! Started logfile: /scr/pima/rdv76_uvs/J1354-0206_X_dfm.log on Fri Jun 15 03:54:45 2018
float field_size
field_size =  1024
float field_cell
field_cell =   0.2000
float taper_size
taper_size =   70.0
float freq
freq       =    8.40599
obs     /scr/pima/rdv76_uvs/J1354-0206_X_uva.fits
! Reading UV FITS file: /scr/pima/rdv76_uvs/J1354-0206_X_uva.fits
! AN table 1: 11 integrations on 6 of 6 possible baselines.
! AN table 2: 27 integrations on 36 of 36 possible baselines.
! AN table 3: 77 integrations on 45 of 45 possible baselines.
! AN table 4: 45 integrations on 3 of 3 possible baselines.
! Apparent sampling: 0.428849 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J1354-0206
! 
! 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  8.40599e+09        8e+06          1        8e+06
!  02        2  8.47599e+09        8e+06          1        8e+06
!  03        3  8.79099e+09        8e+06          1        8e+06
!  04        4  8.89599e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 79 lines of history.
! 
! Reading 7956 visibilities.
select rr, 1,2,3,4,5,6,7,8,9,10,11,12,13,14,15,16 
! Restricting channel ranges to the available 4 channels.
! 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
print "field_size =", field_size
! field_size = 1024 
print "field_cell =", field_cell
! field_cell = 0.2 
print "taper_size =", taper_size
! taper_size = 70 
![@/opt64/bin/pima_mupet_01.dfm J1354-0206_X]
float lim_self
lim_self = 120.0
float lim_val
lim_va   = 1.2
integer clean_niter
clean_niter = 100
float clean_gain
clean_gain = 0.03
float dynam
dynam = 6.0
float soltime1
soltime1 = 120
float soltime2
soltime2 = 20
float thresh
thresh = 0.5
float win_mult
win_mult = 1.8
float time_av
time_av = 16
float old_peak
float new_peak
float flux_cutoff
print "==============================================================="
! =============================================================== 
! 
print "=== Difmap script: pima_mupet_01.dvm version of 2016.05.19 === "
! === Difmap script: pima_mupet_01.dvm version of 2016.05.19 ===  
! 
mapsize field_size, field_cell
! Map grid = 1024x1024 pixels with 0.200x0.200 milli-arcsec cellsize.
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 12 telescope corrections were flagged in sub-array 1.
!  A total of 78 telescope corrections were flagged in sub-array 2.
!  A total of 476 telescope corrections were flagged in sub-array 3.
!  A total of 84 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 2.
!  A total of 12 telescope corrections were flagged in sub-array 1.
!  A total of 78 telescope corrections were flagged in sub-array 2.
!  A total of 476 telescope corrections were flagged in sub-array 3.
!  A total of 84 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 3.
!  A total of 12 telescope corrections were flagged in sub-array 1.
!  A total of 78 telescope corrections were flagged in sub-array 2.
!  A total of 476 telescope corrections were flagged in sub-array 3.
!  A total of 84 telescope corrections were flagged in sub-array 4.
! 
! Correcting IF 4.
!  A total of 12 telescope corrections were flagged in sub-array 1.
!  A total of 78 telescope corrections were flagged in sub-array 2.
!  A total of 476 telescope corrections were flagged in sub-array 3.
!  A total of 84 telescope corrections were flagged in sub-array 4.
! 
! Fit before self-cal, rms=1.239133Jy  sigma=14.505411
! Fit after  self-cal, rms=0.404956Jy  sigma=4.641520
! clrmod: Cleared the established, tentative and continuum models.
! Redundant starting model cleared.
uvw 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.
