! Started logfile: J1911-2006_X_2004_05_27_yyk_uvs.log on Wed Dec  7 01:06:04 2005
obs J1911-2006_X_2004_05_27_yyk_uve.fits
! Reading UV FITS file: J1911-2006_X_2004_05_27_yyk_uve.fits
! AN table 1: 4 integrations on 45 of 45 possible baselines.
! Apparent sampling: 1 visibilities/baseline/integration-bin.
! Found source: J1911-2006
! 
! 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 1378 lines of history.
! 
! Reading 720 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 J1911-2006_X_2004_05_27_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)= 1.46771 Jy 
startmod ,phase_soltime
! Applying default point source starting model.
! Performing phase self-cal over 10 minute time intervals
! Adding 1 model components to the UV plane model.
! The established model now contains 1 components and 1 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.507732Jy  sigma=8.474864
! Fit after  self-cal, rms=0.507646Jy  sigma=8.473996
! 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 
! Your choice of large map pixels excluded 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.6852 mas, bmaj=1.822 mas, bpa=0.2784 degrees
! Estimated noise=2.10348 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 = 1.21137 Jy
! Component: 100  -  total flux cleaned = 1.43905 Jy
! Total flux subtracted in 100 components = 1.43905 Jy
! Clean residual min=-0.039253 max=0.069363 Jy/beam
! Clean residual mean=-0.000740 rms=0.012421 Jy/beam
! Combined flux in latest and established models = 1.43906 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 15 components and 1.43906 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.198450Jy  sigma=3.242177
! Fit after  self-cal, rms=0.198401Jy  sigma=3.240138
! Inverting map 
! Your choice of large map pixels excluded 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
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 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.8237 mas, bmaj=2.148 mas, bpa=-0.7552 degrees
! Estimated noise=1.61534 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 = 0.131481 Jy
! Component: 100  -  total flux cleaned = 0.181366 Jy
! Component: 150  -  total flux cleaned = 0.203955 Jy
! Component: 200  -  total flux cleaned = 0.21449 Jy
! Total flux subtracted in 200 components = 0.21449 Jy
! Clean residual min=-0.035647 max=0.045256 Jy/beam
! Clean residual mean=-0.000352 rms=0.010076 Jy/beam
! Combined flux in latest and established models = 1.65355 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 50 model components to the UV plane model.
! The established model now contains 56 components and 1.65355 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.137149Jy  sigma=2.168868
! Fit after  self-cal, rms=0.137183Jy  sigma=2.165326
! Inverting map 
! Your choice of large map pixels excluded 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
selflims ampcor_selflim
! Selfcal amplitude corrections will be limited to 0.833333 -> 1.2.
! Selfcal phase corrections will not be limited.
gscale
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Amplitude normalization factor in sub-array 1: 1.00152
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.99     FD        0.97     HN        1.04     KP        0.98     
!   LA        0.98     MK        1.00     NL        1.06     OV        1.02     
!   PT        0.95     SC        1.01     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 1.00885
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00     FD        0.99     HN        1.03     KP        0.92     
!   LA        0.96     MK        1.00     NL        1.04     OV        0.98     
!   PT        1.00     SC        0.98     
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 0.99723
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.06     FD        1.03     HN        0.94     KP        0.89     
!   LA        0.98     MK        1.02     NL        1.02     OV        1.04     
!   PT        1.03     SC        1.03     
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 0.975679
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.06     FD        1.03     HN        1.00     KP        0.93     
!   LA        0.98     MK        1.03     NL        1.06     OV        1.05     
!   PT        1.09     SC        1.04     
! 
! 
! Fit before self-cal, rms=0.137183Jy  sigma=2.165326
! Fit after  self-cal, rms=0.111060Jy  sigma=1.710407
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=0.111060Jy  sigma=1.710407
! Fit after  self-cal, rms=0.111074Jy  sigma=1.710333
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.831 mas, bmaj=2.172 mas, bpa=-0.6961 degrees
! Estimated noise=1.6103 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 (-2.6, 20.2).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0478323 Jy
! Component: 100  -  total flux cleaned = 0.0669138 Jy
! Component: 150  -  total flux cleaned = 0.073427 Jy
! Component: 200  -  total flux cleaned = 0.0767942 Jy
! Total flux subtracted in 200 components = 0.0767942 Jy
! Clean residual min=-0.014373 max=0.023244 Jy/beam
! Clean residual mean=-0.000117 rms=0.004931 Jy/beam
! Combined flux in latest and established models = 1.73034 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 38 model components to the UV plane model.
