! Started logfile: J0102+5824_X_2000_03_13_pus_uvs.log on Wed Apr 3 15:23:58 2013 obs J0102+5824_X_2000_03_13_pus_uva.fits ! Reading UV FITS file: J0102+5824_X_2000_03_13_pus_uva.fits ! AN table 1: 212 integrations on 190 of 190 possible baselines. ! AN table 2: 560 integrations on 190 of 190 possible baselines. ! AN table 3: 516 integrations on 190 of 190 possible baselines. ! Apparent sampling: 0.20993 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0102+5824 ! ! 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 205496 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 J0102+5824_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 2220 telescope corrections were flagged in sub-array 1. ! A total of 7229 telescope corrections were flagged in sub-array 2. ! A total of 6766 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 2225 telescope corrections were flagged in sub-array 1. ! A total of 7230 telescope corrections were flagged in sub-array 2. ! A total of 6753 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 2232 telescope corrections were flagged in sub-array 1. ! A total of 7214 telescope corrections were flagged in sub-array 2. ! A total of 6779 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 2224 telescope corrections were flagged in sub-array 1. ! A total of 7202 telescope corrections were flagged in sub-array 2. ! A total of 6777 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=0.724692Jy sigma=0.005948 ! Fit after self-cal, rms=0.608278Jy sigma=0.005107 ! 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 5.24% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec ! Estimated beam: bmin=0.5357 mas, bmaj=0.5708 mas, bpa=5.392 degrees ! Estimated noise=435.418 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 = 0.306664 Jy ! Component: 100 - total flux cleaned = 0.381054 Jy ! Total flux subtracted in 100 components = 0.381054 Jy ! Clean residual min=-0.007774 max=0.032320 Jy/beam ! Clean residual mean=0.000019 rms=0.001423 Jy/beam ! Combined flux in latest and established models = 0.381054 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 0.381054 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.219700Jy sigma=0.001592 ! Fit after self-cal, rms=0.219511Jy sigma=0.001591 ! Inverting map ! Your choice of large map pixels excluded 5.24% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0375871 Jy ! Component: 100 - total flux cleaned = 0.0613795 Jy ! Total flux subtracted in 100 components = 0.0613795 Jy ! Clean residual min=-0.005740 max=0.018530 Jy/beam ! Clean residual mean=0.000011 rms=0.001154 Jy/beam ! Combined flux in latest and established models = 0.442434 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 11 components and 0.442434 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.205281Jy sigma=0.001421 ! Fit after self-cal, rms=0.204994Jy sigma=0.001419 ! Inverting map ! Your choice of large map pixels excluded 5.24% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec ! Added new window around map position (-0.6, -0.6). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0214324 Jy ! Component: 100 - total flux cleaned = 0.0371033 Jy ! Total flux subtracted in 100 components = 0.0371033 Jy ! Clean residual min=-0.004962 max=0.010096 Jy/beam ! Clean residual mean=0.000007 rms=0.001024 Jy/beam ! Combined flux in latest and established models = 0.479537 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 21 components and 0.479537 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.199491Jy sigma=0.001346 ! Fit after self-cal, rms=0.199247Jy sigma=0.001344 ! Inverting map ! Your choice of large map pixels excluded 5.24% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0138992 Jy ! Component: 100 - total flux cleaned = 0.0247282 Jy ! Total flux subtracted in 100 components = 0.0247282 Jy ! Clean residual min=-0.004516 max=0.007199 Jy/beam ! Clean residual mean=0.000004 rms=0.000953 Jy/beam ! Combined flux in latest and established models = 0.504265 