! Started logfile: J0904-3514_X_2010_06_23_pus_uvs.log on Thu Jan 27 23:40:32 2011 obs J0904-3514_X_2010_06_23_pus_uva.fits ! Reading UV FITS file: J0904-3514_X_2010_06_23_pus_uva.fits ! AN table 1: 95 integrations on 105 of 105 possible baselines. ! AN table 2: 95 integrations on 105 of 105 possible baselines. ! Apparent sampling: 0.29599 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0904-3514 ! ! 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 3588 lines of history. ! ! Reading 23620 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 J0904-3514_X_2010_06_23_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 677 telescope corrections were flagged in sub-array 1. ! A total of 585 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 2. ! A total of 677 telescope corrections were flagged in sub-array 1. ! A total of 585 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 3. ! A total of 743 telescope corrections were flagged in sub-array 1. ! A total of 585 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 4. ! A total of 700 telescope corrections were flagged in sub-array 1. ! A total of 585 telescope corrections were flagged in sub-array 2. ! ! Fit before self-cal, rms=0.850113Jy sigma=0.008334 ! Fit after self-cal, rms=0.780304Jy sigma=0.007752 ! clrmod: Cleared the established, tentative and continuum models. ! Redundant starting model cleared. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.782% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=0.6825 mas, bmaj=1.997 mas, bpa=4.33 degrees ! Estimated noise=989.47 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 = 0.17005 Jy ! Component: 100 - total flux cleaned = 0.213177 Jy ! Total flux subtracted in 100 components = 0.213177 Jy ! Clean residual min=-0.009047 max=0.021462 Jy/beam ! Clean residual mean=0.000341 rms=0.004032 Jy/beam ! Combined flux in latest and established models = 0.213177 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 8 components and 0.213177 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.164418Jy sigma=0.001428 ! Fit after self-cal, rms=0.164384Jy sigma=0.001428 ! Inverting map ! Your choice of large map pixels excluded 0.782% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec print "************** FINISHED UNIFORM WEIGHTING CLEAN **************" ! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** ! uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. win_mult = win_mult * 1.6 clean_niter = clean_niter * 2 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.782% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=0.8826 mas, bmaj=2.516 mas, bpa=1.835 degrees ! Estimated noise=475.486 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 = 0.0365839 Jy ! Component: 100 - total flux cleaned = 0.053934 Jy ! Component: 150 - total flux cleaned = 0.0625722 Jy ! Component: 200 - total flux cleaned = 0.0668866 Jy ! Total flux subtracted in 200 components = 0.0668866 Jy ! Clean residual min=-0.005208 max=0.012423 Jy/beam ! Clean residual mean=0.000413 rms=0.002766 Jy/beam ! Combined flux in latest and established models = 0.280063 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 26 components and 0.280063 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.158361Jy sigma=0.001328 ! Fit after self-cal, rms=0.158196Jy sigma=0.001327 ! Inverting map ! Your choice of large map pixels excluded 0.782% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.94 HN 1.20 KK 1.00* ! KP 0.94 LA 0.94 MA 1.00* MK 1.00* ! NL 1.20 NY 1.00* OV 0.97 PT 0.98 ! SC 0.97 TS 1.00* ZC 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 1.00 HN 1.00* KK 1.00* ! KP 0.98 LA 0.94 MA 1.00* MK 0.94 ! NL 1.35 NY 1.00* OV 0.97 PT 0.96 ! SC 1.05 TS 1.00* ZC 1.00* ! ! ! Correcting IF 2. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.96 HN 1.19 KK 1.00* ! KP 0.94 LA 0.98 MA 1.00* MK 1.00* ! NL 1.14 NY 1.00* OV 1.03 PT 0.96 ! SC 1.02 TS 1.00* ZC 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.06 FD 0.98 HN 1.00* KK 1.00* ! KP 0.95 LA 0.97 MA 1.00* MK 0.96 ! NL 1.40 NY 1.00* OV 1.04 PT 0.95 ! SC 1.04 TS 1.00* ZC 1.00* ! ! ! Correcting IF 3. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.94 HN 1.18 KK 1.00* ! KP 0.97 LA 0.94 MA 1.00* MK 1.00* ! NL 1.16 NY 1.00* OV 0.99 PT 0.96 ! SC 0.95 TS 1.00* ZC 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 FD 0.97 HN 1.00* KK 1.00* ! KP 0.93 LA 0.98 MA 1.00* MK 0.99 ! NL 1.31 NY 1.00* OV 1.02 PT 0.96 ! SC 0.99 TS 1.00* ZC 1.00* ! ! ! Correcting IF 4. