! Started logfile: J1658+0741_X_2000_03_13_pus_uvs.log on Wed Apr 3 20:22:58 2013 obs J1658+0741_X_2000_03_13_pus_uva.fits ! Reading UV FITS file: J1658+0741_X_2000_03_13_pus_uva.fits ! AN table 1: 59 integrations on 190 of 190 possible baselines. ! AN table 2: 107 integrations on 190 of 190 possible baselines. ! AN table 3: 126 integrations on 190 of 190 possible baselines. ! Apparent sampling: 0.108526 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1658+0741 ! ! 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 2386 lines of history. ! ! Reading 24084 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 J1658+0741_X_2000_03_13_pus] integer clean_niter clean_niter = 100 float clean_gain clean_gain = 0.03 float dynam dynam = 6.0 float soltime1 soltime1 = 120 float soltime2 soltime2 = 20 float thresh thresh = 0.5 float win_mult win_mult = 1.8 float time_av time_av = 16 float old_peak float new_peak float flux_cutoff mapsize field_size, field_cell ! Map grid = 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 961 telescope corrections were flagged in sub-array 1. ! A total of 1737 telescope corrections were flagged in sub-array 2. ! A total of 1677 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 958 telescope corrections were flagged in sub-array 1. ! A total of 1734 telescope corrections were flagged in sub-array 2. ! A total of 1677 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 955 telescope corrections were flagged in sub-array 1. ! A total of 1753 telescope corrections were flagged in sub-array 2. ! A total of 1753 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 957 telescope corrections were flagged in sub-array 1. ! A total of 1764 telescope corrections were flagged in sub-array 2. ! A total of 1677 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=0.764547Jy sigma=0.007616 ! Fit after self-cal, rms=0.449025Jy sigma=0.004204 ! 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 4.23% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=0.5329 mas, bmaj=1.323 mas, bpa=-3.541 degrees ! Estimated noise=1054.21 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 = 0.508703 Jy ! Component: 100 - total flux cleaned = 0.703897 Jy ! Total flux subtracted in 100 components = 0.703897 Jy ! Clean residual min=-0.024556 max=0.088896 Jy/beam ! Clean residual mean=-0.000121 rms=0.007878 Jy/beam ! Combined flux in latest and established models = 0.703897 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 8 components and 0.703897 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.279463Jy sigma=0.002387 ! Fit after self-cal, rms=0.276763Jy sigma=0.002368 ! Inverting map ! Your choice of large map pixels excluded 4.23% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0982274 Jy ! Component: 100 - total flux cleaned = 0.147653 Jy ! Total flux subtracted in 100 components = 0.147653 Jy ! Clean residual min=-0.016666 max=0.056118 Jy/beam ! Clean residual mean=-0.000131 rms=0.005005 Jy/beam ! Combined flux in latest and established models = 0.85155 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 14 components and 0.85155 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.237310Jy sigma=0.001817 ! Fit after self-cal, rms=0.236644Jy sigma=0.001812 ! Inverting map ! Your choice of large map pixels excluded 4.23% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Added new window around map position (-5.4, 6.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0539568 Jy ! Component: 100 - total flux cleaned = 0.085728 Jy ! Total flux subtracted in 100 components = 0.085728 Jy ! Clean residual min=-0.013303 max=0.027327 Jy/beam ! Clean residual mean=-0.000088 rms=0.003703 Jy/beam ! Combined flux in latest and established models = 0.937278 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 29 components and 0.937278 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.219258Jy sigma=0.001545 ! Fit after self-cal, rms=0.217992Jy sigma=0.001532 ! Inverting map ! Your choice of large map pixels excluded 4.23% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Added new window around map position (-6.6, 5.