! Started logfile: J0856-1105_X_2009_04_21_pus_uvs.log on Sun Jan 23 00:26:53 2011 obs J0856-1105_X_2009_04_21_pus_uva.fits ! Reading UV FITS file: J0856-1105_X_2009_04_21_pus_uva.fits ! AN table 1: 77 integrations on 120 of 120 possible baselines. ! AN table 2: 20 integrations on 120 of 120 possible baselines. ! AN table 3: 14 integrations on 120 of 120 possible baselines. ! Apparent sampling: 0.126952 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0856-1105 ! ! 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 2445 lines of history. ! ! Reading 6764 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 print "field_size =",field_size ! field_size = 512 print "field_cell =",field_cell ! field_cell = 0.2 print "taper_size =",taper_size ! taper_size = 70 ![@muppet J0856-1105_X_2009_04_21_pus] integer clean_niter clean_niter = 100 float clean_gain clean_gain = 0.03 float dynam dynam = 6.0 float soltime1 soltime1 = 120 float soltime2 soltime2 = 20 float thresh thresh = 0.5 float win_mult win_mult = 1.8 float time_av time_av = 16 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. startmod ! Applying default point source starting model. ! Performing phase self-cal ! 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 878 telescope corrections were flagged in sub-array 1. ! A total of 261 telescope corrections were flagged in sub-array 2. ! A total of 99 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 878 telescope corrections were flagged in sub-array 1. ! A total of 261 telescope corrections were flagged in sub-array 2. ! A total of 99 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 878 telescope corrections were flagged in sub-array 1. ! A total of 261 telescope corrections were flagged in sub-array 2. ! A total of 99 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 878 telescope corrections were flagged in sub-array 1. ! A total of 261 telescope corrections were flagged in sub-array 2. ! A total of 99 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=0.653629Jy sigma=0.005505 ! Fit after self-cal, rms=0.541520Jy sigma=0.004642 ! 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 0.479% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec ! Estimated beam: bmin=0.5344 mas, bmaj=1.936 mas, bpa=-1.042 degrees ! Estimated noise=1331.5 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (0, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.359785 Jy ! Component: 100 - total flux cleaned = 0.467518 Jy ! Total flux subtracted in 100 components = 0.467518 Jy ! Clean residual min=-0.014969 max=0.050806 Jy/beam ! Clean residual mean=0.000425 rms=0.004709 Jy/beam ! Combined flux in latest and established models = 0.467518 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 8 components and 0.467518 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.185859Jy sigma=0.001501 ! Fit after self-cal, rms=0.185745Jy sigma=0.001501 ! Inverting map ! Your choice of large map pixels excluded 0.479% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0570355 Jy ! Component: 100 - total flux cleaned = 0.0879325 Jy ! Total flux subtracted in 100 components = 0.0879325 Jy ! Clean residual min=-0.011516 max=0.014902 Jy/beam ! Clean residual mean=0.000185 rms=0.002826 Jy/beam ! Combined flux in latest and established models = 0.555451 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 8 components and 0.555451 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.165260Jy sigma=0.001265 ! Fit after self-cal, rms=0.165178Jy sigma=0.001264 ! Inverting map ! Your choice of large map pixels excluded 0.479% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec print "************** FINISHED UNIFORM WEIGHTING CLEAN **************" ! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** ! uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! 