! Started logfile: /scr/pima/bg219i_uvs/J1333-1112_S_dfm.log on Thu May 19 23:21:59 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/bg219i_uvs/J1333-1112_S_uva.fits
! Reading UV FITS file: /scr/pima/bg219i_uvs/J1333-1112_S_uva.fits
! AN table 1: 31 integrations on 36 of 36 possible baselines.
! AN table 2: 31 integrations on 36 of 36 possible baselines.
! Apparent sampling: 0.916667 visibilities/baseline/integration-bin.
! Found source: J1333-1112
! 
! 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 8184 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 J1333-1112_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 27 telescope corrections were flagged in sub-array 1.
!  A total of 27 telescope corrections were flagged in sub-array 2.
! 
! Correcting IF 2.
!  A total of 27 telescope corrections were flagged in sub-array 1.
!  A total of 27 telescope corrections were flagged in sub-array 2.
! 
! Correcting IF 3.
!  A total of 27 telescope corrections were flagged in sub-array 1.
!  A total of 27 telescope corrections were flagged in sub-array 2.
! 
! Correcting IF 4.
!  A total of 27 telescope corrections were flagged in sub-array 1.
!  A total of 27 telescope corrections were flagged in sub-array 2.
! 
! Fit before self-cal, rms=1.004624Jy  sigma=21.535140
! Fit after  self-cal, rms=0.951540Jy  sigma=20.417402
! 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=3.382 mas, bmaj=8.223 mas, bpa=2.648 degrees
! Estimated noise=0.600966 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 = 0.036661 Jy
! Component: 100  -  total flux cleaned = 0.0471463 Jy
! Total flux subtracted in 100 components = 0.0471463 Jy
! Clean residual min=-0.004165 max=0.004831 Jy/beam
! Clean residual mean=-0.000015 rms=0.001017 Jy/beam
! Combined flux in latest and established models = 0.0471463 Jy
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 16 components and 0.0471463 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067897Jy  sigma=1.349716
! Fit after  self-cal, rms=0.066197Jy  sigma=1.317844
! Inverting map 
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00694918 Jy
! Component: 100  -  total flux cleaned = 0.0103907 Jy
! Total flux subtracted in 100 components = 0.0103907 Jy
! Clean residual min=-0.002850 max=0.004102 Jy/beam
! Clean residual mean=-0.000009 rms=0.000816 Jy/beam
! Combined flux in latest and established models = 0.057537 Jy
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 28 components and 0.057537 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.065368Jy  sigma=1.299515
! Fit after  self-cal, rms=0.065294Jy  sigma=1.298841
! 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=4.092 mas, bmaj=9.705 mas, bpa=1.197 degrees
! Estimated noise=0.393673 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 (5, 6.5).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00441408 Jy
! Component: 100  -  total flux cleaned = 0.00647145 Jy
! Component: 150  -  total flux cleaned = 0.00777266 Jy
! Component: 200  -  total flux cleaned = 0.00833642 Jy
! Total flux subtracted in 200 components = 0.00833642 Jy
! Clean residual min=-0.002084 max=0.002512 Jy/beam
! Clean residual mean=-0.000005 rms=0.000580 Jy/beam
! Combined flux in latest and established models = 0.0658734 Jy
! Performing phase self-cal
! Adding 41 model components to the UV plane model.
! The established model now contains 69 components and 0.0658734 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.065013Jy  sigma=1.292391
! Fit after  self-cal, rms=0.064950Jy  sigma=1.290895
! Inverting map 
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 4.092 x 9.705 at 1.197 degrees (North through East)
! Clean map  min=-0.0019179  max=0.049274 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*    
!   SC        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.04     FD        0.93     HN        1.00     KP        0.95     
!   LA        0.92     NL        1.18     OV        1.02     PT        0.93     
!   SC        1.12     
! 
! 
! Correcting IF 2.
