! Started logfile: J1848+3219_X_2009_04_21_pus_uvs.log on Sun Jan 23 00:38:24 2011 obs J1848+3219_X_2009_04_21_pus_uva.fits ! Reading UV FITS file: J1848+3219_X_2009_04_21_pus_uva.fits ! AN table 1: 52 integrations on 120 of 120 possible baselines. ! AN table 2: 45 integrations on 120 of 120 possible baselines. ! AN table 3: 319 integrations on 120 of 120 possible baselines. ! Apparent sampling: 0.180228 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1848+3219 ! ! There are 4 IFs, and a total of 4 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 8.40997e+09 8e+06 1 8e+06 ! 02 2 8.47997e+09 8e+06 1 8e+06 ! 03 3 8.79497e+09 8e+06 1 8e+06 ! 04 4 8.89997e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 2445 lines of history. ! ! Reading 35988 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 J1848+3219_X_2009_04_21_pus] integer clean_niter clean_niter = 100 float clean_gain clean_gain = 0.03 float dynam dynam = 6.0 float soltime1 soltime1 = 120 float soltime2 soltime2 = 20 float thresh thresh = 0.5 float win_mult win_mult = 1.8 float time_av time_av = 16 float old_peak float new_peak float flux_cutoff mapsize field_size, field_cell ! Map grid = 512x512 pixels with 0.200x0.200 milli-arcsec cellsize. startmod ! Applying default point source starting model. ! Performing phase self-cal ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 1 Jy ! ! Correcting IF 1. ! A total of 516 telescope corrections were flagged in sub-array 1. ! A total of 672 telescope corrections were flagged in sub-array 2. ! A total of 3494 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 516 telescope corrections were flagged in sub-array 1. ! A total of 672 telescope corrections were flagged in sub-array 2. ! A total of 3495 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 516 telescope corrections were flagged in sub-array 1. ! A total of 672 telescope corrections were flagged in sub-array 2. ! A total of 3494 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 516 telescope corrections were flagged in sub-array 1. ! A total of 672 telescope corrections were flagged in sub-array 2. ! A total of 3494 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=0.705399Jy sigma=0.006316 ! Fit after self-cal, rms=0.507732Jy sigma=0.004495 ! 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 6.54% of the data. ! The x-axis pixel size should ideally be below 0.1629 milli-arcsec ! Estimated beam: bmin=0.5435 mas, bmaj=1.028 mas, bpa=6.015 degrees ! Estimated noise=797.207 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 = 0.408521 Jy ! Component: 100 - total flux cleaned = 0.502861 Jy ! Total flux subtracted in 100 components = 0.502861 Jy ! Clean residual min=-0.009259 max=0.036808 Jy/beam ! Clean residual mean=0.000046 rms=0.002944 Jy/beam ! Combined flux in latest and established models = 0.502861 Jy ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 4 components and 0.502861 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.178662Jy sigma=0.001456 ! Fit after self-cal, rms=0.178649Jy sigma=0.001456 ! Inverting map ! Your choice of large map pixels excluded 6.54% of the data. ! The x-axis pixel size should ideally be below 0.1629 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.04146 Jy ! Component: 100 - total flux cleaned = 0.0661874 Jy ! Total flux subtracted in 100 components = 0.0661874 Jy ! Clean residual min=-0.009436 max=0.013200 Jy/beam ! Clean residual mean=-0.000012 rms=0.002092 Jy/beam ! Combined flux in latest and established models = 0.569048 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 17 components and 0.569048 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.168419Jy sigma=0.001326 ! Fit after self-cal, rms=0.168322Jy sigma=0.001325 ! Inverting map ! Your choice of large map pixels excluded 6.54% of the data. ! The x-axis pixel size should ideally be below 0.1629 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0167595 Jy ! Component: 100 - total flux cleaned = 0.0279878 Jy ! Total flux subtracted in 100 components = 0.0279878 Jy ! Clean residual min=-0.008851 max=0.007959 Jy/beam ! Clean residual mean=-0.000036 rms=0.001875 Jy/beam ! Combined flux in latest and established models = 0.597036 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 