! Started logfile: /scr/pima/rv118_uvs/J0137+3122_X_dfm.log on Sun Dec 10 00:06:48 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/J0137+3122_X_uva.fits ! Reading UV FITS file: /scr/pima/rv118_uvs/J0137+3122_X_uva.fits ! AN table 1: 25 integrations on 36 of 36 possible baselines. ! AN table 2: 25 integrations on 3 of 3 possible baselines. ! AN table 3: 29 integrations on 15 of 15 possible baselines. ! AN table 4: 146 integrations on 6 of 6 possible baselines. ! AN table 5: 8 integrations on 28 of 28 possible baselines. ! AN table 6: 45 integrations on 55 of 55 possible baselines. ! Apparent sampling: 0.598997 visibilities/baseline/integration-bin. ! Found source: J0137+3122 ! ! 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 11944 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 J0137+3122_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 79 telescope corrections were flagged in sub-array 1. ! A total of 24 telescope corrections were flagged in sub-array 2. ! A total of 8 telescope corrections were flagged in sub-array 3. ! A total of 354 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 174 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 79 telescope corrections were flagged in sub-array 1. ! A total of 24 telescope corrections were flagged in sub-array 2. ! A total of 8 telescope corrections were flagged in sub-array 3. ! A total of 354 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 174 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 79 telescope corrections were flagged in sub-array 1. ! A total of 24 telescope corrections were flagged in sub-array 2. ! A total of 8 telescope corrections were flagged in sub-array 3. ! A total of 354 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 174 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 79 telescope corrections were flagged in sub-array 1. ! A total of 24 telescope corrections were flagged in sub-array 2. ! A total of 8 telescope corrections were flagged in sub-array 3. ! A total of 354 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 174 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.020519Jy sigma=15.789552 ! Fit after self-cal, rms=0.797869Jy sigma=12.224097 ! 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 8.38% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec ! Estimated beam: bmin=0.5772 mas, bmaj=0.8806 mas, bpa=15.88 degrees ! Estimated noise=0.770205 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 = 0.156532 Jy ! Component: 100 - total flux cleaned = 0.19653 Jy ! Total flux subtracted in 100 components = 0.19653 Jy ! Clean residual min=-0.005592 max=0.018480 Jy/beam ! Clean residual mean=-0.000018 rms=0.001463 Jy/beam ! Combined flux in latest and established models = 0.19653 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.19653 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.087080Jy sigma=1.194559 ! Fit after self-cal, rms=0.087081Jy sigma=1.194248 ! Inverting map ! Your choice of large map pixels excluded 8.38% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec ! Added new window around map position (0.6, -0.6). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.020682 Jy ! Component: 100 - total flux cleaned = 0.0338656 Jy ! Total flux subtracted in 100 components = 0.0338656 Jy ! Clean residual min=-0.004285 max=0.009328 Jy/beam ! Clean residual mean=-0.000012 rms=0.001092 Jy/beam ! Combined flux in latest and established models = 0.230395 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 18 components and 0.230395 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.080485Jy sigma=1.029594 ! Fit after self-cal, rms=0.080151Jy sigma=1.023693 ! Inverting map ! Your choice of large map pixels excluded 8.38% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0107548 Jy ! Component: 100 - total flux cleaned = 0.0176291 Jy ! Total flux subtracted in 100 components = 0.0176291 Jy ! Clean residual min=-0.003823 max=0.006045 Jy/beam ! Clean residual mean=-0.000009 rms=0.000921 Jy/beam ! Combined flux in latest and established models = 0.248024 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 21 components and 0.248024 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.078142Jy sigma=0.969581 ! Fit after