! Started logfile: /scr/pima/bg219h_uvs/J1752-2956_S_uvs.log on Thu Apr  7 09:09:06 2016
obs /scr/pima/bg219h_uvs/J1752-2956_S_uva.fits
! Reading UV FITS file: /scr/pima/bg219h_uvs/J1752-2956_S_uva.fits
! AN table 1: 61 integrations on 10 of 10 possible baselines.
! Apparent sampling: 0.657377 visibilities/baseline/integration-bin.
! Found source: J1752-2956
! 
! 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 1604 visibilities.
select rr, 1,2,3,4,6,7,8 
! 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 
![@/home/lpetrov/bin/01_muppet /scr/pima/bg219h_uvs/J1752-2956_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 74 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 74 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 74 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 74 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=1.005145Jy  sigma=19.191222
! Fit after  self-cal, rms=0.928179Jy  sigma=17.815838
! 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=17.08 mas, bmaj=35.81 mas, bpa=1.571 degrees
! Estimated noise=1.40651 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=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0523973 Jy
! Component: 100  -  total flux cleaned = 0.0647667 Jy
! Total flux subtracted in 100 components = 0.0647667 Jy
! Clean residual min=-0.006478 max=0.006647 Jy/beam
! Clean residual mean=-0.000168 rms=0.002832 Jy/beam
! Combined flux in latest and established models = 0.0647667 Jy
! Performing phase self-cal
! Adding 34 model components to the UV plane model.
! The established model now contains 34 components and 0.0647667 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.062889Jy  sigma=1.168833
! Fit after  self-cal, rms=0.062071Jy  sigma=1.151429
! 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=18.61 mas, bmaj=39.74 mas, bpa=2.723 degrees
! Estimated noise=1.04489 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 = 0.0120376 Jy
! Component: 100  -  total flux cleaned = 0.0161197 Jy
! Component: 150  -  total flux cleaned = 0.0167179 Jy
! Component: 200  -  total flux cleaned = 0.0169146 Jy
! Total flux subtracted in 200 components = 0.0169146 Jy
! Clean residual min=-0.003177 max=0.003208 Jy/beam
! Clean residual mean=-0.000143 rms=0.002204 Jy/beam
! Combined flux in latest and established models = 0.0816813 Jy
! Performing phase self-cal
! Adding 155 model components to the UV plane model.
! The established model now contains 189 components and 0.0816813 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.058588Jy  sigma=1.087221
! Fit after  self-cal, rms=0.058329Jy  sigma=1.082395
! Inverting map 
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 18.61 x 39.74 at 2.723 degrees (North through East)
! Clean map  min=-0.0067303  max=0.06844 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.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.09     KP        0.99     LA        0.88     OV        0.96     
!   PT        0.99     
! 
! 
! Correcting IF 2.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.94     KP        1.06     LA        0.87     OV        0.99     
!   PT        0.94     
! 
! 
! Correcting IF 3.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.04     KP        1.04     LA        0.86     OV        1.02     
!   PT        0.93     
! 
! 
! Correcting IF 4.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.09     KP        1.07     LA        0.89     OV        1.05     
!   PT        0.91     
! 
! 
! Fit before self-cal, rms=0.058329Jy  sigma=1.082395
! Fit after  self-cal, rms=0.056342Jy  sigma=1.074178
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=18.61 mas, bmaj=40.9 mas, bpa=2.086 degrees
! Estimated noise=1.01051 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 = 0.000260796 Jy
! Component: 100  -  total flux cleaned = -0.00111866 Jy
! Component: 150  -  total flux cleaned = -0.0021012 Jy
! Component: 200  -  total flux cleaned = -0.00292785 Jy
! Total flux subtracted in 200 components = -0.00292785 Jy
! Clean residual min=-0.000764 max=0.000762 Jy/beam
! Clean residual mean=-0.000001 rms=0.000346 Jy/beam
! Combined flux in latest and established models = 0.0787534 Jy
! Performing phase self-cal
! Adding 92 model components to the UV plane model.
! The established model now contains 280 components and 0.0787534 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.055925Jy  sigma=1.066363
! Fit after  self-cal, rms=0.055947Jy  sigma=1.064763
! 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=0.055947Jy  sigma=1.064763
! Fit after  self-cal, rms=0.056225Jy  sigma=1.063304
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=18.56 mas, bmaj=40.93 mas, bpa=2.163 degrees
! Estimated noise=1.01047 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000540787 Jy
! Component: 100  -  total flux cleaned = -0.000451076 Jy
! Component: 150  -  total flux cleaned = -0.000381145 Jy
! Component: 200  -  total flux cleaned = -0.000266393 Jy
! Total flux subtracted in 200 components = -0.000266393 Jy
! Clean residual min=-0.000438 max=0.000445 Jy/beam
! Clean residual mean=0.000006 rms=0.000188 Jy/beam
! Combined flux in latest and established models = 0.078487 Jy
selfcal
! Performing phase self-cal
! Adding 93 model components to the UV plane model.
