! Started logfile: J0811+0146_X_2011_06_28_pus_uvs.log on Sat Apr 21 13:00:17 2012 obs J0811+0146_X_2011_06_28_pus_uva.fits ! Reading UV FITS file: J0811+0146_X_2011_06_28_pus_uva.fits ! AN table 1: 102 integrations on 153 of 153 possible baselines. ! AN table 2: 12 integrations on 153 of 153 possible baselines. ! AN table 3: 308 integrations on 153 of 153 possible baselines. ! Apparent sampling: 0.113713 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0811+0146 ! ! 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 5249 lines of history. ! ! Reading 29368 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 J0811+0146_X_2011_06_28_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 1310 telescope corrections were flagged in sub-array 1. ! A total of 126 telescope corrections were flagged in sub-array 2. ! A total of 4020 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 1310 telescope corrections were flagged in sub-array 1. ! A total of 126 telescope corrections were flagged in sub-array 2. ! A total of 4020 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 1310 telescope corrections were flagged in sub-array 1. ! A total of 126 telescope corrections were flagged in sub-array 2. ! A total of 4020 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 1310 telescope corrections were flagged in sub-array 1. ! A total of 126 telescope corrections were flagged in sub-array 2. ! A total of 4020 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=0.677769Jy sigma=0.006318 ! Fit after self-cal, rms=0.236932Jy sigma=0.001849 ! 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 7.53% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 milli-arcsec ! Estimated beam: bmin=0.4855 mas, bmaj=0.9494 mas, bpa=-5.138 degrees ! Estimated noise=807.936 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 = 0.763205 Jy ! Component: 100 - total flux cleaned = 0.940732 Jy ! Total flux subtracted in 100 components = 0.940732 Jy ! Clean residual min=-0.019088 max=0.066110 Jy/beam ! Clean residual mean=0.000085 rms=0.005734 Jy/beam ! Combined flux in latest and established models = 0.940732 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 8 components and 0.940732 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.227815Jy sigma=0.001950 ! Fit after self-cal, rms=0.227833Jy sigma=0.001950 ! Inverting map ! Your choice of large map pixels excluded 7.53% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0701374 Jy ! Component: 100 - total flux cleaned = 0.109366 Jy ! Total flux subtracted in 100 components = 0.109366 Jy ! Clean residual min=-0.014629 max=0.024184 Jy/beam ! Clean residual mean=0.000034 rms=0.003962 Jy/beam ! Combined flux in latest and established models = 1.0501 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 16 components and 1.0501 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.203041Jy sigma=0.001573 ! Fit after self-cal, rms=0.203105Jy sigma=0.001573 ! Inverting map ! Your choice of large map pixels excluded 7.53% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 milli-arcsec ! Added new window around map position (0.4, -2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0254732 Jy ! Component: 100 - total flux cleaned = 0.0405047 Jy ! Total flux subtracted in 100 components = 0.0405047 Jy ! Clean residual min=-0.014367 max=0.018416 Jy/beam ! Clean residual mean=0.000015 rms=0.003617 Jy/beam ! Combined flux in latest and established models = 1.0906 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 20 components and 1.0906 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.199850Jy sigma=0.001511 ! Fit after self-cal, rms=0.199797Jy sigma=0.001510 ! Inverting map ! Your choice of large map pixels excluded 7.53% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 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 7.53% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 milli-arcsec ! Estimated beam: bmin=0.5757 mas, bmaj=1.067 mas, bpa=-4.177 degrees ! Estimated noise=492.137 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 = 0.0229836 Jy ! Component: 100 - total flux cleaned = 0.0266155 Jy ! Component: 150 - total flux cleaned = 