! Started logfile: /scr/pima/rv123_uvs/J0239-0234_X_dfm.log on Sun Dec 23 00:39:29 2018 float field_size field_size = 1024 float field_cell field_cell = 0.2000 float taper_size taper_size = 70.0 float freq freq = 8.36575 obs /scr/pima/rv123_uvs/J0239-0234_X_uva.fits ! Reading UV FITS file: /scr/pima/rv123_uvs/J0239-0234_X_uva.fits ! AN table 1: 2 integrations on 6 of 6 possible baselines. ! AN table 2: 32 integrations on 15 of 15 possible baselines. ! AN table 3: 42 integrations on 21 of 21 possible baselines. ! AN table 4: 10 integrations on 21 of 21 possible baselines. ! AN table 5: 38 integrations on 28 of 28 possible baselines. ! AN table 6: 16 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.467933 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0239-0234 ! ! 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 89 lines of history. ! ! Reading 6304 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 J0239-0234_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 98 telescope corrections were flagged in sub-array 2. ! A total of 95 telescope corrections were flagged in sub-array 3. ! A total of 10 telescope corrections were flagged in sub-array 4. ! A total of 169 telescope corrections were flagged in sub-array 5. ! A total of 71 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 98 telescope corrections were flagged in sub-array 2. ! A total of 95 telescope corrections were flagged in sub-array 3. ! A total of 10 telescope corrections were flagged in sub-array 4. ! A total of 169 telescope corrections were flagged in sub-array 5. ! A total of 71 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 116 telescope corrections were flagged in sub-array 2. ! A total of 142 telescope corrections were flagged in sub-array 3. ! A total of 18 telescope corrections were flagged in sub-array 4. ! A total of 169 telescope corrections were flagged in sub-array 5. ! A total of 71 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 116 telescope corrections were flagged in sub-array 2. ! A total of 142 telescope corrections were flagged in sub-array 3. ! A total of 18 telescope corrections were flagged in sub-array 4. ! A total of 169 telescope corrections were flagged in sub-array 5. ! A total of 71 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.162335Jy sigma=13.089188 ! Fit after self-cal, rms=0.514320Jy sigma=4.768274 ! 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 1.94% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 milli-arcsec ! Estimated beam: bmin=0.6355 mas, bmaj=0.843 mas, bpa=9.913 degrees ! Estimated noise=1.31384 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 = 0.491087 Jy ! Component: 100 - total flux cleaned = 0.618964 Jy ! Total flux subtracted in 100 components = 0.618964 Jy ! Clean residual min=-0.026425 max=0.058698 Jy/beam ! Clean residual mean=-0.000096 rms=0.005499 Jy/beam ! Combined flux in latest and established models = 0.618964 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.618964 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.220099Jy sigma=1.987334 ! Fit after self-cal, rms=0.219990Jy sigma=1.986076 ! Inverting map ! Your choice of large map pixels excluded 1.94% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 milli-arcsec ! Added new window around map position (-0.2, -0.8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0602241 Jy ! Component: 100 - total flux cleaned = 0.0883875 Jy ! Total flux subtracted in 100 components = 0.0883875 Jy ! Clean residual min=-0.024522 max=0.023751 Jy/beam ! Clean residual mean=-0.000149 rms=0.004451 Jy/beam ! Combined flux in latest and established models = 0.707351 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 8 components and 0.707351 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.225707Jy sigma=1.901614 ! Fit after self-cal, rms=0.225417Jy sigma=1.898300 ! Inverting map ! Your choice of large map pixels excluded 1.94% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 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 