! Started logfile: /scr/pima/rv118_uvs/J0815+3635_X_dfm.log on Sun Dec 10 00:08:23 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/rv118_uvs/J0815+3635_X_uva.fits ! Reading UV FITS file: /scr/pima/rv118_uvs/J0815+3635_X_uva.fits ! AN table 1: 4 integrations on 15 of 15 possible baselines. ! AN table 2: 7 integrations on 3 of 3 possible baselines. ! AN table 3: 4 integrations on 45 of 45 possible baselines. ! AN table 4: 13 integrations on 1 of 1 possible baselines. ! AN table 5: 5 integrations on 21 of 21 possible baselines. ! AN table 6: 51 integrations on 66 of 66 possible baselines. ! Apparent sampling: 0.23231 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0815+3635 ! ! 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 3480 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 J0815+3635_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 9 telescope corrections were flagged in sub-array 2. ! A total of 8 telescope corrections were flagged in sub-array 3. ! A total of 26 telescope corrections were flagged in sub-array 4. ! A total of 21 telescope corrections were flagged in sub-array 5. ! A total of 460 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 9 telescope corrections were flagged in sub-array 2. ! A total of 8 telescope corrections were flagged in sub-array 3. ! A total of 26 telescope corrections were flagged in sub-array 4. ! A total of 21 telescope corrections were flagged in sub-array 5. ! A total of 460 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 9 telescope corrections were flagged in sub-array 2. ! A total of 8 telescope corrections were flagged in sub-array 3. ! A total of 26 telescope corrections were flagged in sub-array 4. ! A total of 21 telescope corrections were flagged in sub-array 5. ! A total of 460 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 9 telescope corrections were flagged in sub-array 2. ! A total of 8 telescope corrections were flagged in sub-array 3. ! A total of 26 telescope corrections were flagged in sub-array 4. ! A total of 21 telescope corrections were flagged in sub-array 5. ! A total of 460 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.180492Jy sigma=15.568633 ! Fit after self-cal, rms=0.444327Jy sigma=5.481399 ! 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 6.62% of the data. ! The x-axis pixel size should ideally be below 0.185 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec ! Estimated beam: bmin=0.6172 mas, bmaj=0.8235 mas, bpa=10.35 degrees ! Estimated noise=1.41322 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 = 0.455984 Jy ! Component: 100 - total flux cleaned = 0.585912 Jy ! Total flux subtracted in 100 components = 0.585912 Jy ! Clean residual min=-0.016153 max=0.057428 Jy/beam ! Clean residual mean=-0.000019 rms=0.004098 Jy/beam ! Combined flux in latest and established models = 0.585912 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.585912 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.137878Jy sigma=1.761440 ! Fit after self-cal, rms=0.137648Jy sigma=1.756662 ! Inverting map ! Your choice of large map pixels excluded 6.62% of the data. ! The x-axis pixel size should ideally be below 0.185 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0619983 Jy ! Component: 100 - total flux cleaned = 0.0927992 Jy ! Total flux subtracted in 100 components = 0.0927992 Jy ! Clean residual min=-0.014499 max=0.034620 Jy/beam ! Clean residual mean=-0.000006 rms=0.002613 Jy/beam ! Combined flux in latest and established models = 0.678711 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 13 components and 0.678711 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.110026Jy sigma=1.230151 ! Fit after self-cal, rms=0.109847Jy sigma=1.225467 ! Inverting map ! Your choice of large map pixels excluded 6.62% of the data. ! The x-axis pixel size should ideally be below 0.185 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec ! Added new window around map position (-0.4, 1). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0298949 Jy ! Component: 100 - total flux cleaned = 0.0416306 Jy ! Total flux subtracted in 100 components = 0.0416306 Jy ! Clean residual min=-0.012043 max=0.012798 Jy/beam ! Clean residual mean=-0.000000 rms=0.002173 Jy/beam ! Combined flux in latest and established models = 0.720342 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 16 components and 0.720342 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.101869Jy sigma=1.093234 ! Fit after self-cal, rms=0.100290Jy sigma=1.074418 ! Inverting map ! Your choice of large map pixels excluded 6.62% of the data. ! The x-axis pixel size should ideally be below 0.185 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 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 6.62% of the data. ! The x-axis pixel size should ideally be below 0.185 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec ! Estimated beam: bmin=0.699 mas, bmaj=0.9123 mas, bpa=8.846 degrees ! Estimated noise=1.113 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 = 0.0118782 Jy ! Component: 100 - total flux cleaned = 0.015173 Jy ! Component: 150 - total flux cleaned = 0.0159861 Jy ! Component: 200 - total flux cleaned = 0.0164183 Jy ! Total flux subtracted in 200 components = 0.0164183 Jy ! Clean residual min=-0.009241 max=0.010010 Jy/beam ! Clean residual mean=-0.000004 rms=0.001862 Jy/beam ! Combined flux in latest and established models = 0.73676 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 27 components and 0.73676 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.098845Jy sigma=1.051955 ! Fit after self-cal, rms=0.098382Jy sigma=1.048355 ! Inverting map ! Your choice of large map pixels excluded 6.62% of the data. ! The x-axis pixel size should ideally be below 0.185 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec ! Added new window around map position (-0.6, 2.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00915289 Jy ! Component: 100 - total flux cleaned = 0.0113749 Jy ! Component: 150 - total flux cleaned = 0.0124188 Jy ! Component: 200 - total flux cleaned = 0.0134657 Jy ! Total flux subtracted in 200 components = 0.0134657 Jy ! Clean residual min=-0.008298 max=0.009044 Jy/beam ! Clean residual mean=0.000003 rms=0.001729 Jy/beam ! Combined flux in latest and established models = 0.750226 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 40 components and 0.750226 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.097237Jy sigma=1.028937 ! Fit after self-cal, rms=0.097110Jy sigma=1.027183 ! Inverting map ! Your choice of large map pixels excluded 6.62% of the data. ! The x-axis pixel size should ideally be below 0.185 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.699 x 0.9123 at 8.846 degrees (North through East) ! Clean map min=-0.0068913 max=0.56914 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 KP 0.98 LA 0.98 ON 1.04 ! OV 1.00 PT 0.94 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! MK 0.00* NY 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 FD 1.04 HN 1.01 KK 0.96 ! KP 0.98 NL 0.97 NY 0.98 OV 0.99 ! PT 1.00 SC 1.01 ! ! Telescope amplitude corrections in sub-array 4: ! KK 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 KK 1.05 KP 0.98 LA 1.04 ! NL 0.84 OV 1.00 PT 1.01 ! ! A total of 30 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.08 FD 0.97 HH 1.00 HN 1.04 ! KP 1.03 LA 1.01 NL 1.02 NY 1.01 ! ON 0.97 PT 0.99 SC 0.98 WZ 0.97 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.04 KP 0.96 LA 0.98 ON 1.04 ! OV 1.01 PT 0.96 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! MK 0.00* NY 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 1.04 HN 1.01 KK 0.96 ! KP 0.99 NL 0.96 NY 1.05 OV 0.98 ! PT 1.01 SC 0.98 ! ! Telescope amplitude corrections in sub-array 4: ! KK 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 KK 0.90 KP 1.00 LA 0.98 ! NL 0.80 OV 1.02 PT 1.05 ! ! A total of 30 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.06 FD 0.98 HH 1.03 HN 1.02 ! KP 1.03 LA 1.00 NL 1.03 NY 1.01 ! ON 1.00 PT 1.01 SC 0.98 WZ 0.97 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 KP 0.97 LA 0.97 ON 1.02 ! OV 0.99 PT 0.97 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! MK 0.00* NY 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 FD 1.06 HN 1.04 KK 1.01 ! KP 0.96 NL 0.94 NY 0.98 OV 0.97 ! PT 0.99 SC 0.93 ! ! Telescope amplitude corrections in sub-array 4: ! KK 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 KK 1.00 KP 1.00 LA 1.02 ! NL 0.80 OV 0.98 PT 1.05 ! ! A total of 30 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.05 FD 0.98 HH 0.99 HN 1.01 ! KP 1.03 LA 1.01 NL 1.03 NY 1.01 ! ON 1.01 PT 1.02 SC 0.96 WZ 0.97 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 KP 0.96 LA 0.95 ON 1.06 ! OV 0.99 PT 0.92 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! MK 0.00* NY 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 FD 1.06 HN 1.00 KK 1.00 ! KP 0.97 NL 0.95 NY 1.02 OV 1.03 ! PT 1.00 SC 0.95 ! ! Telescope amplitude corrections in sub-array 4: ! KK 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 KK 1.04 KP 0.94 LA 1.05 ! NL 0.80 OV 1.03 PT 1.04 ! ! A total of 30 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.07 FD 1.00 HH 1.12 HN 1.02 ! KP 1.02 LA 1.00 NL 1.03 NY 1.01 ! ON 1.00 PT 1.04 SC 1.00 WZ 0.96 ! ! ! Fit before self-cal, rms=0.097110Jy sigma=1.027183 ! Fit after self-cal, rms=0.092953Jy sigma=0.951408 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec ! Estimated beam: bmin=0.6912 mas, bmaj=0.9167 mas, bpa=10.59 degrees ! Estimated noise=1.13412 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 = 0.000763891 Jy ! Component: 100 - total flux cleaned = 0.00186753 Jy ! Component: 150 - total flux cleaned = 0.00208976 Jy ! Component: 200 - total flux cleaned = 0.00229036 Jy ! Total flux subtracted in 200 components = 0.00229036 Jy ! Clean residual min=-0.006335 max=0.005907 Jy/beam ! Clean residual mean=-0.000011 rms=0.001300 Jy/beam ! Combined flux in latest and established models = 0.752516 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 47 components and 0.752516 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.092446Jy sigma=0.946362 ! Fit after self-cal, rms=0.092312Jy sigma=0.945496 ! Inverting map ! Your choice of large map pixels excluded 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 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=0.092312Jy sigma=0.945496 ! Fit after self-cal, rms=0.090340Jy sigma=0.919128 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec ! Estimated beam: bmin=0.6937 mas, bmaj=0.9149 mas, bpa=9.796 degrees ! Estimated noise=1.13377 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00221873 Jy ! Component: 100 - total flux cleaned = 0.00260657 Jy ! Component: 150 - total flux cleaned = 0.00261032 Jy ! Component: 200 - total flux cleaned = 0.00289197 Jy ! Total flux subtracted in 200 components = 0.00289197 Jy ! Clean residual min=-0.005222 max=0.005276 Jy/beam ! Clean residual mean=-0.000010 rms=0.001153 Jy/beam ! Combined flux in latest and established models = 0.755408 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 58 components and 0.755408 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.089982Jy sigma=0.915132 ! Fit after self-cal, rms=0.089858Jy sigma=0.914602 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 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 (3.2, 6.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00445036 Jy ! Component: 100 - total flux cleaned = 0.00469845 Jy ! Component: 150 - total flux cleaned = 0.00524169 Jy ! Component: 200 - total flux cleaned = 0.00544423 Jy ! Total flux subtracted in 200 components = 0.00544423 Jy ! Clean residual min=-0.005190 max=0.004982 Jy/beam ! Clean residual mean=-0.000008 rms=0.001115 Jy/beam ! Combined flux in latest and established models = 0.760852 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 69 components and 0.760852 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.089450Jy sigma=0.909975 ! Fit after self-cal, rms=0.089360Jy sigma=0.909663 ! Inverting map ! Your choice of large map pixels excluded 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 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=0.089360Jy sigma=0.909663 ! Fit after self-cal, rms=0.089018Jy sigma=0.902890 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec ! Estimated beam: bmin=0.6944 mas, bmaj=0.9151 mas, bpa=9.621 degrees ! Estimated noise=1.13227 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000838581 