! Started logfile: J0530+1331_X_2003_07_09_pus_uvs.log on Sun Apr 7 11:50:19 2013 obs J0530+1331_X_2003_07_09_pus_uva.fits ! Reading UV FITS file: J0530+1331_X_2003_07_09_pus_uva.fits ! AN table 1: 147 integrations on 171 of 171 possible baselines. ! AN table 2: 214 integrations on 171 of 171 possible baselines. ! AN table 3: 28 integrations on 171 of 171 possible baselines. ! AN table 4: 165 integrations on 171 of 171 possible baselines. ! AN table 5: 52 integrations on 171 of 171 possible baselines. ! AN table 6: 32 integrations on 171 of 171 possible baselines. ! Apparent sampling: 0.0840162 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0530+1331 ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! ! 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 1874 lines of history. ! ! Reading 36664 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 J0530+1331_X_2003_07_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 = 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 1904 telescope corrections were flagged in sub-array 1. ! A total of 3077 telescope corrections were flagged in sub-array 2. ! A total of 532 telescope corrections were flagged in sub-array 3. ! A total of 2611 telescope corrections were flagged in sub-array 4. ! A total of 895 telescope corrections were flagged in sub-array 5. ! A total of 575 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 1904 telescope corrections were flagged in sub-array 1. ! A total of 3077 telescope corrections were flagged in sub-array 2. ! A total of 532 telescope corrections were flagged in sub-array 3. ! A total of 2611 telescope corrections were flagged in sub-array 4. ! A total of 895 telescope corrections were flagged in sub-array 5. ! A total of 578 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 1904 telescope corrections were flagged in sub-array 1. ! A total of 3077 telescope corrections were flagged in sub-array 2. ! A total of 532 telescope corrections were flagged in sub-array 3. ! A total of 2611 telescope corrections were flagged in sub-array 4. ! A total of 895 telescope corrections were flagged in sub-array 5. ! A total of 578 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 1906 telescope corrections were flagged in sub-array 1. ! A total of 3077 telescope corrections were flagged in sub-array 2. ! A total of 532 telescope corrections were flagged in sub-array 3. ! A total of 2611 telescope corrections were flagged in sub-array 4. ! A total of 892 telescope corrections were flagged in sub-array 5. ! A total of 578 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.965951Jy sigma=0.015793 ! Fit after self-cal, rms=1.499154Jy sigma=0.012091 ! 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 1.37% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! Estimated beam: bmin=0.5532 mas, bmaj=1.446 mas, bpa=-5.179 degrees ! Estimated noise=1000.59 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 = 1.86181 Jy ! Component: 100 - total flux cleaned = 2.34826 Jy ! Total flux subtracted in 100 components = 2.34826 Jy ! Clean residual min=-0.067541 max=0.212197 Jy/beam ! Clean residual mean=0.000400 rms=0.016292 Jy/beam ! Combined flux in latest and established models = 2.34826 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 2.34826 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.480150Jy sigma=0.003729 ! Fit after self-cal, rms=0.479989Jy sigma=0.003729 ! Inverting map ! Your choice of large map pixels excluded 1.37% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.231972 Jy ! Component: 100 - total flux cleaned = 0.360412 Jy ! Total flux subtracted in 100 components = 0.360412 Jy ! Clean residual min=-0.051594 max=0.066106 Jy/beam ! Clean residual mean=0.000388 rms=0.011039 Jy/beam ! Combined flux in latest and established models = 2.70867 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 