! Started logfile: /scr/pima/rv120_uvs/J0224+0659_X_dfm.log on Fri Dec 22 22:38:51 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/J0224+0659_X_uva.fits ! Reading UV FITS file: /scr/pima/rv120_uvs/J0224+0659_X_uva.fits ! AN table 1: 216 integrations on 78 of 78 possible baselines. ! AN table 2: 4 integrations on 28 of 28 possible baselines. ! AN table 3: 8 integrations on 21 of 21 possible baselines. ! AN table 4: 26 integrations on 10 of 10 possible baselines. ! Apparent sampling: 0.161606 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0224+0659 ! ! 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 11240 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 J0224+0659_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 2002 telescope corrections were flagged in sub-array 1. ! A total of 10 telescope corrections were flagged in sub-array 2. ! A total of 28 telescope corrections were flagged in sub-array 3. ! A total of 78 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 2002 telescope corrections were flagged in sub-array 1. ! A total of 10 telescope corrections were flagged in sub-array 2. ! A total of 28 telescope corrections were flagged in sub-array 3. ! A total of 78 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 2002 telescope corrections were flagged in sub-array 1. ! A total of 10 telescope corrections were flagged in sub-array 2. ! A total of 28 telescope corrections were flagged in sub-array 3. ! A total of 78 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 2002 telescope corrections were flagged in sub-array 1. ! A total of 10 telescope corrections were flagged in sub-array 2. ! A total of 28 telescope corrections were flagged in sub-array 3. ! A total of 78 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=1.332630Jy sigma=17.072156 ! Fit after self-cal, rms=0.233508Jy sigma=2.965524 ! 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 10.1% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! Estimated beam: bmin=0.532 mas, bmaj=0.9702 mas, bpa=-10.95 degrees ! Estimated noise=0.89491 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 = 0.641441 Jy ! Component: 100 - total flux cleaned = 0.783408 Jy ! Total flux subtracted in 100 components = 0.783408 Jy ! Clean residual min=-0.021658 max=0.048718 Jy/beam ! Clean residual mean=-0.000028 rms=0.003655 Jy/beam ! Combined flux in latest and established models = 0.783408 Jy ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 4 components and 0.783408 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.218895Jy sigma=1.995171 ! Fit after self-cal, rms=0.218868Jy sigma=1.994930 ! Inverting map ! Your choice of large map pixels excluded 10.1% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! Added new window around map position (-0.6, 0.8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0534533 Jy ! Component: 100 - total flux cleaned = 0.0742031 Jy ! Total flux subtracted in 100 components = 0.0742031 Jy ! Clean residual min=-0.019736 max=0.030075 Jy/beam ! Clean residual mean=-0.000016 rms=0.003073 Jy/beam ! Combined flux in latest and established models = 0.857611 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 12 components and 0.857611 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.191013Jy sigma=1.673808 ! Fit after self-cal, rms=0.190863Jy sigma=1.672343 ! Inverting map ! Your choice of large map pixels excluded 10.1% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! Added new window around map position (-1.4, -0.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0144241 Jy ! Component: 100 - total flux cleaned = 0.0165507 Jy ! Total flux subtracted in 100 components = 0.0165507 Jy ! Clean residual min=-0.017620 max=0.019787 Jy/beam ! Clean residual mean=-0.000013 rms=0.002847 Jy/beam ! Combined flux in latest and established models = 0.874162 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 17 components and 0.874162 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.177666Jy sigma=1.556105 ! Fit after self-cal, rms=0.177496Jy sigma=1.553957 ! Inverting map ! Your choice of large map pixels excluded 10.1% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! Added new window around map position (-0.6, -1). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00847159 Jy ! Component: 100 - total flux cleaned = 0.0128943 Jy ! Total flux subtracted in 100 components = 0.0128943 Jy ! Clean residual min=-0.016160 max=0.016655 Jy/beam ! Clean residual mean=-0.000011 rms=0.002705 Jy/beam ! Combined flux in latest and established models = 0.887056 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 20 components and 0.887056 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.167685Jy sigma=1.482636 ! Fit after self-cal, rms=0.167625Jy sigma=1.481907 ! Inverting map ! Your choice of large map pixels excluded 10.1% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! Added new window around map position (-2.4, 0.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00699787 Jy ! Component: 100 - total flux cleaned = 0.00996421 Jy ! Total flux subtracted in 100 components = 0.00996421 Jy ! Clean residual min=-0.015731 max=0.014953 Jy/beam ! Clean residual mean=-0.000010 rms=0.002598 Jy/beam ! Combined flux in latest and established models = 0.89702 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 24 components and 0.89702 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.160179Jy sigma=1.428317 ! Fit after self-cal, rms=0.160113Jy sigma=1.427753 ! Inverting map ! Your choice of large map pixels excluded 10.1% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 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 10.1% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! Estimated beam: bmin=0.5708 mas, bmaj=0.9945 mas, bpa=-10.35 degrees ! Estimated noise=0.584286 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 = 0.0195992 Jy ! Component: 100 - total flux cleaned = 0.0203432 Jy ! Component: 150 - total flux cleaned = 0.0209948 Jy ! Component: 200 - total flux cleaned = 0.0209529 Jy ! Total flux subtracted in 200 components = 0.0209529 Jy ! Clean residual min=-0.016174 max=0.013861 Jy/beam ! Clean residual mean=-0.000026 rms=0.002394 Jy/beam ! Combined flux in latest and established models = 0.917973 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 31 components and 0.917973 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.147999Jy sigma=1.341059 ! Fit after self-cal, rms=0.147858Jy sigma=1.339595 ! Inverting map ! Your choice of large map pixels excluded 10.1% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5708 x 0.9945 at -10.35 degrees (North through East) ! Clean map min=-0.012166 max=0.82224 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 222 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 1.02 HH 0.98 HN 1.07 ! KP 1.06 LA 1.00 NL 1.00 NY 0.98 ! ON 1.00 OV 1.03 PT 1.02 SC 1.02 ! WZ 0.97 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.07 HN 1.04 KK 1.02 LA 0.99 ! MK 0.91 NL 1.00 OV 1.01 PT 0.99 ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! FD 1.02 KK 0.98 KP 1.04 LA 1.02 ! MK 0.90 OV 1.03 PT 1.00 ! ! A total of 42 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.05 KK 0.95 KP 1.08 MK 1.87 ! OV 1.01 ! ! ! Correcting IF 2. ! A total of 222 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.04 FD 1.02 HH 0.94 HN 1.10 ! KP 1.04 LA 1.00 NL 1.00 NY 1.01 ! ON 1.00 OV 1.04 PT 1.03 SC 1.01 ! WZ 0.95 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.06 HN 1.18 KK 1.03 LA 0.98 ! MK 0.93 NL 1.01 OV 1.01 PT 0.96 ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! FD 0.99 KK 1.01 KP 1.02 LA 1.04 ! MK 0.96 OV 1.02 PT 1.01 ! ! A total of 42 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.03 KK 0.96 KP 1.00 MK 2.09 ! OV 1.05 ! ! ! Correcting IF 3. ! A total of 222 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 1.00 HH 0.91 HN 1.07 ! KP 1.03 LA 0.98 NL 0.96 NY 0.97 ! ON 0.99 OV 1.00 PT 1.00 SC 0.97 ! WZ 0.94 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 HN 1.05 KK 0.97 LA 0.95 ! MK 0.89 NL 0.97 OV 0.99 PT 0.96 ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! FD 0.99 KK 0.93 KP 1.00 LA 0.97 ! MK 0.95 OV 0.98 PT 0.96 ! ! A total of 42 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 KK 0.93 KP 1.00 MK 2.47 ! OV 0.98 ! ! ! Correcting IF 4. ! A total of 222 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 1.00 HH 0.92 HN 1.07 ! KP 1.02 LA 0.95 NL 0.97 NY 0.95 ! ON 0.99 OV 1.00 PT 0.99 SC 0.97 ! WZ 0.92 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 HN 1.01 KK 0.88 LA 0.95 ! MK 0.91 NL 0.97 OV 0.94 