! Started logfile: J1147-3812_X_1998_10_01_pus_uvs.log on Wed Feb 6 12:31:36 2008 obs J1147-3812_X_1998_10_01_pus_uva.fits ! Reading UV FITS file: J1147-3812_X_1998_10_01_pus_uva.fits ! AN table 1: 32 integrations on 136 of 136 possible baselines. ! Apparent sampling: 0.220818 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1147-3812 ! ! 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 8.40798e+09 4e+06 1 4e+06 ! 02 2 8.47798e+09 4e+06 1 4e+06 ! 03 3 8.79298e+09 4e+06 1 4e+06 ! 04 4 8.89798e+09 4e+06 1 4e+06 ! ! Polarization(s): RR ! ! Read 2049 lines of history. ! ! Reading 3844 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 J1147-3812_X_1998_10_01_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 283 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 283 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 283 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 283 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.895265Jy sigma=0.008198 ! Fit after self-cal, rms=0.710053Jy sigma=0.006673 ! 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 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 milli-arcsec ! Estimated beam: bmin=0.6219 mas, bmaj=1.856 mas, bpa=-1.794 degrees ! Estimated noise=2679.79 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (0, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.16546 Jy ! Component: 100 - total flux cleaned = 1.4352 Jy ! Total flux subtracted in 100 components = 1.4352 Jy ! Clean residual min=-0.062426 max=0.131999 Jy/beam ! Clean residual mean=0.000540 rms=0.027979 Jy/beam ! Combined flux in latest and established models = 1.4352 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 1.4352 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.428344Jy sigma=0.003915 ! Fit after self-cal, rms=0.428047Jy sigma=0.003913 ! Inverting map ! Your choice of large map pixels excluded 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 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 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 milli-arcsec ! Estimated beam: bmin=0.8731 mas, bmaj=2.352 mas, bpa=5.485 degrees ! Estimated noise=1351.4 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 = 0.219035 Jy ! Component: 100 - total flux cleaned = 0.315332 Jy ! Component: 150 - total flux cleaned = 0.359149 Jy ! Component: 200 - total flux cleaned = 0.376861 Jy ! Total flux subtracted in 200 components = 0.376861 Jy ! Clean residual min=-0.053168 max=0.086398 Jy/beam ! Clean residual mean=0.000129 rms=0.021711 Jy/beam ! Combined flux in latest and established models = 1.81206 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 29 components and 1.81206 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.346106Jy sigma=0.002780 ! Fit after self-cal, rms=0.346213Jy sigma=0.002780 ! Inverting map ! Your choice of large map pixels excluded 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.97 GC 1.00* HN 1.00* ! KK 1.04 KP 0.92 LA 1.03 MK 0.96 ! NL 1.14 NY 1.00* ON 1.00* OV 0.98 ! PT 0.96 SC 0.99 WF 1.00* MC 1.00* ! GN 1.22 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.97 GC 1.00* HN 1.00* ! KK 1.04 KP 0.95 LA 0.99 MK 0.93 ! NL 1.20 NY 1.00* ON 1.00* OV 0.97 ! PT 0.97 SC 0.99 WF 1.00* MC 1.00* ! GN 1.19 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.96 GC 1.00* HN 1.00* ! KK 1.04 KP 0.97 LA 1.00 MK 0.95 ! NL 1.16 NY 1.00* ON 1.00* OV 0.95 ! PT 0.95 SC 1.04 WF 1.00* MC 1.00* ! GN 1.19 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.93 GC 1.00* HN 1.00* ! KK 1.04 KP 0.96 LA 1.02 MK 0.98 ! NL 1.18 NY 1.00* ON 1.00* OV 0.95 ! PT 0.92 SC 1.01 WF 1.00* MC 1.00* ! GN 1.23 ! ! ! Fit before self-cal, rms=0.346213Jy sigma=0.002780 ! Fit after self-cal, rms=0.319937Jy sigma=0.002391 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 milli-arcsec ! Estimated beam: bmin=0.8826 mas, bmaj=2.369 mas, bpa=6.075 degrees ! Estimated noise=1362.07 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 (1.4, -2.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0136758 Jy ! Component: 100 - total flux cleaned = 0.01201 Jy ! Component: 150 - total flux cleaned = 0.00987597 Jy ! Component: 200 - total flux cleaned = 0.00864857 Jy ! Total flux subtracted in 200 components = 0.00864857 Jy ! Clean residual min=-0.013266 max=0.012294 Jy/beam ! Clean residual mean=0.000160 rms=0.003458 Jy/beam ! Combined flux in latest and established models = 1.82071 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 41 components and 1.82071 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.318134Jy sigma=0.002378 ! Fit after self-cal, rms=0.318675Jy sigma=0.002377 ! Inverting map ! Your choice of large map pixels excluded 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 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=0.318675Jy sigma=0.002377 ! Fit after self-cal, rms=0.316584Jy