! Started logfile: J0945-0153_X_2005_06_30_yyk_uvs.log on Sat Oct 8 17:13:57 2005 obs J0945-0153_X_2005_06_30_yyk_uve.fits ! Reading UV FITS file: J0945-0153_X_2005_06_30_yyk_uve.fits ! AN table 1: 18 integrations on 45 of 45 possible baselines. ! Apparent sampling: 1 visibilities/baseline/integration-bin. ! Found source: J0945-0153 ! ! 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 8.40997e+09 8e+06 1 8e+06 ! 02 2 8.47997e+09 8e+06 1 8e+06 ! 03 3 8.79497e+09 8e+06 1 8e+06 ! 04 4 8.89997e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 1460 lines of history. ! ! Reading 3240 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 ![@muppet J0945-0153_X_2005_06_30_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)= 0.116906 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 0.288% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=0.7102 mas, bmaj=1.789 mas, bpa=-0.167 degrees ! Estimated noise=0.960897 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 = 0.0806915 Jy ! Component: 100 - total flux cleaned = 0.0999613 Jy ! Total flux subtracted in 100 components = 0.0999613 Jy ! Clean residual min=-0.005513 max=0.006409 Jy/beam ! Clean residual mean=0.000008 rms=0.001414 Jy/beam ! Combined flux in latest and established models = 0.0999613 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 18 model components to the UV plane model. ! The established model now contains 18 components and 0.0999613 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! A total of 8 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.060883Jy sigma=1.073776 ! Fit after self-cal, rms=0.060015Jy sigma=1.066855 ! Inverting map and beam ! Your choice of large map pixels excluded 0.288% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=0.7102 mas, bmaj=1.789 mas, bpa=-0.167 degrees ! Estimated noise=0.960897 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 0.288% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=0.874 mas, bmaj=2.127 mas, bpa=-0.7211 degrees ! Estimated noise=0.653752 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 = 0.0122514 Jy ! Component: 100 - total flux cleaned = 0.0171531 Jy ! Component: 150 - total flux cleaned = 0.0194614 Jy ! Component: 200 - total flux cleaned = 0.020639 Jy ! Total flux subtracted in 200 components = 0.020639 Jy ! Clean residual min=-0.003445 max=0.004585 Jy/beam ! Clean residual mean=0.000005 rms=0.000770 Jy/beam ! Combined flux in latest and established models = 0.1206 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 39 model components to the UV plane model. ! The established model now contains 47 components and 0.1206 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.058457Jy sigma=1.032695 ! Fit after self-cal, rms=0.058431Jy sigma=1.032277 ! Inverting map ! Your choice of large map pixels excluded 0.288% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Added new window around map position (0.8, 3.6). ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.00413963 Jy ! Component: 100 - total flux cleaned = 0.00447365 Jy ! Component: 150 - total flux cleaned = 0.0045701 Jy ! Component: 200 - total flux cleaned = 0.00461393 Jy ! Total flux subtracted in 200 components = 0.00461393 Jy ! Clean residual min=-0.003075 max=0.002611 Jy/beam ! Clean residual mean=0.000005 rms=0.000689 Jy/beam ! Combined flux in latest and established models = 0.125214 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 32 model components to the UV plane model. ! The established model now contains 77 components and 0.125214 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.058181Jy sigma=1.027328 ! Fit after self-cal, rms=0.058151Jy sigma=1.026897 ! Inverting map ! Your choice of large map pixels excluded 0.288% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.874 x 2.127 at -0.7211 degrees (North through East) ! Clean map min=-0.0028296 max=0.098096 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. ! Amplitude normalization factor in sub-array 1: 1.0066 ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.95 HN 1.03 KP 