0.0284969 Jy ! Component: 200 - total flux cleaned = 0.0293234 Jy ! Total flux subtracted in 200 components = 0.0293234 Jy ! Clean residual min=-0.009562 max=0.012911 Jy/beam ! Clean residual mean=0.000160 rms=0.002525 Jy/beam ! Combined flux in latest and established models = 1.11993 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 27 components and 1.11993 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.197757Jy sigma=0.001471 ! Fit after self-cal, rms=0.197732Jy sigma=0.001470 ! Inverting map ! Your choice of large map pixels excluded 7.53% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 108 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.92 FD 0.97 FT 1.00* HH 1.00* ! HN 0.96 KK 1.09 KP 0.99 MC 1.00* ! MK 0.99 NL 0.99 NY 1.00* OV 0.96 ! PT 0.97 SC 1.00* SH 1.00* TS 1.00* ! WF 1.00 WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.94 FD 1.02 FT 1.00* HH 1.00* ! HN 1.00* KK 0.93 KP 1.01 MC 1.00* ! MK 1.00 NL 1.31 NY 1.00* OV 0.97 ! PT 1.01 SC 1.00* SH 1.00* TS 1.13 ! WF 1.00* WZ 1.00* ! ! A total of 93 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 FD 1.01 FT 1.00* HH 1.03 ! HN 0.97 KK 1.00* KP 1.01 MC 1.03 ! MK 1.00* NL 0.99 NY 1.07 OV 0.98 ! PT 1.01 SC 0.95 SH 0.94 TS 1.13 ! WF 0.99 WZ 0.97 ! ! ! Correcting IF 2. ! A total of 108 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.95 FT 1.00* HH 1.00* ! HN 0.99 KK 1.06 KP 0.97 MC 1.00* ! MK 0.97 NL 1.03 NY 1.00* OV 0.98 ! PT 0.97 SC 1.00* SH 1.00* TS 1.00* ! WF 0.99 WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 1.00 FT 1.00* HH 1.00* ! HN 1.00* KK 0.93 KP 0.98 MC 1.00* ! MK 0.98 NL 1.41 NY 1.00* OV 1.01 ! PT 1.01 SC 1.00* SH 1.00* TS 1.15 ! WF 1.00* WZ 1.00* ! ! A total of 93 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 FD 0.98 FT 1.00* HH 1.04 ! HN 0.97 KK 1.00* KP 0.99 MC 1.03 ! MK 1.00* NL 1.03 NY 1.03 OV 1.00 ! PT 1.03 SC 0.98 SH 0.95 TS 1.17 ! WF 0.99 WZ 0.97 ! ! ! Correcting IF 3. ! A total of 108 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.94 FD 0.98 FT 1.00* HH 1.00* ! HN 0.97 KK 1.12 KP 0.98 MC 1.00* ! MK 0.95 NL 0.97 NY 1.00* OV 0.97 ! PT 0.96 SC 1.00* SH 1.00* TS 1.00* ! WF 1.06 WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 FD 1.03 FT 1.00* HH 1.00* ! HN 1.00* KK 0.99 KP 1.02 MC 1.00* ! MK 0.97 NL 1.29 NY 1.00* OV 0.97 ! PT 0.98 SC 1.00* SH 1.00* TS 1.16 ! WF 1.00* WZ 1.00* ! ! A total of 93 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 FD 1.02 FT 1.00* HH 1.07 ! HN 0.97 KK 1.00* KP 1.00 MC 1.03 ! MK 1.00* NL 0.99 NY 1.04 OV 0.99 ! PT 1.00 SC 0.97 SH 0.97 TS 1.18 ! WF 1.05 WZ 0.96 ! ! ! Correcting IF 4. ! A total of 108 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.99 FT 1.00* HH 1.00* ! HN 0.97 KK 1.07 KP 0.94 MC 1.00* ! MK 1.01 NL 1.00 NY 1.00* OV 1.00 ! PT 0.98 SC 1.00* SH 1.00* TS 1.00* ! WF 1.03 WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 FD 1.03 FT 1.00* HH 1.00* ! HN 1.00* KK 1.02 KP 0.96 MC 1.00* ! MK 1.04 NL 1.34 NY 1.00* OV 1.03 ! PT 1.00 SC 1.00* SH 1.00* TS 1.16 ! WF 1.00* WZ 1.00* ! ! A total of 93 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 1.03 FT 1.00* HH 1.02 ! HN 0.99 KK 1.00* KP 0.97 MC 1.03 ! MK 1.00* NL 1.01 NY 1.04 OV 1.04 ! PT 1.01 SC 0.99 SH 0.96 TS 1.12 ! WF 1.02 WZ 1.03 ! ! ! Fit before self-cal, rms=0.197732Jy sigma=0.001470 ! Fit after self-cal, rms=0.195027Jy sigma=0.001373 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 milli-arcsec ! Estimated beam: bmin=0.5845 mas, bmaj=1.086 mas, bpa=-3.975 degrees ! Estimated noise=495.803 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 = -0.00647914 Jy ! Component: 100 - total flux cleaned = -0.00681379 Jy ! Component: 150 - total flux cleaned = -0.00710631 Jy ! Component: 200 - total flux cleaned = -0.00759551 Jy ! Total flux subtracted in 200 components = -0.00759551 Jy ! Clean residual min=-0.005780 max=0.005311 Jy/beam ! Clean residual mean=0.000113 rms=0.001305 Jy/beam ! Combined flux in latest and established models = 1.11233 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 36 components and 1.11233 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.194593Jy sigma=0.001370 ! Fit after self-cal, rms=0.194670Jy sigma=0.001370 ! Inverting