! Started logfile: J0605-3522_X_2002_01_31_yyk_uvs.log on Wed Jun 27 10:49:44 2007 obs J0605-3522_X_2002_01_31_yyk_uva.fits ! Reading UV FITS file: J0605-3522_X_2002_01_31_yyk_uva.fits ! AN table 1: 35 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.761905 visibilities/baseline/integration-bin. ! Found source: J0605-3522 ! ! 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 8.40947e+09 8e+06 1 8e+06 ! 02 2 8.47947e+09 8e+06 1 8e+06 ! 03 3 8.79447e+09 8e+06 1 8e+06 ! 04 4 8.89947e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 1544 lines of history. ! ! Reading 4800 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 flag NL ! Flagging baselines of antenna 1:NL in the currently selected channels. ![@muppet J0605-3522_X_2002_01_31_yyk] integer clean_niter clean_niter = 100 float clean_gain clean_gain = 0.04 float dynam dynam = 6.0 float amp_soltime1 amp_soltime1 = 10 float amp_soltime2 amp_soltime2 = 1 float phase_soltime1 phase_soltime1=10 float phase_soltime2 phase_soltime2=0.5 float phase_soltime phase_soltime=phase_soltime1 float ampcor_selflim ampcor_selflim=1.20 float thresh thresh = 0.10 float win_mult win_mult = 1.8 float time_av time_av = 30 float old_peak float new_peak float flux_cutoff mapsize field_size, field_cell ! Map grid = 512x512 pixels with 0.200x0.200 milli-arcsec cellsize. phase_soltime=phase_soltime1 print "uvstat(rms)=",uvstat(rms),"Jy" ! uvstat(rms)= 0.216974 Jy 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 0.939% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=0.6775 mas, bmaj=1.759 mas, bpa=5.359 degrees ! Estimated noise=1953.19 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (0, 0). ! clean: niter=100 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.126698 Jy ! Component: 100 - total flux cleaned = 0.150712 Jy ! Total flux subtracted in 100 components = 0.150712 Jy ! Clean residual min=-0.011032 max=0.011176 Jy/beam ! Clean residual mean=-0.000062 rms=0.003240 Jy/beam ! Combined flux in latest and established models = 0.150712 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 11 model components to the UV plane model. ! The established model now contains 11 components and 0.150712 Jy ! ! Correcting IF 1. ! A total of 78 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 78 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 78 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 78 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.153370Jy sigma=0.001209 ! Fit after self-cal, rms=0.153247Jy sigma=0.001208 ! Inverting map and beam ! Your choice of large map pixels excluded 0.939% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=0.6775 mas, bmaj=1.759 mas, bpa=5.359 degrees ! Estimated noise=1953.19 mJy/beam. print "************** FINISHED UNIFORM WEIGHTING CLEAN **************" ! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** ! uvw 0,-2 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -2. ! 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 0.939% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=0.8342 mas, bmaj=2.155 mas, bpa=2.601 degrees ! Estimated noise=1389.77 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0135296 Jy ! Component: 100 - total flux cleaned = 0.0175973 Jy ! Component: 150 - total flux cleaned = 0.0180797 Jy ! Component: 200 - total flux cleaned = 0.018348 Jy ! Total flux subtracted in 200 components = 0.018348 Jy ! Clean residual min=-0.007527 max=0.006627 Jy/beam ! Clean residual mean=0.000019 rms=0.002099 Jy/beam ! Combined flux in latest and established models = 0.16906 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 12 model components to the UV plane model. ! The established model now contains 18 components and 0.16906 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.152561Jy sigma=0.001201 ! Fit after self-cal, rms=0.152545Jy sigma=0.001201 ! Inverting map ! Your choice of large map pixels excluded 0.939% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8342 x 2.155 at 2.601 degrees (North through East) ! Clean map min=-0.0067728 max=0.1515 Jy/beam if(peak(flux) < thresh*2) selflims ampcor_selflim end if ! Selfcal amplitude corrections will be limited to 0.833333 -> 1.2. ! Selfcal phase corrections will not be limited. gscale ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 1.00243 ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.93 HN 1.00* KP 0.99 ! LA 1.12 MK 0.99 NL 1.00* OV 0.91 ! PT 1.02 SC 1.03 ! ! ! Correcting IF 2. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 1.02205 ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.94 HN 1.00* KP 0.91 ! LA 1.14 MK 0.96 NL 1.00* OV 0.89 ! PT 1.01 SC 0.95 ! ! ! Correcting IF 3. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 0.982126 ! Telescope amplitude corrections in sub-array 1: ! BR 0.95 FD 0.90 HN 1.00* KP 1.08 ! LA 1.09 MK 1.01 NL 1.00* OV 0.96 ! PT 1.07 SC 1.11 ! ! ! Correcting IF 4. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 0.986573 ! Telescope amplitude corrections in sub-array 1: ! BR 1.10 FD 0.90 HN 1.00* KP 1.12 ! LA 1.02 MK 1.04 NL 1.00* OV 0.97 ! PT 1.09 SC 0.91 ! ! ! Fit before self-cal, rms=0.152545Jy sigma=0.001201 ! Fit after self-cal, rms=0.152446Jy sigma=0.001195 selfcal false, false, phase_soltime ! Performing phase self-cal over 10 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.152446Jy sigma=0.001195 ! Fit after self-cal, rms=0.152448Jy sigma=0.001195 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.915% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=0.8367 mas, bmaj=2.157 mas, bpa=2.774 degrees ! Estimated noise=1378.56 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -0.000129252 Jy ! Component: 100 - total flux cleaned = 7.66463e-05 Jy ! Component: 150 - total flux cleaned = 0.000199768 Jy ! Component: 200 - total flux cleaned = 0.000254385 Jy ! Total flux subtracted in 200 components = 0.000254385 Jy ! Clean residual min=-0.005600 max=0.004934 Jy/beam ! Clean residual mean=-0.000027 rms=0.001470 Jy/beam ! Combined flux in latest and established models = 0.169314 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 7 model components to the UV plane model. ! The established model now contains 21 components and 0.169314 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.152420Jy sigma=0.001194 ! Fit after self-cal, rms=0.152406Jy sigma=0.001194 ! Inverting map ! Your choice of large map pixels excluded 0.915% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec print "************** FINISHED AMPLITUDE GSCALE SELF-CAL **************" ! ************** FINISHED AMPLITUDE GSCALE SELF-CAL ************** ! phase_soltime=phase_soltime2 selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.152406Jy sigma=0.001194 ! Fit after self-cal, rms=0.150293Jy sigma=0.001178 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.915% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000211509 Jy ! Component: 100 - total flux cleaned = 0.000408062 Jy ! Component: 150 - total flux cleaned = 0.000574956 Jy ! Component: 200 - total flux cleaned = 0.000770715 Jy ! Total flux subtracted in 200 components = 0.000770715 Jy ! Clean residual min=-0.005623 max=0.004827 Jy/beam ! Clean residual mean=-0.000029 rms=0.001454 Jy/beam ! Combined flux in latest and established models = 0.170085 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 11 model components to the UV plane model. ! The established model now contains 25 components and 0.170085 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.150253Jy sigma=0.001178 ! Fit after self-cal, rms=0.149954Jy sigma=0.001176 ! Inverting map ! Your choice of large map pixels excluded 0.915% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec print "*** FINISHED NATURAL WEIGHTING CLEAN with shorter phase_soltime ***" ! *** FINISHED NATURAL WEIGHTING CLEAN with shorter phase_soltime *** ! dynam = dynam - 0.25 restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8367 x 2.157 at 2.774 degrees (North through East) ! Clean map min=-0.0051612 max=0.15218 Jy/beam if(peak(flux) > thresh) selfcal true, true, amp_soltime1 selfcal false, false, phase_soltime 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 false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) selfcal true, true, amp_soltime2 selfcal false, false, phase_soltime 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 