! Started logfile: /vlbi/vcs9/uvm//J0622-0232_C_a_dfm.log on Tue Dec 26 21:46:23 2017 float field_size field_size = 1024 float field_cell field_cell = 0.3000 float taper_size taper_size = 40.0 float freq freq = 4.12800 obs /vlbi/vcs9/uvm//J0622-0232_C_a_uvm.fits ! Reading UV FITS file: /vlbi/vcs9/uvm//J0622-0232_C_a_uvm.fits ! AN table 1: 38 integrations on 36 of 36 possible baselines. ! AN table 2: 18 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.974288 visibilities/baseline/integration-bin. ! Found source: J0622-0232 ! ! 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 4.128e+09 3.2e+07 1 3.2e+07 ! 02 2 4.16e+09 3.2e+07 1 3.2e+07 ! 03 3 4.192e+09 3.2e+07 1 3.2e+07 ! 04 4 4.224e+09 3.2e+07 1 3.2e+07 ! 05 5 4.416e+09 3.2e+07 1 3.2e+07 ! 06 6 4.512e+09 3.2e+07 1 3.2e+07 ! 07 7 4.544e+09 3.2e+07 1 3.2e+07 ! 08 8 4.576e+09 3.2e+07 1 3.2e+07 ! ! Polarization(s): RR ! ! Read 85 lines of history. ! ! Reading 16976 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 = 0.3 print "taper_size =", taper_size ! taper_size = 40 ![@/opt64/bin/pima_mupet_02.dfm J0622-0232_C] 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 0.300x0.300 milli-arcsec cellsize. phase_soltime=phase_soltime1 print "uvstat(rms)=",uvstat(rms),"Jy" ! uvstat(rms)= 0.0335462 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 3 telescope corrections were flagged in sub-array 1. ! A total of 5 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 2. ! A total of 3 telescope corrections were flagged in sub-array 1. ! A total of 5 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 3. ! A total of 3 telescope corrections were flagged in sub-array 1. ! A total of 5 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 4. ! A total of 3 telescope corrections were flagged in sub-array 1. ! A total of 5 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 5. ! A total of 3 telescope corrections were flagged in sub-array 1. ! A total of 5 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 6. ! A total of 3 telescope corrections were flagged in sub-array 1. ! A total of 5 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 7. ! A total of 3 telescope corrections were flagged in sub-array 1. ! A total of 5 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 8. ! A total of 3 telescope corrections were flagged in sub-array 1. ! A total of 5 telescope corrections were flagged in sub-array 2. ! ! Fit before self-cal, rms=1.000327Jy sigma=28.813909 ! Fit after self-cal, rms=0.986555Jy sigma=28.436724 ! 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=1.481 mas, bmaj=3.35 mas, bpa=-2.879 degrees ! Estimated noise=0.312136 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 = 0.011534 Jy ! Component: 100 - total flux cleaned = 0.0129957 Jy ! Total flux subtracted in 100 components = 0.0129957 Jy ! Clean residual min=-0.000973 max=0.000952 Jy/beam ! Clean residual mean=0.000001 rms=0.000232 Jy/beam ! Combined flux in latest and established models = 0.0129957 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.0129957 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=0.030538Jy sigma=0.728630 ! Fit after self-cal, rms=0.030507Jy sigma=0.727618 ! 