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.97 HN 1.19 KK 1.00* ! KP 0.94 LA 0.95 MA 1.00* MK 1.00* ! NL 1.17 NY 1.00* OV 0.96 PT 1.00 ! SC 0.95 TS 1.00* ZC 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 0.99 HN 1.00* KK 1.00* ! KP 0.94 LA 0.98 MA 1.00* MK 0.98 ! NL 1.28 NY 1.00* OV 0.98 PT 0.97 ! SC 1.05 TS 1.00* ZC 1.00* ! ! ! Fit before self-cal, rms=0.158196Jy sigma=0.001327 ! Fit after self-cal, rms=0.176148Jy sigma=0.001302 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.783% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=0.8837 mas, bmaj=2.534 mas, bpa=1.677 degrees ! Estimated noise=476.472 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 = -0.000450498 Jy ! Component: 100 - total flux cleaned = -0.000450888 Jy ! Component: 150 - total flux cleaned = -0.000484129 Jy ! Component: 200 - total flux cleaned = -0.00051764 Jy ! Total flux subtracted in 200 components = -0.00051764 Jy ! Clean residual min=-0.002308 max=0.002920 Jy/beam ! Clean residual mean=0.000037 rms=0.000752 Jy/beam ! Combined flux in latest and established models = 0.279546 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 30 components and 0.279546 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.176135Jy sigma=0.001302 ! Fit after self-cal, rms=0.176681Jy sigma=0.001301 ! Inverting map ! Your choice of large map pixels excluded 0.783% of the data. ! The x-axis pixel size should ideally be below 0.1956 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=0.176681Jy sigma=0.001301 ! Fit after self-cal, rms=0.177808Jy sigma=0.001301 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.783% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=0.8834 mas, bmaj=2.533 mas, bpa=1.686 degrees ! Estimated noise=476.236 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000476491 Jy ! Component: 100 - total flux cleaned = -0.000476779 Jy ! Component: 150 - total flux cleaned = -0.000508647 Jy ! Component: 200 - total flux cleaned = -0.000539657 Jy ! Total flux subtracted in 200 components = -0.000539657 Jy ! Clean residual min=-0.002225 max=0.002865 Jy/beam ! Clean residual mean=0.000035 rms=0.000734 Jy/beam ! Combined flux in latest and established models = 0.279006 Jy selfcal ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 31 components and 0.279006 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.177797Jy sigma=0.001301 ! Fit after self-cal, rms=0.177822Jy sigma=0.001301 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.783% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -6.72189e-05 Jy ! Component: 100 - total flux cleaned = -9.43939e-05 Jy ! Component: 150 - total flux cleaned = -0.000120576 Jy ! Component: 200 - total flux cleaned = -0.000146077 Jy ! Total flux subtracted in 200 components = -0.000146077 Jy ! Clean residual min=-0.002179 max=0.002831 Jy/beam ! Clean residual mean=0.000038 rms=0.000725 Jy/beam ! Combined flux in latest and established models = 0.27886 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 31 components and 0.27886 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.177814Jy sigma=0.001301 ! Fit after self-cal, rms=0.177817Jy sigma=0.001301 ! Inverting map ! Your choice of large map pixels excluded 0.783% of the data. ! The x-axis pixel size should ideally be below 0.1956 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=0.177817Jy sigma=0.001301 ! Fit after self-cal, rms=0.179070Jy sigma=0.001301 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.783% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=0.8829 mas, bmaj=2.53 mas, bpa=1.692 degrees ! Estimated noise=476.036 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00023657 Jy ! Component: 100 - total flux cleaned = -0.000238914 Jy ! Component: 150 - total flux cleaned = -0.000268419 Jy ! Component: 200 - total flux cleaned = -0.000322737 Jy ! Total flux subtracted in 200 components = -0.000322737 Jy ! Clean residual min=-0.002102 max=0.002760 Jy/beam ! Clean residual mean=0.000031 rms=0.000714 Jy/beam ! Combined flux in latest and established models = 0.278537 Jy selfcal ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 31 components and 0.278537 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.179060Jy sigma=0.001301 ! Fit after self-cal, rms=0.179085Jy sigma=0.001301 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.783% of the data. ! The x-axis pixel size should ideally be below 0.1956 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 = -3.26026e-05 Jy ! Component: 100 - total flux cleaned = -5.69999e-05 Jy ! Component: 150 - total flux cleaned = -8.18655e-05 Jy ! Component: 200 - total flux cleaned = -0.000106009 Jy ! Total flux subtracted in 200 components = -0.000106009 Jy ! Clean residual min=-0.002064 max=0.002725 Jy/beam ! Clean residual mean=0.000033 rms=0.000706 Jy/beam ! Combined flux in latest and established models = 0.278431 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 31 components and 0.278431 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.179078Jy