! Started logfile: J1608+1029_X_2001_03_12_pus_uvs.log on Wed Jan 2 19:59:33 2013 obs J1608+1029_X_2001_03_12_pus_uva.fits ! Reading UV FITS file: J1608+1029_X_2001_03_12_pus_uva.fits ! AN table 1: 10 integrations on 136 of 136 possible baselines. ! AN table 2: 66 integrations on 136 of 136 possible baselines. ! AN table 3: 14 integrations on 136 of 136 possible baselines. ! AN table 4: 74 integrations on 136 of 136 possible baselines. ! AN table 5: 32 integrations on 136 of 136 possible baselines. ! AN table 6: 108 integrations on 136 of 136 possible baselines. ! Apparent sampling: 0.173979 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1608+1029 ! ! 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 1753 lines of history. ! ! Reading 28772 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 J1608+1029_X_2001_03_12_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 170 telescope corrections were flagged in sub-array 1. ! A total of 785 telescope corrections were flagged in sub-array 2. ! A total of 119 telescope corrections were flagged in sub-array 3. ! A total of 927 telescope corrections were flagged in sub-array 4. ! A total of 367 telescope corrections were flagged in sub-array 5. ! A total of 984 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 170 telescope corrections were flagged in sub-array 1. ! A total of 786 telescope corrections were flagged in sub-array 2. ! A total of 119 telescope corrections were flagged in sub-array 3. ! A total of 927 telescope corrections were flagged in sub-array 4. ! A total of 367 telescope corrections were flagged in sub-array 5. ! A total of 984 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 170 telescope corrections were flagged in sub-array 1. ! A total of 786 telescope corrections were flagged in sub-array 2. ! A total of 119 telescope corrections were flagged in sub-array 3. ! A total of 927 telescope corrections were flagged in sub-array 4. ! A total of 367 telescope corrections were flagged in sub-array 5. ! A total of 984 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 170 telescope corrections were flagged in sub-array 1. ! A total of 787 telescope corrections were flagged in sub-array 2. ! A total of 119 telescope corrections were flagged in sub-array 3. ! A total of 927 telescope corrections were flagged in sub-array 4. ! A total of 367 telescope corrections were flagged in sub-array 5. ! A total of 984 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.255471Jy sigma=0.011411 ! Fit after self-cal, rms=0.828932Jy sigma=0.007450 ! 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 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec ! Estimated beam: bmin=0.5036 mas, bmaj=1.309 mas, bpa=-4.921 degrees ! Estimated noise=968.754 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 = 1.33096 Jy ! Component: 100 - total flux cleaned = 1.66065 Jy ! Total flux subtracted in 100 components = 1.66065 Jy ! Clean residual min=-0.032350 max=0.141627 Jy/beam ! Clean residual mean=-0.000172 rms=0.011040 Jy/beam ! Combined flux in latest and established models = 1.66065 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 1.66065 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.432711Jy sigma=0.003411 ! Fit after self-cal, rms=0.431970Jy sigma=0.003408 ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.159749 Jy ! Component: 100 - total flux cleaned = 0.248182 Jy ! Total flux subtracted in 100 components = 0.248182 Jy ! Clean residual min=-0.027577 max=0.062105 Jy/beam ! Clean residual mean=-0.000046 rms=0.007606 Jy/beam ! Combined flux in latest and established models = 1.90883 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 15 components and 1.90883 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.368110Jy sigma=0.002426 ! Fit after self-cal, rms=0.367441Jy sigma=0.002423 ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec ! Added new window around map position (-0.8, 0.6). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0655532 Jy ! Component: 100 - total flux cleaned = 0.108573 Jy ! Total flux subtracted in 100 components = 0.108573 Jy ! Clean residual min=-0.028327 max=0.050161 Jy/beam ! Clean residual mean=0.000006 rms=0.006782 Jy/beam ! Combined flux in latest and established models = 2.01741 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 27 components and 2.01741 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.354093Jy sigma=0.002161 ! Fit after self-cal, rms=0.352419Jy sigma=0.002148 ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec ! Added new window around map position (-1.6, 0.8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0451853 Jy ! Component: 100 - total flux cleaned = 0.0736383 Jy ! Total flux subtracted in 100 components = 0.0736383 Jy ! Clean residual min=-0.029799 max=0.036380 Jy/beam ! Clean residual mean=0.000040 rms=0.006308 Jy/beam ! Combined flux in latest and established models = 2.09105 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 35 components and 2.09105 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.347680Jy sigma=0.002035 ! Fit after self-cal, rms=0.346903Jy sigma=0.002027 ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 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 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec ! Estimated beam: bmin=0.5685 mas, bmaj=1.596 mas, bpa=-7.23 degrees ! Estimated noise=571.252 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 = 0.0431028 Jy ! Component: 100 - total flux cleaned = 0.0654056 Jy ! Component: 150 - total flux cleaned = 0.071752 Jy ! Component: 200 - total flux cleaned = 0.0717339 Jy ! Total flux subtracted in 200 components = 0.0717339 Jy ! Clean residual min=-0.028645 max=0.030109 Jy/beam ! Clean residual mean=-0.000076 rms=0.007488 Jy/beam ! Combined flux in latest and established models = 2.16278 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 41 components and 2.16278 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.345357Jy sigma=0.001943 ! Fit after self-cal, rms=0.344848Jy sigma=0.001937 ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 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 0.00* FD 0.00* HH 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MC 0.00* MK 0.00* NL 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TS 0.00* ! WZ 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* HH 1.05 HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MA 1.05 ! MC 1.15 MK 1.00* NL 1.00* ON 1.23 ! OV 1.00* PT 1.00* SC 1.00* TS 0.98 ! WZ 1.17 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 1.06 HH 1.00* HN 1.00* ! KK 0.91 KP 1.07 LA 1.06 MA 1.00* ! MC 1.00* MK 0.95 NL 1.25 ON 1.00* ! OV 0.98 PT 1.00 SC 1.00* TS 0.89 ! WZ 1.00* ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 FD 0.97 HH 1.00* HN 1.02 ! KK 0.93 KP 0.95 LA 0.95 MA 1.00* ! MC 1.00* MK 0.97 NL 0.99 ON 1.00* ! OV 0.93 PT 0.95 SC 1.19 TS 0.98 ! WZ 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.97 FD 0.96 HH 1.00* HN 1.92 ! KK 0.95 KP 0.98 LA 0.94 MA 1.00* ! MC 1.00* MK 0.94 NL 0.96 ON 1.00* ! OV 0.95 PT 0.96 SC 1.01 TS 1.00* ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.98 FD 0.98 HH 1.08 HN 1.07 ! KK 1.00* KP 1.02 LA 0.97 MA 0.97 ! MC 1.06 MK 1.00 NL 0.97 ON 1.15 ! OV 0.96 PT 0.96 SC 0.97 TS 1.00* ! WZ 1.03 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* HH 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MC 0.00* MK 0.00* NL 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TS 0.00* ! WZ 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* HH 1.04 HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MA 1.02 ! MC 1.18 MK 1.00* NL 1.00* ON 1.16 ! OV 1.00* PT 1.00* SC 1.00* TS 0.99 ! WZ 1.19 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.05 HH 1.00* HN 1.00* ! KK 0.92 KP 1.01 LA 1.04 MA 1.00* ! MC 1.00* MK 0.95 NL 1.20 ON 1.00* ! OV 0.99 PT 1.05 SC 1.00* TS 0.89 ! WZ 1.00* ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 FD 0.97 HH 1.00* HN 1.02 ! KK 0.92 KP 0.90 LA 0.94 MA 1.00* ! MC 1.00* MK 0.96 NL 0.95 ON 1.00* ! OV 0.93 PT 0.98 SC 1.17 TS 0.98 ! WZ 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.98 FD 0.95 HH 1.00* HN 1.93 ! KK 0.93 KP 0.92 LA 0.93 MA 1.00* ! MC 1.00* MK 0.94 NL 0.92 ON 1.00* ! OV 0.95 PT 0.99 