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.212% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.654 mas, bmaj=1.856 mas, bpa=-6.949 degrees
! Estimated noise=1.05723 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (0, 0).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.493643 Jy
! Component: 100  -  total flux cleaned = 0.638246 Jy
! Total flux subtracted in 100 components = 0.638246 Jy
! Clean residual min=-0.020892 max=0.061162 Jy/beam
! Clean residual mean=-0.000037 rms=0.004986 Jy/beam
! Combined flux in latest and established models = 0.638245 Jy
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 7 components and 0.638245 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.212261Jy  sigma=2.387820
! Fit after  self-cal, rms=0.212079Jy  sigma=2.386347
! Inverting map 
! Your choice of large map pixels excluded 0.212% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0657035 Jy
! Component: 100  -  total flux cleaned = 0.102865 Jy
! Total flux subtracted in 100 components = 0.102865 Jy
! Clean residual min=-0.013024 max=0.019084 Jy/beam
! Clean residual mean=-0.000016 rms=0.002985 Jy/beam
! Combined flux in latest and established models = 0.741111 Jy
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 23 components and 0.741111 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.182031Jy  sigma=1.992529
! Fit after  self-cal, rms=0.181799Jy  sigma=1.990490
! Inverting map 
! Your choice of large map pixels excluded 0.212% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0241894 Jy
! Component: 100  -  total flux cleaned = 0.0396278 Jy
! Total flux subtracted in 100 components = 0.0396278 Jy
! Clean residual min=-0.011595 max=0.010878 Jy/beam
! Clean residual mean=-0.000009 rms=0.002571 Jy/beam
! Combined flux in latest and established models = 0.780739 Jy
! Performing phase self-cal
! Adding 14 model components to the UV plane model.
! The established model now contains 31 components and 0.780739 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.176302Jy  sigma=1.917104
! Fit after  self-cal, rms=0.176224Jy  sigma=1.916408
! Inverting map 
! Your choice of large map pixels excluded 0.212% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
print "============== Finished uniform weighting clean ==============="
! ============== Finished uniform weighting clean =============== 
! 
uvw 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
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.212% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.7068 mas, bmaj=2.161 mas, bpa=-7.416 degrees
! Estimated noise=0.81529 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0206906 Jy
! Component: 100  -  total flux cleaned = 0.0326179 Jy
! Component: 150  -  total flux cleaned = 0.0401221 Jy
! Component: 200  -  total flux cleaned = 0.0448778 Jy
! Total flux subtracted in 200 components = 0.0448778 Jy
! Clean residual min=-0.008625 max=0.007945 Jy/beam
! Clean residual mean=-0.000004 rms=0.001976 Jy/beam
! Combined flux in latest and established models = 0.825616 Jy
! Performing phase self-cal
! Adding 38 model components to the UV plane model.
! The established model now contains 58 components and 0.825617 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.173759Jy  sigma=1.883885
! Fit after  self-cal, rms=0.173747Jy  sigma=1.883604
! Inverting map 
! Your choice of large map pixels excluded 0.212% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
print "============== Finished natural weighting clean =============="
! ============== Finished natural weighting clean ============== 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7068 x 2.161 at -7.416 degrees (North through East)
! Clean map  min=-0.0081582  max=0.64778 Jy/beam
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Telescope amplitude corrections in sub-array 1:
!   HN        1.21     NL        1.01     OV        0.99     SC        0.96     
! 
!  A total of 9 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.99     FD        0.99     KP        0.98     LA        0.97     
!   NL        0.98     OV        1.04     PT        1.00     SC        1.01     
!   WZ        1.03     
! 
!  A total of 27 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00     FD        1.02     KK        0.95     KP        1.01     
!   LA        0.95     MK        1.02     NL        1.01     OV        1.03     
!   PT        0.98     SC        1.00     
! 
!  A total of 51 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   NY        0.00*    WZ        0.00*    ZC        0.00*    
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   HN        1.11     NL        0.92     OV        1.03     SC        1.01     
! 
!  A total of 9 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00     FD        1.02     KP        1.00     LA        0.97     
!   NL        0.99     OV        1.00     PT        1.02     SC        1.01     
!   WZ        0.95     
! 
!  A total of 27 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.03     FD        1.02     KK        0.98     KP        1.00     
!   LA        0.95     MK        1.00     NL        1.00     OV        1.00     
!   PT        0.99     SC        0.97     
! 