sigma=0.001301 ! Fit after self-cal, rms=0.179080Jy sigma=0.001301 ! Inverting map ! Your choice of large map pixels excluded 0.783% of the data. ! The x-axis pixel size should ideally be below 0.1956 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=0.179080Jy sigma=0.001301 ! Fit after self-cal, rms=0.180067Jy sigma=0.001301 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.783% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=2.554 mas, bmaj=7.685 mas, bpa=0.1848 degrees ! Estimated noise=580.96 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -2.6107e-05 Jy ! Component: 100 - total flux cleaned = -4.44696e-05 Jy ! Component: 150 - total flux cleaned = -4.43615e-05 Jy ! Component: 200 - total flux cleaned = -5.73506e-05 Jy ! Total flux subtracted in 200 components = -5.73506e-05 Jy ! Clean residual min=-0.001726 max=0.002443 Jy/beam ! Clean residual mean=0.000053 rms=0.000759 Jy/beam ! Combined flux in latest and established models = 0.278374 Jy selfcal ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 32 components and 0.278374 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.180061Jy sigma=0.001301 ! Fit after self-cal, rms=0.180074Jy sigma=0.001301 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.783% of the data. ! The x-axis pixel size should ideally be below 0.1956 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 = -1.89956e-06 Jy ! Component: 100 - total flux cleaned = -1.99842e-05 Jy ! Component: 150 - total flux cleaned = -3.35057e-05 Jy ! Component: 200 - total flux cleaned = -3.43616e-05 Jy ! Total flux subtracted in 200 components = -3.43616e-05 Jy ! Clean residual min=-0.001721 max=0.002434 Jy/beam ! Clean residual mean=0.000054 rms=0.000755 Jy/beam ! Combined flux in latest and established models = 0.278339 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 33 components and 0.278339 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.180071Jy sigma=0.001301 ! Fit after self-cal, rms=0.180070Jy sigma=0.001301 ! Inverting map ! Your choice of large map pixels excluded 0.783% of the data. ! The x-axis pixel size should ideally be below 0.1956 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 0.783% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=0.8824 mas, bmaj=2.528 mas, bpa=1.692 degrees ! Estimated noise=475.842 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8824 x 2.528 at 1.692 degrees (North through East) ! Clean map min=-0.0020379 max=0.23016 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 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 0.783% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=0.6773 mas, bmaj=1.996 mas, bpa=4.144 degrees ! Estimated noise=1012.63 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.173523 Jy ! Component: 100 - total flux cleaned = 0.218545 Jy ! Component: 150 - total flux cleaned = 0.240771 Jy ! Component: 200 - total flux cleaned = 0.253768 Jy ! Total flux subtracted in 200 components = 0.253768 Jy ! Clean residual min=-0.004906 max=0.007023 Jy/beam ! Clean residual mean=0.000103 rms=0.001676 Jy/beam ! Combined flux in latest and established models = 0.253768 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 22 model components to the UV plane model. ! The established model now contains 22 components and 0.253768 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.783% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=0.8824 mas, bmaj=2.528 mas, bpa=1.692 degrees ! Estimated noise=475.842 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 = 0.0123432 Jy ! Component: 100 - total flux cleaned = 0.0179492 Jy ! Component: 150 - total flux cleaned = 0.0206732 Jy ! Component: 200 - total flux cleaned = 0.022004 Jy ! Total flux subtracted in 200 components = 0.022004 Jy ! Clean residual min=-0.002027 max=0.002246 Jy/beam ! Clean residual mean=0.000073 rms=0.000694 Jy/beam ! Combined flux in latest and established models = 0.275772 Jy ! Adding 31 model components to the UV plane model. ! The established model now contains 49 components and 0.275772 Jy ! Inverting map ! Your choice of large map pixels excluded 0.783% of the data. ! The x-axis pixel size should ideally be below 0.1956 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 0.783% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=2.554 mas, bmaj=7.685 mas, bpa=0.1848 degrees ! Estimated noise=580.96 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00125305 Jy ! Component: 100 - total flux cleaned = 0.00141413 Jy ! Component: 150 - total flux cleaned = 0.00143998 Jy ! Component: 200 - total flux cleaned = 0.00146327 Jy ! Total flux subtracted in 200 components = 0.00146327 Jy ! Clean residual min=-0.001876 max=0.002420 Jy/beam ! Clean residual mean=0.000091 