! Started logfile: J0228-3719_X_2002_01_31_yyk_uvs.log on Wed Jun 27 10:46:08 2007 obs J0228-3719_X_2002_01_31_yyk_uva.fits ! Reading UV FITS file: J0228-3719_X_2002_01_31_yyk_uva.fits ! AN table 1: 35 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.738413 visibilities/baseline/integration-bin. ! Found source: J0228-3719 ! ! 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 4652 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 J0228-3719_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)= 0.195203 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 0.753% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.6835 mas, bmaj=1.819 mas, bpa=5.272 degrees ! Estimated noise=3029.28 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 = 0.0502945 Jy ! Component: 100 - total flux cleaned = 0.0589208 Jy ! Total flux subtracted in 100 components = 0.0589208 Jy ! Clean residual min=-0.011626 max=0.011529 Jy/beam ! Clean residual mean=-0.000014 rms=0.003278 Jy/beam ! Combined flux in latest and established models = 0.0589207 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 0.0589207 Jy ! ! Correcting IF 1. ! A total of 86 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 86 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 86 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 86 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.187030Jy sigma=0.001310 ! Fit after self-cal, rms=0.186903Jy sigma=0.001308 ! Inverting map and beam ! Your choice of large map pixels excluded 0.725% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.6835 mas, bmaj=1.819 mas, bpa=5.274 degrees ! Estimated noise=3030.2 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 0.725% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.8871 mas, bmaj=2.363 mas, bpa=6.307 degrees ! Estimated noise=1537.03 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 = 0.00597226 Jy ! Component: 100 - total flux cleaned = 0.00719688 Jy ! Component: 150 - total flux cleaned = 0.00728329 Jy ! Component: 200 - total flux cleaned = 0.0072833 Jy ! Total flux subtracted in 200 components = 0.0072833 Jy ! Clean residual min=-0.010604 max=0.008299 Jy/beam ! Clean residual mean=0.000161 rms=0.002530 Jy/beam ! Combined flux in latest and established models = 0.066204 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 0.066204 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.186856Jy sigma=0.001307 ! Fit after self-cal, rms=0.186885Jy sigma=0.001307 ! Inverting map ! Your choice of large map pixels excluded 0.725% 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: 0.8871 x 2.363 at 6.307 degrees (North through East) ! Clean map min=-0.0099152 max=0.057372 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 ! 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 2. ! 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 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=0.186885Jy sigma=0.001307 ! Fit after self-cal, rms=0.186885Jy sigma=0.001307 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=0.186885Jy sigma=0.001307 ! Fit after self-cal, rms=0.186879Jy sigma=0.001306 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.725% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.8871 mas, bmaj=2.363 mas, bpa=6.307 degrees ! Estimated noise=1537.03 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 = 6.24367e-05 Jy ! Component: 100 - total flux cleaned = 2.24148e-05 Jy ! Component: 150 - total flux cleaned = 2.16317e-05 Jy ! Component: 200 - total flux cleaned = 2.21809e-05 Jy ! Total flux subtracted in 200 components = 2.21809e-05 Jy ! Clean residual min=-0.010539 max=0.008275 Jy/beam ! Clean residual mean=0.000165 rms=0.002520 Jy/beam ! Combined flux in latest and established models = 0.0662262 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 10 model components to the UV plane model. ! The established model now contains 19 components and 0.0662262 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.186847Jy sigma=0.001306 ! Fit after self-cal, rms=0.186864Jy sigma=0.001306 ! Inverting map ! Your choice of large map pixels excluded 0.725% 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=0.186864Jy sigma=0.001306 ! Fit after self-cal, rms=0.185235Jy sigma=0.001294 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.725% 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 = 0.00378378 Jy ! Component: 100 - total flux cleaned = 0.00384797 Jy ! Component: 150 - total flux cleaned = 0.00384691 Jy ! Component: 200 - total flux cleaned = 0.00384778 Jy ! Total flux subtracted in 200 components = 0.00384778 