! Started logfile: J0854+2006_X_2001_03_12_pus_uvs.log on Wed Jan 2 19:53:19 2013 obs J0854+2006_X_2001_03_12_pus_uva.fits ! Reading UV FITS file: J0854+2006_X_2001_03_12_pus_uva.fits ! AN table 1: 13 integrations on 136 of 136 possible baselines. ! AN table 2: 88 integrations on 136 of 136 possible baselines. ! AN table 3: 222 integrations on 136 of 136 possible baselines. ! AN table 4: 175 integrations on 136 of 136 possible baselines. ! Apparent sampling: 0.0921923 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0854+2006 ! ! 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 1749 lines of history. ! ! Reading 24976 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 J0854+2006_X_2001_03_12_pus] integer clean_niter clean_niter = 100 float clean_gain clean_gain = 0.03 float dynam dynam = 6.0 float soltime1 soltime1 = 120 float soltime2 soltime2 = 20 float thresh thresh = 0.5 float win_mult win_mult = 1.8 float time_av time_av = 16 float old_peak float new_peak float flux_cutoff mapsize field_size, field_cell ! Map grid = 512x512 pixels with 0.200x0.200 milli-arcsec cellsize. startmod ! Applying default point source starting model. ! Performing phase self-cal ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 1 Jy ! ! Correcting IF 1. ! A total of 188 telescope corrections were flagged in sub-array 1. ! A total of 1059 telescope corrections were flagged in sub-array 2. ! A total of 2663 telescope corrections were flagged in sub-array 3. ! A total of 2397 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 188 telescope corrections were flagged in sub-array 1. ! A total of 1056 telescope corrections were flagged in sub-array 2. ! A total of 2663 telescope corrections were flagged in sub-array 3. ! A total of 2397 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 188 telescope corrections were flagged in sub-array 1. ! A total of 1056 telescope corrections were flagged in sub-array 2. ! A total of 2663 telescope corrections were flagged in sub-array 3. ! A total of 2397 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 188 telescope corrections were flagged in sub-array 1. ! A total of 1056 telescope corrections were flagged in sub-array 2. ! A total of 2663 telescope corrections were flagged in sub-array 3. ! A total of 2397 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=1.345267Jy sigma=0.011476 ! Fit after self-cal, rms=0.858218Jy sigma=0.006997 ! 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 5.59% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec ! Estimated beam: bmin=0.5021 mas, bmaj=1.113 mas, bpa=-3.242 degrees ! Estimated noise=964.861 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 = 1.24218 Jy ! Component: 100 - total flux cleaned = 1.63646 Jy ! Total flux subtracted in 100 components = 1.63646 Jy ! Clean residual min=-0.050913 max=0.190432 Jy/beam ! Clean residual mean=-0.000221 rms=0.012537 Jy/beam ! Combined flux in latest and established models = 1.63646 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 1.63646 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.494214Jy sigma=0.003470 ! Fit after self-cal, rms=0.493421Jy sigma=0.003467 ! Inverting map ! Your choice of large map pixels excluded 5.59% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.217874 Jy ! Component: 100 - total flux cleaned = 0.341018 Jy ! Total flux subtracted in 100 components = 0.341018 Jy ! Clean residual min=-0.027054 max=0.061172 Jy/beam ! Clean residual mean=-0.000230 rms=0.006617 Jy/beam ! Combined flux in latest and established models = 1.97748 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 11 components and 1.97748 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.386693Jy sigma=0.002067 ! Fit after self-cal, rms=0.386172Jy sigma=0.002066 ! Inverting map ! Your choice of large map pixels excluded 5.59% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0729427 Jy ! Component: 100 - total flux cleaned = 0.117507 Jy ! Total flux subtracted in 100 components = 0.117507 