! Started logfile: /scr/pima/rv120_uvs/J2320+0513_X_dfm.log on Fri Dec 22 22:45:16 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/rv120_uvs/J2320+0513_X_uva.fits ! Reading UV FITS file: /scr/pima/rv120_uvs/J2320+0513_X_uva.fits ! AN table 1: 126 integrations on 10 of 10 possible baselines. ! AN table 2: 5 integrations on 15 of 15 possible baselines. ! AN table 3: 2 integrations on 6 of 6 possible baselines. ! AN table 4: 6 integrations on 3 of 3 possible baselines. ! AN table 5: 7 integrations on 36 of 36 possible baselines. ! AN table 6: 27 integrations on 45 of 45 possible baselines. ! AN table 7: 12 integrations on 3 of 3 possible baselines. ! AN table 8: 63 integrations on 3 of 3 possible baselines. ! Apparent sampling: 0.52666 visibilities/baseline/integration-bin. ! Found source: J2320+0513 ! ! 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 6440 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 J2320+0513_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 337 telescope corrections were flagged in sub-array 1. ! A total of 4 telescope corrections were flagged in sub-array 2. ! A total of 12 telescope corrections were flagged in sub-array 4. ! A total of 31 telescope corrections were flagged in sub-array 5. ! A total of 81 telescope corrections were flagged in sub-array 6. ! A total of 18 telescope corrections were flagged in sub-array 7. ! A total of 108 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 2. ! A total of 337 telescope corrections were flagged in sub-array 1. ! A total of 4 telescope corrections were flagged in sub-array 2. ! A total of 12 telescope corrections were flagged in sub-array 4. ! A total of 31 telescope corrections were flagged in sub-array 5. ! A total of 81 telescope corrections were flagged in sub-array 6. ! A total of 18 telescope corrections were flagged in sub-array 7. ! A total of 108 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 3. ! A total of 337 telescope corrections were flagged in sub-array 1. ! A total of 4 telescope corrections were flagged in sub-array 2. ! A total of 12 telescope corrections were flagged in sub-array 4. ! A total of 31 telescope corrections were flagged in sub-array 5. ! A total of 81 telescope corrections were flagged in sub-array 6. ! A total of 18 telescope corrections were flagged in sub-array 7. ! A total of 108 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 4. ! A total of 337 telescope corrections were flagged in sub-array 1. ! A total of 4 telescope corrections were flagged in sub-array 2. ! A total of 12 telescope corrections were flagged in sub-array 4. ! A total of 31 telescope corrections were flagged in sub-array 5. ! A total of 81 telescope corrections were flagged in sub-array 6. ! A total of 18 telescope corrections were flagged in sub-array 7. ! A total of 108 telescope corrections were flagged in sub-array 8. ! ! Fit before self-cal, rms=1.242415Jy sigma=17.299736 ! Fit after self-cal, rms=0.313635Jy sigma=4.163293 ! 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 6.72% of the data. ! The y-axis pixel size should ideally be below 0.1834 milli-arcsec ! Estimated beam: bmin=0.6979 mas, bmaj=1.082 mas, bpa=-14.62 degrees ! Estimated noise=0.981036 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 = 0.55412 Jy ! Component: 100 - total flux cleaned = 0.679172 Jy ! Total flux subtracted in 100 components = 0.679172 Jy ! Clean residual min=-0.013979 max=0.045684 Jy/beam ! Clean residual mean=-0.000023 rms=0.002952 Jy/beam ! Combined flux in latest and established models = 0.679172 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 9 components and 0.679172 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.141761Jy sigma=1.474674 ! Fit after self-cal, rms=0.141687Jy sigma=1.474086 ! Inverting map ! Your choice of large map pixels excluded 6.72% of the data. ! The y-axis pixel size should ideally be below 0.1834 milli-arcsec ! Added new window around map position (-0.6, 1). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.046661 Jy ! Component: 100 - total flux cleaned = 0.067573 Jy ! Total flux subtracted in 100 components = 0.067573 Jy ! Clean residual min=-0.012036 max=0.014006 Jy/beam ! Clean residual mean=-0.000000 rms=0.002045 Jy/beam ! Combined flux in latest and established models = 0.746745 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 15 components and 0.746745 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.126031Jy sigma=1.155128 ! Fit after self-cal, rms=0.125769Jy sigma=1.152552 ! Inverting map ! Your choice of large map pixels excluded 6.72% of the data. ! The y-axis pixel size should ideally be below 0.1834 milli-arcsec ! Added new window around map position (0.4, 3.6). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00826112 Jy ! Component: 100 - total flux cleaned = 0.00948261 Jy ! Total flux subtracted in 100 components = 0.00948261 Jy ! Clean residual min=-0.010433 max=0.011265 Jy/beam ! Clean residual mean=0.000001 rms=0.001928 Jy/beam ! Combined flux in latest and established models = 0.756227 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 21 components and 0.756227 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.123817Jy sigma=1.128750 ! Fit after self-cal, rms=0.123762Jy sigma=1.127568 ! Inverting map ! Your choice of large map pixels excluded 6.72% of the data. ! The y-axis pixel size should ideally be below 0.1834 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 6.72% of the data. ! The y-axis pixel size should ideally be below 0.1834 milli-arcsec ! Estimated beam: bmin=0.8377 mas, bmaj=1.13 mas, bpa=-23.65 degrees ! Estimated noise=0.755212 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 = 0.00178397 Jy ! Component: 100 - total flux cleaned = 0.00205962 Jy ! Component: 150 - total flux cleaned = 0.00205387 Jy ! Component: 200 - total flux cleaned = 0.00231486 Jy ! Total flux subtracted in 200 components = 0.00231486 Jy ! Clean residual min=-0.010350 max=0.009246 Jy/beam ! Clean residual mean=0.000002 rms=0.001762 Jy/beam ! Combined flux in latest and established models = 0.758542 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 29 components and 0.758542 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.121613Jy sigma=1.112744 ! Fit after self-cal, rms=0.121549Jy sigma=1.112389 ! Inverting map ! Your choice of large map pixels excluded 6.72% of the data. ! The y-axis pixel size should ideally be below 0.1834 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8377 x 1.13 at -23.65 degrees (North through East) ! Clean map min=-0.010085 max=0.69362 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 207 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 1.01 HN 1.14 NY 1.00 ON 0.96 ! SC 0.99 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.08 FD 1.01 KP 0.95 LA 1.01 ! PT 1.03 WZ 1.01 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.04 HN 0.99 NL 0.97 WZ 0.96 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! NY 0.00* SC 0.00* WZ 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 FD 0.99 HN 0.99 KP 1.03 ! LA 1.01 NL 0.99 OV 1.01 PT 0.99 ! SC 0.98 ! ! A total of 3 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.98 FD 0.99 HN 0.99 KK 1.03 ! KP 1.01 LA 0.99 MK 0.92 NL 1.02 ! OV 1.00 PT 0.99 ! ! A total of 18 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! HN 0.00* KK 0.00* SC 0.00* ! ! A total of 81 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! HH 0.00* ON 0.00* WZ 0.00* ! ! ! Correcting IF 2. ! A total of 207 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 1.05 HN 1.13 NY 1.02 ON 0.95 ! SC 1.01 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.11 FD 1.00 KP 0.96 LA 1.02 ! PT 1.01 WZ 0.99 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 