! Started logfile: /scr/pima/rv119_uvs/J2230+6946_X_dfm.log on Sun Dec 17 11:38:33 2017 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/rv119_uvs/J2230+6946_X_uva.fits ! Reading UV FITS file: /scr/pima/rv119_uvs/J2230+6946_X_uva.fits ! AN table 1: 3 integrations on 3 of 3 possible baselines. ! AN table 2: 6 integrations on 45 of 45 possible baselines. ! AN table 3: 4 integrations on 45 of 45 possible baselines. ! AN table 4: 7 integrations on 55 of 55 possible baselines. ! AN table 5: 3 integrations on 45 of 45 possible baselines. ! AN table 6: 6 integrations on 3 of 3 possible baselines. ! AN table 7: 10 integrations on 36 of 36 possible baselines. ! AN table 8: 19 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.434448 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J2230+6946 ! ! 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 3844 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 J2230+6946_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 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 3 telescope corrections were flagged in sub-array 1. ! A total of 34 telescope corrections were flagged in sub-array 2. ! A total of 4 telescope corrections were flagged in sub-array 3. ! A total of 43 telescope corrections were flagged in sub-array 4. ! A total of 10 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 48 telescope corrections were flagged in sub-array 7. ! A total of 126 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 2. ! A total of 3 telescope corrections were flagged in sub-array 1. ! A total of 34 telescope corrections were flagged in sub-array 2. ! A total of 4 telescope corrections were flagged in sub-array 3. ! A total of 43 telescope corrections were flagged in sub-array 4. ! A total of 10 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 48 telescope corrections were flagged in sub-array 7. ! A total of 126 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 3. ! A total of 3 telescope corrections were flagged in sub-array 1. ! A total of 34 telescope corrections were flagged in sub-array 2. ! A total of 4 telescope corrections were flagged in sub-array 3. ! A total of 43 telescope corrections were flagged in sub-array 4. ! A total of 10 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 48 telescope corrections were flagged in sub-array 7. ! A total of 126 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 4. ! A total of 3 telescope corrections were flagged in sub-array 1. ! A total of 34 telescope corrections were flagged in sub-array 2. ! A total of 4 telescope corrections were flagged in sub-array 3. ! A total of 43 telescope corrections were flagged in sub-array 4. ! A total of 10 telescope corrections were flagged in sub-array 5. ! A total of 6 telescope corrections were flagged in sub-array 6. ! A total of 48 telescope corrections were flagged in sub-array 7. ! A total of 126 telescope corrections were flagged in sub-array 8. ! ! Fit before self-cal, rms=1.205331Jy sigma=18.873601 ! Fit after self-cal, rms=0.447151Jy sigma=7.041992 ! 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 1.02% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 milli-arcsec ! Estimated beam: bmin=0.7163 mas, bmaj=0.8276 mas, bpa=-0.2015 degrees ! Estimated noise=0.97915 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 = 0.469059 Jy ! Component: 100 - total flux cleaned = 0.653827 Jy ! Total flux subtracted in 100 components = 0.653827 Jy ! Clean residual min=-0.015321 max=0.083088 Jy/beam ! Clean residual mean=0.000014 rms=0.003854 Jy/beam ! Combined flux in latest and established models = 0.653827 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 10 components and 0.653827 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.173593Jy sigma=2.653838 ! Fit after self-cal, rms=0.169250Jy sigma=2.610400 ! Inverting map ! Your choice of large map pixels excluded 1.02% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0937565 Jy ! Component: 100 - total flux cleaned = 0.14134 Jy ! Total flux subtracted in 100 components = 0.14134 Jy ! Clean residual min=-0.012627 max=0.023446 Jy/beam ! Clean residual mean=0.000001 rms=0.001972 Jy/beam ! Combined flux in latest and established models = 0.795167 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 15 components