! Started logfile: J2002+4725_X_2010_10_13_pus_uvs.log on Mon Feb 28 17:18:49 2011 obs J2002+4725_X_2010_10_13_pus_uva.fits ! Reading UV FITS file: J2002+4725_X_2010_10_13_pus_uva.fits ! AN table 1: 27 integrations on 105 of 105 possible baselines. ! AN table 2: 90 integrations on 105 of 105 possible baselines. ! AN table 3: 56 integrations on 105 of 105 possible baselines. ! Apparent sampling: 0.157666 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J2002+4725 ! ! 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 8.40996e+09 8e+06 1 8e+06 ! 02 2 8.47996e+09 8e+06 1 8e+06 ! 03 3 8.79496e+09 8e+06 1 8e+06 ! 04 4 8.89996e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 5978 lines of history. ! ! Reading 11456 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 = 256 print "field_cell =",field_cell ! field_cell = 0.2 print "taper_size =",taper_size ! taper_size = 70 ![@muppet J2002+4725_X_2010_10_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 = 256x256 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 302 telescope corrections were flagged in sub-array 1. ! A total of 879 telescope corrections were flagged in sub-array 2. ! A total of 577 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 302 telescope corrections were flagged in sub-array 1. ! A total of 879 telescope corrections were flagged in sub-array 2. ! A total of 577 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 302 telescope corrections were flagged in sub-array 1. ! A total of 879 telescope corrections were flagged in sub-array 2. ! A total of 577 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 302 telescope corrections were flagged in sub-array 1. ! A total of 879 telescope corrections were flagged in sub-array 2. ! A total of 577 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=0.417985Jy sigma=0.005059 ! Fit after self-cal, rms=0.372736Jy sigma=0.004506 ! 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 1.25% of the data. ! The x-axis pixel size should ideally be below 0.1841 milli-arcsec ! Estimated beam: bmin=0.629 mas, bmaj=0.8967 mas, bpa=-2.441 degrees ! Estimated noise=998.236 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) ! Added new window around map position (0, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.519042 Jy ! Component: 100 - total flux cleaned = 0.699845 Jy ! Total flux subtracted in 100 components = 0.699845 Jy ! Clean residual min=-0.020079 max=0.081616 Jy/beam ! Clean residual mean=0.000854 rms=0.006679 Jy/beam ! Combined flux in latest and established models = 0.699845 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.699845 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.214073Jy sigma=0.002506 ! Fit after self-cal, rms=0.213453Jy sigma=0.002501 ! Inverting map ! Your choice of large map pixels excluded 1.25% of the data. ! The x-axis pixel size should ideally be below 0.1841 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0888936 Jy ! Component: 100 - total flux cleaned = 0.134572 Jy ! Total flux subtracted in 100 components = 0.134572 Jy ! Clean residual min=-0.009677 max=0.022905 Jy/beam ! Clean residual mean=0.000354 rms=0.002902 Jy/beam ! Combined flux in latest and established models = 0.834417 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 14 components and 0.834417 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.160238Jy sigma=0.001633 ! Fit after self-cal, rms=0.160071Jy sigma=0.001631 ! Inverting map ! Your choice of large map pixels excluded 1.25% of the data. ! The x-axis pixel size should ideally be below 0.1841 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0277012 Jy ! Component: 100 - total flux cleaned = 0.0448616 Jy ! Total flux subtracted in 100 components = 0.0448616 Jy ! Clean residual min=-0.008008 max=0.010166 Jy/beam ! Clean residual mean=0.000189 rms=0.002128 Jy/beam ! Combined flux in latest and