! Started logfile: J0539-2839_X_2011_06_28_pus_uvs.log on Sat Apr 21 12:58:42 2012 obs J0539-2839_X_2011_06_28_pus_uva.fits ! Reading UV FITS file: J0539-2839_X_2011_06_28_pus_uva.fits ! AN table 1: 51 integrations on 153 of 153 possible baselines. ! AN table 2: 59 integrations on 153 of 153 possible baselines. ! AN table 3: 89 integrations on 153 of 153 possible baselines. ! AN table 4: 67 integrations on 153 of 153 possible baselines. ! Apparent sampling: 0.0503219 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0539-2839 ! ! 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 5249 lines of history. ! ! Reading 8192 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 J0539-2839_X_2011_06_28_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 648 telescope corrections were flagged in sub-array 1. ! A total of 927 telescope corrections were flagged in sub-array 2. ! A total of 1308 telescope corrections were flagged in sub-array 3. ! A total of 1116 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 648 telescope corrections were flagged in sub-array 1. ! A total of 927 telescope corrections were flagged in sub-array 2. ! A total of 1308 telescope corrections were flagged in sub-array 3. ! A total of 1116 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 648 telescope corrections were flagged in sub-array 1. ! A total of 927 telescope corrections were flagged in sub-array 2. ! A total of 1308 telescope corrections were flagged in sub-array 3. ! A total of 1116 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 648 telescope corrections were flagged in sub-array 1. ! A total of 927 telescope corrections were flagged in sub-array 2. ! A total of 1308 telescope corrections were flagged in sub-array 3. ! A total of 1116 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=0.572074Jy sigma=0.005114 ! Fit after self-cal, rms=0.437435Jy sigma=0.003804 ! 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 2.06% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Estimated beam: bmin=0.6185 mas, bmaj=1.238 mas, bpa=5.896 degrees ! Estimated noise=1441.71 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 = 0.497767 Jy ! Component: 100 - total flux cleaned = 0.691269 Jy ! Total flux subtracted in 100 components = 0.691269 Jy ! Clean residual min=-0.036114 max=0.092648 Jy/beam ! Clean residual mean=0.000456 rms=0.012653 Jy/beam ! Combined flux in latest and established models = 0.691269 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.691269 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.266054Jy sigma=0.002447 ! Fit after self-cal, rms=0.265028Jy sigma=0.002441 ! Inverting map ! Your choice of large map pixels excluded 2.06% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.1065 Jy ! Component: 100 - total flux cleaned = 0.166632 Jy ! Total flux subtracted in 100 components = 0.166632 Jy ! Clean residual min=-0.023701 max=0.041574 Jy/beam ! Clean residual mean=0.000100 rms=0.007029 Jy/beam ! Combined flux in latest and established models = 0.8579 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 12 components and 0.8579 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.217326Jy sigma=0.001768 ! Fit after self-cal, rms=0.216961Jy sigma=0.001766 ! Inverting map ! Your choice of large map pixels excluded 2.06% of the data. ! The x-axis pixel size should ideally be below 0.1679 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 2.06% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Estimated beam: bmin=0.7629 mas, bmaj=1.442 mas, bpa=7.733 degrees ! Estimated noise=914.038 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 (1.4, 0.