self-cal, rms=0.077992Jy sigma=0.966890 ! Inverting map ! Your choice of large map pixels excluded 8.38% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00590736 Jy ! Component: 100 - total flux cleaned = 0.00965286 Jy ! Total flux subtracted in 100 components = 0.00965286 Jy ! Clean residual min=-0.003616 max=0.004278 Jy/beam ! Clean residual mean=-0.000007 rms=0.000856 Jy/beam ! Combined flux in latest and established models = 0.257677 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 27 components and 0.257677 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.077335Jy sigma=0.947341 ! Fit after self-cal, rms=0.077282Jy sigma=0.946412 ! Inverting map ! Your choice of large map pixels excluded 8.38% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 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 8.38% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec ! Estimated beam: bmin=0.6952 mas, bmaj=0.9756 mas, bpa=16.31 degrees ! Estimated noise=0.466452 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 = 0.00691488 Jy ! Component: 100 - total flux cleaned = 0.0106306 Jy ! Component: 150 - total flux cleaned = 0.0127469 Jy ! Component: 200 - total flux cleaned = 0.0139819 Jy ! Total flux subtracted in 200 components = 0.0139819 Jy ! Clean residual min=-0.003209 max=0.004983 Jy/beam ! Clean residual mean=-0.000005 rms=0.000770 Jy/beam ! Combined flux in latest and established models = 0.271659 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 32 components and 0.271659 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.076903Jy sigma=0.932455 ! Fit after self-cal, rms=0.076825Jy sigma=0.931137 ! Inverting map ! Your choice of large map pixels excluded 8.38% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec ! Added new window around map position (-2, -2.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00428085 Jy ! Component: 100 - total flux cleaned = 0.00533815 Jy ! Component: 150 - total flux cleaned = 0.00580813 Jy ! Component: 200 - total flux cleaned = 0.0062044 Jy ! Total flux subtracted in 200 components = 0.0062044 Jy ! Clean residual min=-0.002892 max=0.003857 Jy/beam ! Clean residual mean=-0.000002 rms=0.000703 Jy/beam ! Combined flux in latest and established models = 0.277863 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 42 components and 0.277863 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.076571Jy sigma=0.926052 ! Fit after self-cal, rms=0.076534Jy sigma=0.925615 ! Inverting map ! Your choice of large map pixels excluded 8.38% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec ! Added new window around map position (1.2, -1.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00335507 Jy ! Component: 100 - total flux cleaned = 0.00418626 Jy ! Component: 150 - total flux cleaned = 0.00424989 Jy ! Component: 200 - total flux cleaned = 0.00430443 Jy ! Total flux subtracted in 200 components = 0.00430443 Jy ! Clean residual min=-0.002846 max=0.002958 Jy/beam ! Clean residual mean=0.000001 rms=0.000663 Jy/beam ! Combined flux in latest and established models = 0.282168 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 60 components and 0.282168 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.076395Jy sigma=0.922348 ! Fit after self-cal, rms=0.076376Jy sigma=0.922010 ! Inverting map ! Your choice of large map pixels excluded 8.38% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6952 x 0.9756 at 16.31 degrees (North through East) ! Clean map min=-0.0025604 max=0.20093 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 18 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.04 FD 0.98 KP 0.97 LA 0.98 ! MK 0.96 NL 0.99 NY 0.99 OV 1.01 ! PT 0.98 ! ! A total of 51 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* KK 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! HH 0.94 HN 0.95 NL 1.54 ON 0.92 ! SC 1.05 WZ 0.99 ! ! A total of 126 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HH 0.98 NY 1.05 ON 0.99 WZ 0.96 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.11 FD 0.99 HN 1.04 KP 1.20 ! LA 0.95 NL 0.97 PT 1.03 SC 1.06 ! ! A total of 27 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.00 FD 0.97 HH 0.94 HN 1.03 ! KP 1.00 LA 0.97 NL 0.95 NY 1.00 ! OV 0.98 SC 1.00 WZ 