! Started logfile: /d2/scr/pima/rv101_uvs/J2038+5119_X_uvs.log on Sat Nov 29 16:37:32 2014 obs /d2/scr/pima/rv101_uvs/J2038+5119_X_uva.fits ! Reading UV FITS file: /d2/scr/pima/rv101_uvs/J2038+5119_X_uva.fits ! AN table 1: 17 integrations on 3 of 3 possible baselines. ! AN table 2: 17 integrations on 10 of 10 possible baselines. ! AN table 3: 111 integrations on 6 of 6 possible baselines. ! AN table 4: 17 integrations on 45 of 45 possible baselines. ! AN table 5: 9 integrations on 3 of 3 possible baselines. ! AN table 6: 11 integrations on 3 of 3 possible baselines. ! AN table 7: 14 integrations on 3 of 3 possible baselines. ! AN table 8: 11 integrations on 55 of 55 possible baselines. ! AN table 9: 9 integrations on 1 of 1 possible baselines. ! AN table 10: 19 integrations on 10 of 10 possible baselines. ! AN table 11: 39 integrations on 1 of 1 possible baselines. ! AN table 12: 20 integrations on 55 of 55 possible baselines. ! AN table 13: 9 integrations on 3 of 3 possible baselines. ! AN table 14: 96 integrations on 3 of 3 possible baselines. ! AN table 15: 32 integrations on 1 of 1 possible baselines. ! AN table 16: 9 integrations on 10 of 10 possible baselines. ! AN table 17: 20 integrations on 6 of 6 possible baselines. ! AN table 18: 19 integrations on 6 of 6 possible baselines. ! AN table 19: 19 integrations on 15 of 15 possible baselines. ! Apparent sampling: 0.694391 visibilities/baseline/integration-bin. ! Found source: J2038+5119 ! ! 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 12924 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/J2038+5119_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 30 telescope corrections were flagged in sub-array 1. ! A total of 26 telescope corrections were flagged in sub-array 2. ! A total of 114 telescope corrections were flagged in sub-array 3. ! A total of 71 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 15 telescope corrections were flagged in sub-array 6. ! A total of 21 telescope corrections were flagged in sub-array 7. ! A total of 51 telescope corrections were flagged in sub-array 8. ! A total of 18 telescope corrections were flagged in sub-array 9. ! A total of 32 telescope corrections were flagged in sub-array 10. ! A total of 78 telescope corrections were flagged in sub-array 11. ! A total of 144 telescope corrections were flagged in sub-array 12. ! A total of 9 telescope corrections were flagged in sub-array 13. ! A total of 63 telescope corrections were flagged in sub-array 14. ! A total of 64 telescope corrections were flagged in sub-array 15. ! A total of 10 telescope corrections were flagged in sub-array 16. ! A total of 28 telescope corrections were flagged in sub-array 17. ! A total of 24 telescope corrections were flagged in sub-array 18. ! A total of 44 telescope corrections were flagged in sub-array 19. ! ! Correcting IF 2. ! A total of 30 telescope corrections were flagged in sub-array 1. ! A total of 26 telescope corrections were flagged in sub-array 2. ! A total of 114 telescope corrections were flagged in sub-array 3. ! A total of 71 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 15 telescope corrections were flagged in sub-array 6. ! A total of 21 telescope corrections were flagged in sub-array 7. ! A total of 51 telescope corrections were flagged in sub-array 8. ! A total of 18 telescope corrections were flagged in sub-array 9. ! A total of 32 telescope corrections were flagged in sub-array 10. ! A total of 78 telescope corrections were flagged in sub-array 11. ! A total of 144 telescope corrections were flagged in sub-array 12. ! A total of 9 telescope corrections were flagged in sub-array 13. ! A total of 63 telescope corrections were flagged in sub-array 14. ! A total of 64 telescope corrections were flagged in sub-array 15. ! A total of 10 telescope corrections were flagged in sub-array 16. ! A total of 28 telescope corrections were flagged in sub-array 17. ! A total of 24 telescope corrections were flagged in sub-array 18. ! A total of 44 telescope corrections were flagged in sub-array 19. ! ! Correcting IF 3. ! A total of 51 telescope corrections were flagged in sub-array 1. ! A total of 57 telescope corrections were flagged in sub-array 2. ! A total of 318 telescope corrections were flagged in sub-array 3. ! A total of 104 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 33 telescope corrections were flagged in sub-array 6. ! A total of 21 telescope corrections were flagged in sub-array 7. ! A total of 58 telescope corrections were flagged in sub-array 8. ! A total of 18 telescope corrections were flagged in sub-array 9. ! A total of 64 telescope corrections were flagged in sub-array 10. ! A total of 78 telescope corrections were flagged in sub-array 11. ! A total of 157 telescope corrections were flagged in sub-array 12. ! A total of 27 telescope corrections were flagged in sub-array 13. ! A total of 288 telescope corrections were flagged in sub-array 14. ! A total of 64 telescope corrections were flagged in sub-array 15. ! A total of 10 telescope corrections were flagged in sub-array 16. ! A total of 59 telescope corrections were flagged in sub-array 17. ! A total of 55 telescope corrections were flagged in sub-array 18. ! A total of 76 telescope corrections were flagged in sub-array 19. ! ! Correcting IF 4. ! A total of 51 telescope corrections were flagged in sub-array 1. ! A total of 57 telescope corrections were flagged in sub-array 2. ! A total of 318 telescope corrections were flagged in sub-array 3. ! A total of 104 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 33 telescope corrections were flagged in sub-array 6. ! A total of 