Jy ! Component: 100 - total flux cleaned = 0.00112739 Jy ! Component: 150 - total flux cleaned = 0.00121464 Jy ! Component: 200 - total flux cleaned = 0.0013832 Jy ! Total flux subtracted in 200 components = 0.0013832 Jy ! Clean residual min=-0.004867 max=0.004877 Jy/beam ! Clean residual mean=-0.000009 rms=0.001078 Jy/beam ! Combined flux in latest and established models = 0.762235 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 75 components and 0.762235 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.088783Jy sigma=0.900622 ! Fit after self-cal, rms=0.088709Jy sigma=0.900416 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 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 = 0.000316445 Jy ! Component: 100 - total flux cleaned = 0.000481894 Jy ! Component: 150 - total flux cleaned = 0.000561566 Jy ! Component: 200 - total flux cleaned = 0.000711209 Jy ! Total flux subtracted in 200 components = 0.000711209 Jy ! Clean residual min=-0.004777 max=0.004798 Jy/beam ! Clean residual mean=-0.000009 rms=0.001069 Jy/beam ! Combined flux in latest and established models = 0.762947 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 78 components and 0.762947 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.088546Jy sigma=0.898847 ! Fit after self-cal, rms=0.088453Jy sigma=0.898695 ! Inverting map ! Your choice of large map pixels excluded 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 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=0.088453Jy sigma=0.898695 ! Fit after self-cal, rms=0.088547Jy sigma=0.898551 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec ! Estimated beam: bmin=2.362 mas, bmaj=2.999 mas, bpa=-82.51 degrees ! Estimated noise=1.55295 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00222758 Jy ! Component: 100 - total flux cleaned = 0.00259049 Jy ! Component: 150 - total flux cleaned = 0.00273236 Jy ! Component: 200 - total flux cleaned = 0.00284645 Jy ! Total flux subtracted in 200 components = 0.00284645 Jy ! Clean residual min=-0.006367 max=0.006868 Jy/beam ! Clean residual mean=-0.000025 rms=0.001520 Jy/beam ! Combined flux in latest and established models = 0.765793 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 88 components and 0.765793 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.088565Jy sigma=0.898631 ! Fit after self-cal, rms=0.088571Jy sigma=0.898505 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 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 (-1.6, 9). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00669488 Jy ! Component: 100 - total flux cleaned = 0.0104782 Jy ! Component: 150 - total flux cleaned = 0.0130513 Jy ! Component: 200 - total flux cleaned = 0.0141534 Jy ! Total flux subtracted in 200 components = 0.0141534 Jy ! Clean residual min=-0.004995 max=0.005152 Jy/beam ! Clean residual mean=-0.000007 rms=0.001224 Jy/beam ! Combined flux in latest and established models = 0.779947 Jy ! Performing phase self-cal ! Adding 36 model components to the UV plane model. ! The established model now contains 123 components and 0.779946 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.088267Jy sigma=0.893742 ! Fit after self-cal, rms=0.088228Jy sigma=0.893359 ! Inverting map ! Your choice of large map pixels excluded 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 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 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec ! Estimated beam: bmin=0.6948 mas, bmaj=0.9154 mas, bpa=9.489 degrees ! Estimated noise=1.13149 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6948 x 0.9154 at 9.489 degrees (North through East) ! Clean map min=-0.0050458 max=0.56565 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=0.088228Jy sigma=0.893359 ! Fit after self-cal, rms=0.083477Jy sigma=0.816972 ! Inverting map and beam ! Your choice of large map pixels excluded 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec ! Estimated beam: bmin=0.6947 mas, bmaj=0.9159 mas, bpa=9.475 degrees ! Estimated noise=1.13207 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00179203 Jy ! Component: 100 - total flux cleaned = 0.0028769 Jy ! Component: 150 - total flux cleaned = 0.00336451 Jy ! Component: 200 - total flux cleaned = 0.00358981 Jy ! Total flux subtracted in 200 components = 0.00358981 Jy ! Clean residual min=-0.004443 max=0.003992 Jy/beam ! Clean residual mean=-0.000003 rms=0.000949 Jy/beam ! Combined flux in latest and established models = 0.783536 Jy ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 146 components and 0.783536 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.082992Jy sigma=0.811398 ! Fit after self-cal, rms=0.082924Jy sigma=0.811221 ! Inverting map ! Your choice of large map pixels excluded 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 9.90821e-05 Jy ! Component: 100 - total flux cleaned = 0.000202381 Jy ! Component: 150 - total flux cleaned = 0.000204291 Jy ! Component: 200 - total flux cleaned = 0.000297335 Jy ! Total flux subtracted in 200 components = 0.000297335 Jy ! Clean residual min=-0.004420 max=0.003969 Jy/beam ! Clean residual mean=-0.000003 rms=0.000933 Jy/beam ! Combined flux in latest and established models = 0.783834 Jy ! Performing phase self-cal ! Adding 46 model components to the UV plane model. ! The established model now contains 162 components and 0.783834 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.082639Jy sigma=0.808203 ! Fit after self-cal, rms=0.082594Jy sigma=0.808117 ! Inverting map ! Your choice of large map pixels excluded 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.082594Jy sigma=0.808117 ! Fit after self-cal, rms=0.082424Jy sigma=0.807636 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 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec ! Estimated beam: bmin=0.6168 mas, bmaj=0.8262 mas, bpa=10.57 degrees ! Estimated noise=1.43999 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.450829 Jy ! Component: 100 - total flux cleaned = 0.583167 Jy ! Component: 150 - total flux cleaned = 0.647836 Jy ! Component: 200 - total flux cleaned = 0.683384 Jy ! Total flux subtracted in 200 components = 0.683384 Jy ! Clean residual min=-0.009065 max=0.017282 Jy/beam ! Clean residual mean=-0.000005 rms=0.001860 Jy/beam ! Combined flux in latest and established models = 0.683384 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 0.683384 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec ! Estimated beam: bmin=0.6948 mas, bmaj=0.9161 mas, bpa=9.483 degrees ! Estimated noise=1.13076 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 = 0.0253542 Jy ! Component: 100 - total flux cleaned = 0.0396556 Jy ! Component: 150 - total flux cleaned = 0.049759 Jy ! Component: 200 - total flux cleaned = 0.0577699 Jy ! Total flux subtracted in 200 components = 0.0577699 Jy ! Clean residual min=-0.005678 max=0.006389 Jy/beam ! Clean residual mean=-0.000024 rms=0.001260 Jy/beam ! Combined flux in latest and established models = 0.741154 Jy ! Adding 30 model components to the UV plane model. ! The established model now contains 35 components and 0.741154 Jy ! Inverting map ! Your choice of large map pixels excluded 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec ! Added new window around map position (1.2, -0.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00717222 Jy ! Component: 100 - total flux cleaned = 0.0131964 Jy ! Component: 150 - total flux cleaned = 0.0184857 Jy ! Component: 200 - total flux cleaned = 0.0231653 Jy ! Total flux subtracted in 200 components = 0.0231653 Jy ! Clean residual min=-0.004919 max=0.004495 Jy/beam ! Clean residual mean=-0.000012 rms=0.001047 Jy/beam ! Combined flux in latest and established models = 0.764319 Jy ! Adding 40 model components to the UV plane model. ! The established model now contains 58 components and 0.764319 Jy ! Inverting map ! Your choice of large map pixels excluded 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 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 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec ! Estimated beam: bmin=2.361 mas, bmaj=3 mas, bpa=-82.45 degrees ! Estimated noise=1.55091 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00655797 Jy ! Component: 100 - total flux cleaned = 0.0109413 Jy ! Component: 150 - total flux cleaned = 0.0142066 Jy ! Component: 200 - total flux cleaned = 0.0166924 Jy ! Total flux subtracted in 200 components = 0.0166924 Jy ! Clean residual min=-0.004656 max=0.004870 Jy/beam ! Clean residual mean=-0.000013 rms=0.001157 Jy/beam ! Combined flux in latest and established models = 0.781012 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 = 0.00196095 Jy ! Component: 100 - total flux cleaned = 0.00318019 Jy ! Component: 150 - total flux cleaned = 0.00377791 Jy ! Component: 200 - total flux cleaned = 0.00420728 Jy ! Total flux subtracted in 200 components = 0.00420728 Jy ! Clean residual min=-0.004484 max=0.004739 Jy/beam ! Clean residual mean=-0.000007 rms=0.001118 Jy/beam ! Combined flux in latest and established models = 0.785219 Jy ! Adding 64 model components to the UV plane model. ! The established model now contains 114 components and 0.785219 Jy ! Inverting map ! Your choice of large map pixels excluded 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec ! Estimated beam: bmin=0.6948 mas, bmaj=0.9161 mas, bpa=9.483 degrees ! Estimated noise=1.13076 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00115548 Jy ! Component: 100 - total flux cleaned = -0.000655567 Jy ! Component: 150 - total flux cleaned = -0.000534713 Jy ! Component: 200 - total flux cleaned = -0.00042357 Jy ! Total flux subtracted in 200 components = -0.00042357 Jy ! Clean residual min=-0.004323 max=0.003910 Jy/beam ! Clean residual mean=-0.000003 rms=0.000944 Jy/beam ! Combined flux in latest and established models = 0.784795 Jy selfcal ! Performing phase self-cal ! Adding 32 model components to the UV plane model. ! The established model now contains 142 components and 0.784795 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.082095Jy sigma=0.809412 ! Fit after self-cal, rms=0.082020Jy sigma=0.808093 wmodel J0815+3635_X_map.mod ! Writing 142 model components to file: J0815+3635_X_map.mod wobs J0815+3635_X_uvs.fits ! Writing UV FITS file: J0815+3635_X_uvs.fits wwins J0815+3635_X_map.win ! wwins: Wrote 6 windows to J0815+3635_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 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000628633 Jy ! Component: 100 - total flux cleaned = -0.00113359 Jy ! Component: 150 - total flux cleaned = -0.00141297 Jy ! Component: 200 - total flux cleaned = -0.00147956 Jy ! Component: 250 - total flux cleaned = -0.0012791 Jy ! Component: 300 - total flux cleaned = -0.00140956 Jy ! Component: 350 - total flux cleaned = -0.00140725 Jy ! Component: 400 - total flux cleaned = -0.00153155 Jy ! Component: 450 - total flux cleaned = -0.00146893 Jy ! Component: 500 - total flux cleaned = -0.00177819 Jy ! Component: 550 - total flux cleaned = -0.00183961 Jy ! Component: 600 - total flux cleaned = -0.0026259 Jy ! Component: 650 - total flux cleaned = -0.00280378 Jy ! Component: 700 - total flux cleaned = -0.00321795 Jy ! Component: 750 - total flux cleaned = -0.00351096 Jy ! Component: 800 - total flux cleaned = -0.0037428 Jy ! Component: 850 - total flux cleaned = -0.00414414 Jy ! Component: 900 - total flux cleaned = -0.00442774 Jy ! Component: 950 - total flux cleaned = -0.00470868 Jy ! Component: 1000 - total flux cleaned = -0.00476351 Jy ! Component: 1050 - total flux cleaned = -0.00476389 Jy ! Component: 1100 - total flux cleaned = -0.0050386 Jy ! Component: 1150 - total flux cleaned = -0.0053101 Jy ! Component: 1200 - total flux cleaned = -0.0054174 Jy ! Component: 1250 - total flux cleaned = -0.00547064 Jy ! Component: 1300 - total flux cleaned = -0.00557737 Jy ! Component: 1350 - total flux cleaned = -0.00568319 Jy ! Component: 1400 - total flux cleaned = -0.00594357 Jy ! Component: 1450 - total flux cleaned = -0.0059959 Jy ! Component: 1500 - total flux cleaned = -0.00609898 Jy ! Component: 1550 - total flux cleaned = -0.00620126 Jy ! Component: 1600 - total flux cleaned = -0.00645316 Jy ! Component: 1650 - total flux cleaned = -0.00630269 Jy ! Component: 1700 - total flux cleaned = -0.00635268 Jy ! Component: 1750 - total flux cleaned = -0.00659972 Jy ! Component: 1800 - total flux cleaned = -0.00664822 Jy ! Component: 1850 - total flux cleaned = -0.00684246 Jy ! Component: 1900 - total flux cleaned = -0.0067942 