! Started logfile: /scr/pima/gb073_uvs/J1130+3815_X_uvs.log on Sat Dec 26 09:37:03 2015 obs /scr/pima/gb073_uvs/J1130+3815_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1130+3815_X_uva.fits ! AN table 1: 5 integrations on 6 of 6 possible baselines. ! AN table 2: 5 integrations on 36 of 36 possible baselines. ! AN table 3: 18 integrations on 10 of 10 possible baselines. ! AN table 4: 6 integrations on 45 of 45 possible baselines. ! AN table 5: 6 integrations on 15 of 15 possible baselines. ! Apparent sampling: 0.988 visibilities/baseline/integration-bin. ! Found source: J1130+3815 ! ! 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 5928 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/J1130+3815_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 5 telescope corrections were flagged in sub-array 1. ! A total of 18 telescope corrections were flagged in sub-array 3. ! A total of 1 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 5 telescope corrections were flagged in sub-array 1. ! A total of 18 telescope corrections were flagged in sub-array 3. ! A total of 1 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 5 telescope corrections were flagged in sub-array 1. ! A total of 18 telescope corrections were flagged in sub-array 3. ! A total of 1 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 5 telescope corrections were flagged in sub-array 1. ! A total of 18 telescope corrections were flagged in sub-array 3. ! A total of 1 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 5. ! A total of 5 telescope corrections were flagged in sub-array 1. ! A total of 5 telescope corrections were flagged in sub-array 2. ! A total of 18 telescope corrections were flagged in sub-array 3. ! A total of 7 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 6. ! A total of 5 telescope corrections were flagged in sub-array 1. ! A total of 5 telescope corrections were flagged in sub-array 2. ! A total of 18 telescope corrections were flagged in sub-array 3. ! A total of 7 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 7. ! A total of 5 telescope corrections were flagged in sub-array 1. ! A total of 18 telescope corrections were flagged in sub-array 3. ! A total of 1 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 8. ! A total of 5 telescope corrections were flagged in sub-array 1. ! A total of 18 telescope corrections were flagged in sub-array 3. ! A total of 1 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=1.699729Jy sigma=14.212585 ! Fit after self-cal, rms=0.496983Jy sigma=4.281316 ! 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 1.75% of the data. ! The y-axis pixel size should ideally be below 0.1691 milli-arcsec ! Estimated beam: bmin=0.5189 mas, bmaj=0.7361 mas, bpa=38.41 degrees ! Estimated noise=2.04852 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 = 0.982722 Jy ! Component: 100 - total flux cleaned = 1.27455 Jy ! Total flux subtracted in 100 components = 1.27455 Jy ! Clean residual min=-0.065215 max=0.125208 Jy/beam ! Clean residual mean=-0.000068 rms=0.014077 Jy/beam ! Combined flux in latest and established models = 1.27455 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 1.27455 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=0.348904Jy sigma=2.819686 ! Fit after self-cal, rms=0.347969Jy sigma=2.814974 ! Inverting map ! Your choice of large map pixels excluded 1.75% of the data. ! The y-axis pixel size should ideally be below 0.1691 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.134629 Jy ! Component: 100 - total flux cleaned = 0.207556 Jy ! Total flux subtracted in 100 components = 0.207556 Jy ! Clean residual min=-0.060018 max=0.089138 Jy/beam ! Clean residual mean=-0.000196 rms=0.010864 Jy/beam ! Combined flux in latest and established models = 1.4821 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 9 components and 1.4821 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=0.288352Jy sigma=2.071197 ! Fit after self-cal, rms=0.287916Jy sigma=2.068906 ! Inverting map ! Your choice of large map pixels excluded 1.75% of the data. ! The y-axis pixel size should ideally be below 0.1691 milli-arcsec ! Added new window around map position (0.8, 0). