! Started logfile: /scr/pima/rv121_uvs/J1506+3730_X_dfm.log on Sat Jul 28 00:41:55 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/J1506+3730_X_uva.fits ! Reading UV FITS file: /scr/pima/rv121_uvs/J1506+3730_X_uva.fits ! AN table 1: 29 integrations on 6 of 6 possible baselines. ! AN table 2: 6 integrations on 3 of 3 possible baselines. ! AN table 3: 47 integrations on 78 of 78 possible baselines. ! Apparent sampling: 0.402799 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1506+3730 ! ! 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 6216 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 J1506+3730_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 12 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! A total of 303 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 12 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! A total of 303 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 12 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! A total of 303 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 12 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! A total of 303 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=1.151810Jy sigma=17.311981 ! Fit after self-cal, rms=0.475218Jy sigma=6.957175 ! 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 2.89% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1729 milli-arcsec ! Estimated beam: bmin=0.6273 mas, bmaj=0.9194 mas, bpa=-17.6 degrees ! Estimated noise=0.984637 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 = 0.405497 Jy ! Component: 100 - total flux cleaned = 0.514091 Jy ! Total flux subtracted in 100 components = 0.514091 Jy ! Clean residual min=-0.012771 max=0.045948 Jy/beam ! Clean residual mean=-0.000072 rms=0.002971 Jy/beam ! Combined flux in latest and established models = 0.514091 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.514091 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.130405Jy sigma=1.765114 ! Fit after self-cal, rms=0.130046Jy sigma=1.761904 ! Inverting map ! Your choice of large map pixels excluded 2.89% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1729 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0512904 Jy ! Component: 100 - total flux cleaned = 0.0790746 Jy ! Total flux subtracted in 100 components = 0.0790746 Jy ! Clean residual min=-0.008586 max=0.026421 Jy/beam ! Clean residual mean=-0.000033 rms=0.001915 Jy/beam ! Combined flux in latest and established models = 0.593166 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 11 components and 0.593166 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.102200Jy sigma=1.244250 ! Fit after self-cal, rms=0.101725Jy sigma=1.239194 ! Inverting map ! Your choice of large map pixels excluded 2.89% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1729 milli-arcsec ! Added new window around map position (-1, -1). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0232976 Jy ! Component: 100 - total flux cleaned = 0.0350562 Jy ! Total flux subtracted in 100 components = 0.0350562 Jy ! Clean residual min=-0.007352 max=0.017647 Jy/beam ! Clean residual mean=-0.000017 rms=0.001615 Jy/beam ! Combined flux in latest and established models = 0.628222 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 19 components and 0.628222 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.095417Jy sigma=1.115370 ! Fit after self-cal, rms=0.094434Jy sigma=1.099454 ! Inverting map ! Your choice of large map pixels excluded 2.89% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1729 milli-arcsec ! Added new window around map position (-1.6, -2.