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 0.479% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec ! Estimated beam: bmin=0.6486 mas, bmaj=2.238 mas, bpa=-1.773 degrees ! Estimated noise=1014.77 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0212706 Jy ! Component: 100 - total flux cleaned = 0.0317229 Jy ! Component: 150 - total flux cleaned = 0.0374143 Jy ! Component: 200 - total flux cleaned = 0.0405679 Jy ! Total flux subtracted in 200 components = 0.0405679 Jy ! Clean residual min=-0.010674 max=0.009789 Jy/beam ! Clean residual mean=0.000738 rms=0.002436 Jy/beam ! Combined flux in latest and established models = 0.596019 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 22 components and 0.596019 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.163192Jy sigma=0.001235 ! Fit after self-cal, rms=0.163177Jy sigma=0.001235 ! Inverting map ! Your choice of large map pixels excluded 0.479% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 51 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 FD 0.98 HN 1.05 KB 0.97 ! KK 1.06 KP 1.00 LA 0.99 MK 0.98 ! NL 1.06 NY 1.00* OV 0.96 PT 1.05 ! SC 1.00 TS 0.92 WZ 1.20 ZC 1.00* ! ! A total of 27 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* HN 1.00* KB 1.00 ! KK 1.00* KP 1.00* LA 1.00* MK 1.00* ! NL 1.00* NY 1.00* OV 1.00* PT 1.00* ! SC 1.00* TS 1.06 WZ 1.24 ZC 0.99 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.94 FD 0.97 HN 1.00 KB 1.00* ! KK 0.96 KP 0.96 LA 0.96 MK 0.95 ! NL 0.93 NY 1.00* OV 1.00 PT 0.97 ! SC 0.99 TS 1.00* WZ 1.00* ZC 1.00* ! ! ! Correcting IF 2. ! A total of 51 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 FD 0.98 HN 1.03 KB 0.97 ! KK 1.05 KP 1.02 LA 1.00 MK 1.00 ! NL 1.01 NY 1.00* OV 0.94 PT 1.06 ! SC 1.01 TS 0.91 WZ 1.31 ZC 1.00* ! ! A total of 27 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* HN 1.00* KB 1.01 ! KK 1.00* KP 1.00* LA 1.00* MK 1.00* ! NL 1.00* NY 1.00* OV 1.00* PT 1.00* ! SC 1.00* TS 1.10 WZ 1.23 ZC 0.99 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 0.98 HN 0.99 KB 1.00* ! KK 0.93 KP 0.98 LA 0.98 MK 0.93 ! NL 0.92 NY 1.00* OV 0.99 PT 0.94 ! SC 1.00 TS 1.00* WZ 1.00* ZC 1.00* ! ! ! Correcting IF 3. ! A total of 51 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.04 FD 1.01 HN 1.08 KB 0.91 ! KK 1.11 KP 1.02 LA 0.95 MK 0.98 ! NL 1.05 NY 1.00* OV 0.95 PT 1.03 ! SC 1.05 TS 0.97 WZ 1.28 ZC 1.00* ! ! A total of 27 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* HN 1.00* KB 1.14 ! KK 1.00* KP 1.00* LA 1.00* MK 1.00* ! NL 1.00* NY 1.00* OV 1.00* PT 1.00* ! SC 1.00* TS 1.00 WZ 1.14 ZC 0.99 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 FD 1.00 HN 1.03 KB 1.00* ! KK 0.93 KP 0.94 LA 0.99 MK 0.99 ! NL 0.97 NY 1.00* OV 1.02 PT 0.95 ! SC 0.99 TS 1.00* WZ 1.00* ZC 1.00* ! ! ! Correcting IF 4. ! A total of 51 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.95 FD 1.04 HN 1.04 KB 0.93 ! KK 1.00 KP 1.03 LA 0.99 MK 1.01 ! NL 1.06 NY 1.00* OV 1.03 PT 1.00 ! SC 0.98 TS 0.95 WZ 1.30 ZC 1.00* ! ! A total of 27 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* HN 1.00* KB 1.02 ! KK 1.00* KP 1.00* LA 1.00* MK 1.00* ! NL 1.00* NY 1.00* OV 1.00* PT 1.00* ! SC 1.00* TS 1.02 WZ 1.13 ZC 1.07 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 1.03 HN 1.07 KB 1.00* ! KK 0.93 KP 1.00 LA 1.03 MK 1.02 ! NL 0.96 NY 1.00* OV 0.97 PT 0.92 ! SC 1.03 TS 1.00* WZ 1.00* ZC 1.00* ! ! ! Fit before self-cal, rms=0.163177Jy sigma=0.001235 ! Fit after self-cal, rms=0.162226Jy sigma=0.001197 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.472% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec ! Estimated beam: bmin=0.6752 mas, bmaj=2.21 mas, bpa=-2.371 degrees ! Estimated noise=1039.34 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00264369 Jy ! Component: 100 - total flux cleaned = -0.00296151 Jy ! Component: 150 - total flux cleaned = -0.00302741 Jy ! Component: 200 - total flux cleaned = -0.00308058 