! Started logfile: /scr/pima/rv123_uvs/J0533+4822_X_dfm.log on Sun Dec 23 00:40:33 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/rv123_uvs/J0533+4822_X_uva.fits ! Reading UV FITS file: /scr/pima/rv123_uvs/J0533+4822_X_uva.fits ! AN table 1: 22 integrations on 91 of 91 possible baselines. ! AN table 2: 28 integrations on 45 of 45 possible baselines. ! AN table 3: 8 integrations on 28 of 28 possible baselines. ! AN table 4: 5 integrations on 55 of 55 possible baselines. ! AN table 5: 42 integrations on 66 of 66 possible baselines. ! AN table 6: 3 integrations on 10 of 10 possible baselines. ! Apparent sampling: 0.478744 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0533+4822 ! ! 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 89 lines of history. ! ! Reading 12568 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 J0533+4822_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 22 telescope corrections were flagged in sub-array 1. ! A total of 174 telescope corrections were flagged in sub-array 2. ! A total of 8 telescope corrections were flagged in sub-array 3. ! A total of 17 telescope corrections were flagged in sub-array 4. ! A total of 377 telescope corrections were flagged in sub-array 5. ! A total of 5 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 22 telescope corrections were flagged in sub-array 1. ! A total of 174 telescope corrections were flagged in sub-array 2. ! A total of 8 telescope corrections were flagged in sub-array 3. ! A total of 17 telescope corrections were flagged in sub-array 4. ! A total of 377 telescope corrections were flagged in sub-array 5. ! A total of 5 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 40 telescope corrections were flagged in sub-array 1. ! A total of 178 telescope corrections were flagged in sub-array 2. ! A total of 12 telescope corrections were flagged in sub-array 3. ! A total of 19 telescope corrections were flagged in sub-array 4. ! A total of 391 telescope corrections were flagged in sub-array 5. ! A total of 5 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 40 telescope corrections were flagged in sub-array 1. ! A total of 178 telescope corrections were flagged in sub-array 2. ! A total of 12 telescope corrections were flagged in sub-array 3. ! A total of 19 telescope corrections were flagged in sub-array 4. ! A total of 391 telescope corrections were flagged in sub-array 5. ! A total of 5 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.754986Jy sigma=20.092409 ! Fit after self-cal, rms=0.528648Jy sigma=5.714432 ! 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 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! Estimated beam: bmin=0.5301 mas, bmaj=0.7365 mas, bpa=-39.09 degrees ! Estimated noise=0.92006 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 = 1.04316 Jy ! Component: 100 - total flux cleaned = 1.29753 Jy ! Total flux subtracted in 100 components = 1.29753 Jy ! Clean residual min=-0.033440 max=0.106287 Jy/beam ! Clean residual mean=-0.000152 rms=0.007113 Jy/beam ! Combined flux in latest and established models = 1.29753 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 1.29753 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.352291Jy sigma=3.866875 ! Fit after self-cal, rms=0.352228Jy sigma=3.866223 ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.118422 Jy ! Component: 100 - total flux cleaned = 0.18606 Jy ! Total flux subtracted in 100 components = 0.18606 Jy ! Clean residual min=-0.040334 max=0.043084 Jy/beam ! Clean residual mean=-0.000156 rms=0.006135 Jy/beam ! Combined flux in latest and established models = 1.48359 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 15 components and 1.48359 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.302443Jy sigma=3.369596 ! Fit after self-cal, rms=0.302345Jy sigma=3.368805 ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! Added new window around map position (-1.4, -0.6). