! Started logfile: /scr/pima/rv121_uvs/J1130+3815_X_dfm.log on Sat Jul 28 00:40:49 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/rv121_uvs/J1130+3815_X_uva.fits ! Reading UV FITS file: /scr/pima/rv121_uvs/J1130+3815_X_uva.fits ! AN table 1: 26 integrations on 21 of 21 possible baselines. ! AN table 2: 50 integrations on 15 of 15 possible baselines. ! AN table 3: 3 integrations on 28 of 28 possible baselines. ! AN table 4: 34 integrations on 45 of 45 possible baselines. ! AN table 5: 22 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.378462 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1130+3815 ! ! 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 5904 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 J1130+3815_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 102 telescope corrections were flagged in sub-array 1. ! A total of 176 telescope corrections were flagged in sub-array 2. ! A total of 8 telescope corrections were flagged in sub-array 3. ! A total of 154 telescope corrections were flagged in sub-array 4. ! A total of 152 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 102 telescope corrections were flagged in sub-array 1. ! A total of 176 telescope corrections were flagged in sub-array 2. ! A total of 8 telescope corrections were flagged in sub-array 3. ! A total of 154 telescope corrections were flagged in sub-array 4. ! A total of 152 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 102 telescope corrections were flagged in sub-array 1. ! A total of 176 telescope corrections were flagged in sub-array 2. ! A total of 8 telescope corrections were flagged in sub-array 3. ! A total of 154 telescope corrections were flagged in sub-array 4. ! A total of 152 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 102 telescope corrections were flagged in sub-array 1. ! A total of 176 telescope corrections were flagged in sub-array 2. ! A total of 8 telescope corrections were flagged in sub-array 3. ! A total of 154 telescope corrections were flagged in sub-array 4. ! A total of 152 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=1.347728Jy sigma=18.039833 ! Fit after self-cal, rms=0.273088Jy sigma=3.112795 ! 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 2.55% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=0.7997 mas, bmaj=0.9206 mas, bpa=9.973 degrees ! Estimated noise=1.0573 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 = 0.667461 Jy ! Component: 100 - total flux cleaned = 0.869916 Jy ! Total flux subtracted in 100 components = 0.869916 Jy ! Clean residual min=-0.018242 max=0.089405 Jy/beam ! Clean residual mean=0.000010 rms=0.004748 Jy/beam ! Combined flux in latest and established models = 0.869915 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 10 components and 0.869915 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.198952Jy sigma=2.696106 ! Fit after self-cal, rms=0.198642Jy sigma=2.691592 ! Inverting map ! Your choice of large map pixels excluded 2.55% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.101723 Jy ! Component: 100 - total flux cleaned = 0.161139 Jy ! Total flux subtracted in 100 components = 0.161139 Jy ! Clean residual min=-0.011509 max=0.030577 Jy/beam ! Clean residual mean=-0.000004 rms=0.002620 Jy/beam ! Combined flux in latest and established models = 1.03105 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 22 components and 1.03105 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.130870Jy sigma=1.551342 ! Fit after self-cal, rms=0.129626Jy sigma=1.535792 ! Inverting map ! Your choice of large map pixels excluded 2.55% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0388602 Jy ! Component: 100 - total flux cleaned = 0.0626094 Jy ! Total flux subtracted in 100 components = 0.0626094 Jy ! Clean residual min=-0.009346 max=0.015587 Jy/beam ! Clean residual mean=-0.000009 rms=0.002048 Jy/beam ! Combined flux in latest and established models = 1.09366 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 28 components and 1.09366 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.118088Jy sigma=1.276253 ! Fit after self-cal, rms=0.117572Jy sigma=1.269569 ! Inverting map ! Your choice of large map pixels excluded 2.55% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec ! Added new window around map position (0.2, -1). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0180689 Jy ! Component: 100 - total flux cleaned = 0.028695 Jy ! Total flux subtracted in 100 components = 0.028695 Jy ! Clean residual min=-0.009091 max=0.013120 Jy/beam ! Clean residual mean=-0.000011 rms=0.001885 Jy/beam ! Combined flux in latest and established models = 1.12236 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 34 components and 1.12236 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.115125Jy sigma=1.208399 ! Fit after self-cal, rms=0.114721Jy sigma=1.204615 ! Inverting map ! Your choice of large map pixels excluded 2.55% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec ! Added new window around map position (-1.4, -1). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0125765 Jy ! Component: 100 - total flux cleaned = 0.0179087 Jy ! Total flux subtracted in 100 components = 0.0179087 Jy ! Clean residual min=-0.008712 max=0.010028 Jy/beam ! Clean residual mean=-0.000013 rms=0.001811 Jy/beam ! Combined flux in latest and established models = 1.14027 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 43 components and 1.14027 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.113837Jy sigma=1.186464 ! Fit after self-cal, rms=0.113592Jy sigma=1.183300 ! Inverting map ! Your choice of large map pixels excluded 2.55% of the data. ! The y-axis pixel size should ideally be below 0.1665 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 2.55% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=0.949 mas, bmaj=1.077 mas, bpa=6.204 degrees ! Estimated noise=0.828315 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 = 0.00219521 Jy ! Component: 100 - total flux cleaned = 0.00183891 Jy ! Component: 150 - total flux cleaned = 0.00168982 Jy ! Component: 200 - total flux cleaned = 0.00155542 Jy ! Total flux subtracted in 200 components = 0.00155542 Jy ! Clean residual min=-0.010548 max=0.009159 Jy/beam ! Clean residual mean=-0.000136 rms=0.002565 Jy/beam ! Combined flux in latest and established models = 1.14182 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 54 components and 1.14182 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.113141Jy sigma=1.176650 ! Fit after self-cal, rms=0.113016Jy sigma=1.175842 ! Inverting map ! Your choice of large map pixels excluded 2.55% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec print "============== Finished natural weighting clean ==============" ! ============== Finished natural weighting clean ============== ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.949 x 1.077 at 6.204 degrees (North through East) ! Clean map min=-0.010055 max=0.86588 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 30 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 HN 0.95 NL 1.03 NY 1.03 ! ON 0.94 SC 0.98 WZ 0.98 ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 HH 0.95 HN 1.07 NY 1.03 ! ON 0.93 WZ 0.95 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.00 HN 1.09 LA 1.00 ! NL 0.99 PT 1.01 SC 0.95 WZ 0.99 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 FD 0.98 HN 1.02 KP 1.03 ! LA 0.99 MK 0.98 NL 0.98 OV 0.97 ! PT 1.00 SC 0.97 ! ! A total of 24 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 HN 1.08 KP 1.00 LA 0.98 ! MK 0.98 NL 0.99 NY 1.05 ON 1.03 ! OV 0.98 PT 0.97 ! ! ! Correcting IF 2. ! A total of 30 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 HN 0.95 NL 1.05 NY 0.99 ! ON 0.95 SC 0.97 WZ 0.96 ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 HH 0.99 HN 1.14 NY 1.01 ! ON 0.96 WZ 0.94 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.00 HN 1.21 LA 1.00 ! NL 0.98 PT 1.00 SC 0.98 WZ 1.00 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 FD 0.98 HN 1.09 KP 1.05 ! LA 0.99 MK 0.98 NL 0.98 OV 0.97 ! PT 1.00 SC 0.98 ! ! A total of 24 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 HN 1.12 KP 1.02 LA 0.98 ! MK 1.00 NL 0.97 NY 1.03 ON 1.15 ! OV 0.99 PT 0.96 ! ! ! Correcting IF 3. ! A total of 30 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 HN 0.97 NL 1.06 NY 1.02 ! ON 0.96 SC 0.98 WZ 0.92 ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 HH 1.10 HN 1.10 NY 0.99 ! ON 0.96 WZ 0.96 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 1.02 HN 1.20 LA 1.01 ! NL 0.97 PT 0.99 SC 0.95 WZ 1.03 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 FD 0.99 HN 1.08 KP 1.04 ! LA 1.00 MK 0.99 NL 0.99 OV 0.96 ! PT 1.00 SC 0.98 ! ! A total of 24 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 HN 1.13 KP 0.99 LA 1.01 ! MK 1.02 NL 0.99 NY 1.01 ON 1.14 ! OV 0.98 PT 0.98 ! ! ! Correcting IF 4. ! A total of 30 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.05 HN 0.99 NL 1.08 NY 0.94 ! ON 0.97 SC 0.96 WZ 0.96 ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 HH 1.30 HN 1.14 NY 0.94 ! ON 0.97 WZ 0.94 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 FD 1.01 HN 1.30 LA 1.00 ! NL 1.02 PT 1.00 SC 0.94 WZ 1.02 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 FD 0.98 HN 1.07 KP 1.05 ! LA 1.00 MK 0.98 NL 0.99 OV 0.98 ! PT 1.01 SC 0.99 ! ! A total of 24 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 HN 1.12 KP 1.00 LA 0.99 ! MK 1.00 NL 1.01 NY 1.00 ON 1.18 ! OV 0.98 PT 1.00 ! ! ! Fit before self-cal, rms=0.113016Jy sigma=1.175842 ! Fit after self-cal, rms=0.101757Jy sigma=1.001247 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=0.9585 mas, bmaj=1.125 mas, bpa=-1.409 degrees ! Estimated noise=0.849987 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 = -0.0050568 Jy ! Component: 100 - total flux cleaned = -0.00607464 Jy ! Component: 150 - total flux cleaned = -0.00676258 Jy ! Component: 200 - total flux cleaned = -0.00710996 Jy ! Total flux subtracted in 200 components = -0.00710996 Jy ! Clean residual min=-0.007759 max=0.006692 Jy/beam ! Clean residual mean=-0.000097 rms=0.001886 Jy/beam ! Combined flux in latest and established models = 1.13471 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 65 components and 1.13471 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.100828Jy sigma=0.993750 ! Fit after self-cal, rms=0.100873Jy sigma=0.992942 ! Inverting map ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 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=0.100873Jy sigma=0.992942 ! Fit after self-cal, rms=0.096248Jy sigma=0.898000 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=0.9599 mas, bmaj=1.125 mas, bpa=-1.692 degrees ! Estimated noise=0.848631 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000530203 Jy ! Component: 100 - total flux cleaned = -0.00106065 Jy ! Component: 150 - total flux cleaned = -0.00115728 Jy ! Component: 200 - total flux cleaned = -0.00124261 Jy ! Total flux subtracted in 200 components = -0.00124261 Jy ! Clean residual min=-0.003820 max=0.003545 Jy/beam ! Clean residual mean=-0.000001 rms=0.000870 Jy/beam ! Combined flux in latest and established models = 1.13347 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 69 components and 1.13347 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.095666Jy sigma=0.893579 ! Fit after self-cal, rms=0.095525Jy sigma=0.892826 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 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 = 7.36512e-05 Jy ! Component: 100 - total flux cleaned = 0.000324996 Jy ! Component: 150 - total flux cleaned = 0.000251886 Jy ! Component: 200 - total flux cleaned = 0.000253958 Jy ! Total flux subtracted in 200 components = 0.000253958 Jy ! Clean residual min=-0.003750 max=0.003576 Jy/beam ! Clean residual mean=-0.000002 rms=0.000861 Jy/beam ! Combined flux in latest and established models = 1.13372 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 72 components and 1.13372 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.095272Jy sigma=0.890666 ! Fit after self-cal, rms=0.095184Jy sigma=0.890204 ! Inverting map ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 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=0.095184Jy sigma=0.890204 ! Fit after