! Started logfile: /scr/pima/gb073_uvs/J1223+5037_X_uvs.log on Sat Dec 26 09:38:27 2015 obs /scr/pima/gb073_uvs/J1223+5037_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1223+5037_X_uva.fits ! AN table 1: 5 integrations on 66 of 66 possible baselines. ! AN table 2: 9 integrations on 45 of 45 possible baselines. ! AN table 3: 14 integrations on 66 of 66 possible baselines. ! AN table 4: 6 integrations on 55 of 55 possible baselines. ! Apparent sampling: 0.922574 visibilities/baseline/integration-bin. ! Found source: J1223+5037 ! ! 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 14680 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/J1223+5037_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 9 telescope corrections were flagged in sub-array 1. ! A total of 13 telescope corrections were flagged in sub-array 2. ! A total of 22 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 9 telescope corrections were flagged in sub-array 1. ! A total of 13 telescope corrections were flagged in sub-array 2. ! A total of 22 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 9 telescope corrections were flagged in sub-array 1. ! A total of 13 telescope corrections were flagged in sub-array 2. ! A total of 22 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 9 telescope corrections were flagged in sub-array 1. ! A total of 13 telescope corrections were flagged in sub-array 2. ! A total of 22 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 5. ! A total of 14 telescope corrections were flagged in sub-array 1. ! A total of 21 telescope corrections were flagged in sub-array 2. ! A total of 35 telescope corrections were flagged in sub-array 3. ! A total of 12 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 6. ! A total of 14 telescope corrections were flagged in sub-array 1. ! A total of 21 telescope corrections were flagged in sub-array 2. ! A total of 35 telescope corrections were flagged in sub-array 3. ! A total of 12 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 7. ! A total of 9 telescope corrections were flagged in sub-array 1. ! A total of 13 telescope corrections were flagged in sub-array 2. ! A total of 22 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 8. ! A total of 9 telescope corrections were flagged in sub-array 1. ! A total of 13 telescope corrections were flagged in sub-array 2. ! A total of 22 telescope corrections were flagged in sub-array 3. ! A total of 6 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=1.026857Jy sigma=9.290746 ! Fit after self-cal, rms=0.804714Jy sigma=7.202068 ! 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 2.73% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=0.5898 mas, bmaj=0.6821 mas, bpa=-39.83 degrees ! Estimated noise=1.30345 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 = 0.153496 Jy ! Component: 100 - total flux cleaned = 0.188305 Jy ! Total flux subtracted in 100 components = 0.188305 Jy ! Clean residual min=-0.006751 max=0.012873 Jy/beam ! Clean residual mean=-0.000011 rms=0.001372 Jy/beam ! Combined flux in latest and established models = 0.188305 Jy ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 4 components and 0.188305 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=0.109902Jy sigma=0.745702 ! Fit after self-cal, rms=0.109847Jy sigma=0.745385 ! Inverting map ! Your choice of large map pixels excluded 2.73% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0146402 Jy ! Component: 100 - total flux cleaned = 0.0231906 Jy ! Total flux subtracted in 100 components = 0.0231906 Jy ! Clean residual min=-0.006442 max=0.007345 Jy/beam ! Clean residual mean=-0.000007 rms=0.001197 Jy/beam ! Combined flux in latest and established models = 0.211496 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 11 components and 0.211496 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=0.107572Jy sigma=0.705986 ! Fit after self-cal, rms=0.107527Jy sigma=0.705619 ! Inverting map ! Your choice of large map pixels excluded 2.73% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Added new