! Started logfile: /scr/pima/rv118_uvs/J0019+7327_X_dfm.log on Sun Dec 10 00:06:29 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/J0019+7327_X_uva.fits ! Reading UV FITS file: /scr/pima/rv118_uvs/J0019+7327_X_uva.fits ! AN table 1: 52 integrations on 78 of 78 possible baselines. ! AN table 2: 8 integrations on 36 of 36 possible baselines. ! AN table 3: 10 integrations on 6 of 6 possible baselines. ! Apparent sampling: 0.45277 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0019+7327 ! ! 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 7976 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 J0019+7327_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 275 telescope corrections were flagged in sub-array 1. ! A total of 32 telescope corrections were flagged in sub-array 2. ! A total of 18 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 275 telescope corrections were flagged in sub-array 1. ! A total of 32 telescope corrections were flagged in sub-array 2. ! A total of 18 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 275 telescope corrections were flagged in sub-array 1. ! A total of 32 telescope corrections were flagged in sub-array 2. ! A total of 18 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 275 telescope corrections were flagged in sub-array 1. ! A total of 32 telescope corrections were flagged in sub-array 2. ! A total of 18 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=2.363715Jy sigma=23.079433 ! Fit after self-cal, rms=1.203007Jy sigma=12.019738 ! 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 1.21% of the data. ! The x-axis pixel size should ideally be below 0.1844 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec ! Estimated beam: bmin=0.6762 mas, bmaj=0.7214 mas, bpa=74.82 degrees ! Estimated noise=1.25724 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (0, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.59017 Jy ! Component: 100 - total flux cleaned = 1.99327 Jy ! Total flux subtracted in 100 components = 1.99327 Jy ! Clean residual min=-0.034773 max=0.164093 Jy/beam ! Clean residual mean=0.000013 rms=0.008374 Jy/beam ! Combined flux in latest and established models = 1.99327 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 1.99327 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.466243Jy sigma=4.960274 ! Fit after self-cal, rms=0.465863Jy sigma=4.955937 ! Inverting map ! Your choice of large map pixels excluded 1.21% of the data. ! The x-axis pixel size should ideally be below 0.1844 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.17665 Jy ! Component: 100 - total flux cleaned = 0.274214 Jy ! Total flux subtracted in 100 components = 0.274214 Jy ! Clean residual min=-0.028092 max=0.048239 Jy/beam ! Clean residual mean=-0.000005 rms=0.006182 Jy/beam ! Combined flux in latest and established models = 2.26748 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 13 components and 2.26749 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.382352Jy sigma=4.214610 ! Fit after self-cal, rms=0.382321Jy sigma=4.214386 ! Inverting map ! Your choice of large map pixels excluded 1.21% of the data. ! The x-axis pixel size should ideally be below 0.1844 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0576718 Jy ! Component: 100 - total flux cleaned = 0.0939931 Jy ! Total flux subtracted in 100 components = 0.0939931 Jy ! Clean residual min=-0.026608 max=0.029879 Jy/beam ! Clean residual mean=-0.000011 rms=0.005889 Jy/beam ! Combined flux in latest and established models = 2.36148 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 18 components and 2.36148 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.371897Jy sigma=4.131974 ! Fit after self-cal, rms=0.371860Jy sigma=4.131810 ! Inverting map ! Your choice of large map pixels excluded 1.21% of the data. ! The x-axis pixel size should ideally be below 0.1844 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 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 1.21% of the data. ! The x-axis pixel size should ideally be below 0.1844 