! Started logfile: /scr/pima/gb073_uvs/J2318+2404_X_uvs.log on Sat Dec 26 09:46:22 2015 obs /scr/pima/gb073_uvs/J2318+2404_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J2318+2404_X_uva.fits ! AN table 1: 16 integrations on 6 of 6 possible baselines. ! AN table 2: 24 integrations on 10 of 10 possible baselines. ! AN table 3: 12 integrations on 3 of 3 possible baselines. ! AN table 4: 17 integrations on 66 of 66 possible baselines. ! AN table 5: 6 integrations on 10 of 10 possible baselines. ! AN table 6: 12 integrations on 10 of 10 possible baselines. ! AN table 7: 7 integrations on 10 of 10 possible baselines. ! AN table 8: 8 integrations on 45 of 45 possible baselines. ! AN table 9: 17 integrations on 55 of 55 possible baselines. ! Apparent sampling: 0.740375 visibilities/baseline/integration-bin. ! Found source: J2318+2404 ! ! There are 8 IFs, and a total of 8 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 8.39799e+09 8e+06 1 8e+06 ! 02 2 8.40599e+09 8e+06 1 8e+06 ! 03 3 8.46799e+09 8e+06 1 8e+06 ! 04 4 8.47599e+09 8e+06 1 8e+06 ! 05 5 8.78299e+09 8e+06 1 8e+06 ! 06 6 8.79099e+09 8e+06 1 8e+06 ! 07 7 8.88799e+09 8e+06 1 8e+06 ! 08 8 8.89599e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 0 lines of history. ! ! Reading 18000 visibilities. select RR ! Selecting polarization: RR, channels: 1..8 ! Reading IF 1 channels: 1..1 ! Reading IF 2 channels: 2..2 ! Reading IF 3 channels: 3..3 ! Reading IF 4 channels: 4..4 ! Reading IF 5 channels: 5..5 ! Reading IF 6 channels: 6..6 ! Reading IF 7 channels: 7..7 ! Reading IF 8 channels: 8..8 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/gb073_uvs/J2318+2404_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 64 telescope corrections were flagged in sub-array 1. ! A total of 64 telescope corrections were flagged in sub-array 2. ! A total of 21 telescope corrections were flagged in sub-array 4. ! A total of 16 telescope corrections were flagged in sub-array 6. ! A total of 14 telescope corrections were flagged in sub-array 7. ! A total of 8 telescope corrections were flagged in sub-array 8. ! A total of 45 telescope corrections were flagged in sub-array 9. ! ! Correcting IF 2. ! A total of 64 telescope corrections were flagged in sub-array 1. ! A total of 64 telescope corrections were flagged in sub-array 2. ! A total of 21 telescope corrections were flagged in sub-array 4. ! A total of 16 telescope corrections were flagged in sub-array 6. ! A total of 14 telescope corrections were flagged in sub-array 7. ! A total of 8 telescope corrections were flagged in sub-array 8. ! A total of 45 telescope corrections were flagged in sub-array 9. ! ! Correcting IF 3. ! A total of 64 telescope corrections were flagged in sub-array 1. ! A total of 64 telescope corrections were flagged in sub-array 2. ! A total of 21 telescope corrections were flagged in sub-array 4. ! A total of 16 telescope corrections were flagged in sub-array 6. ! A total of 14 telescope corrections were flagged in sub-array 7. ! A total of 8 telescope corrections were flagged in sub-array 8. ! A total of 45 telescope corrections were flagged in sub-array 9. ! ! Correcting IF 4. ! A total of 64 telescope corrections were flagged in sub-array 1. ! A total of 64 telescope corrections were flagged in sub-array 2. ! A total of 21 telescope corrections were flagged in sub-array 4. ! A total of 16 telescope corrections were flagged in sub-array 6. ! A total of 14 telescope corrections were flagged in sub-array 7. ! A total of 8 telescope corrections were flagged in sub-array 8. ! A total of 45 telescope corrections were flagged in sub-array 9. ! ! Correcting IF 5. ! A total of 64 telescope corrections were flagged in sub-array 1. ! A total of 64 telescope corrections were flagged in sub-array 2. ! A total of 38 telescope corrections were flagged in sub-array 4. ! A total of 16 telescope corrections were flagged in sub-array 6. ! A total of 14 telescope corrections were flagged in sub-array 7. ! A total of 16 telescope corrections were flagged in sub-array 8. ! A total of 62 telescope corrections were flagged in sub-array 9. ! ! Correcting IF 6. ! A total of 64 telescope corrections were flagged in sub-array 1. ! A total of 64 telescope corrections were flagged in sub-array 2. ! A total of 38 telescope corrections were flagged in sub-array 4. ! A total of 16 telescope corrections were flagged