jy
! Component: 100  -  total flux cleaned = 0.0939149 Jy
! Total flux subtracted in 100 components = 0.0939149 Jy
! Clean residual min=-0.020877 max=0.041113 Jy/beam
! Clean residual mean=0.000207 rms=0.004144 Jy/beam
! Combined flux in latest and established models = 0.805754 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 12 components and 0.805754 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.219840Jy  sigma=0.938106
! Fit after  self-cal, rms=0.219551Jy  sigma=0.937127
! Inverting map 
! Your choice of large map pixels excluded 8.66% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
! Added new window around map position (1, -3).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0240204 Jy
! Component: 100  -  total flux cleaned = 0.0258302 Jy
! Total flux subtracted in 100 components = 0.0258302 Jy
! Clean residual min=-0.022882 max=0.032605 Jy/beam
! Clean residual mean=0.000168 rms=0.003903 Jy/beam
! Combined flux in latest and established models = 0.831584 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 20 components and 0.831584 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.206477Jy  sigma=0.882287
! Fit after  self-cal, rms=0.206022Jy  sigma=0.876425
! Inverting map 
! Your choice of large map pixels excluded 8.66% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
! Added new window around map position (0.2, 2.2).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0239433 Jy
! Component: 100  -  total flux cleaned = 0.0232161 Jy
! Total flux subtracted in 100 components = 0.0232161 Jy
! Clean residual min=-0.020586 max=0.028240 Jy/beam
! Clean residual mean=0.000133 rms=0.003726 Jy/beam
! Combined flux in latest and established models = 0.8548 Jy
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 24 components and 0.8548 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.197968Jy  sigma=0.847762
! Fit after  self-cal, rms=0.197766Jy  sigma=0.846290
! Inverting map 
! Your choice of large map pixels excluded 8.66% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
! Added new window around map position (0.4, 5.2).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0228451 Jy
! Component: 100  -  total flux cleaned = 0.0255334 Jy
! Total flux subtracted in 100 components = 0.0255334 Jy
! Clean residual min=-0.019364 max=0.022736 Jy/beam
! Clean residual mean=0.000096 rms=0.003573 Jy/beam
! Combined flux in latest and established models = 0.880333 Jy
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 27 components and 0.880333 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.191096Jy  sigma=0.819315
! Fit after  self-cal, rms=0.191005Jy  sigma=0.818360
! Inverting map 
! Your choice of large map pixels excluded 8.66% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
! Added new window around map position (-0.2, -6.4).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0157676 Jy
! Component: 100  -  total flux cleaned = 0.0163591 Jy
! Total flux subtracted in 100 components = 0.0163591 Jy
! Clean residual min=-0.018060 max=0.020419 Jy/beam
! Clean residual mean=0.000073 rms=0.003464 Jy/beam
! Combined flux in latest and established models = 0.896693 Jy
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 31 components and 0.896692 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.186084Jy  sigma=0.807629
! Fit after  self-cal, rms=0.186038Jy  sigma=0.807111
! Inverting map 
! Your choice of large map pixels excluded 8.66% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
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 
! Your choice of large map pixels excluded 8.66% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
! Estimated beam: bmin=0.6423 mas, bmaj=1.078 mas, bpa=13.5 degrees
! Estimated noise=1.56083 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 (-1, 3).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0308259 Jy
! Component: 100  -  total flux cleaned = 0.03655 Jy
! Component: 150  -  total flux cleaned = 0.0393356 Jy
! Component: 200  -  total flux cleaned = 0.0411616 Jy
! Total flux subtracted in 200 components = 0.0411616 Jy
! Clean residual min=-0.020883 max=0.023253 Jy/beam
! Clean residual mean=0.001453 rms=0.004121 Jy/beam
! Combined flux in latest and established models = 0.937854 Jy
! Performing phase self-cal
! Adding 22 model components to the UV plane model.
! The established model now contains 46 components and 0.937854 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.171908Jy  sigma=0.785786
! Fit after  self-cal, rms=0.171727Jy  sigma=0.784559
! Inverting map 
! Your choice of large map pixels excluded 8.66% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
! Added new window around map position (-0.4, -16.2).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0124914 Jy
! Component: 100  -  total flux cleaned = 0.0178168 Jy
! Component: 150  -  total flux cleaned = 0.0205926 Jy
! Component: 200  -  total flux cleaned = 0.0226967 Jy
! Total flux subtracted in 200 components = 0.0226967 Jy
! Clean residual min=-0.020754 max=0.021204 Jy/beam
! Clean residual mean=0.001132 rms=0.003996 Jy/beam
! Combined flux in latest and established models = 0.960551 Jy
! Performing phase self-cal
! Adding 26 model components to the UV plane model.
