! Started logfile: J0136+4751_X_2000_03_13_pus_uvs.log on Mon Apr 1 13:22:11 2013 obs J0136+4751_X_2000_03_13_pus_uva.fits ! Reading UV FITS file: J0136+4751_X_2000_03_13_pus_uva.fits ! AN table 1: 198 integrations on 190 of 190 possible baselines. ! AN table 2: 69 integrations on 190 of 190 possible baselines. ! AN table 3: 394 integrations on 190 of 190 possible baselines. ! AN table 4: 444 integrations on 190 of 190 possible baselines. ! Apparent sampling: 0.148869 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0136+4751 ! ! 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 8.40997e+09 8e+06 1 8e+06 ! 02 2 8.47997e+09 8e+06 1 8e+06 ! 03 3 8.79497e+09 8e+06 1 8e+06 ! 04 4 8.89997e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 2382 lines of history. ! ! Reading 125020 visibilities. select I ! Polarization I is unavailable. ! 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 = 512 print "field_cell =",field_cell ! field_cell = 0.2 print "taper_size =",taper_size ! taper_size = 70 ![@muppet J0136+4751_X_2000_03_13_pus] 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 = 512x512 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 2549 telescope corrections were flagged in sub-array 1. ! A total of 655 telescope corrections were flagged in sub-array 2. ! A total of 6303 telescope corrections were flagged in sub-array 3. ! A total of 5902 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 2549 telescope corrections were flagged in sub-array 1. ! A total of 655 telescope corrections were flagged in sub-array 2. ! A total of 6303 telescope corrections were flagged in sub-array 3. ! A total of 5902 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 2549 telescope corrections were flagged in sub-array 1. ! A total of 655 telescope corrections were flagged in sub-array 2. ! A total of 6302 telescope corrections were flagged in sub-array 3. ! A total of 5902 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 2549 telescope corrections were flagged in sub-array 1. ! A total of 655 telescope corrections were flagged in sub-array 2. ! A total of 6302 telescope corrections were flagged in sub-array 3. ! A total of 5902 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=1.645789Jy sigma=0.014243 ! Fit after self-cal, rms=1.274127Jy sigma=0.011054 ! 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 3.13% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! Estimated beam: bmin=0.5382 mas, bmaj=0.646 mas, bpa=1.349 degrees ! Estimated noise=489.308 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 = 1.62701 Jy ! Component: 100 - total flux cleaned = 1.99783 Jy ! Total flux subtracted in 100 components = 1.99783 Jy ! Clean residual min=-0.028684 max=0.143286 Jy/beam ! Clean residual mean=-0.000121 rms=0.007117 Jy/beam ! Combined flux in latest and established models = 1.99783 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 1.99783 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.555057Jy sigma=0.004202 ! Fit after self-cal, rms=0.554865Jy sigma=0.004201 ! Inverting map ! Your choice of large map pixels excluded 3.13% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.159933 Jy ! Component: 100 - total flux cleaned = 0.250013 Jy ! Total flux subtracted in 100 components = 0.250013 Jy ! Clean residual min=-0.028222 max=0.049107 Jy/beam ! Clean residual mean=-0.000068 rms=0.005735 Jy/beam ! Combined flux in latest and established models = 2.24784 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 12 components and 2.24784 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.492520Jy sigma=0.003269 ! Fit after self-cal, rms=0.492201Jy sigma=0.003267 ! Inverting map ! Your choice of large map pixels excluded 3.13% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! Added new window around map position (-0.4, 0.8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0650018 Jy ! Component: 100 - total flux cleaned = 0.113772 Jy ! Total flux subtracted in 100 components = 0.113772 Jy ! Clean residual min=-0.029030 max=0.045741 Jy/beam ! Clean residual mean=-0.000044 rms=0.005380 Jy/beam ! Combined flux in latest and established models = 2.36161 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 