! Started logfile: /scr/pima/bg219g_uvs/J1333-1950_S_dfm.log on Thu May 19 21:48:08 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/bg219g_uvs/J1333-1950_S_uva.fits
! Reading UV FITS file: /scr/pima/bg219g_uvs/J1333-1950_S_uva.fits
! AN table 1: 26 integrations on 21 of 21 possible baselines.
! Apparent sampling: 0.943223 visibilities/baseline/integration-bin.
! Found source: J1333-1950
! 
! 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 2060 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 J1333-1950_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=1.021093Jy  sigma=21.273432
! Fit after  self-cal, rms=0.763060Jy  sigma=15.856686
! 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=3.171 mas, bmaj=13.78 mas, bpa=-11.66 degrees
! Estimated noise=0.969825 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 = 0.181911 Jy
! Component: 100  -  total flux cleaned = 0.221752 Jy
! Total flux subtracted in 100 components = 0.221752 Jy
! Clean residual min=-0.008002 max=0.013530 Jy/beam
! Clean residual mean=0.000094 rms=0.002926 Jy/beam
! Combined flux in latest and established models = 0.221752 Jy
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 6 components and 0.221752 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.074255Jy  sigma=1.459157
! Fit after  self-cal, rms=0.074236Jy  sigma=1.458995
! Inverting map 
print "************** FINISHED UNIFORM WEIGHTING CLEAN **************"
! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** 
! 
uvw 0,-1
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
win_mult = win_mult * 1.6
clean_niter = clean_niter * 2
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=3.76 mas, bmaj=15.32 mas, bpa=-10.46 degrees
! Estimated noise=0.801438 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 = 0.0167182 Jy
! Component: 100  -  total flux cleaned = 0.0244699 Jy
! Component: 150  -  total flux cleaned = 0.0288094 Jy
! Component: 200  -  total flux cleaned = 0.0315116 Jy
! Total flux subtracted in 200 components = 0.0315116 Jy
! Clean residual min=-0.007356 max=0.005991 Jy/beam
! Clean residual mean=0.000054 rms=0.001927 Jy/beam
! Combined flux in latest and established models = 0.253263 Jy
! Performing phase self-cal
! Adding 39 model components to the UV plane model.
! The established model now contains 42 components and 0.253263 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.070218Jy  sigma=1.390981
! Fit after  self-cal, rms=0.070159Jy  sigma=1.390529
! Inverting map 
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 3.76 x 15.32 at -10.46 degrees (North through East)
! Clean map  min=-0.0071629  max=0.23718 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     KP        0.97     LA        0.89     MK        1.02     
!   NL        1.15     OV        1.02     PT        1.00     
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.99     KP        0.99     LA        0.91     MK        0.99     
!   NL        1.10     OV        1.01     PT        1.01     
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.99     KP        0.98     LA        0.94     MK        0.99     
!   NL        0.85     OV        1.01     PT        1.04     
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00     KP        1.00     LA        0.93     MK        1.00     
!   NL        1.08     OV        1.02     PT        1.05     
! 
! 
! Fit before self-cal, rms=0.070159Jy  sigma=1.390529
! Fit after  self-cal, rms=0.066294Jy  sigma=1.336034
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=3.767 mas, bmaj=15.34 mas, bpa=-10.46 degrees
! Estimated noise=0.796687 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 = 0.000339979 Jy
! Component: 100  -  total flux cleaned = 0.000206979 Jy
! Component: 150  -  total flux cleaned = 0.000170205 Jy
! Component: 200  -  total flux cleaned = 0.000138484 Jy
! Total flux subtracted in 200 components = 0.000138484 Jy
! Clean residual min=-0.003476 max=0.003515 Jy/beam
! Clean residual mean=-0.000012 rms=0.000990 Jy/beam
! Combined flux in latest and established models = 0.253402 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 49 components and 0.253402 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066239Jy  sigma=1.335136
! Fit after  self-cal, rms=0.066265Jy  sigma=1.334712
! 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=0.066265Jy  sigma=1.334712
! Fit after  self-cal, rms=0.066264Jy  sigma=1.334689
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=3.768 mas, bmaj=15.33 mas, bpa=-10.46 degrees
! Estimated noise=0.796497 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 1.02214e-05 Jy
! Component: 100  -  total flux cleaned = -2.43203e-05 Jy
! Component: 150  -  total flux cleaned = 1.32382e-06 Jy
! Component: 200  -  total flux cleaned = 7.18027e-07 Jy
! Total flux subtracted in 200 components = 7.18027e-07 Jy
! Clean residual min=-0.003429 max=0.003423 Jy/beam
! Clean residual mean=-0.000012 rms=0.000968 Jy/beam
! Combined flux in latest and established models = 0.253402 Jy
selfcal