!  A total of 51 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   NY        0.00*    WZ        0.00*    ZC        0.00*    
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   HN        1.11     NL        1.04     OV        1.02     SC        1.02     
! 
!  A total of 9 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.99     FD        1.01     KP        1.01     LA        0.97     
!   NL        0.97     OV        1.01     PT        1.03     SC        1.01     
!   WZ        1.06     
! 
!  A total of 27 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.01     FD        1.01     KK        0.96     KP        1.01     
!   LA        0.97     MK        1.02     NL        0.99     OV        1.00     
!   PT        1.00     SC        1.00     
! 
!  A total of 51 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   NY        0.00*    WZ        0.00*    ZC        0.00*    
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   HN        1.21     NL        1.12     OV        0.99     SC        1.00     
! 
!  A total of 9 telescope corrections were flagged in sub-array 2.
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.97     FD        1.00     KP        0.99     LA        0.95     
!   NL        0.99     OV        1.01     PT        1.00     SC        1.03     
!   WZ        1.03     
! 
!  A total of 27 telescope corrections were flagged in sub-array 3.
!  Telescope amplitude corrections in sub-array 3:
!   BR        1.00     FD        1.04     KK        0.96     KP        1.00     
!   LA        0.96     MK        1.00     NL        1.00     OV        1.03     
!   PT        1.00     SC        0.96     
! 
!  A total of 51 telescope corrections were flagged in sub-array 4.
!  Telescope amplitude corrections in sub-array 4:
!   NY        0.00*    WZ        0.00*    ZC        0.00*    
! 
! 
! Fit before self-cal, rms=0.173747Jy  sigma=1.883604
! Fit after  self-cal, rms=0.170388Jy  sigma=1.874116
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.7099 mas, bmaj=2.163 mas, bpa=-6.924 degrees
! Estimated noise=0.83273 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000692132 Jy
! Component: 100  -  total flux cleaned = 0.00101294 Jy
! Component: 150  -  total flux cleaned = 0.00101433 Jy
! Component: 200  -  total flux cleaned = 0.000967021 Jy
! Total flux subtracted in 200 components = 0.000967021 Jy
! Clean residual min=-0.006948 max=0.007092 Jy/beam
! Clean residual mean=0.000002 rms=0.001599 Jy/beam
! Combined flux in latest and established models = 0.826584 Jy
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 62 components and 0.826584 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.170317Jy  sigma=1.873342
! Fit after  self-cal, rms=0.170322Jy  sigma=1.873190
! Inverting map 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
selfcal true, true, soltime1
! Performing amp+phase self-cal over 120 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.170322Jy  sigma=1.873190
! Fit after  self-cal, rms=0.170097Jy  sigma=1.868449
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.709 mas, bmaj=2.164 mas, bpa=-6.955 degrees
! Estimated noise=0.833012 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00036117 Jy
! Component: 100  -  total flux cleaned = 0.000573777 Jy
! Component: 150  -  total flux cleaned = 0.000576183 Jy
! Component: 200  -  total flux cleaned = 0.000539913 Jy
! Total flux subtracted in 200 components = 0.000539913 Jy
! Clean residual min=-0.006511 max=0.006710 Jy/beam
! Clean residual mean=0.000006 rms=0.001560 Jy/beam
! Combined flux in latest and established models = 0.827123 Jy
selfcal
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 63 components and 0.827123 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.170064Jy  sigma=1.868074
! Fit after  self-cal, rms=0.170062Jy  sigma=1.867993
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (30.2, -35.4).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00223991 Jy
! Component: 100  -  total flux cleaned = 0.00196651 Jy
! Component: 150  -  total flux cleaned = 0.00141434 Jy
! Component: 200  -  total flux cleaned = 0.000950199 Jy
! Total flux subtracted in 200 components = 0.000950199 Jy
! Clean residual min=-0.005959 max=0.006288 Jy/beam
! Clean residual mean=0.000006 rms=0.001513 Jy/beam
! Combined flux in latest and established models = 0.828074 Jy
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 76 components and 0.828074 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.169775Jy  sigma=1.864937
! Fit after  self-cal, rms=0.169754Jy  sigma=1.864648
! Inverting map 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
selfcal true, true, soltime2
! Performing amp+phase self-cal over 20 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.169754Jy  sigma=1.864648
! Fit after  self-cal, rms=0.169159Jy  sigma=1.859765
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.7083 mas, bmaj=2.165 mas, bpa=-6.976 degrees
! Estimated noise=0.83238 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000960003 Jy
! Component: 100  -  total flux cleaned = 0.000799656 Jy
! Component: 150  -  total flux cleaned = 0.000870994 Jy
! Component: 200  -  total flux cleaned = 0.000801914 Jy
! Total flux subtracted in 200 components = 0.000801914 Jy
! Clean residual min=-0.006170 max=0.006116 Jy/beam
! Clean residual mean=0.000006 rms=0.001436 Jy/beam
! Combined flux in latest and established models = 0.828876 Jy
selfcal
! Performing phase self-cal
! Adding 22 model components to the UV plane model.