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0305713 Jy ! Component: 100 - total flux cleaned = 0.0535941 Jy ! Total flux subtracted in 100 components = 0.0535941 Jy ! Clean residual min=-0.011981 max=0.016835 Jy/beam ! Clean residual mean=-0.000062 rms=0.003018 Jy/beam ! Combined flux in latest and established models = 0.990872 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 41 components and 0.990872 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.211333Jy sigma=0.001419 ! Fit after self-cal, rms=0.210959Jy sigma=0.001417 ! Inverting map ! Your choice of large map pixels excluded 4.23% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 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 4.23% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=0.6649 mas, bmaj=1.625 mas, bpa=-2.481 degrees ! Estimated noise=523.943 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 = 0.0313148 Jy ! Component: 100 - total flux cleaned = 0.0511966 Jy ! Component: 150 - total flux cleaned = 0.0654264 Jy ! Component: 200 - total flux cleaned = 0.0758805 Jy ! Total flux subtracted in 200 components = 0.0758805 Jy ! Clean residual min=-0.010743 max=0.016644 Jy/beam ! Clean residual mean=-0.000105 rms=0.003031 Jy/beam ! Combined flux in latest and established models = 1.06675 Jy ! Performing phase self-cal ! Adding 42 model components to the UV plane model. ! The established model now contains 68 components and 1.06675 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.206397Jy sigma=0.001330 ! Fit after self-cal, rms=0.206000Jy sigma=0.001326 ! Inverting map ! Your choice of large map pixels excluded 4.23% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 69 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.95 GC 1.05 KP 0.98 ! LA 0.94 NL 0.96 OV 0.96 PT 0.97 ! SC 1.01 WF 1.07 HH 1.00* KK 1.07 ! MA 1.00* MC 1.00* MK 1.00* NY 1.00* ! ON 1.00* TS 1.00* WZ 1.00* HN 3.31 ! ! A total of 27 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 FD 0.99 GC 1.00* KP 1.02 ! LA 1.03 NL 1.09 OV 1.02 PT 1.03 ! SC 0.94 WF 1.09 HH 0.97 KK 1.00* ! MA 0.98 MC 1.01 MK 1.00* NY 1.04 ! ON 1.04 TS 1.00* WZ 1.07 HN 0.84 ! ! A total of 36 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 FD 0.99 GC 1.09 KP 1.03 ! LA 1.04 NL 1.06 OV 0.96 PT 0.99 ! SC 1.00* WF 1.00* HH 1.00* KK 1.02 ! MA 0.98 MC 0.93 MK 0.95 NY 0.95 ! ON 0.97 TS 0.95 WZ 0.88 HN 1.00* ! ! ! Correcting IF 2. ! A total of 69 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 0.93 GC 1.05 KP 0.96 ! LA 0.90 NL 1.02 OV 0.96 PT 0.92 ! SC 1.04 WF 1.05 HH 1.00* KK 1.04 ! MA 1.00* MC 1.00* MK 1.00* NY 1.00* ! ON 1.00* TS 1.00* WZ 1.00* HN 0.87 ! ! A total of 36 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.07 FD 0.99 GC 1.00* KP 0.99 ! LA 0.97 NL 0.99 OV 0.99 PT 0.99 ! SC 0.92 WF 1.05 HH 0.95 KK 1.00* ! MA 0.93 MC 1.01 MK 1.00* NY 1.07 ! ON 1.03 TS 1.00* WZ 1.14 HN 0.82 ! ! A total of 36 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 FD 0.98 GC 1.06 KP 0.99 ! LA 1.00 NL 1.10 OV 0.95 PT 0.95 ! SC 1.00* WF 1.00* HH 1.00* KK 0.99 ! MA 0.98 MC 0.91 MK 1.00 NY 1.02 ! ON 0.97 TS 0.98 WZ 0.89 HN 1.00* ! ! ! Correcting IF 3. ! A total of 69 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.97 GC 1.06 KP 0.96 ! LA 0.89 NL 0.95 OV 0.97 PT 0.95 ! SC 1.06 WF 1.03 HH 1.00* KK 1.05 ! MA 1.00* MC 1.00* MK 1.00* NY 1.00* ! ON 1.00* TS 1.00* WZ 1.00* HN 1.09 ! ! A total of 21 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.10 FD 1.02 GC 1.00* KP 1.01 ! LA 0.96 NL 0.95 OV 1.00 PT 1.01 ! SC 0.97 WF 1.17 HH 0.89 KK 1.00* ! MA 0.89 MC 0.99 MK 1.00* NY 1.14 ! ON 0.98 TS 1.00* WZ 1.10 HN 0.89 ! ! A total of 39 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.04 FD 1.02 GC 1.08 KP 1.00 ! LA 1.00 NL 1.03 OV 0.97 PT 0.97 ! SC 1.00* WF 