! Started logfile: /scr/pima/gb073_uvs/J1520+1601_X_uvs.log on Sat Dec 26 09:41:30 2015 obs /scr/pima/gb073_uvs/J1520+1601_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1520+1601_X_uva.fits ! AN table 1: 29 integrations on 3 of 3 possible baselines. ! AN table 2: 29 integrations on 55 of 55 possible baselines. ! AN table 3: 29 integrations on 21 of 21 possible baselines. ! AN table 4: 29 integrations on 10 of 10 possible baselines. ! AN table 5: 29 integrations on 55 of 55 possible baselines. ! AN table 6: 29 integrations on 55 of 55 possible baselines. ! Apparent sampling: 0.854791 visibilities/baseline/integration-bin. ! Found source: J1520+1601 ! ! 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 39464 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/J1520+1601_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 21 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 2 telescope corrections were flagged in sub-array 3. ! A total of 36 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 30 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 21 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 2 telescope corrections were flagged in sub-array 3. ! A total of 36 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 30 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 21 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 2 telescope corrections were flagged in sub-array 3. ! A total of 36 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 30 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 21 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 2 telescope corrections were flagged in sub-array 3. ! A total of 36 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 30 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 5. ! A total of 21 telescope corrections were flagged in sub-array 1. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 31 telescope corrections were flagged in sub-array 3. ! A total of 36 telescope corrections were flagged in sub-array 4. ! A total of 65 telescope corrections were flagged in sub-array 5. ! A total of 59 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 6. ! A total of 21 telescope corrections were flagged in sub-array 1. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 31 telescope corrections were flagged in sub-array 3. ! A total of 36 telescope corrections were flagged in sub-array 4. ! A total of 65 telescope corrections were flagged in sub-array 5. ! A total of 59 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 7. ! A total of 21 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 2 telescope corrections were flagged in sub-array 3. ! A total of 36 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 30 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 8. ! A total of 21 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 2 telescope corrections were flagged in sub-array 3. ! A total of 36 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 30 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.012463Jy sigma=8.794437 ! Fit after self-cal, rms=0.903073Jy sigma=7.770307 ! 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 8.62% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Estimated beam: bmin=0.5053 mas, bmaj=0.9339 mas, bpa=-1.59 degrees ! Estimated noise=1.02249 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 = 0.0755772 Jy ! Component: 100 - total flux cleaned = 0.100007 Jy ! Total flux subtracted in 100 components = 0.100007 Jy ! Clean residual min=-0.004635 max=0.010892 Jy/beam ! Clean residual mean=0.000004 rms=0.001055 Jy/beam ! Combined flux in latest and established models = 0.100007 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 0.100007 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=0.093844Jy sigma=0.694620 ! Fit after self-cal, rms=0.093234Jy sigma=0.691871 ! Inverting map ! Your choice of large map pixels excluded 8.62% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Added new window around map position (-0.6, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0127694 Jy ! Component: 100 - total flux cleaned = 0.0197837 Jy ! Total flux subtracted in 100 components = 0.0197837 Jy ! Clean residual min=-0.003860 max=0.005983 Jy/beam ! Clean residual mean=0.000002 rms=0.000837 Jy/beam ! Combined flux in latest and established models = 0.11979 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 8 components and 0.11979 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=0.091198Jy sigma=0.666686 ! Fit after self-cal, rms=0.091090Jy sigma=0.666101 ! Inverting map ! Your choice of large map pixels excluded 8.62% of the data. ! The x-axis pixel size should ideally be below 0.1645 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 8.62% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Estimated beam: bmin=0.664 mas, bmaj=1.126 mas, bpa=-0.447 degrees ! Estimated noise=0.464235 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 = 0.0060501 Jy ! Component: 100 - total flux cleaned = 0.00855907 Jy ! Component: 150 - total flux cleaned = 0.00949318 Jy ! Component: 200 - total flux cleaned = 0.00961642 Jy ! Total flux subtracted in 200 components = 0.00961642 Jy ! Clean residual min=-0.002255 max=0.002404 Jy/beam ! Clean residual mean=0.000000 rms=0.000501 Jy/beam ! Combined flux in latest and established models = 0.129407 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 14 components and 0.129407 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=0.090773Jy sigma=0.662517 ! Fit after self-cal, rms=0.090718Jy sigma=0.662235 ! Inverting map ! Your choice of large map pixels excluded 8.62% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.664 x 1.126 at -0.447 degrees (North through East) ! Clean map min=-0.0019814 max=0.10099 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 66 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 EF 1.00* FD 0.93 HH 1.19 ! KP 0.93 LA 1.02 MC 0.87 NL 0.93 ! OV 0.96 PT 0.97 SC 0.98 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.96 FD 1.02 KP 1.01 LA 1.04 ! MK 0.95 OV 0.99 PT 0.98 ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 0.88 MC 0.99 ON 0.92 ! ZC 0.83 ! ! Telescope amplitude corrections in sub-array 5: ! 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* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.93 EF 1.00* FD 0.96 KP 1.01 ! LA 1.08 MC 0.90 MK 1.08 NL 0.98 ! ON 0.90 PT 0.94 SC 1.00 ! ! ! Correcting IF 2. ! A total of 66 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 EF 1.00* FD 1.02 HH 1.14 ! KP 1.01 LA 1.09 MC 0.86 NL 0.97 ! OV 0.97 PT 1.02 SC 1.02 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 FD 1.02 KP 0.99 LA 1.07 ! MK 1.02 OV 0.99 PT 1.01 ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! 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* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.98 EF 1.00* FD 0.99 KP 1.02 ! LA 1.07 MC 0.96 MK 1.07 NL 0.97 ! ON 0.92 PT 1.01 SC 1.03 ! ! ! Correcting IF 3. ! A total of 66 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 EF 1.00* FD 0.94 HH 1.01 ! KP 0.96 LA 0.99 MC 0.86 NL 0.97 ! OV 1.03 PT 1.00 SC 0.97 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 FD 1.01 KP 0.93 LA 1.01 ! MK 0.97 OV 1.00 PT 1.00 ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! 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* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.01 EF 1.00* FD 0.97 KP 0.99 ! LA 0.93 MC 0.96 MK 1.08 NL 1.00 ! ON 0.97 PT 0.98 SC 1.08 ! ! ! Correcting IF 4. ! A total of 66 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.93 EF 1.00* FD 1.00 HH 1.12 ! KP 0.92 LA 1.04 MC 0.95 NL 0.99 ! OV 0.96 PT 1.04 SC 1.05 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 1.06 KP 0.98 LA 1.05 ! MK 0.90 OV 0.99 PT 1.06 ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! 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* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.94 EF 1.00* FD 0.99 KP 1.01 ! LA 1.01 MC 1.03 MK 1.14 NL 0.95 ! ON 0.95 PT 1.02 SC 1.04 ! ! ! Correcting IF 5. ! A total of 66 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.03 HH 1.12 ! KP 0.91 LA 0.96 MC 1.11 NL 1.00 ! OV 1.02 PT 0.97 SC 1.03 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.05 KP 0.86 LA 1.06 ! MK 1.00 OV 1.06 PT 0.95 ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! 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* ! ! Telescope amplitude corrections in sub-array 6: ! 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* PT 1.00* SC 1.00* ! ! ! Correcting IF 6. ! A total of 66 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 0.98 HH 1.10 ! KP 0.88 LA 1.01 MC 1.10 NL 1.01 ! OV 1.02 PT 0.93 SC 0.95 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.04 KP 0.87 LA 1.06 ! MK 1.01 OV 1.04 PT 0.93 ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! 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* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.04 KP 0.90 ! LA 1.00 MC 1.13 MK 1.07 NL 0.93 ! ON 1.12 PT 0.91 SC 1.00 ! ! ! Correcting IF 7. ! A total of 66 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! 