! Started logfile: J0502-3541_X_2002_01_31_yyk_uvs.log on Wed Jun 27 10:48:34 2007 obs J0502-3541_X_2002_01_31_yyk_uva.fits ! Reading UV FITS file: J0502-3541_X_2002_01_31_yyk_uva.fits ! AN table 1: 37 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.769369 visibilities/baseline/integration-bin. ! Found source: J0502-3541 ! ! 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 5124 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 J0502-3541_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)= 0.187482 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 0.912% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.6974 mas, bmaj=1.811 mas, bpa=4.725 degrees ! Estimated noise=2566.33 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 = 0.0522155 Jy ! Component: 100 - total flux cleaned = 0.0702514 Jy ! Total flux subtracted in 100 components = 0.0702514 Jy ! Clean residual min=-0.013545 max=0.014436 Jy/beam ! Clean residual mean=-0.000006 rms=0.004166 Jy/beam ! Combined flux in latest and established models = 0.0702514 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 17 model components to the UV plane model. ! The established model now contains 17 components and 0.0702514 Jy ! ! Correcting IF 1. ! A total of 81 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 115 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 81 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 81 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.177125Jy sigma=0.001341 ! Fit after self-cal, rms=0.176914Jy sigma=0.001339 ! Inverting map and beam ! Your choice of large map pixels excluded 0.912% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.6974 mas, bmaj=1.811 mas, bpa=4.725 degrees ! Estimated noise=2566.33 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 0.912% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.9129 mas, bmaj=2.364 mas, bpa=5.453 degrees ! Estimated noise=1398.4 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 = 0.00550012 Jy ! Component: 100 - total flux cleaned = 0.00602569 Jy ! Component: 150 - total flux cleaned = 0.00592593 Jy ! Component: 200 - total flux cleaned = 0.00583069 Jy ! Total flux subtracted in 200 components = 0.00583069 Jy ! Clean residual min=-0.007498 max=0.007326 Jy/beam ! Clean residual mean=0.000014 rms=0.002355 Jy/beam ! Combined flux in latest and established models = 0.0760821 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 9 model components to the UV plane model. ! The established model now contains 25 components and 0.0760821 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.176848Jy sigma=0.001338 ! Fit after self-cal, rms=0.176846Jy sigma=0.001338 ! Inverting map ! Your choice of large map pixels excluded 0.912% 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 ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9129 x 2.364 at 5.453 degrees (North through East) ! Clean map min=-0.0075837 max=0.060329 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=0.176846Jy sigma=0.001338 ! Fit after self-cal, rms=0.176846Jy sigma=0.001338 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=0.176846Jy sigma=0.001338 ! Fit after self-cal, rms=0.176846Jy sigma=0.001338 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.912% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.9129 mas, bmaj=2.364 mas, bpa=5.453 degrees ! Estimated noise=1398.4 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 = -0.000103862 Jy ! Component: 100 - total flux cleaned = -0.000151662 Jy ! Component: 150 - total flux cleaned = -0.000236828 Jy ! Component: 200 - total flux cleaned = -0.000321819 Jy ! Total flux subtracted in 200 components = -0.000321819 Jy ! Clean residual min=-0.007406 max=0.007194 Jy/beam ! Clean residual mean=0.000011 rms=0.002336 Jy/beam ! Combined flux in latest and established models = 0.0757603 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 11 model components to the UV plane model. ! The established model now contains 26 components and 0.0757603 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.176838Jy sigma=0.001338 ! Fit after self-cal, rms=0.176837Jy sigma=0.001338 ! Inverting map ! Your choice of large map pixels excluded 0.912% 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=0.176837Jy sigma=0.001338 ! Fit after self-cal, rms=0.175973Jy sigma=0.001331 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.912% 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 = 0.00165571 Jy ! Component: 100 - total flux cleaned = 0.00158508 Jy ! Component: 150 - total flux cleaned = 0.00140837 Jy ! Component: 200 - total flux cleaned = 0.00124299 Jy ! Total flux subtracted in 200 