false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) print "************** FINISHED AMPLITUDE SELF-CAL **************" end if ! Performing amp+phase self-cal over 10 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.149954Jy sigma=0.001176 ! Fit after self-cal, rms=0.150233Jy sigma=0.001175 ! Performing phase self-cal over 0.5 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.150233Jy sigma=0.001175 ! Fit after self-cal, rms=0.150144Jy sigma=0.001174 ! Inverting map and beam ! Your choice of large map pixels excluded 0.915% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=0.8299 mas, bmaj=2.148 mas, bpa=3.083 degrees ! Estimated noise=1371.53 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000267886 Jy ! Component: 100 - total flux cleaned = 0.000312109 Jy ! Component: 150 - total flux cleaned = 0.000356306 Jy ! Component: 200 - total flux cleaned = 0.000437771 Jy ! Total flux subtracted in 200 components = 0.000437771 Jy ! Clean residual min=-0.005457 max=0.005060 Jy/beam ! Clean residual mean=-0.000029 rms=0.001422 Jy/beam ! Combined flux in latest and established models = 0.170522 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 8 model components to the UV plane model. ! The established model now contains 26 components and 0.170522 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.150131Jy sigma=0.001174 ! Fit after self-cal, rms=0.150089Jy sigma=0.001174 ! Inverting map ! Your choice of large map pixels excluded 0.915% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Performing amp+phase self-cal over 1 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.150089Jy sigma=0.001174 ! Fit after self-cal, rms=0.149807Jy sigma=0.001173 ! Performing phase self-cal over 0.5 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.149807Jy sigma=0.001173 ! Fit after self-cal, rms=0.149790Jy sigma=0.001172 ! Inverting map and beam ! Your choice of large map pixels excluded 0.915% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=0.8234 mas, bmaj=2.135 mas, bpa=3.402 degrees ! Estimated noise=1363.39 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -5.84076e-05 Jy ! Component: 100 - total flux cleaned = 2.63506e-05 Jy ! Component: 150 - total flux cleaned = 9.9182e-05 Jy ! Component: 200 - total flux cleaned = 0.000134338 Jy ! Total flux subtracted in 200 components = 0.000134338 Jy ! Clean residual min=-0.005099 max=0.005269 Jy/beam ! Clean residual mean=-0.000021 rms=0.001372 Jy/beam ! Combined flux in latest and established models = 0.170657 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 11 model components to the UV plane model. ! The established model now contains 28 components and 0.170657 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.149780Jy sigma=0.001172 ! Fit after self-cal, rms=0.149773Jy sigma=0.001172 ! Inverting map ! Your choice of large map pixels excluded 0.915% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! ************** FINISHED AMPLITUDE SELF-CAL ************** uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. win_mult = win_mult * 1.4 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.915% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=2.871 mas, bmaj=9.438 mas, bpa=9.688 degrees ! Estimated noise=1773.21 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal false,false,phase_soltime new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000232709 Jy ! Component: 100 - total flux cleaned = 0.000229367 Jy ! Component: 150 - total flux cleaned = 0.000227378 Jy ! Component: 200 - total flux cleaned = 0.00026637 Jy ! Total flux subtracted in 200 components = 0.00026637 Jy ! Clean residual min=-0.005680 max=0.005015 Jy/beam ! Clean residual mean=-0.000039 rms=0.001841 Jy/beam ! Combined flux in latest and established models = 0.170923 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 6 model components to the UV plane model. ! The established model now contains 32 components and 0.170923 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.149784Jy sigma=0.001172 ! Fit after self-cal, rms=0.149780Jy sigma=0.001172 ! Inverting map ! Your choice of large map pixels excluded 