! Started logfile: /scr/pima/gb073_uvs/J1132+1023_X_uvs.log on Sat Dec 26 09:37:08 2015 obs /scr/pima/gb073_uvs/J1132+1023_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1132+1023_X_uva.fits ! AN table 1: 19 integrations on 6 of 6 possible baselines. ! AN table 2: 18 integrations on 45 of 45 possible baselines. ! AN table 3: 118 integrations on 10 of 10 possible baselines. ! AN table 4: 18 integrations on 66 of 66 possible baselines. ! AN table 5: 22 integrations on 55 of 55 possible baselines. ! AN table 6: 10 integrations on 28 of 28 possible baselines. ! Apparent sampling: 0.767252 visibilities/baseline/integration-bin. ! Found source: J1132+1023 ! ! 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 29352 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/J1132+1023_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 40 telescope corrections were flagged in sub-array 1. ! A total of 23 telescope corrections were flagged in sub-array 2. ! A total of 164 telescope corrections were flagged in sub-array 3. ! A total of 40 telescope corrections were flagged in sub-array 4. ! A total of 30 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 40 telescope corrections were flagged in sub-array 1. ! A total of 23 telescope corrections were flagged in sub-array 2. ! A total of 164 telescope corrections were flagged in sub-array 3. ! A total of 40 telescope corrections were flagged in sub-array 4. ! A total of 30 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 40 telescope corrections were flagged in sub-array 1. ! A total of 23 telescope corrections were flagged in sub-array 2. ! A total of 164 telescope corrections were flagged in sub-array 3. ! A total of 40 telescope corrections were flagged in sub-array 4. ! A total of 30 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 40 telescope corrections were flagged in sub-array 1. ! A total of 23 telescope corrections were flagged in sub-array 2. ! A total of 164 telescope corrections were flagged in sub-array 3. ! A total of 40 telescope corrections were flagged in sub-array 4. ! A total of 30 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 5. ! A total of 40 telescope corrections were flagged in sub-array 1. ! A total of 39 telescope corrections were flagged in sub-array 2. ! A total of 164 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 52 telescope corrections were flagged in sub-array 5. ! A total of 10 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 6. ! A total of 40 telescope corrections were flagged in sub-array 1. ! A total of 39 telescope corrections were flagged in sub-array 2. ! A total of 164 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 52 telescope corrections were flagged in sub-array 5. ! A total of 10 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 7. ! A total of 40 telescope corrections were flagged in sub-array 1. ! A total of 23 telescope corrections were flagged in sub-array 2. ! A total of 164 telescope corrections were flagged in sub-array 3. ! A total of 40 telescope corrections were flagged in sub-array 4. ! A total of 30 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 8. ! A total of 40 telescope corrections were flagged in sub-array 1. ! A total of 23 telescope corrections were flagged in sub-array 2. ! A total of 164 telescope corrections were flagged in sub-array 3. ! A total of 40 telescope corrections were flagged in sub-array 4. ! A total of 30 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=1.023169Jy sigma=8.498973 ! Fit after self-cal, rms=0.836096Jy sigma=6.851922 ! 