! Started logfile: /scr/pima/bg219a_uvs/J0019+7327_S_dfm.log on Thu May 19 23:44:20 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/bg219a_uvs/J0019+7327_S_uva.fits
! Reading UV FITS file: /scr/pima/bg219a_uvs/J0019+7327_S_uva.fits
! AN table 1: 18 integrations on 15 of 15 possible baselines.
! Apparent sampling: 0.833333 visibilities/baseline/integration-bin.
! Found source: J0019+7327
! 
! 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 49 lines of history.
! 
! Reading 900 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 J0019+7327_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 20 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 20 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 20 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 20 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=1.233425Jy  sigma=24.364619
! Fit after  self-cal, rms=0.454703Jy  sigma=8.610235
! 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=2.182 mas, bmaj=9.063 mas, bpa=79.41 degrees
! Estimated noise=1.69041 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 = 0.425446 Jy
! Component: 100  -  total flux cleaned = 0.53743 Jy
! Total flux subtracted in 100 components = 0.53743 Jy
! Clean residual min=-0.028466 max=0.046310 Jy/beam
! Clean residual mean=-0.000017 rms=0.008642 Jy/beam
! Combined flux in latest and established models = 0.53743 Jy
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 14 components and 0.53743 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.156954Jy  sigma=3.094014
! Fit after  self-cal, rms=0.157010Jy  sigma=3.082036
! 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=2.51 mas, bmaj=10.21 mas, bpa=78.75 degrees
! Estimated noise=1.33538 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 = 0.0682064 Jy
! Component: 100  -  total flux cleaned = 0.103176 Jy
! Component: 150  -  total flux cleaned = 0.122844 Jy
! Component: 200  -  total flux cleaned = 0.134174 Jy
! Total flux subtracted in 200 components = 0.134174 Jy
! Clean residual min=-0.011305 max=0.014070 Jy/beam
! Clean residual mean=0.000003 rms=0.003167 Jy/beam
! Combined flux in latest and established models = 0.671605 Jy
! Performing phase self-cal
! Adding 35 model components to the UV plane model.
! The established model now contains 46 components and 0.671605 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.127004Jy  sigma=2.481478
! Fit after  self-cal, rms=0.127019Jy  sigma=2.480328
! Inverting map 
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 2.51 x 10.21 at 78.75 degrees (North through East)
! Clean map  min=-0.010864  max=0.57231 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:
!   LA        0.98     MK        1.04     NL        0.98     OV        1.03     
!   PT        0.98     SC        1.06     
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   LA        0.99     MK        1.01     NL        0.99     OV        1.01     
!   PT        0.98     SC        1.02     
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   LA        1.00     MK        1.02     NL        0.97     OV        1.04     
!   PT        0.96     SC        1.01     
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   LA        0.95     MK        0.98     NL        0.97     OV        1.01     
!   PT        0.95     SC        0.99     
! 
! 
! Fit before self-cal, rms=0.127019Jy  sigma=2.480328
! Fit after  self-cal, rms=0.125781Jy  sigma=2.438311
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=2.526 mas, bmaj=10.24 mas, bpa=78.79 degrees
! Estimated noise=1.32937 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 (80, 39.5).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0041765 Jy
! Component: 100  -  total flux cleaned = 0.00440161 Jy
! Component: 150  -  total flux cleaned = 0.00498355 Jy
! Component: 200  -  total flux cleaned = 0.00500637 Jy
! Total flux subtracted in 200 components = 0.00500637 Jy
! Clean residual min=-0.006048 max=0.006568 Jy/beam
! Clean residual mean=-0.000005 rms=0.001570 Jy/beam
! Combined flux in latest and established models = 0.676611 Jy
! Performing phase self-cal
! Adding 22 model components to the UV plane model.