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* ! KP 1.00* LA 1.00* MC 1.00* NL 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.06 FD 1.07 KP 0.89 LA 1.09 ! MK 1.06 OV 1.00 PT 0.98 ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! 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* ! ! Telescope amplitude corrections in sub-array 6: ! 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* PT 1.00* SC 1.00* ! ! ! Correcting IF 8. ! A total of 66 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 EF 1.00* FD 1.03 HH 1.06 ! KP 0.89 LA 1.06 MC 1.11 NL 1.04 ! OV 1.00 PT 0.96 SC 1.11 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.08 KP 0.85 LA 1.09 ! MK 1.07 OV 1.01 PT 1.09 ! ! A total of 21 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! 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* ! ! Telescope amplitude corrections in sub-array 6: ! 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* PT 1.00* SC 1.00* ! ! ! Fit before self-cal, rms=0.090718Jy sigma=0.662235 ! Fit after self-cal, rms=0.090198Jy sigma=0.661406 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 8.79% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Estimated beam: bmin=0.6594 mas, bmaj=1.182 mas, bpa=-1.204 degrees ! Estimated noise=0.461826 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 = -0.000392662 Jy ! Component: 100 - total flux cleaned = -0.000555003 Jy ! Component: 150 - total flux cleaned = -0.000694927 Jy ! Component: 200 - total flux cleaned = -0.000790323 Jy ! Total flux subtracted in 200 components = -0.000790323 Jy ! Clean residual min=-0.001988 max=0.001983 Jy/beam ! Clean residual mean=-0.000001 rms=0.000422 Jy/beam ! Combined flux in latest and established models = 0.128616 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 23 components and 0.128616 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=0.090161Jy sigma=0.661150 ! Fit after self-cal, rms=0.090182Jy sigma=0.661055 ! Inverting map ! Your choice of large map pixels excluded 8.79% of the data. ! The x-axis pixel size should ideally be below 0.1645 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=0.090182Jy sigma=0.661055 ! Fit after self-cal, rms=0.090004Jy sigma=0.661033 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 8.79% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Estimated beam: bmin=0.6596 mas, bmaj=1.183 mas, bpa=-1.258 degrees ! Estimated noise=0.460255 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000311695 Jy ! Component: 100 - total flux cleaned = -0.000450473 Jy ! Component: 150 - total flux cleaned = -0.000545954 Jy ! Component: 200 - total flux cleaned = -0.00060416 Jy ! Total flux subtracted in 200 components = -0.00060416 Jy ! Clean residual min=-0.001984 max=0.001984 Jy/beam ! Clean residual mean=-0.000001 rms=0.000417 Jy/beam ! Combined flux in latest and established models = 0.128012 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 23 components and 0.128012 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=0.089978Jy sigma=0.660864 ! Fit after self-cal, rms=0.089973Jy sigma=0.660847 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 8.79% of the data. ! The x-axis pixel size should ideally be below 0.1645 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 (-9.2, -1). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00179906 Jy ! Component: 100 - total flux cleaned = 0.00259566 Jy ! Component: 150 - total flux cleaned = 0.00262551 Jy ! Component: 200 - total flux cleaned = 0.00262532 Jy ! Total flux subtracted in 200 components = 0.00262532 Jy ! Clean residual min=-0.001867 max=0.001683 Jy/beam ! Clean residual mean=-0.000002 rms=0.000399 Jy/beam ! Combined flux in latest and established models = 0.130638 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 37 components and 0.130638 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=0.089927Jy sigma=0.660495 ! Fit after self-cal, rms=0.089921Jy sigma=0.660458 ! Inverting map ! Your choice of large map pixels excluded 8.79% of the data. ! The x-axis pixel size should ideally be below 0.1645 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=0.089921Jy sigma=0.660458 ! Fit after self-cal, rms=0.090094Jy sigma=0.659983 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 8.79% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Estimated beam: bmin=0.6594 mas, bmaj=1.182 mas, bpa=-1.262 degrees ! Estimated noise=0.459773 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000535255 Jy ! Component: 100 - total flux cleaned = 0.000591404 Jy ! Component: 150 - total flux cleaned = 0.000642109 Jy ! Component: 200 - total flux cleaned = 