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 5.82% of the data. ! The x-axis pixel size should ideally be below 0.1653 milli-arcsec ! Estimated beam: bmin=0.5475 mas, bmaj=0.8653 mas, bpa=-5.901 degrees ! Estimated noise=1.10387 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 = 0.132403 Jy ! Component: 100 - total flux cleaned = 0.165199 Jy ! Total flux subtracted in 100 components = 0.165199 Jy ! Clean residual min=-0.006976 max=0.014004 Jy/beam ! Clean residual mean=-0.000003 rms=0.001379 Jy/beam ! Combined flux in latest and established models = 0.165199 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.165199 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=0.111582Jy sigma=0.711616 ! Fit after self-cal, rms=0.111548Jy sigma=0.711317 ! Inverting map ! Your choice of large map pixels excluded 5.82% of the data. ! The x-axis pixel size should ideally be below 0.1653 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0155844 Jy ! Component: 100 - total flux cleaned = 0.0239787 Jy ! Total flux subtracted in 100 components = 0.0239787 Jy ! Clean residual min=-0.006150 max=0.005912 Jy/beam ! Clean residual mean=-0.000000 rms=0.001145 Jy/beam ! Combined flux in latest and established models = 0.189178 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 12 components and 0.189178 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=0.109431Jy sigma=0.679588 ! Fit after self-cal, rms=0.109402Jy sigma=0.679316 ! Inverting map ! Your choice of large map pixels excluded 5.82% of the data. ! The x-axis pixel size should ideally be below 0.1653 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 5.82% of the data. ! The x-axis pixel size should ideally be below 0.1653 milli-arcsec ! Estimated beam: bmin=0.6682 mas, bmaj=0.9632 mas, bpa=-6.579 degrees ! Estimated noise=0.574208 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 = 0.00614209 Jy ! Component: 100 - total flux cleaned = 0.00882869 Jy ! Component: 150 - total flux cleaned = 0.00970466 Jy ! Component: 200 - total flux cleaned = 0.00982098 Jy ! Total flux subtracted in 200 components = 0.00982098 Jy ! Clean residual min=-0.004330 max=0.004296 Jy/beam ! Clean residual mean=0.000002 rms=0.000787 Jy/beam ! Combined flux in latest and established models = 0.198999 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 18 components and 0.198999 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=0.109176Jy sigma=0.676015 ! Fit after self-cal, rms=0.109176Jy sigma=0.675955 ! Inverting map ! Your choice of large map pixels excluded 5.82% of the data. ! The x-axis pixel size should ideally be below 0.1653 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6682 x 0.9632 at -6.579 degrees (North through East) ! Clean map min=-0.0035631 max=0.17491 Jy/beam if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 36 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 0.98 KP 0.97 LA 1.08 ! MC 0.93 MK 0.98 NL 0.93 OV 1.02 ! PT 0.94 SC 0.92 ! ! A total of 138 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 0.93 MC 0.98 ON 1.03 ! ZC 0.80 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 EF 1.00* FD 0.96 KP 0.96 ! LA 1.00 MC 0.96 NL 0.96 ON 1.02 ! OV 1.02 PT 0.97 SC 0.96 ZC 0.64 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.98 EF 1.00* FD 0.96 HH 1.16 ! KP 0.97 LA 1.03 MC 0.98 NL 0.96 ! ON 0.97 PT 1.00 SC 0.95 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.01 FD 0.97 KP 1.04 LA 1.05 ! MK 0.96 NL 0.96 PT 0.96 SC 0.90 ! ! ! Correcting IF 2. ! A total of 36 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 FD 1.03 KP 1.02 LA 1.05 ! MC 0.92 MK 1.03 NL 0.94 OV 1.06 ! PT 1.01 SC 1.10 ! ! A total of 138 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 1.00 MC 1.00 ON 0.91 ! ZC 0.86 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.03 EF 1.00* FD 0.97 KP 1.02 ! LA 1.03 MC 0.96 NL 1.00 ON 0.96 ! OV 1.00 PT 1.05 SC 0.95 ZC 0.64 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.97 EF 1.00* FD 1.01 HH 1.23 ! KP 0.99 LA 1.07 MC 0.92 NL 0.97 ! ON 0.96 PT 1.08 SC 0.99 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.04 