! Started logfile: J1700-2610_X_2004_04_30_yyk_uvs.log on Wed Dec  7 00:38:44 2005
obs J1700-2610_X_2004_04_30_yyk_uve.fits
! Reading UV FITS file: J1700-2610_X_2004_04_30_yyk_uve.fits
! AN table 1: 4 integrations on 45 of 45 possible baselines.
! Apparent sampling: 1 visibilities/baseline/integration-bin.
! Found source: J1700-2610
! 
! 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 1544 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 J1700-2610_X_2004_04_30_yyk]
integer clean_niter
clean_niter = 100
float clean_gain
clean_gain = 0.04
float dynam
dynam = 6.0
float amp_soltime1
amp_soltime1 = 10
float amp_soltime2
amp_soltime2 = 1
float phase_soltime1
phase_soltime1=10
float phase_soltime2
phase_soltime2=0.5
float phase_soltime
phase_soltime=phase_soltime1
float ampcor_selflim
ampcor_selflim=1.20
float thresh
thresh = 0.10
float win_mult
win_mult = 1.8
float time_av
time_av = 30
float old_peak
float new_peak
float flux_cutoff
mapsize field_size, field_cell
! Map grid = 512x512 pixels with 0.200x0.200 milli-arcsec cellsize.
phase_soltime=phase_soltime1
print "uvstat(rms)=",uvstat(rms),"Jy"
! uvstat(rms)= 0.43803 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=0.575578Jy  sigma=9.724804
! Fit after  self-cal, rms=0.575523Jy  sigma=9.723785
! 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 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.706 mas, bmaj=1.88 mas, bpa=1.398 degrees
! Estimated noise=2.25877 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 = 0.372634 Jy
! Component: 100  -  total flux cleaned = 0.428182 Jy
! Total flux subtracted in 100 components = 0.428182 Jy
! Clean residual min=-0.013326 max=0.016110 Jy/beam
! Clean residual mean=-0.000053 rms=0.003711 Jy/beam
! Combined flux in latest and established models = 0.428182 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 6 model components to the UV plane model.
! The established model now contains 6 components and 0.428182 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.079383Jy  sigma=1.205635
! Fit after  self-cal, rms=0.079398Jy  sigma=1.205182
! Inverting map 
! Your choice of large map pixels excluded 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8156 mas, bmaj=2.128 mas, bpa=2.646 degrees
! Estimated noise=1.55387 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 = 0.0234384 Jy
! Component: 100  -  total flux cleaned = 0.0321299 Jy
! Component: 150  -  total flux cleaned = 0.0354804 Jy
! Component: 200  -  total flux cleaned = 0.0359817 Jy
! Total flux subtracted in 200 components = 0.0359817 Jy
! Clean residual min=-0.009703 max=0.007953 Jy/beam
! Clean residual mean=0.000010 rms=0.002263 Jy/beam
! Combined flux in latest and established models = 0.464163 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 17 components and 0.464163 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.076063Jy  sigma=1.117049
! Fit after  self-cal, rms=0.076061Jy  sigma=1.116818
! Inverting map 
! Your choice of large map pixels excluded 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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: 0.989005
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.97     FD        0.98     HN        1.18     KP        1.00     
!   LA        1.00     MK        1.00     NL        1.01     OV        1.00     
!   PT        0.97     SC        1.00     
! 
! 
! Correcting IF 2.
!  Amplitude normalization factor in sub-array 1: 1.00684
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.97     FD        0.98     HN        1.13     KP        0.94     
!   LA        0.96     MK        1.00     NL        0.99     OV        0.97     
!   PT        1.03     SC        0.97     
! 
! 
! Correcting IF 3.
!  Amplitude normalization factor in sub-array 1: 0.993129
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.06     FD        1.05     HN        1.05     KP        0.89     
!   LA        0.96     MK        1.02     NL        0.98     OV        1.01     
!   PT        1.02     SC        1.03     
! 
! 
! Correcting IF 4.
!  Amplitude normalization factor in sub-array 1: 0.97301
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.05     FD        1.02     HN        1.08     KP        0.92     
!   LA        1.00     MK        1.00     NL        1.04     OV        1.03     
!   PT        1.13     SC        1.01     
! 
! 