in sub-array 6. ! A total of 14 telescope corrections were flagged in sub-array 7. ! A total of 16 telescope corrections were flagged in sub-array 8. ! A total of 62 telescope corrections were flagged in sub-array 9. ! ! Correcting IF 7. ! A total of 64 telescope corrections were flagged in sub-array 1. ! A total of 64 telescope corrections were flagged in sub-array 2. ! A total of 21 telescope corrections were flagged in sub-array 4. ! A total of 16 telescope corrections were flagged in sub-array 6. ! A total of 14 telescope corrections were flagged in sub-array 7. ! A total of 8 telescope corrections were flagged in sub-array 8. ! A total of 45 telescope corrections were flagged in sub-array 9. ! ! Correcting IF 8. ! A total of 64 telescope corrections were flagged in sub-array 1. ! A total of 64 telescope corrections were flagged in sub-array 2. ! A total of 21 telescope corrections were flagged in sub-array 4. ! A total of 16 telescope corrections were flagged in sub-array 6. ! A total of 14 telescope corrections were flagged in sub-array 7. ! A total of 8 telescope corrections were flagged in sub-array 8. ! A total of 45 telescope corrections were flagged in sub-array 9. ! ! Fit before self-cal, rms=1.006867Jy sigma=8.478939 ! Fit after self-cal, rms=0.900361Jy sigma=7.607982 ! 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 4.68% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 milli-arcsec ! Estimated beam: bmin=0.4684 mas, bmaj=0.9664 mas, bpa=-4.756 degrees ! Estimated noise=1.31369 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 = 0.0791333 Jy ! Component: 100 - total flux cleaned = 0.101934 Jy ! Total flux subtracted in 100 components = 0.101934 Jy ! Clean residual min=-0.004980 max=0.010525 Jy/beam ! Clean residual mean=0.000001 rms=0.001189 Jy/beam ! Combined flux in latest and established models = 0.101934 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.101934 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.102110Jy sigma=0.667526 ! Fit after self-cal, rms=0.101674Jy sigma=0.664976 ! Inverting map ! Your choice of large map pixels excluded 4.68% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0125398 Jy ! Component: 100 - total flux cleaned = 0.019439 Jy ! Total flux subtracted in 100 components = 0.019439 Jy ! Clean residual min=-0.005226 max=0.004857 Jy/beam ! Clean residual mean=0.000001 rms=0.001033 Jy/beam ! Combined flux in latest and established models = 0.121373 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 11 components and 0.121373 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.100159Jy sigma=0.646964 ! Fit after self-cal, rms=0.100071Jy sigma=0.646533 ! Inverting map ! Your choice of large map pixels excluded 4.68% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 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 4.68% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 milli-arcsec ! Estimated beam: bmin=0.5773 mas, bmaj=1.133 mas, bpa=-2.743 degrees ! Estimated noise=0.765144 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 (0.6, -0.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00477628 Jy ! Component: 100 - total flux cleaned = 0.0061995 Jy ! Component: 150 - total flux cleaned = 0.00663564 Jy ! Component: 200 - total flux cleaned = 0.00693275 Jy ! Total flux subtracted in 200 components = 0.00693275 Jy ! Clean residual min=-0.003178 max=0.002881 Jy/beam ! Clean residual mean=0.000009 rms=0.000624 Jy/beam ! Combined flux in latest and established models = 0.128306 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 26 components and 0.128306 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.099793Jy sigma=0.644098 ! Fit after self-cal, rms=0.099780Jy sigma=0.643925 ! Inverting map ! Your choice of large map pixels excluded 4.68% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5773 x 1.133 at -2.743 degrees (North through East) ! Clean map min=-0.0027869 max=0.099896 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. