! Started logfile: J0037-2145_X_2006_12_18_yyk_uvs.log on Mon Jun 16 19:03:47 2008 obs J0037-2145_X_2006_12_18_yyk_uve.fits ! Reading UV FITS file: J0037-2145_X_2006_12_18_yyk_uve.fits ! AN table 1: 14 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.842857 visibilities/baseline/integration-bin. ! Found source: J0037-2145 ! ! 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 2162 lines of history. ! ! Reading 2124 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 J0037-2145_X_2006_12_18_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)= 0.137453 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 0.15% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Estimated beam: bmin=0.6608 mas, bmaj=1.695 mas, bpa=-3.939 degrees ! Estimated noise=1.43356 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 = 0.0731802 Jy ! Component: 100 - total flux cleaned = 0.0972636 Jy ! Total flux subtracted in 100 components = 0.0972636 Jy ! Clean residual min=-0.014072 max=0.045259 Jy/beam ! Clean residual mean=-0.000058 rms=0.004229 Jy/beam ! Combined flux in latest and established models = 0.0972637 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 9 model components to the UV plane model. ! The established model now contains 9 components and 0.0972637 Jy ! ! Correcting IF 1. ! A total of 18 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 11 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 11 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=0.098288Jy sigma=1.601896 ! Fit after self-cal, rms=0.097688Jy sigma=1.584846 ! Inverting map and beam ! Your choice of large map pixels excluded 0.15% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Estimated beam: bmin=0.6608 mas, bmaj=1.695 mas, bpa=-3.939 degrees ! Estimated noise=1.43356 mJy/beam. ! Added new window around map position (1.8, -2.2). ! clean: niter=100 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0439886 Jy ! Component: 100 - total flux cleaned = 0.0592943 Jy ! Total flux subtracted in 100 components = 0.0592943 Jy ! Clean residual min=-0.009837 max=0.016078 Jy/beam ! Clean residual mean=-0.000014 rms=0.002747 Jy/beam ! Combined flux in latest and established models = 0.156558 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 10 model components to the UV plane model. ! The established model now contains 18 components and 0.156558 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.080792Jy sigma=1.271995 ! Fit after self-cal, rms=0.076122Jy sigma=1.186786 ! Inverting map ! Your choice of large map pixels excluded 0.15% of the data. ! The x-axis pixel size should ideally be below 0.1994 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 0.15% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Estimated beam: bmin=0.8817 mas, bmaj=2.168 mas, bpa=-1.274 degrees ! Estimated noise=0.923165 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 = 0.0218945 Jy ! Component: 100 - total flux cleaned = 0.0302741 Jy ! Component: 150 - total flux cleaned = 0.0317406 Jy ! Component: 200 - total flux cleaned = 0.0320243 Jy ! Total flux subtracted in 200 components = 0.0320243 Jy ! Clean residual min=-0.004882 max=0.005665 Jy/beam ! Clean residual mean=0.000044 rms=0.001423 Jy/beam ! Combined flux in latest and established models = 0.188582 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 19 model components to the UV plane model. ! The established model now contains 30 components and 0.188582 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.071876Jy sigma=1.105580 ! Fit after self-cal, rms=0.071476Jy sigma=1.097549 ! Inverting map ! Your choice of large map pixels excluded 0.15% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8817 x 2.168 at -1.274 degrees (North through East) ! Clean map min=-0.0044922 max=0.086336 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: 1.01285 ! Telescope amplitude corrections in sub-array 1: ! BR 0.92 FD 0.96 HN 1.09 KP 1.00 ! LA 0.97 MK 1.04 NL 1.07 OV 0.95 ! PT 0.95 SC 0.91 ! ! ! Correcting IF 2. ! Amplitude normalization factor in sub-array 1: 1.02665 ! Telescope amplitude corrections in sub-array 1: ! BR 1.09 FD 0.88 HN 0.98 KP 0.92 ! LA 0.92 MK 0.97 NL 1.02 OV 0.96 ! PT 1.09 SC 0.91 ! ! ! 