! The established model now contains 85 components and 0.828875 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.169081Jy  sigma=1.859007
! Fit after  self-cal, rms=0.169083Jy  sigma=1.858947
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 7.76192e-05 Jy
! Component: 100  -  total flux cleaned = -4.54813e-05 Jy
! Component: 150  -  total flux cleaned = -4.65315e-05 Jy
! Component: 200  -  total flux cleaned = -9.98313e-05 Jy
! Total flux subtracted in 200 components = -9.98313e-05 Jy
! Clean residual min=-0.006172 max=0.006113 Jy/beam
! Clean residual mean=0.000006 rms=0.001432 Jy/beam
! Combined flux in latest and established models = 0.828776 Jy
! Performing phase self-cal
! Adding 24 model components to the UV plane model.
! The established model now contains 90 components and 0.828776 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.169046Jy  sigma=1.858554
! Fit after  self-cal, rms=0.169045Jy  sigma=1.858540
! Inverting map 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
win_mult = win_mult * 1.2
selfcal true, true, soltime2
! Performing amp+phase self-cal over 20 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.169045Jy  sigma=1.858540
! Fit after  self-cal, rms=0.169016Jy  sigma=1.858473
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=2.661 mas, bmaj=3.597 mas, bpa=6.988 degrees
! Estimated noise=1.09958 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000584491 Jy
! Component: 100  -  total flux cleaned = 0.00020877 Jy
! Component: 150  -  total flux cleaned = 6.0989e-05 Jy
! Component: 200  -  total flux cleaned = 5.85371e-05 Jy
! Total flux subtracted in 200 components = 5.85371e-05 Jy
! Clean residual min=-0.006054 max=0.006529 Jy/beam
! Clean residual mean=0.000013 rms=0.001741 Jy/beam
! Combined flux in latest and established models = 0.828834 Jy
selfcal
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 94 components and 0.828834 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.169018Jy  sigma=1.858585
! Fit after  self-cal, rms=0.169000Jy  sigma=1.858442
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -9.71649e-05 Jy
! Component: 100  -  total flux cleaned = -0.000241915 Jy
! Component: 150  -  total flux cleaned = -0.000286581 Jy
! Component: 200  -  total flux cleaned = -0.000287688 Jy
! Total flux subtracted in 200 components = -0.000287688 Jy
! Clean residual min=-0.006061 max=0.006525 Jy/beam
! Clean residual mean=0.000013 rms=0.001737 Jy/beam
! Combined flux in latest and established models = 0.828546 Jy
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 99 components and 0.828546 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.169019Jy  sigma=1.858694
! Fit after  self-cal, rms=0.169004Jy  sigma=1.858566
! Inverting map 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
win_mult = win_mult / 1.2
print "============== Finished amplitude self-cal =============="
! ============== Finished amplitude self-cal ============== 
restore
! Inverting map and beam 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.708 mas, bmaj=2.164 mas, bpa=-6.98 degrees
! Estimated noise=0.832335 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.708 x 2.164 at -6.98 degrees (North through East)
! Clean map  min=-0.005452  max=0.64874 Jy/beam
if(peak(flux) > thresh)
  selfcal true, true
  clean clean_niter,clean_gain
  selfcal
  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
    new_peak = peak(flux)
    until(new_peak<=flux_cutoff)
  selfcal true, true
  end if
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.169004Jy  sigma=1.858566
! Fit after  self-cal, rms=0.156963Jy  sigma=1.669149