0.000641532 Jy ! Total flux subtracted in 200 components = 0.000641532 Jy ! Clean residual min=-0.001782 max=0.001514 Jy/beam ! Clean residual mean=0.000000 rms=0.000377 Jy/beam ! Combined flux in latest and established models = 0.131279 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 40 components and 0.131279 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=0.090073Jy sigma=0.659872 ! Fit after self-cal, rms=0.090085Jy sigma=0.659841 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 8.79% of the data. ! The x-axis pixel size should ideally be below 0.1645 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 = 0.000142627 Jy ! Component: 100 - total flux cleaned = 0.000117192 Jy ! Component: 150 - total flux cleaned = 9.4515e-05 Jy ! Component: 200 - total flux cleaned = 0.000117217 Jy ! Total flux subtracted in 200 components = 0.000117217 Jy ! Clean residual min=-0.001798 max=0.001536 Jy/beam ! Clean residual mean=0.000000 rms=0.000376 Jy/beam ! Combined flux in latest and established models = 0.131396 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 41 components and 0.131396 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=0.090068Jy sigma=0.659760 ! Fit after self-cal, rms=0.090066Jy sigma=0.659754 ! Inverting map ! Your choice of large map pixels excluded 8.79% of the data. ! The x-axis pixel size should ideally be below 0.1645 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=0.090066Jy sigma=0.659754 ! Fit after self-cal, rms=0.089977Jy sigma=0.659501 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 8.79% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Estimated beam: bmin=2.771 mas, bmaj=3.034 mas, bpa=-36.26 degrees ! Estimated noise=0.572966 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00011841 Jy ! Component: 100 - total flux cleaned = -8.24688e-06 Jy ! Component: 150 - total flux cleaned = 6.66657e-05 Jy ! Component: 200 - total flux cleaned = 0.00010611 Jy ! Total flux subtracted in 200 components = 0.00010611 Jy ! Clean residual min=-0.001738 max=0.001685 Jy/beam ! Clean residual mean=0.000001 rms=0.000476 Jy/beam ! Combined flux in latest and established models = 0.131502 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 50 components and 0.131502 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=0.089973Jy sigma=0.659472 ! Fit after self-cal, rms=0.089982Jy sigma=0.659436 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 8.79% of the data. ! The x-axis pixel size should ideally be below 0.1645 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 = 2.63987e-05 Jy ! Component: 100 - total flux cleaned = 5.70877e-05 Jy ! Component: 150 - total flux cleaned = 0.000108269 Jy ! Component: 200 - total flux cleaned = 0.000119421 Jy ! Total flux subtracted in 200 components = 0.000119421 Jy ! Clean residual min=-0.001727 max=0.001692 Jy/beam ! Clean residual mean=0.000001 rms=0.000475 Jy/beam ! Combined flux in latest and established models = 0.131622 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 52 components and 0.131622 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=0.089981Jy sigma=0.659431 ! Fit after self-cal, rms=0.089982Jy sigma=0.659419 ! Inverting map ! Your choice of large map pixels excluded 8.79% of the data. ! The x-axis pixel size should ideally be below 0.1645 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 8.79% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Estimated beam: bmin=0.6596 mas, bmaj=1.181 mas, bpa=-1.245 degrees ! Estimated noise=0.459434 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6596 x 1.181 at -1.245 degrees (North through East) ! Clean map min=-0.001379 max=0.098894 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 8.79% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Estimated beam: bmin=0.5028 mas, bmaj=0.9517 mas, bpa=-1.94 degrees ! Estimated noise=1.01402 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0745408 Jy ! Component: 100 - total flux cleaned = 0.0995776 Jy ! Component: 150 - total flux cleaned = 0.112277 Jy ! Component: 200 - total flux cleaned = 0.119526 Jy ! Total flux subtracted in 200 components = 0.119526 Jy ! Clean residual min=-0.003286 max=0.003662 Jy/beam ! Clean residual mean=0.000003 rms=0.000767 Jy/beam ! Combined flux in latest and established models = 0.119526 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 8 model components to the UV plane model. ! The established model now contains 8 components and 0.119526 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 8.79% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Estimated