! Started logfile: /scr/pima/rv117_uvs/J0239-0234_X_dfm.log on Sat Dec 9 23:41:02 2017 float field_size field_size = 1024 float field_cell field_cell = 0.2000 float taper_size taper_size = 70.0 float freq freq = 8.36575 obs /scr/pima/rv117_uvs/J0239-0234_X_uva.fits ! Reading UV FITS file: /scr/pima/rv117_uvs/J0239-0234_X_uva.fits ! AN table 1: 12 integrations on 28 of 28 possible baselines. ! AN table 2: 45 integrations on 21 of 21 possible baselines. ! AN table 3: 96 integrations on 66 of 66 possible baselines. ! Apparent sampling: 0.176841 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 74 lines of history. ! ! Reading 5388 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 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 18 telescope corrections were flagged in sub-array 1. ! A total of 131 telescope corrections were flagged in sub-array 2. ! A total of 878 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 18 telescope corrections were flagged in sub-array 1. ! A total of 131 telescope corrections were flagged in sub-array 2. ! A total of 878 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 18 telescope corrections were flagged in sub-array 1. ! A total of 131 telescope corrections were flagged in sub-array 2. ! A total of 878 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 18 telescope corrections were flagged in sub-array 1. ! A total of 131 telescope corrections were flagged in sub-array 2. ! A total of 878 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=1.294652Jy sigma=16.679456 ! Fit after self-cal, rms=0.249829Jy sigma=2.972482 ! clrmod: Cleared the established, tentative and continuum models. ! Redundant starting model cleared. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.29% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec ! Estimated beam: bmin=0.6156 mas, bmaj=0.8114 mas, bpa=-10.9 degrees ! Estimated noise=1.07384 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 = 0.61407 Jy ! Component: 100 - total flux cleaned = 0.751768 Jy ! Total flux subtracted in 100 components = 0.751768 Jy ! Clean residual min=-0.020247 max=0.056068 Jy/beam ! Clean residual mean=0.000030 rms=0.003468 Jy/beam ! Combined flux in latest and established models = 0.751768 Jy ! Performing phase self-cal ! Adding 3 model components to the UV plane model. ! The established model now contains 3 components and 0.751768 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.153799Jy sigma=1.665201 ! Fit after self-cal, rms=0.153822Jy sigma=1.663986 ! Inverting map ! Your choice of large map pixels excluded 5.29% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 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 = 0.0543909 Jy ! Component: 100 - total flux cleaned = 0.0760431 Jy ! Total flux subtracted in 100 components = 0.0760431 Jy ! Clean residual min=-0.017810 max=0.026848 Jy/beam ! Clean residual mean=0.000025 rms=0.002633 Jy/beam ! Combined flux in latest and established models = 0.827811 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 10 components and 0.827811 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.131913Jy sigma=1.327806 ! Fit after self-cal, rms=0.130992Jy sigma=1.311878 ! Inverting map ! Your choice of large map pixels excluded 5.29% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0113441 Jy ! Component: 100 - total flux cleaned = 0.0132779 Jy ! Total flux subtracted in 100 components = 0.0132779 Jy ! Clean residual min=-0.013636 max=0.017817 Jy/beam ! Clean residual mean=0.000024 rms=0.002412 Jy/beam ! Combined flux in latest and established models = 0.841089 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 14 components and 0.841089 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.126600Jy sigma=1.266015 ! Fit after self-cal, rms=0.126325Jy sigma=1.262883 ! Inverting map ! Your choice of large map pixels excluded 5.29% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec ! Added new window around map position (1.2, -2.8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00832018 Jy ! Component: 100 - total flux cleaned = 0.00881401 Jy ! Total flux subtracted in 100 components = 0.00881401 Jy ! Clean residual min=-0.012018 max=0.014667 Jy/beam ! Clean residual mean=0.000023 rms=0.002301 Jy/beam ! Combined flux in latest and established models = 0.849903 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 17 components and 0.849903 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.123650Jy sigma=1.235016 ! Fit after self-cal, rms=0.123402Jy sigma=1.232612 ! Inverting map ! Your choice of large map pixels excluded 5.29% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec print "************** FINISHED UNIFORM WEIGHTING CLEAN **************" ! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** ! uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. win_mult = win_mult * 1.6 clean_niter = clean_niter * 2 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.29% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec ! Estimated beam: bmin=0.688 mas, bmaj=0.7879 mas, bpa=-11.44 degrees ! Estimated noise=0.861077 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 (-1.2, 2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.015472 Jy ! Component: 100 - total flux cleaned = 0.018172 Jy ! Component: 150 - total flux cleaned = 0.0208085 Jy ! Component: 200 - total flux cleaned = 0.0224235 Jy ! Total flux subtracted in 200 components = 0.0224235 Jy ! Clean residual min=-0.010835 max=0.011155 Jy/beam ! Clean residual mean=0.000037 rms=0.002111 Jy/beam ! Combined flux in latest and established models = 0.872326 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 26 components and 0.872326 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.120134Jy sigma=1.196344 ! Fit after self-cal, rms=0.119994Jy sigma=1.194854 ! Inverting map ! Your choice of large map pixels excluded 5.29% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.688 x 0.7879 at -11.44 degrees (North through East) ! Clean map min=-0.0088468 max=0.76889 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 1.00 KP 1.03 LA 1.02 ! MK 1.00 NL 1.02 OV 0.99 PT 1.01 ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 0.91 HN 1.07 NL 1.38 NY 1.04 ! ON 0.99 SC 1.03 WZ 1.00 ! ! A total of 174 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 0.97 HH 0.89 HN 0.94 ! KP 0.98 LA 0.98 NL 0.96 ON 1.00 ! OV 0.97 PT 0.99 SC 0.99 WZ 0.99 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 1.02 KP 1.03 LA 1.01 ! MK 1.00 NL 0.99 OV 0.98 PT 1.01 ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 0.92 HN 1.08 NL 1.34 NY 1.06 ! ON 0.99 SC 1.01 WZ 1.01 ! ! A total of 174 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 FD 0.98 HH 0.87 HN 0.95 ! KP 0.97 LA 0.97 NL 0.97 ON 1.00 ! OV 0.97 PT 0.98 SC 0.98 WZ 0.99 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 1.00 KP 1.01 LA 1.04 ! MK 1.00 NL 1.02 OV 1.00 PT 1.02 ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 0.99 HN 1.07 NL 1.37 NY 1.07 ! ON 1.00 SC 1.02 WZ 0.99 ! ! A total of 174 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 0.97 HH 0.99 HN 0.95 ! KP 0.97 LA 0.96 NL 0.97 ON 0.99 ! OV 0.98 PT 0.97 SC 0.97 WZ 1.00 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 1.00 KP 1.02 LA 1.04 ! MK 0.98 NL 1.02 OV 0.98 PT 1.02 ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 1.10 HN 1.05 NL 1.42 NY 1.08 ! ON 1.02 SC 1.03 WZ 0.98 ! ! A total of 174 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 FD 0.98 HH 1.08 HN 0.95 ! KP 0.98 LA 0.99 NL 0.97 ON 0.99 ! OV 0.99 PT 0.99 SC 0.96 WZ 1.00 ! ! ! Fit before self-cal, rms=0.119994Jy sigma=1.194854 ! Fit after self-cal, rms=0.100865Jy sigma=1.024146 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec ! Estimated beam: bmin=0.6518 mas, bmaj=0.9407 mas, bpa=-5.538 degrees ! Estimated noise=0.906769 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 = -0.000291872 Jy ! Component: 100 - total flux cleaned = -0.00163371 Jy ! Component: 150 - total flux cleaned = -0.00236056 Jy ! Component: 200 - total flux cleaned = -0.0026196 Jy ! Total flux subtracted in 200 components = -0.0026196 Jy ! Clean residual min=-0.005832 max=0.006201 Jy/beam ! Clean residual mean=0.000021 rms=0.001285 Jy/beam ! Combined flux in latest and established models = 0.869707 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 39 components and 0.869707 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.100134Jy sigma=1.017399 ! Fit after self-cal, rms=0.100180Jy sigma=1.016454 ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 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=0.100180Jy sigma=1.016454 ! Fit after self-cal, rms=0.096586Jy sigma=0.946905 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec ! Estimated beam: bmin=0.6509 mas, bmaj=0.9403 mas, bpa=-5.533 degrees ! Estimated noise=0.908276 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -4.91937e-05 Jy ! Component: 100 - total flux cleaned = -0.000575546 Jy ! Component: 150 - total flux cleaned = -0.000682856 Jy ! Component: 200 - total flux cleaned = -0.000784313 Jy ! Total flux subtracted in 200 components = -0.000784313 Jy ! Clean residual min=-0.004382 max=0.004572 Jy/beam ! Clean residual mean=0.000010 rms=0.000967 Jy/beam ! Combined flux in latest and established models = 0.868922 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 49 components and 0.868922 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.096142Jy sigma=0.943185 ! Fit after self-cal, rms=0.096139Jy sigma=0.942726 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 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 (13.8, 14.