! Started logfile: J1215-1731_X_2003_07_09_pus_uvs.log on Sun Apr 7 14:00:45 2013 obs J1215-1731_X_2003_07_09_pus_uva.fits ! Reading UV FITS file: J1215-1731_X_2003_07_09_pus_uva.fits ! AN table 1: 55 integrations on 171 of 171 possible baselines. ! AN table 2: 172 integrations on 171 of 171 possible baselines. ! AN table 3: 510 integrations on 171 of 171 possible baselines. ! AN table 4: 98 integrations on 171 of 171 possible baselines. ! AN table 5: 9 integrations on 171 of 171 possible baselines. ! AN table 6: 3 integrations on 171 of 171 possible baselines. ! Apparent sampling: 0.0590319 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1215-1731 ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! ! There are 4 IFs, and a total of 4 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 8.40997e+09 8e+06 1 8e+06 ! 02 2 8.47997e+09 8e+06 1 8e+06 ! 03 3 8.79497e+09 8e+06 1 8e+06 ! 04 4 8.89997e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 1874 lines of history. ! ! Reading 34200 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 J1215-1731_X_2003_07_09_pus] integer clean_niter clean_niter = 100 float clean_gain clean_gain = 0.03 float dynam dynam = 6.0 float soltime1 soltime1 = 120 float soltime2 soltime2 = 20 float thresh thresh = 0.5 float win_mult win_mult = 1.8 float time_av time_av = 16 float old_peak float new_peak float flux_cutoff mapsize field_size, field_cell ! Map grid = 512x512 pixels with 0.200x0.200 milli-arcsec cellsize. startmod ! Applying default point source starting model. ! Performing phase self-cal ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 1 Jy ! ! Correcting IF 1. ! A total of 767 telescope corrections were flagged in sub-array 1. ! A total of 3011 telescope corrections were flagged in sub-array 2. ! A total of 7555 telescope corrections were flagged in sub-array 3. ! A total of 1547 telescope corrections were flagged in sub-array 4. ! A total of 171 telescope corrections were flagged in sub-array 5. ! A total of 49 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 767 telescope corrections were flagged in sub-array 1. ! A total of 3026 telescope corrections were flagged in sub-array 2. ! A total of 7611 telescope corrections were flagged in sub-array 3. ! A total of 1545 telescope corrections were flagged in sub-array 4. ! A total of 171 telescope corrections were flagged in sub-array 5. ! A total of 49 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 768 telescope corrections were flagged in sub-array 1. ! A total of 3027 telescope corrections were flagged in sub-array 2. ! A total of 7645 telescope corrections were flagged in sub-array 3. ! A total of 1551 telescope corrections were flagged in sub-array 4. ! A total of 171 telescope corrections were flagged in sub-array 5. ! A total of 49 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 803 telescope corrections were flagged in sub-array 1. ! A total of 3026 telescope corrections were flagged in sub-array 2. ! A total of 7587 telescope corrections were flagged in sub-array 3. ! A total of 1554 telescope corrections were flagged in sub-array 4. ! A total of 171 telescope corrections were flagged in sub-array 5. ! A total of 49 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.257161Jy sigma=0.009207 ! Fit after self-cal, rms=0.641700Jy sigma=0.003782 ! 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 5.68% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec ! Estimated beam: bmin=0.6457 mas, bmaj=0.9436 mas, bpa=5.23 degrees ! Estimated noise=1481.32 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 = 0.841914 Jy ! Component: 100 - total flux cleaned = 1.17628 Jy ! Total flux subtracted in 100 components = 1.17628 Jy ! Clean residual min=-0.053308 max=0.150537 Jy/beam ! Clean residual mean=0.000900 rms=0.015434 Jy/beam ! Combined flux in latest and established models = 1.17628 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 11 components and 1.17628 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.523420Jy sigma=0.002709 ! Fit after self-cal, rms=0.521331Jy sigma=0.002695 ! Inverting