! Started logfile: J0905-3927_X_2002_01_31_yyk_uvs.log on Wed Jun 27 10:54:08 2007
obs J0905-3927_X_2002_01_31_yyk_uva.fits
! Reading UV FITS file: J0905-3927_X_2002_01_31_yyk_uva.fits
! AN table 1: 35 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.617778 visibilities/baseline/integration-bin.
! Found source: J0905-3927
! 
! 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  8.40947e+09        8e+06          1        8e+06
!  02        2  8.47947e+09        8e+06          1        8e+06
!  03        3  8.79447e+09        8e+06          1        8e+06
!  04        4  8.89947e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 1544 lines of history.
! 
! Reading 3892 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
flag NL
! Flagging baselines of antenna 1:NL in the currently selected channels.
![@muppet J0905-3927_X_2002_01_31_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)= 0.192553 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 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.6241 mas, bmaj=1.872 mas, bpa=2.373 degrees
! Estimated noise=2726.13 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 = 0.0392397 Jy
! Component: 100  -  total flux cleaned = 0.0480491 Jy
! Total flux subtracted in 100 components = 0.0480491 Jy
! Clean residual min=-0.014281 max=0.016063 Jy/beam
! Clean residual mean=-0.000099 rms=0.004436 Jy/beam
! Combined flux in latest and established models = 0.0480491 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 10 model components to the UV plane model.
! The established model now contains 10 components and 0.0480491 Jy
! 
! Correcting IF 1.
!  A total of 106 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 106 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 106 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 106 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.186808Jy  sigma=0.001446
! Fit after  self-cal, rms=0.186828Jy  sigma=0.001446
! Inverting map and beam 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.6241 mas, bmaj=1.872 mas, bpa=2.373 degrees
! Estimated noise=2726.13 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 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.7944 mas, bmaj=2.128 mas, bpa=1.387 degrees
! Estimated noise=1588.5 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 = 0.00653076 Jy
! Component: 100  -  total flux cleaned = 0.00791596 Jy
! Component: 150  -  total flux cleaned = 0.00807211 Jy
! Component: 200  -  total flux cleaned = 0.00811869 Jy
! Total flux subtracted in 200 components = 0.00811869 Jy
! Clean residual min=-0.010513 max=0.011457 Jy/beam
! Clean residual mean=-0.000085 rms=0.003192 Jy/beam
! Combined flux in latest and established models = 0.0561678 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 10 model components to the UV plane model.
! The established model now contains 19 components and 0.0561678 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.186703Jy  sigma=0.001445
! Fit after  self-cal, rms=0.186724Jy  sigma=0.001445
! Inverting map 
! Your choice of large map pixels excluded 1.17% 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 ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7944 x 2.128 at 1.387 degrees (North through East)
! Clean map  min=-0.0096817  max=0.045281 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
!  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 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=0.186724Jy  sigma=0.001445
! Fit after  self-cal, rms=0.186724Jy  sigma=0.001445
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=0.186724Jy  sigma=0.001445
! Fit after  self-cal, rms=0.186719Jy  sigma=0.001445
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.7944 mas, bmaj=2.128 mas, bpa=1.387 degrees
! Estimated noise=1588.5 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 = 5.60946e-05 Jy
! Component: 100  -  total flux cleaned = 5.70469e-05 Jy
! Component: 150  -  total flux cleaned = 0.000102739 Jy
! Component: 200  -  total flux cleaned = 0.00014534 Jy
! Total flux subtracted in 200 components = 0.00014534 Jy
! Clean residual min=-0.010515 max=0.011099 Jy/beam
! Clean residual mean=-0.000083 rms=0.003136 Jy/beam
! Combined flux in latest and established models = 0.0563131 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 13 model components to the UV plane model.
! The established model now contains 23 components and 0.0563131 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.186699Jy  sigma=0.001445
! Fit after  self-cal, rms=0.186699Jy  sigma=0.001445
! Inverting map 
! Your choice of large map pixels excluded 1.17% 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=0.186699Jy  sigma=0.001445
! Fit after  self-cal, rms=0.185535Jy  sigma=0.001435
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 1.17% 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 = 0.00376182 Jy
! Component: 100  -  total flux cleaned = 0.00376406 Jy
! Component: 150  -  total flux cleaned = 0.00371145 Jy
! Component: 200  -  total flux cleaned = 0.00366328 Jy
! Total flux subtracted in 200 components = 0.00366328 Jy
! Clean residual min=-0.010641 max=0.010324 Jy/beam
! Clean residual mean=-0.000118 rms=0.002938 Jy/beam
! Combined flux in latest and established models = 0.0599764 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 7 model components to the UV plane model.