Jy ! Total flux subtracted in 200 components = -0.00308058 Jy ! Clean residual min=-0.006841 max=0.006351 Jy/beam ! Clean residual mean=-0.000102 rms=0.001800 Jy/beam ! Combined flux in latest and established models = 0.592938 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 27 components and 0.592938 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.162156Jy sigma=0.001196 ! Fit after self-cal, rms=0.162241Jy sigma=0.001196 ! Inverting map ! Your choice of large map pixels excluded 0.472% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec selfcal true, true, soltime1 ! Performing amp+phase self-cal over 120 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.162241Jy sigma=0.001196 ! Fit after self-cal, rms=0.163666Jy sigma=0.001179 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.472% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec ! Estimated beam: bmin=0.6768 mas, bmaj=2.214 mas, bpa=-2.394 degrees ! Estimated noise=1037.33 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00277799 Jy ! Component: 100 - total flux cleaned = -0.00372332 Jy ! Component: 150 - total flux cleaned = -0.00396321 Jy ! Component: 200 - total flux cleaned = -0.00409485 Jy ! Total flux subtracted in 200 components = -0.00409485 Jy ! Clean residual min=-0.005027 max=0.005023 Jy/beam ! Clean residual mean=-0.000033 rms=0.001307 Jy/beam ! Combined flux in latest and established models = 0.588843 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 37 components and 0.588843 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.163619Jy sigma=0.001179 ! Fit after self-cal, rms=0.163681Jy sigma=0.001179 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.472% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000206267 Jy ! Component: 100 - total flux cleaned = -0.000321004 Jy ! Component: 150 - total flux cleaned = -0.000347436 Jy ! Component: 200 - total flux cleaned = -0.000391355 Jy ! Total flux subtracted in 200 components = -0.000391355 Jy ! Clean residual min=-0.005063 max=0.005040 Jy/beam ! Clean residual mean=-0.000023 rms=0.001306 Jy/beam ! Combined flux in latest and established models = 0.588452 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 39 components and 0.588452 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.163677Jy sigma=0.001178 ! Fit after self-cal, rms=0.163675Jy sigma=0.001178 ! Inverting map ! Your choice of large map pixels excluded 0.472% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec selfcal true, true, soltime2 ! Performing amp+phase self-cal over 20 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.163675Jy sigma=0.001178 ! Fit after self-cal, rms=0.168759Jy sigma=0.001174 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.472% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec ! Estimated beam: bmin=0.6793 mas, bmaj=2.212 mas, bpa=-2.35 degrees ! Estimated noise=1039.14 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00121531 Jy ! Component: 100 - total flux cleaned = -0.00131732 Jy ! Component: 150 - total flux cleaned = -0.00139876 Jy ! Component: 200 - total flux cleaned = -0.00143125 Jy ! Total flux subtracted in 200 components = -0.00143125 Jy ! Clean residual min=-0.004708 max=0.004907 Jy/beam ! Clean residual mean=-0.000049 rms=0.001185 Jy/beam ! Combined flux in latest and established models = 0.587021 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 39 components and 0.587021 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.168727Jy sigma=0.001174 ! Fit after self-cal, rms=0.168791Jy sigma=0.001174 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.472% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -7.04511e-05 Jy ! Component: 100 - total flux cleaned = -0.000156137 Jy ! Component: 150 - total flux cleaned = -0.000156777 Jy ! Component: 200 - total flux cleaned = -0.000134469 Jy ! Total flux subtracted