! Started logfile: J0326-3746_X_2002_01_31_yyk_uvs.log on Wed Jun 27 10:47:13 2007 obs J0326-3746_X_2002_01_31_yyk_uva.fits ! Reading UV FITS file: J0326-3746_X_2002_01_31_yyk_uva.fits ! AN table 1: 34 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.768627 visibilities/baseline/integration-bin. ! Found source: J0326-3746 ! ! 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 4704 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 J0326-3746_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)= 0.196706 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 0.813% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.6966 mas, bmaj=1.725 mas, bpa=0.2527 degrees ! Estimated noise=2489.23 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 = 0.061873 Jy ! Component: 100 - total flux cleaned = 0.0735595 Jy ! Total flux subtracted in 100 components = 0.0735595 Jy ! Clean residual min=-0.014051 max=0.014823 Jy/beam ! Clean residual mean=0.000033 rms=0.003849 Jy/beam ! Combined flux in latest and established models = 0.0735595 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 11 model components to the UV plane model. ! The established model now contains 11 components and 0.0735595 Jy ! ! Correcting IF 1. ! A total of 74 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 74 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 102 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 74 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.183749Jy sigma=0.001306 ! Fit after self-cal, rms=0.183499Jy sigma=0.001304 ! Inverting map and beam ! Your choice of large map pixels excluded 0.813% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.6966 mas, bmaj=1.725 mas, bpa=0.2527 degrees ! Estimated noise=2489.23 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 0.813% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.9308 mas, bmaj=2.387 mas, bpa=-3.714 degrees ! Estimated noise=1536.55 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 = 0.00423089 Jy ! Component: 100 - total flux cleaned = 0.00434232 Jy ! Component: 150 - total flux cleaned = 0.00443068 Jy ! Component: 200 - total flux cleaned = 0.00443258 Jy ! Total flux subtracted in 200 components = 0.00443258 Jy ! Clean residual min=-0.008126 max=0.010049 Jy/beam ! Clean residual mean=0.000097 rms=0.002524 Jy/beam ! Combined flux in latest and established models = 0.0779921 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 10 model components to the UV plane model. ! The established model now contains 20 components and 0.0779921 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.183447Jy sigma=0.001304 ! Fit after self-cal, rms=0.183447Jy sigma=0.001304 ! Inverting map ! Your choice of large map pixels excluded 0.813% 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: 0.9308 x 2.387 at -3.714 degrees (North through East) ! Clean map min=-0.0074135 max=0.074769 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=0.183447Jy sigma=0.001304 ! Fit after self-cal, rms=0.183447Jy sigma=0.001304 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=0.183447Jy sigma=0.001304 ! Fit after self-cal, rms=0.183447Jy sigma=0.001304 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.813% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.9308 mas, bmaj=2.387 mas, bpa=-3.714 degrees ! Estimated noise=1536.55 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 = -7.32802e-06 Jy ! Component: 100 - total flux cleaned = -4.99023e-06 Jy ! Component: 150 - total flux cleaned = -7.29559e-05 Jy ! Component: 200 - total flux cleaned = -0.00013453 Jy ! Total flux subtracted in 200 components = -0.00013453 Jy ! Clean residual min=-0.008142 max=0.010090 Jy/beam ! Clean residual mean=0.000096 rms=0.002511 Jy/beam ! Combined flux in latest and established models = 0.0778576 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 11 model components to the UV plane model. ! The established model now contains 22 components and 0.0778576 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.183432Jy sigma=0.001303 ! Fit after self-cal, rms=0.183431Jy sigma=0.001303 ! Inverting map ! Your choice of large map pixels excluded 0.813% 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=0.183431Jy sigma=0.001303 ! Fit after self-cal, rms=0.181157Jy sigma=0.001289 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.813% 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 = 0.00349242 Jy ! Component: 100 - total flux cleaned = 0.00339107 Jy ! Component: 150 - total flux cleaned = 0.00331324 Jy ! Component: 200 - total flux cleaned = 0.00317256 Jy ! Total flux subtracted in 200 components = 0.00317256 Jy ! Clean residual min=-0.008469 max=0.008223 Jy/beam ! Clean residual mean=0.000025 rms=0.002169 Jy/beam ! Combined flux in latest and established models = 0.0810301 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 27 components and 0.0810301 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.181083Jy sigma=0.001288 ! Fit after self-cal, rms=0.180719Jy sigma=0.001286 ! Inverting map ! Your choice of large map pixels excluded 0.813% 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: 0.9308 x 2.387 at -3.714 degrees (North through East) ! Clean map min=-0.0076544 max=0.082275 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 0.813% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=3.171 mas, bmaj=11.13 mas, bpa=4.967 degrees ! Estimated noise=1882.08 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 = -3.61225e-05 Jy ! Component: 100 - total flux cleaned = -3.54154e-05 Jy ! Component: 150 - total flux cleaned = -3.37753e-05 Jy ! Component: 200 - total flux cleaned = -3.32419e-05 Jy ! Total flux subtracted in 200 components = -3.32419e-05 Jy ! Clean residual min=-0.006951 max=0.005971 Jy/beam ! Clean residual mean=0.000037 rms=0.002271 Jy/beam ! Combined flux in latest and established models = 0.0809969 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 0.0809969 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.180718Jy sigma=0.001286 ! Fit after self-cal, rms=0.180635Jy sigma=0.001285 ! Inverting map ! Your choice of large map pixels excluded 0.813% 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 0.813% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.6966 mas, bmaj=1.725 mas, bpa=0.2527 degrees ! Estimated noise=2489.23 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0687879 Jy ! Component: 100 - total flux cleaned = 0.0798988 Jy ! Component: 150 - total flux cleaned = 0.0801478 Jy ! Component: 200 - total flux cleaned = 0.0801514 Jy ! Total flux subtracted in 200 components = 0.0801514 Jy ! Clean residual min=-0.013976 max=0.013740 Jy/beam ! Clean residual mean=-0.000001 rms=0.003826 Jy/beam ! Combined flux in latest and established models = 0.0801514 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 14 model components to the UV plane model. ! The established model now contains 14 components and 0.0801514 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.813% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.9308 mas, bmaj=2.387 mas, bpa=-3.714 degrees ! Estimated noise=1536.55 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 = 0.0016571 Jy ! Component: 100 - total flux cleaned = 0.0015282 Jy ! Component: 150 - total flux cleaned = 0.00132824 Jy ! Component: 200 - total flux cleaned = 0.00124772 Jy ! Total flux subtracted in 200 components = 0.00124772 Jy ! Clean residual min=-0.008528 max=0.008274 Jy/beam ! Clean residual mean=0.000034 rms=0.002140 Jy/beam ! Combined flux in latest and established models = 0.0813992 Jy ! Adding 10 model components to the UV plane model. ! The established model now contains 22 components and 0.0813991 Jy ! Inverting map ! Your choice of large map pixels excluded 0.813% 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 0.813% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=3.171 mas, bmaj=11.13 mas, bpa=4.967 degrees ! Estimated noise=1882.08 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 = -0.000519953 Jy ! Component: 100 - total flux cleaned = -0.000516843 Jy ! Component: 150 - total flux cleaned = -0.000515802 Jy ! Component: 200 - total flux cleaned = -0.00051526 Jy ! Total flux subtracted in 200 components = -0.00051526 Jy ! Clean residual min=-0.006916 max=0.005814 Jy/beam ! Clean residual mean=0.000041 rms=0.002264 Jy/beam ! Combined flux in latest and established models = 0.0808839 Jy ! Adding 5 model components to the UV plane model. ! The established model now contains 27 components and 0.0808839 Jy ! Inverting map ! Your choice of large map pixels excluded 0.813% 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 0.813% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.9308 mas, bmaj=2.387 mas, bpa=-3.714 degrees ! Estimated noise=1536.55 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000210834 Jy ! Component: 100 - total flux cleaned = 0.000203338 Jy ! Component: 150 - total flux cleaned = 0.000201075 Jy ! Component: 200 - total flux cleaned = 0.000139244 Jy ! Total flux subtracted in 200 components = 0.000139244 Jy ! Clean residual min=-0.008472 max=0.008063 Jy/beam ! Clean