map ! Your choice of large map pixels excluded 5.68% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.164993 Jy ! Component: 100 - total flux cleaned = 0.248232 Jy ! Total flux subtracted in 100 components = 0.248232 Jy ! Clean residual min=-0.028322 max=0.042877 Jy/beam ! Clean residual mean=0.000355 rms=0.008548 Jy/beam ! Combined flux in latest and established models = 1.42452 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 20 components and 1.42452 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.466642Jy sigma=0.001765 ! Fit after self-cal, rms=0.465174Jy sigma=0.001754 ! Inverting map ! Your choice of large map pixels excluded 5.68% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 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 5.68% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec ! Estimated beam: bmin=0.94 mas, bmaj=1.336 mas, bpa=6.303 degrees ! Estimated noise=633.092 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 = 0.0717408 Jy ! Component: 100 - total flux cleaned = 0.101084 Jy ! Component: 150 - total flux cleaned = 0.113406 Jy ! Component: 200 - total flux cleaned = 0.117396 Jy ! Total flux subtracted in 200 components = 0.117396 Jy ! Clean residual min=-0.028357 max=0.031431 Jy/beam ! Clean residual mean=0.000669 rms=0.008576 Jy/beam ! Combined flux in latest and established models = 1.54191 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 28 components and 1.54191 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.460223Jy sigma=0.001596 ! Fit after self-cal, rms=0.459770Jy sigma=0.001591 ! Inverting map ! Your choice of large map pixels excluded 5.68% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.97 GC 1.00* GG 1.00* ! HN 1.00* KP 0.97 LA 0.97 MA 1.00* ! MK 1.00* NL 0.92 NY 1.00* ON 1.00* ! OV 0.97 PT 0.95 SC 1.00* TC 0.93 ! TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 249 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* GC 1.00* GG 1.00* ! HN 1.00* KP 1.00* LA 1.00* MA 1.26 ! MK 1.00* NL 1.00* NY 1.00* ON 1.06 ! OV 1.00* PT 1.00* SC 1.00* TC 1.52 ! TS 1.00* WF 1.00* WZ 0.89 ! ! A total of 291 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 0.99 GC 1.00* GG 1.00* ! HN 0.98 KP 0.98 LA 0.99 MA 1.12 ! MK 0.95 NL 1.04 NY 1.00* ON 0.97 ! OV 0.98 PT 0.98 SC 1.03 TC 0.92 ! TS 0.91 WF 1.01 WZ 1.08 ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.23 GC 1.00* GG 1.00* ! HN 1.11 KP 1.00* LA 1.00* MA 0.97 ! MK 1.00* NL 1.40 NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.17 TC 0.85 ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.97 FD 1.15 GC 1.00* GG 1.00* ! HN 1.00* KP 1.00* LA 1.27 MA 1.00* ! MK 1.00* NL 1.00* NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* TC 1.38 ! TS 1.00* WF 1.00* WZ 1.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.96 GC 1.00* GG 1.00* ! HN 1.00* KP 0.97 LA 0.96 MA 1.00* ! MK 1.00* NL 0.92 NY 1.00* ON 1.00* ! OV 0.97 PT 0.99 SC 1.00* TC 0.88 ! TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 234 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* GC 1.00* GG 1.00* ! HN 1.00* KP 1.00* LA 1.00* MA 1.02 ! MK 1.00* NL 1.00* NY 1.00* ON 0.98 ! OV 1.00* PT 1.00* SC 1.00* TC 1.35 ! TS 1.00* WF 1.00* WZ 1.04 ! ! A total of 237 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 0.98 GC 1.00* GG 1.00* ! HN 1.02 KP 0.96 LA 0.99 MA 1.12 ! MK 0.95 NL 1.03 NY 1.00* ON 1.03 ! OV 0.97 PT 1.03 SC 1.03 TC 0.98 ! TS 0.86 WF 1.05 WZ 1.07 ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.22 GC 1.00* GG 1.00* ! HN 1.14 KP 1.00* LA 1.00* MA 1.05 ! MK 1.00* NL 1.41 NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.08 TC 0.86 ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.07 FD 1.14 GC 1.00* GG 1.00* ! HN 1.00* KP 1.00* LA 1.25 MA 1.00* ! MK 1.00* NL 1.00* NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* TC 0.99 ! TS 1.00* WF 1.00* WZ 1.