! Started logfile: /scr/pima/rdv76_uvs/J1624+5741_X_dfm.log on Fri Jun 15 03:55:39 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/J1624+5741_X_uva.fits
! Reading UV FITS file: /scr/pima/rdv76_uvs/J1624+5741_X_uva.fits
! AN table 1: 129 integrations on 55 of 55 possible baselines.
! AN table 2: 279 integrations on 78 of 78 possible baselines.
! Apparent sampling: 0.848598 visibilities/baseline/integration-bin.
! Found source: J1624+5741
! 
! 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 97952 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 J1624+5741_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 142 telescope corrections were flagged in sub-array 1.
!  A total of 521 telescope corrections were flagged in sub-array 2.
! 
! Correcting IF 2.
!  A total of 142 telescope corrections were flagged in sub-array 1.
!  A total of 521 telescope corrections were flagged in sub-array 2.
! 
! Correcting IF 3.
!  A total of 142 telescope corrections were flagged in sub-array 1.
!  A total of 521 telescope corrections were flagged in sub-array 2.
! 
! Correcting IF 4.
!  A total of 142 telescope corrections were flagged in sub-array 1.
!  A total of 521 telescope corrections were flagged in sub-array 2.
! 
! Fit before self-cal, rms=1.075486Jy  sigma=12.828568
! Fit after  self-cal, rms=0.683198Jy  sigma=8.050708
! 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 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 milli-arcsec
! Estimated beam: bmin=0.48 mas, bmaj=0.6256 mas, bpa=29.48 degrees
! Estimated noise=0.405433 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 = 0.256088 Jy
! Component: 100  -  total flux cleaned = 0.311932 Jy
! Total flux subtracted in 100 components = 0.311932 Jy
! Clean residual min=-0.008275 max=0.015618 Jy/beam
! Clean residual mean=0.000012 rms=0.001361 Jy/beam
! Combined flux in latest and established models = 0.311932 Jy
! Performing phase self-cal
! Adding 1 model components to the UV plane model.
! The established model now contains 1 components and 0.311932 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.195285Jy  sigma=2.090240
! Fit after  self-cal, rms=0.195283Jy  sigma=2.090217
! Inverting map 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 milli-arcsec
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0171199 Jy
! Component: 100  -  total flux cleaned = 0.0282373 Jy
! Total flux subtracted in 100 components = 0.0282373 Jy
! Clean residual min=-0.007796 max=0.014378 Jy/beam
! Clean residual mean=0.000010 rms=0.001265 Jy/beam
! Combined flux in latest and established models = 0.340169 Jy
! Performing phase self-cal
! Adding 13 model components to the UV plane model.
! The established model now contains 13 components and 0.340169 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.191713Jy  sigma=2.038282
! Fit after  self-cal, rms=0.191701Jy  sigma=2.038063
! Inverting map 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 milli-arcsec
! Added new window around map position (-2.6, -0.2).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0134389 Jy
! Component: 100  -  total flux cleaned = 0.0219386 Jy
! Total flux subtracted in 100 components = 0.0219386 Jy
! Clean residual min=-0.007226 max=0.013361 Jy/beam
! Clean residual mean=0.000009 rms=0.001205 Jy/beam
! Combined flux in latest and established models = 0.362108 Jy
! Performing phase self-cal
! Adding 15 model components to the UV plane model.
! The established model now contains 21 components and 0.362108 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.189739Jy  sigma=2.008667
! Fit after  self-cal, rms=0.189668Jy  sigma=2.007937
! Inverting map 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 milli-arcsec
! Added new window around map position (-1.2, 0).
! clean: niter=100  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0121989 Jy
! Component: 100  -  total flux cleaned = 0.0195712 Jy
! Total flux subtracted in 100 components = 0.0195712 Jy
! Clean residual min=-0.005799 max=0.007057 Jy/beam
! Clean residual mean=0.000007 rms=0.001142 Jy/beam
! Combined flux in latest and established models = 0.381679 Jy
! Performing phase self-cal
! Adding 10 model components to the UV plane model.
