! Started logfile: /scr/pima/gb073_uvs/J2036+2227_X_uvs.log on Sat Dec 26 09:44:42 2015 obs /scr/pima/gb073_uvs/J2036+2227_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J2036+2227_X_uva.fits ! AN table 1: 32 integrations on 6 of 6 possible baselines. ! AN table 2: 19 integrations on 45 of 45 possible baselines. ! AN table 3: 10 integrations on 36 of 36 possible baselines. ! AN table 4: 19 integrations on 45 of 45 possible baselines. ! AN table 5: 12 integrations on 66 of 66 possible baselines. ! AN table 6: 27 integrations on 10 of 10 possible baselines. ! AN table 7: 15 integrations on 6 of 6 possible baselines. ! AN table 8: 11 integrations on 55 of 55 possible baselines. ! AN table 9: 7 integrations on 6 of 6 possible baselines. ! AN table 10: 8 integrations on 28 of 28 possible baselines. ! Apparent sampling: 0.689848 visibilities/baseline/integration-bin. ! Found source: J2036+2227 ! ! 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 23648 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/J2036+2227_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 101 telescope corrections were flagged in sub-array 1. ! A total of 46 telescope corrections were flagged in sub-array 2. ! A total of 39 telescope corrections were flagged in sub-array 4. ! A total of 25 telescope corrections were flagged in sub-array 5. ! A total of 48 telescope corrections were flagged in sub-array 6. ! A total of 33 telescope corrections were flagged in sub-array 7. ! A total of 25 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 2. ! A total of 101 telescope corrections were flagged in sub-array 1. ! A total of 46 telescope corrections were flagged in sub-array 2. ! A total of 39 telescope corrections were flagged in sub-array 4. ! A total of 25 telescope corrections were flagged in sub-array 5. ! A total of 48 telescope corrections were flagged in sub-array 6. ! A total of 33 telescope corrections were flagged in sub-array 7. ! A total of 25 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 3. ! A total of 101 telescope corrections were flagged in sub-array 1. ! A total of 46 telescope corrections were flagged in sub-array 2. ! A total of 39 telescope corrections were flagged in sub-array 4. ! A total of 25 telescope corrections were flagged in sub-array 5. ! A total of 48 telescope corrections were flagged in sub-array 6. ! A total of 33 telescope corrections were flagged in sub-array 7. ! A total of 25 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 4. ! A total of 101 telescope corrections were flagged in sub-array 1. ! A total of 46 telescope corrections were flagged in sub-array 2. ! A total of 39 telescope corrections were flagged in sub-array 4. ! A total of 25 telescope corrections were flagged in sub-array 5. ! A total of 48 telescope corrections were flagged in sub-array 6. ! A total of 33 telescope corrections were flagged in sub-array 7. ! A total of 25 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 5. ! A total of 101 telescope corrections were flagged in sub-array 1. ! A total of 64 telescope corrections were flagged in sub-array 2. ! A total of 10 telescope corrections were flagged in sub-array 3. ! A total of 39 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 48 telescope corrections were flagged in sub-array 6. ! A total of 33 telescope corrections were flagged in sub-array 7. ! A total of 36 telescope corrections were flagged in sub-array 8. ! A total of 7 telescope corrections were flagged in sub-array 9. ! A total of 8 telescope corrections were flagged in sub-array 10. ! ! Correcting IF 6. ! A total of 101 telescope corrections were flagged in sub-array 1. ! A total of 64 telescope corrections were flagged in sub-array 2. ! A total of 10 telescope corrections were flagged in sub-array 3. ! A total of 39 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 48 telescope corrections were flagged in sub-array 6. ! A total of 33 telescope corrections were flagged in sub-array 7. ! A total of 36 telescope corrections were flagged in sub-array 8. ! A total of 7 telescope corrections were flagged in sub-array 9. ! A total of 8 telescope corrections were flagged in sub-array 10. ! ! Correcting IF 7. ! A total of 101 telescope corrections were flagged in sub-array 1. ! A total of 46 telescope corrections were flagged in sub-array 2. ! A total of 39 telescope