! Started logfile: /d2/scr/pima/rv101_uvs/J2230+6946_X_uvs.log on Sat Nov 29 16:38:37 2014 obs /d2/scr/pima/rv101_uvs/J2230+6946_X_uva.fits ! Reading UV FITS file: /d2/scr/pima/rv101_uvs/J2230+6946_X_uva.fits ! AN table 1: 42 integrations on 55 of 55 possible baselines. ! AN table 2: 32 integrations on 1 of 1 possible baselines. ! AN table 3: 11 integrations on 6 of 6 possible baselines. ! AN table 4: 9 integrations on 3 of 3 possible baselines. ! AN table 5: 84 integrations on 3 of 3 possible baselines. ! AN table 6: 93 integrations on 78 of 78 possible baselines. ! AN table 7: 9 integrations on 1 of 1 possible baselines. ! AN table 8: 85 integrations on 6 of 6 possible baselines. ! AN table 9: 27 integrations on 3 of 3 possible baselines. ! AN table 10: 9 integrations on 21 of 21 possible baselines. ! AN table 11: 10 integrations on 1 of 1 possible baselines. ! AN table 12: 42 integrations on 55 of 55 possible baselines. ! Apparent sampling: 0.594176 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 0 lines of history. ! ! Reading 31016 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/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 233 telescope corrections were flagged in sub-array 1. ! A total of 64 telescope corrections were flagged in sub-array 2. ! A total of 16 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 30 telescope corrections were flagged in sub-array 5. ! A total of 391 telescope corrections were flagged in sub-array 6. ! A total of 18 telescope corrections were flagged in sub-array 7. ! A total of 110 telescope corrections were flagged in sub-array 8. ! A total of 60 telescope corrections were flagged in sub-array 9. ! A total of 22 telescope corrections were flagged in sub-array 10. ! A total of 20 telescope corrections were flagged in sub-array 11. ! A total of 245 telescope corrections were flagged in sub-array 12. ! ! Correcting IF 2. ! A total of 233 telescope corrections were flagged in sub-array 1. ! A total of 64 telescope corrections were flagged in sub-array 2. ! A total of 16 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 30 telescope corrections were flagged in sub-array 5. ! A total of 391 telescope corrections were flagged in sub-array 6. ! A total of 18 telescope corrections were flagged in sub-array 7. ! A total of 110 telescope corrections were flagged in sub-array 8. ! A total of 60 telescope corrections were flagged in sub-array 9. ! A total of 22 telescope corrections were flagged in sub-array 10. ! A total of 20 telescope corrections were flagged in sub-array 11. ! A total of 245 telescope corrections were flagged in sub-array 12. ! ! Correcting IF 3. ! A total of 291 telescope corrections were flagged in sub-array 1. ! A total of 64 telescope corrections were flagged in sub-array 2. ! A total of 23 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 252 telescope corrections were flagged in sub-array 5. ! A total of 500 telescope corrections were flagged in sub-array 6. ! A total of 18 telescope corrections were flagged in sub-array 7. ! A total of 184 telescope corrections were flagged in sub-array 8. ! A total of 81 telescope corrections were flagged in sub-array 9. ! A total of 22 telescope corrections were flagged in sub-array 10. ! A total of 20 telescope corrections were flagged in sub-array 11. ! A total of 322 telescope corrections were flagged in sub-array 12. ! ! Correcting IF 4. ! A total of 291 telescope corrections were flagged in sub-array 1. ! A total of 64 telescope corrections were flagged in sub-array 2. ! A total of 23 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! A total of 252 telescope corrections were flagged in sub-array 5. ! A total of 500 telescope corrections were flagged in sub-array 6. ! A total of 18 telescope corrections were flagged in sub-array 7. ! A total of 184 telescope corrections were flagged in sub-array 8. ! A total of 81 telescope corrections were flagged in sub-array 9. ! A total of 22 telescope corrections were flagged in sub-array 10. ! A total of 20 telescope corrections were flagged in sub-array 11. ! A total of 322 telescope corrections were flagged in sub-array 12. ! ! Fit before self-cal, rms=1.320654Jy sigma=7.964761 ! Fit after self-cal, rms=0.349963Jy sigma=1.916236 ! 