! Started logfile: /scr/pima/rv124_uvs/J0205+3212_X_dfm.log on Mon Dec 24 00:16:21 2018 float field_size field_size = 1024 float field_cell field_cell = 0.2000 float taper_size taper_size = 70.0 float freq freq = 8.36575 obs /scr/pima/rv124_uvs/J0205+3212_X_uva.fits ! Reading UV FITS file: /scr/pima/rv124_uvs/J0205+3212_X_uva.fits ! AN table 1: 9 integrations on 36 of 36 possible baselines. ! AN table 2: 9 integrations on 45 of 45 possible baselines. ! AN table 3: 29 integrations on 15 of 15 possible baselines. ! AN table 4: 83 integrations on 10 of 10 possible baselines. ! AN table 5: 12 integrations on 3 of 3 possible baselines. ! AN table 6: 4 integrations on 28 of 28 possible baselines. ! AN table 7: 51 integrations on 55 of 55 possible baselines. ! AN table 8: 11 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.369717 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0205+3212 ! ! There are 4 IFs, and a total of 4 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 8.36575e+09 8e+06 1 8e+06 ! 02 2 8.44575e+09 8e+06 1 8e+06 ! 03 3 8.80575e+09 8e+06 1 8e+06 ! 04 4 8.92575e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 79 lines of history. ! ! Reading 8048 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 4 channels. ! Selecting polarization: RR, channels: 1..4 ! Reading IF 1 channels: 1..1 ! Reading IF 2 channels: 2..2 ! Reading IF 3 channels: 3..3 ! Reading IF 4 channels: 4..4 print "field_size =", field_size ! field_size = 1024 print "field_cell =", field_cell ! field_cell = 0.2 print "taper_size =", taper_size ! taper_size = 70 ![@/opt64/bin/pima_mupet_01.dfm J0205+3212_X] float lim_self lim_self = 120.0 float lim_val lim_va = 1.2 integer clean_niter clean_niter = 100 float clean_gain clean_gain = 0.03 float dynam dynam = 6.0 float soltime1 soltime1 = 120 float soltime2 soltime2 = 20 float thresh thresh = 0.5 float win_mult win_mult = 1.8 float time_av time_av = 16 float old_peak float new_peak float flux_cutoff print "===============================================================" ! =============================================================== ! print "=== Difmap script: pima_mupet_01.dvm version of 2016.05.19 === " ! === Difmap script: pima_mupet_01.dvm version of 2016.05.19 === ! mapsize field_size, field_cell ! Map grid = 1024x1024 pixels with 0.200x0.200 milli-arcsec cellsize. 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 15 telescope corrections were flagged in sub-array 1. ! A total of 52 telescope corrections were flagged in sub-array 2. ! A total of 110 telescope corrections were flagged in sub-array 3. ! A total of 244 telescope corrections were flagged in sub-array 4. ! A total of 18 telescope corrections were flagged in sub-array 5. ! A total of 12 telescope corrections were flagged in sub-array 6. ! A total of 397 telescope corrections were flagged in sub-array 7. ! A total of 46 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 2. ! A total of 15 telescope corrections were flagged in sub-array 1. ! A total of 52 telescope corrections were flagged in sub-array 2. ! A total of 110 telescope corrections were flagged in sub-array 3. ! A total of 244 telescope corrections were flagged in sub-array 4. ! A total of 18 telescope corrections were flagged in sub-array 5. ! A total of 12 telescope corrections were flagged in sub-array 6. ! A total of 397 telescope corrections were flagged in sub-array 7. ! A total of 46 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 3. ! A total of 15 telescope corrections were flagged in sub-array 1. ! A total of 54 telescope corrections were flagged in sub-array 2. ! A total of 146 telescope corrections were flagged in sub-array 3. ! A total of 298 telescope corrections were flagged in sub-array 4. ! A total of 18 telescope corrections were flagged in sub-array 5. ! A total of 12 telescope corrections were flagged in sub-array 6. ! A total of 425 telescope corrections were flagged