! The established model now contains 26 components and 0.381679 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.188121Jy  sigma=1.984787
! Fit after  self-cal, rms=0.188010Jy  sigma=1.983750
! Inverting map 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 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 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 milli-arcsec
! Estimated beam: bmin=0.6458 mas, bmaj=0.7893 mas, bpa=24.51 degrees
! Estimated noise=0.204203 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 = 0.0147903 Jy
! Component: 100  -  total flux cleaned = 0.0235136 Jy
! Component: 150  -  total flux cleaned = 0.0293459 Jy
! Component: 200  -  total flux cleaned = 0.0333554 Jy
! Total flux subtracted in 200 components = 0.0333554 Jy
! Clean residual min=-0.004555 max=0.009471 Jy/beam
! Clean residual mean=0.000024 rms=0.000981 Jy/beam
! Combined flux in latest and established models = 0.415034 Jy
! Performing phase self-cal
! Adding 36 model components to the UV plane model.
! The established model now contains 41 components and 0.415034 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.186901Jy  sigma=1.966775
! Fit after  self-cal, rms=0.186805Jy  sigma=1.965494
! Inverting map 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 milli-arcsec
! Added new window around map position (-4, -1.8).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00870373 Jy
! Component: 100  -  total flux cleaned = 0.0138675 Jy
! Component: 150  -  total flux cleaned = 0.0175579 Jy
! Component: 200  -  total flux cleaned = 0.0203121 Jy
! Total flux subtracted in 200 components = 0.0203121 Jy
! Clean residual min=-0.004878 max=0.004757 Jy/beam
! Clean residual mean=0.000017 rms=0.000809 Jy/beam
! Combined flux in latest and established models = 0.435346 Jy
! Performing phase self-cal
! Adding 23 model components to the UV plane model.
! The established model now contains 58 components and 0.435346 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.186412Jy  sigma=1.959420
! Fit after  self-cal, rms=0.186353Jy  sigma=1.958655
! Inverting map 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 milli-arcsec
print "============== Finished natural weighting clean =============="
! ============== Finished natural weighting clean ============== 
! 
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.6458 x 0.7893 at 24.51 degrees (North through East)
! Clean map  min=-0.0038622  max=0.33598 Jy/beam
gscale true
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00     FD        1.01     HN        1.04     KP        1.06     
!   LA        1.01     NL        0.99     NY        0.98     OV        1.00     
!   PT        1.02     SC        0.95     ZC        0.95     
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.02     FD        1.00     KK        1.01     KP        1.01     
!   LA        0.96     MK        1.04     NL        1.01     NY        1.00     
!   OV        1.00     PT        1.01     SC        1.01     WZ        1.02     
!   ZC        0.99     
! 
! 
! Correcting IF 2.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.99     FD        1.01     HN        0.97     KP        1.04     
!   LA        1.00     NL        0.97     NY        1.02     OV        1.02     
!   PT        1.02     SC        0.94     ZC        1.00     
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00     FD        1.02     KK        1.02     KP        1.00     
!   LA        0.96     MK        1.04     NL        1.01     NY        1.00     
!   OV        1.00     PT        1.02     SC        1.00     WZ        1.04     
!   ZC        1.00     
! 
! 
! Correcting IF 3.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.97     FD        1.00     HN        1.00     KP        1.06     
!   LA        1.03     NL        1.00     NY        0.95     OV        0.98     
!   PT        1.00     SC        0.96     ZC        0.99     
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        1.00     FD        1.01     KK        1.01     KP        1.00     
!   LA        0.94     MK        1.01     NL        1.01     NY        0.99     
!   OV        0.99     PT        1.00     SC        1.00     WZ        1.03     
!   ZC        1.00     
! 
! 
! Correcting IF 4.
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.95     FD        0.99     HN        1.00     KP        1.03     
!   LA        1.00     NL        0.96     NY        0.98     OV        1.01     
!   PT        1.00     SC        0.96     ZC        0.99     
! 
!  Telescope amplitude corrections in sub-array 2:
!   BR        0.97     FD        1.01     KK        1.02     KP        1.00     
!   LA        0.95     MK        1.01     NL        0.98     NY        0.97     
!   OV        0.99     PT        1.01     SC        1.01     WZ        1.02     
!   ZC        0.97     
! 
! 