SC 1.00 TS 1.00* ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.99 FD 0.97 HH 1.08 HN 1.04 ! KK 1.00* KP 0.96 LA 0.96 MA 0.98 ! MC 1.07 MK 1.01 NL 0.94 ON 1.15 ! OV 0.96 PT 0.99 SC 0.95 TS 1.00* ! WZ 1.04 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* HH 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MC 0.00* MK 0.00* NL 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TS 0.00* ! WZ 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* HH 1.06 HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MA 1.11 ! MC 1.26 MK 1.00* NL 1.00* ON 1.24 ! OV 1.00* PT 1.00* SC 1.00* TS 0.98 ! WZ 1.19 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.03 HH 1.00* HN 1.00* ! KK 0.98 KP 0.99 LA 1.07 MA 1.00* ! MC 1.00* MK 0.97 NL 1.22 ON 1.00* ! OV 1.02 PT 1.07 SC 1.00* TS 0.86 ! WZ 1.00* ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 0.95 HH 1.00* HN 1.04 ! KK 0.99 KP 0.88 LA 0.96 MA 1.00* ! MC 1.00* MK 0.99 NL 0.99 ON 1.00* ! OV 0.96 PT 1.01 SC 1.22 TS 0.96 ! WZ 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 FD 0.92 HH 1.00* HN 2.09 ! KK 1.00 KP 0.91 LA 0.95 MA 1.00* ! MC 1.00* MK 0.96 NL 0.97 ON 1.00* ! OV 0.98 PT 1.01 SC 1.01 TS 1.00* ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.02 FD 0.96 HH 1.12 HN 1.05 ! KK 1.00* KP 0.94 LA 0.98 MA 1.03 ! MC 1.14 MK 1.02 NL 0.98 ON 1.21 ! OV 0.99 PT 1.02 SC 0.98 TS 1.00* ! WZ 1.06 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* HH 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MC 0.00* MK 0.00* NL 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TS 0.00* ! WZ 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* HH 1.03 HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MA 1.15 ! MC 1.19 MK 1.00* NL 1.00* ON 1.27 ! OV 1.00* PT 1.00* SC 1.00* TS 0.99 ! WZ 1.21 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.01 HH 1.00* HN 1.00* ! KK 0.95 KP 1.00 LA 1.05 MA 1.00* ! MC 1.00* MK 1.00 NL 1.24 ON 1.00* ! OV 1.00 PT 1.07 SC 1.00* TS 0.87 ! WZ 1.00* ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 FD 0.94 HH 1.00* HN 1.03 ! KK 0.96 KP 0.90 LA 0.94 MA 1.00* ! MC 1.00* MK 1.01 NL 1.01 ON 1.00* ! OV 0.95 PT 1.00 SC 1.30 TS 0.95 ! WZ 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 FD 0.92 HH 1.00* HN 2.16 ! KK 0.95 KP 0.93 LA 0.92 MA 1.00* ! MC 1.00* MK 0.98 NL 0.97 ON 1.00* ! OV 0.97 PT 1.01 SC 1.07 TS 1.00* ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00 FD 0.95 HH 1.08 HN 1.08 ! KK 1.00* KP 0.96 LA 0.96 MA 1.09 ! MC 1.09 MK 1.06 NL 0.99 ON 1.22 ! OV 0.98 PT 1.02 SC 1.03 TS 1.00* ! WZ 1.06 ! ! ! Fit before self-cal, rms=0.344848Jy sigma=0.001937 ! Fit after self-cal, rms=0.295496Jy sigma=0.001300 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec ! Estimated beam: bmin=0.5752 mas, bmaj=1.654 mas, bpa=-7.244 degrees ! Estimated noise=576.574 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 = -0.00451834 Jy ! Component: 100 - total flux cleaned = -0.00548508 Jy ! Component: 150 - total flux cleaned = -0.00657826 Jy ! Component: 200 - total flux cleaned = -0.00658549 Jy ! Total flux subtracted in 200 components = -0.00658549 Jy ! Clean residual min=-0.009406 max=0.008815 Jy/beam ! Clean residual mean=-0.000059 rms=0.002319 Jy/beam ! Combined flux in latest and established models = 2.15619 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 47 components and 2.15619 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.294098Jy sigma=0.001284 ! Fit after self-cal, rms=0.294337Jy sigma=0.001283 ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 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=0.294337Jy sigma=0.001283 ! Fit after self-cal, rms=0.280864Jy sigma=0.001225 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec ! Estimated beam: bmin=0.5777 mas, bmaj=1.65 mas, bpa=-7.215 degrees ! Estimated noise=577.378 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00757437 Jy ! Component: 100 - total flux cleaned = -0.007902 Jy ! Component: 150 - total flux cleaned = -0.00760747 Jy ! Component: 200 - total flux cleaned = -0.00736693 Jy ! Total flux subtracted in 200 components = -0.00736693 Jy ! Clean residual min=-0.006913 