! Started logfile: 0434-188_X.log on Fri Feb 15 00:45:42 2008
observe 0434-188_X.edt
! Reading UV FITS file: 0434-188_X.edt
! AN table 1: 62 integrations on 136 of 136 possible baselines.
! Apparent sampling: 0.109345 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: 0434-188
! 
! 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 1230 lines of history.
! 
! Reading 3688 visibilities.
![@gonzo8-0.1 0434-188_X]
print "***********************************"
! *********************************** 
print "*** Using gonzo instruction set ***"
! *** Using gonzo instruction set *** 
print "***********************************"
! *********************************** 
float field_size
field_size = 1024
float field_cell
field_cell = 0.1
integer clean_niter
clean_niter = 50
float clean_gain
clean_gain = 0.03
float dynam
dynam = 8.0
float win_mult
win_mult = 1.8
float solint
solint = 3.6/6.0
logical doflt
doflt = true
logical doamp
float new_peak
float flux_cutoff
mapsize field_size,field_cell
! Map grid = 1024x1024 pixels with 0.100x0.100 milli-arcsec cellsize.
select
! 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
startmod
! Applying default point source starting model.
! Performing phase self-cal
! Adding 1 model components to the UV plane model.
! The established model now contains 1 components and 1 Jy
! 
! Correcting IF 1.
!  A total of 960 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 967 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 973 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 972 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.576024Jy  sigma=0.010096
! Fit after  self-cal, rms=0.574097Jy  sigma=0.010127
! clrmod: Cleared the established, tentative and continuum models.
! Redundant starting model cleared.
uvweight 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.
doamp = false
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=0.9248 mas, bmaj=3.21 mas, bpa=4.458 degrees
! Estimated noise=2472.06 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal doamp, doflt, solint
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (0, 0).
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.334502 Jy
! Total flux subtracted in 50 components = 0.334502 Jy
! Clean residual min=-0.032335 max=0.098049 Jy/beam
! Clean residual mean=0.000545 rms=0.014989 Jy/beam
! Combined flux in latest and established models = 0.334502 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 4 model components to the UV plane model.
! The established model now contains 4 components and 0.334502 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.135658Jy  sigma=0.002732
! Fit after  self-cal, rms=0.135657Jy  sigma=0.002732
! Inverting map 
print "****************************************"
! **************************************** 
print "*** Finished Uniform Weighting CLEAN ***"
! *** Finished Uniform Weighting CLEAN *** 
print "****************************************"
! **************************************** 
uvweight 0,-1
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
win_mult = win_mult * 1.6
clean_niter = clean_niter * 2
dynam = dynam - 0.5
doamp = false
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=1.029 mas, bmaj=3.617 mas, bpa=-0.1088 degrees
! Estimated noise=1589.19 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal doamp, doflt, solint
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.101786 Jy
! Component: 100  -  total flux cleaned = 0.143059 Jy
! Total flux subtracted in 100 components = 0.143059 Jy
! Clean residual min=-0.011677 max=0.018258 Jy/beam
! Clean residual mean=0.000271 rms=0.004144 Jy/beam
! Combined flux in latest and established models = 0.477561 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 33 model components to the UV plane model.
! The established model now contains 35 components and 0.477561 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.057004Jy  sigma=0.000965
! Fit after  self-cal, rms=0.056794Jy  sigma=0.000962
! Inverting map 
print "****************************************"
! **************************************** 
print "*** Finished Natural Weighting CLEAN ***"
! *** Finished Natural Weighting CLEAN *** 
print "****************************************"
! **************************************** 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.98     FD        0.96     GC        1.00*    HN        1.02     
!   KK        1.00*    KP        0.97     LA        0.96     MC        1.00*    
!   MK        1.00*    NL        0.96     NY        1.00*    ON        1.00*    
!   OV        0.99     PT        0.97     SC        1.00     WF        1.03     
!   WZ        1.00*    
! 
! 
! Correcting IF 2.
!  A total of 6 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.98     FD        0.96     GC        1.00*    HN        1.01     
!   KK        1.00*    KP        0.97     LA        0.97     MC        1.00*    
!   MK        1.00*    NL        0.97     NY        1.00*    ON        1.00*    
!   OV        0.97     PT        0.96     SC        1.04     WF        1.02     
!   WZ        1.00*    
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.97     FD        0.96     GC        1.00*    HN        1.03     
!   KK        1.00*    KP        0.97     LA        0.97     MC        1.00*    
!   MK        1.00*    NL        0.95     NY        1.00*    ON        1.00*    
!   OV        0.98     PT        0.97     SC        1.04     WF        1.05     
!   WZ        1.00*    
! 
! 