! The established model now contains 27 components and 0.0599764 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.185471Jy  sigma=0.001435
! Fit after  self-cal, rms=0.184802Jy  sigma=0.001430
! Inverting map 
! Your choice of large map pixels excluded 1.17% 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: 0.7944 x 2.128 at 1.387 degrees (North through East)
! Clean map  min=-0.0087333  max=0.051467 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
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 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=3.102 mas, bmaj=11.03 mas, bpa=4.705 degrees
! Estimated noise=2114.87 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 = 0.000553115 Jy
! Component: 100  -  total flux cleaned = 0.000512991 Jy
! Component: 150  -  total flux cleaned = 0.000508636 Jy
! Component: 200  -  total flux cleaned = 0.000470459 Jy
! Total flux subtracted in 200 components = 0.000470459 Jy
! Clean residual min=-0.008107 max=0.009154 Jy/beam
! Clean residual mean=-0.000189 rms=0.003732 Jy/beam
! Combined flux in latest and established models = 0.0604468 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 3 model components to the UV plane model.
! The established model now contains 28 components and 0.0604468 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.184817Jy  sigma=0.001430
! Fit after  self-cal, rms=0.184538Jy  sigma=0.001428
! Inverting map 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1987 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 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.6241 mas, bmaj=1.872 mas, bpa=2.373 degrees
! Estimated noise=2726.13 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0453007 Jy
! Component: 100  -  total flux cleaned = 0.0541164 Jy
! Component: 150  -  total flux cleaned = 0.0557692 Jy
! Component: 200  -  total flux cleaned = 0.0559824 Jy
! Total flux subtracted in 200 components = 0.0559824 Jy
! Clean residual min=-0.013128 max=0.015266 Jy/beam
! Clean residual mean=-0.000093 rms=0.004312 Jy/beam
! Combined flux in latest and established models = 0.0559824 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 10 model components to the UV plane model.
! The established model now contains 10 components and 0.0559824 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.7944 mas, bmaj=2.128 mas, bpa=1.387 degrees
! Estimated noise=1588.5 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 = 0.00511516 Jy
! Component: 100  -  total flux cleaned = 0.00525388 Jy
! Component: 150  -  total flux cleaned = 0.00530877 Jy
! Component: 200  -  total flux cleaned = 0.00530174 Jy
! Total flux subtracted in 200 components = 0.00530174 Jy
! Clean residual min=-0.009453 max=0.009254 Jy/beam
! Clean residual mean=-0.000091 rms=0.002786 Jy/beam
! Combined flux in latest and established models = 0.0612842 Jy
! Adding 13 model components to the UV plane model.
! The established model now contains 22 components and 0.0612842 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.17% 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 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=3.102 mas, bmaj=11.03 mas, bpa=4.705 degrees
! Estimated noise=2114.87 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 = -0.000278109 Jy
! Component: 100  -  total flux cleaned = -0.000322713 Jy
! Component: 150  -  total flux cleaned = -0.00036045 Jy
! Component: 200  -  total flux cleaned = -0.00036514 Jy
! Total flux subtracted in 200 components = -0.00036514 Jy
! Clean residual min=-0.008023 max=0.008317 Jy/beam
! Clean residual mean=-0.000179 rms=0.003704 Jy/beam
! Combined flux in latest and established models = 0.060919 Jy
! Adding 3 model components to the UV plane model.
! The established model now contains 24 components and 0.060919 Jy
! Inverting map 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 1.17% of the data.
!  The x-axis pixel size should ideally be below 0.1987 milli-arcsec
! Estimated beam: bmin=0.7944 mas, bmaj=2.128 mas, bpa=1.387 degrees
! Estimated noise=1588.5 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.000567672 Jy
! Component: 100  -  total flux cleaned = 0.000468503 Jy
! Component: 150  -  total flux cleaned = 0.000466936 Jy
! Component: 200  -  total flux cleaned = 0.000468065 Jy
! Total flux subtracted in 200 components = 0.000468065 Jy
! Clean residual min=-0.009567 max=0.009322 Jy/beam
! Clean residual mean=-0.000091 rms=0.002777 Jy/beam
! Combined flux in latest and established models = 0.0613871 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 10 model components to the UV plane model.
! The established model now contains 29 components and 0.0613871 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.184549Jy  sigma=0.001427
! Fit after  self-cal, rms=0.184408Jy  sigma=0.001427
wmodel J0905-3927_X_2002_01_31_yyk\_map.mod
! Writing 29 model components to file: J0905-3927_X_2002_01_31_yyk_map.mod
wobs J0905-3927_X_2002_01_31_yyk\_uvs.fits
! Applying 35 buffered edits.