window around map position (-1.6, -4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00680052 Jy ! Component: 100 - total flux cleaned = 0.00922491 Jy ! Total flux subtracted in 100 components = 0.00922491 Jy ! Clean residual min=-0.006069 max=0.005548 Jy/beam ! Clean residual mean=-0.000005 rms=0.001153 Jy/beam ! Combined flux in latest and established models = 0.220721 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 15 components and 0.220721 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=0.107103Jy sigma=0.698948 ! Fit after self-cal, rms=0.107081Jy sigma=0.698666 ! Inverting map ! Your choice of large map pixels excluded 2.73% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 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 2.73% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=0.7287 mas, bmaj=0.8088 mas, bpa=-25.52 degrees ! Estimated noise=0.778221 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (-0.6, 0.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.006493 Jy ! Component: 100 - total flux cleaned = 0.00681316 Jy ! Component: 150 - total flux cleaned = 0.00694437 Jy ! Component: 200 - total flux cleaned = 0.00707216 Jy ! Total flux subtracted in 200 components = 0.00707216 Jy ! Clean residual min=-0.004452 max=0.004739 Jy/beam ! Clean residual mean=-0.000015 rms=0.000841 Jy/beam ! Combined flux in latest and established models = 0.227793 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 31 components and 0.227793 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=0.106559Jy sigma=0.692588 ! Fit after self-cal, rms=0.106547Jy sigma=0.692377 ! Inverting map ! Your choice of large map pixels excluded 2.73% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Added new window around map position (3.2, 1.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00483189 Jy ! Component: 100 - total flux cleaned = 0.00583726 Jy ! Component: 150 - total flux cleaned = 0.00626811 Jy ! Component: 200 - total flux cleaned = 0.00656788 Jy ! Total flux subtracted in 200 components = 0.00656788 Jy ! Clean residual min=-0.004400 max=0.003415 Jy/beam ! Clean residual mean=-0.000013 rms=0.000801 Jy/beam ! Combined flux in latest and established models = 0.234361 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 43 components and 0.234361 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=0.106240Jy sigma=0.688979 ! Fit after self-cal, rms=0.106239Jy sigma=0.688766 ! Inverting map ! Your choice of large map pixels excluded 2.73% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7287 x 0.8088 at -25.52 degrees (North through East) ! Clean map min=-0.0034881 max=0.20048 Jy/beam if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.92 EF 1.00* FD 0.96 KP 1.00 ! LA 1.04 MC 1.02 MK 0.94 NL 0.92 ! OV 1.05 PT 0.98 SC 1.12 ZC 0.79 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.93 EF 1.00* FD 0.97 LA 1.08 ! MC 0.94 NL 1.07 ON 0.95 PT 1.03 ! SC 1.02 ZC 0.82 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.94 EF 1.00* FD 0.96 KP 0.98 ! LA 1.04 MC 0.94 MK 1.02 NL 0.96 ! ON 1.07 OV 1.01 PT 0.93 SC 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 EF 1.00* FD 0.92 KP 1.02 ! LA 1.02 MC 0.94 NL 0.91 ON 1.01 ! PT 0.97 SC 0.94 ZC 0.78 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 EF 1.00* FD 0.96 KP 1.06 ! LA 1.02 MC 1.00 MK 0.96 NL 0.97 ! OV 1.03 PT 1.02 SC 1.48 ZC 0.87 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 EF 1.00* FD 1.07 LA 1.13 ! MC 0.91 NL 1.05 ON 0.97 PT 1.05 ! SC 1.03 ZC 0.88 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 EF 1.00* FD 1.06 KP 1.01 ! LA 1.07 MC 0.96 MK 1.05 NL 0.95 ! ON 1.01 OV 1.06 PT 1.02 SC 1.00 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 EF 1.00* FD 0.95 KP 1.06 ! LA 1.10 MC 0.94 NL 0.95 ON 1.05 ! PT 1.05 SC 0.96 ZC 0.81 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 EF 1.00* FD 0.98 KP 0.98 ! LA 1.03 MC 1.19 MK 0.93 NL 0.96 ! OV 0.94 PT 0.96 SC 1.10 ZC 0.84 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 EF 1.00* FD 1.05 LA 1.04 ! MC 0.99 NL 0.99 ON 0.92 PT 1.03 ! SC 0.97 ZC 0.84 