sigma=0.002376 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 milli-arcsec ! Estimated beam: bmin=0.8802 mas, bmaj=2.362 mas, bpa=6.051 degrees ! Estimated noise=1358.25 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0053038 Jy ! Component: 100 - total flux cleaned = 0.00557363 Jy ! Component: 150 - total flux cleaned = 0.00515015 Jy ! Component: 200 - total flux cleaned = 0.00476702 Jy ! Total flux subtracted in 200 components = 0.00476702 Jy ! Clean residual min=-0.012345 max=0.009895 Jy/beam ! Clean residual mean=0.000151 rms=0.003117 Jy/beam ! Combined flux in latest and established models = 1.82548 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 44 components and 1.82548 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.316091Jy sigma=0.002372 ! Fit after self-cal, rms=0.315995Jy sigma=0.002372 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 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 = 0.00139064 Jy ! Component: 100 - total flux cleaned = 0.00139483 Jy ! Component: 150 - total flux cleaned = 0.00124313 Jy ! Component: 200 - total flux cleaned = 0.000964136 Jy ! Total flux subtracted in 200 components = 0.000964136 Jy ! Clean residual min=-0.012063 max=0.009797 Jy/beam ! Clean residual mean=0.000138 rms=0.003020 Jy/beam ! Combined flux in latest and established models = 1.82644 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 52 components and 1.82644 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.315802Jy sigma=0.002371 ! Fit after self-cal, rms=0.315783Jy sigma=0.002370 ! Inverting map ! Your choice of large map pixels excluded 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 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=0.315783Jy sigma=0.002370 ! Fit after self-cal, rms=0.314765Jy sigma=0.002370 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 milli-arcsec ! Estimated beam: bmin=0.8793 mas, bmaj=2.36 mas, bpa=6.025 degrees ! Estimated noise=1356.47 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00163197 Jy ! Component: 100 - total flux cleaned = 0.00193089 Jy ! Component: 150 - total flux cleaned = 0.00206332 Jy ! Component: 200 - total flux cleaned = 0.0021747 Jy ! Total flux subtracted in 200 components = 0.0021747 Jy ! Clean residual min=-0.011504 max=0.009678 Jy/beam ! Clean residual mean=0.000142 rms=0.002906 Jy/beam ! Combined flux in latest and established models = 1.82862 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 58 components and 1.82862 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.314644Jy sigma=0.002369 ! Fit after self-cal, rms=0.314624Jy sigma=0.002369 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 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 = 0.000629402 Jy ! Component: 100 - total flux cleaned = 0.000858208 Jy ! Component: 150 - total flux cleaned = 0.000860418 Jy ! Component: 200 - total flux cleaned = 0.000955312 Jy ! Total flux subtracted in 200 components = 0.000955312 Jy ! Clean residual min=-0.011333 max=0.009585 Jy/beam ! Clean residual mean=0.000129 rms=0.002875 Jy/beam ! Combined flux in latest and established models = 1.82957 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 62 components and 1.82957 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.314547Jy sigma=0.002369 ! Fit after self-cal, rms=0.314545Jy sigma=0.002369 ! Inverting map ! Your choice of large map pixels excluded 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 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=0.314545Jy sigma=0.002369 ! Fit after self-cal, rms=0.313938Jy sigma=0.002368 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 milli-arcsec ! Estimated beam: bmin=2.39 mas, bmaj=10.01 mas, bpa=7.892 degrees ! Estimated noise=1592.06 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000510194 Jy ! Component: 100 - total flux cleaned = -0.000442035 Jy ! Component: 150 - total flux cleaned = -0.000526283 Jy ! Component: 200 - total flux cleaned = -0.000676831 Jy ! Total flux subtracted in 200 components = -0.000676831 Jy ! Clean residual min=-0.008781 max=0.009800 Jy/beam ! Clean residual mean=0.000306 rms=0.003501 Jy/beam ! Combined flux in latest and established models = 1.8289 Jy selfcal ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 69 components and 1.8289 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.313926Jy sigma=0.002368 ! Fit after self-cal, rms=0.313896Jy sigma=0.002368 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 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 = 0.000443121 Jy ! Component: 100 - total flux cleaned = 0.00049589 Jy ! Component: 150 - total flux cleaned = 0.00049646 Jy ! Component: 200 - total flux cleaned = 0.000429391 Jy ! Total flux subtracted in 200 components = 0.000429391 Jy ! Clean residual min=-0.008751 max=0.009781 Jy/beam ! Clean residual