! Started logfile: /scr/pima/rv123_uvs/J1125+2610_X_dfm.log on Sun Dec 23 00:41:57 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/rv123_uvs/J1125+2610_X_uva.fits ! Reading UV FITS file: /scr/pima/rv123_uvs/J1125+2610_X_uva.fits ! AN table 1: 18 integrations on 45 of 45 possible baselines. ! AN table 2: 46 integrations on 45 of 45 possible baselines. ! AN table 3: 3 integrations on 6 of 6 possible baselines. ! AN table 4: 14 integrations on 6 of 6 possible baselines. ! AN table 5: 29 integrations on 15 of 15 possible baselines. ! AN table 6: 77 integrations on 66 of 66 possible baselines. ! Apparent sampling: 0.383457 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 89 lines of history. ! ! Reading 13036 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 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 350 telescope corrections were flagged in sub-array 2. ! A total of 4 telescope corrections were flagged in sub-array 3. ! A total of 48 telescope corrections were flagged in sub-array 4. ! A total of 60 telescope corrections were flagged in sub-array 5. ! A total of 510 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 350 telescope corrections were flagged in sub-array 2. ! A total of 4 telescope corrections were flagged in sub-array 3. ! A total of 48 telescope corrections were flagged in sub-array 4. ! A total of 60 telescope corrections were flagged in sub-array 5. ! A total of 510 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 18 telescope corrections were flagged in sub-array 1. ! A total of 350 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 3. ! A total of 48 telescope corrections were flagged in sub-array 4. ! A total of 74 telescope corrections were flagged in sub-array 5. ! A total of 576 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 18 telescope corrections were flagged in sub-array 1. ! A total of 350 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 3. ! A total of 48 telescope corrections were flagged in sub-array 4. ! A total of 74 telescope corrections were flagged in sub-array 5. ! A total of 576 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.221420Jy sigma=14.995305 ! Fit after self-cal, rms=0.406072Jy sigma=5.006170 ! 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 3.93% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec ! Estimated beam: bmin=0.5722 mas, bmaj=0.8915 mas, bpa=4.745 degrees ! Estimated noise=0.935541 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 = 0.527789 Jy ! Component: 100 - total flux cleaned = 0.679898 Jy ! Total flux subtracted in 100 components = 0.679898 Jy ! Clean residual min=-0.028040 max=0.068539 Jy/beam ! Clean residual mean=-0.000071 rms=0.004548 Jy/beam ! Combined flux in latest and established models = 0.679898 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.679898 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.211505Jy sigma=2.314325 ! Fit after self-cal, rms=0.211415Jy sigma=2.313493 ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0758036 Jy ! Component: 100 - total flux cleaned = 0.11507 Jy ! Total flux subtracted in 100 components = 0.11507 Jy ! Clean residual min=-0.025388 max=0.029819 Jy/beam ! Clean residual mean=-0.000109 rms=0.003617 Jy/beam ! Combined flux in latest and established models = 0.794967 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 8 components and 0.794967 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.187153Jy sigma=1.940577 ! Fit after self-cal, rms=0.187155Jy sigma=1.940152 ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec ! Added new window around map position (1.6, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0231605 Jy ! Component: 100 - total flux cleaned = 0.0239168 Jy ! Total flux subtracted in 100 components = 0.0239168 Jy ! Clean residual min=-0.019738 max=0.026836 Jy/beam ! Clean residual mean=-0.000116 rms=0.003455 Jy/beam ! Combined flux in latest and established models = 0.818884 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 13 components and 0.818884 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.184403Jy sigma=1.902114 ! Fit after self-cal, rms=0.184225Jy sigma=1.900071 ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec ! Added new window around map position (3.2, -5.8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.017884 Jy ! Component: 100 - total flux cleaned = 0.0190238 Jy ! Total flux subtracted in 100 components = 0.0190238 Jy ! Clean residual min=-0.018682 max=0.023433 Jy/beam ! Clean residual mean=-0.000122 rms=0.003348 Jy/beam ! Combined flux in latest and established models = 0.837908 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 17 components and 0.837908 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.182475Jy sigma=1.883293 ! Fit after self-cal, rms=0.182317Jy sigma=1.881027 ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec ! Added new window around map position (-2.8, -4.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0187452 Jy ! Component: 100 - total flux cleaned = 0.020763 Jy ! Total flux subtracted in 100 components = 0.020763 Jy ! Clean residual min=-0.017828 max=0.021056 Jy/beam ! Clean residual mean=-0.000129 rms=0.003250 Jy/beam ! Combined flux in latest and established models = 0.858671 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 23 components and 0.858671 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.180989Jy sigma=1.859342 ! Fit after self-cal, rms=0.180927Jy sigma=1.856680 ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec ! Added new window around map position (-0.2, 6.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0133875 Jy ! Component: 100 - total flux cleaned = 0.0156587 Jy ! Total flux subtracted in 100 components = 0.0156587 Jy ! Clean residual min=-0.016624 max=0.019694 Jy/beam ! Clean residual mean=-0.000135 rms=0.003164 Jy/beam ! Combined flux in latest and established models = 0.87433 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 28 components and 0.87433 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.179582Jy sigma=1.830146 ! Fit after self-cal, rms=0.179558Jy sigma=1.828779 ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec ! Added new window around map position (-1.6, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00579192 Jy ! Component: 100 - total flux cleaned = 0.00530046 Jy ! Total flux subtracted in 100 components = 0.00530046 Jy ! Clean residual min=-0.015604 max=0.017230 Jy/beam ! Clean residual mean=-0.000136 rms=0.003072 Jy/beam ! Combined flux in latest and established models = 0.87963 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 32 components and 0.87963 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.177872Jy sigma=1.805444 ! Fit after self-cal, rms=0.177822Jy sigma=1.804301 ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 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 3.93% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec ! Estimated beam: bmin=0.6136 mas, bmaj=1.043 mas, bpa=6.535 degrees ! Estimated noise=0.587609 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 = -0.0228721 Jy ! Component: 100 - total flux cleaned = -0.0339647 Jy ! Component: 150 - total flux cleaned = -0.0421971 Jy ! Component: 200 - total flux cleaned = -0.0487106 Jy ! Total flux subtracted in 200 components = -0.0487106 Jy ! Clean residual min=-0.021521 max=0.018325 Jy/beam ! Clean residual mean=-0.006322 rms=0.004213 Jy/beam ! Combined flux in latest and established models = 0.830919 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 45 components and 0.830919 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.173528Jy sigma=1.761609 ! Fit after self-cal, rms=0.173418Jy sigma=1.759309 ! Inverting map ! Your choice of large map pixels excluded 3.93% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec print "============== Finished natural weighting clean ==============" ! ============== Finished natural weighting clean ============== ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6136 x 1.043 at 6.535 degrees (North through East) ! Clean map min=-0.020437 max=0.67227 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 0.96 HN 1.02 KP 1.03 ! LA 0.96 NL 1.00 NY 0.75 PT 0.82 ! SC 0.96 WN 1.33 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 0.84 HN 1.02 KP 0.99 ! LA 0.93 MC 1.06 MK 0.96 NL 1.05 ! OV 0.93 SC 0.89 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 MK 1.04 NY 0.74 OV 0.96 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.06 MK 1.06 OV 1.02 YG 1.10 ! ! A total