! Started logfile: /scr/pima/gb073_uvs/J1819+5511_X_uvs.log on Sat Dec 26 09:43:55 2015 obs /scr/pima/gb073_uvs/J1819+5511_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1819+5511_X_uva.fits ! AN table 1: 58 integrations on 66 of 66 possible baselines. ! AN table 2: 29 integrations on 55 of 55 possible baselines. ! AN table 3: 29 integrations on 55 of 55 possible baselines. ! AN table 4: 29 integrations on 21 of 21 possible baselines. ! AN table 5: 29 integrations on 66 of 66 possible baselines. ! Apparent sampling: 0.885127 visibilities/baseline/integration-bin. ! Found source: J1819+5511 ! ! 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 67560 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/J1819+5511_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 58 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 29 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 58 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 29 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 58 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 29 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 58 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 29 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 5. ! A total of 116 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 58 telescope corrections were flagged in sub-array 4. ! A total of 58 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 6. ! A total of 116 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 58 telescope corrections were flagged in sub-array 4. ! A total of 58 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 7. ! A total of 58 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 29 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 8. ! A total of 58 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 29 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=1.012477Jy sigma=10.147982 ! Fit after self-cal, rms=0.874321Jy sigma=8.732091 ! 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 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 milli-arcsec ! Estimated beam: bmin=0.4375 mas, bmaj=0.6494 mas, bpa=-22.11 degrees ! Estimated noise=0.667591 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 = 0.0994153 Jy ! Component: 100 - total flux cleaned = 0.121094 Jy ! Total flux subtracted in 100 components = 0.121094 Jy ! Clean residual min=-0.006705 max=0.008599 Jy/beam ! Clean residual mean=0.000003 rms=0.000728 Jy/beam ! Combined flux in latest and established models = 0.121094 Jy ! Performing phase self-cal ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 0.121094 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=0.084880Jy sigma=0.710413 ! Fit after self-cal, rms=0.084817Jy sigma=0.710214 ! Inverting map ! Your choice of large map pixels excluded 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 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 = 0.00749604 Jy ! Component: 100 - total flux cleaned = 0.00919683 Jy ! Total flux subtracted in 100 components = 0.00919683 Jy ! Clean residual min=-0.006056 max=0.007265 Jy/beam ! Clean residual mean=0.000001 rms=0.000694 Jy/beam ! Combined flux in latest and established models = 0.130291 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 8 components and 0.130291 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=0.084224Jy sigma=0.702118 ! Fit after self-cal, rms=0.084187Jy sigma=0.701602 ! Inverting map ! Your choice of large map pixels excluded 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 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 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 milli-arcsec ! Estimated beam: bmin=0.5903 mas, bmaj=0.8732 mas, bpa=-19.51 degrees ! Estimated noise=0.306382 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 (0.4, -0.