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0438181 Jy ! Component: 100 - total flux cleaned = 0.0603889 Jy ! Total flux subtracted in 100 components = 0.0603889 Jy ! Clean residual min=-0.039362 max=0.038024 Jy/beam ! Clean residual mean=-0.000157 rms=0.005922 Jy/beam ! Combined flux in latest and established models = 1.54398 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 20 components and 1.54398 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.295207Jy sigma=3.306585 ! Fit after self-cal, rms=0.295129Jy sigma=3.305713 ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 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 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! Estimated beam: bmin=0.5951 mas, bmaj=0.8853 mas, bpa=-40.21 degrees ! Estimated noise=0.63475 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 = -0.00789966 Jy ! Component: 100 - total flux cleaned = -0.00494107 Jy ! Component: 150 - total flux cleaned = -0.00189854 Jy ! Component: 200 - total flux cleaned = -0.00187155 Jy ! Total flux subtracted in 200 components = -0.00187155 Jy ! Clean residual min=-0.042299 max=0.033965 Jy/beam ! Clean residual mean=-0.003924 rms=0.007558 Jy/beam ! Combined flux in latest and established models = 1.54211 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 30 components and 1.54211 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.289342Jy sigma=3.255382 ! Fit after self-cal, rms=0.289067Jy sigma=3.251125 ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec print "============== Finished natural weighting clean ==============" ! ============== Finished natural weighting clean ============== ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5951 x 0.8853 at -40.21 degrees (North through East) ! Clean map min=-0.040624 max=1.3795 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 0.98 HN 1.04 KP 1.05 ! LA 0.99 MC 1.01 MK 0.94 NL 1.05 ! NY 0.73 ON 0.98 OV 0.98 PT 0.85 ! SC 0.83 WZ 0.92 ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 0.85 HN 1.05 KP 1.03 ! LA 1.03 MK 0.96 NL 1.06 NY 0.67 ! OV 0.99 WN 1.65 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 KP 1.06 MC 0.87 MK 0.95 ! NY 0.74 OV 0.99 WN 1.55 YG 0.95 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 0.87 HN 1.05 LA 0.99 ! NL 1.02 NY 0.68 OV 0.99 PT 0.86 ! SC 0.85 WN 1.58 WZ 1.05 ! ! A total of 51 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 FD 0.87 HN 1.07 KP 1.06 ! LA 0.98 NL 1.04 NY 0.74 ON 1.15 ! OV 0.96 SC 0.89 WN 1.63 WZ 1.05 ! ! Telescope amplitude corrections in sub-array 6: ! LA 0.98 MK 0.99 OV 0.98 PT 0.87 ! WN 1.60 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 0.95 HN 1.04 KP 1.06 ! LA 1.00 MC 1.08 MK 0.94 NL 1.04 ! NY 0.85 ON 0.93 OV 0.97 PT 0.86 ! SC 0.82 WZ 0.86 ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 0.85 HN 1.03 KP 1.05 ! LA 1.03 MK 0.96 NL 1.08 NY 0.80 ! OV 0.99 WN 1.61 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 KP 1.06 MC 0.93 MK 0.95 ! NY 0.86 OV 0.99 WN 1.52 YG 0.86 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 0.87 HN 1.05 LA 1.00 ! NL 1.02 NY 0.81 OV 0.97 PT 0.86 ! SC 0.85 WN 1.54 WZ 1.01 ! ! A total of 51 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.98 FD 0.86 HN 1.05 KP 1.07 ! LA 0.96 NL 1.02 NY 0.86 ON 1.10 ! OV 0.96 SC 0.89 WN 1.59 WZ 1.05 ! ! Telescope amplitude corrections in sub-array 6: ! LA 1.00 MK 0.99 OV 0.98 PT 0.86 ! WN 1.55 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 0.92 HN 1.03 KP 1.06 ! LA 0.99 MC 1.61 MK 0.96 NL 1.05 ! NY 1.00* ON 1.27 OV 0.97 PT 0.85 ! SC 0.82 WZ 0.91 ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 0.84 HN 1.04 KP 1.04 ! LA 1.03 MK 0.95 NL 1.07 NY 1.00* ! OV 0.98 WN 1.50 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 KP 1.07 MC 1.38 MK 0.96 ! NY 1.00* OV 1.00 WN 1.37 