21 components and 0.597036 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.166879Jy sigma=0.001304 ! Fit after self-cal, rms=0.166861Jy sigma=0.001304 ! Inverting map ! Your choice of large map pixels excluded 6.54% of the data. ! The x-axis pixel size should ideally be below 0.1629 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 6.54% of the data. ! The x-axis pixel size should ideally be below 0.1629 milli-arcsec ! Estimated beam: bmin=0.617 mas, bmaj=1.13 mas, bpa=7.303 degrees ! Estimated noise=444.689 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 = 0.00805163 Jy ! Component: 100 - total flux cleaned = 0.0122379 Jy ! Component: 150 - total flux cleaned = 0.0145901 Jy ! Component: 200 - total flux cleaned = 0.0152868 Jy ! Total flux subtracted in 200 components = 0.0152868 Jy ! Clean residual min=-0.007938 max=0.006461 Jy/beam ! Clean residual mean=-0.000824 rms=0.001496 Jy/beam ! Combined flux in latest and established models = 0.612322 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 28 components and 0.612323 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.166696Jy sigma=0.001300 ! Fit after self-cal, rms=0.166689Jy sigma=0.001300 ! Inverting map ! Your choice of large map pixels excluded 6.54% of the data. ! The x-axis pixel size should ideally be below 0.1629 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 54 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 FD 1.00 HN 1.03 KB 1.00* ! KK 0.99 KP 0.97 LA 0.99 MK 1.01 ! NL 0.96 NY 1.00* OV 0.98 PT 0.97 ! SC 0.98 TS 1.00* WZ 1.00* ZC 1.00* ! ! A total of 33 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* HN 1.00* KB 1.15 ! KK 1.16 KP 1.00* LA 1.00* MK 0.98 ! NL 1.00* NY 0.84 OV 1.00* PT 1.00* ! SC 0.86 TS 1.00* WZ 1.00* ZC 1.00* ! ! A total of 117 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 0.99 HN 1.09 KB 1.02 ! KK 0.98 KP 0.99 LA 0.99 MK 0.99 ! NL 0.98 NY 0.98 OV 1.02 PT 0.99 ! SC 0.99 TS 1.07 WZ 1.06 ZC 0.98 ! ! ! Correcting IF 2. ! A total of 54 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 FD 0.97 HN 1.02 KB 1.00* ! KK 0.96 KP 0.97 LA 0.98 MK 1.02 ! NL 0.96 NY 1.00* OV 0.96 PT 0.97 ! SC 0.98 TS 1.00* WZ 1.00* ZC 1.00* ! ! A total of 33 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* HN 1.00* KB 1.26 ! KK 0.98 KP 1.00* LA 1.00* MK 0.91 ! NL 1.00* NY 1.08 OV 1.00* PT 1.00* ! SC 0.94 TS 1.00* WZ 1.00* ZC 1.00* ! ! A total of 117 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 FD 0.99 HN 1.10 KB 1.05 ! KK 0.96 KP 0.99 LA 0.99 MK 0.97 ! NL 0.96 NY 1.01 OV 0.98 PT 0.97 ! SC 1.01 TS 1.09 WZ 0.99 ZC 0.99 ! ! ! Correcting IF 3. ! A total of 54 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.97 HN 1.04 KB 1.00* ! KK 1.00 KP 0.98 LA 0.99 MK 1.01 ! NL 1.00 NY 1.00* OV 0.99 PT 0.94 ! SC 1.01 TS 1.00* WZ 1.00* ZC 1.00* ! ! A total of 33 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* HN 1.00* KB 1.08 ! KK 1.16 KP 1.00* LA 1.00* MK 0.94 ! NL 1.00* NY 1.04 OV 1.00* PT 1.00* ! SC 1.19 TS 1.00* WZ 1.00* ZC 1.00* ! ! A total of 117 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 1.00 HN 1.11 KB 1.04 ! KK 0.99 KP 0.98 LA 1.00 MK 0.99 ! NL 0.99 NY 1.05 OV 1.02 PT 0.97 ! SC 1.02 TS 1.05 WZ 0.96 ZC 1.00 ! ! ! Correcting IF 4. ! A total of 54 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.94 FD 1.02 HN 1.05 KB 1.00* ! KK 1.03 KP 0.96 LA 0.98 MK 1.00 ! NL 1.02 NY 1.00* OV 1.00 PT 0.93 ! SC 0.99 TS 1.00* WZ 1.00* ZC 1.00* ! ! A total of 33 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* HN 1.00* KB 1.10 ! KK 1.06 KP 1.00* LA 1.00* MK 1.10 ! NL 1.00* NY 0.94 OV 1.00* PT 1.00* ! SC 1.02 TS 1.00* WZ 1.00* ZC 1.00* ! ! A total of 117 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 FD 1.00 HN 1.11 KB 1.04 ! KK 0.97 KP 0.99 LA 0.99 MK 0.99 ! NL 1.00 NY 1.00 OV 1.02 PT 0.96 ! SC 1.05 TS 1.08 WZ 0.98 ZC 0.98 ! ! ! Fit before self-cal, rms=0.166689Jy sigma=0.001300 ! Fit after self-cal, rms=0.165757Jy sigma=0.001243 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 milli-arcsec ! Estimated beam: bmin=0.6258 mas, bmaj=1.129 mas, bpa=7.452 degrees ! Estimated noise=453.239 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 = -0.00435716 Jy ! Component: 100 - total flux cleaned = -0.00511379 Jy ! Component: 150 - total flux cleaned = -0.00550451 