! Started logfile: /scr/pima/rv122_uvs/J0019+7327_X_dfm.log on Fri Jul 13 21:06:01 2018 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/rv122_uvs/J0019+7327_X_uva.fits ! Reading UV FITS file: /scr/pima/rv122_uvs/J0019+7327_X_uva.fits ! AN table 1: 4 integrations on 28 of 28 possible baselines. ! AN table 2: 63 integrations on 45 of 45 possible baselines. ! AN table 3: 11 integrations on 10 of 10 possible baselines. ! AN table 4: 3 integrations on 36 of 36 possible baselines. ! AN table 5: 20 integrations on 10 of 10 possible baselines. ! AN table 6: 2 integrations on 3 of 3 possible baselines. ! AN table 7: 15 integrations on 21 of 21 possible baselines. ! Apparent sampling: 0.423766 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 69 lines of history. ! ! Reading 6248 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 print "===============================================================" ! =============================================================== ! print "=== Difmap script: pima_mupet_01.dvm version of 2016.05.19 === " ! === Difmap script: pima_mupet_01.dvm version of 2016.05.19 === ! 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 16 telescope corrections were flagged in sub-array 1. ! A total of 350 telescope corrections were flagged in sub-array 2. ! A total of 7 telescope corrections were flagged in sub-array 3. ! A total of 9 telescope corrections were flagged in sub-array 4. ! A total of 66 telescope corrections were flagged in sub-array 5. ! A total of 59 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 2. ! A total of 16 telescope corrections were flagged in sub-array 1. ! A total of 350 telescope corrections were flagged in sub-array 2. ! A total of 7 telescope corrections were flagged in sub-array 3. ! A total of 9 telescope corrections were flagged in sub-array 4. ! A total of 66 telescope corrections were flagged in sub-array 5. ! A total of 59 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 3. ! A total of 16 telescope corrections were flagged in sub-array 1. ! A total of 350 telescope corrections were flagged in sub-array 2. ! A total of 7 telescope corrections were flagged in sub-array 3. ! A total of 9 telescope corrections were flagged in sub-array 4. ! A total of 66 telescope corrections were flagged in sub-array 5. ! A total of 59 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 4. ! A total of 16 telescope corrections were flagged in sub-array 1. ! A total of 350 telescope corrections were flagged in sub-array 2. ! A total of 7 telescope corrections were flagged in sub-array 3. ! A total of 9 telescope corrections were flagged in sub-array 4. ! A total of 66 telescope corrections were flagged in sub-array 5. ! A total of 59 telescope corrections were flagged in sub-array 7. ! ! Fit before self-cal, rms=2.084595Jy sigma=23.113829 ! Fit after self-cal, rms=0.830631Jy sigma=9.084786 ! 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 1.34% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=0.6692 mas, bmaj=0.7642 mas, bpa=25.22 degrees ! Estimated noise=1.32895 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 = 1.30292 Jy ! Component: 100 - total flux cleaned = 1.64099 Jy ! Total flux subtracted in 100 components = 1.64099 Jy ! Clean residual min=-0.034977 max=0.139558 Jy/beam ! Clean residual mean=0.000108 rms=0.007211 Jy/beam ! Combined flux in latest and established models = 1.64099 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 1.64099 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.328863Jy sigma=3.568532 ! Fit after self-cal, rms=0.328761Jy sigma=3.568035 ! Inverting map ! Your choice of large map pixels excluded 1.34% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.146609 Jy ! Component: 100 - total flux cleaned = 0.222991 Jy ! Total flux subtracted in 100 components = 0.222991 Jy ! Clean residual min=-0.021899 max=0.042246 Jy/beam ! Clean residual mean=0.000060 rms=0.004747 Jy/beam ! Combined flux in latest and established models = 1.86398 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 11 components and 1.86398 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.224330Jy sigma=2.380627 ! Fit after self-cal, rms=0.224003Jy sigma=2.377382 ! Inverting map ! Your choice of large map pixels excluded 1.34% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! Added new window around map position (0.2, 1.