! Started logfile: J0440-4333_X_2004_05_08_yyk_uvs.log on Tue Dec 6 23:59:17 2005 obs J0440-4333_X_2004_05_08_yyk_uve.fits ! Reading UV FITS file: J0440-4333_X_2004_05_08_yyk_uve.fits ! AN table 1: 5 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.417778 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0440-4333 ! ! 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 1438 lines of history. ! ! Reading 376 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 J0440-4333_X_2004_05_08_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)= 1.55551 Jy startmod ,phase_soltime ! Applying default point source starting model. ! Performing phase self-cal over 10 minute time intervals ! 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 23 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 23 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 23 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.626536Jy sigma=9.420025 ! Fit after self-cal, rms=0.626294Jy sigma=9.416730 ! clrmod: Cleared the established, tentative and continuum models. ! Redundant starting model cleared. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 1.59% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.5886 mas, bmaj=1.791 mas, bpa=-0.3107 degrees ! Estimated noise=4.17245 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 = 1.28407 Jy ! Component: 100 - total flux cleaned = 1.60233 Jy ! Total flux subtracted in 100 components = 1.60233 Jy ! Clean residual min=-0.117036 max=0.109833 Jy/beam ! Clean residual mean=-0.001988 rms=0.033889 Jy/beam ! Combined flux in latest and established models = 1.60233 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 1.60233 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.240935Jy sigma=3.562461 ! Fit after self-cal, rms=0.240777Jy sigma=3.560049 ! Inverting map ! Your choice of large map pixels excluded 1.59% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec 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 1.59% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.6882 mas, bmaj=1.969 mas, bpa=-0.1671 degrees ! Estimated noise=3.06034 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 = 0.152994 Jy ! Component: 100 - total flux cleaned = 0.211191 Jy ! Component: 150 - total flux cleaned = 0.233709 Jy ! Component: 200 - total flux cleaned = 0.239853 Jy ! Total flux subtracted in 200 components = 0.239853 Jy ! Clean residual min=-0.081815 max=0.077269 Jy/beam ! Clean residual mean=-0.000728 rms=0.026971 Jy/beam ! Combined flux in latest and established models = 1.84219 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 11 model components to the UV plane model. ! The established model now contains 13 components and 1.84219 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.172777Jy sigma=2.512733 ! Fit after self-cal, rms=0.172621Jy sigma=2.510148 ! Inverting map ! Your choice of large map pixels excluded 1.59% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! selflims ampcor_selflim ! 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: 1.00224 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.98 HN 1.00* KP 1.00 ! LA 1.02 MK 0.98 NL 1.00* OV 1.00 ! PT 1.00* SC 1.00 ! ! ! Correcting IF 2. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 1.01263 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.99 HN 1.00* KP 0.94 ! LA 1.01 MK 1.00 NL 1.00* OV 0.97 ! PT 1.00* SC 0.96 ! ! ! Correcting IF 3. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 0.995647 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.05 HN 1.00* KP 0.91 ! LA 1.01 MK 1.02 NL 1.00* OV 1.03 ! PT 1.00* SC 1.02 ! ! ! Correcting IF 4. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 0.985089 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.05 HN 1.00* KP 0.94 ! LA 1.04 MK 1.05 NL 1.00* OV 1.02 ! PT 1.00* SC 1.05 ! ! ! Fit before self-cal, rms=0.172621Jy sigma=2.510148 ! Fit after self-cal, rms=0.156214Jy sigma=2.304207 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=0.156214Jy sigma=2.304207 ! Fit after self-cal, rms=0.156152Jy sigma=2.303733 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 1.67% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.6881 mas, bmaj=1.989 mas, bpa=0.5497 degrees ! Estimated noise=3.10269 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 = -0.00453939 Jy ! Component: 100 - total flux cleaned = -0.00398764 Jy ! Component: 150 - total