! Started logfile: /scr/pima/rdv96_uvs/J1352-4412_S_uvs.log on Sat Dec 21 00:24:20 2013
obs /scr/pima/rdv96_uvs/J1352-4412_S_uva.fits
! Reading UV FITS file: /scr/pima/rdv96_uvs/J1352-4412_S_uva.fits
! AN table 1: 2 integrations on 10 of 10 possible baselines.
! AN table 2: 2 integrations on 15 of 15 possible baselines.
! AN table 3: 4 integrations on 21 of 21 possible baselines.
! AN table 4: 2 integrations on 10 of 10 possible baselines.
! Apparent sampling: 0.941558 visibilities/baseline/integration-bin.
! Found source: J1352-4412
! 
! 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 580 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/J1352-4412_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:FD       self-cal  status=correctable  weight=1
! 1:KP       self-cal  status=correctable  weight=1
! 1:LA       self-cal  status=correctable  weight=1
! 1:PT       self-cal  status=correctable  weight=1
! 1:SC       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:OV       self-cal  status=correctable  weight=1
! 2:PT       self-cal  status=correctable  weight=1
! 2:SC       self-cal  status=correctable  weight=1
! 3:FD       self-cal  status=correctable  weight=1
! 3:KP       self-cal  status=correctable  weight=1
! 3:LA       self-cal  status=correctable  weight=1
! 3:MK       self-cal  status=correctable  weight=1
! 3:OV       self-cal  status=correctable  weight=1
! 3:PT       self-cal  status=correctable  weight=1
! 3:SC       self-cal  status=correctable  weight=1
! 4:FD       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:OV       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 1 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 2.
!  A total of 1 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 3.
!  A total of 1 telescope corrections were flagged in sub-array 3.
! 
! Correcting IF 4.
!  A total of 1 telescope corrections were flagged in sub-array 3.
! 
! Fit before self-cal, rms=1.049297Jy  sigma=2.861629
! Fit after  self-cal, rms=0.757600Jy  sigma=2.009734
! 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 
! Estimated beam: bmin=2.547 mas, bmaj=7.631 mas, bpa=-0.7169 degrees
! Estimated noise=17.2778 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 = 0.179439 Jy
! Component: 100  -  total flux cleaned = 0.223557 Jy
! Total flux subtracted in 100 components = 0.223557 Jy
! Clean residual min=-0.012677 max=0.018572 Jy/beam
! Clean residual mean=-0.000252 rms=0.003773 Jy/beam
! Combined flux in latest and established models = 0.223557 Jy
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 18 components and 0.223557 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.086490Jy  sigma=0.240100
! Fit after  self-cal, rms=0.086494Jy  sigma=0.240053
! 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=3.589 mas, bmaj=10.79 mas, bpa=1.251 degrees
! Estimated noise=11.1176 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 = 0.0343031 Jy
! Component: 100  -  total flux cleaned = 0.0471032 Jy
! Component: 150  -  total flux cleaned = 0.0519933 Jy
! Component: 200  -  total flux cleaned = 0.0538899 Jy
! Total flux subtracted in 200 components = 0.0538899 Jy
! Clean residual min=-0.010093 max=0.008204 Jy/beam
! Clean residual mean=-0.000266 rms=0.002763 Jy/beam
! Combined flux in latest and established models = 0.277447 Jy
! Performing phase self-cal
! Adding 41 model components to the UV plane model.
! The established model now contains 57 components and 0.277447 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.076726Jy  sigma=0.201969
! Fit after  self-cal, rms=0.076807Jy  sigma=0.201906
! 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:
!   FD        0.86     KP        1.15     LA        1.30     PT        0.93     
!   SC        1.09     
! 
!  Telescope amplitude corrections in sub-array 2:
!   FD        1.14     KP        1.03     LA        1.32     OV        1.07     
!   PT        0.95     SC        0.85     
! 
!  Telescope amplitude corrections in sub-array 3:
!   FD        0.94     KP        0.98     LA        1.06     MK        0.89     
!   OV        1.07     PT        1.08     SC        0.95     
! 
!  Telescope amplitude corrections in sub-array 4:
!   FD        1.15     KP        1.01     LA        1.09     MK        1.00     
!   OV        1.00     
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   FD        1.05     KP        1.19     LA        0.99     PT        1.04     
!   SC        1.06     
! 