Jy ! Clean residual min=-0.025022 max=0.032056 Jy/beam ! Clean residual mean=-0.000232 rms=0.005539 Jy/beam ! Combined flux in latest and established models = 2.09499 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 13 components and 2.09499 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.376990Jy sigma=0.001850 ! Fit after self-cal, rms=0.376909Jy sigma=0.001850 ! Inverting map ! Your choice of large map pixels excluded 5.59% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 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 5.59% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec ! Estimated beam: bmin=0.6323 mas, bmaj=1.123 mas, bpa=-7.005 degrees ! Estimated noise=636.29 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 = 0.021121 Jy ! Component: 100 - total flux cleaned = 0.0216966 Jy ! Component: 150 - total flux cleaned = 0.0208314 Jy ! Component: 200 - total flux cleaned = 0.0204302 Jy ! Total flux subtracted in 200 components = 0.0204302 Jy ! Clean residual min=-0.031740 max=0.033793 Jy/beam ! Clean residual mean=-0.000296 rms=0.009090 Jy/beam ! Combined flux in latest and established models = 2.11542 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 20 components and 2.11542 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.374842Jy sigma=0.001823 ! Fit after self-cal, rms=0.374803Jy sigma=0.001822 ! Inverting map ! Your choice of large map pixels excluded 5.59% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 33 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* HH 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MC 0.00* MK 0.00* NL 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TS 0.00* ! WZ 0.00* ! ! A total of 69 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 FD 1.10 HH 1.10 HN 1.01 ! KK 1.17 KP 1.00* LA 1.07 MA 1.05 ! MC 1.01 MK 1.00* NL 1.03 ON 0.90 ! OV 1.00* PT 1.02 SC 1.00* TS 1.05 ! WZ 0.98 ! ! A total of 195 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 0.99 HH 1.00* HN 1.01 ! KK 0.93 KP 1.01 LA 0.93 MA 1.22 ! MC 1.10 MK 0.99 NL 1.00 ON 1.29 ! OV 0.97 PT 0.93 SC 1.04 TS 0.97 ! WZ 1.04 ! ! A total of 18 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.00* HH 1.03 HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MA 1.03 ! MC 1.00 MK 1.00* NL 1.00* ON 1.10 ! OV 1.00* PT 1.00* SC 1.00* TS 1.05 ! WZ 1.08 ! ! ! Correcting IF 2. ! A total of 33 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* HH 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MC 0.00* MK 0.00* NL 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TS 0.00* ! WZ 0.00* ! ! A total of 72 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 FD 1.07 HH 1.09 HN 1.01 ! KK 1.16 KP 1.00* LA 1.06 MA 1.02 ! MC 1.02 MK 1.00* NL 1.00 ON 0.88 ! OV 1.00* PT 1.06 SC 1.00* TS 1.11 ! WZ 1.00 ! ! A total of 195 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 0.98 HH 1.00* HN 1.00 ! KK 0.92 KP 0.95 LA 0.93 MA 1.23 ! MC 1.12 MK 0.99 NL 0.96 ON 1.32 ! OV 0.96 PT 0.97 SC 1.02 TS 0.98 ! WZ 1.05 ! ! A total of 18 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.00* HH 1.02 HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MA 1.02 ! MC 1.01 MK 1.00* NL 1.00* ON 1.01 ! OV 1.00* PT 1.00* SC 1.00* TS 1.06 ! WZ 1.08 ! ! ! Correcting IF 3. ! A total of 33 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* HH 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MC 0.00* MK 0.00* NL 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TS 0.00* ! WZ 0.00* ! ! A total of 72 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.08 FD 1.05 HH 1.16 HN 1.01 ! KK 1.22 KP 1.00* LA 1.09 MA 1.07 ! MC 1.08 MK 1.00* NL 1.03 ON 0.93 ! OV 1.00* PT 1.11 SC 1.00* TS 1.06 ! WZ 1.04 ! ! A total of 195 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 FD 0.96 HH 1.00* HN 1.01 ! KK 0.99 KP 0.93 LA 0.95 MA 1.40 ! MC 1.22 MK 1.01 NL 1.00 ON 1.38 ! OV 1.00 PT 1.00 SC 1.06 TS 0.97 ! WZ 1.07 ! ! A total of 18 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.00* HH 1.05 HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MA 1.07 ! MC 1.05 MK 1.00* NL 1.00* ON 1.15 ! OV 1.00* PT 1.00* SC 1.00* TS 1.08 ! WZ 1.12 ! ! ! Correcting IF 4. ! A total of 33 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* HH 0.00* HN 0.00* ! KK 0.00* KP 0.00* LA 0.00* MA 0.00* ! MC 0.00* MK 0.00* NL 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TS 0.00* ! WZ 0.00* ! ! A total of 72 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.06 FD 1.04 HH 1.10 HN 1.03 ! KK 1.17 KP 1.00* LA 1.05 MA 1.15 ! MC 1.01 MK 1.00* NL 1.03 ON 0.90 ! OV 1.00* PT 1.09 SC 1.00* TS 1.09 ! WZ 1.06 ! ! A total of 195 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 0.96 HH 1.00* HN 1.01 ! KK 0.95 KP 0.95 LA 0.92 MA 1.46 ! MC 1.19 MK 1.05 NL 1.01 ON 1.39 ! OV 0.98 PT 0.99 SC 1.11 TS 0.98 ! WZ 1.09 ! ! A total of 18 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.00* HH 1.01 HN 1.00* ! KK 1.00* KP 1.00* LA 1.00* MA 1.13 ! MC 1.01 MK 1.00* NL 1.00* ON 1.08 ! OV 1.00* PT 1.00* SC 1.00* TS 1.09 ! WZ 1.13 ! ! ! Fit before self-cal, rms=0.374803Jy sigma=0.001822 ! Fit after self-cal, rms=0.374992Jy sigma=0.001487 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec ! Estimated beam: bmin=0.6318 mas, bmaj=1.143 mas, bpa=-6.742 degrees ! Estimated noise=665.129 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, -0.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0195337 Jy ! Component: 100 - total flux cleaned = 0.0208863 Jy ! Component: 150 - total flux cleaned = 0.0214463 Jy ! Component: 200 - total flux cleaned = 0.0223373 Jy ! Total flux subtracted in 200 components = 0.0223373 Jy ! Clean residual min=-0.012969 max=0.019569 Jy/beam ! Clean residual mean=-0.000080 rms=0.003364 Jy/beam ! Combined flux in latest and established models = 2.13775 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 36 components and 2.13775 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.372581Jy sigma=0.001462 ! Fit after self-cal, rms=0.372785Jy sigma=0.001459 ! Inverting map ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec ! Added new window around map position (-3.2, -1.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.020523 Jy ! Component: 100 - total flux cleaned = 0.0246672 Jy ! Component: 150 - total flux cleaned = 0.0268903 Jy ! Component: 200 - total flux cleaned = 0.0281698 Jy ! Total flux subtracted in 200 components = 0.0281698 Jy ! Clean residual min=-0.011796 max=0.012461 Jy/beam ! Clean residual mean=-0.000041 rms=0.003030 Jy/beam ! Combined flux in latest and established models = 2.16592 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 51 components and 2.16592 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.371647Jy sigma=0.001445 ! Fit after self-cal, rms=0.371424Jy sigma=0.001443 ! Inverting map ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 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=0.371424Jy sigma=0.001443 ! Fit after self-cal, rms=0.356813Jy sigma=0.001297 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec ! Estimated beam: bmin=0.6315 mas, bmaj=1.141 mas, bpa=-6.755 degrees ! Estimated noise=664.335 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0109996 Jy ! Component: 100 - total flux cleaned = 0.0137456 Jy ! Component: 150 - total flux cleaned = 0.0145216 Jy ! Component: 200 - total flux cleaned = 0.0150358 Jy ! Total flux subtracted in 200 components = 0.0150358 Jy ! Clean residual min=-0.005576 max=0.005718 Jy/beam ! Clean residual mean=0.000009 rms=0.001242 Jy/beam ! Combined flux in latest and established models = 2.18096 Jy selfcal ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 71 components and 2.18096 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.356369Jy sigma=0.001291 ! Fit after self-cal, rms=0.356365Jy sigma=0.001290 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 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 = 0.00426212 Jy ! Component: 100 - total flux cleaned = 0.00441204 Jy ! Component: 150 - total flux cleaned = 0.00467162 