! Fit before self-cal, rms=0.186353Jy  sigma=1.958655
! Fit after  self-cal, rms=0.186403Jy  sigma=1.953883
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 milli-arcsec
! Estimated beam: bmin=0.6457 mas, bmaj=0.7904 mas, bpa=24.67 degrees
! Estimated noise=0.204335 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 = 0.00398721 Jy
! Component: 100  -  total flux cleaned = 0.00564449 Jy
! Component: 150  -  total flux cleaned = 0.00632961 Jy
! Component: 200  -  total flux cleaned = 0.00659541 Jy
! Total flux subtracted in 200 components = 0.00659541 Jy
! Clean residual min=-0.004466 max=0.003355 Jy/beam
! Clean residual mean=0.000011 rms=0.000697 Jy/beam
! Combined flux in latest and established models = 0.441942 Jy
! Performing phase self-cal
! Adding 28 model components to the UV plane model.
! The established model now contains 69 components and 0.441942 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.186315Jy  sigma=1.952548
! Fit after  self-cal, rms=0.186313Jy  sigma=1.952347
! Inverting map 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 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=0.186313Jy  sigma=1.952347
! Fit after  self-cal, rms=0.186826Jy  sigma=1.943139
dynam = dynam - 0.75
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 milli-arcsec
! Estimated beam: bmin=0.6457 mas, bmaj=0.7908 mas, bpa=22.97 degrees
! Estimated noise=0.205108 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00144407 Jy
! Component: 100  -  total flux cleaned = 0.00170247 Jy
! Component: 150  -  total flux cleaned = 0.00187242 Jy
! Component: 200  -  total flux cleaned = 0.00190817 Jy
! Total flux subtracted in 200 components = 0.00190817 Jy
! Clean residual min=-0.002381 max=0.001860 Jy/beam
! Clean residual mean=-0.000010 rms=0.000457 Jy/beam
! Combined flux in latest and established models = 0.44385 Jy
selfcal
! Performing phase self-cal
! Adding 17 model components to the UV plane model.
! The established model now contains 76 components and 0.44385 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.186798Jy  sigma=1.942827
! Fit after  self-cal, rms=0.186803Jy  sigma=1.942792
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 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 = 0.000169813 Jy
! Component: 100  -  total flux cleaned = 0.000241334 Jy
! Component: 150  -  total flux cleaned = 0.000273343 Jy
! Component: 200  -  total flux cleaned = 0.000273203 Jy
! Total flux subtracted in 200 components = 0.000273203 Jy
! Clean residual min=-0.002347 max=0.001883 Jy/beam
! Clean residual mean=-0.000010 rms=0.000455 Jy/beam
! Combined flux in latest and established models = 0.444123 Jy
! Performing phase self-cal
! Adding 22 model components to the UV plane model.
! The established model now contains 82 components and 0.444123 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.186788Jy  sigma=1.942670
! Fit after  self-cal, rms=0.186787Jy  sigma=1.942652
! Inverting map 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 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=0.186787Jy  sigma=1.942652
! Fit after  self-cal, rms=0.186813Jy  sigma=1.942572
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 milli-arcsec
! Estimated beam: bmin=0.6453 mas, bmaj=0.7908 mas, bpa=22.59 degrees
! Estimated noise=0.205111 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.000542253 Jy
! Component: 100  -  total flux cleaned = 0.00060846 Jy
! Component: 150  -  total flux cleaned = 0.000637831 Jy
! Component: 200  -  total flux cleaned = 0.000665649 Jy
! Total flux subtracted in 200 components = 0.000665649 Jy
! Clean residual min=-0.002324 max=0.001821 Jy/beam
! Clean residual mean=-0.000011 rms=0.000450 Jy/beam
! Combined flux in latest and established models = 0.444789 Jy
selfcal
! Performing phase self-cal
! Adding 21 model components to the UV plane model.
! The established model now contains 84 components and 0.444789 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.186796Jy  sigma=1.942416
! Fit after  self-cal, rms=0.186798Jy  sigma=1.942411
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 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 = 9.2801e-05 Jy
! Component: 100  -  total flux cleaned = 0.000119491 Jy
! Component: 150  -  total flux cleaned = 0.000119877 Jy
! Component: 200  -  total flux cleaned = 0.000120159 Jy
! Total flux subtracted in 200 components = 0.000120159 Jy
! Clean residual min=-0.002310 max=0.001841 Jy/beam
! Clean residual mean=-0.000011 rms=0.000449 Jy/beam
! Combined flux in latest and established models = 0.444909 Jy
! Performing phase self-cal
! Adding 25 model components to the UV plane model.