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00423811 Jy ! Component: 100 - total flux cleaned = 0.00501767 Jy ! Component: 150 - total flux cleaned = 0.00520346 Jy ! Component: 200 - total flux cleaned = 0.00528758 Jy ! Total flux subtracted in 200 components = 0.00528758 Jy ! Clean residual min=-0.004352 max=0.004168 Jy/beam ! Clean residual mean=0.000013 rms=0.000940 Jy/beam ! Combined flux in latest and established models = 0.87421 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 57 components and 0.87421 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.095810Jy sigma=0.938932 ! Fit after self-cal, rms=0.095802Jy sigma=0.938645 ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 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=0.095802Jy sigma=0.938645 ! Fit after self-cal, rms=0.093620Jy sigma=0.891955 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec ! Estimated beam: bmin=0.6507 mas, bmaj=0.9394 mas, bpa=-5.514 degrees ! Estimated noise=0.908772 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -4.05968e-05 Jy ! Component: 100 - total flux cleaned = -0.000215248 Jy ! Component: 150 - total flux cleaned = -0.000377104 Jy ! Component: 200 - total flux cleaned = -0.000532551 Jy ! Total flux subtracted in 200 components = -0.000532551 Jy ! Clean residual min=-0.003190 max=0.003547 Jy/beam ! Clean residual mean=0.000009 rms=0.000726 Jy/beam ! Combined flux in latest and established models = 0.873678 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 63 components and 0.873678 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.093421Jy sigma=0.890435 ! Fit after self-cal, rms=0.093434Jy sigma=0.890295 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 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 (1, -5.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00244529 Jy ! Component: 100 - total flux cleaned = 0.00307284 Jy ! Component: 150 - total flux cleaned = 0.00284798 Jy ! Component: 200 - total flux cleaned = 0.00270776 Jy ! Total flux subtracted in 200 components = 0.00270776 Jy ! Clean residual min=-0.003090 max=0.002960 Jy/beam ! Clean residual mean=0.000008 rms=0.000704 Jy/beam ! Combined flux in latest and established models = 0.876385 Jy ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 78 components and 0.876385 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.093249Jy sigma=0.887948 ! Fit after self-cal, rms=0.093238Jy sigma=0.887807 ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 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=0.093238Jy sigma=0.887807 ! Fit after self-cal, rms=0.093235Jy sigma=0.887472 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec ! Estimated beam: bmin=2.746 mas, bmaj=3.331 mas, bpa=-4.625 degrees ! Estimated noise=1.1793 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000782688 Jy ! Component: 100 - total flux cleaned = 0.000776846 Jy ! Component: 150 - total flux cleaned = 0.000773209 Jy ! Component: 200 - total flux cleaned = 0.000734893 Jy ! Total flux subtracted in 200 components = 0.000734893 Jy ! Clean residual min=-0.003216 max=0.002865 Jy/beam ! Clean residual mean=0.000019 rms=0.000795 Jy/beam ! Combined flux in latest and established models = 0.87712 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 87 components and 0.87712 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.093185Jy sigma=0.886932 ! Fit after self-cal, rms=0.093171Jy sigma=0.886859 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 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 = 0.000159542 Jy ! Component: 100 - total flux cleaned = 0.000228073 Jy ! Component: 150 - total flux cleaned = 0.00019957 Jy ! Component: 200 - total flux cleaned = 0.000200388 Jy ! Total flux subtracted in 200 components = 0.000200388 Jy ! Clean residual min=-0.003141 max=0.002878 Jy/beam ! Clean residual mean=0.000019 rms=0.000790 Jy/beam ! Combined flux in latest and established models = 0.877321 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 91 components and 0.877321 