0.95 ! LA 1.02 MK 1.04 NL 1.00 OV 1.04 ! PT 0.98 SC 0.97 ! ! ! Correcting IF 2. ! Amplitude normalization factor in sub-array 1: 1.02072 ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 1.02 HN 1.05 KP 0.93 ! LA 0.94 MK 0.94 NL 1.01 OV 0.98 ! PT 0.95 SC 0.93 ! ! ! Correcting IF 3. ! Amplitude normalization factor in sub-array 1: 1.02059 ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 FD 1.00 HN 0.93 KP 0.89 ! LA 1.00 MK 0.93 NL 0.98 OV 1.07 ! PT 1.08 SC 0.95 ! ! ! Correcting IF 4. ! Amplitude normalization factor in sub-array 1: 1 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* HN 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ! ! ! Fit before self-cal, rms=0.058151Jy sigma=1.026897 ! Fit after self-cal, rms=0.057799Jy sigma=1.021158 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=0.057799Jy sigma=1.021158 ! Fit after self-cal, rms=0.057794Jy sigma=1.020980 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.288% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=0.8647 mas, bmaj=2.108 mas, bpa=-0.2971 degrees ! Estimated noise=0.65227 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 = 0.000815468 Jy ! Component: 100 - total flux cleaned = 0.000815619 Jy ! Component: 150 - total flux cleaned = 0.000723141 Jy ! Component: 200 - total flux cleaned = 0.000664818 Jy ! Total flux subtracted in 200 components = 0.000664818 Jy ! Clean residual min=-0.002808 max=0.002175 Jy/beam ! Clean residual mean=0.000005 rms=0.000586 Jy/beam ! Combined flux in latest and established models = 0.125879 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 22 model components to the UV plane model. ! The established model now contains 93 components and 0.125879 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.057755Jy sigma=1.020355 ! Fit after self-cal, rms=0.057749Jy sigma=1.020193 ! Inverting map ! Your choice of large map pixels excluded 0.288% of the data. ! The x-axis pixel size should ideally be below 0.1993 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=0.057749Jy sigma=1.020193 ! Fit after self-cal, rms=0.054979Jy sigma=0.967648 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.288% of the data. ! The x-axis pixel size should ideally be below 0.1993 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 = 0.000951821 Jy ! Component: 100 - total flux cleaned = 0.000886644 Jy ! Component: 150 - total flux cleaned = 0.000862331 Jy ! Component: 200 - total flux cleaned = 0.000841347 Jy ! Total flux subtracted in 200 components = 0.000841347 Jy ! Clean residual min=-0.002595 max=0.002021 Jy/beam ! Clean residual mean=0.000005 rms=0.000560 Jy/beam ! Combined flux in latest and established models = 0.12672 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 23 model components to the UV plane model. ! The established model now contains 106 components and 0.12672 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.054934Jy sigma=0.967005 ! Fit after self-cal, rms=0.054660Jy sigma=0.963036 ! Inverting map ! Your choice of large map pixels excluded 0.288% of the data. ! The x-axis pixel size should ideally be below 0.1993 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: 0.8647 x 2.108 at -0.2971 degrees (North through East) ! Clean map min=-0.0024084 max=0.0995 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 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 0.288% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=2.199 mas, bmaj=3.651 mas, bpa=4.715 degrees ! Estimated noise=0.840666 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 = -0.000585529 Jy ! Component: 100 - total flux cleaned = -0.000586358 Jy ! Component: 150 - total flux cleaned = -0.000671918 Jy ! Component: 200 - total flux cleaned = -0.00072277 Jy ! Total flux subtracted in 200 components = -0.00072277 Jy ! Clean residual min=-0.002077 max=0.001934 Jy/beam ! Clean residual mean=0.000011 rms=0.000677 Jy/beam ! Combined flux in latest and established models = 0.125998 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 21 model components to the UV plane model. ! The established model now contains 119 components and 0.125998 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.054661Jy sigma=0.962964 ! Fit after self-cal, rms=0.054633Jy sigma=0.962564 ! Inverting map ! Your choice of large map pixels excluded 0.288% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec uvtaper 0,0 ! 