map ! Your choice of large map pixels excluded 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 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=0.194670Jy sigma=0.001370 ! Fit after self-cal, rms=0.193111Jy sigma=0.001350 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 milli-arcsec ! Estimated beam: bmin=0.5855 mas, bmaj=1.086 mas, bpa=-4.319 degrees ! Estimated noise=495.328 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00527126 Jy ! Component: 100 - total flux cleaned = -0.00564718 Jy ! Component: 150 - total flux cleaned = -0.00593791 Jy ! Component: 200 - total flux cleaned = -0.00618146 Jy ! Total flux subtracted in 200 components = -0.00618146 Jy ! Clean residual min=-0.003943 max=0.004179 Jy/beam ! Clean residual mean=0.000110 rms=0.000971 Jy/beam ! Combined flux in latest and established models = 1.10615 Jy selfcal ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 40 components and 1.10615 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.192912Jy sigma=0.001348 ! Fit after self-cal, rms=0.192908Jy sigma=0.001348 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 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 (21.8, -10.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00364985 Jy ! Component: 100 - total flux cleaned = 0.00469983 Jy ! Component: 150 - total flux cleaned = 0.00477164 Jy ! Component: 200 - total flux cleaned = 0.00476776 Jy ! Total flux subtracted in 200 components = 0.00476776 Jy ! Clean residual min=-0.003952 max=0.003599 Jy/beam ! Clean residual mean=0.000086 rms=0.000931 Jy/beam ! Combined flux in latest and established models = 1.11092 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 54 components and 1.11092 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.192815Jy sigma=0.001348 ! Fit after self-cal, rms=0.192810Jy sigma=0.001348 ! Inverting map ! Your choice of large map pixels excluded 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 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=0.192810Jy sigma=0.001348 ! Fit after self-cal, rms=0.192563Jy sigma=0.001339 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 milli-arcsec ! Estimated beam: bmin=0.5866 mas, bmaj=1.088 mas, bpa=-4.289 degrees ! Estimated noise=495.351 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00279538 Jy ! Component: 100 - total flux cleaned = -0.0032387 Jy ! Component: 150 - total flux cleaned = -0.00339271 Jy ! Component: 200 - total flux cleaned = -0.00332828 Jy ! Total flux subtracted in 200 components = -0.00332828 Jy ! Clean residual min=-0.003428 max=0.003287 Jy/beam ! Clean residual mean=0.000100 rms=0.000790 Jy/beam ! Combined flux in latest and established models = 1.10759 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 56 components and 1.10759 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.192489Jy sigma=0.001339 ! Fit after self-cal, rms=0.192493Jy sigma=0.001339 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 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 = 6.97597e-05 Jy ! Component: 100 - total flux cleaned = 6.78358e-05 Jy ! Component: 150 - total flux cleaned = 0.000123116 Jy ! Component: 200 - total flux cleaned = 0.000222054 Jy ! Total flux subtracted in 200 components = 0.000222054 Jy ! Clean residual min=-0.003394 max=0.003274 Jy/beam ! Clean residual mean=0.000099 rms=0.000781 Jy/beam ! Combined flux in latest and established models = 1.10781 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 57 components and 1.10781 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.192467Jy sigma=0.001339 ! Fit after self-cal, rms=0.192462Jy sigma=0.001339 ! Inverting map ! Your choice of large map pixels excluded 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 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=0.192462Jy sigma=0.001339 ! Fit after self-cal, rms=0.192817Jy sigma=0.001338 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 milli-arcsec ! Estimated beam: bmin=2.068 mas, bmaj=3.203 mas, bpa=-12.45 degrees ! Estimated noise=681.002 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000354046 Jy ! Component: 100 - total flux cleaned = 0.000129245 Jy ! Component: 150 - total flux cleaned = 0.000515655 Jy ! Component: 200 - total flux cleaned = 0.000783288 Jy ! Total flux subtracted in 200 components = 0.000783288 Jy ! Clean residual min=-0.002994 max=0.004421 Jy/beam ! Clean residual mean=0.000272 rms=0.001100 Jy/beam ! Combined flux in latest and established models = 1.10859 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 62 components and 1.10859 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.192801Jy sigma=0.001338 ! Fit after self-cal, rms=0.192787Jy sigma=0.001338 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 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 = 5.21232e-05 Jy ! Component: 100 - total flux cleaned = 9.74433e-05 Jy ! Component: 150 - total flux cleaned = 0.000223578 Jy ! Component: 200 - total flux cleaned = 0.00038773 Jy ! Total flux subtracted in 200 components = 0.00038773 Jy ! Clean residual min=-0.003034 max=0.004377 Jy/beam ! Clean residual mean=0.000265 rms=0.001100 Jy/beam ! Combined flux in latest and established models = 1.10898 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 66 components and 1.10898 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.192791Jy sigma=0.001338 ! Fit after self-cal, rms=0.192787Jy sigma=0.001338 ! Inverting map ! Your choice of large map pixels excluded 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 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 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 milli-arcsec ! Estimated beam: bmin=0.5872 mas, bmaj=1.09 mas, bpa=-4.336 degrees ! Estimated noise=495.448 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5872 x 1.09 at -4.336 degrees (North through East) ! Clean map min=-0.0031791 max=0.99549 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=0.192787Jy sigma=0.001338 ! Fit after self-cal, rms=0.179931Jy sigma=0.001221 ! Inverting map and beam ! Your choice of large map pixels excluded 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 milli-arcsec ! Estimated beam: bmin=0.587 mas, bmaj=1.09 mas, bpa=-4.37 degrees ! Estimated noise=494.38 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00172462 Jy ! Component: 100 - total flux cleaned = -0.00214842 Jy ! Component: 150 - total flux cleaned = -0.00258438 Jy ! Component: 200 - total flux cleaned = -0.00291581 Jy ! Total flux subtracted in 200 components = -0.00291581 Jy ! Clean residual min=-0.003147 max=0.002811 Jy/beam ! Clean residual mean=0.000073 rms=0.000685 Jy/beam ! Combined flux in latest and established models = 1.10607 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 69 components and 1.10607 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.179891Jy sigma=0.001221 ! Fit after self-cal, rms=0.179885Jy sigma=0.001221 ! Inverting map ! Your choice of large map pixels excluded 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000281801 Jy ! Component: 100 - total flux cleaned = -0.000479968 Jy ! Component: 150 - total flux cleaned = -0.0006602 Jy ! Component: 200 - total flux cleaned = -0.000745278 Jy ! Total flux subtracted in 200 components = -0.000745278 Jy ! Clean residual min=-0.003016 max=0.002847 Jy/beam ! Clean residual mean=0.000077 rms=0.000676 Jy/beam ! Combined flux in latest and established models = 1.10532 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 70 components and 1.10532 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.179865Jy sigma=0.001221 ! Fit after self-cal, rms=0.179861Jy sigma=0.001221 ! Inverting map ! Your choice of large map pixels excluded 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.179861Jy sigma=0.001221 ! Fit after self-cal, rms=0.180137Jy sigma=0.001221 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 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 milli-arcsec ! Estimated beam: bmin=0.4935 mas, bmaj=0.9516 mas, bpa=-5.649 degrees ! Estimated noise=838.444 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.779639 Jy ! Component: 100 - total flux cleaned = 0.957259 Jy ! Component: 150 - total flux cleaned = 1.0177 Jy ! Component: 200 - total flux cleaned = 1.04755 Jy ! Total flux subtracted in 200 components = 1.04755 Jy ! Clean residual