! Started logfile: /scr/pima/rv102_uvs/J2230+6946_X_uvs.log on Sat Feb 27 22:29:05 2016 obs /scr/pima/rv102_uvs/J2230+6946_X_uva.fits ! Reading UV FITS file: /scr/pima/rv102_uvs/J2230+6946_X_uva.fits ! AN table 1: 292 integrations on 10 of 10 possible baselines. ! AN table 2: 9 integrations on 6 of 6 possible baselines. ! AN table 3: 74 integrations on 78 of 78 possible baselines. ! AN table 4: 14 integrations on 1 of 1 possible baselines. ! AN table 5: 10 integrations on 36 of 36 possible baselines. ! AN table 6: 9 integrations on 45 of 45 possible baselines. ! AN table 7: 145 integrations on 6 of 6 possible baselines. ! AN table 8: 7 integrations on 1 of 1 possible baselines. ! AN table 9: 15 integrations on 1 of 1 possible baselines. ! AN table 10: 146 integrations on 3 of 3 possible baselines. ! AN table 11: 36 integrations on 3 of 3 possible baselines. ! AN table 12: 41 integrations on 66 of 66 possible baselines. ! AN table 13: 40 integrations on 15 of 15 possible baselines. ! AN table 14: 9 integrations on 28 of 28 possible baselines. ! Apparent sampling: 0.606983 visibilities/baseline/integration-bin. ! Found source: J2230+6946 ! ! 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 139 lines of history. ! ! Reading 35256 visibilities. select rr, 1,2,3,4,6,7,8 ! Restricting channel ranges to the available 4 channels. ! 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 /scr/pima/rv102_uvs/J2230+6946_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 764 telescope corrections were flagged in sub-array 1. ! A total of 36 telescope corrections were flagged in sub-array 2. ! A total of 119 telescope corrections were flagged in sub-array 3. ! A total of 28 telescope corrections were flagged in sub-array 4. ! A total of 28 telescope corrections were flagged in sub-array 5. ! A total of 27 telescope corrections were flagged in sub-array 6. ! A total of 292 telescope corrections were flagged in sub-array 7. ! A total of 14 telescope corrections were flagged in sub-array 8. ! A total of 30 telescope corrections were flagged in sub-array 9. ! A total of 438 telescope corrections were flagged in sub-array 10. ! A total of 108 telescope corrections were flagged in sub-array 11. ! A total of 226 telescope corrections were flagged in sub-array 12. ! A total of 138 telescope corrections were flagged in sub-array 13. ! A total of 16 telescope corrections were flagged in sub-array 14. ! ! Correcting IF 2. ! A total of 764 telescope corrections were flagged in sub-array 1. ! A total of 36 telescope corrections were flagged in sub-array 2. ! A total of 119 telescope corrections were flagged in sub-array 3. ! A total of 28 telescope corrections were flagged in sub-array 4. ! A total of 28 telescope corrections were flagged in sub-array 5. ! A total of 27 telescope corrections were flagged in sub-array 6. ! A total of 292 telescope corrections were flagged in sub-array 7. ! A total of 14 telescope corrections were flagged in sub-array 8. ! A total of 30 telescope corrections were flagged in sub-array 9. ! A total of 438 telescope corrections were flagged in sub-array 10. ! A total of 108 telescope corrections were flagged in sub-array 11. ! A total of 226 telescope corrections were flagged in sub-array 12. ! A total of 138 telescope corrections were flagged in sub-array 13. ! A total of 16 telescope corrections were flagged in sub-array 14. ! ! Correcting IF 3. ! A total of 1100 telescope corrections were flagged in sub-array 1. ! A total of 36 telescope corrections were flagged in sub-array 2. ! A total of 190 telescope corrections were flagged in sub-array 3. ! A total of 28 telescope corrections were flagged in sub-array 4. ! A total of 35 telescope corrections were flagged in sub-array 5. ! A total of 27 telescope corrections were flagged in sub-array 6. ! A total of 580 telescope corrections were flagged in sub-array 7. ! A total of 14 telescope corrections were flagged in sub-array 8. ! A total of 30 telescope corrections were flagged in sub-array 9. ! A total of 438 telescope corrections were flagged in sub-array 10. ! A total of 108 telescope corrections were flagged in