! Started logfile: /scr/pima/gb073_uvs/J1037+5711_X_uvs.log on Sat Dec 26 09:36:26 2015 obs /scr/pima/gb073_uvs/J1037+5711_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1037+5711_X_uva.fits ! AN table 1: 29 integrations on 55 of 55 possible baselines. ! AN table 2: 29 integrations on 66 of 66 possible baselines. ! AN table 3: 29 integrations on 55 of 55 possible baselines. ! AN table 4: 29 integrations on 55 of 55 possible baselines. ! Apparent sampling: 0.941932 visibilities/baseline/integration-bin. ! Found source: J1037+5711 ! ! 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 50480 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/J1037+5711_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 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 5. ! A total of 58 telescope corrections were flagged in sub-array 1. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 59 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 6. ! A total of 58 telescope corrections were flagged in sub-array 1. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 59 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 7. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 8. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=1.017503Jy sigma=9.696062 ! Fit after self-cal, rms=0.844386Jy sigma=8.033674 ! 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 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec ! Estimated beam: bmin=0.4513 mas, bmaj=0.6619 mas, bpa=-29.24 degrees ! Estimated noise=0.838673 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 = 0.124518 Jy ! Component: 100 - total flux cleaned = 0.151671 Jy ! Total flux subtracted in 100 components = 0.151671 Jy ! Clean residual min=-0.009818 max=0.010303 Jy/beam ! Clean residual mean=0.000003 rms=0.001024 Jy/beam ! Combined flux in latest and established models = 0.151671 Jy ! Performing phase self-cal ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 0.151671 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=0.094363Jy sigma=0.715914 ! Fit after self-cal, rms=0.094344Jy sigma=0.715801 ! Inverting map ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec ! Added new window around map position (0.4, 0.8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00419795 Jy ! Component: 100 - total flux cleaned = 0.00515931 Jy ! Total flux subtracted in 100 components = 0.00515931 Jy ! Clean residual min=-0.008420 max=0.009553 Jy/beam ! Clean residual mean=0.000002 rms=0.000952 Jy/beam ! Combined flux in latest and established models = 0.156831 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.156831 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=0.093425Jy sigma=0.706315 ! Fit after self-cal, rms=0.093380Jy sigma=0.705772 ! Inverting map ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec ! Added new window around map position (0.4, -1.6). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00246801 Jy ! Component: 100 - total flux cleaned = 0.00302177 Jy ! Total flux subtracted in 100 components = 0.00302177 Jy ! Clean residual min=-0.007496 max=0.006876 Jy/beam ! Clean residual mean=0.000001 rms=0.000902 Jy/beam ! Combined flux in latest and established models = 0.159853 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 11 components and 0.159853 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=0.092765Jy sigma=0.700238 ! Fit after self-cal, rms=0.092731Jy sigma=0.699958 ! Inverting map ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 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 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec ! Estimated beam: bmin=0.6262 mas, bmaj=0.9072 mas, bpa=-24.43 degrees ! Estimated noise=0.387654 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, -2.