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0468586 Jy ! Component: 100 - total flux cleaned = 0.0759014 Jy ! Total flux subtracted in 100 components = 0.0759014 Jy ! Clean residual min=-0.020221 max=0.028531 Jy/beam ! Clean residual mean=0.000044 rms=0.004382 Jy/beam ! Combined flux in latest and established models = 1.93988 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 16 components and 1.93988 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.205985Jy sigma=2.173621 ! Fit after self-cal, rms=0.205699Jy sigma=2.170194 ! Inverting map ! Your choice of large map pixels excluded 1.34% of the data. ! The x-axis pixel size should ideally be below 0.1696 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 1.34% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=0.743 mas, bmaj=1.013 mas, bpa=12.88 degrees ! Estimated noise=0.969978 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 = 0.0413741 Jy ! Component: 100 - total flux cleaned = 0.0592683 Jy ! Component: 150 - total flux cleaned = 0.0615393 Jy ! Component: 200 - total flux cleaned = 0.0629411 Jy ! Total flux subtracted in 200 components = 0.0629411 Jy ! Clean residual min=-0.033496 max=0.034552 Jy/beam ! Clean residual mean=0.000012 rms=0.007443 Jy/beam ! Combined flux in latest and established models = 2.00282 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 24 components and 2.00282 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.196664Jy sigma=2.062018 ! Fit after self-cal, rms=0.196512Jy sigma=2.060215 ! Inverting map ! Your choice of large map pixels excluded 1.34% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec print "============== Finished natural weighting clean ==============" ! ============== Finished natural weighting clean ============== ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.743 x 1.013 at 12.88 degrees (North through East) ! Clean map min=-0.030171 max=1.7231 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 HN 1.11 KP 1.07 LA 1.04 ! MK 0.97 NY 0.90 OV 0.98 PT 0.88 ! ! A total of 15 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 0.92 HN 1.03 KP 1.10 ! LA 1.06 MK 1.01 ON 0.99 OV 1.01 ! PT 0.87 SC 1.01 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 MK 0.99 NY 0.95 ON 0.99 ! OV 1.01 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 FD 0.96 HN 1.04 KP 1.15 ! LA 1.06 NY 0.94 OV 1.01 PT 0.90 ! SC 1.04 ! ! A total of 24 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.95 MK 1.16 NY 0.90 ON 0.90 ! WZ 1.05 ! ! A total of 6 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! HN 0.00* SC 0.00* WZ 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 0.98 KP 1.07 LA 1.05 MK 1.01 ! OV 1.00 PT 0.90 WZ 0.98 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 HN 1.15 KP 1.08 LA 1.05 ! MK 0.96 NY 0.92 OV 1.00 PT 0.89 ! ! A total of 15 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 0.92 HN 1.03 KP 1.11 ! LA 1.07 MK 1.01 ON 0.98 OV 1.01 ! PT 0.88 SC 1.02 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 MK 0.98 NY 0.95 ON 1.00 ! OV 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 FD 0.95 HN 1.08 KP 1.14 ! LA 1.07 NY 0.94 OV 1.00 PT 0.91 ! SC 1.03 ! ! A total of 24 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.96 MK 1.15 NY 0.88 ON 0.92 ! WZ 1.08 ! ! A total of 6 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! HN 0.00* SC 0.00* WZ 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 0.99 KP 1.07 LA 1.06 MK 1.01 ! OV 1.00 PT 0.88 WZ 0.97 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 HN 1.17 KP 1.07 LA 1.05 ! MK 0.96 NY 0.92 OV 0.99 PT 0.89 ! ! A total of 15 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 0.95 HN 1.06 KP 1.11 ! LA 1.07 MK 1.00 ON 0.98 OV 1.01 ! PT 0.89 SC 1.04 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 MK 1.01 NY 0.94 ON 0.99 ! OV 1.01 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 FD 0.96 HN 1.05 KP 1.15 ! LA 1.07 NY 0.93 OV 1.01 PT 0.92 ! SC 1.07 ! ! A total of 24 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.95 MK 1.11 NY 0.88 ON 0.95 ! WZ 1.06 ! ! A total of 6 