! The established model now contains 373 components and 0.078487 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.056149Jy  sigma=1.061937
! Fit after  self-cal, rms=0.056185Jy  sigma=1.061613
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 = 0.000161232 Jy
! Component: 100  -  total flux cleaned = 4.60742e-05 Jy
! Component: 150  -  total flux cleaned = 6.88622e-05 Jy
! Component: 200  -  total flux cleaned = 8.90903e-05 Jy
! Total flux subtracted in 200 components = 8.90903e-05 Jy
! Clean residual min=-0.000317 max=0.000317 Jy/beam
! Clean residual mean=0.000004 rms=0.000139 Jy/beam
! Combined flux in latest and established models = 0.0785761 Jy
! Performing phase self-cal
! Adding 99 model components to the UV plane model.
! The established model now contains 466 components and 0.0785761 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.056158Jy  sigma=1.061192
! Fit after  self-cal, rms=0.056153Jy  sigma=1.061119
! 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=0.056153Jy  sigma=1.061119
! Fit after  self-cal, rms=0.056559Jy  sigma=1.059028
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=18.54 mas, bmaj=40.95 mas, bpa=2.168 degrees
! Estimated noise=1.00842 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000585954 Jy
! Component: 100  -  total flux cleaned = 0.000803723 Jy
! Component: 150  -  total flux cleaned = 0.000966351 Jy
! Component: 200  -  total flux cleaned = 0.0010317 Jy
! Total flux subtracted in 200 components = 0.0010317 Jy
! Clean residual min=-0.000202 max=0.000203 Jy/beam
! Clean residual mean=0.000002 rms=0.000076 Jy/beam
! Combined flux in latest and established models = 0.0796078 Jy
selfcal
! Performing phase self-cal
! Adding 68 model components to the UV plane model.
! The established model now contains 531 components and 0.0796078 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.056545Jy  sigma=1.058885
! Fit after  self-cal, rms=0.056635Jy  sigma=1.058698
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 = 0.000139045 Jy
! Component: 100  -  total flux cleaned = 0.000284315 Jy
! Component: 150  -  total flux cleaned = 0.000356066 Jy
! Component: 200  -  total flux cleaned = 0.000400483 Jy
! Total flux subtracted in 200 components = 0.000400483 Jy
! Clean residual min=-0.000182 max=0.000181 Jy/beam
! Clean residual mean=0.000001 rms=0.000069 Jy/beam
! Combined flux in latest and established models = 0.0800083 Jy
! Performing phase self-cal
! Adding 83 model components to the UV plane model.
! The established model now contains 608 components and 0.0800083 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.056627Jy  sigma=1.058636
! Fit after  self-cal, rms=0.056632Jy  sigma=1.058618
! 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=0.056632Jy  sigma=1.058618
! Fit after  self-cal, rms=0.056696Jy  sigma=1.058535
clean clean_niter,clean_gain
! Inverting map and beam 
! Estimated beam: bmin=18.86 mas, bmaj=40.87 mas, bpa=1.942 degrees
! Estimated noise=1.00773 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000394643 Jy
! Component: 100  -  total flux cleaned = 0.000609474 Jy
! Component: 150  -  total flux cleaned = 0.000755157 Jy
! Component: 200  -  total flux cleaned = 0.000826744 Jy
! Total flux subtracted in 200 components = 0.000826744 Jy
! Clean residual min=-0.000165 max=0.000165 Jy/beam
! Clean residual mean=0.000001 rms=0.000061 Jy/beam
! Combined flux in latest and established models = 0.0808351 Jy
selfcal
! Performing phase self-cal
! Adding 85 model components to the UV plane model.
! The established model now contains 678 components and 0.0808351 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.056688Jy  sigma=1.058483
! Fit after  self-cal, rms=0.056728Jy  sigma=1.058457
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 = 0.000191261 Jy
! Component: 100  -  total flux cleaned = 0.000334872 Jy
! Component: 150  -  total flux cleaned = 0.000391886 Jy
! Component: 200  -  total flux cleaned = 0.000437758 Jy
! Total flux subtracted in 200 components = 0.000437758 Jy
! Clean residual min=-0.000150 max=0.000151 Jy/beam
! Clean residual mean=0.000001 rms=0.000061 Jy/beam
! Combined flux in latest and established models = 0.0812728 Jy
! Performing phase self-cal
! Adding 80 model components to the UV plane model.
! The established model now contains 744 components and 0.0812728 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.056723Jy  sigma=1.058428
! Fit after  self-cal, rms=0.056733Jy  sigma=1.058416
! 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=18.54 mas, bmaj=40.97 mas, bpa=2.146 degrees
! Estimated noise=1.00564 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 18.54 x 40.97 at 2.146 degrees (North through East)
! Clean map  min=-0.0058223  max=0.06593 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=16.74 mas, bmaj=37.43 mas, bpa=1.326 degrees
! Estimated noise=1.37601 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0501824 Jy
! Component: 100  -  total flux cleaned = 0.0514323 Jy
! Component: 150  -  total flux cleaned = 0.0528828 Jy
! Component: 200  -  total flux cleaned = 0.0551913 Jy
! Total flux subtracted in 200 components = 0.0551913 Jy
! Clean residual min=-0.003772 max=0.003744 Jy/beam
! Clean residual mean=-0.000112 rms=0.001835 Jy/beam
! Combined flux in latest and established models = 0.0551913 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 83 model components to the UV plane model.