18 components and 2.36161 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.478550Jy sigma=0.002992 ! Fit after self-cal, rms=0.478199Jy sigma=0.002990 ! Inverting map ! Your choice of large map pixels excluded 3.13% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! Added new window around map position (-2.6, -4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0453557 Jy ! Component: 100 - total flux cleaned = 0.0786846 Jy ! Total flux subtracted in 100 components = 0.0786846 Jy ! Clean residual min=-0.028843 max=0.043399 Jy/beam ! Clean residual mean=-0.000027 rms=0.005165 Jy/beam ! Combined flux in latest and established models = 2.44029 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 19 components and 2.44029 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.472902Jy sigma=0.002860 ! Fit after self-cal, rms=0.472660Jy sigma=0.002858 ! Inverting map ! Your choice of large map pixels excluded 3.13% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! Added new window around map position (2.6, 4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0341129 Jy ! Component: 100 - total flux cleaned = 0.047666 Jy ! Total flux subtracted in 100 components = 0.047666 Jy ! Clean residual min=-0.029645 max=0.034855 Jy/beam ! Clean residual mean=-0.000018 rms=0.005004 Jy/beam ! Combined flux in latest and established models = 2.48796 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 26 components and 2.48796 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.470110Jy sigma=0.002785 ! Fit after self-cal, rms=0.469991Jy sigma=0.002784 ! Inverting map ! Your choice of large map pixels excluded 3.13% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! Added new window around map position (-0.6, -0.8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0305424 Jy ! Component: 100 - total flux cleaned = 0.0391915 Jy ! Total flux subtracted in 100 components = 0.0391915 Jy ! Clean residual min=-0.028171 max=0.032394 Jy/beam ! Clean residual mean=-0.000009 rms=0.004888 Jy/beam ! Combined flux in latest and established models = 2.52715 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 31 components and 2.52715 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.467905Jy sigma=0.002721 ! Fit after self-cal, rms=0.467755Jy sigma=0.002720 ! Inverting map ! Your choice of large map pixels excluded 3.13% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 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 3.13% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! Estimated beam: bmin=0.6172 mas, bmaj=0.7774 mas, bpa=-4.116 degrees ! Estimated noise=252.399 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 = 0.0496288 Jy ! Component: 100 - total flux cleaned = 0.0768732 Jy ! Component: 150 - total flux cleaned = 0.0846066 Jy ! Component: 200 - total flux cleaned = 0.0889645 Jy ! Total flux subtracted in 200 components = 0.0889645 Jy ! Clean residual min=-0.030017 max=0.028487 Jy/beam ! Clean residual mean=-0.000225 rms=0.005763 Jy/beam ! Combined flux in latest and established models = 2.61612 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 40 components and 2.61612 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.465477Jy sigma=0.002606 ! Fit after self-cal, rms=0.465302Jy sigma=0.002604 ! Inverting map ! Your choice of large map pixels excluded 3.13% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 72 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 1.00 GC 1.05 KP 1.05 ! LA 1.05 NL 1.03 OV 0.93 PT 1.01 ! SC 1.10 WF 1.06 HH 1.00* KK 0.96 ! MA 1.02 MC 1.00 MK 0.90 NY 0.93 ! ON 1.00 TS 1.01 WZ 1.12 HN 1.51 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.95 FD 0.94 GC 0.95 KP 0.99 ! LA 0.99 NL 0.97 OV 0.94 PT 0.97 ! SC 0.97 WF 1.05 HH 1.00* KK 1.03 ! MA 1.00* MC 1.18 MK 0.99 NY 0.93 ! ON 1.04 TS 1.02 WZ 0.99 HN 1.00* ! ! A total of 144 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.93 FD 1.01 GC 1.03 KP 1.04 ! LA 1.06 NL 1.03 OV 0.99 PT 1.03 ! SC 0.96 WF 1.09 HH 1.00* KK 0.97 ! MA 1.30 MC 1.13 MK 0.96 NY 0.92 ! ON 1.01 TS 0.96 WZ 0.93 HN 1.20 ! ! A total of 390 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.95 FD 0.97 GC 1.07 KP 1.01 ! LA 0.98 NL 0.96 OV 0.96 PT 1.01 ! SC 0.96 WF 