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec ! Estimated beam: bmin=0.7308 mas, bmaj=0.8859 mas, bpa=62.32 degrees ! Estimated noise=0.874167 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 = 0.0254174 Jy ! Component: 100 - total flux cleaned = 0.03799 Jy ! Component: 150 - total flux cleaned = 0.0437953 Jy ! Component: 200 - total flux cleaned = 0.0453374 Jy ! Total flux subtracted in 200 components = 0.0453374 Jy ! Clean residual min=-0.036689 max=0.035315 Jy/beam ! Clean residual mean=-0.000021 rms=0.007254 Jy/beam ! Combined flux in latest and established models = 2.40682 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 24 components and 2.40682 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.370153Jy sigma=4.116882 ! Fit after self-cal, rms=0.370075Jy sigma=4.116315 ! Inverting map ! Your choice of large map pixels excluded 1.21% of the data. ! The x-axis pixel size should ideally be below 0.1844 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7308 x 0.8859 at 62.32 degrees (North through East) ! Clean map min=-0.032268 max=2.0723 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 30 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 1.00 HN 1.00 KK 0.95 ! KP 0.98 LA 0.99 MK 1.12 NL 0.96 ! NY 0.98 ON 1.01 OV 0.98 PT 1.15 ! SC 1.02 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 1.06 HN 0.97 KK 1.13 ! LA 0.98 NL 0.95 PT 0.99 SC 1.11 ! WZ 0.98 ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! KK 1.07 NY 0.99 ON 1.01 WZ 0.98 ! ! ! Correcting IF 2. ! A total of 30 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 1.00 HN 1.00 KK 0.97 ! KP 0.98 LA 0.98 MK 1.13 NL 0.98 ! NY 0.97 ON 1.03 OV 0.98 PT 1.10 ! SC 1.01 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 1.04 HN 0.97 KK 1.13 ! LA 0.98 NL 0.96 PT 0.99 SC 1.09 ! WZ 0.97 ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! KK 1.10 NY 1.00 ON 1.00 WZ 0.98 ! ! ! Correcting IF 3. ! A total of 30 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 1.01 HN 0.99 KK 0.98 ! KP 0.97 LA 0.98 MK 1.09 NL 0.98 ! NY 0.97 ON 1.03 OV 0.98 PT 1.10 ! SC 1.03 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 1.08 HN 0.97 KK 1.17 ! LA 0.98 NL 0.97 PT 0.97 SC 1.12 ! WZ 0.98 ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! KK 1.10 NY 1.00 ON 1.02 WZ 0.99 ! ! ! Correcting IF 4. ! A total of 30 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 1.00 HN 0.98 KK 0.97 ! KP 0.97 LA 0.98 MK 1.09 NL 0.98 ! NY 0.97 ON 1.03 OV 1.00 PT 1.12 ! SC 1.02 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 1.03 HN 0.98 KK 1.18 ! LA 0.98 NL 0.96 PT 0.97 SC 1.09 ! WZ 0.99 ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! KK 1.10 NY 1.00 ON 1.01 WZ 0.99 ! ! ! Fit before self-cal, rms=0.370075Jy sigma=4.116315 ! Fit after self-cal, rms=0.391529Jy sigma=3.951937 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec ! Estimated beam: bmin=0.7323 mas, bmaj=0.8977 mas, bpa=62.24 degrees ! Estimated noise=0.88575 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 = 0.0020174 Jy ! Component: 100 - total flux cleaned = 0.003469 Jy ! Component: 150 - total flux cleaned = 0.00347697 Jy ! Component: 200 - total flux cleaned = 0.00364306 Jy ! Total flux subtracted in 200 components = 0.00364306 Jy ! Clean residual min=-0.021305 max=0.025357 Jy/beam ! Clean residual mean=0.000002 rms=0.005350 Jy/beam ! Combined flux in latest and established models = 2.41046 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 33 components and 2.41046 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.390939Jy sigma=3.949770 ! Fit after self-cal, rms=0.390915Jy sigma=3.949500 ! Inverting map ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 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=0.390915Jy sigma=3.949500 ! Fit after self-cal, rms=0.397328Jy sigma=3.655234 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec ! Estimated beam: bmin=0.7321 mas, bmaj=0.8979 mas, bpa=62.42 degrees ! Estimated noise=0.8876 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00265068 Jy ! Component: 100 - total flux cleaned = 0.00286036 Jy ! Component: 150 - total flux