min=-0.006043 max=0.015985 Jy/beam ! Clean residual mean=0.000034 rms=0.001606 Jy/beam ! Combined flux in latest and established models = 1.04755 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 17 model components to the UV plane model. ! The established model now contains 17 components and 1.04755 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 milli-arcsec ! Estimated beam: bmin=0.5873 mas, bmaj=1.092 mas, bpa=-4.42 degrees ! Estimated noise=494.43 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 = 0.0227431 Jy ! Component: 100 - total flux cleaned = 0.0348497 Jy ! Component: 150 - total flux cleaned = 0.0419308 Jy ! Component: 200 - total flux cleaned = 0.0463234 Jy ! Total flux subtracted in 200 components = 0.0463234 Jy ! Clean residual min=-0.002953 max=0.004257 Jy/beam ! Clean residual mean=0.000138 rms=0.000755 Jy/beam ! Combined flux in latest and established models = 1.09388 Jy ! Adding 20 model components to the UV plane model. ! The established model now contains 28 components and 1.09388 Jy ! Inverting map ! Your choice of large map pixels excluded 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 milli-arcsec ! Added new window around map position (0.2, -4.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00406462 Jy ! Component: 100 - total flux cleaned = 0.00598051 Jy ! Component: 150 - total flux cleaned = 0.0076359 Jy ! Component: 200 - total flux cleaned = 0.00872608 Jy ! Total flux subtracted in 200 components = 0.00872608 Jy ! Clean residual min=-0.002894 max=0.003172 Jy/beam ! Clean residual mean=0.000076 rms=0.000677 Jy/beam ! Combined flux in latest and established models = 1.1026 Jy ! Adding 22 model components to the UV plane model. ! The established model now contains 41 components and 1.1026 Jy ! Inverting map ! Your choice of large map pixels excluded 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 milli-arcsec ! Added new window around map position (-1, 10.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00240771 Jy ! Component: 100 - total flux cleaned = 0.00286964 Jy ! Component: 150 - total flux cleaned = 0.00343961 Jy ! Component: 200 - total flux cleaned = 0.00383596 Jy ! Total flux subtracted in 200 components = 0.00383596 Jy ! Clean residual min=-0.002696 max=0.002541 Jy/beam ! Clean residual mean=0.000050 rms=0.000643 Jy/beam ! Combined flux in latest and established models = 1.10644 Jy ! Adding 27 model components to the UV plane model. ! The established model now contains 54 components and 1.10644 Jy ! Inverting map ! Your choice of large map pixels excluded 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 milli-arcsec uvw 0,2 ! Uniform weighting is not currently selected. ! Amplitude error weighting is not currently selected. ! Radial weighting is not currently selected. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 milli-arcsec ! Estimated beam: bmin=0.5544 mas, bmaj=0.931 mas, bpa=-0.4688 degrees ! Estimated noise=618.239 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000477397 Jy ! Component: 100 - total flux cleaned = 0.00115259 Jy ! Component: 150 - total flux cleaned = 0.00138539 Jy ! Component: 200 - total flux cleaned = 0.00145826 Jy ! Total flux subtracted in 200 components = 0.00145826 Jy ! Clean residual min=-0.003272 max=0.003616 Jy/beam ! Clean residual mean=0.000054 rms=0.000805 Jy/beam ! Combined flux in latest and established models = 1.1079 Jy clean ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 7.04535e-05 Jy ! Component: 100 - total flux cleaned = 0.000202387 Jy ! Component: 150 - total flux cleaned = 0.000266025 Jy ! Component: 200 - total flux cleaned = 0.000386599 Jy ! Total flux subtracted in 200 components = 0.000386599 Jy ! Clean residual min=-0.003163 max=0.003564 Jy/beam ! Clean residual mean=0.000050 rms=0.000787 Jy/beam ! Combined flux in latest and established models = 1.10828 Jy selfcal ! Performing phase self-cal ! Adding 37 model components to the UV plane model. ! The established model now contains 68 components and 1.10828 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.180247Jy sigma=0.001222 ! Fit after self-cal, rms=0.180202Jy sigma=0.001221 wmodel