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 EF 1.00* FD 0.99 KP 0.99 ! LA 0.98 MC 0.96 MK 0.98 NL 0.93 ! ON 1.02 OV 1.00 PT 1.00 SC 0.98 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 EF 1.00* FD 0.97 KP 0.99 ! LA 0.98 MC 1.13 NL 0.94 ON 1.01 ! PT 1.00 SC 0.88 ZC 0.74 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 EF 1.00* FD 1.05 KP 0.98 ! LA 0.98 MC 1.08 MK 0.97 NL 1.01 ! OV 1.03 PT 1.05 SC 1.50 ZC 0.87 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 EF 1.00* FD 1.09 LA 1.05 ! MC 0.98 NL 1.05 ON 0.96 PT 1.14 ! SC 1.01 ZC 0.80 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 EF 1.00* FD 1.03 KP 1.00 ! LA 0.99 MC 0.92 MK 1.03 NL 0.95 ! ON 1.02 OV 0.99 PT 1.02 SC 1.00 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.94 EF 1.00* FD 1.03 KP 1.01 ! LA 1.02 MC 0.99 NL 0.92 ON 1.00 ! PT 1.04 SC 0.99 ZC 0.77 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00 KP 0.91 ! LA 0.96 MC 1.47 MK 1.07 NL 1.01 ! OV 1.03 PT 1.00 SC 1.33 ZC 0.84 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.07 LA 1.08 ! MC 1.09 NL 1.11 ON 1.11 PT 1.01 ! SC 1.07 ZC 0.88 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 0.98 KP 0.92 ! LA 0.99 MC 1.22 MK 1.00 NL 0.95 ! ON 1.26 OV 1.04 PT 0.97 SC 0.98 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 0.98 KP 0.86 ! LA 1.00 MC 1.32 NL 1.08 ON 1.13 ! PT 0.98 SC 1.03 ZC 0.79 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.98 KP 0.86 ! LA 0.98 MC 1.24 MK 0.96 NL 1.04 ! OV 1.09 PT 0.94 SC 1.32 ZC 0.86 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.08 LA 1.05 ! MC 1.17 NL 0.97 ON 1.28 PT 0.91 ! SC 0.95 ZC 0.90 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.01 KP 0.84 ! LA 0.98 MC 1.32 MK 1.01 NL 0.97 ! ON 1.26 OV 1.06 PT 0.93 SC 0.96 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.05 KP 0.89 ! LA 0.93 MC 1.38 NL 0.94 ON 1.26 ! PT 1.02 SC 0.98 ZC 0.71 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 0.93 EF 1.00* FD 1.00 KP 0.85 ! LA 1.04 MC 1.34 MK 1.05 NL 1.04 ! OV 1.06 PT 1.06 SC 1.33 ZC 0.59 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.95 EF 1.00* FD 1.06 LA 1.08 ! MC 1.35 NL 1.09 ON 1.19 PT 1.11 ! SC 1.04 ZC 0.73 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 EF 1.00* FD 1.05 KP 0.91 ! LA 1.04 MC 1.23 MK 1.09 NL 1.01 ! ON 1.27 OV 0.97 PT 0.97 SC 0.98 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.03 EF 1.00* FD 1.01 KP 0.95 ! LA 0.97 MC 1.44 NL 1.01 ON 1.35 ! PT 0.96 SC 1.00 ZC 0.55 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 EF 1.00* FD 1.03 KP 0.94 ! LA 1.03 MC 1.35 MK 1.04 NL 0.96 ! OV 1.02 PT 0.97 SC 1.67 ZC 0.59 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 EF 1.00* FD 1.04 LA 1.13 ! MC 1.24 NL 1.05 ON 1.15 PT 1.01 ! SC 1.15 ZC 0.65 ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 EF 1.00* FD 1.00 KP 0.87 ! LA 1.03 MC 1.31 MK 1.05 NL 0.97 ! ON 1.27 OV 0.99 PT 1.03 SC 1.02 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.05 EF 1.00* FD 0.96 KP 0.90 ! LA 0.96 MC 1.44 NL 1.05 ON 1.18 ! PT 0.96 SC 0.99 ZC 0.53 ! ! ! Fit before self-cal, rms=0.106239Jy sigma=0.688766 ! Fit after self-cal, rms=0.106559Jy sigma=0.648646 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.74% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=0.7247 mas, bmaj=0.8186 mas, bpa=-24.35 degrees ! Estimated noise=0.776225 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 (2.8, -0.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00115367 Jy ! Component: 100 - total flux cleaned = 0.00122969 Jy ! Component: 150 - total flux cleaned = 0.00129613 Jy ! Component: 200 - total flux cleaned = 0.00135475 Jy ! Total flux subtracted in 200 components = 0.00135475 Jy ! Clean residual min=-0.002300 max=0.002003 Jy/beam ! Clean residual mean=-0.000002 rms=0.000506 Jy/beam ! Combined flux in latest and established models = 0.235716 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 58 components and 0.235716 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=0.106417Jy sigma=0.647483 ! Fit after self-cal, rms=0.106617Jy sigma=0.647025 ! Inverting map ! Your choice of large