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00381024 Jy ! Component: 100 - total flux cleaned = 0.00457081 Jy ! Component: 150 - total flux cleaned = 0.00489402 Jy ! Component: 200 - total flux cleaned = 0.00518229 Jy ! Total flux subtracted in 200 components = 0.00518229 Jy ! Clean residual min=-0.003168 max=0.003538 Jy/beam ! Clean residual mean=0.000001 rms=0.000512 Jy/beam ! Combined flux in latest and established models = 0.165035 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 25 components and 0.165035 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=0.092427Jy sigma=0.697465 ! Fit after self-cal, rms=0.092410Jy sigma=0.697308 ! Inverting map ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec ! Added new window around map position (-1.4, 1.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00172981 Jy ! Component: 100 - total flux cleaned = 0.00225894 Jy ! Component: 150 - total flux cleaned = 0.00253385 Jy ! Component: 200 - total flux cleaned = 0.0026993 Jy ! Total flux subtracted in 200 components = 0.0026993 Jy ! Clean residual min=-0.003090 max=0.002700 Jy/beam ! Clean residual mean=-0.000003 rms=0.000491 Jy/beam ! Combined flux in latest and established models = 0.167734 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 39 components and 0.167734 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=0.092270Jy sigma=0.696363 ! Fit after self-cal, rms=0.092258Jy sigma=0.696262 ! Inverting map ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6262 x 0.9072 at -24.43 degrees (North through East) ! Clean map min=-0.0035886 max=0.15599 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 0.98 EF 1.00* FD 0.97 KP 1.02 ! LA 1.01 MC 0.90 NL 0.94 OV 0.99 ! PT 0.95 SC 1.00 ZC 0.91 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 EF 1.00* FD 1.00 KP 0.99 ! LA 1.04 MC 0.93 NL 0.92 ON 0.98 ! OV 1.00 PT 0.97 SC 0.96 ZC 0.76 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.96 EF 1.00* FD 1.00 KP 1.02 ! LA 1.06 MK 0.95 NL 0.92 ON 1.16 ! OV 1.02 PT 0.97 ZC 0.85 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.96 EF 1.00* FD 0.97 KP 1.00 ! LA 1.06 MC 0.94 NL 0.89 ON 0.97 ! PT 0.95 SC 0.97 ZC 0.90 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 EF 1.00* FD 1.02 KP 1.00 ! LA 1.07 MC 0.97 NL 0.97 OV 1.02 ! PT 1.03 SC 1.03 ZC 0.95 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 EF 1.00* FD 1.04 KP 1.02 ! LA 1.08 MC 0.99 NL 0.97 ON 1.02 ! OV 1.00 PT 1.02 SC 1.02 ZC 0.81 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.96 EF 1.00* FD 1.04 KP 1.05 ! LA 1.09 MK 1.02 NL 1.01 ON 1.12 ! OV 1.05 PT 1.00 ZC 0.91 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.96 EF 1.00* FD 0.99 KP 1.02 ! LA 1.03 MC 1.01 NL 0.97 ON 0.94 ! PT 1.00 SC 0.98 ZC 0.90 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 EF 1.00* FD 1.03 KP 0.93 ! LA 0.96 MC 0.92 NL 0.95 OV 0.99 ! PT 1.02 SC 1.06 ZC 0.93 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 EF 1.00* FD 1.03 KP 0.95 ! LA 0.99 MC 1.01 NL 0.97 ON 1.04 ! OV 0.99 PT 1.05 SC 1.04 ZC 0.75 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 EF 1.00* FD 1.01 KP 0.97 ! LA 1.00 MK 0.96 NL 0.95 ON 1.08 ! OV 1.02 PT 1.00 ZC 0.88 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.92 EF 1.00* FD 1.02 KP 0.95 ! LA 0.99 MC 0.97 NL 0.94 ON 0.98 ! PT 0.97 SC 1.02 ZC 0.88 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 EF 1.00* FD 1.03 KP 0.95 ! LA 1.02 MC 0.92 NL 0.99 OV 0.97 ! PT 1.02 SC 1.05 ZC 0.94 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 EF 1.00* FD 1.08 KP 0.97 ! LA 1.03 MC 1.00 NL 1.00 ON 1.03 ! OV 0.98 PT 1.03 SC 1.00 ZC 0.75 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 EF 1.00* FD 1.06 KP 1.02 ! LA 1.01 MK 0.95 NL 0.98 ON 1.10 ! OV 1.04 PT 1.04 ZC 0.87 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 EF 1.00* FD 1.01 KP 0.98 ! LA 1.01 MC 1.01 NL 0.97 ON 0.99 ! PT 1.03 SC 0.99 ZC 0.86 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.01 KP 0.92 ! LA 0.98 MC 1.44 NL 1.01 OV 1.02 ! PT 0.97 SC 1.04 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.06 KP 0.94 ! LA 1.00 MC 1.33 NL 0.98 ON 1.30 ! OV 1.00 PT 0.97 SC 1.11 ZC 0.80 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.04 KP 0.95 ! LA 1.01 MK 0.99 NL 0.98 ON 1.36 ! OV 1.05 PT 1.02 ZC 0.92 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.06 KP 0.92 ! LA 0.97 MC 1.24 NL 0.99 ON 1.24 ! PT 0.97 SC 1.04 ZC 0.91 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.99 