Jy ! Component: 200 - total flux cleaned = 0.00490966 Jy ! Total flux subtracted in 200 components = 0.00490966 Jy ! Clean residual min=-0.006417 max=0.005186 Jy/beam ! Clean residual mean=0.000016 rms=0.001189 Jy/beam ! Combined flux in latest and established models = 2.18587 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 77 components and 2.18587 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.356206Jy sigma=0.001289 ! Fit after self-cal, rms=0.356192Jy sigma=0.001288 ! Inverting map ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 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=0.356192Jy sigma=0.001288 ! Fit after self-cal, rms=0.357166Jy sigma=0.001287 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec ! Estimated beam: bmin=0.6316 mas, bmaj=1.14 mas, bpa=-6.754 degrees ! Estimated noise=665.45 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00594411 Jy ! Component: 100 - total flux cleaned = 0.0083562 Jy ! Component: 150 - total flux cleaned = 0.008846 Jy ! Component: 200 - total flux cleaned = 0.00907308 Jy ! Total flux subtracted in 200 components = 0.00907308 Jy ! Clean residual min=-0.005197 max=0.005071 Jy/beam ! Clean residual mean=-0.000000 rms=0.001094 Jy/beam ! Combined flux in latest and established models = 2.19494 Jy selfcal ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 83 components and 2.19494 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.357052Jy sigma=0.001285 ! Fit after self-cal, rms=0.357030Jy sigma=0.001285 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 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 = 0.00212661 Jy ! Component: 100 - total flux cleaned = 0.00243883 Jy ! Component: 150 - total flux cleaned = 0.00253202 Jy ! Component: 200 - total flux cleaned = 0.00262036 Jy ! Total flux subtracted in 200 components = 0.00262036 Jy ! Clean residual min=-0.005583 max=0.004872 Jy/beam ! Clean residual mean=0.000003 rms=0.001074 Jy/beam ! Combined flux in latest and established models = 2.19756 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 88 components and 2.19756 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.356979Jy sigma=0.001284 ! Fit after self-cal, rms=0.356974Jy sigma=0.001284 ! Inverting map ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 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=0.356974Jy sigma=0.001284 ! Fit after self-cal, rms=0.357740Jy sigma=0.001284 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec ! Estimated beam: bmin=2.336 mas, bmaj=3.055 mas, bpa=-17.74 degrees ! Estimated noise=933.513 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00551685 Jy ! Component: 100 - total flux cleaned = 0.00825822 Jy ! Component: 150 - total flux cleaned = 0.0098225 Jy ! Component: 200 - total flux cleaned = 0.0106564 Jy ! Total flux subtracted in 200 components = 0.0106564 Jy ! Clean residual min=-0.004521 max=0.004224 Jy/beam ! Clean residual mean=-0.000002 rms=0.001408 Jy/beam ! Combined flux in latest and established models = 2.20822 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 103 components and 2.20822 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.357715Jy sigma=0.001283 ! Fit after self-cal, rms=0.357720Jy sigma=0.001283 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 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 = 0.00135101 Jy ! Component: 100 - total flux cleaned = 0.00169449 Jy ! Component: 150 - total flux cleaned = 0.00189285 Jy ! Component: 200 - total flux cleaned = 0.00205566 Jy ! Total flux subtracted in 200 components = 0.00205566 Jy ! Clean residual min=-0.004685 max=0.003951 Jy/beam ! Clean residual mean=0.000005 rms=0.001390 Jy/beam ! Combined flux in latest and established models = 2.21027 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 113 components and 2.21027 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.357788Jy sigma=0.001284 ! Fit after self-cal, rms=0.357793Jy sigma=0.001284 ! Inverting map ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 