! Started logfile: /scr/pima/rv122_uvs/J0239-0234_X_dfm.log on Fri Jul 13 21:06:24 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/rv122_uvs/J0239-0234_X_uva.fits ! Reading UV FITS file: /scr/pima/rv122_uvs/J0239-0234_X_uva.fits ! AN table 1: 4 integrations on 28 of 28 possible baselines. ! AN table 2: 4 integrations on 28 of 28 possible baselines. ! AN table 3: 5 integrations on 21 of 21 possible baselines. ! AN table 4: 39 integrations on 15 of 15 possible baselines. ! AN table 5: 102 integrations on 55 of 55 possible baselines. ! Apparent sampling: 0.155273 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 69 lines of history. ! ! Reading 4052 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 10 telescope corrections were flagged in sub-array 1. ! A total of 2 telescope corrections were flagged in sub-array 2. ! A total of 11 telescope corrections were flagged in sub-array 3. ! A total of 132 telescope corrections were flagged in sub-array 4. ! A total of 917 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 10 telescope corrections were flagged in sub-array 1. ! A total of 2 telescope corrections were flagged in sub-array 2. ! A total of 11 telescope corrections were flagged in sub-array 3. ! A total of 132 telescope corrections were flagged in sub-array 4. ! A total of 917 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 10 telescope corrections were flagged in sub-array 1. ! A total of 2 telescope corrections were flagged in sub-array 2. ! A total of 11 telescope corrections were flagged in sub-array 3. ! A total of 132 telescope corrections were flagged in sub-array 4. ! A total of 917 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 10 telescope corrections were flagged in sub-array 1. ! A total of 2 telescope corrections were flagged in sub-array 2. ! A total of 11 telescope corrections were flagged in sub-array 3. ! A total of 132 telescope corrections were flagged in sub-array 4. ! A total of 917 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=1.215185Jy sigma=15.084060 ! Fit after self-cal, rms=0.337102Jy sigma=3.957233 ! 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 4.46% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=0.6271 mas, bmaj=0.854 mas, bpa=1.78 degrees ! Estimated noise=1.36539 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 = 0.53017 Jy ! Component: 100 - total flux cleaned = 0.647677 Jy ! Total flux subtracted in 100 components = 0.647677 Jy ! Clean residual min=-0.016696 max=0.044979 Jy/beam ! Clean residual mean=-0.000041 rms=0.003299 Jy/beam ! Combined flux in latest and established models = 0.647677 Jy ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 4 components and 0.647677 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.147355Jy sigma=1.582164 ! Fit after self-cal, rms=0.147349Jy sigma=1.581998 ! Inverting map ! Your choice of large map pixels excluded 4.46% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 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 = 0.0438507 Jy ! Component: 100 - total flux cleaned = 0.0664458 Jy ! Total flux subtracted in 100 components = 0.0664458 Jy ! Clean residual min=-0.011812 max=0.021124 Jy/beam ! Clean residual mean=-0.000030 rms=0.002575 Jy/beam ! Combined flux in latest and established models = 0.714122 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 10 components and 0.714122 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.125306Jy sigma=1.275104 ! Fit after self-cal, rms=0.124852Jy sigma=1.269327 ! Inverting map ! Your choice of large map pixels excluded 4.46% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 milli-arcsec ! Added new window around map position (0, -1.6). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0166127 Jy ! Component: 100 - total flux cleaned = 0.0262442 Jy ! Total flux subtracted in 100 components = 0.0262442 Jy ! Clean residual min=-0.011240 max=0.014933 Jy/beam ! Clean residual mean=-0.000025 rms=0.002414 Jy/beam ! Combined flux in latest and established models = 0.740367 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 13 components and 0.740367 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.120562Jy sigma=1.209756 ! Fit after self-cal, rms=0.120181Jy sigma=1.205634 ! Inverting map ! Your choice of large map pixels excluded 4.46% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 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 4.46% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=0.7297 mas, bmaj=0.8427 mas, bpa=16.92 degrees ! Estimated noise=1.11254 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 (-1.6, -1.