! Started logfile: J2025-2845_X_2005_07_08_yyk_uvs.log on Fri Jan 20 10:58:56 2006
obs J2025-2845_X_2005_07_08_yyk_uve.fits
! Reading UV FITS file: J2025-2845_X_2005_07_08_yyk_uve.fits
! AN table 1: 10 integrations on 45 of 45 possible baselines.
! Apparent sampling: 1 visibilities/baseline/integration-bin.
! Found source: J2025-2845
! 
! 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 1406 lines of history.
! 
! Reading 1800 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 J2025-2845_X_2005_07_08_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)= 0.289714 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 0.311% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.6416 mas, bmaj=1.748 mas, bpa=1.978 degrees
! Estimated noise=1.6104 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 = 0.229825 Jy
! Component: 100  -  total flux cleaned = 0.274073 Jy
! Total flux subtracted in 100 components = 0.274073 Jy
! Clean residual min=-0.007800 max=0.014891 Jy/beam
! Clean residual mean=-0.000037 rms=0.002646 Jy/beam
! Combined flux in latest and established models = 0.274073 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 7 model components to the UV plane model.
! The established model now contains 7 components and 0.274073 Jy
! 
! Correcting IF 1.
!  A total of 5 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 5 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 5 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 5 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.094412Jy  sigma=1.257244
! Fit after  self-cal, rms=0.094211Jy  sigma=1.251812
! Inverting map and beam 
! Your choice of large map pixels excluded 0.311% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.6416 mas, bmaj=1.748 mas, bpa=1.978 degrees
! Estimated noise=1.6104 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 0.311% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8487 mas, bmaj=2.193 mas, bpa=1.691 degrees
! Estimated noise=1.06573 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 (-1, -2.4).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0271227 Jy
! Component: 100  -  total flux cleaned = 0.0377172 Jy
! Component: 150  -  total flux cleaned = 0.0414323 Jy
! Component: 200  -  total flux cleaned = 0.042189 Jy
! Total flux subtracted in 200 components = 0.042189 Jy
! Clean residual min=-0.007642 max=0.006737 Jy/beam
! Clean residual mean=0.000018 rms=0.001726 Jy/beam
! Combined flux in latest and established models = 0.316262 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 31 model components to the UV plane model.
! The established model now contains 38 components and 0.316262 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.090488Jy  sigma=1.144604
! Fit after  self-cal, rms=0.090340Jy  sigma=1.141680
! Inverting map 
! Your choice of large map pixels excluded 0.311% 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: 0.8487 x 2.193 at 1.691 degrees (North through East)
! Clean map  min=-0.0070404  max=0.26794 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: 0.989221
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.96     FD        0.97     HN        1.28     KP        0.96     
!   LA        1.02     MK        0.96     NL        1.03     OV        1.01     
!   PT        0.95     SC        0.98     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 0.984261
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.96     FD        0.99     HN        1.38     KP        0.91     
!   LA        0.98     MK        1.02     NL        1.04     OV        0.97     
!   PT        1.01     SC        0.92     
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 0.990922
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.03     FD        1.01     HN        1.20     KP        0.84     
!   LA        0.96     MK        1.03     NL        1.01     OV        1.02     
!   PT        1.05     SC        0.93     
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 0.932603
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.08     FD        1.05     HN        1.17     KP        0.98     
!   LA        1.00     MK        1.03     NL        1.01     OV        1.04     
!   PT        1.12     SC        1.25     
! 
! 
! Fit before self-cal, rms=0.090340Jy  sigma=1.141680
! Fit after  self-cal, rms=0.087541Jy  sigma=1.090474
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=0.087541Jy  sigma=1.090474
! Fit after  self-cal, rms=0.087552Jy  sigma=1.090439
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.311% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8538 mas, bmaj=2.201 mas, bpa=1.931 degrees
! Estimated noise=1.01252 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 = -0.011602 Jy
! Component: 100  -  total flux cleaned = -0.0142705 Jy
! Component: 150  -  total flux cleaned = -0.0146914 Jy
! Component: 200  -  total flux cleaned = -0.0148082 Jy
! Total flux subtracted in 200 components = -0.0148082 Jy
! Clean residual min=-0.003015 max=0.004501 Jy/beam
! Clean residual mean=-0.000008 rms=0.000945 Jy/beam
! Combined flux in latest and established models = 0.301454 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 28 model components to the UV plane model.