!  Telescope amplitude corrections in sub-array 2:
!   FD        1.01     KP        1.08     LA        1.00     OV        1.05     
!   PT        1.00     SC        1.10     
! 
!  Telescope amplitude corrections in sub-array 3:
!   FD        1.03     KP        1.06     LA        1.14     MK        1.05     
!   OV        1.08     PT        1.02     SC        1.02     
! 
!  Telescope amplitude corrections in sub-array 4:
!   FD        1.09     KP        0.95     LA        1.11     MK        1.02     
!   OV        1.10     
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   FD        1.04     KP        1.02     LA        0.99     PT        1.06     
!   SC        0.92     
! 
!  Telescope amplitude corrections in sub-array 2:
!   FD        1.11     KP        0.97     LA        1.00     OV        0.99     
!   PT        1.01     SC        1.09     
! 
!  Telescope amplitude corrections in sub-array 3:
!   FD        1.10     KP        0.91     LA        0.90     MK        0.99     
!   OV        1.08     PT        1.06     SC        0.96     
! 
!  Telescope amplitude corrections in sub-array 4:
!   FD        1.19     KP        0.91     LA        0.94     MK        0.85     
!   OV        1.03     
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   FD        1.03     KP        1.07     LA        0.80     PT        1.01     
!   SC        0.83     
! 
!  Telescope amplitude corrections in sub-array 2:
!   FD        1.11     KP        0.85     LA        0.86     OV        0.90     
!   PT        0.80     SC        1.08     
! 
!  Telescope amplitude corrections in sub-array 3:
!   FD        1.02     KP        0.84     LA        0.82     MK        1.20     
!   OV        0.94     PT        0.89     SC        1.03     
! 
!  Telescope amplitude corrections in sub-array 4:
!   FD        1.15     KP        0.94     LA        0.73     MK        0.96     
!   OV        0.95     
! 
! 
! Fit before self-cal, rms=0.076807Jy  sigma=0.201906
! Fit after  self-cal, rms=0.065687Jy  sigma=0.166501
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=3.588 mas, bmaj=10.81 mas, bpa=1.358 degrees
! Estimated noise=11.0505 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 = -0.000864808 Jy
! Component: 100  -  total flux cleaned = -0.000828853 Jy
! Component: 150  -  total flux cleaned = -0.000826373 Jy
! Component: 200  -  total flux cleaned = -0.000794871 Jy
! Total flux subtracted in 200 components = -0.000794871 Jy
! Clean residual min=-0.007591 max=0.006802 Jy/beam
! Clean residual mean=-0.000119 rms=0.002097 Jy/beam
! Combined flux in latest and established models = 0.276652 Jy
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 62 components and 0.276652 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.065618Jy  sigma=0.166452
! Fit after  self-cal, rms=0.065802Jy  sigma=0.166324
! 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=0.065802Jy  sigma=0.166324
! Fit after  self-cal, rms=0.065617Jy  sigma=0.166303
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=3.587 mas, bmaj=10.81 mas, bpa=1.333 degrees
! Estimated noise=11.0166 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000822223 Jy
! Component: 100  -  total flux cleaned = -0.000786379 Jy
! Component: 150  -  total flux cleaned = -0.000753496 Jy
! Component: 200  -  total flux cleaned = -0.000755691 Jy
! Total flux subtracted in 200 components = -0.000755691 Jy
! Clean residual min=-0.007529 max=0.006665 Jy/beam
! Clean residual mean=-0.000118 rms=0.002081 Jy/beam
! Combined flux in latest and established models = 0.275896 Jy
selfcal
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 66 components and 0.275896 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.065551Jy  sigma=0.166265
! Fit after  self-cal, rms=0.065562Jy  sigma=0.166258
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 = -4.62669e-05 Jy
! Component: 100  -  total flux cleaned = -4.60735e-05 Jy
! Component: 150  -  total flux cleaned = -1.75113e-05 Jy
! Component: 200  -  total flux cleaned = -1.71169e-05 Jy
! Total flux subtracted in 200 components = -1.71169e-05 Jy
! Clean residual min=-0.007529 max=0.006631 Jy/beam
! Clean residual mean=-0.000118 rms=0.002080 Jy/beam