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! HN 0.00* SC 0.00* WZ 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.00 KP 1.10 LA 1.05 MK 1.02 ! OV 0.99 PT 0.90 WZ 1.03 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 HN 1.19 KP 1.09 LA 1.07 ! MK 0.96 NY 0.92 OV 0.99 PT 0.90 ! ! A total of 15 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 0.96 HN 1.05 KP 1.12 ! LA 1.07 MK 0.99 ON 1.00 OV 1.02 ! PT 0.89 SC 1.04 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 MK 1.01 NY 0.92 ON 1.00 ! OV 1.02 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 FD 0.95 HN 1.07 KP 1.17 ! LA 1.09 NY 0.94 OV 1.02 PT 0.91 ! SC 1.07 ! ! A total of 24 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.97 MK 1.14 NY 0.86 ON 0.97 ! WZ 1.06 ! ! A total of 6 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! HN 0.00* SC 0.00* WZ 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 0.98 KP 1.10 LA 1.08 MK 1.02 ! OV 1.00 PT 0.89 WZ 1.03 ! ! ! Fit before self-cal, rms=0.196512Jy sigma=2.060215 ! Fit after self-cal, rms=0.106242Jy sigma=1.043018 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=0.7323 mas, bmaj=1.021 mas, bpa=12.89 degrees ! Estimated noise=0.995952 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 = -0.00273684 Jy ! Component: 100 - total flux cleaned = -0.00422615 Jy ! Component: 150 - total flux cleaned = -0.00507243 Jy ! Component: 200 - total flux cleaned = -0.00530834 Jy ! Total flux subtracted in 200 components = -0.00530834 Jy ! Clean residual min=-0.010913 max=0.013552 Jy/beam ! Clean residual mean=-0.000018 rms=0.002151 Jy/beam ! Combined flux in latest and established models = 1.99752 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 33 components and 1.99752 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.103723Jy sigma=1.012563 ! Fit after self-cal, rms=0.103484Jy sigma=1.009421 ! Inverting map ! Your choice of large map pixels excluded 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! Added new window around map position (9.6, -6.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00990435 Jy ! Component: 100 - total flux cleaned = 0.0102205 Jy ! Component: 150 - total flux cleaned = 0.00999798 Jy ! Component: 200 - total flux cleaned = 0.00999379 Jy ! Total flux subtracted in 200 components = 0.00999379 Jy ! Clean residual min=-0.010500 max=0.011165 Jy/beam ! Clean residual mean=-0.000017 rms=0.001978 Jy/beam ! Combined flux in latest and established models = 2.00751 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 43 components and 2.00751 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.101902Jy sigma=0.989372 ! Fit after self-cal, rms=0.101727Jy sigma=0.987180 ! Inverting map ! Your choice of large map pixels excluded 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! Added new window around map position (-1.4, -1.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00507742 Jy ! Component: 100 - total flux cleaned = 0.00454095 Jy ! Component: 150 - total flux cleaned = 0.00406449 Jy ! Component: 200 - total flux cleaned = 0.0036263 Jy ! Total flux subtracted in 200 components = 0.0036263 Jy ! Clean residual min=-0.010237 max=0.009988 Jy/beam ! Clean residual mean=-0.000018 rms=0.001846 Jy/beam ! Combined flux in latest and established models = 2.01114 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 55 components and 2.01114 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.100096Jy sigma=0.970824 ! Fit after self-cal, rms=0.099967Jy sigma=0.968981 ! Inverting map ! Your choice of large map pixels excluded 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 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=0.099967Jy sigma=0.968981 ! Fit after self-cal, rms=0.085638Jy sigma=0.809871 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=0.7311 mas, bmaj=1.02 mas, bpa=13.08 degrees ! Estimated noise=0.997667 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000246022 Jy ! Component: 100 - total flux cleaned = -0.00231679 Jy ! Component: 150 - total flux cleaned = -0.00312634 Jy ! Component: 200 - total flux cleaned = -0.0035621 Jy ! Total flux subtracted in 200 components = -0.0035621 Jy ! Clean residual min=-0.005506 max=0.005349 Jy/beam ! Clean residual mean=-0.000000 