self-cal, rms=0.092799Jy sigma=0.855470 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=0.9599 mas, bmaj=1.126 mas, bpa=-2.134 degrees ! Estimated noise=0.848769 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00040711 Jy ! Component: 100 - total flux cleaned = 0.000415197 Jy ! Component: 150 - total flux cleaned = 0.000414198 Jy ! Component: 200 - total flux cleaned = 0.000339695 Jy ! Total flux subtracted in 200 components = 0.000339695 Jy ! Clean residual min=-0.003468 max=0.003513 Jy/beam ! Clean residual mean=0.000002 rms=0.000731 Jy/beam ! Combined flux in latest and established models = 1.13406 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 73 components and 1.13406 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.092592Jy sigma=0.853311 ! Fit after self-cal, rms=0.092510Jy sigma=0.852969 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 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 (25.8, -2.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000795247 Jy ! Component: 100 - total flux cleaned = 0.000414199 Jy ! Component: 150 - total flux cleaned = 0.000331482 Jy ! Component: 200 - total flux cleaned = 0.000255788 Jy ! Total flux subtracted in 200 components = 0.000255788 Jy ! Clean residual min=-0.003539 max=0.003255 Jy/beam ! Clean residual mean=0.000001 rms=0.000719 Jy/beam ! Combined flux in latest and established models = 1.13432 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 83 components and 1.13432 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.092239Jy sigma=0.849672 ! Fit after self-cal, rms=0.092218Jy sigma=0.849393 ! Inverting map ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 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=0.092218Jy sigma=0.849393 ! Fit after self-cal, rms=0.092366Jy sigma=0.849064 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=2.345 mas, bmaj=2.886 mas, bpa=-74.28 degrees ! Estimated noise=1.06721 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000440522 Jy ! Component: 100 - total flux cleaned = 0.000484909 Jy ! Component: 150 - total flux cleaned = 0.000632925 Jy ! Component: 200 - total flux cleaned = 0.000577101 Jy ! Total flux subtracted in 200 components = 0.000577101 Jy ! Clean residual min=-0.002758 max=0.002453 Jy/beam ! Clean residual mean=0.000005 rms=0.000686 Jy/beam ! Combined flux in latest and established models = 1.1349 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 90 components and 1.1349 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.092237Jy sigma=0.848516 ! Fit after self-cal, rms=0.092261Jy sigma=0.847973 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 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 = 2.2482e-06 Jy ! Component: 100 - total flux cleaned = 9.10776e-05 Jy ! Component: 150 - total flux cleaned = 0.000176924 Jy ! Component: 200 - total flux cleaned = 0.000104902 Jy ! Total flux subtracted in 200 components = 0.000104902 Jy ! Clean residual min=-0.002762 max=0.002409 Jy/beam ! Clean residual mean=0.000004 rms=0.000682 Jy/beam ! Combined flux in latest and established models = 1.135 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 92 components and 1.135 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.092188Jy sigma=0.847804 ! Fit after self-cal, rms=0.092182Jy sigma=0.847390 ! Inverting map ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. win_mult = win_mult / 1.2 print "============== Finished amplitude self-cal ==============" ! ============== Finished amplitude self-cal ============== restore ! Inverting map and beam ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=0.9596 mas, bmaj=1.126 mas, bpa=-2.287 degrees ! Estimated noise=0.84861 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9596 x 1.126 at -2.287 degrees (North through East) ! Clean map min=-0.0030604 max=0.87883 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=0.092182Jy sigma=0.847390 ! Fit after self-cal, rms=0.087610Jy sigma=0.770376 ! Inverting map and beam ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=0.9599 mas, bmaj=1.126 mas, bpa=-2.123 