! Started logfile: /scr/pima/rv123_uvs/J0501-0159_X_dfm.log on Sun Dec 23 00:40:02 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/J0501-0159_X_uva.fits ! Reading UV FITS file: /scr/pima/rv123_uvs/J0501-0159_X_uva.fits ! AN table 1: 3 integrations on 28 of 28 possible baselines. ! AN table 2: 5 integrations on 10 of 10 possible baselines. ! AN table 3: 55 integrations on 21 of 21 possible baselines. ! AN table 4: 10 integrations on 21 of 21 possible baselines. ! AN table 5: 16 integrations on 66 of 66 possible baselines. ! AN table 6: 11 integrations on 66 of 66 possible baselines. ! Apparent sampling: 0.451996 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0501-0159 ! ! 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 5932 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 J0501-0159_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 8 telescope corrections were flagged in sub-array 1. ! A total of 7 telescope corrections were flagged in sub-array 2. ! A total of 255 telescope corrections were flagged in sub-array 3. ! A total of 24 telescope corrections were flagged in sub-array 4. ! A total of 76 telescope corrections were flagged in sub-array 5. ! A total of 52 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 8 telescope corrections were flagged in sub-array 1. ! A total of 7 telescope corrections were flagged in sub-array 2. ! A total of 255 telescope corrections were flagged in sub-array 3. ! A total of 24 telescope corrections were flagged in sub-array 4. ! A total of 76 telescope corrections were flagged in sub-array 5. ! A total of 52 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 8 telescope corrections were flagged in sub-array 1. ! A total of 7 telescope corrections were flagged in sub-array 2. ! A total of 265 telescope corrections were flagged in sub-array 3. ! A total of 32 telescope corrections were flagged in sub-array 4. ! A total of 76 telescope corrections were flagged in sub-array 5. ! A total of 52 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 8 telescope corrections were flagged in sub-array 1. ! A total of 7 telescope corrections were flagged in sub-array 2. ! A total of 265 telescope corrections were flagged in sub-array 3. ! A total of 32 telescope corrections were flagged in sub-array 4. ! A total of 76 telescope corrections were flagged in sub-array 5. ! A total of 52 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=2.114970Jy sigma=18.774009 ! Fit after self-cal, rms=1.002368Jy sigma=9.072119 ! 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 3.32% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 milli-arcsec ! Estimated beam: bmin=0.5178 mas, bmaj=0.7821 mas, bpa=1.816 degrees ! Estimated noise=1.78933 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 = 1.39721 Jy ! Component: 100 - total flux cleaned = 1.85431 Jy ! Total flux subtracted in 100 components = 1.85431 Jy ! Clean residual min=-0.083305 max=0.210551 Jy/beam ! Clean residual mean=-0.000314 rms=0.014843 Jy/beam ! Combined flux in latest and established models = 1.85431 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 9 components and 1.85431 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.549644Jy sigma=4.688204 ! Fit after self-cal, rms=0.544198Jy sigma=4.663214 ! Inverting map ! Your choice of large map pixels excluded 3.32% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.243703 Jy ! Component: 100 - total flux cleaned = 0.379595 Jy ! Total flux subtracted in 100 components = 0.379595 Jy ! Clean residual min=-0.069246 max=0.074732 Jy/beam ! Clean residual mean=-0.000519 rms=0.010369 Jy/beam ! Combined flux in latest and established models = 2.2339 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 14 components and 2.2339 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.473765Jy sigma=3.777688 ! Fit after self-cal, rms=0.471509Jy sigma=3.769290 ! Inverting map ! Your choice of large map pixels excluded 3.32% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0840633 