0.915% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec uvtaper 0 ! No UV-taper is currently set. win_mult = win_mult / 1.4 print "************** FINISHED TAPERING SELF-CAL CLEAN **************" ! ************** FINISHED TAPERING SELF-CAL CLEAN ************** ! print "************** CLEARING MODEL AND STARTING OVER **********" ! ************** CLEARING MODEL AND STARTING OVER ********** clrmod true,true,true ! clrmod: Cleared the established, tentative and continuum 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 0.915% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=0.675 mas, bmaj=1.757 mas, bpa=5.591 degrees ! Estimated noise=1916.59 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.127035 Jy ! Component: 100 - total flux cleaned = 0.150401 Jy ! Component: 150 - total flux cleaned = 0.160933 Jy ! Component: 200 - total flux cleaned = 0.166383 Jy ! Total flux subtracted in 200 components = 0.166383 Jy ! Clean residual min=-0.008942 max=0.008264 Jy/beam ! Clean residual mean=-0.000033 rms=0.002387 Jy/beam ! Combined flux in latest and established models = 0.166383 Jy uvw 0,-2 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -2. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Adding 14 model components to the UV plane model. ! The established model now contains 14 components and 0.166383 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.915% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=0.8234 mas, bmaj=2.135 mas, bpa=3.402 degrees ! Estimated noise=1363.39 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=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.00397769 Jy ! Component: 100 - total flux cleaned = 0.00397578 Jy ! Component: 150 - total flux cleaned = 0.00412616 Jy ! Component: 200 - total flux cleaned = 0.00425979 Jy ! Total flux subtracted in 200 components = 0.00425979 Jy ! Clean residual min=-0.005279 max=0.005335 Jy/beam ! Clean residual mean=-0.000022 rms=0.001426 Jy/beam ! Combined flux in latest and established models = 0.170642 Jy ! Adding 11 model components to the UV plane model. ! The established model now contains 21 components and 0.170642 Jy ! Inverting map ! Your choice of large map pixels excluded 0.915% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.915% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=2.871 mas, bmaj=9.438 mas, bpa=9.688 degrees ! Estimated noise=1773.21 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=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000689394 Jy ! Component: 100 - total flux cleaned = 0.000689325 Jy ! Component: 150 - total flux cleaned = 0.000687982 Jy ! Component: 200 - total flux cleaned = 0.000702928 Jy ! Total flux subtracted in 200 components = 0.000702928 Jy ! Clean residual min=-0.005584 max=0.004991 Jy/beam ! Clean residual mean=-0.000036 rms=0.001839 Jy/beam ! Combined flux in latest and established models = 0.171345 Jy ! Adding 5 model components to the UV plane model. ! The established model now contains 25 components and 0.171345 Jy ! Inverting map ! Your choice of large map pixels excluded 0.915% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec uvtaper 0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.915% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! Estimated beam: bmin=0.8234 mas, bmaj=2.135 mas, bpa=3.402 degrees ! Estimated noise=1363.39 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -0.000119501 Jy ! Component: 100 - total flux cleaned = -6.12206e-06 Jy ! Component: 150 - total flux cleaned = -6.17826e-06 Jy ! Component: 200 - total flux cleaned = -4.93804e-06 Jy ! Total flux subtracted in 200 components = -4.93804e-06 Jy ! Clean residual min=-0.005239 max=0.005204 Jy/beam ! Clean residual mean=-0.000018 rms=0.001403 Jy/beam ! Combined flux in latest and established models = 0.17134 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 11 model components to the UV plane model. ! The established model now contains 30 components and 0.17134 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.149811Jy sigma=0.001173 ! Fit after self-cal, rms=0.149807Jy sigma=0.001173 wmodel J0605-3522_X_2002_01_31_yyk\_map.mod ! Writing 30 model components