FD 1.06 KP 1.03 LA 1.06 ! MK 1.01 NL 0.95 PT 1.01 SC 0.95 ! ! ! Correcting IF 3. ! A total of 36 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 FD 1.00 KP 0.97 LA 0.99 ! MC 0.88 MK 0.98 NL 0.94 OV 0.99 ! PT 0.98 SC 1.00 ! ! A total of 138 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 0.85 MC 1.10 ON 0.98 ! ZC 0.81 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 EF 1.00* FD 0.98 KP 0.92 ! LA 0.98 MC 0.91 NL 0.98 ON 0.99 ! OV 1.05 PT 1.02 SC 1.03 ZC 0.62 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.05 EF 1.00* FD 1.01 HH 1.20 ! KP 0.93 LA 0.96 MC 0.94 NL 0.96 ! ON 0.94 PT 1.02 SC 1.09 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.96 FD 0.98 KP 0.92 LA 1.01 ! MK 0.89 NL 0.93 PT 1.05 SC 1.03 ! ! ! Correcting IF 4. ! A total of 36 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 1.02 KP 0.98 LA 1.03 ! MC 0.94 MK 1.02 NL 0.95 OV 1.00 ! PT 1.00 SC 1.03 ! ! A total of 138 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 0.99 MC 1.06 ON 0.99 ! ZC 0.75 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 EF 1.00* FD 0.98 KP 0.97 ! LA 1.01 MC 0.99 NL 0.98 ON 0.96 ! OV 1.02 PT 1.04 SC 1.00 ZC 0.61 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.97 EF 1.00* FD 1.01 HH 1.07 ! KP 0.99 LA 1.00 MC 0.90 NL 1.00 ! ON 0.97 PT 1.04 SC 1.04 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.02 FD 1.00 KP 1.01 LA 0.98 ! MK 0.96 NL 0.95 PT 1.03 SC 0.98 ! ! ! Correcting IF 5. ! A total of 36 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.01 KP 0.89 LA 1.00 ! MC 1.23 MK 1.00 NL 0.98 OV 1.13 ! PT 0.94 SC 0.98 ! ! A total of 138 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 1.02 MC 1.30 ON 1.22 ! ZC 0.80 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.05 KP 0.89 ! LA 0.97 MC 1.22 NL 1.03 ON 1.18 ! OV 1.02 PT 1.00 SC 1.03 ZC 0.67 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.03 HH 1.18 ! KP 0.91 LA 0.97 MC 1.21 NL 0.99 ! ON 1.26 PT 1.03 SC 1.04 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* FD 1.03 KP 0.89 LA 0.99 ! MK 0.91 NL 1.00 PT 0.99 SC 0.98 ! ! ! Correcting IF 6. ! A total of 36 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.03 KP 0.87 LA 0.97 ! MC 1.17 MK 1.01 NL 1.00 OV 1.05 ! PT 0.94 SC 1.03 ! ! A total of 138 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 0.98 MC 1.25 ON 1.29 ! ZC 0.81 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.04 KP 0.83 ! LA 1.04 MC 1.14 NL 1.01 ON 1.24 ! OV 1.10 PT 0.97 SC 0.92 ZC 0.68 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.01 HH 1.13 ! KP 0.93 LA 1.01 MC 1.26 NL 0.98 ! ON 1.22 PT 0.95 SC 0.94 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* FD 1.04 KP 0.86 LA 0.99 ! MK 0.93 NL 0.97 PT 0.91 SC 0.98 ! ! ! Correcting IF 7. ! A total of 36 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 1.03 KP 0.86 LA 1.01 ! MC 1.33 MK 1.10 NL 1.07 OV 1.01 ! PT 1.00 SC 1.17 ! ! A total of 138 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 1.18 MC 1.35 ON 1.24 ! ZC 0.65 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 EF 1.00* FD 1.09 KP 0.91 ! LA 1.03 MC 1.22 NL 1.09 ON 1.34 ! OV 0.99 PT 1.01 SC 0.98 ZC 0.45 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 EF 1.00* FD 1.10 HH 1.34 ! KP 0.91 LA 1.06 MC 1.19 NL 1.05 ! ON 1.30 PT 1.02 SC 1.02 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.06 FD 1.07 KP 0.92 LA 1.02 ! MK 1.07 NL 1.08 PT 0.99 SC 1.03 ! ! ! Correcting IF 8. ! A total of 36 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.05 FD 1.01 KP 0.89 LA 1.04 ! MC 1.31 MK 1.06 NL 1.01 OV 1.02 ! PT 0.96 SC 1.01 ! ! A total of 138 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 1.14 MC 1.33 ON 1.27 ! ZC 0.70 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 EF 1.00* FD 1.03 KP 0.89 ! LA 1.03 MC 1.48 NL 1.08 ON 1.24 ! OV 1.00 PT 1.01 SC 1.03 ZC 0.42 