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 0.77% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 milli-arcsec ! Estimated beam: bmin=0.564 mas, bmaj=0.6803 mas, bpa=55.13 degrees ! Estimated noise=1.45633 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 = 0.551499 Jy ! Component: 100 - total flux cleaned = 0.706811 Jy ! Total flux subtracted in 100 components = 0.706811 Jy ! Clean residual min=-0.017791 max=0.065194 Jy/beam ! Clean residual mean=0.000205 rms=0.004274 Jy/beam ! Combined flux in latest and established models = 0.706811 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 0.706811 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.283757Jy sigma=1.360420 ! Fit after self-cal, rms=0.282411Jy sigma=1.356676 ! Inverting map ! Your choice of large map pixels excluded 0.77% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 milli-arcsec ! Added new window around map position (-0.6, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0731869 Jy ! Component: 100 - total flux cleaned = 0.117298 Jy ! Total flux subtracted in 100 components = 0.117298 Jy ! Clean residual min=-0.013713 max=0.023433 Jy/beam ! Clean residual mean=0.000127 rms=0.002956 Jy/beam ! Combined flux in latest and established models = 0.82411 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 14 components and 0.82411 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.244896Jy sigma=1.103557 ! Fit after self-cal, rms=0.243924Jy sigma=1.100560 ! Inverting map ! Your choice of large map pixels excluded 0.77% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0307169 Jy ! Component: 100 - total flux cleaned = 0.0490664 Jy ! Total flux subtracted in 100 components = 0.0490664 Jy ! Clean residual min=-0.013231 max=0.014509 Jy/beam ! Clean residual mean=0.000095 rms=0.002675 Jy/beam ! Combined flux in latest and established models = 0.873176 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 15 components and 0.873176 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.234355Jy sigma=1.049931 ! Fit after self-cal, rms=0.233986Jy sigma=1.048922 ! Inverting map ! Your choice of large map pixels excluded 0.77% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 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 0.77% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 milli-arcsec ! Estimated beam: bmin=0.673 mas, bmaj=0.8306 mas, bpa=43.01 degrees ! Estimated noise=0.854991 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 = 0.0309207 Jy ! Component: 100 - total flux cleaned = 0.0446539 Jy ! Component: 150 - total flux cleaned = 0.049594 Jy ! Component: 200 - total flux cleaned = 0.0506686 Jy ! Total flux subtracted in 200 components = 0.0506686 Jy ! Clean residual min=-0.012758 max=0.014357 Jy/beam ! Clean residual mean=0.000368 rms=0.002973 Jy/beam ! Combined flux in latest and established models = 0.923844 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 22 components and 0.923844 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.226861Jy sigma=1.037707 ! Fit after self-cal, rms=0.226687Jy sigma=1.036905 ! Inverting map ! Your choice of large map pixels excluded 0.77% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.673 x 0.8306 at 43.01 degrees (North through East) ! Clean map min=-0.011674 max=0.75182 Jy/beam if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 24 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! FD 1.04 HN 1.08 LA 1.07 MA 1.00 ! NL 1.01 NY 1.03 ON 0.82 OV 0.99 ! PT 1.06 SC 1.08 WF 0.83 ! ! Telescope amplitude corrections in sub-array 2: ! MA 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! HN 1.08 NL 1.03 NY 1.09 OV 1.00 ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HN 0.00* NL 0.00* WF 0.00* ! ! A total of 222 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! MA 0.00* NY 0.00* ON 0.00* ! ! A total of 30 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! FD 1.01 HN 