map pixels excluded 2.74% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 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=0.106617Jy sigma=0.647025 ! Fit after self-cal, rms=0.107307Jy sigma=0.644959 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.74% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=0.7254 mas, bmaj=0.819 mas, bpa=-23.89 degrees ! Estimated noise=0.775637 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 3.22219e-05 Jy ! Component: 100 - total flux cleaned = 0.000197063 Jy ! Component: 150 - total flux cleaned = 0.000291815 Jy ! Component: 200 - total flux cleaned = 0.00028947 Jy ! Total flux subtracted in 200 components = 0.00028947 Jy ! Clean residual min=-0.002225 max=0.002004 Jy/beam ! Clean residual mean=-0.000002 rms=0.000482 Jy/beam ! Combined flux in latest and established models = 0.236005 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 65 components and 0.236005 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=0.107235Jy sigma=0.644439 ! Fit after self-cal, rms=0.107251Jy sigma=0.644406 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.74% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 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 = 3.98624e-05 Jy ! Component: 100 - total flux cleaned = 0.000162992 Jy ! Component: 150 - total flux cleaned = 0.000163065 Jy ! Component: 200 - total flux cleaned = 0.000127987 Jy ! Total flux subtracted in 200 components = 0.000127987 Jy ! Clean residual min=-0.002216 max=0.002006 Jy/beam ! Clean residual mean=-0.000002 rms=0.000478 Jy/beam ! Combined flux in latest and established models = 0.236133 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 73 components and 0.236133 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=0.107214Jy sigma=0.644124 ! Fit after self-cal, rms=0.107212Jy sigma=0.644110 ! Inverting map ! Your choice of large map pixels excluded 2.74% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 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=0.107212Jy sigma=0.644110 ! Fit after self-cal, rms=0.107986Jy sigma=0.644023 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.74% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=0.7251 mas, bmaj=0.821 mas, bpa=-23.56 degrees ! Estimated noise=0.775549 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000280407 Jy ! Component: 100 - total flux cleaned = -0.000240393 Jy ! Component: 150 - total flux cleaned = -0.000204224 Jy ! Component: 200 - total flux cleaned = -0.000204143 Jy ! Total flux subtracted in 200 components = -0.000204143 Jy ! Clean residual min=-0.002155 max=0.001989 Jy/beam ! Clean residual mean=-0.000002 rms=0.000474 Jy/beam ! Combined flux in latest and established models = 0.235929 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 73 components and 0.235929 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=0.107944Jy sigma=0.643757 ! Fit after self-cal, rms=0.107952Jy sigma=0.643744 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.74% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 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 = 3.99482e-05 Jy ! Component: 100 - total flux cleaned = -2.12978e-05 Jy ! Component: 150 - total flux cleaned = -5.0393e-05 Jy ! Component: 200 - total flux cleaned = -7.83316e-05 Jy ! Total flux subtracted in 200 components = -7.83316e-05 Jy ! Clean residual min=-0.002141 max=0.001976 Jy/beam ! Clean residual mean=-0.000002 rms=0.000472 Jy/beam ! Combined flux in latest and established models = 0.235851 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 77 components and 0.235851 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=0.107930Jy sigma=0.643582 ! Fit after self-cal, rms=0.107929Jy sigma=0.643576 ! Inverting map ! Your choice of large map pixels excluded 2.74% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 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=0.107929Jy sigma=0.643576 ! Fit after self-cal, rms=0.108531Jy sigma=0.643536 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.74% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=2.436 