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 EF 1.00* FD 1.03 HH 1.50 ! KP 0.88 LA 1.05 MC 1.47 NL 1.03 ! ON 1.26 PT 1.06 SC 1.05 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.10 FD 1.03 KP 0.92 LA 1.00 ! MK 1.03 NL 1.01 PT 1.01 SC 1.05 ! ! ! Fit before self-cal, rms=0.109176Jy sigma=0.675955 ! Fit after self-cal, rms=0.112047Jy sigma=0.655194 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 6.16% of the data. ! The x-axis pixel size should ideally be below 0.1653 milli-arcsec ! Estimated beam: bmin=0.6732 mas, bmaj=1.09 mas, bpa=-7.126 degrees ! Estimated noise=0.581717 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 = -0.00099511 Jy ! Component: 100 - total flux cleaned = -0.00116943 Jy ! Component: 150 - total flux cleaned = -0.00129996 Jy ! Component: 200 - total flux cleaned = -0.00132929 Jy ! Total flux subtracted in 200 components = -0.00132929 Jy ! Clean residual min=-0.002011 max=0.002307 Jy/beam ! Clean residual mean=-0.000001 rms=0.000418 Jy/beam ! Combined flux in latest and established models = 0.19767 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 21 components and 0.197669 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=0.112007Jy sigma=0.654980 ! Fit after self-cal, rms=0.112532Jy sigma=0.654273 ! Inverting map ! Your choice of large map pixels excluded 6.16% of the data. ! The x-axis pixel size should ideally be below 0.1653 milli-arcsec ! Added new window around map position (2, -2.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00214154 Jy ! Component: 100 - total flux cleaned = 0.00224944 Jy ! Component: 150 - total flux cleaned = 0.00221466 Jy ! Component: 200 - total flux cleaned = 0.00221362 Jy ! Total flux subtracted in 200 components = 0.00221362 Jy ! Clean residual min=-0.001823 max=0.001731 Jy/beam ! Clean residual mean=-0.000001 rms=0.000401 Jy/beam ! Combined flux in latest and established models = 0.199883 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 36 components and 0.199883 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=0.112473Jy sigma=0.653933 ! Fit after self-cal, rms=0.112467Jy sigma=0.653847 ! Inverting map ! Your choice of large map pixels excluded 6.16% of the data. ! The x-axis pixel size should ideally be below 0.1653 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=0.112467Jy sigma=0.653847 ! Fit after self-cal, rms=0.118482Jy sigma=0.651783 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.16% of the data. ! The x-axis pixel size should ideally be below 0.1653 milli-arcsec ! Estimated beam: bmin=0.6767 mas, bmaj=1.098 mas, bpa=-6.997 degrees ! Estimated noise=0.58365 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000173277 Jy ! Component: 100 - total flux cleaned = 0.000289278 Jy ! Component: 150 - total flux cleaned = 0.000320975 Jy ! Component: 200 - total flux cleaned = 0.000321252 Jy ! Total flux subtracted in 200 components = 0.000321252 Jy ! Clean residual min=-0.001694 max=0.001526 Jy/beam ! Clean residual mean=-0.000001 rms=0.000364 Jy/beam ! Combined flux in latest and established models = 0.200204 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 39 components and 0.200204 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=0.118453Jy sigma=0.651616 ! Fit after self-cal, rms=0.118735Jy sigma=0.651504 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.16% of the data. ! The x-axis pixel size should ideally be below 0.1653 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 = 0.000244825 Jy ! Component: 100 - total flux cleaned = 0.000245117 Jy ! Component: 150 - total flux cleaned = 0.000246194 Jy ! Component: 200 - total flux cleaned = 0.000246369 Jy ! Total flux subtracted in 200 components = 0.000246369 Jy ! Clean residual min=-0.001671 max=0.001542 Jy/beam ! Clean residual mean=-0.000001 rms=0.000363 Jy/beam ! Combined flux in latest and