! The established model now contains 68 components and 0.676611 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.124864Jy  sigma=2.425487
! Fit after  self-cal, rms=0.124852Jy  sigma=2.424521
! 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=0.124852Jy  sigma=2.424521
! Fit after  self-cal, rms=0.124558Jy  sigma=2.419855
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=2.524 mas, bmaj=10.25 mas, bpa=78.77 degrees
! Estimated noise=1.32676 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00213061 Jy
! Component: 100  -  total flux cleaned = 0.00213355 Jy
! Component: 150  -  total flux cleaned = 0.00173946 Jy
! Component: 200  -  total flux cleaned = 0.00131331 Jy
! Total flux subtracted in 200 components = 0.00131331 Jy
! Clean residual min=-0.005852 max=0.005322 Jy/beam
! Clean residual mean=-0.000006 rms=0.001375 Jy/beam
! Combined flux in latest and established models = 0.677924 Jy
selfcal
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 79 components and 0.677924 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.124420Jy  sigma=2.417786
! Fit after  self-cal, rms=0.124409Jy  sigma=2.417688
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 = -0.000437463 Jy
! Component: 100  -  total flux cleaned = -0.000629788 Jy
! Component: 150  -  total flux cleaned = -0.00086652 Jy
! Component: 200  -  total flux cleaned = -0.000975845 Jy
! Total flux subtracted in 200 components = -0.000975845 Jy
! Clean residual min=-0.005847 max=0.005383 Jy/beam
! Clean residual mean=-0.000005 rms=0.001348 Jy/beam
! Combined flux in latest and established models = 0.676948 Jy
! Performing phase self-cal
! Adding 23 model components to the UV plane model.
! The established model now contains 91 components and 0.676948 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.124352Jy  sigma=2.416806
! Fit after  self-cal, rms=0.124345Jy  sigma=2.416781
! 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=0.124345Jy  sigma=2.416781
! Fit after  self-cal, rms=0.124337Jy  sigma=2.416499
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=2.525 mas, bmaj=10.24 mas, bpa=78.78 degrees
! Estimated noise=1.32606 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000161156 Jy
! Component: 100  -  total flux cleaned = -1.50123e-05 Jy
! Component: 150  -  total flux cleaned = -0.000122066 Jy
! Component: 200  -  total flux cleaned = -0.000171578 Jy
! Total flux subtracted in 200 components = -0.000171578 Jy
! Clean residual min=-0.005687 max=0.005238 Jy/beam
! Clean residual mean=-0.000006 rms=0.001319 Jy/beam
! Combined flux in latest and established models = 0.676777 Jy
selfcal
! Performing phase self-cal
! Adding 22 model components to the UV plane model.
! The established model now contains 99 components and 0.676777 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.124284Jy  sigma=2.415732
! Fit after  self-cal, rms=0.124281Jy  sigma=2.415702
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 = -4.46018e-05 Jy
! Component: 100  -  total flux cleaned = -9.24859e-05 Jy
! Component: 150  -  total flux cleaned = -0.000136239 Jy
! Component: 200  -  total flux cleaned = -0.000136938 Jy
! Total flux subtracted in 200 components = -0.000136938 Jy
! Clean residual min=-0.005734 max=0.005332 Jy/beam
! Clean residual mean=-0.000006 rms=0.001307 Jy/beam
! Combined flux in latest and established models = 0.67664 Jy
! Performing phase self-cal
! Adding 22 model components to the UV plane model.
