! Started logfile: J0238+1636_X_2000_03_13_pus_uvs.log on Wed Apr 3 15:41:23 2013 obs J0238+1636_X_2000_03_13_pus_uva.fits ! Reading UV FITS file: J0238+1636_X_2000_03_13_pus_uva.fits ! AN table 1: 102 integrations on 190 of 190 possible baselines. ! AN table 2: 65 integrations on 190 of 190 possible baselines. ! AN table 3: 85 integrations on 190 of 190 possible baselines. ! AN table 4: 21 integrations on 190 of 190 possible baselines. ! AN table 5: 63 integrations on 190 of 190 possible baselines. ! Apparent sampling: 0.110385 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0238+1636 ! ! 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 2386 lines of history. ! ! Reading 28188 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 J0238+1636_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 1357 telescope corrections were flagged in sub-array 1. ! A total of 1028 telescope corrections were flagged in sub-array 2. ! A total of 1388 telescope corrections were flagged in sub-array 3. ! A total of 217 telescope corrections were flagged in sub-array 4. ! A total of 965 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 1357 telescope corrections were flagged in sub-array 1. ! A total of 1028 telescope corrections were flagged in sub-array 2. ! A total of 1391 telescope corrections were flagged in sub-array 3. ! A total of 217 telescope corrections were flagged in sub-array 4. ! A total of 952 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 1357 telescope corrections were flagged in sub-array 1. ! A total of 1028 telescope corrections were flagged in sub-array 2. ! A total of 1389 telescope corrections were flagged in sub-array 3. ! A total of 217 telescope corrections were flagged in sub-array 4. ! A total of 954 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 1357 telescope corrections were flagged in sub-array 1. ! A total of 1029 telescope corrections were flagged in sub-array 2. ! A total of 1394 telescope corrections were flagged in sub-array 3. ! A total of 217 telescope corrections were flagged in sub-array 4. ! A total of 944 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=1.082793Jy sigma=0.009936 ! Fit after self-cal, rms=0.268806Jy sigma=0.002109 ! 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 0.966% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec ! Estimated beam: bmin=0.5742 mas, bmaj=1.034 mas, bpa=1.546 degrees ! Estimated noise=973.392 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 = 0.623301 Jy ! Component: 100 - total flux cleaned = 0.765896 Jy ! Total flux subtracted in 100 components = 0.765896 Jy ! Clean residual min=-0.014000 max=0.054538 Jy/beam ! Clean residual mean=-0.000109 rms=0.004487 Jy/beam ! Combined flux in latest and established models = 0.765896 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.765896 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.228349Jy sigma=0.001965 ! Fit after self-cal, rms=0.228332Jy sigma=0.001965 ! Inverting map ! Your choice of large map pixels excluded 0.966% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0609339 Jy ! Component: 100 - total flux cleaned = 0.0971064 Jy ! Total flux subtracted in 100 components = 0.0971064 Jy ! Clean residual min=-0.010593 max=0.019543 Jy/beam ! Clean residual mean=-0.000054 rms=0.003220 Jy/beam ! Combined flux in latest and established models = 0.863002 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 18 components and 0.863002 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.201896Jy sigma=0.001593 ! Fit after self-cal, rms=0.201871Jy sigma=0.001593 ! Inverting map ! Your choice of large map pixels excluded 0.966% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0242316 Jy ! Component: 100 - total flux cleaned = 0.0408339 Jy ! Total flux subtracted in 100 components = 0.0408339 Jy ! Clean residual min=-0.010191 max=0.015646 Jy/beam ! Clean