! Fit before self-cal, rms=0.076061Jy  sigma=1.116818
! Fit after  self-cal, rms=0.071486Jy  sigma=1.026914
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=0.071486Jy  sigma=1.026914
! Fit after  self-cal, rms=0.071503Jy  sigma=1.026887
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8223 mas, bmaj=2.136 mas, bpa=2.658 degrees
! Estimated noise=1.52899 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 = -0.00733243 Jy
! Component: 100  -  total flux cleaned = -0.00968758 Jy
! Component: 150  -  total flux cleaned = -0.0100103 Jy
! Component: 200  -  total flux cleaned = -0.0102879 Jy
! Total flux subtracted in 200 components = -0.0102879 Jy
! Clean residual min=-0.005062 max=0.005410 Jy/beam
! Clean residual mean=-0.000023 rms=0.001461 Jy/beam
! Combined flux in latest and established models = 0.453875 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 13 model components to the UV plane model.
! The established model now contains 27 components and 0.453875 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.070904Jy  sigma=1.016045
! Fit after  self-cal, rms=0.070914Jy  sigma=1.015970
! Inverting map 
! Your choice of large map pixels excluded 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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=0.070914Jy  sigma=1.015970
! Fit after  self-cal, rms=0.068254Jy  sigma=0.967641
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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 = -7.42324e-05 Jy
! Component: 100  -  total flux cleaned = -0.000121739 Jy
! Component: 150  -  total flux cleaned = -0.000211994 Jy
! Component: 200  -  total flux cleaned = -0.000299179 Jy
! Total flux subtracted in 200 components = -0.000299179 Jy
! Clean residual min=-0.004830 max=0.005249 Jy/beam
! Clean residual mean=-0.000024 rms=0.001414 Jy/beam
! Combined flux in latest and established models = 0.453576 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 12 model components to the UV plane model.
! The established model now contains 34 components and 0.453576 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.068229Jy  sigma=0.966571
! Fit after  self-cal, rms=0.068161Jy  sigma=0.963216
! Inverting map 
! Your choice of large map pixels excluded 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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: 0.8223 x 2.136 at 2.658 degrees (North through East)
! Clean map  min=-0.0044785  max=0.42887 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=0.068161Jy  sigma=0.963216
! Fit after  self-cal, rms=0.068254Jy  sigma=0.945923
! 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=0.068254Jy  sigma=0.945923
! Fit after  self-cal, rms=0.068287Jy  sigma=0.945642
! Inverting map and beam 
! Your choice of large map pixels excluded 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8245 mas, bmaj=2.142 mas, bpa=2.514 degrees
! Estimated noise=1.52935 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.00119312 Jy
! Component: 100  -  total flux cleaned = -0.00124441 Jy
! Component: 150  -  total flux cleaned = -0.00133657 Jy
! Component: 200  -  total flux cleaned = -0.00137662 Jy
! Total flux subtracted in 200 components = -0.00137662 Jy
! Clean residual min=-0.004754 max=0.005210 Jy/beam
! Clean residual mean=-0.000026 rms=0.001348 Jy/beam
! Combined flux in latest and established models = 0.4522 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 14 model components to the UV plane model.
! The established model now contains 38 components and 0.4522 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.068235Jy  sigma=0.944399
! Fit after  self-cal, rms=0.068250Jy  sigma=0.944357
! Inverting map 
! Your choice of large map pixels excluded 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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=0.068250Jy  sigma=0.944357
! Fit after  self-cal, rms=0.067213Jy  sigma=0.925903
! 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=0.067213Jy  sigma=0.925903
! Fit after  self-cal, rms=0.067220Jy  sigma=0.925897
! Inverting map and beam 
! Your choice of large map pixels excluded 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8261 mas, bmaj=2.145 mas, bpa=2.312 degrees
! Estimated noise=1.53059 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.000465889 Jy
! Component: 100  -  total flux cleaned = -0.000514352 Jy
! Component: 150  -  total flux cleaned = -0.000557184 Jy
! Component: 200  -  total flux cleaned = -0.000633415 Jy
! Total flux subtracted in 200 components = -0.000633415 Jy
! Clean residual min=-0.004733 max=0.005247 Jy/beam
! Clean residual mean=-0.000027 rms=0.001342 Jy/beam
! Combined flux in latest and established models = 0.451566 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 45 components and 0.451566 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067173Jy  sigma=0.924752
! Fit after  self-cal, rms=0.067174Jy  sigma=0.924741
! Inverting map 
! Your choice of large map pixels excluded 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=2.347 mas, bmaj=6.329 mas, bpa=6.457 degrees
! Estimated noise=1.99212 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 = -0.000107776 Jy
! Component: 100  -  total flux cleaned = -0.000111199 Jy
! Component: 150  -  total flux cleaned = -0.000114627 Jy
! Component: 200  -  total flux cleaned = -0.000169155 Jy
! Total flux subtracted in 200 components = -0.000169155 Jy
! Clean residual min=-0.005508 max=0.005814 Jy/beam
! Clean residual mean=-0.000055 rms=0.001852 Jy/beam
! Combined flux in latest and established models = 0.451397 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 4 model components to the UV plane model.
