! Started logfile: 1144-379_X.log on Tue Aug 12 11:13:08 2008
observe 1144-379_X.edt
! Reading UV FITS file: 1144-379_X.edt
! AN table 1: 9 integrations on 171 of 171 possible baselines.
! AN table 2: 4 integrations on 171 of 171 possible baselines.
! AN table 3: 9 integrations on 171 of 171 possible baselines.
! AN table 4: 34 integrations on 171 of 171 possible baselines.
! Apparent sampling: 0.0474102 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: 1144-379
! 
! 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 1526 lines of history.
! 
! Reading 1816 visibilities.
![@gonzo7-0.1-pw 1144-379_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 132 telescope corrections were flagged in sub-array 1.
!  A total of 76 telescope corrections were flagged in sub-array 2.
!  A total of 171 telescope corrections were flagged in sub-array 3.
!  A total of 534 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 2.
!  A total of 132 telescope corrections were flagged in sub-array 1.
!  A total of 76 telescope corrections were flagged in sub-array 2.
!  A total of 171 telescope corrections were flagged in sub-array 3.
!  A total of 534 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 3.
!  A total of 132 telescope corrections were flagged in sub-array 1.
!  A total of 76 telescope corrections were flagged in sub-array 2.
!  A total of 171 telescope corrections were flagged in sub-array 3.
!  A total of 534 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 4.
!  A total of 132 telescope corrections were flagged in sub-array 1.
!  A total of 76 telescope corrections were flagged in sub-array 2.
!  A total of 171 telescope corrections were flagged in sub-array 3.
!  A total of 534 telescope corrections were flagged in sub-array 4.
! 
! Fit before self-cal, rms=0.731588Jy  sigma=9.348010
! Fit after  self-cal, rms=0.730455Jy  sigma=9.354749
! 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=0.7968 mas, bmaj=5.725 mas, bpa=-5.353 degrees
! Estimated noise=3.99638 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 = 1.19398 Jy
! Total flux subtracted in 50 components = 1.19398 Jy
! Clean residual min=-0.092464 max=0.333033 Jy/beam
! Clean residual mean=0.002211 rms=0.040466 Jy/beam
! Combined flux in latest and established models = 1.19398 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 1.19398 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.571335Jy  sigma=7.362179
! Fit after  self-cal, rms=0.571335Jy  sigma=7.362140
! Inverting map 
! clean: niter=50  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.26938 Jy
! Total flux subtracted in 50 components = 0.269379 Jy
! Clean residual min=-0.072817 max=0.111936 Jy/beam
! Clean residual mean=0.001730 rms=0.024613 Jy/beam
! Combined flux in latest and established models = 1.46336 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 15 components and 1.46336 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.403084Jy  sigma=5.118263
! Fit after  self-cal, rms=0.403024Jy  sigma=5.117912
! 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=0.8797 mas, bmaj=9.36 mas, bpa=-5.767 degrees
! Estimated noise=1.82683 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 = 0.243033 Jy
! Component: 100  -  total flux cleaned = 0.352121 Jy
! Total flux subtracted in 100 components = 0.352121 Jy
! Clean residual min=-0.069661 max=0.080534 Jy/beam
! Clean residual mean=0.001843 rms=0.023742 Jy/beam
! Combined flux in latest and established models = 1.81548 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 63 model components to the UV plane model.