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 0.288% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=0.7068 mas, bmaj=1.783 mas, bpa=-0.02905 degrees ! Estimated noise=0.955842 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.083304 Jy ! Component: 100 - total flux cleaned = 0.102124 Jy ! Component: 150 - total flux cleaned = 0.1113 Jy ! Component: 200 - total flux cleaned = 0.116801 Jy ! Total flux subtracted in 200 components = 0.116801 Jy ! Clean residual min=-0.002978 max=0.003551 Jy/beam ! Clean residual mean=0.000005 rms=0.000804 Jy/beam ! Combined flux in latest and established models = 0.116801 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 38 model components to the UV plane model. ! The established model now contains 38 components and 0.116801 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.288% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=0.8647 mas, bmaj=2.108 mas, bpa=-0.2971 degrees ! Estimated noise=0.65227 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 = 0.00522295 Jy ! Component: 100 - total flux cleaned = 0.0078517 Jy ! Component: 150 - total flux cleaned = 0.00905208 Jy ! Component: 200 - total flux cleaned = 0.00935662 Jy ! Total flux subtracted in 200 components = 0.00935662 Jy ! Clean residual min=-0.002685 max=0.002276 Jy/beam ! Clean residual mean=0.000005 rms=0.000570 Jy/beam ! Combined flux in latest and established models = 0.126158 Jy ! Adding 37 model components to the UV plane model. ! The established model now contains 66 components and 0.126158 Jy ! Inverting map ! Your choice of large map pixels excluded 0.288% of the data. ! The x-axis pixel size should ideally be below 0.1993 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 0.288% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=2.199 mas, bmaj=3.651 mas, bpa=4.715 degrees ! Estimated noise=0.840666 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 = 0.000167774 Jy ! Component: 100 - total flux cleaned = 7.37588e-05 Jy ! Component: 150 - total flux cleaned = 1.4239e-08 Jy ! Component: 200 - total flux cleaned = -6.39641e-05 Jy ! Total flux subtracted in 200 components = -6.39641e-05 Jy ! Clean residual min=-0.002177 max=0.001938 Jy/beam ! Clean residual mean=0.000011 rms=0.000691 Jy/beam ! Combined flux in latest and established models = 0.126094 Jy ! Adding 30 model components to the UV plane model. ! The established model now contains 92 components and 0.126094 Jy ! Inverting map ! Your choice of large map pixels excluded 0.288% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.288% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! Estimated beam: bmin=0.8647 mas, bmaj=2.108 mas, bpa=-0.2971 degrees ! Estimated noise=0.65227 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000364127 Jy ! Component: 100 - total flux cleaned = 0.000425767 Jy ! Component: 150 - total flux cleaned = 0.000453049 Jy ! Component: 200 - total flux cleaned = 0.000477469 Jy ! Total flux subtracted in 200 components = 0.000477469 Jy ! Clean residual min=-0.002600 max=0.002024 Jy/beam ! Clean residual mean=0.000005 rms=0.000553 Jy/beam ! Combined flux in latest and established models = 0.126571 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 18 model components to the UV plane model. ! The established model now contains 105 components and 0.126571 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.054637Jy sigma=0.962709 ! Fit after self-cal, rms=0.054635Jy sigma=0.962651 wmodel J0945-0153_X_2005_06_30_yyk\_map.mod ! Writing 105 model components to file: J0945-0153_X_2005_06_30_yyk_map.mod wobs J0945-0153_X_2005_06_30_yyk\_uvs.fits ! Writing UV FITS file: J0945-0153_X_2005_06_30_yyk_uvs.fits wwins J0945-0153_X_2005_06_30_yyk\_map.win ! wwins: Wrote 2 windows to J0945-0153_X_2005_06_30_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 0.288% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000977374 Jy ! Component: 100 - total flux cleaned = -0.00124006 Jy ! Component: 150 - total flux cleaned = -0.00113675 Jy ! Component: 200 - total flux cleaned = -0.00100663 Jy ! Component: 250 - total flux cleaned = -0.000913116 Jy ! Component: 300 - total flux cleaned = -0.000913506 Jy ! Component: 350 - total flux cleaned = -0.000883858 Jy ! Component: 400 - total flux cleaned = -0.000970246 Jy ! Component: 450 - total flux cleaned = -0.00110961 Jy ! Component: 500 - total flux cleaned = -0.00119029 Jy ! Component: 550 - total flux cleaned = -0.00121625 Jy ! Component: 600 - total flux cleaned = -0.00119054 Jy ! Component: 650 - total flux cleaned = -0.00136836 Jy ! Component: 700 - total flux cleaned = -0.00139322 Jy ! Component: 750 - total flux cleaned = -0.00144206 Jy ! Component: 800 - total flux cleaned = -0.00141776 Jy ! Component: 850 - total flux cleaned = -0.00141786 Jy ! Component: 900 - total flux cleaned = -0.00146422 Jy ! Component: 950 - total flux cleaned = -0.00148683 Jy ! Component: 1000 - total flux cleaned = -0.001509 Jy ! Component: 1050 - total flux cleaned = -0.00148662 Jy ! Component: 1100 - total flux cleaned = -0.00146433 Jy ! Component: 1150 - total flux cleaned = -0.00144294 Jy ! Component: 1200 - total flux cleaned = -0.00148593 Jy ! Component: 1250 - total flux cleaned = -0.00146502 Jy ! Component: 1300 - total flux cleaned = -0.00144405 Jy ! Component: 1350 - total flux cleaned = -0.00148563 Jy ! Component: 1400 - total flux cleaned = -0.00146453 Jy ! Component: 1450 - total flux cleaned = -0.00140343 Jy ! Component: 1500 - total flux cleaned = -0.00136322 Jy ! Component: 1550 - total flux cleaned = -0.00142282 Jy ! Component: 1600 - total flux cleaned = -0.00140317 Jy ! Component: 1650 - total flux cleaned = -0.00134476 Jy ! Component: 1700 - total flux cleaned = -0.00136424 Jy ! Component: 1750 - total flux cleaned = -0.00142126 Jy ! Component: 1800 - total flux cleaned = -0.00144008 Jy ! Component: 1850 - total flux cleaned = -0.0014213 Jy ! Component: 1900 - total flux cleaned = -0.00142117 Jy ! Component: 1950 - total flux cleaned = -0.00142125 Jy ! Component: 2000 - total flux cleaned = -0.00145773 Jy ! Total flux subtracted in 2048 components = -0.00145752 Jy ! Clean residual min=-0.000964 max=0.001436 Jy/beam ! Clean residual mean=0.000003 rms=0.000349 Jy/beam ! Combined flux in latest and established models = 0.125114 Jy keep ! Adding 142 model components to the UV plane model. ! The established model now contains 247 components and 0.125114 Jy ![Exited script file: muppet] wmap "J0945-0153_X_2005_06_30_yyk\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.288% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8647 x 2.108 at -0.2971 degrees (North through East) ! Clean map min=-0.0023203 max=0.099961 Jy/beam ! Writing clean map to FITS file: J0945-0153_X_2005_06_30_yyk_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0999612 invert ! Inverting map ! Your choice of large map pixels excluded 0.288% of the data. ! The x-axis pixel size should ideally be below 0.1993 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000346335 device "J0945-0153_X_2005_06_30_yyk\_map.eps/VPS" ! Attempting to open device: 'J0945-0153_X_2005_06_30_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -1.03941 1.03941 2.07882 4.15764 8.31527 16.6305 33.2611 66.5222 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.001 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.099 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8647 x 2.108 at -0.2971 degrees (North through East) ! Clean map min=-0.0023203 max=0.099961 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0945-0153_X_2005_06_30_yyk\_map.gif/gif" ! Attempting to open device: 'J0945-0153_X_2005_06_30_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J0945-0153_X_2005_06_30_yyk_uvs.log closed on Sat Oct 8 17:14:01 2005