21 telescope corrections were flagged in sub-array 7. ! A total of 58 telescope corrections were flagged in sub-array 8. ! A total of 18 telescope corrections were flagged in sub-array 9. ! A total of 64 telescope corrections were flagged in sub-array 10. ! A total of 78 telescope corrections were flagged in sub-array 11. ! A total of 157 telescope corrections were flagged in sub-array 12. ! A total of 27 telescope corrections were flagged in sub-array 13. ! A total of 288 telescope corrections were flagged in sub-array 14. ! A total of 64 telescope corrections were flagged in sub-array 15. ! A total of 10 telescope corrections were flagged in sub-array 16. ! A total of 59 telescope corrections were flagged in sub-array 17. ! A total of 55 telescope corrections were flagged in sub-array 18. ! A total of 76 telescope corrections were flagged in sub-array 19. ! ! Fit before self-cal, rms=2.966521Jy sigma=10.844297 ! Fit after self-cal, rms=1.809818Jy sigma=6.328662 ! 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 0.816% of the data. ! The x-axis pixel size should ideally be below 0.1593 milli-arcsec ! Estimated beam: bmin=0.6519 mas, bmaj=0.8746 mas, bpa=42.05 degrees ! Estimated noise=3.09734 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 = 1.92674 Jy ! Component: 100 - total flux cleaned = 2.40142 Jy ! Total flux subtracted in 100 components = 2.40142 Jy ! Clean residual min=-0.060448 max=0.199648 Jy/beam ! Clean residual mean=0.001442 rms=0.015358 Jy/beam ! Combined flux in latest and established models = 2.40142 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 2.40142 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.681086Jy sigma=2.002873 ! Fit after self-cal, rms=0.680996Jy sigma=2.002111 ! Inverting map ! Your choice of large map pixels excluded 0.816% of the data. ! The x-axis pixel size should ideally be below 0.1593 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.221138 Jy ! Component: 100 - total flux cleaned = 0.349161 Jy ! Total flux subtracted in 100 components = 0.349161 Jy ! Clean residual min=-0.047930 max=0.067213 Jy/beam ! Clean residual mean=0.001016 rms=0.011636 Jy/beam ! Combined flux in latest and established models = 2.75058 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 17 components and 2.75058 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.539478Jy sigma=1.569079 ! Fit after self-cal, rms=0.539012Jy sigma=1.566610 ! Inverting map ! Your choice of large map pixels excluded 0.816% of the data. ! The x-axis pixel size should ideally be below 0.1593 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0846517 Jy ! Component: 100 - total flux cleaned = 0.140419 Jy ! Total flux subtracted in 100 components = 0.140419 Jy ! Clean residual min=-0.048746 max=0.051083 Jy/beam ! Clean residual mean=0.000846 rms=0.011032 Jy/beam ! Combined flux in latest and established models = 2.891 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 22 components and 2.891 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.503659Jy sigma=1.500649 ! Fit after self-cal, rms=0.503428Jy sigma=1.499285 ! Inverting map ! Your choice of large map pixels excluded 0.816% of the data. ! The x-axis pixel size should ideally be below 0.1593 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 0.816% of the data. ! The x-axis pixel size should ideally be below 0.1593 milli-arcsec ! Estimated beam: bmin=0.7602 mas, bmaj=1.012 mas, bpa=42.68 degrees ! Estimated noise=2.40118 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 = 0.0716175 Jy ! Component: 100 - total flux cleaned = 0.107764 Jy ! Component: 150 - total flux cleaned = 0.128225 Jy ! Component: 200 - total flux cleaned = 0.134191 Jy ! Total flux subtracted in 200 components = 0.134191 Jy ! Clean residual min=-0.057419 max=0.072611 Jy/beam ! Clean residual mean=0.004035 rms=0.013486 Jy/beam ! Combined flux in latest and established models = 3.02519 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 26 components and 3.02519 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.479569Jy sigma=1.509298 ! Fit after self-cal, rms=0.479454Jy sigma=1.508516 ! Inverting map ! Your choice of large map pixels excluded 0.816% of the data. ! The x-axis pixel size should ideally be below 0.1593 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7602 x 1.012 at 42.68 degrees (North through East) ! Clean map min=-0.055001 max=2.5827 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 21 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HN 0.00* NY 0.00* ON 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! MA 1.00* NL 1.00* NY 1.00* ON 1.00* ! SC 1.00* ! ! A total of 162 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! MA 1.04 NY 0.96 ON 0.84 WF 0.84 ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! FD 1.00* HN 1.00* LA 1.00* MA 1.00* ! NL 1.00* NY 1.00* ON 1.00* PT 1.00* ! SC 1.00* WF 1.00* ! ! A total of 21 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! FD 0.00* LA 0.00* ON 0.00* ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! NY 0.00* SC 0.00* WF 0.00* ! ! A total of 21 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! HN 0.00* MA 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! FD 1.08 HN 1.06 KP 1.00* LA 1.09 ! MK 1.06 NL 1.00 NY 1.01 OV 1.00 ! PT 1.05 SC 1.00 WF 0.85 ! ! Telescope amplitude corrections in sub-array 9: ! MK 0.00* WF 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 10. ! Telescope amplitude corrections in sub-array 10: ! HN 1.00* MA 1.00* NY 1.00* ON 1.00* ! WF 1.00* ! ! Telescope amplitude corrections in sub-array 11: ! NY 0.00* ON 0.00* ! ! A total of 6 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* ! MK 