! Combined flux in latest and established models = 0.275879 Jy
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 73 components and 0.275879 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.065524Jy  sigma=0.166227
! Fit after  self-cal, rms=0.065534Jy  sigma=0.166221
! 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=0.065534Jy  sigma=0.166221
! Fit after  self-cal, rms=0.064852Jy  sigma=0.164145
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=3.582 mas, bmaj=10.82 mas, bpa=1.194 degrees
! Estimated noise=10.9871 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000847664 Jy
! Component: 100  -  total flux cleaned = -0.000849018 Jy
! Component: 150  -  total flux cleaned = -0.000821878 Jy
! Component: 200  -  total flux cleaned = -0.00079731 Jy
! Total flux subtracted in 200 components = -0.00079731 Jy
! Clean residual min=-0.007362 max=0.006287 Jy/beam
! Clean residual mean=-0.000130 rms=0.002033 Jy/beam
! Combined flux in latest and established models = 0.275082 Jy
selfcal
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 76 components and 0.275082 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.064801Jy  sigma=0.164131
! Fit after  self-cal, rms=0.064809Jy  sigma=0.164119
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 = -4.85097e-05 Jy
! Component: 100  -  total flux cleaned = -2.30857e-05 Jy
! Component: 150  -  total flux cleaned = 2.17208e-06 Jy
! Component: 200  -  total flux cleaned = 4.72887e-05 Jy
! Total flux subtracted in 200 components = 4.72887e-05 Jy
! Clean residual min=-0.007361 max=0.006297 Jy/beam
! Clean residual mean=-0.000130 rms=0.002032 Jy/beam
! Combined flux in latest and established models = 0.275129 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 77 components and 0.275129 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.064778Jy  sigma=0.164099
! Fit after  self-cal, rms=0.064787Jy  sigma=0.164094
! 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=0.064787Jy  sigma=0.164094
! Fit after  self-cal, rms=0.064659Jy  sigma=0.164073
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=11.64 mas, bmaj=44.52 mas, bpa=0.7929 degrees
! Estimated noise=12.1832 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000357769 Jy
! Component: 100  -  total flux cleaned = -0.000357614 Jy
! Component: 150  -  total flux cleaned = -0.00035741 Jy
! Component: 200  -  total flux cleaned = -0.000357168 Jy
! Total flux subtracted in 200 components = -0.000357168 Jy
! Clean residual min=-0.007228 max=0.006126 Jy/beam
! Clean residual mean=-0.000201 rms=0.002566 Jy/beam
! Combined flux in latest and established models = 0.274772 Jy
selfcal
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 85 components and 0.274772 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.064665Jy  sigma=0.164070
! Fit after  self-cal, rms=0.064654Jy  sigma=0.164066
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 = 4.13921e-05 Jy
! Component: 100  -  total flux cleaned = 4.16248e-05 Jy
! Component: 150  -  total flux cleaned = 4.14319e-05 Jy
! Component: 200  -  total flux cleaned = 4.11849e-05 Jy
! Total flux subtracted in 200 components = 4.11849e-05 Jy
! Clean residual min=-0.007225 max=0.006119 Jy/beam
! Clean residual mean=-0.000201 rms=0.002564 Jy/beam
! Combined flux in latest and established models = 0.274813 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 85 components and 0.274813 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.064669Jy  sigma=0.164059
! Fit after  self-cal, rms=0.064658Jy  sigma=0.164056
! 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: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 "/scr/pima/rdv96_uvs/J1352-4412_S\_map.fits"
! Inverting map and beam 
! Estimated beam: bmin=3.583 mas, bmaj=10.83 mas, bpa=1.179 degrees
! Estimated noise=10.9565 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 3.583 x 10.83 at 1.179 degrees (North through East)
! Clean map  min=-0.0071366  max=0.24065 Jy/beam
! Writing clean map to FITS file: /scr/pima/rdv96_uvs/J1352-4412_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=  0.2406  rms=  0.00202  Jy 
quit
! Quitting program
! Log file /scr/pima/rdv96_uvs/J1352-4412_S_uvs.log closed on Sat Dec 21 00:24:22 2013