!  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*    
!   SC        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.08     FD        0.97     HN        0.89     KP        1.06     
!   LA        0.96     NL        0.96     OV        0.99     PT        0.99     
!   SC        1.05     
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.89     FD        0.99     KP        1.01     LA        0.95     
!   MK        1.01     NL        1.09     OV        1.02     PT        0.99     
!   SC        0.87     
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.07     FD        0.88     HN        1.04     KP        1.02     
!   LA        1.03     NL        0.95     OV        0.95     PT        1.17     
!   SC        1.03     
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.98     FD        0.97     KP        1.02     LA        0.97     
!   MK        0.89     NL        1.07     OV        1.00     PT        0.94     
!   SC        0.84     
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.02     FD        0.92     HN        0.91     KP        0.90     
!   LA        0.96     NL        1.07     OV        0.99     PT        1.00     
!   SC        1.04     
! 
! 
! Fit before self-cal, rms=0.064950Jy  sigma=1.290895
! Fit after  self-cal, rms=0.064217Jy  sigma=1.288176
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=4.09 mas, bmaj=9.697 mas, bpa=0.5675 degrees
! Estimated noise=0.387699 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 = 0.00100323 Jy
! Component: 100  -  total flux cleaned = 0.00127392 Jy
! Component: 150  -  total flux cleaned = 0.00135948 Jy
! Component: 200  -  total flux cleaned = 0.00143442 Jy
! Total flux subtracted in 200 components = 0.00143442 Jy
! Clean residual min=-0.001720 max=0.001851 Jy/beam
! Clean residual mean=0.000003 rms=0.000498 Jy/beam
! Combined flux in latest and established models = 0.0673078 Jy
! Performing phase self-cal
! Adding 22 model components to the UV plane model.
! The established model now contains 86 components and 0.0673078 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.064183Jy  sigma=1.287371
! Fit after  self-cal, rms=0.064235Jy  sigma=1.286933
! 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=0.064235Jy  sigma=1.286933
! Fit after  self-cal, rms=0.064129Jy  sigma=1.285818
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=4.098 mas, bmaj=9.674 mas, bpa=0.5673 degrees
! Estimated noise=0.386617 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000123293 Jy
! Component: 100  -  total flux cleaned = 0.000149591 Jy
! Component: 150  -  total flux cleaned = 0.000194086 Jy
! Component: 200  -  total flux cleaned = 0.000233244 Jy
! Total flux subtracted in 200 components = 0.000233244 Jy
! Clean residual min=-0.001629 max=0.001560 Jy/beam
! Clean residual mean=0.000001 rms=0.000475 Jy/beam
! Combined flux in latest and established models = 0.0675411 Jy
selfcal
! Performing phase self-cal
! Adding 20 model components to the UV plane model.
! The established model now contains 97 components and 0.0675411 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.064109Jy  sigma=1.285434
! Fit after  self-cal, rms=0.064125Jy  sigma=1.285274
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 = 0.000133013 Jy
! Component: 100  -  total flux cleaned = 0.000193853 Jy
! Component: 150  -  total flux cleaned = 0.000248334 Jy
! Component: 200  -  total flux cleaned = 0.000281858 Jy
! Total flux subtracted in 200 components = 0.000281858 Jy
! Clean residual min=-0.001639 max=0.001558 Jy/beam
! Clean residual mean=0.000001 rms=0.000472 Jy/beam
! Combined flux in latest and established models = 0.0678229 Jy
! Performing phase self-cal
! Adding 23 model components to the UV plane model.
! The established model now contains 108 components and 0.0678229 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.064113Jy  sigma=1.285054
! Fit after  self-cal, rms=0.064117Jy  sigma=1.285021
! 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=0.064117Jy  sigma=1.285021
! Fit after  self-cal, rms=0.063818Jy  sigma=1.284957
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=4.104 mas, bmaj=9.674 mas, bpa=0.5231 degrees
! Estimated noise=0.384596 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -6.79562e-05 Jy
! Component: 100  -  total flux cleaned = -6.82961e-05 Jy
! Component: 150  -  total flux cleaned = -3.51047e-05 Jy
! Component: 200  -  total flux cleaned = 2.59476e-05 Jy
! Total flux subtracted in 200 components = 2.59476e-05 Jy
! Clean residual min=-0.001636 max=0.001536 Jy/beam
! Clean residual mean=0.000001 rms=0.000465 Jy/beam
! Combined flux in latest and established models = 0.0678489 Jy
selfcal
! Performing phase self-cal
! Adding 29 model components to the UV plane model.
