! Started logfile: /scr/pima/rv102_uvs/J2000-1748_X_dfm.log on Sat Nov 9 10:21:30 2019 float field_size field_size = 1024 float field_cell field_cell = 0.2000 float taper_size taper_size = 70.0 float freq freq = 8.40599 obs /scr/pima/rv102_uvs/J2000-1748_X_uva.fits ! Reading UV FITS file: /scr/pima/rv102_uvs/J2000-1748_X_uva.fits ! AN table 1: 9 integrations on 28 of 28 possible baselines. ! AN table 2: 9 integrations on 1 of 1 possible baselines. ! AN table 3: 9 integrations on 6 of 6 possible baselines. ! AN table 4: 9 integrations on 15 of 15 possible baselines. ! AN table 5: 9 integrations on 6 of 6 possible baselines. ! AN table 6: 133 integrations on 3 of 3 possible baselines. ! AN table 7: 40 integrations on 15 of 15 possible baselines. ! AN table 8: 18 integrations on 10 of 10 possible baselines. ! AN table 9: 17 integrations on 3 of 3 possible baselines. ! AN table 10: 20 integrations on 28 of 28 possible baselines. ! AN table 11: 9 integrations on 15 of 15 possible baselines. ! Apparent sampling: 0.771099 visibilities/baseline/integration-bin. ! Found source: J2000-1748 ! ! 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 8.40599e+09 8e+06 1 8e+06 ! 02 2 8.47599e+09 8e+06 1 8e+06 ! 03 3 8.79099e+09 8e+06 1 8e+06 ! 04 4 8.89599e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 79 lines of history. ! ! Reading 7492 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 J2000-1748_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 8 telescope corrections were flagged in sub-array 1. ! A total of 18 telescope corrections were flagged in sub-array 2. ! A total of 8 telescope corrections were flagged in sub-array 3. ! A total of 13 telescope corrections were flagged in sub-array 4. ! A total of 8 telescope corrections were flagged in sub-array 5. ! A total of 201 telescope corrections were flagged in sub-array 6. ! A total of 100 telescope corrections were flagged in sub-array 7. ! A total of 27 telescope corrections were flagged in sub-array 8. ! A total of 30 telescope corrections were flagged in sub-array 9. ! A total of 69 telescope corrections were flagged in sub-array 10. ! A total of 12 telescope corrections were flagged in sub-array 11. ! ! Correcting IF 2. ! A total of 8 telescope corrections were flagged in sub-array 1. ! A total of 18 telescope corrections were flagged in sub-array 2. ! A total of 8 telescope corrections were flagged in sub-array 3. ! A total of 13 telescope corrections were flagged in sub-array 4. ! A total of 8 telescope corrections were flagged in sub-array 5. ! A total of 201 telescope corrections were flagged in sub-array 6. ! A total of 100 telescope corrections were flagged in sub-array 7. ! A total of 27 telescope corrections were flagged in sub-array 8. ! A total of 30 telescope corrections were flagged in sub-array 9. ! A total of 69 telescope corrections were flagged in sub-array 10. ! A total of 12 telescope corrections were flagged in sub-array 11. ! ! Correcting IF 3. ! A total of 8 telescope corrections were flagged in sub-array 1. ! A total of 18 telescope corrections were flagged in sub-array 2. ! A total of 8 telescope corrections were flagged in sub-array 3. ! A total of 13 telescope corrections were flagged in sub-array 4. ! A total of 8 telescope corrections were flagged in sub-array 5. ! A total of 201 telescope corrections were flagged in sub-array 6. ! A total of 100 telescope corrections were flagged in sub-array 7. ! A total of 27 telescope corrections were flagged in sub-array 8. ! A total of 30 telescope corrections were flagged in sub-array 9. ! A total of 69 telescope corrections were flagged in sub-array 10. ! A total of 12 telescope corrections were flagged in sub-array 11. ! ! Correcting IF 4. ! A total of 8 telescope corrections were flagged in sub-array 1. ! A total of 18 telescope corrections were