components = 0.00124299 Jy ! Clean residual min=-0.007627 max=0.009003 Jy/beam ! Clean residual mean=0.000037 rms=0.002458 Jy/beam ! Combined flux in latest and established models = 0.0770033 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 27 components and 0.0770033 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.175896Jy sigma=0.001330 ! Fit after self-cal, rms=0.175750Jy sigma=0.001328 ! Inverting map ! Your choice of large map pixels excluded 0.912% 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: 0.9129 x 2.364 at 5.453 degrees (North through East) ! Clean map min=-0.0067416 max=0.066718 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 0.912% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=3.138 mas, bmaj=11.1 mas, bpa=9.389 degrees ! Estimated noise=1717.01 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 = -0.000903058 Jy ! Component: 100 - total flux cleaned = -0.00101035 Jy ! Component: 150 - total flux cleaned = -0.00106317 Jy ! Component: 200 - total flux cleaned = -0.00116316 Jy ! Total flux subtracted in 200 components = -0.00116316 Jy ! Clean residual min=-0.007391 max=0.008351 Jy/beam ! Clean residual mean=0.000127 rms=0.002850 Jy/beam ! Combined flux in latest and established models = 0.0758401 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 4 model components to the UV plane model. ! The established model now contains 29 components and 0.0758401 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.175734Jy sigma=0.001328 ! Fit after self-cal, rms=0.175626Jy sigma=0.001327 ! Inverting map ! Your choice of large map pixels excluded 0.912% of the data. ! The x-axis pixel size should ideally be below 0.1986 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 0.912% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.6974 mas, bmaj=1.811 mas, bpa=4.725 degrees ! Estimated noise=2566.33 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0574415 Jy ! Component: 100 - total flux cleaned = 0.0746619 Jy ! Component: 150 - total flux cleaned = 0.0821694 Jy ! Component: 200 - total flux cleaned = 0.0840831 Jy ! Total flux subtracted in 200 components = 0.0840831 Jy ! Clean residual min=-0.012711 max=0.012604 Jy/beam ! Clean residual mean=0.000045 rms=0.003478 Jy/beam ! Combined flux in latest and established models = 0.0840831 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 18 model components to the UV plane model. ! The established model now contains 18 components and 0.0840831 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.912% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.9129 mas, bmaj=2.364 mas, bpa=5.453 degrees ! Estimated noise=1398.4 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 = -0.00538914 Jy ! Component: 100 - total flux cleaned = -0.00661878 Jy ! Component: 150 - total flux cleaned = -0.00678025 Jy ! Component: 200 - total flux cleaned = -0.00687619 Jy ! Total flux subtracted in 200 components = -0.00687619 Jy ! Clean residual min=-0.006915 max=0.008123 Jy/beam ! Clean residual mean=0.000084 rms=0.002246 Jy/beam ! Combined flux in latest and established models = 0.0772069 Jy ! Adding 8 model components to the UV plane model. ! The established model now contains 23 components and 0.0772069 Jy ! Inverting map ! Your choice of large map pixels excluded 0.912% 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 0.912% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=3.138 mas, bmaj=11.1 mas, bpa=9.389 degrees ! Estimated noise=1717.01 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 = -0.00120692 Jy ! Component: 100 - total flux cleaned = -0.001254 Jy ! Component: 150 - total flux cleaned = -0.00134383 Jy ! Component: 200 - total flux cleaned = -0.00138855 Jy ! Total flux subtracted in 200 components = -0.00138855 Jy ! Clean residual min=-0.007063 max=0.008169 Jy/beam ! Clean residual mean=0.000118 rms=0.002763 Jy/beam ! Combined flux in latest and established models = 0.0758184 Jy ! Adding 4 model components to the UV plane model. ! The established model now contains 24 components and 0.0758184 Jy ! Inverting map ! Your choice of large map pixels excluded 0.912% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec uvtaper 0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.912% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.9129 mas, bmaj=2.364 mas, bpa=5.453 degrees ! Estimated noise=1398.4 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000854612 Jy ! Component: 100 - total flux cleaned = 0.000808912 Jy ! Component: 150 - total flux cleaned = 0.000762237 Jy ! Component: 200 - total flux cleaned = 0.000722377 Jy ! Total flux subtracted in 200 components = 0.000722377 