corrections were flagged in sub-array 4. ! A total of 25 telescope corrections were flagged in sub-array 5. ! A total of 48 telescope corrections were flagged in sub-array 6. ! A total of 33 telescope corrections were flagged in sub-array 7. ! A total of 25 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 8. ! A total of 101 telescope corrections were flagged in sub-array 1. ! A total of 46 telescope corrections were flagged in sub-array 2. ! A total of 39 telescope corrections were flagged in sub-array 4. ! A total of 25 telescope corrections were flagged in sub-array 5. ! A total of 48 telescope corrections were flagged in sub-array 6. ! A total of 33 telescope corrections were flagged in sub-array 7. ! A total of 25 telescope corrections were flagged in sub-array 8. ! ! Fit before self-cal, rms=1.008681Jy sigma=9.267875 ! Fit after self-cal, rms=0.909348Jy sigma=8.398781 ! clrmod: Cleared the established, tentative and continuum models. ! Redundant starting model cleared. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 3.97% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 milli-arcsec ! Estimated beam: bmin=0.5917 mas, bmaj=0.9633 mas, bpa=24.73 degrees ! Estimated noise=0.9992 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 = 0.0693717 Jy ! Component: 100 - total flux cleaned = 0.0896748 Jy ! Total flux subtracted in 100 components = 0.0896748 Jy ! Clean residual min=-0.003970 max=0.010883 Jy/beam ! Clean residual mean=0.000006 rms=0.000958 Jy/beam ! Combined flux in latest and established models = 0.0896748 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 9 components and 0.0896748 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=0.089420Jy sigma=0.677420 ! Fit after self-cal, rms=0.088919Jy sigma=0.674584 ! Inverting map ! Your choice of large map pixels excluded 3.97% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 milli-arcsec ! Added new window around map position (-1.2, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0119416 Jy ! Component: 100 - total flux cleaned = 0.0189925 Jy ! Total flux subtracted in 100 components = 0.0189925 Jy ! Clean residual min=-0.003278 max=0.004642 Jy/beam ! Clean residual mean=0.000000 rms=0.000766 Jy/beam ! Combined flux in latest and established models = 0.108667 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 17 components and 0.108667 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=0.087037Jy sigma=0.650227 ! Fit after self-cal, rms=0.086910Jy sigma=0.649145 ! Inverting map ! Your choice of large map pixels excluded 3.97% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00532779 Jy ! Component: 100 - total flux cleaned = 0.00843186 Jy ! Total flux subtracted in 100 components = 0.00843186 Jy ! Clean residual min=-0.003097 max=0.003264 Jy/beam ! Clean residual mean=-0.000002 rms=0.000711 Jy/beam ! Combined flux in latest and established models = 0.117099 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 21 components and 0.117099 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=0.086563Jy sigma=0.644782 ! Fit after self-cal, rms=0.086513Jy sigma=0.644347 ! Inverting map ! Your choice of large map pixels excluded 3.97% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 milli-arcsec print "************** FINISHED UNIFORM WEIGHTING CLEAN **************" ! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** ! uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. win_mult = win_mult * 1.6 clean_niter = clean_niter * 2 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 3.97% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 milli-arcsec ! Estimated beam: bmin=0.7551 mas, bmaj=1.179 mas, bpa=22.77 degrees ! Estimated noise=0.579434 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 = 0.00281702 Jy ! Component: 100 - total flux cleaned = 0.00404133 Jy ! Component: 150 - total flux cleaned = 0.00435697 Jy ! Component: 200 - total flux cleaned = 0.00448735 Jy ! Total flux subtracted in 200 components = 0.00448735 Jy ! Clean residual min=-0.002013 max=0.001979 Jy/beam ! Clean residual mean=0.000002 rms=0.000457 Jy/beam ! Combined flux in latest and established models = 0.121587 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 29 components and 0.121587 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=0.086425Jy sigma=0.643397 ! Fit after self-cal, rms=0.086402Jy