in sub-array 7. ! A total of 50 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 4. ! A total of 15 telescope corrections were flagged in sub-array 1. ! A total of 54 telescope corrections were flagged in sub-array 2. ! A total of 146 telescope corrections were flagged in sub-array 3. ! A total of 298 telescope corrections were flagged in sub-array 4. ! A total of 18 telescope corrections were flagged in sub-array 5. ! A total of 12 telescope corrections were flagged in sub-array 6. ! A total of 425 telescope corrections were flagged in sub-array 7. ! A total of 50 telescope corrections were flagged in sub-array 8. ! ! Fit before self-cal, rms=1.533087Jy sigma=42.995345 ! Fit after self-cal, rms=0.476159Jy sigma=36.684209 ! 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. flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1624 milli-arcsec ! Estimated beam: bmin=0.4411 mas, bmaj=0.5287 mas, bpa=33.53 degrees ! Estimated noise=0.805673 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (0, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.706422 Jy ! Component: 100 - total flux cleaned = 1.03945 Jy ! Total flux subtracted in 100 components = 1.03945 Jy ! Clean residual min=-0.044692 max=0.159771 Jy/beam ! Clean residual mean=-0.000081 rms=0.010784 Jy/beam ! Combined flux in latest and established models = 1.03945 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 9 components and 1.03945 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.375905Jy sigma=5.607493 ! Fit after self-cal, rms=0.372275Jy sigma=5.595198 ! Inverting map ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1624 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.180827 Jy ! Component: 100 - total flux cleaned = 0.279335 Jy ! Total flux subtracted in 100 components = 0.279335 Jy ! Clean residual min=-0.048478 max=0.047339 Jy/beam ! Clean residual mean=-0.000147 rms=0.007999 Jy/beam ! Combined flux in latest and established models = 1.31878 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 10 components and 1.31878 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.270827Jy sigma=4.492653 ! Fit after self-cal, rms=0.270643Jy sigma=4.460577 ! Inverting map ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1624 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0554277 Jy ! Component: 100 - total flux cleaned = 0.0854301 Jy ! Total flux subtracted in 100 components = 0.0854301 Jy ! Clean residual min=-0.053284 max=0.038968 Jy/beam ! Clean residual mean=-0.000168 rms=0.007420 Jy/beam ! Combined flux in latest and established models = 1.40421 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 11 components and 1.40421 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.269133Jy sigma=4.453819 ! Fit after self-cal, rms=0.268996Jy sigma=4.436030 ! Inverting map ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1624 milli-arcsec print "============== Finished uniform weighting clean ===============" ! ============== Finished uniform weighting clean =============== ! uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! 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 ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1624 milli-arcsec ! Estimated beam: bmin=0.383 mas, bmaj=0.7611 mas, bpa=43.65 degrees ! Estimated noise=0.584155 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0239115 Jy ! Component: 100 - total flux cleaned = -0.0239002 Jy ! Component: 150 - total flux cleaned = -0.0234576 Jy ! Component: 200 - total flux cleaned = -0.0230866 Jy ! Total flux subtracted in 200 components = -0.0230866 Jy ! Clean residual min=-0.035570 max=0.016817 Jy/beam ! Clean residual mean=-0.014679 rms=0.004666 Jy/beam ! Combined flux in latest and established models = 1.38113 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 16 components and 1.38113 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.265579Jy sigma=4.794693 ! Fit after