! Writing UV FITS file: J0905-3927_X_2002_01_31_yyk_uvs.fits
wwins J0905-3927_X_2002_01_31_yyk\_map.win
! wwins: Wrote 1 windows to J0905-3927_X_2002_01_31_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 1.17% 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 = -0.00172533 Jy
! Component: 100  -  total flux cleaned = -0.00187043 Jy
! Component: 150  -  total flux cleaned = -0.0016072 Jy
! Component: 200  -  total flux cleaned = -0.000881723 Jy
! Component: 250  -  total flux cleaned = -0.0012163 Jy
! Component: 300  -  total flux cleaned = -0.00142552 Jy
! Component: 350  -  total flux cleaned = -0.00172997 Jy
! Component: 400  -  total flux cleaned = -0.00192385 Jy
! Component: 450  -  total flux cleaned = -0.00219959 Jy
! Component: 500  -  total flux cleaned = -0.00228799 Jy
! Component: 550  -  total flux cleaned = -0.00237645 Jy
! Component: 600  -  total flux cleaned = -0.00262584 Jy
! Component: 650  -  total flux cleaned = -0.00278607 Jy
! Component: 700  -  total flux cleaned = -0.00309765 Jy
! Component: 750  -  total flux cleaned = -0.00324993 Jy
! Component: 800  -  total flux cleaned = -0.00347183 Jy
! Component: 850  -  total flux cleaned = -0.00361595 Jy
! Component: 900  -  total flux cleaned = -0.0038251 Jy
! Component: 950  -  total flux cleaned = -0.00396056 Jy
! Component: 1000  -  total flux cleaned = -0.00409323 Jy
! Component: 1050  -  total flux cleaned = -0.00422414 Jy
! Component: 1100  -  total flux cleaned = -0.00435184 Jy
! Component: 1150  -  total flux cleaned = -0.00435083 Jy
! Component: 1200  -  total flux cleaned = -0.00428877 Jy
! Component: 1250  -  total flux cleaned = -0.00434991 Jy
! Component: 1300  -  total flux cleaned = -0.00435008 Jy
! Component: 1350  -  total flux cleaned = -0.00423292 Jy
! Component: 1400  -  total flux cleaned = -0.00411728 Jy
! Component: 1450  -  total flux cleaned = -0.00405996 Jy
! Component: 1500  -  total flux cleaned = -0.00388944 Jy
! Component: 1550  -  total flux cleaned = -0.00383314 Jy
! Component: 1600  -  total flux cleaned = -0.00405763 Jy
! Component: 1650  -  total flux cleaned = -0.00405746 Jy
! Component: 1700  -  total flux cleaned = -0.004279 Jy
! Component: 1750  -  total flux cleaned = -0.00444403 Jy
! Component: 1800  -  total flux cleaned = -0.00460816 Jy
! Component: 1850  -  total flux cleaned = -0.00466258 Jy
! Component: 1900  -  total flux cleaned = -0.00455384 Jy
! Component: 1950  -  total flux cleaned = -0.00449939 Jy
! Component: 2000  -  total flux cleaned = -0.004391 Jy
! Total flux subtracted in 2048 components = -0.00439076 Jy
! Clean residual min=-0.003227 max=0.002755 Jy/beam
! Clean residual mean=-0.000022 rms=0.001033 Jy/beam
! Combined flux in latest and established models = 0.0569963 Jy
keep
! Adding 110 model components to the UV plane model.
! The established model now contains 139 components and 0.0569964 Jy
![Exited script file: muppet]
wmap "J0905-3927_X_2002_01_31_yyk\_map.fits"
! Inverting map 
! Your choice of large map pixels excluded 1.17% 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: 0.7944 x 2.128 at 1.387 degrees (North through East)
! Clean map  min=-0.0057164  max=0.052677 Jy/beam
! Writing clean map to FITS file: J0905-3927_X_2002_01_31_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.0526768 
invert
! Inverting map 
! Your choice of large map pixels excluded 1.17% 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 0.001019 
device "J0905-3927_X_2002_01_31_yyk\_map.eps/VPS"
! Attempting to open device: 'J0905-3927_X_2002_01_31_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -5.80329 5.80329 11.6066 23.2132 46.4263 92.8527
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.003 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.052 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7944 x 2.128 at 1.387 degrees (North through East)
! Clean map  min=-0.0057164  max=0.052677 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0905-3927_X_2002_01_31_yyk\_map.gif/gif"
! Attempting to open device: 'J0905-3927_X_2002_01_31_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J0905-3927_X_2002_01_31_yyk_uvs.log closed on Wed Jun 27 10:54:14 2007