! Started logfile: /scr/pima/bg219a_uvs/J1250+1621_S_dfm.log on Fri May 20 00:07:02 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/bg219a_uvs/J1250+1621_S_uva.fits
! Reading UV FITS file: /scr/pima/bg219a_uvs/J1250+1621_S_uva.fits
! AN table 1: 58 integrations on 21 of 21 possible baselines.
! Apparent sampling: 0.622332 visibilities/baseline/integration-bin.
! Found source: J1250+1621
! 
! 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 3032 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 J1250+1621_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 98 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 98 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 98 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 98 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=1.021305Jy  sigma=25.620038
! Fit after  self-cal, rms=0.817678Jy  sigma=20.526463
! 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=2.786 mas, bmaj=8.85 mas, bpa=7.473 degrees
! Estimated noise=0.927586 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 = 0.137904 Jy
! Component: 100  -  total flux cleaned = 0.170169 Jy
! Total flux subtracted in 100 components = 0.170169 Jy
! Clean residual min=-0.007718 max=0.012640 Jy/beam
! Clean residual mean=-0.000078 rms=0.002316 Jy/beam
! Combined flux in latest and established models = 0.170169 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 8 components and 0.170169 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.056253Jy  sigma=1.356569
! Fit after  self-cal, rms=0.056263Jy  sigma=1.356451
! 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=3.57 mas, bmaj=9.914 mas, bpa=10.74 degrees
! Estimated noise=0.532617 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 = 0.0162817 Jy
! Component: 100  -  total flux cleaned = 0.0225811 Jy
! Component: 150  -  total flux cleaned = 0.025638 Jy
! Component: 200  -  total flux cleaned = 0.0273931 Jy
! Total flux subtracted in 200 components = 0.0273931 Jy
! Clean residual min=-0.003252 max=0.003830 Jy/beam
! Clean residual mean=-0.000009 rms=0.000872 Jy/beam
! Combined flux in latest and established models = 0.197562 Jy
! Performing phase self-cal
! Adding 32 model components to the UV plane model.
! The established model now contains 33 components and 0.197562 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.052131Jy  sigma=1.245589
! Fit after  self-cal, rms=0.052162Jy  sigma=1.245324
! Inverting map 
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 3.57 x 9.914 at 10.74 degrees (North through East)
! Clean map  min=-0.0032155  max=0.18325 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:
!   FD        1.01     LA        0.97     MK        1.04     NL        0.98     
!   OV        0.99     PT        0.99     SC        1.01     
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   FD        1.03     LA        0.98     MK        0.99     NL        1.02     
!   OV        0.99     PT        0.98     SC        0.99     
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   FD        1.05     LA        1.00     MK        1.01     NL        1.01     
!   OV        0.99     PT        1.00     SC        1.01     
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   FD        1.07     LA        1.00     MK        0.99     NL        0.99     
!   OV        0.98     PT        1.00     SC        1.01     
! 
! 
! Fit before self-cal, rms=0.052162Jy  sigma=1.245324
! Fit after  self-cal, rms=0.052102Jy  sigma=1.237815
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=3.581 mas, bmaj=9.93 mas, bpa=10.75 degrees
! Estimated noise=0.532499 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 = -0.00063596 Jy
! Component: 100  -  total flux cleaned = -0.000710031 Jy
! Component: 150  -  total flux cleaned = -0.000776583 Jy
! Component: 200  -  total flux cleaned = -0.000808394 Jy
! Total flux subtracted in 200 components = -0.000808394 Jy
! Clean residual min=-0.002808 max=0.002594 Jy/beam
! Clean residual mean=0.000007 rms=0.000647 Jy/beam
! Combined flux in latest and established models = 0.196754 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 40 components and 0.196754 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.052049Jy  sigma=1.236888
! Fit after  self-cal, rms=0.052056Jy  sigma=1.236821
! 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=0.052056Jy  sigma=1.236821
! Fit after  self-cal, rms=0.051933Jy  sigma=1.231658
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=3.585 mas, bmaj=9.935 mas, bpa=10.79 degrees
! Estimated noise=0.53202 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000346091 Jy
! Component: 100  -  total flux cleaned = -0.000397506 Jy
! Component: 150  -  total flux cleaned = -0.000420864 Jy
! Component: 200  -  total flux cleaned = -0.000462953 Jy
! Total flux subtracted in 200 components = -0.000462953 Jy
! Clean residual min=-0.002321 max=0.002218 Jy/beam
! Clean residual mean=-0.000012 rms=0.000561 Jy/beam
! Combined flux in latest and established models = 0.196291 Jy
selfcal
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 43 components and 0.196291 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.051905Jy  sigma=1.231233
! Fit after  self-cal, rms=0.051910Jy  sigma=1.231182
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 = 6.31612e-06 Jy
! Component: 100  -  total flux cleaned = -1.17923e-05 Jy
! Component: 150  -  total flux cleaned = -2.88121e-05 Jy
! Component: 200  -  total flux cleaned = -4.48761e-05 Jy
! Total flux subtracted in 200 components = -4.48761e-05 Jy
! Clean residual min=-0.002253 max=0.002202 Jy/beam
! Clean residual mean=-0.000012 rms=0.000556 Jy/beam
! Combined flux in latest and established models = 0.196246 Jy
! Performing phase self-cal
! Adding 8 model components to the UV plane model.
