! Started logfile: /vlbi/vcs9/uvm//J0411+1714_C_a_dfm.log on Tue Dec 26 21:32:14 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//J0411+1714_C_a_uvm.fits ! Reading UV FITS file: /vlbi/vcs9/uvm//J0411+1714_C_a_uvm.fits ! AN table 1: 47 integrations on 15 of 15 possible baselines. ! AN table 2: 50 integrations on 28 of 28 possible baselines. ! Apparent sampling: 0.971021 visibilities/baseline/integration-bin. ! Found source: J0411+1714 ! ! 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 76 lines of history. ! ! Reading 16352 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 J0411+1714_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)= 0.0573198 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 6 telescope corrections were flagged in sub-array 1. ! A total of 11 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 2. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 11 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 3. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 11 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 4. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 11 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 5. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 11 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 6. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 11 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 7. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 11 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 8. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 11 telescope corrections were flagged in sub-array 2. ! ! Fit before self-cal, rms=1.002189Jy sigma=30.823805 ! Fit after self-cal, rms=0.948528Jy sigma=29.149994 ! 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=1.832 mas, bmaj=5.494 mas, bpa=-9.335 degrees ! Estimated noise=0.351824 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 = 0.0437668 Jy ! Component: 100 - total flux cleaned = 0.0513261 Jy ! Total flux subtracted in 100 components = 0.0513261 Jy ! Clean residual min=-0.001437 max=0.002017 Jy/beam ! Clean residual mean=0.000000 rms=0.000399 Jy/beam ! Combined flux in latest and established models = 0.0513261 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 10 model components to the UV plane model. ! The established model now contains 10 components and 0.0513261 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=0.024259Jy sigma=0.696845 ! Fit after self-cal, rms=0.024254Jy sigma=0.696698 ! 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=2.477 mas, bmaj=5.521 mas, bpa=-6.751 degrees ! Estimated noise=0.179941 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 = 0.00297981 Jy ! Component: 100 - total flux cleaned = 0.00387478 Jy ! Component: 150 - total flux cleaned = 0.00402489 Jy ! Component: 200 - total flux cleaned = 0.00410946 Jy ! Total flux subtracted in 200 components = 0.00410946 Jy ! Clean residual min=-0.001309 max=0.001240 Jy/beam ! Clean residual mean=0.000001 rms=0.000287 Jy/beam ! Combined flux in latest and established models = 0.0554355 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 26 model components to the UV plane model. ! The established model now contains 34 components and 0.0554355 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=0.024016Jy sigma=0.689175 ! Fit after self-cal, rms=0.024013Jy sigma=0.689082 ! 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: 1.03824 ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.94 KP 0.90 LA 1.01 ! NL 0.96 OV 1.00 ! ! Amplitude normalization factor in sub-array 2: 0.986355 ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 FD 0.99 HN 1.02 LA 1.01 ! MK 0.89 NL 1.07 OV 1.05 PT 1.04 ! ! ! Correcting IF 2. ! Amplitude normalization factor in sub-array 1: 1.02732 ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.99 KP 0.91 LA 0.95 ! NL 0.99 OV 0.99 ! ! Amplitude normalization factor in sub-array 2: 0.990864 ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 FD 0.96 HN 1.02 LA 0.99 ! MK 0.97 NL 1.01 OV 1.03 PT 1.07 ! ! ! Correcting IF 3. ! Amplitude normalization factor in sub-array 1: 1.03347 ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.90 KP 0.98 LA 0.96 ! NL 1.01 