! The established model now contains 57 components and 0.960551 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.164918Jy  sigma=0.776215
! Fit after  self-cal, rms=0.164728Jy  sigma=0.774477
! Inverting map 
! Your choice of large map pixels excluded 8.66% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
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.
!  A total of 6 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   FD        0.96     HH        0.99     HN        1.09     KP        1.01     
!   LA        1.06     NL        0.96     NY        0.79     PT        1.00     
!   WF        0.87     WZ        2.31     
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.92     FD        0.96     HN        1.06     KP        1.05     
!   LA        1.05     MK        1.02     NL        0.94     OV        0.95     
!   PT        0.99     SC        1.01     WF        0.89     
! 
!  A total of 12 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   HH        0.81     MA        1.10     NY        0.88     WZ        2.52     
! 
!  Telescope amplitude corrections in sub-array 4:
!   HN        0.00*    SC        0.00*    
! 
!  A total of 9 telescope corrections were flagged in sub-array 5.
!  Telescope amplitude corrections in sub-array 5:
!   HH        0.93     HN        1.06     MA        0.96     SC        1.00     
!   WF        0.92     WZ        1.90     
! 
!  A total of 3 telescope corrections were flagged in sub-array 6.
!  Telescope amplitude corrections in sub-array 6:
!   HH        0.90     HN        1.04     MA        0.99     NL        1.18     
!   NY        0.97     SC        1.08     WF        0.87     WZ        1.98     
! 
!  Telescope amplitude corrections in sub-array 7:
!   FD        0.96     HH        0.94     HN        1.01     KP        1.05     
!   LA        1.04     MA        0.93     NL        0.99     PT        1.02     
!   SC        0.97     WF        0.85     WZ        1.53     
! 
! 
! Correcting IF 2.
!  A total of 6 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   FD        0.94     HH        1.06     HN        1.13     KP        0.98     
!   LA        1.03     NL        0.97     NY        0.75     PT        1.01     
!   WF        0.86     WZ        2.54     
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.92     FD        0.98     HN        1.06     KP        0.99     
!   LA        1.03     MK        1.05     NL        0.95     OV        0.94     
!   PT        0.99     SC        1.02     WF        0.90     
! 
!  A total of 12 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   HH        0.81     MA        1.04     NY        0.91     WZ        2.43     
! 
!  Telescope amplitude corrections in sub-array 4:
!   HN        0.00*    SC        0.00*    
! 
!  A total of 9 telescope corrections were flagged in sub-array 5.
!  Telescope amplitude corrections in sub-array 5:
!   HH        1.02     HN        1.07     MA        0.93     SC        0.99     
!   WF        0.94     WZ        1.85     
! 
!  A total of 3 telescope corrections were flagged in sub-array 6.
!  Telescope amplitude corrections in sub-array 6:
!   HH        0.95     HN        1.03     MA        0.98     NL        1.18     
!   NY        0.93     SC        1.08     WF        0.95     WZ        1.98     
! 
!  Telescope amplitude corrections in sub-array 7:
!   FD        0.97     HH        1.02     HN        1.02     KP        0.99     
!   LA        1.00     MA        0.89     NL        0.99     PT        1.02     
!   SC        1.01     WF        0.86     WZ        1.52     
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   FD        0.99     HH        0.97     HN        1.15     KP        0.88     
!   LA        1.09     NL        1.00     NY        1.00*    PT        1.00     
!   WF        0.90     WZ        1.52     
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.99     FD        0.97     HN        1.10     KP        0.86     
!   LA        1.07     MK        1.04     NL        0.98     OV        1.00     
!   PT        0.99     SC        1.01     WF        0.93     
! 
!  A total of 84 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   HH        0.00*    MA        0.00*    NY        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   HN        0.00*    SC        0.00*    
! 
!  A total of 9 telescope corrections were flagged in sub-array 5.
!  Telescope amplitude corrections in sub-array 5:
!   HH        0.93     HN        1.13     MA        0.99     SC        1.05     
!   WF        0.98     WZ        1.82     
! 
!  A total of 9 telescope corrections were flagged in sub-array 6.
!  Telescope amplitude corrections in sub-array 6:
!   HH        0.93     HN        1.09     MA        0.98     NL        1.27     
!   NY        1.00*    SC        1.03     WF        0.96     WZ        1.93     
! 
!  Telescope amplitude corrections in sub-array 7:
!   FD        0.97     HH        0.94     HN        1.07     KP        0.89     
!   LA        1.05     MA        0.93     NL        1.01     PT        1.02     
!   SC        0.98     WF        0.91     WZ        1.61     
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   FD        1.01     HH        1.10     HN        1.12     KP        0.92     
!   LA        1.05     NL        0.98     NY        1.00*    PT        1.05     
!   WF        0.97     WZ        1.58     
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.98     FD        1.01     HN        1.07     KP        0.90     
!   LA        1.05     MK        1.04     NL        1.01     OV        0.97     
!   PT        1.04     SC        1.04     WF        0.98     
! 