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 0.97 GC 1.00* GG 1.00* ! HN 1.00* KP 0.97 LA 0.97 MA 1.00* ! MK 1.00* NL 0.97 NY 1.00* ON 1.00* ! OV 1.00 PT 0.97 SC 1.00* TC 1.65 ! TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 237 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* GC 1.00* GG 1.00* ! HN 1.00* KP 1.00* LA 1.00* MA 0.97 ! MK 1.00* NL 1.00* NY 1.00* ON 0.74 ! OV 1.00* PT 1.00* SC 1.00* TC 3.15 ! TS 1.00* WF 1.00* WZ 1.27 ! ! A total of 264 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 0.98 GC 1.00* GG 1.00* ! HN 0.99 KP 0.92 LA 1.00 MA 1.15 ! MK 0.98 NL 1.04 NY 1.00* ON 0.96 ! OV 1.01 PT 1.04 SC 1.02 TC 1.02 ! TS 1.15 WF 1.04 WZ 1.10 ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.22 GC 1.00* GG 1.00* ! HN 1.13 KP 1.00* LA 1.00* MA 0.72 ! MK 1.00* NL 1.43 NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.05 TC 0.95 ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.08 FD 1.13 GC 1.00* GG 1.00* ! HN 1.00* KP 1.00* LA 1.20 MA 1.00* ! MK 1.00* NL 1.00* NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* TC 0.96 ! TS 1.00* WF 1.00* WZ 1.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.95 GC 1.00* GG 1.00* ! HN 1.00* KP 0.98 LA 0.96 MA 1.00* ! MK 1.00* NL 0.93 NY 1.00* ON 1.00* ! OV 0.99 PT 0.97 SC 1.00* TC 1.00* ! TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 234 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00* GC 1.00* GG 1.00* ! HN 1.00* KP 1.00* LA 1.00* MA 1.05 ! MK 1.00* NL 1.00* NY 1.00* ON 0.83 ! OV 1.00* PT 1.00* SC 1.00* TC 0.52 ! TS 1.00* WF 1.00* WZ 1.06 ! ! A total of 303 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 0.96 GC 1.00* GG 1.00* ! HN 1.02 KP 0.95 LA 0.98 MA 1.02 ! MK 1.00 NL 1.02 NY 1.00* ON 0.91 ! OV 1.01 PT 1.05 SC 1.07 TC 1.03 ! TS 1.18 WF 1.03 WZ 1.12 ! ! A total of 36 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.17 GC 1.00* GG 1.00* ! HN 1.15 KP 1.00* LA 1.00* MA 0.77 ! MK 1.00* NL 1.44 NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.08 TC 1.18 ! TS 1.00* WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.17 FD 1.10 GC 1.00* GG 1.00* ! HN 1.00* KP 1.00* LA 1.06 MA 1.00* ! MK 1.00* NL 1.00* NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* TC 1.60 ! TS 1.00* WF 1.00* WZ 1.00* ! ! ! Fit before self-cal, rms=0.459770Jy sigma=0.001591 ! Fit after self-cal, rms=0.437437Jy sigma=0.001412 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec ! Estimated beam: bmin=0.9371 mas, bmaj=1.355 mas, bpa=6.21 degrees ! Estimated noise=629.999 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 = 0.0011534 Jy ! Component: 100 - total flux cleaned = 0.00114705 Jy ! Component: 150 - total flux cleaned = 0.00112924 Jy ! Component: 200 - total flux cleaned = 0.000948687 Jy ! Total flux subtracted in 200 components = 0.000948687 Jy ! Clean residual min=-0.022214 max=0.023227 Jy/beam ! Clean residual mean=0.001105 rms=0.006128 Jy/beam ! Combined flux in latest and established models = 1.54286 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 32 components and 1.54286 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.437404Jy sigma=0.001409 ! Fit after self-cal, rms=0.437242Jy sigma=0.001409 ! Inverting map ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 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=0.437242Jy sigma=0.001409 ! Fit after self-cal, rms=0.441850Jy sigma=0.001283 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec ! Estimated beam: bmin=0.9251 mas, bmaj=1.358 mas, bpa=6.222 degrees ! Estimated noise=628.816 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000973333 Jy ! Component: 100 - total flux cleaned = 0.000766977 Jy ! Component: 150 - total flux cleaned = 0.000757033 Jy ! Component: 200 - total flux cleaned = 0.000756107 Jy ! Total flux subtracted in 200 components = 0.000756107 Jy ! Clean residual min=-0.009051 max=0.018257 Jy/beam ! Clean residual mean=0.000449 rms=0.002936 Jy/beam ! Combined flux in latest and established models = 1.54362 Jy selfcal ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 33 components and 1.54362 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.441589Jy sigma=0.001279 ! Fit after self-cal, rms=0.441505Jy sigma=0.001279 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (1.8, -1.