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 22 components and 0.504265 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.196669Jy sigma=0.001308 ! Fit after self-cal, rms=0.196584Jy sigma=0.001307 ! Inverting map ! Your choice of large map pixels excluded 5.24% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec ! Added new window around map position (-0.6, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00972097 Jy ! Component: 100 - total flux cleaned = 0.017436 Jy ! Total flux subtracted in 100 components = 0.017436 Jy ! Clean residual min=-0.004241 max=0.005773 Jy/beam ! Clean residual mean=0.000002 rms=0.000918 Jy/beam ! Combined flux in latest and established models = 0.521701 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 26 components and 0.521701 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.195254Jy sigma=0.001287 ! Fit after self-cal, rms=0.195207Jy sigma=0.001287 ! Inverting map ! Your choice of large map pixels excluded 5.24% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec ! Added new window around map position (-1, -1.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00718158 Jy ! Component: 100 - total flux cleaned = 0.0129286 Jy ! Total flux subtracted in 100 components = 0.0129286 Jy ! Clean residual min=-0.004118 max=0.004940 Jy/beam ! Clean residual mean=0.000000 rms=0.000897 Jy/beam ! Combined flux in latest and established models = 0.53463 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 29 components and 0.53463 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.194468Jy sigma=0.001275 ! Fit after self-cal, rms=0.194440Jy sigma=0.001275 ! Inverting map ! Your choice of large map pixels excluded 5.24% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 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 5.24% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec ! Estimated beam: bmin=0.6525 mas, bmaj=0.6887 mas, bpa=12.29 degrees ! Estimated noise=207.567 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 = 0.0155343 Jy ! Component: 100 - total flux cleaned = 0.025465 Jy ! Component: 150 - total flux cleaned = 0.032221 Jy ! Component: 200 - total flux cleaned = 0.0368681 Jy ! Total flux subtracted in 200 components = 0.0368681 Jy ! Clean residual min=-0.004636 max=0.006145 Jy/beam ! Clean residual mean=-0.000002 rms=0.000958 Jy/beam ! Combined flux in latest and established models = 0.571498 Jy ! Performing phase self-cal ! Adding 31 model components to the UV plane model. ! The established model now contains 48 components and 0.571498 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.193397Jy sigma=0.001256 ! Fit after self-cal, rms=0.193312Jy sigma=0.001255 ! Inverting map ! Your choice of large map pixels excluded 5.24% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec ! Added new window around map position (-2.6, -1). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00719444 Jy ! Component: 100 - total flux cleaned = 0.0116592 Jy ! Component: 150 - total flux cleaned = 0.0147754 Jy ! Component: 200 - total flux cleaned = 0.0170188 Jy ! Total flux subtracted in 200 components = 0.0170188 Jy ! Clean residual min=-0.004521 max=0.004468 Jy/beam ! Clean residual mean=-0.000024 rms=0.000903 Jy/beam ! Combined flux in latest and established models = 0.588517 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 61 components and 0.588517 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.193136Jy sigma=0.001251 ! Fit after self-cal, rms=0.193102Jy sigma=0.001250 ! Inverting map ! Your choice of large map pixels excluded 5.24% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 48 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.95 FD 1.00 GC 1.05 KP 1.11 ! LA 1.02 NL 1.01 OV 1.00 PT 1.04 ! SC 1.01 WF 1.03 HH 1.00* KK 1.07 ! MA 0.92 MC 0.92 MK 1.04 NY 0.96 ! ON 0.97 TS 1.03 WZ 0.95 HN 0.74 ! ! A total of 186 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 0.96 GC 1.06 KP 1.02 ! LA 1.02 NL 1.02 OV 1.00 PT 0.99 ! SC 1.04 WF 1.06 HH 1.00* KK 1.08 ! MA 0.95 MC 1.01 MK 1.04 