residual mean=-0.000031 rms=0.002910 Jy/beam ! Combined flux in latest and established models = 0.903836 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 23 components and 0.903836 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.196432Jy sigma=0.001495 ! Fit after self-cal, rms=0.196418Jy sigma=0.001495 ! Inverting map ! Your choice of large map pixels excluded 0.966% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 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 0.966% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec ! Estimated beam: bmin=0.722 mas, bmaj=1.273 mas, bpa=3.941 degrees ! Estimated noise=508.683 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 = 0.0321074 Jy ! Component: 100 - total flux cleaned = 0.0492045 Jy ! Component: 150 - total flux cleaned = 0.059062 Jy ! Component: 200 - total flux cleaned = 0.0648424 Jy ! Total flux subtracted in 200 components = 0.0648424 Jy ! Clean residual min=-0.010341 max=0.013463 Jy/beam ! Clean residual mean=0.000010 rms=0.002946 Jy/beam ! Combined flux in latest and established models = 0.968678 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 36 components and 0.968678 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.194094Jy sigma=0.001416 ! Fit after self-cal, rms=0.194082Jy sigma=0.001416 ! Inverting map ! Your choice of large map pixels excluded 0.966% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 129 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.95 GC 0.99 KP 0.98 ! LA 0.97 NL 0.96 OV 0.98 PT 0.97 ! SC 0.95 WF 1.04 HH 1.00* KK 1.08 ! MA 1.00* MC 1.00* MK 1.02 NY 0.98 ! ON 1.03 TS 1.00* WZ 1.00* HN 1.00* ! ! A total of 9 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* GC 1.64 KP 1.00* ! LA 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.05 WF 1.02 HH 1.00* KK 1.00* ! MA 1.04 MC 1.05 MK 1.00* NY 0.97 ! ON 1.05 TS 0.95 WZ 1.06 HN 1.00* ! ! A total of 168 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00* GC 1.00* KP 1.00* ! LA 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.18 WF 1.22 HH 0.86 KK 1.00* ! MA 1.01 MC 0.99 MK 1.00* NY 0.97 ! ON 1.53 TS 1.00* WZ 1.05 HN 0.73 ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 FD 1.02 GC 1.00 KP 1.05 ! LA 1.08 NL 1.12 OV 1.01 PT 1.06 ! SC 1.00* WF 1.00* HH 1.00* KK 0.97 ! MA 1.00* MC 1.00* MK 0.99 NY 1.02 ! ON 1.00* TS 0.90 WZ 1.00* HN 1.00* ! ! A total of 12 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.96 FD 0.98 GC 0.99 KP 1.00 ! LA 1.02 NL 0.99 OV 0.96 PT 1.00 ! SC 1.04 WF 1.04 HH 1.00* KK 0.99 ! MA 1.00* MC 1.00* MK 0.82 NY 1.07 ! ON 1.00* TS 1.06 WZ 1.00* HN 0.98 ! ! ! Correcting IF 2. ! A total of 129 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 0.95 GC 0.97 KP 0.95 ! LA 0.93 NL 0.98 OV 0.97 PT 0.94 ! SC 0.93 WF 1.04 HH 1.00* KK 1.06 ! MA 1.00* MC 1.00* MK 1.06 NY 0.99 ! ON 0.99 TS 1.00* WZ 1.00* HN 1.00* ! ! A total of 9 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* GC 1.66 KP 1.00* ! LA 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 0.99 WF 1.08 HH 1.00* KK 1.00* ! MA 1.05 MC 1.07 MK 1.00* NY 1.02 ! ON 1.07 TS 0.94 WZ 1.04 HN 1.00* ! ! A total of 171 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00* GC 1.00* KP 1.00* ! LA 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.14 WF 1.22 HH 0.89 KK 1.00* ! MA 1.00 MC 1.00 MK 1.00* NY 1.04 ! ON 1.52 TS 1.00* WZ 1.06 HN 0.62 ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 FD 1.03 GC 0.99 KP 1.01 ! LA 1.05 NL 1.18 OV 1.00 PT 1.02 ! SC 1.00* WF 1.00* HH 1.00* KK 0.98 ! MA 1.00* MC 1.00* MK 1.03 NY 1.08 ! ON 1.00* TS 0.90 WZ 1.00* HN 1.00* ! ! A total of 27 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.96 FD 0.96 GC 0.94 KP 0.99 ! LA 0.97 NL 1.02 OV 0.95 PT 0.98 ! SC 1.03 WF 1.09 HH 1.00* KK 1.00 ! MA 1.00* MC 1.00* MK 0.85 NY 1.12 ! ON 1.00* TS 1.07 WZ 1.00* HN 1.07 ! ! ! Correcting IF 3. ! A total of 129 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 