! Started logfile: J1354-0206_X_2004_05_27_yyk_uvs.log on Wed Dec 7 00:29:04 2005 obs J1354-0206_X_2004_05_27_yyk_uve.fits ! Reading UV FITS file: J1354-0206_X_2004_05_27_yyk_uve.fits ! AN table 1: 4 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.805556 visibilities/baseline/integration-bin. ! Found source: J1354-0206 ! ! 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 1380 lines of history. ! ! Reading 580 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 J1354-0206_X_2004_05_27_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)= 0.668117 Jy startmod ,phase_soltime ! Applying default point source starting model. ! Performing phase self-cal over 10 minute time intervals ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 1 Jy ! ! Correcting IF 1. ! A total of 9 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 9 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 9 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 9 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.376914Jy sigma=7.289191 ! Fit after self-cal, rms=0.376781Jy sigma=7.286429 ! clrmod: Cleared the established, tentative and continuum models. ! Redundant starting model cleared. 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 0.877% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.72 mas, bmaj=2.018 mas, bpa=-4.165 degrees ! Estimated noise=1.89301 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 = 0.566774 Jy ! Component: 100 - total flux cleaned = 0.690986 Jy ! Total flux subtracted in 100 components = 0.690986 Jy ! Clean residual min=-0.018714 max=0.040440 Jy/beam ! Clean residual mean=-0.000222 rms=0.007562 Jy/beam ! Combined flux in latest and established models = 0.690986 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 13 model components to the UV plane model. ! The established model now contains 13 components and 0.690986 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.096699Jy sigma=1.886931 ! Fit after self-cal, rms=0.096651Jy sigma=1.884985 ! Inverting map ! Your choice of large map pixels excluded 0.877% of the data. ! The x-axis pixel size should ideally be below 0.1987 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 0.877% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.7962 mas, bmaj=2.218 mas, bpa=-2.16 degrees ! Estimated noise=1.61565 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 (16.8, -23.8). ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.0592365 Jy ! Component: 100 - total flux cleaned = 0.0837106 Jy ! Component: 150 - total flux cleaned = 0.0944629 Jy ! Component: 200 - total flux cleaned = 0.0961362 Jy ! Total flux subtracted in 200 components = 0.0961362 Jy ! Clean residual min=-0.014034 max=0.011206 Jy/beam ! Clean residual mean=-0.000053 rms=0.003262 Jy/beam ! Combined flux in latest and established models = 0.787122 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 40 model components to the UV plane model. ! The established model now contains 47 components and 0.787122 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.070761Jy sigma=1.279585 ! Fit after self-cal, rms=0.070371Jy sigma=1.272336 ! Inverting map ! Your choice of large map pixels excluded 0.877% 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 ************** ! selflims ampcor_selflim ! 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: 1.0016 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00 HN 0.99 KP 0.99 ! LA 0.98 MK 1.01 NL 1.02 OV 1.02 ! PT 0.97 SC 1.01 ! ! ! Correcting IF 2. ! Amplitude normalization factor in sub-array 1: 1.00669 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00 HN 1.04 KP 0.95 ! LA 0.98 MK 1.02 NL 0.98 OV 0.98 ! PT 1.00 SC 0.99 ! ! ! Correcting IF 3. ! Amplitude normalization factor in sub-array 1: 1.002 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.03 HN 0.92 KP 0.91 ! LA 0.98 MK 1.06 NL 0.98 OV 1.03 ! PT 1.05 SC 1.02 ! ! ! Correcting IF 4. ! Amplitude normalization factor in sub-array 1: 0.982935 ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.03 HN 0.96 KP 0.93 ! LA 0.99 MK 1.08 NL 1.01 OV 1.03 ! PT 1.09 SC 1.04 ! ! ! Fit before self-cal, rms=0.070371Jy sigma=1.272336 ! Fit after self-cal, rms=0.062452Jy sigma=1.078848 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=0.062452Jy sigma=1.078848 ! Fit after self-cal, rms=0.062458Jy sigma=1.078820 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.877% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.8091 mas, bmaj=2.24 mas, bpa=-2.037 degrees ! Estimated noise=1.61565 