1.01 KP 1.00* LA 1.05 ! MA 1.03 MK 1.03 NL 0.99 NY 0.99 ! ON 0.83 OV 0.98 PT 1.02 SC 1.01 ! WF 0.81 ! ! Telescope amplitude corrections in sub-array 7: ! MK 0.00* WF 0.00* ! ! A total of 78 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! MA 1.02 NY 0.95 ON 0.83 WF 0.82 ! ! A total of 21 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! HN 0.00* NY 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 10: ! HN 1.12 KP 1.00* LA 1.15 MK 1.03 ! NL 0.99 OV 1.02 PT 1.07 ! ! Telescope amplitude corrections in sub-array 11: ! NY 0.00* OV 0.00* ! ! A total of 51 telescope corrections were flagged in sub-array 12. ! Telescope amplitude corrections in sub-array 12: ! FD 1.05 HN 1.06 KP 1.00* LA 1.19 ! MA 1.04 NL 1.01 NY 0.95 ON 0.81 ! OV 1.01 PT 1.07 WF 0.80 ! ! ! Correcting IF 2. ! A total of 24 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! FD 1.04 HN 1.12 LA 1.04 MA 0.95 ! NL 1.03 NY 1.01 ON 0.80 OV 0.99 ! PT 0.96 SC 1.06 WF 0.87 ! ! Telescope amplitude corrections in sub-array 2: ! MA 0.00* ON 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! HN 1.12 NL 1.03 NY 1.08 OV 0.96 ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HN 0.00* NL 0.00* WF 0.00* ! ! A total of 222 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! MA 0.00* NY 0.00* ON 0.00* ! ! A total of 30 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! FD 1.02 HN 1.04 KP 1.00* LA 1.01 ! MA 0.99 MK 1.04 NL 0.99 NY 0.98 ! ON 0.83 OV 0.96 PT 0.93 SC 1.04 ! WF 0.84 ! ! Telescope amplitude corrections in sub-array 7: ! MK 0.00* WF 0.00* ! ! A total of 78 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! MA 0.96 NY 0.97 ON 0.81 WF 0.81 ! ! A total of 21 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! HN 0.00* NY 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 10: ! HN 1.14 KP 1.00* LA 1.05 MK 1.05 ! NL 1.00 OV 1.01 PT 0.97 ! ! Telescope amplitude corrections in sub-array 11: ! NY 0.00* OV 0.00* ! ! A total of 51 telescope corrections were flagged in sub-array 12. ! Telescope amplitude corrections in sub-array 12: ! FD 1.05 HN 1.08 KP 1.00* LA 1.14 ! MA 0.95 NL 1.07 NY 0.95 ON 0.81 ! OV 1.00 PT 0.96 WF 0.86 ! ! ! Correcting IF 3. ! A total of 45 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! FD 1.05 HN 1.11 LA 1.09 MA 1.03 ! NL 1.08 NY 1.00* ON 0.96 OV 1.06 ! PT 0.96 SC 1.05 WF 0.89 ! ! Telescope amplitude corrections in sub-array 2: ! MA 0.00* ON 0.00* ! ! A total of 21 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HN 0.00* NL 0.00* NY 0.00* OV 0.00* ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HN 0.00* NL 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! MA 0.00* NY 0.00* ON 0.00* ! ! A total of 51 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! FD 1.03 HN 1.07 KP 1.00* LA 1.08 ! MA 1.07 MK 1.03 NL 1.02 NY 1.00* ! ON 0.98 OV 1.04 PT 0.91 SC 1.02 ! WF 0.86 ! ! Telescope amplitude corrections in sub-array 7: ! MK 0.00* WF 0.00* ! ! A total of 156 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! MA 0.00* NY 0.00* ON 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 9: ! HN 0.00* NY 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 10: ! HN 1.14 KP 1.00* LA 1.12 MK 1.01 ! NL 1.08 OV 1.09 PT 0.97 ! ! Telescope amplitude corrections in sub-array 11: ! NY 0.00* OV 0.00* ! ! A total of 21 telescope corrections were flagged in sub-array 12. ! Telescope amplitude corrections in sub-array 12: ! FD 1.01 HN 1.14 KP 1.00* LA 1.26 ! MA 1.06 NL 1.06 NY 1.00* ON 0.97 ! OV 1.06 PT 0.96 WF 0.91 ! ! ! Correcting IF 4. ! A total of 45 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! FD 1.08 HN 1.09 LA 1.09 MA 1.15 ! NL 1.13 NY 1.00* ON 1.07 OV 1.04 ! PT 0.97 SC 1.07 WF 0.95 ! ! Telescope amplitude corrections in sub-array 2: ! MA 0.00* ON 0.00* ! ! A total of 21 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! HN 0.00* NL 0.00* NY 0.00* OV 0.00* ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HN 0.00* NL 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! MA 0.00* NY 0.00* ON 0.00* ! ! A total of 51 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! FD 1.05 HN 1.09 KP 