rms=0.001053 Jy/beam ! Combined flux in latest and established models = 2.00757 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 67 components and 2.00757 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.084884Jy sigma=0.800496 ! Fit after self-cal, rms=0.084835Jy sigma=0.799809 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 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 = -0.000523441 Jy ! Component: 100 - total flux cleaned = -0.000925088 Jy ! Component: 150 - total flux cleaned = -0.00116298 Jy ! Component: 200 - total flux cleaned = -0.00127231 Jy ! Total flux subtracted in 200 components = -0.00127231 Jy ! Clean residual min=-0.005264 max=0.005038 Jy/beam ! Clean residual mean=-0.000000 rms=0.001023 Jy/beam ! Combined flux in latest and established models = 2.0063 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 72 components and 2.0063 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.084468Jy sigma=0.795277 ! Fit after self-cal, rms=0.084446Jy sigma=0.794931 ! Inverting map ! Your choice of large map pixels excluded 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 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=0.084446Jy sigma=0.794931 ! Fit after self-cal, rms=0.084122Jy sigma=0.792193 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=0.7302 mas, bmaj=1.021 mas, bpa=13.18 degrees ! Estimated noise=0.998293 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0011639 Jy ! Component: 100 - total flux cleaned = 0.000528649 Jy ! Component: 150 - total flux cleaned = 0.000196144 Jy ! Component: 200 - total flux cleaned = -2.73906e-06 Jy ! Total flux subtracted in 200 components = -2.73906e-06 Jy ! Clean residual min=-0.004806 max=0.004739 Jy/beam ! Clean residual mean=-0.000000 rms=0.000984 Jy/beam ! Combined flux in latest and established models = 2.0063 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 75 components and 2.0063 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.083741Jy sigma=0.787529 ! Fit after self-cal, rms=0.083718Jy sigma=0.787245 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 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 = -5.98531e-05 Jy ! Component: 100 - total flux cleaned = -0.000436616 Jy ! Component: 150 - total flux cleaned = -0.000612487 Jy ! Component: 200 - total flux cleaned = -0.000697295 Jy ! Total flux subtracted in 200 components = -0.000697295 Jy ! Clean residual min=-0.004657 max=0.004571 Jy/beam ! Clean residual mean=-0.000000 rms=0.000969 Jy/beam ! Combined flux in latest and established models = 2.0056 Jy ! Performing phase self-cal ! Adding 33 model components to the UV plane model. ! The established model now contains 83 components and 2.0056 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.083520Jy sigma=0.784925 ! Fit after self-cal, rms=0.083516Jy sigma=0.784755 ! Inverting map ! Your choice of large map pixels excluded 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 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=0.083516Jy sigma=0.784755 ! Fit after self-cal, rms=0.083409Jy sigma=0.783901 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=2.486 mas, bmaj=2.873 mas, bpa=-0.5142 degrees ! Estimated noise=1.53513 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00110042 Jy ! Component: 100 - total flux cleaned = -0.0015115 Jy ! Component: 150 - total flux cleaned = -0.00177659 Jy ! Component: 200 - total flux cleaned = -0.00184917 Jy ! Total flux subtracted in 200 components = -0.00184917 Jy ! Clean residual min=-0.004983 max=0.004742 Jy/beam ! Clean residual mean=0.000001 rms=0.001292 Jy/beam ! Combined flux in latest and established models = 2.00375 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 89 components and 2.00375 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.083365Jy sigma=0.784396 ! Fit after self-cal, rms=0.083323Jy sigma=0.783754 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 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 = -0.000330575 Jy ! Component: 100 - total flux cleaned = -0.000401274 Jy ! Component: 150 - total flux cleaned = -0.000469547 Jy ! Component: 200 - total flux cleaned = -0.000528433 Jy ! Total flux subtracted in 200 components = -0.000528433 Jy ! Clean residual min=-0.004932 max=0.004532 Jy/beam ! Clean residual mean=0.000001 rms=0.001269 Jy/beam ! Combined flux in latest and established models = 2.00322 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 92 components and 2.00322 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.083285Jy sigma=0.784219 ! Fit after self-cal, rms=0.083266Jy sigma=0.783838 ! Inverting map ! Your choice of large map pixels excluded 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 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 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=0.7295 mas, bmaj=1.021 mas, bpa=13.25 degrees ! Estimated noise=0.998811 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7295 x 1.021 at 13.25 degrees (North through East) ! Clean map min=-0.0090273 max=1.7204 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=0.083266Jy sigma=0.783838 ! Fit after self-cal, rms=0.065090Jy sigma=0.624847 ! Inverting map and beam ! Your choice of large map pixels excluded 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=0.7296 mas, bmaj=1.021 mas, bpa=13.25 degrees ! Estimated noise=0.998983 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00089362 Jy ! Component: 100 - total flux cleaned = 0.00099504 Jy ! Component: 150 - total flux cleaned = 0.000899105 Jy ! Component: 200 - total flux cleaned = 0.000816649 Jy ! Total flux subtracted in 200 components = 0.000816649 Jy ! Clean residual min=-0.004276 max=0.004558 Jy/beam ! Clean residual mean=0.000001 rms=0.000879 Jy/beam ! Combined flux in latest and established models = 2.00404 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 97 components and 2.00404 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.064764Jy sigma=0.620505 ! Fit after self-cal, rms=0.064759Jy sigma=0.620345 ! Inverting map ! Your choice of large map pixels excluded 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! Added new window around map position (-4, 16.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00393522 Jy ! Component: 100 - total flux cleaned = 0.00429574 Jy ! Component: 150 - total flux cleaned = 0.00437308 Jy ! Component: 200 - total flux cleaned = 0.00437053 Jy ! Total flux subtracted in 200 components = 0.00437053 Jy ! Clean residual min=-0.003863 max=0.003841 Jy/beam ! Clean residual mean=0.000000 rms=0.000841 Jy/beam ! Combined flux in latest and established models = 2.00841 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 108 components and 2.00841 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.064466Jy sigma=0.616265 ! Fit after self-cal, rms=0.064452Jy sigma=0.616013 ! Inverting map ! Your choice of large map pixels excluded 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.064452Jy sigma=0.616013 ! Fit after self-cal, rms=0.064339Jy sigma=0.615119 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 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=0.6592 mas, bmaj=0.7669 mas, bpa=27.67 degrees ! Estimated noise=1.37439 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.31651 Jy ! Component: 100 - total flux cleaned = 1.67297 Jy ! Component: 150 - total flux cleaned = 1.82675 Jy ! Component: 200 - total flux cleaned = 1.90604 Jy ! Total flux subtracted in 200 components = 1.90604 Jy ! Clean residual min=-0.011287 max=0.038597 Jy/beam ! Clean residual mean=0.000027 rms=0.002346 Jy/beam ! Combined flux in latest and established models = 1.90604 Jy uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Adding 14 model components to the UV plane model. ! The established model now contains 14 components and 1.90604 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=0.7291 mas, bmaj=1.022 mas, bpa=13.28 degrees ! Estimated noise=0.999424 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 = 0.0537752 Jy ! Component: 100 - total flux cleaned = 0.0797717 Jy ! Component: 150 - total flux cleaned = 0.0926131 Jy ! Component: 200 - total flux cleaned = 0.0962252 Jy ! Total flux subtracted in 200 components = 0.0962252 Jy ! Clean residual min=-0.008361 max=0.007411 Jy/beam ! Clean residual mean=0.000002 rms=0.001271 Jy/beam ! Combined flux in latest and established models = 2.00226 Jy ! Adding 21 model components to the UV plane model. ! The established