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=1.944 mas, bmaj=4.136 mas, bpa=1.432 degrees ! Estimated noise=0.188374 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 = 0.0001906 Jy ! Component: 100 - total flux cleaned = 0.000143399 Jy ! Component: 150 - total flux cleaned = 0.000103957 Jy ! Component: 200 - total flux cleaned = 6.50919e-05 Jy ! Total flux subtracted in 200 components = 6.50919e-05 Jy ! Clean residual min=-0.000668 max=0.000637 Jy/beam ! Clean residual mean=0.000003 rms=0.000160 Jy/beam ! Combined flux in latest and established models = 0.0130608 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 12 model components to the UV plane model. ! The established model now contains 15 components and 0.0130608 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=0.030486Jy sigma=0.727347 ! Fit after self-cal, rms=0.030485Jy sigma=0.727336 ! 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: 1.06423 ! Telescope amplitude corrections in sub-array 1: ! BR 1.28 FD 0.73 HN 0.92 LA 0.92 ! MK 0.88 NL 1.05 OV 0.86 PT 1.03 ! SC 0.79 ! ! Amplitude normalization factor in sub-array 2: 0.883784 ! Telescope amplitude corrections in sub-array 2: ! BR 1.54 FD 0.77 HN 1.17 KP 0.96 ! LA 0.94 MK 0.63 NL 1.39 OV 1.13 ! PT 1.60 SC 1.20 ! ! ! Correcting IF 2. ! Amplitude normalization factor in sub-array 1: 0.938614 ! Telescope amplitude corrections in sub-array 1: ! BR 1.32 FD 0.81 HN 1.18 LA 0.84 ! MK 1.03 NL 1.31 OV 1.02 PT 1.28 ! SC 0.80 ! ! Amplitude normalization factor in sub-array 2: 1.01902 ! Telescope amplitude corrections in sub-array 2: ! BR 1.60 FD 0.75 HN 1.17 KP 0.86 ! LA 0.72 MK 0.78 NL 1.04 OV 1.18 ! PT 0.83 SC 0.88 ! ! ! Correcting IF 3. ! Amplitude normalization factor in sub-array 1: 0.925363 ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.90 HN 1.37 LA 0.87 ! MK 1.17 NL 0.96 OV 1.22 PT 1.08 ! SC 1.16 ! ! Amplitude normalization factor in sub-array 2: 1.07188 ! Telescope amplitude corrections in sub-array 2: ! BR 0.93 FD 0.98 HN 0.98 KP 1.16 ! LA 0.86 MK 0.88 NL 0.73 OV 0.91 ! PT 0.92 SC 0.98 ! ! ! Correcting IF 4. ! Amplitude normalization factor in sub-array 1: 1.01299 ! Telescope amplitude corrections in sub-array 1: ! BR 1.04 FD 0.84 HN 0.89 LA 1.06 ! MK 0.88 NL 1.10 OV 1.00 PT 1.12 ! SC 0.95 ! ! Amplitude normalization factor in sub-array 2: 0.943053 ! Telescope amplitude corrections in sub-array 2: ! BR 1.17 FD 0.70 HN 1.13 KP 0.96 ! LA 1.30 MK 1.04 NL 1.13 OV 0.96 ! PT 1.18 SC 1.03 ! ! ! Correcting IF 5. ! Amplitude normalization factor in sub-array 1: 0.868805 ! Telescope amplitude corrections in sub-array 1: ! BR 0.90 FD 1.04 HN 1.23 LA 1.37 ! MK 0.80 NL 1.13 OV 1.33 PT 1.34 ! SC 1.23 ! ! Amplitude normalization factor in sub-array 2: 0.810649 ! Telescope amplitude corrections in sub-array 2: ! BR 1.09 FD 0.80 HN 1.26 KP 1.67 ! LA 1.49 MK 1.12 NL 1.09 OV 1.12 ! PT 1.42 SC 1.27 ! ! ! Correcting IF 6. ! Amplitude normalization factor in sub-array 1: 1.02433 ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 1.00 HN 1.03 LA 0.91 ! MK 0.89 NL 0.83 OV 1.09 PT 1.13 ! SC 0.94 ! ! Amplitude normalization factor in sub-array 2: 1.0307 ! Telescope amplitude corrections in sub-array 2: ! BR 0.94 FD 0.93 HN 0.79 KP 1.47 ! LA 0.90 MK 0.99 NL 0.83 OV 0.98 ! PT 0.85 SC 1.03 ! ! ! Correcting IF 7. ! Amplitude normalization factor in sub-array 1: 0.951936 ! Telescope amplitude corrections in sub-array 1: ! BR 1.14 FD 1.13 HN 0.95 LA 1.04 ! MK 1.14 NL 1.08 OV 0.95 PT 1.06 ! SC 0.97 ! ! Amplitude normalization factor in sub-array 2: 1.07582 ! Telescope amplitude corrections in sub-array 2: ! BR 0.81 FD 1.20 HN 0.87 KP 0.88 ! LA 0.83 MK 0.97 NL 0.93 OV 1.05 ! PT 0.88 SC 0.87 ! ! ! Correcting IF 8. ! Amplitude normalization factor in sub-array 1: 1.01546 ! Telescope amplitude corrections in sub-array 1: ! BR 1.08 FD 1.06 HN 0.92 LA 0.92 ! MK 0.93 NL 1.00 OV 0.94 PT 1.00 ! SC 1.01 ! ! Amplitude normalization factor in sub-array 2: 0.964491 ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 