! Started logfile: /scr/pima/rv118_uvs/J1104+3812_X_dfm.log on Sun Dec 10 00:09:09 2017 float field_size field_size = 1024 float field_cell field_cell = 0.2000 float taper_size taper_size = 70.0 float freq freq = 8.36575 obs /scr/pima/rv118_uvs/J1104+3812_X_uva.fits ! Reading UV FITS file: /scr/pima/rv118_uvs/J1104+3812_X_uva.fits ! AN table 1: 4 integrations on 28 of 28 possible baselines. ! AN table 2: 56 integrations on 45 of 45 possible baselines. ! AN table 3: 15 integrations on 6 of 6 possible baselines. ! AN table 4: 29 integrations on 6 of 6 possible baselines. ! AN table 5: 103 integrations on 10 of 10 possible baselines. ! AN table 6: 17 integrations on 3 of 3 possible baselines. ! AN table 7: 34 integrations on 45 of 45 possible baselines. ! AN table 8: 16 integrations on 36 of 36 possible baselines. ! Apparent sampling: 0.434654 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1104+3812 ! ! 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 8.36575e+09 8e+06 1 8e+06 ! 02 2 8.44575e+09 8e+06 1 8e+06 ! 03 3 8.80575e+09 8e+06 1 8e+06 ! 04 4 8.92575e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 79 lines of history. ! ! Reading 10576 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 J1104+3812_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 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 272 telescope corrections were flagged in sub-array 2. ! A total of 22 telescope corrections were flagged in sub-array 3. ! A total of 50 telescope corrections were flagged in sub-array 4. ! A total of 241 telescope corrections were flagged in sub-array 5. ! A total of 15 telescope corrections were flagged in sub-array 6. ! A total of 206 telescope corrections were flagged in sub-array 7. ! A total of 66 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 2. ! A total of 272 telescope corrections were flagged in sub-array 2. ! A total of 22 telescope corrections were flagged in sub-array 3. ! A total of 50 telescope corrections were flagged in sub-array 4. ! A total of 241 telescope corrections were flagged in sub-array 5. ! A total of 15 telescope corrections were flagged in sub-array 6. ! A total of 206 telescope corrections were flagged in sub-array 7. ! A total of 66 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 3. ! A total of 272 telescope corrections were flagged in sub-array 2. ! A total of 22 telescope corrections were flagged in sub-array 3. ! A total of 50 telescope corrections were flagged in sub-array 4. ! A total of 241 telescope corrections were flagged in sub-array 5. ! A total of 15 telescope corrections were flagged in sub-array 6. ! A total of 206 telescope corrections were flagged in sub-array 7. ! A total of 66 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 4. ! A total of 272 telescope corrections were flagged in sub-array 2. ! A total of 22 telescope corrections were flagged in sub-array 3. ! A total of 50 telescope corrections were flagged in sub-array 4. ! A total of 241 telescope corrections were flagged in sub-array 5. ! A total of 15 telescope corrections were flagged in sub-array 6. ! A total of 206 telescope corrections were flagged in sub-array 7. ! A total of 66 telescope corrections were flagged in sub-array 8. ! ! Fit before self-cal, rms=1.048126Jy sigma=15.476444 ! Fit after self-cal, rms=0.693184Jy sigma=9.966842 ! 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 6.04% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1617 milli-arcsec ! Estimated beam: bmin=0.7367 mas, bmaj=0.9059 mas, bpa=35.85 degrees ! Estimated noise=0.843723 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 = 0.241352 Jy ! Component: 100 - total flux cleaned = 0.300708 Jy ! Total flux subtracted in 100 components = 0.300708 Jy ! Clean residual min=-0.007318 max=0.023117 Jy/beam ! Clean residual mean=0.000015 rms=0.001537 Jy/beam ! Combined flux in latest and established models = 0.300708 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.300708 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.094910Jy sigma=1.218070 ! Fit after self-cal, rms=0.094881Jy sigma=1.217192 ! Inverting map ! Your choice of large map pixels excluded 6.04% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1617 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0243292 Jy ! Component: 100 - total flux cleaned = 0.0366136 Jy ! Total flux subtracted in 100 components = 0.0366136 Jy ! Clean residual min=-0.005431 max=0.013077 Jy/beam ! Clean residual mean=0.000006 rms=0.001179 Jy/beam ! Combined flux in latest and established models = 0.337321 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 16 components and 0.337321 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.087630Jy sigma=1.031848 ! Fit after self-cal, rms=0.087553Jy sigma=1.031059 ! Inverting map ! Your choice of large map pixels excluded 6.04% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1617 milli-arcsec ! Added new window around map position (-1, 1). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0121694 Jy ! Component: 100 - total flux cleaned = 0.0182317 Jy ! Total flux subtracted in 100 components = 0.0182317 Jy ! Clean residual min=-0.004945 max=0.007754 Jy/beam ! Clean residual mean=0.000002 rms=0.001080 Jy/beam ! Combined flux in latest and established models = 0.355553 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 25 components and 0.355553 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.085621Jy sigma=0.988080 ! Fit after self-cal, rms=0.085288Jy sigma=0.982351 ! Inverting map ! Your choice of large map pixels excluded 6.04% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1617 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00616876 Jy ! Component: 100 - total flux cleaned = 0.00754722 Jy ! Total flux subtracted in 100 components = 0.00754722 Jy ! Clean residual min=-0.004826 max=0.005136 Jy/beam ! Clean residual mean=0.000000 rms=0.001028 Jy/beam ! Combined flux in latest and established models = 0.3631 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 27 components and 0.3631 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.084797Jy sigma=0.972509 ! Fit after self-cal, rms=0.084697Jy sigma=0.970890 ! Inverting map ! Your choice of large map pixels excluded 6.04% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1617 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 6.04% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1617 milli-arcsec ! Estimated beam: bmin=0.9294 mas, bmaj=1.12 mas, bpa=41.08 degrees ! Estimated noise=0.529782 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 (-1, 3). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00628045 Jy ! Component: 100 - total flux cleaned = 0.00982037 Jy ! Component: 150 - total flux cleaned = 0.0114273 Jy ! Component: 200 - total flux cleaned = 0.0118468 Jy ! Total flux subtracted in 200 components = 0.0118468 Jy ! Clean residual min=-0.004245 max=0.004269 Jy/beam ! Clean residual mean=-0.000041 rms=0.000871 Jy/beam ! Combined flux in latest and established models = 0.374947 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 42 components and 0.374947 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.084231Jy sigma=0.960805 ! Fit after self-cal, rms=0.084168Jy sigma=0.959536 ! Inverting map ! Your choice of large map pixels excluded 6.04% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1617 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9294 x 1.12 at 41.08 degrees (North through East) ! Clean map min=-0.0038629 max=0.30629 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 0.99 KP 0.97 LA 0.97 ! NL 0.97 NY 1.00 OV 1.00 PT 0.96 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 FD 1.02 HN 1.04 KK 1.04 ! KP 1.01 LA 0.99 NL 0.95 ON 1.08 ! OV 1.00 PT 0.98 ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.94 KK 0.87 NY 1.00 OV 1.05 ! ! A total of 18 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! KK 1.08 NY 1.00 ON 0.96 WZ 1.01 ! ! A total of 144 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! HH 0.92 HN 1.29 NY 1.04 ON 1.00 ! WZ 0.92 ! ! A total of 36 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! HH 0.00* NL 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.07 FD 1.01 HH 0.89 HN 1.03 ! LA 0.99 NL 0.99 NY 1.01 PT 1.05 ! SC 0.97 WZ 0.93 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.02 FD 0.96 HN 1.02 KP 1.02 ! LA 1.02 NL 0.98 NY 0.95 PT 1.06 ! SC 0.97 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.97 KP 0.97 LA 1.00 ! NL 0.99 NY 1.08 OV 0.99 PT 0.95 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 1.02 HN 1.02 KK 1.03 ! KP 1.01 LA 0.99 NL 0.96 ON 1.04 ! OV 1.00 PT 0.97 ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 KK 1.04 NY 0.91 OV 1.06 ! ! A total of 18 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! KK 0.96 NY 1.07 ON 1.18 WZ 0.92 ! ! A total of 144 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! HH 1.03 HN 1.35 NY 1.02 ON 1.03 ! WZ 0.94 ! ! A total of 36 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! HH 0.00* NL 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.02 FD 1.02 HH 0.93 HN 1.01 ! LA 0.98 NL 1.00 NY 0.98 PT 1.04 ! SC 0.99 WZ 0.96 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.02 FD 1.00 HN 1.03 KP 1.02 ! LA 1.00 NL 0.96 NY 0.97 PT 1.04 ! SC 0.96 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 1.02 KP 0.98 LA 1.04 ! NL 0.97 NY 1.03 OV 0.95 PT 0.95 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 1.03 HN 1.03 KK 1.06 ! KP 0.98 LA 0.99 NL 0.95 ON 1.11 ! OV 1.02 PT 0.97 ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.09 KK 0.99 NY 1.07 OV 1.02 ! ! A total of 18 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! KK 1.14 NY 0.96 ON 1.05 WZ 1.09 ! ! A total of 144 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! HH 0.94 HN 1.51 NY 1.01 ON 0.99 ! WZ 0.97 ! ! A total of 36 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! HH 0.00* NL 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.01 FD 1.00 HH 0.90 HN 1.03 ! LA 0.98 NL 1.01 NY 1.02 PT 1.06 ! SC 0.98 WZ 0.96 ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.01 FD 1.00 HN 1.03 KP 1.05 ! LA 0.99 NL 0.97 NY 0.96 PT 1.06 ! SC 1.04 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 1.03 KP 1.01 LA 0.98 ! NL 0.96 NY 1.06 OV 0.98 PT 0.98 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 1.03 HN 1.00 KK 1.03 ! KP 0.98 LA 1.00 NL 0.94 ON 1.06 ! OV 1.00 PT 0.97 ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 KK 1.04 NY 0.95 OV 1.00 ! ! A total of 18 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! KK 0.98 NY 1.07 ON 1.00 WZ 1.04 ! ! A total of 144 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! HH 0.94 HN 1.39 NY 1.07 ON 1.01 ! WZ 0.96 ! ! A total of 36 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! HH 0.00* NL 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.04 FD 1.02 HH 0.96 HN 1.04 ! LA 1.00 NL 1.00 NY 1.00 PT 1.07 ! SC 0.94 WZ 0.92 ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.97 FD 0.95 HN 0.98 KP 1.04 ! LA 1.01 NL 1.00 NY 0.90 PT 1.04 ! SC 1.01 ! ! ! Fit before self-cal, rms=0.084168Jy sigma=0.959536 ! Fit after self-cal, rms=0.081953Jy sigma=0.945983 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1655 milli-arcsec ! Estimated beam: bmin=0.9249 mas, bmaj=1.143 mas, bpa=38.84 degrees ! Estimated noise=0.534401 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 = 0.000923482 Jy ! Component: 100 - total flux cleaned = 0.00123108 Jy ! Component: 150 - total flux cleaned = 0.00142493 Jy ! Component: 200 - total flux cleaned = 0.00146733 Jy ! Total flux subtracted in 200 components = 0.00146733 Jy ! Clean residual min=-0.003292 max=0.003454 Jy/beam ! Clean residual mean=-0.000002 rms=0.000727 Jy/beam ! Combined flux in latest and established models = 0.376414 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 51 components and 0.376414 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081851Jy sigma=0.944592 ! Fit after self-cal, rms=0.081952Jy sigma=0.944292 ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1655 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=0.081952Jy sigma=0.944292 ! Fit after self-cal, rms=0.081671Jy sigma=0.934274 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1655 milli-arcsec ! Estimated beam: bmin=0.9269 mas, bmaj=1.143 mas, bpa=38.78 degrees ! Estimated noise=0.533745 