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0576017 Jy ! Component: 100 - total flux cleaned = 0.0649948 Jy ! Total flux subtracted in 100 components = 0.0649948 Jy ! Clean residual min=-0.054981 max=0.078198 Jy/beam ! Clean residual mean=-0.000235 rms=0.009685 Jy/beam ! Combined flux in latest and established models = 1.5471 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 15 components and 1.5471 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=0.270243Jy sigma=1.872483 ! Fit after self-cal, rms=0.268344Jy sigma=1.856395 ! Inverting map ! Your choice of large map pixels excluded 1.75% of the data. ! The y-axis pixel size should ideally be below 0.1691 milli-arcsec ! Added new window around map position (-0.2, -1). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.053559 Jy ! Component: 100 - total flux cleaned = 0.0653374 Jy ! Total flux subtracted in 100 components = 0.0653374 Jy ! Clean residual min=-0.052206 max=0.046900 Jy/beam ! Clean residual mean=-0.000276 rms=0.008676 Jy/beam ! Combined flux in latest and established models = 1.61243 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 19 components and 1.61243 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=0.255466Jy sigma=1.710817 ! Fit after self-cal, rms=0.254218Jy sigma=1.698714 ! Inverting map ! Your choice of large map pixels excluded 1.75% of the data. ! The y-axis pixel size should ideally be below 0.1691 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 1.75% of the data. ! The y-axis pixel size should ideally be below 0.1691 milli-arcsec ! Estimated beam: bmin=0.6127 mas, bmaj=0.8471 mas, bpa=40.61 degrees ! Estimated noise=1.37279 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 = 0.0107167 Jy ! Component: 100 - total flux cleaned = 0.0131586 Jy ! Component: 150 - total flux cleaned = 0.0159991 Jy ! Component: 200 - total flux cleaned = 0.0190684 Jy ! Total flux subtracted in 200 components = 0.0190684 Jy ! Clean residual min=-0.047904 max=0.039085 Jy/beam ! Clean residual mean=-0.000941 rms=0.008631 Jy/beam ! Combined flux in latest and established models = 1.6315 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 23 components and 1.6315 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=0.245085Jy sigma=1.628627 ! Fit after self-cal, rms=0.243950Jy sigma=1.617490 ! Inverting map ! Your choice of large map pixels excluded 1.75% of the data. ! The y-axis pixel size should ideally be below 0.1691 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6127 x 0.8471 at 40.61 degrees (North through East) ! Clean map min=-0.050697 max=1.2672 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 15 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.96 FD 0.96 KP 0.96 LA 1.04 ! MK 1.01 NL 0.91 ON 0.92 OV 0.97 ! PT 0.94 ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.93 FD 0.97 HH 0.96 LA 1.14 ! MC 0.93 NL 0.93 ON 0.98 PT 1.01 ! SC 0.96 ZC 0.85 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 0.97 MC 0.95 ON 0.98 ! SC 1.00 ZC 0.87 ! ! ! Correcting IF 2. ! A total of 15 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 1.01 KP 0.98 LA 1.06 ! MK 1.05 NL 0.95 ON 0.95 OV 1.00 ! PT 0.99 ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 1.00 MC 1.01 ON 1.01 ! ZC 0.86 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 FD 1.02 HH 0.98 LA 1.18 ! MC 0.93 NL 0.95 ON 0.98 PT 1.06 ! SC 0.99 ZC 0.87 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 0.98 MC 0.99 ON 0.96 ! SC 1.03 ZC 0.88 ! ! ! Correcting IF 3. ! A total of 15 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 0.98 KP 0.93 LA 0.98 ! MK 1.00 NL 0.92 ON 0.89 OV 0.97 ! PT 0.98 ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 0.98 MC 1.01 ON 1.03 ! ZC 0.84 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 FD 1.02 HH 0.94 LA 1.08 ! MC 0.94 NL 0.93 ON 0.94 PT 1.03 ! SC 1.04 ZC 0.87 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 0.92 MC 0.98 ON 0.97 ! SC 1.05 ZC 0.89 ! ! ! Correcting IF 4. ! A total of 15 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 