self-cal, rms=0.265613Jy sigma=4.756072 ! Inverting map ! Your choice of large map pixels excluded 6.47% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1624 milli-arcsec print "============== Finished natural weighting clean ==============" ! ============== Finished natural weighting clean ============== ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.383 x 0.7611 at 43.65 degrees (North through East) ! Clean map min=-0.029893 max=0.77893 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.88 HN 1.18 KP 1.09 ! LA 1.02 MK 0.95 NL 1.04 OV 0.95 ! PT 0.87 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 0.95 KP 1.07 LA 1.05 ! MK 0.93 NL 1.09 NY 0.61 OV 0.97 ! PT 0.88 YG 21.91 ! ! A total of 36 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.04 MK 0.86 NY 0.69 WN 1.73 ! WZ 1.03 YG 7.73 ! ! A total of 99 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HH 1.00* NY 0.78 WN 1.64 WZ 0.95 ! YG 5.58 ! ! A total of 18 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! LA 0.00* WN 0.00* WZ 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! FD 0.96 HH 1.00* HN 1.03 LA 1.03 ! NL 1.11 PT 0.94 SC 0.92 WZ 0.96 ! ! A total of 36 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.00 FD 0.90 HH 1.00* HN 1.05 ! KP 1.06 NL 1.09 NY 0.70 PT 0.90 ! SC 0.89 WN 1.61 WZ 1.00 ! ! A total of 12 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! BR 1.01 FD 0.91 HN 1.03 KP 1.06 ! NL 1.05 NY 0.67 OV 0.95 PT 0.88 ! SC 0.86 WZ 1.00 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.89 HN 1.20 KP 1.07 ! LA 1.02 MK 0.95 NL 1.04 OV 0.95 ! PT 0.85 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 0.96 KP 1.07 LA 1.04 ! MK 0.93 NL 1.09 NY 0.71 OV 0.98 ! PT 0.90 YG 23.06 ! ! A total of 36 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.08 MK 0.89 NY 0.81 WN 1.73 ! WZ 1.00 YG 6.11 ! ! A total of 99 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HH 1.00* NY 0.93 WN 1.64 WZ 0.91 ! YG 5.27 ! ! A total of 18 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! LA 0.00* WN 0.00* WZ 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! FD 0.97 HH 1.00* HN 1.04 LA 1.05 ! NL 1.08 PT 0.97 SC 0.90 WZ 0.91 ! ! A total of 36 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.00 FD 0.90 HH 1.00* HN 1.06 ! KP 1.04 NL 1.07 NY 0.82 PT 0.91 ! SC 0.87 WN 1.63 WZ 0.94 ! ! A total of 12 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! BR 1.01 FD 0.90 HN 1.05 KP 1.05 ! NL 1.05 NY 0.79 OV 0.95 PT 0.87 ! SC 0.85 WZ 0.96 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.89 HN 1.17 KP 1.06 ! LA 1.03 MK 0.89 NL 1.04 OV 0.95 ! PT 0.84 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 0.97 KP 1.05 LA 1.04 ! MK 0.91 NL 1.08 NY 1.00* OV 0.96 ! PT 0.87 YG 16.70 ! ! A total of 18 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.06 MK 0.84 NY 1.00* WN 1.60 ! WZ 1.00 YG 7.16 ! ! A total of 117 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HH 0.00* NY 0.00* WN 0.00* WZ 0.00* ! YG 0.00* ! ! A total of 18 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! LA 0.00* WN 0.00* WZ 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! FD 0.98 HH 1.00* HN 1.04 LA 1.05 ! NL 1.07 PT 1.01 SC 0.87 WZ 0.95 ! ! A total of 30 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.00 FD 0.88 HH 1.00* HN 1.06 ! KP 1.04 NL 1.09 NY 1.00* PT 0.95 ! SC 0.87 WN 1.51 WZ 0.99 ! ! A total of 12 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! BR 1.02 FD 0.91 HN 1.03 KP 1.03 ! NL 1.04 NY 1.00* OV 0.94 PT 0.91 ! SC 0.83 WZ 0.99 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.89 HN 1.18 KP 1.07 ! LA 1.04 MK 0.89 NL 1.04 OV 0.96 ! PT 0.84 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 FD 0.99 KP 1.05 LA 1.05 ! MK 0.90 NL 1.05 NY 1.00* OV 0.98 ! PT 0.85 YG 17.14 ! ! A total of 18 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.14 MK 0.78 NY 1.00* WN 1.41 ! WZ 1.06 YG 6.46 ! ! A total of 117 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HH 0.00* NY 0.00* WN 