! Started logfile: /scr/pima/rdv72_uvs/J1823+6857_X_uvs.log on Sat Oct  5 08:49:32 2013
obs /scr/pima/rdv72_uvs/J1823+6857_X_uva.fits
! Reading UV FITS file: /scr/pima/rdv72_uvs/J1823+6857_X_uva.fits
! AN table 1: 32 integrations on 78 of 78 possible baselines.
! AN table 2: 7 integrations on 3 of 3 possible baselines.
! AN table 3: 19 integrations on 1 of 1 possible baselines.
! AN table 4: 6 integrations on 1 of 1 possible baselines.
! AN table 5: 6 integrations on 3 of 3 possible baselines.
! AN table 6: 11 integrations on 1 of 1 possible baselines.
! Apparent sampling: 0.748347 visibilities/baseline/integration-bin.
! Found source: J1823+6857
! 
! 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      1.6e+07          1      1.6e+07
!  02        2  8.47599e+09      1.6e+07          1      1.6e+07
!  03        3  8.79099e+09      1.6e+07          1      1.6e+07
!  04        4  8.89599e+09      1.6e+07          1      1.6e+07
! 
! Polarization(s): RR
! 
! Read 0 lines of history.
! 
! Reading 7696 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/01_muppet /scr/pima/rdv72_uvs/J1823+6857_X]
integer clean_niter
clean_niter = 100
float clean_gain
clean_gain = 0.03
float dynam
dynam = 6.0
float soltime1
soltime1 = 120
float soltime2
soltime2 = 20
float thresh
thresh = 0.5
float win_mult
win_mult = 1.8
float time_av
time_av = 16
float old_peak
float new_peak
float flux_cutoff
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 71 telescope corrections were flagged in sub-array 1.
!  A total of 38 telescope corrections were flagged in sub-array 3.
!  A total of 12 telescope corrections were flagged in sub-array 4.
!  A total of 18 telescope corrections were flagged in sub-array 5.
!  A total of 22 telescope corrections were flagged in sub-array 6.
! 
! Correcting IF 2.
!  A total of 71 telescope corrections were flagged in sub-array 1.
!  A total of 38 telescope corrections were flagged in sub-array 3.
!  A total of 12 telescope corrections were flagged in sub-array 4.
!  A total of 18 telescope corrections were flagged in sub-array 5.
!  A total of 22 telescope corrections were flagged in sub-array 6.
! 
! Correcting IF 3.
!  A total of 71 telescope corrections were flagged in sub-array 1.
!  A total of 38 telescope corrections were flagged in sub-array 3.
!  A total of 12 telescope corrections were flagged in sub-array 4.
!  A total of 18 telescope corrections were flagged in sub-array 5.
!  A total of 22 telescope corrections were flagged in sub-array 6.
! 
! Correcting IF 4.
!  A total of 71 telescope corrections were flagged in sub-array 1.
!  A total of 38 telescope corrections were flagged in sub-array 3.
!  A total of 12 telescope corrections were flagged in sub-array 4.
!  A total of 18 telescope corrections were flagged in sub-array 5.
!  A total of 22 telescope corrections were flagged in sub-array 6.
! 
! Fit before self-cal, rms=1.025919Jy  sigma=2.607247
! Fit after  self-cal, rms=0.828383Jy  sigma=1.864314
! clrmod: Cleared the established, tentative and continuum models.
! Redundant starting model cleared.
