! Started logfile: J1725+7726_X_2006_02_16_yyk_uvs.log on Wed Jul  5 13:10:23 2006
obs J1725+7726_X_2006_02_16_yyk_uva.fits
! Reading UV FITS file: J1725+7726_X_2006_02_16_yyk_uva.fits
! AN table 1: 869 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.246925 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J1725+7726
! 
! 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 2421 lines of history.
! 
! Reading 38624 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 J1725+7726_X_2006_02_16_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.
uvav time_av, true
! Averaging into 30 second bins.
! 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
phase_soltime=phase_soltime1
print "uvstat(rms)=",uvstat(rms),"Jy"
! uvstat(rms)= 0.0958429 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 
! Estimated beam: bmin=0.6091 mas, bmaj=13 mas, bpa=11.66 degrees
! Estimated noise=1.10265 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=100  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0254192 Jy
! Component: 100  -  total flux cleaned = 0.0417394 Jy
! Total flux subtracted in 100 components = 0.0417394 Jy
! Clean residual min=-0.005335 max=0.006680 Jy/beam
! Clean residual mean=-0.000079 rms=0.002275 Jy/beam
! Combined flux in latest and established models = 0.0417394 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 28 model components to the UV plane model.
! The established model now contains 28 components and 0.0417394 Jy
! 
! Correcting IF 1.
!  A total of 105 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 87 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 87 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 105 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.069958Jy  sigma=1.593776
! Fit after  self-cal, rms=0.070002Jy  sigma=1.595015
! Inverting map and beam 
! Estimated beam: bmin=0.6091 mas, bmaj=13 mas, bpa=11.66 degrees
! Estimated noise=1.10274 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 
! Estimated beam: bmin=0.5963 mas, bmaj=14.36 mas, bpa=11.72 degrees
! Estimated noise=0.749767 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 = 0.015183 Jy
! Component: 100  -  total flux cleaned = 0.0263429 Jy
! Component: 150  -  total flux cleaned = 0.0354564 Jy
! Component: 200  -  total flux cleaned = 0.0431002 Jy
! Total flux subtracted in 200 components = 0.0431002 Jy
! Clean residual min=-0.003444 max=0.003518 Jy/beam
! Clean residual mean=-0.000067 rms=0.001657 Jy/beam
! Combined flux in latest and established models = 0.0848396 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 99 model components to the UV plane model.
! The established model now contains 117 components and 0.0848396 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.055045Jy  sigma=1.222926
! Fit after  self-cal, rms=0.054985Jy  sigma=1.221670
! Inverting map 
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5963 x 14.36 at 11.72 degrees (North through East)
! Clean map  min=-0.0034892  max=0.027268 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.
!  A total of 15 telescope corrections were flagged in sub-array 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.
!  A total of 3 telescope corrections were flagged in sub-array 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 3.
!  A total of 3 telescope corrections were flagged in sub-array 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 4.
!  A total of 15 telescope corrections were flagged in sub-array 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*    
! 
! 
! Fit before self-cal, rms=0.054985Jy  sigma=1.221670
! Fit after  self-cal, rms=0.055613Jy  sigma=1.221946
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=0.055613Jy  sigma=1.221946
! Fit after  self-cal, rms=0.055595Jy  sigma=1.220587
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=0.5928 mas, bmaj=14.52 mas, bpa=11.7 degrees
! Estimated noise=0.770066 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 = 0.00634193 Jy
! Component: 100  -  total flux cleaned = 0.0110595 Jy
! Component: 150  -  total flux cleaned = 0.0144024 Jy
! Component: 200  -  total flux cleaned = 0.0165165 Jy
! Total flux subtracted in 200 components = 0.0165165 Jy
! Clean residual min=-0.001880 max=0.001903 Jy/beam
! Clean residual mean=-0.000038 rms=0.000950 Jy/beam
! Combined flux in latest and established models = 0.101356 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 113 model components to the UV plane model.
! The established model now contains 216 components and 0.101356 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.051801Jy  sigma=1.120879
! Fit after  self-cal, rms=0.051787Jy  sigma=1.120031
! Inverting map 
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=0.051787Jy  sigma=1.120031
! Fit after  self-cal, rms=0.046303Jy  sigma=1.001483
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
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 = 0.0035756 Jy
! Component: 100  -  total flux cleaned = 0.00522659 Jy
! Component: 150  -  total flux cleaned = 0.00633628 Jy
! Component: 200  -  total flux cleaned = 0.00665935 Jy
! Total flux subtracted in 200 components = 0.00665935 Jy
! Clean residual min=-0.001285 max=0.001275 Jy/beam
! Clean residual mean=-0.000027 rms=0.000642 Jy/beam
! Combined flux in latest and established models = 0.108015 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 93 model components to the UV plane model.
! The established model now contains 283 components and 0.108015 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.044018Jy  sigma=0.938533
! Fit after  self-cal, rms=0.043574Jy  sigma=0.928031
! Inverting map 
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: 0.5928 x 14.52 at 11.7 degrees (North through East)
! Clean map  min=-0.002694  max=0.031183 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 
! Estimated beam: bmin=2.214 mas, bmaj=10.63 mas, bpa=12.69 degrees
! Estimated noise=1.64216 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 = -0.00158794 Jy
! Component: 100  -  total flux cleaned = -0.00267239 Jy
! Component: 150  -  total flux cleaned = -0.00338291 Jy
! Component: 200  -  total flux cleaned = -0.00402177 Jy
! Total flux subtracted in 200 components = -0.00402177 Jy
! Clean residual min=-0.001987 max=0.001952 Jy/beam
! Clean residual mean=-0.000055 rms=0.000796 Jy/beam
! Combined flux in latest and established models = 0.103994 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 84 model components to the UV plane model.