sub-array 11. ! A total of 272 telescope corrections were flagged in sub-array 12. ! A total of 195 telescope corrections were flagged in sub-array 13. ! A total of 23 telescope corrections were flagged in sub-array 14. ! ! Correcting IF 4. ! A total of 1100 telescope corrections were flagged in sub-array 1. ! A total of 36 telescope corrections were flagged in sub-array 2. ! A total of 190 telescope corrections were flagged in sub-array 3. ! A total of 28 telescope corrections were flagged in sub-array 4. ! A total of 35 telescope corrections were flagged in sub-array 5. ! A total of 27 telescope corrections were flagged in sub-array 6. ! A total of 580 telescope corrections were flagged in sub-array 7. ! A total of 14 telescope corrections were flagged in sub-array 8. ! A total of 30 telescope corrections were flagged in sub-array 9. ! A total of 438 telescope corrections were flagged in sub-array 10. ! A total of 108 telescope corrections were flagged in sub-array 11. ! A total of 272 telescope corrections were flagged in sub-array 12. ! A total of 195 telescope corrections were flagged in sub-array 13. ! A total of 23 telescope corrections were flagged in sub-array 14. ! ! Fit before self-cal, rms=1.185331Jy sigma=11.745564 ! Fit after self-cal, rms=0.623837Jy sigma=7.912545 ! 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 3.05% of the data. ! The x-axis pixel size should ideally be below 0.1716 milli-arcsec ! Estimated beam: bmin=0.5457 mas, bmaj=0.8017 mas, bpa=-27.28 degrees ! Estimated noise=1.02328 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 = 0.3137 Jy ! Component: 100 - total flux cleaned = 0.390525 Jy ! Total flux subtracted in 100 components = 0.390525 Jy ! Clean residual min=-0.053294 max=0.078113 Jy/beam ! Clean residual mean=0.000300 rms=0.009495 Jy/beam ! Combined flux in latest and established models = 0.390525 Jy ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 4 components and 0.390525 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.362842Jy sigma=3.374723 ! Fit after self-cal, rms=0.362350Jy sigma=3.366287 ! Inverting map ! Your choice of large map pixels excluded 3.05% of the data. ! The x-axis pixel size should ideally be below 0.1716 milli-arcsec ! Added new window around map position (-1.4, 3.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0658155 Jy ! Component: 100 - total flux cleaned = 0.0770136 Jy ! Total flux subtracted in 100 components = 0.0770136 Jy ! Clean residual min=-0.048695 max=0.068985 Jy/beam ! Clean residual mean=0.000234 rms=0.008705 Jy/beam ! Combined flux in latest and established models = 0.467539 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 12 components and 0.467539 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.343635Jy sigma=3.094723 ! Fit after self-cal, rms=0.341852Jy sigma=3.075555 ! Inverting map ! Your choice of large map pixels excluded 3.05% of the data. ! The x-axis pixel size should ideally be below 0.1716 milli-arcsec ! Added new window around map position (2.2, -2.6). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0525538 Jy ! Component: 100 - total flux cleaned = 0.0701874 Jy ! Total flux subtracted in 100 components = 0.0701874 Jy ! Clean residual min=-0.045556 max=0.051700 Jy/beam ! Clean residual mean=0.000176 rms=0.008113 Jy/beam ! Combined flux in latest and established models = 0.537726 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 18 components and 0.537726 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.329181Jy sigma=2.866863 ! Fit after self-cal, rms=0.327979Jy sigma=2.856282 ! Inverting map ! Your choice of large map pixels excluded 3.05% of the data. ! The x-axis pixel size should ideally be below 0.1716 milli-arcsec ! Added new window around map position (2.2, 9). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0436259 Jy ! Component: 100 - total flux cleaned = 0.0538103 Jy ! Total flux subtracted in 100 components = 0.0538103 Jy ! Clean residual min=-0.043739 max=0.045931 Jy/beam ! Clean residual mean=0.000131 rms=0.007742 Jy/beam ! Combined flux in latest and established models = 0.591536 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 22 components and 0.591537 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.320822Jy sigma=2.748371 ! Fit after self-cal, rms=0.320120Jy sigma=2.739609 ! Inverting map ! Your choice of large map pixels excluded 3.05% of the data. ! The x-axis pixel size should ideally be below 0.1716 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 3.05% of the data. ! The x-axis pixel size should ideally be below 0.1716 milli-arcsec ! Estimated beam: bmin=0.6379 mas, bmaj=0.8958 mas, bpa=-18.44 degrees ! Estimated noise=0.547772 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 = 0.0621708 Jy ! Component: 100 - total flux cleaned = 0.0775644 Jy ! Component: 150 - total flux cleaned = 0.0877719 Jy ! Component: 200 - total flux cleaned = 0.0943328 Jy ! Total flux subtracted in 200 components = 0.0943328 Jy ! Clean residual min=-0.046452 max=0.044484 Jy/beam ! Clean residual mean=0.000468 rms=0.010028 Jy/beam ! Combined flux in latest and established models = 0.685869 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 31 components and 0.685869 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.311490Jy sigma=2.462294 ! Fit after self-cal, rms=0.310120Jy sigma=2.443241 ! Inverting map ! Your choice of large map pixels excluded 3.05% of the data. ! The x-axis pixel size should ideally be below 0.1716 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6379 x 0.8958 at -18.44 degrees (North through East) ! Clean map min=-0.043761 max=0.37591 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 120 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! MA 1.00* NY 1.00* ON 1.00* WF 1.00* ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! HN 0.00* LA 0.00* PT 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! MA 1.00* MK 1.00* NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* WF 1.00* ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* NY 1.00* OV 1.00* ! PT 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* WF 1.00* ! ! A total of 288 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! MA 0.00* NY 0.00* ON 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! HN 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 9: ! MA 0.00* MK 0.00* ! ! Telescope amplitude corrections in sub-array 10: ! MA 0.00* ON 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 11: ! MA 0.00* NY 0.00* WZ 0.00* ! ! A total of 21 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* WF 1.00* WZ 1.00* ! ! A total of 27 telescope corrections were flagged in sub-array 13. ! Telescope amplitude corrections in sub-array 13: ! HN 1.00* MA 1.00* NY 1.00* ON 1.00* ! WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 14: ! FD 1.00* HN 1.00* LA 1.00* NL 1.00* ! NY 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! ! Correcting IF 2. ! A total of 120 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! MA 1.00* NY 1.00* ON 1.00* WF 1.00* ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! HN 0.00* LA 0.00* PT 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! MA 1.00* MK 1.00* NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* WF 1.00* ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* NY 1.00* OV 1.00* ! PT 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* WF 1.00* ! ! A total of 288 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! MA 0.00* NY 0.00* ON 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! HN 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 9: ! MA 0.00* MK 0.00* ! ! Telescope amplitude corrections in sub-array 10: ! MA 0.00* ON 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 11: ! MA 0.00* NY 0.00* WZ 0.00* ! ! A total of 21 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* WF 1.00* WZ 1.00* ! ! A total of 27 telescope corrections were flagged in sub-array 13. ! Telescope amplitude corrections in sub-array 13: ! HN 1.00* MA 1.00* NY 1.00* ON 1.00* ! WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 14: ! FD 1.00* HN 1.00* LA 1.00* NL 1.00* ! NY 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! ! Correcting IF 3. ! A total of 360 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! MA 0.00* NY 