! Started logfile: /vlbi/vcs9/uvm//J0304+0955_C_a_dfm.log on Tue Dec 26 21:19:30 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//J0304+0955_C_a_uvm.fits ! Reading UV FITS file: /vlbi/vcs9/uvm//J0304+0955_C_a_uvm.fits ! AN table 1: 150 integrations on 36 of 36 possible baselines. ! AN table 2: 157 integrations on 36 of 36 possible baselines. ! Apparent sampling: 0.967789 visibilities/baseline/integration-bin. ! Found source: J0304+0955 ! ! 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 94 lines of history. ! ! Reading 85568 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 J0304+0955_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)= 0.0279672 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 16 telescope corrections were flagged in sub-array 1. ! A total of 66 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 2. ! A total of 16 telescope corrections were flagged in sub-array 1. ! A total of 66 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 3. ! A total of 16 telescope corrections were flagged in sub-array 1. ! A total of 66 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 4. ! A total of 16 telescope corrections were flagged in sub-array 1. ! A total of 66 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 5. ! A total of 16 telescope corrections were flagged in sub-array 1. ! A total of 66 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 6. ! A total of 16 telescope corrections were flagged in sub-array 1. ! A total of 66 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 7. ! A total of 16 telescope corrections were flagged in sub-array 1. ! A total of 66 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 8. ! A total of 16 telescope corrections were flagged in sub-array 1. ! A total of 66 telescope corrections were flagged in sub-array 2. ! ! Fit before self-cal, rms=1.000455Jy sigma=27.808039 ! Fit after self-cal, rms=0.990729Jy sigma=27.560220 ! 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=1.254 mas, bmaj=3.191 mas, bpa=-2.055 degrees ! Estimated noise=0.185713 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 = 0.00810819 Jy ! Component: 100 - total flux cleaned = 0.00920552 Jy ! Total flux subtracted in 100 components = 0.00920552 Jy ! Clean residual min=-0.000921 max=0.000748 Jy/beam ! Clean residual mean=0.000000 rms=0.000170 Jy/beam ! Combined flux in latest and established models = 0.00920552 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 4 model components to the UV plane model. ! The established model now contains 4 components and 0.00920552 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=0.026257Jy sigma=0.664061 ! Fit after self-cal, rms=0.026250Jy sigma=0.663859 ! 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=1.643 mas, bmaj=3.794 mas, bpa=-2.223 degrees ! Estimated noise=0.0869746 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 = -0.000145507 Jy ! Component: 100 - total flux cleaned = -0.000145862 Jy ! Component: 150 - total flux cleaned = -0.000148873 Jy ! Component: 200 - total flux cleaned = -0.000153824 Jy ! Total flux subtracted in 200 components = -0.000153824 Jy ! Clean residual min=-0.000587 max=0.000596 Jy/beam ! Clean residual mean=-0.000001 rms=0.000132 Jy/beam ! Combined flux in latest and established models = 0.00905169 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 10 model components to the UV plane model. ! The established model now contains 14 components and 0.00905169 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=0.026252Jy sigma=0.663838 ! Fit after self-cal, rms=0.026251Jy sigma=0.663823 ! 