! Started logfile: J1036-3744_X_2005_06_30_yyk_uvs.log on Sat Oct  8 17:16:22 2005
obs J1036-3744_X_2005_06_30_yyk_uve.fits
! Reading UV FITS file: J1036-3744_X_2005_06_30_yyk_uve.fits
! AN table 1: 19 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.790643 visibilities/baseline/integration-bin.
! Found source: J1036-3744
! 
! 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  8.40997e+09        8e+06          1        8e+06
!  02        2  8.47997e+09        8e+06          1        8e+06
!  03        3  8.79497e+09        8e+06          1        8e+06
!  04        4  8.89997e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 1460 lines of history.
! 
! Reading 2704 visibilities.
select I
! Polarization I is unavailable.
! 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
![@muppet J1036-3744_X_2005_06_30_yyk]
integer clean_niter
clean_niter = 100
float clean_gain
clean_gain = 0.04
float dynam
dynam = 6.0
float amp_soltime1
amp_soltime1 = 10
float amp_soltime2
amp_soltime2 = 1
float phase_soltime1
phase_soltime1=10
float phase_soltime2
phase_soltime2=0.5
float phase_soltime
phase_soltime=phase_soltime1
float ampcor_selflim
ampcor_selflim=1.20
float thresh
thresh = 0.10
float win_mult
win_mult = 1.8
float time_av
time_av = 30
float old_peak
float new_peak
float flux_cutoff
mapsize field_size, field_cell
! Map grid = 512x512 pixels with 0.200x0.200 milli-arcsec cellsize.
phase_soltime=phase_soltime1
print "uvstat(rms)=",uvstat(rms),"Jy"
! uvstat(rms)= 0.503552 Jy 
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 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.6617 mas, bmaj=1.965 mas, bpa=-0.3008 degrees
! Estimated noise=1.76127 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (0, 0).
! clean: niter=100  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.417066 Jy
! Component: 100  -  total flux cleaned = 0.487677 Jy
! Total flux subtracted in 100 components = 0.487677 Jy
! Clean residual min=-0.022783 max=0.037980 Jy/beam
! Clean residual mean=0.000188 rms=0.006976 Jy/beam
! Combined flux in latest and established models = 0.487677 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 9 model components to the UV plane model.
! The established model now contains 9 components and 0.487677 Jy
! 
! Correcting IF 1.
!  A total of 30 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 30 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 30 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 30 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.141149Jy  sigma=2.002646
! Fit after  self-cal, rms=0.140632Jy  sigma=1.994637
! Inverting map and beam 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.6617 mas, bmaj=1.965 mas, bpa=-0.3008 degrees
! Estimated noise=1.76127 mJy/beam.
print "************** FINISHED UNIFORM WEIGHTING CLEAN **************"
! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** 
! 
uvw 0,-2
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -2.
! 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 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8872 mas, bmaj=2.579 mas, bpa=-0.5421 degrees
! Estimated noise=0.978905 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0342724 Jy
! Component: 100  -  total flux cleaned = 0.0432883 Jy
! Component: 150  -  total flux cleaned = 0.0449806 Jy
! Component: 200  -  total flux cleaned = 0.0450814 Jy
! Total flux subtracted in 200 components = 0.0450814 Jy
! Clean residual min=-0.020058 max=0.026322 Jy/beam
! Clean residual mean=0.000377 rms=0.006307 Jy/beam
! Combined flux in latest and established models = 0.532758 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 7 model components to the UV plane model.