sigma=0.643225 ! Inverting map ! Your choice of large map pixels excluded 3.97% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7551 x 1.179 at 22.77 degrees (North through East) ! Clean map min=-0.0018841 max=0.088519 Jy/beam if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val ! Selfcal amplitude corrections will be limited to 0.833333 -> 1.2. ! Selfcal phase corrections will not be limited. gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 27 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.90 EF 1.00* FD 0.96 HH 1.17 ! LA 1.04 MC 0.94 NL 0.87 PT 1.06 ! SC 1.06 ZC 0.98 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.91 FD 0.96 KP 0.99 LA 0.97 ! MK 1.11 NL 0.93 OV 1.04 PT 1.00 ! SC 1.15 ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* FD 0.96 HH 0.98 LA 0.98 ! MC 0.89 NL 0.99 ON 1.02 PT 1.06 ! SC 0.99 ZC 1.06 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* MK 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! A total of 27 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! HH 0.00* MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.91 EF 1.00* FD 1.01 KP 1.00 ! LA 1.06 MK 1.13 NL 0.89 ON 1.00* ! OV 0.97 PT 1.03 SC 0.94 ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.00* KP 1.00* MK 1.00* OV 1.00* ! ! Telescope amplitude corrections in sub-array 10: ! BR 1.08 FD 0.98 KP 0.98 LA 1.07 ! MK 1.03 NL 0.92 OV 1.00 PT 0.98 ! ! ! Correcting IF 2. ! A total of 27 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! LA 1.00* MC 1.00* NL 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.12 FD 1.03 KP 1.01 LA 1.06 ! MK 0.96 NL 0.95 OV 1.02 PT 0.91 ! SC 1.15 ! ! Telescope amplitude corrections in sub-array 4: ! 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* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* MK 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00 MC 0.89 ON 0.90 ! ZC 1.00 ! ! A total of 27 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! HH 0.00* MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.98 EF 1.00* FD 0.98 KP 0.96 ! LA 1.19 MK 1.05 NL 1.05 ON 1.00* ! OV 1.02 PT 1.02 SC 0.97 ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.05 KP 1.11 MK 0.95 OV 0.88 ! ! Telescope amplitude corrections in sub-array 10: ! BR 1.08 FD 0.97 KP 1.00 LA 1.13 ! MK 1.02 NL 0.95 OV 1.12 PT 0.92 ! ! ! Correcting IF 3. ! A total of 27 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! LA 1.00* MC 1.00* NL 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 FD 0.93 KP 0.88 LA 1.06 ! MK 1.05 NL 0.95 OV 1.00 PT 0.97 ! SC 1.12 ! ! Telescope amplitude corrections in sub-array 4: ! 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* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* MK 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! A total of 27 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! HH 0.00* MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.94 EF 1.00* FD 1.01 KP 0.94 ! LA 0.99 MK 0.92 NL 1.18 ON 1.00* ! OV 0.98 PT 1.00 SC 1.01 ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.00* KP 1.00* MK 1.00* OV 1.00* ! ! Telescope amplitude corrections in sub-array 10: ! BR 1.00 FD 1.04 KP 0.94 LA 1.05 ! MK 0.98 NL 0.87 OV 1.01 PT 1.04 ! ! ! Correcting IF 4. ! A total of 27 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! LA 1.00* MC 1.00* NL 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 1.04 KP 1.02 LA 0.96 ! MK 0.99 NL 1.05 OV 0.94 PT 1.05 ! SC 1.19 ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* FD 1.03 HH 0.89 LA 0.95 ! MC 0.93 NL 1.00 ON 1.14 PT 1.14 ! SC 1.01 ZC 0.99 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* MK 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! A total of 27 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! HH 0.00* MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 0.93 EF 1.00* FD 1.05 KP 0.94 ! LA 1.04 MK 0.84 NL 1.05 ON 1.00* ! OV 1.04 PT 1.01 SC 0.96 ! ! Telescope amplitude corrections in sub-array 9: ! BR 0.89 KP 1.07 MK 0.94 OV 0.96 ! ! Telescope amplitude corrections in sub-array 10: ! BR 1.02 FD 1.05 KP 1.04 LA 0.94 ! MK 1.17 NL 1.02 OV 1.06 PT 0.96 ! ! ! Correcting IF 5. ! A total of 27 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.07 HH 1.06 ! LA 1.00 MC 0.98 NL 1.06 PT 0.94 ! SC 1.03 ZC 0.92 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.05 KP 0.91 LA 1.07 ! MK 1.05 NL 0.93 OV 0.99 PT 0.96 ! SC 1.16 ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* FD 1.07 HH 0.96 LA 0.98 ! MC 1.19 NL 1.00 ON 1.15 PT 1.06 ! SC 1.03 ZC 0.94 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.07 KP 0.86 ! LA 0.99 MC 0.95 MK 1.04 NL 1.13 ! ON 0.92 OV 1.13 PT 1.04 SC 1.08 ! ! A total of 15 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 0.85 MC 1.15 ON 0.92 ! ZC 0.98 ! ! A total of 27 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! HH 0.00* MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.00* EF 1.00* FD 1.06 KP 0.89 ! LA 1.00 MK 1.07 NL 1.02 ON 1.00* ! OV 1.11 PT 1.00 SC 0.95 ! ! A total of 21 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! BR 0.00* KP 0.00* MK 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 10: ! BR 1.00* FD 1.05 KP 0.84 LA 1.03 ! MK 1.09 NL 1.07 OV 1.11 PT 0.99 ! ! ! Correcting IF 6. ! A total of 27 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! LA 1.00* MC 1.00* NL 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.09 KP 0.90 LA 0.99 ! MK 0.98 NL 0.94 OV 1.05 PT 0.95 ! SC 0.89 ! ! Telescope amplitude corrections in sub-array 4: ! 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* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.04 KP 0.92 ! LA 1.05 MC 0.88 MK 1.04 NL 1.14 ! ON 0.96 OV 1.05 PT 0.94 SC 0.91 ! ! A total of 15 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! A total of 27 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! HH 0.00* MC 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* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! A total of 21 telescope corrections were flagged in sub-array 9. ! Telescope amplitude corrections in sub-array 9: ! BR 0.00* KP 0.00* MK 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 10: ! BR 1.00* FD 1.07 KP 0.90 LA 0.97 ! MK 1.07 NL 0.94 OV 1.05 PT 0.88 ! ! ! Correcting IF 7. ! A total of 27 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! LA 1.00* MC 1.00* NL 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! 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* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* MK 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! A total of 27 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! HH 0.00* MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! BR 1.01 EF 1.00* FD 1.01 KP 0.91 ! LA 1.06 MK 1.05 NL 1.09 ON 1.00* ! OV 0.98 PT 0.96 SC 1.01 ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.00* KP 1.00* MK 1.00* OV 1.00* ! ! Telescope amplitude corrections in sub-array 10: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! ! ! Correcting IF 8. ! A total of 27 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! LA 1.00* MC 1.00* NL 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! 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* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* MK 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! A total of 15 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! A total of 27 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! HH 0.00* MC 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* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 9: ! BR 1.02 KP 1.14 MK 0.99 OV 0.99 ! ! Telescope amplitude corrections in sub-array 10: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! ! ! Fit before self-cal, rms=0.086402Jy sigma=0.643225 ! Fit after self-cal, rms=0.086119Jy sigma=0.642904 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 4.07% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 milli-arcsec ! Estimated beam: bmin=0.7521 mas, bmaj=1.229 mas, bpa=21.04 degrees ! Estimated noise=0.583764 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 = 0.000275247 Jy ! Component: 100 - total flux cleaned = 0.00020187 Jy ! Component: 150 - total flux cleaned = 0.000202296 Jy ! Component: 200 - total flux cleaned = 0.000220956 Jy ! Total flux subtracted in 200 components = 0.000220956 Jy ! Clean residual min=-0.001853 max=0.001874 Jy/beam ! Clean residual mean=0.000000 rms=0.000410 Jy/beam ! Combined flux in latest and established models = 0.121807 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 35 components and 0.121807 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=0.086112Jy sigma=0.642768 ! Fit after self-cal, rms=0.086127Jy sigma=0.642647 ! Inverting map ! Your choice of large map pixels