! Started logfile: J1152-0841_X_2010_10_13_pus_uvs.log on Mon Feb 28 17:17:01 2011 obs J1152-0841_X_2010_10_13_pus_uva.fits ! Reading UV FITS file: J1152-0841_X_2010_10_13_pus_uva.fits ! AN table 1: 34 integrations on 105 of 105 possible baselines. ! AN table 2: 155 integrations on 105 of 105 possible baselines. ! AN table 3: 15 integrations on 105 of 105 possible baselines. ! Apparent sampling: 0.140523 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1152-0841 ! ! 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 12040 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 J1152-0841_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 432 telescope corrections were flagged in sub-array 1. ! A total of 1554 telescope corrections were flagged in sub-array 2. ! A total of 111 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 432 telescope corrections were flagged in sub-array 1. ! A total of 1554 telescope corrections were flagged in sub-array 2. ! A total of 111 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 432 telescope corrections were flagged in sub-array 1. ! A total of 1554 telescope corrections were flagged in sub-array 2. ! A total of 111 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 432 telescope corrections were flagged in sub-array 1. ! A total of 1554 telescope corrections were flagged in sub-array 2. ! A total of 111 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=0.450994Jy sigma=0.004652 ! Fit after self-cal, rms=0.421419Jy sigma=0.004384 ! 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 9.83% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! Estimated beam: bmin=0.5641 mas, bmaj=1.282 mas, bpa=19.45 degrees ! Estimated noise=1075.67 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 = 0.927398 Jy ! Component: 100 - total flux cleaned = 1.1692 Jy ! Total flux subtracted in 100 components = 1.1692 Jy ! Clean residual min=-0.042024 max=0.090825 Jy/beam ! Clean residual mean=0.000657 rms=0.014225 Jy/beam ! Combined flux in latest and established models = 1.1692 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 1.1692 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.329094Jy sigma=0.003332 ! Fit after self-cal, rms=0.329121Jy sigma=0.003331 ! Inverting map ! Your choice of large map pixels excluded 9.83% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0910187 Jy ! Component: 100 - total flux cleaned = 0.138014 Jy ! Total flux subtracted in 100 components = 0.138014 Jy ! Clean residual min=-0.036338 max=0.046014 Jy/beam ! Clean residual mean=0.000144 rms=0.012268 Jy/beam ! Combined flux in latest and established models = 1.30722 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 20 components and 1.30722 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.302860Jy sigma=0.002928 ! Fit after self-cal, rms=0.302599Jy sigma=0.002926 ! Inverting map ! Your choice of large map pixels excluded 9.83% of the data. ! The x-axis pixel size should ideally be below 0.1611 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 9.83% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! Estimated beam: bmin=0.8194 mas, bmaj=1.71 mas, bpa=14.12 degrees ! Estimated noise=681.388 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 = 0.0381646 Jy ! Component: 100 - total flux cleaned = 0.0574703 Jy ! Component: 150 - total flux cleaned = 0.0609072 Jy ! Component: 200 - total flux cleaned = 0.0621635 Jy ! Total flux subtracted in 200 components = 0.0621635 Jy ! Clean residual min=-0.042395 max=0.047192 Jy/beam ! Clean residual mean=-0.000257 rms=0.015511 Jy/beam ! Combined flux in latest and established models = 1.36938 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 25 components and 1.36938 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.299019Jy sigma=0.002853 ! Fit after self-cal, rms=0.299005Jy sigma=0.002853 ! Inverting map ! Your choice of large map pixels excluded 9.83% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 33 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* HH 1.00* HN 1.00* ! KB 1.10 KK 0.90 KP 1.00* LA 1.00* ! MK 1.00 NL 1.00* NY 1.00* OV 0.97 ! PT 1.00* SC 1.00* TS 1.01 ! ! A total of 129 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.91 FD 0.85 HH 1.09 HN 1.00 ! KB 1.00* KK 0.93 KP 0.95 LA 0.99 ! MK 0.96 NL 1.11 NY 1.00* OV 0.93 ! PT 0.98 SC 1.00 TS 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.91 FD 0.81 HH 1.00* HN 0.99 ! KB 1.00* KK 1.08 KP 0.94 LA 1.00* ! MK 1.01 NL 0.93 NY 1.00* OV 