1.00 KP 0.95 LA 1.00 ! MK 1.01 NL 0.95 ON 0.93 OV 0.97 ! PT 1.00 ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 0.96 MC 1.03 ON 1.03 ! ZC 0.86 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 FD 1.04 HH 0.93 LA 1.12 ! MC 0.96 NL 0.96 ON 0.97 PT 1.06 ! SC 1.04 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 0.93 MC 0.98 ON 0.98 ! SC 1.05 ZC 0.89 ! ! ! Correcting IF 5. ! A total of 15 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 1.00 KP 0.88 LA 0.99 ! MK 1.03 NL 0.97 ON 1.14 OV 1.03 ! PT 0.95 ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 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: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! SC 1.00* ZC 1.00* ! ! ! Correcting IF 6. ! A total of 15 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 0.99 KP 0.84 LA 1.00 ! MK 1.03 NL 0.98 ON 1.18 OV 1.03 ! PT 0.92 ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 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: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! SC 1.00* ZC 1.00* ! ! ! Correcting IF 7. ! A total of 15 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 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* ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 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: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! SC 1.00* ZC 1.00* ! ! ! Correcting IF 8. ! A total of 15 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* MC 0.00* SC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 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* ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 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: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! SC 1.00* ZC 1.00* ! ! ! Fit before self-cal, rms=0.243950Jy sigma=1.617490 ! Fit after self-cal, rms=0.214613Jy sigma=1.370210 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 milli-arcsec ! Estimated beam: bmin=0.6089 mas, bmaj=0.8732 mas, bpa=42.22 degrees ! Estimated noise=1.3431 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 = -0.0264445 Jy ! Component: 100 - total flux cleaned = -0.0294007 Jy ! Component: 150 - total flux cleaned = -0.0307349 Jy ! Component: 200 - total flux cleaned = -0.0311034 Jy ! Total flux subtracted in 200 components = -0.0311034 Jy ! Clean residual min=-0.034163 max=0.029814 Jy/beam ! Clean residual mean=-0.000169 rms=0.006358 Jy/beam ! Combined flux in latest and established models = 1.6004 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 26 components and 1.6004 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=0.209666Jy sigma=1.343522 ! Fit after self-cal, rms=0.209569Jy sigma=1.341650 ! Inverting map ! Your choice of large map pixels excluded 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 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=0.209569Jy sigma=1.341650 ! Fit after self-cal, rms=0.206246Jy sigma=1.323513 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 milli-arcsec ! Estimated beam: bmin=0.6086 mas, bmaj=0.8741 mas, bpa=42.29 degrees ! Estimated noise=1.32555 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0186524 Jy ! Component: 100 - total flux cleaned = -0.0224097 Jy ! Component: 150 - total flux cleaned = -0.022738 Jy ! Component: 200 - total flux cleaned = -0.0227343 Jy ! Total flux subtracted in 200 components = -0.0227343 Jy ! Clean residual min=-0.032167 max=0.028098 Jy/beam ! Clean residual mean=-0.000154 rms=0.006057 Jy/beam ! Combined flux in latest and established models = 1.57767 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 29 components and 1.57767 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=0.203634Jy sigma=1.311997 ! Fit after self-cal, rms=0.203514Jy sigma=1.311342 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 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 = -0.000306193 Jy ! Component: 100 - total flux cleaned = -4.25197e-05 Jy ! Component: 150 - total flux cleaned = -4.73333e-05 Jy ! Component: 200 - total flux cleaned = -3.65504e-05 Jy ! Total flux subtracted in 200 components = -3.65504e-05 