excluded 4.07% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 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=0.086127Jy sigma=0.642647 ! Fit after self-cal, rms=0.086226Jy sigma=0.642608 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.07% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 milli-arcsec ! Estimated beam: bmin=0.752 mas, bmaj=1.229 mas, bpa=21.05 degrees ! Estimated noise=0.583934 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000128415 Jy ! Component: 100 - total flux cleaned = 0.000147486 Jy ! Component: 150 - total flux cleaned = 0.000147002 Jy ! Component: 200 - total flux cleaned = 0.000162852 Jy ! Total flux subtracted in 200 components = 0.000162852 Jy ! Clean residual min=-0.001877 max=0.001884 Jy/beam ! Clean residual mean=0.000000 rms=0.000408 Jy/beam ! Combined flux in latest and established models = 0.12197 Jy selfcal ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 35 components and 0.12197 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=0.086220Jy sigma=0.642530 ! Fit after self-cal, rms=0.086224Jy sigma=0.642512 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.07% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 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 (-38.2, 27.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00166162 Jy ! Component: 100 - total flux cleaned = 0.0018933 Jy ! Component: 150 - total flux cleaned = 0.00192249 Jy ! Component: 200 - total flux cleaned = 0.00194662 Jy ! Total flux subtracted in 200 components = 0.00194662 Jy ! Clean residual min=-0.001800 max=0.001769 Jy/beam ! Clean residual mean=0.000000 rms=0.000405 Jy/beam ! Combined flux in latest and established models = 0.123917 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 46 components and 0.123917 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=0.086184Jy sigma=0.642169 ! Fit after self-cal, rms=0.086174Jy sigma=0.642114 ! Inverting map ! Your choice of large map pixels excluded 4.07% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 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=0.086174Jy sigma=0.642114 ! Fit after self-cal, rms=0.086199Jy sigma=0.641920 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.07% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 milli-arcsec ! Estimated beam: bmin=0.7518 mas, bmaj=1.228 mas, bpa=21.1 degrees ! Estimated noise=0.5841 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000532253 Jy ! Component: 100 - total flux cleaned = 0.00055853 Jy ! Component: 150 - total flux cleaned = 0.000602931 Jy ! Component: 200 - total flux cleaned = 0.000622596 Jy ! Total flux subtracted in 200 components = 0.000622596 Jy ! Clean residual min=-0.001751 max=0.001770 Jy/beam ! Clean residual mean=0.000000 rms=0.000402 Jy/beam ! Combined flux in latest and established models = 0.12454 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 49 components and 0.12454 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=0.086186Jy sigma=0.641820 ! Fit after self-cal, rms=0.086191Jy sigma=0.641797 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.07% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 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 (43.2, -22.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00133875 Jy ! Component: 100 - total flux cleaned = 0.00156283 Jy ! Component: 150 - total flux cleaned = 0.00164132 Jy ! Component: 200 - total flux cleaned = 0.00168882 Jy ! Total flux subtracted in 200 components = 0.00168882 Jy ! Clean residual min=-0.001724 max=0.001715 Jy/beam ! Clean residual mean=0.000001 rms=0.000395 Jy/beam ! Combined flux in latest and established models = 0.126228 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 65 components and 0.126228 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=0.086152Jy sigma=0.641471 ! Fit after self-cal, rms=0.086150Jy sigma=0.641441 ! Inverting map ! Your choice of large map pixels excluded 4.07% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 milli-arcsec ! Added new window around map position (-29.6, -41.