! Started logfile: /scr/pima/rv122_uvs/J1936+7131_X_dfm.log on Fri Jul 13 21:10:26 2018 float field_size field_size = 1024 float field_cell field_cell = 0.2000 float taper_size taper_size = 70.0 float freq freq = 8.36575 obs /scr/pima/rv122_uvs/J1936+7131_X_uva.fits ! Reading UV FITS file: /scr/pima/rv122_uvs/J1936+7131_X_uva.fits ! AN table 1: 67 integrations on 66 of 66 possible baselines. ! Apparent sampling: 0.431253 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1936+7131 ! ! There are 4 IFs, and a total of 4 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 8.36575e+09 8e+06 1 8e+06 ! 02 2 8.44575e+09 8e+06 1 8e+06 ! 03 3 8.80575e+09 8e+06 1 8e+06 ! 04 4 8.92575e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 69 lines of history. ! ! Reading 7628 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 J1936+7131_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 374 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 374 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 374 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 374 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=1.040671Jy sigma=17.049182 ! Fit after self-cal, rms=0.729051Jy sigma=11.849273 ! 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 2.14% of the data. ! The y-axis pixel size should ideally be below 0.1719 milli-arcsec ! Estimated beam: bmin=0.5386 mas, bmaj=0.8964 mas, bpa=44.29 degrees ! Estimated noise=0.835064 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 = 0.202321 Jy ! Component: 100 - total flux cleaned = 0.261704 Jy ! Total flux subtracted in 100 components = 0.261704 Jy ! Clean residual min=-0.007629 max=0.025498 Jy/beam ! Clean residual mean=-0.000013 rms=0.001629 Jy/beam ! Combined flux in latest and established models = 0.261704 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.261704 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.096125Jy sigma=1.476548 ! Fit after self-cal, rms=0.095903Jy sigma=1.472460 ! Inverting map ! Your choice of large map pixels excluded 2.14% of the data. ! The y-axis pixel size should ideally be below 0.1719 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0278629 Jy ! Component: 100 - total flux cleaned = 0.0420685 Jy ! Total flux subtracted in 100 components = 0.0420685 Jy ! Clean residual min=-0.007113 max=0.013620 Jy/beam ! Clean residual mean=-0.000008 rms=0.001292 Jy/beam ! Combined flux in latest and established models = 0.303773 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 9 components and 0.303773 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.082668Jy sigma=1.210422 ! Fit after self-cal, rms=0.082563Jy sigma=1.207917 ! Inverting map ! Your choice of large map pixels excluded 2.14% of the data. ! The y-axis pixel size should ideally be below 0.1719 milli-arcsec ! Added new window around map position (0, -1.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0126329 Jy ! Component: 100 - total flux cleaned = 0.0205394 Jy ! Total flux subtracted in 100 components = 0.0205394 Jy ! Clean residual min=-0.007042 max=0.008435 Jy/beam ! Clean residual mean=-0.000006 rms=0.001195 Jy/beam ! Combined flux in latest and established models = 0.324312 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 17 components and 0.324312 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.079715Jy sigma=1.139796 ! Fit after self-cal, rms=0.079408Jy sigma=1.135490 ! Inverting map ! Your choice of large map pixels excluded 2.14% of the data. ! The y-axis pixel size should ideally be below 0.1719 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 2.14% of the data. ! The y-axis pixel size should ideally be below 0.1719 milli-arcsec ! Estimated beam: bmin=0.6267 mas, bmaj=1.046 mas, bpa=47.63 degrees ! Estimated noise=0.554836 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 = 0.0136068 Jy ! Component: 100 - total flux cleaned = 0.0209433 Jy ! Component: 150 - total flux cleaned = 0.0254183 Jy ! Component: 200 - total flux cleaned = 0.0282249 Jy ! Total flux subtracted in 200 components = 0.0282249 Jy ! Clean residual min=-0.006671 max=0.005724 Jy/beam ! Clean residual mean=-0.000016 rms=0.001398 Jy/beam ! Combined