0.00* ON 0.00* WF 0.00* ! WZ 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! HN 0.00* LA 0.00* PT 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! MA 1.00* MK 1.00* NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* WF 1.00* ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* NY 1.00* OV 1.00* ! PT 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* WF 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! MA 0.00* NY 0.00* ON 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! HN 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 9: ! MA 0.00* MK 0.00* ! ! Telescope amplitude corrections in sub-array 10: ! MA 0.00* ON 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 11: ! MA 0.00* NY 0.00* WZ 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* ! MA 1.00* NL 1.00* NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* WF 1.00* WZ 1.00* ! ! A total of 45 telescope corrections were flagged in sub-array 13. ! Telescope amplitude corrections in sub-array 13: ! HN 0.00* MA 0.00* NY 0.00* ON 0.00* ! WF 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 14: ! FD 1.00* HN 1.00* LA 1.00* NL 1.00* ! NY 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! ! Correcting IF 4. ! A total of 360 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! MA 0.00* NY 0.00* ON 0.00* WF 0.00* ! WZ 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! HN 0.00* LA 0.00* PT 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! MA 1.00* MK 1.00* NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* WF 1.00* ! WZ 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! NY 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* NY 1.00* OV 1.00* ! PT 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! FD 1.00* HN 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* WF 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! MA 0.00* NY 0.00* ON 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! HN 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 9: ! MA 0.00* MK 0.00* ! ! Telescope amplitude corrections in sub-array 10: ! MA 0.00* ON 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 11: ! MA 0.00* NY 0.00* WZ 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* ! MA 1.00* NL 1.00* NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* WF 1.00* WZ 1.00* ! ! A total of 45 telescope corrections were flagged in sub-array 13. ! Telescope amplitude corrections in sub-array 13: ! HN 0.00* MA 0.00* NY 0.00* ON 0.00* ! WF 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 14: ! FD 1.00* HN 1.00* LA 1.00* NL 1.00* ! NY 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! ! Fit before self-cal, rms=0.310120Jy sigma=2.443241 ! Fit after self-cal, rms=0.298017Jy sigma=2.511537 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 3.36% of the data. ! The x-axis pixel size should ideally be below 0.1716 milli-arcsec ! Estimated beam: bmin=0.6283 mas, bmaj=0.8931 mas, bpa=-17.79 degrees ! Estimated noise=0.546484 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 = 0.00542817 Jy ! Component: 100 - total flux cleaned = 0.0110087 Jy ! Component: 150 - total flux cleaned = 0.016332 Jy ! Component: 200 - total flux cleaned = 0.0202407 Jy ! Total flux subtracted in 200 components = 0.0202407 Jy ! Clean residual min=-0.042030 max=0.040148 Jy/beam ! Clean residual mean=0.000332 rms=0.009064 Jy/beam ! Combined flux in latest and established models = 0.70611 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 37 components and 0.70611 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.296914Jy sigma=2.397734 ! Fit after self-cal, rms=0.296629Jy sigma=2.390521 ! Inverting map ! Your choice of large map pixels excluded 3.36% of the data. ! The x-axis pixel size should ideally be below 0.1716 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=0.296629Jy sigma=2.390521 ! Fit after self-cal, rms=0.296629Jy sigma=2.390521 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.36% of the data. ! The x-axis pixel size should ideally be below 0.1716 milli-arcsec ! Estimated beam: bmin=0.6283 mas, bmaj=0.8931 mas, bpa=-17.79 degrees ! Estimated noise=0.546484 