established models = 0.200451 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 41 components and 0.200451 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=0.118724Jy sigma=0.651475 ! Fit after self-cal, rms=0.118720Jy sigma=0.651469 ! Inverting map ! Your choice of large map pixels excluded 6.16% of the data. ! The x-axis pixel size should ideally be below 0.1653 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=0.118720Jy sigma=0.651469 ! Fit after self-cal, rms=0.122200Jy sigma=0.650817 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.16% of the data. ! The x-axis pixel size should ideally be below 0.1653 milli-arcsec ! Estimated beam: bmin=0.6795 mas, bmaj=1.1 mas, bpa=-6.964 degrees ! Estimated noise=0.584726 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -5.53394e-05 Jy ! Component: 100 - total flux cleaned = -2.68994e-05 Jy ! Component: 150 - total flux cleaned = -2.4657e-06 Jy ! Component: 200 - total flux cleaned = 1.88708e-05 Jy ! Total flux subtracted in 200 components = 1.88708e-05 Jy ! Clean residual min=-0.001600 max=0.001511 Jy/beam ! Clean residual mean=-0.000001 rms=0.000355 Jy/beam ! Combined flux in latest and established models = 0.20047 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 42 components and 0.20047 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=0.122188Jy sigma=0.650759 ! Fit after self-cal, rms=0.122317Jy sigma=0.650724 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.16% of the data. ! The x-axis pixel size should ideally be below 0.1653 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 = 9.80635e-05 Jy ! Component: 100 - total flux cleaned = 0.000117328 Jy ! Component: 150 - total flux cleaned = 0.000100326 Jy ! Component: 200 - total flux cleaned = 6.93682e-05 Jy ! Total flux subtracted in 200 components = 6.93682e-05 Jy ! Clean residual min=-0.001595 max=0.001524 Jy/beam ! Clean residual mean=-0.000001 rms=0.000355 Jy/beam ! Combined flux in latest and established models = 0.200539 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 43 components and 0.200539 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=0.122312Jy sigma=0.650706 ! Fit after self-cal, rms=0.122310Jy sigma=0.650702 ! Inverting map ! Your choice of large map pixels excluded 6.16% of the data. ! The x-axis pixel size should ideally be below 0.1653 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=0.122310Jy sigma=0.650702 ! Fit after self-cal, rms=0.124414Jy sigma=0.650655 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.16% of the data. ! The x-axis pixel size should ideally be below 0.1653 milli-arcsec ! Estimated beam: bmin=2.528 mas, bmaj=3.081 mas, bpa=-6.332 degrees ! Estimated noise=0.718297 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0002618 Jy ! Component: 100 - total flux cleaned = 0.000237342 Jy ! Component: 150 - total flux cleaned = 0.000228034 Jy ! Component: 200 - total flux cleaned = 0.000212754 Jy ! Total flux subtracted in 200 components = 0.000212754 Jy ! Clean residual min=-0.001508 max=0.001503 Jy/beam ! Clean residual mean=-0.000002 rms=0.000408 Jy/beam ! Combined flux in latest and established models = 0.200752 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 54 components and 0.200752 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=0.124410Jy sigma=0.650653 ! Fit after self-cal, rms=0.124469Jy sigma=0.650646 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.16% of the data. ! The x-axis pixel size should ideally be below 0.1653 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 6.82451e-05 Jy ! Component: 100 - total flux cleaned = 6.78024e-05 Jy ! Component: 150 - total flux cleaned = 6.71472e-05 Jy ! Component: 200 - total flux cleaned = 6.66157e-05 Jy ! Total flux subtracted in 200 components = 6.66157e-05 Jy ! Clean residual min=-0.001485 