OV 0.97 ! ! Amplitude normalization factor in sub-array 2: 0.979476 ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 1.00 HN 1.01 LA 0.99 ! MK 0.98 NL 1.12 OV 1.06 PT 1.01 ! ! ! Correcting IF 4. ! Amplitude normalization factor in sub-array 1: 1.03781 ! Telescope amplitude corrections in sub-array 1: ! BR 0.95 FD 0.92 KP 0.97 LA 0.98 ! NL 0.97 OV 0.99 ! ! Amplitude normalization factor in sub-array 2: 0.985453 ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 FD 1.03 HN 0.96 LA 0.98 ! MK 0.98 NL 1.08 OV 1.05 PT 1.00 ! ! ! Correcting IF 5. ! Amplitude normalization factor in sub-array 1: 1.01474 ! Telescope amplitude corrections in sub-array 1: ! BR 1.08 FD 0.95 KP 0.97 LA 0.99 ! NL 1.00 OV 0.93 ! ! Amplitude normalization factor in sub-array 2: 0.982019 ! Telescope amplitude corrections in sub-array 2: ! BR 1.05 FD 0.99 HN 1.03 LA 1.04 ! MK 0.94 NL 1.06 OV 1.05 PT 0.99 ! ! ! Correcting IF 6. ! Amplitude normalization factor in sub-array 1: 1.0336 ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.95 KP 1.00 LA 0.95 ! NL 0.99 OV 0.95 ! ! Amplitude normalization factor in sub-array 2: 0.984589 ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 FD 1.06 HN 0.99 LA 0.98 ! MK 0.97 NL 1.02 OV 1.08 PT 0.99 ! ! ! Correcting IF 7. ! Amplitude normalization factor in sub-array 1: 1.02791 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.92 KP 0.98 LA 0.97 ! NL 0.99 OV 0.98 ! ! Amplitude normalization factor in sub-array 2: 0.991764 ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 FD 0.98 HN 0.98 LA 1.01 ! MK 0.99 NL 1.06 OV 1.05 PT 0.97 ! ! ! Correcting IF 8. ! Amplitude normalization factor in sub-array 1: 1.00882 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.97 KP 1.03 LA 0.99 ! NL 0.95 OV 1.01 ! ! Amplitude normalization factor in sub-array 2: 0.98477 ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 FD 1.00 HN 1.04 LA 1.02 ! MK 0.96 NL 1.05 OV 0.99 PT 1.03 ! ! ! Fit before self-cal, rms=0.024013Jy sigma=0.689082 ! Fit after self-cal, rms=0.023790Jy sigma=0.684954 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=0.023790Jy sigma=0.684954 ! Fit after self-cal, rms=0.023790Jy sigma=0.684953 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=2.427 mas, bmaj=5.549 mas, bpa=-7.137 degrees ! Estimated noise=0.179829 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 = 0.000307074 Jy ! Component: 100 - total flux cleaned = 0.000280604 Jy ! Component: 150 - total flux cleaned = 0.000257962 Jy ! Component: 200 - total flux cleaned = 0.000247927 Jy ! Total flux subtracted in 200 components = 0.000247927 Jy ! Clean residual min=-0.000998 max=0.000975 Jy/beam ! Clean residual mean=0.000001 rms=0.000238 Jy/beam ! Combined flux in latest and established models = 0.0556835 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 21 model components to the UV plane model. ! The established model now contains 49 components and 0.0556835 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=0.023775Jy sigma=0.684516 ! Fit after self-cal, rms=0.023774Jy sigma=0.684510 ! 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=0.023774Jy sigma=0.684510 ! Fit after self-cal, rms=0.023770Jy sigma=0.684293 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 = -4.93253e-06 Jy ! Component: 100 - total flux cleaned = -2.22667e-05 Jy ! Component: 150 - total flux cleaned = -3.87162e-05 Jy ! Component: 200 - total flux cleaned = -5.42218e-05 Jy ! Total flux subtracted in 200 components = -5.42218e-05 Jy ! Clean residual min=-0.000975 max=0.000953 Jy/beam ! Clean residual mean=0.000001 rms=0.000236 Jy/beam ! Combined flux in latest and established models = 0.0556292 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 24 model components to the UV plane model. ! The established model now contains 59 components and 0.0556292 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=0.023765Jy sigma=0.684166 ! Fit after self-cal, rms=0.023766Jy sigma=0.684162 ! 