flux in latest and established models = 0.352537 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 27 components and 0.352537 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.077365Jy sigma=1.088095 ! Fit after self-cal, rms=0.077229Jy sigma=1.086237 ! Inverting map ! Your choice of large map pixels excluded 2.14% of the data. ! The y-axis pixel size should ideally be below 0.1719 milli-arcsec print "============== Finished natural weighting clean ==============" ! ============== Finished natural weighting clean ============== ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6267 x 1.046 at 47.63 degrees (North through East) ! Clean map min=-0.0058972 max=0.27071 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 72 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.95 HN 0.99 KP 1.10 ! LA 1.05 MK 0.99 NY 0.94 ON 0.93 ! OV 1.00 PT 0.88 SC 1.07 WZ 0.99 ! ! ! Correcting IF 2. ! A total of 72 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.95 HN 1.02 KP 1.08 ! LA 1.06 MK 1.00 NY 0.94 ON 0.96 ! OV 1.01 PT 0.87 SC 1.07 WZ 1.00 ! ! ! Correcting IF 3. ! A total of 72 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.96 HN 1.05 KP 1.11 ! LA 1.07 MK 1.01 NY 0.95 ON 0.97 ! OV 1.00 PT 0.91 SC 1.05 WZ 1.02 ! ! ! Correcting IF 4. ! A total of 72 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 0.95 HN 1.06 KP 1.12 ! LA 1.09 MK 1.01 NY 0.94 ON 0.96 ! OV 0.99 PT 0.90 SC 1.05 WZ 1.03 ! ! ! Fit before self-cal, rms=0.077229Jy sigma=1.086237 ! Fit after self-cal, rms=0.072059Jy sigma=1.009013 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 milli-arcsec ! Estimated beam: bmin=0.6189 mas, bmaj=1.061 mas, bpa=47.85 degrees ! Estimated noise=0.560525 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 (0.8, -2.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00207152 Jy ! Component: 100 - total flux cleaned = 0.00230318 Jy ! Component: 150 - total flux cleaned = 0.00257923 Jy ! Component: 200 - total flux cleaned = 0.00272845 Jy ! Total flux subtracted in 200 components = 0.00272845 Jy ! Clean residual min=-0.003336 max=0.003498 Jy/beam ! Clean residual mean=-0.000016 rms=0.000698 Jy/beam ! Combined flux in latest and established models = 0.355265 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 50 components and 0.355265 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.071734Jy sigma=1.003139 ! Fit after self-cal, rms=0.071709Jy sigma=1.002396 ! Inverting map ! Your choice of large map pixels excluded 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 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=0.071709Jy sigma=1.002396 ! Fit after self-cal, rms=0.070446Jy sigma=0.980920 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 milli-arcsec ! Estimated beam: bmin=0.6174 mas, bmaj=1.06 mas, bpa=47.99 degrees ! Estimated noise=0.561335 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00180599 Jy ! Component: 100 - total flux cleaned = 0.0023971 Jy ! Component: 150 - total flux cleaned = 0.00278893 Jy ! Component: 200 - total flux cleaned = 0.00310024 Jy ! Total flux subtracted in 200 components = 0.00310024 Jy ! Clean residual min=-0.002319 max=0.002402 Jy/beam ! Clean residual mean=-0.000001 rms=0.000594 Jy/beam ! Combined flux in latest and established models = 0.358366 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 59 components and 0.358366 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.070326Jy sigma=0.978965 ! Fit after self-cal, rms=0.070300Jy sigma=0.978624 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 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 = 2.84237e-05 Jy ! Component: 100 - total flux cleaned = 0.000260855 Jy ! Component: 150 - total flux cleaned = 0.000514344 Jy ! Component: 200 - total flux cleaned = 0.000676258 Jy ! Total flux subtracted in 200 components = 0.000676258 Jy ! Clean residual min=-0.002318 max=0.002356 Jy/beam ! Clean residual mean=-0.000000 rms=0.000591 Jy/beam ! Combined flux in latest and established models = 0.359042 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 67 components and 0.359042 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.070263Jy sigma=0.977959 ! Fit after