PT 0.96 ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! FD 0.97 KK 0.95 KP 1.01 LA 0.99 ! MK 0.96 OV 1.00 PT 0.96 ! ! A total of 42 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 KK 0.94 KP 0.99 MK 2.43 ! OV 1.01 ! ! ! Fit before self-cal, rms=0.147858Jy sigma=1.339595 ! Fit after self-cal, rms=0.094244Jy sigma=0.991155 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! Estimated beam: bmin=0.5495 mas, bmaj=1.018 mas, bpa=-9.476 degrees ! Estimated noise=0.596026 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 = 0.011991 Jy ! Component: 100 - total flux cleaned = 0.013772 Jy ! Component: 150 - total flux cleaned = 0.0144219 Jy ! Component: 200 - total flux cleaned = 0.0147958 Jy ! Total flux subtracted in 200 components = 0.0147958 Jy ! Clean residual min=-0.004919 max=0.005295 Jy/beam ! Clean residual mean=-0.000024 rms=0.001084 Jy/beam ! Combined flux in latest and established models = 0.932769 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 44 components and 0.932769 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.091977Jy sigma=0.957481 ! Fit after self-cal, rms=0.091919Jy sigma=0.956039 ! Inverting map ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 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=0.091919Jy sigma=0.956039 ! Fit after self-cal, rms=0.091358Jy sigma=0.937490 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! Estimated beam: bmin=0.5507 mas, bmaj=1.019 mas, bpa=-9.457 degrees ! Estimated noise=0.597707 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0002307 Jy ! Component: 100 - total flux cleaned = 0.000488142 Jy ! Component: 150 - total flux cleaned = 0.000398163 Jy ! Component: 200 - total flux cleaned = 0.000398614 Jy ! Total flux subtracted in 200 components = 0.000398614 Jy ! Clean residual min=-0.004247 max=0.004345 Jy/beam ! Clean residual mean=-0.000022 rms=0.000908 Jy/beam ! Combined flux in latest and established models = 0.933168 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 55 components and 0.933168 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.090869Jy sigma=0.932069 ! Fit after self-cal, rms=0.090849Jy sigma=0.931547 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 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 (-12.6, -22.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00220377 Jy ! Component: 100 - total flux cleaned = 0.00231169 Jy ! Component: 150 - total flux cleaned = 0.00250913 Jy ! Component: 200 - total flux cleaned = 0.00259567 Jy ! Total flux subtracted in 200 components = 0.00259567 Jy ! Clean residual min=-0.004337 max=0.004026 Jy/beam ! Clean residual mean=-0.000021 rms=0.000882 Jy/beam ! Combined flux in latest and established models = 0.935763 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 67 components and 0.935763 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.090504Jy sigma=0.927925 ! Fit after self-cal, rms=0.090489Jy sigma=0.927601 ! Inverting map ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 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=0.090489Jy sigma=0.927601 ! Fit after self-cal, rms=0.085869Jy sigma=0.881644 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! Estimated beam: bmin=0.5509 mas, bmaj=1.018 mas, bpa=-9.521 degrees ! Estimated noise=0.597949 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000682452 Jy ! Component: 100 - total flux cleaned = 0.000674873 Jy ! Component: 150 - total flux cleaned = 0.000735491 Jy ! Component: 200 - total flux cleaned = 0.00067192 Jy ! Total flux subtracted in 200 components = 0.00067192 Jy ! Clean residual min=-0.002667 max=0.002667 Jy/beam ! Clean residual mean=-0.000005 rms=0.000585 Jy/beam ! Combined flux in latest and established models = 0.936435 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 76 components and 0.936435 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.085668Jy sigma=0.879581 ! Fit after self-cal, rms=0.085649Jy sigma=0.879408 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 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 (-3, 1.