1.00* NL 1.00* NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* WF 1.00* ! ! A total of 18 telescope corrections were flagged in sub-array 13. ! Telescope amplitude corrections in sub-array 13: ! MK 0.00* NY 0.00* OV 0.00* ! ! A total of 225 telescope corrections were flagged in sub-array 14. ! Telescope amplitude corrections in sub-array 14: ! MA 0.00* NY 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 15: ! MA 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 16: ! LA 1.05 NL 0.97 OV 1.10 PT 1.02 ! WF 0.90 ! ! A total of 24 telescope corrections were flagged in sub-array 17. ! Telescope amplitude corrections in sub-array 17: ! MA 1.00* MK 1.00* NY 1.00* ON 1.00* ! ! A total of 24 telescope corrections were flagged in sub-array 18. ! Telescope amplitude corrections in sub-array 18: ! HN 1.00* MA 1.00* NY 1.00* ON 1.00* ! ! A total of 24 telescope corrections were flagged in sub-array 19. ! Telescope amplitude corrections in sub-array 19: ! HN 1.00* MA 1.00* NL 1.00* NY 1.00* ! ON 1.00* WF 1.00* ! ! ! Correcting IF 2. ! A total of 21 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HN 0.00* NY 0.00* ON 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! MA 1.00* NL 1.00* NY 1.00* ON 1.00* ! SC 1.00* ! ! A total of 162 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! MA 1.00* NY 1.00* ON 1.00* WF 1.00* ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! FD 1.00* HN 1.00* LA 1.00* MA 1.00* ! NL 1.00* NY 1.00* ON 1.00* PT 1.00* ! SC 1.00* WF 1.00* ! ! A total of 21 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! FD 0.00* LA 0.00* ON 0.00* ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! NY 0.00* SC 0.00* WF 0.00* ! ! A total of 21 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! HN 0.00* MA 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! FD 1.06 HN 1.07 KP 1.00* LA 1.03 ! MK 1.04 NL 1.04 NY 0.96 OV 0.99 ! PT 0.99 SC 1.04 WF 0.87 ! ! Telescope amplitude corrections in sub-array 9: ! MK 0.00* WF 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 10. ! Telescope amplitude corrections in sub-array 10: ! HN 1.00* MA 1.00* NY 1.00* ON 1.00* ! WF 1.00* ! ! Telescope amplitude corrections in sub-array 11: ! NY 0.00* ON 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 12. ! Telescope amplitude corrections in sub-array 12: ! FD 1.06 HN 1.07 KP 1.00* LA 1.02 ! MK 1.01 NL 1.02 NY 0.99 ON 0.86 ! OV 0.99 PT 0.96 WF 0.85 ! ! A total of 18 telescope corrections were flagged in sub-array 13. ! Telescope amplitude corrections in sub-array 13: ! MK 0.00* NY 0.00* OV 0.00* ! ! A total of 225 telescope corrections were flagged in sub-array 14. ! Telescope amplitude corrections in sub-array 14: ! MA 0.00* NY 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 15: ! MA 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 16: ! LA 0.98 NL 1.01 OV 1.06 PT 0.93 ! WF 0.95 ! ! A total of 24 telescope corrections were flagged in sub-array 17. ! Telescope amplitude corrections in sub-array 17: ! MA 1.00* MK 1.00* NY 1.00* ON 1.00* ! ! A total of 24 telescope corrections were flagged in sub-array 18. ! Telescope amplitude corrections in sub-array 18: ! HN 1.00* MA 1.00* NY 1.00* ON 1.00* ! ! A total of 24 telescope corrections were flagged in sub-array 19. ! Telescope amplitude corrections in sub-array 19: ! HN 1.07 MA 0.95 NL 1.18 NY 0.97 ! ON 0.85 WF 0.83 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! HN 0.00* NY 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! MA 1.04 NL 1.03 NY 1.00* ON 0.99 ! SC 1.13 ! ! A total of 126 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! MA 0.00* NY 0.00* ON 0.00* WF 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! FD 1.07 HN 1.10 LA 1.06 MA 1.05 ! NL 1.10 NY 1.00* ON 0.98 PT 0.91 ! SC 1.06 WF 0.88 ! ! A total of 21 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! FD 0.00* LA 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! NY 0.00* SC 0.00* WF 0.00* ! ! A total of 21 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! HN 0.00* MA 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! FD 1.06 HN 1.12 KP 1.00* LA 1.09 ! MK 1.02 NL 1.05 NY 1.00* OV 1.06 ! PT 0.93 SC 0.99 WF 0.89 ! ! Telescope amplitude corrections in sub-array 9: ! MK 0.00* WF 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 10. ! Telescope amplitude corrections in sub-array 10: ! HN 1.00* MA 1.00* NY 1.00* ON 1.00* ! WF 1.00* ! ! Telescope amplitude corrections in sub-array 11: ! NY 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 12: ! FD 1.02 HN 1.09 KP 1.00* LA 1.09 ! MK 1.00 NL 1.07 NY 1.00* ON 1.01 ! OV 1.05 PT 0.96 WF 0.88 ! ! Telescope amplitude corrections in sub-array 13: ! MK 0.00* NY 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 14: ! MA 0.00* NY 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 15: ! MA 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 16: ! LA 1.12 NL 1.01 OV 1.14 PT 0.98 ! WF 0.92 ! ! A total of 21 telescope corrections were flagged in sub-array 17. ! Telescope amplitude corrections in sub-array 17: ! MA 0.00* MK 0.00* NY 0.00* ON 0.00* ! ! A total of 21 telescope corrections were flagged in sub-array 18. ! Telescope amplitude corrections in sub-array 18: ! HN 0.00* MA 0.00* NY 0.00* ON 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 19. ! Telescope amplitude corrections in sub-array 19: ! HN 1.00* MA 1.00* NL 1.00* NY 1.00* ! ON 1.00* WF 1.