! Inverting map and beam 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.7069 mas, bmaj=2.164 mas, bpa=-6.948 degrees
! Estimated noise=0.832331 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000323015 Jy
! Component: 100  -  total flux cleaned = -0.000544512 Jy
! Component: 150  -  total flux cleaned = -0.000594002 Jy
! Component: 200  -  total flux cleaned = -0.000640509 Jy
! Total flux subtracted in 200 components = -0.000640509 Jy
! Clean residual min=-0.005412 max=0.006087 Jy/beam
! Clean residual mean=0.000005 rms=0.001369 Jy/beam
! Combined flux in latest and established models = 0.827906 Jy
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 105 components and 0.827906 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.156929Jy  sigma=1.668734
! Fit after  self-cal, rms=0.156935Jy  sigma=1.668713
! Inverting map 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Added new window around map position (39.2, -42.2).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00504748 Jy
! Component: 100  -  total flux cleaned = 0.00661575 Jy
! Component: 150  -  total flux cleaned = 0.00706858 Jy
! Component: 200  -  total flux cleaned = 0.00727596 Jy
! Total flux subtracted in 200 components = 0.00727596 Jy
! Clean residual min=-0.005360 max=0.005789 Jy/beam
! Clean residual mean=0.000004 rms=0.001334 Jy/beam
! Combined flux in latest and established models = 0.835182 Jy
! Performing phase self-cal
! Adding 21 model components to the UV plane model.
! The established model now contains 124 components and 0.835182 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.156742Jy  sigma=1.666767
! Fit after  self-cal, rms=0.156735Jy  sigma=1.666647
! Inverting map 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Added new window around map position (18.6, 16.4).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00279447 Jy
! Component: 100  -  total flux cleaned = 0.0030264 Jy
! Component: 150  -  total flux cleaned = 0.00336745 Jy
! Component: 200  -  total flux cleaned = 0.00367053 Jy
! Total flux subtracted in 200 components = 0.00367053 Jy
! Clean residual min=-0.005421 max=0.005471 Jy/beam
! Clean residual mean=0.000004 rms=0.001302 Jy/beam
! Combined flux in latest and established models = 0.838853 Jy
! Performing phase self-cal
! Adding 23 model components to the UV plane model.
! The established model now contains 140 components and 0.838853 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.156547Jy  sigma=1.664482
! Fit after  self-cal, rms=0.156544Jy  sigma=1.664384
! Inverting map 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Performing amp+phase self-cal
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.156544Jy  sigma=1.664384
! Fit after  self-cal, rms=0.156544Jy  sigma=1.664007
print "============== Clearing model and starting over =========="
! ============== Clearing model and starting over ========== 
clrmod true
! clrmod: Cleared the established and tentative models.
uvw 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.
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.6349 mas, bmaj=1.852 mas, bpa=-7.165 degrees
! Estimated noise=1.06934 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.489656 Jy
! Component: 100  -  total flux cleaned = 0.637171 Jy
! Component: 150  -  total flux cleaned = 0.706248 Jy
! Component: 200  -  total flux cleaned = 0.746503 Jy
! Total flux subtracted in 200 components = 0.746503 Jy
! Clean residual min=-0.009983 max=0.020775 Jy/beam
! Clean residual mean=-0.000015 rms=0.002625 Jy/beam
! Combined flux in latest and established models = 0.746503 Jy
uvw 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.
flux_cutoff = imstat(rms) * dynam
! Adding 19 model components to the UV plane model.