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 = -0.000514107 Jy ! Component: 100 - total flux cleaned = -3.34767e-05 Jy ! Component: 150 - total flux cleaned = 0.000241004 Jy ! Component: 200 - total flux cleaned = 0.000367153 Jy ! Total flux subtracted in 200 components = 0.000367153 Jy ! Clean residual min=-0.006919 max=0.006917 Jy/beam ! Clean residual mean=-0.000011 rms=0.001678 Jy/beam ! Combined flux in latest and established models = 0.787489 Jy ! Performing phase self-cal over 10 minute time intervals ! Adding 16 model components to the UV plane model. ! The established model now contains 63 components and 0.787489 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.061740Jy sigma=1.066081 ! Fit after self-cal, rms=0.061661Jy sigma=1.065550 ! Inverting map ! Your choice of large map pixels excluded 0.877% 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=0.061661Jy sigma=1.065550 ! Fit after self-cal, rms=0.059276Jy sigma=1.033885 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.877% 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 = 1.2523e-05 Jy ! Component: 100 - total flux cleaned = 0.000112194 Jy ! Component: 150 - total flux cleaned = 2.2779e-05 Jy ! Component: 200 - total flux cleaned = 2.49684e-05 Jy ! Total flux subtracted in 200 components = 2.49684e-05 Jy ! Clean residual min=-0.006680 max=0.006477 Jy/beam ! Clean residual mean=-0.000010 rms=0.001635 Jy/beam ! Combined flux in latest and established models = 0.787514 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 22 model components to the UV plane model. ! The established model now contains 70 components and 0.787514 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.059014Jy sigma=1.029091 ! Fit after self-cal, rms=0.058333Jy sigma=1.024164 ! Inverting map ! Your choice of large map pixels excluded 0.877% 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: 0.8091 x 2.24 at -2.037 degrees (North through East) ! Clean map min=-0.0062351 max=0.64942 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=0.058333Jy sigma=1.024164 ! Fit after self-cal, rms=0.057568Jy sigma=0.999807 ! 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=0.057568Jy sigma=0.999807 ! Fit after self-cal, rms=0.057317Jy sigma=0.998183 ! Inverting map and beam ! Your choice of large map pixels excluded 0.877% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.8094 mas, bmaj=2.243 mas, bpa=-2.101 degrees ! Estimated noise=1.61698 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000510408 Jy ! Component: 100 - total flux cleaned = 0.000596533 Jy ! Component: 150 - total flux cleaned = 0.000517169 Jy ! Component: 200 - total flux cleaned = 0.00044376 Jy ! Total flux subtracted in 200 components = 0.00044376 Jy ! Clean residual min=-0.006685 max=0.005761 Jy/beam ! Clean residual mean=-0.000009 rms=0.001554 Jy/beam ! Combined flux in latest and established models = 0.787958 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 18 model components to the UV plane model. ! The established model now contains 82 components and 0.787958 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.057110Jy sigma=0.994003 ! Fit after self-cal, rms=0.057008Jy sigma=0.993078 ! Inverting map ! Your choice of large map pixels excluded 0.877% of the data. ! The x-axis pixel size should ideally be below 0.1987 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=0.057008Jy sigma=0.993078 ! Fit after self-cal, rms=0.055999Jy sigma=0.967138 ! 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=0.055999Jy sigma=0.967138 ! Fit after self-cal, rms=0.055966Jy sigma=0.966884 ! Inverting map and beam ! Your choice of large map pixels excluded 0.877% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.8093 mas, bmaj=2.243 mas, bpa=-2.141 degrees ! Estimated noise=1.61833 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000901565 Jy ! Component: 100 - total flux cleaned = 0.000978519 Jy ! Component: 150 - total flux cleaned = 0.000981007 Jy ! Component: 200 - total flux cleaned = 0.000913262 Jy ! Total flux subtracted in 200 components = 0.000913262 Jy ! Clean residual min=-0.006494 max=0.005510 Jy/beam ! Clean residual mean=-0.000008 rms=0.001517 Jy/beam ! Combined flux in latest and established models = 0.788871 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 21 model components to the UV plane model. ! The established model now contains 88 components and 0.788871 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.055799Jy sigma=0.963242 ! Fit after self-cal, rms=0.055794Jy