Jy ! Clean residual min=-0.011066 max=0.008372 Jy/beam ! Clean residual mean=0.000171 rms=0.002614 Jy/beam ! Combined flux in latest and established models = 0.070074 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 12 model components to the UV plane model. ! The established model now contains 30 components and 0.070074 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.185238Jy sigma=0.001293 ! Fit after self-cal, rms=0.184920Jy sigma=0.001291 ! Inverting map ! Your choice of large map pixels excluded 0.725% 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: 0.8871 x 2.363 at 6.307 degrees (North through East) ! Clean map min=-0.010255 max=0.062511 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 0.725% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=3.111 mas, bmaj=11.58 mas, bpa=7.85 degrees ! Estimated noise=1913.99 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 = 0.000188236 Jy ! Component: 100 - total flux cleaned = 0.000189154 Jy ! Component: 150 - total flux cleaned = 0.000190242 Jy ! Component: 200 - total flux cleaned = 0.000193396 Jy ! Total flux subtracted in 200 components = 0.000193396 Jy ! Clean residual min=-0.010647 max=0.008951 Jy/beam ! Clean residual mean=0.000234 rms=0.003165 Jy/beam ! Combined flux in latest and established models = 0.0702674 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 36 components and 0.0702674 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.184921Jy sigma=0.001291 ! Fit after self-cal, rms=0.184769Jy sigma=0.001290 ! Inverting map ! Your choice of large map pixels excluded 0.725% 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 0.725% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.6835 mas, bmaj=1.819 mas, bpa=5.274 degrees ! Estimated noise=3030.2 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0547914 Jy ! Component: 100 - total flux cleaned = 0.0639576 Jy ! Component: 150 - total flux cleaned = 0.0652021 Jy ! Component: 200 - total flux cleaned = 0.0655451 Jy ! Total flux subtracted in 200 components = 0.0655451 Jy ! Clean residual min=-0.013941 max=0.012541 Jy/beam ! Clean residual mean=0.000044 rms=0.003761 Jy/beam ! Combined flux in latest and established models = 0.0655451 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 12 model components to the UV plane model. ! The established model now contains 12 components and 0.0655451 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.725% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.8871 mas, bmaj=2.363 mas, bpa=6.307 degrees ! Estimated noise=1537.03 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 = 0.00546562 Jy ! Component: 100 - total flux cleaned = 0.00547811 Jy ! Component: 150 - total flux cleaned = 0.00548313 Jy ! Component: 200 - total flux cleaned = 0.00544562 Jy ! Total flux subtracted in 200 components = 0.00544562 Jy ! Clean residual min=-0.010924 max=0.008357 Jy/beam ! Clean residual mean=0.000129 rms=0.002419 Jy/beam ! Combined flux in latest and established models = 0.0709907 Jy ! Adding 12 model components to the UV plane model. ! The established model now contains 21 components and 0.0709907 Jy ! Inverting map ! Your choice of large map pixels excluded 0.725% 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 0.725% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=3.111 mas, bmaj=11.58 mas, bpa=7.85 degrees ! Estimated noise=1913.99 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 = -0.000375023 Jy ! Component: 100 - total flux cleaned = -0.000376009 Jy ! Component: 150 - total flux cleaned = -0.000376726 Jy ! Component: 200 - total flux cleaned = -0.000377089 Jy ! Total flux subtracted in 200 components = -0.000377089 Jy ! Clean residual min=-0.010366 max=0.008951 Jy/beam ! Clean residual mean=0.000212 rms=0.003064 Jy/beam ! Combined flux in latest and established models = 0.0706136 Jy ! Adding 7 model components to the UV plane model. ! The established model now contains 23 components and 0.0706136 Jy ! Inverting map ! Your choice of large map pixels excluded 0.725% 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 0.725% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.8871 mas, bmaj=2.363 mas, bpa=6.307 degrees ! Estimated noise=1537.03 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000168423 Jy ! Component: 100 - total flux cleaned = 0.000168966 Jy ! Component: 150 - total flux cleaned = 0.000136624 Jy ! Component: 200 - total flux cleaned = 0.000139225 Jy ! Total flux subtracted in 200 components = 0.000139225 Jy ! Clean residual min=-0.010823 max=0.008270 Jy/beam ! Clean residual mean=0.000127 