! Started logfile: /scr/pima/rv120_uvs/J1125+2610_X_dfm.log on Fri Dec 22 22:41:42 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/rv120_uvs/J1125+2610_X_uva.fits ! Reading UV FITS file: /scr/pima/rv120_uvs/J1125+2610_X_uva.fits ! AN table 1: 29 integrations on 36 of 36 possible baselines. ! AN table 2: 37 integrations on 21 of 21 possible baselines. ! AN table 3: 11 integrations on 6 of 6 possible baselines. ! AN table 4: 2 integrations on 6 of 6 possible baselines. ! AN table 5: 80 integrations on 36 of 36 possible baselines. ! AN table 6: 8 integrations on 45 of 45 possible baselines. ! AN table 7: 7 integrations on 28 of 28 possible baselines. ! AN table 8: 6 integrations on 36 of 36 possible baselines. ! Apparent sampling: 0.254729 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1125+2610 ! ! 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 5656 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 J1125+2610_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 199 telescope corrections were flagged in sub-array 1. ! A total of 181 telescope corrections were flagged in sub-array 2. ! A total of 20 telescope corrections were flagged in sub-array 3. ! A total of 505 telescope corrections were flagged in sub-array 5. ! A total of 38 telescope corrections were flagged in sub-array 6. ! A total of 34 telescope corrections were flagged in sub-array 7. ! A total of 30 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 2. ! A total of 199 telescope corrections were flagged in sub-array 1. ! A total of 181 telescope corrections were flagged in sub-array 2. ! A total of 20 telescope corrections were flagged in sub-array 3. ! A total of 505 telescope corrections were flagged in sub-array 5. ! A total of 38 telescope corrections were flagged in sub-array 6. ! A total of 34 telescope corrections were flagged in sub-array 7. ! A total of 30 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 3. ! A total of 199 telescope corrections were flagged in sub-array 1. ! A total of 181 telescope corrections were flagged in sub-array 2. ! A total of 20 telescope corrections were flagged in sub-array 3. ! A total of 505 telescope corrections were flagged in sub-array 5. ! A total of 38 telescope corrections were flagged in sub-array 6. ! A total of 34 telescope corrections were flagged in sub-array 7. ! A total of 30 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 4. ! A total of 199 telescope corrections were flagged in sub-array 1. ! A total of 181 telescope corrections were flagged in sub-array 2. ! A total of 20 telescope corrections were flagged in sub-array 3. ! A total of 505 telescope corrections were flagged in sub-array 5. ! A total of 38 telescope corrections were flagged in sub-array 6. ! A total of 34 telescope corrections were flagged in sub-array 7. ! A total of 30 telescope corrections were flagged in sub-array 8. ! ! Fit before self-cal, rms=1.211600Jy sigma=18.084055 ! Fit after self-cal, rms=0.378846Jy sigma=5.060727 ! 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 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1705 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec ! Estimated beam: bmin=0.6731 mas, bmaj=0.9218 mas, bpa=-12.66 degrees ! Estimated noise=1.05549 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 = 0.513383 Jy ! Component: 100 - total flux cleaned = 0.647274 Jy ! Total flux subtracted in 100 components = 0.647274 Jy ! Clean residual min=-0.016137 max=0.052497 Jy/beam ! Clean residual mean=0.000004 rms=0.003646 Jy/beam ! Combined flux in latest and established models = 0.647274 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.647274 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.159169Jy sigma=2.118882 ! Fit after self-cal, rms=0.159074Jy sigma=2.118098 ! Inverting map ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1705 