Jy ! Component: 100 - total flux cleaned = 0.131626 Jy ! Total flux subtracted in 100 components = 0.131626 Jy ! Clean residual min=-0.067706 max=0.058433 Jy/beam ! Clean residual mean=-0.000589 rms=0.009699 Jy/beam ! Combined flux in latest and established models = 2.36553 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 17 components and 2.36553 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.476297Jy sigma=3.748279 ! Fit after self-cal, rms=0.475591Jy sigma=3.745601 ! Inverting map ! Your choice of large map pixels excluded 3.32% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 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 3.32% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 milli-arcsec ! Estimated beam: bmin=0.53 mas, bmaj=0.9815 mas, bpa=-1.473 degrees ! Estimated noise=1.23915 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 = -0.0651954 Jy ! Component: 100 - total flux cleaned = -0.0962482 Jy ! Component: 150 - total flux cleaned = -0.106547 Jy ! Component: 200 - total flux cleaned = -0.108877 Jy ! Total flux subtracted in 200 components = -0.108877 Jy ! Clean residual min=-0.097590 max=0.056577 Jy/beam ! Clean residual mean=-0.024776 rms=0.015584 Jy/beam ! Combined flux in latest and established models = 2.25665 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 25 components and 2.25665 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.464135Jy sigma=3.708217 ! Fit after self-cal, rms=0.464015Jy sigma=3.707863 ! Inverting map ! Your choice of large map pixels excluded 3.32% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 milli-arcsec print "============== Finished natural weighting clean ==============" ! ============== Finished natural weighting clean ============== ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.53 x 0.9815 at -1.473 degrees (North through East) ! Clean map min=-0.094895 max=1.7312 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.85 HN 1.12 KP 0.98 ! LA 0.98 MK 0.85 NL 1.01 OV 0.95 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 KP 1.05 MK 0.87 OV 0.96 ! YG 0.92 ! ! A total of 42 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HH 0.79 MC 0.90 NY 0.83 ON 0.99 ! WN 1.73 WZ 1.07 YG 1.02 ! ! Telescope amplitude corrections in sub-array 4: ! HH 0.78 HN 1.15 NY 0.85 ON 0.98 ! SC 0.98 WN 1.58 WZ 1.04 ! ! A total of 12 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 FD 0.84 HH 0.74 HN 0.98 ! KP 1.04 LA 0.99 NL 1.02 ON 1.03 ! OV 0.96 SC 0.86 WN 1.50 WZ 0.96 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.98 FD 0.83 HN 0.99 KP 0.98 ! LA 0.96 NL 1.01 ON 0.99 OV 0.95 ! PT 0.83 SC 1.11 WN 1.50 WZ 0.95 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 0.84 HN 1.12 KP 0.99 ! LA 0.98 MK 0.83 NL 0.99 OV 0.95 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 KP 1.02 MK 0.88 OV 0.94 ! YG 0.84 ! ! A total of 42 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HH 0.78 MC 0.97 NY 0.92 ON 0.95 ! WN 1.71 WZ 1.05 YG 0.90 ! ! Telescope amplitude corrections in sub-array 4: ! HH 0.77 HN 1.09 NY 0.98 ON 0.91 ! SC 1.02 WN 1.55 WZ 1.01 ! ! A total of 12 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 FD 0.83 HH 0.71 HN 0.96 ! KP 1.05 LA 0.99 NL 1.02 ON 0.97 ! OV 0.97 SC 0.85 WN 1.53 WZ 0.92 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.98 FD 0.81 HN 0.98 KP 1.01 ! LA 0.95 NL 0.99 ON 0.96 OV 0.95 ! PT 0.83 SC 1.11 WN 1.53 WZ 0.93 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.83 HN 1.10 KP 0.99 ! LA 0.96 MK 0.84 NL 1.01 OV 0.95 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 KP 1.00 MK 0.87 OV 0.94 ! YG 0.93 ! ! A total of 48 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HH 0.89 MC 1.37 NY 1.00* ON 1.28 ! WN 1.57 WZ 1.12 YG 0.94 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HH 0.82 HN 1.11 NY 1.00* ON 1.23 ! SC 1.04 WN 1.43 WZ 1.06 ! ! A total of 12 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 FD 0.82 HH 0.75 HN 0.96 ! KP 1.03 LA 0.97 NL 1.00 ON 1.33 ! OV 0.95 SC 0.83 WN 1.39 WZ 0.96 