! Started logfile: J0929-3801_X_2002_01_31_yyk_uvs.log on Wed Jun 27 10:54:53 2007 obs J0929-3801_X_2002_01_31_yyk_uva.fits ! Reading UV FITS file: J0929-3801_X_2002_01_31_yyk_uva.fits ! AN table 1: 45 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.73037 visibilities/baseline/integration-bin. ! Found source: J0929-3801 ! ! 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 5916 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 J0929-3801_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)= 0.29062 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 0.768% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.693 mas, bmaj=1.829 mas, bpa=3.931 degrees ! Estimated noise=2125.82 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 = 0.192219 Jy ! Component: 100 - total flux cleaned = 0.247456 Jy ! Total flux subtracted in 100 components = 0.247456 Jy ! Clean residual min=-0.020100 max=0.023187 Jy/beam ! Clean residual mean=-0.000064 rms=0.006307 Jy/beam ! Combined flux in latest and established models = 0.247456 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 12 model components to the UV plane model. ! The established model now contains 12 components and 0.247456 Jy ! ! Correcting IF 1. ! A total of 110 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 110 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 110 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 110 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.171125Jy sigma=0.001311 ! Fit after self-cal, rms=0.170907Jy sigma=0.001310 ! Inverting map and beam ! Your choice of large map pixels excluded 0.768% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.693 mas, bmaj=1.829 mas, bpa=3.931 degrees ! Estimated noise=2125.82 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 0.768% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.8517 mas, bmaj=2.217 mas, bpa=2.863 degrees ! Estimated noise=1301.78 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 = 0.0306233 Jy ! Component: 100 - total flux cleaned = 0.0396537 Jy ! Component: 150 - total flux cleaned = 0.0423687 Jy ! Component: 200 - total flux cleaned = 0.0425268 Jy ! Total flux subtracted in 200 components = 0.0425268 Jy ! Clean residual min=-0.016998 max=0.012942 Jy/beam ! Clean residual mean=0.000306 rms=0.004455 Jy/beam ! Combined flux in latest and established models = 0.289983 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 17 model components to the UV plane model. ! The established model now contains 23 components and 0.289983 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.168650Jy sigma=0.001281 ! Fit after self-cal, rms=0.168634Jy sigma=0.001281 ! Inverting map ! Your choice of large map pixels excluded 0.768% 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: 0.8517 x 2.217 at 2.863 degrees (North through East) ! Clean map min=-0.016281 max=0.23022 Jy/beam if(peak(flux) < thresh*2) selflims ampcor_selflim end if gscale ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 0.995876 ! Telescope amplitude corrections in sub-array 1: ! BR 1.18 FD 0.92 HN 1.00* KP 0.97 ! LA 1.06 MK 1.00 NL 1.00* OV 0.90 ! PT 0.95 SC 1.06 ! ! ! Correcting IF 2. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 1.01166 ! Telescope amplitude corrections in sub-array 1: ! BR 1.20 FD 0.92 HN 1.00* KP 0.92 ! LA 1.10 MK 0.94 NL 1.00* OV 0.87 ! PT 1.00 SC 0.93 ! ! ! Correcting IF 3. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 0.966369 ! Telescope amplitude corrections in sub-array 1: ! BR 1.36 FD 0.82 HN 1.00* KP 0.97 ! LA 1.12 MK 1.03 NL 1.00* OV 0.94 ! PT 1.07 SC 1.04 ! ! ! Correcting IF 4. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Amplitude normalization factor in sub-array 1: 0.95779 ! Telescope amplitude corrections in sub-array 1: ! BR 1.26 FD 0.84 HN 1.00* KP 1.03 ! LA 1.19 MK 1.07 NL 1.00* OV 1.00 ! PT 1.09 SC 0.97 ! ! ! Fit before self-cal, rms=0.168634Jy sigma=0.001281 ! Fit after self-cal, rms=0.169839Jy sigma=0.001251 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=0.169839Jy sigma=0.001251 ! Fit after self-cal, rms=0.169841Jy sigma=0.001251 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.77% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.8528 mas, bmaj=2.239 mas, bpa=2.781 degrees ! Estimated noise=1254.73 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 = -0.00687404 Jy ! Component: 100 - total flux cleaned = -0.00806613 Jy ! Component: 150 - total flux cleaned = -0.00817884 Jy ! Component: 200 - total flux cleaned = -0.00822758 Jy ! Total flux subtracted in 200 components = -0.00822758 Jy ! Clean residual min=-0.005182 max=0.006650 Jy/beam ! Clean residual mean=-0.000145 rms=0.001586 Jy/beam ! Combined flux in latest and established models = 0.281755 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 15 model components to the UV plane model. ! The established model now contains 36 components and 0.281755 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.169626Jy sigma=0.001250 ! Fit after self-cal, rms=0.169622Jy sigma=0.001250 ! Inverting map ! Your choice of large map pixels excluded 0.77% 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=0.169622Jy sigma=0.001250 ! Fit after self-cal, rms=0.161959Jy sigma=0.001185 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.77% 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 = 0.000389027 Jy ! Component: 100 - total flux cleaned = 0.00013031 Jy ! Component: 150 - total flux cleaned = -2.6247e-05 Jy ! Component: 200 - total flux cleaned = -2.48551e-05 Jy ! Total flux subtracted in 200 components = -2.48551e-05 Jy ! Clean residual min=-0.005121 max=0.006032 Jy/beam ! Clean residual mean=-0.000146 rms=0.001615 Jy/beam ! Combined flux in latest and established models = 0.28173 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 8 model components to the UV plane model. ! The established model now contains 40 components and 0.28173 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.161499Jy sigma=0.001181 ! Fit after self-cal, rms=0.160380Jy sigma=0.001172 ! Inverting map ! Your choice of large map pixels excluded 0.77% 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: 0.8528 x 2.239 at 2.781 degrees (North through East) ! Clean map min=-0.0047674 max=0.23179 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 ! Performing amp+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=0.160380Jy sigma=0.001172 ! Fit after self-cal, rms=0.160596Jy sigma=0.001167 ! 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=0.160596Jy sigma=0.001167 ! Fit after self-cal, rms=0.160382Jy sigma=0.001165 ! Inverting map and beam ! Your choice of large map pixels excluded 0.77% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.8393 mas, bmaj=2.224 mas, bpa=3.553 degrees ! Estimated noise=1241.63 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000172131 Jy ! Component: 100 - total flux cleaned = 8.9546e-05 Jy ! Component: 150 - total flux cleaned = 0.000124256 Jy ! Component: 200 - total flux cleaned = 0.000156881 Jy ! Total flux subtracted in 200 components = 0.000156881 Jy ! Clean residual min=-0.004935 max=0.005453 Jy/beam ! Clean residual mean=-0.000149 rms=0.001449 Jy/beam ! Combined flux in latest and established models = 0.281887 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 49 components and 0.281887 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.160362Jy sigma=0.001165 ! Fit after self-cal, rms=0.160312Jy sigma=0.001165 ! Inverting map ! Your choice of large map pixels excluded 0.77% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Performing amp+phase self-cal over 1 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.160312Jy sigma=0.001165 ! Fit after self-cal, rms=0.161064Jy sigma=0.001162 ! 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=0.161064Jy sigma=0.001162 ! Fit after self-cal, rms=0.161060Jy sigma=0.001162 ! Inverting map and beam ! Your choice of large map pixels excluded 0.77% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.8406 mas, bmaj=2.226 mas, bpa=3.719 degrees ! Estimated noise=1242.97 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000388527 Jy ! Component: 100 - total flux cleaned = 0.00041659 Jy ! Component: 150 - total flux cleaned = 0.000446245 Jy ! Component: 200 - total flux cleaned = 0.000474165 Jy ! Total flux subtracted in 200 components = 0.000474165 Jy ! Clean residual min=-0.004972 max=0.005297 Jy/beam ! Clean residual mean=-0.000151 rms=0.001441 Jy/beam ! Combined flux in latest and established models = 0.282361 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 52 components and 0.282361 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.161048Jy sigma=0.001162 ! Fit after self-cal, rms=0.161053Jy sigma=0.001162 ! Inverting map ! Your choice of large map pixels excluded 