0.91 HN 1.14 KP 1.08 ! LA 1.18 MK 0.90 NL 1.08 OV 1.02 ! PT 1.12 SC 0.94 ! ! ! Fit before self-cal, rms=0.030485Jy sigma=0.727336 ! Fit after self-cal, rms=0.030944Jy sigma=0.723907 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=0.030944Jy sigma=0.723907 ! Fit after self-cal, rms=0.030951Jy sigma=0.723855 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=1.918 mas, bmaj=4.108 mas, bpa=0.32 degrees ! Estimated noise=0.176218 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 = -0.00049754 Jy ! Component: 100 - total flux cleaned = -0.000515713 Jy ! Component: 150 - total flux cleaned = -0.000519548 Jy ! Component: 200 - total flux cleaned = -0.00051117 Jy ! Total flux subtracted in 200 components = -0.00051117 Jy ! Clean residual min=-0.000553 max=0.000480 Jy/beam ! Clean residual mean=-0.000001 rms=0.000122 Jy/beam ! Combined flux in latest and established models = 0.0125496 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 17 model components to the UV plane model. ! The established model now contains 28 components and 0.0125496 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=0.030958Jy sigma=0.723613 ! Fit after self-cal, rms=0.030958Jy sigma=0.723609 ! 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=0.030958Jy sigma=0.723609 ! Fit after self-cal, rms=0.030918Jy sigma=0.721676 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 = 9.31076e-05 Jy ! Component: 100 - total flux cleaned = 9.57445e-05 Jy ! Component: 150 - total flux cleaned = 9.40701e-05 Jy ! Component: 200 - total flux cleaned = 9.27777e-05 Jy ! Total flux subtracted in 200 components = 9.27777e-05 Jy ! Clean residual min=-0.000562 max=0.000482 Jy/beam ! Clean residual mean=-0.000002 rms=0.000123 Jy/beam ! Combined flux in latest and established models = 0.0126424 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 39 components and 0.0126424 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=0.030916Jy sigma=0.721659 ! Fit after self-cal, rms=0.030915Jy sigma=0.721237 ! 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: 1.918 x 4.108 at 0.32 degrees (North through East) ! Clean map min=-0.00053979 max=0.012875 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=1.464 mas, bmaj=3.333 mas, bpa=-3.686 degrees ! Estimated noise=0.293971 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0110797 Jy ! Component: 100 - total flux cleaned = 0.0126736 Jy ! Component: 150 - total flux cleaned = 0.0128565 Jy ! Component: 200 - total flux cleaned = 0.0129366 Jy ! Total flux subtracted in 200 components = 0.0129366 Jy ! Clean residual min=-0.000851 max=0.000844 Jy/beam ! Clean residual mean=-0.000000 rms=0.000190 Jy/beam ! Combined flux in latest and established models = 0.0129366 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 11 model components to the UV plane model. ! The established model now contains 11 components and 0.0129366 Jy ! Inverting map and beam ! Estimated beam: bmin=1.918 mas, bmaj=4.108 mas, bpa=0.32 degrees ! Estimated noise=0.176218 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 = -0.000101189 Jy ! Component: 100 - total flux cleaned = -0.000137004 Jy ! Component: 150 - total flux cleaned = -0.000170117 Jy ! Component: 200 - total flux cleaned = -0.000196439 Jy ! Total flux subtracted in 200 components = -0.000196439 Jy ! Clean residual min=-0.000571 max=0.000496 Jy/beam ! Clean residual mean=-0.000002 rms=0.000124 Jy/beam ! Combined flux in latest and established models = 0.0127401 Jy ! Adding 18 model components to the UV plane model. ! The established model now contains 25 components