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 6.47% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 milli-arcsec
! Estimated beam: bmin=0.4981 mas, bmaj=0.7517 mas, bpa=-55.83 degrees
! Estimated noise=7.28622 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 = 0.148554 Jy
! Component: 100  -  total flux cleaned = 0.202881 Jy
! Total flux subtracted in 100 components = 0.202881 Jy
! Clean residual min=-0.013992 max=0.028100 Jy/beam
! Clean residual mean=0.000024 rms=0.003461 Jy/beam
! Combined flux in latest and established models = 0.202881 Jy
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 7 components and 0.202881 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.121085Jy  sigma=0.358350
! Fit after  self-cal, rms=0.120687Jy  sigma=0.357597
! Inverting map 
! Your choice of large map pixels excluded 6.47% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 milli-arcsec
! Added new window around map position (0, -1).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.028786 Jy
! Component: 100  -  total flux cleaned = 0.0470624 Jy
! Total flux subtracted in 100 components = 0.0470624 Jy
! Clean residual min=-0.011736 max=0.016350 Jy/beam
! Clean residual mean=0.000021 rms=0.002752 Jy/beam
! Combined flux in latest and established models = 0.249944 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 17 components and 0.249944 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.112353Jy  sigma=0.306249
! Fit after  self-cal, rms=0.112383Jy  sigma=0.305485
! Inverting map 
! Your choice of large map pixels excluded 6.47% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 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 6.47% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 milli-arcsec
! Estimated beam: bmin=0.7074 mas, bmaj=0.9328 mas, bpa=-43.36 degrees
! Estimated noise=3.6698 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 = 0.0323969 Jy
! Component: 100  -  total flux cleaned = 0.0503784 Jy
! Component: 150  -  total flux cleaned = 0.0613039 Jy
! Component: 200  -  total flux cleaned = 0.0680773 Jy
! Total flux subtracted in 200 components = 0.0680773 Jy
! Clean residual min=-0.014077 max=0.019771 Jy/beam
! Clean residual mean=0.000037 rms=0.004145 Jy/beam
! Combined flux in latest and established models = 0.318021 Jy
! Performing phase self-cal
! Adding 21 model components to the UV plane model.
! The established model now contains 28 components and 0.318021 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.109229Jy  sigma=0.265806
! Fit after  self-cal, rms=0.109255Jy  sigma=0.264696
! Inverting map 
! Your choice of large map pixels excluded 6.47% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 9 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.36     FD        0.77     KK        1.16     KP        0.96     
!   LA        0.94     MK        0.98     NL        1.14     NY        1.20     
!   OV        1.04     PT        0.88     SC        0.83     WZ        1.08     
!   ZC        1.40     
! 
!  A total of 21 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.00*    KP        0.00*    OV        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   WZ        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   KP        0.00*    OV        0.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   BR        0.00*    OV        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 6:
!   KK        0.00*    MK        0.00*    
! 
! 
! Correcting IF 2.
!  A total of 9 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.25     FD        0.79     KK        1.11     KP        0.94     
!   LA        0.89     MK        1.01     NL        1.14     NY        1.27     
!   OV        1.04     PT        0.94     SC        0.90     WZ        1.01     
!   ZC        1.50     
! 
!  A total of 21 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.00*    KP        0.00*    OV        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   WZ        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   KP        0.00*    OV        0.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   BR        0.00*    OV        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 6:
!   KK        0.00*    MK        0.00*    
! 
! 
! Correcting IF 3.
!  A total of 9 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.46     FD        0.78     KK        1.17     KP        0.85     
!   LA        0.96     MK        1.00     NL        1.18     NY        1.32     
!   OV        1.11     PT        0.94     SC        0.90     WZ        1.12     
!   ZC        1.16     
! 
!  A total of 21 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.00*    KP        0.00*    OV        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   WZ        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   KP        0.00*    OV        0.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   BR        0.00*    OV        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 6:
!   KK        0.00*    MK        0.00*    
! 
! 
! Correcting IF 4.
!  A total of 9 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.33     FD        0.82     KK        1.18     KP        0.91     
!   LA        0.95     MK        1.05     NL        1.29     NY        1.20     
!   OV        1.11     PT        0.95     SC        0.97     WZ        1.13     
!   ZC        1.20     
! 
!  A total of 21 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.00*    KP        0.00*    OV        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   WZ        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   KP        0.00*    OV        0.00*    
! 
!  Telescope amplitude corrections in sub-array 5:
!   BR        0.00*    OV        0.00*    ZC        0.00*    
! 