established models = 0.879279 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 22 components and 0.879279 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.152842Jy sigma=0.001483 ! Fit after self-cal, rms=0.152806Jy sigma=0.001483 ! Inverting map ! Your choice of large map pixels excluded 1.25% of the data. ! The x-axis pixel size should ideally be below 0.1841 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 1.25% of the data. ! The x-axis pixel size should ideally be below 0.1841 milli-arcsec ! Estimated beam: bmin=0.7695 mas, bmaj=1.158 mas, bpa=-1.765 degrees ! Estimated noise=569.987 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 = 0.020825 Jy ! Component: 100 - total flux cleaned = 0.0309574 Jy ! Component: 150 - total flux cleaned = 0.0362133 Jy ! Component: 200 - total flux cleaned = 0.0390333 Jy ! Total flux subtracted in 200 components = 0.0390333 Jy ! Clean residual min=-0.005584 max=0.007254 Jy/beam ! Clean residual mean=0.000328 rms=0.001665 Jy/beam ! Combined flux in latest and established models = 0.918312 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 34 components and 0.918312 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.151077Jy sigma=0.001433 ! Fit after self-cal, rms=0.151062Jy sigma=0.001433 ! Inverting map ! Your choice of large map pixels excluded 1.25% of the data. ! The x-axis pixel size should ideally be below 0.1841 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 27 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.86 HH 1.00* HN 1.00* ! KB 1.00* KK 1.00* KP 0.98 LA 0.98 ! MK 1.00* NL 0.96 NY 1.00* OV 1.00* ! PT 0.98 SC 0.99 TS 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.96 FD 0.84 HH 1.00* HN 1.04 ! KB 1.00* KK 1.07 KP 0.99 LA 0.98 ! MK 1.03 NL 0.99 NY 1.03 OV 0.97 ! PT 0.97 SC 0.98 TS 1.00* ! ! A total of 42 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 FD 0.85 HH 1.00* HN 1.00* ! KB 1.03 KK 0.95 KP 1.00 LA 1.01 ! MK 0.98 NL 0.98 NY 1.00* OV 0.99 ! PT 0.99 SC 1.00* TS 0.95 ! ! ! Correcting IF 2. ! A total of 27 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.97 HH 1.00* HN 1.00* ! KB 1.00* KK 1.00* KP 1.00 LA 0.97 ! MK 1.00* NL 0.99 NY 1.00* OV 1.00* ! PT 1.01 SC 0.99 TS 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 HH 1.00* HN 1.06 ! KB 1.00* KK 1.08 KP 0.98 LA 0.95 ! MK 0.98 NL 1.03 NY 1.04 OV 1.00 ! PT 1.00 SC 1.01 TS 1.00* ! ! A total of 42 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 1.00 HH 1.00* HN 1.00* ! KB 1.04 KK 0.99 KP 1.00 LA 0.98 ! MK 0.94 NL 1.02 NY 1.00* OV 1.00 ! PT 1.00 SC 1.00* TS 0.98 ! ! ! Correcting IF 3. ! A total of 27 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.01 HH 1.00* HN 1.00* ! KB 1.00* KK 1.00* KP 1.00 LA 0.95 ! MK 1.00* NL 0.97 NY 1.00* OV 1.00* ! PT 1.04 SC 0.98 TS 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 HH 1.00* HN 1.09 ! KB 1.00* KK 1.07 KP 1.00 LA 0.94 ! MK 1.06 NL 0.98 NY 1.09 OV 0.99 ! PT 1.03 SC 1.05 TS 1.00* ! ! A total of 42 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 1.01 HH 1.00* HN 1.00* ! KB 1.04 KK 0.95 KP 1.02 LA 0.97 ! MK 0.99 NL 0.99 NY 1.00* OV 0.99 ! PT 1.06 SC 1.00* TS 0.97 ! ! ! Correcting IF 4. ! A total of 27 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.01 HH 1.00* HN 1.00* ! KB 1.00* KK 1.00* KP 1.03 LA 1.03 ! MK 1.00* NL 0.98 NY 1.00* OV 1.00* ! PT 1.00 SC 1.00 TS 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.05 FD 1.00 HH 1.00* HN 1.07 ! KB 1.00* KK 1.07 KP 0.99 LA 1.01 ! MK 1.04 NL 1.02 NY 1.05 OV 1.04 ! PT 1.00 SC 1.05 TS 1.00* ! ! A total of 42 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.05 FD 1.04 HH 1.00* HN 1.00* ! KB 1.02 KK 0.99 KP 1.02 LA 1.04 ! MK 0.99 NL 1.02 NY 1.00* OV 1.03 ! PT 1.02 SC 1.00* TS 0.90 ! ! ! Fit before self-cal, rms=0.151062Jy sigma=0.001433 ! Fit after self-cal, rms=0.147639Jy sigma=0.001321 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 