! Started logfile: J0331-2524_X_2005_07_20_yyk_uvs.log on Fri Jan 20 09:51:03 2006
obs J0331-2524_X_2005_07_20_yyk_uve.fits
! Reading UV FITS file: J0331-2524_X_2005_07_20_yyk_uve.fits
! AN table 1: 14 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.938095 visibilities/baseline/integration-bin.
! Found source: J0331-2524
! 
! 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 1487 lines of history.
! 
! Reading 2364 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 J0331-2524_X_2005_07_20_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)= 0.176179 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 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.6894 mas, bmaj=1.775 mas, bpa=-1.643 degrees
! Estimated noise=1.31043 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 = 0.129304 Jy
! Component: 100  -  total flux cleaned = 0.152278 Jy
! Total flux subtracted in 100 components = 0.152278 Jy
! Clean residual min=-0.007181 max=0.010884 Jy/beam
! Clean residual mean=-0.000035 rms=0.002250 Jy/beam
! Combined flux in latest and established models = 0.152278 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 0.152278 Jy
! 
! Correcting IF 1.
!  A total of 6 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 6 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 7 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 6 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.081759Jy  sigma=1.243644
! Fit after  self-cal, rms=0.080916Jy  sigma=1.236390
! Inverting map and beam 
! Your choice of large map pixels excluded 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.6895 mas, bmaj=1.775 mas, bpa=-1.643 degrees
! Estimated noise=1.31036 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 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.8664 mas, bmaj=2.233 mas, bpa=-0.7004 degrees
! Estimated noise=0.855329 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 (0.2, -2.6).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0201609 Jy
! Component: 100  -  total flux cleaned = 0.0292146 Jy
! Component: 150  -  total flux cleaned = 0.0344409 Jy
! Component: 200  -  total flux cleaned = 0.0374348 Jy
! Total flux subtracted in 200 components = 0.0374348 Jy
! Clean residual min=-0.004840 max=0.006356 Jy/beam
! Clean residual mean=0.000045 rms=0.001611 Jy/beam
! Combined flux in latest and established models = 0.189713 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 38 model components to the UV plane model.
! The established model now contains 45 components and 0.189713 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.078195Jy  sigma=1.166798
! Fit after  self-cal, rms=0.078085Jy  sigma=1.164287
! Inverting map 
! Your choice of large map pixels excluded 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8664 x 2.233 at -0.7004 degrees (North through East)
! Clean map  min=-0.0046402  max=0.15004 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
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    OV        1.00*    
!   PT        1.00*    SC        1.00*    
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 1.02505
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.97     FD        0.97     HN        1.06     KP        0.90     
!   LA        0.96     MK        0.99     NL        0.92     OV        0.95     
!   PT        1.08     SC        0.96     
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 1
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    OV        1.00*    
!   PT        1.00*    SC        1.00*    
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 1
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    OV        1.00*    
!   PT        1.00*    SC        1.00*    
! 
! 
! Fit before self-cal, rms=0.078085Jy  sigma=1.164287
! Fit after  self-cal, rms=0.077861Jy  sigma=1.158716
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=0.077861Jy  sigma=1.158716
! Fit after  self-cal, rms=0.077814Jy  sigma=1.158289
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.8679 mas, bmaj=2.232 mas, bpa=-0.4689 degrees
! Estimated noise=0.853997 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 = 0.00284187 Jy
! Component: 100  -  total flux cleaned = 0.00339931 Jy
! Component: 150  -  total flux cleaned = 0.00372505 Jy
! Component: 200  -  total flux cleaned = 0.00402281 Jy
! Total flux subtracted in 200 components = 0.00402281 Jy
! Clean residual min=-0.004572 max=0.005576 Jy/beam
! Clean residual mean=0.000040 rms=0.001413 Jy/beam
! Combined flux in latest and established models = 0.193736 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 20 model components to the UV plane model.