and 0.795167 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.097186Jy sigma=1.395726 ! Fit after self-cal, rms=0.094732Jy sigma=1.354061 ! Inverting map ! Your choice of large map pixels excluded 1.02% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0304775 Jy ! Component: 100 - total flux cleaned = 0.0451079 Jy ! Total flux subtracted in 100 components = 0.0451079 Jy ! Clean residual min=-0.017763 max=0.010783 Jy/beam ! Clean residual mean=-0.000003 rms=0.001562 Jy/beam ! Combined flux in latest and established models = 0.840275 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 16 components and 0.840275 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.084615Jy sigma=1.178595 ! Fit after self-cal, rms=0.083830Jy sigma=1.165034 ! Inverting map ! Your choice of large map pixels excluded 1.02% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 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 1.02% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 milli-arcsec ! Estimated beam: bmin=0.8556 mas, bmaj=0.9919 mas, bpa=-2.531 degrees ! Estimated noise=0.835564 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 = 0.00558238 Jy ! Component: 100 - total flux cleaned = 0.00559829 Jy ! Component: 150 - total flux cleaned = 0.00540126 Jy ! Component: 200 - total flux cleaned = 0.00539839 Jy ! Total flux subtracted in 200 components = 0.00539839 Jy ! Clean residual min=-0.012828 max=0.006511 Jy/beam ! Clean residual mean=-0.000003 rms=0.001175 Jy/beam ! Combined flux in latest and established models = 0.845673 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 19 components and 0.845673 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.082431Jy sigma=1.140816 ! Fit after self-cal, rms=0.082211Jy sigma=1.136979 ! Inverting map ! Your choice of large map pixels excluded 1.02% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8556 x 0.9919 at -2.531 degrees (North through East) ! Clean map min=-0.0048153 max=0.58229 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HN 0.00* ON 0.00* SC 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 0.97 HN 1.04 KP 1.00 ! LA 0.98 NL 1.01 OV 1.01 PT 0.99 ! SC 0.97 WZ 0.93 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 0.98 HN 1.02 KP 1.00 ! LA 0.99 NL 1.00 NY 1.02 OV 1.00 ! PT 1.02 SC 0.98 ! ! A total of 12 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 0.97 KP 1.01 LA 0.99 ! MK 0.97 NL 0.98 ON 1.02 OV 0.98 ! PT 0.98 SC 0.95 WZ 0.92 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 FD 1.06 KP 1.01 LA 0.99 ! MK 0.94 NL 1.02 NY 0.94 ON 1.07 ! OV 1.00 PT 1.01 ! ! A total of 12 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! NY 0.00* ON 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.01 FD 1.01 HN 0.99 KP 1.02 ! LA 1.00 MK 0.98 NL 1.00 OV 0.99 ! PT 0.99 ! ! A total of 12 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! BR 1.01 FD 0.97 HN 0.98 KP 0.97 ! LA 1.01 NL 1.00 NY 0.96 ON 1.08 ! OV 1.01 PT 1.02 ! ! ! Correcting IF 2. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HN 0.00* ON 0.00* SC 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 0.96 HN 1.02 KP 1.01 ! LA 1.01 NL 1.00 OV 1.00 PT 1.01 ! SC 0.96 WZ 1.06 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 0.97 HN 1.01 KP 1.00 ! LA 0.99 NL 1.00 NY 1.08 OV 1.01 ! PT 1.01 SC 0.98 ! ! A total of 12 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 FD 0.94 KP 0.98 LA 1.00 ! MK 0.95 NL 1.00 ON 1.06 OV 1.00 ! PT 1.00 SC 0.97 WZ 0.85 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 FD 1.05 KP 1.03 LA 0.98 ! MK 0.95 NL 1.02 NY 1.01 ON 0.99 ! OV 1.00 PT 0.98 ! ! A total of 12 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! NY 0.00* ON 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.01 FD 1.03 HN 1.01 KP 1.01 ! LA 0.99 MK 1.00 NL 1.02 OV 0.99 ! PT 0.99 ! ! A total of 12 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! BR 1.00 FD 0.98 HN 0.99 KP 0.97 ! LA 1.03 NL 1.02 NY 0.93 ON 0.99 ! OV 1.01 PT 1.01 ! ! ! Correcting IF 3. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HN 0.00* ON 0.00* SC 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 0.96 HN 1.02 KP 1.02 ! LA 1.05 NL 1.00 OV 0.99 PT 1.00 ! SC 0.96 WZ 1.09 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 0.99 HN 1.01 KP 1.00 ! LA 1.01 NL 0.99 NY 1.03 OV 1.00 ! PT 1.01 SC 0.98 ! ! A total of 12 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 0.93 KP 0.98 LA 0.99 ! MK 0.95 NL 0.99 ON 1.13 OV 1.00 ! PT 0.99 SC 0.98 WZ 0.83 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 FD 1.08 KP 1.03 LA 1.01 ! MK 0.96 NL 1.00 NY 0.96 ON 1.11 ! OV 1.01 PT 1.02 ! ! A total of 12 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! NY 0.00* ON 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.02 FD 1.00 HN 0.99 KP 1.02 ! LA 0.99 MK 1.01 NL 1.03 OV 0.99 ! PT 1.01 ! ! A total of 12 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! BR 1.02 FD 0.96 HN 0.99 KP 0.95 ! LA 0.98 NL 1.01 NY 0.97 ON 0.99 ! OV 1.03 PT 1.03 ! ! ! Correcting IF 4. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HN 0.00* ON 0.00* SC 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 0.97 HN 1.01 KP 1.03 ! LA 0.99 NL 0.98 OV 1.00 PT 1.01 ! SC 1.00 WZ 1.12 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 1.00 HN 1.00 KP 1.00 ! LA 0.99 NL 1.01 NY 1.34 OV 1.01 ! PT 1.02 SC 0.99 ! ! A total of 12 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.03 FD 0.95 KP 1.00 LA 1.02 ! MK 0.99 NL 0.97 ON 1.12 OV 1.00 ! PT 1.01 SC 0.95 WZ 0.80 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 FD 1.07 KP 1.03 LA 0.97 ! MK 0.95 NL 1.00 NY 0.97 ON 1.04 ! OV 1.02 PT 1.03 ! ! A total of 12 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! NY 0.00* ON 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.01 FD 1.00 HN 0.98 KP 1.02 ! LA 1.01 MK 1.02 NL 1.03 OV 0.99 ! PT 0.98 ! ! A total of 12 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! BR 1.02 FD 0.98 HN 0.98 KP 0.97 ! LA 1.02 NL 1.01 NY 0.97 ON 1.01 ! OV 1.02 PT 1.01 ! ! ! Fit before self-cal, rms=0.082211Jy sigma=1.136979 ! Fit after self-cal, rms=0.074141Jy sigma=1.031046 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 milli-arcsec ! Estimated beam: bmin=0.8626 mas, bmaj=0.9896 mas, bpa=-6.352 degrees ! Estimated noise=0.852825 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 = 0.000392524 Jy ! Component: 100 - total flux cleaned = 0.0007285 Jy ! Component: 150 - total flux cleaned = 0.000741313 Jy ! Component: 200 - total flux cleaned = 0.000871992 Jy ! Total flux subtracted in 200 components = 0.000871992 Jy ! Clean residual min=-0.009349 max=0.005079 Jy/beam ! Clean residual mean=-0.000007 rms=0.000992 Jy/beam ! Combined flux in latest and established models = 0.846545 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 22 components and 0.846545 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.073276Jy sigma=1.017193 ! Fit after self-cal, rms=0.073165Jy sigma=1.014404 ! Inverting map ! Your choice of large map pixels excluded 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 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=0.073165Jy sigma=1.014404 ! Fit after self-cal, rms=0.071493Jy sigma=0.985497 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 milli-arcsec ! Estimated beam: bmin=0.8628 mas, bmaj=0.9923 mas, bpa=-7.107 degrees ! Estimated noise=0.852629 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00177149 Jy ! Component: 100 - total flux cleaned = 0.00131429 Jy ! Component: 150 - total flux cleaned = 0.00106861 Jy ! Component: 200 - total flux cleaned = 0.000849324 Jy ! Total flux subtracted in 200 components = 0.000849324 Jy ! Clean residual min=-0.007666 max=0.004239 Jy/beam ! Clean residual mean=-0.000003 rms=0.000888 Jy/beam ! Combined flux in latest and established models = 0.847394 Jy selfcal ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 23 components and 0.847394 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.070738Jy sigma=0.974794 ! Fit after self-cal, rms=0.070611Jy sigma=0.972186 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 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 = 0.000203184 Jy ! Component: 100 - total flux cleaned = -0.000173372 Jy ! Component: 150 - total flux cleaned = -0.0003776 Jy ! Component: 200 - total flux cleaned = -0.00047056 Jy ! Total flux subtracted in 200 components = -0.00047056 Jy ! Clean residual min=-0.007176 max=0.003965 Jy/beam ! Clean residual mean=-0.000003 rms=0.000869 Jy/beam ! Combined flux in latest and established models = 0.846924 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 23 components and 0.846924 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.070013Jy