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00813521 Jy ! Component: 100 - total flux cleaned = 0.0131586 Jy ! Component: 150 - total flux cleaned = 0.0154107 Jy ! Component: 200 - total flux cleaned = 0.0164626 Jy ! Total flux subtracted in 200 components = 0.0164626 Jy ! Clean residual min=-0.040437 max=0.036107 Jy/beam ! Clean residual mean=0.000239 rms=0.008541 Jy/beam ! Combined flux in latest and established models = 0.722573 Jy selfcal ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 43 components and 0.722572 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.294951Jy sigma=2.347147 ! Fit after self-cal, rms=0.295052Jy sigma=2.344411 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.36% of the data. ! The x-axis pixel size should ideally be below 0.1716 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 = 0.00610194 Jy ! Component: 100 - total flux cleaned = 0.00816584 Jy ! Component: 150 - total flux cleaned = 0.00863866 Jy ! Component: 200 - total flux cleaned = 0.00994602 Jy ! Total flux subtracted in 200 components = 0.00994602 Jy ! Clean residual min=-0.038970 max=0.034226 Jy/beam ! Clean residual mean=0.000182 rms=0.008214 Jy/beam ! Combined flux in latest and established models = 0.732518 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 44 components and 0.732518 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.293803Jy sigma=2.317850 ! Fit after self-cal, rms=0.293908Jy sigma=2.316048 ! Inverting map ! Your choice of large map pixels excluded 3.36% of the data. ! The x-axis pixel size should ideally be below 0.1716 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=0.293908Jy sigma=2.316048 ! Fit after self-cal, rms=0.293908Jy sigma=2.316048 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.36% of the data. ! The x-axis pixel size should ideally be below 0.1716 milli-arcsec ! Estimated beam: bmin=0.6283 mas, bmaj=0.8931 mas, bpa=-17.79 degrees ! Estimated noise=0.546484 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00502575 Jy ! Component: 100 - total flux cleaned = 0.00587451 Jy ! Component: 150 - total flux cleaned = 0.00625742 Jy ! Component: 200 - total flux cleaned = 0.00699144 Jy ! Total flux subtracted in 200 components = 0.00699144 Jy ! Clean residual min=-0.037846 max=0.033595 Jy/beam ! Clean residual mean=0.000143 rms=0.007980 Jy/beam ! Combined flux in latest and established models = 0.73951 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 46 components and 0.73951 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.292883Jy sigma=2.298125 ! Fit after self-cal, rms=0.293017Jy sigma=2.297122 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.36% of the data. ! The x-axis pixel size should ideally be below 0.1716 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 = 0.00347671 Jy ! Component: 100 - total flux cleaned = 0.00384577 Jy ! Component: 150 - total flux cleaned = 0.00384536 Jy ! Component: 200 - total flux cleaned = 0.00416379 Jy ! Total flux subtracted in 200 components = 0.00416379 Jy ! Clean residual min=-0.036972 max=0.033320 Jy/beam ! Clean residual mean=0.000119 rms=0.007821 Jy/beam ! Combined flux in latest and established models = 0.743674 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 48 components and 0.743674 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.292110Jy sigma=2.284919 ! Fit after self-cal, rms=0.292232Jy sigma=2.284364 ! Inverting map ! Your choice of large map pixels excluded 3.36% of the data. ! The x-axis pixel size should ideally be below 0.1716 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=0.292232Jy sigma=2.284364 ! Fit after self-cal, rms=0.292232Jy sigma=2.284364 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.36% of the data. ! The x-axis pixel size should ideally be below 0.1716 milli-arcsec ! Estimated beam: bmin=1.941 mas, bmaj=2.83 mas, bpa=33.58 degrees ! Estimated noise=0.978863 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0194556 Jy ! Component: 100 - total flux cleaned = 0.0234312 Jy ! Component: 150 - total flux cleaned = 0.0268514 Jy ! Component: 200 - total flux cleaned = 0.02852 Jy ! Total flux subtracted