NY 0.98 ! ON 0.97 TS 1.05 WZ 1.03 HN 0.65 ! ! A total of 90 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.00 GC 1.04 KP 1.01 ! LA 1.01 NL 0.98 OV 0.97 PT 1.01 ! SC 1.14 WF 1.07 HH 1.00* KK 1.03 ! MA 1.19 MC 1.18 MK 0.99 NY 0.99 ! ON 0.98 TS 1.06 WZ 1.01 HN 0.72 ! ! ! Correcting IF 2. ! A total of 75 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.94 FD 1.00 GC 1.05 KP 1.06 ! LA 0.98 NL 1.02 OV 0.98 PT 1.00 ! SC 1.01 WF 1.01 HH 1.00* KK 1.07 ! MA 0.93 MC 0.94 MK 1.10 NY 1.00 ! ON 0.97 TS 1.05 WZ 0.92 HN 0.78 ! ! A total of 189 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 0.95 GC 1.05 KP 0.99 ! LA 0.98 NL 1.04 OV 0.98 PT 0.95 ! SC 1.01 WF 1.06 HH 1.00* KK 1.09 ! MA 0.94 MC 1.02 MK 1.07 NY 1.02 ! ON 0.95 TS 1.04 WZ 1.02 HN 0.69 ! ! A total of 93 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 0.98 GC 1.01 KP 0.97 ! LA 0.97 NL 1.02 OV 0.95 PT 0.96 ! SC 1.11 WF 1.05 HH 1.00* KK 1.04 ! MA 1.12 MC 1.19 MK 1.02 NY 1.03 ! ON 0.97 TS 1.06 WZ 1.02 HN 0.76 ! ! ! Correcting IF 3. ! A total of 69 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 1.01 GC 1.02 KP 1.05 ! LA 0.96 NL 0.96 OV 0.99 PT 1.01 ! SC 0.99 WF 1.01 HH 1.00* KK 1.05 ! MA 0.88 MC 0.89 MK 1.02 NY 0.98 ! ON 0.96 TS 1.04 WZ 0.97 HN 0.76 ! ! A total of 174 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 FD 0.97 GC 1.04 KP 0.99 ! LA 0.97 NL 0.98 OV 0.97 PT 0.96 ! SC 1.02 WF 1.04 HH 1.00* KK 1.02 ! MA 0.90 MC 0.97 MK 1.02 NY 1.06 ! ON 0.94 TS 1.05 WZ 1.04 HN 0.71 ! ! A total of 90 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.04 FD 1.00 GC 1.01 KP 0.98 ! LA 0.94 NL 0.95 OV 0.94 PT 0.98 ! SC 1.11 WF 1.04 HH 1.00* KK 0.99 ! MA 1.03 MC 1.18 MK 0.97 NY 1.05 ! ON 0.97 TS 1.06 WZ 1.03 HN 0.84 ! ! ! Correcting IF 4. ! A total of 39 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.93 FD 0.99 GC 1.01 KP 1.04 ! LA 0.96 NL 0.98 OV 0.98 PT 1.02 ! SC 1.05 WF 1.03 HH 1.00* KK 1.04 ! MA 0.88 MC 0.86 MK 1.02 NY 0.99 ! ON 0.95 TS 1.02 WZ 0.95 HN 0.75 ! ! A total of 165 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 FD 0.95 GC 1.03 KP 0.96 ! LA 0.98 NL 0.99 OV 0.98 PT 0.98 ! SC 1.07 WF 1.05 HH 1.00* KK 1.04 ! MA 0.90 MC 0.98 MK 1.04 NY 1.02 ! ON 0.94 TS 1.04 WZ 1.02 HN 0.66 ! ! A total of 90 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 0.98 GC 0.99 KP 0.95 ! LA 0.97 NL 0.97 OV 0.95 PT 0.98 ! SC 1.17 WF 1.04 HH 1.00* KK 1.02 ! MA 1.00 MC 1.17 MK 0.97 NY 1.05 ! ON 0.97 TS 1.05 WZ 1.01 HN 0.75 ! ! ! Fit before self-cal, rms=0.193102Jy sigma=0.001250 ! Fit after self-cal, rms=0.188788Jy sigma=0.001224 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec ! Estimated beam: bmin=0.656 mas, bmaj=0.6877 mas, bpa=16.02 degrees ! Estimated noise=208.486 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 = 6.49829e-05 Jy ! Component: 100 - total flux cleaned = 0.000433619 Jy ! Component: 150 - total flux cleaned = 0.000659193 Jy ! Component: 200 - total flux cleaned = 0.000722889 Jy ! Total flux subtracted in 200 components = 0.000722889 Jy ! Clean residual min=-0.002439 max=0.002808 Jy/beam ! Clean residual mean=-0.000028 rms=0.000590 Jy/beam ! Combined flux in latest and established models = 0.58924 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 72 components and 0.58924 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.188707Jy sigma=0.001223 ! Fit after self-cal, rms=0.188691Jy sigma=0.001223 ! Inverting map ! Your choice of large map pixels excluded 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 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=0.188691Jy sigma=0.001223 ! Fit after self-cal, rms=0.187688Jy sigma=0.001196 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec ! Estimated beam: bmin=0.6535 mas, bmaj=0.6911 mas, bpa=13.87 degrees ! Estimated noise=208.478 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00152332 Jy ! Component: 100 - total flux cleaned = 0.00187439 Jy ! Component: 150 - total flux cleaned = 0.00206445 Jy ! Component: 200 - total flux cleaned = 0.00222408 Jy ! Total flux subtracted in 200 components = 0.00222408 Jy ! Clean residual min=-0.001392 max=0.001660 Jy/beam ! Clean residual mean=-0.000002 rms=0.000309 Jy/beam ! Combined flux in latest and established models = 0.591464 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 77 components and 0.591464 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.187656Jy sigma=0.001196 ! Fit after self-cal, rms=0.187702Jy sigma=0.001196 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 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 (-5.6, -1). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00131315 Jy ! Component: 100 - total flux cleaned = 0.00186127 Jy ! Component: 150 - total flux cleaned = 0.00208724 Jy ! Component: 200 - total flux cleaned = 0.00221967 Jy ! Total flux subtracted in 200 components = 0.00221967 Jy ! Clean residual min=-0.001334 max=0.001300 Jy/beam ! Clean residual mean=-0.000005 rms=0.000298 Jy/beam ! Combined flux in latest and established models = 0.593683 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 86 components and 0.593684 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.187683Jy sigma=0.001196 ! Fit after self-cal, rms=0.187680Jy sigma=0.001196 ! Inverting map ! Your choice of large map pixels excluded 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec ! Added new window around map position (-3.6, -2.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000969611 Jy ! Component: 100 - total flux cleaned = 0.00129757 Jy ! Component: 150 - total flux cleaned = 0.00135986 Jy ! Component: 200 - total flux cleaned = 0.00138901 Jy ! Total flux subtracted in 200 components = 0.00138901 Jy ! Clean residual min=-0.001276 max=0.001195 Jy/beam ! Clean residual mean=-0.000006 rms=0.000293 Jy/beam ! Combined flux in latest and established models = 0.595073 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 97 components and 0.595073 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.187667Jy sigma=0.001196 ! Fit after self-cal, rms=0.187665Jy sigma=0.001196 ! Inverting map ! Your choice of large map pixels excluded 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 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=0.187665Jy sigma=0.001196 ! Fit after self-cal, rms=0.188457Jy sigma=0.001194 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec ! Estimated beam: bmin=0.6531 mas, bmaj=0.6917 mas, bpa=13.87 degrees ! Estimated noise=208.657 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000693495 Jy ! Component: 100 - total flux cleaned = 0.00109554 Jy ! Component: 150 - total flux cleaned = 0.00128396 Jy ! Component: 200 - total flux cleaned = 0.00142423 Jy ! Total flux subtracted in 200 components = 0.00142423 Jy ! Clean residual min=-0.001138 max=0.001197 Jy/beam ! Clean residual mean=0.000003 rms=0.000282 Jy/beam ! Combined flux in latest and established models = 0.596497 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 103 components and 0.596497 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.188441Jy sigma=0.001194 ! Fit after self-cal, rms=0.188445Jy sigma=0.001194 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 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 = 0.000155031 Jy ! Component: 100 - total flux cleaned = 0.000233311 Jy ! Component: 150 - total flux cleaned = 0.00028185 Jy ! Component: 200 - total flux cleaned = 0.000304166 Jy ! Total flux subtracted in 200 components = 0.000304166 Jy ! Clean residual min=-0.001130 max=0.001187 Jy/beam ! Clean residual mean=0.000003 rms=0.000280 Jy/beam ! Combined flux in latest and established models = 0.596801 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 105 components and 0.596801 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.188437Jy sigma=0.001194 ! Fit after self-cal, rms=0.188436Jy sigma=0.001194 ! Inverting map ! Your choice of large map pixels excluded 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 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=0.188436Jy sigma=0.001194 ! Fit after self-cal, rms=0.187941Jy sigma=0.001194 