19 components and 2.70868 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.368185Jy sigma=0.002656 ! Fit after self-cal, rms=0.367998Jy sigma=0.002656 ! Inverting map ! Your choice of large map pixels excluded 1.37% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0805738 Jy ! Component: 100 - total flux cleaned = 0.132558 Jy ! Total flux subtracted in 100 components = 0.132558 Jy ! Clean residual min=-0.054316 max=0.050812 Jy/beam ! Clean residual mean=0.000380 rms=0.010183 Jy/beam ! Combined flux in latest and established models = 2.84123 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 27 components and 2.84123 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.359738Jy sigma=0.002580 ! Fit after self-cal, rms=0.359626Jy sigma=0.002579 ! Inverting map ! Your choice of large map pixels excluded 1.37% of the data. ! The x-axis pixel size should ideally be below 0.156 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 1.37% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! Estimated beam: bmin=0.6541 mas, bmaj=1.82 mas, bpa=-9.712 degrees ! Estimated noise=532.658 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (1.2, 1.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0647246 Jy ! Component: 100 - total flux cleaned = 0.0686462 Jy ! Component: 150 - total flux cleaned = 0.0716816 Jy ! Component: 200 - total flux cleaned = 0.072531 Jy ! Total flux subtracted in 200 components = 0.072531 Jy ! Clean residual min=-0.066659 max=0.039895 Jy/beam ! Clean residual mean=0.001879 rms=0.011140 Jy/beam ! Combined flux in latest and established models = 2.91376 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 53 components and 2.91376 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.348819Jy sigma=0.002468 ! Fit after self-cal, rms=0.347344Jy sigma=0.002459 ! Inverting map ! Your choice of large map pixels excluded 1.37% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 36 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.97 GC 1.01 GG 1.00* ! HN 0.96 KP 1.02 LA 0.98 MA 1.10 ! MK 0.90 NL 0.91 NY 1.06 ON 1.00 ! OV 0.92 PT 0.98 SC 0.95 TC 1.00* ! TS 0.97 WF 1.02 WZ 1.01 ! ! A total of 42 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.06 FD 0.90 GC 1.00* GG 1.00* ! HN 0.99 KP 1.10 LA 1.02 MA 1.14 ! MK 1.00* NL 0.95 NY 0.99 ON 0.99 ! OV 1.13 PT 1.04 SC 1.05 TC 1.00* ! TS 1.00* WF 0.99 WZ 1.02 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 159 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.96 FD 0.95 GC 0.94 GG 1.00* ! HN 0.95 KP 0.90 LA 0.95 MA 1.02 ! MK 0.87 NL 1.03 NY 1.10 ON 0.99 ! OV 0.95 PT 0.93 SC 1.00* TC 1.00* ! TS 1.25 WF 1.06 WZ 1.03 ! ! A total of 93 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 33 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! ! Correcting IF 2. ! A total of 36 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.97 GC 1.07 GG 1.00* ! HN 0.97 KP 1.02 LA 0.97 MA 1.07 ! MK 0.92 NL 0.92 NY 1.11 ON 1.01 ! OV 0.91 PT 1.02 SC 0.98 TC 1.00* ! TS 0.99 WF 1.03 WZ 1.04 ! ! A total of 42 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.07 FD 0.89 GC 1.00* GG 1.00* ! HN 0.99 KP 1.09 LA 1.02 MA 1.10 ! MK 1.00* NL 0.95 NY 1.03 ON 1.00 ! OV 1.12 PT 1.08 SC 1.00 TC 1.00* ! TS 1.00* WF 1.01 WZ 1.05 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 159 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 FD 0.95 GC 0.99 GG 1.00* ! HN 0.96 KP 0.86 LA 0.94 MA 1.00 ! MK 0.90 NL 1.01 NY 1.15 ON 1.00 ! OV 0.95 PT 0.97 SC 1.00* TC 1.00* ! TS 1.29 WF 1.08 WZ 1.04 ! ! A total of 93 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 30 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! ! Correcting IF 3. ! A total of 36 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 0.97 GC 1.00 GG 1.00* ! HN 0.96 KP 1.02 LA 0.99 MA 1.10 ! MK 0.92 NL 0.95 NY 1.16 ON 0.99 ! OV 0.95 PT 0.99 SC 0.95 TC 