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! A total of 36 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! FD 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! FD 0.99 KP 0.95 NL 0.96 PT 1.05 ! SC 1.02 ! ! A total of 12 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* SC 1.00* ! ZC 1.00* ! ! A total of 21 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! EF 0.00* MC 0.00* ON 0.00* SC 0.00* ! ZC 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.98 EF 1.00* FD 0.97 KP 1.00 ! LA 1.07 MC 1.04 NL 0.91 ON 0.94 ! PT 0.91 SC 0.91 ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.17 MC 0.92 ON 0.94 ! ZC 0.84 ! ! A total of 36 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! FD 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! FD 1.04 KP 0.91 NL 0.96 PT 1.00 ! SC 0.89 ! ! A total of 12 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.03 MC 1.08 SC 0.88 ! ZC 0.85 ! ! A total of 21 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! EF 0.00* MC 0.00* ON 0.00* SC 0.00* ! ZC 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.98 EF 1.00* FD 1.00 KP 1.06 ! LA 1.06 MC 1.11 NL 0.90 ON 1.14 ! PT 1.04 SC 1.15 ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! A total of 36 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! FD 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! FD 1.00* KP 1.00* NL 1.00* PT 1.00* ! SC 1.00* ! ! A total of 12 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* SC 1.00* ! ZC 1.00* ! ! A total of 21 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! EF 0.00* MC 0.00* ON 0.00* SC 0.00* ! ZC 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.91 EF 1.00* FD 1.10 KP 0.98 ! LA 0.98 MC 1.05 NL 0.90 ON 1.08 ! PT 1.00 SC 1.02 ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! A total of 36 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! FD 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! FD 1.06 KP 1.04 NL 0.92 PT 0.97 ! SC 0.95 ! ! A total of 12 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* SC 1.00* ! ZC 1.00* ! ! A total of 21 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! EF 0.00* MC 0.00* ON 0.00* SC 0.00* ! ZC 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.08 EF 1.00* FD 1.04 KP 0.89 ! LA 0.96 MC 1.14 NL 0.97 ON 1.02 ! PT 1.08 SC 0.98 ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.01 EF 1.00* FD 1.06 HH 1.01 ! LA 1.04 MC 0.88 NL 0.98 ON 0.98 ! PT 1.07 SC 1.03 ZC 0.87 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 0.85 MC 1.00 ON 0.87 ! ZC 1.13 ! ! A total of 36 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! FD 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! FD 0.99 KP 0.88 NL 1.03 PT 0.91 ! SC 0.98 ! ! A total of 12 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.03 MC 1.05 SC 1.11 ! ZC 0.92 ! ! A total of 21 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! EF 0.00* MC 0.00* ON 0.00* SC 0.00* ! ZC 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 0.93 MC 1.16 ON 0.97 ! ZC 1.19 ! ! A total of 36 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! FD 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! FD 1.00* KP 1.00* NL 1.00* PT 1.00* ! SC 1.00* ! ! A total of 12 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* SC 1.00* ! ZC 1.00* ! ! A total of 21 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! EF 0.00* MC 0.00* ON 0.00* SC 0.00* ! ZC 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! A total of 36 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! FD 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! FD 0.89 KP 0.92 NL 1.03 PT 0.98 ! SC 0.97 ! ! A total of 12 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.12 MC 0.86 SC 0.90 ! ZC 0.91 ! ! A total of 21 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! EF 0.00* MC 0.00* ON 0.00* SC 0.00* ! ZC 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! A total of 36 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! FD 0.00* MC 0.00* SC 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! FD 1.00* KP 1.00* NL 1.00* PT 1.00* ! SC 1.00* ! ! A total of 12 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* SC 1.00* ! ZC 1.00* ! ! A total of 21 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! EF 0.00* MC 0.00* ON 0.00* SC 0.00* ! ZC 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.90 EF 1.00* FD 1.00 KP 0.97 ! LA 1.06 MC 1.18 NL 0.94 ON 1.18 ! PT 1.05 SC 1.10 ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! ! Fit before self-cal, rms=0.099780Jy sigma=0.643925 ! Fit after self-cal, rms=0.100506Jy sigma=0.648285 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 4.95% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 milli-arcsec ! Estimated beam: bmin=0.5836 mas, bmaj=1.152 mas, bpa=-2.141 degrees ! Estimated