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0125866 Jy ! Component: 100 - total flux cleaned = 0.0149213 Jy ! Total flux subtracted in 100 components = 0.0149213 Jy ! Clean residual min=-0.006195 max=0.009342 Jy/beam ! Clean residual mean=-0.000010 rms=0.001456 Jy/beam ! Combined flux in latest and established models = 0.643143 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 23 components and 0.643143 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.092978Jy sigma=1.067936 ! Fit after self-cal, rms=0.092676Jy sigma=1.063529 ! Inverting map ! Your choice of large map pixels excluded 2.89% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1729 milli-arcsec ! Added new window around map position (1.2, -0.8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0067104 Jy ! Component: 100 - total flux cleaned = 0.00838074 Jy ! Total flux subtracted in 100 components = 0.00838074 Jy ! Clean residual min=-0.005630 max=0.007601 Jy/beam ! Clean residual mean=-0.000006 rms=0.001391 Jy/beam ! Combined flux in latest and established models = 0.651524 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 29 components and 0.651524 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.091333Jy sigma=1.048188 ! Fit after self-cal, rms=0.091268Jy sigma=1.046558 ! Inverting map ! Your choice of large map pixels excluded 2.89% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1729 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 2.89% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1729 milli-arcsec ! Estimated beam: bmin=0.7074 mas, bmaj=1.081 mas, bpa=-16.68 degrees ! Estimated noise=0.68979 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 (-3.8, -5.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00890481 Jy ! Component: 100 - total flux cleaned = 0.0120427 Jy ! Component: 150 - total flux cleaned = 0.0137443 Jy ! Component: 200 - total flux cleaned = 0.0150475 Jy ! Total flux subtracted in 200 components = 0.0150475 Jy ! Clean residual min=-0.006726 max=0.007760 Jy/beam ! Clean residual mean=-0.000019 rms=0.001496 Jy/beam ! Combined flux in latest and established models = 0.666572 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 42 components and 0.666572 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.089316Jy sigma=1.023094 ! Fit after self-cal, rms=0.089249Jy sigma=1.021128 ! Inverting map ! Your choice of large map pixels excluded 2.89% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1729 milli-arcsec print "============== Finished natural weighting clean ==============" ! ============== Finished natural weighting clean ============== ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7074 x 1.081 at -16.68 degrees (North through East) ! Clean map min=-0.0059129 max=0.50716 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 24 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.74 NY 1.02 ON 0.96 WZ 0.99 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 0.00* HN 0.00* WZ 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.02 HN 1.06 KP 1.01 ! LA 0.99 MK 1.00 NL 1.00 NY 0.99 ! ON 1.01 OV 0.99 PT 0.99 SC 0.98 ! WZ 0.97 ! ! ! Correcting IF 2. ! A total of 24 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.75 NY 1.00 ON 0.96 WZ 0.98 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 0.00* HN 0.00* WZ 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 FD 1.01 HN 1.15 KP 1.00 ! LA 0.99 MK 1.00 NL 0.99 NY 1.00 ! ON 0.98 OV 0.99 PT 1.01 SC 0.97 ! WZ 0.99 ! ! ! Correcting IF 3. ! A total of 24 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.81 NY 0.98 ON 0.95 WZ 0.97 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 0.00* HN 0.00* WZ 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 1.01 HN 1.10 KP 1.01 ! LA 1.01 MK 1.00 NL 0.99 NY 1.00 ! ON 0.99 OV 0.98 PT 1.00 SC 0.95 ! WZ 0.98 ! ! ! Correcting IF 4. ! A total of 24 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.92 NY 0.89 ON 0.97 WZ 0.95 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! HH 0.00* HN 0.00* WZ 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 1.00 HN 1.11 KP 1.02 ! LA 0.98 MK 0.99 NL 0.99 NY 0.99 ! ON 0.98 OV 0.98 PT 1.00 SC 0.96 ! WZ 0.98 ! ! ! Fit before self-cal, rms=0.089249Jy sigma=1.021128 ! Fit after self-cal, rms=0.076002Jy sigma=0.932820 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 