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0537398 Jy ! Component: 100 - total flux cleaned = 0.0794014 Jy ! Total flux subtracted in 100 components = 0.0794014 Jy ! Clean residual min=-0.013060 max=0.027118 Jy/beam ! Clean residual mean=0.000008 rms=0.002854 Jy/beam ! Combined flux in latest and established models = 0.726675 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 12 components and 0.726675 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.139663Jy sigma=1.668258 ! Fit after self-cal, rms=0.139569Jy sigma=1.667052 ! Inverting map ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1705 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec ! Added new window around map position (-1.2, 0.8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0245582 Jy ! Component: 100 - total flux cleaned = 0.0373909 Jy ! Total flux subtracted in 100 components = 0.0373909 Jy ! Clean residual min=-0.012768 max=0.022623 Jy/beam ! Clean residual mean=0.000009 rms=0.002686 Jy/beam ! Combined flux in latest and established models = 0.764066 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 23 components and 0.764066 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.134920Jy sigma=1.562825 ! Fit after self-cal, rms=0.134231Jy sigma=1.551442 ! Inverting map ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1705 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec ! Added new window around map position (1.2, -0.6). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0160423 Jy ! Component: 100 - total flux cleaned = 0.0214906 Jy ! Total flux subtracted in 100 components = 0.0214906 Jy ! Clean residual min=-0.011684 max=0.011561 Jy/beam ! Clean residual mean=0.000010 rms=0.002592 Jy/beam ! Combined flux in latest and established models = 0.785557 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 31 components and 0.785557 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.131957Jy sigma=1.508002 ! Fit after self-cal, rms=0.131906Jy sigma=1.507482 ! Inverting map ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1705 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 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 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1705 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec ! Estimated beam: bmin=0.7947 mas, bmaj=1.134 mas, bpa=-10.16 degrees ! Estimated noise=0.819734 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 = 0.00556508 Jy ! Component: 100 - total flux cleaned = 0.00661612 Jy ! Component: 150 - total flux cleaned = 0.00811569 Jy ! Component: 200 - total flux cleaned = 0.00913438 Jy ! Total flux subtracted in 200 components = 0.00913438 Jy ! Clean residual min=-0.012552 max=0.011218 Jy/beam ! Clean residual mean=0.000014 rms=0.002475 Jy/beam ! Combined flux in latest and established models = 0.794691 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 37 components and 0.794691 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.130160Jy sigma=1.483974 ! Fit after self-cal, rms=0.130132Jy sigma=1.483595 ! Inverting map ! Your choice of large map pixels excluded 4.13% of the data. ! The x-axis pixel size should ideally be below 0.1705 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7947 x 1.134 at -10.16 degrees (North through East) ! Clean map min=-0.011886 max=0.64512 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.99 KK 1.06 KP 0.97 ! LA 1.03 MK 0.92 NL 1.04 OV 1.00 ! PT 1.04 ! ! A total of 30 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 KK 0.99 KP 0.98 MK 1.03 ! NY 1.01 OV 1.02 PT 1.04 ! ! Telescope amplitude corrections in sub-array 3: ! KK 1.38 NY 0.89 ON 0.96 WZ 1.14 ! ! Telescope amplitude corrections in sub-array 4: ! FD 1.00 KP 1.18 LA 1.02 SC 0.90 ! ! A total of 102 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.05 HH 0.98 HN 1.13 LA 1.01 ! NL 0.97 NY 0.93 ON 0.98 SC 1.03 ! WZ 0.95 ! ! A total of 6 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.06 FD 1.03 HN 1.03 KP 1.03 ! LA 0.96 NL 0.98 NY 1.00 ON 0.97 ! OV 1.01 PT 1.01 ! ! A total of 6 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.00 KP 1.03 LA 0.98 MK 2.43 ! ON 0.97 OV 1.02 PT 0.96 WZ 0.97 ! ! A total of 6 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! BR 0.93 FD 0.99 HN 0.92 KK 0.99 ! KP 1.00 LA 0.95 NL 0.98 OV 0.98 ! PT 0.99 ! ! ! Correcting IF 2. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 1.00 KK 1.05 KP 0.98 ! LA 1.05 MK 0.92 NL 1.06 OV 1.00 ! PT 1.02 ! ! A total of 30 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 KK 1.01 KP 0.98 MK 1.03 ! NY 1.05 OV 1.01 PT 1.05 ! ! Telescope amplitude corrections in sub-array 3: ! KK 1.44 NY 0.87 ON 1.01 WZ 1.10 ! ! Telescope amplitude corrections in sub-array 4: ! FD 1.02 KP 1.18 LA 1.00 SC 0.90 ! ! A total of 102 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.04 HH 0.97 HN 1.18 LA 0.98 ! NL 0.98 NY 0.97 ON 0.99 SC 1.00 ! WZ 0.92 ! ! A total of 6 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.05 FD 1.03 HN 1.10 KP 0.98 ! LA 0.97 NL 0.97 NY 1.06 ON 1.00 ! OV 1.02 PT 1.02 ! ! A total of 6 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.02 KP 1.06 LA 1.00 MK 1.98 ! ON 0.92 OV 1.01 PT 0.96 WZ 0.98 ! ! A total of 6 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! BR 0.96 FD 0.99 HN 0.87 KK 0.95 ! KP 0.99 LA 0.94 NL 0.98 OV 1.00 ! PT 0.99 ! ! ! Correcting IF 3. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.99 KK 1.02 KP 1.01 ! LA 1.06 MK 0.93 NL 1.05 OV 1.01 ! PT 1.04 ! ! A total of 30 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 KK 1.01 KP 1.01 MK 1.02 ! NY 1.08 OV 0.99 PT 1.10 ! ! Telescope amplitude corrections in sub-array 3: ! KK 1.42 NY 0.86 ON 1.02 WZ 1.20 ! ! Telescope amplitude corrections in sub-array 4: ! FD 1.02 KP 1.26 LA 1.05 SC 0.86 ! ! A total of 102 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.04 HH 0.96 HN 1.17 LA 1.01 ! NL 1.00 NY 0.98 ON 0.99 SC 1.08 ! WZ 0.93 ! ! A total of 6 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.09 FD 1.02 HN 1.08 KP 1.04 ! LA 0.97 NL 1.01 NY 1.31 ON 1.05 ! OV 1.02 PT 1.02 ! ! A total of 6 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.04 KP 1.03 LA 0.98 MK 2.55 ! ON 0.97 OV 1.00 PT 0.98 WZ 0.97 ! ! A total of 6 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! BR 0.98 FD 0.98 HN 0.94 KK 0.94 ! KP 0.98 LA 0.97 NL 1.00 OV 0.99 ! PT 1.00 ! ! ! Correcting IF 4. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 0.99 KK 1.09 KP 1.00 ! LA 1.05 MK 0.93 NL 1.05 OV 1.01 ! PT 1.05 ! ! A total of 30 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 KK 1.05 KP 1.02 MK 1.04 ! NY 1.07 OV 1.03 PT 1.04 ! ! Telescope amplitude corrections in sub-array 3: ! KK 1.53 NY 0.86 ON 1.20 WZ 1.13 ! ! Telescope amplitude corrections in sub-array 4: ! FD 1.09 KP 1.14 LA 0.99 SC 0.93 ! ! A total of 102 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 HH 1.04 HN 1.18 LA 1.00 ! NL 1.01 NY 0.95 ON 1.04 SC 1.08 ! WZ 0.92 ! ! A total of 6 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.06 FD 1.04 HN 1.01 KP 1.05 ! LA 0.98 NL 1.03 NY 1.01 ON 0.97 ! OV 1.03 PT 0.99 ! ! A total of 6 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.04 KP 1.01 LA 0.96 MK 2.46 ! ON 1.03 OV 1.03 PT 0.98 WZ 1.00 ! ! A total of 6 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! BR 0.97 FD 0.98 HN 0.90 KK 0.95 ! KP 0.97 LA 0.94 NL 0.98 OV 0.97 ! PT 1.02 ! ! ! Fit before self-cal, rms=0.130132Jy sigma=1.483595 ! Fit after self-cal, rms=0.122466Jy sigma=1.173195 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec ! Estimated beam: bmin=0.7809 mas, bmaj=1.113 mas, bpa=-12.59 degrees ! Estimated noise=0.898194 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 = 0.000324936 Jy ! Component: 100 - total flux cleaned = -7.3033e-05 Jy ! Component: 