1.05 HH 1.00* KK 1.08 ! MA 1.02 MC 1.02 MK 1.01 NY 0.98 ! ON 1.01 TS 1.36 WZ 0.97 HN 1.00* ! ! ! Correcting IF 2. ! A total of 72 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.99 GC 1.04 KP 1.02 ! LA 1.01 NL 1.06 OV 0.90 PT 0.97 ! SC 1.09 WF 1.06 HH 1.00* KK 0.96 ! MA 1.01 MC 1.01 MK 0.94 NY 0.96 ! ON 0.99 TS 1.02 WZ 1.12 HN 1.33 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.96 FD 0.93 GC 0.93 KP 0.96 ! LA 0.95 NL 1.00 OV 0.92 PT 0.93 ! SC 0.96 WF 1.04 HH 1.00* KK 1.03 ! MA 1.00* MC 1.20 MK 1.03 NY 0.95 ! ON 1.01 TS 1.02 WZ 0.99 HN 1.00* ! ! A total of 144 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.93 FD 1.00 GC 1.01 KP 1.01 ! LA 1.02 NL 1.06 OV 0.97 PT 0.99 ! SC 0.95 WF 1.08 HH 1.00* KK 0.97 ! MA 0.97 MC 1.15 MK 0.99 NY 0.97 ! ON 1.00 TS 0.98 WZ 0.95 HN 1.24 ! ! A total of 390 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.95 FD 0.95 GC 1.05 KP 0.98 ! LA 0.94 NL 0.99 OV 0.95 PT 0.97 ! SC 0.94 WF 1.06 HH 1.00* KK 1.06 ! MA 1.02 MC 1.03 MK 1.06 NY 1.01 ! ON 1.00 TS 1.38 WZ 0.97 HN 1.00* ! ! ! Correcting IF 3. ! A total of 72 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 1.01 GC 1.04 KP 1.03 ! LA 1.00 NL 1.01 OV 0.90 PT 0.99 ! SC 1.11 WF 1.05 HH 1.00* KK 0.94 ! MA 1.00 MC 0.95 MK 0.90 NY 0.99 ! ON 0.99 TS 1.04 WZ 1.13 HN 1.42 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 0.95 GC 0.95 KP 0.96 ! LA 0.93 NL 0.95 OV 0.92 PT 0.96 ! SC 0.99 WF 1.04 HH 1.00* KK 1.00 ! MA 1.00* MC 1.18 MK 0.99 NY 0.98 ! ON 0.99 TS 1.04 WZ 1.00 HN 1.00* ! ! A total of 144 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.96 FD 1.02 GC 1.01 KP 1.01 ! LA 1.01 NL 0.99 OV 0.97 PT 1.01 ! SC 0.97 WF 1.06 HH 1.00* KK 0.96 ! MA 0.94 MC 1.14 MK 0.95 NY 1.01 ! ON 1.00 TS 1.02 WZ 0.97 HN 1.17 ! ! A total of 390 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 FD 0.97 GC 1.05 KP 0.98 ! LA 0.93 NL 0.93 OV 0.95 PT 0.99 ! SC 0.95 WF 1.06 HH 1.00* KK 1.04 ! MA 1.00 MC 1.01 MK 1.01 NY 1.05 ! ON 1.00 TS 1.42 WZ 0.98 HN 1.00* ! ! ! Correcting IF 4. ! A total of 72 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.99 GC 1.03 KP 1.01 ! LA 1.01 NL 1.02 OV 0.90 PT 1.00 ! SC 1.18 WF 1.07 HH 1.00* KK 0.96 ! MA 0.98 MC 0.90 MK 0.92 NY 0.98 ! ON 0.99 TS 1.27 WZ 1.12 HN 1.34 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 FD 0.93 GC 0.94 KP 0.94 ! LA 0.95 NL 0.96 OV 0.92 PT 0.96 ! SC 1.04 WF 1.05 HH 1.00* KK 1.02 ! MA 1.00* MC 1.20 MK 1.00 NY 0.96 ! ON 1.03 TS 1.03 WZ 0.99 HN 1.00* ! ! A total of 144 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.93 FD 1.00 GC 1.01 KP 0.99 ! LA 1.01 NL 1.00 OV 0.97 PT 1.02 ! SC 1.01 WF 1.07 HH 1.00* KK 0.96 ! MA 0.93 MC 1.16 MK 0.97 NY 0.99 ! ON 1.01 TS 1.03 WZ 0.97 HN 1.14 ! ! A total of 390 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.96 FD 0.95 GC 1.06 KP 0.96 ! LA 0.94 NL 0.95 OV 0.95 PT 1.00 ! SC 1.00 WF 1.07 HH 1.00* KK 1.06 ! MA 0.97 MC 1.00 MK 1.02 NY 1.03 ! ON 1.01 TS 1.40 WZ 0.99 HN 1.00* ! ! ! Fit before self-cal, rms=0.465302Jy sigma=0.002604 ! Fit after self-cal, rms=0.514562Jy sigma=0.001837 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! Estimated beam: bmin=0.6229 mas, bmaj=0.7892 mas, bpa=-7.676 degrees ! Estimated noise=255.236 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 = -0.0394953 Jy ! Component: 100 - total flux cleaned = -0.0456916 Jy ! Component: 150 - total flux cleaned = -0.0496931 Jy ! Component: 200 - total flux cleaned = -0.0535613 Jy ! Total flux subtracted in 200 components = -0.0535613 Jy ! Clean residual min=-0.013165 max=0.010887 Jy/beam ! Clean residual mean=-0.000007 rms=0.002541 Jy/beam ! Combined flux in latest and established models = 2.56256 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 43 components and 2.56256 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.510926Jy sigma=0.001768 ! Fit after self-cal, rms=0.510972Jy sigma=0.001767 ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 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=0.510972Jy sigma=0.001767 ! Fit after self-cal, rms=0.535981Jy sigma=0.001536 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! Estimated beam: bmin=0.6237 mas, bmaj=0.7911 mas, bpa=-7.901 degrees ! Estimated noise=254.915 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0205508 