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! HN 0.00* NY 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! MA 1.07 NL 1.07 NY 1.00* ON 1.04 ! SC 1.16 ! ! A total of 126 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! MA 0.00* NY 0.00* ON 0.00* WF 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! FD 1.14 HN 1.07 LA 1.09 MA 1.08 ! NL 1.09 NY 1.00* ON 1.03 PT 0.96 ! SC 1.08 WF 0.94 ! ! A total of 21 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! FD 0.00* LA 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 6: ! NY 0.00* SC 0.00* WF 0.00* ! ! A total of 21 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! HN 0.00* MA 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! FD 1.09 HN 1.11 KP 1.00* LA 1.07 ! MK 1.08 NL 1.07 NY 1.00* OV 1.02 ! PT 0.97 SC 1.02 WF 0.98 ! ! Telescope amplitude corrections in sub-array 9: ! MK 0.00* WF 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 10. ! Telescope amplitude corrections in sub-array 10: ! HN 1.00* MA 1.00* NY 1.00* ON 1.00* ! WF 1.00* ! ! Telescope amplitude corrections in sub-array 11: ! NY 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 12: ! FD 1.05 HN 1.10 KP 1.00* LA 1.05 ! MK 1.04 NL 1.08 NY 1.00* ON 1.12 ! OV 1.03 PT 1.00 WF 0.97 ! ! Telescope amplitude corrections in sub-array 13: ! MK 0.00* NY 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 14: ! MA 0.00* NY 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 15: ! MA 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 16: ! LA 1.06 NL 1.06 OV 1.13 PT 0.98 ! WF 1.02 ! ! A total of 21 telescope corrections were flagged in sub-array 17. ! Telescope amplitude corrections in sub-array 17: ! MA 0.00* MK 0.00* NY 0.00* ON 0.00* ! ! A total of 21 telescope corrections were flagged in sub-array 18. ! Telescope amplitude corrections in sub-array 18: ! HN 0.00* MA 0.00* NY 0.00* ON 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 19. ! Telescope amplitude corrections in sub-array 19: ! HN 1.00* MA 1.00* NL 1.00* NY 1.00* ! ON 1.00* WF 1.00* ! ! ! Fit before self-cal, rms=0.479454Jy sigma=1.508516 ! Fit after self-cal, rms=0.378224Jy sigma=1.174596 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Estimated beam: bmin=0.7272 mas, bmaj=1.059 mas, bpa=46.33 degrees ! Estimated noise=2.64851 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 (-9.6, -7.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.054676 Jy ! Component: 100 - total flux cleaned = 0.085031 Jy ! Component: 150 - total flux cleaned = 0.107813 Jy ! Component: 200 - total flux cleaned = 0.122156 Jy ! Total flux subtracted in 200 components = 0.122156 Jy ! Clean residual min=-0.036892 max=0.049718 Jy/beam ! Clean residual mean=0.003804 rms=0.008957 Jy/beam ! Combined flux in latest and established models = 3.14734 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 45 components and 3.14735 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.365660Jy sigma=1.140454 ! Fit after self-cal, rms=0.364390Jy sigma=1.135390 ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Added new window around map position (-3.2, -6.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0565713 Jy ! Component: 100 - total flux cleaned = 0.0946314 Jy ! Component: 150 - total flux cleaned = 0.121797 Jy ! Component: 200 - total flux cleaned = 0.14107 Jy ! Total flux subtracted in 200 components = 0.14107 Jy ! Clean residual min=-0.031981 max=0.038071 Jy/beam ! Clean residual mean=0.002653 rms=0.007758 Jy/beam ! Combined flux in latest and established models = 3.28842 Jy ! Performing phase self-cal ! Adding 31 model components to the UV plane model. ! The established model now contains 74 components and 3.28842 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.351635Jy sigma=1.085728 ! Fit after self-cal, rms=0.350452Jy sigma=1.080570 ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 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=0.350452Jy sigma=1.080570 ! Fit after self-cal, rms=0.311452Jy sigma=0.929282 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Estimated beam: bmin=0.727 mas, bmaj=1.06 mas, bpa=46.13 degrees ! Estimated noise=2.66364 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.024065 Jy ! Component: 100 - total flux cleaned = 0.042273 Jy ! Component: 150 - total flux cleaned = 0.0572397 Jy ! Component: 200 - total flux cleaned = 0.069917 Jy ! Total flux subtracted in 200 components = 0.069917 Jy ! Clean residual min=-0.020404 max=0.031557 Jy/beam ! Clean residual mean=0.002091 rms=0.005778 Jy/beam ! Combined flux in latest and established models = 3.35833 Jy selfcal ! Performing phase self-cal ! Adding 35 model components to the UV plane model. ! The established model now contains 93 components and 3.35833 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.307138Jy sigma=0.920526 ! Fit after self-cal, rms=0.306964Jy sigma=0.919874 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 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 (-11.6, -16.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0312779 Jy ! Component: 100 - total flux cleaned = 0.0482219 Jy ! Component: 150 - total flux cleaned = 0.0568326 Jy ! Component: 200 - total flux cleaned = 0.0643748 Jy ! Total flux subtracted in 200 components = 0.0643748 Jy ! Clean residual min=-0.019698 max=0.025787 Jy/beam ! Clean residual mean=0.001648 rms=0.005385 Jy/beam ! Combined flux in latest and established models = 3.42271 Jy ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 112 components and 3.42271 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.302489Jy sigma=0.905829 ! Fit after self-cal, rms=0.302285Jy sigma=0.904351 ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Added new window around map position (7, 5.