mas, bmaj=3.013 mas, bpa=-17.74 degrees ! Estimated noise=1.0366 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000236304 Jy ! Component: 100 - total flux cleaned = -0.000301408 Jy ! Component: 150 - total flux cleaned = -0.000319357 Jy ! Component: 200 - total flux cleaned = -0.000363576 Jy ! Total flux subtracted in 200 components = -0.000363576 Jy ! Clean residual min=-0.002391 max=0.002190 Jy/beam ! Clean residual mean=-0.000006 rms=0.000583 Jy/beam ! Combined flux in latest and established models = 0.235487 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 87 components and 0.235487 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=0.108531Jy sigma=0.643473 ! Fit after self-cal, rms=0.108538Jy sigma=0.643466 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.74% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 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 = -8.1508e-05 Jy ! Component: 100 - total flux cleaned = -5.71296e-05 Jy ! Component: 150 - total flux cleaned = -4.5514e-05 Jy ! Component: 200 - total flux cleaned = -3.4618e-05 Jy ! Total flux subtracted in 200 components = -3.4618e-05 Jy ! Clean residual min=-0.002376 max=0.002150 Jy/beam ! Clean residual mean=-0.000006 rms=0.000582 Jy/beam ! Combined flux in latest and established models = 0.235453 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 90 components and 0.235452 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=0.108539Jy sigma=0.643436 ! Fit after self-cal, rms=0.108539Jy sigma=0.643435 ! Inverting map ! Your choice of large map pixels excluded 2.74% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 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 2.74% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=0.7249 mas, bmaj=0.8225 mas, bpa=-23.29 degrees ! Estimated noise=0.775636 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7249 x 0.8225 at -23.29 degrees (North through East) ! Clean map min=-0.0017201 max=0.20049 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 2.74% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=0.5859 mas, bmaj=0.6892 mas, bpa=-37.88 degrees ! Estimated noise=1.31169 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.154262 Jy ! Component: 100 - total flux cleaned = 0.190119 Jy ! Component: 150 - total flux cleaned = 0.204257 Jy ! Component: 200 - total flux cleaned = 0.211269 Jy ! Total flux subtracted in 200 components = 0.211269 Jy ! Clean residual min=-0.003845 max=0.004007 Jy/beam ! Clean residual mean=-0.000005 rms=0.000844 Jy/beam ! Combined flux in latest and established models = 0.211269 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 10 model components to the UV plane model. ! The established model now contains 10 components and 0.211269 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.74% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=0.7249 mas, bmaj=0.8225 mas, bpa=-23.29 degrees ! Estimated noise=0.775636 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 = 0.00726694 Jy ! Component: 100 - total flux cleaned = 0.0121066 Jy ! Component: 150 - total flux cleaned = 0.0156102 Jy ! Component: 200 - total flux cleaned = 0.0182674 Jy ! Total flux subtracted in 200 components = 0.0182674 Jy ! Clean residual min=-0.002182 max=0.002180 Jy/beam ! Clean residual mean=-0.000004 rms=0.000498 Jy/beam ! Combined flux in latest and established models = 0.229537 Jy ! Adding 29 model components to the UV plane model. ! The established model now contains 34 components and 0.229537 Jy ! Inverting map ! Your choice of large map pixels excluded 2.74% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 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 2.74% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=2.436 mas, bmaj=3.013 mas, bpa=-17.74 degrees ! Estimated noise=1.0366 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00333184 Jy ! Component: 100 - total flux cleaned = 0.00498117 Jy ! Component: 150 - total flux cleaned = 0.00572797 Jy ! Component: 200 - total flux cleaned = 