Jy ! Component: 100 - total flux cleaned = -0.0315505 Jy ! Component: 150 - total flux cleaned = -0.0352377 Jy ! Component: 200 - total flux cleaned = -0.0383904 Jy ! Total flux subtracted in 200 components = -0.0383904 Jy ! Clean residual min=-0.009544 max=0.008324 Jy/beam ! Clean residual mean=-0.000082 rms=0.001493 Jy/beam ! Combined flux in latest and established models = 2.52416 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 44 components and 2.52416 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.534762Jy sigma=0.001510 ! Fit after self-cal, rms=0.534791Jy sigma=0.001510 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 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 = -0.00292288 Jy ! Component: 100 - total flux cleaned = -0.005346 Jy ! Component: 150 - total flux cleaned = -0.00718372 Jy ! Component: 200 - total flux cleaned = -0.00857538 Jy ! Total flux subtracted in 200 components = -0.00857538 Jy ! Clean residual min=-0.008587 max=0.008295 Jy/beam ! Clean residual mean=-0.000087 rms=0.001452 Jy/beam ! Combined flux in latest and established models = 2.51559 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 46 components and 2.51559 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.534445Jy sigma=0.001504 ! Fit after self-cal, rms=0.534429Jy sigma=0.001503 ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 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=0.534429Jy sigma=0.001503 ! Fit after self-cal, rms=0.535241Jy sigma=0.001421 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! Estimated beam: bmin=0.624 mas, bmaj=0.7935 mas, bpa=-8.241 degrees ! Estimated noise=254.953 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0124367 Jy ! Component: 100 - total flux cleaned = -0.0175185 Jy ! Component: 150 - total flux cleaned = -0.0196298 Jy ! Component: 200 - total flux cleaned = -0.0201512 Jy ! Total flux subtracted in 200 components = -0.0201512 Jy ! Clean residual min=-0.006557 max=0.007273 Jy/beam ! Clean residual mean=-0.000065 rms=0.001186 Jy/beam ! Combined flux in latest and established models = 2.49544 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 47 components and 2.49544 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.534779Jy sigma=0.001410 ! Fit after self-cal, rms=0.534765Jy sigma=0.001410 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 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 (-0.8, 1.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0048709 Jy ! Component: 100 - total flux cleaned = 0.00461652 Jy ! Component: 150 - total flux cleaned = 0.00439918 Jy ! Component: 200 - total flux cleaned = 0.00439684 Jy ! Total flux subtracted in 200 components = 0.00439684 Jy ! Clean residual min=-0.005960 max=0.005109 Jy/beam ! Clean residual mean=-0.000062 rms=0.001127 Jy/beam ! Combined flux in latest and established models = 2.49983 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 52 components and 2.49983 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.534574Jy sigma=0.001404 ! Fit after self-cal, rms=0.534553Jy sigma=0.001404 ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 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=0.534553Jy sigma=0.001404 ! Fit after self-cal, rms=0.533862Jy sigma=0.001400 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! Estimated beam: bmin=2.363 mas, bmaj=2.691 mas, bpa=49 degrees ! Estimated noise=397.704 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000831966 Jy ! Component: 100 - total flux cleaned = -0.0026941 Jy ! Component: 150 - total flux cleaned = -0.00409706 Jy ! Component: 200 - total flux cleaned = -0.00517374 Jy ! Total flux subtracted in 200 components = -0.00517374 Jy ! Clean residual min=-0.006520 max=0.009979 Jy/beam ! Clean residual mean=-0.000179 rms=0.002190 Jy/beam ! Combined flux in latest and established models = 2.49466 Jy selfcal ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 68 components and 2.49466 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.533833Jy sigma=0.001397 ! Fit after self-cal, rms=0.533811Jy sigma=0.001396 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 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 (-4.8, 4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00991852 Jy ! Component: 100 - total flux cleaned = 0.0159377 Jy ! Component: 150 - total flux cleaned = 0.0184515 Jy ! Component: 200 - total flux cleaned = 0.0198967 Jy ! Total flux subtracted in 200 components = 0.0198967 Jy ! Clean residual min=-0.006927 max=0.005413 Jy/beam ! Clean residual mean=-0.000178 rms=0.001780 Jy/beam ! Combined flux in latest and established models = 2.51456 Jy ! Performing phase self-cal ! Adding 57 model components to the UV plane model. ! The established model now contains 122 components and 2.51456 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.533781Jy sigma=0.001395 ! Fit after self-cal, rms=0.533770Jy sigma=0.001395 ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 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 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! Estimated beam: bmin=0.6242 mas, bmaj=0.795 mas, bpa=-8.447 degrees ! Estimated noise=254.904 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6242 x 0.795 at -8.447 degrees (North through East) ! Clean map min=-0.0052965 max=2.1674 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=0.533770Jy sigma=0.001395 ! Fit after self-cal, rms=0.565407Jy sigma=0.001196 ! Inverting map and beam ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! Estimated beam: bmin=0.6243 mas, bmaj=0.7947 mas, bpa=-8.3 degrees ! Estimated noise=254.317 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0065839 Jy ! Component: 100 - total flux cleaned = -0.00773872 Jy ! Component: 150 - total flux cleaned = -0.00772591 Jy ! Component: 200 - total flux cleaned = -0.00754795 Jy ! Total flux subtracted in 200 components = -0.00754795 Jy ! Clean residual min=-0.004008 max=0.002821 Jy/beam ! Clean residual mean=-0.000025 rms=0.000626 Jy/beam ! Combined flux in latest and established models = 2.50701 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 125 components and 2.50701 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.565224Jy sigma=0.001191 ! Fit after self-cal, rms=0.565215Jy sigma=0.001191 ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000142527 Jy ! Component: 100 - total flux cleaned = 0.000755439 Jy ! Component: 150 - total flux cleaned = 0.00133121 Jy ! Component: 200 - total flux cleaned = 0.00214083 Jy ! Total flux subtracted in 200 components = 0.00214083 Jy ! Clean residual min=-0.003464 max=0.002562 Jy/beam ! Clean residual mean=-0.000025 rms=0.000597 Jy/beam ! Combined flux in latest and established models = 2.50915 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 134 components and 2.50915 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.565132Jy sigma=0.001189 ! Fit after self-cal, rms=0.565125Jy sigma=0.001189 ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.565125Jy sigma=0.001189 ! Fit after self-cal, rms=0.564798Jy sigma=0.001187 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 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! Estimated beam: bmin=0.542 mas, bmaj=0.6544 mas, bpa=-1.727 degrees ! Estimated noise=499.558 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.65539 Jy ! Component: 100 - total flux cleaned = 2.02031 Jy ! Component: 150 - total flux cleaned = 2.15362 Jy ! Component: 200 - total flux cleaned = 2.22767 Jy ! Total flux subtracted in 200 components = 2.22767 Jy ! Clean residual min=-0.006377 max=0.040352 Jy/beam ! Clean residual mean=-0.000064 rms=0.001998 Jy/beam ! Combined flux in latest and established models = 2.22767 Jy uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Adding 14 model components to the UV plane model. ! The established model now contains 14 components and 2.22767 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! Estimated beam: bmin=0.6245 mas, bmaj=0.7955 mas, bpa=-8.366 degrees ! Estimated noise=254.151 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 = 0.0892107 Jy ! Component: 100 - total flux cleaned = 0.141835 Jy ! Component: 150 - total flux cleaned = 0.175179 Jy ! Component: 200 - total flux cleaned = 0.197267 Jy ! Total flux subtracted in 200 components = 0.197267 Jy ! Clean residual min=-0.003313 max=0.012073 Jy/beam ! Clean residual mean=-0.000061 