! The established model now contains 83 components and 0.0551913 Jy
! Inverting map and beam 
! Estimated beam: bmin=18.54 mas, bmaj=40.97 mas, bpa=2.146 degrees
! Estimated noise=1.00564 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 = 0.00395316 Jy
! Component: 100  -  total flux cleaned = 0.00481297 Jy
! Component: 150  -  total flux cleaned = 0.00612052 Jy
! Component: 200  -  total flux cleaned = 0.00721309 Jy
! Total flux subtracted in 200 components = 0.00721309 Jy
! Clean residual min=-0.002128 max=0.002147 Jy/beam
! Clean residual mean=-0.000077 rms=0.001367 Jy/beam
! Combined flux in latest and established models = 0.0624044 Jy
! Adding 150 model components to the UV plane model.
! The established model now contains 232 components and 0.0624044 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=18.86 mas, bmaj=40.87 mas, bpa=1.942 degrees
! Estimated noise=1.00773 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000101926 Jy
! Component: 100  -  total flux cleaned = 9.99513e-05 Jy
! Component: 150  -  total flux cleaned = 0.000175817 Jy
! Component: 200  -  total flux cleaned = 0.000314145 Jy
! Total flux subtracted in 200 components = 0.000314145 Jy
! Clean residual min=-0.001028 max=0.001034 Jy/beam
! Clean residual mean=-0.000044 rms=0.000683 Jy/beam
! Combined flux in latest and established models = 0.0627185 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 = -0.000112168 Jy
! Component: 100  -  total flux cleaned = -0.000382949 Jy
! Component: 150  -  total flux cleaned = -0.000483523 Jy
! Component: 200  -  total flux cleaned = -0.000526834 Jy
! Total flux subtracted in 200 components = -0.000526834 Jy
! Clean residual min=-0.000726 max=0.000727 Jy/beam
! Clean residual mean=-0.000008 rms=0.000371 Jy/beam
! Combined flux in latest and established models = 0.0621917 Jy
! Adding 231 model components to the UV plane model.
! The established model now contains 460 components and 0.0621917 Jy
! Inverting map 
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Estimated beam: bmin=18.54 mas, bmaj=40.97 mas, bpa=2.146 degrees
! Estimated noise=1.00564 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -4.82539e-05 Jy
! Component: 100  -  total flux cleaned = -4.76542e-06 Jy
! Component: 150  -  total flux cleaned = 0.000160554 Jy
! Component: 200  -  total flux cleaned = 0.00024774 Jy
! Total flux subtracted in 200 components = 0.00024774 Jy
! Clean residual min=-0.000279 max=0.000277 Jy/beam
! Clean residual mean=-0.000005 rms=0.000127 Jy/beam
! Combined flux in latest and established models = 0.0624394 Jy
selfcal
! Performing phase self-cal
! Adding 104 model components to the UV plane model.
! The established model now contains 554 components and 0.0624394 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.056748Jy  sigma=1.058723
! Fit after  self-cal, rms=0.056721Jy  sigma=1.058471
wmodel /scr/pima/bg219h_uvs/J1752-2956_S_map.mod
! Writing 554 model components to file: /scr/pima/bg219h_uvs/J1752-2956_S_map.mod
wobs /scr/pima/bg219h_uvs/J1752-2956_S_uvs.fits
! Writing UV FITS file: /scr/pima/bg219h_uvs/J1752-2956_S_uvs.fits
wwins /scr/pima/bg219h_uvs/J1752-2956_S_map.win
! wwins: No CLEAN windows to write.
! Error occured in command: wwins
![Exited script file: /home/lpetrov/bin/01_muppet]
! 
wmap "/scr/pima/bg219h_uvs/J1752-2956_S\_map.fits"
! Inverting map 
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 18.54 x 40.97 at 2.146 degrees (North through East)
! Clean map  min=-0.0061326  max=0.062449 Jy/beam
! Writing clean map to FITS file: /scr/pima/bg219h_uvs/J1752-2956_S_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.0624489 
invert
! Inverting map 
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000198166 
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.951974 0.951974 1.90395 3.8079 7.61579 15.2316 30.4632 60.9263
print "clev=      ", int(3*image_rms*10000)/10000
! clev=       0.0005 
print "peak=      ", int(1000*peak_flux)/1000
! peak=       0.062 
print "dyn_range= ", int(1000*peak_flux/image_rms)/1000
! dyn_range=  315.134 
quit
! Quitting program
! Log file /scr/pima/bg219h_uvs/J1752-2956_S_uvs.log closed on Thu Apr  7 09:09:09 2016