! Started logfile: J2323-0617_X_2005_07_09_yyk_uvs.log on Fri Jan 20 11:10:52 2006
obs J2323-0617_X_2005_07_09_yyk_uve.fits
! Reading UV FITS file: J2323-0617_X_2005_07_09_yyk_uve.fits
! AN table 1: 13 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.786325 visibilities/baseline/integration-bin.
! Found source: J2323-0617
! 
! 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 1480 lines of history.
! 
! Reading 1840 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 J2323-0617_X_2005_07_09_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)= 0.172208 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 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 milli-arcsec
! Estimated beam: bmin=0.7174 mas, bmaj=1.823 mas, bpa=-1.283 degrees
! Estimated noise=1.19068 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 = 0.132061 Jy
! Component: 100  -  total flux cleaned = 0.160046 Jy
! Total flux subtracted in 100 components = 0.160046 Jy
! Clean residual min=-0.006165 max=0.007970 Jy/beam
! Clean residual mean=0.000000 rms=0.001647 Jy/beam
! Combined flux in latest and established models = 0.160046 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 12 model components to the UV plane model.
! The established model now contains 12 components and 0.160046 Jy
! 
! Correcting IF 1.
!  A total of 17 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 17 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 18 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 17 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.068911Jy  sigma=1.157118
! Fit after  self-cal, rms=0.068695Jy  sigma=1.152503
! Inverting map and beam 
! Your choice of large map pixels excluded 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 milli-arcsec
! Estimated beam: bmin=0.7174 mas, bmaj=1.823 mas, bpa=-1.283 degrees
! Estimated noise=1.19052 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 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 milli-arcsec
! Estimated beam: bmin=0.8894 mas, bmaj=2.106 mas, bpa=-0.1882 degrees
! Estimated noise=0.886764 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 = 0.0115947 Jy
! Component: 100  -  total flux cleaned = 0.0154651 Jy
! Component: 150  -  total flux cleaned = 0.0162753 Jy
! Component: 200  -  total flux cleaned = 0.0164756 Jy
! Total flux subtracted in 200 components = 0.0164756 Jy
! Clean residual min=-0.004935 max=0.004886 Jy/beam
! Clean residual mean=-0.000008 rms=0.001244 Jy/beam
! Combined flux in latest and established models = 0.176522 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 24 model components to the UV plane model.
! The established model now contains 26 components and 0.176522 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067518Jy  sigma=1.125861
! Fit after  self-cal, rms=0.067507Jy  sigma=1.125685
! Inverting map 
! Your choice of large map pixels excluded 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8894 x 2.106 at -0.1882 degrees (North through East)
! Clean map  min=-0.0046013  max=0.15708 Jy/beam
if(peak(flux) < thresh*2)
  selflims ampcor_selflim
  end if
! 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: 1.00922
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.96     FD        0.99     HN        1.00     KP        0.95     
!   LA        0.98     MK        1.03     NL        1.01     OV        1.02     
!   PT        0.98     SC        0.99     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 1.00911
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.97     FD        0.97     HN        1.02     KP        1.06     
!   LA        1.07     MK        0.98     NL        0.97     OV        0.97     
!   PT        0.98     SC        0.93     
! 
! 
! Correcting IF 3.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Amplitude normalization factor in sub-array 1: 1.00164
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.01     FD        1.05     HN        0.98     KP        0.86     
!   LA        0.97     MK        1.12     NL        0.94     OV        1.01     
!   PT        1.03     SC        1.01     
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 0.960922
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.04     FD        1.06     HN        1.02     KP        0.96     
!   LA        0.95     MK        0.96     NL        1.02     OV        1.11     
!   PT        1.09     SC        1.19     
! 
! 
! Fit before self-cal, rms=0.067507Jy  sigma=1.125685
! Fit after  self-cal, rms=0.066499Jy  sigma=1.105852
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=0.066499Jy  sigma=1.105852
! Fit after  self-cal, rms=0.066507Jy  sigma=1.105794
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 milli-arcsec
! Estimated beam: bmin=0.8978 mas, bmaj=2.122 mas, bpa=-0.1957 degrees
! Estimated noise=0.882543 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 = -0.00115024 Jy
! Component: 100  -  total flux cleaned = -0.00125927 Jy
! Component: 150  -  total flux cleaned = -0.00126024 Jy
! Component: 200  -  total flux cleaned = -0.00129068 Jy
! Total flux subtracted in 200 components = -0.00129068 Jy
! Clean residual min=-0.004452 max=0.004676 Jy/beam
! Clean residual mean=-0.000008 rms=0.001088 Jy/beam
! Combined flux in latest and established models = 0.175231 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 11 model components to the UV plane model.