of 18 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! HH 0.82 NY 0.71 ON 0.90 WN 1.60 ! WZ 1.01 YG 1.17 ! ! A total of 24 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.05 FD 1.17 HH 0.89 HN 1.04 ! LA 0.99 NL 0.98 NY 0.82 ON 0.87 ! PT 0.83 SC 0.95 WN 1.51 WZ 0.94 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 0.94 HN 1.02 KP 1.02 ! LA 0.96 NL 0.98 NY 0.92 PT 0.83 ! SC 0.96 WN 1.35 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 0.83 HN 1.01 KP 1.00 ! LA 0.95 MC 1.11 MK 0.97 NL 1.04 ! OV 0.93 SC 0.88 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 MK 1.03 NY 0.86 OV 1.00 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 MK 1.05 OV 1.01 YG 1.05 ! ! A total of 18 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! HH 0.79 NY 0.89 ON 0.88 WN 1.61 ! WZ 0.98 YG 1.12 ! ! A total of 24 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.08 FD 1.19 HH 0.86 HN 1.05 ! LA 1.00 NL 0.99 NY 0.98 ON 0.85 ! PT 0.83 SC 0.96 WN 1.48 WZ 0.90 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.05 FD 0.96 HN 1.00 KP 1.06 ! LA 0.97 NL 1.01 NY 1.00* PT 0.84 ! SC 0.98 WN 1.22 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 FD 0.82 HN 1.06 KP 1.02 ! LA 0.95 MC 1.67 MK 1.00 NL 1.04 ! OV 0.95 SC 0.87 ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* MK 0.00* NY 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 MK 1.10 OV 1.04 YG 1.20 ! ! A total of 24 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! HH 0.90 NY 1.00* ON 1.20 WN 1.40 ! WZ 1.09 YG 1.18 ! ! A total of 36 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.06 FD 1.27 HH 0.97 HN 1.07 ! LA 1.02 NL 1.00 NY 1.00* ON 1.17 ! PT 0.85 SC 0.97 WN 1.44 WZ 0.96 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.04 FD 1.00 HN 1.02 KP 1.04 ! LA 0.98 NL 1.02 NY 1.00* PT 0.85 ! SC 1.00 WN 1.18 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 FD 0.83 HN 1.05 KP 1.00 ! LA 0.94 MC 1.57 MK 1.01 NL 1.05 ! OV 0.96 SC 0.89 ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* MK 0.00* NY 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.06 MK 1.07 OV 0.98 YG 1.03 ! ! A total of 24 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! HH 1.05 NY 1.00* ON 1.17 WN 1.37 ! WZ 1.12 YG 1.21 ! ! A total of 36 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.05 FD 1.31 HH 1.14 HN 1.06 ! LA 1.02 NL 1.00 NY 1.00* ON 1.15 ! PT 0.86 SC 0.99 WN 1.37 WZ 0.99 ! ! ! Fit before self-cal, rms=0.173418Jy sigma=1.759309 ! Fit after self-cal, rms=0.122235Jy sigma=1.108716 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec ! Estimated beam: bmin=0.6223 mas, bmaj=1.03 mas, bpa=6.681 degrees ! Estimated noise=0.602419 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 = -0.00895377 Jy ! Component: 100 - total flux cleaned = -0.0115256 Jy ! Component: 150 - total flux cleaned = -0.0130998 Jy ! Component: 200 - total flux cleaned = -0.0144738 Jy ! Total flux subtracted in 200 components = -0.0144738 Jy ! Clean residual min=-0.008535 max=0.008306 Jy/beam ! Clean residual mean=-0.000808 rms=0.001499 Jy/beam ! Combined flux in latest and established models = 0.816446 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 57 components and 0.816446 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.120073Jy sigma=1.075426 ! Fit after self-cal, rms=0.120114Jy sigma=1.073998 ! Inverting map ! Your choice of large map pixels excluded 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 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=0.120114Jy sigma=1.073998 ! Fit after self-cal, rms=0.118709Jy sigma=1.057856 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec ! Estimated beam: bmin=0.6237 mas, bmaj=1.029 mas, bpa=6.675 degrees ! Estimated noise=0.601081 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00333175 Jy ! Component: 100 - total flux cleaned = -0.004909 Jy ! Component: 150 - total flux cleaned = -0.00579946 Jy ! Component: 200 - total flux cleaned = -0.0061985 Jy ! Total flux subtracted in 200 components = -0.0061985 Jy ! Clean residual min=-0.007424 max=0.007662 Jy/beam ! Clean residual mean=-0.000516 rms=0.001327 Jy/beam ! Combined flux in latest and established models = 0.810247 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 62 components and 0.810247 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.117746Jy sigma=1.042029 ! Fit after self-cal, rms=0.117659Jy sigma=1.041521 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 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 (-2.2, 2.