1.94% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 milli-arcsec ! Estimated beam: bmin=0.6851 mas, bmaj=0.8794 mas, bpa=8.715 degrees ! Estimated noise=1.02256 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 = -0.0448748 Jy ! Component: 100 - total flux cleaned = -0.0642787 Jy ! Component: 150 - total flux cleaned = -0.067116 Jy ! Component: 200 - total flux cleaned = -0.06898 Jy ! Total flux subtracted in 200 components = -0.06898 Jy ! Clean residual min=-0.049531 max=0.020719 Jy/beam ! Clean residual mean=-0.010669 rms=0.006697 Jy/beam ! Combined flux in latest and established models = 0.638371 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 18 components and 0.638371 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.210725Jy sigma=1.881319 ! Fit after self-cal, rms=0.210517Jy sigma=1.879964 ! Inverting map ! Your choice of large map pixels excluded 1.94% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 milli-arcsec print "============== Finished natural weighting clean ==============" ! ============== Finished natural weighting clean ============== ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6851 x 0.8794 at 8.715 degrees (North through East) ! Clean map min=-0.045021 max=0.57086 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! KP 1.08 MK 0.92 OV 0.95 YG 0.87 ! ! Telescope amplitude corrections in sub-array 2: ! HH 0.78 NY 0.80 ON 0.96 WN 1.77 ! WZ 1.07 YG 1.16 ! ! A total of 9 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HH 0.84 HN 1.15 NY 0.79 ON 0.95 ! SC 1.33 WN 1.69 WZ 1.11 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HH 0.84 HN 1.00 NL 1.27 NY 0.74 ! ON 0.88 SC 0.84 WZ 1.03 ! ! A total of 30 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! FD 1.00 HH 0.81 HN 1.02 NL 0.87 ! ON 0.93 SC 1.61 WN 1.51 WZ 0.97 ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.96 FD 0.82 HN 0.97 KP 1.04 ! LA 0.94 MK 0.84 NL 0.97 OV 0.93 ! PT 0.83 SC 0.96 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! KP 1.03 MK 0.85 OV 0.96 YG 0.78 ! ! Telescope amplitude corrections in sub-array 2: ! HH 0.78 NY 0.94 ON 0.93 WN 1.68 ! WZ 1.02 YG 0.99 ! ! A total of 9 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HH 0.84 HN 1.10 NY 0.94 ON 0.89 ! SC 1.42 WN 1.62 WZ 1.10 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HH 0.95 HN 1.06 NL 1.20 NY 0.91 ! ON 0.86 SC 0.77 WZ 1.04 ! ! A total of 30 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! FD 0.98 HH 0.71 HN 1.01 NL 0.86 ! ON 0.86 SC 1.71 WN 1.60 WZ 0.99 ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.98 FD 0.83 HN 0.98 KP 1.02 ! LA 0.95 MK 0.85 NL 0.97 OV 0.92 ! PT 0.83 SC 0.96 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! KP 1.10 MK 0.90 OV 0.94 YG 1.00 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 0.92 NY 1.00* ON 1.27 WN 1.67 ! WZ 1.08 YG 1.10 ! ! A total of 48 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HH 0.92 HN 1.14 NY 1.00* ON 1.21 ! SC 1.57 WN 1.45 WZ 1.05 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HH 0.89 HN 0.98 NL 1.24 NY 1.00* ! ON 1.18 SC 0.85 WZ 1.08 ! ! A total of 30 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! FD 0.94 HH 0.93 HN 1.04 NL 0.86 ! ON 1.23 SC 1.82 WN 1.40 WZ 1.03 ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.98 FD 0.79 HN 0.98 KP 1.04 ! LA 0.96 MK 0.82 NL 0.98 OV 0.92 ! PT 0.81 SC 0.96 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! KP 1.10 MK 0.88 OV 0.87 YG 1.20 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 1.00 NY 1.00* ON 1.28 WN 1.38 ! WZ 1.12 YG 1.24 ! ! A total of 48 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HH 1.08 HN 1.14 NY 1.00* ON 1.18 ! SC 1.41 WN 1.39 WZ 1.10 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HH 1.04 HN 1.04 NL 1.27 NY 1.00* ! ON 1.12 SC 0.87 WZ 1.10 ! ! A total of 30 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! FD 1.00 HH 1.05 HN 1.05 NL 0.85 ! ON 1.21 SC 1.58 WN 1.42 WZ 1.01 ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.00 FD 0.80 HN 0.97 KP 1.03 ! LA 0.94 