and 0.0127401 Jy ! Inverting map clean ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -1.69219e-05 Jy ! Component: 100 - total flux cleaned = -3.44282e-05 Jy ! Component: 150 - total flux cleaned = -4.87221e-05 Jy ! Component: 200 - total flux cleaned = -5.82366e-05 Jy ! Total flux subtracted in 200 components = -5.82366e-05 Jy ! Clean residual min=-0.000562 max=0.000487 Jy/beam ! Clean residual mean=-0.000002 rms=0.000123 Jy/beam ! Combined flux in latest and established models = 0.0126819 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 13 model components to the UV plane model. ! The established model now contains 30 components and 0.0126819 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=0.030915Jy sigma=0.721236 ! Fit after self-cal, rms=0.030918Jy sigma=0.721121 wmodel J0622-0232_C_map.mod ! Writing 30 model components to file: J0622-0232_C_map.mod wobs J0622-0232_C_uvs.fits ! Writing UV FITS file: J0622-0232_C_uvs.fits wwins J0622-0232_C_map.win ! wwins: Wrote 1 windows to J0622-0232_C_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 = -0.000138971 Jy ! Component: 100 - total flux cleaned = -0.000181487 Jy ! Component: 150 - total flux cleaned = -0.000221477 Jy ! Component: 200 - total flux cleaned = -0.000229222 Jy ! Component: 250 - total flux cleaned = -0.000214458 Jy ! Component: 300 - total flux cleaned = -0.000214425 Jy ! Component: 350 - total flux cleaned = -0.000248774 Jy ! Component: 400 - total flux cleaned = -0.000282121 Jy ! Component: 450 - total flux cleaned = -0.000288672 Jy ! Component: 500 - total flux cleaned = -0.000301449 Jy ! Component: 550 - total flux cleaned = -0.00030769 Jy ! Component: 600 - total flux cleaned = -0.000301515 Jy ! Component: 650 - total flux cleaned = -0.000295506 Jy ! Component: 700 - total flux cleaned = -0.0003015 Jy ! Component: 750 - total flux cleaned = -0.000313164 Jy ! Component: 800 - total flux cleaned = -0.00031892 Jy ! Component: 850 - total flux cleaned = -0.000364001 Jy ! Component: 900 - total flux cleaned = -0.000358292 Jy ! Component: 950 - total flux cleaned = -0.00036931 Jy ! Component: 1000 - total flux cleaned = -0.000374881 Jy ! Component: 1050 - total flux cleaned = -0.000390993 Jy ! Component: 1100 - total flux cleaned = -0.000412075 Jy ! Component: 1150 - total flux cleaned = -0.000401659 Jy ! Component: 1200 - total flux cleaned = -0.000437781 Jy ! Component: 1250 - total flux cleaned = -0.000422447 Jy ! Component: 1300 - total flux cleaned = -0.00042749 Jy ! Component: 1350 - total flux cleaned = -0.000432527 Jy ! Component: 1400 - total flux cleaned = -0.000427603 Jy ! Component: 1450 - total flux cleaned = -0.000427655 Jy ! Component: 1500 - total flux cleaned = -0.000432453 Jy ! Component: 1550 - total flux cleaned = -0.000432485 Jy ! Component: 1600 - total flux cleaned = -0.000427709 Jy ! Component: 1650 - total flux cleaned = -0.000432357 Jy ! Component: 1700 - total flux cleaned = -0.000418379 Jy ! Component: 1750 - total flux cleaned = -0.000436801 Jy ! Component: 1800 - total flux cleaned = -0.000441348 Jy ! Component: 1850 - total flux cleaned = -0.000436819 Jy ! Component: 1900 - total flux cleaned = -0.000436843 Jy ! Component: 1950 - total flux cleaned = -0.000450201 Jy ! Component: 2000 - total flux cleaned = -0.000436944 Jy ! Component: 2050 - total flux cleaned = -0.000423844 Jy ! Component: 2100 - total flux cleaned = -0.000419545 Jy ! Component: 2150 - total flux cleaned = -0.000428083 Jy ! Component: 2200 - total flux cleaned = -0.000419548 Jy ! Component: 2250 - total flux cleaned = -0.000415313 Jy ! Component: 