KP 0.92 ! LA 0.97 MC 1.45 NL 1.00 OV 1.05 ! PT 0.97 SC 1.01 ZC 0.91 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.07 KP 0.87 ! LA 1.00 MC 1.27 NL 1.01 ON 1.25 ! OV 1.02 PT 0.96 SC 1.00 ZC 0.77 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00 KP 0.87 ! LA 1.04 MK 1.02 NL 1.00 ON 1.41 ! OV 1.10 PT 0.98 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00 KP 0.90 ! LA 0.97 MC 1.28 NL 0.96 ON 1.26 ! PT 0.97 SC 0.99 ZC 0.88 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 EF 1.00* FD 1.05 KP 0.93 ! LA 1.05 MC 1.47 NL 1.01 OV 1.01 ! PT 1.04 SC 1.04 ZC 0.81 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 EF 1.00* FD 1.09 KP 0.90 ! LA 1.06 MC 1.21 NL 1.03 ON 1.23 ! OV 1.02 PT 1.04 SC 1.08 ZC 0.66 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.93 EF 1.00* FD 1.08 KP 0.92 ! LA 1.07 MK 1.09 NL 1.06 ON 1.46 ! OV 1.01 PT 1.07 ZC 0.74 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 EF 1.00* FD 1.02 KP 0.92 ! LA 1.05 MC 1.40 NL 1.02 ON 1.29 ! PT 1.03 SC 1.00 ZC 0.75 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 EF 1.00* FD 1.04 KP 0.94 ! LA 1.04 MC 1.61 NL 0.97 OV 1.01 ! PT 1.00 SC 1.02 ZC 0.73 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 EF 1.00* FD 1.04 KP 0.95 ! LA 1.03 MC 1.40 NL 1.02 ON 1.30 ! OV 0.97 PT 1.03 SC 1.09 ZC 0.60 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 EF 1.00* FD 1.06 KP 0.94 ! LA 1.04 MK 1.04 NL 1.01 ON 1.45 ! OV 1.04 PT 0.99 ZC 0.72 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.96 EF 1.00* FD 1.04 KP 0.92 ! LA 1.04 MC 1.32 NL 1.01 ON 1.40 ! PT 0.99 SC 1.01 ZC 0.67 ! ! ! Fit before self-cal, rms=0.092258Jy sigma=0.696262 ! Fit after self-cal, rms=0.093133Jy sigma=0.668847 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec ! Estimated beam: bmin=0.6276 mas, bmaj=0.8978 mas, bpa=-25.94 degrees ! Estimated noise=0.387869 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 = 0.00128145 Jy ! Component: 100 - total flux cleaned = 0.00150945 Jy ! Component: 150 - total flux cleaned = 0.00157329 Jy ! Component: 200 - total flux cleaned = 0.00162745 Jy ! Total flux subtracted in 200 components = 0.00162745 Jy ! Clean residual min=-0.001334 max=0.001284 Jy/beam ! Clean residual mean=-0.000001 rms=0.000288 Jy/beam ! Combined flux in latest and established models = 0.169362 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 50 components and 0.169362 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=0.092994Jy sigma=0.667457 ! Fit after self-cal, rms=0.093100Jy sigma=0.667123 ! Inverting map ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 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=0.093100Jy sigma=0.667123 ! Fit after self-cal, rms=0.093604Jy sigma=0.666958 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec ! Estimated beam: bmin=0.6275 mas, bmaj=0.8959 mas, bpa=-26.22 degrees ! Estimated noise=0.388156 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000483273 Jy ! Component: 100 - total flux cleaned = 0.000592624 Jy ! Component: 150 - total flux cleaned = 0.000686058 Jy ! Component: 200 - total flux cleaned = 0.000768521 Jy ! Total flux subtracted in 200 components = 0.000768521 Jy ! Clean residual min=-0.001244 max=0.001257 Jy/beam ! Clean residual mean=-0.000001 rms=0.000279 Jy/beam ! Combined flux in latest and established models = 0.17013 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 56 components and 0.17013 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=0.093537Jy sigma=0.666295 ! Fit after self-cal, rms=0.093539Jy sigma=0.666274 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 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 = 3.77669e-05 Jy ! Component: 100 - total flux cleaned = 7.52008e-05 Jy ! Component: 150 - total flux cleaned = 0.000139437 Jy ! Component: 200 - total flux cleaned = 0.000199544 Jy ! Total flux subtracted in 200 components = 0.000199544 Jy ! Clean residual min=-0.001193 max=0.001249 Jy/beam ! Clean residual mean=-0.000001 rms=0.000275 Jy/beam ! Combined flux in latest and established models = 0.17033 Jy ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 62 components and 0.17033 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=0.093512Jy sigma=0.666011 ! Fit after self-cal, rms=0.093510Jy sigma=0.666003 ! Inverting map ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec ! Added new window around map position (-9.6, -12.