! The established model now contains 13 components and 0.532758 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.140766Jy  sigma=1.913232
! Fit after  self-cal, rms=0.140766Jy  sigma=1.913213
! Inverting map 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8872 x 2.579 at -0.5421 degrees (North through East)
! Clean map  min=-0.019326  max=0.47786 Jy/beam
if(peak(flux) < thresh*2)
  selflims ampcor_selflim
  end if
gscale
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Amplitude normalization factor in sub-array 1: 0.93395
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.17     FD        0.93     HN        1.00*    KP        0.92     
!   LA        0.97     MK        0.98     NL        1.34     OV        1.02     
!   PT        0.95     SC        1.42     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 0.995109
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.21     FD        0.93     HN        1.00*    KP        0.87     
!   LA        0.95     MK        1.00     NL        1.32     OV        0.98     
!   PT        1.00     SC        0.79     
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 0.991608
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.25     FD        0.97     HN        1.00*    KP        0.80     
!   LA        0.96     MK        1.02     NL        1.26     OV        1.01     
!   PT        1.01     SC        0.79     
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 0.947574
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.26     FD        0.97     HN        1.00*    KP        0.93     
!   LA        0.96     MK        1.01     NL        1.32     OV        1.02     
!   PT        1.07     SC        1.03     
! 
! 
! Fit before self-cal, rms=0.140766Jy  sigma=1.913213
! Fit after  self-cal, rms=0.128330Jy  sigma=1.657358
selfcal false, false, phase_soltime
! Performing phase self-cal over 10 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.128330Jy  sigma=1.657358
! Fit after  self-cal, rms=0.128343Jy  sigma=1.657305
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8838 mas, bmaj=2.558 mas, bpa=0.2137 degrees
! Estimated noise=0.902594 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.0313181 Jy
! Component: 100  -  total flux cleaned = -0.0386082 Jy
! Component: 150  -  total flux cleaned = -0.0392993 Jy
! Component: 200  -  total flux cleaned = -0.0393818 Jy
! Total flux subtracted in 200 components = -0.0393818 Jy
! Clean residual min=-0.004956 max=0.006022 Jy/beam
! Clean residual mean=0.000091 rms=0.001379 Jy/beam
! Combined flux in latest and established models = 0.493377 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 8 model components to the UV plane model.
! The established model now contains 18 components and 0.493377 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.123923Jy  sigma=1.556606
! Fit after  self-cal, rms=0.123923Jy  sigma=1.556597
! Inverting map 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
print "************** FINISHED AMPLITUDE GSCALE SELF-CAL **************"
! ************** FINISHED AMPLITUDE GSCALE SELF-CAL ************** 
! 
phase_soltime=phase_soltime2
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.123923Jy  sigma=1.556597
! Fit after  self-cal, rms=0.096953Jy  sigma=1.181617
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 4.32029e-05 Jy
! Component: 100  -  total flux cleaned = -0.00040827 Jy
! Component: 150  -  total flux cleaned = -0.000758471 Jy
! Component: 200  -  total flux cleaned = -0.0010378 Jy
! Total flux subtracted in 200 components = -0.0010378 Jy
! Clean residual min=-0.005443 max=0.005849 Jy/beam
! Clean residual mean=0.000090 rms=0.001448 Jy/beam
! Combined flux in latest and established models = 0.492339 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 9 model components to the UV plane model.
! The established model now contains 23 components and 0.492339 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.096173Jy  sigma=1.170111
! Fit after  self-cal, rms=0.096048Jy  sigma=1.167355
! Inverting map 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
print "*** FINISHED NATURAL WEIGHTING CLEAN with shorter phase_soltime ***"
! *** FINISHED NATURAL WEIGHTING CLEAN with shorter phase_soltime *** 
! 
dynam = dynam - 0.25
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8838 x 2.558 at 0.2137 degrees (North through East)
! Clean map  min=-0.0049407  max=0.4607 Jy/beam
if(peak(flux) > thresh)
  selfcal true, true, amp_soltime1
  selfcal false, false, phase_soltime
  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 false,false,phase_soltime
    new_peak = peak(flux)
    until(new_peak<=flux_cutoff)
  selfcal true, true, amp_soltime2
  selfcal false, false, phase_soltime
  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 false,false,phase_soltime
    new_peak = peak(flux)
    until(new_peak<=flux_cutoff)
  print "************** FINISHED AMPLITUDE SELF-CAL **************"
  end if
! Performing amp+phase self-cal over 10 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.096048Jy  sigma=1.167355
! Fit after  self-cal, rms=0.087087Jy  sigma=1.030649
! Performing phase self-cal over 0.5 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.087087Jy  sigma=1.030649
! Fit after  self-cal, rms=0.087111Jy  sigma=1.030354
! Inverting map and beam 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8781 mas, bmaj=2.545 mas, bpa=0.6117 degrees
! Estimated noise=0.896934 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.000123002 Jy
! Component: 100  -  total flux cleaned = -0.000118265 Jy
! Component: 150  -  total flux cleaned = -9.07411e-05 Jy
! Component: 200  -  total flux cleaned = -9.26277e-05 Jy
! Total flux subtracted in 200 components = -9.26277e-05 Jy
! Clean residual min=-0.003244 max=0.003689 Jy/beam
! Clean residual mean=0.000027 rms=0.000867 Jy/beam
! Combined flux in latest and established models = 0.492246 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 6 model components to the UV plane model.