flagged in sub-array 2. ! A total of 8 telescope corrections were flagged in sub-array 3. ! A total of 13 telescope corrections were flagged in sub-array 4. ! A total of 8 telescope corrections were flagged in sub-array 5. ! A total of 201 telescope corrections were flagged in sub-array 6. ! A total of 100 telescope corrections were flagged in sub-array 7. ! A total of 27 telescope corrections were flagged in sub-array 8. ! A total of 30 telescope corrections were flagged in sub-array 9. ! A total of 69 telescope corrections were flagged in sub-array 10. ! A total of 12 telescope corrections were flagged in sub-array 11. ! ! Fit before self-cal, rms=1.837338Jy sigma=17.924426 ! Fit after self-cal, rms=0.604122Jy sigma=5.725652 ! 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 1.71% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=0.5856 mas, bmaj=2.866 mas, bpa=-9.359 degrees ! Estimated noise=1.38774 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 = 1.18564 Jy ! Component: 100 - total flux cleaned = 1.44419 Jy ! Total flux subtracted in 100 components = 1.44419 Jy ! Clean residual min=-0.041722 max=0.073881 Jy/beam ! Clean residual mean=0.000674 rms=0.008073 Jy/beam ! Combined flux in latest and established models = 1.44419 Jy ! Performing phase self-cal ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 1.44419 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.295166Jy sigma=2.592259 ! Fit after self-cal, rms=0.295162Jy sigma=2.592245 ! Inverting map ! Your choice of large map pixels excluded 1.71% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Added new window around map position (0.8, 3.8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0781954 Jy ! Component: 100 - total flux cleaned = 0.119565 Jy ! Total flux subtracted in 100 components = 0.119565 Jy ! Clean residual min=-0.030440 max=0.050656 Jy/beam ! Clean residual mean=0.000425 rms=0.006568 Jy/beam ! Combined flux in latest and established models = 1.56376 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 13 components and 1.56376 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.271174Jy sigma=2.358306 ! Fit after self-cal, rms=0.270412Jy sigma=2.346947 ! Inverting map ! Your choice of large map pixels excluded 1.71% of the data. ! The x-axis pixel size should ideally be below 0.1918 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 1.71% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=0.7153 mas, bmaj=3.187 mas, bpa=-8.179 degrees ! Estimated noise=1.05002 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 (2, 0.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0307733 Jy ! Component: 100 - total flux cleaned = 0.037633 Jy ! Component: 150 - total flux cleaned = 0.0399714 Jy ! Component: 200 - total flux cleaned = 0.0412843 Jy ! Total flux subtracted in 200 components = 0.0412843 Jy ! Clean residual min=-0.022843 max=0.025655 Jy/beam ! Clean residual mean=-0.000084 rms=0.005861 Jy/beam ! Combined flux in latest and established models = 1.60504 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 38 components and 1.60504 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.263337Jy sigma=2.271367 ! Fit after self-cal, rms=0.262971Jy sigma=2.266348 ! Inverting map ! Your choice of large map pixels excluded 1.71% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec print "============== Finished natural weighting clean ==============" ! ============== Finished natural weighting clean ============== ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7153 x 3.187 at -8.179 degrees (North through East) ! Clean map min=-0.025205 max=1.5052 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! FD 0.99 HN 1.15 KP 1.00 LA 1.00 ! NL 1.11 PT 1.01 SC 0.99 WF 0.88 ! ! Telescope amplitude corrections in sub-array 2: ! MK 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! KP 