! The established model now contains 56 components and 0.193736 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.077634Jy  sigma=1.155122
! Fit after  self-cal, rms=0.077598Jy  sigma=1.154626
! Inverting map 
! Your choice of large map pixels excluded 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 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=0.077598Jy  sigma=1.154626
! Fit after  self-cal, rms=0.066867Jy  sigma=1.014704
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 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 = 0.00180488 Jy
! Component: 100  -  total flux cleaned = 0.00152503 Jy
! Component: 150  -  total flux cleaned = 0.00145229 Jy
! Component: 200  -  total flux cleaned = 0.00144698 Jy
! Total flux subtracted in 200 components = 0.00144698 Jy
! Clean residual min=-0.003931 max=0.005094 Jy/beam
! Clean residual mean=0.000045 rms=0.001285 Jy/beam
! Combined flux in latest and established models = 0.195183 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 16 model components to the UV plane model.
! The established model now contains 65 components and 0.195183 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066656Jy  sigma=1.010754
! Fit after  self-cal, rms=0.065653Jy  sigma=0.999290
! Inverting map 
! Your choice of large map pixels excluded 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 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: 0.8679 x 2.232 at -0.4689 degrees (North through East)
! Clean map  min=-0.0037524  max=0.15294 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=0.065653Jy  sigma=0.999290
! Fit after  self-cal, rms=0.064038Jy  sigma=0.980711
! 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=0.064038Jy  sigma=0.980711
! Fit after  self-cal, rms=0.063889Jy  sigma=0.979133
! Inverting map and beam 
! Your choice of large map pixels excluded 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.8641 mas, bmaj=2.207 mas, bpa=-1.184 degrees
! Estimated noise=0.834342 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.0025405 Jy
! Component: 100  -  total flux cleaned = -0.00287918 Jy
! Component: 150  -  total flux cleaned = -0.00294383 Jy
! Component: 200  -  total flux cleaned = -0.00294354 Jy
! Total flux subtracted in 200 components = -0.00294354 Jy
! Clean residual min=-0.003977 max=0.003304 Jy/beam
! Clean residual mean=0.000026 rms=0.000909 Jy/beam
! Combined flux in latest and established models = 0.192239 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 17 model components to the UV plane model.
! The established model now contains 78 components and 0.192239 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.063743Jy  sigma=0.975831
! Fit after  self-cal, rms=0.063693Jy  sigma=0.975436
! Inverting map 
! Your choice of large map pixels excluded 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 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=0.063693Jy  sigma=0.975436
! Fit after  self-cal, rms=0.062984Jy  sigma=0.967231
! 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=0.062984Jy  sigma=0.967231
! Fit after  self-cal, rms=0.062974Jy  sigma=0.967138
! Inverting map and beam 
! Your choice of large map pixels excluded 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.8638 mas, bmaj=2.193 mas, bpa=-0.9701 degrees
! Estimated noise=0.824861 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.00169587 Jy
! Component: 100  -  total flux cleaned = -0.00189544 Jy
! Component: 150  -  total flux cleaned = -0.00194281 Jy
! Component: 200  -  total flux cleaned = -0.00194055 Jy
! Total flux subtracted in 200 components = -0.00194055 Jy
! Clean residual min=-0.003657 max=0.003045 Jy/beam
! Clean residual mean=0.000025 rms=0.000853 Jy/beam
! Combined flux in latest and established models = 0.190299 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 20 model components to the UV plane model.
! The established model now contains 85 components and 0.190299 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.062895Jy  sigma=0.965182
! Fit after  self-cal, rms=0.062881Jy  sigma=0.965032
! Inverting map 
! Your choice of large map pixels excluded 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 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 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=2.386 mas, bmaj=5.908 mas, bpa=6.068 degrees
! Estimated noise=1.05669 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 = 0.000195478 Jy
! Component: 100  -  total flux cleaned = 0.000245043 Jy
! Component: 150  -  total flux cleaned = 0.000265636 Jy
! Component: 200  -  total flux cleaned = 0.000248005 Jy
! Total flux subtracted in 200 components = 0.000248005 Jy
! Clean residual min=-0.003329 max=0.003521 Jy/beam
! Clean residual mean=0.000048 rms=0.001127 Jy/beam
! Combined flux in latest and established models = 0.190547 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 21 model components to the UV plane model.