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: 2.427 x 5.549 at -7.137 degrees (North through East) ! Clean map min=-0.00095691 max=0.051547 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=1.806 mas, bmaj=5.527 mas, bpa=-9.443 degrees ! Estimated noise=0.349073 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0434528 Jy ! Component: 100 - total flux cleaned = 0.0515778 Jy ! Component: 150 - total flux cleaned = 0.0542858 Jy ! Component: 200 - total flux cleaned = 0.0548544 Jy ! Total flux subtracted in 200 components = 0.0548544 Jy ! Clean residual min=-0.001080 max=0.001222 Jy/beam ! Clean residual mean=0.000000 rms=0.000277 Jy/beam ! Combined flux in latest and established models = 0.0548544 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 18 model components to the UV plane model. ! The established model now contains 18 components and 0.0548544 Jy ! Inverting map and beam ! Estimated beam: bmin=2.427 mas, bmaj=5.549 mas, bpa=-7.137 degrees ! Estimated noise=0.179829 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) ! Added new window around map position (3.3, -1.2). ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000776052 Jy ! Component: 100 - total flux cleaned = 0.00110287 Jy ! Component: 150 - total flux cleaned = 0.00106834 Jy ! Component: 200 - total flux cleaned = 0.00101011 Jy ! Total flux subtracted in 200 components = 0.00101011 Jy ! Clean residual min=-0.000868 max=0.000869 Jy/beam ! Clean residual mean=0.000001 rms=0.000214 Jy/beam ! Combined flux in latest and established models = 0.0558645 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 42 components and 0.0558645 Jy ! Inverting map clean ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -3.69005e-05 Jy ! Component: 100 - total flux cleaned = -8.86424e-05 Jy ! Component: 150 - total flux cleaned = -0.00011566 Jy ! Component: 200 - total flux cleaned = -0.000155302 Jy ! Total flux subtracted in 200 components = -0.000155302 Jy ! Clean residual min=-0.000847 max=0.000828 Jy/beam ! Clean residual mean=0.000001 rms=0.000210 Jy/beam ! Combined flux in latest and established models = 0.0557092 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 24 model components to the UV plane model. ! The established model now contains 54 components and 0.0557092 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=0.023727Jy sigma=0.682825 ! Fit after self-cal, rms=0.023725Jy sigma=0.682750 wmodel J0411+1714_C_map.mod ! Writing 54 model components to file: J0411+1714_C_map.mod wobs J0411+1714_C_uvs.fits ! Writing UV FITS file: J0411+1714_C_uvs.fits wwins J0411+1714_C_map.win ! wwins: Wrote 2 windows to J0411+1714_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 = 2.77703e-05 Jy ! Component: 100 - total flux cleaned = 0.000110628 Jy ! Component: 150 - total flux cleaned = 0.000161246 Jy ! Component: 200 - total flux cleaned = 0.000197156 Jy ! Component: 250 - total flux cleaned = 0.000253918 Jy ! Component: 300 - total flux cleaned = 0.000286261 Jy ! Component: 350 - total flux cleaned = 0.000306792 Jy ! Component: 400 - total flux cleaned = 0.000336752 Jy ! Component: 450 - total flux cleaned = 0.000384564 Jy ! Component: 500 - total flux cleaned = 0.000449299 Jy ! Component: 550 - total flux cleaned = 0.000520528 Jy ! Component: 600 - total flux cleaned = 0.000580542 Jy ! Component: 650 - total flux cleaned = 0.000646756 Jy ! Component: 700 - total flux cleaned = 0.000686553 Jy ! Component: 750 - total flux cleaned = 0.000701983 Jy ! Component: 800 - total flux cleaned = 0.000739626 Jy ! Component: 850 - total flux cleaned = 0.000783461 Jy ! Component: 900 - total flux cleaned = 0.000804848 Jy ! Component: 950 - total flux cleaned = 0.000839507 Jy ! Component: 1000 - total flux cleaned = 0.000846089 Jy ! Component: 1050 - total flux cleaned = 0.000872164 Jy ! Component: 1100 - total flux cleaned = 0.000878417 Jy ! Component: 1150 - total flux cleaned = 0.000903309 Jy ! Component: 1200 - total flux cleaned = 0.000927641 Jy ! Component: 1250 - total flux cleaned = 0.000939431 Jy ! Component: 1300 - total flux cleaned = 0.000945394 Jy ! Component: 1350 - total flux cleaned = 0.000956886 Jy ! Component: 1400 - total flux cleaned = 0.000962512 Jy ! Component: 1450 - total flux cleaned = 0.000962635 Jy ! Component: 1500 - total flux cleaned = 0.00097366 Jy ! Component: 1550 - total flux cleaned = 0.000979103 Jy ! Component: 1600 - total flux cleaned = 0.000989399 Jy ! Component: 1650 - total flux cleaned = 0.000989358 Jy ! Component: 1700 - total flux cleaned = 0.000979418 Jy ! Component: 1750 - total flux cleaned = 0.000984422 Jy ! Component: 1800 - total flux cleaned = 0.000965267 Jy ! Component: 1850 - total flux cleaned = 0.000974762 Jy ! Component: 1900 - total flux cleaned = 0.000979369 Jy ! Component: 1950 - total flux cleaned = 0.000993097 Jy ! Component: 2000 - total flux cleaned = 0.00100672 Jy ! Component: 2050 - total flux cleaned = 0.00100665 Jy ! Component: 2100 - total flux cleaned = 0.00099789 Jy ! Component: 2150 - total flux cleaned = 0.000997889 Jy ! Component: 2200 - total flux cleaned = 0.000989292 Jy ! Component: 2250 - total flux cleaned = 0.000989301 Jy ! Component: 2300 - total flux cleaned = 0.000985182 Jy ! Component: 2350 - total flux cleaned = 0.00098925 Jy ! Component: 2400 - total flux cleaned = 0.00100543 Jy ! Component: 2450 - total flux cleaned = 0.000997415 Jy ! Component: 2500 - total flux cleaned = 0.00100532 Jy ! Component: 2550 - total flux cleaned = 0.00100539 Jy ! Component: 2600 - total flux cleaned = 0.000993924 Jy ! Component: 2650 - total flux cleaned = 0.000997713 Jy ! Component: 2700 - total flux cleaned = 0.000997677 Jy ! Component: 2750 - total flux cleaned = 0.000990261 Jy ! Component: 2800 - total flux cleaned = 0.000993958 Jy ! Component: 2850 - total flux cleaned = 0.000975953 Jy ! Component: 2900 - total flux cleaned = 0.000958067 Jy ! Component: 2950 - total flux cleaned = 0.000951009 Jy ! Component: 3000 - total flux cleaned = 0.000933416 Jy ! Component: 3050 - total flux cleaned = 0.000905703 Jy ! Component: 3100 - total flux cleaned = 0.000885177 Jy ! Component: 3150 - total flux cleaned = 0.000885218 Jy ! Component: 3200 - total flux cleaned = 0.000875121 Jy ! Component: 3250 - total flux cleaned = 0.000855131 Jy ! Component: 3300 - total flux cleaned = 0.000838653 Jy ! Component: 3350 - total flux cleaned = 0.000835359 Jy ! Component: 3400 - total flux cleaned = 0.000828871 Jy ! Component: 3450 - total flux cleaned = 0.000812828 Jy ! Component: 3500 - total flux cleaned = 0.000812821 Jy ! Component: 3550 - total flux cleaned = 0.00080021 Jy ! Component: 3600 - total flux cleaned = 0.00080333 Jy ! Component: 3650 - total flux cleaned = 0.000800241 Jy ! Component: 3700 - total flux cleaned = 0.000791024 Jy ! Component: 3750 - total flux cleaned = 0.000794058 Jy ! Component: 3800 - total flux cleaned = 0.000781933 Jy ! Component: 3850 - total flux cleaned = 0.000787928 Jy ! Component: 3900 - total flux cleaned = 0.000778951 Jy ! Component: 3950 - total flux cleaned = 0.000781934 Jy ! Component: 4000 - total flux cleaned = 0.000779022 Jy ! Component: 4050 - total flux cleaned = 0.000776114 Jy ! Total flux subtracted in 4096 components = 0.000778987 Jy ! Clean residual min=-0.000173 max=0.000169 Jy/beam ! Clean residual mean=0.000001 rms=0.000057 Jy/beam ! Combined flux in latest and established models = 0.0564882 Jy keep ! Adding 324 model components to the UV plane model. ! The established model now contains 378 components and 0.0564882 Jy ![Exited script file: /opt64/bin/pima_mupet_02.dfm] wmap /vlbi/vcs9/uvm//J0411+1714_C_a_map.fits ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 2.427 x 5.549 at -7.137 degrees (North through East) ! Clean map min=-0.00062864 max=0.051539 Jy/beam ! Writing clean map to FITS file: /vlbi/vcs9/uvm//J0411+1714_C_a_map.fits wmodel /vlbi/vcs9/uvm//J0411+1714_C_a_map.mod ! Writing 378 model components to file: /vlbi/vcs9/uvm//J0411+1714_C_a_map.mod wobs /vlbi/vcs9/uvm//J0411+1714_C_a_uvs.fits ! Writing UV FITS file: /vlbi/vcs9/uvm//J0411+1714_C_a_uvs.fits wwins /vlbi/vcs9/uvm//J0411+1714_C_a_map.win ! wwins: Wrote 3 windows to /vlbi/vcs9/uvm//J0411+1714_C_a_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.0515392 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 5.50431e-05 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.320396 0.320396 0.640791 1.28158 2.56316 5.12633 10.2527 20.5053 41.0106 82.0213 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0001 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.051 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 936.342 quit ! Quitting program ! Log file /vlbi/vcs9/uvm//J0411+1714_C_a_dfm.log closed on Tue Dec 26 21:32:17 2017