sigma=0.963479 ! Fit after self-cal, rms=0.069904Jy sigma=0.961058 ! Inverting map ! Your choice of large map pixels excluded 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 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=0.069904Jy sigma=0.961058 ! Fit after self-cal, rms=0.069122Jy sigma=0.958834 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 milli-arcsec ! Estimated beam: bmin=0.8596 mas, bmaj=0.9915 mas, bpa=-7.397 degrees ! Estimated noise=0.851095 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00116291 Jy ! Component: 100 - total flux cleaned = 0.000795177 Jy ! Component: 150 - total flux cleaned = 0.000504292 Jy ! Component: 200 - total flux cleaned = 0.000419485 Jy ! Total flux subtracted in 200 components = 0.000419485 Jy ! Clean residual min=-0.006540 max=0.003794 Jy/beam ! Clean residual mean=-0.000002 rms=0.000846 Jy/beam ! Combined flux in latest and established models = 0.847343 Jy selfcal ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 23 components and 0.847343 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.068574Jy sigma=0.951025 ! Fit after self-cal, rms=0.068477Jy sigma=0.948720 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 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 = 1.55771e-05 Jy ! Component: 100 - total flux cleaned = -0.000186459 Jy ! Component: 150 - total flux cleaned = -0.000357929 Jy ! Component: 200 - total flux cleaned = -0.00035679 Jy ! Total flux subtracted in 200 components = -0.00035679 Jy ! Clean residual min=-0.006009 max=0.003658 Jy/beam ! Clean residual mean=-0.000002 rms=0.000831 Jy/beam ! Combined flux in latest and established models = 0.846987 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 23 components and 0.846987 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.068014Jy sigma=0.942064 ! Fit after self-cal, rms=0.067939Jy sigma=0.940060 ! Inverting map ! Your choice of large map pixels excluded 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 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=0.067939Jy sigma=0.940060 ! Fit after self-cal, rms=0.067670Jy sigma=0.939803 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 milli-arcsec ! Estimated beam: bmin=2.605 mas, bmaj=2.778 mas, bpa=89.58 degrees ! Estimated noise=1.14429 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00104516 Jy ! Component: 100 - total flux cleaned = -0.00104489 Jy ! Component: 150 - total flux cleaned = -0.00104531 Jy ! Component: 200 - total flux cleaned = -0.00104583 Jy ! Total flux subtracted in 200 components = -0.00104583 Jy ! Clean residual min=-0.003547 max=0.003269 Jy/beam ! Clean residual mean=-0.000003 rms=0.000929 Jy/beam ! Combined flux in latest and established models = 0.845941 Jy selfcal ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 24 components and 0.845941 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.067614Jy sigma=0.938701 ! Fit after self-cal, rms=0.067620Jy sigma=0.938548 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 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 = -6.30712e-05 Jy ! Component: 100 - total flux cleaned = -6.21535e-05 Jy ! Component: 150 - total flux cleaned = -6.13908e-05 Jy ! Component: 200 - total flux cleaned = -6.07645e-05 Jy ! Total flux subtracted in 200 components = -6.07645e-05 Jy ! Clean residual min=-0.003551 max=0.003269 Jy/beam ! Clean residual mean=-0.000003 rms=0.000929 Jy/beam ! Combined flux in latest and established models = 0.84588 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 27 components and 0.84588 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.067577Jy sigma=0.937743 ! Fit after self-cal, rms=0.067581Jy sigma=0.937648 ! Inverting map ! Your choice of large map pixels excluded 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 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 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 milli-arcsec ! Estimated beam: bmin=0.8585 mas, bmaj=0.9913 mas, bpa=-7.443 degrees ! Estimated noise=0.850621 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8585 x 0.9913 at -7.443 degrees (North through East) ! Clean map min=-0.003242 max=0.58001 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=0.067581Jy sigma=0.937648 ! Fit after self-cal, rms=0.064696Jy