beam: bmin=0.6596 mas, bmaj=1.181 mas, bpa=-1.245 degrees ! Estimated noise=0.459434 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 = 0.00522403 Jy ! Component: 100 - total flux cleaned = 0.00803183 Jy ! Component: 150 - total flux cleaned = 0.00991562 Jy ! Component: 200 - total flux cleaned = 0.0109831 Jy ! Total flux subtracted in 200 components = 0.0109831 Jy ! Clean residual min=-0.001750 max=0.001649 Jy/beam ! Clean residual mean=0.000001 rms=0.000375 Jy/beam ! Combined flux in latest and established models = 0.130509 Jy ! Adding 18 model components to the UV plane model. ! The established model now contains 20 components and 0.130509 Jy ! Inverting map ! Your choice of large map pixels excluded 8.79% of the data. ! The x-axis pixel size should ideally be below 0.1645 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 8.79% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Estimated beam: bmin=2.771 mas, bmaj=3.034 mas, bpa=-36.26 degrees ! Estimated noise=0.572966 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000726039 Jy ! Component: 100 - total flux cleaned = 0.00103107 Jy ! Component: 150 - total flux cleaned = 0.00110062 Jy ! Component: 200 - total flux cleaned = 0.00111012 Jy ! Total flux subtracted in 200 components = 0.00111012 Jy ! Clean residual min=-0.001707 max=0.001731 Jy/beam ! Clean residual mean=0.000001 rms=0.000473 Jy/beam ! Combined flux in latest and established models = 0.13162 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 = 8.49432e-06 Jy ! Component: 100 - total flux cleaned = 2.41697e-05 Jy ! Component: 150 - total flux cleaned = 2.43908e-05 Jy ! Component: 200 - total flux cleaned = 2.41566e-05 Jy ! Total flux subtracted in 200 components = 2.41566e-05 Jy ! Clean residual min=-0.001714 max=0.001734 Jy/beam ! Clean residual mean=0.000001 rms=0.000472 Jy/beam ! Combined flux in latest and established models = 0.131644 Jy ! Adding 18 model components to the UV plane model. ! The established model now contains 36 components and 0.131644 Jy ! Inverting map ! Your choice of large map pixels excluded 8.79% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 8.79% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Estimated beam: bmin=0.6596 mas, bmaj=1.181 mas, bpa=-1.245 degrees ! Estimated noise=0.459434 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000148692 Jy ! Component: 100 - total flux cleaned = -0.000185427 Jy ! Component: 150 - total flux cleaned = -0.000184765 Jy ! Component: 200 - total flux cleaned = -0.000184968 Jy ! Total flux subtracted in 200 components = -0.000184968 Jy ! Clean residual min=-0.001686 max=0.001579 Jy/beam ! Clean residual mean=0.000001 rms=0.000368 Jy/beam ! Combined flux in latest and established models = 0.131459 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 43 components and 0.131459 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=0.090054Jy sigma=0.659762 ! Fit after self-cal, rms=0.090031Jy sigma=0.659656 wmodel /scr/pima/gb073_uvs/J1520+1601_X_map.mod ! Writing 43 model components to file: /scr/pima/gb073_uvs/J1520+1601_X_map.mod wobs /scr/pima/gb073_uvs/J1520+1601_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1520+1601_X_uvs.fits wwins /scr/pima/gb073_uvs/J1520+1601_X_map.win ! wwins: Wrote 3 windows to /scr/pima/gb073_uvs/J1520+1601_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 8.79% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000600654 Jy ! Component: 100 - total flux cleaned = -0.000889888 Jy ! Component: 150 - total flux cleaned = -0.00111194 Jy ! Component: 200 - total flux cleaned = -0.00127215 Jy ! Component: 250 - total flux cleaned = -0.0014289 Jy ! Component: 300 - total flux cleaned = -0.00160807 Jy ! Component: 350 - total flux cleaned = -0.00178385 Jy ! Component: 400 - total flux cleaned = -0.00188202 Jy ! Component: 450 - total flux cleaned = -0.00195466 Jy ! Component: 500 - total flux cleaned = -0.00202606 Jy ! Component: 550 - total flux cleaned = -0.00211949 Jy ! Component: 600 - total flux cleaned = -0.00214244 Jy ! Component: 650 - total flux cleaned = -0.002188 Jy ! Component: 700 - total flux cleaned = -0.00229967 Jy ! Component: 750 - total flux cleaned = -0.00225515 Jy ! Component: 800 - total flux cleaned = -0.00229903 Jy ! Component: 850 - total flux cleaned = -0.00240712 Jy ! Component: 900 - total flux cleaned = -0.00245019 Jy ! Component: 950 - total flux cleaned = -0.00261932 Jy ! Component: 1000 - total flux cleaned = -0.00268209 Jy ! Component: 1050 - total flux cleaned = -0.00270294 Jy ! Component: 1100 - total flux cleaned = -0.00282672 