!  Telescope amplitude corrections in sub-array 6:
!   KK        0.00*    MK        0.00*    
! 
! 
! Fit before self-cal, rms=0.109255Jy  sigma=0.264696
! Fit after  self-cal, rms=0.115654Jy  sigma=0.221589
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 6.58% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 milli-arcsec
! Estimated beam: bmin=0.7274 mas, bmaj=0.9537 mas, bpa=-36.73 degrees
! Estimated noise=3.74907 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 (0.4, 1.8).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00239531 Jy
! Component: 100  -  total flux cleaned = 0.00224185 Jy
! Component: 150  -  total flux cleaned = 0.00210859 Jy
! Component: 200  -  total flux cleaned = 0.00187533 Jy
! Total flux subtracted in 200 components = 0.00187533 Jy
! Clean residual min=-0.003944 max=0.003847 Jy/beam
! Clean residual mean=-0.000001 rms=0.000893 Jy/beam
! Combined flux in latest and established models = 0.319897 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 35 components and 0.319896 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.114978Jy  sigma=0.220877
! Fit after  self-cal, rms=0.115241Jy  sigma=0.220613
! Inverting map 
! Your choice of large map pixels excluded 6.58% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 milli-arcsec
selfcal true, true, soltime1
! Performing amp+phase self-cal over 120 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.115241Jy  sigma=0.220613
! Fit after  self-cal, rms=0.114426Jy  sigma=0.220571
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 6.58% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 milli-arcsec
! Estimated beam: bmin=0.7279 mas, bmaj=0.9521 mas, bpa=-36.37 degrees
! Estimated noise=3.74726 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00068974 Jy
! Component: 100  -  total flux cleaned = 0.000693516 Jy
! Component: 150  -  total flux cleaned = 0.000600251 Jy
! Component: 200  -  total flux cleaned = 0.000515455 Jy
! Total flux subtracted in 200 components = 0.000515455 Jy
! Clean residual min=-0.003940 max=0.003821 Jy/beam
! Clean residual mean=-0.000001 rms=0.000864 Jy/beam
! Combined flux in latest and established models = 0.320412 Jy
selfcal
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 38 components and 0.320412 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.114119Jy  sigma=0.220340
! Fit after  self-cal, rms=0.114118Jy  sigma=0.220332
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 6.58% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 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 = -9.19399e-05 Jy
! Component: 100  -  total flux cleaned = -0.000245007 Jy
! Component: 150  -  total flux cleaned = -0.000313262 Jy
! Component: 200  -  total flux cleaned = -0.000311995 Jy
! Total flux subtracted in 200 components = -0.000311995 Jy
! Clean residual min=-0.003883 max=0.003775 Jy/beam
! Clean residual mean=-0.000001 rms=0.000855 Jy/beam
! Combined flux in latest and established models = 0.3201 Jy
! Performing phase self-cal
! Adding 15 model components to the UV plane model.
! The established model now contains 41 components and 0.3201 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.113938Jy  sigma=0.220206
! Fit after  self-cal, rms=0.113948Jy  sigma=0.220201
! Inverting map 
! Your choice of large map pixels excluded 6.58% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 milli-arcsec
selfcal true, true, soltime2
! Performing amp+phase self-cal over 20 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.113948Jy  sigma=0.220201
! Fit after  self-cal, rms=0.113089Jy  sigma=0.220183
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 6.58% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 milli-arcsec
! Estimated beam: bmin=0.7298 mas, bmaj=0.9517 mas, bpa=-35.85 degrees
! Estimated noise=3.74612 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000121598 Jy
! Component: 100  -  total flux cleaned = 0.000120023 Jy
! Component: 150  -  total flux cleaned = 0.000177935 Jy
! Component: 200  -  total flux cleaned = 0.000177549 Jy
! Total flux subtracted in 200 components = 0.000177549 Jy
! Clean residual min=-0.003769 max=0.003740 Jy/beam
! Clean residual mean=-0.000001 rms=0.000847 Jy/beam
! Combined flux in latest and established models = 0.320278 Jy
selfcal
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 46 components and 0.320278 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.112954Jy  sigma=0.220095
! Fit after  self-cal, rms=0.112947Jy  sigma=0.220092
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 6.58% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 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 = -4.74441e-06 Jy
! Component: 100  -  total flux cleaned = -3.78373e-06 Jy
! Component: 150  -  total flux cleaned = -1.5728e-06 Jy
! Component: 200  -  total flux cleaned = -2.2449e-06 Jy
! Total flux subtracted in 200 components = -2.2449e-06 Jy
! Clean residual min=-0.003732 max=0.003726 Jy/beam
! Clean residual mean=-0.000001 rms=0.000843 Jy/beam
! Combined flux in latest and established models = 0.320275 Jy
! Performing phase self-cal
! Adding 21 model components to the UV plane model.