0.00* WZ 0.00* ! YG 0.00* ! ! A total of 18 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! LA 0.00* WN 0.00* WZ 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! FD 0.96 HH 1.00* HN 1.05 LA 1.02 ! NL 1.11 PT 1.00 SC 0.93 WZ 0.96 ! ! A total of 30 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.00 FD 0.91 HH 1.00* HN 1.03 ! KP 1.04 NL 1.09 NY 1.00* PT 0.94 ! SC 0.88 WN 1.37 WZ 1.02 ! ! A total of 12 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! BR 1.02 FD 0.92 HN 1.02 KP 1.04 ! NL 1.04 NY 1.00* OV 0.95 PT 0.90 ! SC 0.86 WZ 1.01 ! ! ! Fit before self-cal, rms=0.265613Jy sigma=4.756072 ! Fit after self-cal, rms=0.160238Jy sigma=1.296041 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec ! Estimated beam: bmin=0.7033 mas, bmaj=1.189 mas, bpa=-0.1911 degrees ! Estimated noise=0.917936 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (0.4, 1.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00861208 Jy ! Component: 100 - total flux cleaned = 0.00962877 Jy ! Component: 150 - total flux cleaned = 0.0100717 Jy ! Component: 200 - total flux cleaned = 0.00970303 Jy ! Total flux subtracted in 200 components = 0.00970303 Jy ! Clean residual min=-0.012310 max=0.011295 Jy/beam ! Clean residual mean=-0.000473 rms=0.002452 Jy/beam ! Combined flux in latest and established models = 1.39083 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 29 components and 1.39083 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.156459Jy sigma=1.241403 ! Fit after self-cal, rms=0.155984Jy sigma=1.229549 ! Inverting map ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec selfcal true, true, soltime1 ! Performing amp+phase self-cal over 120 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.155984Jy sigma=1.229549 ! Fit after self-cal, rms=0.134228Jy sigma=1.021780 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec ! Estimated beam: bmin=0.6992 mas, bmaj=1.163 mas, bpa=0.6201 degrees ! Estimated noise=0.91187 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00367119 Jy ! Component: 100 - total flux cleaned = 0.0027058 Jy ! Component: 150 - total flux cleaned = 0.00247889 Jy ! Component: 200 - total flux cleaned = 0.00227249 Jy ! Total flux subtracted in 200 components = 0.00227249 Jy ! Clean residual min=-0.007609 max=0.008209 Jy/beam ! Clean residual mean=-0.000659 rms=0.001476 Jy/beam ! Combined flux in latest and established models = 1.3931 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 33 components and 1.3931 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.132581Jy sigma=0.998309 ! Fit after self-cal, rms=0.132466Jy sigma=0.994988 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (-0.8, 7.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00823121 Jy ! Component: 100 - total flux cleaned = 0.0103833 Jy ! Component: 150 - total flux cleaned = 0.011203 Jy ! Component: 200 - total flux cleaned = 0.0113925 Jy ! Total flux subtracted in 200 components = 0.0113925 Jy ! Clean residual min=-0.007269 max=0.005934 Jy/beam ! Clean residual mean=-0.000797 rms=0.001371 Jy/beam ! Combined flux in latest and established models = 1.4045 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 41 components and 1.4045 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.131531Jy sigma=0.979527 ! Fit after self-cal, rms=0.131495Jy sigma=0.978600 ! Inverting map ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec selfcal true, true, soltime2 ! Performing amp+phase self-cal over 20 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.131495Jy sigma=0.978600 ! Fit after self-cal, rms=0.116400Jy sigma=0.905894 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec ! Estimated beam: bmin=0.6983 mas, bmaj=1.146 mas, bpa=0.7654 degrees ! Estimated noise=0.909092 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00192337 Jy ! Component: 100 - total flux cleaned = 0.00292558 Jy ! Component: 150 - total flux cleaned = 0.00327829 Jy ! Component: 200 - total flux cleaned = 0.00328346 Jy ! Total flux subtracted in 200 components = 0.00328346 Jy ! Clean residual min=-0.005616 max=0.005594 Jy/beam ! Clean residual mean=-0.000591 rms=0.001059 Jy/beam ! Combined flux in latest and established models = 1.40778 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 49 components and 1.40778 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.115596Jy sigma=0.894659 ! Fit after self-cal, rms=0.115638Jy sigma=0.893491 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000716948 Jy ! Component: 100 - total flux cleaned = 0.000889464 Jy ! Component: 150 - total flux cleaned = 0.000724552 Jy ! Component: 200 - total flux cleaned = 0.000877899 Jy ! Total flux subtracted in 200 components = 0.000877899 Jy ! Clean residual min=-0.005432 max=0.005450 Jy/beam ! Clean residual mean=-0.000601 rms=0.001030 Jy/beam ! Combined flux in latest and established models = 1.40866 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 50 components and 1.40866 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.114837Jy sigma=0.886789 ! Fit after self-cal, rms=0.114943Jy sigma=0.886112 ! Inverting map ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. win_mult = win_mult * 1.2 selfcal true, true, soltime2 ! Performing amp+phase self-cal over 20 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.114943Jy sigma=0.886112 ! Fit after self-cal, rms=0.110031Jy sigma=0.883948 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec ! Estimated beam: bmin=2.448 mas, bmaj=3.008 mas, bpa=89.42 degrees ! Estimated noise=1.23554 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00237372 Jy ! Component: 100 - total flux cleaned = 0.00298097 Jy ! Component: 150 - total flux cleaned = 0.00307442 Jy ! Component: 200 - total flux cleaned = 0.00315296 Jy ! Total flux subtracted in 200 components = 0.00315296 Jy ! Clean residual min=-0.005361 max=0.005180 Jy/beam ! Clean residual mean=-0.001413 rms=0.001056 Jy/beam ! Combined flux in latest and established models = 1.41181 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 59 components and 1.41181 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.110217Jy sigma=0.882843 ! Fit after self-cal, rms=0.110252Jy sigma=0.882087 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 6.70678e-05 Jy ! Component: 100 - total flux cleaned = 0.000139954 Jy ! Component: 150 - total flux cleaned = 0.000138547 Jy ! Component: 200 - total flux cleaned = 0.000190146 Jy ! Total flux subtracted in 200 components = 0.000190146 Jy ! Clean residual min=-0.005371 max=0.005045 Jy/beam ! Clean residual mean=-0.001419 rms=0.001043 Jy/beam ! Combined flux in latest and established models = 1.412 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 68 components and 1.412 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.110233Jy sigma=0.881518 ! Fit after self-cal, rms=0.110234Jy sigma=0.881284 ! Inverting map ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. win_mult = win_mult / 1.2 print "============== Finished amplitude self-cal ==============" ! ============== Finished amplitude self-cal ============== restore ! Inverting map and beam ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec ! Estimated beam: bmin=0.699 mas, bmaj=1.146 mas, bpa=0.2893 degrees ! Estimated noise=0.908588 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.699 x 1.146 at 0.2893 degrees (North through East) ! Clean map min=-0.00629 max=1.1482 Jy/beam if(peak(flux) > thresh) selfcal true, true clean clean_niter,clean_gain selfcal 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 new_peak = peak(flux) until(new_peak<=flux_cutoff) selfcal true, true end if ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.110234Jy sigma=0.881284 ! Fit after self-cal, rms=0.123038Jy sigma=0.809888 ! Inverting map and beam ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec ! Estimated beam: bmin=0.6938 mas, bmaj=1.127 