! The established model now contains 45 components and 0.451397 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067207Jy  sigma=0.925238
! Fit after  self-cal, rms=0.067175Jy  sigma=0.924271
! Inverting map 
! Your choice of large map pixels excluded 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.7096 mas, bmaj=1.882 mas, bpa=1.282 degrees
! Estimated noise=2.25404 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.372438 Jy
! Component: 100  -  total flux cleaned = 0.426163 Jy
! Component: 150  -  total flux cleaned = 0.444462 Jy
! Component: 200  -  total flux cleaned = 0.451419 Jy
! Total flux subtracted in 200 components = 0.451419 Jy
! Clean residual min=-0.007209 max=0.007427 Jy/beam
! Clean residual mean=-0.000000 rms=0.001910 Jy/beam
! Combined flux in latest and established models = 0.451419 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 16 model components to the UV plane model.
! The established model now contains 16 components and 0.451419 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8261 mas, bmaj=2.145 mas, bpa=2.312 degrees
! Estimated noise=1.53059 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 = -0.000266013 Jy
! Component: 100  -  total flux cleaned = -0.000386247 Jy
! Component: 150  -  total flux cleaned = -0.000202898 Jy
! Component: 200  -  total flux cleaned = -0.000120641 Jy
! Total flux subtracted in 200 components = -0.000120641 Jy
! Clean residual min=-0.004884 max=0.005077 Jy/beam
! Clean residual mean=-0.000028 rms=0.001388 Jy/beam
! Combined flux in latest and established models = 0.451298 Jy
! Adding 14 model components to the UV plane model.
! The established model now contains 21 components and 0.451298 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=2.347 mas, bmaj=6.329 mas, bpa=6.457 degrees
! Estimated noise=1.99212 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 = -0.000241828 Jy
! Component: 100  -  total flux cleaned = -0.000101002 Jy
! Component: 150  -  total flux cleaned = 5.38487e-05 Jy
! Component: 200  -  total flux cleaned = 9.48039e-05 Jy
! Total flux subtracted in 200 components = 9.48039e-05 Jy
! Clean residual min=-0.005467 max=0.005841 Jy/beam
! Clean residual mean=-0.000055 rms=0.001858 Jy/beam
! Combined flux in latest and established models = 0.451393 Jy
! Adding 8 model components to the UV plane model.
! The established model now contains 27 components and 0.451393 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.8261 mas, bmaj=2.145 mas, bpa=2.312 degrees
! Estimated noise=1.53059 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.000225258 Jy
! Component: 100  -  total flux cleaned = 2.93461e-06 Jy
! Component: 150  -  total flux cleaned = -5.73924e-05 Jy
! Component: 200  -  total flux cleaned = -0.000164895 Jy
! Total flux subtracted in 200 components = -0.000164895 Jy
! Clean residual min=-0.004565 max=0.005003 Jy/beam
! Clean residual mean=-0.000028 rms=0.001351 Jy/beam
! Combined flux in latest and established models = 0.451228 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 8 model components to the UV plane model.