! The established model now contains 86 components and 0.444909 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.186788Jy  sigma=1.942322
! Fit after  self-cal, rms=0.186787Jy  sigma=1.942317
! Inverting map 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 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=0.186787Jy  sigma=1.942317
! Fit after  self-cal, rms=0.186784Jy  sigma=1.942273
clean clean_niter,clean_gain
! Inverting map and beam 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 milli-arcsec
! Estimated beam: bmin=2.35 mas, bmaj=2.942 mas, bpa=-82.24 degrees
! Estimated noise=0.302796 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.0011276 Jy
! Component: 100  -  total flux cleaned = 0.00131425 Jy
! Component: 150  -  total flux cleaned = 0.00135762 Jy
! Component: 200  -  total flux cleaned = 0.00137705 Jy
! Total flux subtracted in 200 components = 0.00137705 Jy
! Clean residual min=-0.002637 max=0.002955 Jy/beam
! Clean residual mean=-0.000036 rms=0.000799 Jy/beam
! Combined flux in latest and established models = 0.446286 Jy
selfcal
! Performing phase self-cal
! Adding 7 model components to the UV plane model.
! The established model now contains 88 components and 0.446286 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.186787Jy  sigma=1.942295
! Fit after  self-cal, rms=0.186788Jy  sigma=1.942288
flux_cutoff = imstat(rms) * dynam
! Inverting map 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 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 = 0.000199121 Jy
! Component: 100  -  total flux cleaned = 0.000217555 Jy
! Component: 150  -  total flux cleaned = 0.000200909 Jy
! Component: 200  -  total flux cleaned = 0.000185675 Jy
! Total flux subtracted in 200 components = 0.000185675 Jy
! Clean residual min=-0.002634 max=0.002919 Jy/beam
! Clean residual mean=-0.000036 rms=0.000798 Jy/beam
! Combined flux in latest and established models = 0.446472 Jy
! Performing phase self-cal
! Adding 11 model components to the UV plane model.
! The established model now contains 90 components and 0.446472 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.186788Jy  sigma=1.942293
! Fit after  self-cal, rms=0.186788Jy  sigma=1.942286
! Inverting map 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 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 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 milli-arcsec
! Estimated beam: bmin=0.645 mas, bmaj=0.7908 mas, bpa=22.31 degrees
! Estimated noise=0.205096 mJy/beam.
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.645 x 0.7908 at 22.31 degrees (North through East)
! Clean map  min=-0.0018975  max=0.33603 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
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 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 milli-arcsec
! Estimated beam: bmin=0.4799 mas, bmaj=0.6258 mas, bpa=27.42 degrees
! Estimated noise=0.407593 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.257193 Jy
! Component: 100  -  total flux cleaned = 0.31344 Jy
! Component: 150  -  total flux cleaned = 0.335011 Jy
! Component: 200  -  total flux cleaned = 0.351021 Jy
! Total flux subtracted in 200 components = 0.351021 Jy
! Clean residual min=-0.004709 max=0.009233 Jy/beam
! Clean residual mean=0.000005 rms=0.001134 Jy/beam
! Combined flux in latest and established models = 0.351021 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 12 model components to the UV plane model.
! The established model now contains 12 components and 0.351021 Jy
! Inverting map and beam 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 milli-arcsec
! Estimated beam: bmin=0.645 mas, bmaj=0.7908 mas, bpa=22.31 degrees
! Estimated noise=0.205096 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 = 0.0271397 Jy
! Component: 100  -  total flux cleaned = 0.0437993 Jy
! Component: 150  -  total flux cleaned = 0.0555914 Jy
! Component: 200  -  total flux cleaned = 0.0643876 Jy
! Total flux subtracted in 200 components = 0.0643876 Jy
! Clean residual min=-0.002760 max=0.005467 Jy/beam
! Clean residual mean=0.000003 rms=0.000726 Jy/beam
! Combined flux in latest and established models = 0.415409 Jy
! Adding 39 model components to the UV plane model.