mas, bpa=-1.367 degrees ! Estimated noise=0.904628 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000476728 Jy ! Component: 100 - total flux cleaned = -0.000476969 Jy ! Component: 150 - total flux cleaned = -0.000486187 Jy ! Component: 200 - total flux cleaned = -0.000627407 Jy ! Total flux subtracted in 200 components = -0.000627407 Jy ! Clean residual min=-0.005077 max=0.004751 Jy/beam ! Clean residual mean=-0.000549 rms=0.000940 Jy/beam ! Combined flux in latest and established models = 1.41137 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 70 components and 1.41137 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.122391Jy sigma=0.804706 ! Fit after self-cal, rms=0.122571Jy sigma=0.803922 ! Inverting map ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000325307 Jy ! Component: 100 - total flux cleaned = 0.000323036 Jy ! Component: 150 - total flux cleaned = 0.000319066 Jy ! Component: 200 - total flux cleaned = 0.000183191 Jy ! Total flux subtracted in 200 components = 0.000183191 Jy ! Clean residual min=-0.005018 max=0.004749 Jy/beam ! Clean residual mean=-0.000552 rms=0.000925 Jy/beam ! Combined flux in latest and established models = 1.41156 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 70 components and 1.41156 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.121861Jy sigma=0.799853 ! Fit after self-cal, rms=0.122032Jy sigma=0.799251 ! Inverting map ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.122032Jy sigma=0.799251 ! Fit after self-cal, rms=0.110711Jy sigma=0.797893 print "============== Clearing model and starting over ==========" ! ============== Clearing model and starting over ========== clrmod true ! clrmod: Cleared the established and tentative 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 ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec ! Estimated beam: bmin=0.6439 mas, bmaj=0.9155 mas, bpa=-9.479 degrees ! Estimated noise=1.19815 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.871993 Jy ! Component: 100 - total flux cleaned = 1.13323 Jy ! Component: 150 - total flux cleaned = 1.25646 Jy ! Component: 200 - total flux cleaned = 1.3237 Jy ! Total flux subtracted in 200 components = 1.3237 Jy ! Clean residual min=-0.016865 max=0.034579 Jy/beam ! Clean residual mean=0.000020 rms=0.003148 Jy/beam ! Combined flux in latest and established models = 1.3237 Jy uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! 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 1.3237 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec ! Estimated beam: bmin=0.6952 mas, bmaj=1.133 mas, bpa=-1.817 degrees ! Estimated noise=0.9051 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=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0411789 Jy ! Component: 100 - total flux cleaned = 0.0624557 Jy ! Component: 150 - total flux cleaned = 0.0696926 Jy ! Component: 200 - total flux cleaned = 0.0715919 Jy ! Total flux subtracted in 200 components = 0.0715919 Jy ! Clean residual min=-0.009650 max=0.009629 Jy/beam ! Clean residual mean=-0.000320 rms=0.001636 Jy/beam ! Combined flux in latest and established models = 1.39529 Jy ! Adding 16 model components to the UV plane model. ! The established model now contains 20 components and 1.39529 Jy ! Inverting map ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec ! Estimated beam: bmin=2.446 mas, bmaj=3.009 mas, bpa=89.64 degrees ! Estimated noise=1.23263 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0103929 Jy ! Component: 100 - total flux cleaned = 0.0133982 Jy ! Component: 150 - total flux cleaned = 0.0143913 Jy ! Component: 200 - total flux cleaned = 0.0149917 Jy ! Total flux subtracted in 200 components = 0.0149917 Jy ! Clean residual min=-0.005453 max=0.004964 Jy/beam ! Clean residual mean=-0.001224 rms=0.001052 Jy/beam ! Combined flux in latest and established models = 1.41028 Jy flux_cutoff = imstat(rms) * dynam 