! The established model now contains 19 components and 0.746503 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.7076 mas, bmaj=2.163 mas, bpa=-6.943 degrees
! Estimated noise=0.831949 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  keep
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0362427 Jy
! Component: 100  -  total flux cleaned = 0.0551648 Jy
! Component: 150  -  total flux cleaned = 0.0663582 Jy
! Component: 200  -  total flux cleaned = 0.0727221 Jy
! Total flux subtracted in 200 components = 0.0727221 Jy
! Clean residual min=-0.006165 max=0.007222 Jy/beam
! Clean residual mean=-0.000002 rms=0.001530 Jy/beam
! Combined flux in latest and established models = 0.819225 Jy
! Adding 32 model components to the UV plane model.
! The established model now contains 41 components and 0.819225 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Added new window around map position (1, -0.4).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00577292 Jy
! Component: 100  -  total flux cleaned = 0.00899819 Jy
! Component: 150  -  total flux cleaned = 0.0117333 Jy
! Component: 200  -  total flux cleaned = 0.0138122 Jy
! Total flux subtracted in 200 components = 0.0138122 Jy
! Clean residual min=-0.005405 max=0.005562 Jy/beam
! Clean residual mean=0.000001 rms=0.001365 Jy/beam
! Combined flux in latest and established models = 0.833037 Jy
! Adding 29 model components to the UV plane model.
! The established model now contains 65 components and 0.833037 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths.
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=2.662 mas, bmaj=3.599 mas, bpa=7.009 degrees
! Estimated noise=1.09972 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00290059 Jy
! Component: 100  -  total flux cleaned = 0.00455625 Jy
! Component: 150  -  total flux cleaned = 0.00628048 Jy
! Component: 200  -  total flux cleaned = 0.00748454 Jy
! Total flux subtracted in 200 components = 0.00748454 Jy
! Clean residual min=-0.005377 max=0.005041 Jy/beam
! Clean residual mean=0.000008 rms=0.001503 Jy/beam
! Combined flux in latest and established models = 0.840522 Jy
flux_cutoff = imstat(rms) * dynam
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  keep
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00077481 Jy
! Component: 100  -  total flux cleaned = 0.00115474 Jy
! Component: 150  -  total flux cleaned = 0.00142844 Jy
! Component: 200  -  total flux cleaned = 0.00161695 Jy
! Total flux subtracted in 200 components = 0.00161695 Jy
! Clean residual min=-0.005315 max=0.004991 Jy/beam
! Clean residual mean=0.000009 rms=0.001478 Jy/beam
! Combined flux in latest and established models = 0.842139 Jy
! Adding 38 model components to the UV plane model.
! The established model now contains 96 components and 0.842138 Jy
! Inverting map 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! Estimated beam: bmin=0.7076 mas, bmaj=2.163 mas, bpa=-6.943 degrees
! Estimated noise=0.831949 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00168687 Jy
! Component: 100  -  total flux cleaned = 0.00128726 Jy
! Component: 150  -  total flux cleaned = 0.00128358 Jy
! Component: 200  -  total flux cleaned = 0.0012747 Jy
! Total flux subtracted in 200 components = 0.0012747 Jy
! Clean residual min=-0.005362 max=0.005173 Jy/beam
! Clean residual mean=0.000004 rms=0.001296 Jy/beam
! Combined flux in latest and established models = 0.843413 Jy
selfcal
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 107 components and 0.843413 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.156497Jy  sigma=1.664786