0.77% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! ************** FINISHED AMPLITUDE SELF-CAL ************** 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 0.77% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=3.025 mas, bmaj=10.93 mas, bpa=6.861 degrees ! Estimated noise=1597.71 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 = 0.000936342 Jy ! Component: 100 - total flux cleaned = 0.000933391 Jy ! Component: 150 - total flux cleaned = 0.000955724 Jy ! Component: 200 - total flux cleaned = 0.000978608 Jy ! Total flux subtracted in 200 components = 0.000978608 Jy ! Clean residual min=-0.005029 max=0.007243 Jy/beam ! Clean residual mean=-0.000259 rms=0.002000 Jy/beam ! Combined flux in latest and established models = 0.28334 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 3 model components to the UV plane model. ! The established model now contains 54 components and 0.28334 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.161054Jy sigma=0.001162 ! Fit after self-cal, rms=0.161060Jy sigma=0.001162 ! Inverting map ! Your choice of large map pixels excluded 0.77% 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 0.77% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.6879 mas, bmaj=1.833 mas, bpa=4.592 degrees ! Estimated noise=2043.27 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.193764 Jy ! Component: 100 - total flux cleaned = 0.244793 Jy ! Component: 150 - total flux cleaned = 0.266409 Jy ! Component: 200 - total flux cleaned = 0.275702 Jy ! Total flux subtracted in 200 components = 0.275702 Jy ! Clean residual min=-0.007696 max=0.008392 Jy/beam ! Clean residual mean=-0.000119 rms=0.002291 Jy/beam ! Combined flux in latest and established models = 0.275702 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 16 model components to the UV plane model. ! The established model now contains 16 components and 0.275702 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.77% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.8406 mas, bmaj=2.226 mas, bpa=3.719 degrees ! Estimated noise=1242.97 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 = 0.00513993 Jy ! Component: 100 - total flux cleaned = 0.00554165 Jy ! Component: 150 - total flux cleaned = 0.00593776 Jy ! Component: 200 - total flux cleaned = 0.00619048 Jy ! Total flux subtracted in 200 components = 0.00619048 Jy ! Clean residual min=-0.005220 max=0.005783 Jy/beam ! Clean residual mean=-0.000154 rms=0.001493 Jy/beam ! Combined flux in latest and established models = 0.281892 Jy ! Adding 24 model components to the UV plane model. ! The established model now contains 34 components and 0.281892 Jy ! Inverting map ! Your choice of large map pixels excluded 0.77% 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 0.77% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=3.025 mas, bmaj=10.93 mas, bpa=6.861 degrees ! Estimated noise=1597.71 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 = 0.00175271 Jy ! Component: 100 - total flux cleaned = 0.00175123 Jy ! Component: 150 - total flux cleaned = 0.00174917 Jy ! Component: 200 - total flux cleaned = 0.0017475 Jy ! Total flux subtracted in 200 components = 0.0017475 Jy ! Clean residual min=-0.005042 max=0.007272 Jy/beam ! Clean residual mean=-0.000257 rms=0.002001 Jy/beam ! Combined flux in latest and established models = 0.28364 Jy ! Adding 6 model components to the UV plane model. ! The established model now contains 38 components and 0.28364 Jy ! Inverting map ! Your choice of large map pixels excluded 0.77% 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 0.77% of the data. ! The x-axis pixel size should ideally be below 0.1986 milli-arcsec ! Estimated beam: bmin=0.8406 mas, bmaj=2.226 mas, bpa=3.719 degrees ! Estimated noise=1242.97 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = -0.000860157 Jy ! Component: 100 - total flux cleaned = -0.000651361 Jy ! Component: 150 - total flux cleaned = -0.000597646 Jy ! Component: 200 - total flux cleaned = -0.00059863 Jy ! Total flux subtracted in 200 components = -0.00059863 Jy ! Clean residual min=-0.004784 max=0.005238 Jy/beam ! Clean residual mean=-0.000148 rms=0.001459 Jy/beam ! Combined flux in latest and established models = 0.283041 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 15 model components to the UV plane model. ! The established model now contains 47 components and 0.283041 