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: 1.2339 ! Telescope amplitude corrections in sub-array 1: ! BR 0.91 FD 0.71 HN 0.78 LA 0.74 ! MK 0.74 NL 0.86 OV 0.83 PT 0.91 ! SC 0.82 ! ! Amplitude normalization factor in sub-array 2: 1.21444 ! Telescope amplitude corrections in sub-array 2: ! BR 0.82 FD 0.57 HN 0.92 KP 0.85 ! LA 0.79 MK 0.79 NL 0.82 PT 0.96 ! SC 0.88 ! ! ! Correcting IF 2. ! Amplitude normalization factor in sub-array 1: 1.11271 ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 FD 0.79 HN 0.85 LA 0.87 ! MK 0.84 NL 0.88 OV 0.99 PT 1.02 ! SC 0.89 ! ! Amplitude normalization factor in sub-array 2: 1.13516 ! Telescope amplitude corrections in sub-array 2: ! BR 0.87 FD 0.58 HN 0.94 KP 0.99 ! LA 0.80 MK 0.95 NL 0.90 PT 0.90 ! SC 0.99 ! ! ! Correcting IF 3. ! Amplitude normalization factor in sub-array 1: 0.958651 ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 1.07 HN 1.01 LA 1.08 ! MK 0.90 NL 0.94 OV 1.25 PT 1.17 ! SC 0.97 ! ! Amplitude normalization factor in sub-array 2: 1.05828 ! Telescope amplitude corrections in sub-array 2: ! BR 0.93 FD 0.65 HN 0.89 KP 1.14 ! LA 0.93 MK 0.99 NL 0.90 PT 1.10 ! SC 0.97 ! ! ! Correcting IF 4. ! Amplitude normalization factor in sub-array 1: 0.877441 ! Telescope amplitude corrections in sub-array 1: ! BR 1.24 FD 1.22 HN 0.89 LA 1.01 ! MK 0.88 NL 1.67 OV 1.40 PT 1.08 ! SC 0.87 ! ! Amplitude normalization factor in sub-array 2: 1.00217 ! Telescope amplitude corrections in sub-array 2: ! BR 0.85 FD 0.83 HN 0.98 KP 1.15 ! LA 0.94 MK 1.07 NL 1.11 PT 1.15 ! SC 0.89 ! ! ! Correcting IF 5. ! Amplitude normalization factor in sub-array 1: 0.904451 ! Telescope amplitude corrections in sub-array 1: ! BR 1.09 FD 0.94 HN 1.16 LA 1.18 ! MK 1.22 NL 0.99 OV 1.12 PT 1.23 ! SC 1.03 ! ! Amplitude normalization factor in sub-array 2: 1.03373 ! Telescope amplitude corrections in sub-array 2: ! BR 0.96 FD 0.77 HN 0.97 KP 0.94 ! LA 0.82 MK 1.03 NL 1.10 PT 1.19 ! SC 0.92 ! ! ! Correcting IF 6. ! Amplitude normalization factor in sub-array 1: 0.888446 ! Telescope amplitude corrections in sub-array 1: ! BR 1.21 FD 1.37 HN 1.11 LA 0.88 ! MK 1.04 NL 1.30 OV 1.12 PT 1.18 ! SC 0.92 ! ! Amplitude normalization factor in sub-array 2: 0.954077 ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 0.96 HN 1.05 KP 1.21 ! LA 0.84 MK 1.10 NL 0.85 PT 1.28 ! SC 1.16 ! ! ! Correcting IF 7. ! Amplitude normalization factor in sub-array 1: 0.859737 ! Telescope amplitude corrections in sub-array 1: ! BR 1.22 FD 1.10 HN 0.98 LA 1.09 ! MK 1.10 NL 1.29 OV 1.31 PT 1.18 ! SC 1.19 ! ! Amplitude normalization factor in sub-array 2: 0.978847 ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 FD 0.89 HN 1.06 KP 1.24 ! LA 0.91 MK 1.01 NL 0.91 PT 1.20 ! SC 1.01 ! ! ! Correcting IF 8. ! Amplitude normalization factor in sub-array 1: 0.904512 ! Telescope amplitude corrections in sub-array 1: ! BR 0.92 FD 1.18 HN 1.06 LA 0.95 ! MK 1.16 NL 1.18 OV 1.16 PT 1.31 ! SC 1.03 ! ! Amplitude normalization factor in sub-array 2: 0.999741 ! Telescope amplitude corrections in sub-array 2: ! BR 0.95 FD 0.87 HN 1.05 KP 1.04 ! LA 0.79 MK 0.84 NL 1.08 PT 1.29 ! SC 1.10 ! ! ! Fit before self-cal, rms=0.026251Jy sigma=0.663823 ! Fit after self-cal, rms=0.026496Jy sigma=0.662265 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=0.026496Jy sigma=0.662265 ! Fit after self-cal, rms=0.026496Jy sigma=0.662249 