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.017332 Jy ! Component: 100 - total flux cleaned = 0.0241038 Jy ! Component: 150 - total flux cleaned = 0.0272586 Jy ! Component: 200 - total flux cleaned = 0.0305344 Jy ! Total flux subtracted in 200 components = 0.0305344 Jy ! Clean residual min=-0.020874 max=0.023871 Jy/beam ! Clean residual mean=0.001413 rms=0.005284 Jy/beam ! Combined flux in latest and established models = 3.45324 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 128 components and 3.45324 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.299057Jy sigma=0.899487 ! Fit after self-cal, rms=0.298923Jy sigma=0.898709 ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Added new window around map position (2, -15.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0196833 Jy ! Component: 100 - total flux cleaned = 0.0229221 Jy ! Component: 150 - total flux cleaned = 0.024519 Jy ! Component: 200 - total flux cleaned = 0.0259939 Jy ! Total flux subtracted in 200 components = 0.0259939 Jy ! Clean residual min=-0.019971 max=0.021436 Jy/beam ! Clean residual mean=0.001216 rms=0.005132 Jy/beam ! Combined flux in latest and established models = 3.47924 Jy ! Performing phase self-cal ! Adding 31 model components to the UV plane model. ! The established model now contains 142 components and 3.47924 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.296336Jy sigma=0.893849 ! Fit after self-cal, rms=0.296221Jy sigma=0.893299 ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Added new window around map position (-2.4, -31.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0195137 Jy ! Component: 100 - total flux cleaned = 0.0255128 Jy ! Component: 150 - total flux cleaned = 0.0284108 Jy ! Component: 200 - total flux cleaned = 0.0321569 Jy ! Total flux subtracted in 200 components = 0.0321569 Jy ! Clean residual min=-0.018984 max=0.020661 Jy/beam ! Clean residual mean=0.001040 rms=0.004968 Jy/beam ! Combined flux in latest and established models = 3.51139 Jy ! Performing phase self-cal ! Adding 33 model components to the UV plane model. ! The established model now contains 158 components and 3.51139 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.293895Jy sigma=0.886805 ! Fit after self-cal, rms=0.293812Jy sigma=0.886272 ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 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=0.293812Jy sigma=0.886272 ! Fit after self-cal, rms=0.248802Jy sigma=0.768203 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Estimated beam: bmin=0.7266 mas, bmaj=1.061 mas, bpa=46.07 degrees ! Estimated noise=2.66662 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0122425 Jy ! Component: 100 - total flux cleaned = 0.0216998 Jy ! Component: 150 - total flux cleaned = 0.0268848 Jy ! Component: 200 - total flux cleaned = 0.0310062 Jy ! Total flux subtracted in 200 components = 0.0310062 Jy ! Clean residual min=-0.015471 max=0.017818 Jy/beam ! Clean residual mean=0.000801 rms=0.003969 Jy/beam ! Combined flux in latest and established models = 3.5424 Jy selfcal ! Performing phase self-cal ! Adding 33 model components to the UV plane model. ! The established model now contains 178 components and 3.5424 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.247442Jy sigma=0.764306 ! Fit after self-cal, rms=0.247371Jy sigma=0.764090 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 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 (-4.8, -4.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0169167 Jy ! Component: 100 - total flux cleaned = 0.0233662 Jy ! Component: 150 - total flux cleaned = 0.023679 Jy ! Component: 200 - total flux cleaned = 0.0239637 Jy ! Total flux subtracted in 200 components = 0.0239637 Jy ! Clean residual min=-0.014881 max=0.017300 Jy/beam ! Clean residual mean=0.000599 rms=0.003830 Jy/beam ! Combined flux in latest and established models = 3.56636 Jy ! Performing phase self-cal ! Adding 31 model components to the UV plane model. ! The established model now contains 194 components and 3.56636 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.245692Jy sigma=0.758935 ! Fit after self-cal, rms=0.245540Jy sigma=0.758404 ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Added new window around map position (1, -13.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0150706 Jy ! Component: 100 - total flux cleaned = 0.0191509 Jy ! Component: 150 - total flux cleaned = 0.0202884 Jy ! Component: 200 - total flux cleaned = 0.0205574 Jy ! Total flux subtracted in 200 components = 0.0205574 Jy ! Clean residual min=-0.014877 max=0.015666 Jy/beam ! Clean residual mean=0.000437 rms=0.003741 Jy/beam ! Combined flux in latest and established models = 3.58692 Jy ! Performing phase self-cal ! Adding 36 model components to the UV plane model. ! The established model now contains 210 components and 3.58692 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.244026Jy sigma=0.754956 ! Fit after self-cal, rms=0.243916Jy sigma=0.754407 ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 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=0.243916Jy sigma=0.754407 ! Fit after self-cal, rms=0.243353Jy sigma=0.752067 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Estimated beam: bmin=1.945 mas, bmaj=2.831 mas, bpa=66.01 degrees ! Estimated noise=4.219 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0182491 Jy ! Component: 100 - total flux cleaned = 0.0256524 Jy ! Component: 150 - total flux cleaned = 0.0291993 Jy ! Component: 200 - total flux cleaned = 0.0318026 Jy ! Total flux subtracted in 200 components = 0.0318026 Jy ! Clean residual min=-0.020922 max=0.020959 Jy/beam ! Clean residual mean=0.001334 rms=0.005408 Jy/beam ! Combined flux in latest and established models = 3.61872 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 218 components and 3.61872 