in 200 components = -0.000134469 Jy ! Clean residual min=-0.004715 max=0.004884 Jy/beam ! Clean residual mean=-0.000046 rms=0.001183 Jy/beam ! Combined flux in latest and established models = 0.586886 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 41 components and 0.586886 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.168782Jy sigma=0.001174 ! Fit after self-cal, rms=0.168782Jy sigma=0.001174 ! Inverting map ! Your choice of large map pixels excluded 0.472% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. win_mult = win_mult * 1.2 selfcal true, true, soltime2 ! Performing amp+phase self-cal over 20 minute time intervals ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.168782Jy sigma=0.001174 ! Fit after self-cal, rms=0.169421Jy sigma=0.001174 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.472% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec ! Estimated beam: bmin=2.335 mas, bmaj=4.209 mas, bpa=-9.467 degrees ! Estimated noise=1351.82 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00100597 Jy ! Component: 100 - total flux cleaned = -0.00100883 Jy ! Component: 150 - total flux cleaned = -0.000981991 Jy ! Component: 200 - total flux cleaned = -0.000931724 Jy ! Total flux subtracted in 200 components = -0.000931724 Jy ! Clean residual min=-0.005969 max=0.005594 Jy/beam ! Clean residual mean=-0.000075 rms=0.001565 Jy/beam ! Combined flux in latest and established models = 0.585954 Jy selfcal ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 43 components and 0.585954 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.169436Jy sigma=0.001174 ! Fit after self-cal, rms=0.169426Jy sigma=0.001174 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.472% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000112889 Jy ! Component: 100 - total flux cleaned = 0.000142233 Jy ! Component: 150 - total flux cleaned = 0.000170246 Jy ! Component: 200 - total flux cleaned = 0.000195854 Jy ! Total flux subtracted in 200 components = 0.000195854 Jy ! Clean residual min=-0.005973 max=0.005590 Jy/beam ! Clean residual mean=-0.000087 rms=0.001564 Jy/beam ! Combined flux in latest and established models = 0.58615 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 44 components and 0.58615 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.169438Jy sigma=0.001174 ! Fit after self-cal, rms=0.169429Jy sigma=0.001174 ! Inverting map ! Your choice of large map pixels excluded 0.472% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. win_mult = win_mult / 1.2 print "************** FINISHED AMPLITUDE SELF-CAL **************" ! ************** FINISHED AMPLITUDE SELF-CAL ************** restore ! Inverting map and beam ! Your choice of large map pixels excluded 0.472% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec ! Estimated beam: bmin=0.6806 mas, bmaj=2.212 mas, bpa=-2.305 degrees ! Estimated noise=1040.22 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6806 x 2.212 at -2.305 degrees (North through East) ! Clean map min=-0.0041229 max=0.49412 Jy/beam if(peak(flux) > thresh) selfcal true, true clean clean_niter,clean_gain selfcal 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 new_peak = peak(flux) until(new_peak<=flux_cutoff) selfcal true, true end if print "************** CLEARING MODEL AND STARTING OVER **********" ! ************** CLEARING MODEL AND STARTING OVER ********** clrmod true ! clrmod: Cleared the established and tentative 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 0.472% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec ! Estimated beam: bmin=0.5611 mas, bmaj=1.905 mas, bpa=-1.861 degrees ! Estimated noise=1376.87 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.367602 Jy ! Component: 100 - total flux cleaned = 0.469611 Jy ! Component: 150 - total flux cleaned = 0.521618 Jy ! Component: 200 - total flux cleaned = 0.549353 