self-cal, rms=0.070250Jy sigma=0.977797 ! Inverting map ! Your choice of large map pixels excluded 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 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=0.070250Jy sigma=0.977797 ! Fit after self-cal, rms=0.070054Jy sigma=0.977315 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 milli-arcsec ! Estimated beam: bmin=0.6159 mas, bmaj=1.061 mas, bpa=47.94 degrees ! Estimated noise=0.56155 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000977253 Jy ! Component: 100 - total flux cleaned = 0.00128664 Jy ! Component: 150 - total flux cleaned = 0.00154307 Jy ! Component: 200 - total flux cleaned = 0.00167875 Jy ! Total flux subtracted in 200 components = 0.00167875 Jy ! Clean residual min=-0.002284 max=0.002382 Jy/beam ! Clean residual mean=-0.000000 rms=0.000572 Jy/beam ! Combined flux in latest and established models = 0.360721 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 73 components and 0.360721 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.070011Jy sigma=0.976563 ! Fit after self-cal, rms=0.069998Jy sigma=0.976438 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 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 = 7.92096e-05 Jy ! Component: 100 - total flux cleaned = 0.000252791 Jy ! Component: 150 - total flux cleaned = 0.000325218 Jy ! Component: 200 - total flux cleaned = 0.000324498 Jy ! Total flux subtracted in 200 components = 0.000324498 Jy ! Clean residual min=-0.002290 max=0.002373 Jy/beam ! Clean residual mean=-0.000000 rms=0.000571 Jy/beam ! Combined flux in latest and established models = 0.361045 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 74 components and 0.361045 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.069977Jy sigma=0.976044 ! Fit after self-cal, rms=0.069969Jy sigma=0.975942 ! Inverting map ! Your choice of large map pixels excluded 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 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=0.069969Jy sigma=0.975942 ! Fit after self-cal, rms=0.069912Jy sigma=0.975789 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 milli-arcsec ! Estimated beam: bmin=2.682 mas, bmaj=3.25 mas, bpa=-75.02 degrees ! Estimated noise=0.804163 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000960841 Jy ! Component: 100 - total flux cleaned = 0.00105647 Jy ! Component: 150 - total flux cleaned = 0.00104674 Jy ! Component: 200 - total flux cleaned = 0.00105686 Jy ! Total flux subtracted in 200 components = 0.00105686 Jy ! Clean residual min=-0.002763 max=0.002805 Jy/beam ! Clean residual mean=-0.000000 rms=0.000821 Jy/beam ! Combined flux in latest and established models = 0.362102 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 82 components and 0.362102 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.069901Jy sigma=0.975532 ! Fit after self-cal, rms=0.069895Jy sigma=0.975495 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 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 = 0.000113527 Jy ! Component: 100 - total flux cleaned = 0.000124897 Jy ! Component: 150 - total flux cleaned = 0.000106234 Jy ! Component: 200 - total flux cleaned = 0.000106853 Jy ! Total flux subtracted in 200 components = 0.000106853 Jy ! Clean residual min=-0.002764 max=0.002811 Jy/beam ! Clean residual mean=0.000000 rms=0.000821 Jy/beam ! Combined flux in latest and established models = 0.362209 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 82 components and 0.362209 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.069894Jy sigma=0.975402 ! Fit after self-cal, rms=0.069890Jy sigma=0.975383 ! Inverting map ! Your choice of large map pixels excluded 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 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 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 milli-arcsec ! Estimated beam: bmin=0.6149 mas, bmaj=1.061 mas, bpa=47.9 degrees ! Estimated noise=0.561993 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6149 x 1.061 at 47.9 degrees (North through East) ! Clean map min=-0.0018244 max=0.2697 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 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 