degrees ! Estimated noise=0.848608 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000150509 Jy ! Component: 100 - total flux cleaned = -0.000307547 Jy ! Component: 150 - total flux cleaned = -0.000455529 Jy ! Component: 200 - total flux cleaned = -0.000525677 Jy ! Total flux subtracted in 200 components = -0.000525677 Jy ! Clean residual min=-0.003500 max=0.003166 Jy/beam ! Clean residual mean=0.000002 rms=0.000690 Jy/beam ! Combined flux in latest and established models = 1.13448 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 96 components and 1.13448 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.087450Jy sigma=0.768453 ! Fit after self-cal, rms=0.087409Jy sigma=0.768329 ! Inverting map ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 7.13794e-05 Jy ! Component: 100 - total flux cleaned = -6.47795e-05 Jy ! Component: 150 - total flux cleaned = -0.000127676 Jy ! Component: 200 - total flux cleaned = -0.000189694 Jy ! Total flux subtracted in 200 components = -0.000189694 Jy ! Clean residual min=-0.003502 max=0.003123 Jy/beam ! Clean residual mean=0.000002 rms=0.000685 Jy/beam ! Combined flux in latest and established models = 1.13429 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 99 components and 1.13429 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.087275Jy sigma=0.766916 ! Fit after self-cal, rms=0.087229Jy sigma=0.766823 ! Inverting map ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.087229Jy sigma=0.766823 ! Fit after self-cal, rms=0.087369Jy sigma=0.766660 print "============== Clearing model and starting over ==========" ! ============== Clearing model and starting over ========== clrmod true ! clrmod: Cleared the established and tentative models. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=0.803 mas, bmaj=0.9523 mas, bpa=0.5808 degrees ! Estimated noise=1.0837 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.676764 Jy ! Component: 100 - total flux cleaned = 0.880589 Jy ! Component: 150 - total flux cleaned = 0.98421 Jy ! Component: 200 - total flux cleaned = 1.0426 Jy ! Total flux subtracted in 200 components = 1.0426 Jy ! Clean residual min=-0.007532 max=0.029408 Jy/beam ! Clean residual mean=0.000003 rms=0.001870 Jy/beam ! Combined flux in latest and established models = 1.0426 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 23 model components to the UV plane model. ! The established model now contains 23 components and 1.0426 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=0.9597 mas, bmaj=1.127 mas, bpa=-2.229 degrees ! Estimated noise=0.848593 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 = 0.0428377 Jy ! Component: 100 - total flux cleaned = 0.0649957 Jy ! Component: 150 - total flux cleaned = 0.0775844 Jy ! Component: 200 - total flux cleaned = 0.085017 Jy ! Total flux subtracted in 200 components = 0.085017 Jy ! Clean residual min=-0.003615 max=0.004576 Jy/beam ! Clean residual mean=0.000016 rms=0.000777 Jy/beam ! Combined flux in latest and established models = 1.12762 Jy ! Adding 22 model components to the UV plane model. ! The established model now contains 38 components and 1.12762 Jy ! Inverting map ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec ! Added new window around map position (-1.2, 0.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00362147 Jy ! Component: 100 - total flux cleaned = 0.00554593 Jy ! Component: 150 - total flux cleaned = 0.00582517 Jy ! Component: 200 - total flux cleaned = 0.00583088 Jy ! Total flux subtracted in 200 components = 0.00583088 Jy ! Clean residual min=-0.003565 max=0.003246 Jy/beam ! Clean residual mean=0.000004 rms=0.000730 Jy/beam ! Combined flux in latest and established models = 1.13345 Jy ! Adding 24 model components to the UV plane model. ! The established model now contains 55 components and 1.13345 Jy ! Inverting map ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=2.346 mas, bmaj=2.886 mas, bpa=-74.3 degrees ! Estimated noise=1.06679 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00144388 Jy ! Component: 100 - total flux cleaned = 0.00141201 Jy ! Component: 150 - total flux cleaned = 0.00144227 Jy ! Component: 200 - total flux cleaned = 0.00138633 Jy ! Total flux subtracted in 200 components = 0.00138633 Jy ! Clean residual min=-0.002718 max=0.002293 Jy/beam ! Clean residual mean=0.000001 rms=0.000659 Jy/beam ! Combined flux in latest and established models = 1.13483 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 = 2.44839e-05 Jy ! Component: 100 - total flux cleaned = 2.31404e-05 Jy ! Component: 150 - total flux cleaned = 2.32211e-05 Jy ! Component: 200 - total flux cleaned = 4.03351e-05 Jy ! Total flux subtracted in 200 components = 4.03351e-05 Jy ! Clean residual min=-0.002719 max=0.002315 Jy/beam ! Clean residual mean=0.000001 rms=0.000659 Jy/beam ! Combined flux in latest and established models = 1.13487 Jy ! Adding 30 model components to the UV plane model. ! The established model now contains 82 components and 1.13488 Jy ! Inverting map ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec ! Estimated beam: bmin=0.9597 mas, bmaj=1.127 mas, bpa=-2.229 degrees ! Estimated noise=0.848593 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00101619 Jy ! Component: 100 - total flux cleaned = -0.00112999 Jy ! Component: 150 - total flux cleaned = -0.00101415 Jy ! Component: 200 - total flux cleaned = -0.00101613 Jy ! Total flux subtracted in 200 components = -0.00101613 Jy ! Clean residual min=-0.003515 max=0.003257 Jy/beam ! Clean residual mean=0.000002 rms=0.000712 Jy/beam ! Combined flux in latest and established models = 1.13386 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 86 components and 1.13386 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.088765Jy sigma=0.784993 ! Fit after self-cal, rms=0.088367Jy sigma=0.781637 wmodel J1130+3815_X_map.mod ! Writing 86 model components to file: J1130+3815_X_map.mod wobs J1130+3815_X_uvs.fits ! Writing UV FITS file: J1130+3815_X_uvs.fits wwins J1130+3815_X_map.win ! wwins: Wrote 5 windows to J1130+3815_X_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000257733 Jy ! Component: 100 - total flux cleaned = -0.000486048 Jy ! Component: 150 - total flux cleaned = -0.000648402 Jy ! Component: 200 - total flux cleaned = -0.000805902 Jy ! Component: 250 - total flux cleaned = -0.00106208 Jy ! Component: 300 - total flux cleaned = -0.00121271 Jy ! Component: 350 - total flux cleaned = -0.00131089 Jy ! Component: 400 - total flux cleaned = -0.00126207 Jy ! Component: 450 - total flux cleaned = -0.00135838 Jy ! Component: 500 - total flux cleaned = -0.00145223 Jy ! Component: 550 - total flux cleaned = -0.00135845 Jy ! Component: 600 - total flux cleaned = -0.00140537 Jy ! Component: 650 - total flux cleaned = -0.00140598 Jy ! Component: 700 - total flux cleaned = -0.00158784 Jy ! Component: 750 - total flux cleaned = -0.00172253 Jy ! Component: 800 - total flux cleaned = -0.00190049 Jy ! Component: 850 - total flux cleaned = -0.00207656 Jy ! Component: 900 - total flux cleaned = -0.00198883 Jy ! Component: 950 - total flux cleaned = -0.00207583 Jy ! Component: 1000 - total flux cleaned = -0.00211899 Jy ! Component: 1050 - total flux cleaned = -0.00216192 Jy ! Component: 1100 - total flux cleaned = -0.0021193 Jy ! Component: 1150 - total flux cleaned = -0.00233123 Jy ! Component: 1200 - total flux cleaned = -0.00224659 Jy ! Component: 1250 - total flux cleaned = -0.00233036 Jy ! Component: 1300 - total flux cleaned = -0.00208044 Jy ! Component: 1350 - total flux cleaned = -0.00216341 Jy ! Component: 1400 - total flux cleaned = -0.00224559 Jy ! Component: 1450 - total flux cleaned = -0.00224587 Jy ! Component: 1500 - total flux cleaned = -0.00228653 Jy ! Component: 1550 - total flux cleaned = -0.00236723 Jy ! Component: 1600 - total flux cleaned = -0.00228648 Jy ! Component: 1650 - total flux cleaned = -0.00228634 Jy ! Component: 1700 - total flux cleaned = -0.00220651 Jy ! Component: 1750 - total flux cleaned = -0.00224597 Jy ! Component: 1800 - total flux cleaned = -0.00208835 Jy ! Component: 1850 - total flux cleaned = -0.00208836 Jy ! Component: 1900 - total flux cleaned = -0.00216688 Jy ! Component: 1950 - total flux cleaned = -0.00205064 Jy ! Component: 2000 - total flux cleaned = -0.00208942 Jy ! Component: 2050 - total flux cleaned = -0.00208908 Jy ! Component: 2100 - total flux cleaned = -0.0018975 Jy ! Component: 2150 - total flux cleaned = -0.00189733 Jy ! Component: 2200 - total flux cleaned = -0.00189744 Jy ! Component: 2250 - total flux cleaned = -0.0018974 Jy ! Component: 2300 - total flux cleaned = -0.00197284 Jy ! Component: 2350 - total flux cleaned = -0.00178565 Jy ! Component: 2400 - total flux cleaned = -0.00193458 Jy ! Component: 2450 - total flux cleaned = -0.00189757 Jy ! Component: 2500 - total flux cleaned = -0.00163858 Jy ! Component: 2550 - total flux cleaned = -0.00182265 Jy ! Component: 2600 - total flux cleaned = -0.00167582 Jy ! Component: 2650 - total flux cleaned = -0.00167556 Jy ! Component: 2700 - total flux cleaned = -0.00178451 Jy ! Component: 2750 - total flux cleaned = -0.00156742 Jy ! Component: 2800 - total flux cleaned = -0.0016395 Jy ! Component: 2850 - total flux cleaned = -0.00153172 Jy ! Component: 2900 - total flux cleaned = -0.00149605 Jy ! Component: 2950 - total flux cleaned = -0.00167424 Jy ! Component: 3000 - total flux cleaned = -0.00156754 Jy ! Component: 3050 - total flux cleaned = -0.00167344 Jy ! Component: 3100 - total flux cleaned = -0.00149743 Jy ! Component: 3150 - total flux cleaned = -0.00146215 Jy ! Component: 3200 - total flux cleaned = -0.00153193 Jy ! Component: 3250 - total flux cleaned = -0.00146233 Jy ! Component: 3300 - total flux cleaned = -0.00132345 Jy ! Component: 3350 - total flux cleaned = -0.00135797 Jy ! Component: 3400 - total flux cleaned = -0.00139253 Jy ! Component: 3450 - total flux cleaned = -0.00135833 Jy ! Component: 3500 - total flux cleaned = -0.00135842 Jy ! Component: 3550 - total flux cleaned = -0.00132416 Jy ! Component: 3600 - total flux cleaned = -0.00129026 Jy ! Component: 3650 - total flux cleaned = -0.00132393 Jy ! Component: 3700 - total flux cleaned = -0.00122293 Jy ! Component: 3750 - total flux cleaned = -0.00115566 Jy ! Component: 3800 - total flux cleaned = -0.00115583 Jy ! Component: 3850 - total flux cleaned = -0.00112257 Jy ! Component: 3900 - total flux cleaned = -0.00115595 Jy ! Component: 3950 - total flux cleaned = -0.0010566 Jy ! Component: 4000 - total flux cleaned = -0.00102364 Jy ! Component: 4050 - total flux cleaned = -0.000957821 Jy ! Total flux subtracted in 4096 components = -0.00102331 Jy ! Clean residual min=-0.002118 max=0.002016 Jy/beam ! Clean residual mean=0.000002 rms=0.000541 Jy/beam ! Combined flux in latest and established models = 1.13284 Jy keep ! Adding 352 model components to the UV plane model. ! The established model now contains 436 components and 1.13284 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv121_uvs/J1130+3815_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9597 x 1.127 at -2.229 degrees (North through East) ! Clean map min=-0.00296 max=0.88061 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv121_uvs/J1130+3815_X_map.fits wmodel /scr/pima/rv121_uvs/J1130+3815_X_map.mod ! Writing 436 model components to file: /scr/pima/rv121_uvs/J1130+3815_X_map.mod wobs /scr/pima/rv121_uvs/J1130+3815_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv121_uvs/J1130+3815_X_uvs.fits wwins /scr/pima/rv121_uvs/J1130+3815_X_map.win ! wwins: Wrote 6 windows to /scr/pima/rv121_uvs/J1130+3815_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.88061 invert ! Inverting map ! Your choice of large map pixels excluded 2.57% of the data. ! The y-axis pixel size should ideally be below 0.1665 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000540878 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.184263 0.184263 0.368525 0.73705 1.4741 2.9482 5.8964 11.7928 23.5856 47.1712 94.3425 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0016 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.88 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 1628.11 quit ! Quitting program ! Log file /scr/pima/rv121_uvs/J1130+3815_X_dfm.log closed on Sat Jul 28 00:40:53 2018