HN 0.98 NL 0.95 WZ 0.97 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! NY 0.00* SC 0.00* WZ 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 FD 1.00 HN 0.99 KP 1.02 ! LA 1.02 NL 0.98 OV 1.01 PT 0.98 ! SC 0.97 ! ! A total of 3 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.99 FD 1.00 HN 0.98 KK 1.02 ! KP 1.00 LA 1.00 MK 0.95 NL 1.04 ! OV 1.01 PT 0.98 ! ! A total of 18 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! HN 0.00* KK 0.00* SC 0.00* ! ! A total of 81 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! HH 0.00* ON 0.00* WZ 0.00* ! ! ! Correcting IF 3. ! A total of 207 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 1.02 HN 1.15 NY 1.01 ON 0.99 ! SC 1.01 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.10 FD 1.01 KP 0.96 LA 1.00 ! PT 1.02 WZ 1.02 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.07 HN 1.00 NL 0.94 WZ 0.95 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! NY 0.00* SC 0.00* WZ 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.98 FD 0.99 HN 0.99 KP 1.02 ! LA 1.01 NL 1.00 OV 1.00 PT 0.98 ! SC 0.99 ! ! A total of 3 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.01 FD 1.01 HN 1.00 KK 1.01 ! KP 1.01 LA 0.99 MK 0.96 NL 1.03 ! OV 0.99 PT 0.99 ! ! A total of 18 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! HN 0.00* KK 0.00* SC 0.00* ! ! A total of 81 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! HH 0.00* ON 0.00* WZ 0.00* ! ! ! Correcting IF 4. ! A total of 207 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 1.03 HN 1.16 NY 0.97 ON 1.04 ! SC 1.01 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.13 FD 1.00 KP 0.98 LA 0.98 ! PT 0.98 WZ 1.07 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.09 HN 0.97 NL 0.96 WZ 0.94 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! NY 0.00* SC 0.00* WZ 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 FD 0.97 HN 0.99 KP 1.03 ! LA 0.99 NL 0.99 OV 1.00 PT 0.99 ! SC 0.98 ! ! A total of 3 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.01 FD 1.00 HN 0.99 KK 1.04 ! KP 1.01 LA 0.98 MK 0.98 NL 1.04 ! OV 1.00 PT 0.98 ! ! A total of 18 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! HN 0.00* KK 0.00* SC 0.00* ! ! A total of 81 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! HH 0.00* ON 0.00* WZ 0.00* ! ! ! Fit before self-cal, rms=0.121549Jy sigma=1.112389 ! Fit after self-cal, rms=0.090273Jy sigma=1.007091 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 milli-arcsec ! Estimated beam: bmin=0.8328 mas, bmaj=1.677 mas, bpa=-11.98 degrees ! Estimated noise=0.771247 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 = -0.00116638 Jy ! Component: 100 - total flux cleaned = -0.00146131 Jy ! Component: 150 - total flux cleaned = -0.00155062 Jy ! Component: 200 - total flux cleaned = -0.00163691 Jy ! Total flux subtracted in 200 components = -0.00163691 Jy ! Clean residual min=-0.008192 max=0.006324 Jy/beam ! Clean residual mean=0.000003 rms=0.001552 Jy/beam ! Combined flux in latest and established models = 0.756905 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 40 components and 0.756905 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.090000Jy sigma=1.003775 ! Fit after self-cal, rms=0.090050Jy sigma=1.003577 ! Inverting map ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 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=0.090050Jy sigma=1.003577 ! Fit after self-cal, rms=0.083478Jy sigma=0.883057 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 milli-arcsec ! Estimated beam: bmin=0.8344 mas, bmaj=1.676 mas, bpa=-11.98 degrees ! Estimated noise=0.773742 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00178559 Jy ! Component: 100 - total flux cleaned = -0.00186348 Jy ! Component: 150 - total flux cleaned = -0.00193328 Jy ! Component: 200 - total flux cleaned = -0.00199314 Jy ! Total flux subtracted in 200 components = -0.00199314 Jy ! Clean residual min=-0.003475 max=0.003706 Jy/beam ! Clean residual mean=0.000009 rms=0.000801 Jy/beam ! Combined flux in latest and established models = 0.754912 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 48 components and 0.754912 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.083205Jy sigma=0.879921 ! Fit after self-cal, rms=0.083215Jy sigma=0.879486 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 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 (-10.2, -46.