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000818972 Jy ! Component: 100 - total flux cleaned = -0.000777082 Jy ! Component: 150 - total flux cleaned = -0.000695533 Jy ! Component: 200 - total flux cleaned = -0.000658687 Jy ! Total flux subtracted in 200 components = -0.000658687 Jy ! Clean residual min=-0.002804 max=0.003107 Jy/beam ! Clean residual mean=-0.000003 rms=0.000631 Jy/beam ! Combined flux in latest and established models = 0.375756 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 58 components and 0.375756 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081603Jy sigma=0.933468 ! Fit after self-cal, rms=0.081599Jy sigma=0.933327 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1655 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 (-6, 9.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00291809 Jy ! Component: 100 - total flux cleaned = 0.00363117 Jy ! Component: 150 - total flux cleaned = 0.0038283 Jy ! Component: 200 - total flux cleaned = 0.00400483 Jy ! Total flux subtracted in 200 components = 0.00400483 Jy ! Clean residual min=-0.002819 max=0.002795 Jy/beam ! Clean residual mean=-0.000015 rms=0.000603 Jy/beam ! Combined flux in latest and established models = 0.37976 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 69 components and 0.37976 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081488Jy sigma=0.931263 ! Fit after self-cal, rms=0.081477Jy sigma=0.931017 ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1655 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=0.081477Jy sigma=0.931017 ! Fit after self-cal, rms=0.080830Jy sigma=0.918317 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1655 milli-arcsec ! Estimated beam: bmin=0.9268 mas, bmaj=1.143 mas, bpa=38.74 degrees ! Estimated noise=0.532833 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000189993 Jy ! Component: 100 - total flux cleaned = 0.00041171 Jy ! Component: 150 - total flux cleaned = 0.000568135 Jy ! Component: 200 - total flux cleaned = 0.00067521 Jy ! Total flux subtracted in 200 components = 0.00067521 Jy ! Clean residual min=-0.002460 max=0.001891 Jy/beam ! Clean residual mean=-0.000016 rms=0.000473 Jy/beam ! Combined flux in latest and established models = 0.380436 Jy selfcal ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 81 components and 0.380436 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.080785Jy sigma=0.917693 ! Fit after self-cal, rms=0.080777Jy sigma=0.917615 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1655 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 = 9.07301e-05 Jy ! Component: 100 - total flux cleaned = 0.000194764 Jy ! Component: 150 - total flux cleaned = 0.000259224 Jy ! Component: 200 - total flux cleaned = 0.000320432 Jy ! Total flux subtracted in 200 components = 0.000320432 Jy ! Clean residual min=-0.002447 max=0.001889 Jy/beam ! Clean residual mean=-0.000017 rms=0.000470 Jy/beam ! Combined flux in latest and established models = 0.380756 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 85 components and 0.380756 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.080747Jy sigma=0.917270 ! Fit after self-cal, rms=0.080738Jy sigma=0.917227 ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1655 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=0.080738Jy sigma=0.917227 ! Fit after self-cal, rms=0.080679Jy sigma=0.917154 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1655 milli-arcsec ! Estimated beam: bmin=2.605 mas, bmaj=3.023 mas, bpa=-86.14 degrees ! Estimated noise=0.608597 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000773192 Jy ! Component: 100 - total flux cleaned = 0.000843597 Jy ! Component: 150 - total flux cleaned = 0.000897782 Jy ! Component: 200 - total flux cleaned = 0.000912329 Jy ! Total flux subtracted in 200 components = 0.000912329 Jy ! Clean residual min=-0.002351 max=0.001836 Jy/beam ! Clean residual mean=-0.000037 rms=0.000529 Jy/beam ! Combined flux in latest and established models = 0.381668 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 92 components and 0.381668 