flux cleaned = -0.00400912 Jy ! Component: 200 - total flux cleaned = -0.00401228 Jy ! Total flux subtracted in 200 components = -0.00401228 Jy ! Clean residual min=-0.075655 max=0.074220 Jy/beam ! Clean residual mean=-0.000634 rms=0.025751 Jy/beam ! Combined flux in latest and established models = 1.83817 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 10 model components to the UV plane model. ! The established model now contains 17 components and 1.83817 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.155497Jy sigma=2.290547 ! Fit after self-cal, rms=0.155372Jy sigma=2.289891 ! Inverting map ! Your choice of large map pixels excluded 1.67% of the data. ! The x-axis pixel size should ideally be below 0.1986 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=0.155372Jy sigma=2.289891 ! Fit after self-cal, rms=0.152549Jy sigma=2.244350 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.67% of the data. ! The x-axis pixel size should ideally be below 0.1986 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 = 0.000835697 Jy ! Component: 100 - total flux cleaned = 0.000840569 Jy ! Component: 150 - total flux cleaned = 0.000842277 Jy ! Component: 200 - total flux cleaned = 0.000849509 Jy ! Total flux subtracted in 200 components = 0.000849509 Jy ! Clean residual min=-0.074274 max=0.073866 Jy/beam ! Clean residual mean=-0.000633 rms=0.025530 Jy/beam ! Combined flux in latest and established models = 1.83902 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 9 model components to the UV plane model. ! The established model now contains 20 components and 1.83902 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.152367Jy sigma=2.240700 ! Fit after self-cal, rms=0.152207Jy sigma=2.237594 ! Inverting map ! Your choice of large map pixels excluded 1.67% of the data. ! The x-axis pixel size should ideally be below 0.1986 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: 0.6881 x 1.989 at 0.5497 degrees (North through East) ! Clean map min=-0.071994 max=1.5256 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=0.152207Jy sigma=2.237594 ! Fit after self-cal, rms=0.147753Jy sigma=2.189048 ! 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=0.147753Jy sigma=2.189048 ! Fit after self-cal, rms=0.147768Jy sigma=2.188804 ! Inverting map and beam ! Your choice of large map pixels excluded 1.67% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.6885 mas, bmaj=1.993 mas, bpa=0.5757 degrees ! Estimated noise=3.10411 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -0.00162988 Jy ! Component: 100 - total flux cleaned = -0.0013265 Jy ! Component: 150 - total flux cleaned = -0.00120425 Jy ! Component: 200 - total flux cleaned = -0.00132689 Jy ! Total flux subtracted in 200 components = -0.00132689 Jy ! Clean residual min=-0.073683 max=0.074934 Jy/beam ! Clean residual mean=-0.000614 rms=0.025697 Jy/beam ! Combined flux in latest and established models = 1.8377 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 22 components and 1.8377 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.147638Jy sigma=2.185856 ! Fit after self-cal, rms=0.147607Jy sigma=2.185591 ! Inverting map ! Your choice of large map pixels excluded 1.67% of the data. ! The x-axis pixel size should ideally be below 0.1986 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=0.147607Jy sigma=2.185591 ! Fit after self-cal, rms=0.145102Jy sigma=2.151064 ! 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=0.145102Jy sigma=2.151064 ! Fit after self-cal, rms=0.145101Jy sigma=2.151062 ! Inverting map and beam ! Your choice of large map pixels excluded 1.67% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.6893 mas, bmaj=1.994 mas, bpa=0.6476 degrees ! Estimated noise=3.10444 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -0.000921088 Jy ! Component: 100 - total flux cleaned = -0.000918895 Jy ! Component: 150 - total flux cleaned = -0.000915434 Jy ! Component: 200 - total flux cleaned = -0.000929166 Jy ! Total flux subtracted in 200 components = -0.000929166 Jy ! Clean residual min=-0.072963 max=0.074711 Jy/beam ! Clean residual mean=-0.000599 rms=0.025603 Jy/beam ! Combined flux in latest and established models = 1.83677 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 9 model components to the UV plane model. ! The established model now contains 24 components and 1.83677 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.144971Jy