model now contains 25 components and 2.00226 Jy ! Inverting map ! Your choice of large map pixels excluded 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 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 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=2.486 mas, bmaj=2.875 mas, bpa=-0.4943 degrees ! Estimated noise=1.53569 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00359834 Jy ! Component: 100 - total flux cleaned = 0.00477991 Jy ! Component: 150 - total flux cleaned = 0.005854 Jy ! Component: 200 - total flux cleaned = 0.00630139 Jy ! Total flux subtracted in 200 components = 0.00630139 Jy ! Clean residual min=-0.004457 max=0.004965 Jy/beam ! Clean residual mean=0.000004 rms=0.001254 Jy/beam ! Combined flux in latest and established models = 2.00856 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 = -4.84717e-06 Jy ! Component: 100 - total flux cleaned = 8.08607e-05 Jy ! Component: 150 - total flux cleaned = 0.000158692 Jy ! Component: 200 - total flux cleaned = 0.00015851 Jy ! Total flux subtracted in 200 components = 0.00015851 Jy ! Clean residual min=-0.004400 max=0.004881 Jy/beam ! Clean residual mean=0.000003 rms=0.001213 Jy/beam ! Combined flux in latest and established models = 2.00872 Jy ! Adding 31 model components to the UV plane model. ! The established model now contains 53 components and 2.00872 Jy ! Inverting map ! Your choice of large map pixels excluded 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! Estimated beam: bmin=0.7291 mas, bmaj=1.022 mas, bpa=13.28 degrees ! Estimated noise=0.999424 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000310579 Jy ! Component: 100 - total flux cleaned = -2.32058e-05 Jy ! Component: 150 - total flux cleaned = 0.000483768 Jy ! Component: 200 - total flux cleaned = 0.000478038 Jy ! Total flux subtracted in 200 components = 0.000478038 Jy ! Clean residual min=-0.006653 max=0.005547 Jy/beam ! Clean residual mean=0.000001 rms=0.001066 Jy/beam ! Combined flux in latest and established models = 2.0092 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 61 components and 2.0092 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.068124Jy sigma=0.673670 ! Fit after self-cal, rms=0.067654Jy sigma=0.666919 wmodel J0019+7327_X_map.mod ! Writing 61 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 5 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 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00123801 Jy ! Component: 100 - total flux cleaned = -0.000957474 Jy ! Component: 150 - total flux cleaned = -0.00059955 Jy ! Component: 200 - total flux cleaned = 3.44636e-06 Jy ! Component: 250 - total flux cleaned = 0.000503809 Jy ! Component: 300 - total flux cleaned = 0.00131408 Jy ! Component: 350 - total flux cleaned = 0.00194361 Jy ! Component: 400 - total flux cleaned = 0.00255879 Jy ! Component: 450 - total flux cleaned = 0.00331242 Jy ! Component: 500 - total flux cleaned = 0.00412504 Jy ! Component: 550 - total flux cleaned = 0.00477631 Jy ! Component: 600 - total flux cleaned = 0.00555823 Jy ! Component: 650 - total flux cleaned = 0.0063238 Jy ! Component: 700 - total flux cleaned = 0.00687017 Jy ! Component: 750 - total flux cleaned = 0.00747697 Jy ! Component: 800 - total flux cleaned = 0.00787489 Jy ! Component: 850 - total flux cleaned = 0.00846174 Jy ! Component: 900 - total flux cleaned = 0.00878237 Jy ! Component: 950 - total flux cleaned = 0.00909964 Jy ! Component: 1000 - total flux cleaned = 0.00960013 Jy ! Component: 1050 - total flux cleaned = 0.00990878 Jy ! Component: 1100 - total flux cleaned = 0.0104558 Jy ! Component: 1150 - total flux cleaned = 0.0108154 Jy ! Component: 1200 - total flux cleaned = 0.0109937 Jy ! Component: 1250 - total flux cleaned = 0.0112863 Jy ! Component: 1300 - total flux cleaned = 0.0116905 Jy ! Component: 1350 - total flux cleaned = 0.0119189 Jy ! Component: 1400 - total flux cleaned = 0.0123144 Jy ! Component: 1450 - total flux cleaned = 0.0126493 Jy ! Component: 1500 - total flux cleaned = 0.0128152 Jy ! Component: 1550 - total flux cleaned = 0.0131985 Jy ! Component: 1600 - total flux cleaned = 0.0136304 Jy ! Component: 1650 - total flux cleaned = 0.0140049 Jy ! Component: 1700 - total flux cleaned = 0.0142172 Jy ! Component: 1750 - total flux cleaned = 0.0144799 Jy ! Component: 1800 - total flux cleaned = 0.0148441 Jy ! Component: 1850 - total flux cleaned = 0.0152034 Jy ! Component: 1900 - total flux cleaned = 0.0153049 Jy ! Component: 1950 - total flux cleaned = 0.0156074 Jy ! Component: 2000 - total flux cleaned = 0.0155578 Jy ! Component: 2050 - total flux cleaned = 0.0158059 Jy ! Component: 2100 - total flux cleaned = 0.0161499 Jy ! Component: 2150 - total flux cleaned = 0.0160521 Jy ! Component: 2200 - total flux cleaned = 0.0161004 Jy ! Component: 2250 - total flux cleaned = 0.0162928 Jy ! Component: 2300 - total flux cleaned = 0.0162927 Jy ! Component: 2350 - total flux cleaned = 0.0163876 Jy ! Component: 2400 - total flux cleaned = 0.0166229 Jy ! Component: 2450 - total flux cleaned = 0.0165758 Jy ! Component: 2500 - total flux cleaned = 0.0166221 Jy ! Component: 2550 - total flux cleaned = 0.0167146 Jy ! Component: 2600 - total flux cleaned = 0.0168509 Jy ! Component: 2650 - total flux cleaned = 0.0168062 Jy ! Component: 2700 - total flux cleaned = 0.0171668 Jy ! Component: 2750 - total flux cleaned = 0.0171666 Jy ! Component: 2800 - total flux cleaned = 0.0174335 Jy ! Component: 2850 - total flux cleaned = 0.0174774 Jy ! Component: 2900 - total flux cleaned = 0.0176528 Jy ! Component: 2950 - total flux cleaned = 0.0176525 Jy ! Component: 3000 - total flux cleaned = 0.0178258 Jy ! Component: 3050 - total flux cleaned = 0.0179982 Jy ! Component: 3100 - total flux cleaned = 0.0181699 Jy ! Component: 3150 - total flux cleaned = 0.0182547 Jy ! Component: 3200 - total flux cleaned = 0.0183819 Jy ! Component: 3250 - total flux cleaned = 0.0183816 Jy ! Component: 3300 - total flux cleaned = 0.0185067 Jy ! Component: 3350 - total flux cleaned = 0.0183404 Jy ! Component: 3400 - total flux cleaned = 0.0185059 Jy ! Component: 3450 - total flux cleaned = 0.0187122 Jy ! Component: 3500 - total flux cleaned = 0.0187121 Jy ! Component: 3550 - total flux cleaned = 0.0186712 Jy ! Component: 3600 - total flux cleaned = 0.0187118 Jy ! Component: 3650 - total flux cleaned = 0.0187521 Jy ! Component: 3700 - total flux cleaned = 0.0187921 Jy ! Component: 3750 - total flux cleaned = 0.0187522 Jy ! Component: 3800 - total flux cleaned = 0.0190309 Jy ! Component: 3850 - total flux cleaned = 0.0190306 Jy ! Component: 3900 - total flux cleaned = 0.0189912 Jy ! Component: 3950 - total flux cleaned = 0.0190699 Jy ! Component: 4000 - total flux cleaned = 0.0190309 Jy ! Component: 4050 - total flux cleaned = 0.0191862 Jy ! Total flux subtracted in 4096 components = 0.0193024 Jy ! Clean residual min=-0.002116 max=0.002341 Jy/beam ! Clean residual mean=0.000002 rms=0.000616 Jy/beam ! Combined flux in latest and established models = 2.0285 Jy keep ! Adding 317 model components to the UV plane model. ! The established model now contains 373 components and 2.0285 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv122_uvs/J0019+7327_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7291 x 1.022 at 13.28 degrees (North through East) ! Clean map min=-0.0031138 max=1.7225 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv122_uvs/J0019+7327_X_map.fits wmodel /scr/pima/rv122_uvs/J0019+7327_X_map.mod ! Writing 373 model components to file: /scr/pima/rv122_uvs/J0019+7327_X_map.mod wobs /scr/pima/rv122_uvs/J0019+7327_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv122_uvs/J0019+7327_X_uvs.fits wwins /scr/pima/rv122_uvs/J0019+7327_X_map.win ! wwins: Wrote 6 windows to /scr/pima/rv122_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 1.72254 invert ! Inverting map ! Your choice of large map pixels excluded 0.731% of the data. ! The x-axis pixel size should ideally be below 0.1696 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00061619 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.107317 0.107317 0.214633 0.429266 0.858533 1.71707 3.43413 6.86826 13.7365 27.473 54.9461 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0018 print "peak= ", int(1000*peak_flux)/1000 ! peak= 1.722 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 2795.47 quit ! Quitting program ! Log file /scr/pima/rv122_uvs/J0019+7327_X_dfm.log closed on Fri Jul 13 21:06:05 2018