rms=0.001295 Jy/beam ! Combined flux in latest and established models = 2.42494 Jy ! Adding 33 model components to the UV plane model. ! The established model now contains 35 components and 2.42494 Jy ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0153819 Jy ! Component: 100 - total flux cleaned = 0.026836 Jy ! Component: 150 - total flux cleaned = 0.0357454 Jy ! Component: 200 - total flux cleaned = 0.042808 Jy ! Total flux subtracted in 200 components = 0.042808 Jy ! Clean residual min=-0.002676 max=0.004542 Jy/beam ! Clean residual mean=-0.000032 rms=0.000769 Jy/beam ! Combined flux in latest and established models = 2.46775 Jy ! Adding 40 model components to the UV plane model. ! The established model now contains 62 components and 2.46775 Jy ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! Added new window around map position (1.4, 0). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0058703 Jy ! Component: 100 - total flux cleaned = 0.0109499 Jy ! Component: 150 - total flux cleaned = 0.0154738 Jy ! Component: 200 - total flux cleaned = 0.0195236 Jy ! Total flux subtracted in 200 components = 0.0195236 Jy ! Clean residual min=-0.002555 max=0.003077 Jy/beam ! Clean residual mean=-0.000023 rms=0.000640 Jy/beam ! Combined flux in latest and established models = 2.48727 Jy ! Adding 59 model components to the UV plane model. ! The established model now contains 92 components and 2.48727 Jy ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! Added new window around map position (6.6, -6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0031735 Jy ! Component: 100 - total flux cleaned = 0.00550342 Jy ! Component: 150 - total flux cleaned = 0.00754711 Jy ! Component: 200 - total flux cleaned = 0.00898656 Jy ! Total flux subtracted in 200 components = 0.00898656 Jy ! Clean residual min=-0.002549 max=0.002361 Jy/beam ! Clean residual mean=-0.000021 rms=0.000587 Jy/beam ! Combined flux in latest and established models = 2.49626 Jy ! Adding 69 model components to the UV plane model. ! The established model now contains 119 components and 2.49626 Jy ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 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 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! Estimated beam: bmin=2.364 mas, bmaj=2.692 mas, bpa=48.86 degrees ! Estimated noise=395.591 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00640703 Jy ! Component: 100 - total flux cleaned = 0.00991739 Jy ! Component: 150 - total flux cleaned = 0.0113013 Jy ! Component: 200 - total flux cleaned = 0.0124693 Jy ! Total flux subtracted in 200 components = 0.0124693 Jy ! Clean residual min=-0.003719 max=0.002566 Jy/beam ! Clean residual mean=-0.000072 rms=0.001031 Jy/beam ! Combined flux in latest and established models = 2.50873 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 = 0.000703704 Jy ! Component: 100 - total flux cleaned = 0.00114278 Jy ! Component: 150 - total flux cleaned = 0.00153033 Jy ! Component: 200 - total flux cleaned = 0.00180776 Jy ! Total flux subtracted in 200 components = 0.00180776 Jy ! Clean residual min=-0.003727 max=0.002376 Jy/beam ! Clean residual mean=-0.000073 rms=0.000953 Jy/beam ! Combined flux in latest and established models = 2.51054 Jy ! Adding 81 model components to the UV plane model. ! The established model now contains 189 components and 2.51054 Jy ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! Estimated beam: bmin=0.6245 mas, bmaj=0.7955 mas, bpa=-8.366 degrees ! Estimated noise=254.151 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000724715 Jy ! Component: 100 - total flux cleaned = 0.00101751 Jy ! Component: 150 - total flux cleaned = 0.00118951 Jy ! Component: 200 - total flux cleaned = 0.00142822 Jy ! Total flux subtracted in 200 components = 0.00142822 Jy ! Clean residual min=-0.002269 max=0.002258 Jy/beam ! Clean residual mean=-0.000018 rms=0.000506 Jy/beam ! Combined flux in latest and established models = 2.51196 Jy selfcal ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 201 components and 2.51196 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.564573Jy sigma=0.001182 ! Fit after self-cal, rms=0.564519Jy sigma=0.001182 wmodel