! The established model now contains 51 components and 0.320275 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.112866Jy  sigma=0.220041
! Fit after  self-cal, rms=0.112873Jy  sigma=0.220038
! Inverting map 
! Your choice of large map pixels excluded 6.58% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 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 20 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.112873Jy  sigma=0.220038
! Fit after  self-cal, rms=0.112473Jy  sigma=0.220031
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 6.58% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 milli-arcsec
! Estimated beam: bmin=2.316 mas, bmaj=3.626 mas, bpa=-4.051 degrees
! Estimated noise=3.98909 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 4.21494e-05 Jy
! Component: 100  -  total flux cleaned = 0.000132596 Jy
! Component: 150  -  total flux cleaned = 0.000210146 Jy
! Component: 200  -  total flux cleaned = 0.000278321 Jy
! Total flux subtracted in 200 components = 0.000278321 Jy
! Clean residual min=-0.004519 max=0.004135 Jy/beam
! Clean residual mean=-0.000002 rms=0.001239 Jy/beam
! Combined flux in latest and established models = 0.320554 Jy
selfcal
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 55 components and 0.320554 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.112451Jy  sigma=0.220000
! Fit after  self-cal, rms=0.112432Jy  sigma=0.219991
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 6.58% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 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 = 9.71963e-06 Jy
! Component: 100  -  total flux cleaned = 5.94453e-05 Jy
! Component: 150  -  total flux cleaned = 0.000128103 Jy
! Component: 200  -  total flux cleaned = 0.000186552 Jy
! Total flux subtracted in 200 components = 0.000186552 Jy
! Clean residual min=-0.004457 max=0.004119 Jy/beam
! Clean residual mean=-0.000002 rms=0.001235 Jy/beam
! Combined flux in latest and established models = 0.32074 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 58 components and 0.32074 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.112418Jy  sigma=0.219978
! Fit after  self-cal, rms=0.112415Jy  sigma=0.219973
! Inverting map 
! Your choice of large map pixels excluded 6.58% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
win_mult = win_mult / 1.2
print "************** FINISHED AMPLITUDE SELF-CAL **************"
! ************** FINISHED AMPLITUDE SELF-CAL ************** 
restore
! Inverting map and beam 
! Your choice of large map pixels excluded 6.58% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 milli-arcsec
! Estimated beam: bmin=0.7308 mas, bmaj=0.9517 mas, bpa=-35.5 degrees
! Estimated noise=3.74476 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7308 x 0.9517 at -35.5 degrees (North through East)
! Clean map  min=-0.0034777  max=0.19908 Jy/beam
if(peak(flux) > thresh)
  selfcal true, true
  clean clean_niter,clean_gain
  selfcal
  flux_cutoff = imstat(rms) * dynam
  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)
  selfcal true, true
  end if
print "************** CLEARING MODEL AND STARTING OVER **********"
! ************** CLEARING MODEL AND STARTING OVER ********** 
clrmod true
! clrmod: Cleared the established and tentative models.
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.