Jy ! Clean residual min=-0.031990 max=0.027163 Jy/beam ! Clean residual mean=-0.000154 rms=0.006032 Jy/beam ! Combined flux in latest and established models = 1.57763 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 30 components and 1.57763 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=0.202820Jy sigma=1.307557 ! Fit after self-cal, rms=0.202748Jy sigma=1.307197 ! Inverting map ! Your choice of large map pixels excluded 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 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=0.202748Jy sigma=1.307197 ! Fit after self-cal, rms=0.195720Jy sigma=1.221062 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 milli-arcsec ! Estimated beam: bmin=0.6102 mas, bmaj=0.8768 mas, bpa=42.2 degrees ! Estimated noise=1.31413 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0163665 Jy ! Component: 100 - total flux cleaned = -0.0249194 Jy ! Component: 150 - total flux cleaned = -0.0269712 Jy ! Component: 200 - total flux cleaned = -0.0271634 Jy ! Total flux subtracted in 200 components = -0.0271634 Jy ! Clean residual min=-0.027686 max=0.023126 Jy/beam ! Clean residual mean=-0.000031 rms=0.005447 Jy/beam ! Combined flux in latest and established models = 1.55047 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 34 components and 1.55047 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=0.193611Jy sigma=1.213659 ! Fit after self-cal, rms=0.193480Jy sigma=1.213163 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 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 = -0.000499084 Jy ! Component: 100 - total flux cleaned = -0.000134007 Jy ! Component: 150 - total flux cleaned = -0.000141272 Jy ! Component: 200 - total flux cleaned = -0.000303212 Jy ! Total flux subtracted in 200 components = -0.000303212 Jy ! Clean residual min=-0.027668 max=0.022875 Jy/beam ! Clean residual mean=-0.000030 rms=0.005433 Jy/beam ! Combined flux in latest and established models = 1.55016 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 36 components and 1.55016 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=0.193058Jy sigma=1.211532 ! Fit after self-cal, rms=0.192990Jy sigma=1.211277 ! Inverting map ! Your choice of large map pixels excluded 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 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=0.192990Jy sigma=1.211277 ! Fit after self-cal, rms=0.189295Jy sigma=1.178160 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 milli-arcsec ! Estimated beam: bmin=2.603 mas, bmaj=2.87 mas, bpa=89.49 degrees ! Estimated noise=1.71869 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0166443 Jy ! Component: 100 - total flux cleaned = -0.0176195 Jy ! Component: 150 - total flux cleaned = -0.0183179 Jy ! Component: 200 - total flux cleaned = -0.0177446 Jy ! Total flux subtracted in 200 components = -0.0177446 Jy ! Clean residual min=-0.024094 max=0.027569 Jy/beam ! Clean residual mean=0.000045 rms=0.007230 Jy/beam ! Combined flux in latest and established models = 1.53242 Jy selfcal ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 40 components and 1.53242 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=0.189787Jy sigma=1.188932 ! Fit after self-cal, rms=0.189377Jy sigma=1.185571 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 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 = 0.00195171 Jy ! Component: 100 - total flux cleaned = 0.00141878 Jy ! Component: 150 - total flux cleaned = 0.00163615 Jy ! Component: 200 - total flux cleaned = 0.00201766 Jy ! Total flux subtracted in 200 components = 0.00201766 Jy ! Clean residual min=-0.023527 max=0.027573 Jy/beam ! Clean residual mean=0.000026 rms=0.007150 Jy/beam ! Combined flux in latest and established models = 1.53443 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 40 components and 1.53443 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=0.190557Jy sigma=1.197807 ! Fit after self-cal, rms=0.190440Jy sigma=1.196335 ! Inverting map ! Your choice of large map pixels excluded 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 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 