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=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000339874 Jy ! Component: 100 - total flux cleaned = 0.000490639 Jy ! Component: 150 - total flux cleaned = 0.000558107 Jy ! Component: 200 - total flux cleaned = 0.000622626 Jy ! Total flux subtracted in 200 components = 0.000622626 Jy ! Clean residual min=-0.005328 max=0.004945 Jy/beam ! Clean residual mean=-0.001243 rms=0.001034 Jy/beam ! Combined flux in latest and established models = 1.41091 Jy ! Adding 31 model components to the UV plane model. ! The established model now contains 48 components and 1.41091 Jy ! Inverting map ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec ! Estimated beam: bmin=0.6952 mas, bmaj=1.133 mas, bpa=-1.817 degrees ! Estimated noise=0.9051 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.83235e-05 Jy ! Component: 100 - total flux cleaned = 9.72005e-06 Jy ! Component: 150 - total flux cleaned = 0.000346068 Jy ! Component: 200 - total flux cleaned = 0.000347428 Jy ! Total flux subtracted in 200 components = 0.000347428 Jy ! Clean residual min=-0.009045 max=0.008530 Jy/beam ! Clean residual mean=-0.000509 rms=0.001445 Jy/beam ! Combined flux in latest and established models = 1.41125 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 51 components and 1.41125 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.134614Jy sigma=1.638763 ! Fit after self-cal, rms=0.112824Jy sigma=1.516557 wmodel J0205+3212_X_map.mod ! Writing 51 model components to file: J0205+3212_X_map.mod wobs J0205+3212_X_uvs.fits ! Writing UV FITS file: J0205+3212_X_uvs.fits wwins J0205+3212_X_map.win ! wwins: Wrote 3 windows to J0205+3212_X_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00115344 Jy ! Component: 100 - total flux cleaned = -0.00154214 Jy ! Component: 150 - total flux cleaned = -0.00203229 Jy ! Component: 200 - total flux cleaned = -0.00250439 Jy ! Component: 250 - total flux cleaned = -0.00307475 Jy ! Component: 300 - total flux cleaned = -0.00373781 Jy ! Component: 350 - total flux cleaned = -0.00449052 Jy ! Component: 400 - total flux cleaned = -0.00522497 Jy ! Component: 450 - total flux cleaned = -0.00594073 Jy ! Component: 500 - total flux cleaned = -0.00694248 Jy ! Component: 550 - total flux cleaned = -0.00782699 Jy ! Component: 600 - total flux cleaned = -0.00888884 Jy ! Component: 650 - total flux cleaned = -0.00964755 Jy ! Component: 700 - total flux cleaned = -0.0104898 Jy ! Component: 750 - total flux cleaned = -0.0113194 Jy ! Component: 800 - total flux cleaned = -0.0119549 Jy ! Component: 850 - total flux cleaned = -0.0125819 Jy ! Component: 900 - total flux cleaned = -0.0132888 Jy ! Component: 950 - total flux cleaned = -0.0139872 Jy ! Component: 1000 - total flux cleaned = -0.0146763 Jy ! Component: 1050 - total flux cleaned = -0.0152721 Jy ! Component: 1100 - total flux cleaned = -0.0158611 Jy ! Component: 1150 - total flux cleaned = -0.0165271 Jy ! Component: 1200 - total flux cleaned = -0.0171021 Jy ! Component: 1250 - total flux cleaned = -0.0175902 Jy ! Component: 1300 - total flux cleaned = -0.0181536 Jy ! Component: 1350 - total flux cleaned = -0.0187114 Jy ! Component: 1400 - total flux cleaned = -0.0191847 Jy ! Component: 1450 - total flux cleaned = -0.0197312 Jy ! Component: 1500 - total flux cleaned = -0.0201172 Jy ! Component: 1550 - total flux cleaned = -0.0207294 Jy ! Component: 1600 - total flux cleaned = -0.0211835 Jy ! Component: 1650 - total flux cleaned = -0.0216336 Jy ! Component: 1700 - total flux cleaned = -0.0220052 Jy ! Component: 1750 - total flux cleaned = -0.022448 Jy ! Component: 1800 - total flux cleaned = -0.0228134 Jy ! Component: 1850 - total flux cleaned = -0.0233205 Jy ! Component: 1900 - total flux cleaned = -0.0234646 Jy ! Component: 1950 - total flux cleaned = -0.0239643 Jy ! Component: 2000 - total flux cleaned = -0.0243184 Jy ! Component: 2050 - total flux cleaned = -0.0246693 Jy ! Component: 