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.161081Jy sigma=0.001162 ! Fit after self-cal, rms=0.161075Jy sigma=0.001162 wmodel J0929-3801_X_2002_01_31_yyk\_map.mod ! Writing 47 model components to file: J0929-3801_X_2002_01_31_yyk_map.mod wobs J0929-3801_X_2002_01_31_yyk\_uvs.fits ! Applying 45 buffered edits. ! Writing UV FITS file: J0929-3801_X_2002_01_31_yyk_uvs.fits wwins J0929-3801_X_2002_01_31_yyk\_map.win ! wwins: Wrote 1 windows to J0929-3801_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 0.77% 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 = -0.000177207 Jy ! Component: 100 - total flux cleaned = -0.000257896 Jy ! Component: 150 - total flux cleaned = -0.000117119 Jy ! Component: 200 - total flux cleaned = -5.25665e-05 Jy ! Component: 250 - total flux cleaned = 0.000374926 Jy ! Component: 300 - total flux cleaned = 0.000663847 Jy ! Component: 350 - total flux cleaned = 0.000775079 Jy ! Component: 400 - total flux cleaned = 0.000670929 Jy ! Component: 450 - total flux cleaned = 0.000470425 Jy ! Component: 500 - total flux cleaned = 0.000273929 Jy ! Component: 550 - total flux cleaned = -5.67879e-05 Jy ! Component: 600 - total flux cleaned = -0.00028304 Jy ! Component: 650 - total flux cleaned = -0.000501494 Jy ! Component: 700 - total flux cleaned = -0.000841692 Jy ! Component: 750 - total flux cleaned = -0.00121237 Jy ! Component: 800 - total flux cleaned = -0.00157223 Jy ! Component: 850 - total flux cleaned = -0.00199974 Jy ! Component: 900 - total flux cleaned = -0.00241533 Jy ! Component: 950 - total flux cleaned = -0.00274712 Jy ! Component: 1000 - total flux cleaned = -0.00321168 Jy ! Component: 1050 - total flux cleaned = -0.00362799 Jy ! Component: 1100 - total flux cleaned = -0.0039997 Jy ! Component: 1150 - total flux cleaned = -0.00442623 Jy ! Component: 1200 - total flux cleaned = -0.00481117 Jy ! Component: 1250 - total flux cleaned = -0.00528151 Jy ! Component: 1300 - total flux cleaned = -0.00580307 Jy ! Component: 1350 - total flux cleaned = -0.00625379 Jy ! Component: 1400 - total flux cleaned = -0.00666682 Jy ! Component: 1450 - total flux cleaned = -0.00707246 Jy ! Component: 1500 - total flux cleaned = -0.00738582 Jy ! Component: 1550 - total flux cleaned = -0.00780634 Jy ! Component: 1600 - total flux cleaned = -0.00824799 Jy ! Component: 1650 - total flux cleaned = -0.00862912 Jy ! Component: 1700 - total flux cleaned = -0.00903211 Jy ! Component: 1750 - total flux cleaned = -0.00945607 Jy ! Component: 1800 - total flux cleaned = -0.00982248 Jy ! Component: 1850 - total flux cleaned = -0.0102368 Jy ! Component: 1900 - total flux cleaned = -0.0106469 Jy ! Component: 1950 - total flux cleaned = -0.0110785 Jy ! Component: 2000 - total flux cleaned = -0.0115314 Jy ! Total flux subtracted in 2048 components = -0.0119059 Jy ! Clean residual min=-0.001401 max=0.001331 Jy/beam ! Clean residual mean=-0.000056 rms=0.000482 Jy/beam ! Combined flux in latest and established models = 0.271136 Jy keep ! Adding 101 model components to the UV plane model. ! The established model now contains 148 components and 0.271135 Jy ![Exited script file: muppet] wmap "J0929-3801_X_2002_01_31_yyk\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.77% 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: 0.8406 x 2.226 at 3.719 degrees (North through East) ! Clean map min=-0.0032317 max=0.22741 Jy/beam ! Writing clean map to FITS file: J0929-3801_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 0.227411 invert ! Inverting map ! Your choice of large map pixels excluded 0.77% 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 0.00048021 device "J0929-3801_X_2002_01_31_yyk\_map.eps/VPS" ! Attempting to open device: 'J0929-3801_X_2002_01_31_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.633493 0.633493 1.26699 2.53397 5.06794 10.1359 20.2718 40.5435 81.0871 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0014 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.227 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8406 x 2.226 at 3.719 degrees (North through East) ! Clean map min=-0.0032317 max=0.22741 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0929-3801_X_2002_01_31_yyk\_map.gif/gif" ! Attempting to open device: 'J0929-3801_X_2002_01_31_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J0929-3801_X_2002_01_31_yyk_uvs.log closed on Wed Jun 27 10:54:59 2007