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 milli-arcsec ! Estimated beam: bmin=0.6105 mas, bmaj=0.8789 mas, bpa=42.28 degrees ! Estimated noise=1.30569 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6105 x 0.8789 at 42.28 degrees (North through East) ! Clean map min=-0.068358 max=1.206 Jy/beam if(peak(flux) > thresh) selfcal true, true clean clean_niter,clean_gain selfcal flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) selfcal true, true end if ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.190440Jy sigma=1.196335 ! Fit after self-cal, rms=0.186223Jy sigma=1.158800 ! Inverting map and beam ! Your choice of large map pixels excluded 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 milli-arcsec ! Estimated beam: bmin=0.6139 mas, bmaj=0.8796 mas, bpa=42.35 degrees ! Estimated noise=1.29652 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0118178 Jy ! Component: 100 - total flux cleaned = -0.0136885 Jy ! Component: 150 - total flux cleaned = -0.0142055 Jy ! Component: 200 - total flux cleaned = -0.0148791 Jy ! Total flux subtracted in 200 components = -0.0148791 Jy ! Clean residual min=-0.025072 max=0.021305 Jy/beam ! Clean residual mean=0.000049 rms=0.004995 Jy/beam ! Combined flux in latest and established models = 1.51956 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 42 components and 1.51956 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=0.184834Jy sigma=1.151956 ! Fit after self-cal, rms=0.184767Jy sigma=1.151584 ! Inverting map ! Your choice of large map pixels excluded 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00142222 Jy ! Component: 100 - total flux cleaned = -0.0014281 Jy ! Component: 150 - total flux cleaned = -0.00160961 Jy ! Component: 200 - total flux cleaned = -0.0017728 Jy ! Total flux subtracted in 200 components = -0.0017728 Jy ! Clean residual min=-0.025020 max=0.021314 Jy/beam ! Clean residual mean=0.000054 rms=0.004988 Jy/beam ! Combined flux in latest and established models = 1.51778 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 42 components and 1.51778 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=0.184288Jy sigma=1.149685 ! Fit after self-cal, rms=0.184281Jy sigma=1.149527 ! Inverting map ! Your choice of large map pixels excluded 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 milli-arcsec ! Performing amp+phase self-cal ! ! 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=0.184281Jy sigma=1.149527 ! Fit after self-cal, rms=0.183801Jy sigma=1.145241 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 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 milli-arcsec ! Estimated beam: bmin=0.516 mas, bmaj=0.7788 mas, bpa=40.72 degrees ! Estimated noise=1.93446 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.920946 Jy ! Component: 100 - total flux cleaned = 1.19217 Jy ! Component: 150 - total flux cleaned = 1.32581 Jy ! Component: 200 - total flux cleaned = 1.40402 Jy ! Total flux subtracted in 200 components = 1.40402 Jy ! Clean residual min=-0.052120 max=0.052118 Jy/beam ! Clean residual mean=0.000058 rms=0.007499 Jy/beam ! Combined flux in latest and established models = 1.40402 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 1.40402 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 milli-arcsec ! Estimated beam: bmin=0.613 mas, bmaj=0.8816 mas, bpa=42.31 degrees ! Estimated noise=1.29015 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 (-0.8, -0.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0654899 Jy ! Component: 100 - total flux cleaned = 0.0751126 Jy ! Component: 150 - total flux cleaned = 0.0829106 Jy ! Component: 200 - total flux cleaned = 0.088146 Jy ! Total flux subtracted in 200 components = 0.088146 Jy ! Clean residual min=-0.031388 max=0.027103 Jy/beam ! Clean residual mean=0.000092 rms=0.005489 Jy/beam ! Combined flux in latest and established models = 1.49217 Jy ! Adding 27 model components to the UV plane model. ! The established model now contains 31 components and 1.49217 Jy ! Inverting map ! Your choice of large map pixels excluded 