! Started logfile: J2258-2758_X_2010_10_13_pus_uvs.log on Mon Feb 28 17:19:17 2011 obs J2258-2758_X_2010_10_13_pus_uva.fits ! Reading UV FITS file: J2258-2758_X_2010_10_13_pus_uva.fits ! AN table 1: 149 integrations on 105 of 105 possible baselines. ! Apparent sampling: 0.100927 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J2258-2758 ! ! 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 8.40996e+09 8e+06 1 8e+06 ! 02 2 8.47996e+09 8e+06 1 8e+06 ! 03 3 8.79496e+09 8e+06 1 8e+06 ! 04 4 8.89996e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 5978 lines of history. ! ! Reading 6316 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 = 256 print "field_cell =",field_cell ! field_cell = 0.2 print "taper_size =",taper_size ! taper_size = 70 ![@muppet J2258-2758_X_2010_10_13_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 = 256x256 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 1647 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 1647 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 1647 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 1647 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=1.431028Jy sigma=0.014981 ! Fit after self-cal, rms=1.427145Jy sigma=0.014977 ! 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 2.64% of the data. ! The x-axis pixel size should ideally be below 0.1618 milli-arcsec ! Estimated beam: bmin=0.7166 mas, bmaj=1.609 mas, bpa=7.412 degrees ! Estimated noise=1712.2 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 = 1.66929 Jy ! Component: 100 - total flux cleaned = 2.0749 Jy ! Total flux subtracted in 100 components = 2.0749 Jy ! Clean residual min=-0.179445 max=0.395012 Jy/beam ! Clean residual mean=0.005271 rms=0.077048 Jy/beam ! Combined flux in latest and established models = 2.0749 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 2.0749 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.821990Jy sigma=0.007928 ! Fit after self-cal, rms=0.821991Jy sigma=0.007928 ! Inverting map ! Your choice of large map pixels excluded 2.64% of the data. ! The x-axis pixel size should ideally be below 0.1618 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 2.64% of the data. ! The x-axis pixel size should ideally be below 0.1618 milli-arcsec ! Estimated beam: bmin=0.9862 mas, bmaj=2.554 mas, bpa=-1.976 degrees ! Estimated noise=995.64 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 = 0.284906 Jy ! Component: 100 - total flux cleaned = 0.427395 Jy ! Component: 150 - total flux cleaned = 0.459687 Jy ! Component: 200 - total flux cleaned = 0.466047 Jy ! Total flux subtracted in 200 components = 0.466047 Jy ! Clean residual min=-0.142842 max=0.350017 Jy/beam ! Clean residual mean=0.015061 rms=0.070617 Jy/beam ! Combined flux in latest and established models = 2.54095 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 14 components and 2.54095 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.743714Jy sigma=0.006872 ! Fit after self-cal, rms=0.743611Jy sigma=0.006872 ! Inverting map ! Your choice of large map pixels excluded 2.64% of the data. ! The x-axis pixel size should ideally be below 0.1618 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 0.85 FD 0.81 HH 1.14 HN 1.08 ! KB 1.07 KK 0.93 KP 0.96 LA 0.98 ! MK 0.90 NL 3.27 NY 1.00* OV 0.92 ! PT 0.95 SC 0.95 TS 1.04 ! ! ! Correcting IF 2. ! A total of 63 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.88 FD 0.94 HH 1.15 HN 1.10 ! KB 1.09 KK 0.97 KP 0.95 LA 0.95 ! MK 0.85 NL 3.41 NY 1.00* OV 0.94 ! PT 0.97 SC 0.97 TS 1.06 ! ! ! Correcting IF 3. ! A total of 63 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.86 FD 0.95 HH 1.09 HN 1.09 ! KB 1.04 KK 0.95 KP 0.96 LA 0.93 ! MK 0.91 NL 3.10 NY 1.00* OV 0.93 ! PT 1.02 SC 0.99 TS 1.02 ! ! ! Correcting IF 4. ! A total of 63 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.89 FD 0.96 HH 1.08 HN 1.07 ! KB 1.03 KK 0.97 KP 0.96 LA 1.00 ! MK 0.90 NL 3.06 NY 1.00* OV 0.97 ! PT 0.97 