! The established model now contains 26 components and 0.492246 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.087089Jy  sigma=1.030036
! Fit after  self-cal, rms=0.087105Jy  sigma=1.030009
! Inverting map 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Added new window around map position (23.2, -6.2).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00300001 Jy
! Component: 100  -  total flux cleaned = 0.00330202 Jy
! Component: 150  -  total flux cleaned = 0.00352871 Jy
! Component: 200  -  total flux cleaned = 0.00367733 Jy
! Total flux subtracted in 200 components = 0.00367733 Jy
! Clean residual min=-0.002894 max=0.002773 Jy/beam
! Clean residual mean=0.000010 rms=0.000776 Jy/beam
! Combined flux in latest and established models = 0.495923 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 18 model components to the UV plane model.
! The established model now contains 44 components and 0.495923 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.087023Jy  sigma=1.027546
! Fit after  self-cal, rms=0.087020Jy  sigma=1.027488
! Inverting map 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Performing amp+phase self-cal over 1 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.087020Jy  sigma=1.027488
! Fit after  self-cal, rms=0.082260Jy  sigma=0.948011
! Performing phase self-cal over 0.5 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.082260Jy  sigma=0.948011
! Fit after  self-cal, rms=0.082274Jy  sigma=0.947988
! Inverting map and beam 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8778 mas, bmaj=2.545 mas, bpa=0.6275 degrees
! Estimated noise=0.897 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.000765308 Jy
! Component: 100  -  total flux cleaned = 0.000766015 Jy
! Component: 150  -  total flux cleaned = 0.000802763 Jy
! Component: 200  -  total flux cleaned = 0.00076605 Jy
! Total flux subtracted in 200 components = 0.00076605 Jy
! Clean residual min=-0.002918 max=0.002966 Jy/beam
! Clean residual mean=0.000003 rms=0.000748 Jy/beam
! Combined flux in latest and established models = 0.49669 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 18 model components to the UV plane model.
! The established model now contains 52 components and 0.496689 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.082248Jy  sigma=0.947358
! Fit after  self-cal, rms=0.082255Jy  sigma=0.947349
! Inverting map 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! ************** FINISHED AMPLITUDE SELF-CAL ************** 
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
win_mult = win_mult * 1.4
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=2.895 mas, bmaj=10.47 mas, bpa=9.409 degrees
! Estimated noise=1.12612 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 1.76273e-05 Jy
! Component: 100  -  total flux cleaned = 1.84342e-05 Jy
! Component: 150  -  total flux cleaned = 1.84314e-05 Jy
! Component: 200  -  total flux cleaned = 1.89384e-05 Jy
! Total flux subtracted in 200 components = 1.89384e-05 Jy
! Clean residual min=-0.002948 max=0.002375 Jy/beam
! Clean residual mean=0.000005 rms=0.000870 Jy/beam
! Combined flux in latest and established models = 0.496708 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 8 model components to the UV plane model.