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.97 FD 0.80 HN 0.96 KP 0.97 ! LA 0.96 NL 0.98 ON 1.30 OV 0.92 ! PT 0.82 SC 1.19 WN 1.38 WZ 0.98 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 0.84 HN 1.11 KP 1.00 ! LA 0.96 MK 0.83 NL 1.01 OV 0.93 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 KP 1.02 MK 0.89 OV 0.92 ! YG 0.98 ! ! A total of 48 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HH 1.02 MC 1.33 NY 1.00* ON 1.23 ! WN 1.47 WZ 1.14 YG 1.04 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HH 0.91 HN 1.14 NY 1.00* ON 1.20 ! SC 0.99 WN 1.35 WZ 1.08 ! ! A total of 12 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 FD 0.83 HH 0.84 HN 0.95 ! KP 1.04 LA 0.97 NL 1.00 ON 1.28 ! OV 0.94 SC 0.85 WN 1.30 WZ 0.99 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.97 FD 0.80 HN 0.96 KP 1.01 ! LA 0.95 NL 0.97 ON 1.25 OV 0.92 ! PT 0.82 SC 1.22 WN 1.28 WZ 0.99 ! ! ! Fit before self-cal, rms=0.464015Jy sigma=3.707863 ! Fit after self-cal, rms=0.191719Jy sigma=1.288209 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 milli-arcsec ! Estimated beam: bmin=0.5409 mas, bmaj=1.033 mas, bpa=-3.793 degrees ! Estimated noise=1.25243 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 = -0.0363895 Jy ! Component: 100 - total flux cleaned = -0.0381611 Jy ! Component: 150 - total flux cleaned = -0.0381511 Jy ! Component: 200 - total flux cleaned = -0.0381492 Jy ! Total flux subtracted in 200 components = -0.0381492 Jy ! Clean residual min=-0.020396 max=0.014149 Jy/beam ! Clean residual mean=-0.001433 rms=0.003073 Jy/beam ! Combined flux in latest and established models = 2.2185 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 31 components and 2.2185 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.180028Jy sigma=1.174902 ! Fit after self-cal, rms=0.179769Jy sigma=1.171201 ! Inverting map ! Your choice of large map pixels excluded 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 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=0.179769Jy sigma=1.171201 ! Fit after self-cal, rms=0.158072Jy sigma=0.992420 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 milli-arcsec ! Estimated beam: bmin=0.5448 mas, bmaj=1.03 mas, bpa=-3.541 degrees ! Estimated noise=1.25622 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0154228 Jy ! Component: 100 - total flux cleaned = -0.0168634 Jy ! Component: 150 - total flux cleaned = -0.016479 Jy ! Component: 200 - total flux cleaned = -0.0161562 Jy ! Total flux subtracted in 200 components = -0.0161562 Jy ! Clean residual min=-0.015834 max=0.013359 Jy/beam ! Clean residual mean=-0.000154 rms=0.002199 Jy/beam ! Combined flux in latest and established models = 2.20235 Jy selfcal ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 32 components and 2.20235 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.153687Jy sigma=0.954898 ! Fit after self-cal, rms=0.153241Jy sigma=0.952298 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 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 = 0.000647348 Jy ! Component: 100 - total flux cleaned = -0.000216415 Jy ! Component: 150 - total flux cleaned = -0.00069858 Jy ! Component: 200 - total flux cleaned = -0.000707411 Jy ! Total flux subtracted in 200 components = -0.000707411 Jy ! Clean residual min=-0.014656 max=0.012436 Jy/beam ! Clean residual mean=-0.000142 rms=0.002127 Jy/beam ! Combined flux in latest and established models = 2.20164 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 32 components and 2.20164 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.152109Jy sigma=0.940493 ! Fit after self-cal, rms=0.151794Jy sigma=0.938800 ! Inverting map ! Your choice of large map pixels excluded 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 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=0.151794Jy sigma=0.938800 ! Fit after self-cal, rms=0.136394Jy sigma=0.866918 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 milli-arcsec ! Estimated beam: bmin=0.547 mas, bmaj=1.033 mas, bpa=-3.43 