! Started logfile: J1127-1857_X_2013_01_09_pus_uvs.log on Mon Nov 3 15:54:27 2014 obs J1127-1857_X_2013_01_09_pus_uva.fits ! Reading UV FITS file: J1127-1857_X_2013_01_09_pus_uva.fits ! AN table 1: Unused. ! AN table 2: Unused. ! AN table 3: 83 integrations on 120 of 120 possible baselines. ! AN table 4: Unused. ! AN table 5: Unused. ! Apparent sampling: 0.161847 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1127-1857 ! ! 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 2994 lines of history. ! ! Reading 6448 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 J1127-1857_X_2013_01_09_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 879 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 879 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 879 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 879 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=2.066189Jy sigma=0.018144 ! Fit after self-cal, rms=2.063816Jy sigma=0.018166 ! 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 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 milli-arcsec ! Estimated beam: bmin=0.6571 mas, bmaj=1.964 mas, bpa=-5.397 degrees ! Estimated noise=1646.94 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 = 2.24054 Jy ! Component: 100 - total flux cleaned = 2.78421 Jy ! Total flux subtracted in 100 components = 2.78421 Jy ! Clean residual min=-0.138020 max=0.222954 Jy/beam ! Clean residual mean=0.000825 rms=0.047797 Jy/beam ! Combined flux in latest and established models = 2.7842 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 2.7842 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.914302Jy sigma=0.006670 ! Fit after self-cal, rms=0.914285Jy sigma=0.006669 ! Inverting map ! Your choice of large map pixels excluded 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 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 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 milli-arcsec ! Estimated beam: bmin=0.8596 mas, bmaj=2.45 mas, bpa=-6.993 degrees ! Estimated noise=1090.58 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 = 0.230221 Jy ! Component: 100 - total flux cleaned = 0.355396 Jy ! Component: 150 - total flux cleaned = 0.429089 Jy ! Component: 200 - total flux cleaned = 0.473164 Jy ! Total flux subtracted in 200 components = 0.473164 Jy ! Clean residual min=-0.169992 max=0.108756 Jy/beam ! Clean residual mean=-0.020371 rms=0.042702 Jy/beam ! Combined flux in latest and established models = 3.25737 Jy ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 33 components and 3.25737 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.879748Jy sigma=0.005949 ! Fit after self-cal, rms=0.879727Jy sigma=0.005948 ! Inverting map ! Your choice of large map pixels excluded 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 1.06 HH 1.00* HN 1.10 ! KP 0.73 LA 1.02 MC 1.00* MK 0.87 ! NL 0.85 NY 1.00* OV 0.95 PT 1.03 ! SC 0.97 TS 1.00* WF 0.96 WZ 1.33 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.05 FD 1.09 HH 1.00* HN 1.15 ! KP 0.71 LA 1.05 MC 1.00* MK 0.91 ! NL 1.00 NY 1.00* OV 0.98 PT 1.11 ! SC 1.06 TS 1.00* WF 1.02 WZ 1.35 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 1.09 HH 1.00* HN 1.12 ! KP 0.62 LA 1.05 MC 1.00* MK 0.90 ! NL 0.93 NY 1.00* OV 0.98 PT 1.03 ! SC 0.97 TS 1.00* WF 1.04 WZ 1.36 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.08 FD 1.18 HH 1.00* HN 1.16 ! KP 0.68 LA 1.11 MC 1.00* MK 0.95 ! NL 0.96 NY 1.00* OV 1.01 PT 1.14 ! SC 1.08 TS 1.00* WF 1.12 WZ 1.41 ! ! ! Fit before self-cal, rms=0.879727Jy sigma=0.005948 ! Fit after self-cal, rms=0.568656Jy sigma=0.003004 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 milli-arcsec ! Estimated beam: bmin=0.8881 mas, bmaj=2.465 mas, bpa=-7.293 degrees ! Estimated noise=1078.68 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 = -0.0770797 Jy ! Component: 100 - total flux cleaned = -0.10868 Jy ! Component: 150 - total flux cleaned = -0.118231 Jy ! Component: 200 - total flux cleaned = -0.119024 Jy ! Total flux subtracted in 200 components = -0.119024 Jy ! Clean residual min=-0.074365 max=0.075247 Jy/beam ! Clean residual mean=-0.007074 rms=0.024096 Jy/beam ! Combined flux in latest and established models = 3.13835 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 40 components and 3.13835 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.543953Jy sigma=0.003007 ! Fit after self-cal, rms=0.544095Jy sigma=0.003007 ! Inverting map ! Your choice of large map pixels excluded 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 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=0.544095Jy sigma=0.003007 ! Fit after self-cal, rms=0.309134Jy sigma=0.001664 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 milli-arcsec ! Estimated beam: bmin=0.8921 