MK 0.84 NL 0.99 OV 0.92 ! PT 0.83 SC 1.01 ! ! ! Fit before self-cal, rms=0.210517Jy sigma=1.879964 ! Fit after self-cal, rms=0.181158Jy sigma=1.121981 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 milli-arcsec ! Estimated beam: bmin=0.6997 mas, bmaj=0.9055 mas, bpa=12.95 degrees ! Estimated noise=1.07574 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 = -0.00382189 Jy ! Component: 100 - total flux cleaned = -0.00301494 Jy ! Component: 150 - total flux cleaned = -0.00301221 Jy ! Component: 200 - total flux cleaned = -0.00270345 Jy ! Total flux subtracted in 200 components = -0.00270345 Jy ! Clean residual min=-0.011578 max=0.012465 Jy/beam ! Clean residual mean=-0.000172 rms=0.002816 Jy/beam ! Combined flux in latest and established models = 0.635668 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 24 components and 0.635668 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.178841Jy sigma=1.106067 ! Fit after self-cal, rms=0.179306Jy sigma=1.103491 ! Inverting map ! Your choice of large map pixels excluded 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 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=0.179306Jy sigma=1.103491 ! Fit after self-cal, rms=0.243746Jy sigma=1.103724 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 milli-arcsec ! Estimated beam: bmin=0.7026 mas, bmaj=0.9166 mas, bpa=18.25 degrees ! Estimated noise=1.09335 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00288161 Jy ! Component: 100 - total flux cleaned = 0.00287874 Jy ! Component: 150 - total flux cleaned = 0.00236147 Jy ! Component: 200 - total flux cleaned = 0.00235729 Jy ! Total flux subtracted in 200 components = 0.00235729 Jy ! Clean residual min=-0.012706 max=0.013047 Jy/beam ! Clean residual mean=0.000203 rms=0.002935 Jy/beam ! Combined flux in latest and established models = 0.638025 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 27 components and 0.638025 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.238145Jy sigma=1.086531 ! Fit after self-cal, rms=0.238376Jy sigma=1.085047 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 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 (-7.6, 13.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00513464 Jy ! Component: 100 - total flux cleaned = 0.00513636 Jy ! Component: 150 - total flux cleaned = 0.00469741 Jy ! Component: 200 - total flux cleaned = 0.004277 Jy ! Total flux subtracted in 200 components = 0.004277 Jy ! Clean residual min=-0.012331 max=0.012385 Jy/beam ! Clean residual mean=0.000113 rms=0.002842 Jy/beam ! Combined flux in latest and established models = 0.642302 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 46 components and 0.642302 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.233989Jy sigma=1.073874 ! Fit after self-cal, rms=0.233891Jy sigma=1.072839 ! Inverting map ! Your choice of large map pixels excluded 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 milli-arcsec ! Added new window around map position (10.4, -24.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00342398 Jy ! Component: 100 - total flux cleaned = 0.00345875 Jy ! Component: 150 - total flux cleaned = 0.00442666 Jy ! Component: 200 - total flux cleaned = 0.00533876 Jy ! Total flux subtracted in 200 components = 0.00533876 Jy ! Clean residual min=-0.012128 max=0.011989 Jy/beam ! Clean residual mean=0.000009 rms=0.002719 Jy/beam ! Combined flux in latest and established models = 0.647641 Jy ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 71 components and 0.647641 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.228443Jy sigma=1.058475 ! Fit after self-cal, rms=0.228344Jy sigma=1.057447 ! Inverting map ! Your choice of large map pixels excluded 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 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=0.228344Jy sigma=1.057447 ! Fit after self-cal, rms=0.187060Jy sigma=0.896004 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 milli-arcsec ! Estimated beam: bmin=0.6974 mas, bmaj=0.9021 