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00580913 Jy ! Component: 100 - total flux cleaned = 0.00806951 Jy ! Component: 150 - total flux cleaned = 0.00870936 Jy ! Component: 200 - total flux cleaned = 0.00878928 Jy ! Total flux subtracted in 200 components = 0.00878928 Jy ! Clean residual min=-0.002989 max=0.002645 Jy/beam ! Clean residual mean=0.000002 rms=0.000400 Jy/beam ! Combined flux in latest and established models = 0.13908 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 21 components and 0.13908 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=0.083785Jy sigma=0.697375 ! Fit after self-cal, rms=0.083741Jy sigma=0.696940 ! Inverting map ! Your choice of large map pixels excluded 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5903 x 0.8732 at -19.51 degrees (North through East) ! Clean map min=-0.0019442 max=0.12385 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 0.97 EF 1.00* FD 0.99 KP 0.98 ! LA 1.04 MC 0.91 NL 0.93 ON 0.94 ! OV 1.01 PT 0.95 SC 1.03 ZC 0.81 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 EF 1.00* FD 0.99 KP 0.98 ! LA 1.06 MK 1.00 NL 0.97 ON 1.21 ! OV 1.03 PT 0.98 ZC 0.92 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 EF 1.00* FD 0.97 KP 0.97 ! LA 1.03 MC 0.95 NL 0.93 ON 1.03 ! PT 0.95 SC 0.99 ZC 0.70 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.95 EF 1.00* LA 1.00 MK 0.94 ! NL 0.91 PT 0.98 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.93 EF 1.00* FD 0.98 KP 0.99 ! LA 1.05 MK 0.99 NL 0.91 ON 1.14 ! OV 1.01 PT 0.92 SC 1.00 ZC 0.87 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 EF 1.00* FD 1.03 KP 1.04 ! LA 1.04 MC 0.99 NL 0.97 ON 0.95 ! OV 1.00 PT 1.01 SC 1.04 ZC 0.85 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 EF 1.00* FD 1.07 KP 1.01 ! LA 1.11 MK 1.03 NL 1.04 ON 1.31 ! OV 0.99 PT 1.04 ZC 0.93 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.04 EF 1.00* FD 1.05 KP 1.03 ! LA 1.03 MC 1.00 NL 0.94 ON 0.95 ! PT 1.01 SC 1.01 ZC 0.72 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 EF 1.00* LA 1.04 MK 1.01 ! NL 0.93 PT 1.00 ZC 0.92 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 EF 1.00* FD 1.03 KP 1.03 ! LA 1.04 MK 1.03 NL 0.95 ON 1.11 ! OV 0.99 PT 1.03 SC 1.02 ZC 0.86 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 EF 1.00* FD 0.98 KP 0.95 ! LA 0.97 MC 0.99 NL 0.93 ON 0.96 ! OV 0.98 PT 0.99 SC 1.10 ZC 0.81 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 EF 1.00* FD 0.97 KP 0.98 ! LA 1.01 MK 0.93 NL 1.02 ON 1.07 ! OV 1.03 PT 1.03 ZC 0.88 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 EF 1.00* FD 0.98 KP 0.97 ! LA 0.99 MC 0.97 NL 0.95 ON 0.97 ! PT 0.99 SC 1.06 ZC 0.69 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 EF 1.00* LA 1.01 MK 0.95 ! NL 0.92 PT 0.98 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.03 EF 1.00* FD 1.01 KP 0.96 ! LA 0.95 MK 0.95 NL 0.92 ON 1.13 ! OV 0.96 PT 0.99 SC 1.01 ZC 0.82 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 EF 1.00* FD 1.03 KP 1.00 ! LA 1.01 MC 0.99 NL 0.99 ON 1.02 ! OV 0.99 PT 1.04 SC 1.06 ZC 0.84 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 EF 1.00* FD 1.01 KP 0.99 ! LA 1.05 MK 1.05 NL 1.01 ON 1.11 ! OV 1.00 PT 1.03 ZC 0.90 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 EF 1.00* FD 0.99 KP 0.95 ! LA 0.97 MC 1.00 NL 0.96 ON 1.09 ! PT 1.01 SC 1.13 ZC 0.71 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.96 EF 1.00* LA 0.99 MK 0.95 ! NL 0.93 PT 1.00 ZC 0.93 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 EF 1.00* FD 1.03 KP 0.96 ! LA 1.00 MK 0.98 NL 0.94 ON 1.07 ! OV 0.99 PT 1.00 SC 1.04 ZC 0.80 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.02 KP 0.91 ! LA 1.03 MC 1.26 NL 0.97 ON 1.68 ! OV 1.03 PT 1.00 SC 1.09 ZC 0.88 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00 KP 0.89 ! LA 1.04 MK 0.99 NL 1.11 ON 1.46 ! OV 1.05 PT 0.97 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.07 KP 0.91 ! LA 1.01 MC 1.26 NL 0.96 ON 1.27 ! PT 0.98 SC 1.11 ZC 0.72 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* LA 1.00 MK 0.95 ! NL 1.03 PT 0.98 ZC 0.85 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 0.99 KP 0.90 ! LA 0.99 MK 1.04 NL 0.98 ON 1.39 ! OV 1.04 PT 0.98 SC 1.04 ZC 0.88 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.02 KP 0.90 ! LA 1.05 MC 1.33 NL 0.96 ON 1.68 ! OV 1.04 PT 0.94 SC 1.05 ZC 0.84 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.04 KP 0.94 ! LA 1.05 MK 0.98 NL 1.06 ON 1.48 ! OV 1.08 PT 0.99 ZC 0.87 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00 KP 0.87 ! LA 0.98 MC 1.22 NL 0.99 ON 1.31 ! PT 0.94 SC 1.08 ZC 0.72 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* LA 1.11 MK 1.09 ! NL 0.92 PT 0.96 ZC 0.82 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.01 KP 0.89 ! LA 1.02 MK 1.01 NL 0.98 ON 1.53 ! OV 1.02 PT 0.95 SC 0.95 ZC 0.84 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 EF 1.00* FD 1.10 KP 0.97 ! LA 