! The established model now contains 41 components and 0.415409 Jy
! Inverting map 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 milli-arcsec
! Added new window around map position (-2, 0.2).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00673612 Jy
! Component: 100  -  total flux cleaned = 0.011869 Jy
! Component: 150  -  total flux cleaned = 0.0158444 Jy
! Component: 200  -  total flux cleaned = 0.0189431 Jy
! Total flux subtracted in 200 components = 0.0189431 Jy
! Clean residual min=-0.002346 max=0.002697 Jy/beam
! Clean residual mean=-0.000006 rms=0.000492 Jy/beam
! Combined flux in latest and established models = 0.434352 Jy
! Adding 41 model components to the UV plane model.
! The established model now contains 66 components and 0.434352 Jy
! Inverting map 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 milli-arcsec
! Added new window around map position (-5.4, -2).
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00279583 Jy
! Component: 100  -  total flux cleaned = 0.00486573 Jy
! Component: 150  -  total flux cleaned = 0.00653923 Jy
! Component: 200  -  total flux cleaned = 0.00791297 Jy
! Total flux subtracted in 200 components = 0.00791297 Jy
! Clean residual min=-0.002342 max=0.001982 Jy/beam
! Clean residual mean=-0.000009 rms=0.000448 Jy/beam
! Combined flux in latest and established models = 0.442265 Jy
! Adding 38 model components to the UV plane model.
! The established model now contains 84 components and 0.442265 Jy
! Inverting map 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 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 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 milli-arcsec
! Estimated beam: bmin=2.35 mas, bmaj=2.942 mas, bpa=-82.24 degrees
! Estimated noise=0.302796 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = 0.00252204 Jy
! Component: 100  -  total flux cleaned = 0.00379529 Jy
! Component: 150  -  total flux cleaned = 0.00430425 Jy
! Component: 200  -  total flux cleaned = 0.00442989 Jy
! Total flux subtracted in 200 components = 0.00442989 Jy
! Clean residual min=-0.002734 max=0.002691 Jy/beam
! Clean residual mean=-0.000034 rms=0.000789 Jy/beam
! Combined flux in latest and established models = 0.446694 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 = 0.00010138 Jy
! Component: 100  -  total flux cleaned = 0.000157342 Jy
! Component: 150  -  total flux cleaned = 0.000169757 Jy
! Component: 200  -  total flux cleaned = 0.000181752 Jy
! Total flux subtracted in 200 components = 0.000181752 Jy
! Clean residual min=-0.002732 max=0.002696 Jy/beam
! Clean residual mean=-0.000035 rms=0.000788 Jy/beam
! Combined flux in latest and established models = 0.446876 Jy
! Adding 24 model components to the UV plane model.
! The established model now contains 97 components and 0.446876 Jy
! Inverting map 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 milli-arcsec
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 milli-arcsec
! Estimated beam: bmin=0.645 mas, bmaj=0.7908 mas, bpa=22.31 degrees
! Estimated noise=0.205096 mJy/beam.
! clean: niter=200  gain=0.03  cutoff=0
! Component: 050  -  total flux cleaned = -0.000540907 Jy
! Component: 100  -  total flux cleaned = -0.000311804 Jy
! Component: 150  -  total flux cleaned = -0.00026033 Jy
! Component: 200  -  total flux cleaned = -0.000188418 Jy
! Total flux subtracted in 200 components = -0.000188418 Jy
! Clean residual min=-0.002368 max=0.001851 Jy/beam
! Clean residual mean=-0.000011 rms=0.000441 Jy/beam
! Combined flux in latest and established models = 0.446688 Jy
selfcal
! Performing phase self-cal
! Adding 18 model components to the UV plane model.