! The established model now contains 59 components and 0.496708 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.082240Jy  sigma=0.947217
! Fit after  self-cal, rms=0.082242Jy  sigma=0.947213
! Inverting map 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
win_mult = win_mult / 1.4
print "************** FINISHED TAPERING SELF-CAL CLEAN **************"
! ************** FINISHED TAPERING SELF-CAL CLEAN ************** 
! 
print "************** CLEARING MODEL AND STARTING OVER **********"
! ************** CLEARING MODEL AND STARTING OVER ********** 
clrmod true,true,true
! clrmod: Cleared the established, tentative and continuum 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 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.653 mas, bmaj=1.953 mas, bpa=0.09565 degrees
! Estimated noise=1.66582 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.405221 Jy
! Component: 100  -  total flux cleaned = 0.467671 Jy
! Component: 150  -  total flux cleaned = 0.483371 Jy
! Component: 200  -  total flux cleaned = 0.488362 Jy
! Total flux subtracted in 200 components = 0.488362 Jy
! Clean residual min=-0.006254 max=0.006570 Jy/beam
! Clean residual mean=-0.000006 rms=0.001479 Jy/beam
! Combined flux in latest and established models = 0.488362 Jy
uvw 0,-2
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -2.
! Radial weighting is not currently selected.
flux_cutoff = imstat(rms) * dynam
! Adding 17 model components to the UV plane model.
! The established model now contains 17 components and 0.488362 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8778 mas, bmaj=2.545 mas, bpa=0.6275 degrees
! Estimated noise=0.897 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 (1.8, 6.2).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00481394 Jy
! Component: 100  -  total flux cleaned = 0.00646749 Jy
! Component: 150  -  total flux cleaned = 0.00694204 Jy
! Component: 200  -  total flux cleaned = 0.00709781 Jy
! Total flux subtracted in 200 components = 0.00709781 Jy
! Clean residual min=-0.002808 max=0.002612 Jy/beam
! Clean residual mean=0.000002 rms=0.000723 Jy/beam
! Combined flux in latest and established models = 0.49546 Jy
! Adding 31 model components to the UV plane model.
! The established model now contains 46 components and 0.49546 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=2.895 mas, bmaj=10.47 mas, bpa=9.409 degrees
! Estimated noise=1.12612 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=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.000485256 Jy
! Component: 100  -  total flux cleaned = 0.000638727 Jy
! Component: 150  -  total flux cleaned = 0.000725776 Jy
! Component: 200  -  total flux cleaned = 0.000745355 Jy
! Total flux subtracted in 200 components = 0.000745355 Jy
! Clean residual min=-0.002708 max=0.002292 Jy/beam
! Clean residual mean=0.000003 rms=0.000831 Jy/beam
! Combined flux in latest and established models = 0.496206 Jy
! Adding 14 model components to the UV plane model.
! The established model now contains 57 components and 0.496205 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8778 mas, bmaj=2.545 mas, bpa=0.6275 degrees
! Estimated noise=0.897 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 1.00582e-05 Jy
! Component: 100  -  total flux cleaned = -0.00011793 Jy
! Component: 150  -  total flux cleaned = -0.000232975 Jy
! Component: 200  -  total flux cleaned = -0.00033827 Jy
! Total flux subtracted in 200 components = -0.00033827 Jy
! Clean residual min=-0.002736 max=0.002550 Jy/beam
! Clean residual mean=0.000003 rms=0.000701 Jy/beam
! Combined flux in latest and established models = 0.495867 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 65 components and 0.495867 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.082077Jy  sigma=0.945119
! Fit after  self-cal, rms=0.082068Jy  sigma=0.944954
wmodel J1036-3744_X_2005_06_30_yyk\_map.mod
! Writing 65 model components to file: J1036-3744_X_2005_06_30_yyk_map.mod
wobs J1036-3744_X_2005_06_30_yyk\_uvs.fits
! Writing UV FITS file: J1036-3744_X_2005_06_30_yyk_uvs.fits
