! Started logfile: /scr/pima/rv119_uvs/J0205+3212_X_dfm.log on Sun Dec 17 11:32:11 2017 float field_size field_size = 1024 float field_cell field_cell = 0.2000 float taper_size taper_size = 70.0 float freq freq = 8.36575 obs /scr/pima/rv119_uvs/J0205+3212_X_uva.fits ! Reading UV FITS file: /scr/pima/rv119_uvs/J0205+3212_X_uva.fits ! AN table 1: 30 integrations on 66 of 66 possible baselines. ! AN table 2: 4 integrations on 28 of 28 possible baselines. ! AN table 3: 6 integrations on 45 of 45 possible baselines. ! AN table 4: 10 integrations on 28 of 28 possible baselines. ! Apparent sampling: 0.259273 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0205+3212 ! ! There are 4 IFs, and a total of 4 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 8.36575e+09 8e+06 1 8e+06 ! 02 2 8.44575e+09 8e+06 1 8e+06 ! 03 3 8.80575e+09 8e+06 1 8e+06 ! 04 4 8.92575e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 79 lines of history. ! ! Reading 2740 visibilities. select rr, 1,2,3,4,5,6,7,8,9,10,11,12,13,14,15,16 ! Restricting channel ranges to the available 4 channels. ! Selecting polarization: RR, channels: 1..4 ! Reading IF 1 channels: 1..1 ! Reading IF 2 channels: 2..2 ! Reading IF 3 channels: 3..3 ! Reading IF 4 channels: 4..4 print "field_size =", field_size ! field_size = 1024 print "field_cell =", field_cell ! field_cell = 0.2 print "taper_size =", taper_size ! taper_size = 70 ![@/opt64/bin/pima_mupet_01.dfm J0205+3212_X] float lim_self lim_self = 120.0 float lim_val lim_va = 1.2 integer clean_niter clean_niter = 100 float clean_gain clean_gain = 0.03 float dynam dynam = 6.0 float soltime1 soltime1 = 120 float soltime2 soltime2 = 20 float thresh thresh = 0.5 float win_mult win_mult = 1.8 float time_av time_av = 16 float old_peak float new_peak float flux_cutoff 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 242 telescope corrections were flagged in sub-array 1. ! A total of 16 telescope corrections were flagged in sub-array 2. ! A total of 2 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 242 telescope corrections were flagged in sub-array 1. ! A total of 16 telescope corrections were flagged in sub-array 2. ! A total of 2 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 242 telescope corrections were flagged in sub-array 1. ! A total of 16 telescope corrections were flagged in sub-array 2. ! A total of 2 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 242 telescope corrections were flagged in sub-array 1. ! A total of 16 telescope corrections were flagged in sub-array 2. ! A total of 2 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=1.494380Jy sigma=19.346814 ! Fit after self-cal, rms=0.219572Jy sigma=2.770840 ! 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 3.16% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=0.6405 mas, bmaj=0.9184 mas, bpa=14.94 degrees ! Estimated noise=1.29233 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 = 0.845836 Jy ! Component: 100 - total flux cleaned = 1.04012 Jy ! Total flux subtracted in 100 components = 1.04012 Jy ! Clean residual min=-0.018334 max=0.074503 Jy/beam ! Clean residual mean=0.000000 rms=0.004515 Jy/beam ! Combined flux in latest and established models = 1.04012 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 1.04012 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.197680Jy sigma=2.457172 ! Fit after self-cal, rms=0.197349Jy sigma=2.455588 ! Inverting map ! Your choice of large map pixels excluded 3.16% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0861763 Jy ! Component: 100 - total flux cleaned = 0.1384 Jy ! Total flux subtracted in 100 components = 0.1384 Jy ! Clean residual min=-0.012931 max=0.027371 Jy/beam ! Clean residual mean=0.000006 rms=0.002999 Jy/beam ! Combined flux in latest and established models = 1.17852 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 16 components and 1.17852 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.148163Jy sigma=1.657821 ! Fit after self-cal, rms=0.147360Jy sigma=1.651071 ! Inverting map ! Your choice of large map pixels excluded 3.16% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0345958 Jy ! Component: 100 - total flux cleaned = 0.0559015 Jy ! Total flux subtracted in 100 components = 0.0559015 Jy ! Clean residual min=-0.012852 max=0.016959 Jy/beam ! Clean residual mean=0.000008 rms=0.002643 Jy/beam ! Combined flux in latest and established models = 1.23443 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 18 components and 1.23443 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.138834Jy sigma=1.484780 ! Fit after self-cal, rms=0.138371Jy sigma=1.480741 ! Inverting map ! Your choice of large map pixels excluded 3.16% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Added new window around map position (-1.2, 1). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0152035 Jy ! Component: 100 - total flux cleaned = 0.0213306 Jy ! Total flux subtracted in 100 components = 0.0213306 Jy ! Clean residual min=-0.012555 max=0.014778 Jy/beam ! Clean residual mean=0.000009 rms=0.002542 Jy/beam ! Combined flux in latest and established models = 1.25576 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 24 components and 1.25576 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.136319Jy sigma=1.443626 ! Fit after self-cal, rms=0.135921Jy sigma=1.440854 ! Inverting map ! Your choice of large map pixels excluded 3.16% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 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 3.16% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=0.7403 mas, bmaj=1.043 mas, bpa=14.24 degrees ! Estimated noise=1.11292 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 (0.2, 2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0114055 Jy ! Component: 100 - total flux cleaned = 0.0143086 Jy ! Component: 150 - total flux cleaned = 0.014991 Jy ! Component: 200 - total flux cleaned = 0.0155896 Jy ! Total flux subtracted in 200 components = 0.0155896 Jy ! Clean residual min=-0.010979 max=0.013003 Jy/beam ! Clean residual mean=0.000018 rms=0.002400 Jy/beam ! Combined flux in latest and established models = 1.27135 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 39 components and 1.27135 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.133398Jy sigma=1.406402 ! Fit after self-cal, rms=0.133104Jy sigma=1.403252 ! Inverting map ! Your choice of large map pixels excluded 3.16% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7403 x 1.043 at 14.24 degrees (North through East) ! Clean map min=-0.01056 max=1.0868 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 12 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.98 HH 0.88 HN 1.03 ! KP 1.01 LA 0.98 NL 1.02 NY 0.99 ! ON 0.93 PT 1.01 SC 0.97 WZ 0.98 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 KP 1.02 LA 0.98 MK 0.98 ! NL 1.00 OV 0.97 PT 0.99 SC 0.95 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 FD 1.00 HN 1.10 KP 0.99 ! LA 1.00 MK 1.02 NL 1.01 NY 1.03 ! OV 0.99 PT 1.00 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 KP 0.96 LA 1.06 MK 1.02 ! NY 1.00 ON 1.13 OV 0.99 PT 1.11 ! ! ! Correcting IF 2. ! A total of 12 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.04 FD 0.99 HH 0.90 HN 1.02 ! KP 0.98 LA 0.99 NL 1.02 NY 0.97 ! ON 0.96 PT 1.02 SC 0.95 WZ 0.97 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 KP 1.01 LA 0.96 MK 0.98 ! NL 1.01 OV 0.97 PT 0.97 SC 0.94 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 1.01 HN 1.10 KP 1.00 ! LA 0.98 MK 1.02 NL 1.01 NY 1.01 ! OV 0.98 PT 1.02 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 KP 0.99 LA 1.05 MK 0.98 ! NY 0.98 ON 1.09 OV 0.99 PT 1.14 ! ! ! Correcting IF 3. ! A total of 12 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 1.00 HH 0.99 HN 1.03 ! KP 1.01 LA 0.99 NL 1.04 NY 0.99 ! ON 0.96 PT 0.99 SC 0.96 WZ 0.95 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 KP 1.01 LA 0.97 MK 1.00 ! NL 1.01 OV 0.98 PT 0.96 SC 0.95 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 FD 0.99 HN 1.10 KP 1.00 ! LA 0.97 MK 1.04 NL 1.01 NY 1.05 ! OV 0.97 PT 1.00 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 KP 0.99 LA 1.06 MK 1.02 ! NY 0.96 ON 1.10 OV 0.99 PT 1.15 ! ! ! Correcting IF 4. ! A total of 12 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.04 FD 0.98 HH 1.17 HN 1.02 ! KP 1.00 LA 