mas, bpa=15.88 degrees ! Estimated noise=1.08478 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00198265 Jy ! Component: 100 - total flux cleaned = 0.00187788 Jy ! Component: 150 - total flux cleaned = 0.00187521 Jy ! Component: 200 - total flux cleaned = 0.00187758 Jy ! Total flux subtracted in 200 components = 0.00187758 Jy ! Clean residual min=-0.005161 max=0.004841 Jy/beam ! Clean residual mean=0.000131 rms=0.000990 Jy/beam ! Combined flux in latest and established models = 0.649519 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 83 components and 0.649519 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.186851Jy sigma=0.894182 ! Fit after self-cal, rms=0.186995Jy sigma=0.893560 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 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 = -0.000261585 Jy ! Component: 100 - total flux cleaned = -0.000425628 Jy ! Component: 150 - total flux cleaned = -0.000579473 Jy ! Component: 200 - total flux cleaned = -0.000800785 Jy ! Total flux subtracted in 200 components = -0.000800785 Jy ! Clean residual min=-0.005199 max=0.004840 Jy/beam ! Clean residual mean=0.000139 rms=0.000979 Jy/beam ! Combined flux in latest and established models = 0.648718 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 90 components and 0.648718 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.186893Jy sigma=0.892629 ! Fit after self-cal, rms=0.186888Jy sigma=0.892599 ! Inverting map ! Your choice of large map pixels excluded 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 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=0.186888Jy sigma=0.892599 ! Fit after self-cal, rms=0.187341Jy sigma=0.892092 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 milli-arcsec ! Estimated beam: bmin=2.62 mas, bmaj=3.226 mas, bpa=-10.33 degrees ! Estimated noise=1.3803 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00173077 Jy ! Component: 100 - total flux cleaned = 0.00146989 Jy ! Component: 150 - total flux cleaned = 0.00138911 Jy ! Component: 200 - total flux cleaned = 0.00138698 Jy ! Total flux subtracted in 200 components = 0.00138698 Jy ! Clean residual min=-0.003655 max=0.004756 Jy/beam ! Clean residual mean=0.000317 rms=0.001022 Jy/beam ! Combined flux in latest and established models = 0.650105 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 98 components and 0.650105 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.187313Jy sigma=0.891709 ! Fit after self-cal, rms=0.187312Jy sigma=0.891640 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 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 (-31, 17). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00456047 Jy ! Component: 100 - total flux cleaned = 0.00712357 Jy ! Component: 150 - total flux cleaned = 0.00897566 Jy ! Component: 200 - total flux cleaned = 0.0100389 Jy ! Total flux subtracted in 200 components = 0.0100389 Jy ! Clean residual min=-0.004100 max=0.003361 Jy/beam ! Clean residual mean=-0.000162 rms=0.000929 Jy/beam ! Combined flux in latest and established models = 0.660144 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 125 components and 0.660144 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.187271Jy sigma=0.889336 ! Fit after self-cal, rms=0.187251Jy sigma=0.889187 ! Inverting map ! Your choice of large map pixels excluded 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 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 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 milli-arcsec ! Estimated beam: bmin=0.6964 mas, bmaj=0.9005 mas, bpa=16.08 degrees ! Estimated noise=1.08707 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6964 x 0.9005 at 16.08 degrees (North through East) ! Clean map min=-0.0053089 max=0.5786 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=0.187251Jy sigma=0.889187 ! Fit after self-cal, rms=0.208312Jy sigma=0.780804 ! Inverting map and beam ! Your choice of large map pixels excluded 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 milli-arcsec ! Estimated beam: bmin=0.6969 mas, bmaj=0.9003 mas, bpa=15.98 degrees ! Estimated noise=1.08958 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00215351 Jy ! Component: 100 - total flux cleaned = 0.00264436 Jy ! Component: 150 - total flux cleaned = 0.00275379 Jy ! Component: 200 - total flux cleaned = 0.00295916 Jy ! Total flux subtracted in 200 components = 0.00295916 Jy ! Clean residual min=-0.004604 max=0.004320 Jy/beam ! Clean residual mean=-0.000036 rms=0.000899 Jy/beam ! Combined flux in latest and established models = 0.663103 Jy ! Performing phase self-cal ! Adding 35 model components to the UV plane model. ! The established model now contains 158 components and 0.663103 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.208071Jy sigma=0.778289 ! Fit after self-cal, rms=0.208071Jy sigma=0.778170 ! Inverting map ! Your choice of large map pixels excluded 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000429993 Jy ! Component: 100 - total flux cleaned = 0.000621846 Jy ! Component: 150 - total flux cleaned = 0.000805427 Jy ! Component: 200 - total flux cleaned = 0.000802551 Jy ! Total flux subtracted in 200 components = 0.000802551 Jy ! Clean residual min=-0.004429 max=0.004280 Jy/beam ! Clean residual mean=-0.000050 rms=0.000884 Jy/beam ! Combined flux in latest and established models = 0.663905 Jy ! Performing phase self-cal ! Adding 46 model components to the UV plane model. ! The established model now contains 169 components and 0.663905 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.207923Jy sigma=0.776700 ! Fit after self-cal, rms=0.207918Jy sigma=0.776663 ! Inverting map ! Your choice of large map pixels excluded 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.207918Jy sigma=0.776663 ! Fit after self-cal, rms=0.208182Jy sigma=0.776296 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 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 milli-arcsec ! Estimated beam: bmin=0.6544 mas, bmaj=0.883 mas, bpa=15.82 degrees ! Estimated noise=1.27138 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.464781 Jy ! Component: 100 - total flux cleaned = 0.577961 Jy ! Component: 150 - total flux cleaned = 0.621032 Jy ! Component: 200 - total flux cleaned = 0.640228 Jy ! Total flux subtracted in 200 components = 0.640228 Jy ! Clean residual min=-0.009292 max=0.008548 Jy/beam ! Clean residual mean=0.000010 rms=0.001462 Jy/beam ! Combined flux in latest and established models = 0.640228 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 0.640228 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 milli-arcsec ! Estimated beam: bmin=0.6963 mas, bmaj=0.8993 mas, bpa=16.14 degrees ! Estimated noise=1.09075 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 = 0.00855175 Jy ! Component: 100 - total flux cleaned = 0.0120667 Jy ! Component: 150 - total flux cleaned = 0.0149091 Jy ! Component: 200 - total flux cleaned = 0.0164139 Jy ! Total flux subtracted in 200 components = 0.0164139 Jy ! Clean residual min=-0.006045 max=0.005164 Jy/beam ! Clean residual mean=0.000129 rms=0.001084 Jy/beam ! Combined flux in latest and established models = 0.656642 Jy ! Adding 27 model components to the UV plane model. ! The established model now contains 35 components and 0.656642 Jy ! Inverting map ! Your choice of large map pixels excluded 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 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 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 milli-arcsec ! Estimated beam: bmin=2.617 mas, bmaj=3.224 mas, bpa=-10.3 degrees ! Estimated noise=1.3873 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0038587 Jy ! Component: 100 - total flux cleaned = 0.00556174 Jy ! Component: 150 - total flux cleaned = 0.00683213 Jy ! Component: 200 - total flux cleaned = 0.0075238 Jy ! Total flux subtracted in 200 components = 0.0075238 Jy ! Clean residual min=-0.003928 max=0.003409 Jy/beam ! Clean residual mean=-0.000040 rms=0.000886 Jy/beam ! Combined flux in latest and established models = 0.664165 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 = 0.000442727 Jy ! Component: 100 - total flux cleaned = 0.000794357 Jy ! Component: 150 - total flux cleaned = 0.00106862 Jy ! Component: 200 - total flux cleaned = 0.00127512 Jy ! Total flux subtracted in 200 components = 0.00127512 Jy ! Clean residual min=-0.003992 max=0.003238 Jy/beam ! Clean residual mean=-0.000100 rms=0.000871 Jy/beam ! Combined flux in latest and established models = 0.665441 Jy ! Adding 42 model components to the UV plane model. ! The established model now contains 75 components and 0.665441 Jy ! Inverting map ! Your choice of large map pixels excluded 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 milli-arcsec ! Estimated beam: bmin=0.6963 mas, bmaj=0.8993 mas, bpa=16.14 degrees ! Estimated noise=1.09075 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000233616 Jy ! Component: 100 - total flux cleaned = -0.000422114 Jy ! Component: 150 - total flux cleaned = -0.000417932 Jy ! Component: 200 - total flux cleaned = -0.000573882 Jy ! Total flux subtracted in 200 components = -0.000573882 Jy ! Clean residual min=-0.004975 max=0.004705 Jy/beam ! Clean residual mean=-0.000027 rms=0.001011 Jy/beam ! Combined flux in latest and established models = 0.664867 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 87 components and 0.664867 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.209573Jy sigma=0.790219 ! Fit after self-cal, rms=0.209397Jy sigma=0.788244 wmodel J0239-0234_X_map.mod ! Writing 87 model components to file: J0239-0234_X_map.mod wobs J0239-0234_X_uvs.fits ! Writing UV FITS file: J0239-0234_X_uvs.fits wwins J0239-0234_X_map.win ! wwins: Wrote 5 windows to J0239-0234_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 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00183541 Jy ! Component: 100 - total flux cleaned = -0.00209729 Jy ! Component: 150 - total flux cleaned = -0.00217883 Jy ! Component: 200 - total flux cleaned = -0.00249475 Jy ! Component: 250 - total flux cleaned = -0.0027272 Jy ! Component: 300 - total flux cleaned = -0.00310284 Jy ! Component: 350 - total flux cleaned = -0.00324891 Jy ! Component: 400 - total flux cleaned = -0.00332005 Jy ! Component: 450 - total flux cleaned = -0.00346108 Jy ! Component: 500 - total flux cleaned = -0.0035305 Jy ! Component: 550 - total flux cleaned = -0.0036668 Jy ! Component: 600 - total flux cleaned = -0.00366696 Jy ! Component: 650 - total flux cleaned = -0.00366789 Jy ! Component: 700 - total flux cleaned = -0.00379844 Jy ! Component: 750 - total flux cleaned = -0.00386241 Jy ! Component: 800 - total flux cleaned = -0.00379883 Jy ! Component: 850 - total flux cleaned = -0.00379915 Jy ! Component: 900 - total flux cleaned = -0.00386099 Jy ! Component: 950 - total flux cleaned = -0.00379982 Jy ! Component: 1000 - total flux cleaned = -0.00379992 Jy ! Component: 1050 - total flux cleaned = -0.00373974 Jy ! Component: 1100 - total flux cleaned = -0.00368055 Jy ! Component: 1150 - total flux cleaned = -0.00362174 Jy ! Component: 1200 - total flux cleaned = -0.00356367 Jy ! Component: 1250 - total flux cleaned = -0.00344899 Jy ! Component: 1300 - total flux cleaned = -0.00344952 Jy ! Component: 1350 - total flux cleaned = -0.00350604 Jy ! Component: 1400 - total flux cleaned = -0.00339416 Jy ! Component: 1450 - total flux cleaned = -0.00344979 Jy ! Component: 1500 - total flux cleaned = -0.00333916 Jy ! Component: 1550 - total flux cleaned = -0.00328459 Jy ! Component: 1600 - total flux cleaned = -0.00323064 Jy ! Component: 1650 - total flux cleaned = -0.00323073 Jy ! Component: 1700 - total flux cleaned = -0.00323064 Jy ! Component: 1750 - total flux cleaned = -0.00312464 Jy ! Component: 1800 - total flux cleaned = -0.00307225 Jy ! Component: 1850 - total flux cleaned = -0.00301994 Jy ! Component: 1900 - total flux cleaned = -0.00307167 Jy ! Component: 1950 - total flux cleaned = -0.00296848 Jy ! Component: 2000 - total flux cleaned = -0.0029172 Jy ! Component: 2050 - total flux