wwins J1036-3744_X_2005_06_30_yyk\_map.win
! wwins: Wrote 3 windows to J1036-3744_X_2005_06_30_yyk_map.win
x = (field_size-8) * field_cell / 4
addwin -x,x,-x,x
clean (field_size*4),0.01
! Inverting map 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.000651018 Jy
! Component: 100  -  total flux cleaned = -0.00104281 Jy
! Component: 150  -  total flux cleaned = -0.00145206 Jy
! Component: 200  -  total flux cleaned = -0.00176318 Jy
! Component: 250  -  total flux cleaned = -0.00213279 Jy
! Component: 300  -  total flux cleaned = -0.00248742 Jy
! Component: 350  -  total flux cleaned = -0.00275986 Jy
! Component: 400  -  total flux cleaned = -0.00295617 Jy
! Component: 450  -  total flux cleaned = -0.00314611 Jy
! Component: 500  -  total flux cleaned = -0.0033915 Jy
! Component: 550  -  total flux cleaned = -0.00348128 Jy
! Component: 600  -  total flux cleaned = -0.00353998 Jy
! Component: 650  -  total flux cleaned = -0.0036253 Jy
! Component: 700  -  total flux cleaned = -0.00368074 Jy
! Component: 750  -  total flux cleaned = -0.00381525 Jy
! Component: 800  -  total flux cleaned = -0.00386699 Jy
! Component: 850  -  total flux cleaned = -0.00394361 Jy
! Component: 900  -  total flux cleaned = -0.00391843 Jy
! Component: 950  -  total flux cleaned = -0.00404243 Jy
! Component: 1000  -  total flux cleaned = -0.00416253 Jy
! Component: 1050  -  total flux cleaned = -0.00418594 Jy
! Component: 1100  -  total flux cleaned = -0.00420957 Jy
! Component: 1150  -  total flux cleaned = -0.00439051 Jy
! Component: 1200  -  total flux cleaned = -0.00447936 Jy
! Component: 1250  -  total flux cleaned = -0.00463192 Jy
! Component: 1300  -  total flux cleaned = -0.00476083 Jy
! Component: 1350  -  total flux cleaned = -0.00488731 Jy
! Component: 1400  -  total flux cleaned = -0.00501152 Jy
! Component: 1450  -  total flux cleaned = -0.00509364 Jy
! Component: 1500  -  total flux cleaned = -0.00525546 Jy
! Component: 1550  -  total flux cleaned = -0.00541481 Jy
! Component: 1600  -  total flux cleaned = -0.00553334 Jy
! Component: 1650  -  total flux cleaned = -0.00572794 Jy
! Component: 1700  -  total flux cleaned = -0.00580479 Jy
! Component: 1750  -  total flux cleaned = -0.00584269 Jy
! Component: 1800  -  total flux cleaned = -0.00588017 Jy
! Component: 1850  -  total flux cleaned = -0.00588005 Jy
! Component: 1900  -  total flux cleaned = -0.00588004 Jy
! Component: 1950  -  total flux cleaned = -0.00588006 Jy
! Component: 2000  -  total flux cleaned = -0.00586188 Jy
! Total flux subtracted in 2048 components = -0.00587989 Jy
! Clean residual min=-0.001031 max=0.000971 Jy/beam
! Clean residual mean=0.000011 rms=0.000340 Jy/beam
! Combined flux in latest and established models = 0.489987 Jy
keep
! Adding 134 model components to the UV plane model.
! The established model now contains 199 components and 0.489987 Jy
![Exited script file: muppet]
wmap "J1036-3744_X_2005_06_30_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8778 x 2.545 at 0.6275 degrees (North through East)
! Clean map  min=-0.0017063  max=0.46717 Jy/beam
! Writing clean map to FITS file: J1036-3744_X_2005_06_30_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.467174 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.378% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000336472 
device "J1036-3744_X_2005_06_30_yyk\_map.eps/VPS"
! Attempting to open device: 'J1036-3744_X_2005_06_30_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.216068 0.216068 0.432137 0.864273 1.72855 3.45709 6.91419 13.8284 27.6568 55.3135
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.001 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.467 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8778 x 2.545 at 0.6275 degrees (North through East)
! Clean map  min=-0.0017063  max=0.46717 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J1036-3744_X_2005_06_30_yyk\_map.gif/gif"
! Attempting to open device: 'J1036-3744_X_2005_06_30_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J1036-3744_X_2005_06_30_yyk_uvs.log closed on Sat Oct  8 17:16:26 2005