1.00* LA 1.05 ! MA 1.13 MK 1.07 NL 1.04 NY 1.00* ! ON 1.07 OV 1.00 PT 0.94 SC 1.05 ! WF 0.94 ! ! Telescope amplitude corrections in sub-array 7: ! MK 0.00* WF 0.00* ! ! A total of 156 telescope corrections were flagged in sub-array 8. ! Telescope amplitude corrections in sub-array 8: ! MA 0.00* NY 0.00* ON 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 9: ! HN 0.00* NY 0.00* WF 0.00* ! ! Telescope amplitude corrections in sub-array 10: ! HN 1.15 KP 1.00* LA 1.12 MK 1.08 ! NL 1.09 OV 1.06 PT 0.99 ! ! Telescope amplitude corrections in sub-array 11: ! NY 0.00* OV 0.00* ! ! A total of 21 telescope corrections were flagged in sub-array 12. ! Telescope amplitude corrections in sub-array 12: ! FD 1.06 HN 1.14 KP 1.00* LA 1.23 ! MA 1.10 NL 1.07 NY 1.00* ON 1.01 ! OV 1.05 PT 0.99 WF 0.93 ! ! ! Fit before self-cal, rms=0.226687Jy sigma=1.036905 ! Fit after self-cal, rms=0.178869Jy sigma=0.915284 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 milli-arcsec ! Estimated beam: bmin=0.6659 mas, bmaj=0.827 mas, bpa=40.86 degrees ! Estimated noise=0.863059 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 = 0.00650281 Jy ! Component: 100 - total flux cleaned = 0.00540603 Jy ! Component: 150 - total flux cleaned = 0.0049581 Jy ! Component: 200 - total flux cleaned = 0.00470716 Jy ! Total flux subtracted in 200 components = 0.00470716 Jy ! Clean residual min=-0.005122 max=0.005488 Jy/beam ! Clean residual mean=0.000095 rms=0.001050 Jy/beam ! Combined flux in latest and established models = 0.928552 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 24 components and 0.928552 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.178310Jy sigma=0.912534 ! Fit after self-cal, rms=0.177970Jy sigma=0.911583 ! Inverting map ! Your choice of large map pixels excluded 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 milli-arcsec ! Added new window around map position (0.6, 0.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00313835 Jy ! Component: 100 - total flux cleaned = 0.00344725 Jy ! Component: 150 - total flux cleaned = 0.00321518 Jy ! Component: 200 - total flux cleaned = 0.00301193 Jy ! Total flux subtracted in 200 components = 0.00301193 Jy ! Clean residual min=-0.004791 max=0.004917 Jy/beam ! Clean residual mean=0.000084 rms=0.000979 Jy/beam ! Combined flux in latest and established models = 0.931563 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 34 components and 0.931563 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.177710Jy sigma=0.910274 ! Fit after self-cal, rms=0.177644Jy sigma=0.910008 ! Inverting map ! Your choice of large map pixels excluded 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 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=0.177644Jy sigma=0.910008 ! Fit after self-cal, rms=0.176384Jy sigma=0.905074 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 milli-arcsec ! Estimated beam: bmin=0.664 mas, bmaj=0.8261 mas, bpa=40.06 degrees ! Estimated noise=0.863358 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00380204 Jy ! Component: 100 - total flux cleaned = 0.00361564 Jy ! Component: 150 - total flux cleaned = 0.00337086 Jy ! Component: 200 - total flux cleaned = 0.00310012 Jy ! Total flux subtracted in 200 components = 0.00310012 Jy ! Clean residual min=-0.004120 max=0.004112 Jy/beam ! Clean residual mean=0.000085 rms=0.000843 Jy/beam ! Combined flux in latest and established models = 0.934664 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 40 components and 0.934664 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.176201Jy sigma=0.904287 ! Fit after self-cal, rms=0.176145Jy sigma=0.904060 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 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 (7.4, 2.