1.00 ! ! ! Correcting IF 2. ! A total of 18 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 1.00 KP 0.97 LA 1.00 ! MK 1.03 NL 0.96 NY 0.95 OV 1.01 ! PT 1.00 ! ! A total of 51 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* KK 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! HH 1.06 HN 1.01 NL 1.50 ON 1.03 ! SC 0.98 WZ 0.90 ! ! A total of 126 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HH 1.05 NY 1.08 ON 0.99 WZ 0.95 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 FD 0.98 HN 1.04 KP 1.15 ! LA 0.96 NL 1.02 PT 1.03 SC 1.02 ! ! A total of 27 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.01 FD 0.98 HH 0.96 HN 1.02 ! KP 1.01 LA 0.96 NL 0.96 NY 1.02 ! OV 1.01 SC 1.01 WZ 0.99 ! ! ! Correcting IF 3. ! A total of 18 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.04 FD 1.02 KP 0.99 LA 1.01 ! MK 1.00 NL 0.98 NY 0.98 OV 1.02 ! PT 1.01 ! ! A total of 51 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* KK 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! HH 0.96 HN 0.97 NL 1.58 ON 0.97 ! SC 1.09 WZ 0.97 ! ! A total of 126 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HH 0.99 NY 1.09 ON 0.98 WZ 0.98 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.16 FD 1.04 HN 1.12 KP 1.04 ! LA 1.06 NL 0.98 PT 0.99 SC 1.02 ! ! A total of 27 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.02 FD 1.00 HH 0.99 HN 1.01 ! KP 1.01 LA 0.98 NL 0.96 NY 0.99 ! OV 1.02 SC 1.00 WZ 1.01 ! ! ! Correcting IF 4. ! A total of 18 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.05 FD 1.01 KP 0.99 LA 1.02 ! MK 1.05 NL 0.98 NY 1.04 OV 1.05 ! PT 1.01 ! ! A total of 51 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* KK 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! HH 1.00 HN 1.04 NL 1.44 ON 1.08 ! SC 1.00 WZ 0.94 ! ! A total of 126 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HH 0.98 NY 1.08 ON 0.99 WZ 0.97 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.05 FD 1.01 HN 0.99 KP 1.09 ! LA 1.02 NL 0.91 PT 1.06 SC 1.00 ! ! A total of 27 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.01 FD 0.97 HH 1.00 HN 1.04 ! KP 1.00 LA 1.02 NL 0.98 NY 0.98 ! OV 1.01 SC 0.96 WZ 0.99 ! ! ! Fit before self-cal, rms=0.076376Jy sigma=0.922010 ! Fit after self-cal, rms=0.079837Jy sigma=0.907013 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 8.95% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec ! Estimated beam: bmin=0.6742 mas, bmaj=1.004 mas, bpa=13.87 degrees ! Estimated noise=0.480642 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 = 0.00110558 Jy ! Component: 100 - total flux cleaned = 0.00151897 Jy ! Component: 150 - total flux cleaned = 0.0016502 Jy ! Component: 200 - total flux cleaned = 0.00176938 Jy ! Total flux subtracted in 200 components = 0.00176938 Jy ! Clean residual min=-0.001921 max=0.001969 Jy/beam ! Clean residual mean=-0.000005 rms=0.000451 Jy/beam ! Combined flux in latest and established models = 0.283937 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 75 components and 0.283937 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.079759Jy sigma=0.905974 ! Fit after self-cal, rms=0.080010Jy sigma=0.905710 ! Inverting map ! Your choice of large map pixels excluded 8.95% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 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=0.080010Jy sigma=0.905710 ! Fit after self-cal, rms=0.080140Jy sigma=0.905314 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 8.95% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec ! Estimated beam: bmin=0.6745 mas, bmaj=1.003 mas, bpa=13.94 degrees ! Estimated noise=0.480706 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000541102 Jy ! Component: 100 - total flux cleaned = 0.00077657 Jy ! Component: 150 - total flux cleaned = 0.00088032 Jy ! Component: 200 - total flux cleaned = 0.000945008 Jy ! Total flux subtracted in 200 components = 0.000945008 Jy ! Clean residual min=-0.001874 max=0.001917 Jy/beam ! Clean residual mean=-0.000005 rms=0.000443 Jy/beam ! Combined flux in latest and established models = 0.284882 Jy selfcal ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 78 components and 0.284882 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.080099Jy sigma=0.904755 ! Fit after