! The established model now contains 32 components and 0.451228 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.067228Jy  sigma=0.926082
! Fit after  self-cal, rms=0.067233Jy  sigma=0.925900
wmodel J1700-2610_X_2004_04_30_yyk\_map.mod
! Writing 32 model components to file: J1700-2610_X_2004_04_30_yyk_map.mod
wobs J1700-2610_X_2004_04_30_yyk\_uvs.fits
! Writing UV FITS file: J1700-2610_X_2004_04_30_yyk_uvs.fits
wwins J1700-2610_X_2004_04_30_yyk\_map.win
! wwins: Wrote 1 windows to J1700-2610_X_2004_04_30_yyk_map.win
x = (field_size-8) * field_cell / 4
addwin -x,x,-x,x
clean (field_size*4),0.01
! Inverting map 
! Your choice of large map pixels excluded 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! clean: niter=2048  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.000656642 Jy
! Component: 100  -  total flux cleaned = 0.000651965 Jy
! Component: 150  -  total flux cleaned = 0.000878414 Jy
! Component: 200  -  total flux cleaned = 0.00151918 Jy
! Component: 250  -  total flux cleaned = 0.00206367 Jy
! Component: 300  -  total flux cleaned = 0.00252092 Jy
! Component: 350  -  total flux cleaned = 0.00296143 Jy
! Component: 400  -  total flux cleaned = 0.00320376 Jy
! Component: 450  -  total flux cleaned = 0.00338007 Jy
! Component: 500  -  total flux cleaned = 0.00360825 Jy
! Component: 550  -  total flux cleaned = 0.00366496 Jy
! Component: 600  -  total flux cleaned = 0.0038797 Jy
! Component: 650  -  total flux cleaned = 0.00393075 Jy
! Component: 700  -  total flux cleaned = 0.00398132 Jy
! Component: 750  -  total flux cleaned = 0.00407959 Jy
! Component: 800  -  total flux cleaned = 0.00427298 Jy
! Component: 850  -  total flux cleaned = 0.00446178 Jy
! Component: 900  -  total flux cleaned = 0.00478361 Jy
! Component: 950  -  total flux cleaned = 0.00509813 Jy
! Component: 1000  -  total flux cleaned = 0.00522982 Jy
! Component: 1050  -  total flux cleaned = 0.00553168 Jy
! Component: 1100  -  total flux cleaned = 0.00569959 Jy
! Component: 1150  -  total flux cleaned = 0.00590676 Jy
! Component: 1200  -  total flux cleaned = 0.00615033 Jy
! Component: 1250  -  total flux cleaned = 0.00622969 Jy
! Component: 1300  -  total flux cleaned = 0.00642469 Jy
! Component: 1350  -  total flux cleaned = 0.00650191 Jy
! Component: 1400  -  total flux cleaned = 0.00661444 Jy
! Component: 1450  -  total flux cleaned = 0.00665242 Jy
! Component: 1500  -  total flux cleaned = 0.00679813 Jy
! Component: 1550  -  total flux cleaned = 0.00683385 Jy
! Component: 1600  -  total flux cleaned = 0.00693951 Jy
! Component: 1650  -  total flux cleaned = 0.00718189 Jy
! Component: 1700  -  total flux cleaned = 0.00725003 Jy
! Component: 1750  -  total flux cleaned = 0.00745157 Jy
! Component: 1800  -  total flux cleaned = 0.00768339 Jy
! Component: 1850  -  total flux cleaned = 0.00784634 Jy
! Component: 1900  -  total flux cleaned = 0.00807257 Jy
! Component: 1950  -  total flux cleaned = 0.00832748 Jy
! Component: 2000  -  total flux cleaned = 0.00848494 Jy
! Total flux subtracted in 2048 components = 0.00867224 Jy
! Clean residual min=-0.001767 max=0.002422 Jy/beam
! Clean residual mean=-0.000008 rms=0.000587 Jy/beam
! Combined flux in latest and established models = 0.459901 Jy
keep
! Adding 124 model components to the UV plane model.
! The established model now contains 156 components and 0.459901 Jy
![Exited script file: muppet]
wmap "J1700-2610_X_2004_04_30_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8261 x 2.145 at 2.312 degrees (North through East)
! Clean map  min=-0.0028973  max=0.43106 Jy/beam
! Writing clean map to FITS file: J1700-2610_X_2004_04_30_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.431061 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.565% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.00058718 
device "J1700-2610_X_2004_04_30_yyk\_map.eps/VPS"
! Attempting to open device: 'J1700-2610_X_2004_04_30_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.408652 0.408652 0.817304 1.63461 3.26921 6.53843 13.0769 26.1537 52.3074
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0017 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.431 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.8261 x 2.145 at 2.312 degrees (North through East)
! Clean map  min=-0.0028973  max=0.43106 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J1700-2610_X_2004_04_30_yyk\_map.gif/gif"
! Attempting to open device: 'J1700-2610_X_2004_04_30_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J1700-2610_X_2004_04_30_yyk_uvs.log closed on Wed Dec  7 00:38:48 2005