sigma=0.880194 ! Inverting map and beam ! Your choice of large map pixels excluded 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 milli-arcsec ! Estimated beam: bmin=0.8593 mas, bmaj=0.9916 mas, bpa=-7.587 degrees ! Estimated noise=0.850598 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00089174 Jy ! Component: 100 - total flux cleaned = 0.000684643 Jy ! Component: 150 - total flux cleaned = 0.000446208 Jy ! Component: 200 - total flux cleaned = 0.000444491 Jy ! Total flux subtracted in 200 components = 0.000444491 Jy ! Clean residual min=-0.005591 max=0.003488 Jy/beam ! Clean residual mean=-0.000002 rms=0.000815 Jy/beam ! Combined flux in latest and established models = 0.846324 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 27 components and 0.846324 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.064259Jy sigma=0.874068 ! Fit after self-cal, rms=0.064193Jy sigma=0.872135 ! Inverting map ! Your choice of large map pixels excluded 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 2.37328e-05 Jy ! Component: 100 - total flux cleaned = -0.000153639 Jy ! Component: 150 - total flux cleaned = -0.00029729 Jy ! Component: 200 - total flux cleaned = -0.000299341 Jy ! Total flux subtracted in 200 components = -0.000299341 Jy ! Clean residual min=-0.005098 max=0.003370 Jy/beam ! Clean residual mean=-0.000002 rms=0.000803 Jy/beam ! Combined flux in latest and established models = 0.846025 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 27 components and 0.846025 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.063821Jy sigma=0.866888 ! Fit after self-cal, rms=0.063772Jy sigma=0.865235 ! Inverting map ! Your choice of large map pixels excluded 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.063772Jy sigma=0.865235 ! Fit after self-cal, rms=0.063543Jy sigma=0.865062 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 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 milli-arcsec ! Estimated beam: bmin=0.7219 mas, bmaj=0.828 mas, bpa=-4.243 degrees ! Estimated noise=0.99064 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.476974 Jy ! Component: 100 - total flux cleaned = 0.665591 Jy ! Component: 150 - total flux cleaned = 0.748041 Jy ! Component: 200 - total flux cleaned = 0.791803 Jy ! Total flux subtracted in 200 components = 0.791803 Jy ! Clean residual min=-0.006267 max=0.021658 Jy/beam ! Clean residual mean=0.000003 rms=0.001446 Jy/beam ! Combined flux in latest and established models = 0.791803 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 17 model components to the UV plane model. ! The established model now contains 17 components and 0.791803 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 milli-arcsec ! Estimated beam: bmin=0.8586 mas, bmaj=0.9912 mas, bpa=-7.498 degrees ! Estimated noise=0.850141 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 = 0.0299537 Jy ! Component: 100 - total flux cleaned = 0.043943 Jy ! Component: 150 - total flux cleaned = 0.0507326 Jy ! Component: 200 - total flux cleaned = 0.0520459 Jy ! Total flux subtracted in 200 components = 0.0520459 Jy ! Clean residual min=-0.004031 max=0.004049 Jy/beam ! Clean residual mean=-0.000001 rms=0.000826 Jy/beam ! Combined flux in latest and established models = 0.843849 Jy ! Adding 16 model components to the UV plane model. ! The established model now contains 23 components and 0.843849 Jy ! Inverting map ! Your choice of large map pixels excluded 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 milli-arcsec ! Added new window around map position (-1.4, 1.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00143088 Jy ! Component: 100 - total flux cleaned = 0.00159075 Jy ! Component: 150 - total flux cleaned = 0.00185638 Jy ! Component: 200 - total flux cleaned = 0.00197882 Jy ! Total flux subtracted in 200 components = 0.00197882 Jy ! Clean residual min=-0.003910 max=0.003504 Jy/beam ! Clean residual mean=-0.000002 rms=0.000806 Jy/beam ! Combined flux in latest and established models = 0.845828 Jy ! Adding 17 model components to the UV plane model. ! The established model now contains 35 components and 0.845828 Jy ! Inverting map ! Your choice of large map pixels excluded 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 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 