max=0.001510 Jy/beam ! Clean residual mean=-0.000002 rms=0.000409 Jy/beam ! Combined flux in latest and established models = 0.200818 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 54 components and 0.200818 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=0.124469Jy sigma=0.650646 ! Fit after self-cal, rms=0.124465Jy sigma=0.650643 ! Inverting map ! Your choice of large map pixels excluded 6.16% of the data. ! The x-axis pixel size should ideally be below 0.1653 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 6.16% of the data. ! The x-axis pixel size should ideally be below 0.1653 milli-arcsec ! Estimated beam: bmin=0.6816 mas, bmaj=1.103 mas, bpa=-6.948 degrees ! Estimated noise=0.585835 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6816 x 1.103 at -6.948 degrees (North through East) ! Clean map min=-0.001238 max=0.1767 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 6.16% of the data. ! The x-axis pixel size should ideally be below 0.1653 milli-arcsec ! Estimated beam: bmin=0.5574 mas, bmaj=0.9207 mas, bpa=-6.956 degrees ! Estimated noise=1.1513 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.134772 Jy ! Component: 100 - total flux cleaned = 0.166486 Jy ! Component: 150 - total flux cleaned = 0.17979 Jy ! Component: 200 - total flux cleaned = 0.186783 Jy ! Total flux subtracted in 200 components = 0.186783 Jy ! Clean residual min=-0.003340 max=0.003779 Jy/beam ! Clean residual mean=-0.000002 rms=0.000799 Jy/beam ! Combined flux in latest and established models = 0.186783 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 12 model components to the UV plane model. ! The established model now contains 12 components and 0.186783 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 6.16% of the data. ! The x-axis pixel size should ideally be below 0.1653 milli-arcsec ! Estimated beam: bmin=0.6816 mas, bmaj=1.103 mas, bpa=-6.948 degrees ! Estimated noise=0.585835 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) ! Added new window around map position (0.6, -0.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00633633 Jy ! Component: 100 - total flux cleaned = 0.00978441 Jy ! Component: 150 - total flux cleaned = 0.0118128 Jy ! Component: 200 - total flux cleaned = 0.0130601 Jy ! Total flux subtracted in 200 components = 0.0130601 Jy ! Clean residual min=-0.001619 max=0.001454 Jy/beam ! Clean residual mean=-0.000001 rms=0.000355 Jy/beam ! Combined flux in latest and established models = 0.199844 Jy ! Adding 20 model components to the UV plane model. ! The established model now contains 28 components and 0.199844 Jy ! Inverting map ! Your choice of large map pixels excluded 6.16% of the data. ! The x-axis pixel size should ideally be below 0.1653 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 6.16% of the data. ! The x-axis pixel size should ideally be below 0.1653 milli-arcsec ! Estimated beam: bmin=2.528 mas, bmaj=3.081 mas, bpa=-6.332 degrees ! Estimated noise=0.718297 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000794702 Jy ! Component: 100 - total flux cleaned = 0.000883807 Jy ! Component: 150 - total flux cleaned = 0.000901443 Jy ! Component: 200 - total flux cleaned = 0.000902676 Jy ! Total flux subtracted in 200 components = 0.000902676 Jy ! Clean residual min=-0.001472 max=0.001488 Jy/beam ! Clean residual mean=-0.000002 rms=0.000409 Jy/beam ! Combined flux in latest and established models = 0.200746 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 = -2.35002e-05 Jy ! Component: 100 - total flux cleaned = -4.38938e-05 Jy ! Component: 150 - total flux cleaned = -6.21417e-05 Jy ! Component: 200 - total flux cleaned = -7.06828e-05 Jy ! Total flux subtracted in 200 components = -7.06828e-05 Jy ! Clean residual min=-0.001475 max=0.001496 Jy/beam ! Clean residual mean=-0.000002 rms=0.000409 