degrees ! Estimated noise=1.25972 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00680787 Jy ! Component: 100 - total flux cleaned = -0.00745584 Jy ! Component: 150 - total flux cleaned = -0.00799047 Jy ! Component: 200 - total flux cleaned = -0.00798796 Jy ! Total flux subtracted in 200 components = -0.00798796 Jy ! Clean residual min=-0.012467 max=0.010952 Jy/beam ! Clean residual mean=0.000268 rms=0.001634 Jy/beam ! Combined flux in latest and established models = 2.19365 Jy selfcal ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 33 components and 2.19365 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.134471Jy sigma=0.850449 ! Fit after self-cal, rms=0.134297Jy sigma=0.848781 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 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 = 0.000883133 Jy ! Component: 100 - total flux cleaned = 0.000458224 Jy ! Component: 150 - total flux cleaned = 7.94371e-05 Jy ! Component: 200 - total flux cleaned = -0.000401512 Jy ! Total flux subtracted in 200 components = -0.000401512 Jy ! Clean residual min=-0.011493 max=0.010162 Jy/beam ! Clean residual mean=0.000274 rms=0.001582 Jy/beam ! Combined flux in latest and established models = 2.19325 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 33 components and 2.19325 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.133552Jy sigma=0.842063 ! Fit after self-cal, rms=0.133346Jy sigma=0.841033 ! Inverting map ! Your choice of large map pixels excluded 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 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=0.133346Jy sigma=0.841033 ! Fit after self-cal, rms=0.132522Jy sigma=0.834941 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 milli-arcsec ! Estimated beam: bmin=2.375 mas, bmaj=3.261 mas, bpa=-12.19 degrees ! Estimated noise=1.86969 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0034886 Jy ! Component: 100 - total flux cleaned = -0.00364237 Jy ! Component: 150 - total flux cleaned = -0.00389401 Jy ! Component: 200 - total flux cleaned = -0.00400715 Jy ! Total flux subtracted in 200 components = -0.00400715 Jy ! Clean residual min=-0.008693 max=0.013506 Jy/beam ! Clean residual mean=0.001511 rms=0.002307 Jy/beam ! Combined flux in latest and established models = 2.18924 Jy selfcal ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 34 components and 2.18924 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.132417Jy sigma=0.832028 ! Fit after self-cal, rms=0.132391Jy sigma=0.830848 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 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 (-3.4, 2.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00664039 Jy ! Component: 100 - total flux cleaned = 0.00961265 Jy ! Component: 150 - total flux cleaned = 0.0111817 Jy ! Component: 200 - total flux cleaned = 0.0126873 Jy ! Total flux subtracted in 200 components = 0.0126873 Jy ! Clean residual min=-0.005645 max=0.007008 Jy/beam ! Clean residual mean=0.000892 rms=0.001786 Jy/beam ! Combined flux in latest and established models = 2.20193 Jy ! Performing phase self-cal ! Adding 44 model components to the UV plane model. ! The established model now contains 78 components and 2.20193 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.131401Jy sigma=0.822201 ! Fit after self-cal, rms=0.131260Jy sigma=0.820889 ! Inverting map ! Your choice of large map pixels excluded 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 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 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 milli-arcsec ! Estimated beam: bmin=0.5483 mas, bmaj=1.032 mas, bpa=-3.359 degrees ! Estimated noise=1.26123 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5483 x 1.032 at -3.359 degrees (North through East) ! Clean map min=-0.010221 max=1.746 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=0.131260Jy sigma=0.820889 ! Fit after self-cal, rms=0.119665Jy sigma=0.738807 ! Inverting map and beam ! Your choice of large map