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00173099 Jy ! Component: 100 - total flux cleaned = 0.00199224 Jy ! Component: 150 - total flux cleaned = 0.00199193 Jy ! Component: 200 - total flux cleaned = 0.00199147 Jy ! Total flux subtracted in 200 components = 0.00199147 Jy ! Clean residual min=-0.002593 max=0.002488 Jy/beam ! Clean residual mean=-0.000004 rms=0.000566 Jy/beam ! Combined flux in latest and established models = 0.938426 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 83 components and 0.938426 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.085465Jy sigma=0.877527 ! Fit after self-cal, rms=0.085451Jy sigma=0.877412 ! Inverting map ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 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=0.085451Jy sigma=0.877412 ! Fit after self-cal, rms=0.085385Jy sigma=0.877055 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! Estimated beam: bmin=2.614 mas, bmaj=2.778 mas, bpa=-3.646 degrees ! Estimated noise=0.878105 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0014713 Jy ! Component: 100 - total flux cleaned = 0.00153802 Jy ! Component: 150 - total flux cleaned = 0.00160997 Jy ! Component: 200 - total flux cleaned = 0.00157707 Jy ! Total flux subtracted in 200 components = 0.00157707 Jy ! Clean residual min=-0.002843 max=0.002942 Jy/beam ! Clean residual mean=-0.000013 rms=0.000728 Jy/beam ! Combined flux in latest and established models = 0.940003 Jy selfcal ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 103 components and 0.940003 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.085396Jy sigma=0.876685 ! Fit after self-cal, rms=0.085383Jy sigma=0.876620 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 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 = 0.000327622 Jy ! Component: 100 - total flux cleaned = 0.000327874 Jy ! Component: 150 - total flux cleaned = 0.000299733 Jy ! Component: 200 - total flux cleaned = 0.000300546 Jy ! Total flux subtracted in 200 components = 0.000300546 Jy ! Clean residual min=-0.002834 max=0.002948 Jy/beam ! Clean residual mean=-0.000013 rms=0.000722 Jy/beam ! Combined flux in latest and established models = 0.940304 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 103 components and 0.940304 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.085392Jy sigma=0.876475 ! Fit after self-cal, rms=0.085386Jy sigma=0.876459 ! Inverting map ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 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 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! Estimated beam: bmin=0.5509 mas, bmaj=1.018 mas, bpa=-9.531 degrees ! Estimated noise=0.59778 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5509 x 1.018 at -9.531 degrees (North through East) ! Clean map min=-0.0027986 max=0.81601 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=0.085386Jy sigma=0.876459 ! Fit after self-cal, rms=0.079302Jy sigma=0.794908 ! Inverting map and beam ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! Estimated beam: bmin=0.5508 mas, bmaj=1.018 mas, bpa=-9.528 degrees ! Estimated noise=0.597839 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000690216 Jy ! Component: 100 - total flux cleaned = 0.000982475 Jy ! Component: 150 - total flux cleaned = 0.00103188 Jy ! Component: 200 - total flux cleaned = 0.00103033 Jy ! Total flux subtracted in 200 components = 0.00103033 Jy ! Clean residual min=-0.002507 max=0.002394 Jy/beam ! Clean residual mean=-0.000004 rms=0.000547 Jy/beam ! Combined flux in latest and established models = 0.941334 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 106 components and 0.941334 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.079189Jy sigma=0.793785 ! Fit after self-cal, rms=0.079181Jy sigma=0.793728 ! Inverting map ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000157685 Jy ! Component: 100 - total flux cleaned = 6.71419e-05 Jy ! Component: 150 - total flux cleaned = 6.65928e-05 Jy ! Component: 200 - total flux cleaned = 2.32952e-05 Jy ! Total flux subtracted in 200 components = 2.32952e-05 Jy ! Clean residual min=-0.002462 max=0.002358 Jy/beam ! Clean residual mean=-0.000004 rms=0.000543 Jy/beam ! Combined flux in latest and established models = 0.941358 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 109 components and 0.941358 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.079110Jy sigma=0.793065 ! Fit after self-cal, rms=0.079107Jy sigma=0.793047 ! Inverting map ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.079107Jy sigma=0.793047 ! Fit after self-cal, rms=0.079114Jy sigma=0.792935 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 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! Estimated beam: bmin=0.5167 mas, bmaj=0.9925 mas, bpa=-9.838 degrees ! Estimated noise=0.921163 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.633862 Jy ! Component: 100 - total flux cleaned = 0.775892 Jy ! Component: 150 - total flux cleaned = 0.834378 Jy ! Component: 200 - total flux cleaned = 0.870706 Jy ! Total flux subtracted in 200 components = 0.870706 Jy ! Clean residual min=-0.009975 max=0.019350 Jy/beam ! Clean residual mean=-0.000014 rms=0.001715 Jy/beam ! Combined flux in latest and established models = 0.870706 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 12 model components to the UV plane model. ! The established model now contains 12 components and 0.870706 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! Estimated beam: bmin=0.5507 mas, bmaj=1.018 mas, bpa=-9.539 degrees ! Estimated noise=0.597769 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 = 0.0325179 Jy ! Component: 100 - total flux cleaned = 0.0498986 Jy ! Component: 150 - total flux cleaned = 0.0512003 Jy ! Component: 200 - total flux cleaned = 0.0529981 Jy ! Total flux subtracted in 200 components = 0.0529981 Jy ! Clean residual min=-0.009249 max=0.010043 Jy/beam ! Clean residual mean=-0.000010 rms=0.001155 Jy/beam ! Combined flux in latest and established models = 0.923705 Jy ! Adding 18 model components to the UV plane model. ! The established model now contains 23 components and 0.923705 Jy ! Inverting map ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! Added new window around map position (0.4, 1). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00219949 Jy ! Component: 100 - total flux cleaned = 0.00316615 Jy ! Component: 150 - total flux cleaned = 0.00454096 Jy ! Component: 200 - total flux cleaned = 0.0053811 Jy ! Total flux subtracted in 200 components = 0.0053811 Jy ! Clean residual min=-0.006401 max=0.006582 Jy/beam ! Clean residual mean=-0.000008 rms=0.000918 Jy/beam ! Combined flux in latest and established models = 0.929086 Jy ! Adding 14 model components to the UV plane model. ! The established model now contains 26 components and 0.929085 Jy ! Inverting map ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00150464 Jy ! Component: 100 - total flux cleaned = 0.00219994 Jy ! Component: 150 - total flux cleaned = 0.00284653 Jy ! Component: 200 - total flux cleaned = 0.00342865 Jy ! Total flux subtracted in 200 components = 0.00342865 Jy ! Clean residual min=-0.004558 max=0.004582 Jy/beam ! Clean residual mean=-0.000007 rms=0.000774 Jy/beam ! Combined flux in latest and established models = 0.932514 Jy ! Adding 17 model components to the UV plane model. ! The established model now contains 29 components and 0.932514 Jy ! Inverting map ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000529881 Jy ! Component: 100 - total flux cleaned = 0.000769605 Jy ! Component: 150 - total flux cleaned = 0.000994157 Jy ! Component: 200 - total flux cleaned = 0.00120179 Jy ! Total flux subtracted in 200 components = 0.00120179 Jy ! Clean residual min=-0.003483 max=0.003735 Jy/beam ! Clean residual mean=-0.000007 rms=0.000689 Jy/beam ! Combined flux in latest and established models = 0.933716 Jy ! Adding 22 model components to the UV plane model. ! The established model now contains 33 components and 0.933716 Jy ! Inverting map ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! Added new window around map position (-5, 1.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000807806 Jy ! Component: 100 - total flux cleaned = 0.00133933 Jy ! Component: 150 - total flux cleaned = 0.00183031 Jy ! Component: 200 - total flux cleaned = 0.00229487 Jy ! Total flux subtracted in 200 components = 0.00229487 Jy ! Clean residual min=-0.002979 max=0.002830 Jy/beam ! Clean residual mean=-0.000006 rms=0.000632 Jy/beam ! Combined flux in latest and established models = 0.936011 Jy ! Adding 30 model components to the UV plane model. ! The established model now contains 45 components and 0.936011 Jy ! Inverting map ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 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 