1.00* HH 1.00* KK 0.97 ! MA 1.06 MC 0.85 MK 0.95 NY 1.19 ! ON 0.90 TS 1.00 WZ 1.00* HN 1.00* ! ! ! Correcting IF 4. ! A total of 69 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.96 GC 1.07 KP 0.96 ! LA 0.91 NL 0.96 OV 0.96 PT 0.96 ! SC 1.09 WF 1.11 HH 1.00* KK 1.04 ! MA 1.00* MC 1.00* MK 1.00* NY 1.00* ! ON 1.00* TS 1.00* WZ 1.00* HN 0.91 ! ! A total of 30 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 FD 1.00 GC 1.00* KP 0.99 ! LA 0.97 NL 1.12 OV 1.00 PT 1.05 ! SC 1.04 WF 1.09 HH 0.87 KK 1.00* ! MA 0.93 MC 1.00 MK 1.00* NY 1.10 ! ON 1.01 TS 1.00* WZ 1.09 HN 0.89 ! ! A total of 36 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 1.00 GC 1.08 KP 0.99 ! LA 1.02 NL 1.04 OV 0.97 PT 0.99 ! SC 1.00* WF 1.00* HH 1.00* KK 0.97 ! MA 0.99 MC 0.96 MK 0.97 NY 1.05 ! ON 0.99 TS 0.98 WZ 0.92 HN 1.00* ! ! ! Fit before self-cal, rms=0.206000Jy sigma=0.001326 ! Fit after self-cal, rms=0.194069Jy sigma=0.001251 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=0.6642 mas, bmaj=1.642 mas, bpa=-2.308 degrees ! Estimated noise=524.462 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 = 0.00512715 Jy ! Component: 100 - total flux cleaned = 0.00668732 Jy ! Component: 150 - total flux cleaned = 0.00759759 Jy ! Component: 200 - total flux cleaned = 0.00807882 Jy ! Total flux subtracted in 200 components = 0.00807882 Jy ! Clean residual min=-0.004871 max=0.009229 Jy/beam ! Clean residual mean=-0.000009 rms=0.001636 Jy/beam ! Combined flux in latest and established models = 1.07483 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 76 components and 1.07483 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.193646Jy sigma=0.001245 ! Fit after self-cal, rms=0.193677Jy sigma=0.001245 ! Inverting map ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Added new window around map position (-1.4, 1.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00882383 Jy ! Component: 100 - total flux cleaned = 0.0108699 Jy ! Component: 150 - total flux cleaned = 0.0115858 Jy ! Component: 200 - total flux cleaned = 0.0124591 Jy ! Total flux subtracted in 200 components = 0.0124591 Jy ! Clean residual min=-0.004219 max=0.006246 Jy/beam ! Clean residual mean=0.000008 rms=0.001404 Jy/beam ! Combined flux in latest and established models = 1.08729 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 88 components and 1.08729 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.193134Jy sigma=0.001239 ! Fit after self-cal, rms=0.192969Jy sigma=0.001238 ! Inverting map ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 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=0.192969Jy sigma=0.001238 ! Fit after self-cal, rms=0.192644Jy sigma=0.001237 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=0.6653 mas, bmaj=1.642 mas, bpa=-2.335 degrees ! Estimated noise=524.859 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0031987 Jy ! Component: 100 - total flux cleaned = 0.00499063 Jy ! Component: 150 - total flux cleaned = 0.00619456 Jy ! Component: 200 - total flux cleaned = 0.00690898 Jy ! Total flux subtracted in 200 components = 0.00690898 Jy ! Clean residual min=-0.003822 max=0.005747 Jy/beam ! Clean residual mean=0.000013 rms=0.001228 Jy/beam ! Combined flux in latest and established models = 1.0942 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 89 components and 1.0942 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.192324Jy sigma=0.001234 ! Fit after self-cal, rms=0.192221Jy sigma=0.001233 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 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 (-15, 11.