! The established model now contains 93 components and 1.73034 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.099463Jy  sigma=1.454656
! Fit after  self-cal, rms=0.099516Jy  sigma=1.453247
! Inverting map 
! Your choice of large map pixels excluded 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 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=0.099516Jy  sigma=1.453247
! Fit after  self-cal, rms=0.091240Jy  sigma=1.331747
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 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)
! Added new window around map position (10.8, -12.2).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0273925 Jy
! Component: 100  -  total flux cleaned = 0.0401311 Jy
! Component: 150  -  total flux cleaned = 0.0422437 Jy
! Component: 200  -  total flux cleaned = 0.0436415 Jy
! Total flux subtracted in 200 components = 0.0436415 Jy
! Clean residual min=-0.011367 max=0.013531 Jy/beam
! Clean residual mean=-0.000049 rms=0.003323 Jy/beam
! Combined flux in latest and established models = 1.77398 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 43 model components to the UV plane model.
! The established model now contains 136 components and 1.77398 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.085629Jy  sigma=1.217840
! Fit after  self-cal, rms=0.084955Jy  sigma=1.206476
! Inverting map 
! Your choice of large map pixels excluded 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 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: 0.831 x 2.172 at -0.6961 degrees (North through East)
! Clean map  min=-0.011062  max=1.4298 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=0.084955Jy  sigma=1.206476
! Fit after  self-cal, rms=0.078079Jy  sigma=1.055944
! 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=0.078079Jy  sigma=1.055944
! Fit after  self-cal, rms=0.078057Jy  sigma=1.055160
! Inverting map and beam 
! Your choice of large map pixels excluded 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.8326 mas, bmaj=2.178 mas, bpa=-0.6602 degrees
! Estimated noise=1.60956 mJy/beam.
! Added new window around map position (1.2, 4.6).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0106579 Jy
! Component: 100  -  total flux cleaned = 0.0101085 Jy
! Component: 150  -  total flux cleaned = 0.00935106 Jy
! Component: 200  -  total flux cleaned = 0.00867498 Jy
! Total flux subtracted in 200 components = 0.00867498 Jy
! Clean residual min=-0.009700 max=0.010177 Jy/beam
! Clean residual mean=-0.000008 rms=0.002603 Jy/beam
! Combined flux in latest and established models = 1.78266 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 24 model components to the UV plane model.
! The established model now contains 156 components and 1.78266 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.075974Jy  sigma=1.013658
! Fit after  self-cal, rms=0.075905Jy  sigma=1.012415
! Inverting map 
! Your choice of large map pixels excluded 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 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=0.075905Jy  sigma=1.012415
! Fit after  self-cal, rms=0.074280Jy  sigma=0.992910
! 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=0.074280Jy  sigma=0.992910
! Fit after  self-cal, rms=0.074279Jy  sigma=0.992902
! Inverting map and beam 
! Your choice of large map pixels excluded 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.8313 mas, bmaj=2.175 mas, bpa=-0.6438 degrees
! Estimated noise=1.60858 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00240543 Jy
! Component: 100  -  total flux cleaned = 0.00220253 Jy
! Component: 150  -  total flux cleaned = 0.00220094 Jy
! Component: 200  -  total flux cleaned = 0.00168608 Jy
! Total flux subtracted in 200 components = 0.00168608 Jy
! Clean residual min=-0.008063 max=0.008269 Jy/beam
! Clean residual mean=-0.000019 rms=0.002410 Jy/beam
! Combined flux in latest and established models = 1.78434 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 26 model components to the UV plane model.
! The established model now contains 165 components and 1.78434 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.073338Jy  sigma=0.977492
! Fit after  self-cal, rms=0.073306Jy  sigma=0.976907
! Inverting map 
! Your choice of large map pixels excluded 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 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 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=2.192 mas, bmaj=5.096 mas, bpa=3.421 degrees
! Estimated noise=2.10574 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 = 0.0014377 Jy
! Component: 100  -  total flux cleaned = 0.00144128 Jy
! Component: 150  -  total flux cleaned = 0.0010246 Jy
! Component: 200  -  total flux cleaned = 0.000832877 Jy
! Total flux subtracted in 200 components = 0.000832877 Jy
! Clean residual min=-0.010770 max=0.009725 Jy/beam
! Clean residual mean=-0.000022 rms=0.003425 Jy/beam
! Combined flux in latest and established models = 1.78517 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 27 model components to the UV plane model.