! The established model now contains 44 components and 0.196246 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.051894Jy  sigma=1.230971
! Fit after  self-cal, rms=0.051895Jy  sigma=1.230948
! 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=0.051895Jy  sigma=1.230948
! Fit after  self-cal, rms=0.051908Jy  sigma=1.230920
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=3.586 mas, bmaj=9.936 mas, bpa=10.81 degrees
! Estimated noise=0.531981 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000174811 Jy
! Component: 100  -  total flux cleaned = -0.00025236 Jy
! Component: 150  -  total flux cleaned = -0.000279911 Jy
! Component: 200  -  total flux cleaned = -0.000318153 Jy
! Total flux subtracted in 200 components = -0.000318153 Jy
! Clean residual min=-0.002233 max=0.002118 Jy/beam
! Clean residual mean=-0.000013 rms=0.000550 Jy/beam
! Combined flux in latest and established models = 0.195928 Jy
selfcal
! Performing phase self-cal
! Adding 12 model components to the UV plane model.
! The established model now contains 48 components and 0.195928 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.051897Jy  sigma=1.230775
! Fit after  self-cal, rms=0.051899Jy  sigma=1.230755
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 = -1.93171e-05 Jy
! Component: 100  -  total flux cleaned = -5.49341e-05 Jy
! Component: 150  -  total flux cleaned = -7.68222e-05 Jy
! Component: 200  -  total flux cleaned = -9.642e-05 Jy
! Total flux subtracted in 200 components = -9.642e-05 Jy
! Clean residual min=-0.002225 max=0.002112 Jy/beam
! Clean residual mean=-0.000013 rms=0.000549 Jy/beam
! Combined flux in latest and established models = 0.195831 Jy
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 54 components and 0.195831 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.051891Jy  sigma=1.230679
! Fit after  self-cal, rms=0.051892Jy  sigma=1.230659
! 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=0.051892Jy  sigma=1.230659
! Fit after  self-cal, rms=0.051903Jy  sigma=1.230638
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=8.63 mas, bmaj=14.78 mas, bpa=-3.212 degrees
! Estimated noise=0.633675 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000259328 Jy
! Component: 100  -  total flux cleaned = -0.00020677 Jy
! Component: 150  -  total flux cleaned = -0.000164868 Jy
! Component: 200  -  total flux cleaned = -0.000139197 Jy
! Total flux subtracted in 200 components = -0.000139197 Jy
! Clean residual min=-0.002364 max=0.001809 Jy/beam
! Clean residual mean=-0.000023 rms=0.000620 Jy/beam
! Combined flux in latest and established models = 0.195692 Jy
selfcal
! Performing phase self-cal
! Adding 5 model components to the UV plane model.
! The established model now contains 58 components and 0.195692 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.051905Jy  sigma=1.230724
! Fit after  self-cal, rms=0.051907Jy  sigma=1.230679
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 = 1.45217e-05 Jy
! Component: 100  -  total flux cleaned = 3.66628e-05 Jy
! Component: 150  -  total flux cleaned = 3.63726e-05 Jy
! Component: 200  -  total flux cleaned = 4.91208e-05 Jy
! Total flux subtracted in 200 components = 4.91208e-05 Jy
! Clean residual min=-0.002367 max=0.001804 Jy/beam
! Clean residual mean=-0.000022 rms=0.000614 Jy/beam
! Combined flux in latest and established models = 0.195741 Jy
! Performing phase self-cal
! Adding 6 model components to the UV plane model.
! The established model now contains 59 components and 0.195741 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.051908Jy  sigma=1.230767
! Fit after  self-cal, rms=0.051910Jy  sigma=1.230735
! 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=3.585 mas, bmaj=9.936 mas, bpa=10.82 degrees
! Estimated noise=0.531957 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 3.585 x 9.936 at 10.82 degrees (North through East)
! Clean map  min=-0.0020132  max=0.18471 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=2.798 mas, bmaj=8.843 mas, bpa=7.555 degrees
! Estimated noise=0.932944 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.138642 Jy
! Component: 100  -  total flux cleaned = 0.170726 Jy
! Component: 150  -  total flux cleaned = 0.184016 Jy
! Component: 200  -  total flux cleaned = 0.190632 Jy
! Total flux subtracted in 200 components = 0.190632 Jy
! Clean residual min=-0.004987 max=0.004204 Jy/beam
! Clean residual mean=-0.000017 rms=0.001296 Jy/beam
! Combined flux in latest and established models = 0.190632 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 13 model components to the UV plane model.