!  A total of 84 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   HH        0.00*    MA        0.00*    NY        0.00*    WZ        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   HN        0.00*    SC        0.00*    
! 
!  A total of 9 telescope corrections were flagged in sub-array 5.
!  Telescope amplitude corrections in sub-array 5:
!   HH        0.95     HN        1.19     MA        1.07     SC        1.04     
!   WF        1.05     WZ        1.89     
! 
!  A total of 9 telescope corrections were flagged in sub-array 6.
!  Telescope amplitude corrections in sub-array 6:
!   HH        0.97     HN        1.16     MA        1.00     NL        1.26     
!   NY        1.00*    SC        1.08     WF        0.99     WZ        1.84     
! 
!  Telescope amplitude corrections in sub-array 7:
!   FD        1.01     HH        1.05     HN        1.08     KP        0.93     
!   LA        1.04     MA        0.99     NL        1.05     PT        1.05     
!   SC        1.00     WF        0.99     WZ        1.65     
! 
! 
! Fit before self-cal, rms=0.164728Jy  sigma=0.774477
! Fit after  self-cal, rms=0.126071Jy  sigma=0.596233
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 8.87% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
! Estimated beam: bmin=0.6548 mas, bmaj=1.155 mas, bpa=14.35 degrees
! Estimated noise=1.60057 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 = -0.0114299 Jy
! Component: 100  -  total flux cleaned = -0.014378 Jy
! Component: 150  -  total flux cleaned = -0.0162652 Jy
! Component: 200  -  total flux cleaned = -0.0176741 Jy
! Total flux subtracted in 200 components = -0.0176741 Jy
! Clean residual min=-0.010059 max=0.009902 Jy/beam
! Clean residual mean=0.000965 rms=0.001920 Jy/beam
! Combined flux in latest and established models = 0.942877 Jy
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 73 components and 0.942877 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.123690Jy  sigma=0.581340
! Fit after  self-cal, rms=0.123877Jy  sigma=0.580755
! Inverting map 
! Your choice of large map pixels excluded 8.87% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
! Added new window around map position (1, 16.4).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00932631 Jy
! Component: 100  -  total flux cleaned = 0.00992979 Jy
! Component: 150  -  total flux cleaned = 0.0104084 Jy
! Component: 200  -  total flux cleaned = 0.0104064 Jy
! Total flux subtracted in 200 components = 0.0104064 Jy
! Clean residual min=-0.008811 max=0.008181 Jy/beam
! Clean residual mean=0.000813 rms=0.001699 Jy/beam
! Combined flux in latest and established models = 0.953283 Jy
! Performing phase self-cal
! Adding 33 model components to the UV plane model.
! The established model now contains 92 components and 0.953283 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.122201Jy  sigma=0.573378
! Fit after  self-cal, rms=0.122208Jy  sigma=0.572873
! Inverting map 
! Your choice of large map pixels excluded 8.87% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
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=0.122208Jy  sigma=0.572873
! Fit after  self-cal, rms=0.122581Jy  sigma=0.570627
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 8.87% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
! Estimated beam: bmin=0.6547 mas, bmaj=1.155 mas, bpa=14.86 degrees
! Estimated noise=1.60141 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00506586 Jy
! Component: 100  -  total flux cleaned = -0.00559079 Jy
! Component: 150  -  total flux cleaned = -0.00606178 Jy
! Component: 200  -  total flux cleaned = -0.00626655 Jy
! Total flux subtracted in 200 components = -0.00626655 Jy
! Clean residual min=-0.008092 max=0.008141 Jy/beam
! Clean residual mean=0.000728 rms=0.001527 Jy/beam
! Combined flux in latest and established models = 0.947017 Jy
selfcal
! Performing phase self-cal
! Adding 25 model components to the UV plane model.
! The established model now contains 97 components and 0.947017 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.121109Jy  sigma=0.564278
! Fit after  self-cal, rms=0.121120Jy  sigma=0.564032
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 8.87% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
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 = -0.000273529 Jy
! Component: 100  -  total flux cleaned = 0.000119966 Jy
! Component: 150  -  total flux cleaned = 0.000304595 Jy
! Component: 200  -  total flux cleaned = 0.000643703 Jy
! Total flux subtracted in 200 components = 0.000643703 Jy
! Clean residual min=-0.007542 max=0.007227 Jy/beam
! Clean residual mean=0.000718 rms=0.001474 Jy/beam
! Combined flux in latest and established models = 0.94766 Jy
! Performing phase self-cal
! Adding 35 model components to the UV plane model.