! The established model now contains 182 components and 1.78517 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.073209Jy  sigma=0.972169
! Fit after  self-cal, rms=0.073101Jy  sigma=0.971281
! Inverting map 
! Your choice of large map pixels excluded 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 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 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.6862 mas, bmaj=1.829 mas, bpa=0.1994 degrees
! Estimated noise=2.10612 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 1.21303 Jy
! Component: 100  -  total flux cleaned = 1.43853 Jy
! Component: 150  -  total flux cleaned = 1.535 Jy
! Component: 200  -  total flux cleaned = 1.58764 Jy
! Total flux subtracted in 200 components = 1.58764 Jy
! Clean residual min=-0.016437 max=0.024369 Jy/beam
! Clean residual mean=-0.000307 rms=0.005822 Jy/beam
! Combined flux in latest and established models = 1.58764 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 36 model components to the UV plane model.
! The established model now contains 36 components and 1.58764 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.8313 mas, bmaj=2.175 mas, bpa=-0.6438 degrees
! Estimated noise=1.60858 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 (3.2, 2.2).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0538316 Jy
! Component: 100  -  total flux cleaned = 0.0891491 Jy
! Component: 150  -  total flux cleaned = 0.114879 Jy
! Component: 200  -  total flux cleaned = 0.134144 Jy
! Total flux subtracted in 200 components = 0.134144 Jy
! Clean residual min=-0.010628 max=0.011008 Jy/beam
! Clean residual mean=-0.000161 rms=0.003407 Jy/beam
! Combined flux in latest and established models = 1.72179 Jy
! Adding 72 model components to the UV plane model.
! The established model now contains 99 components and 1.72179 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 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 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=2.192 mas, bmaj=5.096 mas, bpa=3.421 degrees
! Estimated noise=2.10574 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 = 0.0240582 Jy
! Component: 100  -  total flux cleaned = 0.0387418 Jy
! Component: 150  -  total flux cleaned = 0.0456669 Jy
! Component: 200  -  total flux cleaned = 0.0487086 Jy
! Total flux subtracted in 200 components = 0.0487086 Jy
! Clean residual min=-0.011259 max=0.010034 Jy/beam
! Clean residual mean=-0.000077 rms=0.003700 Jy/beam
! Combined flux in latest and established models = 1.7705 Jy
! Adding 47 model components to the UV plane model.
! The established model now contains 139 components and 1.7705 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! Estimated beam: bmin=0.8313 mas, bmaj=2.175 mas, bpa=-0.6438 degrees
! Estimated noise=1.60858 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00308476 Jy
! Component: 100  -  total flux cleaned = 0.0045415 Jy
! Component: 150  -  total flux cleaned = 0.00517814 Jy
! Component: 200  -  total flux cleaned = 0.00554938 Jy
! Total flux subtracted in 200 components = 0.00554938 Jy
! Clean residual min=-0.007476 max=0.007722 Jy/beam
! Clean residual mean=-0.000025 rms=0.002226 Jy/beam
! Combined flux in latest and established models = 1.77605 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 31 model components to the UV plane model.