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 milli-arcsec ! Estimated beam: bmin=2.605 mas, bmaj=2.779 mas, bpa=89.52 degrees ! Estimated noise=1.14363 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0007228 Jy ! Component: 100 - total flux cleaned = 0.000627761 Jy ! Component: 150 - total flux cleaned = 0.000665433 Jy ! Component: 200 - total flux cleaned = 0.000695967 Jy ! Total flux subtracted in 200 components = 0.000695967 Jy ! Clean residual min=-0.003501 max=0.003215 Jy/beam ! Clean residual mean=-0.000004 rms=0.000919 Jy/beam ! Combined flux in latest and established models = 0.846524 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 = 8.46371e-05 Jy ! Component: 100 - total flux cleaned = 0.000160408 Jy ! Component: 150 - total flux cleaned = 0.000229732 Jy ! Component: 200 - total flux cleaned = 0.000250812 Jy ! Total flux subtracted in 200 components = 0.000250812 Jy ! Clean residual min=-0.003488 max=0.003208 Jy/beam ! Clean residual mean=-0.000004 rms=0.000918 Jy/beam ! Combined flux in latest and established models = 0.846775 Jy ! Adding 20 model components to the UV plane model. ! The established model now contains 51 components and 0.846775 Jy ! Inverting map ! Your choice of large map pixels excluded 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 milli-arcsec ! Estimated beam: bmin=0.8586 mas, bmaj=0.9912 mas, bpa=-7.498 degrees ! Estimated noise=0.850141 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000277471 Jy ! Component: 100 - total flux cleaned = 0.000180081 Jy ! Component: 150 - total flux cleaned = 0.000183392 Jy ! Component: 200 - total flux cleaned = 0.000184259 Jy ! Total flux subtracted in 200 components = 0.000184259 Jy ! Clean residual min=-0.003917 max=0.003343 Jy/beam ! Clean residual mean=-0.000002 rms=0.000792 Jy/beam ! Combined flux in latest and established models = 0.846959 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 55 components and 0.846959 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.062123Jy sigma=0.845857 ! Fit after self-cal, rms=0.061379Jy sigma=0.830280 wmodel J2230+6946_X_map.mod ! Writing 55 model components to file: J2230+6946_X_map.mod wobs J2230+6946_X_uvs.fits ! Writing UV FITS file: J2230+6946_X_uvs.fits wwins J2230+6946_X_map.win ! wwins: Wrote 2 windows to J2230+6946_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 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000393125 Jy ! Component: 100 - total flux cleaned = -0.00069446 Jy ! Component: 150 - total flux cleaned = -0.000870239 Jy ! Component: 200 - total flux cleaned = -0.000985472 Jy ! Component: 250 - total flux cleaned = -0.00109863 Jy ! Component: 300 - total flux cleaned = -0.00104334 Jy ! Component: 350 - total flux cleaned = -0.000989824 Jy ! Component: 400 - total flux cleaned = -0.00104412 Jy ! Component: 450 - total flux cleaned = -0.000991211 Jy ! Component: 500 - total flux cleaned = -0.000887157 Jy ! Component: 550 - total flux cleaned = -0.000732167 Jy ! Component: 600 - total flux cleaned = -0.000732292 Jy ! Component: 650 - total flux cleaned = -0.000579895 Jy ! Component: 700 - total flux cleaned = -0.000479461 Jy ! Component: 750 - total flux cleaned = -0.000429031 Jy ! Component: 800 - total flux cleaned = -0.000231402 Jy ! Component: 850 - total flux cleaned = -0.000231399 Jy ! Component: 900 - total flux cleaned = -0.000182996 Jy ! Component: 950 - total flux cleaned = -8.64363e-05 Jy ! Component: 1000 - total flux cleaned = -0.000182107 Jy ! Component: 1050 - total flux cleaned = -3.97702e-05 Jy ! Component: 1100 - total flux cleaned = 7.15251e-06 Jy ! Component: 1150 - total flux cleaned = -3.91032e-05 Jy ! Component: 1200 - total flux cleaned = 5.39195e-05 Jy ! Component: 1250 - total flux cleaned = 0.000100583 Jy ! Component: 1300 - total flux cleaned = 0.000146591 Jy ! Component: 1350 - total flux cleaned = 0.000420604 Jy ! Component: 1400 - total flux cleaned = 0.000511515 Jy ! Component: 1450 - total flux cleaned = 0.00073713 Jy ! Component: 1500 - total flux cleaned = 0.000647505 Jy ! Component: 1550 - total flux cleaned = 0.000736507 Jy ! Component: 1600 - total flux cleaned = 0.00078087 Jy ! Component: 1650 - total flux cleaned = 0.000957729 Jy ! Component: 1700 - total flux cleaned = 0.00104578 Jy ! Component: 1750 - total flux