150 - total flux cleaned = -0.000424227 Jy ! Component: 200 - total flux cleaned = -0.000581134 Jy ! Total flux subtracted in 200 components = -0.000581134 Jy ! Clean residual min=-0.006239 max=0.007089 Jy/beam ! Clean residual mean=0.000005 rms=0.001557 Jy/beam ! Combined flux in latest and established models = 0.79411 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 56 components and 0.79411 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.121707Jy sigma=1.163366 ! Fit after self-cal, rms=0.121851Jy sigma=1.162854 ! Inverting map ! Your choice of large map pixels excluded 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 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=0.121851Jy sigma=1.162854 ! Fit after self-cal, rms=0.124590Jy sigma=1.013037 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec ! Estimated beam: bmin=0.7815 mas, bmaj=1.109 mas, bpa=-12.08 degrees ! Estimated noise=0.902583 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00112283 Jy ! Component: 100 - total flux cleaned = 0.00113097 Jy ! Component: 150 - total flux cleaned = 0.00100463 Jy ! Component: 200 - total flux cleaned = 0.000793118 Jy ! Total flux subtracted in 200 components = 0.000793118 Jy ! Clean residual min=-0.004840 max=0.004943 Jy/beam ! Clean residual mean=0.000005 rms=0.001036 Jy/beam ! Combined flux in latest and established models = 0.794903 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 62 components and 0.794903 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.124355Jy sigma=1.007695 ! Fit after self-cal, rms=0.124641Jy sigma=1.007340 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 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 (-2.8, 3.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00498109 Jy ! Component: 100 - total flux cleaned = 0.00537126 Jy ! Component: 150 - total flux cleaned = 0.00537234 Jy ! Component: 200 - total flux cleaned = 0.00546686 Jy ! Total flux subtracted in 200 components = 0.00546686 Jy ! Clean residual min=-0.004886 max=0.004013 Jy/beam ! Clean residual mean=0.000007 rms=0.001007 Jy/beam ! Combined flux in latest and established models = 0.80037 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 77 components and 0.80037 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.124368Jy sigma=1.001559 ! Fit after self-cal, rms=0.124350Jy sigma=1.000967 ! Inverting map ! Your choice of large map pixels excluded 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 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=0.124350Jy sigma=1.000967 ! Fit after self-cal, rms=0.123637Jy sigma=0.971024 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec ! Estimated beam: bmin=0.7812 mas, bmaj=1.109 mas, bpa=-12.04 degrees ! Estimated noise=0.903475 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00192966 Jy ! Component: 100 - total flux cleaned = 0.00287019 Jy ! Component: 150 - total flux cleaned = 0.00296088 Jy ! Component: 200 - total flux cleaned = 0.00304614 Jy ! Total flux subtracted in 200 components = 0.00304614 Jy ! Clean residual min=-0.004015 max=0.003875 Jy/beam ! Clean residual mean=0.000006 rms=0.000890 Jy/beam ! Combined flux in latest and established models = 0.803416 Jy selfcal ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 84 components and 0.803416 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.123468Jy sigma=0.967739 ! Fit after self-cal, rms=0.123491Jy sigma=0.967479 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 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 = 0.000490592 Jy ! Component: 100 - total flux cleaned = 0.000711698 Jy ! Component: 150 - total flux cleaned = 0.000780686 Jy ! Component: 200 - total flux cleaned = 0.000782116 Jy ! Total flux subtracted in 200 components = 0.000782116 Jy ! Clean residual min=-0.004053 max=0.003804 Jy/beam ! Clean residual mean=0.000006 rms=0.000883 