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 milli-arcsec ! Estimated beam: bmin=0.5267 mas, bmaj=0.9093 mas, bpa=45.04 degrees ! Estimated noise=0.863908 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.207081 Jy ! Component: 100 - total flux cleaned = 0.268667 Jy ! Component: 150 - total flux cleaned = 0.296182 Jy ! Component: 200 - total flux cleaned = 0.313461 Jy ! Total flux subtracted in 200 components = 0.313461 Jy ! Clean residual min=-0.004781 max=0.009508 Jy/beam ! Clean residual mean=-0.000006 rms=0.001047 Jy/beam ! Combined flux in latest and established models = 0.313461 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 13 model components to the UV plane model. ! The established model now contains 13 components and 0.313461 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 milli-arcsec ! Estimated beam: bmin=0.6149 mas, bmaj=1.061 mas, bpa=47.9 degrees ! Estimated noise=0.561993 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 = 0.0191076 Jy ! Component: 100 - total flux cleaned = 0.0302849 Jy ! Component: 150 - total flux cleaned = 0.0372172 Jy ! Component: 200 - total flux cleaned = 0.0416051 Jy ! Total flux subtracted in 200 components = 0.0416051 Jy ! Clean residual min=-0.002476 max=0.002914 Jy/beam ! Clean residual mean=-0.000004 rms=0.000611 Jy/beam ! Combined flux in latest and established models = 0.355066 Jy ! Adding 28 model components to the UV plane model. ! The established model now contains 31 components and 0.355066 Jy ! Inverting map ! Your choice of large map pixels excluded 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 milli-arcsec ! Added new window around map position (-21.2, -38.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00309306 Jy ! Component: 100 - total flux cleaned = 0.00484786 Jy ! Component: 150 - total flux cleaned = 0.00553024 Jy ! Component: 200 - total flux cleaned = 0.00581653 Jy ! Total flux subtracted in 200 components = 0.00581653 Jy ! Clean residual min=-0.002326 max=0.002509 Jy/beam ! Clean residual mean=-0.000000 rms=0.000565 Jy/beam ! Combined flux in latest and established models = 0.360883 Jy ! Adding 23 model components to the UV plane model. ! The established model now contains 42 components and 0.360883 Jy ! Inverting map ! Your choice of large map pixels excluded 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 milli-arcsec ! Added new window around map position (-23.4, -47.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00108358 Jy ! Component: 100 - total flux cleaned = 0.00135142 Jy ! Component: 150 - total flux cleaned = 0.00164184 Jy ! Component: 200 - total flux cleaned = 0.00182122 Jy ! Total flux subtracted in 200 components = 0.00182122 Jy ! Clean residual min=-0.002291 max=0.002363 Jy/beam ! Clean residual mean=-0.000000 rms=0.000554 Jy/beam ! Combined flux in latest and established models = 0.362704 Jy ! Adding 30 model components to the UV plane model. ! The established model now contains 59 components and 0.362704 Jy ! Inverting map ! Your choice of large map pixels excluded 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 milli-arcsec ! Added new window around map position (40, -38.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00214615 Jy ! Component: 100 - total flux cleaned = 0.00241656 Jy ! Component: 150 - total flux cleaned = 0.00254215 Jy ! Component: 200 - total flux cleaned = 0.00269881 Jy ! Total flux subtracted in 200 components = 0.00269881 Jy ! Clean residual min=-0.002251 max=0.002197 Jy/beam ! Clean residual mean=-0.000002 rms=0.000537 Jy/beam ! Combined flux in latest and established models = 0.365403 Jy ! Adding 38 model components to the UV plane model. ! The established model now contains 73 components and 0.365403 Jy ! Inverting map ! Your choice of large map pixels excluded 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 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 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 milli-arcsec ! Estimated beam: bmin=2.682 mas, bmaj=3.25 mas, bpa=-75.02 degrees ! Estimated noise=0.804163 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000996192 Jy ! Component: 100 - total