0.00594823 Jy ! Total flux subtracted in 200 components = 0.00594823 Jy ! Clean residual min=-0.002430 max=0.002202 Jy/beam ! Clean residual mean=-0.000006 rms=0.000590 Jy/beam ! Combined flux in latest and established models = 0.235485 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 = 6.42824e-05 Jy ! Component: 100 - total flux cleaned = 0.000116727 Jy ! Component: 150 - total flux cleaned = 0.000160327 Jy ! Component: 200 - total flux cleaned = 0.00018697 Jy ! Total flux subtracted in 200 components = 0.00018697 Jy ! Clean residual min=-0.002391 max=0.002158 Jy/beam ! Clean residual mean=-0.000006 rms=0.000585 Jy/beam ! Combined flux in latest and established models = 0.235672 Jy ! Adding 32 model components to the UV plane model. ! The established model now contains 59 components and 0.235672 Jy ! Inverting map ! Your choice of large map pixels excluded 2.74% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.74% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! Estimated beam: bmin=0.7249 mas, bmaj=0.8225 mas, bpa=-23.29 degrees ! Estimated noise=0.775636 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000689444 Jy ! Component: 100 - total flux cleaned = 0.000776026 Jy ! Component: 150 - total flux cleaned = 0.000778112 Jy ! Component: 200 - total flux cleaned = 0.000710001 Jy ! Total flux subtracted in 200 components = 0.000710001 Jy ! Clean residual min=-0.002018 max=0.002017 Jy/beam ! Clean residual mean=-0.000002 rms=0.000470 Jy/beam ! Combined flux in latest and established models = 0.236382 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 73 components and 0.236382 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=0.108520Jy sigma=0.643320 ! Fit after self-cal, rms=0.108503Jy sigma=0.643220 wmodel /scr/pima/gb073_uvs/J1223+5037_X_map.mod ! Writing 73 model components to file: /scr/pima/gb073_uvs/J1223+5037_X_map.mod wobs /scr/pima/gb073_uvs/J1223+5037_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1223+5037_X_uvs.fits wwins /scr/pima/gb073_uvs/J1223+5037_X_map.win ! wwins: Wrote 5 windows to /scr/pima/gb073_uvs/J1223+5037_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 2.74% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00019283 Jy ! Component: 100 - total flux cleaned = -0.000376164 Jy ! Component: 150 - total flux cleaned = -0.000482155 Jy ! Component: 200 - total flux cleaned = -0.000586262 Jy ! Component: 250 - total flux cleaned = -0.00078838 Jy ! Component: 300 - total flux cleaned = -0.000920091 Jy ! Component: 350 - total flux cleaned = -0.00105037 Jy ! Component: 400 - total flux cleaned = -0.00121055 Jy ! Component: 450 - total flux cleaned = -0.00124202 Jy ! Component: 500 - total flux cleaned = -0.00127315 Jy ! Component: 550 - total flux cleaned = -0.00127321 Jy ! Component: 600 - total flux cleaned = -0.00142605 Jy ! Component: 650 - total flux cleaned = -0.00130483 Jy ! Component: 700 - total flux cleaned = -0.00130507 Jy ! Component: 750 - total flux cleaned = -0.00130523 Jy ! Component: 800 - total flux cleaned = -0.00130543 Jy ! Component: 850 - total flux cleaned = -0.00130515 Jy ! Component: 900 - total flux cleaned = -0.00124701 Jy ! Component: 950 - total flux cleaned = -0.00130444 Jy ! Component: 1000 - total flux cleaned = -0.00118959 Jy ! Component: 1050 - total flux cleaned = -0.00118941 Jy ! Component: 1100 - total flux cleaned = -0.00121746 Jy ! Component: 1150 - total flux cleaned = -0.00124573 Jy ! Component: 1200 - total flux cleaned = -0.00124575 Jy ! Component: 1250 - total flux cleaned = -0.00119027 Jy ! Component: 1300 - total flux cleaned = -0.00113554 Jy ! Component: 1350 - total flux cleaned = -0.00113559 Jy ! Component: 1400 - total flux cleaned = -0.00118982 Jy ! Component: 1450 - total flux cleaned = -0.00129803 Jy ! Component: 1500 - total flux cleaned = -0.00124407 Jy ! Component: 1550 - total flux cleaned = -0.00124397 Jy ! Component: 1600 - total flux cleaned = -0.00113788 Jy ! Component: 1650 - total flux cleaned = -0.00105863 Jy ! Component: 1700 - total flux cleaned = -0.00105866 Jy ! Component: 