pixels excluded 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 milli-arcsec ! Estimated beam: bmin=0.5484 mas, bmaj=1.032 mas, bpa=-3.349 degrees ! Estimated noise=1.26002 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00141567 Jy ! Component: 100 - total flux cleaned = 0.00120589 Jy ! Component: 150 - total flux cleaned = 0.00233461 Jy ! Component: 200 - total flux cleaned = 0.0031032 Jy ! Total flux subtracted in 200 components = 0.0031032 Jy ! Clean residual min=-0.005724 max=0.005696 Jy/beam ! Clean residual mean=0.000325 rms=0.001151 Jy/beam ! Combined flux in latest and established models = 2.20503 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 98 components and 2.20503 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.117686Jy sigma=0.721641 ! Fit after self-cal, rms=0.117606Jy sigma=0.720682 ! Inverting map ! Your choice of large map pixels excluded 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000959614 Jy ! Component: 100 - total flux cleaned = 0.00141913 Jy ! Component: 150 - total flux cleaned = 0.0018406 Jy ! Component: 200 - total flux cleaned = 0.00203929 Jy ! Total flux subtracted in 200 components = 0.00203929 Jy ! Clean residual min=-0.005254 max=0.005151 Jy/beam ! Clean residual mean=0.000291 rms=0.001097 Jy/beam ! Combined flux in latest and established models = 2.20707 Jy ! Performing phase self-cal ! Adding 34 model components to the UV plane model. ! The established model now contains 110 components and 2.20707 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.116559Jy sigma=0.712994 ! Fit after self-cal, rms=0.116493Jy sigma=0.712601 ! Inverting map ! Your choice of large map pixels excluded 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.116493Jy sigma=0.712601 ! Fit after self-cal, rms=0.116106Jy sigma=0.710774 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 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 milli-arcsec ! Estimated beam: bmin=0.5377 mas, bmaj=0.79 mas, bpa=3.077 degrees ! Estimated noise=1.76286 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.36664 Jy ! Component: 100 - total flux cleaned = 1.78536 Jy ! Component: 150 - total flux cleaned = 1.97646 Jy ! Component: 200 - total flux cleaned = 2.07185 Jy ! Total flux subtracted in 200 components = 2.07185 Jy ! Clean residual min=-0.025552 max=0.045966 Jy/beam ! Clean residual mean=0.000053 rms=0.003025 Jy/beam ! Combined flux in latest and established models = 2.07185 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 11 model components to the UV plane model. ! The established model now contains 11 components and 2.07185 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 milli-arcsec ! Estimated beam: bmin=0.5489 mas, bmaj=1.031 mas, bpa=-3.295 degrees ! Estimated noise=1.26105 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 = 0.0632277 Jy ! Component: 100 - total flux cleaned = 0.0928777 Jy ! Component: 150 - total flux cleaned = 0.109604 Jy ! Component: 200 - total flux cleaned = 0.114083 Jy ! Total flux subtracted in 200 components = 0.114083 Jy ! Clean residual min=-0.008108 max=0.007609 Jy/beam ! Clean residual mean=0.000778 rms=0.001343 Jy/beam ! Combined flux in latest and established models = 2.18594 Jy ! Adding 27 model components to the UV plane model. ! The established model now contains 31 components and 2.18594 Jy ! Inverting map ! Your choice of large map pixels excluded 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 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 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 milli-arcsec ! Estimated beam: bmin=2.375 mas, bmaj=3.258 mas, bpa=-12.05 degrees ! Estimated noise=1.86795 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00995652 Jy ! Component: 100 - total flux cleaned = 0.0138036 Jy ! Component: 150 - total flux cleaned = 0.0171811 Jy ! Component: 200 - total flux cleaned = 0.0198361 Jy ! Total flux subtracted in 200 components = 0.0198361 Jy ! Clean residual min=-0.004107 max=0.006315 Jy/beam ! Clean residual mean=0.001276 rms=0.001480 Jy/beam ! Combined flux in latest and established models = 2.20577 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) ! Added new window around map position (45, 28.