! The established model now contains 105 components and 0.67664 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.124251Jy  sigma=2.415211
! Fit after  self-cal, rms=0.124250Jy  sigma=2.415193
! 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=0.124250Jy  sigma=2.415193
! Fit after  self-cal, rms=0.124244Jy  sigma=2.415030
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=5.76 mas, bmaj=20.33 mas, bpa=71.13 degrees
! Estimated noise=1.81792 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000270256 Jy
! Component: 100  -  total flux cleaned = -4.30503e-05 Jy
! Component: 150  -  total flux cleaned = -0.000278216 Jy
! Component: 200  -  total flux cleaned = -0.000493052 Jy
! Total flux subtracted in 200 components = -0.000493052 Jy
! Clean residual min=-0.004469 max=0.004437 Jy/beam
! Clean residual mean=-0.000009 rms=0.001254 Jy/beam
! Combined flux in latest and established models = 0.676147 Jy
selfcal
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 115 components and 0.676147 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.124243Jy  sigma=2.415213
! Fit after  self-cal, rms=0.124248Jy  sigma=2.415170
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 = -0.000103054 Jy
! Component: 100  -  total flux cleaned = -0.000333773 Jy
! Component: 150  -  total flux cleaned = -0.000514198 Jy
! Component: 200  -  total flux cleaned = -0.000656101 Jy
! Total flux subtracted in 200 components = -0.000656101 Jy
! Clean residual min=-0.004463 max=0.004352 Jy/beam
! Clean residual mean=-0.000008 rms=0.001233 Jy/beam
! Combined flux in latest and established models = 0.675491 Jy
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 122 components and 0.675491 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.124249Jy  sigma=2.415157
! Fit after  self-cal, rms=0.124245Jy  sigma=2.415132
! 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=2.525 mas, bmaj=10.24 mas, bpa=78.79 degrees
! Estimated noise=1.32589 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 2.525 x 10.24 at 78.79 degrees (North through East)
! Clean map  min=-0.0066378  max=0.56957 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=0.124245Jy  sigma=2.415132
! Fit after  self-cal, rms=0.121540Jy  sigma=2.359597
! Inverting map and beam 
! Estimated beam: bmin=2.527 mas, bmaj=10.26 mas, bpa=78.72 degrees
! Estimated noise=1.3268 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000765284 Jy
! Component: 100  -  total flux cleaned = -0.00101938 Jy
! Component: 150  -  total flux cleaned = -0.000930587 Jy
! Component: 200  -  total flux cleaned = -0.000930455 Jy
! Total flux subtracted in 200 components = -0.000930455 Jy
! Clean residual min=-0.005707 max=0.005142 Jy/beam
! Clean residual mean=-0.000005 rms=0.001272 Jy/beam
! Combined flux in latest and established models = 0.67456 Jy
! Performing phase self-cal
! Adding 25 model components to the UV plane model.
! The established model now contains 139 components and 0.67456 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.121507Jy  sigma=2.358748
! Fit after  self-cal, rms=0.121500Jy  sigma=2.358716
! Inverting map 
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 2.55167e-05 Jy
! Component: 100  -  total flux cleaned = 0.000180106 Jy
! Component: 150  -  total flux cleaned = 0.000216871 Jy
! Component: 200  -  total flux cleaned = 0.000218075 Jy
! Total flux subtracted in 200 components = 0.000218075 Jy
! Clean residual min=-0.005669 max=0.005130 Jy/beam
! Clean residual mean=-0.000005 rms=0.001262 Jy/beam
! Combined flux in latest and established models = 0.674778 Jy
! Performing phase self-cal
! Adding 26 model components to the UV plane model.
! The established model now contains 151 components and 0.674778 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.121478Jy  sigma=2.358318
! Fit after  self-cal, rms=0.121477Jy  sigma=2.358303
! Inverting map 
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.121477Jy  sigma=2.358303
! Fit after  self-cal, rms=0.121483Jy  sigma=2.358279
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=2.192 mas, bmaj=9.091 mas, bpa=79.38 degrees
! Estimated noise=1.6919 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.425979 Jy
! Component: 100  -  total flux cleaned = 0.536102 Jy
! Component: 150  -  total flux cleaned = 0.586716 Jy
! Component: 200  -  total flux cleaned = 0.615345 Jy
! Total flux subtracted in 200 components = 0.615345 Jy
! Clean residual min=-0.014924 max=0.015467 Jy/beam
! Clean residual mean=-0.000010 rms=0.003942 Jy/beam
! Combined flux in latest and established models = 0.615345 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 34 model components to the UV plane model.