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00246359 Jy ! Component: 100 - total flux cleaned = 0.00262302 Jy ! Component: 150 - total flux cleaned = 0.0027545 Jy ! Component: 200 - total flux cleaned = 0.00281105 Jy ! Total flux subtracted in 200 components = 0.00281105 Jy ! Clean residual min=-0.003340 max=0.003432 Jy/beam ! Clean residual mean=0.000005 rms=0.000777 Jy/beam ! Combined flux in latest and established models = 0.757723 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 54 components and 0.757723 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.082984Jy sigma=0.876704 ! Fit after self-cal, rms=0.082991Jy sigma=0.876453 ! Inverting map ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 milli-arcsec ! Added new window around map position (-29.2, -10.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00223336 Jy ! Component: 100 - total flux cleaned = 0.00257246 Jy ! Component: 150 - total flux cleaned = 0.00275468 Jy ! Component: 200 - total flux cleaned = 0.00275421 Jy ! Total flux subtracted in 200 components = 0.00275421 Jy ! Clean residual min=-0.003046 max=0.003102 Jy/beam ! Clean residual mean=0.000003 rms=0.000759 Jy/beam ! Combined flux in latest and established models = 0.760478 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 73 components and 0.760478 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.082823Jy sigma=0.873964 ! Fit after self-cal, rms=0.082820Jy sigma=0.873732 ! Inverting map ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 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=0.082820Jy sigma=0.873732 ! Fit after self-cal, rms=0.082102Jy sigma=0.845063 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 milli-arcsec ! Estimated beam: bmin=0.8339 mas, bmaj=1.679 mas, bpa=-12.01 degrees ! Estimated noise=0.773469 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000426953 Jy ! Component: 100 - total flux cleaned = -0.000612465 Jy ! Component: 150 - total flux cleaned = -0.000554539 Jy ! Component: 200 - total flux cleaned = -0.000556221 Jy ! Total flux subtracted in 200 components = -0.000556221 Jy ! Clean residual min=-0.002621 max=0.002625 Jy/beam ! Clean residual mean=0.000005 rms=0.000605 Jy/beam ! Combined flux in latest and established models = 0.759921 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 84 components and 0.759921 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081959Jy sigma=0.843896 ! Fit after self-cal, rms=0.081960Jy sigma=0.843773 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 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 = -9.37076e-05 Jy ! Component: 100 - total flux cleaned = -9.34479e-05 Jy ! Component: 150 - total flux cleaned = -5.00217e-05 Jy ! Component: 200 - total flux cleaned = -5.21784e-05 Jy ! Total flux subtracted in 200 components = -5.21784e-05 Jy ! Clean residual min=-0.002595 max=0.002596 Jy/beam ! Clean residual mean=0.000005 rms=0.000599 Jy/beam ! Combined flux in latest and established models = 0.759869 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 88 components and 0.759869 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081870Jy sigma=0.843244 ! Fit after self-cal, rms=0.081871Jy sigma=0.843195 ! Inverting map ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 