SC 0.98 TS 0.93 ! ! ! Fit before self-cal, rms=0.743611Jy sigma=0.006872 ! Fit after self-cal, rms=1.153410Jy sigma=0.003494 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 milli-arcsec ! Estimated beam: bmin=0.9652 mas, bmaj=2.807 mas, bpa=-1.817 degrees ! Estimated noise=1035.3 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 = 0.0064764 Jy ! Component: 100 - total flux cleaned = 0.00640122 Jy ! Component: 150 - total flux cleaned = 0.00511081 Jy ! Component: 200 - total flux cleaned = 0.00406523 Jy ! Total flux subtracted in 200 components = 0.00406523 Jy ! Clean residual min=-0.074458 max=0.075398 Jy/beam ! Clean residual mean=0.006545 rms=0.022649 Jy/beam ! Combined flux in latest and established models = 2.54501 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 22 components and 2.54501 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.148749Jy sigma=0.003391 ! Fit after self-cal, rms=1.150427Jy sigma=0.003389 ! Inverting map ! Your choice of large map pixels excluded 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 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=1.150427Jy sigma=0.003389 ! Fit after self-cal, rms=1.174899Jy sigma=0.003342 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 milli-arcsec ! Estimated beam: bmin=0.9667 mas, bmaj=2.826 mas, bpa=-1.792 degrees ! Estimated noise=1041.28 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00517229 Jy ! Component: 100 - total flux cleaned = 0.00418424 Jy ! Component: 150 - total flux cleaned = 0.00255661 Jy ! Component: 200 - total flux cleaned = 0.00185615 Jy ! Total flux subtracted in 200 components = 0.00185615 Jy ! Clean residual min=-0.075937 max=0.072104 Jy/beam ! Clean residual mean=0.003216 rms=0.022288 Jy/beam ! Combined flux in latest and established models = 2.54687 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 25 components and 2.54687 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.171808Jy sigma=0.003310 ! Fit after self-cal, rms=1.171969Jy sigma=0.003310 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 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 = -0.00132838 Jy ! Component: 100 - total flux cleaned = -0.00193989 Jy ! Component: 150 - total flux cleaned = -0.00310287 Jy ! Component: 200 - total flux cleaned = -0.00414778 Jy ! Total flux subtracted in 200 components = -0.00414778 Jy ! Clean residual min=-0.074649 max=0.071834 Jy/beam ! Clean residual mean=0.003488 rms=0.022159 Jy/beam ! Combined flux in latest and established models = 2.54272 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 25 components and 2.54272 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.170259Jy sigma=0.003299 ! Fit after self-cal, rms=1.170272Jy sigma=0.003299 ! Inverting map ! Your choice of large map pixels excluded 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 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=1.170272Jy sigma=0.003299 ! Fit after self-cal, rms=1.309210Jy sigma=0.001547 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 milli-arcsec ! Estimated beam: bmin=0.9634 mas, bmaj=2.786 mas, bpa=-1.334 degrees ! Estimated noise=1045.28 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00210299 Jy ! Component: 100 - total flux cleaned = 0.00281262 Jy ! Component: 150 - total flux cleaned = 0.00279685 Jy ! Component: 200 - total flux cleaned = 0.00329577 Jy ! Total flux subtracted in 200 components = 0.00329577 Jy ! Clean residual min=-0.021116 max=0.026663 Jy/beam ! Clean residual mean=0.002690 rms=0.007373 Jy/beam ! Combined flux in latest and established models = 2.54602 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 27 components and 2.54602 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.308390Jy sigma=0.001516 ! Fit after self-cal, rms=1.309672Jy sigma=0.001514 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 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 = -8.88832e-05 Jy ! Component: 100 - total flux cleaned = -0.000888896 Jy ! Component: 150 - total flux cleaned = -0.00125049 Jy ! Component: 200 - total flux cleaned = -0.00159683 Jy ! Total flux subtracted in 200 components = -0.00159683 Jy ! Clean residual min=-0.020475 max=0.025696 Jy/beam ! Clean residual mean=0.002792 rms=0.007147 Jy/beam ! Combined flux in latest and established models = 2.54442 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 28 components and 2.54442 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.309446Jy sigma=0.001504 ! Fit after self-cal, rms=1.309472Jy sigma=0.001504 ! Inverting map ! Your choice of large map pixels excluded 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 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=1.309472Jy sigma=0.001504 ! Fit after self-cal, rms=1.334078Jy sigma=0.001434 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 milli-arcsec ! Estimated beam: bmin=2.494 mas, bmaj=5.103 mas, bpa=-1.742 degrees ! Estimated noise=1230.48 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00899333 Jy ! Component: 100 - total flux cleaned = -0.00898406 Jy ! Component: 150 - total flux cleaned = -0.00898147 Jy ! Component: 200 - total flux cleaned = -0.0092246 Jy ! Total flux subtracted in 200 components = -0.0092246 Jy ! Clean residual min=-0.012479 max=0.031860 Jy/beam ! Clean residual mean=0.006256 rms=0.008243 Jy/beam ! Combined flux in latest and established models = 2.5352 Jy selfcal ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 29 components and 2.5352 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.333992Jy sigma=0.001430 ! Fit after self-cal, rms=1.334511Jy sigma=0.001427 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 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 = -0.000200575 Jy ! Component: 100 - total flux cleaned = -0.000202879 Jy ! Component: 150 - total flux cleaned = -0.000471523 Jy ! Component: 200 - total flux cleaned = -0.000696398 Jy ! Total flux subtracted in 200 components = -0.000696398 Jy ! Clean residual min=-0.012155 max=0.032148 Jy/beam ! Clean residual mean=0.006338 rms=0.008312 Jy/beam ! Combined flux in latest and established models = 2.5345 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 30 components and 2.5345 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=1.334558Jy sigma=0.001428 ! Fit after self-cal, rms=1.334558Jy sigma=0.001426 ! Inverting map ! Your choice of large map pixels excluded 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 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 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 milli-arcsec ! Estimated beam: bmin=0.9656 mas, bmaj=2.802 mas, bpa=-1.271 degrees ! Estimated noise=1044.65 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9656 x 2.802 at -1.271 degrees (North through East) ! Clean map min=-0.01251 max=2.2182 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=1.334558Jy sigma=0.001426 ! Fit after self-cal, rms=2.965582Jy sigma=0.001268 ! Inverting map and beam ! Your choice of large map pixels excluded 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 milli-arcsec ! Estimated beam: bmin=0.9668 mas, bmaj=2.813 mas, bpa=-1.287 degrees ! Estimated noise=1044.77 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00547492 Jy ! Component: 100 - total flux cleaned = -0.00580416 Jy ! Component: 150 - total flux cleaned = -0.00580676 Jy ! Component: 200 - total flux cleaned = -0.00606833 Jy ! Total flux subtracted in 200 components = -0.00606833 Jy ! Clean residual min=-0.012347 max=0.026672 Jy/beam ! Clean residual mean=0.003067 rms=0.005419 Jy/beam ! Combined flux in latest and established models = 2.52843 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 31 components and 2.52843 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=2.965451Jy sigma=0.001258 ! Fit after self-cal, rms=2.965476Jy sigma=0.001258 ! Inverting map ! Your choice of large map pixels excluded 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 milli-arcsec ! Added new window around map position (-5.6, -4.