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0582404 Jy ! Component: 100 - total flux cleaned = 0.091166 Jy ! Component: 150 - total flux cleaned = 0.1119 Jy ! Component: 200 - total flux cleaned = 0.125544 Jy ! Total flux subtracted in 200 components = 0.125544 Jy ! Clean residual min=-0.019265 max=0.025433 Jy/beam ! Clean residual mean=-0.002049 rms=0.005392 Jy/beam ! Combined flux in latest and established models = 0.983444 Jy ! Performing phase self-cal ! Adding 37 model components to the UV plane model. ! The established model now contains 43 components and 0.983444 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.205706Jy sigma=0.001535 ! Fit after self-cal, rms=0.204445Jy sigma=0.001520 ! Inverting map ! Your choice of large map pixels excluded 2.06% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 63 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.91 FD 0.93 FT 1.00* HH 1.00* ! HN 1.38 KK 1.00* KP 0.97 MC 1.00* ! MK 1.00 NL 1.11 NY 1.00* OV 0.95 ! PT 0.95 SC 0.92 SH 1.00* TS 1.00* ! WF 1.05 WZ 1.00* ! ! A total of 135 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* FT 0.00* HH 0.00* ! HN 0.00* KK 0.00* KP 0.00* MC 0.00* ! MK 0.00* NL 0.00* NY 0.00* OV 0.00* ! PT 0.00* SC 0.00* SH 0.00* TS 0.00* ! WF 0.00* WZ 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 0.95 FT 1.00* HH 0.99 ! HN 1.08 KK 1.00* KP 0.97 MC 1.00* ! MK 1.00* NL 0.99 NY 1.00* OV 0.96 ! PT 0.94 SC 0.93 SH 1.00* TS 1.00* ! WF 0.99 WZ 1.00* ! ! A total of 90 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* FT 0.00* HH 0.00* ! HN 0.00* KK 0.00* KP 0.00* MC 0.00* ! MK 0.00* NL 0.00* NY 0.00* OV 0.00* ! PT 0.00* SC 0.00* SH 0.00* TS 0.00* ! WF 0.00* WZ 0.00* ! ! ! Correcting IF 2. ! A total of 63 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.91 FT 1.00* HH 1.00* ! HN 1.46 KK 1.00* KP 0.95 MC 1.00* ! MK 0.98 NL 1.18 NY 1.00* OV 0.96 ! PT 0.97 SC 0.99 SH 1.00* TS 1.00* ! WF 0.99 WZ 1.00* ! ! A total of 135 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* FT 0.00* HH 0.00* ! HN 0.00* KK 0.00* KP 0.00* MC 0.00* ! MK 0.00* NL 0.00* NY 0.00* OV 0.00* ! PT 0.00* SC 0.00* SH 0.00* TS 0.00* ! WF 0.00* WZ 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 0.93 FT 1.00* HH 1.01 ! HN 1.11 KK 1.00* KP 0.96 MC 1.00* ! MK 1.00* NL 1.04 NY 1.00* OV 0.99 ! PT 0.96 SC 0.95 SH 1.00* TS 1.00* ! WF 0.97 WZ 1.00* ! ! A total of 90 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* FT 0.00* HH 0.00* ! HN 0.00* KK 0.00* KP 0.00* MC 0.00* ! MK 0.00* NL 0.00* NY 0.00* OV 0.00* ! PT 0.00* SC 0.00* SH 0.00* TS 0.00* ! WF 0.00* WZ 0.00* ! ! ! Correcting IF 3. ! A total of 63 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.94 FD 0.97 FT 1.00* HH 1.00* ! HN 1.42 KK 1.00* KP 0.95 MC 1.00* ! MK 0.97 NL 1.11 NY 1.00* OV 0.96 ! PT 0.95 SC 0.94 SH 1.00* TS 1.00* ! WF 1.01 WZ 1.00* ! ! A total of 135 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* FT 0.00* HH 0.00* ! HN 0.00* KK 0.00* KP 0.00* MC 0.00* ! MK 0.00* NL 0.00* NY 0.00* OV 0.00* ! PT 0.00* SC 0.00* SH 0.00* TS 0.00* ! WF 0.00* WZ 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 0.97 FT 1.00* HH 0.94 ! HN 1.08 KK 1.00* KP 0.99 MC 1.00* ! MK 1.00* NL 1.00 NY 1.00* OV 1.00 ! PT 0.94 SC 0.96 SH 1.00* TS 1.00* ! WF 1.01 WZ 1.00* ! ! A total of 90 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* FT 0.00* HH 0.00* ! HN 0.00* KK 0.00* KP 0.00* MC 0.00* ! MK 0.00* NL 0.00* NY 0.00* OV 0.00* ! PT 0.00* SC 0.00* SH 0.00* TS 0.00* ! WF 0.00* WZ 0.00* ! ! ! Correcting IF 4. ! A total of 63 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.97 FT 1.00* HH 1.00* ! HN 1.40 KK 1.00* KP 0.93 MC 1.00* ! MK 0.99 NL 1.14 NY 1.00* OV 1.02 ! PT 0.98 SC 1.03 SH 1.00* TS 1.00* ! WF 1.00 WZ 1.00* ! ! A total of 135 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* FT 0.00* HH 0.00* ! HN 0.00* KK 0.00* KP 0.00* MC 0.00* ! MK 0.00* NL 0.00* NY 0.00* OV 0.00* ! PT 0.00* SC 0.00* SH 0.00* TS 0.00* ! WF 0.00* WZ 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 0.97 FT 1.00* HH 0.94 ! HN 1.11 KK 1.00* KP 0.94 MC 1.00* ! MK 1.00* NL 1.02 NY 1.00* OV 1.04 ! PT 0.97 SC 0.98 SH 1.00* TS 1.00* ! WF 0.98 WZ 1.00* ! ! A total of 90 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* FT 0.00* HH 0.00* ! HN 0.00* KK 0.00* KP 0.00* MC 0.00* ! MK 0.00* NL 0.00* NY 0.00* OV 0.00* ! PT 0.00* SC 0.00* SH 0.00* TS 0.00* ! WF 0.00* WZ 0.00* ! ! ! Fit before self-cal, rms=0.204445Jy sigma=0.001520 ! Fit after self-cal, rms=0.195257Jy sigma=0.001364 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 1.66% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Estimated