residual mean=0.000031 rms=0.002113 Jy/beam ! Combined flux in latest and established models = 0.0810231 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 32 components and 0.0810231 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.180587Jy sigma=0.001285 ! Fit after self-cal, rms=0.180570Jy sigma=0.001285 wmodel J0326-3746_X_2002_01_31_yyk\_map.mod ! Writing 32 model components to file: J0326-3746_X_2002_01_31_yyk_map.mod wobs J0326-3746_X_2002_01_31_yyk\_uvs.fits ! Applying 34 buffered edits. ! Writing UV FITS file: J0326-3746_X_2002_01_31_yyk_uvs.fits wwins J0326-3746_X_2002_01_31_yyk\_map.win ! wwins: Wrote 1 windows to J0326-3746_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 0.813% 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 = -0.00121015 Jy ! Component: 100 - total flux cleaned = -0.00183765 Jy ! Component: 150 - total flux cleaned = -0.00264601 Jy ! Component: 200 - total flux cleaned = -0.00349501 Jy ! Component: 250 - total flux cleaned = -0.00417809 Jy ! Component: 300 - total flux cleaned = -0.00463454 Jy ! Component: 350 - total flux cleaned = -0.00488961 Jy ! Component: 400 - total flux cleaned = -0.00521489 Jy ! Component: 450 - total flux cleaned = -0.00567059 Jy ! Component: 500 - total flux cleaned = -0.00574157 Jy ! Component: 550 - total flux cleaned = -0.00553101 Jy ! Component: 600 - total flux cleaned = -0.00546298 Jy ! Component: 650 - total flux cleaned = -0.00527134 Jy ! Component: 700 - total flux cleaned = -0.00508463 Jy ! Component: 750 - total flux cleaned = -0.00472635 Jy ! Component: 800 - total flux cleaned = -0.00455468 Jy ! Component: 850 - total flux cleaned = -0.00455462 Jy ! Component: 900 - total flux cleaned = -0.0044995 Jy ! Component: 950 - total flux cleaned = -0.00444681 Jy ! Component: 1000 - total flux cleaned = -0.00429229 Jy ! Component: 1050 - total flux cleaned = -0.00414182 Jy ! Component: 1100 - total flux cleaned = -0.0040429 Jy ! Component: 1150 - total flux cleaned = -0.00380111 Jy ! Component: 1200 - total flux cleaned = -0.00384848 Jy ! Component: 1250 - total flux cleaned = -0.00380167 Jy ! Component: 1300 - total flux cleaned = -0.00375524 Jy ! Component: 1350 - total flux cleaned = -0.00379951 Jy ! Component: 1400 - total flux cleaned = -0.00397615 Jy ! Component: 1450 - total flux cleaned = -0.00410679 Jy ! Component: 1500 - total flux cleaned = -0.00419284 Jy ! Component: 1550 - total flux cleaned = -0.00436447 Jy ! Component: 1600 - total flux cleaned = -0.00449184 Jy ! Component: 1650 - total flux cleaned = -0.00466047 Jy ! Component: 1700 - total flux cleaned = -0.00461867 Jy ! Component: 1750 - total flux cleaned = -0.00470244 Jy ! Component: 1800 - total flux cleaned = -0.00474364 Jy ! Component: 1850 - total flux cleaned = -0.004661 Jy ! Component: 1900 - total flux cleaned = -0.00461997 Jy ! Component: 1950 - total flux cleaned = -0.00449727 Jy ! Component: 2000 - total flux cleaned = -0.00445636 Jy ! Total flux subtracted in 2048 components = -0.00445648 Jy ! Clean residual min=-0.002485 max=0.002202 Jy/beam ! Clean residual mean=0.000023 rms=0.000751 Jy/beam ! Combined flux in latest and established models = 0.0765666 Jy keep ! Adding 104 model components to the UV plane model. ! The established model now contains 136 components and 0.0765666 Jy ![Exited script file: muppet] wmap "J0326-3746_X_2002_01_31_yyk\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.813% 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: 0.9308 x 2.387 at -3.714 degrees (North through East) ! Clean map min=-0.0061583 max=0.082746 Jy/beam ! Writing clean map to FITS file: J0326-3746_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 0.0827455 invert ! Inverting map ! Your choice of large map pixels excluded 0.813% 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 0.000751085 device "J0326-3746_X_2002_01_31_yyk\_map.eps/VPS" ! Attempting to open device: 'J0326-3746_X_2002_01_31_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -2.72311 2.72311 5.44623 10.8925 21.7849 43.5698 87.1397 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0022 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.082 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9308 x 2.387 at -3.714 degrees (North through East) ! Clean map min=-0.0061583 max=0.082746 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0326-3746_X_2002_01_31_yyk\_map.gif/gif" ! Attempting to open device: 'J0326-3746_X_2002_01_31_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J0326-3746_X_2002_01_31_yyk_uvs.log closed on Wed Jun 27 10:47:19 2007