! Started logfile: /vlbi/vcs9/uvm//J0310+1705_C_a_dfm.log on Tue Dec 26 21:19:59 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//J0310+1705_C_a_uvm.fits ! Reading UV FITS file: /vlbi/vcs9/uvm//J0310+1705_C_a_uvm.fits ! AN table 1: 47 integrations on 15 of 15 possible baselines. ! AN table 2: 51 integrations on 28 of 28 possible baselines. ! Apparent sampling: 0.971402 visibilities/baseline/integration-bin. ! Found source: J0310+1705 ! ! 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 16576 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 J0310+1705_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)= 0.0301275 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=1.000849Jy sigma=30.333073 ! Fit after self-cal, rms=0.984186Jy sigma=29.845820 ! 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=1.927 mas, bmaj=5.384 mas, bpa=-7.235 degrees ! Estimated noise=0.371853 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 = 0.0138068 Jy ! Component: 100 - total flux cleaned = 0.0156691 Jy ! Total flux subtracted in 100 components = 0.0156691 Jy ! Clean residual min=-0.001138 max=0.001206 Jy/beam ! Clean residual mean=0.000000 rms=0.000293 Jy/beam ! Combined flux in latest and established models = 0.0156691 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 8 model components to the UV plane model. ! The established model now contains 8 components and 0.0156691 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=0.025414Jy sigma=0.725862 ! Fit after self-cal, rms=0.025387Jy sigma=0.725011 ! 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=2.523 mas, bmaj=5.571 mas, bpa=-6.34 degrees ! Estimated noise=0.181249 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 = 0.000353754 Jy ! Component: 100 - total flux cleaned = 0.000462949 Jy ! Component: 150 - total flux cleaned = 0.000499338 Jy ! Component: 200 - total flux cleaned = 0.000499466 Jy ! Total flux subtracted in 200 components = 0.000499466 Jy ! Clean residual min=-0.000671 max=0.000685 Jy/beam ! Clean residual mean=0.000000 rms=0.000169 Jy/beam ! Combined flux in latest and established models = 0.0161685 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 24 model components to the UV plane model. ! The established model now contains 29 components and 0.0161685 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=0.025375Jy sigma=0.724763 ! Fit after self-cal, rms=0.025375Jy sigma=0.724760 ! 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: 1.17043 ! Telescope amplitude corrections in sub-array 1: ! BR 0.91 FD 0.88 KP 0.80 LA 0.70 ! NL 0.98 OV 0.85 ! ! Amplitude normalization factor in sub-array 2: 0.990946 ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 FD 0.95 HN 0.91 LA 1.13 ! MK 0.80 NL 1.13 OV 1.14 PT 0.97 ! ! ! Correcting IF 2. ! Amplitude normalization factor in sub-array 1: 1.03099 ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 FD 1.06 KP 0.91 LA 0.78 ! NL 0.98 OV 1.13 ! ! Amplitude normalization factor in sub-array 2: 1.02753 ! Telescope amplitude corrections in sub-array 2: ! BR 0.91 FD 0.95 HN 0.96 LA 0.88 ! MK 1.11 NL 0.98 OV 0.98 PT 1.01 ! ! ! Correcting IF 3. ! Amplitude normalization factor in sub-array 1: 0.968516 ! Telescope amplitude corrections in sub-array 1: ! BR 1.04 FD 1.13 KP 1.06 LA 1.11 ! NL 0.85 OV 1.01 ! ! Amplitude normalization factor in sub-array 2: 1.02564 ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 0.93 HN 1.12 LA 0.87 ! MK 0.87 NL 1.10 OV 0.93 PT 0.97 ! ! ! Correcting IF 4. ! Amplitude normalization factor in sub-array 1: 1.03087 ! Telescope amplitude corrections in sub-array 1: ! BR 0.95 FD 1.10 KP 1.07 LA 0.87 ! NL 0.94 OV 0.89 ! ! Amplitude normalization factor in sub-array 2: 1.08385 ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 0.94 HN 1.03 LA 0.87 ! MK 0.83 NL 0.95 OV 0.87 PT 0.92 ! ! ! Correcting IF 5. ! Amplitude normalization factor in sub-array 1: 0.960608 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 1.06 KP 1.26 LA 0.83 ! NL 1.13 OV 0.97 ! ! Amplitude