beam: bmin=0.7889 mas, bmaj=1.769 mas, bpa=5.037 degrees ! Estimated noise=953.678 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 = -0.00234486 Jy ! Component: 100 - total flux cleaned = -0.00234152 Jy ! Component: 150 - total flux cleaned = -0.00250383 Jy ! Component: 200 - total flux cleaned = -0.00264965 Jy ! Total flux subtracted in 200 components = -0.00264965 Jy ! Clean residual min=-0.007699 max=0.007002 Jy/beam ! Clean residual mean=-0.000194 rms=0.001724 Jy/beam ! Combined flux in latest and established models = 0.980795 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 54 components and 0.980795 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.194832Jy sigma=0.001360 ! Fit after self-cal, rms=0.195347Jy sigma=0.001359 ! Inverting map ! Your choice of large map pixels excluded 1.66% of the data. ! The x-axis pixel size should ideally be below 0.1679 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=0.195347Jy sigma=0.001359 ! Fit after self-cal, rms=0.195185Jy sigma=0.001354 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.66% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Estimated beam: bmin=0.7859 mas, bmaj=1.763 mas, bpa=5.025 degrees ! Estimated noise=950.934 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000192818 Jy ! Component: 100 - total flux cleaned = -0.000491997 Jy ! Component: 150 - total flux cleaned = -0.00049705 Jy ! Component: 200 - total flux cleaned = -0.000263395 Jy ! Total flux subtracted in 200 components = -0.000263395 Jy ! Clean residual min=-0.006345 max=0.005480 Jy/beam ! Clean residual mean=0.000062 rms=0.001485 Jy/beam ! Combined flux in latest and established models = 0.980531 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 57 components and 0.980531 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.194940Jy sigma=0.001352 ! Fit after self-cal, rms=0.194998Jy sigma=0.001352 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.66% of the data. ! The x-axis pixel size should ideally be below 0.1679 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 = -7.0949e-05 Jy ! Component: 100 - total flux cleaned = 3.47423e-05 Jy ! Component: 150 - total flux cleaned = 0.000128057 Jy ! Component: 200 - total flux cleaned = 0.000128743 Jy ! Total flux subtracted in 200 components = 0.000128743 Jy ! Clean residual min=-0.006228 max=0.005369 Jy/beam ! Clean residual mean=0.000057 rms=0.001437 Jy/beam ! Combined flux in latest and established models = 0.98066 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 62 components and 0.98066 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.194887Jy sigma=0.001351 ! Fit after self-cal, rms=0.194878Jy sigma=0.001351 ! Inverting map ! Your choice of large map pixels excluded 1.66% of the data. ! The x-axis pixel size should ideally be below 0.1679 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=0.194878Jy sigma=0.001351 ! Fit after self-cal, rms=0.195198Jy sigma=0.001350 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.66% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Estimated beam: bmin=0.7832 mas, bmaj=1.755 mas, bpa=5.057 degrees ! Estimated noise=948.906 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 3.87759e-06 Jy ! Component: 100 - total flux cleaned = 0.000207027 Jy ! Component: 150 - total flux cleaned = 0.00020619 Jy ! Component: 200 - total flux cleaned = 0.000285424 Jy ! Total flux subtracted in 200 components = 0.000285424 Jy ! Clean residual min=-0.005403 max=0.005121 Jy/beam ! Clean residual mean=0.000158 rms=0.001367 Jy/beam ! Combined flux in latest and established models = 0.980945 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 65 components and 0.980945 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.195094Jy sigma=0.001349 ! Fit after self-cal, rms=0.195117Jy sigma=0.001349 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.66% of the data. ! The x-axis pixel size should ideally be below 0.1679 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 = -8.22631e-05 Jy ! Component: 100 - total flux cleaned = -8.10612e-05 Jy ! Component: 150 - total flux cleaned = -8.113e-05 Jy ! Component: 200 - total flux cleaned = -8.16537e-05 Jy ! Total flux subtracted in 200 components = -8.16537e-05 Jy ! Clean residual min=-0.005328 max=0.005012 Jy/beam ! Clean residual mean=0.000158 rms=0.001343 Jy/beam ! Combined flux in latest and established models = 0.980864 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 66 components and 0.980864 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.195064Jy sigma=0.001348 ! Fit after self-cal, rms=0.195061Jy sigma=0.001348 ! Inverting map ! Your choice of large map pixels excluded 1.66% of the data. ! The x-axis pixel size should ideally be below 0.1679 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=0.195061Jy sigma=0.001348 ! Fit after self-cal, rms=0.194982Jy sigma=0.001348 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.66% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Estimated beam: bmin=1.957 mas, bmaj=4.609 mas, bpa=-1.03 degrees ! Estimated noise=1199.61 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000615902 Jy ! Component: 100 - total flux cleaned = -0.000613427 Jy ! Component: 150 - total flux cleaned = -0.000611821 Jy ! Component: 200 - total flux cleaned = -0.000609768 Jy ! Total flux subtracted in 200 components = -0.000609768 Jy ! Clean residual min=-0.004927 max=0.005599 Jy/beam ! Clean residual mean=0.000447 rms=0.001422 Jy/beam ! Combined flux in latest and established models = 0.980254 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 72 components and 0.980254 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.194974Jy sigma=0.001348 ! Fit after self-cal, rms=0.194966Jy sigma=0.001348 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.66% of the data. ! The x-axis pixel size should ideally be below 0.1679 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 = 1.12673e-05 Jy ! Component: 100 - total flux cleaned = 5.51948e-05 Jy ! Component: 150 - total flux cleaned = 0.000125103 Jy ! Component: 200 - total flux cleaned = 0.000124752 Jy ! Total flux subtracted in 200 components = 0.000124752 Jy ! Clean residual min=-0.004891 max=0.005607 Jy/beam ! Clean residual mean=0.000442 rms=0.001419 Jy/beam ! Combined flux in latest and established models = 0.980379 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 76 components and 0.980379 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.194969Jy sigma=0.001348 ! Fit after self-cal, rms=0.194951Jy sigma=0.001348 ! Inverting map ! Your choice of large map pixels excluded 1.66% of the data. ! The x-axis pixel size should ideally be below 0.1679 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 1.66% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Estimated beam: bmin=0.7814 mas, bmaj=1.749 mas, bpa=5.115 degrees ! Estimated noise=947.82 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7814 x 1.749 at 5.115 degrees (North through East) ! Clean map min=-0.0049329 max=0.68451 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 ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.194951Jy sigma=0.001348 ! Fit after self-cal, rms=0.189052Jy sigma=0.001226 ! Inverting map and beam ! Your choice of large map pixels excluded 1.66% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Estimated beam: bmin=0.7822 mas, bmaj=1.753 mas, bpa=5.029 degrees ! Estimated noise=946.991 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -8.65315e-05 Jy ! Component: 100 - total flux cleaned = -8.95919e-05 Jy ! Component: 150 - total flux cleaned = -0.000149257 Jy ! Component: 200 - total flux cleaned = -4.65476e-05 Jy ! Total flux subtracted in 200 components = -4.65476e-05 Jy ! Clean residual min=-0.005369 max=0.005090 Jy/beam ! Clean residual mean=0.000141 rms=0.001305 Jy/beam ! Combined flux in latest and established models = 0.980332 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 84 components and 0.980332 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.189010Jy sigma=0.001226 ! Fit after self-cal, rms=0.189013Jy sigma=0.001226 ! Inverting map ! Your choice of large map pixels excluded 