mean=0.000295 rms=0.003517 Jy/beam ! Combined flux in latest and established models = 1.82932 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 70 components and 1.82932 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.313891Jy sigma=0.002368 ! Fit after self-cal, rms=0.313875Jy sigma=0.002368 ! Inverting map ! Your choice of large map pixels excluded 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 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 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 milli-arcsec ! Estimated beam: bmin=0.8788 mas, bmaj=2.359 mas, bpa=6.031 degrees ! Estimated noise=1355.02 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8788 x 2.359 at 6.031 degrees (North through East) ! Clean map min=-0.013684 max=1.5494 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=0.313875Jy sigma=0.002368 ! Fit after self-cal, rms=0.295573Jy sigma=0.002148 ! Inverting map and beam ! Your choice of large map pixels excluded 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 milli-arcsec ! Estimated beam: bmin=0.8797 mas, bmaj=2.362 mas, bpa=6.052 degrees ! Estimated noise=1354.93 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000418337 Jy ! Component: 100 - total flux cleaned = -0.000200552 Jy ! Component: 150 - total flux cleaned = -9.61536e-06 Jy ! Component: 200 - total flux cleaned = 7.3537e-05 Jy ! Total flux subtracted in 200 components = 7.3537e-05 Jy ! Clean residual min=-0.010627 max=0.008789 Jy/beam ! Clean residual mean=0.000145 rms=0.002680 Jy/beam ! Combined flux in latest and established models = 1.8294 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 75 components and 1.8294 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.295497Jy sigma=0.002147 ! Fit after self-cal, rms=0.295511Jy sigma=0.002147 ! Inverting map ! Your choice of large map pixels excluded 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000231399 Jy ! Component: 100 - total flux cleaned = 0.000493461 Jy ! Component: 150 - total flux cleaned = 0.00057855 Jy ! Component: 200 - total flux cleaned = 0.00073146 Jy ! Total flux subtracted in 200 components = 0.00073146 Jy ! Clean residual min=-0.010478 max=0.008700 Jy/beam ! Clean residual mean=0.000135 rms=0.002670 Jy/beam ! Combined flux in latest and established models = 1.83013 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 78 components and 1.83013 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.295470Jy sigma=0.002147 ! Fit after self-cal, rms=0.295484Jy sigma=0.002147 ! Inverting map ! Your choice of large map pixels excluded 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.295484Jy sigma=0.002147 ! Fit after self-cal, rms=0.295255Jy sigma=0.002147 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 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 milli-arcsec ! Estimated beam: bmin=0.6213 mas, bmaj=1.834 mas, bpa=-1.473 degrees ! Estimated noise=2752.26 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.19619 Jy ! Component: 100 - total flux cleaned = 1.47936 Jy ! Component: 150 - total flux cleaned = 1.59767 Jy ! Component: 200 - total flux cleaned = 1.66799 Jy ! Total flux subtracted in 200 components = 1.66799 Jy ! Clean residual min=-0.025076 max=0.038816 Jy/beam ! Clean residual mean=0.000431 rms=0.010003 Jy/beam ! Combined flux in latest and established models = 1.66799 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 28 model components to the UV plane model. ! The established model now contains 28 components and 1.66799 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 milli-arcsec ! Estimated beam: bmin=0.8797 mas, bmaj=2.362 mas, bpa=6.085 degrees ! Estimated noise=1354.04 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 = 0.0781944 Jy ! Component: 100 - total flux cleaned = 0.11486 Jy ! Component: 150 - total flux cleaned = 0.134505 Jy ! Component: 200 - total flux cleaned = 0.145488 Jy ! Total flux subtracted in 200 components = 0.145488 Jy ! Clean residual min=-0.010019 max=0.010109 Jy/beam ! Clean residual mean=0.000354 rms=0.003048 Jy/beam ! Combined flux in latest and established models = 1.81348 Jy ! Adding 42 model components to the UV plane model. ! The established model now contains 59 components and 1.81348 Jy ! Inverting map ! Your choice of large map pixels excluded 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 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 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 milli-arcsec ! Estimated beam: bmin=2.388 mas, bmaj=10.01 mas, bpa=7.885 degrees ! Estimated noise=1590.22 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00790365 Jy ! Component: 100 - total flux cleaned = 0.0111161 Jy ! Component: 150 - total flux cleaned = 0.0116312 Jy ! Component: 200 - total flux cleaned = 0.0116921 Jy ! Total flux subtracted in 200 components = 0.0116921 