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.242792Jy sigma=0.753227 ! Fit after self-cal, rms=0.242577Jy sigma=0.752424 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 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 = 0.00513279 Jy ! Component: 100 - total flux cleaned = 0.00515239 Jy ! Component: 150 - total flux cleaned = 0.00447765 Jy ! Component: 200 - total flux cleaned = 0.00384957 Jy ! Total flux subtracted in 200 components = 0.00384957 Jy ! Clean residual min=-0.020294 max=0.020782 Jy/beam ! Clean residual mean=0.001193 rms=0.005269 Jy/beam ! Combined flux in latest and established models = 3.62257 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 227 components and 3.62257 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.242688Jy sigma=0.754063 ! Fit after self-cal, rms=0.242643Jy sigma=0.753863 ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 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 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Estimated beam: bmin=0.7261 mas, bmaj=1.061 mas, bpa=46.03 degrees ! Estimated noise=2.66856 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7261 x 1.061 at 46.03 degrees (North through East) ! Clean map min=-0.017527 max=2.5953 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=0.242643Jy sigma=0.753863 ! Fit after self-cal, rms=0.221224Jy sigma=0.675929 ! Inverting map and beam ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Estimated beam: bmin=0.7255 mas, bmaj=1.06 mas, bpa=46.08 degrees ! Estimated noise=2.66852 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000863967 Jy ! Component: 100 - total flux cleaned = 0.000523566 Jy ! Component: 150 - total flux cleaned = 0.00141311 Jy ! Component: 200 - total flux cleaned = 0.0016937 Jy ! Total flux subtracted in 200 components = 0.0016937 Jy ! Clean residual min=-0.014396 max=0.016309 Jy/beam ! Clean residual mean=0.000348 rms=0.003485 Jy/beam ! Combined flux in latest and established models = 3.62427 Jy ! Performing phase self-cal ! Adding 32 model components to the UV plane model. ! The established model now contains 237 components and 3.62427 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.220330Jy sigma=0.672673 ! Fit after self-cal, rms=0.220313Jy sigma=0.672576 ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Added new window around map position (-15.8, -32.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0126238 Jy ! Component: 100 - total flux cleaned = 0.0129109 Jy ! Component: 150 - total flux cleaned = 0.0131774 Jy ! Component: 200 - total flux cleaned = 0.0124498 Jy ! Total flux subtracted in 200 components = 0.0124498 Jy ! Clean residual min=-0.016062 max=0.014045 Jy/beam ! Clean residual mean=0.000300 rms=0.003401 Jy/beam ! Combined flux in latest and established models = 3.63671 Jy ! Performing phase self-cal ! Adding 44 model components to the UV plane model. ! The established model now contains 255 components and 3.63671 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.219080Jy sigma=0.668571 ! Fit after self-cal, rms=0.219033Jy sigma=0.668230 ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.219033Jy sigma=0.668230 ! Fit after self-cal, rms=0.218852Jy sigma=0.667567 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 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Estimated beam: bmin=0.6432 mas, bmaj=0.9224 mas, bpa=45.85 degrees ! Estimated noise=3.40444 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.97562 Jy ! Component: 100 - total flux cleaned = 2.46241 Jy ! Component: 150 - total flux cleaned = 2.68215 Jy ! Component: 200 - total flux cleaned = 2.81404 Jy ! Total flux subtracted in 200 components = 2.81404 Jy ! Clean residual min=-0.031827 max=0.070461 Jy/beam ! Clean residual mean=0.001139 rms=0.007817 Jy/beam ! Combined flux in latest and established models = 2.81404 Jy uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Adding 16 model components to the UV plane model. ! The established model now contains 16 components and 2.81404 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Estimated beam: bmin=0.7252 mas, bmaj=1.061 mas, bpa=46.06 degrees ! Estimated noise=2.66867 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 = 0.1181 Jy ! Component: 100 - total flux cleaned = 0.199512 Jy ! Component: 150 - total flux cleaned = 0.265663 Jy ! Component: 200 - total flux cleaned = 0.321149 Jy ! Total flux subtracted in 200 components = 0.321149 Jy ! Clean residual min=-0.020033 max=0.043537 Jy/beam ! Clean residual mean=0.004124 rms=0.007276 Jy/beam ! Combined flux in latest and established models = 3.13519 Jy ! Adding 48 model components to the UV plane model. ! The established model now contains 52 components and 3.13519 Jy ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Added new window around map position (-5.8, -6.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0508888 Jy ! Component: 100 - total flux cleaned = 0.0931343 Jy ! Component: 150 - total flux cleaned = 0.130609 Jy ! Component: 200 - total flux cleaned = 0.164173 Jy ! Total flux subtracted in 200 components = 0.164173 Jy ! Clean residual min=-0.017366 max=0.028153 Jy/beam ! Clean residual mean=0.002827 rms=0.005413 Jy/beam ! Combined flux in latest and established models = 3.29936 Jy ! Adding 64 model components to the UV plane model. ! The established model now contains 97 components and 3.29936 Jy ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Added new window around map position (-0.6, -4.