! The established model now contains 32 components and 0.175231 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066479Jy  sigma=1.105067
! Fit after  self-cal, rms=0.066471Jy  sigma=1.105002
! Inverting map 
! Your choice of large map pixels excluded 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 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=0.066471Jy  sigma=1.105002
! Fit after  self-cal, rms=0.062665Jy  sigma=1.046100
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 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 = 0.000571093 Jy
! Component: 100  -  total flux cleaned = 0.000718384 Jy
! Component: 150  -  total flux cleaned = 0.000777617 Jy
! Component: 200  -  total flux cleaned = 0.000828333 Jy
! Total flux subtracted in 200 components = 0.000828333 Jy
! Clean residual min=-0.004434 max=0.004281 Jy/beam
! Clean residual mean=-0.000008 rms=0.001051 Jy/beam
! Combined flux in latest and established models = 0.176059 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 13 model components to the UV plane model.
! The established model now contains 36 components and 0.176059 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.062655Jy  sigma=1.045470
! Fit after  self-cal, rms=0.062136Jy  sigma=1.039519
! Inverting map 
! Your choice of large map pixels excluded 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 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: 0.8978 x 2.122 at -0.1957 degrees (North through East)
! Clean map  min=-0.0042027  max=0.15774 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=0.062136Jy  sigma=1.039519
! Fit after  self-cal, rms=0.062375Jy  sigma=1.024233
! 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=0.062375Jy  sigma=1.024233
! Fit after  self-cal, rms=0.062279Jy  sigma=1.023078
! Inverting map and beam 
! Your choice of large map pixels excluded 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 milli-arcsec
! Estimated beam: bmin=0.8946 mas, bmaj=2.125 mas, bpa=-0.5304 degrees
! Estimated noise=0.879984 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.000163541 Jy
! Component: 100  -  total flux cleaned = 0.000162936 Jy
! Component: 150  -  total flux cleaned = 0.000181066 Jy
! Component: 200  -  total flux cleaned = 0.000198899 Jy
! Total flux subtracted in 200 components = 0.000198899 Jy
! Clean residual min=-0.004473 max=0.004003 Jy/beam
! Clean residual mean=0.000002 rms=0.000948 Jy/beam
! Combined flux in latest and established models = 0.176258 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 10 model components to the UV plane model.
! The established model now contains 39 components and 0.176258 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.062262Jy  sigma=1.022823
! Fit after  self-cal, rms=0.062242Jy  sigma=1.022443
! Inverting map 
! Your choice of large map pixels excluded 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 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=0.062242Jy  sigma=1.022443
! Fit after  self-cal, rms=0.061646Jy  sigma=1.005183
! 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=0.061646Jy  sigma=1.005183
! Fit after  self-cal, rms=0.061648Jy  sigma=1.004939
! Inverting map and beam 
! Your choice of large map pixels excluded 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 milli-arcsec
! Estimated beam: bmin=0.9057 mas, bmaj=2.139 mas, bpa=-0.4343 degrees
! Estimated noise=0.87712 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.0012397 Jy
! Component: 100  -  total flux cleaned = -0.00144682 Jy
! Component: 150  -  total flux cleaned = -0.00151656 Jy
! Component: 200  -  total flux cleaned = -0.00156257 Jy
! Total flux subtracted in 200 components = -0.00156257 Jy
! Clean residual min=-0.004336 max=0.003886 Jy/beam
! Clean residual mean=0.000002 rms=0.000947 Jy/beam
! Combined flux in latest and established models = 0.174696 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 13 model components to the UV plane model.