milli-arcsec ! Estimated beam: bmin=0.7006 mas, bmaj=1.058 mas, bpa=-16.54 degrees ! Estimated noise=0.69125 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 (-7.8, -6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00667709 Jy ! Component: 100 - total flux cleaned = 0.0097772 Jy ! Component: 150 - total flux cleaned = 0.011976 Jy ! Component: 200 - total flux cleaned = 0.0135556 Jy ! Total flux subtracted in 200 components = 0.0135556 Jy ! Clean residual min=-0.004544 max=0.004255 Jy/beam ! Clean residual mean=0.000034 rms=0.000961 Jy/beam ! Combined flux in latest and established models = 0.680127 Jy ! Performing phase self-cal ! Adding 31 model components to the UV plane model. ! The established model now contains 72 components and 0.680127 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.075090Jy sigma=0.918019 ! Fit after self-cal, rms=0.074957Jy sigma=0.916774 ! Inverting map ! Your choice of large map pixels excluded 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 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=0.074957Jy sigma=0.916774 ! Fit after self-cal, rms=0.072903Jy sigma=0.887245 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 milli-arcsec ! Estimated beam: bmin=0.6993 mas, bmaj=1.06 mas, bpa=-16.73 degrees ! Estimated noise=0.691987 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00277313 Jy ! Component: 100 - total flux cleaned = 0.00357571 Jy ! Component: 150 - total flux cleaned = 0.0040807 Jy ! Component: 200 - total flux cleaned = 0.00445136 Jy ! Total flux subtracted in 200 components = 0.00445136 Jy ! Clean residual min=-0.003592 max=0.003309 Jy/beam ! Clean residual mean=0.000016 rms=0.000741 Jy/beam ! Combined flux in latest and established models = 0.684578 Jy selfcal ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 91 components and 0.684578 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.072670Jy sigma=0.883367 ! Fit after self-cal, rms=0.072608Jy sigma=0.883009 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 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 = 0.000313789 Jy ! Component: 100 - total flux cleaned = 0.000530836 Jy ! Component: 150 - total flux cleaned = 0.000791984 Jy ! Component: 200 - total flux cleaned = 0.000911322 Jy ! Total flux subtracted in 200 components = 0.000911322 Jy ! Clean residual min=-0.003465 max=0.003276 Jy/beam ! Clean residual mean=0.000019 rms=0.000728 Jy/beam ! Combined flux in latest and established models = 0.68549 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 99 components and 0.68549 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.072479Jy sigma=0.881086 ! Fit after self-cal, rms=0.072447Jy sigma=0.880919 ! Inverting map ! Your choice of large map pixels excluded 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 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=0.072447Jy sigma=0.880919 ! Fit after self-cal, rms=0.072230Jy sigma=0.875978 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 milli-arcsec ! Estimated beam: bmin=0.6981 mas, bmaj=1.06 mas, bpa=-16.76 degrees ! Estimated noise=0.692526 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00188722 Jy ! Component: 100 - total flux cleaned = 0.00228378 Jy ! Component: 150 - total flux cleaned = 0.0025263 Jy ! Component: 200 - total flux cleaned = 0.00264022 Jy ! Total flux subtracted in 200 components = 0.00264022 Jy ! Clean residual min=-0.003287 max=0.003161 Jy/beam ! Clean residual mean=0.000013 rms=0.000702 Jy/beam ! Combined flux in latest and established models = 0.68813 Jy selfcal ! Performing phase self-cal ! Adding 32 model components to the UV plane model. ! The established model now contains 105 components and 0.68813 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.072104Jy sigma=0.874092 ! Fit after self-cal, rms=0.072076Jy sigma=0.873955 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 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 = 0.000182137 Jy ! Component: 100 - total flux