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00101575 Jy ! Component: 100 - total flux cleaned = 0.00107818 Jy ! Component: 150 - total flux cleaned = 0.00113353 Jy ! Component: 200 - total flux cleaned = 0.00115972 Jy ! Total flux subtracted in 200 components = 0.00115972 Jy ! Clean residual min=-0.001154 max=0.001170 Jy/beam ! Clean residual mean=-0.000002 rms=0.000270 Jy/beam ! Combined flux in latest and established models = 0.171489 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 70 components and 0.171489 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=0.093485Jy sigma=0.665782 ! Fit after self-cal, rms=0.093485Jy sigma=0.665771 ! Inverting map ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec ! Added new window around map position (9, -19.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00109018 Jy ! Component: 100 - total flux cleaned = 0.00144132 Jy ! Component: 150 - total flux cleaned = 0.00156357 Jy ! Component: 200 - total flux cleaned = 0.00165611 Jy ! Total flux subtracted in 200 components = 0.00165611 Jy ! Clean residual min=-0.001132 max=0.001107 Jy/beam ! Clean residual mean=-0.000002 rms=0.000264 Jy/beam ! Combined flux in latest and established models = 0.173145 Jy ! Performing phase self-cal ! Adding 32 model components to the UV plane model. ! The established model now contains 80 components and 0.173145 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=0.093466Jy sigma=0.665601 ! Fit after self-cal, rms=0.093465Jy sigma=0.665591 ! Inverting map ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 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=0.093465Jy sigma=0.665591 ! Fit after self-cal, rms=0.093913Jy sigma=0.665410 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec ! Estimated beam: bmin=0.6273 mas, bmaj=0.8939 mas, bpa=-26.61 degrees ! Estimated noise=0.388611 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000197192 Jy ! Component: 100 - total flux cleaned = 0.000259607 Jy ! Component: 150 - total flux cleaned = 0.000427871 Jy ! Component: 200 - total flux cleaned = 0.000528648 Jy ! Total flux subtracted in 200 components = 0.000528648 Jy ! Clean residual min=-0.001088 max=0.001144 Jy/beam ! Clean residual mean=-0.000001 rms=0.000257 Jy/beam ! Combined flux in latest and established models = 0.173674 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 83 components and 0.173674 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=0.093887Jy sigma=0.665170 ! Fit after self-cal, rms=0.093891Jy sigma=0.665160 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (0.6, 15). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000684201 Jy ! Component: 100 - total flux cleaned = 0.000758924 Jy ! Component: 150 - total flux cleaned = 0.00087101 Jy ! Component: 200 - total flux cleaned = 0.000933972 Jy ! Total flux subtracted in 200 components = 0.000933972 Jy ! Clean residual min=-0.001086 max=0.001043 Jy/beam ! Clean residual mean=-0.000002 rms=0.000254 Jy/beam ! Combined flux in latest and established models = 0.174608 Jy ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 89 components and 0.174608 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=0.093870Jy sigma=0.664985 ! Fit after self-cal, rms=0.093868Jy sigma=0.664976 ! Inverting map ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 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=0.093868Jy sigma=0.664976 ! Fit after self-cal, rms=0.094177Jy sigma=0.664925 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec ! Estimated beam: bmin=2.733 mas, bmaj=2.975 mas, bpa=74.18 degrees ! Estimated noise=0.49138 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000543573 Jy ! Component: 100 - total flux cleaned = 0.000654704 Jy ! Component: 150 - total flux cleaned = 0.00076401 Jy ! Component: 200 - total