1.05 MC 1.29 NL 1.02 ON 1.74 ! OV 1.02 PT 1.03 SC 1.10 ZC 0.69 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 EF 1.00* FD 1.08 KP 0.93 ! LA 1.07 MK 1.03 NL 1.08 ON 1.42 ! OV 1.05 PT 1.04 ZC 0.66 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 EF 1.00* FD 1.08 KP 0.91 ! LA 1.01 MC 1.36 NL 1.01 ON 1.32 ! PT 0.96 SC 1.13 ZC 0.58 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.96 EF 1.00* LA 1.05 MK 1.08 ! NL 1.02 PT 1.01 ZC 0.81 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 EF 1.00* FD 1.05 KP 0.93 ! LA 1.06 MK 1.08 NL 0.99 ON 1.48 ! OV 1.02 PT 1.03 SC 1.06 ZC 0.71 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 EF 1.00* FD 1.05 KP 0.91 ! LA 1.07 MC 1.36 NL 1.00 ON 1.65 ! OV 1.02 PT 1.05 SC 1.12 ZC 0.64 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.96 EF 1.00* FD 1.01 KP 0.92 ! LA 1.05 MK 1.13 NL 1.08 ON 1.57 ! OV 1.07 PT 0.99 ZC 0.67 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 EF 1.00* FD 1.04 KP 0.89 ! LA 1.00 MC 1.37 NL 0.98 ON 1.35 ! PT 1.02 SC 1.15 ZC 0.54 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 EF 1.00* LA 1.05 MK 1.02 ! NL 1.01 PT 1.00 ZC 0.70 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 EF 1.00* FD 1.04 KP 0.94 ! LA 1.04 MK 1.11 NL 1.01 ON 1.49 ! OV 0.99 PT 1.00 SC 1.04 ZC 0.65 ! ! ! Fit before self-cal, rms=0.083741Jy sigma=0.696940 ! Fit after self-cal, rms=0.085511Jy sigma=0.670578 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 milli-arcsec ! Estimated beam: bmin=0.5829 mas, bmaj=0.8637 mas, bpa=-20.23 degrees ! Estimated noise=0.305299 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 = 0.000631326 Jy ! Component: 100 - total flux cleaned = 0.000738167 Jy ! Component: 150 - total flux cleaned = 0.000697104 Jy ! Component: 200 - total flux cleaned = 0.00069679 Jy ! Total flux subtracted in 200 components = 0.00069679 Jy ! Clean residual min=-0.001111 max=0.001485 Jy/beam ! Clean residual mean=-0.000003 rms=0.000255 Jy/beam ! Combined flux in latest and established models = 0.139777 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 31 components and 0.139777 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=0.085452Jy sigma=0.669851 ! Fit after self-cal, rms=0.085593Jy sigma=0.669307 ! Inverting map ! Your choice of large map pixels excluded 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 milli-arcsec ! Added new window around map position (4.6, -9.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000941986 Jy ! Component: 100 - total flux cleaned = 0.00113594 Jy ! Component: 150 - total flux cleaned = 0.00113653 Jy ! Component: 200 - total flux cleaned = 0.0011364 Jy ! Total flux subtracted in 200 components = 0.0011364 Jy ! Clean residual min=-0.001105 max=0.001258 Jy/beam ! Clean residual mean=-0.000004 rms=0.000249 Jy/beam ! Combined flux in latest and established models = 0.140914 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 41 components and 0.140914 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=0.085559Jy sigma=0.668906 ! Fit after self-cal, rms=0.085553Jy sigma=0.668862 ! Inverting map ! Your choice of large map pixels excluded 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 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=0.085553Jy sigma=0.668862 ! Fit after self-cal, rms=0.086753Jy sigma=0.667037 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 milli-arcsec ! Estimated beam: bmin=0.5819 mas, bmaj=0.8592 mas, bpa=-20.45 degrees ! Estimated noise=0.305049 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00047481 Jy ! Component: 100 - total flux cleaned = 0.000547397 Jy ! Component: 150 - total flux cleaned = 0.000606881 Jy ! Component: 200 - total flux cleaned = 0.00065896 Jy ! Total flux subtracted in 200 components = 0.00065896 Jy ! Clean residual min=-0.001039 max=0.000951 Jy/beam ! Clean residual mean=-0.000002 rms=0.000219 Jy/beam ! Combined flux in latest and established models = 0.141573 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 43 components and 0.141573 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=0.086719Jy sigma=0.666678 ! Fit after self-cal, rms=0.086735Jy sigma=0.666612 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 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 = 0.000176917 Jy ! Component: 100 - total flux cleaned = 0.000201513 Jy ! Component: 150 - total flux cleaned = 