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 6.58% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 milli-arcsec
! Estimated beam: bmin=0.5166 mas, bmaj=0.7389 mas, bpa=-52.11 degrees
! Estimated noise=7.83298 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.154698 Jy
! Component: 100  -  total flux cleaned = 0.210715 Jy
! Component: 150  -  total flux cleaned = 0.240404 Jy
! Component: 200  -  total flux cleaned = 0.260431 Jy
! Total flux subtracted in 200 components = 0.260431 Jy
! Clean residual min=-0.007676 max=0.011758 Jy/beam
! Clean residual mean=0.000008 rms=0.001986 Jy/beam
! Combined flux in latest and established models = 0.260431 Jy
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.
flux_cutoff = imstat(rms) * dynam
! Adding 23 model components to the UV plane model.
! The established model now contains 23 components and 0.260431 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 6.58% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 milli-arcsec
! Estimated beam: bmin=0.7308 mas, bmaj=0.9517 mas, bpa=-35.5 degrees
! Estimated noise=3.74476 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  keep
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0262139 Jy
! Component: 100  -  total flux cleaned = 0.039676 Jy
! Component: 150  -  total flux cleaned = 0.047324 Jy
! Component: 200  -  total flux cleaned = 0.0519537 Jy
! Total flux subtracted in 200 components = 0.0519537 Jy
! Clean residual min=-0.004298 max=0.004290 Jy/beam
! Clean residual mean=0.000003 rms=0.000946 Jy/beam
! Combined flux in latest and established models = 0.312385 Jy
! Adding 33 model components to the UV plane model.
! The established model now contains 38 components and 0.312385 Jy
! Inverting map 
! Your choice of large map pixels excluded 6.58% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 milli-arcsec
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 6.58% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 milli-arcsec
! Estimated beam: bmin=2.316 mas, bmaj=3.626 mas, bpa=-4.051 degrees
! Estimated noise=3.98909 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00491389 Jy
! Component: 100  -  total flux cleaned = 0.00689479 Jy
! Component: 150  -  total flux cleaned = 0.00740238 Jy
! Component: 200  -  total flux cleaned = 0.0075483 Jy
! Total flux subtracted in 200 components = 0.0075483 Jy
! Clean residual min=-0.004532 max=0.004008 Jy/beam
! Clean residual mean=-0.000001 rms=0.001198 Jy/beam
! Combined flux in latest and established models = 0.319933 Jy
flux_cutoff = imstat(rms) * dynam
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  keep
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000116757 Jy
! Component: 100  -  total flux cleaned = 0.000196527 Jy
! Component: 150  -  total flux cleaned = 0.000264968 Jy
! Component: 200  -  total flux cleaned = 0.000295485 Jy
! Total flux subtracted in 200 components = 0.000295485 Jy
! Clean residual min=-0.004512 max=0.004061 Jy/beam
! Clean residual mean=-0.000002 rms=0.001196 Jy/beam
! Combined flux in latest and established models = 0.320228 Jy
! Adding 21 model components to the UV plane model.