1.66% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -5.75016e-05 Jy ! Component: 100 - total flux cleaned = -1.06433e-05 Jy ! Component: 150 - total flux cleaned = -9.97113e-06 Jy ! Component: 200 - total flux cleaned = -1.10566e-05 Jy ! Total flux subtracted in 200 components = -1.10566e-05 Jy ! Clean residual min=-0.005284 max=0.005069 Jy/beam ! Clean residual mean=0.000142 rms=0.001294 Jy/beam ! Combined flux in latest and established models = 0.980321 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 86 components and 0.980321 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.188991Jy sigma=0.001226 ! Fit after self-cal, rms=0.188992Jy sigma=0.001226 ! Inverting map ! Your choice of large map pixels excluded 1.66% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.188992Jy sigma=0.001226 ! Fit after self-cal, rms=0.188755Jy sigma=0.001225 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 1.66% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Estimated beam: bmin=0.6535 mas, bmaj=1.525 mas, bpa=5.08 degrees ! Estimated noise=1189.56 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.516829 Jy ! Component: 100 - total flux cleaned = 0.714119 Jy ! Component: 150 - total flux cleaned = 0.816479 Jy ! Component: 200 - total flux cleaned = 0.873344 Jy ! Total flux subtracted in 200 components = 0.873344 Jy ! Clean residual min=-0.014097 max=0.028284 Jy/beam ! Clean residual mean=0.000212 rms=0.004996 Jy/beam ! Combined flux in latest and established models = 0.873344 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 17 model components to the UV plane model. ! The established model now contains 17 components and 0.873344 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 1.66% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Estimated beam: bmin=0.781 mas, bmaj=1.749 mas, bpa=5.028 degrees ! Estimated noise=945.801 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 = 0.0414406 Jy ! Component: 100 - total flux cleaned = 0.0650658 Jy ! Component: 150 - total flux cleaned = 0.0795348 Jy ! Component: 200 - total flux cleaned = 0.0888308 Jy ! Total flux subtracted in 200 components = 0.0888308 Jy ! Clean residual min=-0.005385 max=0.006315 Jy/beam ! Clean residual mean=0.000386 rms=0.001565 Jy/beam ! Combined flux in latest and established models = 0.962174 Jy ! Adding 28 model components to the UV plane model. ! The established model now contains 36 components and 0.962174 Jy ! Inverting map ! Your choice of large map pixels excluded 1.66% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec uvw 0,2 ! Uniform weighting is not currently selected. ! Amplitude error weighting is not currently selected. ! Radial weighting is not currently selected. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.66% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! Estimated beam: bmin=0.739 mas, bmaj=1.553 mas, bpa=11.72 degrees ! Estimated noise=1322.29 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00696379 Jy ! Component: 100 - total flux cleaned = 0.00963084 Jy ! Component: 150 - total flux cleaned = 0.0105231 Jy ! Component: 200 - total flux cleaned = 0.0110365 Jy ! Total flux subtracted in 200 components = 0.0110365 Jy ! Clean residual min=-0.006212 max=0.006717 Jy/beam ! Clean residual mean=0.000275 rms=0.001759 Jy/beam ! Combined flux in latest and established models = 0.973211 Jy clean ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000453103 Jy ! Component: 100 - total flux cleaned = 0.000863382 Jy ! Component: 150 - total flux cleaned = 0.00105286 Jy ! Component: 200 - total flux cleaned = 0.00123057 Jy ! Total flux subtracted in 200 components = 0.00123057 Jy ! Clean residual min=-0.006036 max=0.006698 Jy/beam ! Clean residual mean=0.000233 rms=0.001706 Jy/beam ! Combined flux in latest and established models = 0.974441 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 49 components and 0.974441 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.189463Jy sigma=0.001233 ! Fit after self-cal, rms=0.189346Jy sigma=0.001231 wmodel J0539-2839_X_2011_06_28_pus_map.mod ! Writing 49 model components