! Started logfile: J2339-2310_X_2005_07_09_yyk_uvs.log on Fri Jan 20 11:11:44 2006 obs J2339-2310_X_2005_07_09_yyk_uve.fits ! Reading UV FITS file: J2339-2310_X_2005_07_09_yyk_uve.fits ! AN table 1: 11 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.929293 visibilities/baseline/integration-bin. ! Found source: J2339-2310 ! ! 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 1480 lines of history. ! ! Reading 1840 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 J2339-2310_X_2005_07_09_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)= 0.109311 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 0.228% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.7131 mas, bmaj=1.783 mas, bpa=7.392 degrees ! Estimated noise=1.78672 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 = 0.0700455 Jy ! Component: 100 - total flux cleaned = 0.0867716 Jy ! Total flux subtracted in 100 components = 0.0867716 Jy ! Clean residual min=-0.007973 max=0.009140 Jy/beam ! Clean residual mean=-0.000002 rms=0.002215 Jy/beam ! Combined flux in latest and established models = 0.0867716 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 0.0867716 Jy ! ! Correcting IF 1. ! A total of 14 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 23 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 16 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 14 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.066882Jy sigma=1.102697 ! Fit after self-cal, rms=0.063655Jy sigma=1.055302 ! Inverting map and beam ! Your choice of large map pixels excluded 0.228% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.7131 mas, bmaj=1.783 mas, bpa=7.392 degrees ! Estimated noise=1.78672 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 0.228% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=1.043 mas, bmaj=2.755 mas, bpa=15.1 degrees ! Estimated noise=1.04937 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 = 0.0130394 Jy ! Component: 100 - total flux cleaned = 0.0164901 Jy ! Component: 150 - total flux cleaned = 0.0172993 Jy ! Component: 200 - total flux cleaned = 0.0173602 Jy ! Total flux subtracted in 200 components = 0.0173602 Jy ! Clean residual min=-0.005214 max=0.005439 Jy/beam ! Clean residual mean=0.000017 rms=0.001358 Jy/beam ! Combined flux in latest and established models = 0.104132 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 15 model components to the UV plane model. ! The established model now contains 28 components and 0.104132 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.062675Jy sigma=1.019801 ! Fit after self-cal, rms=0.062654Jy sigma=1.019621 ! Inverting map ! Your choice of large map pixels excluded 0.228% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.043 x 2.755 at 15.1 degrees (North through East) ! Clean map min=-0.0051699 max=0.086884 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: 1.0374 ! Telescope amplitude corrections in sub-array 1: ! BR 0.90 FD 0.96 HN 1.00* KP 0.96 ! LA 0.96 MK 0.85 NL 1.11 OV 1.00 ! PT 0.96 SC 0.95 ! ! ! Correcting IF 2. ! Amplitude normalization factor in sub-array 1: 0.999649 ! Telescope amplitude corrections in sub-array 1: ! BR 1.06 FD 1.01 HN 1.00* KP 0.95 ! LA 0.98 MK 1.00* NL 1.19 OV 0.94 ! PT 0.94 SC 0.93 ! ! ! Correcting IF 3. ! 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* ! ! ! 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=0.062654Jy sigma=1.019621 ! Fit after self-cal, rms=0.062391Jy sigma=1.013610 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=0.062391Jy sigma=1.013610 ! Fit after self-cal, rms=0.062388Jy sigma=1.013539 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.228% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=1.015 mas, bmaj=2.676 mas, bpa=14.67 degrees ! Estimated noise=1.04141 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 = 0.000541706 Jy ! Component: 100 - total flux cleaned = 0.000476237 Jy ! Component: 150 - total flux cleaned = 0.000393667 Jy ! Component: 200 - total flux cleaned = 0.000341971 Jy ! Total flux subtracted in 200 components = 0.000341971 Jy ! Clean residual min=-0.004666 max=0.004922 Jy/beam ! Clean residual mean=0.000021 rms=0.001235 Jy/beam ! Combined flux in latest and established models = 0.104474 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 14 model components to the UV plane model. ! The established model now contains 36 components and 0.104474 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.062320Jy sigma=1.012921 ! Fit after self-cal, rms=0.062314Jy sigma=1.012831 ! Inverting map ! Your choice of large map pixels excluded 0.228% of the data. ! The x-axis pixel size should ideally be below 0.1987 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=0.062314Jy sigma=1.012831 ! Fit after self-cal, rms=0.057011Jy sigma=0.935712 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.228% of the data. ! The x-axis pixel