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0198492 Jy ! Component: 100 - total flux cleaned = 0.0305254 Jy ! Component: 150 - total flux cleaned = 0.03684 Jy ! Component: 200 - total flux cleaned = 0.0375788 Jy ! Total flux subtracted in 200 components = 0.0375788 Jy ! Clean residual min=-0.012556 max=0.013097 Jy/beam ! Clean residual mean=-0.000038 rms=0.002687 Jy/beam ! Combined flux in latest and established models = 0.777945 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 31 components and 0.777945 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.116675Jy sigma=1.168248 ! Fit after self-cal, rms=0.116248Jy sigma=1.161875 ! Inverting map ! Your choice of large map pixels excluded 4.46% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 milli-arcsec print "============== Finished natural weighting clean ==============" ! ============== Finished natural weighting clean ============== ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7297 x 0.8427 at 16.92 degrees (North through East) ! Clean map min=-0.011125 max=0.66668 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.94 HN 1.10 KP 1.08 ! LA 1.04 MK 1.01 PT 0.93 SC 1.00 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 HN 1.05 KP 1.10 LA 1.06 ! MK 0.99 OV 0.97 PT 0.88 SC 1.00 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.04 FD 0.95 KP 1.04 LA 1.07 ! MK 0.95 OV 1.01 PT 0.93 ! ! A total of 30 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HH 1.00 HN 1.05 NY 0.98 ON 0.94 ! SC 1.00 WZ 0.93 ! ! A total of 111 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 FD 1.00 HH 1.11 HN 1.01 ! KP 1.09 LA 1.06 ON 0.99 OV 1.00 ! PT 0.90 SC 1.03 WZ 0.96 ! ! ! Correcting IF 2. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.95 HN 1.15 KP 1.09 ! LA 1.05 MK 1.02 PT 0.93 SC 0.99 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.05 HN 1.10 KP 1.10 LA 1.05 ! MK 0.98 OV 0.98 PT 0.90 SC 0.99 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.05 FD 0.90 KP 1.05 LA 1.06 ! MK 0.97 OV 0.99 PT 0.94 ! ! A total of 30 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HH 0.97 HN 1.12 NY 0.99 ON 0.94 ! SC 1.04 WZ 0.96 ! ! A total of 111 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.05 FD 1.01 HH 1.14 HN 1.00 ! KP 1.06 LA 1.09 ON 1.01 OV 1.02 ! PT 0.89 SC 1.02 WZ 0.94 ! ! ! Correcting IF 3. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 0.97 HN 1.14 KP 1.12 ! LA 1.04 MK 1.02 PT 0.92 SC 1.00 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 HN 1.09 KP 1.12 LA 1.06 ! MK 1.00 OV 0.98 PT 0.89 SC 1.02 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 0.94 KP 1.08 LA 1.09 ! MK 0.96 OV 1.00 PT 0.94 ! ! A total of 30 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HH 1.05 HN 1.04 NY 1.02 ON 0.97 ! SC 1.01 WZ 0.96 ! ! A total of 111 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.03 FD 1.02 HH 1.15 HN 1.00 ! KP 1.09 LA 1.10 ON 1.05 OV 1.00 ! PT 0.89 SC 1.01 WZ 0.98 ! ! ! Correcting IF 4. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.94 HN 1.17 KP 1.10 ! LA 1.08 MK 0.99 PT 0.93 SC 0.98 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 HN 1.12 KP 1.08 LA 1.05 ! MK 0.95 OV 0.98 PT 0.91 SC 1.03 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.04 FD 0.91 KP 1.09 LA 1.09 ! MK 0.96 OV 1.00 PT 0.98 ! ! A total of 30 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HH 1.04 HN 1.07 NY 0.95 ON 0.97 ! SC 0.96 WZ 0.99 ! ! A total of 111 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 FD 1.01 HH 1.14 HN 1.05 ! KP 1.09 LA 1.09 ON 0.97 OV 1.01 ! PT 0.87 SC 0.99 WZ 1.00 ! ! ! Fit before self-cal, rms=0.116248Jy sigma=1.161875 ! Fit after self-cal, rms=0.100323Jy sigma=0.921298 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=0.6857 mas, bmaj=0.9938 mas, bpa=4.035 degrees ! Estimated noise=1.19588 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 = -0.00164815 Jy ! Component: 100 - total flux cleaned = -0.00212527 Jy ! Component: 150 - total flux cleaned = -0.00226566 Jy ! Component: 200 - total flux cleaned = -0.0026404 Jy ! Total flux subtracted in 200 components = -0.0026404 Jy ! Clean residual min=-0.007060 max=0.005882 Jy/beam ! Clean residual mean=-0.000013 rms=0.001262 Jy/beam ! Combined flux in latest and established models = 0.775305 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 41 components and 0.775305 