! The established model now contains 34 components and 0.615345 Jy
! Inverting map and beam 
! Estimated beam: bmin=2.528 mas, bmaj=10.26 mas, bpa=78.73 degrees
! Estimated noise=1.32683 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 = 0.0243131 Jy
! Component: 100  -  total flux cleaned = 0.0355278 Jy
! Component: 150  -  total flux cleaned = 0.0432189 Jy
! Component: 200  -  total flux cleaned = 0.0490578 Jy
! Total flux subtracted in 200 components = 0.0490578 Jy
! Clean residual min=-0.007630 max=0.006877 Jy/beam
! Clean residual mean=-0.000007 rms=0.001886 Jy/beam
! Combined flux in latest and established models = 0.664403 Jy
! Adding 45 model components to the UV plane model.
! The established model now contains 72 components and 0.664403 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=5.76 mas, bmaj=20.35 mas, bpa=71.1 degrees
! Estimated noise=1.816 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00837559 Jy
! Component: 100  -  total flux cleaned = 0.00987654 Jy
! Component: 150  -  total flux cleaned = 0.0107383 Jy
! Component: 200  -  total flux cleaned = 0.0114911 Jy
! Total flux subtracted in 200 components = 0.0114911 Jy
! Clean residual min=-0.005360 max=0.005004 Jy/beam
! Clean residual mean=-0.000007 rms=0.001551 Jy/beam
! Combined flux in latest and established models = 0.675894 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 = 0.000416142 Jy
! Component: 100  -  total flux cleaned = 0.000491715 Jy
! Component: 150  -  total flux cleaned = 0.000375909 Jy
! Component: 200  -  total flux cleaned = 0.000215459 Jy
! Total flux subtracted in 200 components = 0.000215459 Jy
! Clean residual min=-0.005245 max=0.004501 Jy/beam
! Clean residual mean=-0.000007 rms=0.001368 Jy/beam
! Combined flux in latest and established models = 0.676109 Jy
! Adding 66 model components to the UV plane model.
! The established model now contains 131 components and 0.676109 Jy
! Inverting map 
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Estimated beam: bmin=2.528 mas, bmaj=10.26 mas, bpa=78.73 degrees
! Estimated noise=1.32683 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.00111196 Jy
! Component: 100  -  total flux cleaned = -0.00133682 Jy
! Component: 150  -  total flux cleaned = -0.0017214 Jy
! Component: 200  -  total flux cleaned = -0.00223327 Jy
! Total flux subtracted in 200 components = -0.00223327 Jy
! Clean residual min=-0.006045 max=0.005109 Jy/beam
! Clean residual mean=-0.000004 rms=0.001329 Jy/beam
! Combined flux in latest and established models = 0.673876 Jy
selfcal
! Performing phase self-cal
! Adding 19 model components to the UV plane model.
! The established model now contains 149 components and 0.673876 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.121638Jy  sigma=2.360554
! Fit after  self-cal, rms=0.121619Jy  sigma=2.360171
wmodel /J0019+7327_S_map.mod
! wmodel: Unable to open new model file: /J0019+7327_S_map.mod
! Error occured in command: wmodel
![Exited script file: /opt64/bin/pima_mupet_01.dfm]
! 
wmap /scr/pima/bg219a_uvs/J0019+7327_S_map.fits
! Inverting map 
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 2.528 x 10.26 at 78.73 degrees (North through East)
! Clean map  min=-0.0060369  max=0.56833 Jy/beam
! Writing clean map to FITS file: /scr/pima/bg219a_uvs/J0019+7327_S_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is", peak_flux
! The peak flux is 0.568333 
invert
! Inverting map 
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.00131791 
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.69567 0.69567 1.39134 2.78268 5.56536 11.1307 22.2615 44.5229 89.0458
print "clev=      ", int(3*image_rms*10000)/10000
! clev=       0.0039 
print "peak=      ", int(1000*peak_flux)/1000
! peak=       0.568 
print "dyn_range= ", int(1000*peak_flux/image_rms)/1000
! dyn_range=  431.238 
quit
! Quitting program
! Log file /scr/pima/bg219a_uvs/J0019+7327_S_dfm.log closed on Thu May 19 23:44:23 2016