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 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 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 milli-arcsec ! Estimated beam: bmin=2.601 mas, bmaj=2.881 mas, bpa=89.98 degrees ! Estimated noise=1.68724 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0199784 Jy ! Component: 100 - total flux cleaned = 0.0192308 Jy ! Component: 150 - total flux cleaned = 0.0185397 Jy ! Component: 200 - total flux cleaned = 0.0179697 Jy ! Total flux subtracted in 200 components = 0.0179697 Jy ! Clean residual min=-0.023370 max=0.023838 Jy/beam ! Clean residual mean=0.000110 rms=0.006601 Jy/beam ! Combined flux in latest and established models = 1.51014 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 = -0.000471365 Jy ! Component: 100 - total flux cleaned = -0.000484422 Jy ! Component: 150 - total flux cleaned = -0.000869427 Jy ! Component: 200 - total flux cleaned = -0.00119198 Jy ! Total flux subtracted in 200 components = -0.00119198 Jy ! Clean residual min=-0.022382 max=0.024174 Jy/beam ! Clean residual mean=0.000116 rms=0.006551 Jy/beam ! Combined flux in latest and established models = 1.50894 Jy ! Adding 16 model components to the UV plane model. ! The established model now contains 38 components and 1.50894 Jy ! Inverting map ! Your choice of large map pixels excluded 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 milli-arcsec ! Estimated beam: bmin=0.613 mas, bmaj=0.8816 mas, bpa=42.31 degrees ! Estimated noise=1.29015 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000284432 Jy ! Component: 100 - total flux cleaned = 0.00117447 Jy ! Component: 150 - total flux cleaned = 0.00191811 Jy ! Component: 200 - total flux cleaned = 0.00256132 Jy ! Total flux subtracted in 200 components = 0.00256132 Jy ! Clean residual min=-0.026963 max=0.021369 Jy/beam ! Clean residual mean=0.000034 rms=0.004917 Jy/beam ! Combined flux in latest and established models = 1.51151 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 45 components and 1.51151 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=0.181496Jy sigma=1.147904 ! Fit after self-cal, rms=0.180668Jy sigma=1.139934 wmodel /scr/pima/gb073_uvs/J1130+3815_X_map.mod ! Writing 45 model components to file: /scr/pima/gb073_uvs/J1130+3815_X_map.mod wobs /scr/pima/gb073_uvs/J1130+3815_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1130+3815_X_uvs.fits wwins /scr/pima/gb073_uvs/J1130+3815_X_map.win ! wwins: Wrote 4 windows to /scr/pima/gb073_uvs/J1130+3815_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 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.0118908 Jy ! Component: 100 - total flux cleaned = -0.0220279 Jy ! Component: 150 - total flux cleaned = -0.0286775 Jy ! Component: 200 - total flux cleaned = -0.0346289 Jy ! Component: 250 - total flux cleaned = -0.0392908 Jy ! Component: 300 - total flux cleaned = -0.0427604 Jy ! Component: 350 - total flux cleaned = -0.044792 Jy ! Component: 400 - total flux cleaned = -0.0471076 Jy ! Component: 450 - total flux cleaned = -0.0490465 Jy ! Component: 500 - total flux cleaned = -0.0506318 Jy ! Component: 550 - total flux cleaned = -0.0525046 Jy ! Component: 600 - total flux cleaned = -0.0546472 Jy ! Component: 650 - total flux cleaned = -0.0567567 Jy ! Component: 700 - total flux cleaned = -0.0582434 Jy ! Component: 750 - total flux cleaned = -0.0597147 Jy ! Component: 800 - total flux cleaned = -0.0617419 Jy ! Component: 850 - total flux cleaned = -0.0637399 Jy ! Component: 900 - total flux cleaned = -0.0651517 Jy ! Component: 950 - total flux cleaned = -0.0671004 Jy ! Component: 1000 - total flux cleaned = -0.0695714 Jy ! Component: 1050 - total flux cleaned = -0.0706522 Jy ! Component: 1100 - total flux cleaned = -0.0717245 Jy ! Component: 1150 - total flux cleaned = -0.07384 Jy ! Component: 1200 - total flux cleaned = -0.0748853 Jy ! Component: 1250 - total flux cleaned = -0.0766951 Jy ! Component: 1300 - total flux cleaned = -0.0774645 Jy ! Component: 1350 - total flux cleaned = -0.0797405 Jy ! Component: 1400 - total flux cleaned = -0.0812406 Jy ! Component: 1450 - total flux cleaned = -0.082474 Jy ! Component: 1500 - total flux cleaned = -0.0836943 Jy ! Component: 1550 - total flux cleaned = -0.0844244 Jy ! Component: 1600 - total flux cleaned = -0.0863382 Jy ! Component: 1650 - total flux cleaned = -0.0872867 Jy ! Component: 1700 - total flux cleaned = -0.0884599 Jy ! Component: 1750 - total flux cleaned = -0.0898526 Jy ! Component: 1800 - total flux cleaned = -0.0910024 Jy ! Component: 1850 - total flux cleaned = -0.0919124 Jy ! Component: 1900 - total flux cleaned = -0.0932621 Jy ! Component: 1950 - total flux cleaned = -0.0943765 Jy ! Component: 2000 - total flux cleaned = -0.0950401 Jy ! Component: 2050 - total flux cleaned = -0.0965673 Jy ! Component: 2100 - total flux cleaned = -0.0965661 Jy ! Component: 2150 - total flux cleaned = -0.0978507 Jy ! Component: 2200 - total flux cleaned = -0.0982744 Jy ! Component: 2250 - total flux cleaned = -0.0993262 Jy ! Component: 2300 - total flux cleaned = -0.0991172 Jy ! Component: 2350 - total flux cleaned = -0.100152 Jy ! Component: 2400 - total flux cleaned = -0.101175 Jy ! Component: 2450 - total flux cleaned = -0.101781 Jy ! Component: 2500 - total flux cleaned = -0.102384 Jy ! Component: 2550 - total flux cleaned = -0.10338 Jy ! Component: 2600 - total flux cleaned = -0.103573 Jy ! Component: 2650 - total flux cleaned = -0.104355 Jy ! Component: 2700 - total flux cleaned = -0.104743 Jy ! Component: 2750 - total flux cleaned = -0.105514 Jy ! Component: 2800 - total flux cleaned = -0.106088 Jy ! Component: 2850 - total flux cleaned = -0.106656 Jy ! Component: 2900 - total flux cleaned = -0.107594 Jy ! Component: 2950 - total flux cleaned = -0.108337 Jy ! Component: 3000 - total flux cleaned = -0.108891 Jy ! Component: 3050 - total flux cleaned = -0.109257 Jy ! Component: 3100 - total flux cleaned = -0.1098 Jy ! Component: 3150 - total flux cleaned = -0.110521 Jy ! Component: 3200 - total flux cleaned = -0.110878 Jy ! Component: 3250 - total flux cleaned = -0.112116 Jy ! Component: 3300 - total flux cleaned = -0.112466 Jy ! Component: 3350 - total flux cleaned = -0.11264 Jy ! Component: 3400 - total flux cleaned = -0.113852 Jy ! Component: 3450 - total flux cleaned = -0.114711 Jy ! Component: 3500 - total flux cleaned = -0.114881 Jy ! Component: 3550 - total flux cleaned = -0.115557 Jy ! Component: 3600 - total flux cleaned = -0.115893 Jy ! Component: 3650 - total flux cleaned = -0.116395 Jy ! Component: 3700 - total flux cleaned = -0.117388 Jy ! Component: 3750 - total flux cleaned = -0.118044 Jy ! Component: 3800 - total flux cleaned = -0.118043 Jy ! Component: 3850 - total flux cleaned = -0.118528 Jy ! Component: 3900 - total flux cleaned = -0.11901 Jy ! Component: 3950 - total flux cleaned = -0.119647 Jy ! Component: 4000 - total flux cleaned = -0.120121 Jy ! Component: 4050 - total flux cleaned = -0.121218 Jy ! Total flux subtracted in 4096 components = -0.121062 Jy ! Clean residual min=-0.008752 max=0.007763 Jy/beam ! Clean residual mean=0.000149 rms=0.002527 Jy/beam ! Combined flux in latest and established models = 1.39044 Jy keep ! Adding 313 model components to the UV plane model. ! The established model now contains 358 components and 1.39044 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1130+3815_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.613 x 0.8816 at 42.31 degrees (North through East) ! Clean map min=-0.056322 max=1.1937 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1130+3815_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 1.19371 invert ! Inverting map ! Your choice of large map pixels excluded 1.79% of the data. ! The y-axis pixel size should ideally be below 0.1691 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00252279 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.634022 0.634022 1.26804 2.53609 5.07217 10.1443 20.2887 40.5774 81.1548 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0075 print "peak= ", int(1000*peak_flux)/1000 ! peak= 1.193 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 473.169 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1130+3815_X_uvs.log closed on Sat Dec 26 09:37:07 2015