mas, bmaj=2.473 mas, bpa=-7.364 degrees ! Estimated noise=1075.52 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0293017 Jy ! Component: 100 - total flux cleaned = -0.0444088 Jy ! Component: 150 - total flux cleaned = -0.0488807 Jy ! Component: 200 - total flux cleaned = -0.0505452 Jy ! Total flux subtracted in 200 components = -0.0505452 Jy ! Clean residual min=-0.034217 max=0.022911 Jy/beam ! Clean residual mean=-0.003754 rms=0.007975 Jy/beam ! Combined flux in latest and established models = 3.0878 Jy selfcal ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 41 components and 3.0878 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.304723Jy sigma=0.001637 ! Fit after self-cal, rms=0.305111Jy sigma=0.001637 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 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 = -0.00194491 Jy ! Component: 100 - total flux cleaned = -0.00268853 Jy ! Component: 150 - total flux cleaned = -0.00357307 Jy ! Component: 200 - total flux cleaned = -0.00453228 Jy ! Total flux subtracted in 200 components = -0.00453228 Jy ! Clean residual min=-0.033051 max=0.023429 Jy/beam ! Clean residual mean=-0.003575 rms=0.007878 Jy/beam ! Combined flux in latest and established models = 3.08327 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 41 components and 3.08327 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.304790Jy sigma=0.001632 ! Fit after self-cal, rms=0.304763Jy sigma=0.001632 ! Inverting map ! Your choice of large map pixels excluded 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 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=0.304763Jy sigma=0.001632 ! Fit after self-cal, rms=0.257190Jy sigma=0.001217 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 milli-arcsec ! Estimated beam: bmin=0.8924 mas, bmaj=2.476 mas, bpa=-7.335 degrees ! Estimated noise=1075.07 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0166666 Jy ! Component: 100 - total flux cleaned = -0.0193938 Jy ! Component: 150 - total flux cleaned = -0.020329 Jy ! Component: 200 - total flux cleaned = -0.0214361 Jy ! Total flux subtracted in 200 components = -0.0214361 Jy ! Clean residual min=-0.012063 max=0.007177 Jy/beam ! Clean residual mean=-0.001672 rms=0.002541 Jy/beam ! Combined flux in latest and established models = 3.06183 Jy selfcal ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 43 components and 3.06183 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.255349Jy sigma=0.001202 ! Fit after self-cal, rms=0.255396Jy sigma=0.001202 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 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 = -0.000813431 Jy ! Component: 100 - total flux cleaned = -0.00166339 Jy ! Component: 150 - total flux cleaned = -0.00222732 Jy ! Component: 200 - total flux cleaned = -0.00289087 Jy ! Total flux subtracted in 200 components = -0.00289087 Jy ! Clean residual min=-0.011245 max=0.007832 Jy/beam ! Clean residual mean=-0.001563 rms=0.002411 Jy/beam ! Combined flux in latest and established models = 3.05894 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 44 components and 3.05894 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.255035Jy sigma=0.001198 ! Fit after self-cal, rms=0.255024Jy sigma=0.001198 ! Inverting map ! Your choice of large map pixels excluded 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 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=0.255024Jy sigma=0.001198 ! Fit after self-cal, rms=0.254738Jy sigma=0.001191 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 milli-arcsec ! Estimated beam: bmin=2.037 mas, bmaj=3.504 mas, bpa=-6.036 degrees ! Estimated noise=1337.37 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00954021 Jy ! Component: 100 - total flux cleaned = -0.0123927 Jy ! Component: 150 - total flux cleaned = -0.0128583 Jy ! Component: 200 - total flux cleaned = -0.0132649 Jy ! Total flux subtracted in 200 components = -0.0132649 Jy ! Clean residual min=-0.009570 max=0.005207 Jy/beam ! Clean residual mean=-0.002287 rms=0.002382 Jy/beam ! Combined flux in latest and established models = 3.04568 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 49 components and 3.04568 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.254216Jy sigma=0.001189 ! Fit after self-cal, rms=0.254192Jy sigma=0.001189 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 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 = -0.000624266 Jy ! Component: 100 - total flux cleaned = -0.000785497 Jy ! Component: 150 - total flux cleaned = -0.000994709 Jy ! Component: 200 - total flux cleaned = -0.00124416 Jy ! Total flux subtracted in 200 components = -0.00124416 Jy ! Clean residual min=-0.009129 max=0.004979 Jy/beam ! Clean residual mean=-0.002182 rms=0.002342 