Jy ! Clean residual min=-0.007664 max=0.008242 Jy/beam ! Clean residual mean=0.000384 rms=0.003324 Jy/beam ! Combined flux in latest and established models = 1.82517 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 = 5.57571e-05 Jy ! Component: 100 - total flux cleaned = 0.000108684 Jy ! Component: 150 - total flux cleaned = 0.000161278 Jy ! Component: 200 - total flux cleaned = 0.000161745 Jy ! Total flux subtracted in 200 components = 0.000161745 Jy ! Clean residual min=-0.007598 max=0.008299 Jy/beam ! Clean residual mean=0.000379 rms=0.003301 Jy/beam ! Combined flux in latest and established models = 1.82533 Jy ! Adding 12 model components to the UV plane model. ! The established model now contains 69 components and 1.82533 Jy ! Inverting map ! Your choice of large map pixels excluded 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 milli-arcsec ! Estimated beam: bmin=0.8797 mas, bmaj=2.362 mas, bpa=6.085 degrees ! Estimated noise=1354.04 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00206571 Jy ! Component: 100 - total flux cleaned = -0.00158677 Jy ! Component: 150 - total flux cleaned = -0.00130467 Jy ! Component: 200 - total flux cleaned = -0.00117637 Jy ! Total flux subtracted in 200 components = -0.00117637 Jy ! Clean residual min=-0.009463 max=0.008600 Jy/beam ! Clean residual mean=0.000220 rms=0.002708 Jy/beam ! Combined flux in latest and established models = 1.82415 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 77 components and 1.82415 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.295455Jy sigma=0.002148 ! Fit after self-cal, rms=0.295417Jy sigma=0.002147 wmodel J1147-3812_X_1998_10_01_pus_map.mod ! Writing 77 model components to file: J1147-3812_X_1998_10_01_pus_map.mod wobs J1147-3812_X_1998_10_01_pus_uvs.fits ! Writing UV FITS file: J1147-3812_X_1998_10_01_pus_uvs.fits wwins J1147-3812_X_1998_10_01_pus_map.win ! wwins: Wrote 2 windows to J1147-3812_X_1998_10_01_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 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 milli-arcsec ! clean: niter=1024 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00220074 Jy ! Component: 100 - total flux cleaned = -0.00208432 Jy ! Component: 150 - total flux cleaned = -0.00157064 Jy ! Component: 200 - total flux cleaned = -0.00097784 Jy ! Component: 250 - total flux cleaned = -0.000528316 Jy ! Component: 300 - total flux cleaned = 0.000113042 Jy ! Component: 350 - total flux cleaned = 0.000518364 Jy ! Component: 400 - total flux cleaned = 0.00119862 Jy ! Component: 450 - total flux cleaned = 0.00185224 Jy ! Component: 500 - total flux cleaned = 0.00257575 Jy ! Component: 550 - total flux cleaned = 0.00310104 Jy ! Component: 600 - total flux cleaned = 0.00361072 Jy ! Component: 650 - total flux cleaned = 0.00402354 Jy ! Component: 700 - total flux cleaned = 0.00442593 Jy ! Component: 750 - total flux cleaned = 0.00481854 Jy ! Component: 800 - total flux cleaned = 0.00527575 Jy ! Component: 850 - total flux cleaned = 0.00571933 Jy ! Component: 900 - total flux cleaned = 0.00608013 Jy ! Component: 950 - total flux cleaned = 0.00650231 Jy ! Component: 1000 - total flux cleaned = 0.00691407 Jy ! Total flux subtracted in 1024 components = 0.00725036 Jy ! Clean residual min=-0.003459 max=0.004608 Jy/beam ! Clean residual mean=0.000257 rms=0.001339 Jy/beam ! Combined flux in latest and established models = 1.8314 Jy keep ! Adding 43 model components to the UV plane model. ! The established model now contains 120 components and 1.8314 Jy ![Exited script file: muppet] wmap "J1147-3812_X_1998_10_01_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8797 x 2.362 at 6.085 degrees (North through East) ! Clean map min=-0.0063853 max=1.5752 Jy/beam ! Writing clean map to FITS file: J1147-3812_X_1998_10_01_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 1.57518 invert ! Inverting map ! Your choice of large map pixels excluded 1.64% of the data. ! The x-axis pixel size should ideally be below 0.1903 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00130679 device "J1147-3812_X_1998_10_01_pus\_map.eps/VPS" ! Attempting to open device: 'J1147-3812_X_1998_10_01_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.248884 0.248884 0.497768 0.995535 1.99107 3.98214 7.96428 15.9286 31.8571 63.7142 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0039 print "peak=",int(1000*peak_flux)/1000 ! peak= 1.575 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8797 x 2.362 at 6.085 degrees (North through East) ! Clean map min=-0.0063853 max=1.5752 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J1147-3812_X_1998_10_01_pus\_map.gif/vgif" ! Attempting to open device: 'J1147-3812_X_1998_10_01_pus_map.gif/vgif' mapplot cln quit ! Quitting program ! Log file J1147-3812_X_1998_10_01_pus_uvs.log closed on Wed Feb 6 12:31:38 2008