Jy/beam ! Combined flux in latest and established models = 0.200676 Jy ! Adding 22 model components to the UV plane model. ! The established model now contains 43 components and 0.200676 Jy ! Inverting map ! Your choice of large map pixels excluded 6.16% of the data. ! The x-axis pixel size should ideally be below 0.1653 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 6.16% of the data. ! The x-axis pixel size should ideally be below 0.1653 milli-arcsec ! Estimated beam: bmin=0.6816 mas, bmaj=1.103 mas, bpa=-6.948 degrees ! Estimated noise=0.585835 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000281323 Jy ! Component: 100 - total flux cleaned = -0.000281179 Jy ! Component: 150 - total flux cleaned = -0.000262049 Jy ! Component: 200 - total flux cleaned = -0.0002447 Jy ! Total flux subtracted in 200 components = -0.0002447 Jy ! Clean residual min=-0.001543 max=0.001480 Jy/beam ! Clean residual mean=-0.000001 rms=0.000350 Jy/beam ! Combined flux in latest and established models = 0.200431 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 57 components and 0.200431 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=0.124474Jy sigma=0.650763 ! Fit after self-cal, rms=0.124441Jy sigma=0.650726 wmodel /scr/pima/gb073_uvs/J1132+1023_X_map.mod ! Writing 57 model components to file: /scr/pima/gb073_uvs/J1132+1023_X_map.mod wobs /scr/pima/gb073_uvs/J1132+1023_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1132+1023_X_uvs.fits wwins /scr/pima/gb073_uvs/J1132+1023_X_map.win ! wwins: Wrote 3 windows to /scr/pima/gb073_uvs/J1132+1023_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 6.16% of the data. ! The x-axis pixel size should ideally be below 0.1653 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000229709 Jy ! Component: 100 - total flux cleaned = -0.000419159 Jy ! Component: 150 - total flux cleaned = -0.000550062 Jy ! Component: 200 - total flux cleaned = -0.000626769 Jy ! Component: 250 - total flux cleaned = -0.000726115 Jy ! Component: 300 - total flux cleaned = -0.000702442 Jy ! Component: 350 - total flux cleaned = -0.000798202 Jy ! Component: 400 - total flux cleaned = -0.000915032 Jy ! Component: 450 - total flux cleaned = -0.000984053 Jy ! Component: 500 - total flux cleaned = -0.00109734 Jy ! Component: 550 - total flux cleaned = -0.00125415 Jy ! Component: 600 - total flux cleaned = -0.00134255 Jy ! Component: 650 - total flux cleaned = -0.00140794 Jy ! Component: 700 - total flux cleaned = -0.00151651 Jy ! Component: 750 - total flux cleaned = -0.00162347 Jy ! Component: 800 - total flux cleaned = -0.00168694 Jy ! Component: 850 - total flux cleaned = -0.00177125 Jy ! Component: 900 - total flux cleaned = -0.00177136 Jy ! Component: 950 - total flux cleaned = -0.0019784 Jy ! Component: 1000 - total flux cleaned = -0.001999 Jy ! Component: 1050 - total flux cleaned = -0.00206011 Jy ! Component: 1100 - total flux cleaned = -0.00206 Jy ! Component: 1150 - total flux cleaned = -0.00220053 Jy ! Component: 1200 - total flux cleaned = -0.00212065 Jy ! Component: 1250 - total flux cleaned = -0.00221965 Jy ! Component: 1300 - total flux cleaned = -0.00221972 Jy ! Component: 1350 - total flux cleaned = -0.00229783 Jy ! Component: 1400 - total flux cleaned = -0.00235605 Jy ! Component: 1450 - total flux cleaned = -0.00237527 Jy ! Component: 1500 - total flux cleaned = -0.00245227 Jy ! Component: 1550 - total flux cleaned = -0.00247142 Jy ! Component: 1600 - total flux cleaned = -0.00256643 Jy ! Component: 1650 - total flux cleaned = -0.00267936 Jy ! Component: 1700 - total flux cleaned = -0.00271677 Jy ! Component: 1750 - total flux cleaned = -0.00279123 Jy ! Component: 1800 - total flux cleaned = -0.00284688 Jy ! Component: 1850 - total flux cleaned = -0.00288386 Jy ! Component: 1900 - total flux cleaned = -0.00295689 Jy ! Component: 1950 - total flux cleaned = -0.00297513 Jy ! Component: 2000 - total flux cleaned = -0.00304764 Jy ! Component: 2050 - total flux cleaned = -0.00308364 Jy ! Component: 2100 - total flux cleaned = -0.00317335 Jy ! Component: 2150 - total flux cleaned = -0.00311979 Jy ! Component: 2200 - total flux cleaned = -0.00313745 Jy ! Component: 2250 - total flux cleaned = -0.0031553 Jy ! Component: 2300 - total flux cleaned = -0.00324325 Jy ! Component: 2350 - total flux cleaned = -0.00329579 Jy ! Component: 2400 - total flux cleaned = -0.00327843 Jy ! Component: 2450 - total flux cleaned = -0.00327846 Jy ! Component: 2500 - total flux cleaned = -0.00329564 Jy ! Component: 2550 - total flux cleaned = -0.00327845 Jy ! Component: 2600 - total flux cleaned = -0.00332966 Jy ! Component: 2650 - total flux cleaned = -0.00336374 Jy ! Component: 2700 - total flux cleaned = -0.00336366 Jy ! Component: 2750 - total flux cleaned = -0.00333007 Jy ! Component: 2800 - total flux cleaned = -0.0033468 Jy ! Component: 2850 - total flux cleaned = -0.00339688 Jy ! Component: 2900 - total flux cleaned = -0.00339694 Jy ! Component: 2950 - total flux cleaned = -0.00339702 Jy ! Component: 3000 - total flux cleaned = -0.00341353 Jy ! Component: 3050 - total flux cleaned = -0.00338065 Jy ! Component: 3100 - total flux cleaned = -0.00334796 Jy ! Component: 3150 - total flux cleaned = -0.00347831 Jy ! Component: 3200 - total flux cleaned = -0.00342951 Jy ! Component: 3250 - total flux cleaned = -0.00341333 Jy ! Component: 3300 - total flux cleaned = -0.00346167 Jy ! Component: 3350 - total flux cleaned = -0.00342957 Jy ! Component: 3400 - total flux cleaned = -0.00334962 Jy ! Component: 3450 - total flux cleaned = -0.00341318 Jy ! Component: 3500 - total flux cleaned = -0.00334976 Jy ! Component: 3550 - total flux cleaned = -0.0033972 Jy ! Component: 3600 - total flux cleaned = -0.00338148 Jy ! Component: 3650 - total flux cleaned = -0.00331876 Jy ! Component: 3700 - total flux cleaned = -0.00334994 Jy ! Component: 3750 - total flux cleaned = -0.00335002 Jy ! Component: 3800 - total flux cleaned = -0.00336537 Jy ! Component: 3850 - total flux cleaned = -0.00331908 Jy ! Component: 3900 - total flux cleaned = -0.00330383 Jy ! Component: 3950 - total flux cleaned = -0.00324256 Jy ! Component: 4000 - total flux cleaned = -0.00319675 Jy ! Component: 4050 - total flux cleaned = -0.00321201 Jy ! Total flux subtracted in 4096 components = -0.00322718 Jy ! Clean residual min=-0.000927 max=0.000895 Jy/beam ! Clean residual mean=-0.000001 rms=0.000249 Jy/beam ! Combined flux in latest and established models = 0.197204 Jy keep ! Adding 337 model components to the UV plane model. ! The established model now contains 394 components and 0.197204 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1132+1023_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 6.16% of the data. ! The x-axis pixel size should ideally be below 0.1653 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6816 x 1.103 at -6.948 degrees (North through East) ! Clean map min=-0.001314 max=0.17674 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1132+1023_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.176742 invert ! Inverting map ! Your choice of large map pixels excluded 6.16% of the data. ! The x-axis pixel size should ideally be below 0.1653 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000249019 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.422681 0.422681 0.845362 1.69072 3.38145 6.7629 13.5258 27.0516 54.1032 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0007 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.176 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 709.755 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1132+1023_X_uvs.log closed on Sat Dec 26 09:37:13 2015