! Correcting IF 4.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.97     FD        0.96     GC        1.00*    HN        1.05     
!   KK        1.00*    KP        0.96     LA        0.96     MC        1.00*    
!   MK        1.00*    NL        0.95     NY        1.00*    ON        1.00*    
!   OV        0.99     PT        0.96     SC        1.06     WF        1.13     
!   WZ        1.00*    
! 
! 
! Fit before self-cal, rms=0.056794Jy  sigma=0.000962
! Fit after  self-cal, rms=0.051503Jy  sigma=0.000828
dynam = dynam - 0.5
doamp = false
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=1.049 mas, bmaj=3.656 mas, bpa=0.1134 degrees
! Estimated noise=1550.18 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal doamp, doflt, solint
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00157013 Jy
! Component: 100  -  total flux cleaned = 0.00180494 Jy
! Total flux subtracted in 100 components = 0.00180494 Jy
! Clean residual min=-0.007365 max=0.008494 Jy/beam
! Clean residual mean=0.000002 rms=0.001966 Jy/beam
! Combined flux in latest and established models = 0.479366 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 9 model components to the UV plane model.
! The established model now contains 44 components and 0.479366 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.051209Jy  sigma=0.000824
! Fit after  self-cal, rms=0.051248Jy  sigma=0.000823
! Inverting map 
dynam = dynam - 1.0
doamp = true
solint = solint * (6.0/3.6)
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 doamp, doflt, solint
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000234251 Jy
! Component: 100  -  total flux cleaned = 0.000444497 Jy
! Total flux subtracted in 100 components = 0.000444497 Jy
! Clean residual min=-0.007289 max=0.008172 Jy/beam
! Clean residual mean=0.000001 rms=0.001926 Jy/beam
! Combined flux in latest and established models = 0.479811 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 8 model components to the UV plane model.
! The established model now contains 45 components and 0.479811 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.051024Jy  sigma=0.000820
! Fit after  self-cal, rms=0.050394Jy  sigma=0.000810
! Inverting map and beam 
! Estimated beam: bmin=1.048 mas, bmaj=3.652 mas, bpa=0.1055 degrees
! Estimated noise=1551.26 mJy/beam.
doamp = false
solint = solint / (6.0/3.6)
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 doamp, doflt, solint
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00170794 Jy
! Component: 100  -  total flux cleaned = 0.00200903 Jy
! Total flux subtracted in 100 components = 0.00200903 Jy
! Clean residual min=-0.006978 max=0.007590 Jy/beam
! Clean residual mean=0.000003 rms=0.001867 Jy/beam
! Combined flux in latest and established models = 0.48182 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 11 model components to the UV plane model.
! The established model now contains 51 components and 0.48182 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.050168Jy  sigma=0.000807
! Fit after  self-cal, rms=0.050172Jy  sigma=0.000807
! Inverting map 
print "***********************************"
! *********************************** 
print "*** Finished Amplitude Self-Cal ***"
! *** Finished Amplitude Self-Cal *** 
print "***********************************"
! *********************************** 
save 0434-188_X
! Writing UV FITS file: 0434-188_X.uvf
! Writing 51 model components to file: 0434-188_X.mod
! wwins: Wrote 1 windows to 0434-188_X.win
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 1.048 x 3.652 at 0.1055 degrees (North through East)
! Clean map  min=-0.0067294  max=0.4196 Jy/beam
! Writing clean map to FITS file: 0434-188_X.fits
! Writing difmap environment to: 0434-188_X.par
print "****************************"
! **************************** 
print "*** Now, make some plots ***"
! *** Now, make some plots *** 
print "****************************"
! **************************** 
![@gonzo_plot 0434-188_X]
device 0434-188_Xuv.ps/vps,1,2
! Attempting to open device: '0434-188_Xuv.ps/vps'
radplot
! Using default options string "m1"
uvplot
! Using default options string ""
device 0434-188_Xim.ps/vps
! Attempting to open device: '0434-188_Xim.ps/vps'
uvweight 0,-1
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
loglevs -1,2048,2
! The new contour levels are:
!  -1 1 2 4 8 16 32 64 128 256 512 1024 2048
cmul = imstat(rms)*3
! Inverting map and beam 
! Estimated beam: bmin=1.048 mas, bmaj=3.652 mas, bpa=0.1055 degrees
! Estimated noise=1551.26 mJy/beam.
mappl cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 1.048 x 3.652 at 0.1055 degrees (North through East)
! Clean map  min=-0.0067294  max=0.4196 Jy/beam
![Exited script file: gonzo_plot]
![Exited script file: gonzo8-0.1]
quit
! Quitting program
! Log file 0434-188_X.log closed on Fri Feb 15 00:45:46 2008