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.099798Jy sigma=0.915941 ! Fit after self-cal, rms=0.099906Jy sigma=0.915120 ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 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=0.099906Jy sigma=0.915120 ! Fit after self-cal, rms=0.098498Jy sigma=0.896466 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=0.6859 mas, bmaj=0.9941 mas, bpa=3.955 degrees ! Estimated noise=1.19522 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0019428 Jy ! Component: 100 - total flux cleaned = -0.00257786 Jy ! Component: 150 - total flux cleaned = -0.00304873 Jy ! Component: 200 - total flux cleaned = -0.0032224 Jy ! Total flux subtracted in 200 components = -0.0032224 Jy ! Clean residual min=-0.005458 max=0.005010 Jy/beam ! Clean residual mean=-0.000009 rms=0.001094 Jy/beam ! Combined flux in latest and established models = 0.772083 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 51 components and 0.772083 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.098217Jy sigma=0.893736 ! Fit after self-cal, rms=0.098150Jy sigma=0.893278 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 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 = -0.000312221 Jy ! Component: 100 - total flux cleaned = -0.00074785 Jy ! Component: 150 - total flux cleaned = -0.000982068 Jy ! Component: 200 - total flux cleaned = -0.00112756 Jy ! Total flux subtracted in 200 components = -0.00112756 Jy ! Clean residual min=-0.005085 max=0.004880 Jy/beam ! Clean residual mean=-0.000009 rms=0.001083 Jy/beam ! Combined flux in latest and established models = 0.770955 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 52 components and 0.770955 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.097940Jy sigma=0.891733 ! Fit after self-cal, rms=0.097898Jy sigma=0.891486 ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 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=0.097898Jy sigma=0.891486 ! Fit after self-cal, rms=0.096974Jy sigma=0.878133 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=0.6851 mas, bmaj=0.9909 mas, bpa=4.061 degrees ! Estimated noise=1.19436 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 5.18972e-05 Jy ! Component: 100 - total flux cleaned = -0.000389846 Jy ! Component: 150 - total flux cleaned = -0.000467256 Jy ! Component: 200 - total flux cleaned = -0.000608411 Jy ! Total flux subtracted in 200 components = -0.000608411 Jy ! Clean residual min=-0.004570 max=0.004086 Jy/beam ! Clean residual mean=-0.000003 rms=0.000982 Jy/beam ! Combined flux in latest and established models = 0.770346 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 56 components and 0.770346 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.096735Jy sigma=0.876456 ! Fit after self-cal, rms=0.096699Jy sigma=0.876125 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 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 = -0.000148546 Jy ! Component: 100 - total flux cleaned = -0.000426707 Jy ! Component: 150 - total flux cleaned = -0.000554813 Jy ! Component: 200 - total flux cleaned = -0.000673641 Jy ! Total flux subtracted in 200 components = -0.000673641 Jy ! Clean residual min=-0.004497 max=0.004056 Jy/beam ! Clean residual mean=-0.000003 rms=0.000975 Jy/beam ! Combined flux in latest and established models = 0.769673 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 56 components and 0.769673 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.096556Jy sigma=0.875205 ! Fit after self-cal, rms=0.096533Jy sigma=0.875073 ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 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=0.096533Jy sigma=0.875073 ! Fit after self-cal, rms=0.096451Jy sigma=0.874751 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=2.653 mas, bmaj=3.334 mas, bpa=11.85 degrees ! Estimated noise=1.57424 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00125721 Jy ! Component: 100 - total flux cleaned = -0.00144103 Jy ! Component: 150 - total flux cleaned = -0.00158873 Jy ! Component: 200 - total flux cleaned = -0.0017062 Jy ! Total flux subtracted in 200 components = -0.0017062 Jy ! Clean residual min=-0.004156 max=0.003830 Jy/beam ! Clean residual mean=-0.000008 rms=0.001159 Jy/beam ! Combined flux in latest and established models = 0.767967 Jy selfcal ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 61 components and 0.767967 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.096435Jy sigma=0.874854 ! Fit after self-cal, rms=0.096414Jy