Jy/beam ! Combined flux in latest and established models = 0.804198 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 88 components and 0.804199 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.123396Jy sigma=0.966027 ! Fit after self-cal, rms=0.123403Jy sigma=0.965930 ! Inverting map ! Your choice of large map pixels excluded 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 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=0.123403Jy sigma=0.965930 ! Fit after self-cal, rms=0.123673Jy sigma=0.964955 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec ! Estimated beam: bmin=2.483 mas, bmaj=3.179 mas, bpa=-88.5 degrees ! Estimated noise=1.16206 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00239686 Jy ! Component: 100 - total flux cleaned = 0.00234193 Jy ! Component: 150 - total flux cleaned = 0.00229822 Jy ! Component: 200 - total flux cleaned = 0.00226028 Jy ! Total flux subtracted in 200 components = 0.00226028 Jy ! Clean residual min=-0.004204 max=0.003529 Jy/beam ! Clean residual mean=0.000012 rms=0.001022 Jy/beam ! Combined flux in latest and established models = 0.806459 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 93 components and 0.806459 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.123607Jy sigma=0.964441 ! Fit after self-cal, rms=0.123626Jy sigma=0.964229 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 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 = 0.000258331 Jy ! Component: 100 - total flux cleaned = 0.000228899 Jy ! Component: 150 - total flux cleaned = 0.000176138 Jy ! Component: 200 - total flux cleaned = 0.000153428 Jy ! Total flux subtracted in 200 components = 0.000153428 Jy ! Clean residual min=-0.004217 max=0.003513 Jy/beam ! Clean residual mean=0.000012 rms=0.001019 Jy/beam ! Combined flux in latest and established models = 0.806612 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 97 components and 0.806612 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.123612Jy sigma=0.964087 ! Fit after self-cal, rms=0.123623Jy sigma=0.964028 ! Inverting map ! Your choice of large map pixels excluded 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 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 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec ! Estimated beam: bmin=0.781 mas, bmaj=1.109 mas, bpa=-12.01 degrees ! Estimated noise=0.903373 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.781 x 1.109 at -12.01 degrees (North through East) ! Clean map min=-0.0035895 max=0.64385 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=0.123623Jy sigma=0.964028 ! Fit after self-cal, rms=0.138602Jy sigma=0.854921 ! Inverting map and beam ! Your choice of large map pixels excluded 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec ! Estimated beam: bmin=0.7809 mas, bmaj=1.107 mas, bpa=-12.03 degrees ! Estimated noise=0.903557 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000205041 Jy ! Component: 100 - total flux cleaned = 0.000370623 Jy ! Component: 150 - total flux cleaned = 0.000443973 Jy ! Component: 200 - total flux cleaned = 0.000574032 Jy ! Total flux subtracted in 200 components = 0.000574032 Jy ! Clean residual min=-0.003716 max=0.003613 Jy/beam ! Clean residual mean=0.000004 rms=0.000851 Jy/beam ! Combined flux in latest and established models = 0.807186 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 99 components and 0.807186 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.138503Jy sigma=0.853172 ! Fit after self-cal, rms=0.138441Jy sigma=0.853113 ! Inverting map ! Your choice of large map pixels excluded 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000118755 Jy ! Component: 100 - total flux cleaned = 0.000176601 Jy ! Component: 150 - total flux cleaned = 0.000231158 Jy ! Component: 200 - total flux cleaned = 0.000283367 Jy ! Total flux subtracted in 200 components = 0.000283367 Jy ! Clean residual min=-0.003745 max=0.003573 Jy/beam ! Clean residual mean=0.000004 rms=0.000849 Jy/beam ! Combined flux in latest and established models = 0.80747 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 103 components and 0.80747 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.138366Jy sigma=0.852334 ! Fit after self-cal, rms=0.138320Jy sigma=0.852299 ! Inverting map ! Your choice of large map pixels excluded 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.138320Jy sigma=0.852299 ! Fit after self-cal, rms=0.138656Jy sigma=0.851621 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 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec ! Estimated beam: bmin=0.6629 mas, bmaj=0.9241 mas, bpa=-11.98 degrees ! Estimated noise=1.12789 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.515126 Jy ! Component: 100 - total flux cleaned = 0.650407 Jy ! Component: 150 - total flux cleaned = 0.704212 Jy ! Component: 200 - total flux cleaned = 0.733586 Jy ! Total flux subtracted in 200 components = 0.733586 Jy ! Clean residual min=-0.006644 max=0.015033 Jy/beam ! Clean residual mean=0.000001 rms=0.001530 Jy/beam ! Combined flux in latest and established models = 0.733586 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 21 model components to the UV plane model. ! The established model now contains 21 components and 0.733586 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec ! Estimated beam: bmin=0.7809 mas, bmaj=1.106 mas, bpa=-11.98 degrees ! Estimated noise=0.903617 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 = 0.0258074 Jy ! Component: 100 - total flux cleaned = 0.0413675 Jy ! Component: 150 - total flux cleaned = 0.0517726 Jy ! Component: 200 - total flux cleaned = 0.0591287 Jy ! Total flux subtracted in 200 components = 0.0591287 Jy ! Clean residual min=-0.004478 max=0.006022 Jy/beam ! Clean residual mean=0.000001 rms=0.000939 Jy/beam ! Combined flux in latest and established models = 0.792715 Jy ! Adding 33 model components to the UV plane model. ! The established model now contains 41 components and 0.792715 Jy ! Inverting map ! Your choice of large map pixels excluded 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec ! Added new window around map position (-2.4, 1.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00624512 Jy ! Component: 100 - total flux cleaned = 0.0104981 Jy ! Component: 150 - total flux cleaned = 0.0133787 Jy ! Component: 200 - total flux cleaned = 0.0146683 Jy ! Total flux subtracted in 200 components = 0.0146683 Jy ! Clean residual min=-0.004228 max=0.003686 Jy/beam ! Clean residual mean=0.000004 rms=0.000855 Jy/beam ! Combined flux in latest and established models = 0.807383 Jy ! Adding 33 model components to the UV plane model. ! The established model now contains 63 components and 0.807383 Jy ! Inverting map ! Your choice of large map pixels excluded 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 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 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec ! Estimated beam: bmin=2.478 mas, bmaj=3.182 mas, bpa=-88.3 degrees ! Estimated noise=1.16406 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00266379 Jy ! Component: 100 - total flux cleaned = 0.00317433 Jy ! Component: 150 - total flux cleaned = 0.00312838 Jy ! Component: 200 - total flux cleaned = 0.00313001 Jy ! Total flux subtracted in 200 components = 0.00313001 Jy ! Clean residual min=-0.003717 max=0.003557 Jy/beam ! Clean residual mean=0.000010 rms=0.000949 Jy/beam ! Combined flux in latest and established models = 0.810513 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 = -3.24732e-05 Jy ! Component: 100 - total flux cleaned = -3.19983e-05 Jy ! Component: 150 - total flux cleaned = -5.72378e-05 Jy ! Component: 200 - total flux cleaned = -5.55782e-05 Jy ! Total flux subtracted