! The established model now contains 13 components and 0.190632 Jy
! Inverting map and beam 
! Estimated beam: bmin=3.585 mas, bmaj=9.936 mas, bpa=10.82 degrees
! Estimated noise=0.531957 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 = 0.00351807 Jy
! Component: 100  -  total flux cleaned = 0.00446694 Jy
! Component: 150  -  total flux cleaned = 0.00482689 Jy
! Component: 200  -  total flux cleaned = 0.00491507 Jy
! Total flux subtracted in 200 components = 0.00491507 Jy
! Clean residual min=-0.002540 max=0.002155 Jy/beam
! Clean residual mean=-0.000014 rms=0.000583 Jy/beam
! Combined flux in latest and established models = 0.195547 Jy
! Adding 20 model components to the UV plane model.
! The established model now contains 30 components and 0.195547 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=8.63 mas, bmaj=14.78 mas, bpa=-3.212 degrees
! Estimated noise=0.633675 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000576656 Jy
! Component: 100  -  total flux cleaned = 0.000596499 Jy
! Component: 150  -  total flux cleaned = 0.000613118 Jy
! Component: 200  -  total flux cleaned = 0.000620527 Jy
! Total flux subtracted in 200 components = 0.000620527 Jy
! Clean residual min=-0.002475 max=0.001797 Jy/beam
! Clean residual mean=-0.000019 rms=0.000625 Jy/beam
! Combined flux in latest and established models = 0.196168 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 = -7.21319e-06 Jy
! Component: 100  -  total flux cleaned = -7.45766e-06 Jy
! Component: 150  -  total flux cleaned = -1.47921e-05 Jy
! Component: 200  -  total flux cleaned = -1.51686e-05 Jy
! Total flux subtracted in 200 components = -1.51686e-05 Jy
! Clean residual min=-0.002470 max=0.001791 Jy/beam
! Clean residual mean=-0.000019 rms=0.000622 Jy/beam
! Combined flux in latest and established models = 0.196153 Jy
! Adding 7 model components to the UV plane model.
! The established model now contains 36 components and 0.196153 Jy
! Inverting map 
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Estimated beam: bmin=3.585 mas, bmaj=9.936 mas, bpa=10.82 degrees
! Estimated noise=0.531957 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000216434 Jy
! Component: 100  -  total flux cleaned = -0.000287509 Jy
! Component: 150  -  total flux cleaned = -0.000318618 Jy
! Component: 200  -  total flux cleaned = -0.00031833 Jy
! Total flux subtracted in 200 components = -0.00031833 Jy
! Clean residual min=-0.002306 max=0.002073 Jy/beam
! Clean residual mean=-0.000012 rms=0.000556 Jy/beam
! Combined flux in latest and established models = 0.195834 Jy
selfcal
! Performing phase self-cal
! Adding 9 model components to the UV plane model.
! The established model now contains 42 components and 0.195834 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.051940Jy  sigma=1.231208
! Fit after  self-cal, rms=0.051942Jy  sigma=1.231162
wmodel /J1250+1621_S_map.mod
! wmodel: Unable to open new model file: /J1250+1621_S_map.mod
! Error occured in command: wmodel
![Exited script file: /opt64/bin/pima_mupet_01.dfm]
! 
wmap /scr/pima/bg219a_uvs/J1250+1621_S_map.fits
! Inverting map 
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 3.585 x 9.936 at 10.82 degrees (North through East)
! Clean map  min=-0.0022732  max=0.18437 Jy/beam
! Writing clean map to FITS file: /scr/pima/bg219a_uvs/J1250+1621_S_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is", peak_flux
! The peak flux is 0.184374 
invert
! Inverting map 
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000554019 
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.901459 0.901459 1.80292 3.60584 7.21167 14.4233 28.8467 57.6934
print "clev=      ", int(3*image_rms*10000)/10000
! clev=       0.0016 
print "peak=      ", int(1000*peak_flux)/1000
! peak=       0.184 
print "dyn_range= ", int(1000*peak_flux/image_rms)/1000
! dyn_range=  332.793 
quit
! Quitting program
! Log file /scr/pima/bg219a_uvs/J1250+1621_S_dfm.log closed on Fri May 20 00:07:04 2016