sigma=0.874671 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 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 = -0.000474202 Jy ! Component: 100 - total flux cleaned = -0.000584865 Jy ! Component: 150 - total flux cleaned = -0.000672417 Jy ! Component: 200 - total flux cleaned = -0.000720576 Jy ! Total flux subtracted in 200 components = -0.000720576 Jy ! Clean residual min=-0.004242 max=0.003869 Jy/beam ! Clean residual mean=-0.000009 rms=0.001157 Jy/beam ! Combined flux in latest and established models = 0.767246 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 63 components and 0.767246 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.096438Jy sigma=0.875251 ! Fit after self-cal, rms=0.096431Jy sigma=0.875171 ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 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 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=0.6848 mas, bmaj=0.9895 mas, bpa=4.073 degrees ! Estimated noise=1.19496 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6848 x 0.9895 at 4.073 degrees (North through East) ! Clean map min=-0.0051083 max=0.66807 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=0.096431Jy sigma=0.875171 ! Fit after self-cal, rms=0.088370Jy sigma=0.776503 ! Inverting map and beam ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=0.6846 mas, bmaj=0.9895 mas, bpa=4.149 degrees ! Estimated noise=1.19452 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000651022 Jy ! Component: 100 - total flux cleaned = 0.000649673 Jy ! Component: 150 - total flux cleaned = 0.000581453 Jy ! Component: 200 - total flux cleaned = 0.000583069 Jy ! Total flux subtracted in 200 components = 0.000583069 Jy ! Clean residual min=-0.004117 max=0.003973 Jy/beam ! Clean residual mean=-0.000004 rms=0.000963 Jy/beam ! Combined flux in latest and established models = 0.767829 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 63 components and 0.767829 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.088202Jy sigma=0.775325 ! Fit after self-cal, rms=0.088176Jy sigma=0.775195 ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 2.709e-05 Jy ! Component: 100 - total flux cleaned = -3.28392e-05 Jy ! Component: 150 - total flux cleaned = -3.36332e-05 Jy ! Component: 200 - total flux cleaned = -8.33462e-05 Jy ! Total flux subtracted in 200 components = -8.33462e-05 Jy ! Clean residual min=-0.004050 max=0.003934 Jy/beam ! Clean residual mean=-0.000004 rms=0.000959 Jy/beam ! Combined flux in latest and established models = 0.767746 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 65 components and 0.767746 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.088066Jy sigma=0.774505 ! Fit after self-cal, rms=0.088052Jy sigma=0.774438 ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.088052Jy sigma=0.774438 ! Fit after self-cal, rms=0.088066Jy sigma=0.774209 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 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=0.6003 mas, bmaj=1.003 mas, bpa=-0.7446 degrees ! Estimated noise=1.46255 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.531836 Jy ! Component: 100 - total flux cleaned = 0.655151 Jy ! Component: 150 - total flux cleaned = 0.700806 Jy ! Component: 200 - total flux cleaned = 0.723549 Jy ! Total flux subtracted in 200 components = 0.723549 Jy ! Clean residual min=-0.007121 max=0.012429 Jy/beam ! Clean residual mean=-0.000007 rms=0.001515 Jy/beam ! Combined flux in latest and established models = 0.723549 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 10 model components to the UV plane model. ! The established model now contains 10 components and 0.723549 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=0.6844 mas, bmaj=0.9889 mas, bpa=4.116 degrees ! Estimated noise=1.19522 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 = 0.0208204 Jy ! Component: 100 - total flux cleaned = 0.0325178 Jy ! Component: 150 - total flux cleaned = 0.0378876 Jy ! Component: 200 - total flux cleaned = 0.038989 Jy ! Total flux subtracted in 200 components = 0.038989 Jy ! Clean residual min=-0.004861 max=0.005212 Jy/beam ! Clean residual mean=-0.000005 rms=0.001057 Jy/beam ! Combined flux in latest and established models = 0.762538 Jy ! Adding 22 model components to the UV plane model. ! The established model now contains 27 components and 0.762538 Jy ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 milli-arcsec ! Added new window around map position (0, 1). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00207261 Jy ! Component: 100 - total flux cleaned = 0.00257874 Jy ! Component: 150 - total flux cleaned = 0.00300888 Jy ! Component: 200 - total flux cleaned = 0.00337989 Jy ! Total flux subtracted in 200 components = 0.00337989 Jy ! Clean residual min=-0.004436 max=0.004195 Jy/beam ! Clean residual mean=-0.000004 rms=0.000981 Jy/beam ! Combined flux in latest and established models = 0.765918 Jy ! Adding 13 model components to the UV plane model. ! The established model now contains 36 components and 0.765918 Jy ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 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 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=2.654 mas, bmaj=3.335 mas, bpa=12.11 degrees ! Estimated noise=1.57505 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000998497 Jy ! Component: 100 - total flux cleaned = 0.000937988 Jy ! Component: 150 - total flux cleaned = 0.000892182 Jy ! Component: 200 - total flux cleaned = 0.000852511 Jy ! Total flux subtracted in 200 components = 0.000852511 Jy ! Clean residual min=-0.004147 max=0.003677 Jy/beam ! Clean residual mean=-0.000010 rms=0.001151 Jy/beam ! Combined flux in latest and established models = 0.766771 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 = -3.25337e-05 Jy ! Component: 100 - total flux cleaned = -6.0716e-05 Jy ! Component: 150 - total flux cleaned = -8.56507e-05 Jy ! Component: 200 - total flux cleaned = -0.000108059 Jy ! Total flux subtracted in 200 components = -0.000108059 Jy ! Clean residual min=-0.004213 max=0.003712 Jy/beam ! Clean residual mean=-0.000010 rms=0.001144 Jy/beam ! Combined flux in latest and established models = 0.766662 Jy ! Adding 20 model components to the UV plane model. ! The established model now contains 53 components and 0.766662 Jy ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 milli-arcsec ! Estimated beam: bmin=0.6844 mas, bmaj=0.9889 mas, bpa=4.116 degrees ! Estimated noise=1.19522 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000232086 Jy ! Component: 100 - total flux cleaned = 0.000234739 Jy ! Component: 150 - total flux cleaned = 0.00031463 Jy ! Component: 200 - total flux cleaned = 0.00031183 Jy ! Total flux subtracted in 200 components = 0.00031183 Jy ! Clean residual min=-0.004574 max=0.003847 Jy/beam ! Clean residual mean=-0.000004 rms=0.000962 Jy/beam ! Combined flux in latest and established models = 0.766974 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 62 components and 0.766974 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.087945Jy sigma=0.774384 ! Fit after self-cal, rms=0.087861Jy sigma=0.773156 wmodel J0239-0234_X_map.mod ! Writing 62 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 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000940604 Jy ! Component: 100 - total flux cleaned = -0.00115573 Jy ! Component: 150 - total flux cleaned = -0.00157312 Jy ! Component: 200 - total flux cleaned = -0.00164258 Jy ! Component: 250 - total flux cleaned = -0.00197818 Jy ! Component: 300 - total flux cleaned = -0.00204205 Jy ! Component: 350 - total flux cleaned = -0.00204121 Jy ! Component: 400 - total flux cleaned = -0.00197786 Jy ! Component: 450 - total flux cleaned = -0.00210317 Jy ! Component: 500 - total flux cleaned = -0.00216474 Jy ! Component: 550 - total flux cleaned = -0.0022246 Jy ! Component: 600 - total flux cleaned = -0.00216478 Jy ! Component: 650 - total flux cleaned = -0.00210569 Jy ! Component: 700 - total flux cleaned = -0.00228168 Jy ! Component: 750 - total flux cleaned = -0.00228137 Jy ! Component: 800 - total flux cleaned = -0.00239524 Jy ! Component: 850 - total flux cleaned = -0.00228242 Jy ! Component: 900 - total flux cleaned = -0.00233841 Jy ! Component: 950 - total flux cleaned = -0.00239298 Jy ! Component: 1000 - total flux cleaned = -0.00212018 Jy ! Component: 1050 - total flux cleaned = -0.00228211 Jy ! Component: 1100 - total flux cleaned = -0.00206671 Jy ! Component: 1150 - total flux cleaned = -0.00196049 Jy ! Component: 1200 - total flux cleaned = -0.00190737 Jy ! Component: 1250 - total flux cleaned = -0.00175081 Jy ! Component: 1300 - total flux cleaned = -0.00159532 Jy ! Component: 1350 - total flux cleaned = -0.00144141 Jy ! Component: 1400 - total flux cleaned = -0.0013913 Jy ! Component: 1450 - total flux cleaned = -0.00128994 Jy ! Component: 1500 - total flux cleaned = -0.0013405 Jy ! Component: 1550 - total flux cleaned = -0.00119066 