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.080675Jy sigma=0.917049 ! Fit after self-cal, rms=0.080674Jy sigma=0.917019 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1655 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 = 0.000116154 Jy ! Component: 100 - total flux cleaned = 0.000129606 Jy ! Component: 150 - total flux cleaned = 0.000167758 Jy ! Component: 200 - total flux cleaned = 0.000191105 Jy ! Total flux subtracted in 200 components = 0.000191105 Jy ! Clean residual min=-0.002336 max=0.001837 Jy/beam ! Clean residual mean=-0.000038 rms=0.000527 Jy/beam ! Combined flux in latest and established models = 0.381859 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 96 components and 0.381859 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.080675Jy sigma=0.916976 ! Fit after self-cal, rms=0.080674Jy sigma=0.916971 ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1655 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 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1655 milli-arcsec ! Estimated beam: bmin=0.927 mas, bmaj=1.143 mas, bpa=38.71 degrees ! Estimated noise=0.532277 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.927 x 1.143 at 38.71 degrees (North through East) ! Clean map min=-0.0020237 max=0.3043 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 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1655 milli-arcsec ! Estimated beam: bmin=0.7314 mas, bmaj=0.9046 mas, bpa=35 degrees ! Estimated noise=0.85077 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.238561 Jy ! Component: 100 - total flux cleaned = 0.299445 Jy ! Component: 150 - total flux cleaned = 0.325245 Jy ! Component: 200 - total flux cleaned = 0.339578 Jy ! Total flux subtracted in 200 components = 0.339578 Jy ! Clean residual min=-0.003954 max=0.007267 Jy/beam ! Clean residual mean=0.000013 rms=0.000928 Jy/beam ! Combined flux in latest and established models = 0.339578 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 18 model components to the UV plane model. ! The established model now contains 18 components and 0.339578 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1655 milli-arcsec ! Estimated beam: bmin=0.927 mas, bmaj=1.143 mas, bpa=38.71 degrees ! Estimated noise=0.532277 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 = 0.0132633 Jy ! Component: 100 - total flux cleaned = 0.0208091 Jy ! Component: 150 - total flux cleaned = 0.0259537 Jy ! Component: 200 - total flux cleaned = 0.029836 Jy ! Total flux subtracted in 200 components = 0.029836 Jy ! Clean residual min=-0.002494 max=0.002643 Jy/beam ! Clean residual mean=0.000008 rms=0.000545 Jy/beam ! Combined flux in latest and established models = 0.369414 Jy ! Adding 41 model components to the UV plane model. ! The established model now contains 51 components and 0.369414 Jy ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1655 milli-arcsec ! Added new window around map position (-2.8, 4.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00307486 Jy ! Component: 100 - total flux cleaned = 0.00546909 Jy ! Component: 150 - total flux cleaned = 0.00681321 Jy ! Component: 200 - total flux cleaned = 0.00782896 Jy ! Total flux subtracted in 200 components = 0.00782896 Jy ! Clean residual min=-0.002350 max=0.001928 Jy/beam ! Clean residual mean=-0.000008 rms=0.000484 Jy/beam ! Combined flux in latest and established models = 0.377243 Jy ! Adding 35 model components to the UV plane model. ! The established model now contains 68 components and 0.377243 Jy ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1655 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 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1655 milli-arcsec ! Estimated beam: bmin=2.605 mas, bmaj=3.023 mas, bpa=-86.14 degrees ! Estimated noise=0.608597 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0018513 Jy ! Component: 100 - total flux cleaned = 0.00297608 Jy ! Component: 150 - total flux cleaned = 0.00352036 Jy ! Component: 200 - total flux cleaned = 0.00392434 Jy ! Total flux subtracted in 200 components = 0.00392434 Jy ! Clean residual min=-0.002335 