Jy/beam ! Combined flux in latest and established models = 3.04443 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 51 components and 3.04443 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.254112Jy sigma=0.001188 ! Fit after self-cal, rms=0.254102Jy sigma=0.001188 ! Inverting map ! Your choice of large map pixels excluded 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 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 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 milli-arcsec ! Estimated beam: bmin=0.8927 mas, bmaj=2.478 mas, bpa=-7.311 degrees ! Estimated noise=1074.4 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8927 x 2.478 at -7.311 degrees (North through East) ! Clean map min=-0.008176 max=2.86 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=0.254102Jy sigma=0.001188 ! Fit after self-cal, rms=0.239435Jy sigma=0.001073 ! Inverting map and beam ! Your choice of large map pixels excluded 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 milli-arcsec ! Estimated beam: bmin=0.8936 mas, bmaj=2.48 mas, bpa=-7.299 degrees ! Estimated noise=1074.33 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00573139 Jy ! Component: 100 - total flux cleaned = -0.00638201 Jy ! Component: 150 - total flux cleaned = -0.0068187 Jy ! Component: 200 - total flux cleaned = -0.00721503 Jy ! Total flux subtracted in 200 components = -0.00721503 Jy ! Clean residual min=-0.008518 max=0.006068 Jy/beam ! Clean residual mean=-0.000866 rms=0.001847 Jy/beam ! Combined flux in latest and established models = 3.03722 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 53 components and 3.03722 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.239180Jy sigma=0.001070 ! Fit after self-cal, rms=0.239173Jy sigma=0.001070 ! Inverting map ! Your choice of large map pixels excluded 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00039988 Jy ! Component: 100 - total flux cleaned = -0.000724448 Jy ! Component: 150 - total flux cleaned = -0.00102524 Jy ! Component: 200 - total flux cleaned = -0.00129924 Jy ! Total flux subtracted in 200 components = -0.00129924 Jy ! Clean residual min=-0.008078 max=0.006030 Jy/beam ! Clean residual mean=-0.000815 rms=0.001808 Jy/beam ! Combined flux in latest and established models = 3.03592 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 57 components and 3.03592 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.239078Jy sigma=0.001069 ! Fit after self-cal, rms=0.239074Jy sigma=0.001069 ! Inverting map ! Your choice of large map pixels excluded 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.239074Jy sigma=0.001069 ! Fit after self-cal, rms=0.238978Jy sigma=0.001068 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 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 milli-arcsec ! Estimated beam: bmin=0.6851 mas, bmaj=1.974 mas, bpa=-5.83 degrees ! Estimated noise=1614.2 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 2.19592 Jy ! Component: 100 - total flux cleaned = 2.68752 Jy ! Component: 150 - total flux cleaned = 2.85478 Jy ! Component: 200 - total flux cleaned = 2.93363 Jy ! Total flux subtracted in 200 components = 2.93363 Jy ! Clean residual min=-0.015558 max=0.036001 Jy/beam ! Clean residual mean=0.000408 rms=0.005590 Jy/beam ! Combined flux in latest and established models = 2.93363 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 10 model components to the UV plane model. ! The established model now contains 10 components and 2.93363 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 milli-arcsec ! Estimated beam: bmin=0.8938 mas, bmaj=2.48 mas, bpa=-7.288 degrees ! Estimated noise=1073.95 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 = 0.0503148 Jy ! Component: 100 - total flux cleaned = 0.0747544 Jy ! Component: 150 - total flux cleaned = 0.0880334 Jy ! Component: 200 - total flux cleaned = 0.0914066 Jy ! Total flux subtracted in 200 components = 0.0914066 Jy ! Clean residual min=-0.007545 max=0.009278 Jy/beam ! Clean residual mean=-0.000440 rms=0.002194 Jy/beam ! Combined flux in latest and established models = 3.02504 Jy ! Adding 31 model components to the UV plane model. ! The established model now contains 37 components and 3.02504 Jy ! Inverting map ! Your choice of large map pixels excluded 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 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 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 milli-arcsec ! Estimated beam: bmin=2.039 mas, bmaj=3.512 mas, bpa=-6.019 degrees ! Estimated noise=1334.62 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00330121 Jy ! Component: 100 - total flux cleaned = 0.00330022 Jy ! Component: 150 - total flux cleaned = 0.00329269 Jy ! Component: 200 - total flux cleaned = 