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00136399 Jy ! Component: 100 - total flux cleaned = 0.0014306 Jy ! Component: 150 - total flux cleaned = 0.00151156 Jy ! Component: 200 - total flux cleaned = 0.00155977 Jy ! Total flux subtracted in 200 components = 0.00155977 Jy ! Clean residual min=-0.001648 max=0.001633 Jy/beam ! Clean residual mean=0.000000 rms=0.000386 Jy/beam ! Combined flux in latest and established models = 0.127788 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 78 components and 0.127788 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=0.086111Jy sigma=0.641135 ! Fit after self-cal, rms=0.086105Jy sigma=0.641100 ! Inverting map ! Your choice of large map pixels excluded 4.07% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 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=0.086105Jy sigma=0.641100 ! Fit after self-cal, rms=0.086112Jy sigma=0.640905 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.07% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 milli-arcsec ! Estimated beam: bmin=2.606 mas, bmaj=2.983 mas, bpa=-3.157 degrees ! Estimated noise=0.713328 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -3.14098e-05 Jy ! Component: 100 - total flux cleaned = -7.86809e-05 Jy ! Component: 150 - total flux cleaned = -3.98274e-05 Jy ! Component: 200 - total flux cleaned = -3.93102e-06 Jy ! Total flux subtracted in 200 components = -3.93102e-06 Jy ! Clean residual min=-0.001642 max=0.001677 Jy/beam ! Clean residual mean=0.000001 rms=0.000454 Jy/beam ! Combined flux in latest and established models = 0.127784 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 84 components and 0.127784 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=0.086108Jy sigma=0.640882 ! Fit after self-cal, rms=0.086110Jy sigma=0.640870 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.07% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 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 = -2.16572e-05 Jy ! Component: 100 - total flux cleaned = 1.43964e-05 Jy ! Component: 150 - total flux cleaned = 4.63816e-05 Jy ! Component: 200 - total flux cleaned = 5.63857e-05 Jy ! Total flux subtracted in 200 components = 5.63857e-05 Jy ! Clean residual min=-0.001624 max=0.001665 Jy/beam ! Clean residual mean=0.000001 rms=0.000452 Jy/beam ! Combined flux in latest and established models = 0.127841 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 91 components and 0.127841 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=0.086106Jy sigma=0.640859 ! Fit after self-cal, rms=0.086106Jy sigma=0.640853 ! Inverting map ! Your choice of large map pixels excluded 4.07% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 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 4.07% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 milli-arcsec ! Estimated beam: bmin=0.7519 mas, bmaj=1.229 mas, bpa=21.13 degrees ! Estimated noise=0.583688 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7519 x 1.229 at 21.13 degrees (North through East) ! Clean map min=-0.0014368 max=0.088198 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 4.07% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 milli-arcsec ! Estimated beam: bmin=0.5873 mas, bmaj=0.9975 mas, bpa=23.28 degrees ! Estimated noise=0.999691 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0685322 Jy ! Component: 100 - total flux cleaned = 0.0904875 Jy ! Component: 150 - total flux cleaned = 0.103103 Jy ! Component: 200 - total flux cleaned = 0.110556 Jy ! Total flux subtracted in 200 components = 0.110556 Jy ! Clean residual min=-0.003077 max=0.003816 Jy/beam ! Clean residual mean=-0.000000 rms=0.000704 Jy/beam ! Combined flux in latest and established models = 0.110556 Jy uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Adding 16 model components to the UV plane model. ! The established model now contains 16 components and 0.110556 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 4.07% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 milli-arcsec ! Estimated beam: bmin=0.7519 mas, bmaj=1.229 mas, bpa=21.13 degrees ! Estimated noise=0.583688 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 = 0.00559898 Jy ! Component: 100 - total flux cleaned = 0.00868612 Jy ! Component: 150 - total flux cleaned = 0.0110414 Jy ! Component: 200 - total flux cleaned = 0.0129194 Jy ! Total flux subtracted in 200 components = 0.0129194 Jy ! Clean residual min=-0.001753 max=0.001708 Jy/beam ! Clean residual mean=0.000000 rms=0.000396 Jy/beam ! Combined flux in latest and established models = 0.123475 Jy ! Adding 23 model components to the UV plane model. ! The established