1750 - total flux cleaned = -0.00108497 Jy ! Component: 1800 - total flux cleaned = -0.0011368 Jy ! Component: 1850 - total flux cleaned = -0.00108509 Jy ! Component: 1900 - total flux cleaned = -0.00105948 Jy ! Component: 1950 - total flux cleaned = -0.000931593 Jy ! Component: 2000 - total flux cleaned = -0.00100809 Jy ! Component: 2050 - total flux cleaned = -0.00110938 Jy ! Component: 2100 - total flux cleaned = -0.00108401 Jy ! Component: 2150 - total flux cleaned = -0.00105919 Jy ! Component: 2200 - total flux cleaned = -0.00100929 Jy ! Component: 2250 - total flux cleaned = -0.000984526 Jy ! Component: 2300 - total flux cleaned = -0.000984502 Jy ! Component: 2350 - total flux cleaned = -0.000960005 Jy ! Component: 2400 - total flux cleaned = -0.000837491 Jy ! Component: 2450 - total flux cleaned = -0.000886339 Jy ! Component: 2500 - total flux cleaned = -0.00086205 Jy ! Component: 2550 - total flux cleaned = -0.000741199 Jy ! Component: 2600 - total flux cleaned = -0.000668966 Jy ! Component: 2650 - total flux cleaned = -0.000693024 Jy ! Component: 2700 - total flux cleaned = -0.000692987 Jy ! Component: 2750 - total flux cleaned = -0.000716643 Jy ! Component: 2800 - total flux cleaned = -0.000669216 Jy ! Component: 2850 - total flux cleaned = -0.000645559 Jy ! Component: 2900 - total flux cleaned = -0.000786654 Jy ! Component: 2950 - total flux cleaned = -0.000716418 Jy ! Component: 3000 - total flux cleaned = -0.0006933 Jy ! Component: 3050 - total flux cleaned = -0.000739903 Jy ! Component: 3100 - total flux cleaned = -0.00069365 Jy ! Component: 3150 - total flux cleaned = -0.000739866 Jy ! Component: 3200 - total flux cleaned = -0.000739802 Jy ! Component: 3250 - total flux cleaned = -0.000785518 Jy ! Component: 3300 - total flux cleaned = -0.000785646 Jy ! Component: 3350 - total flux cleaned = -0.000785754 Jy ! Component: 3400 - total flux cleaned = -0.000785706 Jy ! Component: 3450 - total flux cleaned = -0.000808224 Jy ! Component: 3500 - total flux cleaned = -0.000853142 Jy ! Component: 3550 - total flux cleaned = -0.000830721 Jy ! Component: 3600 - total flux cleaned = -0.000808393 Jy ! Component: 3650 - total flux cleaned = -0.000897299 Jy ! Component: 3700 - total flux cleaned = -0.000830765 Jy ! Component: 3750 - total flux cleaned = -0.000808815 Jy ! Component: 3800 - total flux cleaned = -0.000830672 Jy ! Component: 3850 - total flux cleaned = -0.000808757 Jy ! Component: 3900 - total flux cleaned = -0.000917997 Jy ! Component: 3950 - total flux cleaned = -0.000852666 Jy ! Component: 4000 - total flux cleaned = -0.000961056 Jy ! Component: 4050 - total flux cleaned = -0.00096107 Jy ! Total flux subtracted in 4096 components = -0.000874801 Jy ! Clean residual min=-0.001320 max=0.001147 Jy/beam ! Clean residual mean=-0.000001 rms=0.000348 Jy/beam ! Combined flux in latest and established models = 0.235507 Jy keep ! Adding 370 model components to the UV plane model. ! The established model now contains 443 components and 0.235507 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1223+5037_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 2.74% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7249 x 0.8225 at -23.29 degrees (North through East) ! Clean map min=-0.001557 max=0.20184 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1223+5037_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.201836 invert ! Inverting map ! Your choice of large map pixels excluded 2.74% of the data. ! The x-axis pixel size should ideally be below 0.1786 milli-arcsec ! The y-axis pixel size should ideally be below 0.187 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000347968 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.517204 0.517204 1.03441 2.06882 4.13763 8.27527 16.5505 33.1011 66.2022 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.001 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.201 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 580.041 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1223+5037_X_uvs.log closed on Sat Dec 26 09:38:31 2015