0.98 LA 1.00 MK 0.99 PT 1.01 ! ! Telescope amplitude corrections in sub-array 4: ! FD 0.96 KP 0.96 LA 0.95 MK 0.99 ! NL 0.95 PT 1.00 ! ! Telescope amplitude corrections in sub-array 5: ! FD 1.19 KP 1.27 MK 0.93 PT 1.15 ! ! A total of 198 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! MA 0.00* ON 0.00* WZ 0.00* ! ! A total of 48 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! HN 1.26 MA 1.01 ON 1.01 SC 1.01 ! WF 0.92 WZ 0.94 ! ! A total of 24 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! HN 1.34 MA 0.99 ON 0.99 WF 0.96 ! WZ 0.92 ! ! A total of 21 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! MA 0.00* WF 0.00* WZ 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 10. ! Telescope amplitude corrections in sub-array 10: ! FD 1.00 HN 1.08 LA 1.03 MA 1.02 ! PT 1.04 SC 0.99 WF 0.89 WZ 0.95 ! ! Telescope amplitude corrections in sub-array 11: ! FD 0.96 HN 1.05 LA 1.00 PT 0.97 ! SC 0.98 WF 0.87 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! FD 0.97 HN 1.17 KP 0.97 LA 1.00 ! NL 1.10 PT 1.02 SC 1.00 WF 0.87 ! ! Telescope amplitude corrections in sub-array 2: ! MK 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! KP 0.96 LA 1.01 MK 0.94 PT 1.00 ! ! Telescope amplitude corrections in sub-array 4: ! FD 0.95 KP 0.94 LA 0.95 MK 0.95 ! NL 0.92 PT 1.01 ! ! Telescope amplitude corrections in sub-array 5: ! FD 1.16 KP 1.29 MK 0.94 PT 1.11 ! ! A total of 198 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! MA 0.00* ON 0.00* WZ 0.00* ! ! A total of 48 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! HN 1.23 MA 0.95 ON 1.04 SC 1.02 ! WF 0.91 WZ 0.98 ! ! A total of 24 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! HN 1.19 MA 0.95 ON 1.04 WF 0.89 ! WZ 1.02 ! ! A total of 21 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! MA 0.00* WF 0.00* WZ 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 10. ! Telescope amplitude corrections in sub-array 10: ! FD 1.01 HN 1.09 LA 1.01 MA 1.00 ! PT 1.05 SC 0.96 WF 0.88 WZ 1.02 ! ! Telescope amplitude corrections in sub-array 11: ! FD 0.96 HN 1.04 LA 0.99 PT 0.96 ! SC 0.99 WF 0.86 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! FD 0.97 HN 1.14 KP 0.98 LA 0.99 ! NL 1.13 PT 1.01 SC 0.99 WF 0.86 ! ! Telescope amplitude corrections in sub-array 2: ! MK 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! KP 0.97 LA 0.98 MK 0.96 PT 1.01 ! ! Telescope amplitude corrections in sub-array 4: ! FD 0.97 KP 0.95 LA 0.94 MK 0.96 ! NL 0.94 PT 0.98 ! ! Telescope amplitude corrections in sub-array 5: ! FD 1.17 KP 1.26 MK 0.94 PT 1.11 ! ! A total of 198 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! MA 0.00* ON 0.00* WZ 0.00* ! ! A total of 48 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! HN 1.16 MA 1.02 ON 1.03 SC 1.01 ! WF 0.89 WZ 0.98 ! ! A total of 24 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! HN 1.17 MA 1.04 ON 0.98 WF 0.92 ! WZ 0.98 ! ! A total of 21 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! MA 0.00* WF 0.00* WZ 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 10. ! Telescope amplitude corrections in sub-array 10: ! FD 1.00 HN 1.05 LA 1.01 MA 1.10 ! PT 1.02 SC 0.96 WF 0.85 WZ 1.02 ! ! Telescope amplitude corrections in sub-array 11: ! FD 0.95 HN 0.98 LA 0.97 PT 0.96 ! SC 0.98 WF 0.87 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! FD 0.98 HN 1.11 KP 0.99 LA 1.00 ! NL 1.15 PT 0.99 SC 0.97 WF 0.86 ! ! Telescope amplitude corrections in sub-array 2: ! MK 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! KP 0.97 LA 0.98 MK 0.99 PT 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! FD 0.94 KP 0.95 LA 0.95 MK 0.99 ! NL 0.93 PT 0.98 ! ! Telescope amplitude corrections in sub-array 5: ! FD 1.15 KP 1.22 MK 0.95 PT 1.05 ! ! A total of 198 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! MA 0.00* ON 0.00* WZ 0.00* ! ! A total