0.99 NL 1.04 NY 0.96 ! ON 0.97 PT 1.01 SC 0.94 WZ 0.95 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 KP 1.00 LA 0.98 MK 0.98 ! NL 1.01 OV 0.97 PT 0.98 SC 0.92 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 FD 0.98 HN 1.10 KP 1.00 ! LA 1.00 MK 1.02 NL 1.00 NY 1.02 ! OV 0.98 PT 1.02 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 KP 0.98 LA 1.07 MK 1.01 ! NY 0.97 ON 1.18 OV 0.98 PT 1.15 ! ! ! Fit before self-cal, rms=0.133104Jy sigma=1.403252 ! Fit after self-cal, rms=0.116777Jy sigma=1.238086 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=0.7415 mas, bmaj=1.04 mas, bpa=14 degrees ! Estimated noise=1.11843 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 (-0.2, 7). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0104342 Jy ! Component: 100 - total flux cleaned = 0.0129623 Jy ! Component: 150 - total flux cleaned = 0.0135223 Jy ! Component: 200 - total flux cleaned = 0.0137651 Jy ! Total flux subtracted in 200 components = 0.0137651 Jy ! Clean residual min=-0.010542 max=0.009071 Jy/beam ! Clean residual mean=0.000016 rms=0.001877 Jy/beam ! Combined flux in latest and established models = 1.28511 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 55 components and 1.28511 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.115306Jy sigma=1.217694 ! Fit after self-cal, rms=0.115157Jy sigma=1.216231 ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 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=0.115157Jy sigma=1.216231 ! Fit after self-cal, rms=0.099449Jy sigma=1.050310 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=0.7425 mas, bmaj=1.039 mas, bpa=13.93 degrees ! Estimated noise=1.12033 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00143843 Jy ! Component: 100 - total flux cleaned = -0.00122955 Jy ! Component: 150 - total flux cleaned = -0.00106391 Jy ! Component: 200 - total flux cleaned = -0.000757029 Jy ! Total flux subtracted in 200 components = -0.000757029 Jy ! Clean residual min=-0.005775 max=0.005808 Jy/beam ! Clean residual mean=0.000019 rms=0.001367 Jy/beam ! Combined flux in latest and established models = 1.28435 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 64 components and 1.28435 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.098676Jy sigma=1.040533 ! Fit after self-cal, rms=0.098497Jy sigma=1.039853 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 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 = 0.000216857 Jy ! Component: 100 - total flux cleaned = 0.000495392 Jy ! Component: 150 - total flux cleaned = 0.00049726 Jy ! Component: 200 - total flux cleaned = 0.000377343 Jy ! Total flux subtracted in 200 components = 0.000377343 Jy ! Clean residual min=-0.005764 max=0.005821 Jy/beam ! Clean residual mean=0.000019 rms=0.001356 Jy/beam ! Combined flux in latest and established models = 1.28473 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 70 components and 1.28473 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.098081Jy sigma=1.034964 ! Fit after self-cal, rms=0.097951Jy sigma=1.034720 ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Added new window around map position (-35.2, -18). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00453526 Jy ! Component: 100 - total flux cleaned = 0.00543331 Jy ! Component: 150 - total flux cleaned = 0.00566386 Jy ! Component: 200 - total flux cleaned = 0.00577673 Jy ! Total flux subtracted in 200 components = 0.00577673 Jy ! Clean residual min=-0.005772 max=0.005558 Jy/beam ! Clean residual mean=0.000018 rms=0.001338 Jy/beam ! Combined flux in latest and established models = 1.29051 Jy ! Performing phase self-cal ! Adding 31 model components to the UV plane model. ! The established model now contains 82 components and 1.29051 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.097508Jy sigma=1.028883 ! Fit after self-cal, rms=0.097379Jy sigma=1.028500 ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 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=0.097379Jy sigma=1.028500 ! Fit after self-cal, rms=0.092381Jy sigma=0.974009 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=0.742 mas, bmaj=1.039 mas, bpa=13.73 degrees ! Estimated noise=1.12266 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 9.06896e-05 Jy ! Component: 100 - total flux cleaned = -6.51509e-05 Jy ! Component: 150 - total flux cleaned = 0.000307783 Jy ! Component: 200 - total flux cleaned = 0.000418484 Jy ! Total flux subtracted in 200 components = 0.000418484 Jy ! Clean residual min=-0.004919 max=0.005547 Jy/beam ! Clean residual mean=0.000017 rms=0.001143 Jy/beam ! Combined flux in latest and established models = 1.29093 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 91 components and 1.29093 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.091964Jy sigma=0.968330 ! Fit after self-cal, rms=0.091769Jy sigma=0.967825 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 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 (-2.2, 11). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00478116 Jy ! Component: 100 - total flux cleaned = 0.00571934 Jy ! Component: 150 - total flux cleaned = 0.00617896 Jy ! Component: 200 - total flux cleaned = 0.00661244 Jy ! Total flux subtracted in 200 components = 0.00661244 Jy ! Clean residual min=-0.004673 max=0.004768 Jy/beam ! Clean residual mean=0.000015 rms=0.001120 Jy/beam ! Combined flux in latest and established models = 1.29754 Jy ! Performing phase self-cal ! Adding 31 model components to the UV plane model. ! The established model now contains 103 components and 1.29754 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.091235Jy sigma=0.962287 ! Fit after self-cal, rms=0.091145Jy sigma=0.961999 ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 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=0.091145Jy sigma=0.961999 ! Fit after self-cal, rms=0.091147Jy sigma=0.960961 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=2.536 mas, bmaj=2.791 mas, bpa=79.3 degrees ! Estimated noise=1.55157 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00391845 Jy ! Component: 100 - total flux cleaned = 0.00585314 Jy ! Component: 150 - total flux cleaned = 0.00665752 Jy ! Component: 200 - total flux cleaned = 0.0071562 Jy ! Total flux subtracted in 200 components = 0.0071562 Jy ! Clean residual min=-0.006702 max=0.006234 Jy/beam ! Clean residual mean=0.000033 rms=0.001680 Jy/beam ! Combined flux in latest and established models = 1.30469 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 118 components and 1.30469 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.091142Jy sigma=0.961049 ! Fit after self-cal, rms=0.091121Jy sigma=0.960843 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 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 = 0.00067717 Jy ! Component: 100 - total flux cleaned = 0.0012048 Jy ! Component: 150 - total flux cleaned = 0.00166814 Jy ! Component: 200 - total flux cleaned = 0.00199106 Jy ! Total flux subtracted in 200 components = 0.00199106 Jy ! Clean residual min=-0.006652 max=0.006231 Jy/beam ! Clean residual mean=0.000031 rms=0.001677 Jy/beam ! Combined flux in latest and established models = 1.30669 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 121 components and 1.30669 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.091131Jy sigma=0.960790 ! Fit after self-cal, rms=0.091105Jy sigma=0.960687 ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 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 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=0.7416 mas, bmaj=1.039 mas, bpa=13.64 degrees ! Estimated noise=1.12378 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7416 x 1.039 at 13.64 degrees (North through East) ! Clean map min=-0.0064544 max=1.0892 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=0.091105Jy sigma=0.960687 ! Fit after self-cal, rms=0.086178Jy sigma=0.881230 ! Inverting map and beam ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=0.7414 mas, bmaj=1.039 mas, bpa=13.67 degrees ! Estimated noise=1.12389 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000224717 Jy ! Component: 100 - total flux cleaned = -0.000445331 Jy ! Component: 150 - total flux cleaned = -0.000756262 Jy ! Component: 200 - total flux cleaned = -0.000758347 Jy ! Total flux subtracted in 200 components = -0.000758347 Jy ! Clean residual min=-0.004804 max=0.004543 Jy/beam ! Clean residual mean=0.000014 rms=0.001103 Jy/beam ! Combined flux in latest and established models = 1.30593 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 126 components and 1.30593 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.085882Jy sigma=0.877673 ! Fit after self-cal, rms=0.085727Jy sigma=0.877379 ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -9.19761e-05 Jy ! Component: 100 - total flux cleaned = -0.00018554 Jy ! Component: 150 - total flux cleaned = -9.66897e-05 Jy ! Component: 200 - total flux cleaned = -9.87478e-05 Jy ! Total flux subtracted in 200 components = -9.87478e-05 Jy ! Clean residual min=-0.004781 max=0.004564 Jy/beam ! Clean residual mean=0.000013 rms=0.001099 Jy/beam ! Combined flux in latest and established models = 1.30583 Jy ! Performing phase self-cal ! Adding 34 model components to the UV plane model. ! The established model now contains 132 components and 1.30583 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.085491Jy sigma=0.875235 ! Fit after self-cal, rms=0.085404Jy sigma=0.875082 ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.085404Jy sigma=0.875082 ! Fit after self-cal, rms=0.085442Jy sigma=0.874425 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 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=0.6414 mas, bmaj=0.9117 mas, bpa=14.24 degrees ! Estimated noise=1.30666 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.84727 Jy ! Component: 100 - total flux cleaned = 1.04759 Jy ! Component: 150 - total flux cleaned = 1.13654 Jy ! Component: 200 - total flux cleaned = 1.18586 Jy ! Total flux subtracted in 200 components = 1.18586 Jy ! Clean residual min=-0.008007 max=0.024676 Jy/beam ! Clean residual mean=0.000007 rms=0.001907 Jy/beam ! Combined flux in latest and established models = 1.18586 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 14 model components to the UV plane model. ! The established model now contains 14 components and 1.18586 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=0.7412 mas, bmaj=1.04 mas, bpa=13.61 degrees ! Estimated noise=1.12543 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 = 0.0380636 Jy ! Component: 100 - total flux cleaned = 0.0583719 Jy ! Component: 150 - total flux cleaned = 0.0710597 Jy ! Component: 200 - total flux cleaned = 0.080183 Jy ! Total flux subtracted in 200 components = 0.080183 Jy ! Clean residual min=-0.005306 max=0.006265 Jy/beam ! Clean residual mean=0.000022 rms=0.001259 Jy/beam ! Combined flux in latest and established models = 1.26605 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 32 components and 1.26605 Jy ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Added new window around map position (-2.6, 8.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0053896 Jy ! Component: 100 - total flux cleaned = 0.0100371 Jy ! Component: 150 - total flux cleaned = 0.0139208 Jy ! Component: 200 - total flux cleaned = 0.0176293 Jy ! Total flux subtracted in 200 components = 0.0176293 Jy ! Clean residual min=-0.004855 max=0.005048 Jy/beam ! Clean residual mean=0.000018 rms=0.001173 Jy/beam ! Combined flux in latest and established models = 1.28368 Jy ! Adding 33 model components to the UV plane model. ! The established model now contains 49 components and 1.28368 Jy ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Added new window around map position (-8, 7.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0041873 Jy ! Component: 100 - total flux cleaned = 0.00698632 Jy ! Component: 150 - total flux cleaned = 0.00957563 Jy ! Component: 200 - total flux cleaned = 0.0118199 Jy ! Total flux subtracted in 200 components = 0.0118199 Jy ! Clean residual min=-0.004777 max=0.004611 Jy/beam ! Clean residual mean=0.000016 rms=0.001135 Jy/beam ! Combined flux in latest and established models = 1.2955 Jy ! Adding 43 model components to the UV plane model. ! The established model now contains 65 components and 1.2955 Jy ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 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 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=2.538 