! Started logfile: /scr/pima/bg219h_uvs/J1522-2730_S_dfm.log on Thu May 19 22:31:02 2016
float field_size
field_size =  1024
float field_cell
field_cell =   0.5000
float taper_size
taper_size =   20.0
float freq
freq       =    2.22000
obs     /scr/pima/bg219h_uvs/J1522-2730_S_uva.fits
! Reading UV FITS file: /scr/pima/bg219h_uvs/J1522-2730_S_uva.fits
! AN table 1: 7 integrations on 28 of 28 possible baselines.
! Apparent sampling: 0.719388 visibilities/baseline/integration-bin.
! Found source: J1522-2730
! 
! 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     2.22e+09      3.2e+07          1      3.2e+07
!  02        2    2.252e+09      3.2e+07          1      3.2e+07
!  03        3    2.284e+09      3.2e+07          1      3.2e+07
!  04        4    2.348e+09      3.2e+07          1      3.2e+07
! 
! Polarization(s): RR
! 
! Read 54 lines of history.
! 
! Reading 564 visibilities.
select rr, 1,2,3,4,5,6,7,8,9,10,11,12,13,14,15,16 
! Restricting channel ranges to the available 4 channels.
! 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 = 0.5 
print "taper_size =", taper_size
! taper_size = 20 
![@/opt64/bin/pima_mupet_01.dfm J1522-2730_S]
float lim_self
lim_self = 120.0
float lim_val
lim_va   = 1.2
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 0.500x0.500 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 14 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 14 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 14 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 14 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=1.449349Jy  sigma=20.522590
! Fit after  self-cal, rms=0.189175Jy  sigma=3.476410
! 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 
! Estimated beam: bmin=3.589 mas, bmaj=13.48 mas, bpa=-11.21 degrees
! Estimated noise=3.54368 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 = 0.698449 Jy
! Component: 100  -  total flux cleaned = 0.856241 Jy
! Total flux subtracted in 100 components = 0.856241 Jy
! Clean residual min=-0.106691 max=0.192970 Jy/beam
! Clean residual mean=-0.000240 rms=0.038235 Jy/beam
! Combined flux in latest and established models = 0.856242 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 8 components and 0.856242 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.230299Jy  sigma=3.616500
! Fit after  self-cal, rms=0.230288Jy  sigma=3.616451
! 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=4.14 mas, bmaj=16.4 mas, bpa=-11.41 degrees
! Estimated noise=2.86721 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (16, -48).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.15983 Jy
! Component: 100  -  total flux cleaned = 0.209785 Jy
! Component: 150  -  total flux cleaned = 0.222302 Jy
! Component: 200  -  total flux cleaned = 0.229856 Jy
! Total flux subtracted in 200 components = 0.229856 Jy
! Clean residual min=-0.026643 max=0.030517 Jy/beam
! Clean residual mean=-0.000176 rms=0.008498 Jy/beam
! Combined flux in latest and established models = 1.0861 Jy
! Performing phase self-cal
! Adding 37 model components to the UV plane model.
! The established model now contains 45 components and 1.0861 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.120419Jy  sigma=1.788746
! Fit after  self-cal, rms=0.115095Jy  sigma=1.732469
! Inverting map 
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 4.14 x 16.4 at -11.41 degrees (North through East)
! Clean map  min=-0.025075  max=0.85338 Jy/beam
if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val
! Selfcal amplitude corrections will be limited to 0.833333 -> 1.2.
! Selfcal phase corrections will not be limited.
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    KP        1.00*    LA        1.00*    
!   MK        1.00*    NL        1.00*    OV        1.00*    PT        1.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.97     FD        1.00*    KP        0.98     LA        1.01     
!   MK        1.01     NL        1.17     OV        1.00     PT        1.00     
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    KP        1.00*    LA        1.00*    
!   MK        1.00*    NL        1.00*    OV        1.00*    PT        1.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    KP        1.00*    LA        1.00*    
!   MK        1.00*    NL        1.00*    OV        1.00*    PT        1.00*    
! 
! 