of 48 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! HN 1.15 MA 1.08 ON 1.08 SC 0.99 ! WF 0.88 WZ 0.94 ! ! A total of 24 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! HN 1.15 MA 1.11 ON 1.07 WF 0.92 ! WZ 0.92 ! ! A total of 21 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! MA 0.00* WF 0.00* WZ 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 10. ! Telescope amplitude corrections in sub-array 10: ! FD 0.98 HN 1.02 LA 1.00 MA 1.17 ! PT 1.01 SC 0.95 WF 0.85 WZ 0.96 ! ! Telescope amplitude corrections in sub-array 11: ! FD 0.94 HN 1.02 LA 0.96 PT 0.94 ! SC 1.00 WF 0.87 ! ! ! Fit before self-cal, rms=0.262971Jy sigma=2.266348 ! Fit after self-cal, rms=0.207675Jy sigma=1.666501 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=0.6737 mas, bmaj=3.018 mas, bpa=-8.83 degrees ! Estimated noise=1.16398 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 = -0.00114411 Jy ! Component: 100 - total flux cleaned = 0.00015062 Jy ! Component: 150 - total flux cleaned = -0.000250524 Jy ! Component: 200 - total flux cleaned = -0.000599779 Jy ! Total flux subtracted in 200 components = -0.000599779 Jy ! Clean residual min=-0.010531 max=0.008957 Jy/beam ! Clean residual mean=-0.000304 rms=0.002326 Jy/beam ! Combined flux in latest and established models = 1.60444 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 51 components and 1.60444 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.206945Jy sigma=1.659904 ! Fit after self-cal, rms=0.207061Jy sigma=1.658357 ! Inverting map ! Your choice of large map pixels excluded 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 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=0.207061Jy sigma=1.658357 ! Fit after self-cal, rms=0.204190Jy sigma=1.630876 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=0.6737 mas, bmaj=3.018 mas, bpa=-8.834 degrees ! Estimated noise=1.1641 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00310549 Jy ! Component: 100 - total flux cleaned = -0.00310192 Jy ! Component: 150 - total flux cleaned = -0.00325985 Jy ! Component: 200 - total flux cleaned = -0.00325705 Jy ! Total flux subtracted in 200 components = -0.00325705 Jy ! Clean residual min=-0.009182 max=0.007389 Jy/beam ! Clean residual mean=-0.000397 rms=0.001905 Jy/beam ! Combined flux in latest and established models = 1.60118 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 63 components and 1.60118 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.203783Jy sigma=1.627377 ! Fit after self-cal, rms=0.203764Jy sigma=1.626951 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 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 = -0.00153099 Jy ! Component: 100 - total flux cleaned = -0.00195741 Jy ! Component: 150 - total flux cleaned = -0.00208218 Jy ! Component: 200 - total flux cleaned = -0.00207769 Jy ! Total flux subtracted in 200 components = -0.00207769 Jy ! Clean residual min=-0.008741 max=0.007445 Jy/beam ! Clean residual mean=-0.000351 rms=0.001871 Jy/beam ! Combined flux in latest and established models = 1.59911 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 69 components and 1.59911 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.203555Jy sigma=1.625342 ! Fit after self-cal, rms=0.203545Jy sigma=1.625150 ! Inverting map ! Your choice of large map pixels excluded 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 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=0.203545Jy sigma=1.625150 ! Fit after self-cal, rms=0.202532Jy sigma=1.610202 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=0.6737 mas, bmaj=3.016 mas, bpa=-8.835 degrees ! Estimated noise=1.16385 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00409763 Jy ! Component: 100 - total flux cleaned = -0.00443767 Jy ! Component: 150 - total flux cleaned = -0.00471741 Jy ! Component: 200 - total flux