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00439265 Jy ! Component: 100 - total flux cleaned = 0.00624279 Jy ! Component: 150 - total flux cleaned = 0.00795325 Jy ! Component: 200 - total flux cleaned = 0.00941526 Jy ! Total flux subtracted in 200 components = 0.00941526 Jy ! Clean residual min=-0.003860 max=0.004201 Jy/beam ! Clean residual mean=0.000009 rms=0.001032 Jy/beam ! Combined flux in latest and established models = 1.10362 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 106 components and 1.10362 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.191983Jy sigma=0.001231 ! Fit after self-cal, rms=0.191941Jy sigma=0.001230 ! Inverting map ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Added new window around map position (-1.6, 5.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00383162 Jy ! Component: 100 - total flux cleaned = 0.0043631 Jy ! Component: 150 - total flux cleaned = 0.00519162 Jy ! Component: 200 - total flux cleaned = 0.0058601 Jy ! Total flux subtracted in 200 components = 0.0058601 Jy ! Clean residual min=-0.003684 max=0.003452 Jy/beam ! Clean residual mean=0.000004 rms=0.000941 Jy/beam ! Combined flux in latest and established models = 1.10948 Jy ! Performing phase self-cal ! Adding 32 model components to the UV plane model. ! The established model now contains 124 components and 1.10948 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.191737Jy sigma=0.001229 ! Fit after self-cal, rms=0.191699Jy sigma=0.001229 ! Inverting map ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 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=0.191699Jy sigma=0.001229 ! Fit after self-cal, rms=0.190788Jy sigma=0.001228 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=0.6664 mas, bmaj=1.64 mas, bpa=-2.328 degrees ! Estimated noise=524.518 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00139451 Jy ! Component: 100 - total flux cleaned = 0.00243299 Jy ! Component: 150 - total flux cleaned = 0.00276417 Jy ! Component: 200 - total flux cleaned = 0.00322157 Jy ! Total flux subtracted in 200 components = 0.00322157 Jy ! Clean residual min=-0.003620 max=0.003158 Jy/beam ! Clean residual mean=0.000003 rms=0.000856 Jy/beam ! Combined flux in latest and established models = 1.1127 Jy selfcal ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 128 components and 1.1127 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.190633Jy sigma=0.001227 ! Fit after self-cal, rms=0.190586Jy sigma=0.001227 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 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 = 0.000376119 Jy ! Component: 100 - total flux cleaned = 0.000980406 Jy ! Component: 150 - total flux cleaned = 0.0011181 Jy ! Component: 200 - total flux cleaned = 0.00125126 Jy ! Total flux subtracted in 200 components = 0.00125126 Jy ! Clean residual min=-0.003548 max=0.003190 Jy/beam ! Clean residual mean=0.000005 rms=0.000835 Jy/beam ! Combined flux in latest and established models = 1.11395 Jy ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 134 components and 1.11395 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.190463Jy sigma=0.001226 ! Fit after self-cal, rms=0.190433Jy sigma=0.001226 ! Inverting map ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 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=0.190433Jy sigma=0.001226 ! Fit after self-cal, rms=0.190004Jy sigma=0.001226 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=2.679 mas, bmaj=3.374 mas, bpa=25.91 degrees ! Estimated noise=660.19 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00199044 Jy ! Component: 100 - total flux cleaned = 0.00294548 Jy ! Component: 150 - total flux cleaned = 0.00331933 Jy ! Component: 200 - total flux cleaned = 0.00345379 Jy ! Total flux subtracted in 200 components = 0.00345379 Jy ! Clean residual min=-0.004075 max=0.004190 Jy/beam ! Clean residual mean=0.000023 rms=0.001148 Jy/beam ! Combined flux in latest and established models = 1.1174 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 152 components and 1.1174 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.190011Jy sigma=0.001226 ! Fit after self-cal, rms=0.189988Jy sigma=0.001226 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 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 = 0.000173363 Jy ! Component: 100 - total flux cleaned = 0.00038365 Jy ! Component: 150 - total flux cleaned = 0.000456488 Jy ! Component: 200 - total flux cleaned = 0.000521398 Jy ! Total flux subtracted in 200 components = 0.000521398 Jy ! Clean residual min=-0.004004 max=0.004141 Jy/beam ! Clean residual mean=0.000027 rms=0.001130 Jy/beam ! Combined flux in latest and established models = 1.11792 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 156 components and 1.11792 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.189979Jy sigma=0.001226 ! Fit after self-cal, rms=0.189964Jy sigma=0.001226 ! Inverting map ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 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 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=0.6673 mas, bmaj=1.638 mas, bpa=-2.316 degrees ! Estimated noise=524.584 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6673 x 1.638 at -2.316 degrees (North through East) ! Clean map min=-0.0032423 max=0.66369 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=0.189964Jy sigma=0.001226 ! Fit after self-cal, rms=0.186507Jy sigma=0.001126 ! Inverting map and beam ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=0.6658 mas, bmaj=1.627 mas, bpa=-2.219 degrees ! Estimated noise=523.571 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000427093 Jy ! Component: 100 - total flux cleaned = 0.000275489 Jy ! Component: 150 - total flux cleaned = 0.000138271 Jy ! Component: 200 - total flux cleaned = 7.69042e-05 Jy ! Total flux subtracted in 200 components = 7.69042e-05 Jy ! Clean residual min=-0.003626 max=0.003037 Jy/beam ! Clean residual mean=0.000007 rms=0.000765 Jy/beam ! Combined flux in latest and established models = 1.118 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 163 components and 1.118 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.186377Jy sigma=0.001126 ! Fit after self-cal, rms=0.186350Jy sigma=0.001125 ! Inverting map ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00021421 Jy ! Component: 100 - total flux cleaned = 0.000211321 Jy ! Component: 150 - total flux cleaned = 0.000152748 Jy ! Component: 200 - total flux cleaned = 4.1465e-05 Jy ! Total flux subtracted in 200 components = 4.1465e-05 Jy ! Clean residual min=-0.003543 max=0.003108 Jy/beam ! Clean residual mean=0.000006 rms=0.000759 Jy/beam ! Combined flux in latest and established models = 1.11804 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 168 components and 1.11804 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.186265Jy sigma=0.001125 ! Fit after self-cal, rms=0.186246Jy sigma=0.001125 ! Inverting map ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.186246Jy sigma=0.001125 ! Fit after self-cal, rms=0.192779Jy sigma=0.001125 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 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=0.5371 mas, bmaj=1.302 mas, bpa=-3.215 degrees ! Estimated noise=1073.46 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.510245 Jy ! Component: 100 - total flux cleaned = 0.70395 Jy ! Component: 150 - total flux cleaned = 0.800924 Jy ! Component: 200 - total flux cleaned = 0.861685 Jy ! Total flux subtracted in 200 components = 0.861685 Jy ! Clean residual min=-0.012889 max=0.033540 Jy/beam ! Clean residual mean=-0.000077 rms=0.004005 Jy/beam ! Combined flux in latest and established models = 0.861685 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 16 model components to the UV plane model. ! The established model now contains 16 components and 0.861685 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=0.6666 mas, bmaj=1.626 mas, bpa=-2.204 degrees ! Estimated noise=523.707 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (-6, 5.