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00553768 Jy ! Component: 100 - total flux cleaned = 0.00738705 Jy ! Component: 150 - total flux cleaned = 0.00875924 Jy ! Component: 200 - total flux cleaned = 0.00998769 Jy ! Total flux subtracted in 200 components = 0.00998769 Jy ! Clean residual min=-0.003986 max=0.005456 Jy/beam ! Clean residual mean=0.000745 rms=0.001376 Jy/beam ! Combined flux in latest and established models = 2.21576 Jy ! Adding 82 model components to the UV plane model. ! The established model now contains 110 components and 2.21576 Jy ! Inverting map ! Your choice of large map pixels excluded 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 milli-arcsec ! Estimated beam: bmin=0.5489 mas, bmaj=1.031 mas, bpa=-3.295 degrees ! Estimated noise=1.26105 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00446357 Jy ! Component: 100 - total flux cleaned = -0.00502338 Jy ! Component: 150 - total flux cleaned = -0.0044834 Jy ! Component: 200 - total flux cleaned = -0.00424057 Jy ! Total flux subtracted in 200 components = -0.00424057 Jy ! Clean residual min=-0.006241 max=0.005211 Jy/beam ! Clean residual mean=0.000347 rms=0.001100 Jy/beam ! Combined flux in latest and established models = 2.21152 Jy selfcal ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 130 components and 2.21152 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.117540Jy sigma=0.740616 ! Fit after self-cal, rms=0.116577Jy sigma=0.735119 wmodel J0501-0159_X_map.mod ! Writing 130 model components to file: J0501-0159_X_map.mod wobs J0501-0159_X_uvs.fits ! Writing UV FITS file: J0501-0159_X_uvs.fits wwins J0501-0159_X_map.win ! wwins: Wrote 3 windows to J0501-0159_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 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000186891 Jy ! Component: 100 - total flux cleaned = 0.000384725 Jy ! Component: 150 - total flux cleaned = 0.00110505 Jy ! Component: 200 - total flux cleaned = 0.00180118 Jy ! Component: 250 - total flux cleaned = 0.00247987 Jy ! Component: 300 - total flux cleaned = 0.00322746 Jy ! Component: 350 - total flux cleaned = 0.00403993 Jy ! Component: 400 - total flux cleaned = 0.00475688 Jy ! Component: 450 - total flux cleaned = 0.00561626 Jy ! Component: 500 - total flux cleaned = 0.00638352 Jy ! Component: 550 - total flux cleaned = 0.007063 Jy ! Component: 600 - total flux cleaned = 0.00758314 Jy ! Component: 650 - total flux cleaned = 0.00794982 Jy ! Component: 700 - total flux cleaned = 0.00845679 Jy ! Component: 750 - total flux cleaned = 0.00874272 Jy ! Component: 800 - total flux cleaned = 0.00909695 Jy ! Component: 850 - total flux cleaned = 0.00944709 Jy ! Component: 900 - total flux cleaned = 0.00972464 Jy ! Component: 950 - total flux cleaned = 0.00993076 Jy ! Component: 1000 - total flux cleaned = 0.0102028 Jy ! Component: 1050 - total flux cleaned = 0.0104053 Jy ! Component: 1100 - total flux cleaned = 0.0106061 Jy ! Component: 1150 - total flux cleaned = 0.01054 Jy ! Component: 1200 - total flux cleaned = 0.0109356 Jy ! Component: 1250 - total flux cleaned = 0.0110665 Jy ! Component: 1300 - total flux cleaned = 0.0111959 Jy ! Component: 1350 - total flux cleaned = 0.0113887 Jy ! Component: 1400 - total flux cleaned = 0.011516 Jy ! Component: 1450 - total flux cleaned = 0.0116424 Jy ! Component: 1500 - total flux cleaned = 0.0117677 Jy ! Component: 1550 - total flux cleaned = 0.0117678 Jy ! Component: 1600 - total flux cleaned = 0.0118915 Jy ! Component: 1650 - total flux cleaned = 0.011953 Jy ! Component: 1700 - total flux cleaned = 0.012014 Jy ! Component: 1750 - total flux cleaned = 0.012075 Jy ! Component: 1800 - total flux cleaned = 0.0121355 Jy ! Component: 1850 - total flux cleaned = 0.012256 Jy ! Component: 1900 - total flux cleaned = 