mas, bmaj=2.792 mas, bpa=79.38 degrees ! Estimated noise=1.55283 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00537029 Jy ! Component: 100 - total flux cleaned = 0.00895967 Jy ! Component: 150 - total flux cleaned = 0.0112867 Jy ! Component: 200 - total flux cleaned = 0.0123251 Jy ! Total flux subtracted in 200 components = 0.0123251 Jy ! Clean residual min=-0.006514 max=0.006266 Jy/beam ! Clean residual mean=0.000033 rms=0.001685 Jy/beam ! Combined flux in latest and established models = 1.30782 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 = 0.000612084 Jy ! Component: 100 - total flux cleaned = 0.00102922 Jy ! Component: 150 - total flux cleaned = 0.00141157 Jy ! Component: 200 - total flux cleaned = 0.00170752 Jy ! Total flux subtracted in 200 components = 0.00170752 Jy ! Clean residual min=-0.006502 max=0.006323 Jy/beam ! Clean residual mean=0.000032 rms=0.001676 Jy/beam ! Combined flux in latest and established models = 1.30953 Jy ! Adding 39 model components to the UV plane model. ! The established model now contains 99 components and 1.30953 Jy ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! Estimated beam: bmin=0.7412 mas, bmaj=1.04 mas, bpa=13.61 degrees ! Estimated noise=1.12543 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00110431 Jy ! Component: 100 - total flux cleaned = -0.00123497 Jy ! Component: 150 - total flux cleaned = -0.000883375 Jy ! Component: 200 - total flux cleaned = -0.000438752 Jy ! Total flux subtracted in 200 components = -0.000438752 Jy ! Clean residual min=-0.004783 max=0.004774 Jy/beam ! Clean residual mean=0.000013 rms=0.001104 Jy/beam ! Combined flux in latest and established models = 1.30909 Jy selfcal ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 110 components and 1.30909 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.086277Jy sigma=0.879435 ! Fit after self-cal, rms=0.085426Jy sigma=0.875386 wmodel J0205+3212_X_map.mod ! Writing 110 model components to file: J0205+3212_X_map.mod wobs J0205+3212_X_uvs.fits ! Writing UV FITS file: J0205+3212_X_uvs.fits wwins J0205+3212_X_map.win ! wwins: Wrote 8 windows to J0205+3212_X_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000807151 Jy ! Component: 100 - total flux cleaned = -0.0016531 Jy ! Component: 150 - total flux cleaned = -0.00214763 Jy ! Component: 200 - total flux cleaned = -0.00271102 Jy ! Component: 250 - total flux cleaned = -0.00286894 Jy ! Component: 300 - total flux cleaned = -0.00317754 Jy ! Component: 350 - total flux cleaned = -0.00317693 Jy ! Component: 400 - total flux cleaned = -0.00325291 Jy ! Component: 450 - total flux cleaned = -0.00340281 Jy ! Component: 500 - total flux cleaned = -0.00347652 Jy ! Component: 550 - total flux cleaned = -0.0036931 Jy ! Component: 600 - total flux cleaned = -0.00383502 Jy ! Component: 650 - total flux cleaned = -0.00390538 Jy ! Component: 700 - total flux cleaned = -0.00390616 Jy ! Component: 750 - total flux cleaned = -0.00404314 Jy ! Component: 800 - total flux cleaned = -0.00383844 Jy ! Component: 850 - total flux cleaned = -0.00377072 Jy ! Component: 900 - total flux cleaned = -0.0037708 Jy ! Component: 950 - total flux cleaned = -0.00383705 Jy ! Component: 1000 - total flux cleaned = -0.00370408 Jy ! Component: 1050 - total flux cleaned = -0.00370342 Jy ! Component: 1100 - total flux cleaned = -0.00344353 Jy ! Component: 1150 - total flux cleaned = -0.00350713 Jy ! Component: 1200 - total flux cleaned = -0.00325067 Jy ! Component: 1250 - total flux cleaned = -0.0030594 Jy ! Component: 1300 - total flux cleaned = -0.0029966 Jy ! Component: 1350 - total flux cleaned = -0.00287062 Jy ! Component: 1400 - total flux cleaned = -0.002683 Jy ! Component: 1450 - total flux cleaned = -0.00255889 Jy ! Component: 1500 - total flux cleaned = -0.00231194 Jy ! Component: 1550 - total flux cleaned = -0.00249688 Jy ! Component: 1600 - total flux cleaned = -0.00243478 Jy ! Component: 1650 - total flux cleaned = -0.00225239 Jy ! Component: 1700 - total flux cleaned = -0.00231271 Jy ! Component: 1750 - total flux cleaned = -0.00183148 Jy ! Component: 1800 - total flux cleaned = -0.00165164 Jy ! Component: 1850 - total flux cleaned = -0.001592 Jy ! Component: 1900 - total flux cleaned = -0.00153293 Jy ! Component: 1950 - total flux cleaned = -0.000944227 Jy ! Component: 2000 - total flux cleaned = -0.000768948 Jy ! Component: 2050 - total flux cleaned = -0.000360669 Jy ! Component: 2100 - total flux cleaned = -0.000303248 Jy ! Component: 2150 - total flux cleaned = -0.000188175 Jy ! Component: 2200 - total flux cleaned = -7.31064e-05 Jy ! Component: 2250 - total flux cleaned = 9.84603e-05 Jy ! Component: 2300 - total flux cleaned = 0.000553885 Jy ! Component: 2350 - total flux cleaned = 0.00049686 Jy ! Component: 2400 - total flux cleaned = 0.000609601 Jy ! Component: 2450 - total flux cleaned = 0.000890413 Jy ! Component: 2500 - total flux cleaned = 0.0010025 Jy ! Component: 2550 - total flux cleaned = 0.00122499 Jy ! Component: 2600 - total flux cleaned = 0.00155747 Jy ! Component: 2650 - total flux cleaned = 0.00205425 Jy ! Component: 2700 - total flux cleaned = 0.00194417 Jy ! Component: 2750 - total flux cleaned = 0.00205337 Jy ! Component: 2800 - total flux cleaned = 0.00205341 Jy ! Component: 2850 - total flux cleaned = 0.00248794 Jy ! Component: 2900 - total flux cleaned = 0.00286628 Jy ! Component: 2950 - total flux cleaned = 0.00302758 Jy ! Component: 3000 - total flux cleaned = 0.00308134 Jy ! Component: 3050 - total flux cleaned = 0.00334895 Jy ! Component: 3100 - total flux cleaned = 0.00350913 Jy ! Component: 3150 - total flux cleaned = 0.0039338 Jy ! Component: 3200 - total flux cleaned = 0.00377495 Jy ! Component: 3250 - total flux cleaned = 0.00419639 Jy ! Component: 3300 - total flux cleaned = 0.0043534 Jy ! Component: 3350 - total flux cleaned = 0.00440574 Jy ! Component: 3400 - total flux cleaned = 0.0045096 Jy ! Component: 3450 - total flux cleaned = 0.00456134 Jy ! Component: 3500 - total flux cleaned = 0.0047164 Jy ! Component: 3550 - total flux cleaned = 0.00481963 Jy ! Component: 3600 - total flux cleaned = 0.00487093 Jy ! Component: 3650 - total flux cleaned = 0.00497301 Jy ! Component: 3700 - total flux cleaned = 0.00507506 Jy ! Component: 3750 - total flux cleaned = 0.00502422 Jy ! Component: 3800 - total flux cleaned = 0.00532837 Jy ! Component: 3850 - total flux cleaned = 0.00537912 Jy ! Component: 3900 - total flux cleaned = 0.00573087 Jy ! Component: 3950 - total flux cleaned = 0.00578119 Jy ! Component: 4000 - total flux cleaned = 0.00568108 Jy ! Component: 4050 - total flux cleaned = 0.00573099 Jy ! Total flux subtracted in 4096 components = 0.00587993 Jy ! Clean residual min=-0.002597 max=0.003053 Jy/beam ! Clean residual mean=0.000010 rms=0.000830 Jy/beam ! Combined flux in latest and established models = 1.31497 Jy keep ! Adding 378 model components to the UV plane model. ! The established model now contains 487 components and 1.31497 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv119_uvs/J0205+3212_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7412 x 1.04 at 13.61 degrees (North through East) ! Clean map min=-0.0048822 max=1.0934 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv119_uvs/J0205+3212_X_map.fits wmodel /scr/pima/rv119_uvs/J0205+3212_X_map.mod ! Writing 487 model components to file: /scr/pima/rv119_uvs/J0205+3212_X_map.mod wobs /scr/pima/rv119_uvs/J0205+3212_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv119_uvs/J0205+3212_X_uvs.fits wwins /scr/pima/rv119_uvs/J0205+3212_X_map.win ! wwins: Wrote 9 windows to /scr/pima/rv119_uvs/J0205+3212_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 1.09335 invert ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.169 milli-arcsec ! The y-axis pixel size should ideally be below 0.1714 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000829179 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.227514 0.227514 0.455029 0.910058 1.82012 3.64023 7.28046 14.5609 29.1219 58.2437 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0024 print "peak= ", int(1000*peak_flux)/1000 ! peak= 1.093 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 1318.6 quit ! Quitting program ! Log file /scr/pima/rv119_uvs/J0205+3212_X_dfm.log closed on Sun Dec 17 11:32:16 2017