noise=0.776526 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 = 0.000165452 Jy ! Component: 100 - total flux cleaned = 0.000221097 Jy ! Component: 150 - total flux cleaned = 0.000268304 Jy ! Component: 200 - total flux cleaned = 0.000348403 Jy ! Total flux subtracted in 200 components = 0.000348403 Jy ! Clean residual min=-0.003419 max=0.003013 Jy/beam ! Clean residual mean=0.000009 rms=0.000596 Jy/beam ! Combined flux in latest and established models = 0.128654 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 30 components and 0.128654 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.100434Jy sigma=0.647787 ! Fit after self-cal, rms=0.100451Jy sigma=0.647682 ! Inverting map ! Your choice of large map pixels excluded 4.95% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 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. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.100451Jy sigma=0.647682 ! Fit after self-cal, rms=0.100399Jy sigma=0.647380 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.95% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 milli-arcsec ! Estimated beam: bmin=0.5825 mas, bmaj=1.151 mas, bpa=-2.19 degrees ! Estimated noise=0.776159 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 5.94487e-05 Jy ! Component: 100 - total flux cleaned = 5.61072e-05 Jy ! Component: 150 - total flux cleaned = 0.000126329 Jy ! Component: 200 - total flux cleaned = 0.000190474 Jy ! Total flux subtracted in 200 components = 0.000190474 Jy ! Clean residual min=-0.003436 max=0.003006 Jy/beam ! Clean residual mean=0.000009 rms=0.000589 Jy/beam ! Combined flux in latest and established models = 0.128845 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 32 components and 0.128845 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.100355Jy sigma=0.647092 ! Fit after self-cal, rms=0.100359Jy sigma=0.647049 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.95% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 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 = -0.000175439 Jy ! Component: 100 - total flux cleaned = -0.000142818 Jy ! Component: 150 - total flux cleaned = -0.000113446 Jy ! Component: 200 - total flux cleaned = -0.00011386 Jy ! Total flux subtracted in 200 components = -0.00011386 Jy ! Clean residual min=-0.003430 max=0.003013 Jy/beam ! Clean residual mean=0.000009 rms=0.000588 Jy/beam ! Combined flux in latest and established models = 0.128731 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 35 components and 0.128731 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.100325Jy sigma=0.646841 ! Fit after self-cal, rms=0.100325Jy sigma=0.646825 ! Inverting map ! Your choice of large map pixels excluded 4.95% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 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. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.100325Jy sigma=0.646825 ! Fit after self-cal, rms=0.100296Jy sigma=0.646463 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.95% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 milli-arcsec ! Estimated beam: bmin=0.5829 mas, bmaj=1.15 mas, bpa=-2.167 degrees ! Estimated noise=0.775778 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000229544 Jy ! Component: 100 - total flux cleaned = -0.000286237 Jy ! Component: 150 - total flux cleaned = -0.000286991 Jy ! Component: 200 - total flux cleaned = -0.000287828 Jy ! Total flux subtracted in 200 components = -0.000287828 Jy ! Clean residual min=-0.003351 max=0.003014 Jy/beam ! Clean residual mean=0.000009 rms=0.000580 Jy/beam ! Combined flux in latest and established models = 0.128443 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 35 components and 0.128443 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.100269Jy sigma=0.646284 ! Fit after self-cal, rms=0.100299Jy sigma=0.646263 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.95% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 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 = -6.25027e-05 Jy ! Component: 100 - total flux cleaned = -8.83499e-05 Jy ! Component: 150 - total flux cleaned = -8.83374e-05 Jy ! Component: 200 - total flux cleaned = -8.89569e-05 Jy ! Total flux subtracted in 200 components = -8.89569e-05 Jy ! Clean residual min=-0.003352 max=0.003023 Jy/beam ! Clean residual mean=0.000009 rms=0.000580 Jy/beam ! Combined flux in latest and established models = 0.128354 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 36 components and 0.128354 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.100279Jy sigma=0.646140 ! Fit after self-cal, rms=0.100280Jy sigma=0.646133 ! Inverting map ! Your choice of large map pixels excluded 4.95% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 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. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.100280Jy sigma=0.646133 ! Fit after self-cal, rms=0.100249Jy sigma=0.646122 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.95% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 milli-arcsec ! Estimated beam: bmin=2.74 mas, bmaj=3.283 mas, bpa=-52.8 degrees ! Estimated noise=0.991128 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000423483 Jy ! Component: 100 - total flux cleaned = -0.000494275 Jy ! Component: 150 - total flux cleaned = -0.000524506 Jy ! Component: 200 - total flux cleaned = -0.000553861 Jy ! Total flux subtracted in 200 components = -0.000553861 Jy ! Clean residual min=-0.003038 max=0.003572 Jy/beam ! Clean residual mean=0.000020 rms=0.000815 Jy/beam ! Combined flux in latest and established models = 0.1278 Jy selfcal ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 42 components and 0.1278 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.100256Jy sigma=0.646142 ! Fit after self-cal, rms=0.100256Jy sigma=0.646134 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.95% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 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 (44.2, 1.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00313424 Jy ! Component: 100 - total flux cleaned = 0.00439666 Jy ! Component: 150 - total flux cleaned = 0.00511318 Jy ! Component: 200 - total flux cleaned = 0.00556959 Jy ! Total flux subtracted in 200 components = 0.00556959 Jy ! Clean residual min=-0.002990 max=0.002895 Jy/beam ! Clean residual mean=0.000019 rms=0.000703 Jy/beam ! Combined flux in latest and established models = 0.13337 Jy ! Performing phase self-cal ! Adding 41 model components to the UV plane model. ! The established model now contains 83 components and 0.13337 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.100210Jy sigma=0.645611 ! Fit after self-cal, rms=0.100200Jy sigma=0.645526 ! Inverting map ! Your choice of large map pixels excluded 4.95% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 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 4.95% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 milli-arcsec ! Estimated beam: bmin=0.5829 mas, bmaj=1.149 mas, bpa=-2.151 degrees ! Estimated noise=0.775681 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5829 x 1.149 at -2.151 degrees (North through East) ! Clean map min=-0.0048531 max=0.10017 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 4.95% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 milli-arcsec ! Estimated beam: bmin=0.4683 mas, bmaj=0.9681 mas, bpa=-3.698 degrees ! Estimated noise=1.32319 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0781278 Jy ! Component: 100 - total flux cleaned = 0.102148 Jy ! Component: 150 - total flux cleaned = 0.114425 Jy ! Component: 200 - total flux cleaned = 0.121559 Jy ! Total flux subtracted in 200 components = 0.121559 Jy ! Clean residual min=-0.004883 max=0.005086 Jy/beam ! Clean residual mean=0.000002 rms=0.001027 Jy/beam ! Combined flux in latest and established models = 0.121559 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 0.121559 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 4.95% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 milli-arcsec ! Estimated beam: bmin=0.5829 mas, bmaj=1.149 mas, bpa=-2.151 degrees ! Estimated noise=0.775681 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 = 0.00486474 Jy ! Component: 100 - total flux cleaned = 0.00665338 Jy ! Component: 150 - total flux cleaned = 0.00791466 Jy ! Component: 200 - total flux cleaned = 0.00883068 Jy ! Total flux subtracted in 200 components = 0.00883068 Jy ! Clean residual min=-0.003237 max=0.003122 Jy/beam ! Clean residual mean=0.000008 rms=0.000580 Jy/beam ! Combined flux in latest and established models = 0.130389 Jy ! Adding 29 model components to the UV plane model. ! The established model now contains 39 components and 0.130389 Jy ! Inverting map ! Your choice of large map pixels