model now contains 31 components and 0.123475 Jy ! Inverting map ! Your choice of large map pixels excluded 4.07% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 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 4.07% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 milli-arcsec ! Estimated beam: bmin=2.606 mas, bmaj=2.983 mas, bpa=-3.157 degrees ! Estimated noise=0.713328 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00147838 Jy ! Component: 100 - total flux cleaned = 0.00234759 Jy ! Component: 150 - total flux cleaned = 0.00300499 Jy ! Component: 200 - total flux cleaned = 0.00332864 Jy ! Total flux subtracted in 200 components = 0.00332864 Jy ! Clean residual min=-0.001638 max=0.001645 Jy/beam ! Clean residual mean=0.000001 rms=0.000452 Jy/beam ! Combined flux in latest and established models = 0.126804 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 = 0.000171917 Jy ! Component: 100 - total flux cleaned = 0.000309298 Jy ! Component: 150 - total flux cleaned = 0.000450419 Jy ! Component: 200 - total flux cleaned = 0.000564084 Jy ! Total flux subtracted in 200 components = 0.000564084 Jy ! Clean residual min=-0.001630 max=0.001629 Jy/beam ! Clean residual mean=0.000001 rms=0.000452 Jy/beam ! Combined flux in latest and established models = 0.127368 Jy ! Adding 30 model components to the UV plane model. ! The established model now contains 61 components and 0.127368 Jy ! Inverting map ! Your choice of large map pixels excluded 4.07% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 4.07% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 milli-arcsec ! Estimated beam: bmin=0.7519 mas, bmaj=1.229 mas, bpa=21.13 degrees ! Estimated noise=0.583688 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000574163 Jy ! Component: 100 - total flux cleaned = 0.000695869 Jy ! Component: 150 - total flux cleaned = 0.000805913 Jy ! Component: 200 - total flux cleaned = 0.00090785 Jy ! Total flux subtracted in 200 components = 0.00090785 Jy ! Clean residual min=-0.001665 max=0.001723 Jy/beam ! Clean residual mean=0.000000 rms=0.000386 Jy/beam ! Combined flux in latest and established models = 0.128276 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 74 components and 0.128276 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=0.086149Jy sigma=0.641181 ! Fit after self-cal, rms=0.086154Jy sigma=0.641115 wmodel /scr/pima/gb073_uvs/J2036+2227_X_map.mod ! Writing 74 model components to file: /scr/pima/gb073_uvs/J2036+2227_X_map.mod wobs /scr/pima/gb073_uvs/J2036+2227_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J2036+2227_X_uvs.fits wwins /scr/pima/gb073_uvs/J2036+2227_X_map.win ! wwins: Wrote 5 windows to /scr/pima/gb073_uvs/J2036+2227_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 4.07% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 2.04942e-06 Jy ! Component: 100 - total flux cleaned = 3.13258e-05 Jy ! Component: 150 - total flux cleaned = -2.66075e-05 Jy ! Component: 200 - total flux cleaned = -0.000109757 Jy ! Component: 250 - total flux cleaned = -0.000136762 Jy ! Component: 300 - total flux cleaned = -0.000242762 Jy ! Component: 350 - total flux cleaned = -0.000346675 Jy ! Component: 400 - total flux cleaned = -0.000448895 Jy ! Component: 450 - total flux cleaned = -0.000499469 Jy ! Component: 500 - total flux cleaned = -0.000573506 Jy ! Component: 550 - total flux cleaned = -0.00057317 Jy ! Component: 600 - total flux cleaned = -0.000668762 Jy ! Component: 650 - total flux cleaned = -0.000668514 Jy ! Component: 700 - total flux cleaned = -0.000621559 Jy ! Component: 750 - total flux cleaned = -0.000714559 Jy ! Component: 800 - total flux cleaned = -0.000760135 Jy ! Component: 850 - total flux cleaned = -0.000828459 Jy ! Component: 900 - total flux cleaned = -0.000963394 Jy ! Component: 950 - total flux cleaned = -0.00109689 Jy ! Component: 1000 - total flux cleaned = -0.00114107 Jy ! Component: 1050 - total flux cleaned = -0.00120673 Jy ! Component: 1100 - total flux cleaned = -0.00140166 Jy ! Component: 1150 - total flux cleaned = -0.00144474 Jy ! Component: 1200 - total flux cleaned = -0.00155135 Jy ! Component: 1250 - total flux cleaned = -0.00161446 Jy ! Component: 1300 - total flux cleaned = -0.00169815 Jy ! Component: 1350 - total flux cleaned = -0.00167714 Jy ! Component: 1400 - total flux cleaned = -0.00169783 Jy ! Component: 