! The established model now contains 46 components and 0.174696 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.061643Jy  sigma=1.004557
! Fit after  self-cal, rms=0.061643Jy  sigma=1.004453
! Inverting map 
! Your choice of large map pixels excluded 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 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 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 milli-arcsec
! Estimated beam: bmin=2.191 mas, bmaj=3.856 mas, bpa=6.306 degrees
! Estimated noise=1.11179 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 = 2.04491e-07 Jy
! Component: 100  -  total flux cleaned = 2.37307e-06 Jy
! Component: 150  -  total flux cleaned = 3.01585e-05 Jy
! Component: 200  -  total flux cleaned = 5.26169e-05 Jy
! Total flux subtracted in 200 components = 5.26169e-05 Jy
! Clean residual min=-0.004373 max=0.003745 Jy/beam
! Clean residual mean=0.000002 rms=0.001235 Jy/beam
! Combined flux in latest and established models = 0.174748 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 51 components and 0.174748 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.061643Jy  sigma=1.004699
! Fit after  self-cal, rms=0.061641Jy  sigma=1.004549
! Inverting map 
! Your choice of large map pixels excluded 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 milli-arcsec
uvtaper 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 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 milli-arcsec
! Estimated beam: bmin=0.7257 mas, bmaj=1.841 mas, bpa=-1.621 degrees
! Estimated noise=1.19752 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.133833 Jy
! Component: 100  -  total flux cleaned = 0.161275 Jy
! Component: 150  -  total flux cleaned = 0.170616 Jy
! Component: 200  -  total flux cleaned = 0.174963 Jy
! Total flux subtracted in 200 components = 0.174963 Jy
! Clean residual min=-0.005188 max=0.004176 Jy/beam
! Clean residual mean=0.000006 rms=0.001152 Jy/beam
! Combined flux in latest and established models = 0.174963 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 22 model components to the UV plane model.
! The established model now contains 22 components and 0.174963 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 milli-arcsec
! Estimated beam: bmin=0.9057 mas, bmaj=2.139 mas, bpa=-0.4343 degrees
! Estimated noise=0.87712 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 = -0.00032492 Jy
! Component: 100  -  total flux cleaned = -0.000264336 Jy
! Component: 150  -  total flux cleaned = -0.000164707 Jy
! Component: 200  -  total flux cleaned = -0.000122925 Jy
! Total flux subtracted in 200 components = -0.000122925 Jy
! Clean residual min=-0.004360 max=0.004075 Jy/beam
! Clean residual mean=0.000002 rms=0.000958 Jy/beam
! Combined flux in latest and established models = 0.17484 Jy
! Adding 14 model components to the UV plane model.
! The established model now contains 31 components and 0.17484 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 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 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 milli-arcsec
! Estimated beam: bmin=2.191 mas, bmaj=3.856 mas, bpa=6.306 degrees
! Estimated noise=1.11179 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 = -5.06779e-05 Jy
! Component: 100  -  total flux cleaned = -1.74171e-05 Jy
! Component: 150  -  total flux cleaned = 7.94132e-06 Jy
! Component: 200  -  total flux cleaned = 2.88258e-05 Jy
! Total flux subtracted in 200 components = 2.88258e-05 Jy
! Clean residual min=-0.004403 max=0.003804 Jy/beam
! Clean residual mean=0.000002 rms=0.001238 Jy/beam
! Combined flux in latest and established models = 0.174869 Jy
! Adding 6 model components to the UV plane model.
! The established model now contains 35 components and 0.174869 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 milli-arcsec
! Estimated beam: bmin=0.9057 mas, bmaj=2.139 mas, bpa=-0.4343 degrees
! Estimated noise=0.87712 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -8.11333e-05 Jy
! Component: 100  -  total flux cleaned = -7.90255e-05 Jy
! Component: 150  -  total flux cleaned = -7.85167e-05 Jy
! Component: 200  -  total flux cleaned = -0.000138401 Jy
! Total flux subtracted in 200 components = -0.000138401 Jy
! Clean residual min=-0.004392 max=0.003961 Jy/beam
! Clean residual mean=0.000002 rms=0.000950 Jy/beam
! Combined flux in latest and established models = 0.174731 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 11 model components to the UV plane model.