Jy ! Total flux subtracted in 200 components = 0.549353 Jy ! Clean residual min=-0.007010 max=0.013108 Jy/beam ! Clean residual mean=0.000112 rms=0.001883 Jy/beam ! Combined flux in latest and established models = 0.549353 Jy uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Adding 8 model components to the UV plane model. ! The established model now contains 8 components and 0.549353 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.472% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec ! Estimated beam: bmin=0.6806 mas, bmaj=2.212 mas, bpa=-2.305 degrees ! Estimated noise=1040.22 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=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0189574 Jy ! Component: 100 - total flux cleaned = 0.0277672 Jy ! Component: 150 - total flux cleaned = 0.0323086 Jy ! Component: 200 - total flux cleaned = 0.0347582 Jy ! Total flux subtracted in 200 components = 0.0347582 Jy ! Clean residual min=-0.004704 max=0.004929 Jy/beam ! Clean residual mean=0.000014 rms=0.001195 Jy/beam ! Combined flux in latest and established models = 0.584111 Jy ! Adding 35 model components to the UV plane model. ! The established model now contains 36 components and 0.584111 Jy ! Inverting map ! Your choice of large map pixels excluded 0.472% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.472% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec ! Estimated beam: bmin=2.335 mas, bmaj=4.209 mas, bpa=-9.467 degrees ! Estimated noise=1351.82 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00183301 Jy ! Component: 100 - total flux cleaned = 0.00188408 Jy ! Component: 150 - total flux cleaned = 0.00192266 Jy ! Component: 200 - total flux cleaned = 0.00199244 Jy ! Total flux subtracted in 200 components = 0.00199244 Jy ! Clean residual min=-0.005983 max=0.005612 Jy/beam ! Clean residual mean=-0.000084 rms=0.001576 Jy/beam ! Combined flux in latest and established models = 0.586104 Jy flux_cutoff = imstat(rms) * dynam 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=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 3.06487e-05 Jy ! Component: 100 - total flux cleaned = 5.71012e-05 Jy ! Component: 150 - total flux cleaned = 5.77938e-05 Jy ! Component: 200 - total flux cleaned = 6.11606e-05 Jy ! Total flux subtracted in 200 components = 6.11606e-05 Jy ! Clean residual min=-0.005969 max=0.005587 Jy/beam ! Clean residual mean=-0.000087 rms=0.001566 Jy/beam ! Combined flux in latest and established models = 0.586165 Jy ! Adding 9 model components to the UV plane model. ! The established model now contains 39 components and 0.586165 Jy ! Inverting map ! Your choice of large map pixels excluded 0.472% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.472% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec ! Estimated beam: bmin=0.6806 mas, bmaj=2.212 mas, bpa=-2.305 degrees ! Estimated noise=1040.22 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000490716 Jy ! Component: 100 - total flux cleaned = 0.000546012 Jy ! Component: 150 - total flux cleaned = 0.00050391 Jy ! Component: 200 - total flux cleaned = 0.000467625 Jy ! Total flux subtracted in 200 components = 0.000467625 Jy ! Clean residual min=-0.004628 max=0.004847 Jy/beam ! Clean residual mean=-0.000049 rms=0.001183 Jy/beam ! Combined flux in latest and established models = 0.586633 Jy selfcal ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 40 components and 0.586633 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.169456Jy sigma=0.001174 ! Fit after self-cal, rms=0.169460Jy sigma=0.001174 wmodel J0856-1105_X_2009_04_21_pus_map.mod ! Writing 40 model components to file: J0856-1105_X_2009_04_21_pus_map.mod wobs J0856-1105_X_2009_04_21_pus_uvs.fits ! Writing UV FITS file: J0856-1105_X_2009_04_21_pus_uvs.fits wwins J0856-1105_X_2009_04_21_pus_map.win ! wwins: Wrote 1 windows to