! Started logfile: /d2/scr/pima/rv101_uvs/J0958+4725_X_uvs.log on Sat Nov 29 16:32:43 2014 obs /d2/scr/pima/rv101_uvs/J0958+4725_X_uva.fits ! Reading UV FITS file: /d2/scr/pima/rv101_uvs/J0958+4725_X_uva.fits ! AN table 1: 37 integrations on 55 of 55 possible baselines. ! AN table 2: 9 integrations on 28 of 28 possible baselines. ! AN table 3: 39 integrations on 1 of 1 possible baselines. ! AN table 4: 25 integrations on 36 of 36 possible baselines. ! AN table 5: 9 integrations on 1 of 1 possible baselines. ! AN table 6: 9 integrations on 3 of 3 possible baselines. ! AN table 7: 102 integrations on 3 of 3 possible baselines. ! AN table 8: 9 integrations on 6 of 6 possible baselines. ! AN table 9: 108 integrations on 6 of 6 possible baselines. ! AN table 10: 9 integrations on 6 of 6 possible baselines. ! AN table 11: 35 integrations on 15 of 15 possible baselines. ! AN table 12: 34 integrations on 66 of 66 possible baselines. ! Apparent sampling: 0.430847 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0958+4725 ! ! 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 8.40599e+09 8e+06 1 8e+06 ! 02 2 8.47599e+09 8e+06 1 8e+06 ! 03 3 8.79099e+09 8e+06 1 8e+06 ! 04 4 8.89599e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 0 lines of history. ! ! Reading 12224 visibilities. select RR ! 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 = 1024 print "field_cell =", field_cell ! field_cell = 0.2 print "taper_size =", taper_size ! taper_size = 70 ![@/home/lpetrov/bin/01_muppet /d2/scr/pima/rv101_uvs/J0958+4725_X] float lim_self lim_self = 120.0 float lim_val lim_va = 1.2 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 = 1024x1024 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 265 telescope corrections were flagged in sub-array 1. ! A total of 16 telescope corrections were flagged in sub-array 2. ! A total of 78 telescope corrections were flagged in sub-array 3. ! A total of 169 telescope corrections were flagged in sub-array 4. ! A total of 18 telescope corrections were flagged in sub-array 5. ! A total of 9 telescope corrections were flagged in sub-array 6. ! A total of 42 telescope corrections were flagged in sub-array 7. ! A total of 12 telescope corrections were flagged in sub-array 8. ! A total of 201 telescope corrections were flagged in sub-array 9. ! A total of 8 telescope corrections were flagged in sub-array 10. ! A total of 88 telescope corrections were flagged in sub-array 11. ! A total of 249 telescope corrections were flagged in sub-array 12. ! ! Correcting IF 2. ! A total of 265 telescope corrections were flagged in sub-array 1. ! A total of 16 telescope corrections were flagged in sub-array 2. ! A total of 78 telescope corrections were flagged in sub-array 3. ! A total of 169 telescope corrections were flagged in sub-array 4. ! A total of 18 telescope corrections were flagged in sub-array 5. ! A total of 9 telescope corrections were flagged in sub-array 6. ! A total of 42 telescope corrections were flagged in sub-array 7. ! A total of 12 telescope corrections were flagged in sub-array 8. ! A total of 201 telescope corrections were flagged in sub-array 9. ! A total of 8 telescope corrections were flagged in sub-array 10. ! A total of 88 telescope corrections were flagged in sub-array 11. ! A total of 249 telescope corrections were flagged in sub-array 12. ! ! Correcting IF 3. ! A total of 342 telescope corrections were flagged in sub-array 1. ! A total of 16 telescope corrections were flagged in sub-array 2. ! A total of 78 telescope corrections were flagged in sub-array 3. ! A total of 176 telescope corrections were flagged in sub-array 4. ! A total of 18 telescope corrections were flagged in sub-array 5. ! A total of 27 telescope corrections were flagged in sub-array 6. ! A total of 306 telescope corrections were flagged in sub-array 7. ! A total of 12 telescope corrections were flagged in sub-array 8. ! A total of 387 telescope corrections were flagged in sub-array 9. ! A total of 8 telescope corrections were flagged in sub-array 10. ! A total of 151 telescope corrections were flagged in sub-array 11. ! A total of 315 telescope corrections were flagged in sub-array 12. ! ! Correcting IF 4. ! A total of 342 telescope corrections