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0319032 Jy ! Component: 100 - total flux cleaned = 0.0597286 Jy ! Component: 150 - total flux cleaned = 0.0850324 Jy ! Component: 200 - total flux cleaned = 0.10811 Jy ! Total flux subtracted in 200 components = 0.10811 Jy ! Clean residual min=-0.016137 max=0.021154 Jy/beam ! Clean residual mean=0.001992 rms=0.004475 Jy/beam ! Combined flux in latest and established models = 3.40747 Jy ! Adding 56 model components to the UV plane model. ! The established model now contains 119 components and 3.40747 Jy ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Added new window around map position (-42, -8.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0228259 Jy ! Component: 100 - total flux cleaned = 0.040169 Jy ! Component: 150 - total flux cleaned = 0.0562339 Jy ! Component: 200 - total flux cleaned = 0.0705074 Jy ! Total flux subtracted in 200 components = 0.0705074 Jy ! Clean residual min=-0.015449 max=0.017575 Jy/beam ! Clean residual mean=0.001501 rms=0.003953 Jy/beam ! Combined flux in latest and established models = 3.47798 Jy ! Adding 66 model components to the UV plane model. ! The established model now contains 141 components and 3.47798 Jy ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Added new window around map position (-3, -2.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0160321 Jy ! Component: 100 - total flux cleaned = 0.02756 Jy ! Component: 150 - total flux cleaned = 0.0389181 Jy ! Component: 200 - total flux cleaned = 0.0490417 Jy ! Total flux subtracted in 200 components = 0.0490417 Jy ! Clean residual min=-0.014480 max=0.016230 Jy/beam ! Clean residual mean=0.001135 rms=0.003636 Jy/beam ! Combined flux in latest and established models = 3.52702 Jy ! Adding 66 model components to the UV plane model. ! The established model now contains 167 components and 3.52702 Jy ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Added new window around map position (11, -5.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.013764 Jy ! Component: 100 - total flux cleaned = 0.0229951 Jy ! Component: 150 - total flux cleaned = 0.0321275 Jy ! Component: 200 - total flux cleaned = 0.040742 Jy ! Total flux subtracted in 200 components = 0.040742 Jy ! Clean residual min=-0.013706 max=0.014760 Jy/beam ! Clean residual mean=0.000840 rms=0.003418 Jy/beam ! Combined flux in latest and established models = 3.56776 Jy ! Adding 65 model components to the UV plane model. ! The established model now contains 190 components and 3.56776 Jy ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Added new window around map position (-1.4, -8.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0135099 Jy ! Component: 100 - total flux cleaned = 0.0219462 Jy ! Component: 150 - total flux cleaned = 0.0290694 Jy ! Component: 200 - total flux cleaned = 0.0351094 Jy ! Total flux subtracted in 200 components = 0.0351094 Jy ! Clean residual min=-0.013191 max=0.013714 Jy/beam ! Clean residual mean=0.000576 rms=0.003270 Jy/beam ! Combined flux in latest and established models = 3.60287 Jy ! Adding 58 model components to the UV plane model. ! The established model now contains 206 components and 3.60287 Jy ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 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 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Estimated beam: bmin=1.943 mas, bmaj=2.83 mas, bpa=66.05 degrees ! Estimated noise=4.22891 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0176163 Jy ! Component: 100 - total flux cleaned = 0.0292947 Jy ! Component: 150 - total flux cleaned = 0.0359861 Jy ! Component: 200 - total flux cleaned = 0.0395227 Jy ! Total flux subtracted in 200 components = 0.0395227 Jy ! Clean residual min=-0.015092 max=0.017817 Jy/beam ! Clean residual mean=0.001022 rms=0.004201 Jy/beam ! Combined flux in latest and established models = 3.64239 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 = 0.0011891 Jy ! Component: 100 - total flux cleaned = 0.00231491 Jy ! Component: 150 - total flux cleaned = 0.00284678 Jy ! Component: 200 - total flux cleaned = 0.00310137 Jy ! Total flux subtracted in 200 components = 0.00310137 Jy ! Clean residual min=-0.014825 max=0.017368 Jy/beam ! Clean residual mean=0.000973 rms=0.004097 Jy/beam ! Combined flux in latest and established models = 3.6455 Jy ! Adding 38 model components to the UV plane model. ! The established model now contains 234 components and 3.6455 Jy ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! Estimated beam: bmin=0.7252 mas, bmaj=1.061 mas, bpa=46.06 degrees ! Estimated noise=2.66867 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00672176 Jy ! Component: 100 - total flux cleaned = -0.00705971 Jy ! Component: 150 - total flux cleaned = -0.00615138 Jy ! Component: 200 - total flux cleaned = -0.00527101 Jy ! Total flux subtracted in 200 components = -0.00527101 Jy ! Clean residual min=-0.013132 max=0.013282 Jy/beam ! Clean residual mean=0.000319 rms=0.003127 Jy/beam ! Combined flux in latest and established models = 3.64023 Jy selfcal ! Performing phase self-cal ! Adding 37 model components to the UV plane model. ! The established model now contains 252 components and 3.64023 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.215851Jy sigma=0.658395 ! Fit after self-cal, rms=0.214868Jy sigma=0.653335 wmodel /d2/scr/pima/rv101_uvs/J2038+5119_X_map.mod ! Writing 252 model components to file: /d2/scr/pima/rv101_uvs/J2038+5119_X_map.mod wobs /d2/scr/pima/rv101_uvs/J2038+5119_X_uvs.fits ! Writing UV FITS file: /d2/scr/pima/rv101_uvs/J2038+5119_X_uvs.fits wwins /d2/scr/pima/rv101_uvs/J2038+5119_X_map.win ! wwins: Wrote 16 windows to /d2/scr/pima/rv101_uvs/J2038+5119_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 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.00289213 