cleaned = -0.00471344 Jy ! Total flux subtracted in 200 components = -0.00471344 Jy ! Clean residual min=-0.007127 max=0.006354 Jy/beam ! Clean residual mean=-0.000437 rms=0.001617 Jy/beam ! Combined flux in latest and established models = 1.59439 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 76 components and 1.59439 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.202236Jy sigma=1.607831 ! Fit after self-cal, rms=0.202243Jy sigma=1.607509 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 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 = -0.00119855 Jy ! Component: 100 - total flux cleaned = -0.00155668 Jy ! Component: 150 - total flux cleaned = -0.00177249 Jy ! Component: 200 - total flux cleaned = -0.00206469 Jy ! Total flux subtracted in 200 components = -0.00206469 Jy ! Clean residual min=-0.006897 max=0.006364 Jy/beam ! Clean residual mean=-0.000392 rms=0.001590 Jy/beam ! Combined flux in latest and established models = 1.59233 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 79 components and 1.59233 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.202088Jy sigma=1.606431 ! Fit after self-cal, rms=0.202086Jy sigma=1.606307 ! Inverting map ! Your choice of large map pixels excluded 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 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=0.202086Jy sigma=1.606307 ! Fit after self-cal, rms=0.202178Jy sigma=1.605619 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=2.403 mas, bmaj=3.774 mas, bpa=-11.51 degrees ! Estimated noise=1.56882 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00371987 Jy ! Component: 100 - total flux cleaned = -0.00371955 Jy ! Component: 150 - total flux cleaned = -0.0037236 Jy ! Component: 200 - total flux cleaned = -0.00363022 Jy ! Total flux subtracted in 200 components = -0.00363022 Jy ! Clean residual min=-0.007223 max=0.006148 Jy/beam ! Clean residual mean=-0.000846 rms=0.001898 Jy/beam ! Combined flux in latest and established models = 1.5887 Jy selfcal ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 97 components and 1.5887 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.202105Jy sigma=1.605453 ! Fit after self-cal, rms=0.202103Jy sigma=1.605196 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 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 = -0.00067667 Jy ! Component: 100 - total flux cleaned = -0.000599182 Jy ! Component: 150 - total flux cleaned = -0.000527001 Jy ! Component: 200 - total flux cleaned = -0.00052394 Jy ! Total flux subtracted in 200 components = -0.00052394 Jy ! Clean residual min=-0.007053 max=0.006152 Jy/beam ! Clean residual mean=-0.000819 rms=0.001879 Jy/beam ! Combined flux in latest and established models = 1.58817 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 102 components and 1.58817 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.202090Jy sigma=1.605299 ! Fit after self-cal, rms=0.202090Jy sigma=1.605199 ! Inverting map ! Your choice of large map pixels excluded 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 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 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=0.6737 mas, bmaj=3.016 mas, bpa=-8.842 degrees ! Estimated noise=1.16367 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6737 x 3.016 at -8.842 degrees (North through East) ! Clean map min=-0.011987 max=1.5061 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=0.202090Jy sigma=1.605199 ! Fit after self-cal, rms=0.179826Jy sigma=1.357333 ! Inverting map and beam ! Your choice of large map pixels excluded 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=0.6736 mas, bmaj=3.016 mas, bpa=-8.852 degrees ! Estimated noise=1.16338 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00146534 Jy ! Component: 100 - total flux cleaned = -0.00136721 Jy ! Component: 150 - total flux cleaned = -0.00127462 Jy ! Component: 200 - total flux cleaned = -0.0012744 Jy ! Total flux subtracted in 200 components = -0.0012744 Jy ! Clean residual min=-0.006907 max=0.005841 Jy/beam ! Clean residual mean=-0.000429 rms=0.001501 Jy/beam ! Combined flux in latest and established models = 1.5869 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 109 components and 1.5869 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.179688Jy sigma=1.356141 ! Fit after self-cal, rms=0.179678Jy sigma=1.356003 ! Inverting map ! Your choice of large map pixels excluded 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000541413 Jy ! Component: 100 - total flux cleaned = -0.000707936 Jy ! Component: 150 - total flux cleaned = -0.000708033 Jy ! Component: 200 - total flux cleaned = -0.000707783 Jy ! Total flux subtracted in 200 components = -0.000707783 Jy ! Clean residual min=-0.006781 max=0.005754 Jy/beam ! Clean residual mean=-0.000413 rms=0.001487 Jy/beam ! Combined flux in latest and established models = 1.58619 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 113 components and 1.58619 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.179590Jy sigma=1.355371 ! Fit after self-cal, rms=0.179588Jy sigma=1.355301 ! Inverting map ! Your choice of large map pixels excluded 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.179588Jy sigma=1.355301 ! Fit after self-cal, rms=0.179688Jy sigma=1.354995 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 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=0.5628 mas, bmaj=2.779 mas, bpa=-9.848 degrees ! Estimated noise=1.47524 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.17838 Jy ! Component: 100 - total flux cleaned = 1.4357 Jy ! Component: 150 - total flux cleaned = 1.50726 Jy ! Component: 200 - total flux cleaned = 1.54302 Jy ! Total flux subtracted in 200 components = 1.54302 Jy ! Clean residual min=-0.010291 max=0.017251 Jy/beam ! Clean residual mean=0.000096 rms=0.002543 Jy/beam ! Combined flux in latest and established models = 1.54303 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 10 model components to the UV plane model. ! The established model now contains 10 components and 1.54303 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=0.6737 mas, bmaj=3.016 mas, bpa=-8.857 degrees ! Estimated noise=1.16352 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 = 0.0250289 Jy ! Component: 100 - total flux cleaned = 0.0383354 Jy ! Component: 150 - total flux cleaned = 0.0444572 Jy ! Component: 200 - total flux cleaned = 0.0463435 Jy ! Total flux subtracted in 200 components = 0.0463435 Jy ! Clean residual min=-0.007973 max=0.006168 Jy/beam ! Clean residual mean=-0.000514 rms=0.001674 Jy/beam ! Combined flux in latest and established models = 1.58937 Jy ! Adding 20 model components to the UV plane model. ! The established model now contains 27 components and 1.58937 Jy ! Inverting map ! Your choice of large map pixels excluded 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 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 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=2.402 mas, bmaj=3.775 mas, bpa=-11.58 degrees ! Estimated noise=1.56943 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00027974 Jy ! Component: 100 - total flux cleaned = -0.000715343 Jy ! Component: 150 - total flux cleaned = -0.00122598 Jy ! Component: 200 - total flux cleaned = -0.00166286 Jy ! Total flux subtracted in 200 components = -0.00166286 Jy ! Clean residual min=-0.008780 max=0.005535 Jy/beam ! Clean residual mean=-0.001125 rms=0.001992 Jy/beam ! Combined flux in latest and established models = 1.58771 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 = -0.000376702 Jy ! Component: 100 - total flux cleaned = -0.000378372 Jy ! Component: 150 - total flux cleaned = -0.000588934 Jy ! Component: 