1.00* ! TS 1.01 WF 0.97 WZ 1.00 ! ! A total of 42 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.10 FD 0.90 GC 1.00* GG 1.00* ! HN 0.98 KP 1.10 LA 1.03 MA 1.17 ! MK 1.00* NL 0.98 NY 1.07 ON 1.04 ! OV 1.16 PT 1.05 SC 1.03 TC 1.00* ! TS 1.00* WF 0.97 WZ 1.07 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 159 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 FD 0.95 GC 1.02 GG 1.00* ! HN 0.95 KP 0.80 LA 0.95 MA 0.98 ! MK 0.89 NL 1.01 NY 1.20 ON 1.03 ! OV 0.98 PT 0.99 SC 1.00* TC 1.00* ! TS 1.32 WF 1.20 WZ 1.01 ! ! A total of 93 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 30 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! ! Correcting IF 4. ! A total of 42 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.95 GC 1.00 GG 1.00* ! HN 0.99 KP 1.02 LA 0.97 MA 1.06 ! MK 0.96 NL 0.92 NY 1.14 ON 0.89 ! OV 0.94 PT 0.99 SC 1.00 TC 1.00* ! TS 0.98 WF 1.01 WZ 0.98 ! ! A total of 42 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.06 FD 0.89 GC 1.00* GG 1.00* ! HN 1.01 KP 1.10 LA 1.01 MA 1.22 ! MK 1.00* NL 0.95 NY 1.06 ON 1.11 ! OV 1.15 PT 1.06 SC 1.09 TC 1.00* ! TS 1.00* WF 0.97 WZ 1.08 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 159 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 FD 0.93 GC 1.05 GG 1.00* ! HN 0.97 KP 0.85 LA 0.94 MA 0.99 ! MK 0.94 NL 1.00 NY 1.18 ON 1.15 ! OV 0.98 PT 1.00 SC 1.00* TC 1.00* ! TS 1.32 WF 1.17 WZ 0.98 ! ! A total of 96 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! A total of 30 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! ! Fit before self-cal, rms=0.347344Jy sigma=0.002459 ! Fit after self-cal, rms=0.265286Jy sigma=0.001632 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! Estimated beam: bmin=0.6579 mas, bmaj=1.853 mas, bpa=-9.233 degrees ! Estimated noise=539.518 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 = 0.0248299 Jy ! Component: 100 - total flux cleaned = 0.0296762 Jy ! Component: 150 - total flux cleaned = 0.0310391 Jy ! Component: 200 - total flux cleaned = 0.0314181 Jy ! Total flux subtracted in 200 components = 0.0314181 Jy ! Clean residual min=-0.021793 max=0.019391 Jy/beam ! Clean residual mean=0.000808 rms=0.004959 Jy/beam ! Combined flux in latest and established models = 2.94518 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 72 components and 2.94518 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.262928Jy sigma=0.001605 ! Fit after self-cal, rms=0.262735Jy sigma=0.001603 ! Inverting map ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 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=0.262735Jy sigma=0.001603 ! Fit after self-cal, rms=0.235830Jy sigma=0.001343 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! Estimated beam: bmin=0.6586 mas, bmaj=1.853 mas, bpa=-9.255 degrees ! Estimated noise=539.387 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00901918 Jy ! Component: 100 - total flux cleaned = 0.0129455 Jy ! Component: 150 - total flux cleaned = 0.0151971 Jy ! Component: 200 - total flux cleaned = 0.0165624 Jy ! Total flux subtracted in 200 components = 0.0165624 Jy ! Clean residual min=-0.007056 max=0.010168 Jy/beam ! Clean residual mean=0.000657 rms=0.002010 Jy/beam ! Combined flux in latest and established models = 2.96175 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 82 components and 2.96174 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.234557Jy sigma=0.001332 ! Fit after self-cal, rms=0.234430Jy sigma=0.001331 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 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 (1.8, 5.