! The established model now contains 57 components and 0.320228 Jy
! Inverting map 
! Your choice of large map pixels excluded 6.58% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 6.58% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 milli-arcsec
! Estimated beam: bmin=0.7308 mas, bmaj=0.9517 mas, bpa=-35.5 degrees
! Estimated noise=3.74476 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000380967 Jy
! Component: 100  -  total flux cleaned = -0.000379119 Jy
! Component: 150  -  total flux cleaned = -0.000331549 Jy
! Component: 200  -  total flux cleaned = -0.000331056 Jy
! Total flux subtracted in 200 components = -0.000331056 Jy
! Clean residual min=-0.003672 max=0.003529 Jy/beam
! Clean residual mean=-0.000000 rms=0.000819 Jy/beam
! Combined flux in latest and established models = 0.319897 Jy
selfcal
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 66 components and 0.319897 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.112261Jy  sigma=0.219828
! Fit after  self-cal, rms=0.112224Jy  sigma=0.219805
wmodel /scr/pima/rdv72_uvs/J1823+6857_X_map.mod
! Writing 66 model components to file: /scr/pima/rdv72_uvs/J1823+6857_X_map.mod
wobs /scr/pima/rdv72_uvs/J1823+6857_X_uvs.fits
! Writing UV FITS file: /scr/pima/rdv72_uvs/J1823+6857_X_uvs.fits
wwins /scr/pima/rdv72_uvs/J1823+6857_X_map.win
! wwins: Wrote 3 windows to /scr/pima/rdv72_uvs/J1823+6857_X_map.win
x = (field_size-8) * field_cell / 4
addwin -x,x,-x,x
clean (field_size*4),0.01
! Inverting map 
! Your choice of large map pixels excluded 6.58% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 milli-arcsec
! clean: niter=4096  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.000610268 Jy
! Component: 100  -  total flux cleaned = -0.000432179 Jy
! Component: 150  -  total flux cleaned = 0.000261304 Jy
! Component: 200  -  total flux cleaned = 0.000708809 Jy
! Component: 250  -  total flux cleaned = 0.0010896 Jy
! Component: 300  -  total flux cleaned = 0.00130217 Jy
! Component: 350  -  total flux cleaned = 0.00140583 Jy
! Component: 400  -  total flux cleaned = 0.00135391 Jy
! Component: 450  -  total flux cleaned = 0.00130246 Jy
! Component: 500  -  total flux cleaned = 0.00115433 Jy
! Component: 550  -  total flux cleaned = 0.00105762 Jy
! Component: 600  -  total flux cleaned = 0.00110415 Jy
! Component: 650  -  total flux cleaned = 0.00110379 Jy
! Component: 700  -  total flux cleaned = 0.00101128 Jy
! Component: 750  -  total flux cleaned = 0.00078533 Jy
! Component: 800  -  total flux cleaned = 0.000651791 Jy
! Component: 850  -  total flux cleaned = 0.000652063 Jy
! Component: 900  -  total flux cleaned = 0.000521659 Jy
! Component: 950  -  total flux cleaned = 0.000521075 Jy
! Component: 1000  -  total flux cleaned = 0.000478584 Jy
! Component: 1050  -  total flux cleaned = 0.000520453 Jy
! Component: 1100  -  total flux cleaned = 0.000519992 Jy
! Component: 1150  -  total flux cleaned = 0.000437811 Jy
! Component: 1200  -  total flux cleaned = 0.000437532 Jy
! Component: 1250  -  total flux cleaned = 0.000317102 Jy
! Component: 1300  -  total flux cleaned = 0.000476035 Jy
! Component: 1350  -  total flux cleaned = 0.000435945 Jy
! Component: 1400  -  total flux cleaned = 0.000513586 Jy
! Component: 1450  -  total flux cleaned = 0.00039745 Jy
! Component: 1500  -  total flux cleaned = 0.000513312 Jy
! Component: 1550  -  total flux cleaned = 0.000665644 Jy
! Component: 1600  -  total flux cleaned = 0.000666227 Jy
! Component: 1650  -  total flux cleaned = 0.000778565 Jy
! Component: 1700  -  total flux cleaned = 0.000741453 Jy
! Component: 1750  -  total flux cleaned = 0.000888641 Jy
! Component: 1800  -  total flux cleaned = 0.000705918 Jy
! Component: 1850  -  total flux cleaned = 0.000669934 Jy
! Component: 1900  -  total flux cleaned = 0.000777895 Jy