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.01756 Jy ! Component: 100 - total flux cleaned = 0.0209305 Jy ! Component: 150 - total flux cleaned = 0.0206681 Jy ! Component: 200 - total flux cleaned = 0.0206676 Jy ! Total flux subtracted in 200 components = 0.0206676 Jy ! Clean residual min=-0.007778 max=0.010248 Jy/beam ! Clean residual mean=0.000190 rms=0.002285 Jy/beam ! Combined flux in latest and established models = 1.56429 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 44 components and 1.56429 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.440743Jy sigma=0.001266 ! Fit after self-cal, rms=0.440718Jy sigma=0.001264 ! Inverting map ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec ! Added new window around map position (-0.2, 11.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00963416 Jy ! Component: 100 - total flux cleaned = 0.0142028 Jy ! Component: 150 - total flux cleaned = 0.0156455 Jy ! Component: 200 - total flux cleaned = 0.016116 Jy ! Total flux subtracted in 200 components = 0.016116 Jy ! Clean residual min=-0.006779 max=0.007692 Jy/beam ! Clean residual mean=-0.000023 rms=0.001974 Jy/beam ! Combined flux in latest and established models = 1.5804 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 55 components and 1.5804 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.440432Jy sigma=0.001259 ! Fit after self-cal, rms=0.440455Jy sigma=0.001259 ! Inverting map ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 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=0.440455Jy sigma=0.001259 ! Fit after self-cal, rms=0.442765Jy sigma=0.001254 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec ! Estimated beam: bmin=0.9312 mas, bmaj=1.358 mas, bpa=6.376 degrees ! Estimated noise=629.669 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0072218 Jy ! Component: 100 - total flux cleaned = 0.00794498 Jy ! Component: 150 - total flux cleaned = 0.00825907 Jy ! Component: 200 - total flux cleaned = 0.008549 Jy ! Total flux subtracted in 200 components = 0.008549 Jy ! Clean residual min=-0.005673 max=0.007836 Jy/beam ! Clean residual mean=0.000097 rms=0.001639 Jy/beam ! Combined flux in latest and established models = 1.58895 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 62 components and 1.58895 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.442504Jy sigma=0.001251 ! Fit after self-cal, rms=0.442515Jy sigma=0.001250 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 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 (8.6, -4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00622129 Jy ! Component: 100 - total flux cleaned = 0.00711005 Jy ! Component: 150 - total flux cleaned = 0.00726431 Jy ! Component: 200 - total flux cleaned = 0.00739886 Jy ! Total flux subtracted in 200 components = 0.00739886 Jy ! Clean residual min=-0.005203 max=0.006365 Jy/beam ! Clean residual mean=0.000003 rms=0.001456 Jy/beam ! Combined flux in latest and established models = 1.59635 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 75 components and 1.59635 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.442350Jy sigma=0.001248 ! Fit after self-cal, rms=0.442399Jy sigma=0.001247 ! Inverting map ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec ! Added new window around map position (1.8, 20). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00584852 Jy ! Component: 100 - total flux cleaned = 0.00760422 Jy ! Component: 150 - total flux cleaned = 0.00809537 Jy ! Component: 200 - total flux cleaned = 0.00832867 Jy ! Total flux subtracted in 200 components = 0.00832867 Jy ! Clean residual min=-0.005119 max=0.005695 Jy/beam ! Clean residual mean=-0.000074 rms=0.001326 Jy/beam ! Combined flux in latest and established models = 1.60468 Jy ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 90 components and 1.60468 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.442271Jy sigma=0.001246 ! Fit after self-cal, rms=0.442313Jy sigma=0.001246 ! Inverting map ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 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=0.442313Jy sigma=0.001246 ! Fit after self-cal, rms=0.444251Jy sigma=0.001244 