max=0.005607 Jy/beam ! Clean residual mean=-0.000034 rms=0.001275 Jy/beam ! Combined flux in latest and established models = 2.14883 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 49 components and 2.14883 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.279706Jy sigma=0.001215 ! Fit after self-cal, rms=0.279762Jy sigma=0.001215 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 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 = 0.00026453 Jy ! Component: 100 - total flux cleaned = 0.0004843 Jy ! Component: 150 - total flux cleaned = 0.000675779 Jy ! Component: 200 - total flux cleaned = 0.00083709 Jy ! Total flux subtracted in 200 components = 0.00083709 Jy ! Clean residual min=-0.005308 max=0.004840 Jy/beam ! Clean residual mean=-0.000034 rms=0.001215 Jy/beam ! Combined flux in latest and established models = 2.14966 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 51 components and 2.14966 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.279378Jy sigma=0.001212 ! Fit after self-cal, rms=0.279356Jy sigma=0.001211 ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 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=0.279356Jy sigma=0.001211 ! Fit after self-cal, rms=0.279736Jy sigma=0.001208 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec ! Estimated beam: bmin=0.5792 mas, bmaj=1.65 mas, bpa=-7.229 degrees ! Estimated noise=577.334 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00374426 Jy ! Component: 100 - total flux cleaned = -0.0037546 Jy ! Component: 150 - total flux cleaned = -0.00357495 Jy ! Component: 200 - total flux cleaned = -0.00342671 Jy ! Total flux subtracted in 200 components = -0.00342671 Jy ! Clean residual min=-0.004879 max=0.004876 Jy/beam ! Clean residual mean=-0.000024 rms=0.001032 Jy/beam ! Combined flux in latest and established models = 2.14624 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 53 components and 2.14624 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.279323Jy sigma=0.001204 ! Fit after self-cal, rms=0.279287Jy sigma=0.001204 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 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 = 8.50486e-05 Jy ! Component: 100 - total flux cleaned = 0.000221409 Jy ! Component: 150 - total flux cleaned = 0.000343035 Jy ! Component: 200 - total flux cleaned = 0.000343548 Jy ! Total flux subtracted in 200 components = 0.000343548 Jy ! Clean residual min=-0.004371 max=0.004659 Jy/beam ! Clean residual mean=-0.000024 rms=0.001002 Jy/beam ! Combined flux in latest and established models = 2.14658 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 54 components and 2.14658 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.279116Jy sigma=0.001203 ! Fit after self-cal, rms=0.279110Jy sigma=0.001203 ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec ! Added new window around map position (-5.4, 5.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00411594 Jy ! Component: 100 - total flux cleaned = 0.00586152 Jy ! Component: 150 - total flux cleaned = 0.00659992 Jy ! Component: 200 - total flux cleaned = 0.00707656 Jy ! Total flux subtracted in 200 components = 0.00707656 Jy ! Clean residual min=-0.004330 max=0.003818 Jy/beam ! Clean residual mean=-0.000019 rms=0.000928 Jy/beam ! Combined flux in latest and established models = 2.15366 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 66 components and 2.15366 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.279009Jy sigma=0.001201 ! Fit after self-cal, rms=0.278990Jy sigma=0.001201 ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 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=0.278990Jy sigma=0.001201 ! Fit after self-cal, rms=0.279646Jy sigma=0.001200 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec ! Estimated beam: bmin=2.353 mas, bmaj=3.348 mas, bpa=-14.29 degrees ! Estimated noise=781.175 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00227399 Jy ! Component: 100 - total flux cleaned = 0.00371261 Jy ! Component: 150 - total flux cleaned = 0.00477609 Jy ! Component: 200 - total flux cleaned = 0.00551664 Jy ! Total flux subtracted