! Fit before self-cal, rms=0.115095Jy  sigma=1.732469
! Fit after  self-cal, rms=0.113671Jy  sigma=1.701447
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=4.137 mas, bmaj=16.37 mas, bpa=-11.46 degrees
! Estimated noise=2.88393 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 = 0.0109893 Jy
! Component: 100  -  total flux cleaned = 0.0120462 Jy
! Component: 150  -  total flux cleaned = 0.013476 Jy
! Component: 200  -  total flux cleaned = 0.0138074 Jy
! Total flux subtracted in 200 components = 0.0138074 Jy
! Clean residual min=-0.024310 max=0.024620 Jy/beam
! Clean residual mean=-0.000137 rms=0.006602 Jy/beam
! Combined flux in latest and established models = 1.0999 Jy
! Performing phase self-cal
! Adding 26 model components to the UV plane model.
! The established model now contains 70 components and 1.09991 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.111837Jy  sigma=1.681291
! Fit after  self-cal, rms=0.111599Jy  sigma=1.676488
! Inverting map 
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=0.111599Jy  sigma=1.676488
! Fit after  self-cal, rms=0.111400Jy  sigma=1.673791
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=4.134 mas, bmaj=16.37 mas, bpa=-11.47 degrees
! Estimated noise=2.89106 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00619734 Jy
! Component: 100  -  total flux cleaned = 0.00601028 Jy
! Component: 150  -  total flux cleaned = 0.00584215 Jy
! Component: 200  -  total flux cleaned = 0.00567398 Jy
! Total flux subtracted in 200 components = 0.00567398 Jy
! Clean residual min=-0.024261 max=0.023635 Jy/beam
! Clean residual mean=-0.000135 rms=0.006539 Jy/beam
! Combined flux in latest and established models = 1.10558 Jy
selfcal
! Performing phase self-cal
! Adding 23 model components to the UV plane model.
! The established model now contains 83 components and 1.10558 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.110508Jy  sigma=1.665036
! Fit after  self-cal, rms=0.110401Jy  sigma=1.661955
flux_cutoff = imstat(rms) * dynam
! Inverting map 
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000436426 Jy
! Component: 100  -  total flux cleaned = 0.000622374 Jy
! Component: 150  -  total flux cleaned = 0.000461114 Jy
! Component: 200  -  total flux cleaned = 0.000304128 Jy
! Total flux subtracted in 200 components = 0.000304128 Jy
! Clean residual min=-0.024049 max=0.023449 Jy/beam
! Clean residual mean=-0.000131 rms=0.006492 Jy/beam
! Combined flux in latest and established models = 1.10588 Jy
! Performing phase self-cal
! Adding 35 model components to the UV plane model.
! The established model now contains 102 components and 1.10588 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.109729Jy  sigma=1.654750
! Fit after  self-cal, rms=0.109648Jy  sigma=1.651979
! Inverting map 
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=0.109648Jy  sigma=1.651979
! Fit after  self-cal, rms=0.109619Jy  sigma=1.651545
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=4.133 mas, bmaj=16.37 mas, bpa=-11.47 degrees
! Estimated noise=2.89417 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0021304 Jy
! Component: 100  -  total flux cleaned = 0.00194487 Jy
! Component: 150  -  total flux cleaned = 0.00163545 Jy
! Component: 200  -  total flux cleaned = 0.00149366 Jy
! Total flux subtracted in 200 components = 0.00149366 Jy
! Clean residual min=-0.023811 max=0.023353 Jy/beam
! Clean residual mean=-0.000128 rms=0.006450 Jy/beam
! Combined flux in latest and established models = 1.10738 Jy
selfcal
! Performing phase self-cal
! Adding 31 model components to the UV plane model.
! The established model now contains 111 components and 1.10738 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.109033Jy  sigma=1.643904
! Fit after  self-cal, rms=0.108952Jy  sigma=1.641228
flux_cutoff = imstat(rms) * dynam
! Inverting map 
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000382087 Jy
! Component: 100  -  total flux cleaned = 0.000522085 Jy
! Component: 150  -  total flux cleaned = 0.000370263 Jy
! Component: 200  -  total flux cleaned = 0.000232596 Jy
! Total flux subtracted in 200 components = 0.000232596 Jy
! Clean residual min=-0.023589 max=0.023287 Jy/beam
! Clean residual mean=-0.000125 rms=0.006407 Jy/beam
! Combined flux in latest and established models = 1.10761 Jy
! Performing phase self-cal
! Adding 35 model components to the UV plane model.