sigma=2.149041 ! Fit after self-cal, rms=0.144940Jy sigma=2.148783 ! Inverting map ! Your choice of large map pixels excluded 1.67% of the data. ! The x-axis pixel size should ideally be below 0.1986 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 1.67% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=2.614 mas, bmaj=9.211 mas, bpa=2.567 degrees ! Estimated noise=4.5379 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 = -0.0103478 Jy ! Component: 100 - total flux cleaned = -0.0103629 Jy ! Component: 150 - total flux cleaned = -0.0103746 Jy ! Component: 200 - total flux cleaned = -0.0103837 Jy ! Total flux subtracted in 200 components = -0.0103837 Jy ! Clean residual min=-0.149450 max=0.141559 Jy/beam ! Clean residual mean=-0.001372 rms=0.057453 Jy/beam ! Combined flux in latest and established models = 1.82638 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 28 components and 1.82638 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.146407Jy sigma=2.169382 ! Fit after self-cal, rms=0.145686Jy sigma=2.158790 ! Inverting map ! Your choice of large map pixels excluded 1.67% of the data. ! The x-axis pixel size should ideally be below 0.1986 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 1.67% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.5904 mas, bmaj=1.797 mas, bpa=-0.3981 degrees ! Estimated noise=4.20844 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 1.29002 Jy ! Component: 100 - total flux cleaned = 1.60372 Jy ! Component: 150 - total flux cleaned = 1.74839 Jy ! Component: 200 - total flux cleaned = 1.8176 Jy ! Total flux subtracted in 200 components = 1.8176 Jy ! Clean residual min=-0.059037 max=0.057737 Jy/beam ! Clean residual mean=-0.000605 rms=0.018634 Jy/beam ! Combined flux in latest and established models = 1.8176 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 11 model components to the UV plane model. ! The established model now contains 11 components and 1.8176 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 1.67% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.6893 mas, bmaj=1.994 mas, bpa=0.6476 degrees ! Estimated noise=3.10444 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 = 0.0148929 Jy ! Component: 100 - total flux cleaned = 0.0177269 Jy ! Component: 150 - total flux cleaned = 0.0186272 Jy ! Component: 200 - total flux cleaned = 0.0186309 Jy ! Total flux subtracted in 200 components = 0.0186309 Jy ! Clean residual min=-0.074675 max=0.074640 Jy/beam ! Clean residual mean=-0.000597 rms=0.025717 Jy/beam ! Combined flux in latest and established models = 1.83623 Jy ! Adding 10 model components to the UV plane model. ! The established model now contains 18 components and 1.83623 Jy ! Inverting map ! Your choice of large map pixels excluded 1.67% of the data. ! The x-axis pixel size should ideally be below 0.1986 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 1.67% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=2.614 mas, bmaj=9.211 mas, bpa=2.567 degrees ! Estimated noise=4.5379 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 = -0.0109774 Jy ! Component: 100 - total flux cleaned = -0.0109629 Jy ! Component: 150 - total flux cleaned = -0.0109471 Jy ! Component: 200 - total flux cleaned = -0.0109352 Jy ! Total flux subtracted in 200 components = -0.0109352 Jy ! Clean residual min=-0.149366 max=0.141900 Jy/beam ! Clean residual mean=-0.001376 rms=0.057447 Jy/beam ! Combined flux in latest and established models = 1.82529 Jy ! Adding 3 model components to the UV plane model. ! The established model now contains 21 components and 1.82529 Jy ! Inverting map ! Your choice of large map pixels excluded 1.67% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 1.67% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.6893 mas, bmaj=1.994 mas, bpa=0.6476 degrees ! Estimated noise=3.10444 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0100966 Jy ! Component: 100 - total flux cleaned = 0.00952164 Jy ! Component: 150 - total flux cleaned = 0.00990729 Jy ! Component: 200 - total flux cleaned = 0.00986956 Jy ! Total flux subtracted in 200 components = 0.00986956 Jy ! Clean residual min=-0.074285 max=0.072899 Jy/beam ! Clean residual mean=-0.000607 rms=0.025587 Jy/beam ! Combined flux in latest and established models = 1.83516 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 15 model components to