cleaned = 0.00286476 Jy ! Component: 200 - total flux cleaned = 0.00276076 Jy ! Total flux subtracted in 200 components = 0.00276076 Jy ! Clean residual min=-0.019922 max=0.020544 Jy/beam ! Clean residual mean=0.000027 rms=0.004422 Jy/beam ! Combined flux in latest and established models = 2.41322 Jy selfcal ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 38 components and 2.41322 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.397085Jy sigma=3.655159 ! Fit after self-cal, rms=0.397081Jy sigma=3.655089 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 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 (-43.8, -14.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00423691 Jy ! Component: 100 - total flux cleaned = 0.00485811 Jy ! Component: 150 - total flux cleaned = 0.00397586 Jy ! Component: 200 - total flux cleaned = 0.00462334 Jy ! Total flux subtracted in 200 components = 0.00462334 Jy ! Clean residual min=-0.018536 max=0.020392 Jy/beam ! Clean residual mean=0.000026 rms=0.004368 Jy/beam ! Combined flux in latest and established models = 2.41784 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 59 components and 2.41784 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.395763Jy sigma=3.639878 ! Fit after self-cal, rms=0.395663Jy sigma=3.638365 ! Inverting map ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec ! Added new window around map position (45.8, 10.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00193192 Jy ! Component: 100 - total flux cleaned = 0.00250011 Jy ! Component: 150 - total flux cleaned = 0.0042758 Jy ! Component: 200 - total flux cleaned = 0.00501107 Jy ! Total flux subtracted in 200 components = 0.00501107 Jy ! Clean residual min=-0.018768 max=0.018986 Jy/beam ! Clean residual mean=0.000024 rms=0.004307 Jy/beam ! Combined flux in latest and established models = 2.42285 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 77 components and 2.42285 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.394201Jy sigma=3.625019 ! Fit after self-cal, rms=0.394152Jy sigma=3.624091 ! Inverting map ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec ! Added new window around map position (-38.2, 10). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00347507 Jy ! Component: 100 - total flux cleaned = 0.0023318 Jy ! Component: 150 - total flux cleaned = 0.00270497 Jy ! Component: 200 - total flux cleaned = 0.00272104 Jy ! Total flux subtracted in 200 components = 0.00272104 Jy ! Clean residual min=-0.018615 max=0.018183 Jy/beam ! Clean residual mean=0.000024 rms=0.004246 Jy/beam ! Combined flux in latest and established models = 2.42558 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 97 components and 2.42558 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.392495Jy sigma=3.609879 ! Fit after self-cal, rms=0.392407Jy sigma=3.608813 ! Inverting map ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec ! Added new window around map position (-43.6, 12.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00722041 Jy ! Component: 100 - total flux cleaned = 0.00827371 Jy ! Component: 150 - total flux cleaned = 0.00825615 Jy ! Component: 200 - total flux cleaned = 0.00824188 Jy ! Total flux subtracted in 200 components = 0.00824188 Jy ! Clean residual min=-0.018391 max=0.017150 Jy/beam ! Clean residual mean=0.000020 rms=0.004185 Jy/beam ! Combined flux in latest and established models = 2.43382 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 114 components and 2.43382 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.391199Jy sigma=3.594630 ! Fit after self-cal, rms=0.391149Jy sigma=3.593827 ! Inverting map ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 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=0.391149Jy sigma=3.593827 ! Fit after self-cal, rms=0.391118Jy sigma=3.584659 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec ! Estimated beam: bmin=0.7321 mas, bmaj=0.8982 mas, bpa=62.38 degrees ! Estimated noise=0.890587 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00781449 Jy ! Component: 100 - total flux cleaned = 