flux cleaned = 0.000848035 Jy ! Total flux subtracted in 200 components = 0.000848035 Jy ! Clean residual min=-0.001215 max=0.001090 Jy/beam ! Clean residual mean=-0.000005 rms=0.000302 Jy/beam ! Combined flux in latest and established models = 0.175456 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 103 components and 0.175456 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=0.094177Jy sigma=0.664930 ! Fit after self-cal, rms=0.094180Jy sigma=0.664927 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 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 = 0.000103985 Jy ! Component: 100 - total flux cleaned = 0.000135403 Jy ! Component: 150 - total flux cleaned = 0.000173642 Jy ! Component: 200 - total flux cleaned = 0.000209385 Jy ! Total flux subtracted in 200 components = 0.000209385 Jy ! Clean residual min=-0.001218 max=0.001079 Jy/beam ! Clean residual mean=-0.000006 rms=0.000301 Jy/beam ! Combined flux in latest and established models = 0.175665 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 111 components and 0.175665 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=0.094181Jy sigma=0.664945 ! Fit after self-cal, rms=0.094181Jy sigma=0.664945 ! Inverting map ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 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 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec ! Estimated beam: bmin=0.6273 mas, bmaj=0.8927 mas, bpa=-26.82 degrees ! Estimated noise=0.389054 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6273 x 0.8927 at -26.82 degrees (North through East) ! Clean map min=-0.00099816 max=0.15556 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 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec ! Estimated beam: bmin=0.4504 mas, bmaj=0.6489 mas, bpa=-31.89 degrees ! Estimated noise=0.834983 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.123874 Jy ! Component: 100 - total flux cleaned = 0.150886 Jy ! Component: 150 - total flux cleaned = 0.1585 Jy ! Component: 200 - total flux cleaned = 0.161366 Jy ! Total flux subtracted in 200 components = 0.161366 Jy ! Clean residual min=-0.002794 max=0.003070 Jy/beam ! Clean residual mean=0.000002 rms=0.000587 Jy/beam ! Combined flux in latest and established models = 0.161366 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 9 model components to the UV plane model. ! The established model now contains 9 components and 0.161366 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec ! Estimated beam: bmin=0.6273 mas, bmaj=0.8927 mas, bpa=-26.82 degrees ! Estimated noise=0.389054 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 = 0.00357819 Jy ! Component: 100 - total flux cleaned = 0.00590012 Jy ! Component: 150 - total flux cleaned = 0.00769849 Jy ! Component: 200 - total flux cleaned = 0.00900581 Jy ! Total flux subtracted in 200 components = 0.00900581 Jy ! Clean residual min=-0.001240 max=0.001265 Jy/beam ! Clean residual mean=0.000003 rms=0.000272 Jy/beam ! Combined flux in latest and established models = 0.170372 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 31 components and 0.170372 Jy ! Inverting map ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec ! Added new window around map position (-0.4, -0.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000936601 Jy ! Component: 100 - total flux cleaned = 0.00165653 Jy ! Component: 150 - total flux cleaned = 0.00214413 Jy ! Component: 200 - total flux cleaned = 0.00251725 Jy ! Total flux subtracted in 200 components = 0.00251725 Jy ! Clean residual min=-0.001082 max=0.001064 Jy/beam ! Clean residual mean=0.000000 rms=0.000259 Jy/beam ! Combined flux in latest and established models = 0.172889 Jy ! Adding 30 model components to the UV plane model. ! The established model now contains 48 components and 0.172889 Jy ! Inverting map ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 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 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec ! Estimated beam: bmin=2.733 mas, bmaj=2.975 mas, bpa=74.18 degrees ! Estimated noise=0.49138 