normalization factor in sub-array 2: 1.01207 ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 FD 0.93 HN 0.88 LA 1.02 ! MK 0.93 NL 0.89 OV 0.97 PT 1.26 ! ! ! Correcting IF 6. ! Amplitude normalization factor in sub-array 1: 0.922059 ! Telescope amplitude corrections in sub-array 1: ! BR 1.23 FD 0.96 KP 1.08 LA 1.07 ! NL 1.11 OV 1.05 ! ! Amplitude normalization factor in sub-array 2: 0.916752 ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 FD 1.13 HN 1.38 LA 1.00 ! MK 1.02 NL 1.31 OV 0.93 PT 0.93 ! ! ! Correcting IF 7. ! Amplitude normalization factor in sub-array 1: 1.03347 ! Telescope amplitude corrections in sub-array 1: ! BR 0.86 FD 0.87 KP 1.08 LA 1.06 ! NL 0.96 OV 0.98 ! ! Amplitude normalization factor in sub-array 2: 0.918614 ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 1.14 HN 1.24 LA 1.11 ! MK 0.75 NL 1.17 OV 1.28 PT 1.03 ! ! ! Correcting IF 8. ! Amplitude normalization factor in sub-array 1: 0.950814 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 1.11 KP 1.03 LA 0.99 ! NL 0.92 OV 1.26 ! ! Amplitude normalization factor in sub-array 2: 0.975773 ! Telescope amplitude corrections in sub-array 2: ! BR 0.96 FD 1.04 HN 1.00 LA 1.01 ! MK 0.96 NL 1.28 OV 1.03 PT 0.91 ! ! ! Fit before self-cal, rms=0.025375Jy sigma=0.724760 ! Fit after self-cal, rms=0.025559Jy sigma=0.722081 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=0.025559Jy sigma=0.722081 ! Fit after self-cal, rms=0.025560Jy sigma=0.722069 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=2.472 mas, bmaj=5.549 mas, bpa=-7.06 degrees ! Estimated noise=0.175545 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 = -0.000177376 Jy ! Component: 100 - total flux cleaned = -0.000142766 Jy ! Component: 150 - total flux cleaned = -0.000138424 Jy ! Component: 200 - total flux cleaned = -0.000138403 Jy ! Total flux subtracted in 200 components = -0.000138403 Jy ! Clean residual min=-0.000573 max=0.000598 Jy/beam ! Clean residual mean=0.000001 rms=0.000139 Jy/beam ! Combined flux in latest and established models = 0.0160301 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 15 model components to the UV plane model. ! The established model now contains 40 components and 0.0160301 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=0.025561Jy sigma=0.721971 ! Fit after self-cal, rms=0.025561Jy sigma=0.721970 ! 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=0.025561Jy sigma=0.721970 ! Fit after self-cal, rms=0.025502Jy sigma=0.719769 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) ! Added new window around map position (-65.1, 25.2). ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000199246 Jy ! Component: 100 - total flux cleaned = 0.000119792 Jy ! Component: 150 - total flux cleaned = 0.000108426 Jy ! Component: 200 - total flux cleaned = 0.000108529 Jy ! Total flux subtracted in 200 components = 0.000108529 Jy ! Clean residual min=-0.000519 max=0.000501 Jy/beam ! Clean residual mean=0.000001 rms=0.000126 Jy/beam ! Combined flux in latest and established models = 0.0161387 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 21 model components to the UV plane model. ! The established model now contains 61 components and 0.0161387 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=0.025485Jy sigma=0.719292 ! Fit after self-cal, rms=0.025475Jy sigma=0.718930 ! 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: 2.472 x 5.549 at -7.06 degrees (North through East) ! Clean map min=-0.00050063 max=0.015554 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=1.906 mas, bmaj=5.369 mas, bpa=-7.383 degrees ! Estimated noise=0.363894 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0136211 Jy ! Component: 100 - total flux cleaned = 0.0158445 Jy ! Component: 150 - total flux cleaned = 0.0161707 Jy ! Component: 200 - total flux cleaned = 0.0161429 Jy ! Total flux subtracted in 200 components = 0.0161429 Jy ! Clean residual min=-0.000840 max=0.000962 Jy/beam ! Clean residual mean=0.000001 rms=0.000229 Jy/beam ! Combined flux in latest and established models = 0.0161429 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 31 model components to the UV plane model. ! The established model now contains 31 components and 0.0161429 Jy ! Inverting map and beam ! Estimated beam: bmin=2.472 mas, bmaj=5.549 mas, bpa=-7.06 degrees ! Estimated noise=0.175545 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 (-74.1, -6.9). ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000461491 Jy ! Component: 100 - total flux cleaned = 0.000651929 Jy ! Component: 150 - total flux cleaned = 0.000805822 Jy ! Component: 200 - total flux cleaned = 0.000884994 Jy ! Total flux subtracted in 200 components = 0.000884994 Jy ! Clean residual min=-0.000430 max=0.000499 Jy/beam ! Clean residual mean=0.000001 rms=0.000115 Jy/beam ! Combined flux in latest and established models = 0.0170279 Jy ! Adding 37 model components to the UV plane model. ! The established model now contains 67 components and 0.0170279 Jy ! Inverting map clean ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -2.03666e-05 Jy ! Component: 100 - total flux cleaned = 1.22722e-07 Jy ! Component: 150 - total flux cleaned = -9.07325e-06 Jy ! Component: 200 - total flux cleaned = -3.38873e-05 Jy ! Total flux subtracted in 200 components = -3.38873e-05 Jy ! Clean residual min=-0.000418 max=0.000459 Jy/beam ! Clean residual mean=0.000001 rms=0.000110 Jy/beam ! Combined flux in latest and established models = 0.016994 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 34 model components to the UV plane model. ! The established model now contains 85 components and 0.016994 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=0.025461Jy sigma=0.718433 ! Fit after self-cal, rms=0.025457Jy sigma=0.718288 wmodel J0310+1705_C_map.mod ! Writing 85 model components to file: J0310+1705_C_map.mod wobs J0310+1705_C_uvs.fits ! Writing UV FITS file: J0310+1705_C_uvs.fits wwins J0310+1705_C_map.win ! wwins: Wrote 3 windows to J0310+1705_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 = 7.58474e-05 Jy ! Component: 100 - total flux cleaned = 0.000167179 Jy ! Component: 150 - total flux cleaned = 0.000231308 Jy ! Component: 200 - total flux cleaned = 0.000265044 Jy ! Component: 250 - total flux cleaned = 0.000265395 Jy ! Component: 300 - total flux cleaned = 0.000290098 Jy ! Component: 350 - total flux cleaned = 0.000266281 Jy ! Component: 400 - total flux cleaned = 0.000277769 Jy ! Component: 450 - total flux cleaned = 0.000288875 Jy ! Component: 500 - total flux cleaned = 0.000299583 Jy ! Component: 550 - total flux cleaned = 0.000320965 Jy ! Component: 600 - total flux cleaned = 0.000346976 Jy ! Component: 650 - total flux cleaned = 0.000377409 Jy ! Component: 700 - total flux cleaned = 0.000397385 Jy ! Component: 750 - total flux cleaned = 0.000451485 Jy ! Component: 800 - total flux cleaned = 0.000504446 Jy ! Component: 850 - total flux cleaned = 0.000546998 Jy ! Component: 900 - total flux cleaned = 0.000598221 Jy ! Component: 950 - total flux cleaned = 0.000653015 Jy ! Component: 1000 - total flux cleaned = 0.000693481 Jy ! Component: 1050 - total flux cleaned = 0.000746548 Jy ! Component: 1100 - total flux cleaned = 0.000781378 Jy ! Component: 1150 - total flux cleaned = 0.000820069 Jy ! Component: 1200 - total flux cleaned = 0.000866632 Jy ! Component: 1250 - total flux cleaned = 0.000908217 Jy ! Component: 1300 - total flux cleaned = 0.000949248 Jy ! Component: 1350 - total flux cleaned = 0.000997738 Jy ! Component: 1400 - total flux cleaned = 0.0010295 Jy ! Component: 1450 - total flux cleaned = 0.00106484 Jy ! Component: 1500 - total flux cleaned = 0.00109582 Jy ! Component: 1550 - total flux cleaned = 0.00110731 Jy ! Component: 1600 - total flux cleaned = 0.0011338 Jy ! Component: 1650 - total flux cleaned = 0.00116375 Jy ! Component: 1700 - total flux cleaned = 0.00119337 Jy ! Component: 1750 - total flux cleaned = 0.00122261 Jy ! Component: 1800 - total flux cleaned = 0.0012443 Jy ! Component: 