! The established model now contains 63 components and 0.301454 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.086344Jy  sigma=1.064397
! Fit after  self-cal, rms=0.086343Jy  sigma=1.064366
! Inverting map 
! Your choice of large map pixels excluded 0.311% 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=0.086343Jy  sigma=1.064366
! Fit after  self-cal, rms=0.084142Jy  sigma=1.019467
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.311% 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)
! Added new window around map position (4, 12.8).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00354467 Jy
! Component: 100  -  total flux cleaned = 0.00388946 Jy
! Component: 150  -  total flux cleaned = 0.00429762 Jy
! Component: 200  -  total flux cleaned = 0.0045326 Jy
! Total flux subtracted in 200 components = 0.0045326 Jy
! Clean residual min=-0.003187 max=0.003417 Jy/beam
! Clean residual mean=0.000002 rms=0.000851 Jy/beam
! Combined flux in latest and established models = 0.305986 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 25 model components to the UV plane model.
! The established model now contains 84 components and 0.305986 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.083885Jy  sigma=1.014840
! Fit after  self-cal, rms=0.083930Jy  sigma=1.011713
! Inverting map 
! Your choice of large map pixels excluded 0.311% 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: 0.8538 x 2.201 at 1.931 degrees (North through East)
! Clean map  min=-0.0029333  max=0.25635 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=0.083930Jy  sigma=1.011713
! Fit after  self-cal, rms=0.083258Jy  sigma=0.981337
! 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=0.083258Jy  sigma=0.981337
! Fit after  self-cal, rms=0.083366Jy  sigma=0.980981
! Inverting map and beam 
! Your choice of large map pixels excluded 0.311% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8517 mas, bmaj=2.201 mas, bpa=2.051 degrees
! Estimated noise=1.01087 mJy/beam.
! Added new window around map position (12.2, -22.2).
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00141186 Jy
! Component: 100  -  total flux cleaned = 0.00114533 Jy
! Component: 150  -  total flux cleaned = 0.00107729 Jy
! Component: 200  -  total flux cleaned = 0.00107866 Jy
! Total flux subtracted in 200 components = 0.00107866 Jy
! Clean residual min=-0.002622 max=0.002851 Jy/beam
! Clean residual mean=-0.000011 rms=0.000719 Jy/beam
! Combined flux in latest and established models = 0.307065 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 19 model components to the UV plane model.
! The established model now contains 100 components and 0.307065 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.083133Jy  sigma=0.977096
! Fit after  self-cal, rms=0.083179Jy  sigma=0.976893
! Inverting map 
! Your choice of large map pixels excluded 0.311% 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=0.083179Jy  sigma=0.976893
! Fit after  self-cal, rms=0.083395Jy  sigma=0.955508
! 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=0.083395Jy  sigma=0.955508
! Fit after  self-cal, rms=0.083422Jy  sigma=0.955470
! Inverting map and beam 
! Your choice of large map pixels excluded 0.311% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8522 mas, bmaj=2.202 mas, bpa=1.981 degrees
! Estimated noise=1.01101 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0005861 Jy
! Component: 100  -  total flux cleaned = 0.000589606 Jy
! Component: 150  -  total flux cleaned = 0.000644474 Jy
! Component: 200  -  total flux cleaned = 0.000693156 Jy
! Total flux subtracted in 200 components = 0.000693156 Jy
! Clean residual min=-0.002560 max=0.002788 Jy/beam
! Clean residual mean=-0.000009 rms=0.000701 Jy/beam
! Combined flux in latest and established models = 0.307758 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 22 model components to the UV plane model.
! The established model now contains 108 components and 0.307758 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.083356Jy  sigma=0.954115
! Fit after  self-cal, rms=0.083366Jy  sigma=0.954086
! Inverting map 
! Your choice of large map pixels excluded 0.311% 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 0.311% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=2.545 mas, bmaj=7.081 mas, bpa=7.715 degrees
! Estimated noise=1.28683 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 = 0.000316959 Jy
! Component: 100  -  total flux cleaned = 0.000455489 Jy
! Component: 150  -  total flux cleaned = 0.00040921 Jy
! Component: 200  -  total flux cleaned = 0.000431099 Jy
! Total flux subtracted in 200 components = 0.000431099 Jy
! Clean residual min=-0.002716 max=0.002696 Jy/beam
! Clean residual mean=-0.000008 rms=0.000821 Jy/beam
! Combined flux in latest and established models = 0.308189 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 25 model components to the UV plane model.