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=0.081871Jy sigma=0.843195 ! Fit after self-cal, rms=0.081896Jy sigma=0.842978 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 milli-arcsec ! Estimated beam: bmin=2.523 mas, bmaj=3.771 mas, bpa=-12.55 degrees ! Estimated noise=0.918454 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000350267 Jy ! Component: 100 - total flux cleaned = 0.000448983 Jy ! Component: 150 - total flux cleaned = 0.00051545 Jy ! Component: 200 - total flux cleaned = 0.000535361 Jy ! Total flux subtracted in 200 components = 0.000535361 Jy ! Clean residual min=-0.002346 max=0.002547 Jy/beam ! Clean residual mean=0.000008 rms=0.000626 Jy/beam ! Combined flux in latest and established models = 0.760405 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 98 components and 0.760405 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081888Jy sigma=0.842831 ! Fit after self-cal, rms=0.081889Jy sigma=0.842807 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 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 = 6.63321e-05 Jy ! Component: 100 - total flux cleaned = 8.59974e-05 Jy ! Component: 150 - total flux cleaned = 0.000103226 Jy ! Component: 200 - total flux cleaned = 8.64538e-05 Jy ! Total flux subtracted in 200 components = 8.64538e-05 Jy ! Clean residual min=-0.002333 max=0.002533 Jy/beam ! Clean residual mean=0.000008 rms=0.000623 Jy/beam ! Combined flux in latest and established models = 0.760491 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 100 components and 0.760491 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081885Jy sigma=0.842714 ! Fit after self-cal, rms=0.081885Jy sigma=0.842701 ! Inverting map ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 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 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 milli-arcsec ! Estimated beam: bmin=0.8336 mas, bmaj=1.68 mas, bpa=-12.04 degrees ! Estimated noise=0.773181 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8336 x 1.68 at -12.04 degrees (North through East) ! Clean map min=-0.0022648 max=0.70004 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=0.081885Jy sigma=0.842701 ! Fit after self-cal, rms=0.074748Jy sigma=0.734576 ! Inverting map and beam ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 milli-arcsec ! Estimated beam: bmin=0.8333 mas, bmaj=1.681 mas, bpa=-12.04 degrees ! Estimated noise=0.772862 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000100486 Jy ! Component: 100 - total flux cleaned = -0.000238446 Jy ! Component: 150 - total flux cleaned = -0.000240794 Jy ! Component: 200 - total flux cleaned = -0.000243252 Jy ! Total flux subtracted in 200 components = -0.000243252 Jy ! Clean residual min=-0.002597 max=0.002500 Jy/beam ! Clean residual mean=0.000005 rms=0.000580 Jy/beam ! Combined flux in latest and established models = 0.760248 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 103 components and 0.760248 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.074659Jy sigma=0.733915 ! Fit after self-cal, rms=0.074662Jy sigma=0.733860 ! Inverting map ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -3.8748e-05 Jy ! Component: 100 - total flux cleaned = -3.92589e-05 Jy ! Component: 150 - total flux cleaned = -3.9233e-05 Jy ! Component: 200 - total flux cleaned = -4.00747e-05 Jy ! Total flux subtracted in 200 components = -4.00747e-05 Jy ! Clean residual min=-0.002570 max=0.002482 Jy/beam ! Clean residual mean=0.000004 rms=0.000577 Jy/beam ! Combined flux in latest and established models = 0.760208 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 106 components and 0.760208 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.074590Jy sigma=0.733461 ! Fit after self-cal, rms=0.074592Jy sigma=0.733425 ! Inverting map ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.074592Jy sigma=0.733425 ! Fit