J0811+0146_X_2011_06_28_pus_map.mod ! Writing 68 model components to file: J0811+0146_X_2011_06_28_pus_map.mod wobs J0811+0146_X_2011_06_28_pus_uvs.fits ! Writing UV FITS file: J0811+0146_X_2011_06_28_pus_uvs.fits wwins J0811+0146_X_2011_06_28_pus_map.win ! wwins: Wrote 5 windows to J0811+0146_X_2011_06_28_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 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.00015378 Jy ! Component: 100 - total flux cleaned = 9.73284e-05 Jy ! Component: 150 - total flux cleaned = 0.000151259 Jy ! Component: 200 - total flux cleaned = 0.000514817 Jy ! Component: 250 - total flux cleaned = 0.000765992 Jy ! Component: 300 - total flux cleaned = 0.000912598 Jy ! Component: 350 - total flux cleaned = 0.00100805 Jy ! Component: 400 - total flux cleaned = 0.00105379 Jy ! Component: 450 - total flux cleaned = 0.000915846 Jy ! Component: 500 - total flux cleaned = 0.00091594 Jy ! Component: 550 - total flux cleaned = 0.000915568 Jy ! Component: 600 - total flux cleaned = 0.000785332 Jy ! Component: 650 - total flux cleaned = 0.000871629 Jy ! Component: 700 - total flux cleaned = 0.000870537 Jy ! Component: 750 - total flux cleaned = 0.000787228 Jy ! Component: 800 - total flux cleaned = 0.000788165 Jy ! Component: 850 - total flux cleaned = 0.000868921 Jy ! Component: 900 - total flux cleaned = 0.000949211 Jy ! Component: 950 - total flux cleaned = 0.000988594 Jy ! Component: 1000 - total flux cleaned = 0.00102758 Jy ! Component: 1050 - total flux cleaned = 0.00114306 Jy ! Component: 1100 - total flux cleaned = 0.00118092 Jy ! Component: 1150 - total flux cleaned = 0.00121885 Jy ! Component: 1200 - total flux cleaned = 0.00121919 Jy ! Component: 1250 - total flux cleaned = 0.00136734 Jy ! Component: 1300 - total flux cleaned = 0.00147725 Jy ! Component: 1350 - total flux cleaned = 0.00151349 Jy ! Component: 1400 - total flux cleaned = 0.00165754 Jy ! Component: 1450 - total flux cleaned = 0.00162215 Jy ! Component: 1500 - total flux cleaned = 0.00176355 Jy ! Component: 1550 - total flux cleaned = 0.00186819 Jy ! Component: 1600 - total flux cleaned = 0.00186786 Jy ! Component: 1650 - total flux cleaned = 0.00193641 Jy ! Component: 1700 - total flux cleaned = 0.00203835 Jy ! Component: 1750 - total flux cleaned = 0.00197071 Jy ! Component: 1800 - total flux cleaned = 0.00207144 Jy ! Component: 1850 - total flux cleaned = 0.00210474 Jy ! Component: 1900 - total flux cleaned = 0.00220384 Jy ! Component: 1950 - total flux cleaned = 0.00226915 Jy ! Component: 2000 - total flux cleaned = 0.00230149 Jy ! Total flux subtracted in 2048 components = 0.00233364 Jy ! Clean residual min=-0.001884 max=0.001797 Jy/beam ! Clean residual mean=0.000027 rms=0.000570 Jy/beam ! Combined flux in latest and established models = 1.11062 Jy keep ! Adding 175 model components to the UV plane model. ! The established model now contains 243 components and 1.11062 Jy ![Exited script file: muppet] wmap "J0811+0146_X_2011_06_28_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5544 x 0.931 at -0.4688 degrees (North through East) ! Clean map min=-0.0023571 max=0.9839 Jy/beam ! Writing clean map to FITS file: J0811+0146_X_2011_06_28_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.983901 invert ! Inverting map ! Your choice of large map pixels excluded 7.5% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! The y-axis pixel size should ideally be below 0.1874 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000569238 device "J0811+0146_X_2011_06_28_pus\_map.eps/VPS" ! Attempting to open device: 'J0811+0146_X_2011_06_28_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.173565 0.173565 0.347131 0.694262 1.38852 2.77705 5.55409 11.1082 22.2164 44.4328 88.8655 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0017 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.983 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5544 x 0.931 at -0.4688 degrees (North through East) ! Clean map min=-0.0023571 max=0.9839 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0811+0146_X_2011_06_28_pus\_map.gif/vgif" ! Attempting to open device: 'J0811+0146_X_2011_06_28_pus_map.gif/vgif' mapplot cln