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0051369 Jy ! Component: 100 - total flux cleaned = 0.00536556 Jy ! Component: 150 - total flux cleaned = 0.00554071 Jy ! Component: 200 - total flux cleaned = 0.00554097 Jy ! Total flux subtracted in 200 components = 0.00554097 Jy ! Clean residual min=-0.006775 max=0.005746 Jy/beam ! Clean residual mean=-0.000585 rms=0.001187 Jy/beam ! Combined flux in latest and established models = 0.815788 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 78 components and 0.815788 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.117017Jy sigma=1.031643 ! Fit after self-cal, rms=0.116944Jy sigma=1.031102 ! Inverting map ! Your choice of large map pixels excluded 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 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=0.116944Jy sigma=1.031102 ! Fit after self-cal, rms=0.114826Jy sigma=1.002867 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec ! Estimated beam: bmin=0.6251 mas, bmaj=1.027 mas, bpa=6.746 degrees ! Estimated noise=0.600655 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00061044 Jy ! Component: 100 - total flux cleaned = -0.00119272 Jy ! Component: 150 - total flux cleaned = -0.00119588 Jy ! Component: 200 - total flux cleaned = -0.000894114 Jy ! Total flux subtracted in 200 components = -0.000894114 Jy ! Clean residual min=-0.005812 max=0.005459 Jy/beam ! Clean residual mean=-0.000421 rms=0.000993 Jy/beam ! Combined flux in latest and established models = 0.814894 Jy selfcal ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 82 components and 0.814894 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.114316Jy sigma=0.994775 ! Fit after self-cal, rms=0.114290Jy sigma=0.994565 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 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 = 0.000128181 Jy ! Component: 100 - total flux cleaned = 0.000512259 Jy ! Component: 150 - total flux cleaned = 0.000750462 Jy ! Component: 200 - total flux cleaned = 0.000860654 Jy ! Total flux subtracted in 200 components = 0.000860654 Jy ! Clean residual min=-0.005304 max=0.005202 Jy/beam ! Clean residual mean=-0.000432 rms=0.000955 Jy/beam ! Combined flux in latest and established models = 0.815754 Jy ! Performing phase self-cal ! Adding 31 model components to the UV plane model. ! The established model now contains 85 components and 0.815754 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.114048Jy sigma=0.990789 ! Fit after self-cal, rms=0.114034Jy sigma=0.990723 ! Inverting map ! Your choice of large map pixels excluded 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 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=0.114034Jy sigma=0.990723 ! Fit after self-cal, rms=0.113613Jy sigma=0.984309 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec ! Estimated beam: bmin=2.467 mas, bmaj=2.831 mas, bpa=-80.92 degrees ! Estimated noise=0.87403 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000583514 Jy ! Component: 100 - total flux cleaned = -0.000141365 Jy ! Component: 150 - total flux cleaned = -0.000584382 Jy ! Component: 200 - total flux cleaned = -0.000582852 Jy ! Total flux subtracted in 200 components = -0.000582852 Jy ! Clean residual min=-0.005447 max=0.005252 Jy/beam ! Clean residual mean=-0.000977 rms=0.001420 Jy/beam ! Combined flux in latest and established models = 0.815172 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 98 components and 0.815171 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.113561Jy sigma=0.982863 ! Fit after self-cal, rms=0.113539Jy sigma=0.982558 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 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 = 0.000192288 Jy ! Component: 100 - total flux cleaned = 0.000330131 Jy ! Component: 150 - total flux cleaned = 0.000579993 Jy ! Component: 200 - total flux cleaned = 0.000634992 Jy ! Total flux subtracted in 200 components = 0.000634992 Jy ! Clean residual min=-0.005472 max=0.005141 Jy/beam ! Clean residual mean=-0.000999 rms=0.001371 Jy/beam ! Combined flux in latest and established models = 0.815806 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 104 components and 0.815806 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.113543Jy sigma=0.982507 ! Fit after self-cal, rms=0.113538Jy sigma=0.982442 ! Inverting map ! Your choice of large map pixels excluded 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 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 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec ! Estimated beam: bmin=0.6264 mas, bmaj=1.025 mas, bpa=6.792 degrees ! Estimated noise=0.600445 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6264 x 1.025 at 6.792 degrees (North through East) ! Clean map min=-0.0060448 max=0.67229 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=0.113538Jy sigma=0.982442 ! Fit after self-cal, rms=0.107137Jy sigma=0.871928 ! Inverting map and beam ! Your choice of large map pixels excluded 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec ! Estimated beam: bmin=0.6264 mas, bmaj=1.025 mas, bpa=6.779 degrees ! Estimated noise=0.600103 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00236857 Jy ! Component: 100 - total flux cleaned = -0.00265571 Jy ! Component: 150 - total flux cleaned = -0.00278283 Jy ! Component: 200 - total flux cleaned = -0.00267202 Jy ! Total flux subtracted in 200 components = -0.00267202 Jy ! Clean residual min=-0.003577 max=0.004463 Jy/beam ! Clean residual mean=-0.000310 rms=0.000815 Jy/beam ! Combined flux in latest and established models = 0.813134 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 109 components and 0.813134 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.106822Jy sigma=0.866730 ! Fit after self-cal, rms=0.106816Jy sigma=0.866633 ! Inverting map ! Your choice of large map pixels excluded 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec ! Added new window around map position (2.6, 3.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00287113 Jy ! Component: 100 - total flux cleaned = 0.00265158 Jy ! Component: 150 - total flux cleaned = 0.00274564 Jy ! Component: 200 - total flux cleaned = 0.00283352 Jy ! Total flux subtracted in 200 components = 0.00283352 Jy ! Clean residual min=-0.003536 max=0.003351 Jy/beam ! Clean residual mean=-0.000345 rms=0.000771 Jy/beam ! Combined flux in latest and established models = 0.815968 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 113 components and 0.815968 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.106547Jy sigma=0.863289 ! Fit after self-cal, rms=0.106533Jy sigma=0.863076 ! Inverting map ! Your choice of large map pixels excluded 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.106533Jy sigma=0.863076 ! Fit after self-cal, rms=0.106446Jy sigma=0.861821 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 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec ! Estimated beam: bmin=0.5819 mas, bmaj=0.8905 mas, bpa=6.028 degrees ! Estimated noise=0.936052 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.522101 Jy ! Component: 100 - total flux cleaned = 0.66063 Jy ! Component: 150 - total flux cleaned = 0.726997 Jy ! Component: 200 - total flux cleaned = 0.762246 Jy ! Total flux subtracted in 200 components = 0.762246 Jy ! Clean residual min=-0.014406 max=0.016959 Jy/beam ! Clean residual mean=0.000002 rms=0.001493 Jy/beam ! Combined flux in latest and established models = 0.762246 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 9 model components to the UV plane model. ! The established model now contains 9 components and 0.762246 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec ! Estimated beam: bmin=0.6274 mas, bmaj=1.024 mas, bpa=6.821 degrees ! Estimated noise=0.600267 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 = 0.0269474 Jy ! Component: 100 - total flux cleaned = 0.0365064 Jy ! Component: 150 - total flux cleaned = 0.0413364 Jy ! Component: 200 - total flux cleaned = 0.0449258 Jy ! Total flux subtracted in 200 components = 0.0449258 Jy ! Clean residual min=-0.010129 max=0.008013 Jy/beam ! Clean residual mean=-0.000164 rms=0.001182 Jy/beam ! Combined flux in latest and established models = 0.807172 Jy ! Adding 22 model components to the UV plane model. ! The established model now contains 25 