were flagged in sub-array 1. ! A total of 16 telescope corrections were flagged in sub-array 2. ! A total of 78 telescope corrections were flagged in sub-array 3. ! A total of 176 telescope corrections were flagged in sub-array 4. ! A total of 18 telescope corrections were flagged in sub-array 5. ! A total of 27 telescope corrections were flagged in sub-array 6. ! A total of 306 telescope corrections were flagged in sub-array 7. ! A total of 12 telescope corrections were flagged in sub-array 8. ! A total of 387 telescope corrections were flagged in sub-array 9. ! A total of 8 telescope corrections were flagged in sub-array 10. ! A total of 151 telescope corrections were flagged in sub-array 11. ! A total of 315 telescope corrections were flagged in sub-array 12. ! ! Fit before self-cal, rms=1.375063Jy sigma=7.552120 ! Fit after self-cal, rms=0.274566Jy sigma=1.337576 ! 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 0.733% of the data. ! The x-axis pixel size should ideally be below 0.193 milli-arcsec ! Estimated beam: bmin=0.6474 mas, bmaj=0.84 mas, bpa=-20.39 degrees ! Estimated noise=2.118 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 = 0.66107 Jy ! Component: 100 - total flux cleaned = 0.80847 Jy ! Total flux subtracted in 100 components = 0.80847 Jy ! Clean residual min=-0.018176 max=0.048921 Jy/beam ! Clean residual mean=0.000174 rms=0.004834 Jy/beam ! Combined flux in latest and established models = 0.80847 Jy ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 4 components and 0.80847 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.286737Jy sigma=1.184556 ! Fit after self-cal, rms=0.286703Jy sigma=1.184468 ! Inverting map ! Your choice of large map pixels excluded 0.733% of the data. ! The x-axis pixel size should ideally be below 0.193 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0517866 Jy ! Component: 100 - total flux cleaned = 0.081308 Jy ! Total flux subtracted in 100 components = 0.081308 Jy ! Clean residual min=-0.017089 max=0.018638 Jy/beam ! Clean residual mean=0.000094 rms=0.004060 Jy/beam ! Combined flux in latest and established models = 0.889778 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 15 components and 0.889778 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.264050Jy sigma=1.071566 ! Fit after self-cal, rms=0.263968Jy sigma=1.071308 ! Inverting map ! Your choice of large map pixels excluded 0.733% of the data. ! The x-axis pixel size should ideally be below 0.193 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 0.733% of the data. ! The x-axis pixel size should ideally be below 0.193 milli-arcsec ! Estimated beam: bmin=0.7904 mas, bmaj=0.9815 mas, bpa=-14.99 degrees ! Estimated noise=1.66268 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 = 0.0420935 Jy ! Component: 100 - total flux cleaned = 0.0615828 Jy ! Component: 150 - total flux cleaned = 0.0718154 Jy ! Component: 200 - total flux cleaned = 0.0753351 Jy ! Total flux subtracted in 200 components = 0.0753351 Jy ! Clean residual min=-0.024956 max=0.024045 Jy/beam ! Clean residual mean=0.000340 rms=0.005728 Jy/beam ! Combined flux in latest and established models = 0.965113 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 23 components and 0.965113 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.252065Jy sigma=1.056507 ! Fit after self-cal, rms=0.251996Jy sigma=1.056155 ! Inverting map ! Your choice of large map pixels excluded 0.733% of the data. ! The x-axis pixel size should ideally be below 0.193 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7904 x 0.9815 at -14.99 degrees (North through East) ! Clean map min=-0.023365 max=0.88645 Jy/beam if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val ! Selfcal amplitude corrections will be limited to 0.833333 -> 1.2. ! Selfcal phase corrections will not be limited. gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 69 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! FD 1.00* HN 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 1.00* NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! FD 1.06 HN 1.04 LA 1.06 NL 0.98 ! OV 0.98 PT 1.04 SC 1.11 WF 0.85 ! ! Telescope amplitude corrections in sub-array 3: ! NY 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! FD 