excluded 4.95% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 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 4.95% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 milli-arcsec ! Estimated beam: bmin=2.74 mas, bmaj=3.283 mas, bpa=-52.8 degrees ! Estimated noise=0.991128 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00186822 Jy ! Component: 100 - total flux cleaned = 0.00229556 Jy ! Component: 150 - total flux cleaned = 0.00259407 Jy ! Component: 200 - total flux cleaned = 0.00295545 Jy ! Total flux subtracted in 200 components = 0.00295545 Jy ! Clean residual min=-0.002969 max=0.003112 Jy/beam ! Clean residual mean=0.000018 rms=0.000705 Jy/beam ! Combined flux in latest and established models = 0.133345 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) ! Added new window around map position (50.4, -25.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0022016 Jy ! Component: 100 - total flux cleaned = 0.00237234 Jy ! Component: 150 - total flux cleaned = 0.0022025 Jy ! Component: 200 - total flux cleaned = 0.00212626 Jy ! Total flux subtracted in 200 components = 0.00212626 Jy ! Clean residual min=-0.002636 max=0.002483 Jy/beam ! Clean residual mean=0.000015 rms=0.000663 Jy/beam ! Combined flux in latest and established models = 0.135471 Jy ! Adding 48 model components to the UV plane model. ! The established model now contains 85 components and 0.135471 Jy ! Inverting map ! Your choice of large map pixels excluded 4.95% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 4.95% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 milli-arcsec ! Estimated beam: bmin=0.5829 mas, bmaj=1.149 mas, bpa=-2.151 degrees ! Estimated noise=0.775681 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00028294 Jy ! Component: 100 - total flux cleaned = 0.000496241 Jy ! Component: 150 - total flux cleaned = 0.000757579 Jy ! Component: 200 - total flux cleaned = 0.000816088 Jy ! Total flux subtracted in 200 components = 0.000816088 Jy ! Clean residual min=-0.002862 max=0.002487 Jy/beam ! Clean residual mean=0.000005 rms=0.000537 Jy/beam ! Combined flux in latest and established models = 0.136287 Jy selfcal ! Performing phase self-cal ! Adding 31 model components to the UV plane model. ! The established model now contains 109 components and 0.136287 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.100214Jy sigma=0.645488 ! Fit after self-cal, rms=0.100190Jy sigma=0.645274 wmodel /scr/pima/gb073_uvs/J2318+2404_X_map.mod ! Writing 109 model components to file: /scr/pima/gb073_uvs/J2318+2404_X_map.mod wobs /scr/pima/gb073_uvs/J2318+2404_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J2318+2404_X_uvs.fits wwins /scr/pima/gb073_uvs/J2318+2404_X_map.win ! wwins: Wrote 4 windows to /scr/pima/gb073_uvs/J2318+2404_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 4.95% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000962918 Jy ! Component: 100 - total flux cleaned = -0.00172451 Jy ! Component: 150 - total flux cleaned = -0.00218981 Jy ! Component: 200 - total flux cleaned = -0.00239268 Jy ! Component: 250 - total flux cleaned = -0.00239296 Jy ! Component: 300 - total flux cleaned = -0.00231669 Jy ! Component: 350 - total flux cleaned = -0.00227922 Jy ! Component: 400 - total flux cleaned = -0.00231617 Jy ! Component: 450 - total flux cleaned = -0.00238838 Jy ! Component: 500 - total flux cleaned = -0.00238845 Jy ! Component: 550 - total flux cleaned = -0.00245982 Jy ! Component: 600 - total flux cleaned = -0.00256385 Jy ! Component: 650 - total flux cleaned = -0.00263186 Jy ! Component: 700 - total flux cleaned = -0.00259725 Jy ! Component: 750 - total flux cleaned = -0.00259719 Jy ! Component: 800 - total flux cleaned = -0.00256443 Jy ! Component: 850 - total flux cleaned = -0.00263027 Jy ! Component: 900 - total flux cleaned = -0.00259778 Jy ! Component: 950 - total flux cleaned = -0.00263005 Jy ! Component: 1000 - total flux cleaned = -0.00272538 Jy ! Component: 1050 - total flux cleaned = -0.00272496 Jy ! Component: 1100 - total flux cleaned = -0.00272504 Jy ! Component: 1150 - total flux cleaned = -0.00281774 Jy ! Component: 1200 - total flux cleaned = -0.00269504 Jy ! Component: 1250 - total flux cleaned = -0.00281671 Jy ! Component: 1300 - total flux cleaned = -0.00284677 Jy ! Component: 1350 - total flux cleaned = -0.00296664 Jy ! Component: 1400 - total flux cleaned = -0.0029369 Jy ! Component: 1450 - total flux cleaned = -0.00299565 Jy ! Component: 1500 - total flux cleaned = -0.00317105 Jy ! Component: 1550 - total flux cleaned = -0.003287 Jy ! Component: 1600 - total flux cleaned = -0.00337338 Jy ! Component: 1650 - total flux cleaned = -0.00345869 Jy ! Component: 1700 - total flux cleaned = -0.00348698 Jy ! Component: 1750 - total flux cleaned = -0.00359982 Jy ! Component: 1800 - total flux cleaned = -0.00365539 Jy ! Component: 1850 - total flux cleaned = -0.00376663 Jy ! Component: 1900 - total flux cleaned = -0.00379411 Jy ! Component: 1950 - total flux cleaned = -0.00398569 Jy ! Component: 2000 - total flux cleaned = -0.00409426 Jy ! Component: 2050 - total flux cleaned = -0.00420216 Jy ! Component: 2100 - total flux cleaned = -0.00433638 Jy ! Component: 2150 - total flux cleaned = -0.00438974 Jy ! Component: 2200 - total flux cleaned = -0.00446928 Jy ! Component: 2250 - total flux cleaned = -0.00460114 Jy ! Component: 2300 - total flux cleaned = -0.00467964 Jy ! Component: 2350 - total flux cleaned = -0.00486198 Jy ! Component: 2400 - total flux cleaned = -0.00481031 Jy ! Component: 2450 - total flux cleaned = -0.00491306 Jy ! Component: 2500 - total flux cleaned = -0.00496426 Jy ! Component: 2550 - total flux cleaned = -0.00496421 Jy ! Component: 2600 - total flux cleaned = -0.00498949 Jy ! Component: 2650 - total flux cleaned = -0.00511538 Jy ! Component: 2700 - total flux cleaned = -0.00516547 Jy ! Component: 2750 - total flux cleaned = -0.00526497 Jy ! Component: 2800 - total flux cleaned = -0.00528991 Jy ! Component: 2850 - total flux cleaned = -0.0053884 Jy ! Component: 2900 - total flux cleaned = -0.00531514 Jy ! Component: 2950 - total flux cleaned = -0.00543708 Jy ! Component: 3000 - total flux cleaned = -0.00553405 Jy ! Component: 3050 - total flux cleaned = -0.00553387 Jy ! Component: 3100 - total flux cleaned = -0.00562993 Jy ! Component: 3150 - total flux cleaned = -0.00567745 Jy ! Component: 3200 - total flux cleaned = -0.00560617 Jy ! Component: 3250 - total flux cleaned = -0.00577165 Jy ! Component: 3300 - total flux cleaned = -0.00560691 Jy ! Component: 3350 - total flux cleaned = -0.00579437 Jy ! Component: 3400 - total flux cleaned = -0.00581766 Jy ! Component: 3450 - total flux cleaned = -0.00593376 Jy ! Component: 3500 - total flux cleaned = -0.00586429 Jy ! Component: 3550 - total flux cleaned = -0.00602511 Jy ! Component: 3600 - total flux cleaned = -0.00604796 Jy ! Component: 3650 - total flux cleaned = -0.00607074 Jy ! Component: 3700 - total flux cleaned = -0.00600275 Jy ! Component: 3750 - total flux cleaned = -0.00609317 Jy ! Component: 3800 - total flux cleaned = -0.00611558 Jy ! Component: 3850 - total flux cleaned = -0.00609329 Jy ! Component: 3900 - total flux cleaned = -0.00618247 Jy ! Component: 3950 - total flux cleaned = -0.00622683 Jy ! Component: 4000 - total flux cleaned = -0.00629325 Jy ! Component: 4050 - total flux cleaned = -0.00631549 Jy ! Total flux subtracted in 4096 components = -0.00635943 Jy ! Clean residual min=-0.001482 max=0.001405 Jy/beam ! Clean residual mean=0.000001 rms=0.000353 Jy/beam ! Combined flux in latest and established models = 0.129928 Jy keep ! Adding 315 model components to the UV plane model. ! The established model now contains 423 components and 0.129928 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J2318+2404_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 4.95% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5829 x 1.149 at -2.151 degrees (North through East) ! Clean map min=-0.0034174 max=0.099631 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J2318+2404_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0996309 invert ! Inverting map ! Your choice of large map pixels excluded 4.95% of the data. ! The x-axis pixel size should ideally be below 0.1768 milli-arcsec ! The y-axis pixel size should ideally be below 0.1887 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000352792 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -1.0623 1.0623 2.12459 4.24919 8.49837 16.9967 33.9935 67.987 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.001 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.099 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 282.407 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J2318+2404_X_uvs.log closed on Sat Dec 26 09:46:26 2015