! Started logfile: 0919-260_X.log on Wed May 14 12:00:05 2008
observe 0919-260_X.edt
! Reading UV FITS file: 0919-260_X.edt
! AN table 1: 8 integrations on 153 of 153 possible baselines.
! Apparent sampling: 0.0506536 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: 0919-260
! 
! 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 938 lines of history.
! 
! Reading 248 visibilities.
![@gonzo8-0.1-pw 0919-260_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 118 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 118 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 118 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 119 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.324799Jy  sigma=0.004328
! Fit after  self-cal, rms=0.324113Jy  sigma=0.004334
! 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
peakw win_mult
! Inverting map and beam 
! Estimated beam: bmin=1.222 mas, bmaj=3.232 mas, bpa=-14.09 degrees
! Estimated noise=6781.82 mJy/beam.
! Added new window around map position (0, 0).
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=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.934535 Jy
! Total flux subtracted in 50 components = 0.934535 Jy
! Clean residual min=-0.104313 max=0.260623 Jy/beam
! Clean residual mean=0.000092 rms=0.047100 Jy/beam
! Combined flux in latest and established models = 0.934535 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 1 model components to the UV plane model.
! The established model now contains 1 components and 0.934535 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.374450Jy  sigma=0.004955
! Fit after  self-cal, rms=0.374451Jy  sigma=0.004955
! 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=1.466 mas, bmaj=3.619 mas, bpa=-14.89 degrees
! Estimated noise=5329.67 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 = 0.29205 Jy
! Component: 100  -  total flux cleaned = 0.411767 Jy
! Total flux subtracted in 100 components = 0.411767 Jy
! Clean residual min=-0.053856 max=0.086068 Jy/beam
! Clean residual mean=0.000170 rms=0.025424 Jy/beam
! Combined flux in latest and established models = 1.3463 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 33 components and 1.3463 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.153855Jy  sigma=0.001777
! Fit after  self-cal, rms=0.153433Jy  sigma=0.001770
! 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 9 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.97     GC        1.00*    HH        1.00*    
!   HN        1.01     KK        1.00*    KP        0.94     LA        0.97     
!   MC        1.00*    MK        1.00*    NL        1.17     NY        1.00*    
!   ON        1.00*    OV        1.00*    PT        1.00*    SC        1.01     
!   WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 2.
!  A total of 9 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.97     GC        1.00*    HH        1.00*    
!   HN        1.01     KK        1.00*    KP        0.94     LA        0.95     
!   MC        1.00*    MK        1.00*    NL        1.11     NY        1.00*    
!   ON        1.00*    OV        1.00*    PT        1.00*    SC        0.98     
!   WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 3.
!  A total of 9 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.97     GC        1.00*    HH        1.00*    
!   HN        0.94     KK        1.00*    KP        1.03     LA        0.94     
!   MC        1.00*    MK        1.00*    NL        1.12     NY        1.00*    
!   ON        1.00*    OV        1.00*    PT        1.00*    SC        1.00     
!   WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 4.
!  A total of 9 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.01     GC        1.00*    HH        1.00*    
!   HN        0.97     KK        1.00*    KP        0.99     LA        0.92     
!   MC        1.00*    MK        1.00*    NL        1.10     NY        1.00*    
!   ON        1.00*    OV        1.00*    PT        1.00*    SC        1.12     
!   WF        1.00*    WZ        1.00*    
! 
! 
! Fit before self-cal, rms=0.153433Jy  sigma=0.001770
! Fit after  self-cal, rms=0.107918Jy  sigma=0.000881
dynam = dynam - 0.5
doamp = false
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=1.196 mas, bmaj=3.317 mas, bpa=-15.75 degrees
! Estimated noise=7063.8 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 = -0.00307627 Jy
! Component: 100  -  total flux cleaned = -0.00560505 Jy
! Total flux subtracted in 100 components = -0.00560505 Jy
! Clean residual min=-0.024781 max=0.026727 Jy/beam
! Clean residual mean=-0.000081 rms=0.007593 Jy/beam
! Combined flux in latest and established models = 1.3407 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 12 model components to the UV plane model.
! The established model now contains 45 components and 1.3407 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.105292Jy  sigma=0.000857
! Fit after  self-cal, rms=0.105328Jy  sigma=0.000856
! 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 = -0.000213555 Jy
! Component: 100  -  total flux cleaned = -0.00218142 Jy
! Total flux subtracted in 100 components = -0.00218142 Jy
! Clean residual min=-0.025063 max=0.025500 Jy/beam
! Clean residual mean=-0.000086 rms=0.007349 Jy/beam
! Combined flux in latest and established models = 1.33852 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 20 model components to the UV plane model.
! The established model now contains 61 components and 1.33852 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.104672Jy  sigma=0.000850
! Fit after  self-cal, rms=0.103798Jy  sigma=0.000844
! Inverting map and beam 
! Estimated beam: bmin=1.195 mas, bmaj=3.317 mas, bpa=-15.84 degrees
! Estimated noise=7079.33 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 = 0.00274383 Jy
! Component: 100  -  total flux cleaned = 0.00273978 Jy
! Total flux subtracted in 100 components = 0.00273978 Jy
! Clean residual min=-0.024713 max=0.025189 Jy/beam
! Clean residual mean=-0.000092 rms=0.007162 Jy/beam
! Combined flux in latest and established models = 1.34126 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 15 model components to the UV plane model.
! The established model now contains 71 components and 1.34126 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.103236Jy  sigma=0.000840
! Fit after  self-cal, rms=0.103257Jy  sigma=0.000839
! Inverting map 
print "***********************************"
! *********************************** 
print "*** Finished Amplitude Self-Cal ***"
! *** Finished Amplitude Self-Cal *** 
print "***********************************"
! *********************************** 
save 0919-260_X
! Writing UV FITS file: 0919-260_X.uvf
! Writing 71 model components to file: 0919-260_X.mod
! wwins: Wrote 1 windows to 0919-260_X.win
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 1.195 x 3.317 at -15.84 degrees (North through East)
! Clean map  min=-0.024507  max=1.1971 Jy/beam
! Writing clean map to FITS file: 0919-260_X.fits
! Writing difmap environment to: 0919-260_X.par
print "****************************"
! **************************** 
print "*** Now, make some plots ***"
! *** Now, make some plots *** 
print "****************************"
! **************************** 
![@gonzo_plot 0919-260_X]
device 0919-260_Xuv.ps/vps,1,2
! Attempting to open device: '0919-260_Xuv.ps/vps'
radplot
! Using default options string "m1"
uvplot
! Using default options string ""
device 0919-260_Xim.ps/vps
! Attempting to open device: '0919-260_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=1.195 mas, bmaj=3.317 mas, bpa=-15.84 degrees
! Estimated noise=7079.33 mJy/beam.
mappl cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 1.195 x 3.317 at -15.84 degrees (North through East)
! Clean map  min=-0.024507  max=1.1971 Jy/beam
![Exited script file: gonzo_plot]
![Exited script file: gonzo8-0.1-pw]
quit
! Quitting program
! Log file 0919-260_X.log closed on Wed May 14 12:00:13 2008