sigma=0.962951 ! Inverting map ! Your choice of large map pixels excluded 0.877% of the data. ! The x-axis pixel size should ideally be below 0.1987 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 0.877% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=2.112 mas, bmaj=4.538 mas, bpa=-6.866 degrees ! Estimated noise=2.14745 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 = -0.00016912 Jy ! Component: 100 - total flux cleaned = -0.000385881 Jy ! Component: 150 - total flux cleaned = -0.000518683 Jy ! Component: 200 - total flux cleaned = -0.000693208 Jy ! Total flux subtracted in 200 components = -0.000693208 Jy ! Clean residual min=-0.006634 max=0.005031 Jy/beam ! Clean residual mean=-0.000013 rms=0.001818 Jy/beam ! Combined flux in latest and established models = 0.788178 Jy ! Performing phase self-cal over 0.5 minute time intervals ! Adding 6 model components to the UV plane model. ! The established model now contains 91 components and 0.788178 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.055822Jy sigma=0.962571 ! Fit after self-cal, rms=0.055815Jy sigma=0.962073 ! Inverting map ! Your choice of large map pixels excluded 0.877% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec uvtaper 0,0 ! 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 0.877% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.7257 mas, bmaj=2.029 mas, bpa=-4.132 degrees ! Estimated noise=1.89765 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.567123 Jy ! Component: 100 - total flux cleaned = 0.688238 Jy ! Component: 150 - total flux cleaned = 0.73884 Jy ! Component: 200 - total flux cleaned = 0.762118 Jy ! Total flux subtracted in 200 components = 0.762118 Jy ! Clean residual min=-0.008657 max=0.009862 Jy/beam ! Clean residual mean=-0.000051 rms=0.002373 Jy/beam ! Combined flux in latest and established models = 0.762118 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 30 model components to the UV plane model. ! The established model now contains 30 components and 0.762118 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.877% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.8093 mas, bmaj=2.243 mas, bpa=-2.141 degrees ! Estimated noise=1.61833 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 = 0.0148239 Jy ! Component: 100 - total flux cleaned = 0.0221984 Jy ! Component: 150 - total flux cleaned = 0.0247708 Jy ! Component: 200 - total flux cleaned = 0.0253381 Jy ! Total flux subtracted in 200 components = 0.0253381 Jy ! Clean residual min=-0.006310 max=0.005201 Jy/beam ! Clean residual mean=-0.000014 rms=0.001610 Jy/beam ! Combined flux in latest and established models = 0.787456 Jy ! Adding 35 model components to the UV plane model. ! The established model now contains 56 components and 0.787456 Jy ! Inverting map ! Your choice of large map pixels excluded 0.877% 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 0.877% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=2.112 mas, bmaj=4.538 mas, bpa=-6.866 degrees ! Estimated noise=2.14745 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 = -2.98117e-05 Jy ! Component: 100 - total flux cleaned = 0.00016578 Jy ! Component: 150 - total flux cleaned = 0.000170408 Jy ! Component: 200 - total flux cleaned = 0.000171877 Jy ! Total flux subtracted in 200 components = 0.000171877 Jy ! Clean residual min=-0.006147 max=0.005161 Jy/beam ! Clean residual mean=-0.000019 rms=0.001836 Jy/beam ! Combined flux in latest and established models = 0.787628 Jy ! Adding 10 model components to the UV plane model. ! The established model now contains 63 components and 0.787628 Jy ! Inverting map ! Your choice of large map pixels excluded 0.877% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.877% of the data. ! The x-axis pixel size should ideally be below 0.1987 milli-arcsec ! Estimated beam: bmin=0.8093 mas, bmaj=2.243 mas, bpa=-2.141 degrees ! Estimated noise=1.61833 mJy/beam. ! clean: niter=200 gain=0.04 cutoff=0 ! Component: 050 - total flux cleaned = 0.000472507 Jy ! Component: 100 - total flux cleaned = 0.000479983 Jy ! Component: 150 - total flux cleaned = 0.000478036 Jy ! Component: 200 - total flux cleaned = 0.000555939 Jy ! Total flux subtracted in 200 components = 0.00055594 Jy ! Clean residual min=-0.006249 max=0.005294 Jy/beam ! Clean residual mean=-0.000011 rms=0.001511 Jy/beam ! Combined flux in latest and established models = 0.788184 Jy selfcal false, false, phase_soltime ! Performing phase self-cal over 0.5 minute time intervals ! Adding 