YG 0.98 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 0.87 HN 1.04 LA 1.01 ! NL 1.02 NY 1.00* OV 0.98 PT 0.84 ! SC 0.82 WN 1.51 WZ 1.07 ! ! A total of 51 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.97 FD 0.85 HN 1.07 KP 1.07 ! LA 0.98 NL 1.03 NY 1.00* ON 1.61 ! OV 0.96 SC 0.88 WN 1.60 WZ 1.10 ! ! Telescope amplitude corrections in sub-array 6: ! LA 0.98 MK 0.99 OV 0.97 PT 0.86 ! WN 1.47 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 0.94 HN 1.04 KP 1.06 ! LA 0.98 MC 1.55 MK 0.97 NL 1.06 ! NY 1.00* ON 1.23 OV 0.97 PT 0.85 ! SC 0.82 WZ 0.94 ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 0.86 HN 1.04 KP 1.05 ! LA 1.04 MK 0.96 NL 1.05 NY 1.00* ! OV 0.99 WN 1.44 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 KP 1.06 MC 1.34 MK 0.96 ! NY 1.00* OV 1.01 WN 1.30 YG 1.10 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 FD 0.89 HN 1.03 LA 0.99 ! NL 1.02 NY 1.00* OV 0.96 PT 0.85 ! SC 0.86 WN 1.38 WZ 1.10 ! ! A total of 51 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 FD 0.84 HN 1.08 KP 1.08 ! LA 0.97 NL 1.03 NY 1.00* ON 1.57 ! OV 0.97 SC 0.88 WN 1.48 WZ 1.11 ! ! Telescope amplitude corrections in sub-array 6: ! LA 0.98 MK 0.99 OV 0.95 PT 0.87 ! WN 1.39 ! ! ! Fit before self-cal, rms=0.289067Jy sigma=3.251125 ! Fit after self-cal, rms=0.115677Jy sigma=1.169107 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! Estimated beam: bmin=0.5983 mas, bmaj=0.8794 mas, bpa=-40.14 degrees ! Estimated noise=0.639031 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 = -0.00530801 Jy ! Component: 100 - total flux cleaned = -0.0102896 Jy ! Component: 150 - total flux cleaned = -0.0132861 Jy ! Component: 200 - total flux cleaned = -0.0152133 Jy ! Total flux subtracted in 200 components = -0.0152133 Jy ! Clean residual min=-0.007734 max=0.008920 Jy/beam ! Clean residual mean=-0.000523 rms=0.001469 Jy/beam ! Combined flux in latest and established models = 1.52689 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 34 components and 1.52689 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.109835Jy sigma=1.079923 ! Fit after self-cal, rms=0.109622Jy sigma=1.076276 ! Inverting map ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! Added new window around map position (0.8, 2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00693448 Jy ! Component: 100 - total flux cleaned = 0.00826428 Jy ! Component: 150 - total flux cleaned = 0.00849112 Jy ! Component: 200 - total flux cleaned = 0.00868627 Jy ! Total flux subtracted in 200 components = 0.00868627 Jy ! Clean residual min=-0.007353 max=0.007422 Jy/beam ! Clean residual mean=-0.000547 rms=0.001381 Jy/beam ! Combined flux in latest and established models = 1.53558 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 44 components and 1.53558 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.108739Jy sigma=1.058002 ! Fit after self-cal, rms=0.108652Jy sigma=1.057265 ! Inverting map ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! Added new window around map position (-12.2, -7.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00532103 Jy ! Component: 100 - total flux cleaned = 0.00655129 Jy ! Component: 150 - total flux cleaned = 0.00717853 Jy ! Component: 200 - total flux cleaned = 0.00774992 Jy ! Total flux subtracted in 200 components = 0.00774992 Jy ! Clean residual min=-0.006886 max=0.005926 Jy/beam ! Clean residual mean=-0.000570 rms=0.001334 Jy/beam ! Combined flux in latest and established models = 1.54333 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 52 components and 1.54333 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.108196Jy sigma=1.048358 ! Fit after self-cal, rms=0.108166Jy sigma=1.048004 ! Inverting map ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 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=0.108166Jy sigma=1.048004 ! Fit after self-cal, rms=0.094942Jy