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00259192 Jy ! Component: 100 - total flux cleaned = 0.00270314 Jy ! Component: 150 - total flux cleaned = 0.0024708 Jy ! Component: 200 - total flux cleaned = 0.00247236 Jy ! Total flux subtracted in 200 components = 0.00247236 Jy ! Clean residual min=-0.003903 max=0.003602 Jy/beam ! Clean residual mean=0.000077 rms=0.000804 Jy/beam ! Combined flux in latest and established models = 0.937136 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 53 components and 0.937136 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.176028Jy sigma=0.903422 ! Fit after self-cal, rms=0.176009Jy sigma=0.903336 ! Inverting map ! Your choice of large map pixels excluded 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 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=0.176009Jy sigma=0.903336 ! Fit after self-cal, rms=0.175877Jy sigma=0.903162 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 milli-arcsec ! Estimated beam: bmin=0.6633 mas, bmaj=0.8257 mas, bpa=39.82 degrees ! Estimated noise=0.863861 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00233273 Jy ! Component: 100 - total flux cleaned = 0.00276444 Jy ! Component: 150 - total flux cleaned = 0.00276499 Jy ! Component: 200 - total flux cleaned = 0.00282003 Jy ! Total flux subtracted in 200 components = 0.00282003 Jy ! Clean residual min=-0.003733 max=0.003457 Jy/beam ! Clean residual mean=0.000074 rms=0.000776 Jy/beam ! Combined flux in latest and established models = 0.939956 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 56 components and 0.939956 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.175796Jy sigma=0.902784 ! Fit after self-cal, rms=0.175779Jy sigma=0.902714 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 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 = -0.000121886 Jy ! Component: 100 - total flux cleaned = -7.93647e-05 Jy ! Component: 150 - total flux cleaned = 2.06278e-05 Jy ! Component: 200 - total flux cleaned = 0.000115418 Jy ! Total flux subtracted in 200 components = 0.000115418 Jy ! Clean residual min=-0.003645 max=0.003394 Jy/beam ! Clean residual mean=0.000074 rms=0.000765 Jy/beam ! Combined flux in latest and established models = 0.940072 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 62 components and 0.940072 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.175739Jy sigma=0.902491 ! Fit after self-cal, rms=0.175730Jy sigma=0.902446 ! Inverting map ! Your choice of large map pixels excluded 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 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=0.175730Jy sigma=0.902446 ! Fit after self-cal, rms=0.175672Jy sigma=0.902386 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 milli-arcsec ! Estimated beam: bmin=2.003 mas, bmaj=2.894 mas, bpa=76.12 degrees ! Estimated noise=1.31513 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00247897 Jy ! Component: 100 - total flux cleaned = 0.00338846 Jy ! Component: 150 - total flux cleaned = 0.00379026 Jy ! Component: 200 - total flux cleaned = 0.00410935 Jy ! Total flux subtracted in 200 components = 0.00410935 Jy ! Clean residual min=-0.004322 max=0.004053 Jy/beam ! Clean residual mean=0.000231 rms=0.001060 Jy/beam ! Combined flux in latest and established models = 0.944181 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 72 components and 0.944181 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.175674Jy sigma=0.902418 ! Fit after self-cal, rms=0.175671Jy sigma=0.902388 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 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 = 0.000467413 Jy ! Component: 100 - total flux cleaned = 0.000598718 Jy ! Component: 150 - total flux cleaned = 0.000655543 Jy ! Component: 200 - total flux cleaned = 0.000708363 Jy ! Total flux subtracted in 200 components = 0.000708363 Jy ! Clean residual min=-0.004190 max=0.004010 Jy/beam ! Clean residual mean=0.000222 rms=0.001051 Jy/beam ! Combined flux in latest and established models = 0.944889 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 77 components and 0.944889 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.175677Jy sigma=0.902459 ! Fit after self-cal, rms=0.175678Jy sigma=0.902451 ! Inverting map ! Your choice of large map pixels excluded 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 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 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 