cleaned = 0.000292102 Jy ! Component: 150 - total flux cleaned = 0.000343472 Jy ! Component: 200 - total flux cleaned = 0.000442883 Jy ! Total flux subtracted in 200 components = 0.000442883 Jy ! Clean residual min=-0.003226 max=0.003132 Jy/beam ! Clean residual mean=0.000014 rms=0.000696 Jy/beam ! Combined flux in latest and established models = 0.688573 Jy ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 108 components and 0.688573 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.072002Jy sigma=0.872884 ! Fit after self-cal, rms=0.071986Jy sigma=0.872810 ! Inverting map ! Your choice of large map pixels excluded 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 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=0.071986Jy sigma=0.872810 ! Fit after self-cal, rms=0.071985Jy sigma=0.872524 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 milli-arcsec ! Estimated beam: bmin=2.481 mas, bmaj=3.228 mas, bpa=40.88 degrees ! Estimated noise=0.927711 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00293663 Jy ! Component: 100 - total flux cleaned = 0.00400861 Jy ! Component: 150 - total flux cleaned = 0.00450482 Jy ! Component: 200 - total flux cleaned = 0.00488921 Jy ! Total flux subtracted in 200 components = 0.00488921 Jy ! Clean residual min=-0.003356 max=0.004048 Jy/beam ! Clean residual mean=0.000057 rms=0.000980 Jy/beam ! Combined flux in latest and established models = 0.693462 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 118 components and 0.693462 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.071968Jy sigma=0.872295 ! Fit after self-cal, rms=0.071943Jy sigma=0.872081 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 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 (-8.8, -10.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00384208 Jy ! Component: 100 - total flux cleaned = 0.00482588 Jy ! Component: 150 - total flux cleaned = 0.00551729 Jy ! Component: 200 - total flux cleaned = 0.00578612 Jy ! Total flux subtracted in 200 components = 0.00578612 Jy ! Clean residual min=-0.003032 max=0.003779 Jy/beam ! Clean residual mean=0.000091 rms=0.000901 Jy/beam ! Combined flux in latest and established models = 0.699248 Jy ! Performing phase self-cal ! Adding 47 model components to the UV plane model. ! The established model now contains 165 components and 0.699248 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.071820Jy sigma=0.870102 ! Fit after self-cal, rms=0.071805Jy sigma=0.869848 ! Inverting map ! Your choice of large map pixels excluded 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 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 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 milli-arcsec ! Estimated beam: bmin=0.6973 mas, bmaj=1.059 mas, bpa=-16.8 degrees ! Estimated noise=0.693073 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6973 x 1.059 at -16.8 degrees (North through East) ! Clean map min=-0.0024854 max=0.50464 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=0.071805Jy sigma=0.869848 ! Fit after self-cal, rms=0.067366Jy sigma=0.805003 ! Inverting map and beam ! Your choice of large map pixels excluded 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 milli-arcsec ! Estimated beam: bmin=0.6974 mas, bmaj=1.058 mas, bpa=-16.83 degrees ! Estimated noise=0.693394 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00189237 Jy ! Component: 100 - total flux cleaned = 0.00281311 Jy ! Component: 150 - total flux cleaned = 0.00333203 Jy ! Component: 200 - total flux cleaned = 0.00367683 Jy ! Total flux subtracted in 200 components = 0.00367683 Jy ! Clean residual min=-0.002926 max=0.002927 Jy/beam ! Clean residual mean=0.000031 rms=0.000623 Jy/beam ! Combined flux in latest and established models = 0.702925 Jy ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 193 components and 0.702925 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.067165Jy sigma=0.801941 ! Fit after self-cal, rms=0.067147Jy