the UV plane model. ! The established model now contains 32 components and 1.83516 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.145278Jy sigma=2.152585 ! Fit after self-cal, rms=0.145224Jy sigma=2.150970 wmodel J0440-4333_X_2004_05_08_yyk\_map.mod ! Writing 32 model components to file: J0440-4333_X_2004_05_08_yyk_map.mod wobs J0440-4333_X_2004_05_08_yyk\_uvs.fits ! Writing UV FITS file: J0440-4333_X_2004_05_08_yyk_uvs.fits wwins J0440-4333_X_2004_05_08_yyk\_map.win ! wwins: Wrote 1 windows to J0440-4333_X_2004_05_08_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 1.67% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00426203 Jy ! Component: 100 - total flux cleaned = -0.00537277 Jy ! Component: 150 - total flux cleaned = -0.00729726 Jy ! Component: 200 - total flux cleaned = -0.00812606 Jy ! Component: 250 - total flux cleaned = -0.00809407 Jy ! Component: 300 - total flux cleaned = -0.00809758 Jy ! Component: 350 - total flux cleaned = -0.00868583 Jy ! Component: 400 - total flux cleaned = -0.00866295 Jy ! Component: 450 - total flux cleaned = -0.00816124 Jy ! Component: 500 - total flux cleaned = -0.00772798 Jy ! Component: 550 - total flux cleaned = -0.00856982 Jy ! Component: 600 - total flux cleaned = -0.00936283 Jy ! Component: 650 - total flux cleaned = -0.0105037 Jy ! Component: 700 - total flux cleaned = -0.0127268 Jy ! Component: 750 - total flux cleaned = -0.0145382 Jy ! Component: 800 - total flux cleaned = -0.0159681 Jy ! Component: 850 - total flux cleaned = -0.0166868 Jy ! Component: 900 - total flux cleaned = -0.0174081 Jy ! Component: 950 - total flux cleaned = -0.0185065 Jy ! Component: 1000 - total flux cleaned = -0.0196192 Jy ! Component: 1050 - total flux cleaned = -0.0203666 Jy ! Component: 1100 - total flux cleaned = -0.021502 Jy ! Component: 1150 - total flux cleaned = -0.0222743 Jy ! Component: 1200 - total flux cleaned = -0.0234492 Jy ! Component: 1250 - total flux cleaned = -0.0242417 Jy ! Component: 1300 - total flux cleaned = -0.025451 Jy ! Component: 1350 - total flux cleaned = -0.0266845 Jy ! Component: 1400 - total flux cleaned = -0.0283537 Jy ! Component: 1450 - total flux cleaned = -0.0292031 Jy ! Component: 1500 - total flux cleaned = -0.030072 Jy ! Component: 1550 - total flux cleaned = -0.0309573 Jy ! Component: 1600 - total flux cleaned = -0.0323233 Jy ! Component: 1650 - total flux cleaned = -0.032804 Jy ! Component: 1700 - total flux cleaned = -0.0323252 Jy ! Component: 1750 - total flux cleaned = -0.0328143 Jy ! Component: 1800 - total flux cleaned = -0.0333296 Jy ! Component: 1850 - total flux cleaned = -0.0333305 Jy ! Component: 1900 - total flux cleaned = -0.0333268 Jy ! Component: 1950 - total flux cleaned = -0.0338757 Jy ! Component: 2000 - total flux cleaned = -0.0344468 Jy ! Total flux subtracted in 2048 components = -0.0344529 Jy ! Clean residual min=-0.031368 max=0.033237 Jy/beam ! Clean residual mean=-0.000609 rms=0.010970 Jy/beam ! Combined flux in latest and established models = 1.80071 Jy keep ! Adding 113 model components to the UV plane model. ! The established model now contains 145 components and 1.80071 Jy ![Exited script file: muppet] wmap "J0440-4333_X_2004_05_08_yyk\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 1.67% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6893 x 1.994 at 0.6476 degrees (North through East) ! Clean map min=-0.053381 max=1.5488 Jy/beam ! Writing clean map to FITS file: J0440-4333_X_2004_05_08_yyk_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 1.54876 invert ! Inverting map ! Your choice of large map pixels excluded 1.67% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.0106989 device "J0440-4333_X_2004_05_08_yyk\_map.eps/VPS" ! Attempting to open device: 'J0440-4333_X_2004_05_08_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -2.0724 2.0724 4.1448 8.2896 16.5792 33.1584 66.3168 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.032 print "peak=",int(peak_flux*1000)/1000 ! peak= 1.548 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6893 x 1.994 at 0.6476 degrees (North through East) ! Clean map min=-0.053381 max=1.5488 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0440-4333_X_2004_05_08_yyk\_map.gif/gif" ! Attempting to open device: 'J0440-4333_X_2004_05_08_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J0440-4333_X_2004_05_08_yyk_uvs.log closed on Tue Dec 6 23:59:21 2005