milli-arcsec ! Estimated beam: bmin=0.6628 mas, bmaj=0.8255 mas, bpa=39.63 degrees ! Estimated noise=0.864229 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6628 x 0.8255 at 39.63 degrees (North through East) ! Clean map min=-0.0027466 max=0.74273 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=0.175678Jy sigma=0.902451 ! Fit after self-cal, rms=0.167083Jy sigma=0.840141 ! Inverting map and beam ! Your choice of large map pixels excluded 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 milli-arcsec ! Estimated beam: bmin=0.6629 mas, bmaj=0.8253 mas, bpa=39.65 degrees ! Estimated noise=0.864711 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000350441 Jy ! Component: 100 - total flux cleaned = 0.000411779 Jy ! Component: 150 - total flux cleaned = 0.000310717 Jy ! Component: 200 - total flux cleaned = 0.000218766 Jy ! Total flux subtracted in 200 components = 0.000218766 Jy ! Clean residual min=-0.003399 max=0.003070 Jy/beam ! Clean residual mean=0.000054 rms=0.000727 Jy/beam ! Combined flux in latest and established models = 0.945108 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 82 components and 0.945108 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.167034Jy sigma=0.839894 ! Fit after self-cal, rms=0.167029Jy sigma=0.839865 ! Inverting map ! Your choice of large map pixels excluded 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000239415 Jy ! Component: 100 - total flux cleaned = -0.000374554 Jy ! Component: 150 - total flux cleaned = -0.000374227 Jy ! Component: 200 - total flux cleaned = -0.000374858 Jy ! Total flux subtracted in 200 components = -0.000374858 Jy ! Clean residual min=-0.003400 max=0.003013 Jy/beam ! Clean residual mean=0.000056 rms=0.000722 Jy/beam ! Combined flux in latest and established models = 0.944733 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 85 components and 0.944733 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.167002Jy sigma=0.839708 ! Fit after self-cal, rms=0.166998Jy sigma=0.839686 ! Inverting map ! Your choice of large map pixels excluded 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.166998Jy sigma=0.839686 ! Fit after self-cal, rms=0.166910Jy sigma=0.839654 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 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 milli-arcsec ! Estimated beam: bmin=0.5591 mas, bmaj=0.6755 mas, bpa=51.59 degrees ! Estimated noise=1.51562 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.558957 Jy ! Component: 100 - total flux cleaned = 0.734323 Jy ! Component: 150 - total flux cleaned = 0.815494 Jy ! Component: 200 - total flux cleaned = 0.859714 Jy ! Total flux subtracted in 200 components = 0.859714 Jy ! Clean residual min=-0.007682 max=0.022766 Jy/beam ! Clean residual mean=0.000074 rms=0.001907 Jy/beam ! Combined flux in latest and established models = 0.859713 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 10 model components to the UV plane model. ! The established model now contains 10 components and 0.859713 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 milli-arcsec ! Estimated beam: bmin=0.6624 mas, bmaj=0.8252 mas, bpa=39.48 degrees ! Estimated noise=0.864762 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 = 0.0373432 Jy ! Component: 100 - total flux cleaned = 0.0566007 Jy ! Component: 150 - total flux cleaned = 0.0673935 Jy ! Component: 200 - total flux cleaned = 0.0737185 Jy ! Total flux subtracted in 200 components = 0.0737185 Jy ! Clean residual min=-0.004128 max=0.003709 Jy/beam ! Clean residual mean=0.000099 rms=0.000806 Jy/beam ! Combined flux in latest and established models = 0.933432 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 26 components and 0.933432 Jy ! Inverting map ! Your choice of large map pixels excluded 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 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 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 milli-arcsec ! Estimated beam: bmin=2.002 mas, bmaj=2.894 mas, bpa=76.09 degrees ! Estimated noise=1.31744 