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.093137Jy sigma=0.886658 ! Fit after self-cal, rms=0.093122Jy sigma=0.886627 ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 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 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec ! Estimated beam: bmin=0.6506 mas, bmaj=0.9387 mas, bpa=-5.506 degrees ! Estimated noise=0.909106 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6506 x 0.9387 at -5.506 degrees (North through East) ! Clean map min=-0.0045594 max=0.7685 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=0.093122Jy sigma=0.886627 ! Fit after self-cal, rms=0.084438Jy sigma=0.770957 ! Inverting map and beam ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec ! Estimated beam: bmin=0.6502 mas, bmaj=0.938 mas, bpa=-5.436 degrees ! Estimated noise=0.909424 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000253728 Jy ! Component: 100 - total flux cleaned = -3.01051e-06 Jy ! Component: 150 - total flux cleaned = -0.000118877 Jy ! Component: 200 - total flux cleaned = -0.000175135 Jy ! Total flux subtracted in 200 components = -0.000175135 Jy ! Clean residual min=-0.002917 max=0.003002 Jy/beam ! Clean residual mean=0.000009 rms=0.000682 Jy/beam ! Combined flux in latest and established models = 0.877146 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 99 components and 0.877145 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.084297Jy sigma=0.769952 ! Fit after self-cal, rms=0.084301Jy sigma=0.769898 ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec ! Added new window around map position (49.2, 33.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00257377 Jy ! Component: 100 - total flux cleaned = 0.00289796 Jy ! Component: 150 - total flux cleaned = 0.00278635 Jy ! Component: 200 - total flux cleaned = 0.00273258 Jy ! Total flux subtracted in 200 components = 0.00273258 Jy ! Clean residual min=-0.002941 max=0.002991 Jy/beam ! Clean residual mean=0.000010 rms=0.000672 Jy/beam ! Combined flux in latest and established models = 0.879878 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 110 components and 0.879878 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.084122Jy sigma=0.768644 ! Fit after self-cal, rms=0.084122Jy sigma=0.768542 ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.084122Jy sigma=0.768542 ! Fit after self-cal, rms=0.084130Jy sigma=0.768333 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 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec ! Estimated beam: bmin=0.5955 mas, bmaj=0.9556 mas, bpa=-7.27 degrees ! Estimated noise=1.1193 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.608167 Jy ! Component: 100 - total flux cleaned = 0.750091 Jy ! Component: 150 - total flux cleaned = 0.806967 Jy ! Component: 200 - total flux cleaned = 0.833632 Jy ! Total flux subtracted in 200 components = 0.833632 Jy ! Clean residual min=-0.006645 max=0.014763 Jy/beam ! Clean residual mean=0.000010 rms=0.001263 Jy/beam ! Combined flux in latest and established models = 0.833632 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 0.833632 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec ! Estimated beam: bmin=0.65 mas, bmaj=0.9377 mas, bpa=-5.438 degrees ! Estimated noise=0.909735 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) ! Added new window around map position (-0.6, 0). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0179021 Jy ! Component: 100 - total flux cleaned = 0.0274811 Jy ! Component: 150 - total flux cleaned = 0.0296523 Jy ! Component: 200 - total flux cleaned = 0.0314893 Jy ! Total flux subtracted in 200 components = 0.0314893 Jy ! Clean residual min=-0.004390 max=0.005662 Jy/beam ! Clean residual mean=0.000008 rms=0.000853 Jy/beam ! Combined flux in latest and established models = 0.865121 Jy ! Adding 13 model components to the UV plane model. ! The established model now contains 18 components and 0.865121 Jy ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec ! Added new window around map position (0.6, -3.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00241883 Jy ! Component: 100 - total flux cleaned = 0.00364729 Jy ! Component: 150 - total flux cleaned = 0.00493316 Jy ! Component: 200 - total flux cleaned = 0.00594006 Jy ! Total flux subtracted in 200 components = 0.00594006 Jy ! Clean residual min=-0.003343 max=0.003430 Jy/beam ! Clean residual mean=0.000009 rms=0.000777 Jy/beam ! Combined flux in latest and established models = 0.871061 Jy ! Adding 19 model components to the UV plane model. ! The established model now contains 30 components and 0.871061 Jy ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec ! Added new window around map position (-13.6, -43.