! The established model now contains 131 components and 0.308189 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.083363Jy  sigma=0.954035
! Fit after  self-cal, rms=0.083375Jy  sigma=0.954027
! Inverting map 
! Your choice of large map pixels excluded 0.311% of the data.
!  The x-axis pixel size should ideally be below 0.1989 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 0.311% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.645 mas, bmaj=1.75 mas, bpa=1.929 degrees
! Estimated noise=1.5651 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.223896 Jy
! Component: 100  -  total flux cleaned = 0.267027 Jy
! Component: 150  -  total flux cleaned = 0.281512 Jy
! Component: 200  -  total flux cleaned = 0.289612 Jy
! Total flux subtracted in 200 components = 0.289612 Jy
! Clean residual min=-0.006108 max=0.005771 Jy/beam
! Clean residual mean=-0.000021 rms=0.001513 Jy/beam
! Combined flux in latest and established models = 0.289612 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 0.289612 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.311% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8522 mas, bmaj=2.202 mas, bpa=1.981 degrees
! Estimated noise=1.01101 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 = 0.00993357 Jy
! Component: 100  -  total flux cleaned = 0.0148256 Jy
! Component: 150  -  total flux cleaned = 0.0167813 Jy
! Component: 200  -  total flux cleaned = 0.0172919 Jy
! Total flux subtracted in 200 components = 0.0172919 Jy
! Clean residual min=-0.002796 max=0.002858 Jy/beam
! Clean residual mean=-0.000007 rms=0.000764 Jy/beam
! Combined flux in latest and established models = 0.306904 Jy
! Adding 39 model components to the UV plane model.
! The established model now contains 67 components and 0.306904 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.311% 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 0.311% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=2.545 mas, bmaj=7.081 mas, bpa=7.715 degrees
! Estimated noise=1.28683 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 = 0.00127758 Jy
! Component: 100  -  total flux cleaned = 0.00128547 Jy
! Component: 150  -  total flux cleaned = 0.00117409 Jy
! Component: 200  -  total flux cleaned = 0.00107375 Jy
! Total flux subtracted in 200 components = 0.00107375 Jy
! Clean residual min=-0.002677 max=0.002514 Jy/beam
! Clean residual mean=-0.000005 rms=0.000827 Jy/beam
! Combined flux in latest and established models = 0.307978 Jy
! Adding 29 model components to the UV plane model.
! The established model now contains 93 components and 0.307978 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.311% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.311% of the data.
!  The x-axis pixel size should ideally be below 0.1989 milli-arcsec
! Estimated beam: bmin=0.8522 mas, bmaj=2.202 mas, bpa=1.981 degrees
! Estimated noise=1.01101 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.000116378 Jy
! Component: 100  -  total flux cleaned = -0.000106329 Jy
! Component: 150  -  total flux cleaned = -0.000169908 Jy
! Component: 200  -  total flux cleaned = -0.000223916 Jy
! Total flux subtracted in 200 components = -0.000223916 Jy
! Clean residual min=-0.002654 max=0.002794 Jy/beam
! Clean residual mean=-0.000006 rms=0.000713 Jy/beam
! Combined flux in latest and established models = 0.307754 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 21 model components to the UV plane model.