0.98 GC 1.00 KP 0.98 ! LA 0.92 NL 0.95 OV 0.98 PT 0.99 ! SC 0.95 WF 1.06 HH 1.00* KK 1.08 ! MA 1.00* MC 1.00* MK 1.04 NY 1.12 ! ON 1.03 TS 1.00* WZ 1.00* HN 1.00* ! ! A total of 9 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* GC 1.62 KP 1.00* ! LA 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.05 WF 1.02 HH 1.00* KK 1.00* ! MA 1.02 MC 1.07 MK 1.00* NY 1.07 ! ON 1.04 TS 1.00 WZ 1.08 HN 1.00* ! ! A total of 168 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00* GC 1.00* KP 1.00* ! LA 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.28 WF 1.21 HH 0.87 KK 1.00* ! MA 1.01 MC 0.97 MK 1.00* NY 1.15 ! ON 1.71 TS 1.00* WZ 1.12 HN 0.80 ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 FD 1.05 GC 1.02 KP 1.05 ! LA 1.06 NL 1.12 OV 1.02 PT 1.04 ! SC 1.00* WF 1.00* HH 1.00* KK 0.98 ! MA 1.00* MC 1.00* MK 1.01 NY 1.14 ! ON 1.00* TS 0.92 WZ 1.00* HN 1.00* ! ! A total of 30 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 FD 1.00 GC 0.96 KP 1.01 ! LA 0.97 NL 0.98 OV 0.97 PT 1.00 ! SC 1.08 WF 1.12 HH 1.00* KK 0.99 ! MA 1.00* MC 1.00* MK 0.83 NY 1.19 ! ON 1.00* TS 1.11 WZ 1.00* HN 0.89 ! ! ! Correcting IF 4. ! A total of 129 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.96 GC 1.00 KP 0.95 ! LA 0.95 NL 0.98 OV 0.99 PT 0.98 ! SC 1.01 WF 1.11 HH 1.00* KK 1.09 ! MA 1.00* MC 1.00* MK 1.06 NY 1.11 ! ON 1.08 TS 1.00* WZ 1.00* HN 1.00* ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* GC 1.55 KP 1.00* ! LA 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.04 WF 1.05 HH 1.00* KK 1.00* ! MA 1.05 MC 1.03 MK 1.00* NY 1.07 ! ON 1.08 TS 1.01 WZ 1.10 HN 1.00* ! ! A total of 171 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00* GC 1.00* KP 1.00* ! LA 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.21 WF 1.24 HH 0.87 KK 1.00* ! MA 0.97 MC 0.97 MK 1.00* NY 1.05 ! ON 1.60 TS 1.00* WZ 1.13 HN 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 1.04 GC 0.99 KP 1.02 ! LA 1.05 NL 1.13 OV 1.01 PT 1.08 ! SC 1.00* WF 1.00* HH 1.00* KK 1.00 ! MA 1.00* MC 1.00* MK 1.02 NY 1.14 ! ON 1.00* TS 0.95 WZ 1.00* HN 1.00* ! ! A total of 36 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 FD 0.98 GC 0.99 KP 0.98 ! LA 0.98 NL 1.01 OV 0.98 PT 1.02 ! SC 1.15 WF 1.13 HH 1.00* KK 1.02 ! MA 1.00* MC 1.00* MK 0.84 NY 1.17 ! ON 1.00* TS 1.11 WZ 1.00* HN 1.14 ! ! ! Fit before self-cal, rms=0.194082Jy sigma=0.001416 ! Fit after self-cal, rms=0.182590Jy sigma=0.001228 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec ! Estimated beam: bmin=0.7198 mas, bmaj=1.268 mas, bpa=4.404 degrees ! Estimated noise=519.995 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 = -0.00321313 Jy ! Component: 100 - total flux cleaned = -0.00409588 Jy ! Component: 150 - total flux cleaned = -0.00471504 Jy ! Component: 200 - total flux cleaned = -0.00522592 Jy ! Total flux subtracted in 200 components = -0.00522592 Jy ! Clean residual min=-0.004245 max=0.003834 Jy/beam ! Clean residual mean=-0.000028 rms=0.000983 Jy/beam ! Combined flux in latest and established models = 0.963453 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 38 components and 0.963453 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.182406Jy sigma=0.001227 ! Fit after self-cal, rms=0.182705Jy sigma=0.001226 ! Inverting map ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 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=0.182705Jy sigma=0.001226 ! Fit after self-cal, rms=0.181552Jy sigma=0.001213 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec ! Estimated beam: bmin=0.7228 mas, bmaj=1.269 mas, bpa=4.478 degrees ! Estimated noise=520.519 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00258112 Jy ! Component: 100 - total flux cleaned = -0.00321409 Jy ! Component: 150 - total flux cleaned = -0.00383466 Jy ! Component: 200 - total flux cleaned = -0.00425858 Jy ! Total flux subtracted in 200 components = -0.00425858 Jy ! Clean residual min=-0.003328 max=0.002627 Jy/beam ! Clean residual mean=-0.000021 rms=0.000763 Jy/beam ! Combined flux in latest and established models = 0.959194 Jy selfcal ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 40 components and 0.959194 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.181357Jy sigma=0.001211 ! Fit after self-cal, rms=0.181476Jy sigma=0.001211 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 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 = -0.00039498 Jy ! Component: 100 - total flux cleaned = -0.00074975 Jy ! Component: 150 - total flux cleaned = -0.00104819 Jy ! Component: 200 - total flux cleaned = -0.00129912 Jy ! Total flux subtracted in 200 components = -0.00129912 Jy ! Clean residual min=-0.003290 max=0.002731 Jy/beam ! Clean residual mean=-0.000023 rms=0.000764 Jy/beam ! Combined flux in latest and established models = 0.957895 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 40 components and 0.957895 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.181426Jy sigma=0.001211 ! Fit after self-cal, rms=0.181425Jy sigma=0.001211 ! Inverting map ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 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=0.181425Jy sigma=0.001211 ! Fit after self-cal, rms=0.181879Jy sigma=0.001210 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec ! Estimated beam: bmin=0.7253 mas, bmaj=1.271 mas, bpa=4.541 degrees ! Estimated noise=521.242 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00175024 Jy ! Component: 100 - total flux cleaned = -0.00223218 Jy ! Component: 150 - total flux cleaned = -0.00270844 Jy ! Component: 200 - total flux cleaned = -0.00310298 Jy ! Total flux subtracted in 200 components = -0.00310298 Jy ! Clean residual min=-0.003144 max=0.002570 Jy/beam ! Clean residual mean=-0.000020 rms=0.000719 Jy/beam ! Combined flux in latest and established models = 0.954792 Jy selfcal ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 40 components and 0.954792 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.181769Jy sigma=0.001209 ! Fit after self-cal, rms=0.181766Jy sigma=0.001209 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 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 = -0.000425541 Jy ! Component: 100 - total flux cleaned = -0.000660834 Jy ! Component: 150 - total flux cleaned = -0.000942653 Jy ! Component: 200 - total flux cleaned = -0.00115317 Jy ! Total flux subtracted in 200 components = -0.00115317 Jy ! Clean residual min=-0.003112 max=0.002554 Jy/beam ! Clean residual mean=-0.000022 rms=0.000721 Jy/beam ! Combined flux in latest and established models = 0.953639 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 40 components and 0.953639 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.181735Jy sigma=0.001209 ! Fit after self-cal, rms=0.181736Jy sigma=0.001209 ! Inverting map ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 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=0.181736Jy sigma=0.001209 ! Fit after self-cal, rms=0.182136Jy sigma=0.001209 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec ! Estimated beam: bmin=2.337 mas, bmaj=2.59 mas, bpa=27.62 degrees ! Estimated noise=695.255 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0013012 Jy ! Component: 100 - total flux cleaned = -0.00130399 Jy ! Component: 150 - total flux cleaned = -0.00130519 Jy ! Component: 200 - total flux cleaned = -0.00130635 Jy ! Total flux subtracted in 200 components = -0.00130635 Jy ! Clean residual min=-0.003855 max=0.003327 Jy/beam ! Clean residual mean=-0.000048 rms=0.001044 Jy/beam ! Combined flux in latest and established models = 0.952332 Jy selfcal ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 42 components and 0.952332 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.182162Jy sigma=0.001209 ! Fit after self-cal, rms=0.182155Jy