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 53 components and 0.253402 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066235Jy  sigma=1.334245
! Fit after  self-cal, rms=0.066236Jy  sigma=1.334218
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 = -8.66435e-06 Jy
! Component: 100  -  total flux cleaned = 1.56882e-05 Jy
! Component: 150  -  total flux cleaned = 6.11722e-05 Jy
! Component: 200  -  total flux cleaned = 6.2041e-05 Jy
! Total flux subtracted in 200 components = 6.2041e-05 Jy
! Clean residual min=-0.003358 max=0.003391 Jy/beam
! Clean residual mean=-0.000013 rms=0.000956 Jy/beam
! Combined flux in latest and established models = 0.253465 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 55 components and 0.253464 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066218Jy  sigma=1.333941
! Fit after  self-cal, rms=0.066218Jy  sigma=1.333933
! 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=0.066218Jy  sigma=1.333933
! Fit after  self-cal, rms=0.066213Jy  sigma=1.333919
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=3.769 mas, bmaj=15.32 mas, bpa=-10.46 degrees
! Estimated noise=0.796293 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000136844 Jy
! Component: 100  -  total flux cleaned = 0.000157913 Jy
! Component: 150  -  total flux cleaned = 0.000157867 Jy
! Component: 200  -  total flux cleaned = 0.000158363 Jy
! Total flux subtracted in 200 components = 0.000158363 Jy
! Clean residual min=-0.003293 max=0.003349 Jy/beam
! Clean residual mean=-0.000013 rms=0.000944 Jy/beam
! Combined flux in latest and established models = 0.253623 Jy
selfcal
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 56 components and 0.253623 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066200Jy  sigma=1.333679
! Fit after  self-cal, rms=0.066200Jy  sigma=1.333675
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 = 4.13723e-05 Jy
! Component: 100  -  total flux cleaned = 6.08355e-05 Jy
! Component: 150  -  total flux cleaned = 6.13248e-05 Jy
! Component: 200  -  total flux cleaned = 6.12933e-05 Jy
! Total flux subtracted in 200 components = 6.12933e-05 Jy
! Clean residual min=-0.003245 max=0.003369 Jy/beam
! Clean residual mean=-0.000013 rms=0.000936 Jy/beam
! Combined flux in latest and established models = 0.253684 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 57 components and 0.253684 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066190Jy  sigma=1.333488
! Fit after  self-cal, rms=0.066190Jy  sigma=1.333486
! 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=0.066190Jy  sigma=1.333486
! Fit after  self-cal, rms=0.066188Jy  sigma=1.333470
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=8.461 mas, bmaj=18.62 mas, bpa=7.905 degrees
! Estimated noise=0.979029 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 8.58027e-05 Jy
! Component: 100  -  total flux cleaned = 0.000103474 Jy
! Component: 150  -  total flux cleaned = 0.000140265 Jy
! Component: 200  -  total flux cleaned = 0.000171552 Jy
! Total flux subtracted in 200 components = 0.000171552 Jy
! Clean residual min=-0.003808 max=0.003769 Jy/beam
! Clean residual mean=-0.000022 rms=0.001227 Jy/beam
! Combined flux in latest and established models = 0.253856 Jy
selfcal
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 67 components and 0.253856 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066181Jy  sigma=1.333470
! Fit after  self-cal, rms=0.066183Jy  sigma=1.333418
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 = -4.5502e-06 Jy
! Component: 100  -  total flux cleaned = 1.04879e-05 Jy
! Component: 150  -  total flux cleaned = 1.07304e-05 Jy
! Component: 200  -  total flux cleaned = 3.64259e-05 Jy
! Total flux subtracted in 200 components = 3.64259e-05 Jy
! Clean residual min=-0.003761 max=0.003782 Jy/beam
! Clean residual mean=-0.000023 rms=0.001223 Jy/beam
! Combined flux in latest and established models = 0.253892 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 69 components and 0.253892 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066178Jy  sigma=1.333417
! Fit after  self-cal, rms=0.066179Jy  sigma=1.333397
! 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=3.769 mas, bmaj=15.31 mas, bpa=-10.46 degrees
! Estimated noise=0.796091 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 3.769 x 15.31 at -10.46 degrees (North through East)
! Clean map  min=-0.0030741  max=0.23565 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=3.183 mas, bmaj=13.7 mas, bpa=-11.67 degrees
! Estimated noise=0.970726 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.182043 Jy
! Component: 100  -  total flux cleaned = 0.22183 Jy
! Component: 150  -  total flux cleaned = 0.234668 Jy
! Component: 200  -  total flux cleaned = 0.241873 Jy
! Total flux subtracted in 200 components = 0.241873 Jy
! Clean residual min=-0.005580 max=0.005276 Jy/beam
! Clean residual mean=0.000019 rms=0.001545 Jy/beam
! Combined flux in latest and established models = 0.241873 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 16 model components to the UV plane model.