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0236204 Jy ! Component: 100 - total flux cleaned = 0.0342597 Jy ! Component: 150 - total flux cleaned = 0.0370824 Jy ! Component: 200 - total flux cleaned = 0.0399105 Jy ! Total flux subtracted in 200 components = 0.0399105 Jy ! Clean residual min=-0.011276 max=0.010683 Jy/beam ! Clean residual mean=0.000672 rms=0.003273 Jy/beam ! Combined flux in latest and established models = 2.56834 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 44 components and 2.56834 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=2.965108Jy sigma=0.001216 ! Fit after self-cal, rms=2.965433Jy sigma=0.001213 ! Inverting map ! Your choice of large map pixels excluded 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=2.965433Jy sigma=0.001213 ! Fit after self-cal, rms=2.907161Jy sigma=0.001205 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 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 milli-arcsec ! Estimated beam: bmin=0.7068 mas, bmaj=1.738 mas, bpa=5.233 degrees ! Estimated noise=1812.18 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.71489 Jy ! Component: 100 - total flux cleaned = 2.10943 Jy ! Component: 150 - total flux cleaned = 2.23716 Jy ! Component: 200 - total flux cleaned = 2.31679 Jy ! Total flux subtracted in 200 components = 2.31679 Jy ! Clean residual min=-0.029916 max=0.052453 Jy/beam ! Clean residual mean=0.002405 rms=0.010664 Jy/beam ! Combined flux in latest and established models = 2.31679 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 18 model components to the UV plane model. ! The established model now contains 18 components and 2.31679 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 milli-arcsec ! Estimated beam: bmin=0.9676 mas, bmaj=2.829 mas, bpa=-1.305 degrees ! Estimated noise=1044.22 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) ! Added new window around map position (-0.8, -0.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0940259 Jy ! Component: 100 - total flux cleaned = 0.144316 Jy ! Component: 150 - total flux cleaned = 0.176253 Jy ! Component: 200 - total flux cleaned = 0.198362 Jy ! Total flux subtracted in 200 components = 0.198362 Jy ! Clean residual min=-0.008998 max=0.015316 Jy/beam ! Clean residual mean=0.004499 rms=0.004408 Jy/beam ! Combined flux in latest and established models = 2.51516 Jy ! Adding 40 model components to the UV plane model. ! The established model now contains 53 components and 2.51516 Jy ! Inverting map ! Your choice of large map pixels excluded 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 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 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 milli-arcsec ! Estimated beam: bmin=2.5 mas, bmaj=5.117 mas, bpa=-1.598 degrees ! Estimated noise=1226.3 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0233315 Jy ! Component: 100 - total flux cleaned = 0.0372934 Jy ! Component: 150 - total flux cleaned = 0.0466217 Jy ! Component: 200 - total flux cleaned = 0.0518696 Jy ! Total flux subtracted in 200 components = 0.0518696 Jy ! Clean residual min=-0.008417 max=0.013913 Jy/beam ! Clean residual mean=0.002269 rms=0.003815 Jy/beam ! Combined flux in latest and established models = 2.56703 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 = 0.00150792 Jy ! Component: 100 - total flux cleaned = 0.00270022 Jy ! Component: 150 - total flux cleaned = 0.00398535 Jy ! Component: 200 - total flux cleaned = 0.00499995 Jy ! Total flux subtracted in 200 components = 0.00499995 Jy ! Clean residual min=-0.008272 max=0.013224 Jy/beam ! Clean residual mean=0.001716 rms=0.003524 Jy/beam ! Combined flux in latest and established models = 2.57203 Jy ! Adding 39 model components to the UV plane model. ! The established model now contains 90 components and 2.57203 Jy ! Inverting map ! Your