sigma=0.001209 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 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 = 8.99691e-05 Jy ! Component: 100 - total flux cleaned = 8.77217e-05 Jy ! Component: 150 - total flux cleaned = 8.55447e-05 Jy ! Component: 200 - total flux cleaned = 9.67275e-05 Jy ! Total flux subtracted in 200 components = 9.67275e-05 Jy ! Clean residual min=-0.003854 max=0.003310 Jy/beam ! Clean residual mean=-0.000047 rms=0.001042 Jy/beam ! Combined flux in latest and established models = 0.952429 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 42 components and 0.952429 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.182163Jy sigma=0.001209 ! Fit after self-cal, rms=0.182161Jy sigma=0.001209 ! Inverting map ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. win_mult = win_mult / 1.2 print "************** FINISHED AMPLITUDE SELF-CAL **************" ! ************** FINISHED AMPLITUDE SELF-CAL ************** restore ! Inverting map and beam ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec ! Estimated beam: bmin=0.7272 mas, bmaj=1.273 mas, bpa=4.57 degrees ! Estimated noise=521.863 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7272 x 1.273 at 4.57 degrees (North through East) ! Clean map min=-0.0025504 max=0.85006 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=0.182161Jy sigma=0.001209 ! Fit after self-cal, rms=0.168934Jy sigma=0.001106 ! Inverting map and beam ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec ! Estimated beam: bmin=0.727 mas, bmaj=1.273 mas, bpa=4.575 degrees ! Estimated noise=520.355 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0021625 Jy ! Component: 100 - total flux cleaned = -0.0026217 Jy ! Component: 150 - total flux cleaned = -0.00307249 Jy ! Component: 200 - total flux cleaned = -0.00345671 Jy ! Total flux subtracted in 200 components = -0.00345671 Jy ! Clean residual min=-0.003149 max=0.002553 Jy/beam ! Clean residual mean=-0.000020 rms=0.000671 Jy/beam ! Combined flux in latest and established models = 0.948972 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 42 components and 0.948972 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.168849Jy sigma=0.001106 ! Fit after self-cal, rms=0.168852Jy sigma=0.001106 ! Inverting map ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000339225 Jy ! Component: 100 - total flux cleaned = -0.000617969 Jy ! Component: 150 - total flux cleaned = -0.000823131 Jy ! Component: 200 - total flux cleaned = -0.00103213 Jy ! Total flux subtracted in 200 components = -0.00103213 Jy ! Clean residual min=-0.003124 max=0.002539 Jy/beam ! Clean residual mean=-0.000022 rms=0.000672 Jy/beam ! Combined flux in latest and established models = 0.94794 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 42 components and 0.94794 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.168829Jy sigma=0.001106 ! Fit after self-cal, rms=0.168831Jy sigma=0.001106 ! Inverting map ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.168831Jy sigma=0.001106 ! Fit after self-cal, rms=0.169078Jy sigma=0.001105 print "************** CLEARING MODEL AND STARTING OVER **********" ! ************** CLEARING MODEL AND STARTING OVER ********** clrmod true ! clrmod: Cleared the established and tentative models. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec ! Estimated beam: bmin=0.5835 mas, bmaj=1.044 mas, bpa=1.338 degrees ! Estimated noise=991.845 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.646098 Jy ! Component: 100 - total flux cleaned = 0.789283 Jy ! Component: 150 - total flux cleaned = 0.842507 Jy ! Component: 200 - total flux cleaned = 0.873479 Jy ! Total flux subtracted in 200 components = 0.873479 Jy ! Clean residual min=-0.006113 max=0.016332 Jy/beam ! Clean residual mean=-0.000054 rms=0.001614 Jy/beam ! Combined flux in latest and established models = 0.873479 