! The established model now contains 76 components and 1.81548 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.282037Jy  sigma=3.404333
! Fit after  self-cal, rms=0.281974Jy  sigma=3.403722
! Inverting map 
print "****************************************"
! **************************************** 
print "*** Finished Natural Weighting CLEAN ***"
! *** Finished Natural Weighting CLEAN *** 
print "****************************************"
! **************************************** 
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.90     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.00*    KP        1.05     LA        0.85     
!   MA        1.00*    MK        1.00*    NL        1.15     NY        1.00*    
!   OV        1.00*    PT        1.05     SC        1.18     TS        1.00*    
!   WF        1.02     WZ        1.00*    GG        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.00*    FD        0.00*    GC        0.00*    HH        0.00*    
!   HN        0.00*    KK        0.00*    KP        0.00*    LA        0.00*    
!   MA        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TS        0.00*    
!   WF        0.00*    WZ        0.00*    GG        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.00*    FD        0.00*    GC        0.00*    HH        0.00*    
!   HN        0.00*    KK        0.00*    KP        0.00*    LA        0.00*    
!   MA        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TS        0.00*    
!   WF        0.00*    WZ        0.00*    GG        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        0.90     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.05     KP        1.01     LA        0.86     
!   MA        1.00*    MK        1.08     NL        1.00*    NY        1.00*    
!   OV        0.92     PT        0.87     SC        1.00*    TS        1.00*    
!   WF        1.00*    WZ        1.00*    GG        1.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        0.99     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.00*    KP        0.94     LA        0.85     
!   MA        1.00*    MK        1.00*    NL        1.00     NY        1.00*    
!   OV        1.00*    PT        1.24     SC        0.92     TS        1.00*    
!   WF        1.01     WZ        1.00*    GG        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.00*    FD        0.00*    GC        0.00*    HH        0.00*    
!   HN        0.00*    KK        0.00*    KP        0.00*    LA        0.00*    
!   MA        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TS        0.00*    
!   WF        0.00*    WZ        0.00*    GG        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.00*    FD        0.00*    GC        0.00*    HH        0.00*    
!   HN        0.00*    KK        0.00*    KP        0.00*    LA        0.00*    
!   MA        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TS        0.00*    
!   WF        0.00*    WZ        0.00*    GG        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        0.99     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.07     KP        0.92     LA        0.85     
!   MA        1.00*    MK        1.00     NL        1.00*    NY        1.00*    
!   OV        1.01     PT        1.03     SC        1.00*    TS        1.00*    
!   WF        1.00*    WZ        1.00*    GG        1.00*    
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.03     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.00*    KP        0.85     LA        1.02     
!   MA        1.00*    MK        1.00*    NL        1.04     NY        1.00*    
!   OV        1.00*    PT        1.18     SC        0.85     TS        1.00*    
!   WF        1.11     WZ        1.00*    GG        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.00*    FD        0.00*    GC        0.00*    HH        0.00*    
!   HN        0.00*    KK        0.00*    KP        0.00*    LA        0.00*    
!   MA        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TS        0.00*    
!   WF        0.00*    WZ        0.00*    GG        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.00*    FD        0.00*    GC        0.00*    HH        0.00*    
!   HN        0.00*    KK        0.00*    KP        0.00*    LA        0.00*    
!   MA        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TS        0.00*    
!   WF        0.00*    WZ        0.00*    GG        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        0.99     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.06     KP        0.81     LA        1.02     
!   MA        1.00*    MK        1.07     NL        1.00*    NY        1.00*    
!   OV        0.91     PT        0.94     SC        1.00*    TS        1.00*    
!   WF        1.00*    WZ        1.00*    GG        1.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.18     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.00*    KP        0.83     LA        1.23     
!   MA        1.00*    MK        1.00*    NL        1.11     NY        1.00*    
!   OV        1.00*    PT        1.25     SC        0.92     TS        1.00*    
!   WF        1.01     WZ        1.00*    GG        1.00*    
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.00*    FD        0.00*    GC        0.00*    HH        0.00*    
!   HN        0.00*    KK        0.00*    KP        0.00*    LA        0.00*    
!   MA        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TS        0.00*    
!   WF        0.00*    WZ        0.00*    GG        0.00*    
! 
!  Telescope amplitude corrections in sub-array 3:
!   BR        0.00*    FD        0.00*    GC        0.00*    HH        0.00*    
!   HN        0.00*    KK        0.00*    KP        0.00*    LA        0.00*    
!   MA        0.00*    MK        0.00*    NL        0.00*    NY        0.00*    
!   OV        0.00*    PT        0.00*    SC        0.00*    TS        0.00*    
!   WF        0.00*    WZ        0.00*    GG        0.00*    
! 
!  Telescope amplitude corrections in sub-array 4:
!   BR        1.00*    FD        1.11     GC        1.00*    HH        1.00*    
!   HN        1.00*    KK        1.02     KP        0.83     LA        1.20     
!   MA        1.00*    MK        1.12     NL        1.00*    NY        1.00*    
!   OV        0.99     PT        0.96     SC        1.00*    TS        1.00*    
!   WF        1.00*    WZ        1.00*    GG        1.00*    
! 