in 200 components = -5.55782e-05 Jy ! Clean residual min=-0.003697 max=0.003557 Jy/beam ! Clean residual mean=0.000009 rms=0.000945 Jy/beam ! Combined flux in latest and established models = 0.810457 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 85 components and 0.810457 Jy ! Inverting map ! Your choice of large map pixels excluded 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec ! Estimated beam: bmin=0.7809 mas, bmaj=1.106 mas, bpa=-11.98 degrees ! Estimated noise=0.903617 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000337636 Jy ! Component: 100 - total flux cleaned = 0.000338104 Jy ! Component: 150 - total flux cleaned = 0.000335364 Jy ! Component: 200 - total flux cleaned = 0.000273912 Jy ! Total flux subtracted in 200 components = 0.000273912 Jy ! Clean residual min=-0.004057 max=0.003534 Jy/beam ! Clean residual mean=0.000004 rms=0.000841 Jy/beam ! Combined flux in latest and established models = 0.810731 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 92 components and 0.810731 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.138706Jy sigma=0.854653 ! Fit after self-cal, rms=0.137934Jy sigma=0.851969 wmodel J1125+2610_X_map.mod ! Writing 92 model components to file: J1125+2610_X_map.mod wobs J1125+2610_X_uvs.fits ! Writing UV FITS file: J1125+2610_X_uvs.fits wwins J1125+2610_X_map.win ! wwins: Wrote 5 windows to J1125+2610_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 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00148242 Jy ! Component: 100 - total flux cleaned = -0.00187944 Jy ! Component: 150 - total flux cleaned = -0.00200358 Jy ! Component: 200 - total flux cleaned = -0.00200265 Jy ! Component: 250 - total flux cleaned = -0.00176547 Jy ! Component: 300 - total flux cleaned = -0.00170776 Jy ! Component: 350 - total flux cleaned = -0.00159266 Jy ! Component: 400 - total flux cleaned = -0.00147897 Jy ! Component: 450 - total flux cleaned = -0.00131055 Jy ! Component: 500 - total flux cleaned = -0.00114373 Jy ! Component: 550 - total flux cleaned = -0.0010887 Jy ! Component: 600 - total flux cleaned = -0.00103402 Jy ! Component: 650 - total flux cleaned = -0.00108697 Jy ! Component: 700 - total flux cleaned = -0.00119337 Jy ! Component: 750 - total flux cleaned = -0.00119425 Jy ! Component: 800 - total flux cleaned = -0.00124648 Jy ! Component: 850 - total flux cleaned = -0.00155764 Jy ! Component: 900 - total flux cleaned = -0.00145437 Jy ! Component: 950 - total flux cleaned = -0.00165819 Jy ! Component: 1000 - total flux cleaned = -0.00160703 Jy ! Component: 1050 - total flux cleaned = -0.00165751 Jy ! Component: 1100 - total flux cleaned = -0.00175793 Jy ! Component: 1150 - total flux cleaned = -0.00185706 Jy ! Component: 1200 - total flux cleaned = -0.00156023 Jy ! Component: 1250 - total flux cleaned = -0.00156048 Jy ! Component: 1300 - total flux cleaned = -0.00160937 Jy ! Component: 1350 - total flux cleaned = -0.00151205 Jy ! Component: 1400 - total flux cleaned = -0.00141549 Jy ! Component: 1450 - total flux cleaned = -0.00146369 Jy ! Component: 1500 - total flux cleaned = -0.00160703 Jy ! Component: 1550 - total flux cleaned = -0.00127374 Jy ! Component: 1600 - total flux cleaned = -0.00122638 Jy ! Component: 1650 - total flux cleaned = -0.00122616 Jy ! Component: 1700 - total flux cleaned = -0.00131983 Jy ! Component: 1750 - total flux cleaned = -0.00127335 Jy ! Component: 1800 - total flux cleaned = -0.00113419 Jy ! Component: 1850 - total flux cleaned = -0.00122657 Jy ! Component: 1900 - total flux cleaned = -0.00131801 Jy ! Component: 1950 - total flux cleaned = -0.00127259 Jy ! Component: 2000 - total flux cleaned = -0.00104547 Jy ! Component: 2050 - total flux cleaned = -0.00118089 Jy ! Component: 2100 - total flux cleaned = -0.00113571 Jy ! Component: 2150 - total flux cleaned = -0.000911745 Jy ! Component: 2200 - total flux