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0016715 Jy ! Component: 100 - total flux cleaned = 0.00253496 Jy ! Component: 150 - total flux cleaned = 0.00362267 Jy ! Component: 200 - total flux cleaned = 0.00463516 Jy ! Total flux subtracted in 200 components = 0.00463516 Jy ! Clean residual min=-0.003257 max=0.003031 Jy/beam ! Clean residual mean=0.000008 rms=0.000739 Jy/beam ! Combined flux in latest and established models = 0.875696 Jy ! Adding 27 model components to the UV plane model. ! The established model now contains 41 components and 0.875696 Jy ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 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 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec ! Estimated beam: bmin=2.745 mas, bmaj=3.333 mas, bpa=-4.728 degrees ! Estimated noise=1.18116 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00273001 Jy ! Component: 100 - total flux cleaned = 0.00457279 Jy ! Component: 150 - total flux cleaned = 0.00550095 Jy ! Component: 200 - total flux cleaned = 0.00587272 Jy ! Total flux subtracted in 200 components = 0.00587272 Jy ! Clean residual min=-0.003200 max=0.002804 Jy/beam ! Clean residual mean=0.000021 rms=0.000777 Jy/beam ! Combined flux in latest and established models = 0.881569 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 = 0.000250349 Jy ! Component: 100 - total flux cleaned = 0.000365873 Jy ! Component: 150 - total flux cleaned = 0.000437869 Jy ! Component: 200 - total flux cleaned = 0.00050479 Jy ! Total flux subtracted in 200 components = 0.00050479 Jy ! Clean residual min=-0.003119 max=0.002792 Jy/beam ! Clean residual mean=0.000021 rms=0.000771 Jy/beam ! Combined flux in latest and established models = 0.882074 Jy ! Adding 28 model components to the UV plane model. ! The established model now contains 68 components and 0.882074 Jy ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec ! Estimated beam: bmin=0.65 mas, bmaj=0.9377 mas, bpa=-5.438 degrees ! Estimated noise=0.909735 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000582348 Jy ! Component: 100 - total flux cleaned = -0.000471263 Jy ! Component: 150 - total flux cleaned = -0.000469054 Jy ! Component: 200 - total flux cleaned = -0.000365549 Jy ! Total flux subtracted in 200 components = -0.000365549 Jy ! Clean residual min=-0.003165 max=0.002923 Jy/beam ! Clean residual mean=0.000009 rms=0.000706 Jy/beam ! Combined flux in latest and established models = 0.881708 Jy selfcal ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 78 components and 0.881708 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.084965Jy sigma=0.774416 ! Fit after self-cal, rms=0.084787Jy sigma=0.773088 wmodel J0239-0234_X_map.mod ! Writing 78 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 10 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 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00114602 Jy ! Component: 100 - total flux cleaned = -0.00201846 Jy ! Component: 150 - total flux cleaned = -0.00286644 Jy ! Component: 200 - total flux cleaned = -0.00359033 Jy ! Component: 250 - total flux cleaned = -0.00404624 Jy ! Component: 300 - total flux cleaned = -0.00459326 Jy ! Component: 350 - total flux cleaned = -0.00493534 Jy ! Component: 400 - total flux cleaned = -0.00512839 Jy ! Component: 450 - total flux cleaned = -0.00546207 Jy ! Component: 500 - total flux cleaned = -0.00583676 Jy ! Component: 550 - total flux cleaned = -0.00597584 Jy ! Component: 600 - total flux cleaned = -0.0062501 Jy ! Component: 650 - total flux cleaned = -0.00652081 Jy ! Component: 700 - total flux cleaned = -0.00656544 Jy ! Component: 750 - total flux cleaned = -0.00687571 Jy ! Component: 800 - total flux cleaned = -0.00683154 Jy ! Component: 850 - total flux cleaned = -0.00687538 Jy ! Component: 900 - total flux cleaned = -0.00700467 Jy ! Component: 950 - total flux cleaned = -0.00691899 Jy ! Component: 1000 - total flux cleaned = -0.00704615 Jy ! Component: 1050 - total flux cleaned = -0.00700419 Jy ! Component: 1100 - total flux cleaned = -0.0071292 Jy ! Component: 1150 - total flux cleaned = -0.00717066 Jy ! Component: 1200 - total flux cleaned = -0.00717075 Jy ! Component: 1250 - total flux cleaned = -0.00741543 Jy ! Component: 1300 - total flux cleaned = -0.00741529 Jy ! Component: 1350 - total flux cleaned = -0.00741527 Jy ! Component: 1400 - total flux cleaned = -0.00745551 Jy ! Component: 1450 - total flux cleaned = -0.00753486 Jy ! Component: 1500 - total flux cleaned = -0.0076533 Jy ! Component: 1550 - total flux cleaned = -0.00769223 Jy ! Component: 1600 - total flux cleaned = -0.00773098 Jy ! Component: 1650 - total flux cleaned = -0.00773104 Jy ! Component: 1700 - total flux cleaned = -0.00769269 Jy ! Component: 1750 - total flux cleaned = -0.00765431 Jy ! Component: 1800 - total flux cleaned = -0.00776857 Jy ! Component: 1850 - total flux cleaned = -0.00776889 Jy ! Component: 1900 - total flux cleaned = -0.00761821 Jy ! Component: 1950 - total flux cleaned = -0.00773034 Jy ! Component: 2000 - total flux cleaned = -0.00769312 Jy ! Component: 2050 - total flux cleaned = -0.00773036 Jy ! Component: 2100 - total flux cleaned = -0.00780318 Jy ! Component: 2150 - total flux cleaned = -0.0079491 Jy ! Component: 2200 - total flux cleaned = -0.00802176 Jy ! Component: 2250 - total flux cleaned = -0.00787698 Jy ! Component: 2300 - total flux cleaned = -0.00780529 Jy ! Component: 2350 - total flux cleaned = -0.00802014 Jy ! Component: 2400 - total flux cleaned = -0.00798455 Jy ! Component: 2450 - total flux cleaned = -0.0079493 Jy ! Component: 2500 - total flux cleaned = -0.00812554 Jy ! Component: 2550 - total flux cleaned = -0.00830075 Jy ! Component: 2600 - total flux cleaned = -0.00826553 Jy ! Component: 2650 - total flux cleaned = -0.00833494 Jy ! Component: 2700 - total flux cleaned = -0.0081968 Jy ! Component: 2750 - total flux cleaned = -0.00812795 Jy ! Component: 2800 - total flux cleaned = -0.00829923 Jy ! Component: 2850 - total flux cleaned = -0.00850391 Jy ! Component: 2900 - total flux cleaned = -0.0084702 Jy ! Component: 2950 - total flux cleaned = -0.0086053 Jy ! Component: 3000 - total flux cleaned = -0.00857162 Jy ! Component: 3050 - total flux cleaned = -0.00857148 Jy ! Component: 3100 - total flux cleaned = -0.00863827 Jy ! Component: 3150 - total flux cleaned = -0.0085719 Jy ! Component: 3200 - total flux cleaned = -0.00867125 Jy ! Component: 3250 - total flux cleaned = -0.0088359 Jy ! Component: 3300 - total flux cleaned = -0.00883583 Jy ! Component: 3350 - total flux cleaned = -0.008999 Jy ! Component: 3400 - total flux cleaned = -0.00899891 Jy ! Component: 3450 - total flux cleaned = -0.0089021 Jy ! Component: 3500 - total flux cleaned = -0.00899899 Jy ! Component: 3550 - total flux cleaned = -0.00899868 Jy ! Component: 3600 - total flux cleaned = -0.00880683 Jy ! Component: 3650 - total flux cleaned = -0.00887034 Jy ! Component: 3700 - total flux cleaned = -0.00896541 Jy ! Component: 3750 - total flux cleaned = -0.00912306 Jy ! Component: 3800 - total flux cleaned = -0.00906009 Jy ! Component: 3850 - total flux cleaned = -0.00893474 Jy ! Component: 3900 - total flux cleaned = -0.00877872 Jy ! Component: 3950 - total flux cleaned = -0.00880961 Jy ! Component: 4000 - total flux cleaned = -0.00871681 Jy ! Component: 4050 - total flux cleaned = -0.00868599 Jy ! Total flux subtracted in 4096 components = -0.00883989 Jy ! Clean residual min=-0.001783 max=0.001592 Jy/beam ! Clean residual mean=0.000007 rms=0.000500 Jy/beam ! Combined flux in latest and established models = 0.872868 Jy keep ! Adding 350 model components to the UV plane model. ! The established model now contains 427 components and 0.872869 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv117_uvs/J0239-0234_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.65 x 0.9377 at -5.438 degrees (North through East) ! Clean map min=-0.0022406 max=0.7634 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv117_uvs/J0239-0234_X_map.fits wmodel /scr/pima/rv117_uvs/J0239-0234_X_map.mod ! Writing 427 model components to file: /scr/pima/rv117_uvs/J0239-0234_X_map.mod wobs /scr/pima/rv117_uvs/J0239-0234_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv117_uvs/J0239-0234_X_uvs.fits wwins /scr/pima/rv117_uvs/J0239-0234_X_map.win ! wwins: Wrote 11 windows to /scr/pima/rv117_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 0.763399 invert ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1939 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000499156 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.196158 0.196158 0.392316 0.784632 1.56926 3.13853 6.27706 12.5541 25.1082 50.2164 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0014 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.763 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 1529.38 quit ! Quitting program ! Log file /scr/pima/rv117_uvs/J0239-0234_X_dfm.log closed on Sat Dec 9 23:41:06 2017