200 - total flux cleaned = -0.000685634 Jy ! Total flux subtracted in 200 components = -0.000685634 Jy ! Clean residual min=-0.008379 max=0.005421 Jy/beam ! Clean residual mean=-0.001091 rms=0.001930 Jy/beam ! Combined flux in latest and established models = 1.58702 Jy ! Adding 27 model components to the UV plane model. ! The established model now contains 51 components and 1.58702 Jy ! Inverting map ! Your choice of large map pixels excluded 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! Estimated beam: bmin=0.6737 mas, bmaj=3.016 mas, bpa=-8.857 degrees ! Estimated noise=1.16352 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0010967 Jy ! Component: 100 - total flux cleaned = 0.000938148 Jy ! Component: 150 - total flux cleaned = 0.000795386 Jy ! Component: 200 - total flux cleaned = 0.000654048 Jy ! Total flux subtracted in 200 components = 0.000654048 Jy ! Clean residual min=-0.006471 max=0.005902 Jy/beam ! Clean residual mean=-0.000481 rms=0.001504 Jy/beam ! Combined flux in latest and established models = 1.58767 Jy selfcal ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 70 components and 1.58767 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.179895Jy sigma=1.356258 ! Fit after self-cal, rms=0.179824Jy sigma=1.355157 wmodel J2000-1748_X_map.mod ! Writing 70 model components to file: J2000-1748_X_map.mod wobs J2000-1748_X_uvs.fits ! Writing UV FITS file: J2000-1748_X_uvs.fits wwins J2000-1748_X_map.win ! wwins: Wrote 3 windows to J2000-1748_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 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00251044 Jy ! Component: 100 - total flux cleaned = -0.00446129 Jy ! Component: 150 - total flux cleaned = -0.00600681 Jy ! Component: 200 - total flux cleaned = -0.0072981 Jy ! Component: 250 - total flux cleaned = -0.00874216 Jy ! Component: 300 - total flux cleaned = -0.0096816 Jy ! Component: 350 - total flux cleaned = -0.0103267 Jy ! Component: 400 - total flux cleaned = -0.0110499 Jy ! Component: 450 - total flux cleaned = -0.0116706 Jy ! Component: 500 - total flux cleaned = -0.0120192 Jy ! Component: 550 - total flux cleaned = -0.0125364 Jy ! Component: 600 - total flux cleaned = -0.0129608 Jy ! Component: 650 - total flux cleaned = -0.0132127 Jy ! Component: 700 - total flux cleaned = -0.0138743 Jy ! Component: 750 - total flux cleaned = -0.0142011 Jy ! Component: 800 - total flux cleaned = -0.0147656 Jy ! Component: 850 - total flux cleaned = -0.0153227 Jy ! Component: 900 - total flux cleaned = -0.0156374 Jy ! Component: 950 - total flux cleaned = -0.0161814 Jy ! Component: 1000 - total flux cleaned = -0.0165649 Jy ! Component: 1050 - total flux cleaned = -0.0168691 Jy ! Component: 1100 - total flux cleaned = -0.0172465 Jy ! Component: 1150 - total flux cleaned = -0.0176937 Jy ! Component: 1200 - total flux cleaned = -0.0181363 Jy ! Component: 1250 - total flux cleaned = -0.0183551 Jy ! Component: 1300 - total flux cleaned = -0.0190057 Jy ! Component: 1350 - total flux cleaned = -0.019292 Jy ! Component: 1400 - total flux cleaned = -0.0195053 Jy ! Component: 1450 - total flux cleaned = -0.0199271 Jy ! Component: 1500 - total flux cleaned = -0.0202753 Jy ! Component: 1550 - total flux cleaned = -0.0206205 Jy ! Component: 1600 - total flux cleaned = -0.0209628 Jy ! Component: 1650 - total flux cleaned = -0.0213023 Jy ! Component: 1700 - total flux cleaned = -0.0216385 Jy ! Component: 1750 - total flux cleaned = -0.021905 Jy ! Component: 1800 - total flux cleaned = -0.0222361 Jy ! Component: 1850 - total flux cleaned = -0.0225649 Jy ! Component: 1900 - total flux cleaned = -0.0228906 Jy ! Component: 1950 - total flux cleaned = -0.0232137 Jy ! Component: 2000 - total flux cleaned = -0.0234701 Jy ! Component: 2050 - total flux cleaned = -0.0237245 Jy ! Component: 2100 - total flux cleaned = -0.0239771 Jy ! Component: 2150 - total flux cleaned = -0.0242907 Jy ! Component: 2200 - total flux cleaned = -0.0244774 Jy ! Component: 2250 - total flux cleaned = -0.0247861 Jy ! Component: 2300 - total flux cleaned = -0.0250317 Jy ! Component: 2350 - total flux cleaned = -0.0252751 Jy ! Component: 2400 - total flux cleaned = -0.0255169 Jy ! Component: 2450 - total flux cleaned = -0.0257569 Jy ! Component: 2500 - total flux cleaned = -0.025995 Jy ! Component: 2550 - total flux cleaned = -0.0261724 Jy ! Component: 2600 - total flux cleaned = -0.0265246 Jy ! Component: 2650 - total flux cleaned = -0.0268158 Jy ! Component: 2700 - total flux cleaned = -0.0270471 Jy ! Component: 2750 - total flux cleaned = -0.0272765 Jy ! Component: 2800 - total flux cleaned = -0.0273905 Jy ! Component: 2850 - total flux cleaned = -0.0276744 Jy ! Component: 2900 - total flux cleaned = -0.0279 Jy ! Component: 2950 - total flux cleaned = -0.0280679 Jy ! Component: 3000 - total flux cleaned = -0.0282904 Jy ! Component: 3050 - total flux cleaned = -0.0284563 Jy ! Component: 3100 - total flux cleaned = -0.028786 Jy ! Component: 3150 - total flux cleaned = -0.0288403 Jy ! Component: 3200 - total flux cleaned = -0.0291115 Jy ! Component: 3250 - total flux cleaned = -0.0292192 Jy ! Component: 3300 - total flux cleaned = -0.0293799 Jy ! Component: 3350 - total flux cleaned = -0.0295398 Jy ! Component: 3400 - total flux cleaned = -0.0296455 Jy ! Component: 3450 - total flux cleaned = -0.0298035 Jy ! Component: 3500 - total flux cleaned = -0.0299081 Jy ! Component: 3550 - total flux cleaned = -0.0300121 Jy ! Component: 3600 - total flux cleaned = -0.0300639 Jy ! Component: 3650 - total flux cleaned = -0.0302696 Jy ! Component: 3700 - total flux cleaned = -0.0302699 Jy ! Component: 3750 - total flux cleaned = -0.0303716 Jy ! Component: 3800 - total flux cleaned = -0.0305233 Jy ! Component: 3850 - total flux cleaned = -0.0305735 Jy ! Component: 3900 - total flux cleaned = -0.0307238 Jy ! Component: 3950 - total flux cleaned = -0.0308731 Jy ! Component: 4000 - total flux cleaned = -0.0309225 Jy ! Component: 4050 - total flux cleaned = -0.0310704 Jy ! Total flux subtracted in 4096 components = -0.0311685 Jy ! Clean residual min=-0.002554 max=0.002828 Jy/beam ! Clean residual mean=-0.000073 rms=0.000860 Jy/beam ! Combined flux in latest and established models = 1.55651 Jy keep ! Adding 320 model components to the UV plane model. ! The established model now contains 390 components and 1.55651 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv102_uvs/J2000-1748_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6737 x 3.016 at -8.857 degrees (North through East) ! Clean map min=-0.0059678 max=1.5118 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv102_uvs/J2000-1748_X_map.fits wmodel /scr/pima/rv102_uvs/J2000-1748_X_map.mod ! Writing 390 model components to file: /scr/pima/rv102_uvs/J2000-1748_X_map.mod wobs /scr/pima/rv102_uvs/J2000-1748_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv102_uvs/J2000-1748_X_uvs.fits wwins /scr/pima/rv102_uvs/J2000-1748_X_map.win ! wwins: Wrote 4 windows to /scr/pima/rv102_uvs/J2000-1748_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 1.51176 invert ! Inverting map ! Your choice of large map pixels excluded 2.2% of the data. ! The x-axis pixel size should ideally be below 0.1918 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000859209 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.170505 0.170505 0.341011 0.682021 1.36404 2.72809 5.45617 10.9123 21.8247 43.6494 87.2987 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0025 print "peak= ", int(1000*peak_flux)/1000 ! peak= 1.511 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 1759.47 quit ! Quitting program ! Log file /scr/pima/rv102_uvs/J2000-1748_X_dfm.log closed on Sat Nov 9 10:21:34 2019