cleaned = -0.00104569 Jy ! Component: 2250 - total flux cleaned = -0.000956706 Jy ! Component: 2300 - total flux cleaned = -0.00108955 Jy ! Component: 2350 - total flux cleaned = -0.0010901 Jy ! Component: 2400 - total flux cleaned = -0.00100257 Jy ! Component: 2450 - total flux cleaned = -0.00104625 Jy ! Component: 2500 - total flux cleaned = -0.00126305 Jy ! Component: 2550 - total flux cleaned = -0.00100371 Jy ! Component: 2600 - total flux cleaned = -0.00100367 Jy ! Component: 2650 - total flux cleaned = -0.00104664 Jy ! Component: 2700 - total flux cleaned = -0.000833437 Jy ! Component: 2750 - total flux cleaned = -0.0010457 Jy ! Component: 2800 - total flux cleaned = -0.000961073 Jy ! Component: 2850 - total flux cleaned = -0.00108745 Jy ! Component: 2900 - total flux cleaned = -0.000919536 Jy ! Component: 2950 - total flux cleaned = -0.00112875 Jy ! Component: 3000 - total flux cleaned = -0.00104533 Jy ! Component: 3050 - total flux cleaned = -0.00108681 Jy ! Component: 3100 - total flux cleaned = -0.000921579 Jy ! Component: 3150 - total flux cleaned = -0.00104524 Jy ! Component: 3200 - total flux cleaned = -0.000921869 Jy ! Component: 3250 - total flux cleaned = -0.000962698 Jy ! Component: 3300 - total flux cleaned = -0.000922045 Jy ! Component: 3350 - total flux cleaned = -0.000922049 Jy ! Component: 3400 - total flux cleaned = -0.000962546 Jy ! Component: 3450 - total flux cleaned = -0.0010028 Jy ! Component: 3500 - total flux cleaned = -0.000962617 Jy ! Component: 3550 - total flux cleaned = -0.000842455 Jy ! Component: 3600 - total flux cleaned = -0.000842501 Jy ! Component: 3650 - total flux cleaned = -0.000961702 Jy ! Component: 3700 - total flux cleaned = -0.000763551 Jy ! Component: 3750 - total flux cleaned = -0.000645005 Jy ! Component: 3800 - total flux cleaned = -0.000684673 Jy ! Component: 3850 - total flux cleaned = -0.000645675 Jy ! Component: 3900 - total flux cleaned = -0.00056761 Jy ! Component: 3950 - total flux cleaned = -0.000411731 Jy ! Component: 4000 - total flux cleaned = -0.000450576 Jy ! Component: 4050 - total flux cleaned = -0.000528112 Jy ! Total flux subtracted in 4096 components = -0.000528268 Jy ! Clean residual min=-0.001926 max=0.002310 Jy/beam ! Clean residual mean=0.000001 rms=0.000636 Jy/beam ! Combined flux in latest and established models = 0.810203 Jy keep ! Adding 357 model components to the UV plane model. ! The established model now contains 449 components and 0.810203 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv120_uvs/J1125+2610_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7809 x 1.106 at -11.98 degrees (North through East) ! Clean map min=-0.0036939 max=0.65001 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv120_uvs/J1125+2610_X_map.fits wmodel /scr/pima/rv120_uvs/J1125+2610_X_map.mod ! Writing 449 model components to file: /scr/pima/rv120_uvs/J1125+2610_X_map.mod wobs /scr/pima/rv120_uvs/J1125+2610_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv120_uvs/J1125+2610_X_uvs.fits wwins /scr/pima/rv120_uvs/J1125+2610_X_map.win ! wwins: Wrote 6 windows to /scr/pima/rv120_uvs/J1125+2610_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.650012 invert ! Inverting map ! Your choice of large map pixels excluded 4.31% of the data. ! The x-axis pixel size should ideally be below 0.1706 milli-arcsec ! The y-axis pixel size should ideally be below 0.1702 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000635347 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.293232 0.293232 0.586464 1.17293 2.34586 4.69171 9.38342 18.7668 37.5337 75.0674 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0019 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.65 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 1023.08 quit ! Quitting program ! Log file /scr/pima/rv120_uvs/J1125+2610_X_dfm.log closed on Fri Dec 22 22:41:47 2017