after self-cal, rms=0.074604Jy sigma=0.733328 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 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 milli-arcsec ! Estimated beam: bmin=0.6954 mas, bmaj=1.489 mas, bpa=-9.591 degrees ! Estimated noise=0.984387 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.551693 Jy ! Component: 100 - total flux cleaned = 0.676842 Jy ! Component: 150 - total flux cleaned = 0.719732 Jy ! Component: 200 - total flux cleaned = 0.738615 Jy ! Total flux subtracted in 200 components = 0.738615 Jy ! Clean residual min=-0.004186 max=0.008296 Jy/beam ! Clean residual mean=-0.000001 rms=0.000949 Jy/beam ! Combined flux in latest and established models = 0.738615 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 13 model components to the UV plane model. ! The established model now contains 13 components and 0.738615 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 milli-arcsec ! Estimated beam: bmin=0.833 mas, bmaj=1.682 mas, bpa=-12.06 degrees ! Estimated noise=0.77269 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 = 0.00934475 Jy ! Component: 100 - total flux cleaned = 0.0142272 Jy ! Component: 150 - total flux cleaned = 0.0163711 Jy ! Component: 200 - total flux cleaned = 0.0173399 Jy ! Total flux subtracted in 200 components = 0.0173399 Jy ! Clean residual min=-0.002998 max=0.003245 Jy/beam ! Clean residual mean=0.000008 rms=0.000646 Jy/beam ! Combined flux in latest and established models = 0.755955 Jy ! Adding 20 model components to the UV plane model. ! The established model now contains 29 components and 0.755955 Jy ! Inverting map ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 milli-arcsec ! Added new window around map position (-1.4, 5.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00206107 Jy ! Component: 100 - total flux cleaned = 0.0023563 Jy ! Component: 150 - total flux cleaned = 0.00262249 Jy ! Component: 200 - total flux cleaned = 0.00296876 Jy ! Total flux subtracted in 200 components = 0.00296876 Jy ! Clean residual min=-0.002586 max=0.002687 Jy/beam ! Clean residual mean=0.000006 rms=0.000613 Jy/beam ! Combined flux in latest and established models = 0.758924 Jy ! Adding 24 model components to the UV plane model. ! The established model now contains 42 components and 0.758924 Jy ! Inverting map ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 milli-arcsec ! Added new window around map position (6.8, -3). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000358208 Jy ! Component: 100 - total flux cleaned = 0.00052077 Jy ! Component: 150 - total flux cleaned = 0.000750512 Jy ! Component: 200 - total flux cleaned = 0.000960768 Jy ! Total flux subtracted in 200 components = 0.000960768 Jy ! Clean residual min=-0.002522 max=0.002524 Jy/beam ! Clean residual mean=0.000005 rms=0.000595 Jy/beam ! Combined flux in latest and established models = 0.759885 Jy ! Adding 25 model components to the UV plane model. ! The established model now contains 54 components and 0.759885 Jy ! Inverting map ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 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 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 milli-arcsec ! Estimated beam: bmin=2.523 mas, bmaj=3.772 mas, bpa=-12.56 degrees ! Estimated noise=0.918335 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00100755 Jy ! Component: 100 - total flux cleaned = 0.00100895 Jy ! Component: 150 - total flux cleaned = 0.00104243 Jy ! Component: 200 - total flux cleaned = 0.00107013 Jy ! Total flux subtracted in 200 components = 0.00107013 Jy ! Clean residual min=-0.002202 max=0.002376 Jy/beam ! Clean residual mean=0.000008 rms=0.000596 Jy/beam ! Combined flux in latest and established models = 0.760955 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 = -5.87038e-07 Jy ! Component: 100 - total flux cleaned = -3.97251e-07 Jy ! Component: 150 - total flux cleaned = 4.84121e-05 Jy ! Component: 200 - total flux cleaned = 4.79898e-05 Jy ! Total flux subtracted in 200 components = 4.79898e-05 Jy ! Clean residual min=-0.002166 max=0.002352 Jy/beam ! Clean residual mean=0.000008 rms=0.000591 Jy/beam ! Combined flux in latest and established models = 0.761003 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 79 components and 0.761003 Jy ! Inverting map ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 milli-arcsec ! Estimated beam: bmin=0.833 mas, bmaj=1.682 mas, bpa=-12.06 degrees ! Estimated noise=0.77269 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 8.6585e-05 Jy ! Component: 100 - total flux cleaned = -4.64302e-05 Jy ! Component: 150 - total flux cleaned = -0.000174984 Jy ! Component: 200 - total flux cleaned = -0.000176255 Jy ! Total flux subtracted in 200 components = -0.000176255 Jy ! Clean residual min=-0.002523 max=0.002529 Jy/beam ! Clean residual mean=0.000004 rms=0.000580 Jy/beam ! Combined flux in latest and established models = 0.760827 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 85 components and 0.760827 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.075347Jy sigma=0.735350 ! Fit after self-cal, rms=0.075256Jy sigma=0.734440 wmodel J2320+0513_X_map.mod ! Writing 85 model components to file: J2320+0513_X_map.mod wobs J2320+0513_X_uvs.fits ! Writing UV FITS file: J2320+0513_X_uvs.fits wwins J2320+0513_X_map.win ! wwins: Wrote 7 windows to J2320+0513_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 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 5.06062e-05 Jy ! Component: 100 - total flux cleaned = 4.28729e-06 Jy ! Component: 150 - total flux cleaned = -3.82889e-05 Jy ! Component: 200 - total flux cleaned = 4.24682e-06 Jy ! Component: 250 - total flux cleaned = -3.74922e-05 Jy ! Component: 300 - total flux cleaned = -3.77824e-05 Jy ! Component: 350 - total flux cleaned = -3.84133e-05 Jy ! Component: 400 - total flux cleaned = 8.48448e-07 Jy ! Component: 450 - total flux cleaned = 3.95868e-05 Jy ! Component: 500 - total flux cleaned = 7.7572e-05 Jy ! Component: 550 - total flux cleaned = 7.8039e-05 Jy ! Component: 600 - total flux cleaned = 0.000263699 Jy ! Component: 650 - total flux cleaned = 0.000520001 Jy ! Component: 700 - total flux cleaned = 0.000591969 Jy ! Component: 750 - total flux cleaned = 0.000699887 Jy ! Component: 800 - total flux cleaned = 0.000877129 Jy ! Component: 850 - total flux cleaned = 0.00105275 Jy ! Component: 900 - total flux cleaned = 0.00122611 Jy ! Component: 950 - total flux cleaned = 0.00132913 Jy ! Component: 1000 - total flux cleaned = 0.00149963 Jy ! Component: 1050 - total flux cleaned = 0.00153331 Jy ! Component: 1100 - total flux cleaned = 0.00170119 Jy ! Component: 1150 - total flux cleaned = 0.00186758 Jy ! Component: 1200 - total flux cleaned = 0.00203255 Jy ! Component: 1250 - total flux cleaned = 0.00219621 Jy ! Component: 1300 - total flux cleaned = 0.00232634 Jy ! Component: 1350 - total flux cleaned = 0.00242307 Jy ! Component: 1400 - total flux cleaned = 0.00255138 Jy ! Component: 1450 - total flux cleaned = 0.00264674 Jy ! Component: 1500 - total flux cleaned = 0.00271009 Jy ! Component: 1550 - total flux cleaned = 0.00280475 Jy ! Component: 1600 - total flux cleaned = 0.0028982 Jy ! Component: 1650 - total flux cleaned = 0.00292942 Jy ! Component: 1700 - total flux cleaned = 0.00308354 Jy ! Component: 1750 - total flux cleaned = 0.00311437 Jy ! Component: 1800 - total flux cleaned = 0.00335805 Jy ! Component: 1850 - total flux cleaned = 0.00335808 Jy ! Component: 1900 - total flux cleaned = 0.00341842 Jy ! Component: 1950 - total flux cleaned = 0.00341853 Jy ! Component: 2000 - total flux cleaned = 0.00344825 Jy ! Component: 2050 - total flux cleaned = 0.00359651 Jy ! Component: 2100 - total flux cleaned = 0.00362577 Jy ! Component: 2150 - total flux cleaned = 0.00377192 Jy ! Component: 2200 - total flux cleaned = 0.00377192 Jy ! Component: 2250 - total flux cleaned = 0.00380075 Jy ! Component: 2300 - total flux cleaned = 0.00397362 Jy ! Component: 2350 - total flux cleaned = 0.00417411 Jy ! Component: 2400 - total flux cleaned = 0.00420251 Jy ! Component: 2450 - total flux cleaned = 0.00420271 Jy ! Component: 2500 - total flux cleaned = 0.00431562 Jy ! Component: 2550 - total flux cleaned = 0.00440014 Jy ! Component: 2600 - total flux cleaned = 0.00451183 Jy ! Component: 2650 - total flux cleaned = 0.00462313 Jy ! Component: 2700 - total flux cleaned = 0.00465077 Jy ! Component: 2750 - total flux cleaned = 0.00465086 Jy ! Component: 2800 - total flux cleaned = 0.00476092 Jy ! Component: 2850 - total flux cleaned = 0.00465157 Jy ! Component: 2900 - total flux cleaned = 0.00476057 Jy ! Component: 2950 - total flux cleaned = 0.00473346 Jy ! Component: 3000 - total flux cleaned = 0.00484116 Jy ! Component: 3050 - total flux cleaned = 0.00478756 Jy ! Component: 3100 - total flux cleaned = 0.00489453 Jy ! Component: 3150 - total flux cleaned = 0.00492098 Jy ! Component: 3200 - total flux cleaned = 0.00494747 Jy ! Component: 3250 - total flux cleaned = 0.00500015 Jy ! Component: 3300 - total flux cleaned = 0.00497368 Jy ! Component: 3350 - total flux cleaned = 0.00502622 Jy ! Component: 3400 - total flux cleaned = 0.00505209 Jy ! Component: 3450 - total flux cleaned = 0.00507807 Jy ! Component: 3500 - total flux cleaned = 0.00510373 Jy ! Component: 3550 - total flux cleaned = 0.00507842 Jy ! Component: 3600 - total flux cleaned = 0.00500139 Jy ! Component: 3650 - total flux cleaned = 0.00510345 Jy ! Component: 3700 - total flux cleaned = 0.0051543 Jy ! Component: 3750 - total flux cleaned = 0.00505314 Jy ! Component: 3800 - total flux cleaned = 0.0051791 Jy ! Component: 3850 - total flux cleaned = 0.00517929 Jy ! Component: 3900 - total flux cleaned = 0.00517932 Jy ! Component: 3950 - total flux cleaned = 0.00525408 Jy ! Component: 4000 - total flux cleaned = 0.00520464 Jy ! Component: 4050 - total flux cleaned = 0.00517998 Jy ! Total flux subtracted in 4096 components = 0.00518013 Jy ! Clean residual min=-0.001232 max=0.001429 Jy/beam ! Clean residual mean=0.000002 rms=0.000410 Jy/beam ! Combined flux in latest and established models = 0.766007 Jy keep ! Adding 301 model components to the UV plane model. ! The established model now contains 386 components and 0.766007 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv120_uvs/J2320+0513_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.833 x 1.682 at -12.06 degrees (North through East) ! Clean map min=-0.0021472 max=0.70286 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv120_uvs/J2320+0513_X_map.fits wmodel /scr/pima/rv120_uvs/J2320+0513_X_map.mod ! Writing 386 model components to file: /scr/pima/rv120_uvs/J2320+0513_X_map.mod wobs /scr/pima/rv120_uvs/J2320+0513_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv120_uvs/J2320+0513_X_uvs.fits wwins /scr/pima/rv120_uvs/J2320+0513_X_map.win ! wwins: Wrote 8 windows to /scr/pima/rv120_uvs/J2320+0513_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.702862 invert ! Inverting map ! Your choice of large map pixels excluded 1.85% of the data. ! The y-axis pixel size should ideally be below 0.1835 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000409226 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.174668 0.174668 0.349337 0.698674 1.39735 2.79469 5.58939 11.1788 22.3576 44.7151 89.4302 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0012 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.702 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 1717.54 quit ! Quitting program ! Log file /scr/pima/rv120_uvs/J2320+0513_X_dfm.log closed on Fri Dec 22 22:45:21 2017