! The established model now contains 353 components and 0.103994 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.041861Jy  sigma=0.890329
! Fit after  self-cal, rms=0.041732Jy  sigma=0.882941
! Inverting map 
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 
! Estimated beam: bmin=0.6082 mas, bmaj=12.98 mas, bpa=11.65 degrees
! Estimated noise=1.19009 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.02712 Jy
! Component: 100  -  total flux cleaned = 0.0444707 Jy
! Component: 150  -  total flux cleaned = 0.0568092 Jy
! Component: 200  -  total flux cleaned = 0.0653841 Jy
! Total flux subtracted in 200 components = 0.0653841 Jy
! Clean residual min=-0.004539 max=0.004615 Jy/beam
! Clean residual mean=-0.000059 rms=0.001827 Jy/beam
! Combined flux in latest and established models = 0.0653841 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 69 model components to the UV plane model.
! The established model now contains 69 components and 0.0653841 Jy
! Inverting map and beam 
! Estimated beam: bmin=0.5928 mas, bmaj=14.52 mas, bpa=11.7 degrees
! Estimated noise=0.770066 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 = 0.0107246 Jy
! Component: 100  -  total flux cleaned = 0.0185936 Jy
! Component: 150  -  total flux cleaned = 0.0241205 Jy
! Component: 200  -  total flux cleaned = 0.0285903 Jy
! Total flux subtracted in 200 components = 0.0285903 Jy
! Clean residual min=-0.002697 max=0.002742 Jy/beam
! Clean residual mean=-0.000051 rms=0.001269 Jy/beam
! Combined flux in latest and established models = 0.0939744 Jy
! Adding 89 model components to the UV plane model.
! The established model now contains 141 components and 0.0939744 Jy
! Inverting map 
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 
! Estimated beam: bmin=2.214 mas, bmaj=10.63 mas, bpa=12.69 degrees
! Estimated noise=1.64216 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 = 0.011352 Jy
! Component: 100  -  total flux cleaned = 0.0100861 Jy
! Component: 150  -  total flux cleaned = 0.0105813 Jy
! Component: 200  -  total flux cleaned = 0.0101078 Jy
! Total flux subtracted in 200 components = 0.0101078 Jy
! Clean residual min=-0.002604 max=0.002610 Jy/beam
! Clean residual mean=-0.000078 rms=0.001107 Jy/beam
! Combined flux in latest and established models = 0.104082 Jy
! Adding 105 model components to the UV plane model.
! The established model now contains 240 components and 0.104082 Jy
! Inverting map 
uvtaper 0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Estimated beam: bmin=0.5928 mas, bmaj=14.52 mas, bpa=11.7 degrees
! Estimated noise=0.770066 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.00123896 Jy
! Component: 100  -  total flux cleaned = -0.00231299 Jy
! Component: 150  -  total flux cleaned = -0.00338475 Jy
! Component: 200  -  total flux cleaned = -0.00427737 Jy
! Total flux subtracted in 200 components = -0.00427737 Jy
! Clean residual min=-0.000439 max=0.000442 Jy/beam
! Clean residual mean=-0.000005 rms=0.000170 Jy/beam
! Combined flux in latest and established models = 0.0998048 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 54 model components to the UV plane model.
! The established model now contains 293 components and 0.0998047 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.041579Jy  sigma=0.877093
! Fit after  self-cal, rms=0.041559Jy  sigma=0.874741
wmodel J1725+7726_X_2006_02_16_yyk\_map.mod
! Writing 293 model components to file: J1725+7726_X_2006_02_16_yyk_map.mod
wobs J1725+7726_X_2006_02_16_yyk\_uvs.fits
! Writing UV FITS file: J1725+7726_X_2006_02_16_yyk_uvs.fits
wwins J1725+7726_X_2006_02_16_yyk\_map.win
! wwins: No CLEAN windows to write.
! Error occured in command: wwins
![Exited script file: muppet]
! 
wmap "J1725+7726_X_2006_02_16_yyk\_map.fits"
! Inverting map 
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5928 x 14.52 at 11.7 degrees (North through East)
! Clean map  min=-0.0038325  max=0.034893 Jy/beam
! Writing clean map to FITS file: J1725+7726_X_2006_02_16_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.0348932 
invert
! Inverting map 
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000212656 
device "J1725+7726_X_2006_02_16_yyk\_map.eps/VPS"
! Attempting to open device: 'J1725+7726_X_2006_02_16_yyk_map.eps/VPS'
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -1.82834 1.82834 3.65669 7.31337 14.6267 29.2535 58.507
print "clev=",int(3*image_rms*10000)/10000
! clev= 0.0006 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.034 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.5928 x 14.52 at 11.7 degrees (North through East)
! Clean map  min=-0.0038325  max=0.034893 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J1725+7726_X_2006_02_16_yyk\_map.gif/gif"
! Attempting to open device: 'J1725+7726_X_2006_02_16_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J1725+7726_X_2006_02_16_yyk_uvs.log closed on Wed Jul  5 13:10:57 2006