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=1.618 mas, bmaj=3.763 mas, bpa=-2.298 degrees ! Estimated noise=0.0816078 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 = -0.000292745 Jy ! Component: 100 - total flux cleaned = -0.000246682 Jy ! Component: 150 - total flux cleaned = -0.00021837 Jy ! Component: 200 - total flux cleaned = -0.000196118 Jy ! Total flux subtracted in 200 components = -0.000196118 Jy ! Clean residual min=-0.000474 max=0.000403 Jy/beam ! Clean residual mean=-0.000001 rms=0.000093 Jy/beam ! Combined flux in latest and established models = 0.00885557 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 10 model components to the UV plane model. ! The established model now contains 21 components and 0.00885557 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=0.026502Jy sigma=0.662114 ! Fit after self-cal, rms=0.026502Jy sigma=0.662105 ! 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=0.026502Jy sigma=0.662105 ! Fit after self-cal, rms=0.026451Jy sigma=0.660048 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 = 0.000160986 Jy ! Component: 100 - total flux cleaned = 0.00022977 Jy ! Component: 150 - total flux cleaned = 0.000255065 Jy ! Component: 200 - total flux cleaned = 0.000260132 Jy ! Total flux subtracted in 200 components = 0.000260132 Jy ! Clean residual min=-0.000466 max=0.000408 Jy/beam ! Clean residual mean=-0.000001 rms=0.000092 Jy/beam ! Combined flux in latest and established models = 0.00911571 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 19 model components to the UV plane model. ! The established model now contains 32 components and 0.00911571 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=0.026447Jy sigma=0.660023 ! Fit after self-cal, rms=0.026444Jy sigma=0.659812 ! 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 3.763 at -2.298 degrees (North through East) ! Clean map min=-0.00043711 max=0.0088288 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=1.25 mas, bmaj=3.188 mas, bpa=-2.232 degrees ! Estimated noise=0.178051 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.00795301 Jy ! Component: 100 - total flux cleaned = 0.00905658 Jy ! Component: 150 - total flux cleaned = 0.00920567 Jy ! Component: 200 - total flux cleaned = 0.00921416 Jy ! Total flux subtracted in 200 components = 0.00921416 Jy ! Clean residual min=-0.000678 max=0.000645 Jy/beam ! Clean residual mean=0.000000 rms=0.000146 Jy/beam ! Combined flux in latest and established models = 0.00921416 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 13 model components to the UV plane model. ! The established model now contains 13 components and 0.00921416 Jy ! Inverting map and beam ! Estimated beam: bmin=1.618 mas, bmaj=3.763 mas, bpa=-2.298 degrees ! Estimated noise=0.0816078 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 = -0.000118382 Jy ! Component: 100 - total flux cleaned = -9.28125e-05 Jy ! Component: 150 - total flux cleaned = -7.4862e-05 Jy ! Component: 200 - total flux cleaned = -6.81884e-05 Jy ! Total flux subtracted in 200 components = -6.81884e-05 Jy ! Clean residual min=-0.000472 max=0.000415 Jy/beam ! Clean residual mean=-0.000001 rms=0.000092 Jy/beam ! Combined flux in latest and established models = 0.00914597 Jy ! Adding 14 model components to the UV plane model. ! The established model now contains 26 components and 0.00914597 Jy ! Inverting map clean ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 2.42378e-06 Jy ! Component: 