Jy ! Component: 1600 - total flux cleaned = -0.000993417 Jy ! Component: 1650 - total flux cleaned = -0.000895374 Jy ! Component: 1700 - total flux cleaned = -0.000797677 Jy ! Component: 1750 - total flux cleaned = -0.00099113 Jy ! Component: 1800 - total flux cleaned = -0.000943027 Jy ! Component: 1850 - total flux cleaned = -0.000895288 Jy ! Component: 1900 - total flux cleaned = -0.00103774 Jy ! Component: 1950 - total flux cleaned = -0.00103736 Jy ! Component: 2000 - total flux cleaned = -0.0010378 Jy ! Component: 2050 - total flux cleaned = -0.00103782 Jy ! Component: 2100 - total flux cleaned = -0.0010842 Jy ! Component: 2150 - total flux cleaned = -0.00103815 Jy ! Component: 2200 - total flux cleaned = -0.00126584 Jy ! Component: 2250 - total flux cleaned = -0.00122047 Jy ! Component: 2300 - total flux cleaned = -0.00122066 Jy ! Component: 2350 - total flux cleaned = -0.00104141 Jy ! Component: 2400 - total flux cleaned = -0.00108626 Jy ! Component: 2450 - total flux cleaned = -0.00121917 Jy ! Component: 2500 - total flux cleaned = -0.00108701 Jy ! Component: 2550 - total flux cleaned = -0.00117507 Jy ! Component: 2600 - total flux cleaned = -0.00117509 Jy ! Component: 2650 - total flux cleaned = -0.00104518 Jy ! Component: 2700 - total flux cleaned = -0.000873039 Jy ! Component: 2750 - total flux cleaned = -0.000873138 Jy ! Component: 2800 - total flux cleaned = -0.00104352 Jy ! Component: 2850 - total flux cleaned = -0.00100144 Jy ! Component: 2900 - total flux cleaned = -0.00091721 Jy ! Component: 2950 - total flux cleaned = -0.000958992 Jy ! Component: 3000 - total flux cleaned = -0.000917587 Jy ! Component: 3050 - total flux cleaned = -0.000875937 Jy ! Component: 3100 - total flux cleaned = -0.000669914 Jy ! Component: 3150 - total flux cleaned = -0.000792784 Jy ! Component: 3200 - total flux cleaned = -0.000629778 Jy ! Component: 3250 - total flux cleaned = -0.000710708 Jy ! Component: 3300 - total flux cleaned = -0.000670413 Jy ! Component: 3350 - total flux cleaned = -0.000469565 Jy ! Component: 3400 - total flux cleaned = -0.00054987 Jy ! Component: 3450 - total flux cleaned = -0.00043067 Jy ! Component: 3500 - total flux cleaned = -0.000469913 Jy ! Component: 3550 - total flux cleaned = -0.000312898 Jy ! Component: 3600 - total flux cleaned = -0.000312845 Jy ! Component: 3650 - total flux cleaned = -0.000273755 Jy ! Component: 3700 - total flux cleaned = -0.000428645 Jy ! Component: 3750 - total flux cleaned = -0.000467094 Jy ! Component: 3800 - total flux cleaned = -0.000390294 Jy ! Component: 3850 - total flux cleaned = -0.000466687 Jy ! Component: 3900 - total flux cleaned = -0.000352511 Jy ! Component: 3950 - total flux cleaned = -0.00061731 Jy ! Component: 4000 - total flux cleaned = -0.000580011 Jy ! Component: 4050 - total flux cleaned = -0.000542133 Jy ! Total flux subtracted in 4096 components = -0.000766018 Jy ! Clean residual min=-0.002050 max=0.002341 Jy/beam ! Clean residual mean=0.000003 rms=0.000610 Jy/beam ! Combined flux in latest and established models = 0.766208 Jy keep ! Adding 328 model components to the UV plane model. ! The established model now contains 390 components and 0.766208 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv122_uvs/J0239-0234_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6844 x 0.9889 at 4.116 degrees (North through East) ! Clean map min=-0.0045739 max=0.66733 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv122_uvs/J0239-0234_X_map.fits wmodel /scr/pima/rv122_uvs/J0239-0234_X_map.mod ! Writing 390 model components to file: /scr/pima/rv122_uvs/J0239-0234_X_map.mod wobs /scr/pima/rv122_uvs/J0239-0234_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv122_uvs/J0239-0234_X_uvs.fits wwins /scr/pima/rv122_uvs/J0239-0234_X_map.win ! wwins: Wrote 6 windows to /scr/pima/rv122_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 0.667328 invert ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! The y-axis pixel size should ideally be below 0.1938 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000609303 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.273915 0.273915 0.547829 1.09566 2.19132 4.38263 8.76527 17.5305 35.0611 70.1221 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0018 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.667 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 1095.23 quit ! Quitting program ! Log file /scr/pima/rv122_uvs/J0239-0234_X_dfm.log closed on Fri Jul 13 21:06:28 2018