! Fit after  self-cal, rms=0.156476Jy  sigma=1.664391
wmodel J1354-0206_X_map.mod
! Writing 107 model components to file: J1354-0206_X_map.mod
wobs   J1354-0206_X_uvs.fits
! Writing UV FITS file: J1354-0206_X_uvs.fits
wwins  J1354-0206_X_map.win
! wwins: Wrote 5 windows to J1354-0206_X_map.win
x = (field_size-8) * field_cell / 4
addwin -x,x,-x,x
clean (field_size*4),0.01
! Inverting map 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! clean: niter=4096  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.000791848 Jy
! Component: 100  -  total flux cleaned = -0.00106912 Jy
! Component: 150  -  total flux cleaned = -0.00115824 Jy
! Component: 200  -  total flux cleaned = -0.0012465 Jy
! Component: 250  -  total flux cleaned = -0.000907877 Jy
! Component: 300  -  total flux cleaned = -0.000824404 Jy
! Component: 350  -  total flux cleaned = -0.000579963 Jy
! Component: 400  -  total flux cleaned = -0.000659776 Jy
! Component: 450  -  total flux cleaned = -0.00050223 Jy
! Component: 500  -  total flux cleaned = -0.00050153 Jy
! Component: 550  -  total flux cleaned = -0.000424659 Jy
! Component: 600  -  total flux cleaned = -0.00065039 Jy
! Component: 650  -  total flux cleaned = -0.000648336 Jy
! Component: 700  -  total flux cleaned = -0.000575832 Jy
! Component: 750  -  total flux cleaned = -0.000503406 Jy
! Component: 800  -  total flux cleaned = -0.000573349 Jy
! Component: 850  -  total flux cleaned = -0.000431018 Jy
! Component: 900  -  total flux cleaned = -0.000432473 Jy
! Component: 950  -  total flux cleaned = -0.000362655 Jy
! Component: 1000  -  total flux cleaned = -0.0002945 Jy
! Component: 1050  -  total flux cleaned = -9.16817e-05 Jy
! Component: 1100  -  total flux cleaned = -0.00022565 Jy
! Component: 1150  -  total flux cleaned = -0.000290894 Jy
! Component: 1200  -  total flux cleaned = -0.000159814 Jy
! Component: 1250  -  total flux cleaned = -0.000290066 Jy
! Component: 1300  -  total flux cleaned = -9.63035e-05 Jy
! Component: 1350  -  total flux cleaned = -0.00016194 Jy
! Component: 1400  -  total flux cleaned = -0.000351876 Jy
! Component: 1450  -  total flux cleaned = -0.00041524 Jy
! Component: 1500  -  total flux cleaned = -0.000416164 Jy
! Component: 1550  -  total flux cleaned = -0.000601898 Jy
! Component: 1600  -  total flux cleaned = -0.000662467 Jy
! Component: 1650  -  total flux cleaned = -0.000662505 Jy
! Component: 1700  -  total flux cleaned = -0.000722534 Jy
! Component: 1750  -  total flux cleaned = -0.000662687 Jy
! Component: 1800  -  total flux cleaned = -0.000722131 Jy
! Component: 1850  -  total flux cleaned = -0.000546049 Jy
! Component: 1900  -  total flux cleaned = -0.000896656 Jy
! Component: 1950  -  total flux cleaned = -0.0005479 Jy
! Component: 2000  -  total flux cleaned = -0.000606024 Jy
! Component: 2050  -  total flux cleaned = -0.000605803 Jy
! Component: 2100  -  total flux cleaned = -0.000548822 Jy
! Component: 2150  -  total flux cleaned = -0.000661698 Jy
! Component: 2200  -  total flux cleaned = -0.000718201 Jy
! Component: 2250  -  total flux cleaned = -0.000662089 Jy
! Component: 2300  -  total flux cleaned = -0.000773199 Jy
! Component: 2350  -  total flux cleaned = -0.000718339 Jy
! Component: 2400  -  total flux cleaned = -0.000718296 Jy
! Component: 2450  -  total flux cleaned = -0.000719014 Jy
! Component: 2500  -  total flux cleaned = -0.000665511 Jy
! Component: 2550  -  total flux cleaned = -0.000665681 Jy