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00677686 Jy ! Component: 100 - total flux cleaned = 0.0101624 Jy ! Component: 150 - total flux cleaned = 0.0121165 Jy ! Component: 200 - total flux cleaned = 0.0128561 Jy ! Total flux subtracted in 200 components = 0.0128561 Jy ! Clean residual min=-0.004303 max=0.003754 Jy/beam ! Clean residual mean=0.000189 rms=0.001023 Jy/beam ! Combined flux in latest and established models = 0.946288 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 = 0.000365761 Jy ! Component: 100 - total flux cleaned = 0.000537807 Jy ! Component: 150 - total flux cleaned = 0.000630003 Jy ! Component: 200 - total flux cleaned = 0.000712664 Jy ! Total flux subtracted in 200 components = 0.000712664 Jy ! Clean residual min=-0.004213 max=0.003714 Jy/beam ! Clean residual mean=0.000178 rms=0.001013 Jy/beam ! Combined flux in latest and established models = 0.947001 Jy ! Adding 29 model components to the UV plane model. ! The established model now contains 49 components and 0.947001 Jy ! Inverting map ! Your choice of large map pixels excluded 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 milli-arcsec ! Estimated beam: bmin=0.6624 mas, bmaj=0.8252 mas, bpa=39.48 degrees ! Estimated noise=0.864762 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000327352 Jy ! Component: 100 - total flux cleaned = 0.000421103 Jy ! Component: 150 - total flux cleaned = 0.000503734 Jy ! Component: 200 - total flux cleaned = 0.000580535 Jy ! Total flux subtracted in 200 components = 0.000580535 Jy ! Clean residual min=-0.003694 max=0.003136 Jy/beam ! Clean residual mean=0.000046 rms=0.000732 Jy/beam ! Combined flux in latest and established models = 0.947581 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 56 components and 0.947581 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.166955Jy sigma=0.839950 ! Fit after self-cal, rms=0.166912Jy sigma=0.839672 wmodel /d2/scr/pima/rv101_uvs/J2230+6946_X_map.mod ! Writing 56 model components to file: /d2/scr/pima/rv101_uvs/J2230+6946_X_map.mod wobs /d2/scr/pima/rv101_uvs/J2230+6946_X_uvs.fits ! Writing UV FITS file: /d2/scr/pima/rv101_uvs/J2230+6946_X_uvs.fits wwins /d2/scr/pima/rv101_uvs/J2230+6946_X_map.win ! wwins: Wrote 4 windows to /d2/scr/pima/rv101_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 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000703227 Jy ! Component: 100 - total flux cleaned = -0.000930404 Jy ! Component: 150 - total flux cleaned = -0.00104188 Jy ! Component: 200 - total flux cleaned = -0.00125734 Jy ! Component: 250 - total flux cleaned = -0.00136318 Jy ! Component: 300 - total flux cleaned = -0.00151917 Jy ! Component: 350 - total flux cleaned = -0.00162121 Jy ! Component: 400 - total flux cleaned = -0.00167183 Jy ! Component: 450 - total flux cleaned = -0.00157432 Jy ! Component: 500 - total flux cleaned = -0.00167104 Jy ! Component: 550 - total flux cleaned = -0.00147842 Jy ! Component: 600 - total flux cleaned = -0.00143099 Jy ! Component: 650 - total flux cleaned = -0.00138443 Jy ! Component: 700 - total flux cleaned = -0.00147752 Jy ! Component: 750 - total flux cleaned = -0.00147691 Jy ! Component: 800 - total flux cleaned = -0.00147716 Jy ! Component: 850 - total flux cleaned = -0.00147773 Jy ! Component: 900 - total flux cleaned = -0.00161136 Jy ! Component: 950 - total flux cleaned = -0.00156767 Jy ! Component: 1000 - total flux cleaned = -0.0017426 Jy ! Component: 1050 - total flux cleaned = -0.001699 Jy ! Component: 1100 - total flux cleaned = -0.00165569 Jy ! Component: 1150 - total flux cleaned = -0.00165532 Jy ! Component: 1200 - total flux cleaned = -0.00169777 Jy ! Component: 1250 - total flux cleaned = -0.00165587 Jy ! Component: 1300 - total flux cleaned = -0.00173917 Jy ! Component: 1350 - total flux cleaned = -0.00169807 Jy ! Component: 1400 - total flux cleaned = -0.00182049 Jy ! Component: 1450 - total flux cleaned = -0.00161706 Jy ! Component: 1500 - total flux cleaned = -0.00173856 Jy ! Component: 1550 - total flux cleaned = -0.0014971 Jy ! Component: 1600 - total flux cleaned = -0.00141758 Jy ! Component: 1650 - total