J0856-1105_X_2009_04_21_pus_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 0.472% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.00035854 Jy ! Component: 100 - total flux cleaned = 0.000753351 Jy ! Component: 150 - total flux cleaned = 0.00112885 Jy ! Component: 200 - total flux cleaned = 0.00148973 Jy ! Component: 250 - total flux cleaned = 0.00176792 Jy ! Component: 300 - total flux cleaned = 0.00203823 Jy ! Component: 350 - total flux cleaned = 0.00217063 Jy ! Component: 400 - total flux cleaned = 0.00223607 Jy ! Component: 450 - total flux cleaned = 0.00229947 Jy ! Component: 500 - total flux cleaned = 0.00229994 Jy ! Component: 550 - total flux cleaned = 0.00236019 Jy ! Component: 600 - total flux cleaned = 0.00235936 Jy ! Component: 650 - total flux cleaned = 0.00230072 Jy ! Component: 700 - total flux cleaned = 0.00224283 Jy ! Component: 750 - total flux cleaned = 0.00212961 Jy ! Component: 800 - total flux cleaned = 0.00207358 Jy ! Component: 850 - total flux cleaned = 0.00201837 Jy ! Component: 900 - total flux cleaned = 0.00185548 Jy ! Component: 950 - total flux cleaned = 0.00185559 Jy ! Component: 1000 - total flux cleaned = 0.00174945 Jy ! Component: 1050 - total flux cleaned = 0.00164479 Jy ! Component: 1100 - total flux cleaned = 0.00159346 Jy ! Component: 1150 - total flux cleaned = 0.0014919 Jy ! Component: 1200 - total flux cleaned = 0.0015426 Jy ! Component: 1250 - total flux cleaned = 0.00144282 Jy ! Component: 1300 - total flux cleaned = 0.00144302 Jy ! Component: 1350 - total flux cleaned = 0.00144329 Jy ! Component: 1400 - total flux cleaned = 0.00139525 Jy ! Component: 1450 - total flux cleaned = 0.00144329 Jy ! Component: 1500 - total flux cleaned = 0.00134837 Jy ! Component: 1550 - total flux cleaned = 0.00139546 Jy ! Component: 1600 - total flux cleaned = 0.00130218 Jy ! Component: 1650 - total flux cleaned = 0.00130216 Jy ! Component: 1700 - total flux cleaned = 0.00125652 Jy ! Component: 1750 - total flux cleaned = 0.00121123 Jy ! Component: 1800 - total flux cleaned = 0.00121096 Jy ! Component: 1850 - total flux cleaned = 0.00112178 Jy ! Component: 1900 - total flux cleaned = 0.00103361 Jy ! Component: 1950 - total flux cleaned = 0.00103383 Jy ! Component: 2000 - total flux cleaned = 0.00103347 Jy ! Total flux subtracted in 2048 components = 0.000947535 Jy ! Clean residual min=-0.002155 max=0.002253 Jy/beam ! Clean residual mean=-0.000072 rms=0.000812 Jy/beam ! Combined flux in latest and established models = 0.58758 Jy keep ! Adding 146 model components to the UV plane model. ! The established model now contains 186 components and 0.58758 Jy ![Exited script file: muppet] wmap "J0856-1105_X_2009_04_21_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.472% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6806 x 2.212 at -2.305 degrees (North through East) ! Clean map min=-0.0035453 max=0.49469 Jy/beam ! Writing clean map to FITS file: J0856-1105_X_2009_04_21_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.494689 invert ! Inverting map ! Your choice of large map pixels excluded 0.472% of the data. ! The x-axis pixel size should ideally be below 0.1937 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000811917 device "J0856-1105_X_2009_04_21_pus\_map.eps/VPS" ! Attempting to open device: 'J0856-1105_X_2009_04_21_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.492381 0.492381 0.984761 1.96952 3.93904 7.87809 15.7562 31.5124 63.0247 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0024 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.494 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6806 x 2.212 at -2.305 degrees (North through East) ! Clean map min=-0.0035453 max=0.49469 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0856-1105_X_2009_04_21_pus\_map.gif/vgif" ! Attempting to open device: 'J0856-1105_X_2009_04_21_pus_map.gif/vgif' mapplot cln