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec ! Estimated beam: bmin=2.527 mas, bmaj=2.818 mas, bpa=-53.2 degrees ! Estimated noise=329.181 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00109881 Jy ! Component: 100 - total flux cleaned = 0.00127794 Jy ! Component: 150 - total flux cleaned = 0.00137757 Jy ! Component: 200 - total flux cleaned = 0.00139442 Jy ! Total flux subtracted in 200 components = 0.00139442 Jy ! Clean residual min=-0.001440 max=0.001736 Jy/beam ! Clean residual mean=0.000009 rms=0.000441 Jy/beam ! Combined flux in latest and established models = 0.598195 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 113 components and 0.598195 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.187939Jy sigma=0.001194 ! Fit after self-cal, rms=0.187934Jy sigma=0.001194 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 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 = 0.000229081 Jy ! Component: 100 - total flux cleaned = 0.00024392 Jy ! Component: 150 - total flux cleaned = 0.000244574 Jy ! Component: 200 - total flux cleaned = 0.000254275 Jy ! Total flux subtracted in 200 components = 0.000254275 Jy ! Clean residual min=-0.001440 max=0.001734 Jy/beam ! Clean residual mean=0.000008 rms=0.000441 Jy/beam ! Combined flux in latest and established models = 0.59845 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 115 components and 0.598449 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.187935Jy sigma=0.001194 ! Fit after self-cal, rms=0.187936Jy sigma=0.001194 ! Inverting map ! Your choice of large map pixels excluded 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 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 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec ! Estimated beam: bmin=0.6531 mas, bmaj=0.6921 mas, bpa=13.81 degrees ! Estimated noise=208.867 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6531 x 0.6921 at 13.81 degrees (North through East) ! Clean map min=-0.00092311 max=0.41671 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 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 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec ! Estimated beam: bmin=0.5361 mas, bmaj=0.5747 mas, bpa=8.384 degrees ! Estimated noise=438.839 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.30931 Jy ! Component: 100 - total flux cleaned = 0.387843 Jy ! Component: 150 - total flux cleaned = 0.426464 Jy ! Component: 200 - total flux cleaned = 0.452413 Jy ! Total flux subtracted in 200 components = 0.452413 Jy ! Clean residual min=-0.002628 max=0.015112 Jy/beam ! Clean residual mean=0.000014 rms=0.000842 Jy/beam ! Combined flux in latest and established models = 0.452413 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 0.452413 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec ! Estimated beam: bmin=0.6531 mas, bmaj=0.6921 mas, bpa=13.81 degrees ! Estimated noise=208.867 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 = 0.0457713 Jy ! Component: 100 - total flux cleaned = 0.0730214 Jy ! Component: 150 - total flux cleaned = 0.0908908 Jy ! Component: 200 - total flux cleaned = 0.103349 Jy ! Total flux subtracted in 200 components = 0.103349 Jy ! Clean residual min=-0.001733 max=0.007259 Jy/beam ! Clean residual mean=0.000054 rms=0.000740 Jy/beam ! Combined flux in latest and established models = 0.555762 Jy ! Adding 43 model components to the UV plane model. ! The established model now contains 45 components and 0.555762 Jy ! Inverting map ! Your choice of large map pixels excluded 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec ! Added new window around map position (-1.4, -0.