! Started logfile: J0013-1513_X_2006_12_18_yyk_uvs.log on Mon Jun 16 19:01:50 2008 obs J0013-1513_X_2006_12_18_yyk_uve.fits ! Reading UV FITS file: J0013-1513_X_2006_12_18_yyk_uve.fits ! AN table 1: 15 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.862222 visibilities/baseline/integration-bin. ! Found source: J0013-1513 ! ! 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 2161 lines of history. ! ! Reading 2328 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 J0013-1513_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)= 0.116264 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 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1999 milli-arcsec ! Estimated beam: bmin=0.6731 mas, bmaj=1.741 mas, bpa=-3.032 degrees ! Estimated noise=1.23674 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 = 0.0595384 Jy ! Component: 100 - total flux cleaned = 0.0822434 Jy ! Total flux subtracted in 100 components = 0.0822434 Jy ! Clean residual min=-0.009073 max=0.012107 Jy/beam ! Clean residual mean=-0.000029 rms=0.002623 Jy/beam ! Combined flux in latest and established models = 0.0822434 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 15 model components to the UV plane model. ! The established model now contains 15 components and 0.0822434 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 14 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=0.082779Jy sigma=1.484115 ! Fit after self-cal, rms=0.074384Jy sigma=1.277185 ! Inverting map and beam ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1999 milli-arcsec ! Estimated beam: bmin=0.6731 mas, bmaj=1.741 mas, bpa=-3.032 degrees ! Estimated noise=1.23674 mJy/beam. ! clean: niter=100 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0226287 Jy ! Component: 100 - total flux cleaned = 0.0330793 Jy ! Total flux subtracted in 100 components = 0.0330793 Jy ! Clean residual min=-0.005142 max=0.005945 Jy/beam ! Clean residual mean=0.000005 rms=0.001430 Jy/beam ! Combined flux in latest and established models = 0.115323 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 15 model components to the UV plane model. ! The established model now contains 23 components and 0.115323 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.068121Jy sigma=1.139297 ! Fit after self-cal, rms=0.068070Jy sigma=1.138678 ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1999 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 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1999 milli-arcsec ! Estimated beam: bmin=0.8632 mas, bmaj=2.24 mas, bpa=-3.884 degrees ! Estimated noise=0.823926 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 = 0.00742337 Jy ! Component: 100 - total flux cleaned = 0.00996525 Jy ! Component: 150 - total flux cleaned = 0.0107797 Jy ! Component: 200 - total flux cleaned = 0.0108827 Jy ! Total flux subtracted in 200 components = 0.0108827 Jy ! Clean residual min=-0.002942 max=0.003368 Jy/beam ! Clean residual mean=0.000012 rms=0.000871 Jy/beam ! Combined flux in latest and established models = 0.126205 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 15 model components to the UV plane model. ! The established model now contains 32 components and 0.126205 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.067621Jy sigma=1.128421 ! Fit after self-cal, rms=0.067605Jy sigma=1.128222 ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1999 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8632 x 2.24 at -3.884 degrees (North through East) ! Clean map min=-0.0026948 max=0.087977 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=0.067605Jy sigma=1.128222 ! Fit after self-cal, rms=0.067605Jy sigma=1.128222 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=0.067605Jy sigma=1.128222 ! Fit after self-cal, rms=0.067597Jy sigma=1.128099 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1999 milli-arcsec ! Estimated beam: bmin=0.8632 mas, bmaj=2.24 mas, bpa=-3.884 degrees ! Estimated noise=0.823926 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 = 1.14596e-05 Jy ! Component: 100 - total flux cleaned = 0.000157262 Jy ! Component: 150 - total flux cleaned = 0.000207602 Jy ! Component: 200 - total flux cleaned = 0.000253579 Jy ! Total flux subtracted in 200 components = 0.000253579 Jy ! Clean residual min=-0.002950 max=0.003328 Jy/beam ! Clean residual mean=0.000012 rms=0.000867 Jy/beam ! Combined flux in latest and established models = 0.126459 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 11 model components to the UV plane model. ! The established model now contains 34 components and 0.126459 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.067591Jy sigma=1.127804 ! Fit after self-cal, rms=0.067580Jy sigma=1.127681 ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1999 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=0.067580Jy sigma=1.127681 ! Fit after self-cal, rms=0.058212Jy sigma=0.951485 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1999 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 = 0.00503734 Jy ! Component: 100 - total flux cleaned = 0.004901 Jy ! Component: 150 - total flux cleaned = 0.00480101 Jy ! Component: 200 - total flux cleaned = 0.00471961 Jy ! Total flux subtracted in 200 components = 0.00471961 Jy ! Clean residual min=-0.003285 max=0.003565 Jy/beam ! Clean residual mean=0.000014 rms=0.000831 Jy/beam ! Combined flux in latest and established models = 0.131179 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 41 components and 0.131179 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.057516Jy sigma=0.938900 ! Fit after self-cal, rms=0.057188Jy sigma=0.934725 ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1999 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: 0.8632 x 2.24 at -3.884 degrees (North through East) ! Clean map min=-0.0031502 max=0.094567 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 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1999 milli-arcsec ! Estimated beam: bmin=2.095 mas, bmaj=4.534 mas, bpa=0.6236 degrees ! Estimated noise=1.05977 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 = -4.64463e-07 Jy ! Component: 100 - total flux cleaned = -0.00012077 Jy ! Component: 150 - total flux cleaned = -0.000224762 Jy ! Component: 200 - total flux cleaned = -0.000287369 Jy ! Total flux subtracted in 200 components = -0.000287369 Jy ! Clean residual min=-0.003733 max=0.003864 Jy/beam ! Clean residual mean=0.000028 rms=0.001020 Jy/beam ! Combined flux in latest and established models = 0.130891 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 7 model components to the UV plane model. ! The established model now contains 44 components and 0.130891 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.057205Jy sigma=0.935146 ! Fit after self-cal, rms=0.057152Jy sigma=0.934602 ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1999 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 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1999 milli-arcsec ! Estimated beam: bmin=0.6731 mas, bmaj=1.741 mas, bpa=-3.032 degrees ! Estimated noise=1.23674 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0784296 Jy ! Component: 100 - total flux cleaned = 0.105706 Jy ! Component: 150 - total flux cleaned = 0.118633 Jy ! Component: 200 - total flux cleaned = 0.125032 Jy ! Total flux subtracted in 200 components = 0.125032 Jy ! Clean residual min=-0.004512 max=0.004725 Jy/beam ! Clean residual mean=0.000006 rms=0.001132 Jy/beam ! Combined flux in latest and established models = 0.125032 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 15 model components to the UV plane model. ! The established model now contains 15 components and 0.125032 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1999 milli-arcsec ! Estimated beam: bmin=0.8632 mas, bmaj=2.24 mas, bpa=-3.884 degrees ! Estimated noise=0.823926 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 = 0.00403858 Jy ! Component: 100 - total flux cleaned = 0.00538696 Jy ! Component: 150 - total flux cleaned = 0.00544969 Jy ! Component: 200 - total flux cleaned = 0.00547983 Jy ! Total flux subtracted in 200 components = 0.00547983 Jy ! Clean residual min=-0.003391 max=0.003548 Jy/beam ! Clean residual mean=0.000012 rms=0.000803 Jy/beam ! Combined flux in latest and established models = 0.130512 Jy ! Adding 11 model components to the UV plane model. ! The established model now contains 23 components and 0.130512 Jy ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1999 milli-arcsec ! Added new window around map position (16.2, 16.6). ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.00264785 Jy ! Component: 100 - total flux cleaned = 0.00272023 Jy ! Component: 150 - total flux cleaned = 0.00299994 Jy ! Component: 200 - total flux cleaned = 0.00299826 Jy ! Total flux subtracted in 200 components = 0.00299826 Jy ! Clean residual min=-0.003243 max=0.002556 Jy/beam ! Clean residual mean=0.000009 rms=0.000732 Jy/beam ! Combined flux in latest and established models = 0.13351 Jy ! Adding 24 model components to the UV plane model. ! The established model now contains 47 components and 0.13351 Jy ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1999 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 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1999 milli-arcsec ! Estimated beam: bmin=2.095 mas, bmaj=4.534 mas, bpa=0.6236 degrees ! Estimated noise=1.05977 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 = 0.000396503 Jy ! Component: 100 - total flux cleaned = 0.000640045 Jy ! Component: 150 - total flux cleaned = 0.000807652 Jy ! Component: 200 - total flux cleaned = 0.000924291 Jy ! Total flux subtracted in 200 components = 0.000924291 Jy ! Clean residual min=-0.003769 max=0.003216 Jy/beam ! Clean residual mean=0.000023 rms=0.000879 Jy/beam ! Combined flux in latest and established models = 0.134435 Jy ! Adding 19 model components to the UV plane model. ! The established model now contains 63 components and 0.134435 Jy ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1999 milli-arcsec uvtaper 0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1999 milli-arcsec ! Estimated beam: bmin=0.8632 mas, bmaj=2.24 mas, bpa=-3.884 degrees ! Estimated