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00925426 Jy ! Component: 100 - total flux cleaned = 0.0126908 Jy ! Component: 150 - total flux cleaned = 0.0148951 Jy ! Component: 200 - total flux cleaned = 0.0168085 Jy ! Total flux subtracted in 200 components = 0.0168085 Jy ! Clean residual min=-0.007038 max=0.007315 Jy/beam ! Clean residual mean=0.000543 rms=0.001777 Jy/beam ! Combined flux in latest and established models = 2.97855 Jy ! Performing phase self-cal ! Adding 33 model components to the UV plane model. ! The established model now contains 102 components and 2.97855 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.233734Jy sigma=0.001325 ! Fit after self-cal, rms=0.233674Jy sigma=0.001324 ! Inverting map ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 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=0.233674Jy sigma=0.001324 ! Fit after self-cal, rms=0.231256Jy sigma=0.001303 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! Estimated beam: bmin=0.6598 mas, bmaj=1.854 mas, bpa=-9.267 degrees ! Estimated noise=540.126 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00347164 Jy ! Component: 100 - total flux cleaned = 0.00577605 Jy ! Component: 150 - total flux cleaned = 0.0079092 Jy ! Component: 200 - total flux cleaned = 0.00903071 Jy ! Total flux subtracted in 200 components = 0.00903071 Jy ! Clean residual min=-0.005391 max=0.005860 Jy/beam ! Clean residual mean=0.000432 rms=0.001230 Jy/beam ! Combined flux in latest and established models = 2.98758 Jy selfcal ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 115 components and 2.98758 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.230647Jy sigma=0.001298 ! Fit after self-cal, rms=0.230594Jy sigma=0.001298 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 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 = 0.00209429 Jy ! Component: 100 - total flux cleaned = 0.00328362 Jy ! Component: 150 - total flux cleaned = 0.00405029 Jy ! Component: 200 - total flux cleaned = 0.00475544 Jy ! Total flux subtracted in 200 components = 0.00475544 Jy ! Clean residual min=-0.005107 max=0.005042 Jy/beam ! Clean residual mean=0.000402 rms=0.001170 Jy/beam ! Combined flux in latest and established models = 2.99234 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 120 components and 2.99234 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.230298Jy sigma=0.001296 ! Fit after self-cal, rms=0.230269Jy sigma=0.001295 ! Inverting map ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 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=0.230269Jy sigma=0.001295 ! Fit after self-cal, rms=0.230321Jy sigma=0.001294 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! Estimated beam: bmin=2.305 mas, bmaj=3.178 mas, bpa=-11.49 degrees ! Estimated noise=673.814 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00513569 Jy ! Component: 100 - total flux cleaned = 0.00677159 Jy ! Component: 150 - total flux cleaned = 0.00801354 Jy ! Component: 200 - total flux cleaned = 0.00888491 Jy ! Total flux subtracted in 200 components = 0.00888491 Jy ! Clean residual min=-0.003934 max=0.005526 Jy/beam ! Clean residual mean=0.000646 rms=0.001352 Jy/beam ! Combined flux in latest and established models = 3.00122 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 136 components and 3.00122 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.230175Jy sigma=0.001293 ! Fit after self-cal, rms=0.230144Jy sigma=0.001293 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 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 = 0.00106275 Jy ! Component: 100 - total flux cleaned = 0.00154982 Jy ! Component: 150 - total flux cleaned = 0.00182695 Jy ! Component: 200 - total flux cleaned = 0.00212852 Jy ! Total flux subtracted in 200 components = 0.00212852 Jy ! Clean residual min=-0.003940 max=0.005237 Jy/beam ! Clean residual mean=0.000612 rms=0.001363 Jy/beam ! Combined flux in latest and established models = 3.00335 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 140 components and 3.00335 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.230051Jy sigma=0.001292 ! Fit after