! The established model now contains 120 components and 1.10761 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.108405Jy  sigma=1.634209
! Fit after  self-cal, rms=0.108334Jy  sigma=1.631684
! 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 20 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.108334Jy  sigma=1.631684
! Fit after  self-cal, rms=0.108332Jy  sigma=1.631634
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=8.353 mas, bmaj=22.85 mas, bpa=7.943 degrees
! Estimated noise=3.28613 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000863254 Jy
! Component: 100  -  total flux cleaned = 0.00104495 Jy
! Component: 150  -  total flux cleaned = 0.00132056 Jy
! Component: 200  -  total flux cleaned = 0.000965064 Jy
! Total flux subtracted in 200 components = 0.000965064 Jy
! Clean residual min=-0.023115 max=0.026173 Jy/beam
! Clean residual mean=-0.000163 rms=0.007575 Jy/beam
! Combined flux in latest and established models = 1.10857 Jy
selfcal
! Performing phase self-cal
! Adding 22 model components to the UV plane model.
! The established model now contains 137 components and 1.10857 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.107978Jy  sigma=1.624389
! Fit after  self-cal, rms=0.107923Jy  sigma=1.622305
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 = 2.39853e-06 Jy
! Component: 100  -  total flux cleaned = 0.000133073 Jy
! Component: 150  -  total flux cleaned = -0.000125042 Jy
! Component: 200  -  total flux cleaned = -0.000459198 Jy
! Total flux subtracted in 200 components = -0.000459198 Jy
! Clean residual min=-0.023033 max=0.026041 Jy/beam
! Clean residual mean=-0.000162 rms=0.007540 Jy/beam
! Combined flux in latest and established models = 1.10812 Jy
! Performing phase self-cal
! Adding 27 model components to the UV plane model.
! The established model now contains 145 components and 1.10812 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.107610Jy  sigma=1.615569
! Fit after  self-cal, rms=0.107568Jy  sigma=1.613660
! Inverting map 
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 
! Estimated beam: bmin=4.133 mas, bmaj=16.37 mas, bpa=-11.47 degrees
! Estimated noise=2.89496 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 4.133 x 16.37 at -11.47 degrees (North through East)
! Clean map  min=-0.024135  max=0.84414 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
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.107568Jy  sigma=1.613660
! Fit after  self-cal, rms=0.104481Jy  sigma=1.566740
! Inverting map and beam 
! Estimated beam: bmin=4.14 mas, bmaj=16.39 mas, bpa=-11.43 degrees
! Estimated noise=2.88391 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00169374 Jy
! Component: 100  -  total flux cleaned = 0.000915941 Jy
! Component: 150  -  total flux cleaned = 6.90725e-05 Jy
! Component: 200  -  total flux cleaned = -0.000675159 Jy
! Total flux subtracted in 200 components = -0.000675159 Jy
! Clean residual min=-0.022851 max=0.022394 Jy/beam
! Clean residual mean=-0.000137 rms=0.006223 Jy/beam
! Combined flux in latest and established models = 1.10744 Jy
! Performing phase self-cal
! Adding 43 model components to the UV plane model.
! The established model now contains 182 components and 1.10744 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.104500Jy  sigma=1.547400
! Fit after  self-cal, rms=0.104443Jy  sigma=1.545684
! Inverting map 
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000215095 Jy
! Component: 100  -  total flux cleaned = -0.000127213 Jy
! Component: 150  -  total flux cleaned = -0.000261335 Jy
! Component: 200  -  total flux cleaned = -0.000264665 Jy
! Total flux subtracted in 200 components = -0.000264665 Jy
! Clean residual min=-0.022481 max=0.022268 Jy/beam
! Clean residual mean=-0.000134 rms=0.006162 Jy/beam
! Combined flux in latest and established models = 1.10718 Jy
! Performing phase self-cal
! Adding 40 model components to the UV plane model.
! The established model now contains 200 components and 1.10718 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.104145Jy  sigma=1.536681
! Fit after  self-cal, rms=0.104098Jy  sigma=1.534899
! Inverting map 
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.104098Jy  sigma=1.534899
! Fit after  self-cal, rms=0.104044Jy  sigma=1.534259
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 
! Estimated beam: bmin=3.584 mas, bmaj=13.5 mas, bpa=-11.28 degrees
! Estimated noise=3.57758 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.712644 Jy
! Component: 100  -  total flux cleaned = 0.926699 Jy
! Component: 150  -  total flux cleaned = 0.986658 Jy
! Component: 200  -  total flux cleaned = 1.00443 Jy
! Total flux subtracted in 200 components = 1.00443 Jy
! Clean residual min=-0.037971 max=0.041624 Jy/beam
! Clean residual mean=-0.000112 rms=0.012566 Jy/beam
! Combined flux in latest and established models = 1.00443 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 29 model components to the UV plane model.