components and 0.807172 Jy ! Inverting map ! Your choice of large map pixels excluded 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 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 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec ! Estimated beam: bmin=2.464 mas, bmaj=2.829 mas, bpa=-81.16 degrees ! Estimated noise=0.873224 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00861062 Jy ! Component: 100 - total flux cleaned = 0.0104942 Jy ! Component: 150 - total flux cleaned = 0.0108955 Jy ! Component: 200 - total flux cleaned = 0.0108992 Jy ! Total flux subtracted in 200 components = 0.0108992 Jy ! Clean residual min=-0.005526 max=0.004326 Jy/beam ! Clean residual mean=-0.000874 rms=0.001324 Jy/beam ! Combined flux in latest and established models = 0.818071 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 = 0.000159023 Jy ! Component: 100 - total flux cleaned = 0.0002917 Jy ! Component: 150 - total flux cleaned = 0.000292424 Jy ! Component: 200 - total flux cleaned = 0.00050708 Jy ! Total flux subtracted in 200 components = 0.00050708 Jy ! Clean residual min=-0.004998 max=0.003479 Jy/beam ! Clean residual mean=-0.000893 rms=0.001166 Jy/beam ! Combined flux in latest and established models = 0.818578 Jy ! Adding 39 model components to the UV plane model. ! The established model now contains 61 components and 0.818579 Jy ! Inverting map ! Your choice of large map pixels excluded 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec ! Estimated beam: bmin=0.6274 mas, bmaj=1.024 mas, bpa=6.821 degrees ! Estimated noise=0.600267 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00253282 Jy ! Component: 100 - total flux cleaned = 0.00252728 Jy ! Component: 150 - total flux cleaned = 0.00293251 Jy ! Component: 200 - total flux cleaned = 0.00329704 Jy ! Total flux subtracted in 200 components = 0.00329704 Jy ! Clean residual min=-0.006347 max=0.005617 Jy/beam ! Clean residual mean=-0.000344 rms=0.000826 Jy/beam ! Combined flux in latest and established models = 0.821876 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 75 components and 0.821875 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.107933Jy sigma=0.876158 ! Fit after self-cal, rms=0.107716Jy sigma=0.873077 wmodel J1125+2610_X_map.mod ! Writing 75 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 8 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 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00058234 Jy ! Component: 100 - total flux cleaned = -0.000746416 Jy ! Component: 150 - total flux cleaned = -0.000519058 Jy ! Component: 200 - total flux cleaned = -0.000517105 Jy ! Component: 250 - total flux cleaned = -0.000517193 Jy ! Component: 300 - total flux cleaned = -0.000838198 Jy ! Component: 350 - total flux cleaned = -0.00108674 Jy ! Component: 400 - total flux cleaned = -0.00138969 Jy ! Component: 450 - total flux cleaned = -0.00180391 Jy ! Component: 500 - total flux cleaned = -0.00226669 Jy ! Component: 550 - total flux cleaned = -0.00254997 Jy ! Component: 600 - total flux cleaned = -0.00288532 Jy ! Component: 650 - total flux cleaned = -0.00343352 Jy ! Component: 700 - total flux cleaned = -0.00381104 Jy ! Component: 750 - total flux cleaned = -0.00428942 Jy ! Component: 800 - total flux cleaned = -0.00470768 Jy ! Component: 850 - total flux cleaned = -0.00522407 Jy ! Component: 900 - total flux cleaned = -0.00563143 Jy ! Component: 950 - total flux cleaned = -0.00613341 Jy ! Component: 1000 - total flux cleaned = -0.00657928 Jy ! Component: 1050 - total flux cleaned = -0.00701917 Jy ! Component: 1100 - total flux cleaned = -0.00745399 Jy ! Component: 1150 - total flux cleaned = -0.00788369 Jy ! Component: 1200 - total flux cleaned = -0.00830804 Jy ! Component: 1250 - total flux cleaned = -0.00868117 Jy ! Component: 1300 - total flux cleaned = -0.00909569 Jy ! Component: 1350 - total flux cleaned = -0.00941487 Jy ! Component: 1400 - total flux cleaned = -0.00973057 Jy ! Component: 1450 - total flux cleaned = -0.00999886 Jy ! Component: 1500 - total flux cleaned = -0.0103528 Jy ! Component: 1550 - total flux cleaned = -0.0106158 Jy ! Component: 1600 - total flux cleaned = -0.0109632 Jy ! Component: 1650 - total flux cleaned = -0.0112215 Jy ! Component: 1700 - total flux cleaned = -0.0114771 Jy ! Component: 1750 - total flux cleaned = -0.0117307 Jy ! Component: 1800 - total flux cleaned = -0.0119406 Jy ! Component: 1850 - total flux cleaned = -0.0122317 Jy ! Component: 1900 - total flux cleaned = -0.0124791 Jy ! Component: 1950 - total flux cleaned = -0.0128061 Jy ! Component: 2000 - total flux cleaned = -0.0130086 Jy ! Component: 2050 - total flux cleaned = -0.0132097 Jy ! Component: 2100 - total flux cleaned = -0.0134889 Jy ! Component: 2150 - total flux cleaned = -0.0136869 Jy ! Component: 2200 - total flux cleaned = -0.0139227 Jy ! Component: 2250 - total flux cleaned = -0.0140789 Jy ! Component: 2300 - total flux cleaned = -0.0143111 Jy ! Component: 2350 - total flux cleaned = -0.0145032 Jy ! Component: 2400 - total flux cleaned = -0.0146556 Jy ! Component: 2450 - total flux cleaned = -0.0148453 Jy ! Component: 2500 - total flux cleaned = -0.0149582 Jy ! Component: 2550 - total flux cleaned = -0.0151453 Jy ! Component: 2600 - total flux cleaned = -0.0152568 Jy ! Component: 2650 - total flux cleaned = -0.0154045 Jy ! Component: 2700 - total flux cleaned = -0.0155878 Jy ! Component: 2750 - total flux cleaned = -0.0156972 Jy ! Component: 2800 - total flux cleaned = -0.0158059 Jy ! Component: 2850 - total flux cleaned = -0.0159859 Jy ! Component: 2900 - total flux cleaned = -0.0160216 Jy ! Component: 2950 - total flux cleaned = -0.0161283 Jy ! Component: 3000 - total flux cleaned = -0.0161638 Jy ! Component: 3050 - total flux cleaned = -0.0163401 Jy ! Component: 3100 - total flux cleaned = -0.0164102 Jy ! Component: 3150 - total flux cleaned = -0.016445 Jy ! Component: 3200 - total flux cleaned = -0.0165838 Jy ! Component: 3250 - total flux cleaned = -0.0166529 Jy ! Component: 3300 - total flux cleaned = -0.0167217 Jy ! Component: 3350 - total flux cleaned = -0.0168242 Jy ! Component: 3400 - total flux cleaned = -0.0169262 Jy ! Component: 3450 - total flux cleaned = -0.0169938 Jy ! Component: 3500 - total flux cleaned = -0.0170946 Jy ! Component: 3550 - total flux cleaned = -0.0171616 Jy ! Component: 3600 - total flux cleaned = -0.0171949 Jy ! Component: 3650 - total flux cleaned = -0.0172946 Jy ! Component: 3700 - total flux cleaned = -0.0173604 Jy ! Component: 3750 - total flux cleaned = -0.0174262 Jy ! Component: 3800 - total flux cleaned = -0.017524 Jy ! Component: 3850 - total flux cleaned = -0.0175564 Jy ! Component: 3900 - total flux cleaned = -0.0176213 Jy ! Component: 3950 - total flux cleaned = -0.0176537 Jy ! Component: 4000 - total flux cleaned = -0.0177179 Jy ! Component: 4050 - total flux cleaned = -0.0177819 Jy ! Total flux subtracted in 4096 components = -0.0178774 Jy ! Clean residual min=-0.002248 max=0.001649 Jy/beam ! Clean residual mean=-0.000074 rms=0.000501 Jy/beam ! Combined flux in latest and established models = 0.803998 Jy keep ! Adding 307 model components to the UV plane model. ! The established model now contains 379 components and 0.803998 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv123_uvs/J1125+2610_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6274 x 1.024 at 6.821 degrees (North through East) ! Clean map min=-0.00525 max=0.66908 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv123_uvs/J1125+2610_X_map.fits wmodel /scr/pima/rv123_uvs/J1125+2610_X_map.mod ! Writing 379 model components to file: /scr/pima/rv123_uvs/J1125+2610_X_map.mod wobs /scr/pima/rv123_uvs/J1125+2610_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv123_uvs/J1125+2610_X_uvs.fits wwins /scr/pima/rv123_uvs/J1125+2610_X_map.win ! wwins: Wrote 9 windows to /scr/pima/rv123_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 0.669079 invert ! Inverting map ! Your choice of large map pixels excluded 3.74% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1772 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000500621 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.224467 0.224467 0.448934 0.897868 1.79574 3.59147 7.18295 14.3659 28.7318 57.4636 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0015 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.669 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 1336.5 quit ! Quitting program ! Log file /scr/pima/rv123_uvs/J1125+2610_X_dfm.log closed on Sun Dec 23 00:42:02 2018