! The established model now contains 117 components and 0.0678489 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.063806Jy  sigma=1.284729
! Fit after  self-cal, rms=0.063810Jy  sigma=1.284668
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 = 8.21425e-05 Jy
! Component: 100  -  total flux cleaned = 0.000132335 Jy
! Component: 150  -  total flux cleaned = 0.000147258 Jy
! Component: 200  -  total flux cleaned = 0.00017542 Jy
! Total flux subtracted in 200 components = 0.00017542 Jy
! Clean residual min=-0.001641 max=0.001524 Jy/beam
! Clean residual mean=0.000001 rms=0.000463 Jy/beam
! Combined flux in latest and established models = 0.0680243 Jy
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 119 components and 0.0680243 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.063800Jy  sigma=1.284526
! Fit after  self-cal, rms=0.063803Jy  sigma=1.284507
! 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=0.063803Jy  sigma=1.284507
! Fit after  self-cal, rms=0.063788Jy  sigma=1.283841
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=8.237 mas, bmaj=14.21 mas, bpa=5.109 degrees
! Estimated noise=0.464737 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -1.85546e-05 Jy
! Component: 100  -  total flux cleaned = -7.81525e-05 Jy
! Component: 150  -  total flux cleaned = -0.000149215 Jy
! Component: 200  -  total flux cleaned = -0.000168971 Jy
! Total flux subtracted in 200 components = -0.000168971 Jy
! Clean residual min=-0.002167 max=0.002008 Jy/beam
! Clean residual mean=0.000001 rms=0.000595 Jy/beam
! Combined flux in latest and established models = 0.0678554 Jy
selfcal
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 128 components and 0.0678554 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.063783Jy  sigma=1.283801
! Fit after  self-cal, rms=0.063796Jy  sigma=1.283713
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 = -1.18133e-05 Jy
! Component: 100  -  total flux cleaned = -2.36284e-05 Jy
! Component: 150  -  total flux cleaned = -5.34436e-05 Jy
! Component: 200  -  total flux cleaned = -6.22263e-05 Jy
! Total flux subtracted in 200 components = -6.22263e-05 Jy
! Clean residual min=-0.002129 max=0.001995 Jy/beam
! Clean residual mean=0.000001 rms=0.000594 Jy/beam
! Combined flux in latest and established models = 0.0677931 Jy
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 133 components and 0.0677931 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.063792Jy  sigma=1.283713
! Fit after  self-cal, rms=0.063797Jy  sigma=1.283692
! 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=4.107 mas, bmaj=9.66 mas, bpa=0.6019 degrees
! Estimated noise=0.385116 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 4.107 x 9.66 at 0.6019 degrees (North through East)
! Clean map  min=-0.0016268  max=0.047231 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 
! Estimated beam: bmin=3.399 mas, bmaj=8.145 mas, bpa=2.002 degrees
! Estimated noise=0.587884 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0376044 Jy
! Component: 100  -  total flux cleaned = 0.0493646 Jy
! Component: 150  -  total flux cleaned = 0.0555391 Jy
! Component: 200  -  total flux cleaned = 0.0595859 Jy
! Total flux subtracted in 200 components = 0.0595859 Jy
! Clean residual min=-0.002530 max=0.003145 Jy/beam
! Clean residual mean=-0.000004 rms=0.000719 Jy/beam
! Combined flux in latest and established models = 0.0595859 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 27 model components to the UV plane model.