! Component: 1950  -  total flux cleaned = 0.000741789 Jy
! Component: 2000  -  total flux cleaned = 0.000812455 Jy
! Component: 2050  -  total flux cleaned = 0.000741722 Jy
! Component: 2100  -  total flux cleaned = 0.000777077 Jy
! Component: 2150  -  total flux cleaned = 0.000811885 Jy
! Component: 2200  -  total flux cleaned = 0.000707908 Jy
! Component: 2250  -  total flux cleaned = 0.000949883 Jy
! Component: 2300  -  total flux cleaned = 0.000915261 Jy
! Component: 2350  -  total flux cleaned = 0.000983555 Jy
! Component: 2400  -  total flux cleaned = 0.000847706 Jy
! Component: 2450  -  total flux cleaned = 0.00101722 Jy
! Component: 2500  -  total flux cleaned = 0.000949927 Jy
! Component: 2550  -  total flux cleaned = 0.000983435 Jy
! Component: 2600  -  total flux cleaned = 0.00108365 Jy
! Component: 2650  -  total flux cleaned = 0.000984098 Jy
! Component: 2700  -  total flux cleaned = 0.00111588 Jy
! Component: 2750  -  total flux cleaned = 0.000951873 Jy
! Component: 2800  -  total flux cleaned = 0.00098449 Jy
! Component: 2850  -  total flux cleaned = 0.000886737 Jy
! Component: 2900  -  total flux cleaned = 0.000886771 Jy
! Component: 2950  -  total flux cleaned = 0.00101566 Jy
! Component: 3000  -  total flux cleaned = 0.000919423 Jy
! Component: 3050  -  total flux cleaned = 0.000951475 Jy
! Component: 3100  -  total flux cleaned = 0.00107867 Jy
! Component: 3150  -  total flux cleaned = 0.000951738 Jy
! Component: 3200  -  total flux cleaned = 0.00104662 Jy
! Component: 3250  -  total flux cleaned = 0.00107786 Jy
! Component: 3300  -  total flux cleaned = 0.00120319 Jy
! Component: 3350  -  total flux cleaned = 0.00117192 Jy
! Component: 3400  -  total flux cleaned = 0.00110973 Jy
! Component: 3450  -  total flux cleaned = 0.00117147 Jy
! Component: 3500  -  total flux cleaned = 0.00120207 Jy
! Component: 3550  -  total flux cleaned = 0.00117141 Jy
! Component: 3600  -  total flux cleaned = 0.00129364 Jy
! Component: 3650  -  total flux cleaned = 0.0012328 Jy
! Component: 3700  -  total flux cleaned = 0.00126304 Jy
! Component: 3750  -  total flux cleaned = 0.00129333 Jy
! Component: 3800  -  total flux cleaned = 0.00141377 Jy
! Component: 3850  -  total flux cleaned = 0.00123361 Jy
! Component: 3900  -  total flux cleaned = 0.00132338 Jy
! Component: 3950  -  total flux cleaned = 0.00120409 Jy
! Component: 4000  -  total flux cleaned = 0.00126358 Jy
! Component: 4050  -  total flux cleaned = 0.00138199 Jy
! Total flux subtracted in 4096 components = 0.00126399 Jy
! Clean residual min=-0.001817 max=0.001781 Jy/beam
! Clean residual mean=0.000000 rms=0.000484 Jy/beam
! Combined flux in latest and established models = 0.321161 Jy
keep
! Adding 296 model components to the UV plane model.
! The established model now contains 362 components and 0.321161 Jy
![Exited script file: /home/lpetrov/bin/01_muppet]
wmap "/scr/pima/rdv72_uvs/J1823+6857_X\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 6.58% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7308 x 0.9517 at -35.5 degrees (North through East)
! Clean map  min=-0.002446  max=0.19376 Jy/beam
! Writing clean map to FITS file: /scr/pima/rdv72_uvs/J1823+6857_X_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.193759 
invert
! Inverting map 
! Your choice of large map pixels excluded 6.58% of the data.
!  The x-axis pixel size should ideally be below 0.1954 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1827 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000477456 
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.739253 0.739253 1.47851 2.95701 5.91402 11.828 23.6561 47.3122 94.6244
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0014 
print "peak=",int(1000*peak_flux)/1000
! peak= 0.193 
quit
! Quitting program
! Log file /scr/pima/rdv72_uvs/J1823+6857_X_uvs.log closed on Sat Oct  5 08:49:36 2013