Jy ! Component: 1150 - total flux cleaned = -0.00284696 Jy ! Component: 1200 - total flux cleaned = -0.00292797 Jy ! Component: 1250 - total flux cleaned = -0.00300824 Jy ! Component: 1300 - total flux cleaned = -0.00310769 Jy ! Component: 1350 - total flux cleaned = -0.00320614 Jy ! Component: 1400 - total flux cleaned = -0.00330431 Jy ! Component: 1450 - total flux cleaned = -0.00342085 Jy ! Component: 1500 - total flux cleaned = -0.00349783 Jy ! Component: 1550 - total flux cleaned = -0.00361284 Jy ! Component: 1600 - total flux cleaned = -0.00380272 Jy ! Component: 1650 - total flux cleaned = -0.00384017 Jy ! Component: 1700 - total flux cleaned = -0.00389636 Jy ! Component: 1750 - total flux cleaned = -0.00395189 Jy ! Component: 1800 - total flux cleaned = -0.0040627 Jy ! Component: 1850 - total flux cleaned = -0.0041543 Jy ! Component: 1900 - total flux cleaned = -0.00426335 Jy ! Component: 1950 - total flux cleaned = -0.00438975 Jy ! Component: 2000 - total flux cleaned = -0.0042999 Jy ! Component: 2050 - total flux cleaned = -0.00438902 Jy ! Component: 2100 - total flux cleaned = -0.00438908 Jy ! Component: 2150 - total flux cleaned = -0.00454757 Jy ! Component: 2200 - total flux cleaned = -0.00463514 Jy ! Component: 2250 - total flux cleaned = -0.00463529 Jy ! Component: 2300 - total flux cleaned = -0.00475632 Jy ! Component: 2350 - total flux cleaned = -0.00479076 Jy ! Component: 2400 - total flux cleaned = -0.004859 Jy ! Component: 2450 - total flux cleaned = -0.00492687 Jy ! Component: 2500 - total flux cleaned = -0.00504517 Jy ! Component: 2550 - total flux cleaned = -0.00512909 Jy ! Component: 2600 - total flux cleaned = -0.00519563 Jy ! Component: 2650 - total flux cleaned = -0.00526211 Jy ! Component: 2700 - total flux cleaned = -0.00527853 Jy ! Component: 2750 - total flux cleaned = -0.00532769 Jy ! Component: 2800 - total flux cleaned = -0.00544202 Jy ! Component: 2850 - total flux cleaned = -0.00550696 Jy ! Component: 2900 - total flux cleaned = -0.00550711 Jy ! Component: 2950 - total flux cleaned = -0.00565158 Jy ! Component: 3000 - total flux cleaned = -0.00569951 Jy ! Component: 3050 - total flux cleaned = -0.00573131 Jy ! Component: 3100 - total flux cleaned = -0.00584176 Jy ! Component: 3150 - total flux cleaned = -0.00585743 Jy ! Component: 3200 - total flux cleaned = -0.00596677 Jy ! Component: 3250 - total flux cleaned = -0.0059823 Jy ! Component: 3300 - total flux cleaned = -0.00602874 Jy ! Component: 3350 - total flux cleaned = -0.00604419 Jy ! Component: 3400 - total flux cleaned = -0.00610548 Jy ! Component: 3450 - total flux cleaned = -0.00618168 Jy ! Component: 3500 - total flux cleaned = -0.00622705 Jy ! Component: 3550 - total flux cleaned = -0.00624203 Jy ! Component: 3600 - total flux cleaned = -0.00624217 Jy ! Component: 3650 - total flux cleaned = -0.00628708 Jy ! Component: 3700 - total flux cleaned = -0.00637631 Jy ! Component: 3750 - total flux cleaned = -0.00640588 Jy ! Component: 3800 - total flux cleaned = -0.00646482 Jy ! Component: 3850 - total flux cleaned = -0.00650891 Jy ! Component: 3900 - total flux cleaned = -0.00656738 Jy ! Component: 3950 - total flux cleaned = -0.00653827 Jy ! Component: 4000 - total flux cleaned = -0.00665411 Jy ! Component: 4050 - total flux cleaned = -0.00672617 Jy ! Total flux subtracted in 4096 components = -0.00675491 Jy ! Clean residual min=-0.000770 max=0.000910 Jy/beam ! Clean residual mean=0.000001 rms=0.000232 Jy/beam ! Combined flux in latest and established models = 0.124704 Jy keep ! Adding 316 model components to the UV plane model. ! The established model now contains 359 components and 0.124704 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1520+1601_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 8.79% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6596 x 1.181 at -1.245 degrees (North through East) ! Clean map min=-0.0013797 max=0.098353 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1520+1601_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0983535 invert ! Inverting map ! Your choice of large map pixels excluded 8.79% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000231345 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.705653 0.705653 1.41131 2.82261 5.64522 11.2904 22.5809 45.1618 90.3236 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0006 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.098 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 425.138 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1520+1601_X_uvs.log closed on Sat Dec 26 09:41:35 2015