1.00* ! PT 0.93 SC 0.95 TS 1.00* ! ! ! Correcting IF 2. ! A total of 33 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* HH 1.00* HN 1.00* ! KB 1.14 KK 0.96 KP 1.00* LA 1.00* ! MK 0.96 NL 1.00* NY 1.00* OV 1.01 ! PT 1.00* SC 1.00* TS 1.02 ! ! A total of 129 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.96 FD 0.99 HH 1.08 HN 1.01 ! KB 1.00* KK 0.96 KP 0.94 LA 0.97 ! MK 0.92 NL 1.16 NY 1.00* OV 0.96 ! PT 1.00 SC 1.02 TS 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 FD 0.93 HH 1.00* HN 1.01 ! KB 1.00* KK 1.11 KP 0.94 LA 1.00* ! MK 0.96 NL 0.97 NY 1.00* OV 1.00* ! PT 0.96 SC 0.98 TS 1.00* ! ! ! Correcting IF 3. ! A total of 33 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* HH 1.00* HN 1.00* ! KB 1.13 KK 0.95 KP 1.00* LA 1.00* ! MK 0.99 NL 1.00* NY 1.00* OV 1.00 ! PT 1.00* SC 1.00* TS 1.01 ! ! A total of 129 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.94 FD 1.01 HH 1.07 HN 1.04 ! KB 1.00* KK 0.95 KP 0.95 LA 0.96 ! MK 0.97 NL 1.11 NY 1.00* OV 0.95 ! PT 1.04 SC 1.04 TS 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.94 FD 0.94 HH 1.00* HN 1.04 ! KB 1.00* KK 1.13 KP 0.95 LA 1.00* ! MK 1.02 NL 0.92 NY 1.00* OV 1.00* ! PT 0.99 SC 1.00 TS 1.00* ! ! ! Correcting IF 4. ! A total of 33 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* HH 1.00* HN 1.00* ! KB 1.13 KK 0.93 KP 1.00* LA 1.00* ! MK 0.98 NL 1.00* NY 1.00* OV 1.07 ! PT 1.00* SC 1.00* TS 0.91 ! ! A total of 129 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 1.02 HH 1.08 HN 1.01 ! KB 1.00* KK 1.01 KP 0.95 LA 1.02 ! MK 0.96 NL 1.14 NY 1.00* OV 0.99 ! PT 1.01 SC 1.03 TS 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 0.94 HH 1.00* HN 1.01 ! KB 1.00* KK 1.16 KP 0.95 LA 1.00* ! MK 1.02 NL 0.95 NY 1.00* OV 1.00* ! PT 0.95 SC 0.99 TS 1.00* ! ! ! Fit before self-cal, rms=0.299005Jy sigma=0.002853 ! Fit after self-cal, rms=0.295870Jy sigma=0.002619 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! Estimated beam: bmin=0.8547 mas, bmaj=1.766 mas, bpa=11.12 degrees ! Estimated noise=690.875 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 = -0.0125705 Jy ! Component: 100 - total flux cleaned = -0.0131555 Jy ! Component: 150 - total flux cleaned = -0.0134336 Jy ! Component: 200 - total flux cleaned = -0.0136981 Jy ! Total flux subtracted in 200 components = -0.0136981 Jy ! Clean residual min=-0.035459 max=0.042119 Jy/beam ! Clean residual mean=0.001240 rms=0.014185 Jy/beam ! Combined flux in latest and established models = 1.35568 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 29 components and 1.35568 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.295034Jy sigma=0.002618 ! Fit after self-cal, rms=0.295013Jy sigma=0.002618 ! Inverting map ! Your choice of large map pixels excluded 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 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=0.295013Jy sigma=0.002618 ! Fit after self-cal, rms=0.291921Jy sigma=0.002325 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! Estimated beam: bmin=0.8541 mas, bmaj=1.766 mas, bpa=11.01 degrees ! Estimated noise=693.015 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00463926 Jy ! Component: 100 - total flux cleaned = 0.00464186 Jy ! Component: 150 - total flux cleaned = 0.00464962 Jy ! Component: 200 - total flux cleaned = 0.00445081 Jy ! Total flux subtracted in 200 components = 0.00445081 Jy ! Clean residual min=-0.032730 max=0.038370 Jy/beam ! Clean residual mean=0.000443 rms=0.012289 Jy/beam ! Combined flux in latest and established models = 1.36013 Jy selfcal ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 33 components and 1.36013 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.291939Jy sigma=0.002321 ! Fit after self-cal, rms=0.291929Jy sigma=0.002321 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 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 = 9.93869e-05 Jy ! Component: 100 - total flux cleaned = -0.000497547 Jy ! Component: 150 - total flux cleaned = -0.000677082 Jy ! Component: 200 - total flux cleaned = -0.000844724 Jy ! Total flux subtracted in 200 components = -0.000844724 Jy ! Clean residual min=-0.032773 max=0.038367 Jy/beam ! Clean residual mean=0.000461 rms=0.012289 Jy/beam ! Combined flux in latest and established models = 1.35929 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 35 components and 1.35929 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.291900Jy sigma=0.002320 ! Fit after self-cal, rms=0.291874Jy sigma=0.002319 ! Inverting