0.00994774 Jy ! Component: 150 - total flux cleaned = 0.0111256 Jy ! Component: 200 - total flux cleaned = 0.0122524 Jy ! Total flux subtracted in 200 components = 0.0122524 Jy ! Clean residual min=-0.018892 max=0.018153 Jy/beam ! Clean residual mean=0.000021 rms=0.004119 Jy/beam ! Combined flux in latest and established models = 2.44607 Jy selfcal ! Performing phase self-cal ! Adding 38 model components to the UV plane model. ! The established model now contains 121 components and 2.44607 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.390326Jy sigma=3.576326 ! Fit after self-cal, rms=0.390325Jy sigma=3.576042 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 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 = 0.00311902 Jy ! Component: 100 - total flux cleaned = 0.00381395 Jy ! Component: 150 - total flux cleaned = 0.00380476 Jy ! Component: 200 - total flux cleaned = 0.00444038 Jy ! Total flux subtracted in 200 components = 0.00444038 Jy ! Clean residual min=-0.019243 max=0.017042 Jy/beam ! Clean residual mean=0.000020 rms=0.004098 Jy/beam ! Combined flux in latest and established models = 2.45051 Jy ! Performing phase self-cal ! Adding 47 model components to the UV plane model. ! The established model now contains 127 components and 2.45051 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.389823Jy sigma=3.570429 ! Fit after self-cal, rms=0.389832Jy sigma=3.570335 ! Inverting map ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 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=0.389832Jy sigma=3.570335 ! Fit after self-cal, rms=0.390509Jy sigma=3.569892 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec ! Estimated beam: bmin=2.211 mas, bmaj=2.98 mas, bpa=-83.03 degrees ! Estimated noise=1.3216 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00828405 Jy ! Component: 100 - total flux cleaned = 0.0133148 Jy ! Component: 150 - total flux cleaned = 0.0172839 Jy ! Component: 200 - total flux cleaned = 0.0204252 Jy ! Total flux subtracted in 200 components = 0.0204252 Jy ! Clean residual min=-0.018152 max=0.013740 Jy/beam ! Clean residual mean=0.000045 rms=0.004537 Jy/beam ! Combined flux in latest and established models = 2.47094 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 137 components and 2.47093 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.390418Jy sigma=3.569667 ! Fit after self-cal, rms=0.390417Jy sigma=3.569567 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 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 = 0.00286608 Jy ! Component: 100 - total flux cleaned = 0.00386387 Jy ! Component: 150 - total flux cleaned = 0.00427948 Jy ! Component: 200 - total flux cleaned = 0.00477825 Jy ! Total flux subtracted in 200 components = 0.00477825 Jy ! Clean residual min=-0.018094 max=0.013503 Jy/beam ! Clean residual mean=0.000043 rms=0.004496 Jy/beam ! Combined flux in latest and established models = 2.47571 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 143 components and 2.47571 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.390428Jy sigma=3.569897 ! Fit after self-cal, rms=0.390429Jy sigma=3.569878 ! Inverting map ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. win_mult = win_mult / 1.2 print "************** FINISHED AMPLITUDE SELF-CAL **************" ! ************** FINISHED AMPLITUDE SELF-CAL ************** restore ! Inverting map and beam ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec ! Estimated beam: bmin=0.732 mas, bmaj=0.8981 mas, bpa=62.39 degrees ! Estimated noise=0.891194 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.732 x 0.8981 at 62.39 degrees (North through East) ! Clean map min=-0.022615 max=2.0847 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=0.390429Jy sigma=3.569878 ! Fit after self-cal, rms=34.346153Jy sigma=0.797817 ! Inverting map and beam ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec ! Estimated beam: bmin=0.7327 mas, bmaj=0.8974 mas, bpa=62.28 degrees ! Estimated noise=0.891067 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0109419 Jy ! Component: 100 - total flux cleaned = -0.0131636 Jy ! Component: 150 - total flux cleaned = -0.0146743 Jy ! Component: 200 - total flux cleaned = -0.0163014 Jy ! Total flux subtracted in 200 components = -0.0163014 Jy ! Clean residual min=-0.005797 max=0.005624 Jy/beam ! Clean residual mean=-0.000000 rms=0.001143 Jy/beam ! Combined flux in latest and established models = 2.45941 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 151 components and 2.45941 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=34.346142Jy sigma=0.762986 ! Fit after self-cal, rms=34.345421Jy sigma=0.760826 ! Inverting map ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0033543 Jy ! Component: 100 - total flux cleaned = -0.00336337 Jy ! Component: 150 - total flux cleaned = -0.00336332 Jy ! Component: 200 - total flux cleaned = -0.00335499 Jy ! Total flux subtracted in 200 components = -0.00335499 Jy ! Clean residual min=-0.004966 max=0.004860 Jy/beam ! Clean residual mean=0.000001 rms=0.001069 Jy/beam ! Combined flux in latest and established models = 2.45606 Jy ! Performing phase self-cal ! Adding 35 model components to the UV plane model. ! The established model now contains 154 components and 2.45606 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=34.345448Jy sigma=0.746906 ! Fit after self-cal, rms=34.345005Jy sigma=0.746302 ! Inverting map ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=34.345005Jy sigma=0.746302 ! Fit after self-cal, rms=36.225834Jy sigma=0.739205 print "************** CLEARING MODEL AND STARTING OVER **********" ! ************** CLEARING MODEL AND STARTING OVER ********** clrmod true ! clrmod: Cleared the established and tentative models. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec ! Estimated beam: bmin=0.6818 mas, bmaj=0.7368 mas, bpa=77.47 degrees ! Estimated noise=1.2894 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.61671 Jy ! Component: 100 - total flux cleaned = 2.01819 Jy ! Component: 150 - total flux cleaned = 2.1869 Jy ! Component: 200 - total flux cleaned = 2.27757 Jy ! Total flux subtracted in 200 components = 2.27757 Jy ! Clean residual min=-0.010873 max=0.045518 Jy/beam ! Clean residual mean=0.000009 rms=0.002344 Jy/beam ! Combined flux in latest and established models = 2.27757 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 15 model components to the UV plane model. ! The established model now contains 15 components and 2.27757 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec ! Estimated beam: bmin=0.7328 mas, bmaj=0.8975 mas, bpa=62.31 degrees ! Estimated noise=0.890211 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 = 0.0663344 Jy ! Component: 100 - total flux cleaned = 0.100709 Jy ! Component: 150 - total flux cleaned = 0.119497 Jy ! Component: 200 - total flux cleaned = 0.131139 Jy ! Total flux subtracted in 200 components = 0.131139 Jy ! Clean residual min=-0.005035 max=0.009160 Jy/beam ! Clean residual mean=0.000012 rms=0.001115 Jy/beam ! Combined flux in latest and established models = 2.40871 Jy ! Adding 22 model components to the UV plane model. ! The established model now contains 30 components and 2.40871 Jy ! Inverting map ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec ! Added new window around map position (1, -0.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00936151 Jy ! Component: 100 - total flux cleaned = 0.0164619 Jy ! Component: 150 - total flux cleaned = 0.0198165 Jy ! Component: 200 - total flux cleaned = 0.0213289 Jy ! Total flux subtracted in 200 components = 0.0213289 Jy ! Clean residual min=-0.005050 max=0.005046 Jy/beam ! Clean residual mean=0.000005 rms=0.000967 Jy/beam ! Combined flux in latest and established models = 2.43004 Jy ! Adding 27 model components to the UV plane model. ! The established model now contains 45 components and 2.43004 Jy ! Inverting map ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec ! Estimated beam: bmin=2.216 mas, bmaj=2.984 mas, bpa=-82.96 degrees ! Estimated noise=1.31724 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00473034 Jy ! Component: 100 - total flux cleaned = 0.00672811 Jy ! Component: 150 - total flux cleaned = 0.00724952 Jy ! Component: 200 - total flux cleaned = 0.00778718 Jy ! Total flux subtracted in 200 components = 0.00778718 Jy ! Clean residual min=-0.004572 max=0.004171 Jy/beam ! Clean residual mean=0.000008 rms=0.001244 Jy/beam ! Combined flux in latest and established models = 2.43783 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 = 0.000392996 Jy ! Component: 100 - total flux cleaned = 0.000815303 Jy ! Component: 150 - total flux cleaned = 0.00113037 Jy ! Component: 200 - total flux cleaned = 0.00152703 Jy ! Total flux subtracted in 200 components = 0.00152703 Jy ! Clean residual min=-0.004424 max=0.004155 Jy/beam ! Clean residual mean=0.000006 rms=0.001217 Jy/beam ! Combined flux in latest and established models = 2.43936 Jy ! Adding 28 model components to the UV plane model. ! The established model now contains 71 components and 2.43936 Jy ! Inverting map ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec ! Estimated beam: bmin=0.7328 mas, bmaj=0.8975 mas, bpa=62.31 degrees ! Estimated noise=0.890211 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00021816 Jy ! Component: 100 - total flux cleaned = 0.000296627 Jy ! Component: 150 - total flux cleaned = 0.000456583 Jy ! Component: 200 - total flux cleaned = 0.000308893 Jy ! Total flux subtracted in 200 components = 0.000308893 Jy ! Clean residual min=-0.005343 max=0.004430 Jy/beam ! Clean residual mean=0.000002 rms=0.000910 Jy/beam ! Combined flux in latest and established models = 2.43966 Jy selfcal ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 85 components and 2.43966 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=36.225910Jy sigma=0.730981 ! Fit after self-cal, rms=36.224709Jy sigma=0.717048 wmodel J0019+7327_X_map.mod ! Writing 85 model components to file: J0019+7327_X_map.mod wobs J0019+7327_X_uvs.fits ! Writing UV FITS file: J0019+7327_X_uvs.fits wwins J0019+7327_X_map.win ! wwins: Wrote 6 windows to J0019+7327_X_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000528813 Jy ! Component: 100 - total flux cleaned = 0.0011225 Jy ! Component: 150 - total flux cleaned = 0.0015468 Jy ! Component: 200 - total flux cleaned = 0.0018193 Jy ! Component: 250 - total flux cleaned = 0.00215096 Jy ! Component: 300 - total flux cleaned = 0.00228066 Jy ! Component: 350 - total flux cleaned = 0.0025355 Jy ! Component: 400 - total flux cleaned = 0.00247379 Jy ! Component: 450 - total flux cleaned = 0.00253526 Jy ! Component: 500 - total flux cleaned = 0.00235486 Jy ! Component: 550 - total flux cleaned = 0.0023563 Jy ! Component: 600 - total flux cleaned = 0.00235613 Jy ! Component: 650 - total flux cleaned = 0.00212585 Jy ! Component: 700 - total flux cleaned = 0.0022407 Jy ! Component: 750 - total flux cleaned = 0.0021836 Jy ! Component: 800 - total flux cleaned = 0.00207159 Jy ! Component: 850 - total flux cleaned = 0.00196109 Jy ! Component: 900 - total flux cleaned = 0.00179728 Jy ! Component: 950 - total flux cleaned = 0.00174323 Jy ! Component: 1000 - total flux cleaned = 0.00163616 Jy ! Component: 1050 - total flux cleaned = 0.00158341 Jy ! Component: 1100 - total flux cleaned = 0.00147837 Jy ! Component: 1150 - total flux cleaned = 0.00137378 Jy ! Component: 1200 - total flux cleaned = 0.00147754 Jy ! Component: 1250 - total flux cleaned = 0.00132422 Jy ! Component: 1300 - total flux cleaned = 0.00127317 Jy ! Component: 1350 - total flux cleaned = 0.00132436 Jy ! Component: 1400 - total flux cleaned = 0.0013734 Jy ! Component: 1450 - total flux cleaned = 0.00112413 Jy ! Component: 1500 - total flux cleaned = 0.00112384 Jy ! Component: 1550 - total flux cleaned = 0.0010745 Jy ! Component: 1600 - total flux cleaned = 0.000976974 Jy ! Component: 1650 - total flux cleaned = 0.00117095 Jy ! Component: 1700 - total flux cleaned = 0.000978159 Jy ! Component: 1750 - total flux cleaned = 0.00121783 Jy ! Component: 1800 - total flux cleaned = 0.00140844 Jy ! Component: 1850 - total flux cleaned = 0.00169322 Jy ! Component: 1900 - total flux cleaned = 0.0015041 Jy ! Component: 1950 - total flux cleaned = 