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: 0.976011 ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 1.09 HN 0.99 KP 0.93 ! LA 0.97 MK 1.01 NL 1.07 OV 0.99 ! PT 1.17 SC 0.99 ! ! ! Fit before self-cal, rms=0.071476Jy sigma=1.097549 ! Fit after self-cal, rms=0.070900Jy sigma=1.086206 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=0.070900Jy sigma=1.086206 ! Fit after self-cal, rms=0.070896Jy sigma=1.086185 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.15% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Estimated beam: bmin=0.8723 mas, bmaj=2.141 mas, bpa=0.1787 degrees ! Estimated noise=0.921435 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 = 0.00219393 Jy ! Component: 100 - total flux cleaned = 0.00179951 Jy ! Component: 150 - total flux cleaned = 0.00180144 Jy ! Component: 200 - total flux cleaned = 0.00180335 Jy ! Total flux subtracted in 200 components = 0.00180335 Jy ! Clean residual min=-0.003980 max=0.003986 Jy/beam ! Clean residual mean=0.000026 rms=0.001052 Jy/beam ! Combined flux in latest and established models = 0.190386 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 19 model components to the UV plane model. ! The established model now contains 39 components and 0.190386 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.070419Jy sigma=1.078606 ! Fit after self-cal, rms=0.070345Jy sigma=1.077316 ! Inverting map ! Your choice of large map pixels excluded 0.15% of the data. ! The x-axis pixel size should ideally be below 0.1994 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=0.070345Jy sigma=1.077316 ! Fit after self-cal, rms=0.063123Jy sigma=0.956832 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.15% of the data. ! The x-axis pixel size should ideally be below 0.1994 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 = 0.00277078 Jy ! Component: 100 - total flux cleaned = 0.00372296 Jy ! Component: 150 - total flux cleaned = 0.00411198 Jy ! Component: 200 - total flux cleaned = 0.00411736 Jy ! Total flux subtracted in 200 components = 0.00411736 Jy ! Clean residual min=-0.003840 max=0.003265 Jy/beam ! Clean residual mean=0.000018 rms=0.000955 Jy/beam ! Combined flux in latest and established models = 0.194503 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 15 model components to the UV plane model. ! The established model now contains 41 components and 0.194503 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.062700Jy sigma=0.949654 ! Fit after self-cal, rms=0.062168Jy sigma=0.943106 ! Inverting map ! Your choice of large map pixels excluded 0.15% of the data. ! The x-axis pixel size should ideally be below 0.1994 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: 0.8723 x 2.141 at 0.1787 degrees (North through East) ! Clean map min=-0.003649 max=0.090623 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 0.15% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Estimated beam: bmin=2.184 mas, bmaj=5.109 mas, bpa=2.421 degrees ! Estimated noise=1.18754 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 = 0.000477324 Jy ! Component: 100 - total flux cleaned = 0.000548396 Jy ! Component: 150 - total flux cleaned = 0.000524579 Jy ! Component: 200 - total flux cleaned = 0.000500818 Jy ! Total flux subtracted in 200 components = 0.000500818 Jy ! Clean residual min=-0.004501 max=0.003656 Jy/beam ! Clean residual mean=0.000036 rms=0.001157 Jy/beam ! Combined flux in latest and established models = 0.195004 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 10 model components to the UV plane model. ! The established model now contains 45 components and 0.195004 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.062099Jy sigma=0.941875 ! Fit after self-cal, rms=0.061988Jy sigma=0.940911 ! Inverting map ! Your choice of large map pixels excluded 0.15% of