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec ! Estimated beam: bmin=2.488 mas, bmaj=4.065 mas, bpa=4.735 degrees ! Estimated noise=686.311 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00611176 Jy ! Component: 100 - total flux cleaned = 0.0082269 Jy ! Component: 150 - total flux cleaned = 0.00926591 Jy ! Component: 200 - total flux cleaned = 0.0096857 Jy ! Total flux subtracted in 200 components = 0.0096857 Jy ! Clean residual min=-0.004544 max=0.004111 Jy/beam ! Clean residual mean=-0.000167 rms=0.001352 Jy/beam ! Combined flux in latest and established models = 1.61436 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 105 components and 1.61436 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.444251Jy sigma=0.001243 ! Fit after self-cal, rms=0.444271Jy sigma=0.001243 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 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 = 0.00192269 Jy ! Component: 100 - total flux cleaned = 0.00216165 Jy ! Component: 150 - total flux cleaned = 0.00243432 Jy ! Component: 200 - total flux cleaned = 0.00255089 Jy ! Total flux subtracted in 200 components = 0.00255089 Jy ! Clean residual min=-0.004364 max=0.003759 Jy/beam ! Clean residual mean=-0.000219 rms=0.001272 Jy/beam ! Combined flux in latest and established models = 1.61692 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 113 components and 1.61692 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.444279Jy sigma=0.001243 ! Fit after self-cal, rms=0.444287Jy sigma=0.001243 ! Inverting map ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 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 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec ! Estimated beam: bmin=0.9353 mas, bmaj=1.359 mas, bpa=6.423 degrees ! Estimated noise=630.547 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9353 x 1.359 at 6.423 degrees (North through East) ! Clean map min=-0.0054397 max=1.1801 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=0.444287Jy sigma=0.001243 ! Fit after self-cal, rms=0.592855Jy sigma=0.001076 ! Inverting map and beam ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec ! Estimated beam: bmin=0.9261 mas, bmaj=1.357 mas, bpa=5.978 degrees ! Estimated noise=628.561 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00179435 Jy ! Component: 100 - total flux cleaned = 0.00191666 Jy ! Component: 150 - total flux cleaned = 0.00202404 Jy ! Component: 200 - total flux cleaned = 0.00212501 Jy ! Total flux subtracted in 200 components = 0.00212501 Jy ! Clean residual min=-0.003819 max=0.004352 Jy/beam ! Clean residual mean=-0.000069 rms=0.001028 Jy/beam ! Combined flux in latest and established models = 1.61904 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 119 components and 1.61904 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.592753Jy sigma=0.001074 ! Fit after self-cal, rms=0.592884Jy sigma=0.001074 ! Inverting map ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000695286 Jy ! Component: 100 - total flux cleaned = 0.000693763 Jy ! Component: 150 - total flux cleaned = 0.000602217 Jy ! Component: 200 - total flux cleaned = 0.000601346 Jy ! Total flux subtracted in 200 components = 0.000601346 Jy ! Clean residual min=-0.003712 max=0.004163 Jy/beam ! Clean residual mean=-0.000076 rms=0.001002 Jy/beam ! Combined flux in latest and established models = 1.61964 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 126 components and 1.61964 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.592813Jy sigma=0.001073 ! Fit after self-cal, rms=0.592904Jy sigma=0.001073 ! Inverting map ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.592904Jy sigma=0.001073 ! Fit after self-cal, rms=0.605099Jy sigma=0.001073 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 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec ! Estimated beam: bmin=0.6351 mas, bmaj=0.959 mas, bpa=4.792 degrees ! Estimated noise=1574.81 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.847562 Jy ! Component: 100 - total flux cleaned = 1.19144 Jy ! Component: 150 - total flux cleaned = 1.35727 