max=0.001807 Jy/beam ! Clean residual mean=-0.000034 rms=0.000527 Jy/beam ! Combined flux in latest and established models = 0.381167 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 = 0.000333425 Jy ! Component: 100 - total flux cleaned = 0.000631588 Jy ! Component: 150 - total flux cleaned = 0.0008614 Jy ! Component: 200 - total flux cleaned = 0.00104012 Jy ! Total flux subtracted in 200 components = 0.00104012 Jy ! Clean residual min=-0.002322 max=0.001817 Jy/beam ! Clean residual mean=-0.000039 rms=0.000519 Jy/beam ! Combined flux in latest and established models = 0.382207 Jy ! Adding 36 model components to the UV plane model. ! The established model now contains 94 components and 0.382207 Jy ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1655 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1655 milli-arcsec ! Estimated beam: bmin=0.927 mas, bmaj=1.143 mas, bpa=38.71 degrees ! Estimated noise=0.532277 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000586935 Jy ! Component: 100 - total flux cleaned = -0.00075103 Jy ! Component: 150 - total flux cleaned = -0.000826645 Jy ! Component: 200 - total flux cleaned = -0.000862922 Jy ! Total flux subtracted in 200 components = -0.000862922 Jy ! Clean residual min=-0.002352 max=0.001919 Jy/beam ! Clean residual mean=-0.000017 rms=0.000465 Jy/beam ! Combined flux in latest and established models = 0.381344 Jy selfcal ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 112 components and 0.381344 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.080647Jy sigma=0.916764 ! Fit after self-cal, rms=0.080574Jy sigma=0.916460 wmodel J1104+3812_X_map.mod ! Writing 112 model components to file: J1104+3812_X_map.mod wobs J1104+3812_X_uvs.fits ! Writing UV FITS file: J1104+3812_X_uvs.fits wwins J1104+3812_X_map.win ! wwins: Wrote 5 windows to J1104+3812_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 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1655 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00099514 Jy ! Component: 100 - total flux cleaned = -0.00144337 Jy ! Component: 150 - total flux cleaned = -0.00186845 Jy ! Component: 200 - total flux cleaned = -0.00224361 Jy ! Component: 250 - total flux cleaned = -0.00257391 Jy ! Component: 300 - total flux cleaned = -0.00289605 Jy ! Component: 350 - total flux cleaned = -0.0031489 Jy ! Component: 400 - total flux cleaned = -0.00333552 Jy ! Component: 450 - total flux cleaned = -0.00351899 Jy ! Component: 500 - total flux cleaned = -0.00373016 Jy ! Component: 550 - total flux cleaned = -0.00396762 Jy ! Component: 600 - total flux cleaned = -0.00423196 Jy ! Component: 650 - total flux cleaned = -0.00446362 Jy ! Component: 700 - total flux cleaned = -0.00466479 Jy ! Component: 750 - total flux cleaned = -0.00486323 Jy ! Component: 800 - total flux cleaned = -0.00503213 Jy ! Component: 850 - total flux cleaned = -0.00525463 Jy ! Component: 900 - total flux cleaned = -0.00536502 Jy ! Component: 950 - total flux cleaned = -0.00555698 Jy ! Component: 1000 - total flux cleaned = -0.00572029 Jy ! Component: 1050 - total flux cleaned = -0.00585496 Jy ! Component: 1100 - total flux cleaned = -0.00596257 Jy ! Component: 1150 - total flux cleaned = -0.00614848 Jy ! Component: 1200 - total flux cleaned = -0.00622776 Jy ! Component: 1250 - total flux cleaned = -0.00638544 Jy ! Component: 1300 - total flux cleaned = -0.00648975 Jy ! Component: 1350 - total flux cleaned = -0.0065419 Jy ! Component: 1400 - total flux cleaned = -0.00669657 Jy ! Component: 1450 - total flux cleaned = -0.00672224 Jy ! Component: 1500 - total flux cleaned = -0.00679898 Jy ! Component: 1550 - total flux cleaned = -0.00695128 Jy ! Component: 1600 - total flux cleaned = -0.00700173 Jy ! Component: 1650 - total flux cleaned = -0.0070018 Jy ! Component: 1700 - total flux cleaned = -0.0071019 Jy ! Component: 1750 - total flux cleaned = -0.00712677 Jy ! Component: 1800 - total flux cleaned = -0.0072254 Jy ! Component: 1850 - total flux cleaned = -0.00720074 Jy ! Component: 1900 - total flux cleaned = -0.00724978 Jy ! Component: 1950 - total flux