! Component: 2600  -  total flux cleaned = -0.00077166 Jy
! Component: 2650  -  total flux cleaned = -0.000771919 Jy
! Component: 2700  -  total flux cleaned = -0.000877112 Jy
! Component: 2750  -  total flux cleaned = -0.000668369 Jy
! Component: 2800  -  total flux cleaned = -0.000616426 Jy
! Component: 2850  -  total flux cleaned = -0.000565276 Jy
! Component: 2900  -  total flux cleaned = -0.000359475 Jy
! Component: 2950  -  total flux cleaned = -0.000308774 Jy
! Component: 3000  -  total flux cleaned = -0.000308217 Jy
! Component: 3050  -  total flux cleaned = -0.000106136 Jy
! Component: 3100  -  total flux cleaned = 0.000144962 Jy
! Component: 3150  -  total flux cleaned = 0.000145266 Jy
! Component: 3200  -  total flux cleaned = 0.000194646 Jy
! Component: 3250  -  total flux cleaned = 0.000342661 Jy
! Component: 3300  -  total flux cleaned = 0.000539701 Jy
! Component: 3350  -  total flux cleaned = 0.000783467 Jy
! Component: 3400  -  total flux cleaned = 0.000832009 Jy
! Component: 3450  -  total flux cleaned = 0.000928522 Jy
! Component: 3500  -  total flux cleaned = 0.000976711 Jy
! Component: 3550  -  total flux cleaned = 0.00121601 Jy
! Component: 3600  -  total flux cleaned = 0.00126366 Jy
! Component: 3650  -  total flux cleaned = 0.00135853 Jy
! Component: 3700  -  total flux cleaned = 0.00135841 Jy
! Component: 3750  -  total flux cleaned = 0.00145166 Jy
! Component: 3800  -  total flux cleaned = 0.00163813 Jy
! Component: 3850  -  total flux cleaned = 0.00182334 Jy
! Component: 3900  -  total flux cleaned = 0.00173101 Jy
! Component: 3950  -  total flux cleaned = 0.00168541 Jy
! Component: 4000  -  total flux cleaned = 0.00200489 Jy
! Component: 4050  -  total flux cleaned = 0.00209542 Jy
! Total flux subtracted in 4096 components = 0.00223094 Jy
! Clean residual min=-0.002416 max=0.002499 Jy/beam
! Clean residual mean=0.000003 rms=0.000776 Jy/beam
! Combined flux in latest and established models = 0.845644 Jy
keep
! Adding 302 model components to the UV plane model.
! The established model now contains 409 components and 0.845644 Jy
![Exited script file: /opt64/bin/pima_mupet_01.dfm]
wmap   /scr/pima/rdv76_uvs/J1354-0206_X_map.fits
! Inverting map 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.7076 x 2.163 at -6.943 degrees (North through East)
! Clean map  min=-0.0053555  max=0.64882 Jy/beam
! Writing clean map to FITS file: /scr/pima/rdv76_uvs/J1354-0206_X_map.fits
wmodel /scr/pima/rdv76_uvs/J1354-0206_X_map.mod
! Writing 409 model components to file: /scr/pima/rdv76_uvs/J1354-0206_X_map.mod
wobs   /scr/pima/rdv76_uvs/J1354-0206_X_uvs.fits
! Writing UV FITS file: /scr/pima/rdv76_uvs/J1354-0206_X_uvs.fits
wwins  /scr/pima/rdv76_uvs/J1354-0206_X_map.win
! wwins: Wrote 6 windows to /scr/pima/rdv76_uvs/J1354-0206_X_map.win
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is", peak_flux
! The peak flux is 0.648819 
invert
! Inverting map 
! Your choice of large map pixels excluded 0.225% of the data.
!  The x-axis pixel size should ideally be below 0.1992 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000771824 
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.356875 0.356875 0.71375 1.4275 2.855 5.71 11.42 22.84 45.68 91.36
print "clev=      ", int(3*image_rms*10000)/10000
! clev=       0.0023 
print "peak=      ", int(1000*peak_flux)/1000
! peak=       0.648 
print "dyn_range= ", int(1000*peak_flux/image_rms)/1000
! dyn_range=  840.63 
quit
! Quitting program
! Log file /scr/pima/rdv76_uvs/J1354-0206_X_dfm.log closed on Fri Jun 15 03:54:50 2018