flux cleaned = -0.0012988 Jy ! Component: 1700 - total flux cleaned = -0.00122004 Jy ! Component: 1750 - total flux cleaned = -0.000946295 Jy ! Component: 1800 - total flux cleaned = -0.000907332 Jy ! Component: 1850 - total flux cleaned = -0.000674912 Jy ! Component: 1900 - total flux cleaned = -0.000675449 Jy ! Component: 1950 - total flux cleaned = -0.000675598 Jy ! Component: 2000 - total flux cleaned = -0.000523487 Jy ! Component: 2050 - total flux cleaned = -0.000334276 Jy ! Component: 2100 - total flux cleaned = -0.000334363 Jy ! Component: 2150 - total flux cleaned = -0.000259676 Jy ! Component: 2200 - total flux cleaned = -0.000259402 Jy ! Component: 2250 - total flux cleaned = -3.72675e-05 Jy ! Component: 2300 - total flux cleaned = 7.32546e-05 Jy ! Component: 2350 - total flux cleaned = 0.000183026 Jy ! Component: 2400 - total flux cleaned = 0.000256374 Jy ! Component: 2450 - total flux cleaned = 0.000329046 Jy ! Component: 2500 - total flux cleaned = 0.000437523 Jy ! Component: 2550 - total flux cleaned = 0.00050943 Jy ! Component: 2600 - total flux cleaned = 0.000617022 Jy ! Component: 2650 - total flux cleaned = 0.000617029 Jy ! Component: 2700 - total flux cleaned = 0.000865616 Jy ! Component: 2750 - total flux cleaned = 0.00111301 Jy ! Component: 2800 - total flux cleaned = 0.00111267 Jy ! Component: 2850 - total flux cleaned = 0.00125252 Jy ! Component: 2900 - total flux cleaned = 0.00135733 Jy ! Component: 2950 - total flux cleaned = 0.00160063 Jy ! Component: 3000 - total flux cleaned = 0.00160064 Jy ! Component: 3050 - total flux cleaned = 0.00173819 Jy ! Component: 3100 - total flux cleaned = 0.00187546 Jy ! Component: 3150 - total flux cleaned = 0.00197801 Jy ! Component: 3200 - total flux cleaned = 0.0022502 Jy ! Component: 3250 - total flux cleaned = 0.00221635 Jy ! Component: 3300 - total flux cleaned = 0.00238504 Jy ! Component: 3350 - total flux cleaned = 0.00255316 Jy ! Component: 3400 - total flux cleaned = 0.00278733 Jy ! Component: 3450 - total flux cleaned = 0.00298723 Jy ! Component: 3500 - total flux cleaned = 0.00292097 Jy ! Component: 3550 - total flux cleaned = 0.00315233 Jy ! Component: 3600 - total flux cleaned = 0.0033173 Jy ! Component: 3650 - total flux cleaned = 0.00338297 Jy ! Component: 3700 - total flux cleaned = 0.00357933 Jy ! Component: 3750 - total flux cleaned = 0.00377471 Jy ! Component: 3800 - total flux cleaned = 0.0039369 Jy ! Component: 3850 - total flux cleaned = 0.00393683 Jy ! Component: 3900 - total flux cleaned = 0.00390471 Jy ! Component: 3950 - total flux cleaned = 0.00422606 Jy ! Component: 4000 - total flux cleaned = 0.00429012 Jy ! Component: 4050 - total flux cleaned = 0.00457742 Jy ! Total flux subtracted in 4096 components = 0.0045774 Jy ! Clean residual min=-0.002059 max=0.002307 Jy/beam ! Clean residual mean=0.000036 rms=0.000510 Jy/beam ! Combined flux in latest and established models = 0.952159 Jy keep ! Adding 333 model components to the UV plane model. ! The established model now contains 389 components and 0.952159 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/d2/scr/pima/rv101_uvs/J2230+6946_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6624 x 0.8252 at 39.48 degrees (North through East) ! Clean map min=-0.0024506 max=0.74336 Jy/beam ! Writing clean map to FITS file: /d2/scr/pima/rv101_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 0.743363 invert ! Inverting map ! Your choice of large map pixels excluded 0.832% of the data. ! The x-axis pixel size should ideally be below 0.1988 milli-arcsec ! The y-axis pixel size should ideally be below 0.1594 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000508789 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.205333 0.205333 0.410666 0.821332 1.64266 3.28533 6.57065 13.1413 26.2826 52.5652 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0015 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.743 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 1461.04 quit ! Quitting program ! Log file /d2/scr/pima/rv101_uvs/J2230+6946_X_uvs.log closed on Sat Nov 29 16:38:43 2014