choice of large map pixels excluded 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 milli-arcsec ! Estimated beam: bmin=0.9676 mas, bmaj=2.829 mas, bpa=-1.305 degrees ! Estimated noise=1044.22 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000778521 Jy ! Component: 100 - total flux cleaned = 0.00208123 Jy ! Component: 150 - total flux cleaned = 0.00318198 Jy ! Component: 200 - total flux cleaned = 0.00436018 Jy ! Total flux subtracted in 200 components = 0.00436018 Jy ! Clean residual min=-0.007540 max=0.010431 Jy/beam ! Clean residual mean=0.000657 rms=0.002678 Jy/beam ! Combined flux in latest and established models = 2.57639 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 103 components and 2.57639 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=2.907686Jy sigma=0.001246 ! Fit after self-cal, rms=2.908119Jy sigma=0.001240 wmodel J2258-2758_X_2010_10_13_pus_map.mod ! Writing 103 model components to file: J2258-2758_X_2010_10_13_pus_map.mod wobs J2258-2758_X_2010_10_13_pus_uvs.fits ! Writing UV FITS file: J2258-2758_X_2010_10_13_pus_uvs.fits wwins J2258-2758_X_2010_10_13_pus_map.win ! wwins: Wrote 3 windows to J2258-2758_X_2010_10_13_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 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 milli-arcsec ! clean: niter=1024 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.00289198 Jy ! Component: 100 - total flux cleaned = 0.00416777 Jy ! Component: 150 - total flux cleaned = 0.00531847 Jy ! Component: 200 - total flux cleaned = 0.00613731 Jy ! Component: 250 - total flux cleaned = 0.0065753 Jy ! Component: 300 - total flux cleaned = 0.00719411 Jy ! Component: 350 - total flux cleaned = 0.00788774 Jy ! Component: 400 - total flux cleaned = 0.00855476 Jy ! Component: 450 - total flux cleaned = 0.00937769 Jy ! Component: 500 - total flux cleaned = 0.00999474 Jy ! Component: 550 - total flux cleaned = 0.0105088 Jy ! Component: 600 - total flux cleaned = 0.0110075 Jy ! Component: 650 - total flux cleaned = 0.0114105 Jy ! Component: 700 - total flux cleaned = 0.0116468 Jy ! Component: 750 - total flux cleaned = 0.0118013 Jy ! Component: 800 - total flux cleaned = 0.0118777 Jy ! Component: 850 - total flux cleaned = 0.0119523 Jy ! Component: 900 - total flux cleaned = 0.0120253 Jy ! Component: 950 - total flux cleaned = 0.0122392 Jy ! Component: 1000 - total flux cleaned = 0.0123092 Jy ! Total flux subtracted in 1024 components = 0.0123786 Jy ! Clean residual min=-0.003932 max=0.003749 Jy/beam ! Clean residual mean=0.000076 rms=0.001485 Jy/beam ! Combined flux in latest and established models = 2.58876 Jy keep ! Adding 56 model components to the UV plane model. ! The established model now contains 159 components and 2.58876 Jy ![Exited script file: muppet] wmap "J2258-2758_X_2010_10_13_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9676 x 2.829 at -1.305 degrees (North through East) ! Clean map min=-0.01081 max=2.2417 Jy/beam ! Writing clean map to FITS file: J2258-2758_X_2010_10_13_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 2.24174 invert ! Inverting map ! Your choice of large map pixels excluded 2.75% of the data. ! The x-axis pixel size should ideally be below 0.1618 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00150224 device "J2258-2758_X_2010_10_13_pus\_map.eps/VPS" ! Attempting to open device: 'J2258-2758_X_2010_10_13_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.201037 0.201037 0.402074 0.804149 1.6083 3.2166 6.43319 12.8664 25.7328 51.4655 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0045 print "peak=",int(1000*peak_flux)/1000 ! peak= 2.241 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9676 x 2.829 at -1.305 degrees (North through East) ! Clean map min=-0.01081 max=2.2417 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J2258-2758_X_2010_10_13_pus\_map.gif/vgif" ! Attempting to open device: 'J2258-2758_X_2010_10_13_pus_map.gif/vgif' mapplot cln