milli-arcsec ! Estimated beam: bmin=0.78 mas, bmaj=1.168 mas, bpa=-2.371 degrees ! Estimated noise=575.372 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 = -0.00418708 Jy ! Component: 100 - total flux cleaned = -0.00516826 Jy ! Component: 150 - total flux cleaned = -0.00547458 Jy ! Component: 200 - total flux cleaned = -0.00562573 Jy ! Total flux subtracted in 200 components = -0.00562573 Jy ! Clean residual min=-0.004763 max=0.003742 Jy/beam ! Clean residual mean=0.000003 rms=0.001081 Jy/beam ! Combined flux in latest and established models = 0.912686 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 35 components and 0.912686 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.147476Jy sigma=0.001320 ! Fit after self-cal, rms=0.147531Jy sigma=0.001320 ! Inverting map ! Your choice of large map pixels excluded 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 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=0.147531Jy sigma=0.001320 ! Fit after self-cal, rms=0.147069Jy sigma=0.001306 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 milli-arcsec ! Estimated beam: bmin=0.7788 mas, bmaj=1.169 mas, bpa=-2.333 degrees ! Estimated noise=574.971 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0010143 Jy ! Component: 100 - total flux cleaned = -0.00122053 Jy ! Component: 150 - total flux cleaned = -0.00132459 Jy ! Component: 200 - total flux cleaned = -0.00138733 Jy ! Total flux subtracted in 200 components = -0.00138733 Jy ! Clean residual min=-0.003553 max=0.002918 Jy/beam ! Clean residual mean=0.000044 rms=0.000845 Jy/beam ! Combined flux in latest and established models = 0.911299 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 36 components and 0.911299 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.147040Jy sigma=0.001306 ! Fit after self-cal, rms=0.147042Jy sigma=0.001306 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 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 = -0.000146926 Jy ! Component: 100 - total flux cleaned = -0.000174995 Jy ! Component: 150 - total flux cleaned = -0.000200191 Jy ! Component: 200 - total flux cleaned = -0.000246859 Jy ! Total flux subtracted in 200 components = -0.000246859 Jy ! Clean residual min=-0.003562 max=0.002905 Jy/beam ! Clean residual mean=0.000048 rms=0.000842 Jy/beam ! Combined flux in latest and established models = 0.911052 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 37 components and 0.911052 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.147029Jy sigma=0.001305 ! Fit after self-cal, rms=0.147027Jy sigma=0.001305 ! Inverting map ! Your choice of large map pixels excluded 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 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=0.147027Jy sigma=0.001305 ! Fit after self-cal, rms=0.146736Jy sigma=0.001299 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 milli-arcsec ! Estimated beam: bmin=0.7786 mas, bmaj=1.171 mas, bpa=-2.29 degrees ! Estimated noise=575.03 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000799927 Jy ! Component: 100 - total flux cleaned = -0.00093451 Jy ! Component: 150 - total flux cleaned = -0.000972286 Jy ! Component: 200 - total flux cleaned = -0.00103429 Jy ! Total flux subtracted in 200 components = -0.00103429 Jy ! Clean residual min=-0.002644 max=0.002712 Jy/beam ! Clean residual mean=0.000077 rms=0.000724 Jy/beam ! Combined flux in latest and established models = 0.910018 Jy selfcal ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 38 components and 0.910018 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.146711Jy sigma=0.001299 ! Fit after self-cal, rms=0.146712Jy sigma=0.001299 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 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 = 2.22198e-05 Jy ! Component: 100 - total flux cleaned = -4.88905e-05 Jy ! Component: 150 - total flux cleaned = -8.99977e-05 