flux cleaned = 0.00143737 Jy ! Component: 150 - total flux cleaned = 0.0017198 Jy ! Component: 200 - total flux cleaned = 0.00189177 Jy ! Total flux subtracted in 200 components = 0.00189177 Jy ! Clean residual min=-0.002586 max=0.002517 Jy/beam ! Clean residual mean=-0.000006 rms=0.000711 Jy/beam ! Combined flux in latest and established models = 0.367294 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 = 0.000153546 Jy ! Component: 100 - total flux cleaned = 0.000290176 Jy ! Component: 150 - total flux cleaned = 0.000378037 Jy ! Component: 200 - total flux cleaned = 0.000458132 Jy ! Total flux subtracted in 200 components = 0.000458132 Jy ! Clean residual min=-0.002580 max=0.002544 Jy/beam ! Clean residual mean=-0.000006 rms=0.000706 Jy/beam ! Combined flux in latest and established models = 0.367753 Jy ! Adding 28 model components to the UV plane model. ! The established model now contains 99 components and 0.367753 Jy ! Inverting map ! Your choice of large map pixels excluded 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 milli-arcsec ! Estimated beam: bmin=0.6149 mas, bmaj=1.061 mas, bpa=47.9 degrees ! Estimated noise=0.561993 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00075606 Jy ! Component: 100 - total flux cleaned = -0.000937584 Jy ! Component: 150 - total flux cleaned = -0.000903633 Jy ! Component: 200 - total flux cleaned = -0.000936788 Jy ! Total flux subtracted in 200 components = -0.000936788 Jy ! Clean residual min=-0.002270 max=0.002144 Jy/beam ! Clean residual mean=-0.000002 rms=0.000531 Jy/beam ! Combined flux in latest and established models = 0.366816 Jy selfcal ! Performing phase self-cal ! Adding 34 model components to the UV plane model. ! The established model now contains 119 components and 0.366816 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.069737Jy sigma=0.973143 ! Fit after self-cal, rms=0.069670Jy sigma=0.972269 wmodel J1936+7131_X_map.mod ! Writing 119 model components to file: J1936+7131_X_map.mod wobs J1936+7131_X_uvs.fits ! Writing UV FITS file: J1936+7131_X_uvs.fits wwins J1936+7131_X_map.win ! wwins: Wrote 6 windows to J1936+7131_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 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 5.12779e-05 Jy ! Component: 100 - total flux cleaned = -0.000222467 Jy ! Component: 150 - total flux cleaned = -0.0002605 Jy ! Component: 200 - total flux cleaned = -0.000185982 Jy ! Component: 250 - total flux cleaned = -0.000221984 Jy ! Component: 300 - total flux cleaned = -5.68226e-06 Jy ! Component: 350 - total flux cleaned = 2.96002e-05 Jy ! Component: 400 - total flux cleaned = 6.49949e-05 Jy ! Component: 450 - total flux cleaned = 9.98468e-05 Jy ! Component: 500 - total flux cleaned = 0.000100198 Jy ! Component: 550 - total flux cleaned = 0.00023604 Jy ! Component: 600 - total flux cleaned = 0.00026908 Jy ! Component: 650 - total flux cleaned = 0.00026887 Jy ! Component: 700 - total flux cleaned = 0.000169844 Jy ! Component: 750 - total flux cleaned = 0.000202609 Jy ! Component: 800 - total flux cleaned = 0.000267589 Jy ! Component: 850 - total flux cleaned = 0.000267416 Jy ! Component: 900 - total flux cleaned = 0.000235245 Jy ! Component: 950 - total flux cleaned = 0.000266904 Jy ! Component: 1000 - total flux cleaned = 0.000329625 Jy ! Component: 1050 - total flux cleaned = 0.000329583 Jy ! Component: 1100 - total flux cleaned = 0.000360237 Jy ! Component: 1150 - total flux cleaned = 0.000421361 Jy ! Component: 1200 - total flux cleaned = 0.000421246 Jy ! Component: 1250 - total flux cleaned = 0.000421291 Jy ! Component: 1300 - total flux cleaned = 0.000361007 Jy ! Component: 1350 - total flux cleaned = 0.000481101 Jy ! Component: 1400 - total flux cleaned = 0.000510467 Jy ! Component: 1450 - total flux cleaned = 0.000569663 Jy ! Component: 1500 - total flux cleaned = 0.000658233 Jy ! Component: 1550 - total flux cleaned = 0.000482081 Jy ! Component: 1600 - total flux cleaned = 0.000715621 Jy ! Component: 1650 - total flux cleaned = 0.000744626 Jy ! Component: 1700 - total flux cleaned = 0.000744861 Jy ! Component: 1750 - total flux cleaned = 0.000888022 Jy ! Component: 1800 - total flux