map ! Your choice of large map pixels excluded 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 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=0.291874Jy sigma=0.002319 ! Fit after self-cal, rms=0.600134Jy sigma=0.001349 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! Estimated beam: bmin=0.8494 mas, bmaj=1.762 mas, bpa=11.13 degrees ! Estimated noise=693.409 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00521047 Jy ! Component: 100 - total flux cleaned = 0.0052004 Jy ! Component: 150 - total flux cleaned = 0.00496944 Jy ! Component: 200 - total flux cleaned = 0.00496779 Jy ! Total flux subtracted in 200 components = 0.00496779 Jy ! Clean residual min=-0.007205 max=0.006280 Jy/beam ! Clean residual mean=0.000385 rms=0.001450 Jy/beam ! Combined flux in latest and established models = 1.36426 Jy selfcal ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 38 components and 1.36426 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.599919Jy sigma=0.001343 ! Fit after self-cal, rms=0.602099Jy sigma=0.001341 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 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 = -0.000141838 Jy ! Component: 100 - total flux cleaned = -0.000533668 Jy ! Component: 150 - total flux cleaned = -0.000716316 Jy ! Component: 200 - total flux cleaned = -0.00105035 Jy ! Total flux subtracted in 200 components = -0.00105035 Jy ! Clean residual min=-0.006362 max=0.006187 Jy/beam ! Clean residual mean=0.000408 rms=0.001375 Jy/beam ! Combined flux in latest and established models = 1.36321 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 38 components and 1.36321 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.601990Jy sigma=0.001338 ! Fit after self-cal, rms=0.602018Jy sigma=0.001338 ! Inverting map ! Your choice of large map pixels excluded 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! Added new window around map position (1.4, 0.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000861834 Jy ! Component: 100 - total flux cleaned = 0.00106495 Jy ! Component: 150 - total flux cleaned = 0.0012309 Jy ! Component: 200 - total flux cleaned = 0.00123729 Jy ! Total flux subtracted in 200 components = 0.00123729 Jy ! Clean residual min=-0.005297 max=0.004625 Jy/beam ! Clean residual mean=0.000379 rms=0.001220 Jy/beam ! Combined flux in latest and established models = 1.36444 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 46 components and 1.36444 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.601882Jy sigma=0.001333 ! Fit after self-cal, rms=0.601940Jy sigma=0.001333 ! Inverting map ! Your choice of large map pixels excluded 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 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=0.601940Jy sigma=0.001333 ! Fit after self-cal, rms=0.606487Jy sigma=0.001329 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! Estimated beam: bmin=2.281 mas, bmaj=3.566 mas, bpa=-4.465 degrees ! Estimated noise=829.26 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00376432 Jy ! Component: 100 - total flux cleaned = 0.00393317 Jy ! Component: 150 - total flux cleaned = 0.00393472 Jy ! Component: 200 - total flux cleaned = 0.00393455 Jy ! Total flux subtracted in 200 components = 0.00393455 Jy ! Clean residual min=-0.002786 max=0.004114 Jy/beam ! Clean residual mean=0.000551 rms=0.001172 Jy/beam ! Combined flux in latest and established models = 1.36838 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 60 components and 1.36838 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.606478Jy sigma=0.001328 ! Fit after self-cal, rms=0.606561Jy sigma=0.001328 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 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 = 0.000623528 Jy ! Component: 100 - total flux cleaned = 0.000564712 Jy ! Component: 150 - total flux cleaned = 0.000619656 Jy ! Component: 200 - total flux cleaned = 0.00061674 Jy ! Total flux subtracted in 200 components = 0.00061674 Jy ! Clean residual min=-0.002715 max=0.004208 Jy/beam ! Clean residual mean=0.000523 rms=0.001130 Jy/beam ! Combined flux in latest and established models = 1.36899 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 65 components and 1.36899 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.606567Jy sigma=0.001327 ! Fit after self-cal, rms=0.606580Jy sigma=0.001327 ! Inverting map ! Your choice of large map pixels excluded 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 