Jy ! Component: 200 - total flux cleaned = -0.000127853 Jy ! Total flux subtracted in 200 components = -0.000127853 Jy ! Clean residual min=-0.002640 max=0.002716 Jy/beam ! Clean residual mean=0.000079 rms=0.000721 Jy/beam ! Combined flux in latest and established models = 0.90989 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 38 components and 0.90989 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.146706Jy sigma=0.001299 ! Fit after self-cal, rms=0.146704Jy sigma=0.001299 ! Inverting map ! Your choice of large map pixels excluded 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 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=0.146704Jy sigma=0.001299 ! Fit after self-cal, rms=0.146834Jy sigma=0.001299 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 milli-arcsec ! Estimated beam: bmin=2.415 mas, bmaj=2.934 mas, bpa=36.65 degrees ! Estimated noise=734.716 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00102097 Jy ! Component: 100 - total flux cleaned = -0.00122565 Jy ! Component: 150 - total flux cleaned = -0.00122589 Jy ! Component: 200 - total flux cleaned = -0.00123207 Jy ! Total flux subtracted in 200 components = -0.00123207 Jy ! Clean residual min=-0.002281 max=0.002303 Jy/beam ! Clean residual mean=0.000189 rms=0.000720 Jy/beam ! Combined flux in latest and established models = 0.908658 Jy selfcal ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 38 components and 0.908658 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.146828Jy sigma=0.001299 ! Fit after self-cal, rms=0.146827Jy sigma=0.001299 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 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 = -4.72871e-05 Jy ! Component: 100 - total flux cleaned = -4.70755e-05 Jy ! Component: 150 - total flux cleaned = -4.72905e-05 Jy ! Component: 200 - total flux cleaned = -4.75847e-05 Jy ! Total flux subtracted in 200 components = -4.75847e-05 Jy ! Clean residual min=-0.002280 max=0.002291 Jy/beam ! Clean residual mean=0.000191 rms=0.000718 Jy/beam ! Combined flux in latest and established models = 0.90861 Jy ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 38 components and 0.90861 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.146824Jy sigma=0.001299 ! Fit after self-cal, rms=0.146823Jy sigma=0.001299 ! Inverting map ! Your choice of large map pixels excluded 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 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 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 milli-arcsec ! Estimated beam: bmin=0.7784 mas, bmaj=1.173 mas, bpa=-2.27 degrees ! Estimated noise=575.259 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7784 x 1.173 at -2.27 degrees (North through East) ! Clean map min=-0.00228 max=0.71852 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=0.146823Jy sigma=0.001299 ! Fit after self-cal, rms=0.139072Jy sigma=0.001187 ! Inverting map and beam ! Your choice of large map pixels excluded 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 milli-arcsec ! Estimated beam: bmin=0.7779 mas, bmaj=1.174 mas, bpa=-2.293 degrees ! Estimated noise=574.586 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00037067 Jy ! Component: 100 - total flux cleaned = -0.000507096 Jy ! Component: 150 - total flux cleaned = -0.000587832 Jy ! Component: 200 - total flux cleaned = -0.000634576 Jy ! Total flux subtracted in 200 components = -0.000634576 Jy ! Clean residual min=-0.002761 max=0.002611 Jy/beam ! Clean residual mean=0.000095 rms=0.000698 Jy/beam ! Combined flux in latest and established models = 0.907975 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 38 components and 0.907975 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.139059Jy sigma=0.001187 ! Fit after self-cal, rms=0.139057Jy sigma=0.001187 ! Inverting map ! Your choice of large map pixels excluded 