cleaned = 0.000887916 Jy ! Component: 1850 - total flux cleaned = 0.000972983 Jy ! Component: 1900 - total flux cleaned = 0.00114285 Jy ! Component: 1950 - total flux cleaned = 0.00122701 Jy ! Component: 2000 - total flux cleaned = 0.00131092 Jy ! Component: 2050 - total flux cleaned = 0.00147815 Jy ! Component: 2100 - total flux cleaned = 0.0013949 Jy ! Component: 2150 - total flux cleaned = 0.00153291 Jy ! Component: 2200 - total flux cleaned = 0.00161541 Jy ! Component: 2250 - total flux cleaned = 0.00183419 Jy ! Component: 2300 - total flux cleaned = 0.00183408 Jy ! Component: 2350 - total flux cleaned = 0.00199666 Jy ! Component: 2400 - total flux cleaned = 0.00210479 Jy ! Component: 2450 - total flux cleaned = 0.00207787 Jy ! Component: 2500 - total flux cleaned = 0.00215789 Jy ! Component: 2550 - total flux cleaned = 0.00205138 Jy ! Component: 2600 - total flux cleaned = 0.00223735 Jy ! Component: 2650 - total flux cleaned = 0.00226388 Jy ! Component: 2700 - total flux cleaned = 0.00236922 Jy ! Component: 2750 - total flux cleaned = 0.00244789 Jy ! Component: 2800 - total flux cleaned = 0.00252629 Jy ! Component: 2850 - total flux cleaned = 0.00242219 Jy ! Component: 2900 - total flux cleaned = 0.00260341 Jy ! Component: 2950 - total flux cleaned = 0.00268065 Jy ! Component: 3000 - total flux cleaned = 0.00278347 Jy ! Component: 3050 - total flux cleaned = 0.00252747 Jy ! Component: 3100 - total flux cleaned = 0.00260392 Jy ! Component: 3150 - total flux cleaned = 0.00280724 Jy ! Component: 3200 - total flux cleaned = 0.00283272 Jy ! Component: 3250 - total flux cleaned = 0.00283273 Jy ! Component: 3300 - total flux cleaned = 0.00268182 Jy ! Component: 3350 - total flux cleaned = 0.00265692 Jy ! Component: 3400 - total flux cleaned = 0.00265701 Jy ! Component: 3450 - total flux cleaned = 0.00275627 Jy ! Component: 3500 - total flux cleaned = 0.0027564 Jy ! Component: 3550 - total flux cleaned = 0.00280587 Jy ! Component: 3600 - total flux cleaned = 0.00280582 Jy ! Component: 3650 - total flux cleaned = 0.00290388 Jy ! Component: 3700 - total flux cleaned = 0.00285499 Jy ! Component: 3750 - total flux cleaned = 0.00283053 Jy ! Component: 3800 - total flux cleaned = 0.00292777 Jy ! Component: 3850 - total flux cleaned = 0.00292779 Jy ! Component: 3900 - total flux cleaned = 0.00292788 Jy ! Component: 3950 - total flux cleaned = 0.00285576 Jy ! Component: 4000 - total flux cleaned = 0.0030236 Jy ! Component: 4050 - total flux cleaned = 0.00307152 Jy ! Total flux subtracted in 4096 components = 0.00314306 Jy ! Clean residual min=-0.001314 max=0.001353 Jy/beam ! Clean residual mean=-0.000002 rms=0.000397 Jy/beam ! Combined flux in latest and established models = 0.369959 Jy keep ! Adding 362 model components to the UV plane model. ! The established model now contains 481 components and 0.369959 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv122_uvs/J1936+7131_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6149 x 1.061 at 47.9 degrees (North through East) ! Clean map min=-0.0018405 max=0.26943 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv122_uvs/J1936+7131_X_map.fits wmodel /scr/pima/rv122_uvs/J1936+7131_X_map.mod ! Writing 481 model components to file: /scr/pima/rv122_uvs/J1936+7131_X_map.mod wobs /scr/pima/rv122_uvs/J1936+7131_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv122_uvs/J1936+7131_X_uvs.fits wwins /scr/pima/rv122_uvs/J1936+7131_X_map.win ! wwins: Wrote 7 windows to /scr/pima/rv122_uvs/J1936+7131_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.269435 invert ! Inverting map ! Your choice of large map pixels excluded 2.23% of the data. ! The y-axis pixel size should ideally be below 0.1719 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000396767 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.441777 0.441777 0.883555 1.76711 3.53422 7.06844 14.1369 28.2738 56.5475 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0011 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.269 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 679.074 quit ! Quitting program ! Log file /scr/pima/rv122_uvs/J1936+7131_X_dfm.log closed on Fri Jul 13 21:10:30 2018