0.00178516 Jy ! Component: 2000 - total flux cleaned = 0.00183195 Jy ! Component: 2050 - total flux cleaned = 0.00192446 Jy ! Component: 2100 - total flux cleaned = 0.00187854 Jy ! Component: 2150 - total flux cleaned = 0.00210775 Jy ! Component: 2200 - total flux cleaned = 0.00201645 Jy ! Component: 2250 - total flux cleaned = 0.00206172 Jy ! Component: 2300 - total flux cleaned = 0.00228735 Jy ! Component: 2350 - total flux cleaned = 0.00210758 Jy ! Component: 2400 - total flux cleaned = 0.0021073 Jy ! Component: 2450 - total flux cleaned = 0.00219638 Jy ! Component: 2500 - total flux cleaned = 0.00246194 Jy ! Component: 2550 - total flux cleaned = 0.00232933 Jy ! Component: 2600 - total flux cleaned = 0.00232885 Jy ! Component: 2650 - total flux cleaned = 0.00245955 Jy ! Component: 2700 - total flux cleaned = 0.00241612 Jy ! Component: 2750 - total flux cleaned = 0.00228618 Jy ! Component: 2800 - total flux cleaned = 0.00263058 Jy ! Component: 2850 - total flux cleaned = 0.00258795 Jy ! Component: 2900 - total flux cleaned = 0.00258759 Jy ! Component: 2950 - total flux cleaned = 0.00267275 Jy ! Component: 3000 - total flux cleaned = 0.00254583 Jy ! Component: 3050 - total flux cleaned = 0.00254579 Jy ! Component: 3100 - total flux cleaned = 0.00262982 Jy ! Component: 3150 - total flux cleaned = 0.00250449 Jy ! Component: 3200 - total flux cleaned = 0.00250449 Jy ! Component: 3250 - total flux cleaned = 0.00262848 Jy ! Component: 3300 - total flux cleaned = 0.00262859 Jy ! Component: 3350 - total flux cleaned = 0.00238183 Jy ! Component: 3400 - total flux cleaned = 0.00242273 Jy ! Component: 3450 - total flux cleaned = 0.00250456 Jy ! Component: 3500 - total flux cleaned = 0.00246391 Jy ! Component: 3550 - total flux cleaned = 0.00238273 Jy ! Component: 3600 - total flux cleaned = 0.00238314 Jy ! Component: 3650 - total flux cleaned = 0.00234315 Jy ! Component: 3700 - total flux cleaned = 0.00230324 Jy ! Component: 3750 - total flux cleaned = 0.00222321 Jy ! Component: 3800 - total flux cleaned = 0.00234233 Jy ! Component: 3850 - total flux cleaned = 0.00230268 Jy ! Component: 3900 - total flux cleaned = 0.00222377 Jy ! Component: 3950 - total flux cleaned = 0.00194846 Jy ! Component: 4000 - total flux cleaned = 0.00198785 Jy ! Component: 4050 - total flux cleaned = 0.00194892 Jy ! Total flux subtracted in 4096 components = 0.00190994 Jy ! Clean residual min=-0.002314 max=0.002107 Jy/beam ! Clean residual mean=0.000000 rms=0.000634 Jy/beam ! Combined flux in latest and established models = 2.44157 Jy keep ! Adding 365 model components to the UV plane model. ! The established model now contains 447 components and 2.44157 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv118_uvs/J0019+7327_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7328 x 0.8975 at 62.31 degrees (North through East) ! Clean map min=-0.0035431 max=2.0909 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv118_uvs/J0019+7327_X_map.fits wmodel /scr/pima/rv118_uvs/J0019+7327_X_map.mod ! Writing 447 model components to file: /scr/pima/rv118_uvs/J0019+7327_X_map.mod wobs /scr/pima/rv118_uvs/J0019+7327_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv118_uvs/J0019+7327_X_uvs.fits wwins /scr/pima/rv118_uvs/J0019+7327_X_map.win ! wwins: Wrote 7 windows to /scr/pima/rv118_uvs/J0019+7327_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 2.09094 invert ! Inverting map ! Your choice of large map pixels excluded 1.13% of the data. ! The x-axis pixel size should ideally be below 0.1849 milli-arcsec ! The y-axis pixel size should ideally be below 0.1811 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000633074 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.0908308 0.0908308 0.181662 0.363323 0.726647 1.45329 2.90659 5.81317 11.6263 23.2527 46.5054 93.0108 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0018 print "peak= ", int(1000*peak_flux)/1000 ! peak= 2.09 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 3302.84 quit ! Quitting program ! Log file /scr/pima/rv118_uvs/J0019+7327_X_dfm.log closed on Sun Dec 10 00:06:33 2017