cleaned = -0.00734729 Jy ! Component: 2000 - total flux cleaned = -0.00732294 Jy ! Component: 2050 - total flux cleaned = -0.00749206 Jy ! Component: 2100 - total flux cleaned = -0.00742 Jy ! Component: 2150 - total flux cleaned = -0.00749187 Jy ! Component: 2200 - total flux cleaned = -0.00756351 Jy ! Component: 2250 - total flux cleaned = -0.00765861 Jy ! Component: 2300 - total flux cleaned = -0.00768234 Jy ! Component: 2350 - total flux cleaned = -0.00772944 Jy ! Component: 2400 - total flux cleaned = -0.00777626 Jy ! Component: 2450 - total flux cleaned = -0.00784603 Jy ! Component: 2500 - total flux cleaned = -0.00779948 Jy ! Component: 2550 - total flux cleaned = -0.00789219 Jy ! Component: 2600 - total flux cleaned = -0.00793828 Jy ! Component: 2650 - total flux cleaned = -0.00786928 Jy ! Component: 2700 - total flux cleaned = -0.00805227 Jy ! Component: 2750 - total flux cleaned = -0.00805212 Jy ! Component: 2800 - total flux cleaned = -0.00809749 Jy ! Component: 2850 - total flux cleaned = -0.00812008 Jy ! Component: 2900 - total flux cleaned = -0.0082103 Jy ! Component: 2950 - total flux cleaned = -0.00823278 Jy ! Component: 3000 - total flux cleaned = -0.00829983 Jy ! Component: 3050 - total flux cleaned = -0.00838882 Jy ! Component: 3100 - total flux cleaned = -0.00841098 Jy ! Component: 3150 - total flux cleaned = -0.00845519 Jy ! Component: 3200 - total flux cleaned = -0.00843314 Jy ! Component: 3250 - total flux cleaned = -0.00856502 Jy ! Component: 3300 - total flux cleaned = -0.00863066 Jy ! Component: 3350 - total flux cleaned = -0.00863082 Jy ! Component: 3400 - total flux cleaned = -0.00869593 Jy ! Component: 3450 - total flux cleaned = -0.00880428 Jy ! Component: 3500 - total flux cleaned = -0.00889062 Jy ! Component: 3550 - total flux cleaned = -0.00899823 Jy ! Component: 3600 - total flux cleaned = -0.00899817 Jy ! Component: 3650 - total flux cleaned = -0.00906229 Jy ! Component: 3700 - total flux cleaned = -0.00925411 Jy ! Component: 3750 - total flux cleaned = -0.00925403 Jy ! Component: 3800 - total flux cleaned = -0.00933887 Jy ! Component: 3850 - total flux cleaned = -0.0093811 Jy ! Component: 3900 - total flux cleaned = -0.00933895 Jy ! Component: 3950 - total flux cleaned = -0.00940193 Jy ! Component: 4000 - total flux cleaned = -0.00954855 Jy ! Component: 4050 - total flux cleaned = -0.009632 Jy ! Total flux subtracted in 4096 components = -0.00965281 Jy ! Clean residual min=-0.001342 max=0.001177 Jy/beam ! Clean residual mean=-0.000006 rms=0.000349 Jy/beam ! Combined flux in latest and established models = 0.371692 Jy keep ! Adding 333 model components to the UV plane model. ! The established model now contains 445 components and 0.371691 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv118_uvs/J1104+3812_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1655 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.927 x 1.143 at 38.71 degrees (North through East) ! Clean map min=-0.0018684 max=0.30485 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv118_uvs/J1104+3812_X_map.fits wmodel /scr/pima/rv118_uvs/J1104+3812_X_map.mod ! Writing 445 model components to file: /scr/pima/rv118_uvs/J1104+3812_X_map.mod wobs /scr/pima/rv118_uvs/J1104+3812_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv118_uvs/J1104+3812_X_uvs.fits wwins /scr/pima/rv118_uvs/J1104+3812_X_map.win ! wwins: Wrote 6 windows to /scr/pima/rv118_uvs/J1104+3812_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.304849 invert ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1741 milli-arcsec ! The y-axis pixel size should ideally be below 0.1655 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000348529 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.342985 0.342985 0.68597 1.37194 2.74388 5.48776 10.9755 21.951 43.9021 87.8041 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.001 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.304 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 874.674 quit ! Quitting program ! Log file /scr/pima/rv118_uvs/J1104+3812_X_dfm.log closed on Sun Dec 10 00:09:13 2017