sigma=0.801798 ! Inverting map ! Your choice of large map pixels excluded 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000661985 Jy ! Component: 100 - total flux cleaned = 0.000664242 Jy ! Component: 150 - total flux cleaned = 0.000666059 Jy ! Component: 200 - total flux cleaned = 0.000607074 Jy ! Total flux subtracted in 200 components = 0.000607074 Jy ! Clean residual min=-0.002927 max=0.002920 Jy/beam ! Clean residual mean=0.000032 rms=0.000616 Jy/beam ! Combined flux in latest and established models = 0.703532 Jy ! Performing phase self-cal ! Adding 47 model components to the UV plane model. ! The established model now contains 207 components and 0.703532 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.067032Jy sigma=0.800210 ! Fit after self-cal, rms=0.067025Jy sigma=0.800175 ! Inverting map ! Your choice of large map pixels excluded 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.067025Jy sigma=0.800175 ! Fit after self-cal, rms=0.067008Jy sigma=0.799881 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 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 milli-arcsec ! Estimated beam: bmin=0.6198 mas, bmaj=0.9186 mas, bpa=-17.8 degrees ! Estimated noise=0.983557 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.402781 Jy ! Component: 100 - total flux cleaned = 0.517937 Jy ! Component: 150 - total flux cleaned = 0.574019 Jy ! Component: 200 - total flux cleaned = 0.604686 Jy ! Total flux subtracted in 200 components = 0.604686 Jy ! Clean residual min=-0.005455 max=0.014939 Jy/beam ! Clean residual mean=-0.000038 rms=0.001335 Jy/beam ! Combined flux in latest and established models = 0.604687 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 14 model components to the UV plane model. ! The established model now contains 14 components and 0.604687 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 milli-arcsec ! Estimated beam: bmin=0.6972 mas, bmaj=1.058 mas, bpa=-16.85 degrees ! Estimated noise=0.693914 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 = 0.0246777 Jy ! Component: 100 - total flux cleaned = 0.0384247 Jy ! Component: 150 - total flux cleaned = 0.0480688 Jy ! Component: 200 - total flux cleaned = 0.055869 Jy ! Total flux subtracted in 200 components = 0.055869 Jy ! Clean residual min=-0.003675 max=0.005610 Jy/beam ! Clean residual mean=-0.000112 rms=0.001017 Jy/beam ! Combined flux in latest and established models = 0.660556 Jy ! Adding 51 model components to the UV plane model. ! The established model now contains 56 components and 0.660556 Jy ! Inverting map ! Your choice of large map pixels excluded 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 milli-arcsec ! Added new window around map position (-3.2, -3). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00668788 Jy ! Component: 100 - total flux cleaned = 0.0122091 Jy ! Component: 150 - total flux cleaned = 0.0169455 Jy ! Component: 200 - total flux cleaned = 0.0210492 Jy ! Total flux subtracted in 200 components = 0.0210492 Jy ! Clean residual min=-0.003398 max=0.003220 Jy/beam ! Clean residual mean=-0.000043 rms=0.000744 Jy/beam ! Combined flux in latest and established models = 0.681605 Jy ! Adding 61 model components to the UV plane model. ! The established model now contains 93 components and 0.681605 Jy ! Inverting map ! Your choice of large map pixels excluded 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 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 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 milli-arcsec ! Estimated beam: bmin=2.48 mas, bmaj=3.225 mas, bpa=40.87 degrees ! Estimated noise=0.929758 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00616002 Jy ! Component: 100 - total flux cleaned = 0.0103753 Jy ! Component: 150 - total flux cleaned = 0.0135694 Jy ! Component: 200 - total flux cleaned = 0.0158623 Jy ! Total flux subtracted in 200 components = 0.0158623 Jy ! Clean residual min=-0.002913 max=0.003244 Jy/beam ! Clean residual mean=0.000014 