rms=0.000755 Jy/beam ! Combined flux in latest and established models = 0.277235 Jy flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.06714e-05 Jy ! Component: 100 - total flux cleaned = 3.14592e-05 Jy ! Component: 150 - total flux cleaned = 4.127e-05 Jy ! Component: 200 - total flux cleaned = 6.03841e-05 Jy ! Total flux subtracted in 200 components = 6.03841e-05 Jy ! Clean residual min=-0.001862 max=0.002421 Jy/beam ! Clean residual mean=0.000089 rms=0.000752 Jy/beam ! Combined flux in latest and established models = 0.277295 Jy ! Adding 5 model components to the UV plane model. ! The established model now contains 50 components and 0.277295 Jy ! Inverting map ! Your choice of large map pixels excluded 0.783% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.783% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! Estimated beam: bmin=0.8824 mas, bmaj=2.528 mas, bpa=1.692 degrees ! Estimated noise=475.842 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000442359 Jy ! Component: 100 - total flux cleaned = -0.000437577 Jy ! Component: 150 - total flux cleaned = -0.000407085 Jy ! Component: 200 - total flux cleaned = -0.000406575 Jy ! Total flux subtracted in 200 components = -0.000406575 Jy ! Clean residual min=-0.001934 max=0.002211 Jy/beam ! Clean residual mean=0.000051 rms=0.000671 Jy/beam ! Combined flux in latest and established models = 0.276889 Jy selfcal ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 52 components and 0.276889 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.180057Jy sigma=0.001301 ! Fit after self-cal, rms=0.180067Jy sigma=0.001301 wmodel J0904-3514_X_2010_06_23_pus_map.mod ! Writing 52 model components to file: J0904-3514_X_2010_06_23_pus_map.mod wobs J0904-3514_X_2010_06_23_pus_uvs.fits ! Writing UV FITS file: J0904-3514_X_2010_06_23_pus_uvs.fits wwins J0904-3514_X_2010_06_23_pus_map.win ! wwins: Wrote 1 windows to J0904-3514_X_2010_06_23_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 0.783% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! clean: niter=1024 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000678707 Jy ! Component: 100 - total flux cleaned = 0.000993367 Jy ! Component: 150 - total flux cleaned = 0.00108991 Jy ! Component: 200 - total flux cleaned = 0.00112072 Jy ! Component: 250 - total flux cleaned = 0.00118145 Jy ! Component: 300 - total flux cleaned = 0.00118146 Jy ! Component: 350 - total flux cleaned = 0.00126567 Jy ! Component: 400 - total flux cleaned = 0.00132039 Jy ! Component: 450 - total flux cleaned = 0.00140026 Jy ! Component: 500 - total flux cleaned = 0.00147768 Jy ! Component: 550 - total flux cleaned = 0.00155337 Jy ! Component: 600 - total flux cleaned = 0.00162714 Jy ! Component: 650 - total flux cleaned = 0.00165113 Jy ! Component: 700 - total flux cleaned = 0.00174401 Jy ! Component: 750 - total flux cleaned = 0.0017894 Jy ! Component: 800 - total flux cleaned = 0.00183366 Jy ! Component: 850 - total flux cleaned = 0.00183335 Jy ! Component: 900 - total flux cleaned = 0.00181203 Jy ! Component: 950 - total flux cleaned = 0.00181207 Jy ! Component: 1000 - total flux cleaned = 0.00181196 Jy ! Total flux subtracted in 1024 components = 0.00183211 Jy ! Clean residual min=-0.001028 max=0.001147 Jy/beam ! Clean residual mean=0.000025 rms=0.000422 Jy/beam ! Combined flux in latest and established models = 0.278721 Jy keep ! Adding 65 model components to the UV plane model. ! The established model now contains 117 components and 0.278721 Jy ![Exited script file: muppet] wmap "J0904-3514_X_2010_06_23_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.783% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8824 x 2.528 at 1.692 degrees (North through East) ! Clean map min=-0.0018 max=0.23403 Jy/beam ! Writing clean map to FITS file: J0904-3514_X_2010_06_23_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.23403 invert ! Inverting map ! Your choice of large map pixels excluded 0.783% of the data. ! The x-axis pixel size should ideally be below 0.1956 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000421524 device "J0904-3514_X_2010_06_23_pus\_map.eps/VPS" ! Attempting to open device: 'J0904-3514_X_2010_06_23_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.540346 0.540346 1.08069 2.16138 4.32277 8.64554 17.2911 34.5822 69.1643 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0012 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.234 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8824 x 2.528 at 1.692 degrees (North through East) ! Clean map min=-0.0018 max=0.23403 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0904-3514_X_2010_06_23_pus\_map.gif/vgif" ! Attempting to open device: 'J0904-3514_X_2010_06_23_pus_map.gif/vgif' mapplot cln