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00093095 Jy ! Component: 100 - total flux cleaned = 0.00158995 Jy ! Component: 150 - total flux cleaned = 0.00208212 Jy ! Component: 200 - total flux cleaned = 0.00231965 Jy ! Total flux subtracted in 200 components = 0.00231965 Jy ! Clean residual min=-0.001223 max=0.001086 Jy/beam ! Clean residual mean=-0.000004 rms=0.000304 Jy/beam ! Combined flux in latest and established models = 0.175209 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 = 0.000192411 Jy ! Component: 100 - total flux cleaned = 0.000302322 Jy ! Component: 150 - total flux cleaned = 0.000379839 Jy ! Component: 200 - total flux cleaned = 0.000431396 Jy ! Total flux subtracted in 200 components = 0.000431396 Jy ! Clean residual min=-0.001225 max=0.001071 Jy/beam ! Clean residual mean=-0.000005 rms=0.000302 Jy/beam ! Combined flux in latest and established models = 0.175641 Jy ! Adding 28 model components to the UV plane model. ! The established model now contains 74 components and 0.17564 Jy ! Inverting map ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec ! Estimated beam: bmin=0.6273 mas, bmaj=0.8927 mas, bpa=-26.82 degrees ! Estimated noise=0.389054 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000213734 Jy ! Component: 100 - total flux cleaned = -0.000213408 Jy ! Component: 150 - total flux cleaned = -0.000154853 Jy ! Component: 200 - total flux cleaned = -0.000100641 Jy ! Total flux subtracted in 200 components = -0.000100641 Jy ! Clean residual min=-0.001013 max=0.001044 Jy/beam ! Clean residual mean=-0.000002 rms=0.000251 Jy/beam ! Combined flux in latest and established models = 0.17554 Jy selfcal ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 89 components and 0.17554 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=0.094177Jy sigma=0.665002 ! Fit after self-cal, rms=0.094161Jy sigma=0.664903 wmodel /scr/pima/gb073_uvs/J1037+5711_X_map.mod ! Writing 89 model components to file: /scr/pima/gb073_uvs/J1037+5711_X_map.mod wobs /scr/pima/gb073_uvs/J1037+5711_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1037+5711_X_uvs.fits wwins /scr/pima/gb073_uvs/J1037+5711_X_map.win ! wwins: Wrote 9 windows to /scr/pima/gb073_uvs/J1037+5711_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 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000159544 Jy ! Component: 100 - total flux cleaned = 0.000158914 Jy ! Component: 150 - total flux cleaned = 0.000104176 Jy ! Component: 200 - total flux cleaned = 5.05163e-05 Jy ! Component: 250 - total flux cleaned = -1.99023e-05 Jy ! Component: 300 - total flux cleaned = -7.17377e-05 Jy ! Component: 350 - total flux cleaned = -8.86661e-05 Jy ! Component: 400 - total flux cleaned = -0.000156375 Jy ! Component: 450 - total flux cleaned = -0.000139826 Jy ! Component: 500 - total flux cleaned = -0.000189673 Jy ! Component: 550 - total flux cleaned = -0.000173428 Jy ! Component: 600 - total flux cleaned = -0.000238667 Jy ! Component: 650 - total flux cleaned = -0.000254621 Jy ! Component: 700 - total flux cleaned = -0.000254505 Jy ! Component: 750 - total flux cleaned = -0.000191173 Jy ! Component: 800 - total flux cleaned = -0.000254224 Jy ! Component: 850 - total flux cleaned = -0.000238685 Jy ! Component: 900 - total flux cleaned = -0.00026959 Jy ! Component: 950 - total flux cleaned = -0.000284914 Jy ! Component: 1000 - total flux cleaned = -0.000300229 Jy ! Component: 1050 - total flux cleaned = -0.000315238 Jy ! Component: 1100 - total flux cleaned = -0.000360603 Jy ! Component: 1150 - total flux cleaned = -0.000345459 Jy ! Component: 1200 - total flux cleaned = -0.000345568 Jy ! Component: 1250 - total flux cleaned = -0.000315806 Jy ! Component: 1300 - total flux cleaned = -0.000345415 Jy ! Component: 1350 - total flux cleaned = -0.000316052 Jy ! Component: 1400 - total flux cleaned = -0.000374519 Jy ! Component: 1450 - total flux cleaned = -0.000360029 Jy ! Component: 1500 - total flux cleaned = -0.000316699 Jy ! Component: 1550 - total flux cleaned = -0.000359971 Jy ! Component: 1600 - total flux cleaned = -0.000402951 Jy ! Component: 1650 - total flux