sigma=0.913034 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! Estimated beam: bmin=0.5998 mas, bmaj=0.8839 mas, bpa=-40.21 degrees ! Estimated noise=0.638952 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00289772 Jy ! Component: 100 - total flux cleaned = -0.00292528 Jy ! Component: 150 - total flux cleaned = -0.00205206 Jy ! Component: 200 - total flux cleaned = -0.00175424 Jy ! Total flux subtracted in 200 components = -0.00175424 Jy ! Clean residual min=-0.004193 max=0.003978 Jy/beam ! Clean residual mean=-0.000230 rms=0.000859 Jy/beam ! Combined flux in latest and established models = 1.54158 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 59 components and 1.54158 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.093993Jy sigma=0.899676 ! Fit after self-cal, rms=0.093958Jy sigma=0.899430 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 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 = 0.000452308 Jy ! Component: 100 - total flux cleaned = 0.000715468 Jy ! Component: 150 - total flux cleaned = 0.000830816 Jy ! Component: 200 - total flux cleaned = 0.000943113 Jy ! Total flux subtracted in 200 components = 0.000943113 Jy ! Clean residual min=-0.004112 max=0.003589 Jy/beam ! Clean residual mean=-0.000233 rms=0.000833 Jy/beam ! Combined flux in latest and established models = 1.54252 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 59 components and 1.54252 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.093638Jy sigma=0.894962 ! Fit after self-cal, rms=0.093620Jy sigma=0.894882 ! Inverting map ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 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=0.093620Jy sigma=0.894882 ! Fit after self-cal, rms=0.092145Jy sigma=0.885833 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! Estimated beam: bmin=0.6008 mas, bmaj=0.8844 mas, bpa=-40.27 degrees ! Estimated noise=0.638549 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00323348 Jy ! Component: 100 - total flux cleaned = -0.00250963 Jy ! Component: 150 - total flux cleaned = -0.00226671 Jy ! Component: 200 - total flux cleaned = -0.00204083 Jy ! Total flux subtracted in 200 components = -0.00204083 Jy ! Clean residual min=-0.003734 max=0.003138 Jy/beam ! Clean residual mean=-0.000181 rms=0.000738 Jy/beam ! Combined flux in latest and established models = 1.54048 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 63 components and 1.54048 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.091673Jy sigma=0.880050 ! Fit after self-cal, rms=0.091661Jy sigma=0.879978 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 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 = 0.000447544 Jy ! Component: 100 - total flux cleaned = 0.000548646 Jy ! Component: 150 - total flux cleaned = 0.000825541 Jy ! Component: 200 - total flux cleaned = 0.000736658 Jy ! Total flux subtracted in 200 components = 0.000736658 Jy ! Clean residual min=-0.003624 max=0.002924 Jy/beam ! Clean residual mean=-0.000183 rms=0.000721 Jy/beam ! Combined flux in latest and established models = 1.54121 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 68 components and 1.54122 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.091469Jy sigma=0.877429 ! Fit after self-cal, rms=0.091458Jy sigma=0.877385 ! Inverting map ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 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=0.091458Jy sigma=0.877385 ! Fit after self-cal, rms=0.091223Jy sigma=0.875764 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! Estimated beam: bmin=2.338 mas, bmaj=2.612 mas, bpa=7.118 degrees ! Estimated noise=1.05652 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000242553 Jy ! Component: 100 - total flux cleaned = -0.000339214 Jy ! Component: 150 - total flux cleaned = -0.000986648 Jy ! Component: 200 - total flux cleaned = -0.00149026 