cleaned = 0.00113292 Jy ! Component: 1800 - total flux cleaned = 0.00130667 Jy ! Component: 1850 - total flux cleaned = 0.00134991 Jy ! Component: 1900 - total flux cleaned = 0.00139308 Jy ! Component: 1950 - total flux cleaned = 0.00143634 Jy ! Component: 2000 - total flux cleaned = 0.00169226 Jy ! Component: 2050 - total flux cleaned = 0.00169196 Jy ! Component: 2100 - total flux cleaned = 0.0016496 Jy ! Component: 2150 - total flux cleaned = 0.00169171 Jy ! Component: 2200 - total flux cleaned = 0.0019013 Jy ! Component: 2250 - total flux cleaned = 0.00190124 Jy ! Component: 2300 - total flux cleaned = 0.00181798 Jy ! Component: 2350 - total flux cleaned = 0.00190107 Jy ! Component: 2400 - total flux cleaned = 0.00194254 Jy ! Component: 2450 - total flux cleaned = 0.00186052 Jy ! Component: 2500 - total flux cleaned = 0.0019832 Jy ! Component: 2550 - total flux cleaned = 0.00194254 Jy ! Component: 2600 - total flux cleaned = 0.00214502 Jy ! Component: 2650 - total flux cleaned = 0.00202416 Jy ! Component: 2700 - total flux cleaned = 0.00202404 Jy ! Component: 2750 - total flux cleaned = 0.00182398 Jy ! Component: 2800 - total flux cleaned = 0.0018642 Jy ! Component: 2850 - total flux cleaned = 0.00198329 Jy ! Component: 2900 - total flux cleaned = 0.00198345 Jy ! Component: 2950 - total flux cleaned = 0.00194388 Jy ! Component: 3000 - total flux cleaned = 0.00190456 Jy ! Component: 3050 - total flux cleaned = 0.00206055 Jy ! Component: 3100 - total flux cleaned = 0.00202113 Jy ! Component: 3150 - total flux cleaned = 0.00190441 Jy ! Component: 3200 - total flux cleaned = 0.00174972 Jy ! Component: 3250 - total flux cleaned = 0.00171116 Jy ! Component: 3300 - total flux cleaned = 0.0016724 Jy ! Component: 3350 - total flux cleaned = 0.00178714 Jy ! Component: 3400 - total flux cleaned = 0.00174891 Jy ! Component: 3450 - total flux cleaned = 0.00186297 Jy ! Component: 3500 - total flux cleaned = 0.00178717 Jy ! Component: 3550 - total flux cleaned = 0.00174965 Jy ! Component: 3600 - total flux cleaned = 0.00182462 Jy ! Component: 3650 - total flux cleaned = 0.00174957 Jy ! Component: 3700 - total flux cleaned = 0.00193649 Jy ! Component: 3750 - total flux cleaned = 0.00186176 Jy ! Component: 3800 - total flux cleaned = 0.00193608 Jy ! Component: 3850 - total flux cleaned = 0.00201025 Jy ! Component: 3900 - total flux cleaned = 0.00186251 Jy ! Component: 3950 - total flux cleaned = 0.00193615 Jy ! Component: 4000 - total flux cleaned = 0.00189947 Jy ! Component: 4050 - total flux cleaned = 0.00197247 Jy ! Total flux subtracted in 4096 components = 0.00204563 Jy ! Clean residual min=-0.002638 max=0.002310 Jy/beam ! Clean residual mean=-0.000000 rms=0.000604 Jy/beam ! Combined flux in latest and established models = 0.849005 Jy keep ! Adding 374 model components to the UV plane model. ! The established model now contains 428 components and 0.849004 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv119_uvs/J2230+6946_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8586 x 0.9912 at -7.498 degrees (North through East) ! Clean map min=-0.0028534 max=0.57701 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv119_uvs/J2230+6946_X_map.fits wmodel /scr/pima/rv119_uvs/J2230+6946_X_map.mod ! Writing 428 model components to file: /scr/pima/rv119_uvs/J2230+6946_X_map.mod wobs /scr/pima/rv119_uvs/J2230+6946_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv119_uvs/J2230+6946_X_uvs.fits wwins /scr/pima/rv119_uvs/J2230+6946_X_map.win ! wwins: Wrote 3 windows to /scr/pima/rv119_uvs/J2230+6946_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.577015 invert ! Inverting map ! Your choice of large map pixels excluded 0.817% of the data. ! The x-axis pixel size should ideally be below 0.1718 milli-arcsec ! The y-axis pixel size should ideally be below 0.1731 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00060369 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.313869 0.313869 0.627738 1.25548 2.51095 5.0219 10.0438 20.0876 40.1752 80.3505 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0018 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.577 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 955.812 quit ! Quitting program ! Log file /scr/pima/rv119_uvs/J2230+6946_X_dfm.log closed on Sun Dec 17 11:38:38 2017