2100 - total flux cleaned = -0.0249477 Jy ! Component: 2150 - total flux cleaned = -0.0252933 Jy ! Component: 2200 - total flux cleaned = -0.0255674 Jy ! Component: 2250 - total flux cleaned = -0.0258394 Jy ! Component: 2300 - total flux cleaned = -0.0262442 Jy ! Component: 2350 - total flux cleaned = -0.0265119 Jy ! Component: 2400 - total flux cleaned = -0.0267112 Jy ! Component: 2450 - total flux cleaned = -0.0269754 Jy ! Component: 2500 - total flux cleaned = -0.0272373 Jy ! Component: 2550 - total flux cleaned = -0.0274974 Jy ! Component: 2600 - total flux cleaned = -0.0278199 Jy ! Component: 2650 - total flux cleaned = -0.0280118 Jy ! Component: 2700 - total flux cleaned = -0.0282659 Jy ! Component: 2750 - total flux cleaned = -0.0284556 Jy ! Component: 2800 - total flux cleaned = -0.0285812 Jy ! Component: 2850 - total flux cleaned = -0.0289552 Jy ! Component: 2900 - total flux cleaned = -0.029079 Jy ! Component: 2950 - total flux cleaned = -0.0293249 Jy ! Component: 3000 - total flux cleaned = -0.0295076 Jy ! Component: 3050 - total flux cleaned = -0.0297504 Jy ! Component: 3100 - total flux cleaned = -0.0300518 Jy ! Component: 3150 - total flux cleaned = -0.0301112 Jy ! Component: 3200 - total flux cleaned = -0.0302306 Jy ! Component: 3250 - total flux cleaned = -0.0304674 Jy ! Component: 3300 - total flux cleaned = -0.0305851 Jy ! Component: 3350 - total flux cleaned = -0.0308767 Jy ! Component: 3400 - total flux cleaned = -0.030993 Jy ! Component: 3450 - total flux cleaned = -0.0311655 Jy ! Component: 3500 - total flux cleaned = -0.0313373 Jy ! Component: 3550 - total flux cleaned = -0.0314509 Jy ! Component: 3600 - total flux cleaned = -0.0316202 Jy ! Component: 3650 - total flux cleaned = -0.0316763 Jy ! Component: 3700 - total flux cleaned = -0.0318993 Jy ! Component: 3750 - total flux cleaned = -0.0319545 Jy ! Component: 3800 - total flux cleaned = -0.0321751 Jy ! Component: 3850 - total flux cleaned = -0.032175 Jy ! Component: 3900 - total flux cleaned = -0.0322842 Jy ! Component: 3950 - total flux cleaned = -0.0325006 Jy ! Component: 4000 - total flux cleaned = -0.0325544 Jy ! Component: 4050 - total flux cleaned = -0.0326616 Jy ! Total flux subtracted in 4096 components = -0.0327682 Jy ! Clean residual min=-0.003579 max=0.002704 Jy/beam ! Clean residual mean=-0.000116 rms=0.000823 Jy/beam ! Combined flux in latest and established models = 1.37849 Jy keep ! Adding 313 model components to the UV plane model. ! The established model now contains 358 components and 1.37849 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv124_uvs/J0205+3212_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6952 x 1.133 at -1.817 degrees (North through East) ! Clean map min=-0.0068461 max=1.145 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv124_uvs/J0205+3212_X_map.fits wmodel /scr/pima/rv124_uvs/J0205+3212_X_map.mod ! Writing 358 model components to file: /scr/pima/rv124_uvs/J0205+3212_X_map.mod wobs /scr/pima/rv124_uvs/J0205+3212_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv124_uvs/J0205+3212_X_uvs.fits wwins /scr/pima/rv124_uvs/J0205+3212_X_map.win ! wwins: Wrote 4 windows to /scr/pima/rv124_uvs/J0205+3212_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 1.14499 invert ! Inverting map ! Your choice of large map pixels excluded 4.58% of the data. ! The x-axis pixel size should ideally be below 0.1755 milli-arcsec ! The y-axis pixel size should ideally be below 0.1633 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000821856 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.215335 0.215335 0.43067 0.861339 1.72268 3.44536 6.89071 13.7814 27.5629 55.1257 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0024 print "peak= ", int(1000*peak_flux)/1000 ! peak= 1.144 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 1393.18 quit ! Quitting program ! Log file /scr/pima/rv124_uvs/J0205+3212_X_dfm.log closed on Mon Dec 24 00:16:26 2018