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 18 model components to the UV plane model. ! The established model now contains 18 components and 0.873479 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec ! Estimated beam: bmin=0.7286 mas, bmaj=1.275 mas, bpa=4.568 degrees ! Estimated noise=520.592 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 = 0.0314269 Jy ! Component: 100 - total flux cleaned = 0.0483419 Jy ! Component: 150 - total flux cleaned = 0.0579654 Jy ! Component: 200 - total flux cleaned = 0.0635124 Jy ! Total flux subtracted in 200 components = 0.0635124 Jy ! Clean residual min=-0.002907 max=0.003566 Jy/beam ! Clean residual mean=-0.000033 rms=0.000730 Jy/beam ! Combined flux in latest and established models = 0.936991 Jy ! Adding 24 model components to the UV plane model. ! The established model now contains 32 components and 0.936991 Jy ! Inverting map ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec ! Added new window around map position (-0.6, 0). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00369049 Jy ! Component: 100 - total flux cleaned = 0.0060365 Jy ! Component: 150 - total flux cleaned = 0.00693852 Jy ! Component: 200 - total flux cleaned = 0.00750897 Jy ! Total flux subtracted in 200 components = 0.00750897 Jy ! Clean residual min=-0.002782 max=0.002587 Jy/beam ! Clean residual mean=-0.000021 rms=0.000654 Jy/beam ! Combined flux in latest and established models = 0.9445 Jy ! Adding 16 model components to the UV plane model. ! The established model now contains 46 components and 0.9445 Jy ! Inverting map ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec ! Estimated beam: bmin=2.34 mas, bmaj=2.592 mas, bpa=27.53 degrees ! Estimated noise=691.215 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00169216 Jy ! Component: 100 - total flux cleaned = 0.00203892 Jy ! Component: 150 - total flux cleaned = 0.00215891 Jy ! Component: 200 - total flux cleaned = 0.00217865 Jy ! Total flux subtracted in 200 components = 0.00217865 Jy ! Clean residual min=-0.003429 max=0.003091 Jy/beam ! Clean residual mean=-0.000048 rms=0.000968 Jy/beam ! Combined flux in latest and established models = 0.946679 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 = 1.7536e-05 Jy ! Component: 100 - total flux cleaned = 3.30837e-05 Jy ! Component: 150 - total flux cleaned = 4.69672e-05 Jy ! Component: 200 - total flux cleaned = 5.96015e-05 Jy ! Total flux subtracted in 200 components = 5.96015e-05 Jy ! Clean residual min=-0.003395 max=0.003060 Jy/beam ! Clean residual mean=-0.000048 rms=0.000963 Jy/beam ! Combined flux in latest and established models = 0.946739 Jy ! Adding 12 model components to the UV plane model. ! The established model now contains 56 components and 0.946739 Jy ! Inverting map ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec ! Estimated beam: bmin=0.7286 mas, bmaj=1.275 mas, bpa=4.568 degrees ! Estimated noise=520.592 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000446355 Jy ! Component: 100 - total flux cleaned = -0.000409001 Jy ! Component: 150 - total flux cleaned = -0.00037618 Jy ! Component: 200 - total flux cleaned = -0.000344751 Jy ! Total flux subtracted in 200 components = -0.000344751 Jy ! Clean residual min=-0.002811 max=0.002656 Jy/beam ! Clean residual mean=-0.000018 rms=0.000644 Jy/beam ! Combined flux in latest and established models = 0.946394 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 69 components and 0.946394 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.168924Jy sigma=0.001105 ! Fit after self-cal, rms=0.168933Jy sigma=0.001105 wmodel J0238+1636_X_2000_03_13_pus_map.mod ! Writing 69 model components to file: J0238+1636_X_2000_03_13_pus_map.mod wobs J0238+1636_X_2000_03_13_pus_uvs.fits ! Writing UV FITS file: J0238+1636_X_2000_03_13_pus_uvs.fits wwins J0238+1636_X_2000_03_13_pus_map.win ! wwins: Wrote 2 windows to