self-cal, rms=0.080096Jy sigma=0.904732 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 8.95% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 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 (38.8, 2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00184355 Jy ! Component: 100 - total flux cleaned = 0.00209211 Jy ! Component: 150 - total flux cleaned = 0.00219679 Jy ! Component: 200 - total flux cleaned = 0.00232312 Jy ! Total flux subtracted in 200 components = 0.00232312 Jy ! Clean residual min=-0.001916 max=0.001731 Jy/beam ! Clean residual mean=-0.000004 rms=0.000430 Jy/beam ! Combined flux in latest and established models = 0.287205 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 89 components and 0.287205 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.080045Jy sigma=0.903792 ! Fit after self-cal, rms=0.080040Jy sigma=0.903738 ! Inverting map ! Your choice of large map pixels excluded 8.95% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 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=0.080040Jy sigma=0.903738 ! Fit after self-cal, rms=0.080306Jy sigma=0.903660 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 8.95% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec ! Estimated beam: bmin=0.6748 mas, bmaj=1.003 mas, bpa=13.97 degrees ! Estimated noise=0.480741 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000390373 Jy ! Component: 100 - total flux cleaned = 0.000518467 Jy ! Component: 150 - total flux cleaned = 0.000517582 Jy ! Component: 200 - total flux cleaned = 0.000573338 Jy ! Total flux subtracted in 200 components = 0.000573338 Jy ! Clean residual min=-0.001926 max=0.001716 Jy/beam ! Clean residual mean=-0.000004 rms=0.000423 Jy/beam ! Combined flux in latest and established models = 0.287779 Jy selfcal ! Performing phase self-cal ! Adding 33 model components to the UV plane model. ! The established model now contains 95 components and 0.287779 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.080280Jy sigma=0.903307 ! Fit after self-cal, rms=0.080282Jy sigma=0.903298 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 8.95% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 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 = 0.000179312 Jy ! Component: 100 - total flux cleaned = 0.000205905 Jy ! Component: 150 - total flux cleaned = 0.000232002 Jy ! Component: 200 - total flux cleaned = 0.000282266 Jy ! Total flux subtracted in 200 components = 0.000282266 Jy ! Clean residual min=-0.001913 max=0.001723 Jy/beam ! Clean residual mean=-0.000004 rms=0.000421 Jy/beam ! Combined flux in latest and established models = 0.288061 Jy ! Performing phase self-cal ! Adding 38 model components to the UV plane model. ! The established model now contains 99 components and 0.288061 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.080265Jy sigma=0.903055 ! Fit after self-cal, rms=0.080263Jy sigma=0.903052 ! Inverting map ! Your choice of large map pixels excluded 8.95% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 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=0.080263Jy sigma=0.903052 ! Fit after self-cal, rms=0.080246Jy sigma=0.903009 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 8.95% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec ! Estimated beam: bmin=2.459 mas, bmaj=3.095 mas, bpa=76.21 degrees ! Estimated noise=0.630084 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000858774 Jy ! Component: 100 - total flux cleaned = 0.000857705 Jy ! Component: 150 - total flux cleaned = 0.00089745 Jy ! Component: 200 - total flux cleaned = 0.000929401 Jy ! Total flux subtracted in 200 components = 0.000929401 Jy ! Clean residual min=-0.001849 max=0.001968 Jy/beam ! Clean residual mean=-0.000010 rms=0.000496 Jy/beam ! Combined flux in latest and established models = 0.28899 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 109 components and 0.28899 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.080237Jy sigma=0.903018 ! Fit after self-cal, rms=0.080232Jy sigma=0.903003 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 8.95% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 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 = 0.000197298 Jy ! Component: 100 - total flux cleaned = 0.000269194 Jy ! Component: 150 - total flux cleaned = 0.000334723 Jy ! Component: 200 - total flux cleaned = 0.000382812 Jy ! Total flux subtracted in 200 components = 0.000382812 Jy ! Clean residual min=-0.001854 max=0.002005 Jy/beam ! Clean residual mean=-0.000009 rms=0.000495 Jy/beam ! Combined flux in latest and established models = 0.289373 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 115 components and 0.289373 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.080229Jy sigma=0.903006 ! Fit after self-cal, rms=0.080229Jy sigma=0.903003 ! Inverting map ! Your choice of large map pixels excluded 8.95% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. win_mult = win_mult / 1.2 print "************** FINISHED AMPLITUDE SELF-CAL **************" ! ************** FINISHED AMPLITUDE SELF-CAL ************** restore ! Inverting map and beam ! Your choice of large map pixels excluded 8.95% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec ! Estimated beam: bmin=0.6751 mas, bmaj=1.003 mas, bpa=14.01 degrees ! Estimated noise=0.480787 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6751 x 1.003 at 14.01 degrees (North through East) ! Clean map min=-0.0021649 max=0.20054 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 print "************** CLEARING MODEL AND STARTING OVER **********" ! ************** CLEARING MODEL AND STARTING OVER ********** clrmod true ! clrmod: Cleared the established and tentative models. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 8.95% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec ! Estimated beam: bmin=0.5576 mas, bmaj=0.8941 mas, bpa=13.92 degrees ! Estimated noise=0.807122 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.156225 Jy ! Component: 100 - total flux cleaned = 0.19854 Jy ! Component: 150 - total flux cleaned = 0.222743 Jy ! Component: 200 - total flux cleaned = 0.238166 Jy ! Total flux subtracted in 200 components = 0.238166 Jy ! Clean residual min=-0.003858 max=0.008226 Jy/beam ! Clean residual mean=-0.000009 rms=0.000949 Jy/beam ! Combined flux in latest and established models = 0.238166 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 17 model components to the UV plane model. ! The established model now contains 17 components and 0.238166 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 8.95% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec ! Estimated beam: bmin=0.6751 mas, bmaj=1.003 mas, bpa=14.01 degrees ! Estimated noise=0.480787 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 = 0.0154784 Jy ! Component: 100 - total flux cleaned = 0.0243546 Jy ! Component: 150 - total flux cleaned = 0.0303615 Jy ! Component: 200 - total flux cleaned = 0.0347004 Jy ! Total flux subtracted in 200 components = 0.0347004 Jy ! Clean residual min=-0.002260 max=0.002747 Jy/beam ! Clean residual mean=-0.000010 rms=0.000549 Jy/beam ! Combined flux in latest and established models = 0.272866 Jy ! Adding 39 model components to the UV plane model. ! The established model now contains 46 components and 0.272866 Jy ! Inverting map ! Your choice of large map pixels excluded 8.95% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec ! Added new window around map position (-3.8, -1). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00337516 Jy ! Component: 100 - total flux cleaned = 0.00605418 Jy ! Component: 150 - total flux cleaned = 0.0082614 Jy ! Component: 200 - total flux cleaned = 0.0100982 Jy ! Total flux subtracted in 200 components = 0.0100982 Jy ! Clean residual min=-0.001895 max=0.001890 Jy/beam ! Clean residual mean=-0.000006 rms=0.000449 Jy/beam ! Combined flux in latest and established models = 0.282964 Jy ! Adding 35 model components to the UV plane model. ! The established model now contains 68 components and 0.282964 Jy ! Inverting map ! Your choice of large map pixels excluded 8.95% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 8.95% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec ! Estimated beam: bmin=2.459 mas, bmaj=3.095 mas, bpa=76.21 degrees ! Estimated noise=0.630084 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00250053 Jy ! Component: 100 - total flux cleaned = 0.00402106 Jy ! Component: 150 - total flux cleaned = 