Jy ! Component: 200 - total flux cleaned = -0.00561988 Jy ! Total flux subtracted in 200 components = -0.00561988 Jy ! Clean residual min=-0.005891 max=0.005036 Jy/beam ! Clean residual mean=-0.000086 rms=0.001197 Jy/beam ! Combined flux in latest and established models = 0.606703 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 31 components and 0.606703 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.165592Jy sigma=0.001243 ! Fit after self-cal, rms=0.165619Jy sigma=0.001243 ! Inverting map ! Your choice of large map pixels excluded 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 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=0.165619Jy sigma=0.001243 ! Fit after self-cal, rms=0.166602Jy sigma=0.001217 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 milli-arcsec ! Estimated beam: bmin=0.6275 mas, bmaj=1.129 mas, bpa=7.225 degrees ! Estimated noise=453.006 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00316898 Jy ! Component: 100 - total flux cleaned = -0.00318015 Jy ! Component: 150 - total flux cleaned = -0.00318147 Jy ! Component: 200 - total flux cleaned = -0.00318384 Jy ! Total flux subtracted in 200 components = -0.00318384 Jy ! Clean residual min=-0.002495 max=0.002873 Jy/beam ! Clean residual mean=-0.000152 rms=0.000576 Jy/beam ! Combined flux in latest and established models = 0.603519 Jy selfcal ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 32 components and 0.603519 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.166501Jy sigma=0.001216 ! Fit after self-cal, rms=0.166571Jy sigma=0.001216 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 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) ! Added new window around map position (-0.8, 0.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00275581 Jy ! Component: 100 - total flux cleaned = 0.00317111 Jy ! Component: 150 - total flux cleaned = 0.00338657 Jy ! Component: 200 - total flux cleaned = 0.00352029 Jy ! Total flux subtracted in 200 components = 0.00352029 Jy ! Clean residual min=-0.002457 max=0.001828 Jy/beam ! Clean residual mean=-0.000178 rms=0.000540 Jy/beam ! Combined flux in latest and established models = 0.607039 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 41 components and 0.607039 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.166512Jy sigma=0.001216 ! Fit after self-cal, rms=0.166502Jy sigma=0.001216 ! Inverting map ! Your choice of large map pixels excluded 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 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=0.166502Jy sigma=0.001216 ! Fit after self-cal, rms=0.166119Jy sigma=0.001215 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 milli-arcsec ! Estimated beam: bmin=0.6285 mas, bmaj=1.13 mas, bpa=7.074 degrees ! Estimated noise=452.969 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000563582 Jy ! Component: 100 - total flux cleaned = -0.000498442 Jy ! Component: 150 - total flux cleaned = -0.000397263 Jy ! Component: 200 - total flux cleaned = -0.000312472 Jy ! Total flux subtracted in 200 components = -0.000312472 Jy ! Clean residual min=-0.002193 max=0.001919 Jy/beam ! Clean residual mean=-0.000092 rms=0.000513 Jy/beam ! Combined flux in latest and established models = 0.606727 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 43 components and 0.606727 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.166073Jy sigma=0.001215 ! Fit after self-cal, rms=0.166063Jy sigma=0.001215 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 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 = 0.000338212 Jy ! Component: 100 - total flux cleaned = 0.000408347 Jy ! Component: 150 - total flux cleaned = 0.000498258 Jy ! Component: 200 - total flux cleaned = 0.000551858 Jy ! Total flux subtracted in 200 components = 0.000551858 Jy ! Clean residual min=-0.002209 max=0.001922 Jy/beam ! Clean residual mean=-0.000096 rms=0.000507 Jy/beam ! Combined flux in latest and established models = 0.607279 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 47 components and 0.607279 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.166049Jy sigma=0.001215 ! Fit after self-cal, rms=0.166048Jy sigma=0.001215 ! Inverting map ! Your choice of large map pixels excluded 