1.05 KP 1.00* LA 1.10 MK 1.06 ! NL 1.04 NY 1.02 OV 1.01 PT 1.04 ! WF 0.98 ! ! Telescope amplitude corrections in sub-array 5: ! NY 0.00* OV 0.00* ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! MK 0.00* NY 0.00* OV 0.00* ! ! A total of 264 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! MA 0.00* NY 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! HN 1.04 NL 0.99 SC 1.11 WF 0.83 ! ! A total of 63 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! MA 1.00* NY 1.00* ON 1.00* WF 1.00* ! ! Telescope amplitude corrections in sub-array 10: ! HN 1.00* NL 1.00* OV 1.00* WF 1.00* ! ! A total of 48 telescope corrections were flagged in sub-array 11. ! Telescope amplitude corrections in sub-array 11: ! HN 1.00* MA 1.00* NL 1.00* NY 1.00* ! ON 1.00* WF 1.00* ! ! A total of 51 telescope corrections were flagged in sub-array 12. ! Telescope amplitude corrections in sub-array 12: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! MA 1.00* NL 1.00* NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* WF 1.00* ! ! ! Correcting IF 2. ! A total of 69 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! FD 1.00* HN 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 1.00* NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! FD 1.08 HN 1.08 LA 1.03 NL 1.00 ! OV 0.97 PT 0.92 SC 1.15 WF 0.84 ! ! Telescope amplitude corrections in sub-array 3: ! NY 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! FD 1.09 KP 1.00* LA 1.04 MK 1.05 ! NL 1.05 NY 1.00 OV 1.02 PT 0.94 ! WF 0.91 ! ! Telescope amplitude corrections in sub-array 5: ! NY 0.00* OV 0.00* ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! MK 0.00* NY 0.00* OV 0.00* ! ! A total of 264 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! MA 0.00* NY 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! HN 1.11 NL 1.01 SC 1.16 WF 0.90 ! ! A total of 63 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! MA 1.00* NY 1.00* ON 1.00* WF 1.00* ! ! Telescope amplitude corrections in sub-array 10: ! HN 1.12 NL 0.99 OV 1.02 WF 0.86 ! ! A total of 48 telescope corrections were flagged in sub-array 11. ! Telescope amplitude corrections in sub-array 11: ! HN 1.00* MA 1.00* NL 1.00* NY 1.00* ! ON 1.00* WF 1.00* ! ! A total of 51 telescope corrections were flagged in sub-array 12. ! Telescope amplitude corrections in sub-array 12: ! FD 1.04 HN 1.06 KP 1.00* LA 1.11 ! MA 0.99 NL 1.02 NY 0.96 ON 0.84 ! OV 1.00 PT 0.99 SC 1.09 WF 0.84 ! ! ! Correcting IF 3. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! FD 0.99 HN 1.05 LA 1.05 MA 1.07 ! MK 1.05 NL 1.01 NY 1.00* ON 0.98 ! OV 1.05 PT 1.00* SC 1.07 ! ! Telescope amplitude corrections in sub-array 2: ! FD 1.03 HN 1.06 LA 1.03 NL 1.02 ! OV 1.04 PT 0.90 SC 1.12 WF 0.87 ! ! Telescope amplitude corrections in sub-array 3: ! NY 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! FD 1.10 KP 1.00* LA 1.13 MK 1.02 ! NL 1.06 NY 1.00* OV 1.05 PT 0.94 ! WF 0.97 ! ! Telescope amplitude corrections in sub-array 5: ! NY 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! MK 0.00* NY 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! MA 0.00* NY 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! HN 1.05 NL 1.08 SC 1.10 WF 0.91 ! ! A total of 45 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! MA 0.00* NY 0.00* ON 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 10: ! HN 1.08 NL 1.02 OV 1.05 WF 0.94 ! ! A total of 24 telescope corrections were flagged in sub-array 11. ! Telescope amplitude corrections in sub-array 11: ! HN 1.00* MA 1.00* NL 1.00* NY 1.00* ! ON 1.00* WF 1.00* ! ! A total of 24 telescope corrections were flagged in sub-array 12. ! Telescope amplitude corrections in sub-array 12: ! FD 1.03 HN 1.12 KP 1.00* LA 1.14 ! MA 1.07 NL 1.05 NY 1.00* ON 0.98 ! OV 1.04 PT 0.97 SC 1.07 WF 0.93 ! ! ! Correcting IF 4. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! FD 1.06 HN 1.02 LA 1.04 MA 1.13 ! MK 1.11 NL 1.06 NY 1.00* ON 1.06 ! OV 1.01 PT 1.00* SC 1.08 ! ! Telescope amplitude corrections in sub-array 2: ! FD 1.07 HN 1.07 LA 1.03 NL 1.03 ! OV 1.03 PT 0.94 SC 1.14 WF 0.98 ! ! Telescope amplitude corrections in sub-array 3: ! NY 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! FD 1.11 KP 1.00* LA 1.07 MK 1.09 ! NL 1.06 NY 1.00* OV 1.07 PT 0.97 ! WF 1.13 ! ! Telescope amplitude corrections in sub-array 5: ! NY 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! MK 0.00* NY 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! MA 0.00* NY 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! HN 1.03 NL 1.14 SC 1.14 WF 1.00 ! ! A total of 45 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! MA 0.00* NY 0.00* ON 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 10: ! HN 1.08 NL 1.01 OV 1.05 WF 1.03 ! ! A total of 24 telescope corrections were flagged in sub-array 11. ! Telescope amplitude corrections in sub-array 11: ! HN 1.16 MA 1.09 NL 1.06 NY 1.00* ! ON 1.05 WF 0.95 ! ! A total of 24 telescope corrections were flagged in sub-array 12. ! Telescope amplitude corrections in sub-array 12: ! FD 1.06 HN 1.13 KP 1.00* LA 1.13 ! MA 1.10 NL 1.03 NY 1.00* ON 1.01 ! OV 0.99 PT 0.98 SC 1.06 WF 1.03 ! ! ! Fit before self-cal, rms=0.251996Jy sigma=1.056155 ! Fit after self-cal, rms=0.213659Jy sigma=0.915010 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 milli-arcsec ! Estimated beam: bmin=0.764 mas, bmaj=0.9788 mas, bpa=-20.71 degrees ! Estimated noise=1.78468 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 = 0.0117369 Jy ! Component: 100 - total flux cleaned = 0.0120138 Jy ! Component: 150 - total flux cleaned = 0.0120238 Jy ! Component: 200 - total flux cleaned = 0.0117191 Jy ! Total flux subtracted in 200 components = 0.0117191 Jy ! Clean residual min=-0.012858 max=0.013899 Jy/beam ! Clean residual mean=0.000198 rms=0.003185 Jy/beam ! Combined flux in latest and established models = 0.976832 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 26 components and 0.976832 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.211935Jy sigma=0.915119 ! Fit after self-cal, rms=0.211854Jy sigma=0.914884 ! Inverting map ! Your choice of large map pixels excluded 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 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=0.211854Jy sigma=0.914884 ! Fit after self-cal, rms=0.211233Jy sigma=0.903676 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 milli-arcsec ! Estimated beam: bmin=0.7632 mas, bmaj=0.9778 mas, bpa=-20.75 degrees ! Estimated noise=1.80377 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00972508 Jy ! Component: 100 - total flux cleaned = 0.0109152 Jy ! Component: 150 - total flux cleaned = 0.0110509 Jy ! Component: 200 - total flux cleaned = 0.011039 Jy ! Total flux subtracted in 200 components = 0.011039 Jy ! Clean residual min=-0.012309 max=0.012438 Jy/beam ! Clean residual mean=0.000208 rms=0.003008 Jy/beam ! Combined flux in latest and established models = 0.987871 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 27 components and 0.987871 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.209967Jy sigma=0.904407 ! Fit after self-cal, rms=0.209929Jy sigma=0.904334 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 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 = -1.73017e-05 Jy ! Component: 100 - total flux cleaned = -1.66903e-05 Jy ! Component: 150 - total flux cleaned = -0.00010033 Jy ! Component: 200 - total flux cleaned = -0.000100632 Jy ! Total flux subtracted in 200 components = -0.000100632 Jy ! Clean residual min=-0.012226 max=0.012321 Jy/beam ! Clean residual mean=0.000208 rms=0.003003 Jy/beam ! Combined flux in latest and established models = 0.98777 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 29 components and 0.98777 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.209734Jy sigma=0.904406 ! Fit after self-cal, rms=0.209717Jy sigma=0.904346 ! Inverting map ! Your choice of large map pixels excluded 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 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=0.209717Jy sigma=0.904346 ! Fit after self-cal, rms=0.208468Jy sigma=0.900016 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 milli-arcsec ! Estimated beam: bmin=0.7624 mas, bmaj=0.9774 mas, bpa=-20.7 degrees ! Estimated noise=1.81784 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0067558 Jy ! Component: 100 - total flux cleaned = 0.00968255 Jy ! Component: 150 - total flux cleaned = 0.0100596 Jy ! Component: 200 - total flux cleaned = 0.0100603 Jy ! Total flux subtracted in 200 components = 0.0100603 Jy ! Clean residual min=-0.011568 max=0.012119 Jy/beam ! Clean residual mean=0.000217 rms=0.002908 Jy/beam ! Combined flux in latest and established models = 0.997831 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 30 components and 0.997831 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.207825Jy sigma=0.900920 ! Fit after self-cal, rms=0.207794Jy sigma=0.900860 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 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 = -3.74708e-07 Jy ! Component: 100 - total flux cleaned = 2.97523e-06 Jy ! Component: 150 - total flux cleaned = -5.16143e-05 Jy ! Component: 200 - total flux cleaned = -0.000101596 Jy ! Total flux subtracted in 200 components = -0.000101596 Jy ! Clean residual min=-0.011578 max=0.012059 Jy/beam ! Clean residual mean=0.000218 rms=0.002905 Jy/beam ! Combined flux in latest and established models = 0.997729 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 31 components and 0.997729 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.207721Jy sigma=0.900827 ! Fit after self-cal, rms=0.207715Jy sigma=0.900782 ! Inverting map ! Your choice of large map pixels excluded 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 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=0.207715Jy sigma=0.900782 ! Fit after self-cal, rms=0.206619Jy sigma=0.897990 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 milli-arcsec ! Estimated beam: bmin=2.159 mas, bmaj=2.573 mas, bpa=59.37 degrees ! Estimated noise=2.50176 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00582729 Jy ! Component: 100 - total flux cleaned = 0.00619926 Jy ! Component: 150 - total flux cleaned = 0.00647734 Jy ! Component: 200 - total flux cleaned = 0.00668665 Jy ! Total flux subtracted in 200 components = 0.00668665 Jy ! Clean residual min=-0.012643 max=0.012922 Jy/beam ! Clean residual mean=0.000681 rms=0.003420 Jy/beam ! Combined flux in latest and established models = 1.00442 Jy selfcal ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 34 components and 1.00442 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.206509Jy sigma=0.899444 ! Fit after self-cal, rms=0.206409Jy sigma=0.898829 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 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 = -0.000950019 Jy ! Component: 100 - total flux cleaned = -0.000948986 Jy ! Component: 150 - total flux cleaned = -0.000774721 Jy ! Component: 200 - total flux cleaned = -0.000703524 Jy ! Total flux subtracted in 200 components = -0.000703524 Jy ! Clean residual min=-0.012625 max=0.012989 Jy/beam ! Clean residual mean=0.000696 rms=0.003398 Jy/beam ! Combined flux in latest and established models = 1.00371 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 34 components and 1.00371 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.206539Jy sigma=0.900716 ! Fit after self-cal, rms=0.206514Jy sigma=0.900428 ! Inverting map ! Your choice of large map pixels excluded 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 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 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 milli-arcsec ! Estimated beam: bmin=0.7616 mas, bmaj=0.9764 mas, bpa=-20.74 degrees ! Estimated noise=1.82713 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7616 x 0.9764 at -20.74 degrees (North through East) ! Clean map min=-0.0098648 max=0.91675 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=0.206514Jy sigma=0.900428 ! Fit after self-cal, rms=0.198220Jy sigma=0.841740 ! Inverting map and beam ! Your choice of large map pixels excluded 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 milli-arcsec ! Estimated beam: bmin=0.7624 mas, bmaj=0.9747 mas, bpa=-21.33 degrees ! Estimated noise=1.83946 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00655245 Jy ! Component: 100 - total flux cleaned = 0.00807686 Jy ! Component: 150 - total flux cleaned = 0.00864252 Jy ! Component: 200 - total flux cleaned = 0.0089995 Jy ! Total flux subtracted in 200 components = 0.0089995 Jy ! Clean residual min=-0.010046 max=0.011286 Jy/beam ! Clean residual mean=0.000163 rms=0.002598 Jy/beam ! Combined flux in latest and established models = 1.01271 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 36 components and 1.01271 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.197705Jy sigma=0.841624 ! Fit after self-cal, rms=0.197700Jy sigma=0.841498 ! Inverting map ! Your choice of large map pixels excluded 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 milli-arcsec ! Added new window around map position (-8.4, -26.