self-cal, rms=0.230038Jy sigma=0.001292 ! Inverting map ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. win_mult = win_mult / 1.2 print "************** FINISHED AMPLITUDE SELF-CAL **************" ! ************** FINISHED AMPLITUDE SELF-CAL ************** restore ! Inverting map and beam ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! Estimated beam: bmin=0.6607 mas, bmaj=1.855 mas, bpa=-9.276 degrees ! Estimated noise=540.383 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6607 x 1.855 at -9.276 degrees (North through East) ! Clean map min=-0.0041078 max=2.4454 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=0.230038Jy sigma=0.001292 ! Fit after self-cal, rms=0.207459Jy sigma=0.001115 ! Inverting map and beam ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! Estimated beam: bmin=0.6609 mas, bmaj=1.854 mas, bpa=-9.268 degrees ! Estimated noise=539.821 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00267729 Jy ! Component: 100 - total flux cleaned = -0.00241884 Jy ! Component: 150 - total flux cleaned = -0.00230588 Jy ! Component: 200 - total flux cleaned = -0.0022035 Jy ! Total flux subtracted in 200 components = -0.0022035 Jy ! Clean residual min=-0.003674 max=0.003869 Jy/beam ! Clean residual mean=0.000211 rms=0.000883 Jy/beam ! Combined flux in latest and established models = 3.00115 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 146 components and 3.00115 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.207085Jy sigma=0.001114 ! Fit after self-cal, rms=0.207062Jy sigma=0.001114 ! Inverting map ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! Added new window around map position (-1.4, 12.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0022581 Jy ! Component: 100 - total flux cleaned = 0.00236271 Jy ! Component: 150 - total flux cleaned = 0.00235655 Jy ! Component: 200 - total flux cleaned = 0.00253889 Jy ! Total flux subtracted in 200 components = 0.00253889 Jy ! Clean residual min=-0.003462 max=0.003654 Jy/beam ! Clean residual mean=0.000199 rms=0.000847 Jy/beam ! Combined flux in latest and established models = 3.00369 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 156 components and 3.00369 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.206885Jy sigma=0.001113 ! Fit after self-cal, rms=0.206869Jy sigma=0.001113 ! Inverting map ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! Added new window around map position (-23, -9.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00251135 Jy ! Component: 100 - total flux cleaned = 0.00270227 Jy ! Component: 150 - total flux cleaned = 0.00278521 Jy ! Component: 200 - total flux cleaned = 0.00295038 Jy ! Total flux subtracted in 200 components = 0.00295038 Jy ! Clean residual min=-0.003328 max=0.003329 Jy/beam ! Clean residual mean=0.000180 rms=0.000819 Jy/beam ! Combined flux in latest and established models = 3.00664 Jy ! Performing phase self-cal ! Adding 31 model components to the UV plane model. ! The established model now contains 166 components and 3.00664 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.206741Jy sigma=0.001112 ! Fit after self-cal, rms=0.206733Jy sigma=0.001112 ! Inverting map ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.206733Jy sigma=0.001112 ! Fit after self-cal, rms=0.206797Jy sigma=0.001111 print "************** CLEARING MODEL AND STARTING OVER **********" ! ************** CLEARING MODEL AND STARTING OVER ********** clrmod true ! clrmod: Cleared the established and tentative models. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! Estimated beam: bmin=0.5615 mas, bmaj=1.467 mas, bpa=-5.315 degrees ! Estimated noise=994.875 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.85646 Jy ! Component: 100 - total flux cleaned = 2.31664 Jy ! Component: 150 - total flux cleaned = 2.52373 Jy ! Component: 200 - total flux cleaned = 2.62935 Jy ! Total flux subtracted in 200 components = 2.62935 Jy ! Clean residual min=-0.016215 max=0.053772 Jy/beam ! Clean residual mean=0.000139 rms=0.005216 Jy/beam ! Combined flux in latest and established models = 2.62936 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 2.62936 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! Estimated beam: bmin=0.6618 mas, bmaj=1.854 mas, bpa=-9.268 degrees ! Estimated noise=539.798 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 = 0.108551 Jy ! Component: 100 - total flux cleaned = 0.175935 Jy ! Component: 150 - total flux cleaned = 0.221891 Jy ! Component: 200 - total flux cleaned = 0.254956 Jy ! Total flux subtracted in 200 components = 0.254956 Jy ! Clean residual min=-0.007391 max=0.018792 Jy/beam ! Clean residual mean=0.000863 rms=0.003615 Jy/beam ! Combined flux in latest and established models = 2.88431 Jy ! Adding 55 model components to the UV plane model. ! The established model now contains 64 components and 2.88431 Jy ! Inverting map ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0244369 Jy ! Component: 100 - total flux cleaned = 0.0430131 Jy ! Component: 150 - total flux cleaned = 0.0574091 Jy ! Component: 200 - total flux cleaned = 0.06874 Jy ! Total flux subtracted in 200 components = 0.06874 Jy ! Clean residual min=-0.004799 max=0.006765 Jy/beam ! Clean residual mean=0.000454 rms=0.001596 Jy/beam ! Combined flux in latest and established models = 2.95305 Jy ! Adding 55 model components to the UV plane model. ! The established model now contains 101 components and 2.95305 Jy ! Inverting map ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 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 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! Estimated beam: bmin=2.304 mas, bmaj=3.177 mas, bpa=-11.38 degrees ! Estimated noise=672.402 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0165485 Jy ! Component: 100 - total flux cleaned = 0.0264394 Jy ! Component: 150 - total flux cleaned = 0.0331239 Jy ! Component: 200 - total flux cleaned = 0.0380204 Jy ! Total flux subtracted in 200 components = 0.0380204 Jy ! Clean residual min=-0.002865 max=0.004934 Jy/beam ! Clean residual mean=0.000535 rms=0.001174 Jy/beam ! Combined flux in latest and established models = 2.99107 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 = 0.00389455 Jy ! Component: 100 - total flux cleaned = 0.00680303 Jy ! Component: 150 - total flux cleaned = 0.00838357 Jy ! Component: 200 - total flux cleaned = 0.00965996 Jy ! Total flux subtracted in 200 components = 0.00965996 Jy ! Clean residual min=-0.002487 max=0.003730 Jy/beam ! Clean residual mean=0.000388 rms=0.000959 Jy/beam ! Combined flux in latest and established models = 3.00073 Jy ! Adding 85 model components to the UV plane model. ! The established model now contains 166 components and 3.00073 Jy ! Inverting map ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! Estimated beam: bmin=0.6618 mas, bmaj=1.854 mas, bpa=-9.268 degrees ! Estimated noise=539.798 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000364932 Jy ! Component: 100 - total flux cleaned = 0.00115543 Jy ! Component: 150 - total flux cleaned = 0.00166669 Jy ! Component: 200 - total flux cleaned = 0.00213575 Jy ! Total flux subtracted in 200 components = 0.00213575 Jy ! Clean residual min=-0.003452 max=0.003224 Jy/beam ! Clean residual mean=0.000147 rms=0.000812 Jy/beam ! Combined flux in latest and established models = 3.00287 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 181 components and 3.00287 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.206622Jy sigma=0.001115 ! Fit after self-cal, rms=0.206511Jy sigma=0.001114 wmodel J0530+1331_X_2003_07_09_pus_map.mod ! Writing 181 model components to file: J0530+1331_X_2003_07_09_pus_map.mod wobs J0530+1331_X_2003_07_09_pus_uvs.fits ! Writing UV FITS file: J0530+1331_X_2003_07_09_pus_uvs.fits wwins J0530+1331_X_2003_07_09_pus_map.win ! wwins: Wrote 5 windows to J0530+1331_X_2003_07_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 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000271556 Jy ! Component: 100 - total flux cleaned = 0.000470348 Jy ! Component: 150 - total flux cleaned = 0.00107085 Jy ! Component: 200 - total flux cleaned = 0.00170231 Jy ! Component: 250 - total flux cleaned = 0.00236713 Jy ! Component: 300 - total flux cleaned = 0.00311454 Jy ! Component: 350 - total flux cleaned = 0.00374603 Jy ! Component: 400 - total flux cleaned = 0.00445837 Jy ! Component: 450 - total flux cleaned = 0.00492402 Jy ! Component: 500 - total flux cleaned = 0.00551928 Jy ! Component: 550 - total flux cleaned = 0.00596972 Jy ! Component: 600 - total flux cleaned = 0.00654684 Jy ! Component: 650 - total flux cleaned = 0.00707207 Jy ! Component: 700 - total flux cleaned = 0.00759022 Jy ! Component: 750 - total flux cleaned = 0.00801661 Jy ! Component: 800 - total flux cleaned = 0.00843851 Jy ! Component: 850 - total flux cleaned = 0.00881363 Jy ! Component: 900 - total flux cleaned = 0.00914376 Jy ! Component: 950 - total flux cleaned = 0.00951172 Jy ! Component: 1000 - total flux cleaned = 0.00975507 Jy ! Component: 1050 - total flux cleaned = 0.0101159 Jy ! Component: 1100 - total flux cleaned = 0.0103945 Jy ! Component: 1150 - total flux cleaned = 0.0106307 Jy ! Component: 1200 - total flux cleaned = 0.011021 Jy ! Component: 1250 - total flux cleaned = 0.0112144 Jy ! Component: 1300 - total flux cleaned = 0.0114834 Jy ! Component: 1350 - total flux cleaned = 0.0117503 Jy ! Component: 1400 - total flux cleaned = 0.0119768 Jy ! Component: 1450 - total flux cleaned = 0.0121643 Jy ! Component: 1500 - total flux cleaned = 0.0124254 Jy ! Component: 1550 - total flux cleaned = 0.0126843 Jy ! Component: 1600 - total flux cleaned = 0.0129778 Jy ! Component: 1650 - total flux cleaned = 0.0130873 Jy ! Component: 1700 - total flux cleaned = 0.0133408 Jy ! Component: 1750 - total flux cleaned = 0.0135565 Jy ! Component: 1800 - total flux cleaned = 0.013771 Jy ! Component: 1850 - total flux cleaned = 0.0139839 Jy ! Component: 1900 - total flux cleaned = 0.0141954 Jy ! Component: 1950 - total flux cleaned = 0.0144406 Jy ! Component: 2000 - total flux cleaned = 0.014684 Jy ! Total flux subtracted in 2048 components = 0.014753 Jy ! Clean residual min=-0.002187 max=0.001739 Jy/beam ! Clean residual mean=0.000066 rms=0.000623 Jy/beam ! Combined flux in latest and established models = 3.01762 Jy keep ! Adding 153 model components to the UV plane model. ! The established model now contains 334 components and 3.01762 Jy ![Exited script file: muppet] wmap "J0530+1331_X_2003_07_09_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6618 x 1.854 at -9.268 degrees (North through East) ! Clean map min=-0.0030832 max=2.4443 Jy/beam ! Writing clean map to FITS file: J0530+1331_X_2003_07_09_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 2.44432 invert ! Inverting map ! Your choice of large map pixels excluded 1.43% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.0006229 device "J0530+1331_X_2003_07_09_pus\_map.eps/VPS" ! Attempting to open device: 'J0530+1331_X_2003_07_09_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.0764508 0.0764508 0.152902 0.305803 0.611606 1.22321 2.44642 4.89285 9.7857 19.5714 39.1428 78.2856 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0018 print "peak=",int(1000*peak_flux)/1000 ! peak= 2.444 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6618 x 1.854 at -9.268 degrees (North through East) ! Clean map min=-0.0030832 max=2.4443 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. quit ! Quitting program ! Log file J0530+1331_X_2003_07_09_pus_uvs.log closed on Sun Apr 7 11:50:36 2013