! Started logfile: /vlbi/vcs9/uvm//J0148+1028_X_a_dfm.log on Tue Dec 26 21:08:09 2017 float field_size field_size = 1024 float field_cell field_cell = 0.2000 float taper_size taper_size = 70.0 float freq freq = 7.39200 obs /vlbi/vcs9/uvm//J0148+1028_X_a_uvm.fits ! Reading UV FITS file: /vlbi/vcs9/uvm//J0148+1028_X_a_uvm.fits ! AN table 1: 29 integrations on 15 of 15 possible baselines. ! AN table 2: 53 integrations on 21 of 21 possible baselines. ! Apparent sampling: 0.95478 visibilities/baseline/integration-bin. ! Found source: J0148+1028 ! ! There are 8 IFs, and a total of 8 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 7.392e+09 3.2e+07 1 3.2e+07 ! 02 2 7.424e+09 3.2e+07 1 3.2e+07 ! 03 3 7.456e+09 3.2e+07 1 3.2e+07 ! 04 4 7.552e+09 3.2e+07 1 3.2e+07 ! 05 5 7.744e+09 3.2e+07 1 3.2e+07 ! 06 6 7.776e+09 3.2e+07 1 3.2e+07 ! 07 7 7.808e+09 3.2e+07 1 3.2e+07 ! 08 8 7.84e+09 3.2e+07 1 3.2e+07 ! ! Polarization(s): RR ! ! Read 85 lines of history. ! ! Reading 11824 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 8 channels. ! Selecting polarization: RR, channels: 1..8 ! Reading IF 1 channels: 1..1 ! Reading IF 2 channels: 2..2 ! Reading IF 3 channels: 3..3 ! Reading IF 4 channels: 4..4 ! Reading IF 5 channels: 5..5 ! Reading IF 6 channels: 6..6 ! Reading IF 7 channels: 7..7 ! Reading IF 8 channels: 8..8 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_02.dfm J0148+1028_X] integer clean_niter clean_niter = 100 float clean_gain clean_gain = 0.04 float dynam dynam = 6.0 float amp_soltime1 amp_soltime1 = 60 float amp_soltime2 amp_soltime2 = 5 float phase_soltime1 phase_soltime1=10 float phase_soltime2 phase_soltime2=0.5 float phase_soltime phase_soltime=phase_soltime1 float ampcor_selflim ampcor_selflim=1.20 float thresh thresh = 0.1 float win_mult win_mult = 1.8 float time_av time_av = 30 float old_peak float new_peak float flux_cutoff print "===============================================================" ! =============================================================== ! print "=== Difmap script: pima_mupet_02.dvm version of 2017.12.26 === " ! === Difmap script: pima_mupet_02.dvm version of 2017.12.26 === ! mapsize field_size, field_cell ! Map grid = 1024x1024 pixels with 0.200x0.200 milli-arcsec cellsize. phase_soltime=phase_soltime1 print "uvstat(rms)=",uvstat(rms),"Jy" ! uvstat(rms)= 0.0367453 Jy 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 8 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 2. ! A total of 8 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 3. ! A total of 8 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 4. ! A total of 8 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 5. ! A total of 8 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 6. ! A total of 8 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 7. ! A total of 8 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 8. ! A total of 8 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! ! Fit before self-cal, rms=1.000853Jy sigma=24.905379 ! Fit after self-cal, rms=0.982195Jy sigma=24.444792 ! 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. peakwin win_mult ! Inverting map and beam ! Estimated beam: bmin=1.306 mas, bmaj=3.783 mas, bpa=-10.45 degrees ! Estimated noise=0.429864 mJy/beam. ! Added new window around map position (0, 0). 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 false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=100 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0153231 Jy ! Component: 100 - total flux cleaned = 0.0201002 Jy ! Total flux subtracted in 100 components = 0.0201002 Jy ! Clean residual min=-0.002343 max=0.002609 Jy/beam ! Clean residual mean=-0.000004 rms=0.000733 Jy/beam ! Combined flux in latest and established models = 0.0201002 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 45 model components to the UV plane model. ! The established model now contains 45 components and 0.0201002 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.031520Jy sigma=0.722330 ! Fit after self-cal, rms=0.031510Jy sigma=0.722090 ! Inverting map print "============== Finished uniform weighting CLEAN ==============" ! ============== Finished uniform weighting CLEAN ============== ! uvw 0,-2 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -2. ! 