100 - total flux cleaned = 4.31329e-06 Jy ! Component: 150 - total flux cleaned = 5.87521e-06 Jy ! Component: 200 - total flux cleaned = 7.23155e-06 Jy ! Total flux subtracted in 200 components = 7.23155e-06 Jy ! Clean residual min=-0.000466 max=0.000415 Jy/beam ! Clean residual mean=-0.000001 rms=0.000092 Jy/beam ! Combined flux in latest and established models = 0.0091532 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 15 model components to the UV plane model. ! The established model now contains 34 components and 0.0091532 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=0.026443Jy sigma=0.659816 ! Fit after self-cal, rms=0.026443Jy sigma=0.659780 wmodel J0304+0955_C_map.mod ! Writing 34 model components to file: J0304+0955_C_map.mod wobs J0304+0955_C_uvs.fits ! Writing UV FITS file: J0304+0955_C_uvs.fits wwins J0304+0955_C_map.win ! wwins: Wrote 1 windows to J0304+0955_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 = -0.000133631 Jy ! Component: 100 - total flux cleaned = -0.000197621 Jy ! Component: 150 - total flux cleaned = -0.000217561 Jy ! Component: 200 - total flux cleaned = -0.000205508 Jy ! Component: 250 - total flux cleaned = -0.000193878 Jy ! Component: 300 - total flux cleaned = -0.000182624 Jy ! Component: 350 - total flux cleaned = -0.000155936 Jy ! Component: 400 - total flux cleaned = -0.000125261 Jy ! Component: 450 - total flux cleaned = -9.07593e-05 Jy ! Component: 500 - total flux cleaned = -6.20146e-05 Jy ! Component: 550 - total flux cleaned = -2.4709e-05 Jy ! Component: 600 - total flux cleaned = 1.60716e-05 Jy ! Component: 650 - total flux cleaned = 6.02857e-05 Jy ! Component: 700 - total flux cleaned = 0.000103411 Jy ! Component: 750 - total flux cleaned = 0.000145549 Jy ! Component: 800 - total flux cleaned = 0.000190951 Jy ! Component: 850 - total flux cleaned = 0.000231393 Jy ! Component: 900 - total flux cleaned = 0.000267063 Jy ! Component: 950 - total flux cleaned = 0.000305924 Jy ! Component: 1000 - total flux cleaned = 0.000347945 Jy ! Component: 1050 - total flux cleaned = 0.000389315 Jy ! Component: 1100 - total flux cleaned = 0.000422657 Jy ! Component: 1150 - total flux cleaned = 0.000448175 Jy ! Component: 1200 - total flux cleaned = 0.000469777 Jy ! Component: 1250 - total flux cleaned = 0.000494535 Jy ! Component: 1300 - total flux cleaned = 0.000522453 Jy ! Component: 1350 - total flux cleaned = 0.000529343 Jy ! Component: 1400 - total flux cleaned = 0.000559902 Jy ! Component: 1450 - total flux cleaned = 0.000576613 Jy ! Component: 1500 - total flux cleaned = 0.000589853 Jy ! Component: 1550 - total flux cleaned = 0.000602989 Jy ! Component: 1600 - total flux cleaned = 0.000628843 Jy ! Component: 1650 - total flux cleaned = 0.000651221 Jy ! Component: 1700 - total flux cleaned = 0.000667038 Jy ! Component: 1750 - total flux cleaned = 0.000695138 Jy ! Component: 1800 - total flux cleaned = 0.000713603 Jy ! Component: 1850 - total flux cleaned = 0.000731825 Jy ! Component: 1900 - total flux cleaned = 0.000740881 Jy ! Component: 1950 - total flux cleaned = 0.000764776 Jy ! Component: 2000 - total flux cleaned = 0.000782514 Jy ! Component: 2050 - total flux cleaned = 0.000800079 Jy ! Component: 2100 - total flux cleaned = 0.000829074 Jy ! Component: 2150 - total flux cleaned = 0.000826182 Jy ! Component: 2200 - total flux cleaned = 0.000854635 Jy ! Component: 2250 - total flux cleaned = 0.000871538 Jy ! Component: 2300 - total flux cleaned = 0.000885535 Jy ! Component: 2350 - total flux cleaned = 0.000904927 Jy ! Component: 2400 - total flux cleaned = 0.000921346 Jy ! Component: 2450 - total flux cleaned = 0.000945783 Jy ! Component: 2500 - total flux cleaned = 0.000956538 Jy ! Component: 2550 - total flux cleaned = 0.000980556 Jy ! Component: 2600 - total flux cleaned = 0.000988512 Jy ! Component: 2650 - total flux cleaned = 0.00100162 Jy ! Component: 2700 - total flux cleaned = 0.00100685 Jy ! Component: 2750 - total flux cleaned = 0.00103264 Jy ! Component: 2800 - total flux cleaned = 0.00104288 Jy ! Component: 2850 - total flux cleaned = 0.00105307 Jy ! Component: 2900 - total flux cleaned = 0.00107573 Jy ! Component: 2950 - total flux cleaned = 0.00107826 Jy ! Component: 3000 - total flux cleaned = 0.00108818 Jy ! Component: 3050 - total flux cleaned = 0.00110294 Jy ! Component: 3100 - total flux cleaned = 0.00110784 Jy ! Component: 3150 - total flux cleaned = 0.00112723 Jy ! Component: 3200 - total flux cleaned = 0.00112965 Jy ! Component: 3250 - total flux cleaned = 0.00113443 Jy ! Component: 3300 - total flux cleaned = 0.00113918 Jy ! Component: 3350 - total flux cleaned = 0.00115095 Jy ! Component: 3400 - total flux cleaned = 0.00115799 Jy ! Component: 3450 - total flux cleaned = 0.00116963 Jy ! Component: 3500 - total flux cleaned = 0.00116268 Jy ! Component: 3550 - total flux cleaned = 0.00117415 Jy ! Component: 3600 - total flux cleaned = 0.00118784 Jy ! Component: 3650 - total flux cleaned = 0.00119463 Jy ! Component: 3700 - total flux cleaned = 0.00119687 Jy ! Component: 3750 - total flux cleaned = 0.00121255 Jy ! Component: 3800 - total flux cleaned = 0.00122365 Jy ! Component: 3850 - total flux cleaned = 0.00122585 Jy ! Component: 3900 - total flux cleaned = 0.00123021 Jy ! Component: 3950 - total flux cleaned = 0.00123891 Jy ! Component: 4000 - total flux cleaned = 0.00123889 Jy ! Component: 4050 - total flux cleaned = 0.00124534 Jy ! Total flux subtracted in 4096 components = 0.00125603 Jy ! Clean residual min=-0.000109 max=0.000137 Jy/beam ! Clean residual mean=-0.000000 rms=0.000038 Jy/beam ! Combined flux in latest and established models = 0.0104092 Jy keep ! Adding 336 model components to the UV plane model. ! The established model now contains 370 components and 0.0104092 Jy ![Exited script file: /opt64/bin/pima_mupet_02.dfm] wmap /vlbi/vcs9/uvm//J0304+0955_C_a_map.fits ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.618 x 3.763 at -2.298 degrees (North through East) ! Clean map min=-0.00026006 max=0.0088901 Jy/beam ! Writing clean map to FITS file: /vlbi/vcs9/uvm//J0304+0955_C_a_map.fits wmodel /vlbi/vcs9/uvm//J0304+0955_C_a_map.mod ! Writing 370 model components to file: /vlbi/vcs9/uvm//J0304+0955_C_a_map.mod wobs /vlbi/vcs9/uvm//J0304+0955_C_a_uvs.fits ! Writing UV FITS file: /vlbi/vcs9/uvm//J0304+0955_C_a_uvs.fits wwins /vlbi/vcs9/uvm//J0304+0955_C_a_map.win ! wwins: Wrote 2 windows to /vlbi/vcs9/uvm//J0304+0955_C_a_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.00889012 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 3.82332e-05 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -1.29019 1.29019 2.58038 5.16077 10.3215 20.6431 41.2861 82.5723 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0001 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.008 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 232.523 quit ! Quitting program ! Log file /vlbi/vcs9/uvm//J0304+0955_C_a_dfm.log closed on Tue Dec 26 21:19:35 2017