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 2.15312e-05 Jy ! Component: 100 - total flux cleaned = -5.99088e-05 Jy ! Component: 150 - total flux cleaned = -9.59211e-05 Jy ! Component: 200 - total flux cleaned = -0.00014329 Jy ! Total flux subtracted in 200 components = -0.00014329 Jy ! Clean residual min=-0.002766 max=0.002610 Jy/beam ! Clean residual mean=0.000098 rms=0.000695 Jy/beam ! Combined flux in latest and established models = 0.907832 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 38 components and 0.907832 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.139053Jy sigma=0.001186 ! Fit after self-cal, rms=0.139051Jy sigma=0.001186 ! Inverting map ! Your choice of large map pixels excluded 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.139051Jy sigma=0.001186 ! Fit after self-cal, rms=0.139145Jy sigma=0.001186 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 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 milli-arcsec ! Estimated beam: bmin=0.6346 mas, bmaj=0.903 mas, bpa=-3.326 degrees ! Estimated noise=1029.98 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.530512 Jy ! Component: 100 - total flux cleaned = 0.712935 Jy ! Component: 150 - total flux cleaned = 0.799354 Jy ! Component: 200 - total flux cleaned = 0.842723 Jy ! Total flux subtracted in 200 components = 0.842723 Jy ! Clean residual min=-0.006262 max=0.020865 Jy/beam ! Clean residual mean=0.000258 rms=0.002289 Jy/beam ! Combined flux in latest and established models = 0.842724 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 11 model components to the UV plane model. ! The established model now contains 11 components and 0.842724 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 milli-arcsec ! Estimated beam: bmin=0.7774 mas, bmaj=1.175 mas, bpa=-2.3 degrees ! Estimated noise=574.625 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 = 0.0345474 Jy ! Component: 100 - total flux cleaned = 0.0503072 Jy ! Component: 150 - total flux cleaned = 0.0579006 Jy ! Component: 200 - total flux cleaned = 0.0616184 Jy ! Total flux subtracted in 200 components = 0.0616184 Jy ! Clean residual min=-0.002746 max=0.002686 Jy/beam ! Clean residual mean=0.000135 rms=0.000713 Jy/beam ! Combined flux in latest and established models = 0.904342 Jy ! Adding 22 model components to the UV plane model. ! The established model now contains 26 components and 0.904342 Jy ! Inverting map ! Your choice of large map pixels excluded 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 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 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 milli-arcsec ! Estimated beam: bmin=2.415 mas, bmaj=2.936 mas, bpa=36.58 degrees ! Estimated noise=733.567 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00174687 Jy ! Component: 100 - total flux cleaned = 0.00222611 Jy ! Component: 150 - total flux cleaned = 0.00234979 Jy ! Component: 200 - total flux cleaned = 0.00235442 Jy ! Total flux subtracted in 200 components = 0.00235442 Jy ! Clean residual min=-0.002202 max=0.002358 Jy/beam ! Clean residual mean=0.000227 rms=0.000700 Jy/beam ! Combined flux in latest and established models = 0.906696 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 = 4.23683e-06 Jy ! Component: 100 - total flux cleaned = 8.18552e-06 Jy ! Component: 150 - total flux cleaned = 1.18115e-05 Jy ! Component: 200 - total flux cleaned = 1.46516e-05 Jy ! Total flux subtracted in 200 components = 1.46516e-05 Jy ! Clean residual min=-0.002198 max=0.002356 Jy/beam ! Clean residual mean=0.000227 rms=0.000700 Jy/beam ! Combined flux in latest and established models = 0.906711 Jy ! Adding 11 model components to the UV plane model. ! The established model now contains 33 components and 0.906711 Jy ! Inverting map ! Your choice of large map pixels excluded 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 milli-arcsec ! Estimated beam: bmin=0.7774 mas, bmaj=1.175 mas, bpa=-2.3 degrees ! Estimated noise=574.625 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000411025 Jy ! Component: 100 - total flux cleaned = -0.000251136 Jy ! Component: 150 - total flux cleaned = -6.69104e-05 Jy ! Component: 200 - total flux cleaned = 0.000131791 Jy ! Total flux subtracted in 200 components = 0.000131791 Jy ! Clean residual min=-0.002746 max=0.002506 Jy/beam ! Clean residual mean=0.000091 rms=0.000694 Jy/beam ! Combined flux in latest and established models = 0.906843 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 37 components and 0.906843 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.139137Jy sigma=0.001186 ! Fit after self-cal, rms=0.139126Jy sigma=0.001186 wmodel J2002+4725_X_2010_10_13_pus_map.mod ! Writing 37 model components to file: J2002+4725_X_2010_10_13_pus_map.mod wobs J2002+4725_X_2010_10_13_pus_uvs.fits ! Writing UV FITS file: J2002+4725_X_2010_10_13_pus_uvs.fits wwins J2002+4725_X_2010_10_13_pus_map.win ! wwins: Wrote 1 windows to J2002+4725_X_2010_10_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 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 milli-arcsec ! clean: niter=1024 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -7.1203e-05 Jy ! Component: 100 - total flux cleaned = 0.000188156 Jy ! Component: 150 - total flux cleaned = 0.000435512 Jy ! Component: 200 - total flux cleaned = 0.000554111 Jy ! Component: 250 - total flux cleaned = 0.000553505 Jy ! Component: 300 - total flux cleaned = 0.000590372 Jy ! Component: 350 - total flux cleaned = 0.000663196 Jy ! Component: 400 - total flux cleaned = 0.000698933 Jy ! Component: 450 - total flux cleaned = 0.000769494 Jy ! Component: 500 - total flux cleaned = 0.000769418 Jy ! Component: 550 - total flux cleaned = 0.000769177 Jy ! Component: 600 - total flux cleaned = 0.000735747 Jy ! Component: 650 - total flux cleaned = 0.000736154 Jy ! Component: 700 - total flux cleaned = 0.000801243 Jy ! Component: 750 - total flux cleaned = 0.00080121 Jy ! Component: 800 - total flux cleaned = 0.000896397 Jy ! Component: 850 - total flux cleaned = 0.00092763 Jy ! Component: 900 - total flux cleaned = 0.000989753 Jy ! Component: 950 - total flux cleaned = 0.00105096 Jy ! Component: 1000 - total flux cleaned = 0.0011117 Jy ! Total flux subtracted in 1024 components = 0.0011118 Jy ! Clean residual min=-0.001545 max=0.001771 Jy/beam ! Clean residual mean=0.000066 rms=0.000579 Jy/beam ! Combined flux in latest and established models = 0.907955 Jy keep ! Adding 73 model components to the UV plane model. ! The established model now contains 110 components and 0.907955 Jy ![Exited script file: muppet] wmap "J2002+4725_X_2010_10_13_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7774 x 1.175 at -2.3 degrees (North through East) ! Clean map min=-0.0021623 max=0.71917 Jy/beam ! Writing clean map to FITS file: J2002+4725_X_2010_10_13_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.719168 invert ! Inverting map ! Your choice of large map pixels excluded 0.845% of the data. ! The x-axis pixel size should ideally be below 0.1916 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000579303 device "J2002+4725_X_2010_10_13_pus\_map.eps/VPS" ! Attempting to open device: 'J2002+4725_X_2010_10_13_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.241655 0.241655 0.483311 0.966621 1.93324 3.86648 7.73297 15.4659 30.9319 61.8638 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0017 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.719 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7774 x 1.175 at -2.3 degrees (North through East) ! Clean map min=-0.0021623 max=0.71917 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J2002+4725_X_2010_10_13_pus\_map.gif/vgif" ! Attempting to open device: 'J2002+4725_X_2010_10_13_pus_map.gif/vgif' mapplot cln