! The established model now contains 104 components and 0.446688 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.186767Jy  sigma=1.942094
! Fit after  self-cal, rms=0.186750Jy  sigma=1.941909
wmodel J1624+5741_X_map.mod
! Writing 104 model components to file: J1624+5741_X_map.mod
wobs   J1624+5741_X_uvs.fits
! Writing UV FITS file: J1624+5741_X_uvs.fits
wwins  J1624+5741_X_map.win
! wwins: Wrote 6 windows to J1624+5741_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 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 milli-arcsec
! clean: niter=4096  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = -0.000995452 Jy
! Component: 100  -  total flux cleaned = -0.00170051 Jy
! Component: 150  -  total flux cleaned = -0.00230166 Jy
! Component: 200  -  total flux cleaned = -0.00275535 Jy
! Component: 250  -  total flux cleaned = -0.00307173 Jy
! Component: 300  -  total flux cleaned = -0.00331965 Jy
! Component: 350  -  total flux cleaned = -0.00344189 Jy
! Component: 400  -  total flux cleaned = -0.0036522 Jy
! Component: 450  -  total flux cleaned = -0.00382983 Jy
! Component: 500  -  total flux cleaned = -0.00394651 Jy
! Component: 550  -  total flux cleaned = -0.00391815 Jy
! Component: 600  -  total flux cleaned = -0.00397535 Jy
! Component: 650  -  total flux cleaned = -0.00403143 Jy
! Component: 700  -  total flux cleaned = -0.00405926 Jy
! Component: 750  -  total flux cleaned = -0.00405966 Jy
! Component: 800  -  total flux cleaned = -0.00411433 Jy
! Component: 850  -  total flux cleaned = -0.00419584 Jy
! Component: 900  -  total flux cleaned = -0.00422279 Jy
! Component: 950  -  total flux cleaned = -0.00424909 Jy
! Component: 1000  -  total flux cleaned = -0.00419579 Jy
! Component: 1050  -  total flux cleaned = -0.00424848 Jy
! Component: 1100  -  total flux cleaned = -0.00422211 Jy
! Component: 1150  -  total flux cleaned = -0.00411809 Jy
! Component: 1200  -  total flux cleaned = -0.00416997 Jy
! Component: 1250  -  total flux cleaned = -0.00414445 Jy
! Component: 1300  -  total flux cleaned = -0.00422132 Jy
! Component: 1350  -  total flux cleaned = -0.00422125 Jy
! Component: 1400  -  total flux cleaned = -0.00419605 Jy
! Component: 1450  -  total flux cleaned = -0.00414579 Jy
! Component: 1500  -  total flux cleaned = -0.00422089 Jy
! Component: 1550  -  total flux cleaned = -0.00429551 Jy
! Component: 1600  -  total flux cleaned = -0.00414654 Jy
! Component: 1650  -  total flux cleaned = -0.00419591 Jy
! Component: 1700  -  total flux cleaned = -0.004147 Jy
! Component: 1750  -  total flux cleaned = -0.00412266 Jy
! Component: 1800  -  total flux cleaned = -0.00414703 Jy
! Component: 1850  -  total flux cleaned = -0.00414701 Jy
! Component: 1900  -  total flux cleaned = -0.00414724 Jy
! Component: 1950  -  total flux cleaned = -0.00412337 Jy
! Component: 2000  -  total flux cleaned = -0.00409948 Jy
! Component: 2050  -  total flux cleaned = -0.00405195 Jy
! Component: 2100  -  total flux cleaned = -0.00405198 Jy
! Component: 2150  -  total flux cleaned = -0.00405197 Jy
! Component: 2200  -  total flux cleaned = -0.00407536 Jy
! Component: 2250  -  total flux cleaned = -0.00416869 Jy
! Component: 2300  -  total flux cleaned = -0.00414536 Jy
! Component: 2350  -  total flux cleaned = -0.00414526 Jy
! Component: 2400  -  total flux cleaned = -0.00414513 Jy
! Component: 2450  -  total flux cleaned = -0.00409904 Jy
! Component: 2500  -  total flux cleaned = -0.00414491 Jy
! Component: 2550  -  total flux cleaned = -0.00421352 Jy
! Component: 2600  -  total flux cleaned = -0.00419074 Jy
! Component: 2650  -  total flux cleaned = -0.00410002 Jy