22 model components to the UV plane model. ! The established model now contains 78 components and 0.788184 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.055949Jy sigma=0.964669 ! Fit after self-cal, rms=0.055884Jy sigma=0.963509 wmodel J1354-0206_X_2004_05_27_yyk\_map.mod ! Writing 78 model components to file: J1354-0206_X_2004_05_27_yyk_map.mod wobs J1354-0206_X_2004_05_27_yyk\_uvs.fits ! Writing UV FITS file: J1354-0206_X_2004_05_27_yyk_uvs.fits wwins J1354-0206_X_2004_05_27_yyk\_map.win ! wwins: Wrote 2 windows to J1354-0206_X_2004_05_27_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 0.877% 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 = -0.00209531 Jy ! Component: 100 - total flux cleaned = -0.00275271 Jy ! Component: 150 - total flux cleaned = -0.00327253 Jy ! Component: 200 - total flux cleaned = -0.00392131 Jy ! Component: 250 - total flux cleaned = -0.00437146 Jy ! Component: 300 - total flux cleaned = -0.00515945 Jy ! Component: 350 - total flux cleaned = -0.00563961 Jy ! Component: 400 - total flux cleaned = -0.00610291 Jy ! Component: 450 - total flux cleaned = -0.00641823 Jy ! Component: 500 - total flux cleaned = -0.00654003 Jy ! Component: 550 - total flux cleaned = -0.00671876 Jy ! Component: 600 - total flux cleaned = -0.00677839 Jy ! Component: 650 - total flux cleaned = -0.00700379 Jy ! Component: 700 - total flux cleaned = -0.00727364 Jy ! Component: 750 - total flux cleaned = -0.00722042 Jy ! Component: 800 - total flux cleaned = -0.00727185 Jy ! Component: 850 - total flux cleaned = -0.00731993 Jy ! Component: 900 - total flux cleaned = -0.00736895 Jy ! Component: 950 - total flux cleaned = -0.00760894 Jy ! Component: 1000 - total flux cleaned = -0.00793657 Jy ! Component: 1050 - total flux cleaned = -0.00816503 Jy ! Component: 1100 - total flux cleaned = -0.0083442 Jy ! Component: 1150 - total flux cleaned = -0.00847671 Jy ! Component: 1200 - total flux cleaned = -0.00869275 Jy ! Component: 1250 - total flux cleaned = -0.00877735 Jy ! Component: 1300 - total flux cleaned = -0.00898532 Jy ! Component: 1350 - total flux cleaned = -0.00910801 Jy ! Component: 1400 - total flux cleaned = -0.00918904 Jy ! Component: 1450 - total flux cleaned = -0.00922887 Jy ! Component: 1500 - total flux cleaned = -0.00926864 Jy ! Component: 1550 - total flux cleaned = -0.00938441 Jy ! Component: 1600 - total flux cleaned = -0.00942244 Jy ! Component: 1650 - total flux cleaned = -0.0095338 Jy ! Component: 1700 - total flux cleaned = -0.00956995 Jy ! Component: 1750 - total flux cleaned = -0.00953382 Jy ! Component: 1800 - total flux cleaned = -0.00964058 Jy ! Component: 1850 - total flux cleaned = -0.0096056 Jy ! Component: 1900 - total flux cleaned = -0.00974389 Jy ! Component: 1950 - total flux cleaned = -0.00984562 Jy ! Component: 2000 - total flux cleaned = -0.010013 Jy ! Total flux subtracted in 2048 components = -0.0101449 Jy ! Clean residual min=-0.001693 max=0.001722 Jy/beam ! Clean residual mean=-0.000004 rms=0.000610 Jy/beam ! Combined flux in latest and established models = 0.778039 Jy keep ! Adding 109 model components to the UV plane model. ! The established model now contains 187 components and 0.778039 Jy ![Exited script file: muppet] wmap "J1354-0206_X_2004_05_27_yyk\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.877% 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: 0.8093 x 2.243 at -2.141 degrees (North through East) ! Clean map min=-0.0043623 max=0.65122 Jy/beam ! Writing clean map to FITS file: J1354-0206_X_2004_05_27_yyk_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.651217 invert ! Inverting map ! Your choice of large map pixels excluded 0.877% 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 0.000609883 device "J1354-0206_X_2004_05_27_yyk\_map.eps/VPS" ! Attempting to open device: 'J1354-0206_X_2004_05_27_yyk_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.280958 0.280958 0.561917 1.12383 2.24767 4.49533 8.99067 17.9813 35.9627 71.9253 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0018 print "peak=",int(peak_flux*1000)/1000 ! peak= 0.651 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8093 x 2.243 at -2.141 degrees (North through East) ! Clean map min=-0.0043623 max=0.65122 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J1354-0206_X_2004_05_27_yyk\_map.gif/gif" ! Attempting to open device: 'J1354-0206_X_2004_05_27_yyk_map.gif/gif' mapplot cln quit ! Quitting program ! Log file J1354-0206_X_2004_05_27_yyk_uvs.log closed on Wed Dec 7 00:29:07 2005