! Started logfile: 0919-260_S.log on Tue Apr 29 23:14:54 2008
observe 0919-260_S.edt
! Reading UV FITS file: 0919-260_S.edt
! AN table 1: 10 integrations on 153 of 153 possible baselines.
! Apparent sampling: 0.0431373 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  2.22497e+09        8e+06          1        8e+06
!  02        2  2.24497e+09        8e+06          1        8e+06
!  03        3  2.33497e+09        8e+06          1        8e+06
!  04        4  2.36497e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 963 lines of history.
! 
! Reading 264 visibilities.
![@gonzo6-0.4 0919-260_S]
print "***********************************"
! *********************************** 
print "*** Using gonzo instruction set ***"
! *** Using gonzo instruction set *** 
print "***********************************"
! *********************************** 
float field_size
field_size = 1024
float field_cell
field_cell = 0.4
integer clean_niter
clean_niter = 50
float clean_gain
clean_gain = 0.03
float dynam
dynam = 6.0
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 0.400x0.400 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 157 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 168 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 164 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 166 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.242367Jy  sigma=0.002296
! Fit after  self-cal, rms=0.237211Jy  sigma=0.002281
! 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=4.571 mas, bmaj=12.95 mas, bpa=-13.55 degrees
! Estimated noise=8816.77 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 = 0.65998 Jy
! Total flux subtracted in 50 components = 0.65998 Jy
! Clean residual min=-0.090158 max=0.184197 Jy/beam
! Clean residual mean=-0.000637 rms=0.036307 Jy/beam
! Combined flux in latest and established models = 0.65998 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 2 model components to the UV plane model.
! The established model now contains 2 components and 0.65998 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.242046Jy  sigma=0.002817
! Fit after  self-cal, rms=0.242046Jy  sigma=0.002816
! 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=4.771 mas, bmaj=11.05 mas, bpa=-9.811 degrees
! Estimated noise=7456.63 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 = 0.182835 Jy
! Component: 100  -  total flux cleaned = 0.269786 Jy
! Total flux subtracted in 100 components = 0.269786 Jy
! Clean residual min=-0.036702 max=0.040177 Jy/beam
! Clean residual mean=-0.000221 rms=0.011293 Jy/beam
! Combined flux in latest and established models = 0.929766 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 22 model components to the UV plane model.
! The established model now contains 23 components and 0.929766 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.094494Jy  sigma=0.001037
! Fit after  self-cal, rms=0.093922Jy  sigma=0.001033
! 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        0.96     FD        0.97     GC        1.00*    HH        1.00*    
!   HN        0.96     KK        1.00*    KP        0.96     LA        0.98     
!   MC        1.00*    MK        1.00*    NL        0.98     NY        1.00*    
!   ON        1.00*    OV        0.93     PT        1.00*    SC        1.04     
!   WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 2.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    GC        1.00*    HH        1.00*    
!   HN        0.95     KK        1.00*    KP        1.00     LA        0.96     
!   MC        1.00*    MK        1.00*    NL        0.98     NY        1.00*    
!   ON        1.00*    OV        1.00*    PT        1.00*    SC        0.99     
!   WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.93     GC        1.00*    HH        1.00*    
!   HN        0.97     KK        1.00*    KP        0.96     LA        0.99     
!   MC        1.00*    MK        1.00*    NL        0.98     NY        1.00*    
!   ON        1.00*    OV        1.00*    PT        1.00*    SC        1.03     
!   WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.95     GC        1.00*    HH        1.00*    
!   HN        0.94     KK        1.00*    KP        1.00     LA        1.00*    
!   MC        1.00*    MK        1.00*    NL        0.99     NY        1.00*    
!   ON        1.00*    OV        1.00*    PT        1.00*    SC        1.03     
!   WF        1.00*    WZ        1.00*    
! 
! 
! Fit before self-cal, rms=0.093922Jy  sigma=0.001033
! Fit after  self-cal, rms=0.077321Jy  sigma=0.000826
dynam = dynam - 0.5
doamp = false
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=4.651 mas, bmaj=11.22 mas, bpa=-11.32 degrees
! Estimated noise=7505.94 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 = 0.0205442 Jy
! Component: 100  -  total flux cleaned = 0.022702 Jy
! Total flux subtracted in 100 components = 0.022702 Jy
! Clean residual min=-0.019417 max=0.024465 Jy/beam
! Clean residual mean=-0.000036 rms=0.005833 Jy/beam
! Combined flux in latest and established models = 0.952468 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 32 components and 0.952468 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.070848Jy  sigma=0.000735
! Fit after  self-cal, rms=0.070710Jy  sigma=0.000734
! 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)
! Added new window around map position (-0.4, 60.8).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0206541 Jy
! Component: 100  -  total flux cleaned = 0.0263533 Jy
! Total flux subtracted in 100 components = 0.0263533 Jy
! Clean residual min=-0.015054 max=0.017810 Jy/beam
! Clean residual mean=-0.000018 rms=0.004633 Jy/beam
! Combined flux in latest and established models = 0.978822 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 52 components and 0.978822 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.066189Jy  sigma=0.000655
! Fit after  self-cal, rms=0.063836Jy  sigma=0.000639
! Inverting map and beam 
! Estimated beam: bmin=4.644 mas, bmaj=11.23 mas, bpa=-11.32 degrees
! Estimated noise=7466.45 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)
! Added new window around map position (-98.4, -80.8).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0127121 Jy
! Component: 100  -  total flux cleaned = 0.0181377 Jy
! Total flux subtracted in 100 components = 0.0181377 Jy
! Clean residual min=-0.011815 max=0.012997 Jy/beam
! Clean residual mean=0.000000 rms=0.003388 Jy/beam
! Combined flux in latest and established models = 0.996959 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 25 model components to the UV plane model.
! The established model now contains 77 components and 0.996959 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.060398Jy  sigma=0.000573
! Fit after  self-cal, rms=0.060196Jy  sigma=0.000571
! Inverting map 
print "***********************************"
! *********************************** 
print "*** Finished Amplitude Self-Cal ***"
! *** Finished Amplitude Self-Cal *** 
print "***********************************"
! *********************************** 
save 0919-260_S
! Writing UV FITS file: 0919-260_S.uvf
! Writing 77 model components to file: 0919-260_S.mod
! wwins: Wrote 3 windows to 0919-260_S.win
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 4.644 x 11.23 at -11.32 degrees (North through East)
! Clean map  min=-0.011704  max=0.80873 Jy/beam
! Writing clean map to FITS file: 0919-260_S.fits
! Writing difmap environment to: 0919-260_S.par
print "****************************"
! **************************** 
print "*** Now, make some plots ***"
! *** Now, make some plots *** 
print "****************************"
! **************************** 
![@gonzo_plot 0919-260_S]
device 0919-260_Suv.ps/vps,1,2
! Attempting to open device: '0919-260_Suv.ps/vps'
radplot
! Using default options string "m1"
uvplot
! Using default options string ""
device 0919-260_Sim.ps/vps
! Attempting to open device: '0919-260_Sim.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=4.644 mas, bmaj=11.23 mas, bpa=-11.32 degrees
! Estimated noise=7466.45 mJy/beam.
mappl cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 4.644 x 11.23 at -11.32 degrees (North through East)
! Clean map  min=-0.011704  max=0.80873 Jy/beam
![Exited script file: gonzo_plot]
![Exited script file: gonzo6-0.4]
quit
! Quitting program
! Log file 0919-260_S.log closed on Tue Apr 29 23:14:57 2008