! The established model now contains 107 components and 0.94766 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.120236Jy  sigma=0.561647
! Fit after  self-cal, rms=0.120247Jy  sigma=0.561496
! Inverting map 
! Your choice of large map pixels excluded 8.87% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
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=0.120247Jy  sigma=0.561496
! Fit after  self-cal, rms=0.121182Jy  sigma=0.559702
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 8.87% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
! Estimated beam: bmin=0.6547 mas, bmaj=1.156 mas, bpa=15.3 degrees
! Estimated noise=1.60206 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00448619 Jy
! Component: 100  -  total flux cleaned = -0.00510752 Jy
! Component: 150  -  total flux cleaned = -0.00568271 Jy
! Component: 200  -  total flux cleaned = -0.00568408 Jy
! Total flux subtracted in 200 components = -0.00568408 Jy
! Clean residual min=-0.007135 max=0.007149 Jy/beam
! Clean residual mean=0.000647 rms=0.001370 Jy/beam
! Combined flux in latest and established models = 0.941976 Jy
selfcal
! Performing phase self-cal
! Adding 22 model components to the UV plane model.
! The established model now contains 109 components and 0.941976 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.120160Jy  sigma=0.555708
! Fit after  self-cal, rms=0.120198Jy  sigma=0.555573
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 8.87% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
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 = -0.000226886 Jy
! Component: 100  -  total flux cleaned = -6.97834e-05 Jy
! Component: 150  -  total flux cleaned = 7.47522e-05 Jy
! Component: 200  -  total flux cleaned = 7.48693e-05 Jy
! Total flux subtracted in 200 components = 7.48693e-05 Jy
! Clean residual min=-0.006721 max=0.006598 Jy/beam
! Clean residual mean=0.000646 rms=0.001331 Jy/beam
! Combined flux in latest and established models = 0.942051 Jy
! Performing phase self-cal
! Adding 29 model components to the UV plane model.
! The established model now contains 111 components and 0.942051 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.119573Jy  sigma=0.553919
! Fit after  self-cal, rms=0.119582Jy  sigma=0.553819
! Inverting map 
! Your choice of large map pixels excluded 8.87% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 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=0.119582Jy  sigma=0.553819
! Fit after  self-cal, rms=0.120147Jy  sigma=0.552924
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 8.87% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
! Estimated beam: bmin=2.296 mas, bmaj=3.327 mas, bpa=-16.35 degrees
! Estimated noise=1.7202 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00362805 Jy
! Component: 100  -  total flux cleaned = 0.00416798 Jy
! Component: 150  -  total flux cleaned = 0.00416854 Jy
! Component: 200  -  total flux cleaned = 0.00417239 Jy
! Total flux subtracted in 200 components = 0.00417239 Jy
! Clean residual min=-0.005897 max=0.006850 Jy/beam
! Clean residual mean=0.000937 rms=0.001768 Jy/beam
! Combined flux in latest and established models = 0.946223 Jy
selfcal
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 126 components and 0.946223 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.120207Jy  sigma=0.552306
! Fit after  self-cal, rms=0.120185Jy  sigma=0.552252
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 8.87% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
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 = 0.000346965 Jy
! Component: 100  -  total flux cleaned = 0.000274284 Jy
! Component: 150  -  total flux cleaned = 0.000276099 Jy
! Component: 200  -  total flux cleaned = 0.00027569 Jy
! Total flux subtracted in 200 components = 0.00027569 Jy
! Clean residual min=-0.005758 max=0.006651 Jy/beam
! Clean residual mean=0.000927 rms=0.001720 Jy/beam
! Combined flux in latest and established models = 0.946499 Jy
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 129 components and 0.946499 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.120206Jy  sigma=0.551783
! Fit after  self-cal, rms=0.120200Jy  sigma=0.551757
! Inverting map 
! Your choice of large map pixels excluded 8.87% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
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:FD
! Syntax error in line:
! 1:FD
! ^
! 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 "/d2/scr/pima/rdv96_uvs/J2101+0341_X\_map.fits"
! Inverting map and beam 
! Your choice of large map pixels excluded 8.63% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
! Estimated beam: bmin=0.6521 mas, bmaj=1.096 mas, bpa=17.44 degrees
! Estimated noise=1.60414 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6521 x 1.096 at 17.44 degrees (North through East)
! Clean map  min=-0.0060066  max=0.7128 Jy/beam
! Writing clean map to FITS file: /d2/scr/pima/rdv96_uvs/J2101+0341_X_map.fits
float peak_flux
peak_flux = peak(flux,max)
invert
! Inverting map 
! Your choice of large map pixels excluded 8.63% of the data.
!  The x-axis pixel size should ideally be below 0.1667 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1952 milli-arcsec
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=  0.7127  rms=  0.00146  Jy 
quit
! Quitting program
! Log file /d2/scr/pima/rdv96_uvs/J2101+0341_X_uvs.log closed on Fri Dec 20 23:46:53 2013