! The established model now contains 97 components and 0.190547 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.062872Jy  sigma=0.964922
! Fit after  self-cal, rms=0.062867Jy  sigma=0.964869
! Inverting map 
! Your choice of large map pixels excluded 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 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 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.6873 mas, bmaj=1.758 mas, bpa=-1.999 degrees
! Estimated noise=1.26639 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.129688 Jy
! Component: 100  -  total flux cleaned = 0.155922 Jy
! Component: 150  -  total flux cleaned = 0.167958 Jy
! Component: 200  -  total flux cleaned = 0.175151 Jy
! Total flux subtracted in 200 components = 0.175151 Jy
! Clean residual min=-0.006085 max=0.004914 Jy/beam
! Clean residual mean=-0.000005 rms=0.001370 Jy/beam
! Combined flux in latest and established models = 0.175151 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 0.175151 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.8638 mas, bmaj=2.193 mas, bpa=-0.9701 degrees
! Estimated noise=0.824861 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 = 0.0071477 Jy
! Component: 100  -  total flux cleaned = 0.0107977 Jy
! Component: 150  -  total flux cleaned = 0.0116701 Jy
! Component: 200  -  total flux cleaned = 0.0123856 Jy
! Total flux subtracted in 200 components = 0.0123856 Jy
! Clean residual min=-0.003286 max=0.003252 Jy/beam
! Clean residual mean=0.000018 rms=0.000892 Jy/beam
! Combined flux in latest and established models = 0.187537 Jy
! Adding 25 model components to the UV plane model.
! The established model now contains 52 components and 0.187537 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 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 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=2.386 mas, bmaj=5.908 mas, bpa=6.068 degrees
! Estimated noise=1.05669 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 = 0.00164588 Jy
! Component: 100  -  total flux cleaned = 0.00177196 Jy
! Component: 150  -  total flux cleaned = 0.00188225 Jy
! Component: 200  -  total flux cleaned = 0.00200859 Jy
! Total flux subtracted in 200 components = 0.00200859 Jy
! Clean residual min=-0.003115 max=0.003619 Jy/beam
! Clean residual mean=0.000045 rms=0.001138 Jy/beam
! Combined flux in latest and established models = 0.189545 Jy
! Adding 17 model components to the UV plane model.
! The established model now contains 65 components and 0.189545 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! Estimated beam: bmin=0.8638 mas, bmaj=2.193 mas, bpa=-0.9701 degrees
! Estimated noise=0.824861 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.000110268 Jy
! Component: 100  -  total flux cleaned = -0.000168208 Jy
! Component: 150  -  total flux cleaned = -7.34591e-05 Jy
! Component: 200  -  total flux cleaned = -3.1478e-05 Jy
! Total flux subtracted in 200 components = -3.1478e-05 Jy
! Clean residual min=-0.003547 max=0.003163 Jy/beam
! Clean residual mean=0.000023 rms=0.000866 Jy/beam
! Combined flux in latest and established models = 0.189514 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 17 model components to the UV plane model.