2300 - total flux cleaned = -0.000406929 Jy ! Component: 2350 - total flux cleaned = -0.000402793 Jy ! Component: 2400 - total flux cleaned = -0.00041933 Jy ! Component: 2450 - total flux cleaned = -0.000415248 Jy ! Component: 2500 - total flux cleaned = -0.000435648 Jy ! Component: 2550 - total flux cleaned = -0.000427571 Jy ! Component: 2600 - total flux cleaned = -0.00045569 Jy ! Component: 2650 - total flux cleaned = -0.000455669 Jy ! Component: 2700 - total flux cleaned = -0.000467499 Jy ! Component: 2750 - total flux cleaned = -0.000467482 Jy ! Component: 2800 - total flux cleaned = -0.000467515 Jy ! Component: 2850 - total flux cleaned = -0.000490778 Jy ! Component: 2900 - total flux cleaned = -0.000479256 Jy ! Component: 2950 - total flux cleaned = -0.000494584 Jy ! Component: 3000 - total flux cleaned = -0.000517366 Jy ! Component: 3050 - total flux cleaned = -0.000524891 Jy ! Component: 3100 - total flux cleaned = -0.000539862 Jy ! Component: 3150 - total flux cleaned = -0.00053988 Jy ! Component: 3200 - total flux cleaned = -0.000550977 Jy ! Component: 3250 - total flux cleaned = -0.000562027 Jy ! Component: 3300 - total flux cleaned = -0.000572986 Jy ! Component: 3350 - total flux cleaned = -0.00056935 Jy ! Component: 3400 - total flux cleaned = -0.000572966 Jy ! Component: 3450 - total flux cleaned = -0.000580124 Jy ! Component: 3500 - total flux cleaned = -0.000594413 Jy ! Component: 3550 - total flux cleaned = -0.000594373 Jy ! Component: 3600 - total flux cleaned = -0.000580308 Jy ! Component: 3650 - total flux cleaned = -0.000601354 Jy ! Component: 3700 - total flux cleaned = -0.000590885 Jy ! Component: 3750 - total flux cleaned = -0.000597773 Jy ! Component: 3800 - total flux cleaned = -0.000594346 Jy ! Component: 3850 - total flux cleaned = -0.000594365 Jy ! Component: 3900 - total flux cleaned = -0.00058414 Jy ! Component: 3950 - total flux cleaned = -0.000597715 Jy ! Component: 4000 - total flux cleaned = -0.000607836 Jy ! Component: 4050 - total flux cleaned = -0.000594474 Jy ! Total flux subtracted in 4096 components = -0.000621116 Jy ! Clean residual min=-0.000196 max=0.000198 Jy/beam ! Clean residual mean=-0.000001 rms=0.000061 Jy/beam ! Combined flux in latest and established models = 0.0120608 Jy keep ! Adding 255 model components to the UV plane model. ! The established model now contains 285 components and 0.0120608 Jy ![Exited script file: /opt64/bin/pima_mupet_02.dfm] wmap /vlbi/vcs9/uvm//J0622-0232_C_a_map.fits ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.918 x 4.108 at 0.32 degrees (North through East) ! Clean map min=-0.00038434 max=0.012855 Jy/beam ! Writing clean map to FITS file: /vlbi/vcs9/uvm//J0622-0232_C_a_map.fits wmodel /vlbi/vcs9/uvm//J0622-0232_C_a_map.mod ! Writing 285 model components to file: /vlbi/vcs9/uvm//J0622-0232_C_a_map.mod wobs /vlbi/vcs9/uvm//J0622-0232_C_a_uvs.fits ! Writing UV FITS file: /vlbi/vcs9/uvm//J0622-0232_C_a_uvs.fits wwins /vlbi/vcs9/uvm//J0622-0232_C_a_map.win ! wwins: Wrote 2 windows to /vlbi/vcs9/uvm//J0622-0232_C_a_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.0128549 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 5.95404e-05 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -1.38952 1.38952 2.77904 5.55809 11.1162 22.2324 44.4647 88.9294 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0001 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.012 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 215.901 quit ! Quitting program ! Log file /vlbi/vcs9/uvm//J0622-0232_C_a_dfm.log closed on Tue Dec 26 21:46:26 2017