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 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec ! Estimated beam: bmin=0.6317 mas, bmaj=1.139 mas, bpa=-6.748 degrees ! Estimated noise=666.481 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6317 x 1.139 at -6.748 degrees (North through East) ! Clean map min=-0.0034282 max=1.7118 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=0.357793Jy sigma=0.001284 ! Fit after self-cal, rms=0.727247Jy sigma=0.001144 ! Inverting map and beam ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec ! Estimated beam: bmin=0.632 mas, bmaj=1.139 mas, bpa=-6.683 degrees ! Estimated noise=667.073 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00220774 Jy ! Component: 100 - total flux cleaned = 0.00255219 Jy ! Component: 150 - total flux cleaned = 0.00265494 Jy ! Component: 200 - total flux cleaned = 0.0026526 Jy ! Total flux subtracted in 200 components = 0.0026526 Jy ! Clean residual min=-0.004584 max=0.004074 Jy/beam ! Clean residual mean=-0.000000 rms=0.000961 Jy/beam ! Combined flux in latest and established models = 2.21293 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 116 components and 2.21293 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.727204Jy sigma=0.001143 ! Fit after self-cal, rms=0.727224Jy sigma=0.001143 ! Inverting map ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000132766 Jy ! Component: 100 - total flux cleaned = 0.000133646 Jy ! Component: 150 - total flux cleaned = 0.000133177 Jy ! Component: 200 - total flux cleaned = 0.000130761 Jy ! Total flux subtracted in 200 components = 0.000130761 Jy ! Clean residual min=-0.004548 max=0.004031 Jy/beam ! Clean residual mean=-0.000000 rms=0.000952 Jy/beam ! Combined flux in latest and established models = 2.21306 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 120 components and 2.21306 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.727208Jy sigma=0.001142 ! Fit after self-cal, rms=0.727194Jy sigma=0.001142 ! Inverting map ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.727194Jy sigma=0.001142 ! Fit after self-cal, rms=0.735598Jy sigma=0.001142 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 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec ! Estimated beam: bmin=0.507 mas, bmaj=1.132 mas, bpa=-3.19 degrees ! Estimated noise=990.606 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.25132 Jy ! Component: 100 - total flux cleaned = 1.63468 Jy ! Component: 150 - total flux cleaned = 1.84212 Jy ! Component: 200 - total flux cleaned = 1.95745 Jy ! Total flux subtracted in 200 components = 1.95745 Jy ! Clean residual min=-0.016341 max=0.056449 Jy/beam ! Clean residual mean=-0.000029 rms=0.004135 Jy/beam ! Combined flux in latest and established models = 1.95745 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 8 model components to the UV plane model. ! The established model now contains 8 components and 1.95745 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec ! Estimated beam: bmin=0.632 mas, bmaj=1.139 mas, bpa=-6.671 degrees ! Estimated noise=668.089 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 = 0.0944441 Jy ! Component: 100 - total flux cleaned = 0.14593 Jy ! Component: 150 - total flux cleaned = 0.179561 Jy ! Component: 200 - total flux cleaned = 0.202828 Jy ! Total flux subtracted in 200 components = 0.202828 Jy ! Clean residual min=-0.006561 max=0.013849 Jy/beam ! Clean residual mean=-0.000071 rms=0.002081 Jy/beam ! Combined flux in latest and established models = 2.16028 Jy ! Adding 28 model components to the UV plane model. ! The established model now contains 31 components and 2.16028 Jy ! Inverting map ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec ! Added new window around map position (-2.2, -0.