0.00507885 Jy ! Component: 200 - total flux cleaned = 0.00578049 Jy ! Total flux subtracted in 200 components = 0.00578049 Jy ! Clean residual min=-0.001920 max=0.002052 Jy/beam ! Clean residual mean=-0.000010 rms=0.000510 Jy/beam ! Combined flux in latest and established models = 0.288745 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 = 0.000282722 Jy ! Component: 100 - total flux cleaned = 0.000425183 Jy ! Component: 150 - total flux cleaned = 0.000518204 Jy ! Component: 200 - total flux cleaned = 0.000570006 Jy ! Total flux subtracted in 200 components = 0.000570006 Jy ! Clean residual min=-0.001870 max=0.002078 Jy/beam ! Clean residual mean=-0.000009 rms=0.000503 Jy/beam ! Combined flux in latest and established models = 0.289315 Jy ! Adding 40 model components to the UV plane model. ! The established model now contains 93 components and 0.289315 Jy ! Inverting map ! Your choice of large map pixels excluded 8.95% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 8.95% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec ! Estimated beam: bmin=0.6751 mas, bmaj=1.003 mas, bpa=14.01 degrees ! Estimated noise=0.480787 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000326942 Jy ! Component: 100 - total flux cleaned = -0.000406328 Jy ! Component: 150 - total flux cleaned = -0.000511313 Jy ! Component: 200 - total flux cleaned = -0.000544748 Jy ! Total flux subtracted in 200 components = -0.000544748 Jy ! Clean residual min=-0.001747 max=0.001823 Jy/beam ! Clean residual mean=-0.000004 rms=0.000419 Jy/beam ! Combined flux in latest and established models = 0.28877 Jy selfcal ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 111 components and 0.28877 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.080143Jy sigma=0.902718 ! Fit after self-cal, rms=0.080142Jy sigma=0.902411 wmodel J0137+3122_X_map.mod ! Writing 111 model components to file: J0137+3122_X_map.mod wobs J0137+3122_X_uvs.fits ! Writing UV FITS file: J0137+3122_X_uvs.fits wwins J0137+3122_X_map.win ! wwins: Wrote 6 windows to J0137+3122_X_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! Your choice of large map pixels excluded 8.95% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000166213 Jy ! Component: 100 - total flux cleaned = 0.000198086 Jy ! Component: 150 - total flux cleaned = 0.000138412 Jy ! Component: 200 - total flux cleaned = 1.95981e-05 Jy ! Component: 250 - total flux cleaned = -9.66821e-05 Jy ! Component: 300 - total flux cleaned = -9.73544e-05 Jy ! Component: 350 - total flux cleaned = -9.81078e-05 Jy ! Component: 400 - total flux cleaned = -0.000181549 Jy ! Component: 450 - total flux cleaned = -0.000181364 Jy ! Component: 500 - total flux cleaned = -0.000234963 Jy ! Component: 550 - total flux cleaned = -0.000261939 Jy ! Component: 600 - total flux cleaned = -0.000314441 Jy ! Component: 650 - total flux cleaned = -0.000262071 Jy ! Component: 700 - total flux cleaned = -0.000236118 Jy ! Component: 750 - total flux cleaned = -0.000184519 Jy ! Component: 800 - total flux cleaned = -0.000184413 Jy ! Component: 850 - total flux cleaned = -8.33131e-05 Jy ! Component: 900 - total flux cleaned = -0.000133523 Jy ! Component: 950 - total flux cleaned = -8.35098e-05 Jy ! Component: 1000 - total flux cleaned = 0.000113516 Jy ! Component: 1050 - total flux cleaned = -3.35608e-05 Jy ! Component: 1100 - total flux cleaned = 8.80426e-05 Jy ! Component: 1150 - total flux cleaned = 0.000136259 Jy ! Component: 1200 - total flux cleaned = 0.000231699 Jy ! Component: 1250 - total flux cleaned = 0.0002552 Jy ! Component: 1300 - total flux cleaned = 0.000255574 Jy ! Component: 1350 - total flux cleaned = 0.000372305 Jy ! Component: 1400 - total flux cleaned = 0.000418746 Jy ! Component: 1450 - total flux cleaned = 0.000279689 Jy ! Component: 1500 - total flux cleaned = 0.000348746 Jy ! Component: 1550 - total flux cleaned = 0.000417139 Jy ! Component: 1600 - total flux cleaned = 0.00041709 Jy ! Component: 1650 - total flux cleaned = 0.000484742 Jy ! Component: 1700 - total flux cleaned = 0.000507189 Jy ! Component: 1750 - total flux cleaned = 0.000440313 Jy ! Component: 1800 - total flux cleaned = 0.00050684 Jy ! Component: 1850 - total flux cleaned = 0.000529005 Jy ! Component: 1900 - total flux cleaned = 0.000573209 Jy ! Component: 1950 - total flux cleaned = 0.000594863 Jy ! Component: 2000 - total flux cleaned = 0.000573258 Jy ! Component: 2050 - total flux cleaned = 0.000594912 Jy ! Component: 2100 - total flux cleaned = 0.000551826 Jy ! Component: 2150 - total flux cleaned = 0.000743839 Jy ! Component: 2200 - total flux cleaned = 0.000595277 Jy ! Component: 2250 - total flux cleaned = 0.000679637 Jy ! Component: 2300 - total flux cleaned = 0.000616876 Jy ! Component: 2350 - total flux cleaned = 0.000679591 Jy ! Component: 2400 - total flux cleaned = 0.000700365 Jy ! Component: 2450 - total flux cleaned = 0.000721066 Jy ! Component: 2500 - total flux cleaned = 0.000638663 Jy ! Component: 2550 - total flux cleaned = 0.00076137 Jy ! Component: 2600 - total flux cleaned = 0.000761406 Jy ! Component: 2650 - total flux cleaned = 0.000680383 Jy ! Component: 2700 - total flux cleaned = 0.000720457 Jy ! Component: 2750 - total flux cleaned = 0.000680307 Jy ! Component: 2800 - total flux cleaned = 0.000600354 Jy ! Component: 2850 - total flux cleaned = 0.000560638 Jy ! Component: 2900 - total flux cleaned = 0.000758504 Jy ! Component: 2950 - total flux cleaned = 0.000659963 Jy ! Component: 3000 - total flux cleaned = 0.000699144 Jy ! Component: 3050 - total flux cleaned = 0.000699054 Jy ! Component: 3100 - total flux cleaned = 0.000601896 Jy ! Component: 3150 - total flux cleaned = 0.000679305 Jy ! Component: 3200 - total flux cleaned = 0.000544412 Jy ! Component: 3250 - total flux cleaned = 0.000640251 Jy ! Component: 3300 - total flux cleaned = 0.000582988 Jy ! Component: 3350 - total flux cleaned = 0.000563748 Jy ! Component: 3400 - total flux cleaned = 0.000525752 Jy ! Component: 3450 - total flux cleaned = 0.00048804 Jy ! Component: 3500 - total flux cleaned = 0.000450381 Jy ! Component: 3550 - total flux cleaned = 0.000412874 Jy ! Component: 3600 - total flux cleaned = 0.00031962 Jy ! Component: 3650 - total flux cleaned = 0.000282508 Jy ! Component: 3700 - total flux cleaned = 0.000282489 Jy ! Component: 3750 - total flux cleaned = 0.000245555 Jy ! Component: 3800 - total flux cleaned = 0.000190354 Jy ! Component: 3850 - total flux cleaned = 0.000153786 Jy ! Component: 3900 - total flux cleaned = 0.000171949 Jy ! Component: 3950 - total flux cleaned = 9.93445e-05 Jy ! Component: 4000 - total flux cleaned = 4.50646e-05 Jy ! Component: 4050 - total flux cleaned = 4.50843e-05 Jy ! Total flux subtracted in 4096 components = 2.71427e-05 Jy ! Clean residual min=-0.001193 max=0.001106 Jy/beam ! Clean residual mean=-0.000003 rms=0.000294 Jy/beam ! Combined flux in latest and established models = 0.288797 Jy keep ! Adding 331 model components to the UV plane model. ! The established model now contains 442 components and 0.288797 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv118_uvs/J0137+3122_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 8.95% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6751 x 1.003 at 14.01 degrees (North through East) ! Clean map min=-0.0013471 max=0.2009 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv118_uvs/J0137+3122_X_map.fits wmodel /scr/pima/rv118_uvs/J0137+3122_X_map.mod ! Writing 442 model components to file: /scr/pima/rv118_uvs/J0137+3122_X_map.mod wobs /scr/pima/rv118_uvs/J0137+3122_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv118_uvs/J0137+3122_X_uvs.fits wwins /scr/pima/rv118_uvs/J0137+3122_X_map.win ! wwins: Wrote 7 windows to /scr/pima/rv118_uvs/J0137+3122_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.2009 invert ! Inverting map ! Your choice of large map pixels excluded 8.95% of the data. ! The x-axis pixel size should ideally be below 0.1694 milli-arcsec ! The y-axis pixel size should ideally be below 0.1741 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000293953 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.438955 0.438955 0.87791 1.75582 3.51164 7.02328 14.0466 28.0931 56.1862 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0008 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.2 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 683.441 quit ! Quitting program ! Log file /scr/pima/rv118_uvs/J0137+3122_X_dfm.log closed on Sun Dec 10 00:06:52 2017