size should ideally be below 0.1987 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 = 0.00157828 Jy ! Component: 100 - total flux cleaned = 0.00166982 Jy ! Component: 150 - total flux cleaned = 0.00170636 Jy ! Component: 200 - total flux cleaned = 0.00170716 Jy ! Total flux subtracted in 200 components = 0.00170716 Jy ! Clean residual min=-0.004681 max=0.004412 Jy/beam ! Clean residual mean=0.000023 rms=0.001200 Jy/beam ! Combined flux in latest and established models = 0.106181 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 41 components and 0.106181 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.056989Jy sigma=0.934091 ! Fit after self-cal, rms=0.056323Jy sigma=0.928736 ! Inverting map ! Your choice of large map pixels excluded 0.228% of the data. ! The x-axis pixel size should ideally be below 0.1987 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: 1.015 x 2.676 at 14.67 degrees (North through East) ! Clean map min=-0.0043754 max=0.088653 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 0.228% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=2.639 mas, bmaj=6.744 mas, bpa=13.65 degrees ! Estimated noise=1.23183 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 = 0.000738538 Jy ! Component: 100 - total flux cleaned = 0.000737196 Jy ! Component: 150 - total flux cleaned = 0.000735997 Jy ! Component: 200 - total flux cleaned = 0.000735168 Jy ! Total flux subtracted in 200 components = 0.000735168 Jy ! Clean residual min=-0.004817 max=0.004296 Jy/beam ! Clean residual mean=0.000039 rms=0.001383 Jy/beam ! Combined flux in latest and established models = 0.106916 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 5 model components to the UV plane model. ! The established model now contains 43 components and 0.106916 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.056353Jy sigma=0.928883 ! Fit after self-cal, rms=0.056193Jy sigma=0.927786 ! Inverting map ! Your choice of large map pixels excluded 0.228% of the data. ! The x-axis pixel size should ideally be below 0.1987 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 0.228% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.7056 mas, bmaj=1.768 mas, bpa=7.096 degrees ! Estimated noise=1.75795 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0747257 Jy ! Component: 100 - total flux cleaned = 0.0920857 Jy ! Component: 150 - total flux cleaned = 0.0986342 Jy ! Component: 200 - total flux cleaned = 0.10167 Jy ! Total flux subtracted in 200 components = 0.10167 Jy ! Clean residual min=-0.006933 max=0.005862 Jy/beam ! Clean residual mean=0.000009 rms=0.001698 Jy/beam ! Combined flux in latest and established models = 0.10167 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 25 model components to the UV plane model. ! The established model now contains 25 components and 0.10167 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.228% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=1.015 mas, bmaj=2.676 mas, bpa=14.67 degrees ! Estimated noise=1.04141 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 = 0.00356403 Jy ! Component: 100 - total flux cleaned = 0.00377188 Jy ! Component: 150 - total flux cleaned = 0.00384782 Jy ! Component: 200 - total flux cleaned = 0.00384836 Jy ! Total flux subtracted in 200 components = 0.00384836 Jy ! Clean residual min=-0.004748 max=0.004413 Jy/beam ! Clean residual mean=0.000022 rms=0.001206 Jy/beam ! Combined flux in latest and established models = 0.105519 Jy ! Adding 13 model components to the UV plane model. ! The established model now contains 35 components and 0.105519 Jy ! Inverting map ! Your choice of large map pixels excluded 0.228% of the data. ! The x-axis pixel size should ideally be below 0.1987 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 0.228% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=2.639 mas, bmaj=6.744 mas, bpa=13.65 degrees ! Estimated noise=1.23183 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 = 0.000869599 Jy ! Component: 100 - total flux cleaned = 0.000869524 Jy ! Component: 150 - total flux cleaned = 0.000870185 Jy ! Component: 200 - total flux cleaned = 0.000870753 Jy ! Total flux subtracted in 200 components = 0.000870753 Jy ! Clean residual min=-0.004807 max=0.004314 Jy/beam ! Clean residual mean=0.000038 rms=0.001384 Jy/beam ! Combined flux in latest and established models = 0.10639 Jy ! Adding 3 model components to the UV plane model. ! The established model now contains 35 components and 0.10639 Jy ! Inverting map ! Your choice of large map pixels excluded 0.228% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec uvtaper 0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.228% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=1.015 mas, bmaj=2.676 mas, bpa=14.67 degrees ! Estimated noise=1.04141 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -0.000646744 Jy ! Component: 100 - total flux cleaned = -0.000574117 Jy ! Component: 150 - total flux cleaned = -0.000575588 Jy ! Component: 200 - total flux cleaned = -0.000571498 Jy ! Total flux subtracted in 200 components = -0.000571498 Jy ! Clean residual min=-0.004724 max=0.004408 Jy/beam ! Clean residual mean=0.000022 rms=0.001199 Jy/beam ! Combined flux in latest and established models = 0.105818 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 7 model components to the UV plane model. ! The established model now contains 37 components and 0.105818 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.056154Jy sigma=0.928076 ! Fit after self-cal, rms=0.056111Jy sigma=0.927644 wmodel J2339-2310_X_2005_07_09_yyk\_map.mod ! Writing 37 model components to file: J2339-2310_X_2005_07_09_yyk_map.mod wobs J2339-2310_X_2005_07_09_yyk\_uvs.fits ! Writing UV FITS file: J2339-2310_X_2005_07_09_yyk_uvs.fits wwins J2339-2310_X_2005_07_09_yyk\_map.win ! wwins: Wrote 1 windows to J2339-2310_X_2005_07_09_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 0.228% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000968165 Jy ! Component: 100 - total flux cleaned = -0.00150172 Jy ! Component: 150 - total flux cleaned = -0.00199417 Jy ! Component: 200 - total flux cleaned = -0.00225912 Jy ! Component: 250 - total flux cleaned = -0.00214147 Jy ! Component: 300 - total flux cleaned = -0.0019094 Jy ! Component: 350 - total flux cleaned = -0.0018518 Jy ! Component: 400 - total flux cleaned = -0.00195673 Jy ! Component: 450 - total flux cleaned = -0.00200726 Jy ! Component: 500 - total flux cleaned = -0.00195684 Jy ! Component: 550 - total flux cleaned = -0.001907 Jy ! Component: 600 - total flux cleaned = -0.00162207 Jy ! Component: 650 - total flux cleaned = -0.00153034 Jy ! Component: 700 - total flux cleaned = -0.00125886 Jy ! Component: 750 - total flux cleaned = -0.000993331 Jy ! Component: 800 - total flux cleaned = -0.000689861 Jy ! Component: 850 - total flux cleaned = -0.000477835 Jy ! Component: 900 - total flux cleaned = -0.000272581 Jy ! Component: 950 - total flux cleaned = -0.000273457 Jy ! Component: 1000 - total flux cleaned = -0.000233533 Jy ! Component: 1050 - total flux cleaned = 3.97946e-05 Jy ! Component: 1100 - total flux cleaned = 0.000231309 Jy ! Component: 1150 - total flux cleaned = 0.000419659 Jy ! Component: 1200 - total flux cleaned = 0.000604605 Jy ! Component: 1250 - total flux cleaned = 0.000896522 Jy ! Component: 1300 - total flux cleaned = 0.00103969 Jy ! Component: 1350 - total flux cleaned = 0.0013234 Jy ! Component: 1400 - total flux cleaned = 0.00156648 Jy ! Component: 1450 - total flux cleaned = 0.00163454 Jy ! Component: 1500 - total flux cleaned = 0.00187143 Jy ! Component: 1550 - total flux cleaned = 0.00193866 Jy ! Component: 1600 - total flux cleaned = 0.00216916 Jy ! Component: 1650 - total flux cleaned = 0.00233127 Jy ! Component: 1700 - total flux cleaned = 0.00245903 Jy ! Component: 1750 - total flux cleaned = 0.00261686 Jy ! Component: 1800 - total flux cleaned = 0.00277302 Jy ! Component: 1850 - total flux cleaned = 0.00298898 Jy ! Component: 1900 - total flux cleaned = 0.00314071 Jy ! Component: 1950 - total flux cleaned = 0.00326102 Jy ! Component: 2000 - total flux cleaned = 0.00326111 Jy ! Total flux subtracted in 2048 components = 0.00332028 Jy ! Clean residual min=-0.001703 max=0.001951 Jy/beam ! Clean residual mean=0.000021 rms=0.000560 Jy/beam ! Combined flux in latest and established models = 0.109138 Jy keep ! Adding 111 model components to the UV plane model. ! The established model now contains 148 components and 0.109138 Jy ![Exited script file: muppet] wmap "J2339-2310_X_2005_07_09_yyk\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.228% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.015 x 2.676 at 14.67 degrees (North through East) ! Clean map min=-0.0029983 max=0.089933 Jy/beam ! Writing clean map to FITS file: J2339-2310_X_2005_07_09_yyk_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0899329 invert ! Inverting map ! Your choice of large map pixels excluded 0.228% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000561253 device "J2339-2310_X_2005_07_09_yyk\_map.eps/VPS" ! Attempting to open device: 'J2339-2310_X_2005_07_09_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -1.87224 1.87224 3.74448 7.48896 14.9779 29.9559 59.9117 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0016 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.089 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.015 x 2.676 at 14.67 degrees (North through East) ! Clean map min=-0.0029983 max=0.089933 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J2339-2310_X_2005_07_09_yyk\_map.gif/gif" ! Attempting to open device: 'J2339-2310_X_2005_07_09_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J2339-2310_X_2005_07_09_yyk_uvs.log closed on Fri Jan 20 11:11:48 2006