! The established model now contains 27 components and 0.0595859 Jy
! Inverting map and beam 
! Estimated beam: bmin=4.107 mas, bmaj=9.66 mas, bpa=0.6019 degrees
! Estimated noise=0.385116 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)
! Added new window around map position (11, 11.5).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00362411 Jy
! Component: 100  -  total flux cleaned = 0.0055253 Jy
! Component: 150  -  total flux cleaned = 0.00667097 Jy
! Component: 200  -  total flux cleaned = 0.00710937 Jy
! Total flux subtracted in 200 components = 0.00710937 Jy
! Clean residual min=-0.001656 max=0.001713 Jy/beam
! Clean residual mean=-0.000000 rms=0.000472 Jy/beam
! Combined flux in latest and established models = 0.0666953 Jy
! Adding 38 model components to the UV plane model.
! The established model now contains 65 components and 0.0666953 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=8.237 mas, bmaj=14.21 mas, bpa=5.109 degrees
! Estimated noise=0.464737 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000571222 Jy
! Component: 100  -  total flux cleaned = 0.000813741 Jy
! Component: 150  -  total flux cleaned = 0.0010142 Jy
! Component: 200  -  total flux cleaned = 0.00111315 Jy
! Total flux subtracted in 200 components = 0.00111315 Jy
! Clean residual min=-0.002167 max=0.002074 Jy/beam
! Clean residual mean=0.000000 rms=0.000594 Jy/beam
! Combined flux in latest and established models = 0.0678084 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 = 5.79759e-05 Jy
! Component: 100  -  total flux cleaned = 7.79739e-05 Jy
! Component: 150  -  total flux cleaned = 8.70003e-05 Jy
! Component: 200  -  total flux cleaned = 9.5644e-05 Jy
! Total flux subtracted in 200 components = 9.5644e-05 Jy
! Clean residual min=-0.002154 max=0.002054 Jy/beam
! Clean residual mean=0.000000 rms=0.000591 Jy/beam
! Combined flux in latest and established models = 0.0679041 Jy
! Adding 51 model components to the UV plane model.
! The established model now contains 115 components and 0.0679041 Jy
! Inverting map 
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Estimated beam: bmin=4.107 mas, bmaj=9.66 mas, bpa=0.6019 degrees
! Estimated noise=0.385116 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -2.52775e-05 Jy
! Component: 100  -  total flux cleaned = -1.40949e-06 Jy
! Component: 150  -  total flux cleaned = 3.63609e-05 Jy
! Component: 200  -  total flux cleaned = 5.37202e-05 Jy
! Total flux subtracted in 200 components = 5.37202e-05 Jy
! Clean residual min=-0.001613 max=0.001676 Jy/beam
! Clean residual mean=-0.000001 rms=0.000453 Jy/beam
! Combined flux in latest and established models = 0.0679578 Jy
selfcal
! Performing phase self-cal
! Adding 26 model components to the UV plane model.
! The established model now contains 138 components and 0.0679578 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.063793Jy  sigma=1.283606
! Fit after  self-cal, rms=0.063785Jy  sigma=1.283447
wmodel /J1333-1112_S_map.mod
! wmodel: Unable to open new model file: /J1333-1112_S_map.mod
! Error occured in command: wmodel
![Exited script file: /opt64/bin/pima_mupet_01.dfm]
! 
wmap /scr/pima/bg219i_uvs/J1333-1112_S_map.fits
! Inverting map 
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 4.107 x 9.66 at 0.6019 degrees (North through East)
! Clean map  min=-0.0015879  max=0.046884 Jy/beam
! Writing clean map to FITS file: /scr/pima/bg219i_uvs/J1333-1112_S_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is", peak_flux
! The peak flux is 0.0468837 
invert
! Inverting map 
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.00045297 
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -2.89847 2.89847 5.79695 11.5939 23.1878 46.3756 92.7511
print "clev=      ", int(3*image_rms*10000)/10000
! clev=       0.0013 
print "peak=      ", int(1000*peak_flux)/1000
! peak=       0.046 
print "dyn_range= ", int(1000*peak_flux/image_rms)/1000
! dyn_range=  103.502 
quit
! Quitting program
! Log file /scr/pima/bg219i_uvs/J1333-1112_S_dfm.log closed on Thu May 19 23:22:01 2016