in 200 components = 0.00551664 Jy ! Clean residual min=-0.004693 max=0.004344 Jy/beam ! Clean residual mean=-0.000024 rms=0.001172 Jy/beam ! Combined flux in latest and established models = 2.15917 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 85 components and 2.15917 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.279586Jy sigma=0.001199 ! Fit after self-cal, rms=0.279556Jy sigma=0.001199 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 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 = 0.000334947 Jy ! Component: 100 - total flux cleaned = 0.000820385 Jy ! Component: 150 - total flux cleaned = 0.00112911 Jy ! Component: 200 - total flux cleaned = 0.00136426 Jy ! Total flux subtracted in 200 components = 0.00136426 Jy ! Clean residual min=-0.004698 max=0.004052 Jy/beam ! Clean residual mean=-0.000022 rms=0.001147 Jy/beam ! Combined flux in latest and established models = 2.16054 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 91 components and 2.16054 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.279558Jy sigma=0.001199 ! Fit after self-cal, rms=0.279553Jy sigma=0.001199 ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 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 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec ! Estimated beam: bmin=0.5802 mas, bmaj=1.65 mas, bpa=-7.245 degrees ! Estimated noise=577.41 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5802 x 1.65 at -7.245 degrees (North through East) ! Clean map min=-0.0033329 max=1.7417 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=0.279553Jy sigma=0.001199 ! Fit after self-cal, rms=0.258633Jy sigma=0.001083 ! Inverting map and beam ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec ! Estimated beam: bmin=0.5802 mas, bmaj=1.65 mas, bpa=-7.257 degrees ! Estimated noise=576.569 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00189965 Jy ! Component: 100 - total flux cleaned = -0.00221372 Jy ! Component: 150 - total flux cleaned = -0.00212628 Jy ! Component: 200 - total flux cleaned = -0.00197509 Jy ! Total flux subtracted in 200 components = -0.00197509 Jy ! Clean residual min=-0.003525 max=0.003116 Jy/beam ! Clean residual mean=-0.000008 rms=0.000763 Jy/beam ! Combined flux in latest and established models = 2.15856 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 94 components and 2.15856 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.258525Jy sigma=0.001082 ! Fit after self-cal, rms=0.258528Jy sigma=0.001082 ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00011628 Jy ! Component: 100 - total flux cleaned = 3.10584e-05 Jy ! Component: 150 - total flux cleaned = 0.000230778 Jy ! Component: 200 - total flux cleaned = 0.000355594 Jy ! Total flux subtracted in 200 components = 0.000355594 Jy ! Clean residual min=-0.003442 max=0.003144 Jy/beam ! Clean residual mean=-0.000008 rms=0.000753 Jy/beam ! Combined flux in latest and established models = 2.15892 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 97 components and 2.15892 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.258475Jy sigma=0.001081 ! Fit after self-cal, rms=0.258473Jy sigma=0.001081 ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.258473Jy sigma=0.001081 ! Fit after self-cal, rms=0.258669Jy sigma=0.001081 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 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec ! Estimated beam: bmin=0.5097 mas, bmaj=1.343 mas, bpa=-4.884 degrees ! Estimated noise=969.302 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.33936 Jy ! Component: 100 - total flux cleaned = 1.66664 Jy ! Component: 150 - total flux cleaned = 1.81944 Jy ! Component: 200 - total flux cleaned = 1.91017 Jy ! Total flux subtracted in 200 components = 1.91017 Jy ! Clean residual min=-0.011799 max=0.048029 Jy/beam ! Clean residual mean=-0.000113 rms=0.003736 Jy/beam ! Combined flux in latest and established models = 1.91017 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 15 model components to the UV plane model. ! The established model now contains 15 components and 1.91017 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec ! Estimated beam: bmin=0.5806 mas, bmaj=1.65 mas, bpa=-7.267 degrees ! Estimated noise=576.461 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 = 0.0924961 Jy ! Component: 100 - total flux cleaned = 0.143965 Jy ! Component: 150 - total flux cleaned = 0.17549 Jy ! Component: 200 - total flux cleaned = 0.195659 Jy ! Total flux subtracted in 200 components = 0.195659 Jy ! Clean residual min=-0.005228 max=0.011450 Jy/beam ! Clean residual mean=-0.000070 rms=0.001549 Jy/beam ! Combined flux in latest and established models = 2.10582 Jy ! Adding 33 model components to the UV plane model. ! The established model now contains 42 components and 2.10582 Jy ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec ! Added new window around map position (-0.2, 1.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0135903 Jy ! Component: 100 - total flux cleaned = 0.0227677 Jy ! Component: 150 - total flux cleaned = 0.0296189 Jy ! Component: 200 - total flux cleaned = 0.0349417 Jy ! Total flux subtracted in 200 components = 0.0349417 Jy ! Clean residual min=-0.003969 max=0.005575 Jy/beam ! Clean residual mean=-0.000025 rms=0.000920 Jy/beam ! Combined flux in latest and established models = 2.14077 Jy ! Adding 25 model components to the UV plane model. ! The established model now contains 58 components and 2.14077 Jy ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec ! Added new window around map position (-2.4, 2.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00560727 Jy ! Component: 100 - total flux cleaned = 0.00952551 Jy ! Component: 150 - total flux cleaned = 0.0122646 Jy ! Component: 200 - total flux cleaned = 0.0141493 Jy ! Total flux subtracted in 200 components = 0.0141493 Jy ! Clean residual min=-0.003524 max=0.003191 Jy/beam ! Clean residual mean=-0.000011 rms=0.000779 Jy/beam ! Combined flux in latest and established models = 2.15492 Jy ! Adding 25 model components to the UV plane model. ! The established model now contains 74 components and 2.15492 Jy ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 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 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec ! Estimated beam: bmin=2.352 mas, bmaj=3.348 mas, bpa=-14.3 degrees ! Estimated noise=779.652 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0030906 Jy ! Component: 100 - total flux cleaned = 0.00504354 Jy ! Component: 150 - total flux cleaned = 0.00641889 Jy ! Component: 200 - total flux cleaned = 0.00739931 Jy ! Total flux subtracted in 200 components = 0.00739931 Jy ! Clean residual min=-0.003573 max=0.003448 Jy/beam ! Clean residual mean=-0.000009 rms=0.000974 Jy/beam ! Combined flux in latest and established models = 2.16231 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 = 0.000446349 Jy ! Component: 100 - total flux cleaned = 0.000641072 Jy ! Component: 150 - total flux cleaned = 0.000769663 Jy ! Component: 200 - total flux cleaned = 0.000866774 Jy ! Total flux subtracted in 200 components = 0.000866774 Jy ! Clean residual min=-0.003570 max=0.003433 Jy/beam ! Clean residual mean=-0.000007 rms=0.000969 Jy/beam ! Combined flux in latest and established models = 2.16318 Jy ! Adding 54 model components to the UV plane model. ! The established model now contains 124 components and 2.16318 Jy ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec ! Estimated beam: bmin=0.5806 mas, bmaj=1.65 mas, bpa=-7.267 degrees ! Estimated noise=576.461 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000292473 Jy ! Component: 100 - total flux cleaned = -0.00037844 Jy ! Component: 150 - total flux cleaned = -0.000380713 Jy ! Component: 200 - total flux cleaned = -0.000452095 Jy ! Total flux subtracted in 200 components = -0.000452095 Jy ! Clean residual min=-0.003427 max=0.002938 Jy/beam ! Clean residual mean=-0.000004 rms=0.000735 Jy/beam ! Combined flux in latest and established models = 2.16273 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 131 components and 2.16273 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.259121Jy sigma=0.001085 ! Fit after self-cal, rms=0.258977Jy sigma=0.001084 wmodel