rms=0.002404 Jy/beam ! Combined flux in latest and established models = 0.0707528 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 10 model components to the UV plane model. ! The established model now contains 30 components and 0.0707528 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.184776Jy sigma=0.001290 ! Fit after self-cal, rms=0.184694Jy sigma=0.001290 wmodel J0228-3719_X_2002_01_31_yyk\_map.mod ! Writing 30 model components to file: J0228-3719_X_2002_01_31_yyk_map.mod wobs J0228-3719_X_2002_01_31_yyk\_uvs.fits ! Applying 35 buffered edits. ! Writing UV FITS file: J0228-3719_X_2002_01_31_yyk_uvs.fits wwins J0228-3719_X_2002_01_31_yyk\_map.win ! wwins: Wrote 1 windows to J0228-3719_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 0.725% 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 = -0.00356382 Jy ! Component: 100 - total flux cleaned = -0.00292762 Jy ! Component: 150 - total flux cleaned = -0.00303422 Jy ! Component: 200 - total flux cleaned = -0.00314511 Jy ! Component: 250 - total flux cleaned = -0.00295516 Jy ! Component: 300 - total flux cleaned = -0.00258771 Jy ! Component: 350 - total flux cleaned = -0.00241263 Jy ! Component: 400 - total flux cleaned = -0.00233147 Jy ! Component: 450 - total flux cleaned = -0.00202002 Jy ! Component: 500 - total flux cleaned = -0.00187017 Jy ! Component: 550 - total flux cleaned = -0.00143577 Jy ! Component: 600 - total flux cleaned = -0.000947938 Jy ! Component: 650 - total flux cleaned = -0.000477254 Jy ! Component: 700 - total flux cleaned = -0.000280021 Jy ! Component: 750 - total flux cleaned = -8.70663e-05 Jy ! Component: 800 - total flux cleaned = 0.000101805 Jy ! Component: 850 - total flux cleaned = 0.000410211 Jy ! Component: 900 - total flux cleaned = 0.000590363 Jy ! Component: 950 - total flux cleaned = 0.000708801 Jy ! Component: 1000 - total flux cleaned = 0.000826638 Jy ! Component: 1050 - total flux cleaned = 0.00111481 Jy ! Component: 1100 - total flux cleaned = 0.00128436 Jy ! Component: 1150 - total flux cleaned = 0.00150772 Jy ! Component: 1200 - total flux cleaned = 0.00156229 Jy ! Component: 1250 - total flux cleaned = 0.00188741 Jy ! Component: 1300 - total flux cleaned = 0.00204738 Jy ! Component: 1350 - total flux cleaned = 0.0022049 Jy ! Component: 1400 - total flux cleaned = 0.00256854 Jy ! Component: 1450 - total flux cleaned = 0.00261972 Jy ! Component: 1500 - total flux cleaned = 0.00256893 Jy ! Component: 1550 - total flux cleaned = 0.0025694 Jy ! Component: 1600 - total flux cleaned = 0.00271858 Jy ! Component: 1650 - total flux cleaned = 0.00281666 Jy ! Component: 1700 - total flux cleaned = 0.00281619 Jy ! Component: 1750 - total flux cleaned = 0.00286458 Jy ! Component: 1800 - total flux cleaned = 0.0029608 Jy ! Component: 1850 - total flux cleaned = 0.00296093 Jy ! Component: 1900 - total flux cleaned = 0.00300822 Jy ! Component: 1950 - total flux cleaned = 0.00300829 Jy ! Component: 2000 - total flux cleaned = 0.00291389 Jy ! Total flux subtracted in 2048 components = 0.00291322 Jy ! Clean residual min=-0.002713 max=0.002590 Jy/beam ! Clean residual mean=0.000023 rms=0.000879 Jy/beam ! Combined flux in latest and established models = 0.073666 Jy keep ! Adding 101 model components to the UV plane model. ! The established model now contains 131 components and 0.073666 Jy ![Exited script file: muppet] wmap "J0228-3719_X_2002_01_31_yyk\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.725% 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: 0.8871 x 2.363 at 6.307 degrees (North through East) ! Clean map min=-0.0062811 max=0.061372 Jy/beam ! Writing clean map to FITS file: J0228-3719_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 0.061372 invert ! Inverting map ! Your choice of large map pixels excluded 0.725% 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 0.000876139 device "J0228-3719_X_2002_01_31_yyk\_map.eps/VPS" ! Attempting to open device: 'J0228-3719_X_2002_01_31_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -4.28276 4.28276 8.56553 17.1311 34.2621 68.5242 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0026 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.061 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8871 x 2.363 at 6.307 degrees (North through East) ! Clean map min=-0.0062811 max=0.061372 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0228-3719_X_2002_01_31_yyk\_map.gif/gif" ! Attempting to open device: 'J0228-3719_X_2002_01_31_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J0228-3719_X_2002_01_31_yyk_uvs.log closed on Wed Jun 27 10:46:13 2007