! The established model now contains 165 components and 1.77605 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.072329Jy  sigma=0.963024
! Fit after  self-cal, rms=0.071584Jy  sigma=0.950237
wmodel J1911-2006_X_2004_05_27_yyk\_map.mod
! Writing 165 model components to file: J1911-2006_X_2004_05_27_yyk_map.mod
wobs J1911-2006_X_2004_05_27_yyk\_uvs.fits
! Writing UV FITS file: J1911-2006_X_2004_05_27_yyk_uvs.fits
wwins J1911-2006_X_2004_05_27_yyk\_map.win
! wwins: Wrote 5 windows to J1911-2006_X_2004_05_27_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 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.00282276 Jy
! Component: 100  -  total flux cleaned = -0.00436498 Jy
! Component: 150  -  total flux cleaned = -0.00481225 Jy
! Component: 200  -  total flux cleaned = -0.00512597 Jy
! Component: 250  -  total flux cleaned = -0.00532421 Jy
! Component: 300  -  total flux cleaned = -0.00551437 Jy
! Component: 350  -  total flux cleaned = -0.00542731 Jy
! Component: 400  -  total flux cleaned = -0.00543222 Jy
! Component: 450  -  total flux cleaned = -0.00534829 Jy
! Component: 500  -  total flux cleaned = -0.00502542 Jy
! Component: 550  -  total flux cleaned = -0.00502558 Jy
! Component: 600  -  total flux cleaned = -0.00509955 Jy
! Component: 650  -  total flux cleaned = -0.00495243 Jy
! Component: 700  -  total flux cleaned = -0.00488295 Jy
! Component: 750  -  total flux cleaned = -0.00474463 Jy
! Component: 800  -  total flux cleaned = -0.00474364 Jy
! Component: 850  -  total flux cleaned = -0.00474292 Jy
! Component: 900  -  total flux cleaned = -0.00474104 Jy
! Component: 950  -  total flux cleaned = -0.00461873 Jy
! Component: 1000  -  total flux cleaned = -0.00485926 Jy
! Component: 1050  -  total flux cleaned = -0.00485895 Jy
! Component: 1100  -  total flux cleaned = -0.00491618 Jy
! Component: 1150  -  total flux cleaned = -0.00502734 Jy
! Component: 1200  -  total flux cleaned = -0.00480624 Jy
! Component: 1250  -  total flux cleaned = -0.0047536 Jy
! Component: 1300  -  total flux cleaned = -0.00464925 Jy
! Component: 1350  -  total flux cleaned = -0.00480476 Jy
! Component: 1400  -  total flux cleaned = -0.00480439 Jy
! Component: 1450  -  total flux cleaned = -0.00475512 Jy
! Component: 1500  -  total flux cleaned = -0.00475625 Jy
! Component: 1550  -  total flux cleaned = -0.0048981 Jy
! Component: 1600  -  total flux cleaned = -0.0048974 Jy
! Component: 1650  -  total flux cleaned = -0.00494294 Jy
! Component: 1700  -  total flux cleaned = -0.00498782 Jy
! Component: 1750  -  total flux cleaned = -0.00507671 Jy
! Component: 1800  -  total flux cleaned = -0.00512059 Jy
! Component: 1850  -  total flux cleaned = -0.00524928 Jy
! Component: 1900  -  total flux cleaned = -0.00537603 Jy
! Component: 1950  -  total flux cleaned = -0.00550064 Jy
! Component: 2000  -  total flux cleaned = -0.00550049 Jy
! Total flux subtracted in 2048 components = -0.00566198 Jy
! Clean residual min=-0.002463 max=0.002126 Jy/beam
! Clean residual mean=-0.000020 rms=0.000768 Jy/beam
! Combined flux in latest and established models = 1.77038 Jy
keep
! Adding 155 model components to the UV plane model.
! The established model now contains 320 components and 1.77038 Jy
![Exited script file: muppet]
wmap "J1911-2006_X_2004_05_27_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8313 x 2.175 at -0.6438 degrees (North through East)
! Clean map  min=-0.0050746  max=1.432 Jy/beam
! Writing clean map to FITS file: J1911-2006_X_2004_05_27_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 1.43201 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.556% of the data.
!  The x-axis pixel size should ideally be below 0.199 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000751058 
device "J1911-2006_X_2004_05_27_yyk\_map.eps/VPS"
! Attempting to open device: 'J1911-2006_X_2004_05_27_yyk_map.eps/VPS'
loglevs 4*100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.629375 0.629375 1.25875 2.5175 5.035 10.07 20.14 40.28 80.56
print "clev=",int(4*3*image_rms*10000)/10000
! clev= 0.009 
print "peak=",int(peak_flux*1000)/1000
! peak= 1.432 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8313 x 2.175 at -0.6438 degrees (North through East)
! Clean map  min=-0.0050746  max=1.432 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J1911-2006_X_2004_05_27_yyk\_map.gif/gif"
! Attempting to open device: 'J1911-2006_X_2004_05_27_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J1911-2006_X_2004_05_27_yyk_uvs.log closed on Wed Dec  7 01:06:08 2005