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 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! Estimated beam: bmin=0.8494 mas, bmaj=1.766 mas, bpa=10.98 degrees ! Estimated noise=693.685 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8494 x 1.766 at 10.98 degrees (North through East) ! Clean map min=-0.0036538 max=1.2353 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=0.606580Jy sigma=0.001327 ! Fit after self-cal, rms=1.012333Jy sigma=0.001193 ! Inverting map and beam ! Your choice of large map pixels excluded 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! Estimated beam: bmin=0.8485 mas, bmaj=1.764 mas, bpa=11.05 degrees ! Estimated noise=693.579 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00176803 Jy ! Component: 100 - total flux cleaned = 0.00177491 Jy ! Component: 150 - total flux cleaned = 0.00176868 Jy ! Component: 200 - total flux cleaned = 0.00190247 Jy ! Total flux subtracted in 200 components = 0.00190247 Jy ! Clean residual min=-0.004377 max=0.004584 Jy/beam ! Clean residual mean=0.000276 rms=0.001064 Jy/beam ! Combined flux in latest and established models = 1.3709 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 68 components and 1.3709 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.012236Jy sigma=0.001191 ! Fit after self-cal, rms=1.012292Jy sigma=0.001191 ! Inverting map ! Your choice of large map pixels excluded 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -8.83936e-05 Jy ! Component: 100 - total flux cleaned = -0.000222459 Jy ! Component: 150 - total flux cleaned = -0.000103094 Jy ! Component: 200 - total flux cleaned = -0.000105937 Jy ! Total flux subtracted in 200 components = -0.000105937 Jy ! Clean residual min=-0.004125 max=0.004474 Jy/beam ! Clean residual mean=0.000278 rms=0.001036 Jy/beam ! Combined flux in latest and established models = 1.37079 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 71 components and 1.37079 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.012216Jy sigma=0.001189 ! Fit after self-cal, rms=1.012256Jy sigma=0.001189 ! Inverting map ! Your choice of large map pixels excluded 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.012256Jy sigma=0.001189 ! Fit after self-cal, rms=1.013994Jy sigma=0.001189 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 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! Estimated beam: bmin=0.5897 mas, bmaj=1.3 mas, bpa=16.81 degrees ! Estimated noise=1078.92 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.930993 Jy ! Component: 100 - total flux cleaned = 1.16151 Jy ! Component: 150 - total flux cleaned = 1.24969 Jy ! Component: 200 - total flux cleaned = 1.29324 Jy ! Total flux subtracted in 200 components = 1.29324 Jy ! Clean residual min=-0.012728 max=0.020690 Jy/beam ! Clean residual mean=0.000342 rms=0.002861 Jy/beam ! Combined flux in latest and established models = 1.29324 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 15 model components to the UV plane model. ! The established model now contains 15 components and 1.29324 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! Estimated beam: bmin=0.8478 mas, bmaj=1.765 mas, bpa=10.97 degrees ! Estimated noise=693.402 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 = 0.0371121 Jy ! Component: 100 - total flux cleaned = 0.0549667 Jy ! Component: 150 - total flux cleaned = 0.0651287 Jy ! Component: 200 - total flux cleaned = 0.0712244 Jy ! Total flux subtracted in 200 components = 0.0712244 Jy ! Clean residual min=-0.003703 max=0.004554 Jy/beam ! Clean residual mean=0.000384 rms=0.001163 Jy/beam ! Combined flux in latest and established models = 1.36446 Jy ! Adding 30 model components to the UV plane model. ! The established model now contains 37 components and 1.36446 Jy ! Inverting map ! Your choice of large map pixels excluded 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 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 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! Estimated beam: bmin=2.278 mas, bmaj=3.563 mas, bpa=-4.393 degrees ! Estimated noise=830.481 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00445869 Jy ! Component: 100 - total flux cleaned = 0.00656957 Jy ! Component: 150 - total flux cleaned = 0.00765539 Jy ! Component: 200 - total flux cleaned = 0.0079472 Jy ! Total flux subtracted in 200 components = 0.0079472 Jy ! Clean residual min=-0.002747 max=0.003767 Jy/beam ! Clean residual mean=0.000440 rms=0.001095 Jy/beam ! Combined flux in latest