noise=0.823926 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -0.000275256 Jy ! Component: 100 - total flux cleaned = -0.000230348 Jy ! Component: 150 - total flux cleaned = -0.000231063 Jy ! Component: 200 - total flux cleaned = -0.000192335 Jy ! Total flux subtracted in 200 components = -0.000192335 Jy ! Clean residual min=-0.003168 max=0.002539 Jy/beam ! Clean residual mean=0.000010 rms=0.000713 Jy/beam ! Combined flux in latest and established models = 0.134242 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 20 model components to the UV plane model. ! The established model now contains 78 components and 0.134242 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.056709Jy sigma=0.925558 ! Fit after self-cal, rms=0.056673Jy sigma=0.925003 wmodel J0013-1513_X_2006_12_18_yyk\_map.mod ! Writing 78 model components to file: J0013-1513_X_2006_12_18_yyk_map.mod wobs J0013-1513_X_2006_12_18_yyk\_uvs.fits ! Writing UV FITS file: J0013-1513_X_2006_12_18_yyk_uvs.fits wwins J0013-1513_X_2006_12_18_yyk\_map.win ! wwins: Wrote 2 windows to J0013-1513_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 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1999 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00124806 Jy ! Component: 100 - total flux cleaned = -0.00148506 Jy ! Component: 150 - total flux cleaned = -0.00131033 Jy ! Component: 200 - total flux cleaned = -0.00114582 Jy ! Component: 250 - total flux cleaned = -0.000947748 Jy ! Component: 300 - total flux cleaned = -0.000832426 Jy ! Component: 350 - total flux cleaned = -0.000647321 Jy ! Component: 400 - total flux cleaned = -0.00050433 Jy ! Component: 450 - total flux cleaned = -0.000540347 Jy ! Component: 500 - total flux cleaned = -0.000403858 Jy ! Component: 550 - total flux cleaned = -0.000304293 Jy ! Component: 600 - total flux cleaned = -0.00020584 Jy ! Component: 650 - total flux cleaned = -0.000141383 Jy ! Component: 700 - total flux cleaned = 1.57296e-05 Jy ! Component: 750 - total flux cleaned = 0.000169089 Jy ! Component: 800 - total flux cleaned = 0.00016844 Jy ! Component: 850 - total flux cleaned = 0.000287589 Jy ! Component: 900 - total flux cleaned = 0.000257714 Jy ! Component: 950 - total flux cleaned = 0.000286557 Jy ! Component: 1000 - total flux cleaned = 0.000230168 Jy ! Component: 1050 - total flux cleaned = 0.000257807 Jy ! Component: 1100 - total flux cleaned = 0.000203295 Jy ! Component: 1150 - total flux cleaned = 0.000123088 Jy ! Component: 1200 - total flux cleaned = 0.000123104 Jy ! Component: 1250 - total flux cleaned = 1.88253e-05 Jy ! Component: 1300 - total flux cleaned = -3.21807e-05 Jy ! Component: 1350 - total flux cleaned = -3.2064e-05 Jy ! Component: 1400 - total flux cleaned = -7.61624e-06 Jy ! Component: 1450 - total flux cleaned = -8.19323e-05 Jy ! Component: 1500 - total flux cleaned = -0.000106256 Jy ! Component: 1550 - total flux cleaned = -0.000178005 Jy ! Component: 1600 - total flux cleaned = -0.000178172 Jy ! Component: 1650 - total flux cleaned = -0.000131338 Jy ! Component: 1700 - total flux cleaned = -6.13677e-05 Jy ! Component: 1750 - total flux cleaned = -3.85829e-05 Jy ! Component: 1800 - total flux cleaned = 5.21085e-05 Jy ! Component: 1850 - total flux cleaned = 0.00018607 Jy ! Component: 1900 - total flux cleaned = 0.000208288 Jy ! Component: 1950 - total flux cleaned = 0.000295806 Jy ! Component: 2000 - total flux cleaned = 0.000360803 Jy ! Total flux subtracted in 2048 components = 0.000446998 Jy ! Clean residual min=-0.001395 max=0.001556 Jy/beam ! Clean residual mean=0.000004 rms=0.000409 Jy/beam ! Combined flux in latest and established models = 0.134689 Jy keep ! Adding 138 model components to the UV plane model. ! The established model now contains 216 components and 0.134689 Jy ![Exited script file: muppet] wmap "J0013-1513_X_2006_12_18_yyk\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1999 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8632 x 2.24 at -3.884 degrees (North through East) ! Clean map min=-0.0023663 max=0.095725 Jy/beam ! Writing clean map to FITS file: J0013-1513_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 0.0957249 invert ! Inverting map ! Your choice of large map pixels excluded 0.183% of the data. ! The x-axis pixel size should ideally be below 0.1999 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000406706 device "J0013-1513_X_2006_12_18_yyk\_map.eps/VPS" ! Attempting to open device: 'J0013-1513_X_2006_12_18_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -1.27461 1.27461 2.54922 5.09844 10.1969 20.3938 40.7875 81.5751 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0012 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.095 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8632 x 2.24 at -3.884 degrees (North through East) ! Clean map min=-0.0023663 max=0.095725 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0013-1513_X_2006_12_18_yyk\_map.gif/gif" ! Attempting to open device: 'J0013-1513_X_2006_12_18_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J0013-1513_X_2006_12_18_yyk_uvs.log closed on Mon Jun 16 19:01:56 2008