cleaned = -0.00286639 Jy ! Component: 2100 - total flux cleaned = -0.0027656 Jy ! Component: 2150 - total flux cleaned = -0.00276558 Jy ! Component: 2200 - total flux cleaned = -0.00266605 Jy ! Component: 2250 - total flux cleaned = -0.00266597 Jy ! Component: 2300 - total flux cleaned = -0.00256761 Jy ! Component: 2350 - total flux cleaned = -0.00251888 Jy ! Component: 2400 - total flux cleaned = -0.00251914 Jy ! Component: 2450 - total flux cleaned = -0.00251898 Jy ! Component: 2500 - total flux cleaned = -0.00242308 Jy ! Component: 2550 - total flux cleaned = -0.00242315 Jy ! Component: 2600 - total flux cleaned = -0.00237568 Jy ! Component: 2650 - total flux cleaned = -0.00237562 Jy ! Component: 2700 - total flux cleaned = -0.00228201 Jy ! Component: 2750 - total flux cleaned = -0.00228214 Jy ! Component: 2800 - total flux cleaned = -0.00223588 Jy ! Component: 2850 - total flux cleaned = -0.00223578 Jy ! Component: 2900 - total flux cleaned = -0.00214428 Jy ! Component: 2950 - total flux cleaned = -0.00219003 Jy ! Component: 3000 - total flux cleaned = -0.00214458 Jy ! Component: 3050 - total flux cleaned = -0.00209935 Jy ! Component: 3100 - total flux cleaned = -0.0020546 Jy ! Component: 3150 - total flux cleaned = -0.0020547 Jy ! Component: 3200 - total flux cleaned = -0.00201032 Jy ! Component: 3250 - total flux cleaned = -0.00201023 Jy ! Component: 3300 - total flux cleaned = -0.00201008 Jy ! Component: 3350 - total flux cleaned = -0.00196629 Jy ! Component: 3400 - total flux cleaned = -0.00196637 Jy ! Component: 3450 - total flux cleaned = -0.00192325 Jy ! Component: 3500 - total flux cleaned = -0.00192326 Jy ! Component: 3550 - total flux cleaned = -0.00192321 Jy ! Component: 3600 - total flux cleaned = -0.00183781 Jy ! Component: 3650 - total flux cleaned = -0.00183792 Jy ! Component: 3700 - total flux cleaned = -0.00179564 Jy ! Component: 3750 - total flux cleaned = -0.00175352 Jy ! Component: 3800 - total flux cleaned = -0.00175359 Jy ! Component: 3850 - total flux cleaned = -0.00175361 Jy ! Component: 3900 - total flux cleaned = -0.00175354 Jy ! Component: 3950 - total flux cleaned = -0.00171216 Jy ! Component: 4000 - total flux cleaned = -0.00171209 Jy ! Component: 4050 - total flux cleaned = -0.00167097 Jy ! Total flux subtracted in 4096 components = -0.00163024 Jy ! Clean residual min=-0.002260 max=0.002362 Jy/beam ! Clean residual mean=0.000010 rms=0.000643 Jy/beam ! Combined flux in latest and established models = 0.663237 Jy keep ! Adding 307 model components to the UV plane model. ! The established model now contains 392 components and 0.663236 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv123_uvs/J0239-0234_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6963 x 0.8993 at 16.14 degrees (North through East) ! Clean map min=-0.0039643 max=0.57439 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv123_uvs/J0239-0234_X_map.fits wmodel /scr/pima/rv123_uvs/J0239-0234_X_map.mod ! Writing 392 model components to file: /scr/pima/rv123_uvs/J0239-0234_X_map.mod wobs /scr/pima/rv123_uvs/J0239-0234_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv123_uvs/J0239-0234_X_uvs.fits wwins /scr/pima/rv123_uvs/J0239-0234_X_map.win ! wwins: Wrote 6 windows to /scr/pima/rv123_uvs/J0239-0234_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.574393 invert ! Inverting map ! Your choice of large map pixels excluded 2.08% of the data. ! The x-axis pixel size should ideally be below 0.1725 milli-arcsec ! The y-axis pixel size should ideally be below 0.1955 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000641469 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.335033 0.335033 0.670066 1.34013 2.68027 5.36053 10.7211 21.4421 42.8843 85.7685 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0019 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.574 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 895.433 quit ! Quitting program ! Log file /scr/pima/rv123_uvs/J0239-0234_X_dfm.log closed on Sun Dec 23 00:39:33 2018