Jy ! Component: 200 - total flux cleaned = 1.43994 Jy ! Total flux subtracted in 200 components = 1.43994 Jy ! Clean residual min=-0.015024 max=0.038475 Jy/beam ! Clean residual mean=0.000356 rms=0.004218 Jy/beam ! Combined flux in latest and established models = 1.43994 Jy uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Adding 19 model components to the UV plane model. ! The established model now contains 19 components and 1.43994 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec ! Estimated beam: bmin=0.9281 mas, bmaj=1.359 mas, bpa=5.971 degrees ! Estimated noise=628.772 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 = 0.0662185 Jy ! Component: 100 - total flux cleaned = 0.0996636 Jy ! Component: 150 - total flux cleaned = 0.120467 Jy ! Component: 200 - total flux cleaned = 0.134617 Jy ! Total flux subtracted in 200 components = 0.134617 Jy ! Clean residual min=-0.004175 max=0.008304 Jy/beam ! Clean residual mean=0.000481 rms=0.001830 Jy/beam ! Combined flux in latest and established models = 1.57456 Jy ! Adding 50 model components to the UV plane model. ! The established model now contains 58 components and 1.57456 Jy ! Inverting map ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec ! Added new window around map position (-0.6, -0.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00996328 Jy ! Component: 100 - total flux cleaned = 0.0172568 Jy ! Component: 150 - total flux cleaned = 0.0229838 Jy ! Component: 200 - total flux cleaned = 0.0276695 Jy ! Total flux subtracted in 200 components = 0.0276695 Jy ! Clean residual min=-0.003355 max=0.004886 Jy/beam ! Clean residual mean=0.000154 rms=0.001161 Jy/beam ! Combined flux in latest and established models = 1.60223 Jy ! Adding 41 model components to the UV plane model. ! The established model now contains 85 components and 1.60223 Jy ! Inverting map ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 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 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec ! Estimated beam: bmin=2.485 mas, bmaj=4.059 mas, bpa=4.751 degrees ! Estimated noise=686.345 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00537858 Jy ! Component: 100 - total flux cleaned = 0.00886463 Jy ! Component: 150 - total flux cleaned = 0.0115472 Jy ! Component: 200 - total flux cleaned = 0.0136596 Jy ! Total flux subtracted in 200 components = 0.0136596 Jy ! Clean residual min=-0.003511 max=0.004447 Jy/beam ! Clean residual mean=-0.000019 rms=0.001207 Jy/beam ! Combined flux in latest and established models = 1.61589 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 = 0.00170262 Jy ! Component: 100 - total flux cleaned = 0.00283839 Jy ! Component: 150 - total flux cleaned = 0.00333637 Jy ! Component: 200 - total flux cleaned = 0.00374192 Jy ! Total flux subtracted in 200 components = 0.00374192 Jy ! Clean residual min=-0.003427 max=0.004209 Jy/beam ! Clean residual mean=-0.000094 rms=0.001121 Jy/beam ! Combined flux in latest and established models = 1.61963 Jy ! Adding 47 model components to the UV plane model. ! The established model now contains 124 components and 1.61963 Jy ! Inverting map ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec ! Estimated beam: bmin=0.9281 mas, bmaj=1.359 mas, bpa=5.971 degrees ! Estimated noise=628.772 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000526686 Jy ! Component: 100 - total flux cleaned = -0.000529752 Jy ! Component: 150 - total flux cleaned = -0.000340402 Jy ! Component: 200 - total flux cleaned = -0.000156803 Jy ! Total flux subtracted in 200 components = -0.000156803 Jy ! Clean residual min=-0.003333 max=0.004011 Jy/beam ! Clean residual mean=-0.000049 rms=0.000918 Jy/beam ! Combined flux in latest and established models = 1.61947 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 139 components and 1.61947 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.604985Jy sigma=0.001071 ! Fit after self-cal, rms=0.605436Jy sigma=0.001070 wmodel J1215-1731_X_2003_07_09_pus_map.mod ! Writing 139 model components to file: J1215-1731_X_2003_07_09_pus_map.mod wobs