! 
! Fit before self-cal, rms=0.281974Jy  sigma=3.403722
! Fit after  self-cal, rms=0.123172Jy  sigma=1.006360
dynam = dynam - 0.5
doamp = false
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=0.8952 mas, bmaj=9.465 mas, bpa=-5.734 degrees
! Estimated noise=1.78369 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 = -0.0136274 Jy
! Component: 100  -  total flux cleaned = -0.0146248 Jy
! Total flux subtracted in 100 components = -0.0146248 Jy
! Clean residual min=-0.012419 max=0.011642 Jy/beam
! Clean residual mean=0.000058 rms=0.003385 Jy/beam
! Combined flux in latest and established models = 1.80085 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 14 model components to the UV plane model.
! The established model now contains 90 components and 1.80085 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.120782Jy  sigma=0.989658
! Fit after  self-cal, rms=0.120780Jy  sigma=0.988551
! 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 = -0.000705703 Jy
! Component: 100  -  total flux cleaned = -0.00145797 Jy
! Total flux subtracted in 100 components = -0.00145797 Jy
! Clean residual min=-0.011576 max=0.011572 Jy/beam
! Clean residual mean=0.000073 rms=0.003310 Jy/beam
! Combined flux in latest and established models = 1.79939 Jy
! Performing amp+phase self-cal over 1 minute time intervals
! Adding 10 model components to the UV plane model.
! The established model now contains 96 components and 1.79939 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.120091Jy  sigma=0.983089
! Fit after  self-cal, rms=0.115110Jy  sigma=0.906082
! Inverting map and beam 
! Estimated beam: bmin=0.897 mas, bmaj=9.484 mas, bpa=-5.72 degrees
! Estimated noise=1.77901 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 = -0.0106972 Jy
! Component: 100  -  total flux cleaned = -0.0117808 Jy
! Total flux subtracted in 100 components = -0.0117808 Jy
! Clean residual min=-0.009320 max=0.010163 Jy/beam
! Clean residual mean=0.000053 rms=0.002595 Jy/beam
! Combined flux in latest and established models = 1.78761 Jy
! Performing phase self-cal over 0.6 minute time intervals
! Adding 10 model components to the UV plane model.
! The established model now contains 100 components and 1.78761 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.113465Jy  sigma=0.896162
! Fit after  self-cal, rms=0.113428Jy  sigma=0.895565
! Inverting map 
print "***********************************"
! *********************************** 
print "*** Finished Amplitude Self-Cal ***"
! *** Finished Amplitude Self-Cal *** 
print "***********************************"
! *********************************** 
save 1144-379_X
! Writing UV FITS file: 1144-379_X.uvf
! Writing 100 model components to file: 1144-379_X.mod
! wwins: Wrote 1 windows to 1144-379_X.win
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.897 x 9.484 at -5.72 degrees (North through East)
! Clean map  min=-0.0089589  max=1.5746 Jy/beam
! Writing clean map to FITS file: 1144-379_X.fits
! Writing difmap environment to: 1144-379_X.par
print "****************************"
! **************************** 
print "*** Now, make some plots ***"
! *** Now, make some plots *** 
print "****************************"
! **************************** 
![@gonzo_plot 1144-379_X]
device 1144-379_Xuv.ps/vps,1,2
! Attempting to open device: '1144-379_Xuv.ps/vps'
radplot
! Using default options string "m1"
uvplot
! Using default options string ""
device 1144-379_Xim.ps/vps
! Attempting to open device: '1144-379_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=0.897 mas, bmaj=9.484 mas, bpa=-5.72 degrees
! Estimated noise=1.77901 mJy/beam.
mappl cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.897 x 9.484 at -5.72 degrees (North through East)
! Clean map  min=-0.0089589  max=1.5746 Jy/beam
![Exited script file: gonzo_plot]
![Exited script file: gonzo7-0.1-pw]
quit
! Quitting program
! Log file 1144-379_X.log closed on Tue Aug 12 11:13:14 2008