! Started logfile: 0342+147_X.log on Wed May 14 12:17:34 2008
observe 0342+147_X.edt
! Reading UV FITS file: 0342+147_X.edt
! AN table 1: 5 integrations on 153 of 153 possible baselines.
! Apparent sampling: 0.0235294 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: 0342+147
! 
! 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 72 visibilities.
![@gonzo8-0.1 0342+147_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 83 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 82 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 84 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 82 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.730814Jy  sigma=0.006131
! Fit after  self-cal, rms=0.718965Jy  sigma=0.006118
! 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=0.8347 mas, bmaj=1.138 mas, bpa=2.696 degrees
! Estimated noise=19110.9 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=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.21038 Jy
! Total flux subtracted in 50 components = 0.21038 Jy
! Clean residual min=-0.057880 max=0.059354 Jy/beam
! Clean residual mean=-0.000056 rms=0.019741 Jy/beam
! Combined flux in latest and established models = 0.21038 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 0.21038 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.124934Jy  sigma=0.001158
! Fit after  self-cal, rms=0.124957Jy  sigma=0.001158
! 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=1.001 mas, bmaj=1.322 mas, bpa=31.6 degrees
! Estimated noise=14213.6 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 = 0.0263395 Jy
! Component: 100  -  total flux cleaned = 0.0194159 Jy
! Total flux subtracted in 100 components = 0.0194159 Jy
! Clean residual min=-0.022691 max=0.022960 Jy/beam
! Clean residual mean=-0.000018 rms=0.008274 Jy/beam
! Combined flux in latest and established models = 0.229796 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 40 model components to the UV plane model.
! The established model now contains 40 components and 0.229796 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.072520Jy  sigma=0.000599
! Fit after  self-cal, rms=0.072315Jy  sigma=0.000594
! 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        1.00*    FD        1.00*    GC        1.09     HH        1.00*    
!   HN        1.00*    KK        1.05     KP        0.89     LA        1.00*    
!   MC        1.00*    MK        1.00*    NL        1.00*    NY        1.00*    
!   ON        1.00*    OV        1.06     PT        1.00*    SC        1.00*    
!   WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    GC        0.86     HH        1.00*    
!   HN        1.00*    KK        1.10     KP        0.97     LA        1.00*    
!   MC        1.00*    MK        1.00*    NL        1.00*    NY        1.00*    
!   ON        1.00*    OV        0.94     PT        1.00*    SC        1.00*    
!   WF        1.00*    WZ        1.00*    
! 
! 
! Correcting IF 3.
!  A total of 6 telescope corrections were flagged in sub-array 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.00*    FD        0.00*    GC        0.00*    HH        0.00*    
!   HN        0.00*    KK        0.00*    KP        0.00*    LA        0.00*    
!   MC        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   ON        0.00*    OV        0.00*    PT        0.00*    SC        0.00*    
!   WF        0.00*    WZ        0.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    GC        1.15     HH        1.00*    
!   HN        1.00*    KK        1.05     KP        1.01     LA        1.00*    
!   MC        1.00*    MK        1.00*    NL        1.00*    NY        1.00*    
!   ON        1.00*    OV        0.92     PT        1.00*    SC        1.00*    
!   WF        1.00*    WZ        1.00*    
! 
! 
! Fit before self-cal, rms=0.072315Jy  sigma=0.000594
! Fit after  self-cal, rms=0.067182Jy  sigma=0.000532
dynam = dynam - 0.5
doamp = false
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=0.9715 mas, bmaj=1.238 mas, bpa=9.911 degrees
! Estimated noise=16411.8 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 = 0.00260408 Jy
! Component: 100  -  total flux cleaned = 0.000686968 Jy
! Total flux subtracted in 100 components = 0.000686968 Jy
! Clean residual min=-0.007291 max=0.007379 Jy/beam
! Clean residual mean=0.000001 rms=0.001954 Jy/beam
! Combined flux in latest and established models = 0.230483 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 62 components and 0.230483 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.062159Jy  sigma=0.000488
! Fit after  self-cal, rms=0.062275Jy  sigma=0.000486
! 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 = 0.000260137 Jy
! Component: 100  -  total flux cleaned = -0.000447507 Jy
! Total flux subtracted in 100 components = -0.000447507 Jy
! Clean residual min=-0.005913 max=0.005857 Jy/beam
! Clean residual mean=-0.000001 rms=0.001666 Jy/beam
! Combined flux in latest and established models = 0.230036 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 16 model components to the UV plane model.
! The established model now contains 75 components and 0.230036 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.059723Jy  sigma=0.000467
! Fit after  self-cal, rms=0.030338Jy  sigma=0.000192
! Inverting map and beam 
! Estimated beam: bmin=0.9688 mas, bmaj=1.244 mas, bpa=9.508 degrees
! Estimated noise=16456.7 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 = 0.0017222 Jy
! Component: 100  -  total flux cleaned = 0.00232585 Jy
! Total flux subtracted in 100 components = 0.00232585 Jy
! Clean residual min=-0.002994 max=0.003049 Jy/beam
! Clean residual mean=0.000000 rms=0.000865 Jy/beam
! Combined flux in latest and established models = 0.232361 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 21 model components to the UV plane model.
! The established model now contains 96 components and 0.232361 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.027929Jy  sigma=0.000182
! Fit after  self-cal, rms=0.028969Jy  sigma=0.000179
! Inverting map 
print "***********************************"
! *********************************** 
print "*** Finished Amplitude Self-Cal ***"
! *** Finished Amplitude Self-Cal *** 
print "***********************************"
! *********************************** 
save 0342+147_X
! Writing UV FITS file: 0342+147_X.uvf
! Writing 96 model components to file: 0342+147_X.mod
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.9688 x 1.244 at 9.508 degrees (North through East)
! Clean map  min=-0.032714  max=0.22292 Jy/beam
! Writing clean map to FITS file: 0342+147_X.fits
! Writing difmap environment to: 0342+147_X.par
print "****************************"
! **************************** 
print "*** Now, make some plots ***"
! *** Now, make some plots *** 
print "****************************"
! **************************** 
![@gonzo_plot 0342+147_X]
device 0342+147_Xuv.ps/vps,1,2
! Attempting to open device: '0342+147_Xuv.ps/vps'
radplot
! Using default options string "m1"
uvplot
! Using default options string ""
device 0342+147_Xim.ps/vps
! Attempting to open device: '0342+147_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=0.9688 mas, bmaj=1.244 mas, bpa=9.508 degrees
! Estimated noise=16456.7 mJy/beam.
mappl cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.9688 x 1.244 at 9.508 degrees (North through East)
! Clean map  min=-0.032714  max=0.22292 Jy/beam
![Exited script file: gonzo_plot]
![Exited script file: gonzo8-0.1]
quit
! Quitting program
! Log file 0342+147_X.log closed on Wed May 14 12:17:41 2008