Jy ! Total flux subtracted in 200 components = -0.00149026 Jy ! Clean residual min=-0.004860 max=0.004442 Jy/beam ! Clean residual mean=-0.000549 rms=0.001216 Jy/beam ! Combined flux in latest and established models = 1.53972 Jy selfcal ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 85 components and 1.53972 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.091178Jy sigma=0.875037 ! Fit after self-cal, rms=0.091103Jy sigma=0.874370 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 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 = 0.000332994 Jy ! Component: 100 - total flux cleaned = 1.95788e-05 Jy ! Component: 150 - total flux cleaned = -0.000337599 Jy ! Component: 200 - total flux cleaned = -0.000425241 Jy ! Total flux subtracted in 200 components = -0.000425241 Jy ! Clean residual min=-0.004703 max=0.004208 Jy/beam ! Clean residual mean=-0.000544 rms=0.001209 Jy/beam ! Combined flux in latest and established models = 1.5393 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 97 components and 1.5393 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.091107Jy sigma=0.874553 ! Fit after self-cal, rms=0.091089Jy sigma=0.874427 ! Inverting map ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 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 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! Estimated beam: bmin=0.6014 mas, bmaj=0.8849 mas, bpa=-40.34 degrees ! Estimated noise=0.638216 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6014 x 0.8849 at -40.34 degrees (North through East) ! Clean map min=-0.0092218 max=1.3676 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=0.091089Jy sigma=0.874427 ! Fit after self-cal, rms=0.081665Jy sigma=0.746332 ! Inverting map and beam ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! Estimated beam: bmin=0.6015 mas, bmaj=0.8858 mas, bpa=-40.38 degrees ! Estimated noise=0.637068 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00314953 Jy ! Component: 100 - total flux cleaned = -0.00323641 Jy ! Component: 150 - total flux cleaned = -0.00315854 Jy ! Component: 200 - total flux cleaned = -0.00330821 Jy ! Total flux subtracted in 200 components = -0.00330821 Jy ! Clean residual min=-0.003012 max=0.002807 Jy/beam ! Clean residual mean=-0.000117 rms=0.000608 Jy/beam ! Combined flux in latest and established models = 1.53599 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 99 components and 1.53599 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081392Jy sigma=0.743340 ! Fit after self-cal, rms=0.081387Jy sigma=0.743310 ! Inverting map ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 7.92546e-05 Jy ! Component: 100 - total flux cleaned = -5.55761e-05 Jy ! Component: 150 - total flux cleaned = -0.00011939 Jy ! Component: 200 - total flux cleaned = -0.000180762 Jy ! Total flux subtracted in 200 components = -0.000180762 Jy ! Clean residual min=-0.002941 max=0.002803 Jy/beam ! Clean residual mean=-0.000117 rms=0.000603 Jy/beam ! Combined flux in latest and established models = 1.53581 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 102 components and 1.53581 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081280Jy sigma=0.742029 ! Fit after self-cal, rms=0.081276Jy sigma=0.742009 ! Inverting map ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081276Jy sigma=0.742009 ! Fit after self-cal, rms=0.081143Jy sigma=0.741032 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 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! Estimated beam: bmin=0.5408 mas, bmaj=0.7494 mas, bpa=-40.68 degrees ! Estimated noise=0.9359 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.05455 Jy ! Component: 100 - total flux cleaned = 1.29091 Jy ! Component: 150 - total flux cleaned = 1.37998 Jy ! Component: 200 - total flux cleaned = 1.42677 Jy ! Total flux subtracted in 200 components = 1.42677 Jy ! Clean