! The established model now contains 16 components and 0.241873 Jy
! Inverting map and beam 
! Estimated beam: bmin=3.769 mas, bmaj=15.31 mas, bpa=-10.46 degrees
! Estimated noise=0.796091 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 = 0.00542992 Jy
! Component: 100  -  total flux cleaned = 0.00847664 Jy
! Component: 150  -  total flux cleaned = 0.0103174 Jy
! Component: 200  -  total flux cleaned = 0.0108445 Jy
! Total flux subtracted in 200 components = 0.0108445 Jy
! Clean residual min=-0.003740 max=0.003485 Jy/beam
! Clean residual mean=-0.000009 rms=0.001028 Jy/beam
! Combined flux in latest and established models = 0.252718 Jy
! Adding 21 model components to the UV plane model.
! The established model now contains 34 components and 0.252718 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=8.461 mas, bmaj=18.62 mas, bpa=7.905 degrees
! Estimated noise=0.979029 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000854642 Jy
! Component: 100  -  total flux cleaned = 0.000942925 Jy
! Component: 150  -  total flux cleaned = 0.000941131 Jy
! Component: 200  -  total flux cleaned = 0.000945322 Jy
! Total flux subtracted in 200 components = 0.000945322 Jy
! Clean residual min=-0.004209 max=0.003984 Jy/beam
! Clean residual mean=-0.000022 rms=0.001292 Jy/beam
! Combined flux in latest and established models = 0.253663 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 = 2.88774e-05 Jy
! Component: 100  -  total flux cleaned = 2.97819e-05 Jy
! Component: 150  -  total flux cleaned = 5.31774e-05 Jy
! Component: 200  -  total flux cleaned = 9.60695e-05 Jy
! Total flux subtracted in 200 components = 9.60695e-05 Jy
! Clean residual min=-0.004073 max=0.003987 Jy/beam
! Clean residual mean=-0.000022 rms=0.001266 Jy/beam
! Combined flux in latest and established models = 0.253759 Jy
! Adding 22 model components to the UV plane model.
! The established model now contains 53 components and 0.253759 Jy
! Inverting map 
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Estimated beam: bmin=3.769 mas, bmaj=15.31 mas, bpa=-10.46 degrees
! Estimated noise=0.796091 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000139778 Jy
! Component: 100  -  total flux cleaned = 1.32269e-05 Jy
! Component: 150  -  total flux cleaned = -8.02963e-06 Jy
! Component: 200  -  total flux cleaned = -8.67273e-06 Jy
! Total flux subtracted in 200 components = -8.67273e-06 Jy
! Clean residual min=-0.003403 max=0.003357 Jy/beam
! Clean residual mean=-0.000012 rms=0.000954 Jy/beam
! Combined flux in latest and established models = 0.25375 Jy
selfcal
! Performing phase self-cal
! Adding 16 model components to the UV plane model.
! The established model now contains 66 components and 0.25375 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066211Jy  sigma=1.334026
! Fit after  self-cal, rms=0.066213Jy  sigma=1.333979
wmodel /J1333-1950_S_map.mod
! wmodel: Unable to open new model file: /J1333-1950_S_map.mod
! Error occured in command: wmodel
![Exited script file: /opt64/bin/pima_mupet_01.dfm]
! 
wmap /scr/pima/bg219g_uvs/J1333-1950_S_map.fits
! Inverting map 
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 3.769 x 15.31 at -10.46 degrees (North through East)
! Clean map  min=-0.0033118  max=0.23536 Jy/beam
! Writing clean map to FITS file: /scr/pima/bg219g_uvs/J1333-1950_S_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is", peak_flux
! The peak flux is 0.23536 
invert
! Inverting map 
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000955824 
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -1.21833 1.21833 2.43667 4.87334 9.74668 19.4934 38.9867 77.9734
print "clev=      ", int(3*image_rms*10000)/10000
! clev=       0.0028 
print "peak=      ", int(1000*peak_flux)/1000
! peak=       0.235 
print "dyn_range= ", int(1000*peak_flux/image_rms)/1000
! dyn_range=  246.237 
quit
! Quitting program
! Log file /scr/pima/bg219g_uvs/J1333-1950_S_dfm.log closed on Thu May 19 21:48:10 2016