0.0123756 Jy ! Component: 1950 - total flux cleaned = 0.0123755 Jy ! Component: 2000 - total flux cleaned = 0.0124346 Jy ! Component: 2050 - total flux cleaned = 0.0124933 Jy ! Component: 2100 - total flux cleaned = 0.01261 Jy ! Component: 2150 - total flux cleaned = 0.0126102 Jy ! Component: 2200 - total flux cleaned = 0.0127257 Jy ! Component: 2250 - total flux cleaned = 0.0127831 Jy ! Component: 2300 - total flux cleaned = 0.0128974 Jy ! Component: 2350 - total flux cleaned = 0.012954 Jy ! Component: 2400 - total flux cleaned = 0.0128976 Jy ! Component: 2450 - total flux cleaned = 0.0130661 Jy ! Component: 2500 - total flux cleaned = 0.0130662 Jy ! Component: 2550 - total flux cleaned = 0.0131776 Jy ! Component: 2600 - total flux cleaned = 0.013288 Jy ! Component: 2650 - total flux cleaned = 0.0132881 Jy ! Component: 2700 - total flux cleaned = 0.0133429 Jy ! Component: 2750 - total flux cleaned = 0.0134519 Jy ! Component: 2800 - total flux cleaned = 0.0135062 Jy ! Component: 2850 - total flux cleaned = 0.0135602 Jy ! Component: 2900 - total flux cleaned = 0.0136675 Jy ! Component: 2950 - total flux cleaned = 0.0136674 Jy ! Component: 3000 - total flux cleaned = 0.0137737 Jy ! Component: 3050 - total flux cleaned = 0.0138268 Jy ! Component: 3100 - total flux cleaned = 0.0138269 Jy ! Component: 3150 - total flux cleaned = 0.0138791 Jy ! Component: 3200 - total flux cleaned = 0.0139312 Jy ! Component: 3250 - total flux cleaned = 0.0140352 Jy ! Component: 3300 - total flux cleaned = 0.0140869 Jy ! Component: 3350 - total flux cleaned = 0.0140869 Jy ! Component: 3400 - total flux cleaned = 0.0141381 Jy ! Component: 3450 - total flux cleaned = 0.014189 Jy ! Component: 3500 - total flux cleaned = 0.0142909 Jy ! Component: 3550 - total flux cleaned = 0.0142909 Jy ! Component: 3600 - total flux cleaned = 0.014291 Jy ! Component: 3650 - total flux cleaned = 0.0143413 Jy ! Component: 3700 - total flux cleaned = 0.0144414 Jy ! Component: 3750 - total flux cleaned = 0.0144416 Jy ! Component: 3800 - total flux cleaned = 0.0145407 Jy ! Component: 3850 - total flux cleaned = 0.0146394 Jy ! Component: 3900 - total flux cleaned = 0.0146884 Jy ! Component: 3950 - total flux cleaned = 0.0146881 Jy ! Component: 4000 - total flux cleaned = 0.014688 Jy ! Component: 4050 - total flux cleaned = 0.0146882 Jy ! Total flux subtracted in 4096 components = 0.0147368 Jy ! Clean residual min=-0.002755 max=0.002756 Jy/beam ! Clean residual mean=0.000091 rms=0.000756 Jy/beam ! Combined flux in latest and established models = 2.22626 Jy keep ! Adding 302 model components to the UV plane model. ! The established model now contains 419 components and 2.22626 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv123_uvs/J0501-0159_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5489 x 1.031 at -3.295 degrees (North through East) ! Clean map min=-0.0060459 max=1.7329 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv123_uvs/J0501-0159_X_map.fits wmodel /scr/pima/rv123_uvs/J0501-0159_X_map.mod ! Writing 419 model components to file: /scr/pima/rv123_uvs/J0501-0159_X_map.mod wobs /scr/pima/rv123_uvs/J0501-0159_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv123_uvs/J0501-0159_X_uvs.fits wwins /scr/pima/rv123_uvs/J0501-0159_X_map.win ! wwins: Wrote 4 windows to /scr/pima/rv123_uvs/J0501-0159_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 1.73294 invert ! Inverting map ! Your choice of large map pixels excluded 3.5% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1965 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000756165 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.130905 0.130905 0.261809 0.523619 1.04724 2.09448 4.18895 8.3779 16.7558 33.5116 67.0232 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0022 print "peak= ", int(1000*peak_flux)/1000 ! peak= 1.732 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 2291.74 quit ! Quitting program ! Log file /scr/pima/rv123_uvs/J0501-0159_X_dfm.log closed on Sun Dec 23 00:40:06 2018