and established models = 1.37241 Jy flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000118075 Jy ! Component: 100 - total flux cleaned = 0.000151714 Jy ! Component: 150 - total flux cleaned = 0.000168436 Jy ! Component: 200 - total flux cleaned = 0.000182894 Jy ! Total flux subtracted in 200 components = 0.000182894 Jy ! Clean residual min=-0.002771 max=0.003722 Jy/beam ! Clean residual mean=0.000432 rms=0.001088 Jy/beam ! Combined flux in latest and established models = 1.37259 Jy ! Adding 22 model components to the UV plane model. ! The established model now contains 57 components and 1.37259 Jy ! Inverting map ! Your choice of large map pixels excluded 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! Estimated beam: bmin=0.8478 mas, bmaj=1.765 mas, bpa=10.97 degrees ! Estimated noise=693.402 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000385391 Jy ! Component: 100 - total flux cleaned = -0.000383782 Jy ! Component: 150 - total flux cleaned = -0.000479557 Jy ! Component: 200 - total flux cleaned = -0.000566276 Jy ! Total flux subtracted in 200 components = -0.000566276 Jy ! Clean residual min=-0.003509 max=0.003871 Jy/beam ! Clean residual mean=0.000221 rms=0.000978 Jy/beam ! Combined flux in latest and established models = 1.37202 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 67 components and 1.37202 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.014061Jy sigma=0.001207 ! Fit after self-cal, rms=1.014096Jy sigma=0.001201 wmodel J1152-0841_X_2010_10_13_pus_map.mod ! Writing 67 model components to file: J1152-0841_X_2010_10_13_pus_map.mod wobs J1152-0841_X_2010_10_13_pus_uvs.fits ! Writing UV FITS file: J1152-0841_X_2010_10_13_pus_uvs.fits wwins J1152-0841_X_2010_10_13_pus_map.win ! wwins: Wrote 2 windows to J1152-0841_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 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! clean: niter=1024 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000316596 Jy ! Component: 100 - total flux cleaned = 2.34462e-05 Jy ! Component: 150 - total flux cleaned = 0.000474984 Jy ! Component: 200 - total flux cleaned = 0.000844111 Jy ! Component: 250 - total flux cleaned = 0.00131719 Jy ! Component: 300 - total flux cleaned = 0.00183282 Jy ! Component: 350 - total flux cleaned = 0.00233501 Jy ! Component: 400 - total flux cleaned = 0.00282362 Jy ! Component: 450 - total flux cleaned = 0.00330102 Jy ! Component: 500 - total flux cleaned = 0.0038715 Jy ! Component: 550 - total flux cleaned = 0.00437844 Jy ! Component: 600 - total flux cleaned = 0.00482531 Jy ! Component: 650 - total flux cleaned = 0.00516631 Jy ! Component: 700 - total flux cleaned = 0.00545314 Jy ! Component: 750 - total flux cleaned = 0.00564165 Jy ! Component: 800 - total flux cleaned = 0.00582782 Jy ! Component: 850 - total flux cleaned = 0.00610216 Jy ! Component: 900 - total flux cleaned = 0.00632691 Jy ! Component: 950 - total flux cleaned = 0.00654931 Jy ! Component: 1000 - total flux cleaned = 0.00681225 Jy ! Total flux subtracted in 1024 components = 0.00689908 Jy ! Clean residual min=-0.002422 max=0.002934 Jy/beam ! Clean residual mean=0.000094 rms=0.000800 Jy/beam ! Combined flux in latest and established models = 1.37892 Jy keep ! Adding 54 model components to the UV plane model. ! The established model now contains 118 components and 1.37892 Jy ![Exited script file: muppet] wmap "J1152-0841_X_2010_10_13_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8478 x 1.765 at 10.97 degrees (North through East) ! Clean map min=-0.0033431 max=1.2407 Jy/beam ! Writing clean map to FITS file: J1152-0841_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 1.24071 invert ! Inverting map ! Your choice of large map pixels excluded 8.75% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000801002 device "J1152-0841_X_2010_10_13_pus\_map.eps/VPS" ! Attempting to open device: 'J1152-0841_X_2010_10_13_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.19368 0.19368 0.387361 0.774722 1.54944 3.09889 6.19777 12.3955 24.7911 49.5822 99.1644 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0024 print "peak=",int(1000*peak_flux)/1000 ! peak= 1.24 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8478 x 1.765 at 10.97 degrees (North through East) ! Clean map min=-0.0033431 max=1.2407 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J1152-0841_X_2010_10_13_pus\_map.gif/vgif" ! Attempting to open device: 'J1152-0841_X_2010_10_13_pus_map.gif/vgif' mapplot cln