in 200 components = 0.02852 Jy ! Clean residual min=-0.072081 max=0.058692 Jy/beam ! Clean residual mean=-0.000197 rms=0.017281 Jy/beam ! Combined flux in latest and established models = 0.772193 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 52 components and 0.772193 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.292551Jy sigma=2.274637 ! Fit after self-cal, rms=0.292054Jy sigma=2.267257 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.36% of the data. ! The x-axis pixel size should ideally be below 0.1716 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 = 0.00368551 Jy ! Component: 100 - total flux cleaned = 0.00416582 Jy ! Component: 150 - total flux cleaned = 0.00493257 Jy ! Component: 200 - total flux cleaned = 0.0056189 Jy ! Total flux subtracted in 200 components = 0.0056189 Jy ! Clean residual min=-0.070504 max=0.055329 Jy/beam ! Clean residual mean=-0.000328 rms=0.016518 Jy/beam ! Combined flux in latest and established models = 0.777812 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 55 components and 0.777812 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.292349Jy sigma=2.275932 ! Fit after self-cal, rms=0.292126Jy sigma=2.273490 ! Inverting map ! Your choice of large map pixels excluded 3.36% of the data. ! The x-axis pixel size should ideally be below 0.1716 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 3.36% of the data. ! The x-axis pixel size should ideally be below 0.1716 milli-arcsec ! Estimated beam: bmin=0.6283 mas, bmaj=0.8931 mas, bpa=-17.79 degrees ! Estimated noise=0.546484 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6283 x 0.8931 at -17.79 degrees (North through East) ! Clean map min=-0.042503 max=0.35286 Jy/beam if(peak(flux) > thresh) selfcal true, true clean clean_niter,clean_gain selfcal flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) selfcal true, true end if print "************** CLEARING MODEL AND STARTING OVER **********" ! ************** CLEARING MODEL AND STARTING OVER ********** clrmod true ! clrmod: Cleared the established and tentative models. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.36% of the data. ! The x-axis pixel size should ideally be below 0.1716 milli-arcsec ! Estimated beam: bmin=0.5397 mas, bmaj=0.8025 mas, bpa=-26.52 degrees ! Estimated noise=1.03558 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.299729 Jy ! Component: 100 - total flux cleaned = 0.42282 Jy ! Component: 150 - total flux cleaned = 0.502336 Jy ! Component: 200 - total flux cleaned = 0.558935 Jy ! Total flux subtracted in 200 components = 0.558935 Jy ! Clean residual min=-0.043080 max=0.050287 Jy/beam ! Clean residual mean=0.000171 rms=0.007981 Jy/beam ! Combined flux in latest and established models = 0.558935 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 15 model components to the UV plane model. ! The established model now contains 15 components and 0.558935 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 3.36% of the data. ! The x-axis pixel size should ideally be below 0.1716 milli-arcsec ! Estimated beam: bmin=0.6283 mas, bmaj=0.8931 mas, bpa=-17.79 degrees ! Estimated noise=0.546484 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 = 0.0773324 Jy ! Component: 100 - total flux cleaned = 0.121822 Jy ! Component: 150 - total flux cleaned = 0.15337 Jy ! Component: 200 - total flux cleaned = 0.166622 Jy ! Total flux subtracted in 200 components = 0.166622 Jy ! Clean residual min=-0.043295 max=0.039968 Jy/beam ! Clean residual mean=0.000218 rms=0.008637 Jy/beam ! Combined flux in latest and established models = 0.725557 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 31 components and 0.725557 Jy ! Inverting map ! Your choice of large map pixels excluded 3.36% of the data. ! The x-axis pixel size should ideally be below 0.1716 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 3.36% of the data. ! The x-axis pixel size should ideally be below 0.1716 milli-arcsec ! Estimated beam: bmin=1.941 mas, bmaj=2.83 mas, bpa=33.58 degrees ! Estimated noise=0.978863 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0320019 Jy ! Component: 100 - total flux cleaned = 0.0412073 Jy ! Component: 150 - total flux cleaned = 0.0481731 Jy ! Component: 200 - total flux cleaned = 0.0534471 Jy ! Total flux subtracted in 200 components = 0.0534471 Jy ! Clean residual min=-0.070631 max=0.056200 Jy/beam ! Clean residual mean=-0.000369 rms=0.016801 Jy/beam ! Combined flux in latest and established models = 0.779005 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 = 0.00107165 Jy ! Component: 100 - total flux cleaned = 0.00205077 Jy ! Component: 150 - total flux cleaned = 0.00300092 Jy ! Component: 200 - total flux cleaned = 0.00386546 Jy ! Total flux subtracted in 200 components = 0.00386546 Jy ! Clean residual min=-0.069701 max=0.054015 Jy/beam ! Clean residual mean=-0.000463 rms=0.016409 Jy/beam ! Combined flux in latest and established models = 0.78287 Jy ! Adding 15 model components to the UV plane model. ! The established model now contains 41 components and 0.78287 Jy ! Inverting map ! Your choice of large map pixels excluded 3.36% of the data. ! The x-axis pixel size should ideally be below 0.1716 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 3.36% of the data. ! The x-axis pixel size should ideally be below 0.1716 milli-arcsec ! Estimated beam: bmin=0.6283 mas, bmaj=0.8931 mas, bpa=-17.79 degrees ! Estimated noise=0.546484 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00150641 Jy ! Component: 100 - total flux cleaned = -0.000236811 Jy ! Component: 150 - total flux cleaned = -0.000943891 Jy ! Component: 200 - total flux cleaned = -0.00216322 Jy ! Total flux subtracted in 200 components = -0.00216322 Jy ! Clean residual min=-0.037292 max=0.034251 Jy/beam ! Clean residual mean=-0.000099 rms=0.007568 Jy/beam ! Combined flux in latest and established models = 0.780707 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 47 components and 0.780707 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.301658Jy sigma=2.317781 ! Fit after self-cal, rms=0.301427Jy sigma=2.306044 wmodel /scr/pima/rv102_uvs/J2230+6946_X_map.mod ! Writing 47 model components to file: /scr/pima/rv102_uvs/J2230+6946_X_map.mod wobs /scr/pima/rv102_uvs/J2230+6946_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv102_uvs/J2230+6946_X_uvs.fits wwins /scr/pima/rv102_uvs/J2230+6946_X_map.win ! wwins: Wrote 4 windows to /scr/pima/rv102_uvs/J2230+6946_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 3.36% of the data. ! The x-axis pixel size should ideally be below 0.1716 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.0159359 Jy ! Component: 100 - total flux cleaned = -0.0222411 Jy ! Component: 150 - total flux cleaned = -0.0263812 Jy ! Component: 200 - total flux cleaned = -0.0275034 Jy ! Component: 250 - total flux cleaned = -0.0290935 Jy ! Component: 300 - total flux cleaned = -0.029594 Jy ! Component: 350 - total flux cleaned = -0.0311013 Jy ! Component: 400 - total flux cleaned = -0.0330336 Jy ! Component: 450 - total flux cleaned = -0.033037 Jy ! Component: 500 - total flux cleaned = -0.0330353 Jy ! Component: 550 - total flux cleaned = -0.0325847 Jy ! Component: 600 - total flux cleaned = -0.0330211 Jy ! Component: 650 - total flux cleaned = -0.0338606 Jy ! Component: 700 - total flux cleaned = -0.0334426 Jy ! Component: 750 - total flux cleaned = -0.0346414 Jy ! Component: 800 - total flux cleaned = -0.0342441 Jy ! Component: 850 - total flux cleaned = -0.0342428 Jy ! Component: 900 - total flux cleaned = -0.0346154 Jy ! Component: 950 - total flux cleaned = -0.0346135 Jy ! Component: 1000 - total flux cleaned = -0.0342561 Jy ! Component: 1050 - total flux cleaned = -0.0339077 Jy ! Component: 1100 - total flux cleaned = -0.0339153 Jy ! Component: 1150 - total flux cleaned = -0.0349338 Jy ! Component: 1200 - total flux cleaned = -0.0342586 Jy ! Component: 1250 - total flux cleaned = -0.0342593 Jy ! Component: 1300 - total flux cleaned = -0.0336122 Jy ! Component: 1350 - total flux cleaned = -0.0339307 Jy ! Component: 1400 - total flux cleaned = -0.033308 Jy ! Component: 1450 - total flux cleaned = -0.0333101 Jy ! Component: 1500 - total flux cleaned = -0.0320977 Jy ! Component: 1550 - total flux cleaned = -0.0320992 Jy ! Component: 1600 - total flux cleaned = -0.0321 Jy ! Component: 1650 - total flux cleaned = -0.031811 Jy ! Component: 1700 - total flux cleaned = -0.0315268 Jy ! Component: 1750 - total flux cleaned = -0.0312442 Jy ! Component: 1800 - total flux cleaned = -0.0304092 Jy ! Component: 1850 - total flux cleaned = -0.0309658 Jy ! Component: 1900 - total flux cleaned = -0.0298736 Jy ! Component: 1950 - total flux cleaned = -0.0306805 Jy ! Component: 2000 - total flux cleaned = -0.0298754 Jy ! Component: 2050 - total flux cleaned = -0.0296129 Jy ! Component: 2100 - total flux cleaned = -0.0293539 Jy ! Component: 2150 - total flux cleaned = -0.0301309 Jy ! Component: 2200 - total flux cleaned = -0.029362 Jy ! Component: 2250 - total flux cleaned = -0.0298703 Jy ! Component: 2300 - total flux cleaned = -0.0298675 Jy ! Component: 2350 - total flux cleaned = -0.0298684 Jy ! Component: 2400 - total flux cleaned = -0.0296211 Jy ! Component: 2450 - total flux cleaned = -0.03011 Jy ! Component: 2500 - total flux cleaned = -0.0288976 Jy ! Component: 2550 - total flux cleaned = -0.0293791 Jy ! Component: 2600 - total flux cleaned = -0.0291418 Jy ! Component: 2650 - total flux cleaned = -0.0284321 Jy ! Component: 2700 - total flux cleaned = -0.0296071 Jy ! Component: 2750 - total flux cleaned = -0.0284426 Jy ! Component: 2800 - total flux cleaned = -0.0289031 Jy ! Component: 2850 - total flux cleaned = -0.0284438 Jy ! Component: 2900 - total flux cleaned = -0.0284457 Jy ! Component: 2950 - total flux cleaned = -0.0275405 Jy ! Component: 3000 - total flux cleaned = -0.0275414 Jy ! Component: 3050 - total flux cleaned = -0.0273183 Jy ! Component: 3100 - total flux cleaned = -0.026876 Jy ! Component: 3150 - total flux cleaned = -0.0264363 Jy ! Component: 3200 - total flux cleaned = -0.0264375 Jy ! Component: 3250 - total flux cleaned = -0.0260028 Jy ! Component: 3300 - total flux cleaned = -0.0249262 Jy ! Component: 3350 - total flux cleaned = -0.0253541 Jy ! Component: 3400 - total flux cleaned = -0.0245024 Jy ! Component: 3450 - total flux cleaned = -0.0234447 Jy ! Component: 3500 - total flux cleaned = -0.0230233 Jy ! Component: 3550 - total flux cleaned = -0.0226066 Jy ! Component: 3600 - total flux cleaned = -0.0226053 Jy ! Component: 3650 - total flux cleaned = -0.0219868 Jy ! Component: 3700 - total flux cleaned = -0.0209625 Jy ! Component: 3750 - total flux cleaned = -0.0203528 Jy ! Component: 3800 - total flux cleaned = -0.019948 Jy ! Component: 3850 - total flux cleaned = -0.0189425 Jy ! Component: 3900 - total flux cleaned = -0.0187422 Jy ! Component: 3950 - total flux cleaned = -0.017947 Jy ! Component: 4000 - total flux cleaned = -0.0179458 Jy ! Component: 4050 - total flux cleaned = -0.0173558 Jy ! Total flux subtracted in 4096 components = -0.0171605 Jy ! Clean residual min=-0.011411 max=0.009754 Jy/beam ! Clean residual mean=-0.000131 rms=0.003255 Jy/beam ! Combined flux in latest and established models = 0.763546 Jy keep ! Adding 340 model components to the UV plane model. ! The established model now contains 387 components and 0.763547 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/rv102_uvs/J2230+6946_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 3.36% of the data. ! The x-axis pixel size should ideally be below 0.1716 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6283 x 0.8931 at -17.79 degrees (North through East) ! Clean map min=-0.021231 max=0.33259 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv102_uvs/J2230+6946_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.332594 invert ! Inverting map ! Your choice of large map pixels excluded 3.36% of the data. ! The x-axis pixel size should ideally be below 0.1716 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00325446 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -2.93552 2.93552 5.87105 11.7421 23.4842 46.9684 93.9368 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0097 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.332 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 102.196 quit ! Quitting program ! Log file /scr/pima/rv102_uvs/J2230+6946_X_uvs.log closed on Sat Feb 27 22:29:11 2016