1850 - total flux cleaned = 0.00126571 Jy ! Component: 1900 - total flux cleaned = 0.00127982 Jy ! Component: 1950 - total flux cleaned = 0.00130081 Jy ! Component: 2000 - total flux cleaned = 0.00131813 Jy ! Component: 2050 - total flux cleaned = 0.00133859 Jy ! Component: 2100 - total flux cleaned = 0.00135551 Jy ! Component: 2150 - total flux cleaned = 0.0013689 Jy ! Component: 2200 - total flux cleaned = 0.00139209 Jy ! Component: 2250 - total flux cleaned = 0.0014085 Jy ! Component: 2300 - total flux cleaned = 0.00142152 Jy ! Component: 2350 - total flux cleaned = 0.00144402 Jy ! Component: 2400 - total flux cleaned = 0.00146633 Jy ! Component: 2450 - total flux cleaned = 0.00147891 Jy ! Component: 2500 - total flux cleaned = 0.00150074 Jy ! Component: 2550 - total flux cleaned = 0.00151311 Jy ! Component: 2600 - total flux cleaned = 0.0015284 Jy ! Component: 2650 - total flux cleaned = 0.00154352 Jy ! Component: 2700 - total flux cleaned = 0.0015495 Jy ! Component: 2750 - total flux cleaned = 0.00156143 Jy ! Component: 2800 - total flux cleaned = 0.00158206 Jy ! Component: 2850 - total flux cleaned = 0.00159665 Jy ! Component: 2900 - total flux cleaned = 0.00161405 Jy ! Component: 2950 - total flux cleaned = 0.00162552 Jy ! Component: 3000 - total flux cleaned = 0.00163691 Jy ! Component: 3050 - total flux cleaned = 0.00165387 Jy ! Component: 3100 - total flux cleaned = 0.00165391 Jy ! Component: 3150 - total flux cleaned = 0.00166788 Jy ! Component: 3200 - total flux cleaned = 0.00167339 Jy ! Component: 3250 - total flux cleaned = 0.00167891 Jy ! Component: 3300 - total flux cleaned = 0.00168711 Jy ! Component: 3350 - total flux cleaned = 0.00169256 Jy ! Component: 3400 - total flux cleaned = 0.00170336 Jy ! Component: 3450 - total flux cleaned = 0.00171404 Jy ! Component: 3500 - total flux cleaned = 0.00171137 Jy ! Component: 3550 - total flux cleaned = 0.00170874 Jy ! Component: 3600 - total flux cleaned = 0.0017219 Jy ! Component: 3650 - total flux cleaned = 0.00172714 Jy ! Component: 3700 - total flux cleaned = 0.00174013 Jy ! Component: 3750 - total flux cleaned = 0.00174012 Jy ! Component: 3800 - total flux cleaned = 0.00175556 Jy ! Component: 3850 - total flux cleaned = 0.0017709 Jy ! Component: 3900 - total flux cleaned = 0.00178618 Jy ! Component: 3950 - total flux cleaned = 0.00178869 Jy ! Component: 4000 - total flux cleaned = 0.0017887 Jy ! Component: 4050 - total flux cleaned = 0.00179375 Jy ! Total flux subtracted in 4096 components = 0.00180123 Jy ! Clean residual min=-0.000142 max=0.000169 Jy/beam ! Clean residual mean=0.000001 rms=0.000046 Jy/beam ! Combined flux in latest and established models = 0.0187952 Jy keep ! Adding 281 model components to the UV plane model. ! The established model now contains 366 components and 0.0187952 Jy ![Exited script file: /opt64/bin/pima_mupet_02.dfm] wmap /vlbi/vcs9/uvm//J0310+1705_C_a_map.fits ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 2.472 x 5.549 at -7.06 degrees (North through East) ! Clean map min=-0.00036861 max=0.015504 Jy/beam ! Writing clean map to FITS file: /vlbi/vcs9/uvm//J0310+1705_C_a_map.fits wmodel /vlbi/vcs9/uvm//J0310+1705_C_a_map.mod ! Writing 366 model components to file: /vlbi/vcs9/uvm//J0310+1705_C_a_map.mod wobs /vlbi/vcs9/uvm//J0310+1705_C_a_uvs.fits ! Writing UV FITS file: /vlbi/vcs9/uvm//J0310+1705_C_a_uvs.fits wwins /vlbi/vcs9/uvm//J0310+1705_C_a_map.win ! wwins: Wrote 4 windows to /vlbi/vcs9/uvm//J0310+1705_C_a_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.0155038 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 4.61638e-05 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.893276 0.893276 1.78655 3.5731 7.1462 14.2924 28.5848 57.1696 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0001 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.015 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 335.842 quit ! Quitting program ! Log file /vlbi/vcs9/uvm//J0310+1705_C_a_dfm.log closed on Tue Dec 26 21:20:02 2017