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0164433 Jy ! Component: 100 - total flux cleaned = 0.0280564 Jy ! Component: 150 - total flux cleaned = 0.0365322 Jy ! Component: 200 - total flux cleaned = 0.0428604 Jy ! Total flux subtracted in 200 components = 0.0428604 Jy ! Clean residual min=-0.004489 max=0.005771 Jy/beam ! Clean residual mean=-0.000018 rms=0.001126 Jy/beam ! Combined flux in latest and established models = 2.20314 Jy ! Adding 34 model components to the UV plane model. ! The established model now contains 52 components and 2.20314 Jy ! Inverting map ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec ! Added new window around map position (-4.4, -1.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00594276 Jy ! Component: 100 - total flux cleaned = 0.0101365 Jy ! Component: 150 - total flux cleaned = 0.0119563 Jy ! Component: 200 - total flux cleaned = 0.0128316 Jy ! Total flux subtracted in 200 components = 0.0128316 Jy ! Clean residual min=-0.004420 max=0.004520 Jy/beam ! Clean residual mean=-0.000001 rms=0.000992 Jy/beam ! Combined flux in latest and established models = 2.21597 Jy ! Adding 30 model components to the UV plane model. ! The established model now contains 68 components and 2.21597 Jy ! Inverting map ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec ! Added new window around map position (-17.4, 1.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00218571 Jy ! Component: 100 - total flux cleaned = 0.00289025 Jy ! Component: 150 - total flux cleaned = 0.00332183 Jy ! Component: 200 - total flux cleaned = 0.00393917 Jy ! Total flux subtracted in 200 components = 0.00393917 Jy ! Clean residual min=-0.004275 max=0.004115 Jy/beam ! Clean residual mean=0.000003 rms=0.000965 Jy/beam ! Combined flux in latest and established models = 2.21991 Jy ! Adding 27 model components to the UV plane model. ! The established model now contains 76 components and 2.21991 Jy ! Inverting map ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 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 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec ! Estimated beam: bmin=2.335 mas, bmaj=3.053 mas, bpa=-17.73 degrees ! Estimated noise=936.101 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00150069 Jy ! Component: 100 - total flux cleaned = 0.00213831 Jy ! Component: 150 - total flux cleaned = 0.00270077 Jy ! Component: 200 - total flux cleaned = 0.00315019 Jy ! Total flux subtracted in 200 components = 0.00315019 Jy ! Clean residual min=-0.003676 max=0.003586 Jy/beam ! Clean residual mean=0.000017 rms=0.001129 Jy/beam ! Combined flux in latest and established models = 2.22306 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 = 0.000118836 Jy ! Component: 100 - total flux cleaned = 0.000200312 Jy ! Component: 150 - total flux cleaned = 0.000250984 Jy ! Component: 200 - total flux cleaned = 0.000322811 Jy ! Total flux subtracted in 200 components = 0.000322811 Jy ! Clean residual min=-0.003608 max=0.003590 Jy/beam ! Clean residual mean=0.000017 rms=0.001123 Jy/beam ! Combined flux in latest and established models = 2.22338 Jy ! Adding 25 model components to the UV plane model. ! The established model now contains 95 components and 2.22338 Jy ! Inverting map ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec ! Estimated beam: bmin=0.632 mas, bmaj=1.139 mas, bpa=-6.671 degrees ! Estimated noise=668.089 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0013059 Jy ! Component: 100 - total flux cleaned = -0.00150365 Jy ! Component: 150 - total flux cleaned = -0.00159285 Jy ! Component: 200 - total flux cleaned = -0.00141666 Jy ! Total flux subtracted in 200 components = -0.00141666 Jy ! Clean residual min=-0.003918 max=0.004000 Jy/beam ! Clean residual mean=0.000005 rms=0.000941 Jy/beam ! Combined flux in latest and established models = 2.22196 Jy selfcal ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 102 components and 2.22196 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.736889Jy sigma=0.001161 ! Fit after self-cal, rms=0.736984Jy sigma=0.001160 wmodel J0854+2006_X_2001_03_12_pus_map.mod ! Writing 102 model components to file: J0854+2006_X_2001_03_12_pus_map.mod