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00904087 Jy ! Component: 100 - total flux cleaned = 0.0157355 Jy ! Component: 150 - total flux cleaned = 0.020856 Jy ! Component: 200 - total flux cleaned = 0.0248379 Jy ! Total flux subtracted in 200 components = 0.0248379 Jy ! Clean residual min=-0.001210 max=0.002645 Jy/beam ! Clean residual mean=0.000023 rms=0.000385 Jy/beam ! Combined flux in latest and established models = 0.5806 Jy ! Adding 54 model components to the UV plane model. ! The established model now contains 78 components and 0.5806 Jy ! Inverting map ! Your choice of large map pixels excluded 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 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 = 0.00323401 Jy ! Component: 100 - total flux cleaned = 0.00582052 Jy ! Component: 150 - total flux cleaned = 0.00793865 Jy ! Component: 200 - total flux cleaned = 0.00969421 Jy ! Total flux subtracted in 200 components = 0.00969421 Jy ! Clean residual min=-0.001086 max=0.001400 Jy/beam ! Clean residual mean=0.000012 rms=0.000301 Jy/beam ! Combined flux in latest and established models = 0.590294 Jy ! Adding 53 model components to the UV plane model. ! The established model now contains 103 components and 0.590294 Jy ! Inverting map ! Your choice of large map pixels excluded 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec ! Added new window around map position (-6.6, -2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00154421 Jy ! Component: 100 - total flux cleaned = 0.00280186 Jy ! Component: 150 - total flux cleaned = 0.00386487 Jy ! Component: 200 - total flux cleaned = 0.00476747 Jy ! Total flux subtracted in 200 components = 0.00476747 Jy ! Clean residual min=-0.001080 max=0.001143 Jy/beam ! Clean residual mean=0.000006 rms=0.000279 Jy/beam ! Combined flux in latest and established models = 0.595062 Jy ! Adding 49 model components to the UV plane model. ! The established model now contains 117 components and 0.595061 Jy ! Inverting map ! Your choice of large map pixels excluded 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 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 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec ! Estimated beam: bmin=2.527 mas, bmaj=2.818 mas, bpa=-53.2 degrees ! Estimated noise=329.181 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00183995 Jy ! Component: 100 - total flux cleaned = 0.00288371 Jy ! Component: 150 - total flux cleaned = 0.00350896 Jy ! Component: 200 - total flux cleaned = 0.00367552 Jy ! Total flux subtracted in 200 components = 0.00367552 Jy ! Clean residual min=-0.001383 max=0.001700 Jy/beam ! Clean residual mean=0.000008 rms=0.000430 Jy/beam ! Combined flux in latest and established models = 0.598737 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 = 0.000134793 Jy ! Component: 100 - total flux cleaned = 0.000232588 Jy ! Component: 150 - total flux cleaned = 0.000313476 Jy ! Component: 200 - total flux cleaned = 0.000348224 Jy ! Total flux subtracted in 200 components = 0.000348224 Jy ! Clean residual min=-0.001368 max=0.001675 Jy/beam ! Clean residual mean=0.000007 rms=0.000427 Jy/beam ! Combined flux in latest and established models = 0.599085 Jy ! Adding 57 model components to the UV plane model. ! The established model now contains 155 components and 0.599085 Jy ! Inverting map ! Your choice of large map pixels excluded 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec ! Estimated beam: bmin=0.6531 mas, bmaj=0.6921 mas, bpa=13.81 degrees ! Estimated noise=208.867 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000957112 Jy ! Component: 100 - total flux cleaned = -0.000982714 Jy ! Component: 150 - total flux cleaned = -0.000961942 Jy ! Component: 200 - total flux cleaned = -0.000923808 Jy ! Total flux subtracted in 200 components = -0.000923808 Jy ! Clean residual min=-0.001095 max=0.001142 Jy/beam ! Clean residual mean=0.000003 rms=0.000271 Jy/beam ! Combined flux in latest and established models = 0.598162 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 161 components and 0.598162 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.187935Jy sigma=0.001194 ! Fit after self-cal, rms=0.187926Jy sigma=0.001194 wmodel J0102+5824_X_2000_03_13_pus_map.mod ! Writing 161 model components to file: J0102+5824_X_2000_03_13_pus_map.mod wobs J0102+5824_X_2000_03_13_pus_uvs.fits ! Writing UV FITS file: J0102+5824_X_2000_03_13_pus_uvs.fits wwins J0102+5824_X_2000_03_13_pus_map.win ! wwins: Wrote 10 windows to J0102+5824_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 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000305773 Jy ! Component: 100 - total flux cleaned = 0.000406032 Jy ! Component: 150 - total flux cleaned = 0.000387833 Jy ! Component: 200 - total flux cleaned = 0.000369633 Jy ! Component: 250 - total flux cleaned = 0.000333735 Jy ! Component: 300 - total flux cleaned = 0.000316097 Jy ! Component: 350 - total flux cleaned = 0.000247157 Jy ! Component: 400 - total flux cleaned = 0.000281363 Jy ! Component: 450 - total flux cleaned = 0.000331573 Jy ! Component: 500 - total flux cleaned = 0.000314629 Jy ! Component: 550 - total flux cleaned = 0.000265188 Jy ! Component: 600 - total flux cleaned = 0.00024881 Jy ! Component: 650 - total flux cleaned = 0.000184555 Jy ! Component: 700 - total flux cleaned = 0.000152815 Jy ! Component: 750 - total flux cleaned = 0.000137032 Jy ! Component: 800 - total flux cleaned = 5.8775e-05 Jy ! Component: 850 - total flux cleaned = 2.78137e-05 Jy ! Component: 900 - total flux cleaned = 7.40527e-05 Jy ! Component: 950 - total flux cleaned = 2.78053e-05 Jy ! Component: 1000 - total flux cleaned = -2.56131e-06 Jy ! Component: 1050 - total flux cleaned = 1.26291e-05 Jy ! Component: 1100 - total flux cleaned = -1.75237e-05 Jy ! Component: 1150 - total flux cleaned = -2.5483e-06 Jy ! Component: 1200 - total flux cleaned = -3.24371e-05 Jy ! Component: 1250 - total flux cleaned = -4.71743e-05 Jy ! Component: 1300 - total flux cleaned = -6.19421e-05 Jy ! Component: 1350 - total flux cleaned = -6.19778e-05 Jy ! Component: 1400 - total flux cleaned = -7.64975e-05 Jy ! Component: 1450 - total flux cleaned = -0.000119865 Jy ! Component: 1500 - total flux cleaned = -9.10236e-05 Jy ! Component: 1550 - total flux cleaned = -1.91207e-05 Jy ! Component: 1600 - total flux cleaned = -6.2058e-05 Jy ! Component: 1650 - total flux cleaned = -6.2167e-05 Jy ! Component: 1700 - total flux cleaned = -7.63274e-05 Jy ! Component: 1750 - total flux cleaned = -9.0418e-05 Jy ! Component: 1800 - total flux cleaned = -7.63692e-05 Jy ! Component: 1850 - total flux cleaned = -0.000118456 Jy ! Component: 1900 - total flux cleaned = -9.05083e-05 Jy ! Component: 1950 - total flux cleaned = -0.000118246 Jy ! Component: 2000 - total flux cleaned = -0.000159762 Jy ! Total flux subtracted in 2048 components = -0.00013221 Jy ! Clean residual min=-0.000735 max=0.000699 Jy/beam ! Clean residual mean=-0.000001 rms=0.000247 Jy/beam ! Combined flux in latest and established models = 0.598029 Jy keep ! Adding 191 model components to the UV plane model. ! The established model now contains 352 components and 0.59803 Jy ![Exited script file: muppet] wmap "J0102+5824_X_2000_03_13_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6531 x 0.6921 at 13.81 degrees (North through East) ! Clean map min=-0.00083845 max=0.41825 Jy/beam ! Writing clean map to FITS file: J0102+5824_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 0.418249 invert ! Inverting map ! Your choice of large map pixels excluded 5.27% of the data. ! The x-axis pixel size should ideally be below 0.156 milli-arcsec ! The y-axis pixel size should ideally be below 0.1673 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000247248 device "J0102+5824_X_2000_03_13_pus\_map.eps/VPS" ! Attempting to open device: 'J0102+5824_X_2000_03_13_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.177345 0.177345 0.35469 0.70938 1.41876 2.83752 5.67504 11.3501 22.7002 45.4003 90.8006 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0007 print "peak=",int(1000*peak_flux)/1000 ! peak= 0.418 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6531 x 0.6921 at 13.81 degrees (North through East) ! Clean map min=-0.00083845 max=0.41825 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. quit ! Quitting program ! Log file J0102+5824_X_2000_03_13_pus_uvs.log closed on Wed Apr 3 15:24:51 2013