J1215-1731_X_2003_07_09_pus_uvs.fits ! Writing UV FITS file: J1215-1731_X_2003_07_09_pus_uvs.fits wwins J1215-1731_X_2003_07_09_pus_map.win ! wwins: Wrote 6 windows to J1215-1731_X_2003_07_09_pus_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec ! clean: niter=2048 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.00159769 Jy ! Component: 100 - total flux cleaned = 0.00203087 Jy ! Component: 150 - total flux cleaned = 0.00208809 Jy ! Component: 200 - total flux cleaned = 0.00214221 Jy ! Component: 250 - total flux cleaned = 0.00203552 Jy ! Component: 300 - total flux cleaned = 0.00183029 Jy ! Component: 350 - total flux cleaned = 0.00178009 Jy ! Component: 400 - total flux cleaned = 0.0016337 Jy ! Component: 450 - total flux cleaned = 0.0015376 Jy ! Component: 500 - total flux cleaned = 0.00130243 Jy ! Component: 550 - total flux cleaned = 0.00116455 Jy ! Component: 600 - total flux cleaned = 0.00107396 Jy ! Component: 650 - total flux cleaned = 0.000895049 Jy ! Component: 700 - total flux cleaned = 0.000851211 Jy ! Component: 750 - total flux cleaned = 0.000721381 Jy ! Component: 800 - total flux cleaned = 0.000550638 Jy ! Component: 850 - total flux cleaned = 0.000550408 Jy ! Component: 900 - total flux cleaned = 0.000383564 Jy ! Component: 950 - total flux cleaned = 0.000260097 Jy ! Component: 1000 - total flux cleaned = 0.000178394 Jy ! Component: 1050 - total flux cleaned = 0.000137913 Jy ! Component: 1100 - total flux cleaned = -2.14289e-05 Jy ! Component: 1150 - total flux cleaned = -6.10286e-05 Jy ! Component: 1200 - total flux cleaned = -0.000217841 Jy ! Component: 1250 - total flux cleaned = -0.000334167 Jy ! Component: 1300 - total flux cleaned = -0.000526224 Jy ! Component: 1350 - total flux cleaned = -0.000640194 Jy ! Component: 1400 - total flux cleaned = -0.000715515 Jy ! Component: 1450 - total flux cleaned = -0.000902453 Jy ! Component: 1500 - total flux cleaned = -0.00101373 Jy ! Component: 1550 - total flux cleaned = -0.00101403 Jy ! Component: 1600 - total flux cleaned = -0.00123286 Jy ! Component: 1650 - total flux cleaned = -0.001269 Jy ! Component: 1700 - total flux cleaned = -0.00137665 Jy ! Component: 1750 - total flux cleaned = -0.00148349 Jy ! Component: 1800 - total flux cleaned = -0.00155431 Jy ! Component: 1850 - total flux cleaned = -0.00162445 Jy ! Component: 1900 - total flux cleaned = -0.00165919 Jy ! Component: 1950 - total flux cleaned = -0.00169414 Jy ! Component: 2000 - total flux cleaned = -0.00179742 Jy ! Total flux subtracted in 2048 components = -0.00186543 Jy ! Clean residual min=-0.002038 max=0.001994 Jy/beam ! Clean residual mean=-0.000058 rms=0.000597 Jy/beam ! Combined flux in latest and established models = 1.6176 Jy keep ! Adding 150 model components to the UV plane model. ! The established model now contains 287 components and 1.61761 Jy ![Exited script file: muppet] wmap "J1215-1731_X_2003_07_09_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9281 x 1.359 at 5.971 degrees (North through East) ! Clean map min=-0.0026731 max=1.1869 Jy/beam ! Writing clean map to FITS file: J1215-1731_X_2003_07_09_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 1.1869 invert ! Inverting map ! Your choice of large map pixels excluded 5.6% of the data. ! The x-axis pixel size should ideally be below 0.1832 milli-arcsec ! The y-axis pixel size should ideally be below 0.1778 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000592568 device "J1215-1731_X_2003_07_09_pus\_map.eps/VPS" ! Attempting to open device: 'J1215-1731_X_2003_07_09_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.149777 0.149777 0.299553 0.599106 1.19821 2.39643 4.79285 9.5857 19.1714 38.3428 76.6856 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0017 print "peak=",int(1000*peak_flux)/1000 ! peak= 1.186 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9281 x 1.359 at 5.971 degrees (North through East) ! Clean map min=-0.0026731 max=1.1869 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. quit ! Quitting program ! Log file J1215-1731_X_2003_07_09_pus_uvs.log closed on Sun Apr 7 14:01:04 2013