rms=0.000860 Jy/beam ! Combined flux in latest and established models = 0.697467 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 = 0.00121879 Jy ! Component: 100 - total flux cleaned = 0.0022522 Jy ! Component: 150 - total flux cleaned = 0.00290624 Jy ! Component: 200 - total flux cleaned = 0.00348359 Jy ! Total flux subtracted in 200 components = 0.00348359 Jy ! Clean residual min=-0.002782 max=0.003360 Jy/beam ! Clean residual mean=0.000040 rms=0.000820 Jy/beam ! Combined flux in latest and established models = 0.700951 Jy ! Adding 111 model components to the UV plane model. ! The established model now contains 197 components and 0.700951 Jy ! Inverting map ! Your choice of large map pixels excluded 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 milli-arcsec ! Estimated beam: bmin=0.6972 mas, bmaj=1.058 mas, bpa=-16.85 degrees ! Estimated noise=0.693914 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000353782 Jy ! Component: 100 - total flux cleaned = 0.000918353 Jy ! Component: 150 - total flux cleaned = 0.00107089 Jy ! Component: 200 - total flux cleaned = 0.0012144 Jy ! Total flux subtracted in 200 components = 0.0012144 Jy ! Clean residual min=-0.003107 max=0.002522 Jy/beam ! Clean residual mean=0.000019 rms=0.000616 Jy/beam ! Combined flux in latest and established models = 0.702165 Jy selfcal ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 219 components and 0.702165 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.067456Jy sigma=0.802819 ! Fit after self-cal, rms=0.067288Jy sigma=0.801037 wmodel J1506+3730_X_map.mod ! Writing 219 model components to file: J1506+3730_X_map.mod wobs J1506+3730_X_uvs.fits ! Writing UV FITS file: J1506+3730_X_uvs.fits wwins J1506+3730_X_map.win ! wwins: Wrote 8 windows to J1506+3730_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 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00104256 Jy ! Component: 100 - total flux cleaned = -0.000668453 Jy ! Component: 150 - total flux cleaned = -0.00026506 Jy ! Component: 200 - total flux cleaned = 3.84951e-05 Jy ! Component: 250 - total flux cleaned = 0.00020948 Jy ! Component: 300 - total flux cleaned = 0.000419162 Jy ! Component: 350 - total flux cleaned = 0.000664906 Jy ! Component: 400 - total flux cleaned = 0.000906337 Jy ! Component: 450 - total flux cleaned = 0.00118328 Jy ! Component: 500 - total flux cleaned = 0.00145641 Jy ! Component: 550 - total flux cleaned = 0.00172556 Jy ! Component: 600 - total flux cleaned = 0.00195326 Jy ! Component: 650 - total flux cleaned = 0.00199145 Jy ! Component: 700 - total flux cleaned = 0.00217777 Jy ! Component: 750 - total flux cleaned = 0.00243541 Jy ! Component: 800 - total flux cleaned = 0.00258111 Jy ! Component: 850 - total flux cleaned = 0.00261733 Jy ! Component: 900 - total flux cleaned = 0.00276074 Jy ! Component: 950 - total flux cleaned = 0.00304416 Jy ! Component: 1000 - total flux cleaned = 0.00307966 Jy ! Component: 1050 - total flux cleaned = 0.00339295 Jy ! Component: 1100 - total flux cleaned = 0.00346183 Jy ! Component: 1150 - total flux cleaned = 0.00353075 Jy ! Component: 1200 - total flux cleaned = 0.00380284 Jy ! Component: 1250 - total flux cleaned = 0.00383639 Jy ! Component: 1300 - total flux cleaned = 0.00393729 Jy ! Component: 1350 - total flux cleaned = 0.00400377 Jy ! Component: 1400 - total flux cleaned = 0.0041033 Jy ! Component: 1450 - total flux cleaned = 0.00420187 Jy ! Component: 1500 - total flux cleaned = 0.0043656 Jy ! Component: 1550 - total flux cleaned = 0.0045279 Jy ! Component: 1600 - total flux cleaned = 0.004528 Jy ! Component: 1650 - total flux cleaned = 0.00459197 Jy ! Component: 1700 - total flux cleaned = 0.00462395 Jy ! Component: 1750 - total flux cleaned = 0.00475095 Jy ! Component: 1800 - total flux cleaned = 0.00494009 Jy ! Component: 1850 - total flux cleaned = 0.00494011 Jy ! Component: 1900 - total flux cleaned = 0.00484658 Jy ! Component: 1950 - total flux cleaned = 0.0049086 Jy ! Component: 2000 - total flux cleaned = 0.0049396 Jy ! Component: 2050 - total flux cleaned = 0.00512385 Jy ! Component: 2100 - total flux cleaned = 0.00500139 Jy ! Component: 2150 - total flux cleaned = 0.00518387 Jy ! Component: 2200 - total flux cleaned = 0.00512297 Jy ! Component: 2250 - total flux cleaned = 0.00524329 Jy ! Component: 2300 - total flux cleaned = 0.00527323 Jy ! Component: 2350 - total flux cleaned = 0.00521353 Jy ! Component: 2400 - total flux cleaned = 0.00533212 Jy ! Component: 2450 - total flux cleaned = 0.00533204 Jy ! Component: 2500 - total flux cleaned = 0.00536148 Jy ! Component: 2550 - total flux cleaned = 0.00556628 Jy ! Component: 2600 - total flux cleaned = 0.00553701 Jy ! Component: 2650 - total flux cleaned = 0.00553699 Jy ! Component: 2700 - total flux cleaned = 0.00553681 Jy ! Component: 2750 - total flux cleaned = 0.00559412 Jy ! Component: 2800 - total flux cleaned = 0.00559399 Jy ! Component: 2850 - total flux cleaned = 0.00573641 Jy ! Component: 2900 - total flux cleaned = 0.00562295 Jy ! Component: 2950 - total flux cleaned = 0.00582066 Jy ! Component: 3000 - total flux cleaned = 0.00584892 Jy ! Component: 3050 - total flux cleaned = 0.00579295 Jy ! Component: 3100 - total flux cleaned = 0.00587635 Jy ! Component: 3150 - total flux cleaned = 0.00582087 Jy ! Component: 3200 - total flux cleaned = 0.00593162 Jy ! Component: 3250 - total flux cleaned = 0.00590429 Jy ! Component: 3300 - total flux cleaned = 0.00601409 Jy ! Component: 3350 - total flux cleaned = 0.00587737 Jy ! Component: 3400 - total flux cleaned = 0.00601353 Jy ! Component: 3450 - total flux cleaned = 0.00604066 Jy ! Component: 3500 - total flux cleaned = 0.00614872 Jy ! Component: 3550 - total flux cleaned = 0.00614885 Jy ! Component: 3600 - total flux cleaned = 0.00609525 Jy ! Component: 3650 - total flux cleaned = 0.00622871 Jy ! Component: 3700 - total flux cleaned = 0.00617552 Jy ! Component: 3750 - total flux cleaned = 0.00625489 Jy ! Component: 3800 - total flux cleaned = 0.00628119 Jy ! Component: 3850 - total flux cleaned = 0.00630742 Jy ! Component: 3900 - total flux cleaned = 0.00649064 Jy ! Component: 3950 - total flux cleaned = 0.00641251 Jy ! Component: 4000 - total flux cleaned = 0.0064642 Jy ! Component: 4050 - total flux cleaned = 0.00651605 Jy ! Total flux subtracted in 4096 components = 0.00669683 Jy ! Clean residual min=-0.001491 max=0.001544 Jy/beam ! Clean residual mean=0.000005 rms=0.000424 Jy/beam ! Combined flux in latest and established models = 0.708862 Jy keep ! Adding 352 model components to the UV plane model. ! The established model now contains 570 components and 0.708862 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv121_uvs/J1506+3730_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6972 x 1.058 at -16.85 degrees (North through East) ! Clean map min=-0.0021839 max=0.50638 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv121_uvs/J1506+3730_X_map.fits wmodel /scr/pima/rv121_uvs/J1506+3730_X_map.mod ! Writing 570 model components to file: /scr/pima/rv121_uvs/J1506+3730_X_map.mod wobs /scr/pima/rv121_uvs/J1506+3730_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv121_uvs/J1506+3730_X_uvs.fits wwins /scr/pima/rv121_uvs/J1506+3730_X_map.win ! wwins: Wrote 9 windows to /scr/pima/rv121_uvs/J1506+3730_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.506375 invert ! Inverting map ! Your choice of large map pixels excluded 2.81% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1753 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000424 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.251197 0.251197 0.502395 1.00479 2.00958 4.01916 8.03831 16.0766 32.1533 64.3065 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0012 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.506 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 1194.28 quit ! Quitting program ! Log file /scr/pima/rv121_uvs/J1506+3730_X_dfm.log closed on Sat Jul 28 00:42:00 2018