Jy ! Clean residual min=-0.006879 max=0.008037 Jy/beam ! Clean residual mean=0.000078 rms=0.002216 Jy/beam ! Combined flux in latest and established models = 0.0765408 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 8 model components to the UV plane model. ! The established model now contains 27 components and 0.0765408 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.175583Jy sigma=0.001327 ! Fit after self-cal, rms=0.175535Jy sigma=0.001326 wmodel J0502-3541_X_2002_01_31_yyk\_map.mod ! Writing 27 model components to file: J0502-3541_X_2002_01_31_yyk_map.mod wobs J0502-3541_X_2002_01_31_yyk\_uvs.fits ! Applying 37 buffered edits. ! Writing UV FITS file: J0502-3541_X_2002_01_31_yyk_uvs.fits wwins J0502-3541_X_2002_01_31_yyk\_map.win ! wwins: Wrote 1 windows to J0502-3541_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 0.912% 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 = 0.00313258 Jy ! Component: 100 - total flux cleaned = 0.00279589 Jy ! Component: 150 - total flux cleaned = 0.00226353 Jy ! Component: 200 - total flux cleaned = 0.00197095 Jy ! Component: 250 - total flux cleaned = 0.0018805 Jy ! Component: 300 - total flux cleaned = 0.00170234 Jy ! Component: 350 - total flux cleaned = 0.00153785 Jy ! Component: 400 - total flux cleaned = 0.00146035 Jy ! Component: 450 - total flux cleaned = 0.00123488 Jy ! Component: 500 - total flux cleaned = 0.00116336 Jy ! Component: 550 - total flux cleaned = 0.00136897 Jy ! Component: 600 - total flux cleaned = 0.00143667 Jy ! Component: 650 - total flux cleaned = 0.00175834 Jy ! Component: 700 - total flux cleaned = 0.00200543 Jy ! Component: 750 - total flux cleaned = 0.00212505 Jy ! Component: 800 - total flux cleaned = 0.00247365 Jy ! Component: 850 - total flux cleaned = 0.00281355 Jy ! Component: 900 - total flux cleaned = 0.00303499 Jy ! Component: 950 - total flux cleaned = 0.00330295 Jy ! Component: 1000 - total flux cleaned = 0.00356477 Jy ! Component: 1050 - total flux cleaned = 0.00376984 Jy ! Component: 1100 - total flux cleaned = 0.00401963 Jy ! Component: 1150 - total flux cleaned = 0.00426332 Jy ! Component: 1200 - total flux cleaned = 0.00435908 Jy ! Component: 1250 - total flux cleaned = 0.00445269 Jy ! Component: 1300 - total flux cleaned = 0.00445339 Jy ! Component: 1350 - total flux cleaned = 0.00467858 Jy ! Component: 1400 - total flux cleaned = 0.00489878 Jy ! Component: 1450 - total flux cleaned = 0.00507142 Jy ! Component: 1500 - total flux cleaned = 0.00524095 Jy ! Component: 1550 - total flux cleaned = 0.00536549 Jy ! Component: 1600 - total flux cleaned = 0.00544741 Jy ! Component: 1650 - total flux cleaned = 0.00536673 Jy ! Component: 1700 - total flux cleaned = 0.00544611 Jy ! Component: 1750 - total flux cleaned = 0.0054462 Jy ! Component: 1800 - total flux cleaned = 0.0053686 Jy ! Component: 1850 - total flux cleaned = 0.0052926 Jy ! Component: 1900 - total flux cleaned = 0.00521695 Jy ! Component: 1950 - total flux cleaned = 0.00510465 Jy ! Component: 2000 - total flux cleaned = 0.00503034 Jy ! Total flux subtracted in 2048 components = 0.00492002 Jy ! Clean residual min=-0.002036 max=0.002114 Jy/beam ! Clean residual mean=0.000022 rms=0.000704 Jy/beam ! Combined flux in latest and established models = 0.0814608 Jy keep ! Adding 110 model components to the UV plane model. ! The established model now contains 137 components and 0.0814608 Jy ![Exited script file: muppet] wmap "J0502-3541_X_2002_01_31_yyk\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.912% 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: 0.9129 x 2.364 at 5.453 degrees (North through East) ! Clean map min=-0.003774 max=0.068127 Jy/beam ! Writing clean map to FITS file: J0502-3541_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 0.0681271 invert ! Inverting map ! Your choice of large map pixels excluded 0.912% 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 0.000687807 device "J0502-3541_X_2002_01_31_yyk\_map.eps/VPS" ! Attempting to open device: 'J0502-3541_X_2002_01_31_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -3.02878 3.02878 6.05756 12.1151 24.2302 48.4605 96.921 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.002 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.068 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9129 x 2.364 at 5.453 degrees (North through East) ! Clean map min=-0.003774 max=0.068127 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0502-3541_X_2002_01_31_yyk\_map.gif/gif" ! Attempting to open device: 'J0502-3541_X_2002_01_31_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J0502-3541_X_2002_01_31_yyk_uvs.log closed on Wed Jun 27 10:48:40 2007