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 ! Estimated beam: bmin=1.589 mas, bmaj=3.827 mas, bpa=-9.962 degrees ! Estimated noise=0.261409 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0039832 Jy ! Component: 100 - total flux cleaned = 0.006668 Jy ! Component: 150 - total flux cleaned = 0.00861037 Jy ! Component: 200 - total flux cleaned = 0.0100265 Jy ! Total flux subtracted in 200 components = 0.0100265 Jy ! Clean residual min=-0.002136 max=0.002336 Jy/beam ! Clean residual mean=-0.000007 rms=0.000704 Jy/beam ! Combined flux in latest and established models = 0.0301268 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 33 model components to the UV plane model. ! The established model now contains 74 components and 0.0301268 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.031079Jy sigma=0.709642 ! Fit after self-cal, rms=0.031078Jy sigma=0.709591 ! Inverting map print "============== Finished natural weighting CLEAN ==============" ! ============== Finished natural weighting CLEAN ============== ! gscale ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Amplitude normalization factor in sub-array 1: 1.01307 ! Telescope amplitude corrections in sub-array 1: ! HN 1.18 KP 0.82 LA 0.81 NL 1.30 ! OV 1.13 PT 0.68 ! ! Amplitude normalization factor in sub-array 2: 0.9129 ! Telescope amplitude corrections in sub-array 2: ! BR 0.89 FD 1.61 HN 0.96 KP 0.83 ! LA 0.97 NL 1.33 OV 1.07 ! ! ! Correcting IF 2. ! Amplitude normalization factor in sub-array 1: 0.937631 ! Telescope amplitude corrections in sub-array 1: ! HN 1.45 KP 0.80 LA 0.75 NL 1.32 ! OV 1.45 PT 0.62 ! ! Amplitude normalization factor in sub-array 2: 0.859544 ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 1.65 HN 1.27 KP 0.81 ! LA 1.02 NL 1.31 OV 1.08 ! ! ! Correcting IF 3. ! Amplitude normalization factor in sub-array 1: 0.983051 ! Telescope amplitude corrections in sub-array 1: ! HN 1.40 KP 0.80 LA 0.76 NL 1.22 ! OV 1.21 PT 0.72 ! ! Amplitude normalization factor in sub-array 2: 0.90393 ! Telescope amplitude corrections in sub-array 2: ! BR 1.18 FD 1.43 HN 0.95 KP 0.78 ! LA 1.03 NL 1.21 OV 1.18 ! ! ! Correcting IF 4. ! Amplitude normalization factor in sub-array 1: 1.03884 ! Telescope amplitude corrections in sub-array 1: ! HN 1.14 KP 0.73 LA 0.87 NL 1.34 ! OV 1.01 PT 0.69 ! ! Amplitude normalization factor in sub-array 2: 0.942711 ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 FD 1.14 HN 0.97 KP 0.83 ! LA 1.34 NL 1.11 OV 0.99 ! ! ! Correcting IF 5. ! Amplitude normalization factor in sub-array 1: 1.07217 ! Telescope amplitude corrections in sub-array 1: ! HN 1.18 KP 0.73 LA 0.87 NL 1.11 ! OV 1.04 PT 0.67 ! ! Amplitude normalization factor in sub-array 2: 0.970694 ! Telescope amplitude corrections in sub-array 2: ! BR 0.90 FD 1.28 HN 0.91 KP 0.79 ! LA 1.13 NL 1.20 OV 1.01 ! ! ! Correcting IF 6. ! Amplitude normalization factor in sub-array 1: 1.00351 ! Telescope amplitude corrections in sub-array 1: ! HN 1.22 KP 0.74 LA 0.91 NL 1.19 ! OV 1.11 PT 0.81 ! ! Amplitude normalization factor in sub-array 2: 0.932215 ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 1.42 HN 0.75 KP 0.85 ! LA 1.34 NL 1.22 OV 0.93 ! ! ! Correcting IF 7. ! Amplitude normalization factor in sub-array 1: 1.05367 ! Telescope amplitude corrections in sub-array 1: ! HN 1.16 KP 0.76 LA 0.78 NL 1.20 ! OV 1.05 PT 0.74 ! ! Amplitude normalization factor in sub-array 2: 0.926664 ! Telescope amplitude corrections in sub-array 2: ! BR 0.83 FD 1.23 HN 0.90 KP 0.95 ! LA 1.37 NL 1.28 OV 0.99 ! ! ! Correcting IF 8. ! Amplitude normalization factor in sub-array 1: 1.10611 ! Telescope amplitude corrections