residual min=-0.008170 max=0.023748 Jy/beam ! Clean residual mean=-0.000014 rms=0.001388 Jy/beam ! Combined flux in latest and established models = 1.42677 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 1.42677 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! Estimated beam: bmin=0.6019 mas, bmaj=0.8862 mas, bpa=-40.44 degrees ! Estimated noise=0.636805 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 = 0.0365697 Jy ! Component: 100 - total flux cleaned = 0.0566464 Jy ! Component: 150 - total flux cleaned = 0.0701726 Jy ! Component: 200 - total flux cleaned = 0.079955 Jy ! Total flux subtracted in 200 components = 0.079955 Jy ! Clean residual min=-0.004764 max=0.006481 Jy/beam ! Clean residual mean=-0.000029 rms=0.000825 Jy/beam ! Combined flux in latest and established models = 1.50673 Jy ! Adding 23 model components to the UV plane model. ! The established model now contains 28 components and 1.50673 Jy ! Inverting map ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! Added new window around map position (0, 0.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0058321 Jy ! Component: 100 - total flux cleaned = 0.00923123 Jy ! Component: 150 - total flux cleaned = 0.0122645 Jy ! Component: 200 - total flux cleaned = 0.0150053 Jy ! Total flux subtracted in 200 components = 0.0150053 Jy ! Clean residual min=-0.003316 max=0.003545 Jy/beam ! Clean residual mean=-0.000064 rms=0.000652 Jy/beam ! Combined flux in latest and established models = 1.52173 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 42 components and 1.52173 Jy ! Inverting map ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! Added new window around map position (-2, -1.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00241693 Jy ! Component: 100 - total flux cleaned = 0.00398692 Jy ! Component: 150 - total flux cleaned = 0.00536055 Jy ! Component: 200 - total flux cleaned = 0.00627281 Jy ! Total flux subtracted in 200 components = 0.00627281 Jy ! Clean residual min=-0.003054 max=0.003151 Jy/beam ! Clean residual mean=-0.000079 rms=0.000602 Jy/beam ! Combined flux in latest and established models = 1.528 Jy ! Adding 29 model components to the UV plane model. ! The established model now contains 53 components and 1.528 Jy ! Inverting map ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! Added new window around map position (2.4, 3.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00230845 Jy ! Component: 100 - total flux cleaned = 0.00311373 Jy ! Component: 150 - total flux cleaned = 0.00400785 Jy ! Component: 200 - total flux cleaned = 0.00460435 Jy ! Total flux subtracted in 200 components = 0.00460435 Jy ! Clean residual min=-0.002997 max=0.002585 Jy/beam ! Clean residual mean=-0.000089 rms=0.000576 Jy/beam ! Combined flux in latest and established models = 1.53261 Jy ! Adding 31 model components to the UV plane model. ! The established model now contains 67 components and 1.53261 Jy ! Inverting map ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 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 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! Estimated beam: bmin=2.339 mas, bmaj=2.61 mas, bpa=7.113 degrees ! Estimated noise=1.05218 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00213977 Jy ! Component: 100 - total flux cleaned = 0.00276717 Jy ! Component: 150 - total flux cleaned = 0.0028704 Jy ! Component: 200 - total flux cleaned = 0.00291222 Jy ! Total flux subtracted in 200 components = 0.00291222 Jy ! Clean residual min=-0.004002 max=0.003415 Jy/beam ! Clean residual mean=-0.000359 rms=0.001026 Jy/beam ! Combined flux in latest and established models = 1.53552 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 = 3.40163e-05 Jy ! Component: 100 - total flux cleaned = 3.50066e-06 Jy ! Component: 150 - total flux cleaned = 5.08132e-06 Jy ! Component: 200 - total