! Started logfile: 1954-388_X.log on Thu Aug 14 11:14:36 2008
observe 1954-388_X.edt2
! Reading UV FITS file: 1954-388_X.edt2
! AN table 1: 18 integrations on 171 of 171 possible baselines.
! Apparent sampling: 0.103639 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: 1954-388
! 
! 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 1530 lines of history.
! 
! Reading 1276 visibilities.
![@gonzo7-0.1 1954-388_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 = 7.0
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 243 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 243 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 243 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 249 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.436674Jy  sigma=5.908214
! Fit after  self-cal, rms=0.436656Jy  sigma=5.910504
! 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=0.6788 mas, bmaj=1.986 mas, bpa=-10.45 degrees
! Estimated noise=2.91043 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 = 0.504352 Jy
! Total flux subtracted in 50 components = 0.504351 Jy
! Clean residual min=-0.071895 max=0.166230 Jy/beam
! Clean residual mean=-0.001044 rms=0.029177 Jy/beam
! Combined flux in latest and established models = 0.504351 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 5 model components to the UV plane model.
! The established model now contains 5 components and 0.504351 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.352262Jy  sigma=6.934020
! Fit after  self-cal, rms=0.351741Jy  sigma=6.932774
! 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=0.92 mas, bmaj=2.889 mas, bpa=1.467 degrees
! Estimated noise=1.62239 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 = 0.25614 Jy
! Component: 100  -  total flux cleaned = 0.379009 Jy
! Total flux subtracted in 100 components = 0.379009 Jy
! Clean residual min=-0.035770 max=0.085375 Jy/beam
! Clean residual mean=-0.000629 rms=0.015392 Jy/beam
! Combined flux in latest and established models = 0.883361 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 32 model components to the UV plane model.
! The established model now contains 34 components and 0.883361 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.181102Jy  sigma=2.902449
! Fit after  self-cal, rms=0.179412Jy  sigma=2.880806
! 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 12 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.85     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.00*    KP        1.00     LA        0.86     
!   MA        1.00*    MK        1.13     NL        1.10     NY        1.00*    
!   OV        0.95     PT        0.86     SC        1.16     TS        1.00*    
!   WF        1.45     WZ        1.00*    GG        1.00*    
! 
! 
! Correcting IF 2.
!  A total of 12 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.89     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.00*    KP        0.91     LA        0.86     
!   MA        1.00*    MK        1.02     NL        0.94     NY        1.00*    
!   OV        1.00     PT        1.01     SC        1.01     TS        1.00*    
!   WF        1.38     WZ        1.00*    GG        1.00*    
! 
! 
! Correcting IF 3.
!  A total of 12 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.89     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.00*    KP        0.78     LA        0.98     
!   MA        1.00*    MK        1.08     NL        0.95     NY        1.00*    
!   OV        0.89     PT        0.96     SC        0.89     TS        1.00*    
!   WF        1.38     WZ        1.00*    GG        1.00*    
! 
! 
! Correcting IF 4.
!  A total of 6 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.98     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.00*    KP        0.81     LA        1.17     
!   MA        1.00*    MK        1.07     NL        1.04     NY        1.00*    
!   OV        0.97     PT        0.97     SC        0.90     TS        1.00*    
!   WF        1.30     WZ        1.00*    GG        1.00*    
! 
! 
! Fit before self-cal, rms=0.179412Jy  sigma=2.880806
! Fit after  self-cal, rms=0.132935Jy  sigma=1.339496
dynam = dynam - 0.5
doamp = false
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=0.9329 mas, bmaj=2.936 mas, bpa=2.788 degrees
! Estimated noise=1.57483 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 (-3.9, 8.3).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.011146 Jy
! Component: 100  -  total flux cleaned = 0.00833724 Jy
! Total flux subtracted in 100 components = 0.00833724 Jy
! Clean residual min=-0.008666 max=0.010454 Jy/beam
! Clean residual mean=-0.000019 rms=0.002511 Jy/beam
! Combined flux in latest and established models = 0.891698 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 43 components and 0.891698 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.129157Jy  sigma=1.310245
! Fit after  self-cal, rms=0.128676Jy  sigma=1.300016
! 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 = 7.40302e-05 Jy
! Component: 100  -  total flux cleaned = -0.0012971 Jy
! Total flux subtracted in 100 components = -0.0012971 Jy
! Clean residual min=-0.008419 max=0.010185 Jy/beam
! Clean residual mean=-0.000020 rms=0.002358 Jy/beam
! Combined flux in latest and established models = 0.890401 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 12 model components to the UV plane model.
! The established model now contains 53 components and 0.890401 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.127727Jy  sigma=1.296108
! Fit after  self-cal, rms=0.124597Jy  sigma=1.198732
! Inverting map and beam 
! Estimated beam: bmin=0.9307 mas, bmaj=2.934 mas, bpa=2.78 degrees
! Estimated noise=1.5629 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 = -0.00181055 Jy
! Component: 100  -  total flux cleaned = -0.00180293 Jy
! Total flux subtracted in 100 components = -0.00180293 Jy
! Clean residual min=-0.008043 max=0.009356 Jy/beam
! Clean residual mean=-0.000037 rms=0.002198 Jy/beam
! Combined flux in latest and established models = 0.888598 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 65 components and 0.888598 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.123954Jy  sigma=1.197446
! Fit after  self-cal, rms=0.123808Jy  sigma=1.195365
! Inverting map 
print "***********************************"
! *********************************** 
print "*** Finished Amplitude Self-Cal ***"
! *** Finished Amplitude Self-Cal *** 
print "***********************************"
! *********************************** 
save 1954-388_X
! Writing UV FITS file: 1954-388_X.uvf
! Writing 65 model components to file: 1954-388_X.mod
! wwins: Wrote 2 windows to 1954-388_X.win
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.9307 x 2.934 at 2.78 degrees (North through East)
! Clean map  min=-0.0079334  max=0.60681 Jy/beam
! Writing clean map to FITS file: 1954-388_X.fits
! Writing difmap environment to: 1954-388_X.par
print "****************************"
! **************************** 
print "*** Now, make some plots ***"
! *** Now, make some plots *** 
print "****************************"
! **************************** 
![@gonzo_plot 1954-388_X]
device 1954-388_Xuv.ps/vps,1,2
! Attempting to open device: '1954-388_Xuv.ps/vps'
radplot
! Using default options string "m1"
uvplot
! Using default options string ""
device 1954-388_Xim.ps/vps
! Attempting to open device: '1954-388_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=0.9307 mas, bmaj=2.934 mas, bpa=2.78 degrees
! Estimated noise=1.5629 mJy/beam.
mappl cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.9307 x 2.934 at 2.78 degrees (North through East)
! Clean map  min=-0.0079334  max=0.60681 Jy/beam
![Exited script file: gonzo_plot]
![Exited script file: gonzo7-0.1]
quit
! Quitting program
! Log file 1954-388_X.log closed on Thu Aug 14 11:14:42 2008