! Component: 2700  -  total flux cleaned = -0.00410011 Jy
! Component: 2750  -  total flux cleaned = -0.00419023 Jy
! Component: 2800  -  total flux cleaned = -0.00416759 Jy
! Component: 2850  -  total flux cleaned = -0.00421231 Jy
! Component: 2900  -  total flux cleaned = -0.00418996 Jy
! Component: 2950  -  total flux cleaned = -0.00418999 Jy
! Component: 3000  -  total flux cleaned = -0.00419001 Jy
! Component: 3050  -  total flux cleaned = -0.00421216 Jy
! Component: 3100  -  total flux cleaned = -0.00421209 Jy
! Component: 3150  -  total flux cleaned = -0.00416816 Jy
! Component: 3200  -  total flux cleaned = -0.0040369 Jy
! Component: 3250  -  total flux cleaned = -0.00421141 Jy
! Component: 3300  -  total flux cleaned = -0.00425505 Jy
! Component: 3350  -  total flux cleaned = -0.00419005 Jy
! Component: 3400  -  total flux cleaned = -0.00412526 Jy
! Component: 3450  -  total flux cleaned = -0.00410371 Jy
! Component: 3500  -  total flux cleaned = -0.00418977 Jy
! Component: 3550  -  total flux cleaned = -0.00416841 Jy
! Component: 3600  -  total flux cleaned = -0.00414715 Jy
! Component: 3650  -  total flux cleaned = -0.00416839 Jy
! Component: 3700  -  total flux cleaned = -0.00412605 Jy
! Component: 3750  -  total flux cleaned = -0.00418955 Jy
! Component: 3800  -  total flux cleaned = -0.00421073 Jy
! Component: 3850  -  total flux cleaned = -0.00414772 Jy
! Component: 3900  -  total flux cleaned = -0.00412679 Jy
! Component: 3950  -  total flux cleaned = -0.00408502 Jy
! Component: 4000  -  total flux cleaned = -0.00400161 Jy
! Component: 4050  -  total flux cleaned = -0.00408484 Jy
! Total flux subtracted in 4096 components = -0.00412635 Jy
! Clean residual min=-0.001320 max=0.001217 Jy/beam
! Clean residual mean=-0.000007 rms=0.000341 Jy/beam
! Combined flux in latest and established models = 0.442561 Jy
keep
! Adding 390 model components to the UV plane model.
! The established model now contains 494 components and 0.442562 Jy
![Exited script file: /opt64/bin/pima_mupet_01.dfm]
wmap   /scr/pima/rdv76_uvs/J1624+5741_X_map.fits
! Inverting map 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 milli-arcsec
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 0.645 x 0.7908 at 22.31 degrees (North through East)
! Clean map  min=-0.0016149  max=0.33606 Jy/beam
! Writing clean map to FITS file: /scr/pima/rdv76_uvs/J1624+5741_X_map.fits
wmodel /scr/pima/rdv76_uvs/J1624+5741_X_map.mod
! Writing 494 model components to file: /scr/pima/rdv76_uvs/J1624+5741_X_map.mod
wobs   /scr/pima/rdv76_uvs/J1624+5741_X_uvs.fits
! Writing UV FITS file: /scr/pima/rdv76_uvs/J1624+5741_X_uvs.fits
wwins  /scr/pima/rdv76_uvs/J1624+5741_X_map.win
! wwins: Wrote 7 windows to /scr/pima/rdv76_uvs/J1624+5741_X_map.win
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is", peak_flux
! The peak flux is 0.336057 
invert
! Inverting map 
! Your choice of large map pixels excluded 5.86% of the data.
!  The x-axis pixel size should ideally be below 0.1651 milli-arcsec
!  The y-axis pixel size should ideally be below 0.1719 milli-arcsec
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000341112 
loglevs 100*3*image_rms/peak_flux
! The new contour levels are:
!  -0.304512 0.304512 0.609025 1.21805 2.4361 4.8722 9.74439 19.4888 38.9776 77.9551
print "clev=      ", int(3*image_rms*10000)/10000
! clev=       0.001 
print "peak=      ", int(1000*peak_flux)/1000
! peak=       0.336 
print "dyn_range= ", int(1000*peak_flux/image_rms)/1000
! dyn_range=  985.181 
quit
! Quitting program
! Log file /scr/pima/rdv76_uvs/J1624+5741_X_dfm.log closed on Fri Jun 15 03:55:48 2018