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0685233 Jy ! Component: 100 - total flux cleaned = 0.113146 Jy ! Component: 150 - total flux cleaned = 0.144537 Jy ! Component: 200 - total flux cleaned = 0.167272 Jy ! Total flux subtracted in 200 components = 0.167272 Jy ! Clean residual min=-0.007410 max=0.013026 Jy/beam ! Clean residual mean=-0.000131 rms=0.002652 Jy/beam ! Combined flux in latest and established models = 1.02896 Jy ! Adding 43 model components to the UV plane model. ! The established model now contains 49 components and 1.02896 Jy ! Inverting map ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Added new window around map position (-0.2, 1.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0171288 Jy ! Component: 100 - total flux cleaned = 0.0302115 Jy ! Component: 150 - total flux cleaned = 0.0403907 Jy ! Component: 200 - total flux cleaned = 0.0485085 Jy ! Total flux subtracted in 200 components = 0.0485085 Jy ! Clean residual min=-0.004467 max=0.006016 Jy/beam ! Clean residual mean=-0.000033 rms=0.001378 Jy/beam ! Combined flux in latest and established models = 1.07747 Jy ! Adding 37 model components to the UV plane model. ! The established model now contains 74 components and 1.07747 Jy ! Inverting map ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Added new window around map position (-4.8, 4.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0069151 Jy ! Component: 100 - total flux cleaned = 0.0126358 Jy ! Component: 150 - total flux cleaned = 0.0175346 Jy ! Component: 200 - total flux cleaned = 0.0217539 Jy ! Total flux subtracted in 200 components = 0.0217539 Jy ! Clean residual min=-0.003469 max=0.003983 Jy/beam ! Clean residual mean=-0.000003 rms=0.000981 Jy/beam ! Combined flux in latest and established models = 1.09922 Jy ! Adding 37 model components to the UV plane model. ! The established model now contains 98 components and 1.09922 Jy ! Inverting map ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 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 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=2.675 mas, bmaj=3.374 mas, bpa=26.04 degrees ! Estimated noise=660.512 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0051967 Jy ! Component: 100 - total flux cleaned = 0.00886379 Jy ! Component: 150 - total flux cleaned = 0.0116727 Jy ! Component: 200 - total flux cleaned = 0.0138808 Jy ! Total flux subtracted in 200 components = 0.0138808 Jy ! Clean residual min=-0.004337 max=0.004313 Jy/beam ! Clean residual mean=0.000021 rms=0.001168 Jy/beam ! Combined flux in latest and established models = 1.1131 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 = 0.001746 Jy ! Component: 100 - total flux cleaned = 0.00313301 Jy ! Component: 150 - total flux cleaned = 0.00424096 Jy ! Component: 200 - total flux cleaned = 0.00500012 Jy ! Total flux subtracted in 200 components = 0.00500012 Jy ! Clean residual min=-0.004233 max=0.004397 Jy/beam ! Clean residual mean=0.000027 rms=0.001079 Jy/beam ! Combined flux in latest and established models = 1.1181 Jy ! Adding 60 model components to the UV plane model. ! The established model now contains 148 components and 1.1181 Jy ! Inverting map ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=0.6666 mas, bmaj=1.626 mas, bpa=-2.204 degrees ! Estimated noise=523.707 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000333549 Jy ! Component: 100 - total flux cleaned = 0.000526699 Jy ! Component: 150 - total flux cleaned = 0.000702577 Jy ! Component: 200 - total flux cleaned = 0.000864129 Jy ! Total flux subtracted in 200 components = 0.000864129 Jy ! Clean residual min=-0.003407 max=0.003276 Jy/beam ! Clean residual mean=0.000008 rms=0.000769 Jy/beam ! Combined flux in latest and established models = 1.11896 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 159 components and 1.11896 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.193310Jy sigma=0.001128 ! Fit after self-cal, rms=0.193293Jy sigma=0.001127 wmodel J1658+0741_X_2000_03_13_pus_map.mod ! Writing 159 model components to file: J1658+0741_X_2000_03_13_pus_map.mod wobs J1658+0741_X_2000_03_13_pus_uvs.fits ! Writing UV FITS file: J1658+0741_X_2000_03_13_pus_uvs.fits wwins J1658+0741_X_2000_03_13_pus_map.win ! wwins: Wrote 9 windows to J1658+0741_X_2000_03_13_pus_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000237041 Jy ! Component: 100 - total flux cleaned = 8.41746e-05 Jy ! Component: 150 - total flux cleaned = -6.27648e-05 Jy ! Component: 200 - total flux cleaned = 3.06343e-05 Jy ! Component: 250 - total flux cleaned = 0.000121362 Jy ! Component: 300 - total flux cleaned = 0.000298443 Jy ! Component: 350 - total flux cleaned = 0.000470017 Jy ! Component: 400 - total flux cleaned = 0.00046935 Jy ! Component: 450 - total flux cleaned = 0.000508385 Jy ! Component: 500 - total flux cleaned = 0.000508316 Jy ! Component: 550 - total flux cleaned = 0.000704422 Jy ! Component: 600 - total flux cleaned = 0.000781741 Jy ! Component: 650 - total flux cleaned = 0.000857193 Jy ! Component: 700 - total flux cleaned = 0.000857471 Jy ! Component: 750 - total flux cleaned = 0.000673293 Jy ! Component: 800 - total flux cleaned = 0.000674457 Jy ! Component: 850 - total flux cleaned = 0.000710593 Jy ! Component: 900 - total flux cleaned = 0.000675229 Jy ! Component: 950 - total flux cleaned = 0.000569853 Jy ! Component: 1000 - total flux cleaned = 0.000569856 Jy ! Component: 1050 - total flux cleaned = 0.000569501 Jy ! Component: 1100 - total flux cleaned = 0.000500966 Jy ! Component: 1150 - total flux cleaned = 0.000366214 Jy ! Component: 1200 - total flux cleaned = 0.000399346 Jy ! Component: 1250 - total flux cleaned = 0.000300174 Jy ! Component: 1300 - total flux cleaned = 0.00020206 Jy ! Component: 1350 - total flux cleaned = 0.000202002 Jy ! Component: 1400 - total flux cleaned = 0.000298544 Jy ! Component: 1450 - total flux cleaned = 0.000137793 Jy ! Component: 1500 - total flux cleaned = 0.000169647 Jy ! Component: 1550 - total flux cleaned = 0.000201221 Jy ! Component: 1600 - total flux cleaned = 0.00020127 Jy ! Component: 1650 - total flux cleaned = 0.000169919 Jy ! Component: 1700 - total flux cleaned = 0.000232174 Jy ! Component: 1750 - total flux cleaned = 0.000201777 Jy ! Component: 1800 - total flux cleaned = 0.000263067 Jy ! Component: 1850 - total flux cleaned = 0.000262977 Jy ! Component: 1900 - total flux cleaned = 0.00038362 Jy ! Component: 1950 - total flux cleaned = 0.000473159 Jy ! Component: 2000 - total flux cleaned = 0.000413464 Jy ! Total flux subtracted in 2048 components = 0.00041348 Jy ! Clean residual min=-0.001758 max=0.001473 Jy/beam ! Clean residual mean=0.000000 rms=0.000524 Jy/beam ! Combined flux in latest and established models = 1.11938 Jy keep ! Adding 146 model components to the UV plane model. ! The established model now contains 303 components and 1.11938 Jy ![Exited script file: muppet] wmap "J1658+0741_X_2000_03_13_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6666 x 1.626 at -2.204 degrees (North through East) ! Clean map min=-0.0028231 max=0.65967 Jy/beam ! Writing clean map to FITS file: J1658+0741_X_2000_03_13_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.659667 invert ! Inverting map ! Your choice of large map pixels excluded 4.34% of the data. ! The x-axis pixel size should ideally be below 0.164 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000524146 device "J1658+0741_X_2000_03_13_pus\_map.eps/VPS" ! Attempting to open device: 'J1658+0741_X_2000_03_13_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.238368 0.238368 0.476737 0.953474 1.90695 3.8139 7.62779 15.2556 30.5112 61.0223 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0015 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.659 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6666 x 1.626 at -2.204 degrees (North through East) ! Clean map min=-0.0028231 max=0.65967 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. quit ! Quitting program ! Log file J1658+0741_X_2000_03_13_pus_uvs.log closed on Wed Apr 3 20:23:09 2013