1450 - total flux cleaned = -0.00175938 Jy ! Component: 1500 - total flux cleaned = -0.0018 Jy ! Component: 1550 - total flux cleaned = -0.00188086 Jy ! Component: 1600 - total flux cleaned = -0.00184053 Jy ! Component: 1650 - total flux cleaned = -0.00198023 Jy ! Component: 1700 - total flux cleaned = -0.00197975 Jy ! Component: 1750 - total flux cleaned = -0.00199943 Jy ! Component: 1800 - total flux cleaned = -0.00201886 Jy ! Component: 1850 - total flux cleaned = -0.00213588 Jy ! Component: 1900 - total flux cleaned = -0.00213575 Jy ! Component: 1950 - total flux cleaned = -0.00221273 Jy ! Component: 2000 - total flux cleaned = -0.0023656 Jy ! Component: 2050 - total flux cleaned = -0.00230823 Jy ! Component: 2100 - total flux cleaned = -0.00242185 Jy ! Component: 2150 - total flux cleaned = -0.00245933 Jy ! Component: 2200 - total flux cleaned = -0.0024968 Jy ! Component: 2250 - total flux cleaned = -0.00255278 Jy ! Component: 2300 - total flux cleaned = -0.00273796 Jy ! Component: 2350 - total flux cleaned = -0.00281157 Jy ! Component: 2400 - total flux cleaned = -0.00284826 Jy ! Component: 2450 - total flux cleaned = -0.00301243 Jy ! Component: 2500 - total flux cleaned = -0.00303063 Jy ! Component: 2550 - total flux cleaned = -0.00312088 Jy ! Component: 2600 - total flux cleaned = -0.00319282 Jy ! Component: 2650 - total flux cleaned = -0.00328249 Jy ! Component: 2700 - total flux cleaned = -0.00338929 Jy ! Component: 2750 - total flux cleaned = -0.00344234 Jy ! Component: 2800 - total flux cleaned = -0.00361875 Jy ! Component: 2850 - total flux cleaned = -0.00361864 Jy ! Component: 2900 - total flux cleaned = -0.00377593 Jy ! Component: 2950 - total flux cleaned = -0.00382803 Jy ! Component: 3000 - total flux cleaned = -0.00386265 Jy ! Component: 3050 - total flux cleaned = -0.00400054 Jy ! Component: 3100 - total flux cleaned = -0.00403487 Jy ! Component: 3150 - total flux cleaned = -0.00408616 Jy ! Component: 3200 - total flux cleaned = -0.00415423 Jy ! Component: 3250 - total flux cleaned = -0.00420498 Jy ! Component: 3300 - total flux cleaned = -0.00430607 Jy ! Component: 3350 - total flux cleaned = -0.00439008 Jy ! Component: 3400 - total flux cleaned = -0.0044568 Jy ! Component: 3450 - total flux cleaned = -0.00450674 Jy ! Component: 3500 - total flux cleaned = -0.00462278 Jy ! Component: 3550 - total flux cleaned = -0.00475478 Jy ! Component: 3600 - total flux cleaned = -0.00480413 Jy ! Component: 3650 - total flux cleaned = -0.00482045 Jy ! Component: 3700 - total flux cleaned = -0.00498328 Jy ! Component: 3750 - total flux cleaned = -0.00499959 Jy ! Component: 3800 - total flux cleaned = -0.00509647 Jy ! Component: 3850 - total flux cleaned = -0.00512872 Jy ! Component: 3900 - total flux cleaned = -0.00522481 Jy ! Component: 3950 - total flux cleaned = -0.00520889 Jy ! Component: 4000 - total flux cleaned = -0.00520895 Jy ! Component: 4050 - total flux cleaned = -0.00531976 Jy ! Total flux subtracted in 4096 components = -0.00549337 Jy ! Clean residual min=-0.001093 max=0.001044 Jy/beam ! Clean residual mean=-0.000001 rms=0.000263 Jy/beam ! Combined flux in latest and established models = 0.122782 Jy keep ! Adding 346 model components to the UV plane model. ! The established model now contains 420 components and 0.122782 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J2036+2227_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 4.07% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7519 x 1.229 at 21.13 degrees (North through East) ! Clean map min=-0.0013321 max=0.088288 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J2036+2227_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0882883 invert ! Inverting map ! Your choice of large map pixels excluded 4.07% of the data. ! The x-axis pixel size should ideally be below 0.1814 milli-arcsec ! The y-axis pixel size should ideally be below 0.1937 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000261865 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.889808 0.889808 1.77962 3.55923 7.11846 14.2369 28.4738 56.9477 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0007 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.088 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 337.151 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J2036+2227_X_uvs.log closed on Sat Dec 26 09:44:48 2015