! The established model now contains 104 components and 0.307754 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.083338Jy  sigma=0.955352
! Fit after  self-cal, rms=0.083309Jy  sigma=0.955213
wmodel J2025-2845_X_2005_07_08_yyk\_map.mod
! Writing 104 model components to file: J2025-2845_X_2005_07_08_yyk_map.mod
wobs J2025-2845_X_2005_07_08_yyk\_uvs.fits
! Writing UV FITS file: J2025-2845_X_2005_07_08_yyk_uvs.fits
wwins J2025-2845_X_2005_07_08_yyk\_map.win
! wwins: Wrote 4 windows to J2025-2845_X_2005_07_08_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 0.311% 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 = 0.000475324 Jy
! Component: 100  -  total flux cleaned = 0.000668213 Jy
! Component: 150  -  total flux cleaned = 0.000986767 Jy
! Component: 200  -  total flux cleaned = 0.00111842 Jy
! Component: 250  -  total flux cleaned = 0.00120243 Jy
! Component: 300  -  total flux cleaned = 0.00148608 Jy
! Component: 350  -  total flux cleaned = 0.00160421 Jy
! Component: 400  -  total flux cleaned = 0.00179581 Jy
! Component: 450  -  total flux cleaned = 0.00198213 Jy
! Component: 500  -  total flux cleaned = 0.00201949 Jy
! Component: 550  -  total flux cleaned = 0.00219779 Jy
! Component: 600  -  total flux cleaned = 0.00219763 Jy
! Component: 650  -  total flux cleaned = 0.00229968 Jy
! Component: 700  -  total flux cleaned = 0.00226638 Jy
! Component: 750  -  total flux cleaned = 0.00226689 Jy
! Component: 800  -  total flux cleaned = 0.00236378 Jy
! Component: 850  -  total flux cleaned = 0.00236353 Jy
! Component: 900  -  total flux cleaned = 0.00236335 Jy
! Component: 950  -  total flux cleaned = 0.00239396 Jy
! Component: 1000  -  total flux cleaned = 0.00242446 Jy
! Component: 1050  -  total flux cleaned = 0.00254348 Jy
! Component: 1100  -  total flux cleaned = 0.00257248 Jy
! Component: 1150  -  total flux cleaned = 0.00251443 Jy
! Component: 1200  -  total flux cleaned = 0.00257196 Jy
! Component: 1250  -  total flux cleaned = 0.00265677 Jy
! Component: 1300  -  total flux cleaned = 0.00262849 Jy
! Component: 1350  -  total flux cleaned = 0.00260117 Jy
! Component: 1400  -  total flux cleaned = 0.00265555 Jy
! Component: 1450  -  total flux cleaned = 0.00257496 Jy
! Component: 1500  -  total flux cleaned = 0.00268138 Jy
! Component: 1550  -  total flux cleaned = 0.00268074 Jy
! Component: 1600  -  total flux cleaned = 0.00270624 Jy
! Component: 1650  -  total flux cleaned = 0.00270614 Jy
! Component: 1700  -  total flux cleaned = 0.00283292 Jy
! Component: 1750  -  total flux cleaned = 0.0029081 Jy
! Component: 1800  -  total flux cleaned = 0.00298251 Jy
! Component: 1850  -  total flux cleaned = 0.00313066 Jy
! Component: 1900  -  total flux cleaned = 0.00320411 Jy
! Component: 1950  -  total flux cleaned = 0.00347029 Jy
! Component: 2000  -  total flux cleaned = 0.00358973 Jy
! Total flux subtracted in 2048 components = 0.00370775 Jy
! Clean residual min=-0.001375 max=0.001289 Jy/beam
! Clean residual mean=-0.000004 rms=0.000440 Jy/beam
! Combined flux in latest and established models = 0.311462 Jy
keep
! Adding 130 model components to the UV plane model.
! The established model now contains 234 components and 0.311462 Jy
![Exited script file: muppet]
wmap "J2025-2845_X_2005_07_08_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.311% 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: 0.8522 x 2.202 at 1.981 degrees (North through East)
! Clean map  min=-0.0021561  max=0.25903 Jy/beam
! Writing clean map to FITS file: J2025-2845_X_2005_07_08_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.259027 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.311% 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 0.000437988 
device "J2025-2845_X_2005_07_08_yyk\_map.eps/VPS"
! Attempting to open device: 'J2025-2845_X_2005_07_08_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.50727 0.50727 1.01454 2.02908 4.05816 8.11631 16.2326 32.4652 64.9305
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0013 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.259 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8522 x 2.202 at 1.981 degrees (North through East)
! Clean map  min=-0.0021561  max=0.25903 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J2025-2845_X_2005_07_08_yyk\_map.gif/gif"
! Attempting to open device: 'J2025-2845_X_2005_07_08_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J2025-2845_X_2005_07_08_yyk_uvs.log closed on Fri Jan 20 10:59:01 2006