flux cleaned = -2.02875e-05 Jy ! Total flux subtracted in 200 components = -2.02875e-05 Jy ! Clean residual min=-0.003973 max=0.003322 Jy/beam ! Clean residual mean=-0.000359 rms=0.001020 Jy/beam ! Combined flux in latest and established models = 1.5355 Jy ! Adding 35 model components to the UV plane model. ! The established model now contains 98 components and 1.5355 Jy ! Inverting map ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! Estimated beam: bmin=0.6019 mas, bmaj=0.8862 mas, bpa=-40.44 degrees ! Estimated noise=0.636805 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000161272 Jy ! Component: 100 - total flux cleaned = -3.19223e-05 Jy ! Component: 150 - total flux cleaned = 0.000141595 Jy ! Component: 200 - total flux cleaned = 0.000193567 Jy ! Total flux subtracted in 200 components = 0.000193567 Jy ! Clean residual min=-0.002713 max=0.002427 Jy/beam ! Clean residual mean=-0.000097 rms=0.000557 Jy/beam ! Combined flux in latest and established models = 1.53569 Jy selfcal ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 108 components and 1.53569 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081519Jy sigma=0.741987 ! Fit after self-cal, rms=0.081407Jy sigma=0.740533 wmodel J0533+4822_X_map.mod ! Writing 108 model components to file: J0533+4822_X_map.mod wobs J0533+4822_X_uvs.fits ! Writing UV FITS file: J0533+4822_X_uvs.fits wwins J0533+4822_X_map.win ! wwins: Wrote 7 windows to J0533+4822_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 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00106685 Jy ! Component: 100 - total flux cleaned = -0.00145395 Jy ! Component: 150 - total flux cleaned = -0.00170262 Jy ! Component: 200 - total flux cleaned = -0.00202647 Jy ! Component: 250 - total flux cleaned = -0.00242339 Jy ! Component: 300 - total flux cleaned = -0.00273486 Jy ! Component: 350 - total flux cleaned = -0.00315663 Jy ! Component: 400 - total flux cleaned = -0.00349684 Jy ! Component: 450 - total flux cleaned = -0.00390699 Jy ! Component: 500 - total flux cleaned = -0.0042389 Jy ! Component: 550 - total flux cleaned = -0.0045308 Jy ! Component: 600 - total flux cleaned = -0.00489119 Jy ! Component: 650 - total flux cleaned = -0.00514083 Jy ! Component: 700 - total flux cleaned = -0.0053883 Jy ! Component: 750 - total flux cleaned = -0.00559903 Jy ! Component: 800 - total flux cleaned = -0.00577301 Jy ! Component: 850 - total flux cleaned = -0.00604894 Jy ! Component: 900 - total flux cleaned = -0.00628828 Jy ! Component: 950 - total flux cleaned = -0.00659353 Jy ! Component: 1000 - total flux cleaned = -0.00672847 Jy ! Component: 1050 - total flux cleaned = -0.00699613 Jy ! Component: 1100 - total flux cleaned = -0.00732812 Jy ! Component: 1150 - total flux cleaned = -0.00752579 Jy ! Component: 1200 - total flux cleaned = -0.00772229 Jy ! Component: 1250 - total flux cleaned = -0.00798245 Jy ! Component: 1300 - total flux cleaned = -0.00817627 Jy ! Component: 1350 - total flux cleaned = -0.00843329 Jy ! Component: 1400 - total flux cleaned = -0.0086567 Jy ! Component: 1450 - total flux cleaned = -0.00887849 Jy ! Component: 1500 - total flux cleaned = -0.00919351 Jy ! Component: 1550 - total flux cleaned = -0.00931874 Jy ! Component: 1600 - total flux cleaned = -0.00953662 Jy ! Component: 1650 - total flux cleaned = -0.00975366 Jy ! Component: 1700 - total flux cleaned = -0.0100305 Jy ! Component: 1750 - total flux cleaned = -0.0102141 Jy ! Component: 1800 - total flux cleaned = -0.0103663 Jy ! Component: 1850 - total flux cleaned = -0.0106087 Jy ! Component: 1900 - total flux cleaned = -0.0107291 Jy ! Component: 1950 - total flux cleaned = -0.0108192 Jy ! Component: 2000 - total flux cleaned = -0.0110576 Jy ! Component: 2050 - total flux cleaned = -0.0113246 Jy ! Component: 2100 - total flux cleaned = -0.0113836 Jy ! Component: 2150 - total flux cleaned = -0.0116186 Jy ! Component: 2200 - total flux cleaned = -0.0118232 Jy ! Component: 2250 - total flux cleaned = -0.0119104 Jy ! Component: 2300 - total flux cleaned = -0.0122286 Jy ! Component: 2350 - total flux cleaned = -0.0123148 Jy ! Component: 2400 - total flux cleaned = -0.0124868 Jy ! Component: 2450 - total flux cleaned = -0.0125725 Jy ! Component: 2500 - total flux cleaned = -0.0127714 Jy ! Component: 2550 - total flux cleaned = -0.0129695 Jy ! Component: 2600 - total flux cleaned = -0.0131667 Jy ! Component: 2650 - total flux cleaned = -0.0132791 Jy ! Component: 2700 - total flux cleaned = -0.0134468 Jy ! Component: 2750 - total flux cleaned = -0.013586 Jy ! Component: 2800 - total flux cleaned = -0.0137246 Jy ! Component: 2850 - total flux cleaned = -0.0138627 Jy ! Component: 2900 - total flux cleaned = -0.0140828 Jy ! Component: 2950 - total flux cleaned = -0.0142198 Jy ! Component: 3000 - total flux cleaned = -0.0143839 Jy ! Component: 3050 - total flux cleaned = -0.01452 Jy ! Component: 3100 - total flux cleaned = -0.0146013 Jy ! Component: 3150 - total flux cleaned = -0.0147364 Jy ! Component: 3200 - total flux cleaned = -0.0148711 Jy ! Component: 3250 - total flux cleaned = -0.0150857 Jy ! Component: 3300 - total flux cleaned = -0.0151391 Jy ! Component: 3350 - total flux cleaned = -0.015299 Jy ! Component: 3400 - total flux cleaned = -0.0154582 Jy ! Component: 3450 - total flux cleaned = -0.015564 Jy ! Component: 3500 - total flux cleaned = -0.0156693 Jy ! Component: 3550 - total flux cleaned = -0.0158531 Jy ! Component: 3600 - total flux cleaned = -0.0159838 Jy ! Component: 3650 - total flux cleaned = -0.0161664 Jy ! Component: 3700 - total flux cleaned = -0.0162443 Jy ! Component: 3750 - total flux cleaned = -0.0162702 Jy ! Component: 3800 - total flux cleaned = -0.016451 Jy ! Component: 3850 - total flux cleaned = -0.0166055 Jy ! Component: 3900 - total flux cleaned = -0.0166568 Jy ! Component: 3950 - total flux cleaned = -0.0168104 Jy ! Component: 4000 - total flux cleaned = -0.0169635 Jy ! Component: 4050 - total flux cleaned = -0.016989 Jy ! Total flux subtracted in 4096 components = -0.0171918 Jy ! Clean residual min=-0.001507 max=0.001429 Jy/beam ! Clean residual mean=-0.000049 rms=0.000415 Jy/beam ! Combined flux in latest and established models = 1.5185 Jy keep ! Adding 385 model components to the UV plane model. ! The established model now contains 493 components and 1.5185 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv123_uvs/J0533+4822_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6019 x 0.8862 at -40.44 degrees (North through East) ! Clean map min=-0.0056315 max=1.3707 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv123_uvs/J0533+4822_X_map.fits wmodel /scr/pima/rv123_uvs/J0533+4822_X_map.mod ! Writing 493 model components to file: /scr/pima/rv123_uvs/J0533+4822_X_map.mod wobs /scr/pima/rv123_uvs/J0533+4822_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv123_uvs/J0533+4822_X_uvs.fits wwins /scr/pima/rv123_uvs/J0533+4822_X_map.win ! wwins: Wrote 8 windows to /scr/pima/rv123_uvs/J0533+4822_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 1.37073 invert ! Inverting map ! Your choice of large map pixels excluded 2.97% of the data. ! The x-axis pixel size should ideally be below 0.1738 milli-arcsec ! The y-axis pixel size should ideally be below 0.1587 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000415215 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.0908743 0.0908743 0.181749 0.363497 0.726994 1.45399 2.90798 5.81595 11.6319 23.2638 46.5276 93.0553 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0012 print "peak= ", int(1000*peak_flux)/1000 ! peak= 1.37 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 3301.26 quit ! Quitting program ! Log file /scr/pima/rv123_uvs/J0533+4822_X_dfm.log closed on Sun Dec 23 00:40:38 2018