cleaned = -0.000388742 Jy ! Component: 1700 - total flux cleaned = -0.000374568 Jy ! Component: 1750 - total flux cleaned = -0.000374459 Jy ! Component: 1800 - total flux cleaned = -0.000360444 Jy ! Component: 1850 - total flux cleaned = -0.000388577 Jy ! Component: 1900 - total flux cleaned = -0.000402496 Jy ! Component: 1950 - total flux cleaned = -0.000416464 Jy ! Component: 2000 - total flux cleaned = -0.000416421 Jy ! Component: 2050 - total flux cleaned = -0.000334011 Jy ! Component: 2100 - total flux cleaned = -0.000361493 Jy ! Component: 2150 - total flux cleaned = -0.000361625 Jy ! Component: 2200 - total flux cleaned = -0.000388844 Jy ! Component: 2250 - total flux cleaned = -0.000388886 Jy ! Component: 2300 - total flux cleaned = -0.00037543 Jy ! Component: 2350 - total flux cleaned = -0.00041566 Jy ! Component: 2400 - total flux cleaned = -0.000348781 Jy ! Component: 2450 - total flux cleaned = -0.00030887 Jy ! Component: 2500 - total flux cleaned = -0.000388595 Jy ! Component: 2550 - total flux cleaned = -0.000388514 Jy ! Component: 2600 - total flux cleaned = -0.000401669 Jy ! Component: 2650 - total flux cleaned = -0.000362217 Jy ! Component: 2700 - total flux cleaned = -0.000440624 Jy ! Component: 2750 - total flux cleaned = -0.000453601 Jy ! Component: 2800 - total flux cleaned = -0.00045359 Jy ! Component: 2850 - total flux cleaned = -0.000440538 Jy ! Component: 2900 - total flux cleaned = -0.000427689 Jy ! Component: 2950 - total flux cleaned = -0.000427658 Jy ! Component: 3000 - total flux cleaned = -0.000453258 Jy ! Component: 3050 - total flux cleaned = -0.00047892 Jy ! Component: 3100 - total flux cleaned = -0.000453444 Jy ! Component: 3150 - total flux cleaned = -0.000491556 Jy ! Component: 3200 - total flux cleaned = -0.000504229 Jy ! Component: 3250 - total flux cleaned = -0.000466324 Jy ! Component: 3300 - total flux cleaned = -0.000466315 Jy ! Component: 3350 - total flux cleaned = -0.000453754 Jy ! Component: 3400 - total flux cleaned = -0.000491321 Jy ! Component: 3450 - total flux cleaned = -0.000453957 Jy ! Component: 3500 - total flux cleaned = -0.000429077 Jy ! Component: 3550 - total flux cleaned = -0.000478636 Jy ! Component: 3600 - total flux cleaned = -0.000441544 Jy ! Component: 3650 - total flux cleaned = -0.000453862 Jy ! Component: 3700 - total flux cleaned = -0.000478431 Jy ! Component: 3750 - total flux cleaned = -0.000405008 Jy ! Component: 3800 - total flux cleaned = -0.000441619 Jy ! Component: 3850 - total flux cleaned = -0.000429439 Jy ! Component: 3900 - total flux cleaned = -0.000465899 Jy ! Component: 3950 - total flux cleaned = -0.000441643 Jy ! Component: 4000 - total flux cleaned = -0.000405464 Jy ! Component: 4050 - total flux cleaned = -0.00039343 Jy ! Total flux subtracted in 4096 components = -0.000405417 Jy ! Clean residual min=-0.000741 max=0.000706 Jy/beam ! Clean residual mean=-0.000000 rms=0.000194 Jy/beam ! Combined flux in latest and established models = 0.175134 Jy keep ! Adding 358 model components to the UV plane model. ! The established model now contains 447 components and 0.175134 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1037+5711_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6273 x 0.8927 at -26.82 degrees (North through East) ! Clean map min=-0.00088404 max=0.15588 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1037+5711_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.155883 invert ! Inverting map ! Your choice of large map pixels excluded 6.95% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! The y-axis pixel size should ideally be below 0.1745 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000192918 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.371273 0.371273 0.742547 1.48509 2.97019 5.94038 11.8808 23.7615 47.523 95.046 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0005 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.155 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 808.029 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1037+5711_X_uvs.log closed on Sat Dec 26 09:36:32 2015