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00512272 Jy ! Component: 100 - total flux cleaned = 0.00470989 Jy ! Component: 150 - total flux cleaned = 0.00414991 Jy ! Component: 200 - total flux cleaned = 0.00384352 Jy ! Total flux subtracted in 200 components = 0.00384352 Jy ! Clean residual min=-0.009937 max=0.010877 Jy/beam ! Clean residual mean=0.000147 rms=0.002539 Jy/beam ! Combined flux in latest and established models = 1.01656 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 51 components and 1.01655 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.196904Jy sigma=0.838429 ! Fit after self-cal, rms=0.196789Jy sigma=0.838051 ! Inverting map ! Your choice of large map pixels excluded 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 milli-arcsec ! Added new window around map position (0, -16.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00541676 Jy ! Component: 100 - total flux cleaned = 0.00521227 Jy ! Component: 150 - total flux cleaned = 0.00422937 Jy ! Component: 200 - total flux cleaned = 0.00354966 Jy ! Total flux subtracted in 200 components = 0.00354966 Jy ! Clean residual min=-0.009566 max=0.010488 Jy/beam ! Clean residual mean=0.000123 rms=0.002452 Jy/beam ! Combined flux in latest and established models = 1.0201 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 61 components and 1.0201 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.195916Jy sigma=0.834213 ! Fit after self-cal, rms=0.195852Jy sigma=0.833773 ! Inverting map ! Your choice of large map pixels excluded 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 milli-arcsec ! Added new window around map position (4, -33.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00656138 Jy ! Component: 100 - total flux cleaned = 0.00773408 Jy ! Component: 150 - total flux cleaned = 0.00735613 Jy ! Component: 200 - total flux cleaned = 0.00667071 Jy ! Total flux subtracted in 200 components = 0.00667071 Jy ! Clean residual min=-0.009095 max=0.009840 Jy/beam ! Clean residual mean=0.000098 rms=0.002365 Jy/beam ! Combined flux in latest and established models = 1.02678 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 73 components and 1.02678 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.194989Jy sigma=0.831021 ! Fit after self-cal, rms=0.194968Jy sigma=0.830809 ! Inverting map ! Your choice of large map pixels excluded 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.194968Jy sigma=0.830809 ! Fit after self-cal, rms=0.194679Jy sigma=0.827898 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 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 milli-arcsec ! Estimated beam: bmin=0.6415 mas, bmaj=0.8407 mas, bpa=-23.6 degrees ! Estimated noise=2.3414 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.709134 Jy ! Component: 100 - total flux cleaned = 0.871184 Jy ! Component: 150 - total flux cleaned = 0.931271 Jy ! Component: 200 - total flux cleaned = 0.96401 Jy ! Total flux subtracted in 200 components = 0.96401 Jy ! Clean residual min=-0.013440 max=0.016523 Jy/beam ! Clean residual mean=0.000071 rms=0.002954 Jy/beam ! Combined flux in latest and established models = 0.96401 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 0.96401 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 milli-arcsec ! Estimated beam: bmin=0.7616 mas, bmaj=0.974 mas, bpa=-21.15 degrees ! Estimated noise=1.84387 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 = 0.029006 Jy ! Component: 100 - total flux cleaned = 0.0467724 Jy ! Component: 150 - total flux cleaned = 0.0575977 Jy ! Component: 200 - total flux cleaned = 0.0623716 Jy ! Total flux subtracted in 200 components = 0.0623716 Jy ! Clean residual min=-0.009443 max=0.010195 Jy/beam ! Clean residual mean=0.000138 rms=0.002514 Jy/beam ! Combined flux in latest and established models = 1.02638 Jy ! Adding 22 model components to the UV plane model. ! The established model now contains 32 components and 1.02638 Jy ! Inverting map ! Your choice of large map pixels excluded 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 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 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 milli-arcsec ! Estimated beam: bmin=2.156 mas, bmaj=2.568 mas, bpa=59.3 degrees ! Estimated noise=2.53324 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00583987 Jy ! Component: 100 - total flux cleaned = 0.00786411 Jy ! Component: 150 - total flux cleaned = 0.00867917 Jy ! Component: 200 - total flux cleaned = 0.00868003 Jy ! Total flux subtracted in 200 components = 0.00868003 Jy ! Clean residual min=-0.010725 max=0.010722 Jy/beam ! Clean residual mean=0.000247 rms=0.002688 Jy/beam ! Combined flux in latest and established models = 1.03506 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 = 4.36328e-06 Jy ! Component: 100 - total flux cleaned = -0.000136319 Jy ! Component: 150 - total flux cleaned = -0.000394169 Jy ! Component: 200 - total flux cleaned = -0.000515764 Jy ! Total flux subtracted in 200 components = -0.000515764 Jy ! Clean residual min=-0.010553 max=0.010764 Jy/beam ! Clean residual mean=0.000248 rms=0.002655 Jy/beam ! Combined flux in latest and established models = 1.03455 Jy ! Adding 30 model components to the UV plane model. ! The established model now contains 57 components and 1.03455 Jy ! Inverting map ! Your choice of large map pixels excluded 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 milli-arcsec ! Estimated beam: bmin=0.7616 mas, bmaj=0.974 mas, bpa=-21.15 degrees ! Estimated noise=1.84387 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00406017 Jy ! Component: 100 - total flux cleaned = 0.00483285 Jy ! Component: 150 - total flux cleaned = 0.00483098 Jy ! Component: 200 - total flux cleaned = 0.00462118 Jy ! Total flux subtracted in 200 components = 0.00462118 Jy ! Clean residual min=-0.009145 max=0.009677 Jy/beam ! Clean residual mean=0.000057 rms=0.002362 Jy/beam ! Combined flux in latest and established models = 1.03917 Jy selfcal ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 80 components and 1.03917 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.195172Jy sigma=0.831520 ! Fit after self-cal, rms=0.195089Jy sigma=0.830657 wmodel /d2/scr/pima/rv101_uvs/J0958+4725_X_map.mod ! Writing 80 model components to file: /d2/scr/pima/rv101_uvs/J0958+4725_X_map.mod wobs /d2/scr/pima/rv101_uvs/J0958+4725_X_uvs.fits ! Writing UV FITS file: /d2/scr/pima/rv101_uvs/J0958+4725_X_uvs.fits wwins /d2/scr/pima/rv101_uvs/J0958+4725_X_map.win ! wwins: Wrote 4 windows to /d2/scr/pima/rv101_uvs/J0958+4725_X_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 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.00400671 Jy ! Component: 100 - total flux cleaned = 0.00609941 Jy ! Component: 150 - total flux cleaned = 0.00761904 Jy ! Component: 200 - total flux cleaned = 0.00827889 Jy ! Component: 250 - total flux cleaned = 0.00957244 Jy ! Component: 300 - total flux cleaned = 0.0105228 Jy ! Component: 350 - total flux cleaned = 0.0114552 Jy ! Component: 400 - total flux cleaned = 0.0122174 Jy ! Component: 450 - total flux cleaned = 0.0126654 Jy ! Component: 500 - total flux cleaned = 0.0129598 Jy ! Component: 550 - total flux cleaned = 0.0132511 Jy ! Component: 600 - total flux cleaned = 0.0138263 Jy ! Component: 650 - total flux cleaned = 0.0143908 Jy ! Component: 700 - total flux cleaned = 0.0143899 Jy ! Component: 750 - total flux cleaned = 0.014527 Jy ! Component: 800 - total flux cleaned = 0.0146628 Jy ! Component: 850 - total flux cleaned = 0.0150658 Jy ! Component: 900 - total flux cleaned = 0.0151977 Jy ! Component: 950 - total flux cleaned = 0.0155918 Jy ! Component: 1000 - total flux cleaned = 0.0157207 Jy ! Component: 1050 - total flux cleaned = 0.015978 Jy ! Component: 1100 - total flux cleaned = 0.015977 Jy ! Component: 1150 - total flux cleaned = 0.0162296 Jy ! Component: 1200 - total flux cleaned = 0.015977 Jy ! Component: 1250 - total flux cleaned = 0.0164748 Jy ! Component: 1300 - total flux cleaned = 0.0163523 Jy ! Component: 1350 - total flux cleaned = 0.0167179 Jy ! Component: 1400 - total flux cleaned = 0.0165965 Jy ! Component: 1450 - total flux cleaned = 0.0169548 Jy ! Component: 1500 - total flux cleaned = 0.0166003 Jy ! Component: 1550 - total flux cleaned = 0.0169542 Jy ! Component: 1600 - total flux cleaned = 0.0168364 Jy ! Component: 1650 - total flux cleaned = 0.0169525 Jy ! Component: 1700 - total flux cleaned = 0.0172977 Jy ! Component: 1750 - total flux cleaned = 0.0172984 Jy ! Component: 1800 - total flux cleaned = 0.0172979 Jy ! Component: 1850 - total flux cleaned = 0.0174086 Jy ! Component: 1900 - total flux cleaned = 0.0171877 Jy ! Component: 1950 - total flux cleaned = 0.0175184 Jy ! Component: 2000 - total flux cleaned = 0.0176285 Jy ! Component: 2050 - total flux cleaned = 0.0170854 Jy ! Component: 2100 - total flux cleaned = 0.0179483 Jy ! Component: 2150 - total flux cleaned = 0.0174129 Jy ! Component: 2200 - total flux cleaned = 0.0174117 Jy ! Component: 2250 - total flux cleaned = 0.0177282 Jy ! Component: 2300 - total flux cleaned = 0.0176233 Jy ! Component: 2350 - total flux cleaned = 0.0175204 Jy ! Component: 2400 - total flux cleaned = 0.0173147 Jy ! Component: 2450 - total flux cleaned = 0.0176229 Jy ! Component: 2500 - total flux cleaned = 0.0174187 Jy ! Component: 2550 - total flux cleaned = 0.0172159 Jy ! Component: 2600 - total flux cleaned = 0.0172163 Jy ! Component: 2650 - total flux cleaned = 0.0173159 Jy ! Component: 2700 - total flux cleaned = 0.0170187 Jy ! Component: 2750 - total flux cleaned = 0.017413 Jy ! Component: 2800 - total flux cleaned = 0.0168252 Jy ! Component: 2850 - total flux cleaned = 0.0172141 Jy ! Component: 2900 - total flux cleaned = 0.0166343 Jy ! Component: 2950 - total flux cleaned = 0.0164419 Jy ! Component: 3000 - total flux cleaned = 0.0167284 Jy ! Component: 3050 - total flux cleaned = 0.0165394 Jy ! Component: 3100 - total flux cleaned = 0.0170101 Jy ! Component: 3150 - total flux cleaned = 0.0164475 Jy ! Component: 3200 - total flux cleaned = 0.0167266 Jy ! Component: 3250 - total flux cleaned = 0.0166336 Jy ! Component: 3300 - total flux cleaned = 0.0166336 Jy ! Component: 3350 - total flux cleaned = 0.0165415 Jy ! Component: 3400 - total flux cleaned = 0.0165416 Jy ! Component: 3450 - total flux cleaned = 0.0166325 Jy ! Component: 3500 - total flux cleaned = 0.0164528 Jy ! Component: 3550 - total flux cleaned = 0.0166317 Jy ! Component: 3600 - total flux cleaned = 0.0163649 Jy ! Component: 3650 - total flux cleaned = 0.0167185 Jy ! Component: 3700 - total flux cleaned = 0.01663 Jy ! Component: 3750 - total flux cleaned = 0.0166295 Jy ! Component: 3800 - total flux cleaned = 0.0166285 Jy ! Component: 3850 - total flux cleaned = 0.0166283 Jy ! Component: 3900 - total flux cleaned = 0.0165421 Jy ! Component: 3950 - total flux cleaned = 0.0166279 Jy ! Component: 4000 - total flux cleaned = 0.0166282 Jy ! Component: 4050 - total flux cleaned = 0.0167967 Jy ! Total flux subtracted in 4096 components = 0.0167964 Jy ! Clean residual min=-0.004581 max=0.005015 Jy/beam ! Clean residual mean=-0.000042 rms=0.001412 Jy/beam ! Combined flux in latest and established models = 1.05596 Jy keep ! Adding 346 model components to the UV plane model. ! The established model now contains 426 components and 1.05596 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/d2/scr/pima/rv101_uvs/J0958+4725_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7616 x 0.974 at -21.15 degrees (North through East) ! Clean map min=-0.010101 max=0.92809 Jy/beam ! Writing clean map to FITS file: /d2/scr/pima/rv101_uvs/J0958+4725_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.928094 invert ! Inverting map ! Your choice of large map pixels excluded 0.905% of the data. ! The x-axis pixel size should ideally be below 0.193 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00140794 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.455105 0.455105 0.91021 1.82042 3.64084 7.28168 14.5634 29.1267 58.2535 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0042 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.928 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 659.188 quit ! Quitting program ! Log file /d2/scr/pima/rv101_uvs/J0958+4725_X_uvs.log closed on Sat Nov 29 16:32:48 2014