to file: J0539-2839_X_2011_06_28_pus_map.mod wobs J0539-2839_X_2011_06_28_pus_uvs.fits ! Writing UV FITS file: J0539-2839_X_2011_06_28_pus_uvs.fits wwins J0539-2839_X_2011_06_28_pus_map.win ! wwins: Wrote 2 windows to J0539-2839_X_2011_06_28_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 1.66% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.00214804 Jy ! Component: 100 - total flux cleaned = 0.00371776 Jy ! Component: 150 - total flux cleaned = 0.00403195 Jy ! Component: 200 - total flux cleaned = 0.00413431 Jy ! Component: 250 - total flux cleaned = 0.0042323 Jy ! Component: 300 - total flux cleaned = 0.00432513 Jy ! Component: 350 - total flux cleaned = 0.0044137 Jy ! Component: 400 - total flux cleaned = 0.00458465 Jy ! Component: 450 - total flux cleaned = 0.00466659 Jy ! Component: 500 - total flux cleaned = 0.0047481 Jy ! Component: 550 - total flux cleaned = 0.00498388 Jy ! Component: 600 - total flux cleaned = 0.00505901 Jy ! Component: 650 - total flux cleaned = 0.00520888 Jy ! Component: 700 - total flux cleaned = 0.00542816 Jy ! Component: 750 - total flux cleaned = 0.00564284 Jy ! Component: 800 - total flux cleaned = 0.00578357 Jy ! Component: 850 - total flux cleaned = 0.00585277 Jy ! Component: 900 - total flux cleaned = 0.0059208 Jy ! Component: 950 - total flux cleaned = 0.0059874 Jy ! Component: 1000 - total flux cleaned = 0.0059882 Jy ! Component: 1050 - total flux cleaned = 0.00611661 Jy ! Component: 1100 - total flux cleaned = 0.00624143 Jy ! Component: 1150 - total flux cleaned = 0.0062419 Jy ! Component: 1200 - total flux cleaned = 0.00636267 Jy ! Component: 1250 - total flux cleaned = 0.0064217 Jy ! Component: 1300 - total flux cleaned = 0.00653767 Jy ! Component: 1350 - total flux cleaned = 0.00648034 Jy ! Component: 1400 - total flux cleaned = 0.0065929 Jy ! Component: 1450 - total flux cleaned = 0.00659258 Jy ! Component: 1500 - total flux cleaned = 0.00659208 Jy ! Component: 1550 - total flux cleaned = 0.00664529 Jy ! Component: 1600 - total flux cleaned = 0.00659297 Jy ! Component: 1650 - total flux cleaned = 0.00664524 Jy ! Component: 1700 - total flux cleaned = 0.00664537 Jy ! Component: 1750 - total flux cleaned = 0.00659504 Jy ! Component: 1800 - total flux cleaned = 0.00654564 Jy ! Component: 1850 - total flux cleaned = 0.0064968 Jy ! Component: 1900 - total flux cleaned = 0.00644868 Jy ! Component: 1950 - total flux cleaned = 0.00640092 Jy ! Component: 2000 - total flux cleaned = 0.00640072 Jy ! Total flux subtracted in 2048 components = 0.00626107 Jy ! Clean residual min=-0.002760 max=0.003058 Jy/beam ! Clean residual mean=-0.000007 rms=0.000838 Jy/beam ! Combined flux in latest and established models = 0.980702 Jy keep ! Adding 150 model components to the UV plane model. ! The established model now contains 199 components and 0.980703 Jy ![Exited script file: muppet] wmap "J0539-2839_X_2011_06_28_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 1.66% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.739 x 1.553 at 11.72 degrees (North through East) ! Clean map min=-0.003911 max=0.67578 Jy/beam ! Writing clean map to FITS file: J0539-2839_X_2011_06_28_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.675783 invert ! Inverting map ! Your choice of large map pixels excluded 1.66% of the data. ! The x-axis pixel size should ideally be below 0.1679 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000827173 device "J0539-2839_X_2011_06_28_pus\_map.eps/VPS" ! Attempting to open device: 'J0539-2839_X_2011_06_28_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.367206 0.367206 0.734413 1.46883 2.93765 5.8753 11.7506 23.5012 47.0024 94.0049 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0024 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.675 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.739 x 1.553 at 11.72 degrees (North through East) ! Clean map min=-0.003911 max=0.67578 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0539-2839_X_2011_06_28_pus\_map.gif/vgif" ! Attempting to open device: 'J0539-2839_X_2011_06_28_pus_map.gif/vgif' mapplot cln