J0136+4751_X_2000_03_13_pus_map.mod ! Writing 201 model components to file: J0136+4751_X_2000_03_13_pus_map.mod wobs J0136+4751_X_2000_03_13_pus_uvs.fits ! Writing UV FITS file: J0136+4751_X_2000_03_13_pus_uvs.fits wwins J0136+4751_X_2000_03_13_pus_map.win ! wwins: Wrote 9 windows to J0136+4751_X_2000_03_13_pus_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 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000771977 Jy ! Component: 100 - total flux cleaned = -0.00132895 Jy ! Component: 150 - total flux cleaned = -0.00185879 Jy ! Component: 200 - total flux cleaned = -0.0023664 Jy ! Component: 250 - total flux cleaned = -0.00271699 Jy ! Component: 300 - total flux cleaned = -0.00302551 Jy ! Component: 350 - total flux cleaned = -0.00326109 Jy ! Component: 400 - total flux cleaned = -0.00352482 Jy ! Component: 450 - total flux cleaned = -0.00371955 Jy ! Component: 500 - total flux cleaned = -0.00397545 Jy ! Component: 550 - total flux cleaned = -0.00425958 Jy ! Component: 600 - total flux cleaned = -0.00444678 Jy ! Component: 650 - total flux cleaned = -0.00478538 Jy ! Component: 700 - total flux cleaned = -0.00496744 Jy ! Component: 750 - total flux cleaned = -0.00514767 Jy ! Component: 800 - total flux cleaned = -0.00526671 Jy ! Component: 850 - total flux cleaned = -0.00535557 Jy ! Component: 900 - total flux cleaned = -0.00553137 Jy ! Component: 950 - total flux cleaned = -0.0055895 Jy ! Component: 1000 - total flux cleaned = -0.00573365 Jy ! Component: 1050 - total flux cleaned = -0.00584804 Jy ! Component: 1100 - total flux cleaned = -0.00598971 Jy ! Component: 1150 - total flux cleaned = -0.00615862 Jy ! Component: 1200 - total flux cleaned = -0.00621469 Jy ! Component: 1250 - total flux cleaned = -0.0064369 Jy ! Component: 1300 - total flux cleaned = -0.00654727 Jy ! Component: 1350 - total flux cleaned = -0.00671164 Jy ! Component: 1400 - total flux cleaned = -0.00684776 Jy ! Component: 1450 - total flux cleaned = -0.00695594 Jy ! Component: 1500 - total flux cleaned = -0.00706357 Jy ! Component: 1550 - total flux cleaned = -0.00714393 Jy ! Component: 1600 - total flux cleaned = -0.00727683 Jy ! Component: 1650 - total flux cleaned = -0.0073826 Jy ! Component: 1700 - total flux cleaned = -0.00751377 Jy ! Component: 1750 - total flux cleaned = -0.00759209 Jy ! Component: 1800 - total flux cleaned = -0.00766987 Jy ! Component: 1850 - total flux cleaned = -0.00779903 Jy ! Component: 1900 - total flux cleaned = -0.00790191 Jy ! Component: 1950 - total flux cleaned = -0.00805516 Jy ! Component: 2000 - total flux cleaned = -0.00802959 Jy ! Total flux subtracted in 2048 components = -0.00823209 Jy ! Clean residual min=-0.001304 max=0.001268 Jy/beam ! Clean residual mean=-0.000015 rms=0.000436 Jy/beam ! Combined flux in latest and established models = 2.50373 Jy keep ! Adding 169 model components to the UV plane model. ! The established model now contains 366 components and 2.50373 Jy ![Exited script file: muppet] wmap "J0136+4751_X_2000_03_13_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6245 x 0.7955 at -8.366 degrees (North through East) ! Clean map min=-0.0021358 max=2.1703 Jy/beam ! Writing clean map to FITS file: J0136+4751_X_2000_03_13_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 2.17033 invert ! Inverting map ! Your choice of large map pixels excluded 3.18% of the data. ! The x-axis pixel size should ideally be below 0.1567 milli-arcsec ! The y-axis pixel size should ideally be below 0.1864 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000436004 device "J0136+4751_X_2000_03_13_pus\_map.eps/VPS" ! Attempting to open device: 'J0136+4751_X_2000_03_13_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.0602678 0.0602678 0.120536 0.241071 0.482142 0.964285 1.92857 3.85714 7.71428 15.4286 30.8571 61.7142 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0013 print "peak=",int(1000*peak_flux)/1000 ! peak= 2.17 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6245 x 0.7955 at -8.366 degrees (North through East) ! Clean map min=-0.0021358 max=2.1703 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. quit ! Quitting program ! Log file J0136+4751_X_2000_03_13_pus_uvs.log closed on Mon Apr 1 13:22:52 2013