! The established model now contains 77 components and 0.189514 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.062942Jy  sigma=0.966201
! Fit after  self-cal, rms=0.062924Jy  sigma=0.965849
wmodel J0331-2524_X_2005_07_20_yyk\_map.mod
! Writing 77 model components to file: J0331-2524_X_2005_07_20_yyk_map.mod
wobs J0331-2524_X_2005_07_20_yyk\_uvs.fits
! Writing UV FITS file: J0331-2524_X_2005_07_20_yyk_uvs.fits
wwins J0331-2524_X_2005_07_20_yyk\_map.win
! wwins: Wrote 2 windows to J0331-2524_X_2005_07_20_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 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.000341231 Jy
! Component: 100  -  total flux cleaned = 0.000351642 Jy
! Component: 150  -  total flux cleaned = 0.000752821 Jy
! Component: 200  -  total flux cleaned = 0.00113525 Jy
! Component: 250  -  total flux cleaned = 0.00136517 Jy
! Component: 300  -  total flux cleaned = 0.00158675 Jy
! Component: 350  -  total flux cleaned = 0.00171637 Jy
! Component: 400  -  total flux cleaned = 0.00171685 Jy
! Component: 450  -  total flux cleaned = 0.00183961 Jy
! Component: 500  -  total flux cleaned = 0.00183905 Jy
! Component: 550  -  total flux cleaned = 0.0018003 Jy
! Component: 600  -  total flux cleaned = 0.00191578 Jy
! Component: 650  -  total flux cleaned = 0.00195353 Jy
! Component: 700  -  total flux cleaned = 0.00210065 Jy
! Component: 750  -  total flux cleaned = 0.00224465 Jy
! Component: 800  -  total flux cleaned = 0.00245622 Jy
! Component: 850  -  total flux cleaned = 0.00249117 Jy
! Component: 900  -  total flux cleaned = 0.00266283 Jy
! Component: 950  -  total flux cleaned = 0.0027301 Jy
! Component: 1000  -  total flux cleaned = 0.00283017 Jy
! Component: 1050  -  total flux cleaned = 0.00292829 Jy
! Component: 1100  -  total flux cleaned = 0.00296097 Jy
! Component: 1150  -  total flux cleaned = 0.00299266 Jy
! Component: 1200  -  total flux cleaned = 0.00302346 Jy
! Component: 1250  -  total flux cleaned = 0.00305391 Jy
! Component: 1300  -  total flux cleaned = 0.00293205 Jy
! Component: 1350  -  total flux cleaned = 0.00305251 Jy
! Component: 1400  -  total flux cleaned = 0.00305262 Jy
! Component: 1450  -  total flux cleaned = 0.00314065 Jy
! Component: 1500  -  total flux cleaned = 0.00319853 Jy
! Component: 1550  -  total flux cleaned = 0.00322739 Jy
! Component: 1600  -  total flux cleaned = 0.00308683 Jy
! Component: 1650  -  total flux cleaned = 0.00308728 Jy
! Component: 1700  -  total flux cleaned = 0.00311499 Jy
! Component: 1750  -  total flux cleaned = 0.00311481 Jy
! Component: 1800  -  total flux cleaned = 0.00316909 Jy
! Component: 1850  -  total flux cleaned = 0.0032755 Jy
! Component: 1900  -  total flux cleaned = 0.00330178 Jy
! Component: 1950  -  total flux cleaned = 0.00332769 Jy
! Component: 2000  -  total flux cleaned = 0.00345584 Jy
! Total flux subtracted in 2048 components = 0.00342968 Jy
! Clean residual min=-0.001465 max=0.001360 Jy/beam
! Clean residual mean=0.000012 rms=0.000481 Jy/beam
! Combined flux in latest and established models = 0.192944 Jy
keep
! Adding 147 model components to the UV plane model.
! The established model now contains 224 components and 0.192944 Jy
![Exited script file: muppet]
wmap "J0331-2524_X_2005_07_20_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8638 x 2.193 at -0.9701 degrees (North through East)
! Clean map  min=-0.0030175  max=0.15056 Jy/beam
! Writing clean map to FITS file: J0331-2524_X_2005_07_20_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.150563 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.305% of the data.
!  The x-axis pixel size should ideally be below 0.1996 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000479149 
device "J0331-2524_X_2005_07_20_yyk\_map.eps/VPS"
! Attempting to open device: 'J0331-2524_X_2005_07_20_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.954714 0.954714 1.90943 3.81886 7.63772 15.2754 30.5509 61.1017
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0014 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.15 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8638 x 2.193 at -0.9701 degrees (North through East)
! Clean map  min=-0.0030175  max=0.15056 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0331-2524_X_2005_07_20_yyk\_map.gif/gif"
! Attempting to open device: 'J0331-2524_X_2005_07_20_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J0331-2524_X_2005_07_20_yyk_uvs.log closed on Fri Jan 20 09:51:07 2006