J0238+1636_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 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000494048 Jy ! Component: 100 - total flux cleaned = -0.00120455 Jy ! Component: 150 - total flux cleaned = -0.00187821 Jy ! Component: 200 - total flux cleaned = -0.00232392 Jy ! Component: 250 - total flux cleaned = -0.00267945 Jy ! Component: 300 - total flux cleaned = -0.0031033 Jy ! Component: 350 - total flux cleaned = -0.00344261 Jy ! Component: 400 - total flux cleaned = -0.00381164 Jy ! Component: 450 - total flux cleaned = -0.0040652 Jy ! Component: 500 - total flux cleaned = -0.00431458 Jy ! Component: 550 - total flux cleaned = -0.00459481 Jy ! Component: 600 - total flux cleaned = -0.0046985 Jy ! Component: 650 - total flux cleaned = -0.0050061 Jy ! Component: 700 - total flux cleaned = -0.00524183 Jy ! Component: 750 - total flux cleaned = -0.00547454 Jy ! Component: 800 - total flux cleaned = -0.00550726 Jy ! Component: 850 - total flux cleaned = -0.00554 Jy ! Component: 900 - total flux cleaned = -0.00573291 Jy ! Component: 950 - total flux cleaned = -0.00582843 Jy ! Component: 1000 - total flux cleaned = -0.00582804 Jy ! Component: 1050 - total flux cleaned = -0.00585967 Jy ! Component: 1100 - total flux cleaned = -0.00598386 Jy ! Component: 1150 - total flux cleaned = -0.00607598 Jy ! Component: 1200 - total flux cleaned = -0.00610644 Jy ! Component: 1250 - total flux cleaned = -0.00622751 Jy ! Component: 1300 - total flux cleaned = -0.00637797 Jy ! Component: 1350 - total flux cleaned = -0.0064373 Jy ! Component: 1400 - total flux cleaned = -0.00652647 Jy ! Component: 1450 - total flux cleaned = -0.00658507 Jy ! Component: 1500 - total flux cleaned = -0.00675942 Jy ! Component: 1550 - total flux cleaned = -0.00675916 Jy ! Component: 1600 - total flux cleaned = -0.00681659 Jy ! Component: 1650 - total flux cleaned = -0.00698699 Jy ! Component: 1700 - total flux cleaned = -0.00701514 Jy ! Component: 1750 - total flux cleaned = -0.00707127 Jy ! Component: 1800 - total flux cleaned = -0.00729405 Jy ! Component: 1850 - total flux cleaned = -0.00737696 Jy ! Component: 1900 - total flux cleaned = -0.00729422 Jy ! Component: 1950 - total flux cleaned = -0.00745848 Jy ! Component: 2000 - total flux cleaned = -0.00751253 Jy ! Total flux subtracted in 2048 components = -0.00759393 Jy ! Clean residual min=-0.001664 max=0.001541 Jy/beam ! Clean residual mean=-0.000013 rms=0.000495 Jy/beam ! Combined flux in latest and established models = 0.9388 Jy keep ! Adding 182 model components to the UV plane model. ! The established model now contains 251 components and 0.9388 Jy ![Exited script file: muppet] wmap "J0238+1636_X_2000_03_13_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7286 x 1.275 at 4.568 degrees (North through East) ! Clean map min=-0.0022675 max=0.84969 Jy/beam ! Writing clean map to FITS file: J0238+1636_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 0.849691 invert ! Inverting map ! Your choice of large map pixels excluded 0.934% of the data. ! The x-axis pixel size should ideally be below 0.1583 milli-arcsec ! The y-axis pixel size should ideally be below 0.1726 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000494644 device "J0238+1636_X_2000_03_13_pus\_map.eps/VPS" ! Attempting to open device: 'J0238+1636_X_2000_03_13_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.174644 0.174644 0.349287 0.698574 1.39715 2.7943 5.58859 11.1772 22.3544 44.7087 89.4175 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0014 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.849 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7286 x 1.275 at 4.568 degrees (North through East) ! Clean map min=-0.0022675 max=0.84969 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. quit ! Quitting program ! Log file J0238+1636_X_2000_03_13_pus_uvs.log closed on Wed Apr 3 15:41:34 2013