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 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=0.166048Jy sigma=0.001215 ! Fit after self-cal, rms=0.165765Jy sigma=0.001214 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 milli-arcsec ! Estimated beam: bmin=2.378 mas, bmaj=2.705 mas, bpa=-9.299 degrees ! Estimated noise=666.561 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000464969 Jy ! Component: 100 - total flux cleaned = -0.000457506 Jy ! Component: 150 - total flux cleaned = -0.000404156 Jy ! Component: 200 - total flux cleaned = -0.00034744 Jy ! Total flux subtracted in 200 components = -0.00034744 Jy ! Clean residual min=-0.002347 max=0.002109 Jy/beam ! Clean residual mean=-0.000137 rms=0.000665 Jy/beam ! Combined flux in latest and established models = 0.606931 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 58 components and 0.606931 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.165762Jy sigma=0.001214 ! Fit after self-cal, rms=0.165752Jy sigma=0.001214 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 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 = 0.000115339 Jy ! Component: 100 - total flux cleaned = 0.000135513 Jy ! Component: 150 - total flux cleaned = 0.00015066 Jy ! Component: 200 - total flux cleaned = 0.00015144 Jy ! Total flux subtracted in 200 components = 0.00015144 Jy ! Clean residual min=-0.002371 max=0.002092 Jy/beam ! Clean residual mean=-0.000141 rms=0.000662 Jy/beam ! Combined flux in latest and established models = 0.607083 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 69 components and 0.607083 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.165753Jy sigma=0.001214 ! Fit after self-cal, rms=0.165752Jy sigma=0.001214 ! Inverting map ! Your choice of large map pixels excluded 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 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 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 milli-arcsec ! Estimated beam: bmin=0.6291 mas, bmaj=1.13 mas, bpa=6.997 degrees ! Estimated noise=452.894 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6291 x 1.13 at 6.997 degrees (North through East) ! Clean map min=-0.0016595 max=0.53041 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=0.165752Jy sigma=0.001214 ! Fit after self-cal, rms=0.162649Jy sigma=0.001135 ! Inverting map and beam ! Your choice of large map pixels excluded 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 milli-arcsec ! Estimated beam: bmin=0.6294 mas, bmaj=1.13 mas, bpa=7.062 degrees ! Estimated noise=452.609 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000236661 Jy ! Component: 100 - total flux cleaned = -0.000158835 Jy ! Component: 150 - total flux cleaned = -0.000159095 Jy ! Component: 200 - total flux cleaned = -0.000157755 Jy ! Total flux subtracted in 200 components = -0.000157755 Jy ! Clean residual min=-0.001905 max=0.002007 Jy/beam ! Clean residual mean=-0.000042 rms=0.000480 Jy/beam ! Combined flux in latest and established models = 0.606925 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 70 components and 0.606925 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.162633Jy sigma=0.001135 ! Fit after self-cal, rms=0.162633Jy sigma=0.001135 ! Inverting map ! Your choice of large map pixels excluded 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 6.19636e-05 Jy ! Component: 100 - total flux cleaned = 8.22709e-05 Jy ! Component: 150 - total flux cleaned = 4.32984e-05 Jy ! Component: 200 - total flux cleaned = 8.26194e-06 Jy ! Total flux subtracted in 200 components = 8.26194e-06 Jy ! Clean residual min=-0.001947 max=0.001984 Jy/beam ! Clean residual mean=-0.000042 rms=0.000479 Jy/beam ! Combined flux in latest and established models = 0.606933 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 72 components and 0.606933 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.162627Jy sigma=0.001135 ! Fit after self-cal, rms=0.162627Jy sigma=0.001135 ! Inverting map ! Your choice of large map pixels excluded 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.162627Jy sigma=0.001135 ! Fit after self-cal, rms=0.162597Jy sigma=0.001135 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 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 milli-arcsec ! Estimated beam: bmin=0.5573 mas, bmaj=1.029 mas, bpa=6.283 degrees ! Estimated noise=804.997 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.408849 Jy ! Component: 100 - total flux cleaned = 0.501173 Jy ! Component: 150 - total flux cleaned = 0.537641 Jy ! Component: 200 - total flux cleaned = 0.558902 Jy ! Total flux subtracted in 200 components = 0.558902 Jy ! Clean residual min=-0.005200 max=0.011076 Jy/beam ! Clean residual mean=0.000034 rms=0.001211 Jy/beam ! Combined flux in latest and established models = 0.558902 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 19 model components to the UV plane model. ! The established model now contains 19 components and 0.558902 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 milli-arcsec ! Estimated beam: bmin=0.6296 mas, bmaj=1.13 mas, bpa=7.005 degrees ! Estimated noise=452.743 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 = 0.0184299 Jy ! Component: 100 - total flux cleaned = 0.0288453 Jy ! Component: 150 - total flux cleaned = 0.0354106 Jy ! Component: 200 - total flux cleaned = 0.0397373 Jy ! Total flux subtracted in 200 components = 0.0397373 Jy ! Clean residual min=-0.001959 max=0.002335 Jy/beam ! Clean residual mean=0.000046 rms=0.000545 Jy/beam ! Combined flux in latest and established models = 0.598639 Jy ! Adding 28 model components to the UV plane model. ! The established model now contains 39 components and 0.598639 Jy ! Inverting map ! Your choice of large map pixels excluded 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00289648 Jy ! Component: 100 - total flux cleaned = 0.00488755 Jy ! Component: 150 - total flux cleaned = 0.00629101 Jy ! Component: 200 - total flux cleaned = 0.00685153 Jy ! Total flux subtracted in 200 components = 0.00685153 Jy ! Clean residual min=-0.001910 max=0.002057 Jy/beam ! Clean residual mean=-0.000003 rms=0.000488 Jy/beam ! Combined flux in latest and established models = 0.605491 Jy ! Adding 28 model components to the UV plane model. ! The established model now contains 52 components and 0.605491 Jy ! Inverting map ! Your choice of large map pixels excluded 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 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 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 milli-arcsec ! Estimated beam: bmin=2.378 mas, bmaj=2.705 mas, bpa=-9.32 degrees ! Estimated noise=665.235 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000838774 Jy ! Component: 100 - total flux cleaned = 0.000874316 Jy ! Component: 150 - total flux cleaned = 0.000901752 Jy ! Component: 200 - total flux cleaned = 0.000922679 Jy ! Total flux subtracted in 200 components = 0.000922679 Jy ! Clean residual min=-0.002163 max=0.002193 Jy/beam ! Clean residual mean=-0.000033 rms=0.000650 Jy/beam ! Combined flux in latest and established models = 0.606413 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 = -8.6239e-06 Jy ! Component: 100 - total flux cleaned = -1.72036e-05 Jy ! Component: 150 - total flux cleaned = -1.69039e-05 Jy ! Component: 200 - total flux cleaned = -2.43584e-05 Jy ! Total flux subtracted in 200 components = -2.43584e-05 Jy ! Clean residual min=-0.002169 max=0.002194 Jy/beam ! Clean residual mean=-0.000033 rms=0.000649 Jy/beam ! Combined flux in latest and established models = 0.606389 Jy ! Adding 19 model components to the UV plane model. ! The established model now contains 68 components and 0.606389 Jy ! Inverting map ! Your choice of large map pixels excluded 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 milli-arcsec ! Estimated beam: bmin=0.6296 mas, bmaj=1.13 mas, bpa=7.005 degrees ! Estimated noise=452.743 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000184841 Jy ! Component: 100 - total flux cleaned = 0.000216504 Jy ! Component: 150 - total flux cleaned = 0.000306029 Jy ! Component: 200 - total flux cleaned = 0.000360613 Jy ! Total flux subtracted in 200 components = 0.000360613 Jy ! Clean residual min=-0.001895 max=0.002062 Jy/beam ! Clean residual mean=-0.000012 rms=0.000481 Jy/beam ! Combined flux in latest and established models = 0.60675 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 71 components and 0.60675 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.162679Jy sigma=0.001136 ! Fit after self-cal, rms=0.162670Jy sigma=0.001136 wmodel J1848+3219_X_2009_04_21_pus_map.mod ! Writing 71 model components to file: J1848+3219_X_2009_04_21_pus_map.mod wobs J1848+3219_X_2009_04_21_pus_uvs.fits ! Writing UV FITS file: J1848+3219_X_2009_04_21_pus_uvs.fits wwins J1848+3219_X_2009_04_21_pus_map.win ! wwins: Wrote 2 windows to J1848+3219_X_2009_04_21_pus_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! Your choice of large map pixels excluded 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000304407 Jy ! Component: 100 - total flux cleaned = 0.000270002 Jy ! Component: 150 - total flux cleaned = 0.000270408 Jy ! Component: 200 - total flux cleaned = 0.000206867 Jy ! Component: 250 - total flux cleaned = 2.03613e-05 Jy ! Component: 300 - total flux cleaned = -0.000101729 Jy ! Component: 350 - total flux cleaned = -0.000131539 Jy ! Component: 400 - total flux cleaned = -0.000160848 Jy ! Component: 450 - total flux cleaned = -0.000248086 Jy ! Component: 500 - total flux cleaned = -0.0003625 Jy ! Component: 550 - total flux cleaned = -0.000418649 Jy ! Component: 600 - total flux cleaned = -0.000474378 Jy ! Component: 650 - total flux cleaned = -0.00055724 Jy ! Component: 700 - total flux cleaned = -0.000612085 Jy ! Component: 750 - total flux cleaned = -0.000773989 Jy ! Component: 800 - total flux cleaned = -0.0007473 Jy ! Component: 850 - total flux cleaned = -0.00087941 Jy ! Component: 900 - total flux cleaned = -0.000879598 Jy ! Component: 950 - total flux cleaned = -0.00093152 Jy ! Component: 1000 - total flux cleaned = -0.000957243 Jy ! Component: 1050 - total flux cleaned = -0.000982804 Jy ! Component: 1100 - total flux cleaned = -0.00103332 Jy ! Component: 1150 - total flux cleaned = -0.00105814 Jy ! Component: 1200 - total flux cleaned = -0.00103337 Jy ! Component: 1250 - total flux cleaned = -0.00108268 Jy ! Component: 1300 - total flux cleaned = -0.00115575 Jy ! Component: 1350 - total flux cleaned = -0.00110734 Jy ! Component: 1400 - total flux cleaned = -0.00117956 Jy ! Component: 1450 - total flux cleaned = -0.00117963 Jy ! Component: 1500 - total flux cleaned = -0.00117968 Jy ! Component: 1550 - total flux cleaned = -0.00125037 Jy ! Component: 1600 - total flux cleaned = -0.00129721 Jy ! Component: 1650 - total flux cleaned = -0.00129703 Jy ! Component: 1700 - total flux cleaned = -0.00132017 Jy ! Component: 1750 - total flux cleaned = -0.00134307 Jy ! Component: 1800 - total flux cleaned = -0.00141143 Jy ! Component: 1850 - total flux cleaned = -0.00143398 Jy ! Component: 1900 - total flux cleaned = -0.00141149 Jy ! Component: 1950 - total flux cleaned = -0.00145624 Jy ! Component: 2000 - total flux cleaned = -0.00145639 Jy ! Total flux subtracted in 2048 components = -0.00154475 Jy ! Clean residual min=-0.001217 max=0.001200 Jy/beam ! Clean residual mean=-0.000000 rms=0.000391 Jy/beam ! Combined flux in latest and established models = 0.605205 Jy keep ! Adding 158 model components to the UV plane model. ! The established model now contains 229 components and 0.605205 Jy ![Exited script file: muppet] wmap "J1848+3219_X_2009_04_21_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6296 x 1.13 at 7.005 degrees (North through East) ! Clean map min=-0.001518 max=0.53075 Jy/beam ! Writing clean map to FITS file: J1848+3219_X_2009_04_21_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.530752 invert ! Inverting map ! Your choice of large map pixels excluded 6.38% of the data. ! The x-axis pixel size should ideally be below 0.1629 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000391407 device "J1848+3219_X_2009_04_21_pus\_map.eps/VPS" ! Attempting to open device: 'J1848+3219_X_2009_04_21_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.221237 0.221237 0.442474 0.884948 1.7699 3.53979 7.07958 14.1592 28.3183 56.6367 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0011 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.53 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6296 x 1.13 at 7.005 degrees (North through East) ! Clean map min=-0.001518 max=0.53075 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J1848+3219_X_2009_04_21_pus\_map.gif/vgif" ! Attempting to open device: 'J1848+3219_X_2009_04_21_pus_map.gif/vgif' mapplot cln