the data. ! The x-axis pixel size should ideally be below 0.1994 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 0.15% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Estimated beam: bmin=0.6592 mas, bmaj=1.683 mas, bpa=-3.35 degrees ! Estimated noise=1.42523 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.094043 Jy ! Component: 100 - total flux cleaned = 0.135256 Jy ! Component: 150 - total flux cleaned = 0.157989 Jy ! Component: 200 - total flux cleaned = 0.171487 Jy ! Total flux subtracted in 200 components = 0.171487 Jy ! Clean residual min=-0.005584 max=0.006809 Jy/beam ! Clean residual mean=-0.000017 rms=0.001499 Jy/beam ! Combined flux in latest and established models = 0.171487 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 13 model components to the UV plane model. ! The established model now contains 13 components and 0.171487 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.15% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Estimated beam: bmin=0.8723 mas, bmaj=2.141 mas, bpa=0.1787 degrees ! Estimated noise=0.921435 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) ! Added new window around map position (1, -0.6). ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0132081 Jy ! Component: 100 - total flux cleaned = 0.0194161 Jy ! Component: 150 - total flux cleaned = 0.021831 Jy ! Component: 200 - total flux cleaned = 0.0226071 Jy ! Total flux subtracted in 200 components = 0.0226071 Jy ! Clean residual min=-0.003786 max=0.003325 Jy/beam ! Clean residual mean=0.000013 rms=0.000948 Jy/beam ! Combined flux in latest and established models = 0.194094 Jy ! Adding 30 model components to the UV plane model. ! The established model now contains 41 components and 0.194094 Jy ! Inverting map ! Your choice of large map pixels excluded 0.15% of the data. ! The x-axis pixel size should ideally be below 0.1994 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 0.15% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Estimated beam: bmin=2.184 mas, bmaj=5.109 mas, bpa=2.421 degrees ! Estimated noise=1.18754 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 = 0.00122932 Jy ! Component: 100 - total flux cleaned = 0.00115487 Jy ! Component: 150 - total flux cleaned = 0.00109521 Jy ! Component: 200 - total flux cleaned = 0.00104066 Jy ! Total flux subtracted in 200 components = 0.00104066 Jy ! Clean residual min=-0.004841 max=0.003623 Jy/beam ! Clean residual mean=0.000034 rms=0.001164 Jy/beam ! Combined flux in latest and established models = 0.195135 Jy ! Adding 16 model components to the UV plane model. ! The established model now contains 56 components and 0.195135 Jy ! Inverting map ! Your choice of large map pixels excluded 0.15% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec uvtaper 0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.15% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! Estimated beam: bmin=0.8723 mas, bmaj=2.141 mas, bpa=0.1787 degrees ! Estimated noise=0.921435 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -0.00035889 Jy ! Component: 100 - total flux cleaned = -0.000358668 Jy ! Component: 150 - total flux cleaned = -0.000460949 Jy ! Component: 200 - total flux cleaned = -0.000508218 Jy ! Total flux subtracted in 200 components = -0.000508218 Jy ! Clean residual min=-0.003884 max=0.003194 Jy/beam ! Clean residual mean=0.000015 rms=0.000923 Jy/beam ! Combined flux in latest and established models = 0.194627 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 17 model components to the UV plane model. ! The established model now contains 66 components and 0.194627 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.061744Jy sigma=0.938650 ! Fit after self-cal, rms=0.061657Jy sigma=0.937895 wmodel J0037-2145_X_2006_12_18_yyk\_map.mod ! Writing 66 model components to file: J0037-2145_X_2006_12_18_yyk_map.mod wobs J0037-2145_X_2006_12_18_yyk\_uvs.fits ! Writing UV FITS file: J0037-2145_X_2006_12_18_yyk_uvs.fits wwins J0037-2145_X_2006_12_18_yyk\_map.win ! wwins: Wrote 3 windows to J0037-2145_X_2006_12_18_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 0.15% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000781687 Jy ! Component: 100 - total flux cleaned = -0.000780703 Jy ! Component: 150 - total flux cleaned = -0.000464787 Jy ! Component: 200 - total flux cleaned = -5.84467e-05 Jy ! Component: 250 - total flux cleaned = 0.000382942 Jy ! Component: 300 - total flux cleaned = 0.000765104 Jy ! Component: 350 - total flux cleaned = 0.000997864 Jy ! Component: 400 - total flux cleaned = 0.00149695 Jy ! Component: 450 - total flux cleaned = 0.00176301 Jy ! Component: 500 - total flux cleaned = 0.00215495 Jy ! Component: 550 - total flux cleaned = 0.00249583 Jy ! Component: 600 - total flux cleaned = 0.00266266 Jy ! Component: 650 - total flux cleaned = 0.00295027 Jy ! Component: 700 - total flux cleaned = 0.00327114 Jy ! Component: 750 - total flux cleaned = 0.00350766 Jy ! Component: 800 - total flux cleaned = 0.00378032 Jy ! Component: 850 - total flux cleaned = 0.00393386 Jy ! Component: 900 - total flux cleaned = 0.00401025 Jy ! Component: 950 - total flux cleaned = 0.00426945 Jy ! Component: 1000 - total flux cleaned = 0.00434239 Jy ! Component: 1050 - total flux cleaned = 0.00445079 Jy ! Component: 1100 - total flux cleaned = 0.00459334 Jy ! Component: 1150 - total flux cleaned = 0.00455841 Jy ! Component: 1200 - total flux cleaned = 0.00466249 Jy ! Component: 1250 - total flux cleaned = 0.00480007 Jy ! Component: 1300 - total flux cleaned = 0.00483413 Jy ! Component: 1350 - total flux cleaned = 0.00490111 Jy ! Component: 1400 - total flux cleaned = 0.00493409 Jy ! Component: 1450 - total flux cleaned = 0.00480449 Jy ! Component: 1500 - total flux cleaned = 0.00490179 Jy ! Component: 1550 - total flux cleaned = 0.00493349 Jy ! Component: 1600 - total flux cleaned = 0.00490193 Jy ! Component: 1650 - total flux cleaned = 0.00490171 Jy ! Component: 1700 - total flux cleaned = 0.00490206 Jy ! Component: 1750 - total flux cleaned = 0.00487154 Jy ! Component: 1800 - total flux cleaned = 0.00487107 Jy ! Component: 1850 - total flux cleaned = 0.00481121 Jy ! Component: 1900 - total flux cleaned = 0.00484017 Jy ! Component: 1950 - total flux cleaned = 0.00475261 Jy ! Component: 2000 - total flux cleaned = 0.00460872 Jy ! Total flux subtracted in 2048 components = 0.00458071 Jy ! Clean residual min=-0.001968 max=0.001643 Jy/beam ! Clean residual mean=0.000002 rms=0.000541 Jy/beam ! Combined flux in latest and established models = 0.199208 Jy keep ! Adding 142 model components to the UV plane model. ! The established model now contains 208 components and 0.199208 Jy ![Exited script file: muppet] wmap "J0037-2145_X_2006_12_18_yyk\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.15% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8723 x 2.141 at 0.1787 degrees (North through East) ! Clean map min=-0.0029688 max=0.093517 Jy/beam ! Writing clean map to FITS file: J0037-2145_X_2006_12_18_yyk_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.093517 invert ! Inverting map ! Your choice of large map pixels excluded 0.15% of the data. ! The x-axis pixel size should ideally be below 0.1994 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000534544 device "J0037-2145_X_2006_12_18_yyk\_map.eps/VPS" ! Attempting to open device: 'J0037-2145_X_2006_12_18_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -1.7148 1.7148 3.42961 6.85921 13.7184 27.4368 54.8737 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0016 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.093 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8723 x 2.141 at 0.1787 degrees (North through East) ! Clean map min=-0.0029688 max=0.093517 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0037-2145_X_2006_12_18_yyk\_map.gif/gif" ! Attempting to open device: 'J0037-2145_X_2006_12_18_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J0037-2145_X_2006_12_18_yyk_uvs.log closed on Mon Jun 16 19:03:52 2008