J1608+1029_X_2001_03_12_pus_map.mod ! Writing 131 model components to file: J1608+1029_X_2001_03_12_pus_map.mod wobs J1608+1029_X_2001_03_12_pus_uvs.fits ! Writing UV FITS file: J1608+1029_X_2001_03_12_pus_uvs.fits wwins J1608+1029_X_2001_03_12_pus_map.win ! wwins: Wrote 6 windows to J1608+1029_X_2001_03_12_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 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00106187 Jy ! Component: 100 - total flux cleaned = -0.00170828 Jy ! Component: 150 - total flux cleaned = -0.00221937 Jy ! Component: 200 - total flux cleaned = -0.00266379 Jy ! Component: 250 - total flux cleaned = -0.00295085 Jy ! Component: 300 - total flux cleaned = -0.00309065 Jy ! Component: 350 - total flux cleaned = -0.00318209 Jy ! Component: 400 - total flux cleaned = -0.00331662 Jy ! Component: 450 - total flux cleaned = -0.00344914 Jy ! Component: 500 - total flux cleaned = -0.00340636 Jy ! Component: 550 - total flux cleaned = -0.00349276 Jy ! Component: 600 - total flux cleaned = -0.00340808 Jy ! Component: 650 - total flux cleaned = -0.00336653 Jy ! Component: 700 - total flux cleaned = -0.00328362 Jy ! Component: 750 - total flux cleaned = -0.00328325 Jy ! Component: 800 - total flux cleaned = -0.00320284 Jy ! Component: 850 - total flux cleaned = -0.00320317 Jy ! Component: 900 - total flux cleaned = -0.00308613 Jy ! Component: 950 - total flux cleaned = -0.0031253 Jy ! Component: 1000 - total flux cleaned = -0.00301091 Jy ! Component: 1050 - total flux cleaned = -0.00312472 Jy ! Component: 1100 - total flux cleaned = -0.00312455 Jy ! Component: 1150 - total flux cleaned = -0.00308693 Jy ! Component: 1200 - total flux cleaned = -0.00293934 Jy ! Component: 1250 - total flux cleaned = -0.00293973 Jy ! Component: 1300 - total flux cleaned = -0.00294006 Jy ! Component: 1350 - total flux cleaned = -0.00283257 Jy ! Component: 1400 - total flux cleaned = -0.00279739 Jy ! Component: 1450 - total flux cleaned = -0.00272703 Jy ! Component: 1500 - total flux cleaned = -0.0027966 Jy ! Component: 1550 - total flux cleaned = -0.00276164 Jy ! Component: 1600 - total flux cleaned = -0.002727 Jy ! Component: 1650 - total flux cleaned = -0.0026588 Jy ! Component: 1700 - total flux cleaned = -0.00262492 Jy ! Component: 1750 - total flux cleaned = -0.00259092 Jy ! Component: 1800 - total flux cleaned = -0.00262472 Jy ! Component: 1850 - total flux cleaned = -0.00252436 Jy ! Component: 1900 - total flux cleaned = -0.00249111 Jy ! Component: 1950 - total flux cleaned = -0.00232664 Jy ! Component: 2000 - total flux cleaned = -0.00242462 Jy ! Total flux subtracted in 2048 components = -0.00242465 Jy ! Clean residual min=-0.001795 max=0.001837 Jy/beam ! Clean residual mean=-0.000002 rms=0.000575 Jy/beam ! Combined flux in latest and established models = 2.1603 Jy keep ! Adding 149 model components to the UV plane model. ! The established model now contains 280 components and 2.16031 Jy ![Exited script file: muppet] wmap "J1608+1029_X_2001_03_12_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5806 x 1.65 at -7.267 degrees (North through East) ! Clean map min=-0.0025773 max=1.7457 Jy/beam ! Writing clean map to FITS file: J1608+1029_X_2001_03_12_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 1.74574 invert ! Inverting map ! Your choice of large map pixels excluded 5.09% of the data. ! The x-axis pixel size should ideally be below 0.1561 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000574221 device "J1608+1029_X_2001_03_12_pus\_map.eps/VPS" ! Attempting to open device: 'J1608+1029_X_2001_03_12_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.0986782 0.0986782 0.197356 0.394713 0.789425 1.57885 3.1577 6.3154 12.6308 25.2616 50.5232 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0017 print "peak=",int(1000*peak_flux)/1000 ! peak= 1.745 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5806 x 1.65 at -7.267 degrees (North through East) ! Clean map min=-0.0025773 max=1.7457 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. quit ! Quitting program ! Log file J1608+1029_X_2001_03_12_pus_uvs.log closed on Wed Jan 2 19:59:43 2013