in sub-array 1: ! HN 1.01 KP 0.72 LA 0.84 NL 1.20 ! OV 0.90 PT 0.75 ! ! Amplitude normalization factor in sub-array 2: 0.909153 ! Telescope amplitude corrections in sub-array 2: ! BR 0.86 FD 1.39 HN 0.98 KP 0.84 ! LA 1.43 NL 1.26 OV 0.94 ! ! ! Fit before self-cal, rms=0.031078Jy sigma=0.709591 ! Fit after self-cal, rms=0.031396Jy sigma=0.696037 selfcal false, false, phase_soltime ! Performing phase self-cal over 10 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.031396Jy sigma=0.696037 ! Fit after self-cal, rms=0.031403Jy sigma=0.695957 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=1.618 mas, bmaj=3.709 mas, bpa=-10.09 degrees ! Estimated noise=0.229147 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -0.001459 Jy ! Component: 100 - total flux cleaned = -0.00168959 Jy ! Component: 150 - total flux cleaned = -0.00172097 Jy ! Component: 200 - total flux cleaned = -0.00173471 Jy ! Total flux subtracted in 200 components = -0.00173471 Jy ! Clean residual min=-0.001284 max=0.001321 Jy/beam ! Clean residual mean=-0.000004 rms=0.000368 Jy/beam ! Combined flux in latest and established models = 0.028392 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 28 model components to the UV plane model. ! The established model now contains 98 components and 0.028392 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.031378Jy sigma=0.694216 ! Fit after self-cal, rms=0.031378Jy sigma=0.694213 ! Inverting map print "============== Finished amplitude gscale SELF-CAL ==============" ! ============== Finished amplitude gscale SELF-CAL ============== ! phase_soltime=phase_soltime2 selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.031378Jy sigma=0.694213 ! Fit after self-cal, rms=0.031369Jy sigma=0.692527 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 9.34866e-05 Jy ! Component: 100 - total flux cleaned = 9.30824e-05 Jy ! Component: 150 - total flux cleaned = 8.47522e-05 Jy ! Component: 200 - total flux cleaned = 7.11963e-05 Jy ! Total flux subtracted in 200 components = 7.11963e-05 Jy ! Clean residual min=-0.001217 max=0.001291 Jy/beam ! Clean residual mean=-0.000004 rms=0.000360 Jy/beam ! Combined flux in latest and established models = 0.0284632 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 13 model components to the UV plane model. ! The established model now contains 104 components and 0.0284632 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.031365Jy sigma=0.692411 ! Fit after self-cal, rms=0.031378Jy sigma=0.692312 ! Inverting map print "=== Finished natural weighting clean with shorter phase_soltime " ! === Finished natural weighting clean with shorter phase_soltime ! dynam = dynam - 0.25 restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.618 x 3.709 at -10.09 degrees (North through East) ! Clean map min=-0.0011977 max=0.016496 Jy/beam if(peak(flux) > thresh) selfcal true, true, amp_soltime1 selfcal false, false, phase_soltime 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 false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) print "============== Finished amplitude self-cal ==============" end if print "============== Clearing model and starting over ==========" ! ============== Clearing model and starting over ========== clrmod true,true,true ! clrmod: Cleared the established, tentative and continuum 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 ! Estimated beam: bmin=1.334 mas, bmaj=3.63 mas, bpa=-10.4 degrees ! Estimated noise=0.393756 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.014063 Jy ! Component: 100 - total flux cleaned = 0.0183719 Jy ! Component: 150 - total flux cleaned = 0.021057 Jy ! Component: 200 - total flux cleaned = 0.0228393 Jy ! Total flux subtracted in 200 components = 0.0228393 Jy ! Clean residual min=-0.001444 max=0.001666 Jy/beam ! Clean residual mean=-0.000002 rms=0.000423 Jy/beam ! Combined flux in latest and established models = 0.0228393 Jy uvw 0,-2 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -2. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Adding 80 model components to the UV plane model. ! The established model now contains 80 components and 0.0228393 Jy ! Inverting map and beam ! Estimated beam: bmin=1.618 mas, bmaj=3.709 mas, bpa=-10.09 degrees ! Estimated noise=0.229147 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=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.00199626 Jy ! Component: 100 - total flux cleaned = 0.00316023 Jy ! Component: 150 - total flux cleaned = 0.0039026 Jy ! Component: 200 - total flux cleaned = 0.00438974 Jy ! Total flux subtracted in 200 components = 0.00438974 Jy ! Clean residual min=-0.001332 max=0.001371 Jy/beam ! Clean residual mean=-0.000005 rms=0.000388 Jy/beam ! Combined flux in latest and established models = 0.027229 Jy ! Adding 32 model components to the UV plane model. ! The established model now contains 108 components and 0.027229 Jy ! Inverting map clean ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000233506 Jy ! Component: 100 - total flux cleaned = 0.000312284 Jy ! Component: 150 - total flux cleaned = 0.000363853 Jy ! Component: 200 - total flux cleaned = 0.000402619 Jy ! Total flux subtracted in 200 components = 0.000402619 Jy ! Clean residual min=-0.001318 max=0.001324 Jy/beam ! Clean residual mean=-0.000005 rms=0.000380 Jy/beam ! Combined flux in latest and established models = 0.0276317 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 20 model components to the UV plane model. ! The established model now contains 116 components and 0.0276317 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.031381Jy sigma=0.692815 ! Fit after self-cal, rms=0.031390Jy sigma=0.692824 wmodel J0148+1028_X_map.mod ! Writing 116 model components to file: J0148+1028_X_map.mod wobs J0148+1028_X_uvs.fits ! Writing UV FITS file: J0148+1028_X_uvs.fits wwins J0148+1028_X_map.win ! wwins: Wrote 1 windows to J0148+1028_X_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000101759 Jy ! Component: 100 - total flux cleaned = 0.00023129 Jy ! Component: 150 - total flux cleaned = 0.00038729 Jy ! Component: 200 - total flux cleaned = 0.000510608 Jy ! Component: 250 - total flux cleaned = 0.000691391 Jy ! Component: 300 - total flux cleaned = 0.000892926 Jy ! Component: 350 - total flux cleaned = 0.000965881 Jy ! Component: 400 - total flux cleaned = 0.00105051 Jy ! Component: 450 - total flux cleaned = 0.00113161 Jy ! Component: 500 - total flux cleaned = 0.00117113 Jy ! Component: 550 - total flux cleaned = 0.0012455 Jy ! Component: 600 - total flux cleaned = 0.0012455 Jy ! Component: 650 - total flux cleaned = 0.00128028 Jy ! Component: 700 - total flux cleaned = 0.00133552 Jy ! Component: 750 - total flux cleaned = 0.00132492 Jy ! Component: 800 - total flux cleaned = 0.00136641 Jy ! Component: 850 - total flux cleaned = 0.00137648 Jy ! Component: 900 - total flux cleaned = 0.00139591 Jy ! Component: 950 - total flux cleaned = 0.00137709 Jy ! Component: 1000 - total flux cleaned = 0.00143162 Jy ! Component: 1050 - total flux cleaned = 0.00140514 Jy ! Component: 1100 - total flux cleaned = 0.0014309 Jy ! Component: 1150 - total flux cleaned = 0.00143936 Jy ! Component: 1200 - total flux cleaned = 0.00144757 Jy ! Component: 1250 - total flux cleaned = 0.00145541 Jy ! Component: 1300 - total flux cleaned = 0.00146296 Jy ! Component: 1350 - total flux cleaned = 0.00148541 Jy ! Component: 1400 - total flux cleaned = 0.00151429 Jy ! Component: 1450 - total flux cleaned = 0.00153555 Jy ! Component: 1500 - total flux cleaned = 0.00154241 Jy ! Component: 1550 - total flux cleaned = 0.00155618 Jy ! Component: 1600 - total flux cleaned = 0.00157619 Jy ! Component: 1650 - total flux cleaned = 0.00158269 Jy ! Component: 1700 - total flux cleaned = 0.00160817 Jy ! Component: 1750 - total flux cleaned = 0.00160809 Jy ! Component: 1800 - total flux cleaned = 0.00163886 Jy ! Component: 1850 - total flux cleaned = 0.00165682 Jy ! Component: 1900 - total flux cleaned = 0.00164491 Jy ! Component: 1950 - total flux cleaned = 0.00162731 Jy ! Component: 2000 - total flux cleaned = 0.00159844 Jy ! Component: 2050 - total flux cleaned = 0.00159282 Jy ! Component: 2100 - total flux cleaned = 0.00157034 Jy ! Component: 2150 - total flux cleaned = 0.00152603 Jy ! Component: 2200 - total flux cleaned = 0.00149873 Jy ! Component: 2250 - total flux cleaned = 0.00148797 Jy ! Component: 2300 - total flux cleaned = 0.00145591 Jy ! Component: 2350 - total flux cleaned = 0.00141908 Jy ! Component: 2400 - total flux cleaned = 0.00139824 Jy ! Component: 2450 - total flux cleaned = 0.00136725 Jy ! Component: 2500 - total flux cleaned = 0.00133145 Jy ! Component: 2550 - total flux cleaned = 0.00130103 Jy ! Component: 2600 - total flux cleaned = 0.00125597 Jy ! Component: 2650 - total flux cleaned = 0.00125102 Jy ! Component: 2700 - total flux cleaned = 0.0012265 Jy ! Component: 2750 - total flux cleaned = 0.00121679 Jy ! Component: 2800 - total flux cleaned = 0.00119757 Jy ! Component: 2850 - total flux cleaned = 0.00118331 Jy ! Component: 2900 - total flux cleaned = 0.00116446 Jy ! Component: 2950 - total flux cleaned = 0.00115506 Jy ! Component: 3000 - total flux cleaned = 0.00114111 Jy ! Component: 3050 - total flux cleaned = 0.00114106 Jy ! Component: 3100 - total flux cleaned = 0.00113645 Jy ! Component: 3150 - total flux cleaned = 0.00113188 Jy ! Component: 3200 - total flux cleaned = 0.00111835 Jy ! Component: 3250 - total flux cleaned = 0.00112285 Jy ! Component: 3300 - total flux cleaned = 0.00113179 Jy ! Component: 3350 - total flux cleaned = 0.00114066 Jy ! Component: 3400 - total flux cleaned = 0.00113179 Jy ! Component: 3450 - total flux cleaned = 0.00113622 Jy ! Component: 3500 - total flux cleaned = 0.00113619 Jy ! Component: 3550 - total flux cleaned = 0.00114489 Jy ! Component: 3600 - total flux cleaned = 0.00114056 Jy ! Component: 3650 - total flux cleaned = 0.00116226 Jy ! Component: 3700 - total flux cleaned = 0.0011709 Jy ! Component: 3750 - total flux cleaned = 0.00118377 Jy ! Component: 3800 - total flux cleaned = 0.00117949 Jy ! Component: 3850 - total flux cleaned = 0.00119232 Jy ! Component: 3900 - total flux cleaned = 0.00120082 Jy ! Component: 3950 - total flux cleaned = 0.00121782 Jy ! Component: 4000 - total flux cleaned = 0.00123901 Jy ! Component: 4050 - total flux cleaned = 0.00126012 Jy ! Total flux subtracted in 4096 components = 0.00126433 Jy ! Clean residual min=-0.000262 max=0.000257 Jy/beam ! Clean residual mean=-0.000000 rms=0.000077 Jy/beam ! Combined flux in latest and established models = 0.028896 Jy keep ! Adding 334 model components to the UV plane model. ! The established model now contains 450 components and 0.028896 Jy ![Exited script file: /opt64/bin/pima_mupet_02.dfm] wmap /vlbi/vcs9/uvm//J0148+1028_X_a_map.fits ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.618 x 3.709 at -10.09 degrees (North through East) ! Clean map min=-0.000505 max=0.016481 Jy/beam ! Writing clean map to FITS file: /vlbi/vcs9/uvm//J0148+1028_X_a_map.fits wmodel /vlbi/vcs9/uvm//J0148+1028_X_a_map.mod ! Writing 450 model components to file: /vlbi/vcs9/uvm//J0148+1028_X_a_map.mod wobs /vlbi/vcs9/uvm//J0148+1028_X_a_uvs.fits ! Writing UV FITS file: /vlbi/vcs9/uvm//J0148+1028_X_a_uvs.fits wwins /vlbi/vcs9/uvm//J0148+1028_X_a_map.win ! wwins: Wrote 2 windows to /vlbi/vcs9/uvm//J0148+1028_X_a_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.0164811 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 7.45094e-05 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -1.35627 1.35627 2.71253 5.42507 10.8501 21.7003 43.4005 86.8011 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0002 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.016 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 221.195 quit ! Quitting program ! Log file /vlbi/vcs9/uvm//J0148+1028_X_a_dfm.log closed on Tue Dec 26 21:08:12 2017