0.00328522 Jy ! Total flux subtracted in 200 components = 0.00328522 Jy ! Clean residual min=-0.007021 max=0.005698 Jy/beam ! Clean residual mean=-0.001194 rms=0.002070 Jy/beam ! Combined flux in latest and established models = 3.02832 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 = -4.21653e-06 Jy ! Component: 100 - total flux cleaned = -7.34102e-06 Jy ! Component: 150 - total flux cleaned = -1.11095e-05 Jy ! Component: 200 - total flux cleaned = -1.56714e-05 Jy ! Total flux subtracted in 200 components = -1.56714e-05 Jy ! Clean residual min=-0.006807 max=0.005507 Jy/beam ! Clean residual mean=-0.001188 rms=0.002022 Jy/beam ! Combined flux in latest and established models = 3.02831 Jy ! Adding 11 model components to the UV plane model. ! The established model now contains 44 components and 3.02831 Jy ! Inverting map ! Your choice of large map pixels excluded 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 milli-arcsec ! Estimated beam: bmin=0.8938 mas, bmaj=2.48 mas, bpa=-7.288 degrees ! Estimated noise=1073.95 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00281256 Jy ! Component: 100 - total flux cleaned = 0.00302309 Jy ! Component: 150 - total flux cleaned = 0.00264468 Jy ! Component: 200 - total flux cleaned = 0.00247452 Jy ! Total flux subtracted in 200 components = 0.00247452 Jy ! Clean residual min=-0.007179 max=0.008007 Jy/beam ! Clean residual mean=-0.000678 rms=0.001917 Jy/beam ! Combined flux in latest and established models = 3.03078 Jy selfcal ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 48 components and 3.03078 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.239566Jy sigma=0.001076 ! Fit after self-cal, rms=0.239478Jy sigma=0.001075 wmodel J1127-1857_X_2013_01_09_pus_map.mod ! Writing 48 model components to file: J1127-1857_X_2013_01_09_pus_map.mod wobs J1127-1857_X_2013_01_09_pus_uvs.fits ! Writing UV FITS file: J1127-1857_X_2013_01_09_pus_uvs.fits wwins J1127-1857_X_2013_01_09_pus_map.win ! wwins: Wrote 1 windows to J1127-1857_X_2013_01_09_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 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 milli-arcsec ! clean: niter=1024 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000210008 Jy ! Component: 100 - total flux cleaned = -0.000513122 Jy ! Component: 150 - total flux cleaned = -0.00153956 Jy ! Component: 200 - total flux cleaned = -0.00272694 Jy ! Component: 250 - total flux cleaned = -0.00345013 Jy ! Component: 300 - total flux cleaned = -0.0040444 Jy ! Component: 350 - total flux cleaned = -0.00452245 Jy ! Component: 400 - total flux cleaned = -0.00517191 Jy ! Component: 450 - total flux cleaned = -0.00580133 Jy ! Component: 500 - total flux cleaned = -0.00632579 Jy ! Component: 550 - total flux cleaned = -0.00666619 Jy ! Component: 600 - total flux cleaned = -0.00708273 Jy ! Component: 650 - total flux cleaned = -0.00732797 Jy ! Component: 700 - total flux cleaned = -0.00772821 Jy ! Component: 750 - total flux cleaned = -0.00804127 Jy ! Component: 800 - total flux cleaned = -0.0083482 Jy ! Component: 850 - total flux cleaned = -0.00864898 Jy ! Component: 900 - total flux cleaned = -0.00894377 Jy ! Component: 950 - total flux cleaned = -0.00916065 Jy ! Component: 1000 - total flux cleaned = -0.00937301 Jy ! Total flux subtracted in 1024 components = -0.00951296 Jy ! Clean residual min=-0.003921 max=0.003494 Jy/beam ! Clean residual mean=-0.000310 rms=0.001322 Jy/beam ! Combined flux in latest and established models = 3.02127 Jy keep ! Adding 60 model components to the UV plane model. ! The established model now contains 108 components and 3.02127 Jy ![Exited script file: muppet] wmap "J1127-1857_X_2013_01_09_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8938 x 2.48 at -7.288 degrees (North through East) ! Clean map min=-0.0055218 max=2.8624 Jy/beam ! Writing clean map to FITS file: J1127-1857_X_2013_01_09_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 2.86243 invert ! Inverting map ! Your choice of large map pixels excluded 0.441% of the data. ! The x-axis pixel size should ideally be below 0.1974 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.0013199 device "J1127-1857_X_2013_01_09_pus\_map.eps/VPS" ! Attempting to open device: 'J1127-1857_X_2013_01_09_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.138334 0.138334 0.276668 0.553336 1.10667 2.21335 4.42669 8.85338 17.7068 35.4135 70.827 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0039 print "peak=",int(1000*peak_flux)/1000 ! peak= 2.862 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8938 x 2.48 at -7.288 degrees (North through East) ! Clean map min=-0.0055218 max=2.8624 Jy/beam quit ! Quitting program ! Log file J1127-1857_X_2013_01_09_pus_uvs.log closed on Mon Nov 3 15:54:28 2014