! The established model now contains 41 components and 0.174731 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.061644Jy  sigma=1.005003
! Fit after  self-cal, rms=0.061641Jy  sigma=1.004889
wmodel J2323-0617_X_2005_07_09_yyk\_map.mod
! Writing 41 model components to file: J2323-0617_X_2005_07_09_yyk_map.mod
wobs J2323-0617_X_2005_07_09_yyk\_uvs.fits
! Writing UV FITS file: J2323-0617_X_2005_07_09_yyk_uvs.fits
wwins J2323-0617_X_2005_07_09_yyk\_map.win
! wwins: Wrote 1 windows to J2323-0617_X_2005_07_09_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 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.000958347 Jy
! Component: 100  -  total flux cleaned = -0.00153906 Jy
! Component: 150  -  total flux cleaned = -0.00212115 Jy
! Component: 200  -  total flux cleaned = -0.00288319 Jy
! Component: 250  -  total flux cleaned = -0.00355885 Jy
! Component: 300  -  total flux cleaned = -0.00410752 Jy
! Component: 350  -  total flux cleaned = -0.00449234 Jy
! Component: 400  -  total flux cleaned = -0.00476992 Jy
! Component: 450  -  total flux cleaned = -0.00486039 Jy
! Component: 500  -  total flux cleaned = -0.00490467 Jy
! Component: 550  -  total flux cleaned = -0.00486168 Jy
! Component: 600  -  total flux cleaned = -0.00494599 Jy
! Component: 650  -  total flux cleaned = -0.00494704 Jy
! Component: 700  -  total flux cleaned = -0.00510887 Jy
! Component: 750  -  total flux cleaned = -0.0050296 Jy
! Component: 800  -  total flux cleaned = -0.00510769 Jy
! Component: 850  -  total flux cleaned = -0.00510724 Jy
! Component: 900  -  total flux cleaned = -0.00510746 Jy
! Component: 950  -  total flux cleaned = -0.00510703 Jy
! Component: 1000  -  total flux cleaned = -0.00510639 Jy
! Component: 1050  -  total flux cleaned = -0.00510637 Jy
! Component: 1100  -  total flux cleaned = -0.00517665 Jy
! Component: 1150  -  total flux cleaned = -0.0051769 Jy
! Component: 1200  -  total flux cleaned = -0.00517639 Jy
! Component: 1250  -  total flux cleaned = -0.00517588 Jy
! Component: 1300  -  total flux cleaned = -0.00514362 Jy
! Component: 1350  -  total flux cleaned = -0.00520816 Jy
! Component: 1400  -  total flux cleaned = -0.00517611 Jy
! Component: 1450  -  total flux cleaned = -0.00508231 Jy
! Component: 1500  -  total flux cleaned = -0.00514401 Jy
! Component: 1550  -  total flux cleaned = -0.00520396 Jy
! Component: 1600  -  total flux cleaned = -0.00523325 Jy
! Component: 1650  -  total flux cleaned = -0.00514483 Jy
! Component: 1700  -  total flux cleaned = -0.00526098 Jy
! Component: 1750  -  total flux cleaned = -0.00526144 Jy
! Component: 1800  -  total flux cleaned = -0.00534678 Jy
! Component: 1850  -  total flux cleaned = -0.00534699 Jy
! Component: 1900  -  total flux cleaned = -0.00542971 Jy
! Component: 1950  -  total flux cleaned = -0.00548429 Jy
! Component: 2000  -  total flux cleaned = -0.00548419 Jy
! Total flux subtracted in 2048 components = -0.0055644 Jy
! Clean residual min=-0.001851 max=0.001377 Jy/beam
! Clean residual mean=-0.000001 rms=0.000517 Jy/beam
! Combined flux in latest and established models = 0.169166 Jy
keep
! Adding 138 model components to the UV plane model.
! The established model now contains 179 components and 0.169166 Jy
![Exited script file: muppet]
wmap "J2323-0617_X_2005_07_09_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.9057 x 2.139 at -0.4343 degrees (North through East)
! Clean map  min=-0.0026766  max=0.15748 Jy/beam
! Writing clean map to FITS file: J2323-0617_X_2005_07_09_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.157478 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.28% of the data.
!  The x-axis pixel size should ideally be below 0.1998 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000510104 
device "J2323-0617_X_2005_07_09_yyk\_map.eps/VPS"
! Attempting to open device: 'J2323-0617_X_2005_07_09_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.971762 0.971762 1.94352 3.88705 7.7741 15.5482 31.0964 62.1928
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0015 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.157 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.9057 x 2.139 at -0.4343 degrees (North through East)
! Clean map  min=-0.0026766  max=0.15748 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J2323-0617_X_2005_07_09_yyk\_map.gif/gif"
! Attempting to open device: 'J2323-0617_X_2005_07_09_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J2323-0617_X_2005_07_09_yyk_uvs.log closed on Fri Jan 20 11:10:56 2006