Jy ! Component: 100 - total flux cleaned = 0.0026758 Jy ! Component: 150 - total flux cleaned = 0.00288654 Jy ! Component: 200 - total flux cleaned = 0.00288332 Jy ! Component: 250 - total flux cleaned = 0.00349978 Jy ! Component: 300 - total flux cleaned = 0.00390597 Jy ! Component: 350 - total flux cleaned = 0.00450342 Jy ! Component: 400 - total flux cleaned = 0.00509215 Jy ! Component: 450 - total flux cleaned = 0.0056698 Jy ! Component: 500 - total flux cleaned = 0.00643421 Jy ! Component: 550 - total flux cleaned = 0.00737776 Jy ! Component: 600 - total flux cleaned = 0.00830879 Jy ! Component: 650 - total flux cleaned = 0.00885985 Jy ! Component: 700 - total flux cleaned = 0.00922726 Jy ! Component: 750 - total flux cleaned = 0.00994827 Jy ! Component: 800 - total flux cleaned = 0.0101285 Jy ! Component: 850 - total flux cleaned = 0.0106603 Jy ! Component: 900 - total flux cleaned = 0.0110117 Jy ! Component: 950 - total flux cleaned = 0.011532 Jy ! Component: 1000 - total flux cleaned = 0.0117037 Jy ! Component: 1050 - total flux cleaned = 0.0122153 Jy ! Component: 1100 - total flux cleaned = 0.0125549 Jy ! Component: 1150 - total flux cleaned = 0.0132231 Jy ! Component: 1200 - total flux cleaned = 0.0133871 Jy ! Component: 1250 - total flux cleaned = 0.0135528 Jy ! Component: 1300 - total flux cleaned = 0.0142057 Jy ! Component: 1350 - total flux cleaned = 0.0143683 Jy ! Component: 1400 - total flux cleaned = 0.0151728 Jy ! Component: 1450 - total flux cleaned = 0.0153317 Jy ! Component: 1500 - total flux cleaned = 0.0158073 Jy ! Component: 1550 - total flux cleaned = 0.0161233 Jy ! Component: 1600 - total flux cleaned = 0.0167485 Jy ! Component: 1650 - total flux cleaned = 0.0172152 Jy ! Component: 1700 - total flux cleaned = 0.0175228 Jy ! Component: 1750 - total flux cleaned = 0.0179827 Jy ! Component: 1800 - total flux cleaned = 0.0184383 Jy ! Component: 1850 - total flux cleaned = 0.0188907 Jy ! Component: 1900 - total flux cleaned = 0.0194919 Jy ! Component: 1950 - total flux cleaned = 0.019641 Jy ! Component: 2000 - total flux cleaned = 0.0200862 Jy ! Component: 2050 - total flux cleaned = 0.0208217 Jy ! Component: 2100 - total flux cleaned = 0.0214061 Jy ! Component: 2150 - total flux cleaned = 0.021696 Jy ! Component: 2200 - total flux cleaned = 0.021839 Jy ! Component: 2250 - total flux cleaned = 0.0224129 Jy ! Component: 2300 - total flux cleaned = 0.0229833 Jy ! Component: 2350 - total flux cleaned = 0.0232658 Jy ! Component: 2400 - total flux cleaned = 0.0236881 Jy ! Component: 2450 - total flux cleaned = 0.0241084 Jy ! Component: 2500 - total flux cleaned = 0.0245263 Jy ! Component: 2550 - total flux cleaned = 0.0249429 Jy ! Component: 2600 - total flux cleaned = 0.0257681 Jy ! Component: 2650 - total flux cleaned = 0.0261783 Jy ! Component: 2700 - total flux cleaned = 0.0263137 Jy ! Component: 2750 - total flux cleaned = 0.0265847 Jy ! Component: 2800 - total flux cleaned = 0.027258 Jy ! Component: 2850 - total flux cleaned = 0.0275249 Jy ! Component: 2900 - total flux cleaned = 0.0276583 Jy ! Component: 2950 - total flux cleaned = 0.0280552 Jy ! Component: 3000 - total flux cleaned = 0.0288461 Jy ! Component: 3050 - total flux cleaned = 0.0289777 Jy ! Component: 3100 - total flux cleaned = 0.0291075 Jy ! Component: 3150 - total flux cleaned = 0.0294966 Jy ! Component: 3200 - total flux cleaned = 0.029626 Jy ! Component: 3250 - total flux cleaned = 0.0297552 Jy ! Component: 3300 - total flux cleaned = 0.030011 Jy ! Component: 3350 - total flux cleaned = 0.0306465 Jy ! Component: 3400 - total flux cleaned = 0.0306467 Jy ! Component: 3450 - total flux cleaned = 0.0308986 Jy ! Component: 3500 - total flux cleaned = 0.0306483 Jy ! Component: 3550 - total flux cleaned = 0.0312726 Jy ! Component: 3600 - total flux cleaned = 0.0317689 Jy ! Component: 3650 - total flux cleaned = 0.0318922 Jy ! Component: 3700 - total flux cleaned = 0.032015 Jy ! Component: 3750 - total flux cleaned = 0.0322594 Jy ! Component: 3800 - total flux cleaned = 0.0322591 Jy ! Component: 3850 - total flux cleaned = 0.0323801 Jy ! Component: 3900 - total flux cleaned = 0.032983 Jy ! Component: 3950 - total flux cleaned = 0.0332228 Jy ! Component: 4000 - total flux cleaned = 0.0334616 Jy ! Component: 4050 - total flux cleaned = 0.0334609 Jy ! Total flux subtracted in 4096 components = 0.0333419 Jy ! Clean residual min=-0.007574 max=0.007519 Jy/beam ! Clean residual mean=0.000104 rms=0.002070 Jy/beam ! Combined flux in latest and established models = 3.67357 Jy keep ! Adding 393 model components to the UV plane model. ! The established model now contains 645 components and 3.67357 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/d2/scr/pima/rv101_uvs/J2038+5119_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7252 x 1.061 at 46.06 degrees (North through East) ! Clean map min=-0.017283 max=2.6003 Jy/beam ! Writing clean map to FITS file: /d2/scr/pima/rv101_uvs/J2038+5119_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 2.60027 invert ! Inverting map ! Your choice of large map pixels excluded 0.543% of the data. ! The x-axis pixel size should ideally be below 0.1672 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00205332 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.236897 0.236897 0.473793 0.947586 1.89517 3.79035 7.58069 15.1614 30.3228 60.6455 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0061 print "peak= ", int(1000*peak_flux)/1000 ! peak= 2.6 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 1266.38 quit ! Quitting program ! Log file /d2/scr/pima/rv101_uvs/J2038+5119_X_uvs.log closed on Sat Nov 29 16:37:39 2014