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! Estimated beam: bmin=2.611 mas, bmaj=2.779 mas, bpa=-3.292 degrees ! Estimated noise=0.878692 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00420077 Jy ! Component: 100 - total flux cleaned = 0.00587258 Jy ! Component: 150 - total flux cleaned = 0.00626588 Jy ! Component: 200 - total flux cleaned = 0.00658101 Jy ! Total flux subtracted in 200 components = 0.00658101 Jy ! Clean residual min=-0.002659 max=0.002664 Jy/beam ! Clean residual mean=-0.000014 rms=0.000719 Jy/beam ! Combined flux in latest and established models = 0.942592 Jy flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000217633 Jy ! Component: 100 - total flux cleaned = 0.000330508 Jy ! Component: 150 - total flux cleaned = 0.000462266 Jy ! Component: 200 - total flux cleaned = 0.000521983 Jy ! Total flux subtracted in 200 components = 0.000521983 Jy ! Clean residual min=-0.002620 max=0.002718 Jy/beam ! Clean residual mean=-0.000013 rms=0.000707 Jy/beam ! Combined flux in latest and established models = 0.943114 Jy ! Adding 36 model components to the UV plane model. ! The established model now contains 79 components and 0.943114 Jy ! Inverting map ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! Estimated beam: bmin=0.5507 mas, bmaj=1.018 mas, bpa=-9.539 degrees ! Estimated noise=0.597769 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000738941 Jy ! Component: 100 - total flux cleaned = -0.000605986 Jy ! Component: 150 - total flux cleaned = -0.000600365 Jy ! Component: 200 - total flux cleaned = -0.000481682 Jy ! Total flux subtracted in 200 components = -0.000481682 Jy ! Clean residual min=-0.002589 max=0.002539 Jy/beam ! Clean residual mean=-0.000005 rms=0.000572 Jy/beam ! Combined flux in latest and established models = 0.942632 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 84 components and 0.942632 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.080006Jy sigma=0.797715 ! Fit after self-cal, rms=0.079871Jy sigma=0.796705 wmodel J0224+0659_X_map.mod ! Writing 84 model components to file: J0224+0659_X_map.mod wobs J0224+0659_X_uvs.fits ! Writing UV FITS file: J0224+0659_X_uvs.fits wwins J0224+0659_X_map.win ! wwins: Wrote 9 windows to J0224+0659_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 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000294689 Jy ! Component: 100 - total flux cleaned = -0.000338353 Jy ! Component: 150 - total flux cleaned = -0.000554766 Jy ! Component: 200 - total flux cleaned = -0.000724246 Jy ! Component: 250 - total flux cleaned = -0.000849531 Jy ! Component: 300 - total flux cleaned = -0.000972315 Jy ! Component: 350 - total flux cleaned = -0.00105235 Jy ! Component: 400 - total flux cleaned = -0.00125061 Jy ! Component: 450 - total flux cleaned = -0.00140707 Jy ! Component: 500 - total flux cleaned = -0.00156145 Jy ! Component: 550 - total flux cleaned = -0.00175213 Jy ! Component: 600 - total flux cleaned = -0.00197767 Jy ! Component: 650 - total flux cleaned = -0.00201466 Jy ! Component: 700 - total flux cleaned = -0.00208848 Jy ! Component: 750 - total flux cleaned = -0.00216184 Jy ! Component: 800 - total flux cleaned = -0.00237846 Jy ! Component: 850 - total flux cleaned = -0.0024143 Jy ! Component: 900 - total flux cleaned = -0.00244984 Jy ! Component: 950 - total flux cleaned = -0.00262563 Jy ! Component: 1000 - total flux cleaned = -0.00273038 Jy ! Component: 1050 - total flux cleaned = -0.00279925 Jy ! Component: 1100 - total flux cleaned = -0.00293656 Jy ! Component: 1150 - total flux cleaned = -0.00303816 Jy ! Component: 1200 - total flux cleaned = -0.00310563 Jy ! Component: 1250 - total flux cleaned = -0.00313905 Jy ! Component: 1300 - total flux cleaned = -0.0032386 Jy ! Component: 1350 - total flux cleaned = -0.0033046 Jy ! Component: 1400 - total flux cleaned = -0.00343559 Jy ! Component: 1450 - total flux cleaned = -0.00353339 Jy ! Component: 1500 - total flux cleaned = -0.0036622 Jy ! Component: 1550 - total flux cleaned = -0.0037581 Jy ! Component: 1600 - total flux cleaned = -0.0038531 Jy ! Component: 1650 - total flux cleaned = -0.00394767 Jy ! Component: 1700 - total flux cleaned = -0.00388504 Jy ! Component: 1750 - total flux cleaned = -0.00394774 Jy ! Component: 1800 - total flux cleaned = -0.0040715 Jy ! Component: 1850 - total flux cleaned = -0.00410198 Jy ! Component: 1900 - total flux cleaned = -0.00422412 Jy ! Component: 1950 - total flux cleaned = -0.00428471 Jy ! Component: 2000 - total flux cleaned = -0.00425457 Jy ! Component: 2050 - total flux cleaned = -0.00434471 Jy ! Component: 2100 - total flux cleaned = -0.00437451 Jy ! Component: 2150 - total flux cleaned = -0.00455234 Jy ! Component: 2200 - total flux cleaned = -0.004493 Jy ! Component: 2250 - total flux cleaned = -0.00452232 Jy ! Component: 2300 - total flux cleaned = -0.00449329 Jy ! Component: 2350 - total flux cleaned = -0.00458024 Jy ! Component: 2400 - total flux cleaned = -0.00463789 Jy ! Component: 2450 - total flux cleaned = -0.00458034 Jy ! Component: 2500 - total flux cleaned = -0.00469415 Jy ! Component: 2550 - total flux cleaned = -0.00466577 Jy ! Component: 2600 - total flux cleaned = -0.00469395 Jy ! Component: 2650 - total flux cleaned = -0.00480596 Jy ! Component: 2700 - total flux cleaned = -0.00483366 Jy ! Component: 2750 - total flux cleaned = -0.00491681 Jy ! Component: 2800 - total flux cleaned = -0.00491672 Jy ! Component: 2850 - total flux cleaned = -0.00494438 Jy ! Component: 2900 - total flux cleaned = -0.00494442 Jy ! Component: 2950 - total flux cleaned = -0.00488966 Jy ! Component: 3000 - total flux cleaned = -0.00507932 Jy ! Component: 3050 - total flux cleaned = -0.00505232 Jy ! Component: 3100 - total flux cleaned = -0.00491817 Jy ! Component: 3150 - total flux cleaned = -0.00505153 Jy ! Component: 3200 - total flux cleaned = -0.00499847 Jy ! Component: 3250 - total flux cleaned = -0.00521006 Jy ! Component: 3300 - total flux cleaned = -0.00515737 Jy ! Component: 3350 - total flux cleaned = -0.00515739 Jy ! Component: 3400 - total flux cleaned = -0.0051833 Jy ! Component: 3450 - total flux cleaned = -0.00531309 Jy ! Component: 3500 - total flux cleaned = -0.00531324 Jy ! Component: 3550 - total flux cleaned = -0.00528758 Jy ! Component: 3600 - total flux cleaned = -0.00538992 Jy ! Component: 3650 - total flux cleaned = -0.00536451 Jy ! Component: 3700 - total flux cleaned = -0.00546608 Jy ! Component: 3750 - total flux cleaned = -0.00551656 Jy ! Component: 3800 - total flux cleaned = -0.00549129 Jy ! Component: 3850 - total flux cleaned = -0.00564152 Jy ! Component: 3900 - total flux cleaned = -0.00551667 Jy ! Component: 3950 - total flux cleaned = -0.00554165 Jy ! Component: 4000 - total flux cleaned = -0.00571474 Jy ! Component: 4050 - total flux cleaned = -0.00564086 Jy ! Total flux subtracted in 4096 components = -0.00568991 Jy ! Clean residual min=-0.001296 max=0.001673 Jy/beam ! Clean residual mean=-0.000003 rms=0.000393 Jy/beam ! Combined flux in latest and established models = 0.936942 Jy keep ! Adding 336 model components to the UV plane model. ! The established model now contains 415 components and 0.936942 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv120_uvs/J0224+0659_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5507 x 1.018 at -9.539 degrees (North through East) ! Clean map min=-0.0025636 max=0.81437 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv120_uvs/J0224+0659_X_map.fits wmodel /scr/pima/rv120_uvs/J0224+0659_X_map.mod ! Writing 415 model components to file: /scr/pima/rv120_uvs/J0224+0659_X_map.mod wobs /scr/pima/rv120_uvs/J0224+0659_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv120_uvs/J0224+0659_X_uvs.fits wwins /scr/pima/rv120_uvs/J0224+0659_X_map.win ! wwins: Wrote 10 windows to /scr/pima/rv120_uvs/J0224+0659_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.814375 invert ! Inverting map ! Your choice of large map pixels excluded 8.81% of the data. ! The x-axis pixel size should ideally be below 0.1644 milli-arcsec ! The y-axis pixel size should ideally be below 0.1809 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000391574 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.144248 0.144248 0.288496 0.576993 1.15399 2.30797 4.61594 9.23188 18.4638 36.9275 73.8551 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0011 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.814 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 2079.75 quit ! Quitting program ! Log file /scr/pima/rv120_uvs/J0224+0659_X_dfm.log closed on Fri Dec 22 22:38:57 2017