to file: J0605-3522_X_2002_01_31_yyk_map.mod wobs J0605-3522_X_2002_01_31_yyk\_uvs.fits ! Applying 35 buffered edits. ! Writing UV FITS file: J0605-3522_X_2002_01_31_yyk_uvs.fits wwins J0605-3522_X_2002_01_31_yyk\_map.win ! wwins: Wrote 1 windows to J0605-3522_X_2002_01_31_yyk_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 0.915% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -8.65252e-05 Jy ! Component: 100 - total flux cleaned = 0.000220918 Jy ! Component: 150 - total flux cleaned = 0.000916321 Jy ! Component: 200 - total flux cleaned = 0.00123928 Jy ! Component: 250 - total flux cleaned = 0.00130046 Jy ! Component: 300 - total flux cleaned = 0.00141451 Jy ! Component: 350 - total flux cleaned = 0.0015184 Jy ! Component: 400 - total flux cleaned = 0.00172031 Jy ! Component: 450 - total flux cleaned = 0.00201223 Jy ! Component: 500 - total flux cleaned = 0.00229139 Jy ! Component: 550 - total flux cleaned = 0.00260407 Jy ! Component: 600 - total flux cleaned = 0.00295131 Jy ! Component: 650 - total flux cleaned = 0.00332861 Jy ! Component: 700 - total flux cleaned = 0.0035715 Jy ! Component: 750 - total flux cleaned = 0.00380789 Jy ! Component: 800 - total flux cleaned = 0.00403836 Jy ! Component: 850 - total flux cleaned = 0.00433669 Jy ! Component: 900 - total flux cleaned = 0.00448254 Jy ! Component: 950 - total flux cleaned = 0.00476634 Jy ! Component: 1000 - total flux cleaned = 0.00487036 Jy ! Component: 1050 - total flux cleaned = 0.00504094 Jy ! Component: 1100 - total flux cleaned = 0.00517449 Jy ! Component: 1150 - total flux cleaned = 0.00536982 Jy ! Component: 1200 - total flux cleaned = 0.00540167 Jy ! Component: 1250 - total flux cleaned = 0.00546435 Jy ! Component: 1300 - total flux cleaned = 0.00549552 Jy ! Component: 1350 - total flux cleaned = 0.00558629 Jy ! Component: 1400 - total flux cleaned = 0.00561609 Jy ! Component: 1450 - total flux cleaned = 0.00573281 Jy ! Component: 1500 - total flux cleaned = 0.00587682 Jy ! Component: 1550 - total flux cleaned = 0.00596167 Jy ! Component: 1600 - total flux cleaned = 0.00604574 Jy ! Component: 1650 - total flux cleaned = 0.00610112 Jy ! Component: 1700 - total flux cleaned = 0.0062376 Jy ! Component: 1750 - total flux cleaned = 0.00631844 Jy ! Component: 1800 - total flux cleaned = 0.00631832 Jy ! Component: 1850 - total flux cleaned = 0.00637109 Jy ! Component: 1900 - total flux cleaned = 0.00639738 Jy ! Component: 1950 - total flux cleaned = 0.00650206 Jy ! Component: 2000 - total flux cleaned = 0.00652794 Jy ! Total flux subtracted in 2048 components = 0.0066571 Jy ! Clean residual min=-0.001418 max=0.001514 Jy/beam ! Clean residual mean=-0.000001 rms=0.000494 Jy/beam ! Combined flux in latest and established models = 0.177997 Jy keep ! Adding 116 model components to the UV plane model. ! The established model now contains 146 components and 0.177997 Jy ![Exited script file: muppet] wmap "J0605-3522_X_2002_01_31_yyk\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.915% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8234 x 2.135 at 3.402 degrees (North through East) ! Clean map min=-0.0035897 max=0.14502 Jy/beam ! Writing clean map to FITS file: J0605-3522_X_2002_01_31_yyk_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.145023 invert ! Inverting map ! Your choice of large map pixels excluded 0.915% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000480849 device "J0605-3522_X_2002_01_31_yyk\_map.eps/VPS" ! Attempting to open device: 'J0605-3522_X_2002_01_31_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.994704 0.994704 1.98941 3.97882 7.95764 15.9153 31.8305 63.6611 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0014 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.145 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8234 x 2.135 at 3.402 degrees (North through East) ! Clean map min=-0.0035897 max=0.14502 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0605-3522_X_2002_01_31_yyk\_map.gif/gif" ! Attempting to open device: 'J0605-3522_X_2002_01_31_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J0605-3522_X_2002_01_31_yyk_uvs.log closed on Wed Jun 27 10:49:51 2007