Jy ! Component: 1950 - total flux cleaned = -0.0070345 Jy ! Component: 2000 - total flux cleaned = -0.00713032 Jy ! Component: 2050 - total flux cleaned = -0.00741472 Jy ! Component: 2100 - total flux cleaned = -0.00750895 Jy ! Component: 2150 - total flux cleaned = -0.00746175 Jy ! Component: 2200 - total flux cleaned = -0.00764768 Jy ! Component: 2250 - total flux cleaned = -0.00797033 Jy ! Component: 2300 - total flux cleaned = -0.00797031 Jy ! Component: 2350 - total flux cleaned = -0.0081073 Jy ! Component: 2400 - total flux cleaned = -0.00828826 Jy ! Component: 2450 - total flux cleaned = -0.00842303 Jy ! Component: 2500 - total flux cleaned = -0.00860193 Jy ! Component: 2550 - total flux cleaned = -0.00851294 Jy ! Component: 2600 - total flux cleaned = -0.00869017 Jy ! Component: 2650 - total flux cleaned = -0.00895458 Jy ! Component: 2700 - total flux cleaned = -0.00891046 Jy ! Component: 2750 - total flux cleaned = -0.00891052 Jy ! Component: 2800 - total flux cleaned = -0.00899741 Jy ! Component: 2850 - total flux cleaned = -0.00908334 Jy ! Component: 2900 - total flux cleaned = -0.00934055 Jy ! Component: 2950 - total flux cleaned = -0.00946854 Jy ! Component: 3000 - total flux cleaned = -0.00925659 Jy ! Component: 3050 - total flux cleaned = -0.00946771 Jy ! Component: 3100 - total flux cleaned = -0.00955112 Jy ! Component: 3150 - total flux cleaned = -0.00950939 Jy ! Component: 3200 - total flux cleaned = -0.00955124 Jy ! Component: 3250 - total flux cleaned = -0.0095924 Jy ! Component: 3300 - total flux cleaned = -0.00951003 Jy ! Component: 3350 - total flux cleaned = -0.00975613 Jy ! Component: 3400 - total flux cleaned = -0.00967443 Jy ! Component: 3450 - total flux cleaned = -0.00959327 Jy ! Component: 3500 - total flux cleaned = -0.00983565 Jy ! Component: 3550 - total flux cleaned = -0.0095947 Jy ! Component: 3600 - total flux cleaned = -0.00975469 Jy ! Component: 3650 - total flux cleaned = -0.00971489 Jy ! Component: 3700 - total flux cleaned = -0.00975468 Jy ! Component: 3750 - total flux cleaned = -0.00987292 Jy ! Component: 3800 - total flux cleaned = -0.00971568 Jy ! Component: 3850 - total flux cleaned = -0.00979401 Jy ! Component: 3900 - total flux cleaned = -0.00987169 Jy ! Component: 3950 - total flux cleaned = -0.00987165 Jy ! Component: 4000 - total flux cleaned = -0.00998729 Jy ! Component: 4050 - total flux cleaned = -0.00998737 Jy ! Total flux subtracted in 4096 components = -0.00991086 Jy ! Clean residual min=-0.002066 max=0.002294 Jy/beam ! Clean residual mean=-0.000003 rms=0.000618 Jy/beam ! Combined flux in latest and established models = 0.774884 Jy keep ! Adding 344 model components to the UV plane model. ! The established model now contains 486 components and 0.774884 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv118_uvs/J0815+3635_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6948 x 0.9161 at 9.483 degrees (North through East) ! Clean map min=-0.0027553 max=0.56521 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv118_uvs/J0815+3635_X_map.fits wmodel /scr/pima/rv118_uvs/J0815+3635_X_map.mod ! Writing 486 model components to file: /scr/pima/rv118_uvs/J0815+3635_X_map.mod wobs /scr/pima/rv118_uvs/J0815+3635_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv118_uvs/J0815+3635_X_uvs.fits wwins /scr/pima/rv118_uvs/J0815+3635_X_map.win ! wwins: Wrote 7 windows to /scr/pima/rv118_uvs/J0815+3635_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.565213 invert ! Inverting map ! Your choice of large map pixels excluded 6.08% of the data. ! The x-axis pixel size should ideally be below 0.1921 milli-arcsec ! The y-axis pixel size should ideally be below 0.1676 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000616899 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.327433 0.327433 0.654867 1.30973 2.61947 5.23893 10.4779 20.9557 41.9115 83.823 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0018 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.565 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 916.216 quit ! Quitting program ! Log file /scr/pima/rv118_uvs/J0815+3635_X_dfm.log closed on Sun Dec 10 00:08:28 2017