wobs J0854+2006_X_2001_03_12_pus_uvs.fits ! Writing UV FITS file: J0854+2006_X_2001_03_12_pus_uvs.fits wwins J0854+2006_X_2001_03_12_pus_map.win ! wwins: Wrote 6 windows to J0854+2006_X_2001_03_12_pus_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.00029289 Jy ! Component: 100 - total flux cleaned = 0.00140804 Jy ! Component: 150 - total flux cleaned = 0.00248037 Jy ! Component: 200 - total flux cleaned = 0.00345617 Jy ! Component: 250 - total flux cleaned = 0.00427951 Jy ! Component: 300 - total flux cleaned = 0.00495938 Jy ! Component: 350 - total flux cleaned = 0.00568476 Jy ! Component: 400 - total flux cleaned = 0.00610127 Jy ! Component: 450 - total flux cleaned = 0.00662734 Jy ! Component: 500 - total flux cleaned = 0.00685816 Jy ! Component: 550 - total flux cleaned = 0.00719897 Jy ! Component: 600 - total flux cleaned = 0.00747933 Jy ! Component: 650 - total flux cleaned = 0.00775564 Jy ! Component: 700 - total flux cleaned = 0.0079746 Jy ! Component: 750 - total flux cleaned = 0.0082452 Jy ! Component: 800 - total flux cleaned = 0.00829847 Jy ! Component: 850 - total flux cleaned = 0.00840434 Jy ! Component: 900 - total flux cleaned = 0.00824666 Jy ! Component: 950 - total flux cleaned = 0.00824726 Jy ! Component: 1000 - total flux cleaned = 0.00824742 Jy ! Component: 1050 - total flux cleaned = 0.00824743 Jy ! Component: 1100 - total flux cleaned = 0.00834931 Jy ! Component: 1150 - total flux cleaned = 0.00824869 Jy ! Component: 1200 - total flux cleaned = 0.00844895 Jy ! Component: 1250 - total flux cleaned = 0.0083497 Jy ! Component: 1300 - total flux cleaned = 0.00839937 Jy ! Component: 1350 - total flux cleaned = 0.0083507 Jy ! Component: 1400 - total flux cleaned = 0.00849679 Jy ! Component: 1450 - total flux cleaned = 0.00849657 Jy ! Component: 1500 - total flux cleaned = 0.00864073 Jy ! Component: 1550 - total flux cleaned = 0.00859325 Jy ! Component: 1600 - total flux cleaned = 0.00878261 Jy ! Component: 1650 - total flux cleaned = 0.00882982 Jy ! Component: 1700 - total flux cleaned = 0.00887657 Jy ! Component: 1750 - total flux cleaned = 0.00878401 Jy ! Component: 1800 - total flux cleaned = 0.00901488 Jy ! Component: 1850 - total flux cleaned = 0.00869386 Jy ! Component: 1900 - total flux cleaned = 0.00905861 Jy ! Component: 1950 - total flux cleaned = 0.00883153 Jy ! Component: 2000 - total flux cleaned = 0.0088317 Jy ! Total flux subtracted in 2048 components = 0.00878706 Jy ! Clean residual min=-0.002609 max=0.002415 Jy/beam ! Clean residual mean=-0.000003 rms=0.000762 Jy/beam ! Combined flux in latest and established models = 2.23075 Jy keep ! Adding 148 model components to the UV plane model. ! The established model now contains 250 components and 2.23075 Jy ![Exited script file: muppet] wmap "J0854+2006_X_2001_03_12_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.632 x 1.139 at -6.671 degrees (North through East) ! Clean map min=-0.0028011 max=1.7173 Jy/beam ! Writing clean map to FITS file: J0854+2006_X_2001_03_12_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 1.71734 invert ! Inverting map ! Your choice of large map pixels excluded 5.57% of the data. ! The x-axis pixel size should ideally be below 0.1558 milli-arcsec ! The y-axis pixel size should ideally be below 0.1927 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000761316 device "J0854+2006_X_2001_03_12_pus\_map.eps/VPS" ! Attempting to open device: 'J0854+2006_X_2001_03_12_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.132993 0.132993 0.265986 0.531973 1.06395 2.12789 4.25578 8.51157 17.0231 34.0463 68.0925 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0022 print "peak=",int(1000*peak_flux)/1000 ! peak= 1.717 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.632 x 1.139 at -6.671 degrees (North through East) ! Clean map min=-0.0028011 max=1.7173 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. quit ! Quitting program ! Log file J0854+2006_X_2001_03_12_pus_uvs.log closed on Wed Jan 2 19:53:31 2013