! The established model now contains 29 components and 1.00443 Jy
! Inverting map and beam 
! Estimated beam: bmin=4.141 mas, bmaj=16.4 mas, bpa=-11.42 degrees
! Estimated noise=2.88142 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 = 0.0455183 Jy
! Component: 100  -  total flux cleaned = 0.0708182 Jy
! Component: 150  -  total flux cleaned = 0.0859519 Jy
! Component: 200  -  total flux cleaned = 0.0928091 Jy
! Total flux subtracted in 200 components = 0.0928091 Jy
! Clean residual min=-0.022227 max=0.022921 Jy/beam
! Clean residual mean=-0.000107 rms=0.006647 Jy/beam
! Combined flux in latest and established models = 1.09723 Jy
! Adding 57 model components to the UV plane model.
! The established model now contains 85 components and 1.09723 Jy
! Inverting map 
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 20 mega-wavelengths.
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=8.352 mas, bmaj=22.93 mas, bpa=7.911 degrees
! Estimated noise=3.2659 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00717523 Jy
! Component: 100  -  total flux cleaned = 0.00829717 Jy
! Component: 150  -  total flux cleaned = 0.00888605 Jy
! Component: 200  -  total flux cleaned = 0.00942583 Jy
! Total flux subtracted in 200 components = 0.00942583 Jy
! Clean residual min=-0.022861 max=0.024844 Jy/beam
! Clean residual mean=-0.000129 rms=0.007761 Jy/beam
! Combined flux in latest and established models = 1.10666 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 = 0.000327352 Jy
! Component: 100  -  total flux cleaned = 0.000774642 Jy
! Component: 150  -  total flux cleaned = 0.00104366 Jy
! Component: 200  -  total flux cleaned = 0.00143063 Jy
! Total flux subtracted in 200 components = 0.00143063 Jy
! Clean residual min=-0.022700 max=0.024607 Jy/beam
! Clean residual mean=-0.000133 rms=0.007682 Jy/beam
! Combined flux in latest and established models = 1.10809 Jy
! Adding 46 model components to the UV plane model.
! The established model now contains 124 components and 1.10809 Jy
! Inverting map 
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Estimated beam: bmin=4.141 mas, bmaj=16.4 mas, bpa=-11.42 degrees
! Estimated noise=2.88142 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000176879 Jy
! Component: 100  -  total flux cleaned = 0.000498108 Jy
! Component: 150  -  total flux cleaned = 0.000759453 Jy
! Component: 200  -  total flux cleaned = 0.000993992 Jy
! Total flux subtracted in 200 components = 0.000993992 Jy
! Clean residual min=-0.021510 max=0.022073 Jy/beam
! Clean residual mean=-0.000103 rms=0.006324 Jy/beam
! Combined flux in latest and established models = 1.10909 Jy
selfcal
! Performing phase self-cal
! Adding 26 model components to the UV plane model.
! The established model now contains 147 components and 1.10909 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.104073Jy  sigma=1.521036
! Fit after  self-cal, rms=0.103752Jy  sigma=1.516567
wmodel /J1522-2730_S_map.mod
! wmodel: Unable to open new model file: /J1522-2730_S_map.mod
! Error occured in command: wmodel
![Exited script file: /opt64/bin/pima_mupet_01.dfm]
! 
wmap /scr/pima/bg219h_uvs/J1522-2730_S_map.fits
! Inverting map 
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 4.141 x 16.4 at -11.42 degrees (North through East)
! Clean map  min=-0.022391  max=0.79743 Jy/beam
! Writing clean map to FITS file: /scr/pima/bg219h_uvs/J1522-2730_S_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is", peak_flux
! The peak flux is 0.797432 
invert
! Inverting map 
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.00627991 
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -2.36255 2.36255 4.7251 9.4502 18.9004 37.8008 75.6016
print "clev=      ", int(3*image_rms*10000)/10000
! clev=       0.0188 
print "peak=      ", int(1000*peak_flux)/1000
! peak=       0.797 
print "dyn_range= ", int(1000*peak_flux/image_rms)/1000
! dyn_range=  126.981 
quit
! Quitting program
! Log file /scr/pima/bg219h_uvs/J1522-2730_S_dfm.log closed on Thu May 19 22:31:05 2016