0.000179574 Jy ! Component: 200 - total flux cleaned = 0.000179762 Jy ! Total flux subtracted in 200 components = 0.000179762 Jy ! Clean residual min=-0.001031 max=0.000931 Jy/beam ! Clean residual mean=-0.000002 rms=0.000217 Jy/beam ! Combined flux in latest and established models = 0.141752 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 46 components and 0.141752 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=0.086720Jy sigma=0.666458 ! Fit after self-cal, rms=0.086717Jy sigma=0.666443 ! Inverting map ! Your choice of large map pixels excluded 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 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=0.086717Jy sigma=0.666443 ! Fit after self-cal, rms=0.086802Jy sigma=0.666340 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 milli-arcsec ! Estimated beam: bmin=0.5812 mas, bmaj=0.8557 mas, bpa=-20.66 degrees ! Estimated noise=0.304823 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000246097 Jy ! Component: 100 - total flux cleaned = 0.000219709 Jy ! Component: 150 - total flux cleaned = 0.000241367 Jy ! Component: 200 - total flux cleaned = 0.00024179 Jy ! Total flux subtracted in 200 components = 0.00024179 Jy ! Clean residual min=-0.001021 max=0.000927 Jy/beam ! Clean residual mean=-0.000002 rms=0.000212 Jy/beam ! Combined flux in latest and established models = 0.141994 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 49 components and 0.141994 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=0.086784Jy sigma=0.666155 ! Fit after self-cal, rms=0.086782Jy sigma=0.666140 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 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 = 0.000112198 Jy ! Component: 100 - total flux cleaned = 9.41576e-05 Jy ! Component: 150 - total flux cleaned = 6.07962e-05 Jy ! Component: 200 - total flux cleaned = 4.5127e-05 Jy ! Total flux subtracted in 200 components = 4.5127e-05 Jy ! Clean residual min=-0.001013 max=0.000916 Jy/beam ! Clean residual mean=-0.000002 rms=0.000211 Jy/beam ! Combined flux in latest and established models = 0.142039 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 53 components and 0.142039 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=0.086774Jy sigma=0.666056 ! Fit after self-cal, rms=0.086772Jy sigma=0.666049 ! Inverting map ! Your choice of large map pixels excluded 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 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=0.086772Jy sigma=0.666049 ! Fit after self-cal, rms=0.086816Jy sigma=0.665999 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 milli-arcsec ! Estimated beam: bmin=2.683 mas, bmaj=2.912 mas, bpa=45.92 degrees ! Estimated noise=0.41042 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000129268 Jy ! Component: 100 - total flux cleaned = 0.000112445 Jy ! Component: 150 - total flux cleaned = 9.82543e-05 Jy ! Component: 200 - total flux cleaned = 8.08838e-05 Jy ! Total flux subtracted in 200 components = 8.08838e-05 Jy ! Clean residual min=-0.001226 max=0.000986 Jy/beam ! Clean residual mean=-0.000005 rms=0.000273 Jy/beam ! Combined flux in latest and established models = 0.14212 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 65 components and 0.14212 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=0.086817Jy sigma=0.665997 ! Fit after self-cal, rms=0.086819Jy sigma=0.665989 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 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 = -1.43846e-07 Jy ! Component: 100 - total flux cleaned = -1.13004e-05 Jy ! Component: 150 - total flux cleaned = -2.09653e-05 Jy ! Component: 200 - total flux cleaned = -2.9662e-05 Jy ! Total flux subtracted in 200 components = -2.9662e-05 Jy ! Clean residual min=-0.001226 max=0.000989 Jy/beam ! Clean residual mean=-0.000005 rms=0.000273 Jy/beam ! Combined flux in latest and established models = 0.14209 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 71 components and 0.14209 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=0.086819Jy sigma=0.665993 ! Fit after self-cal, rms=0.086819Jy sigma=0.665994 ! Inverting map ! Your choice of large map pixels excluded 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 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 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 milli-arcsec ! Estimated beam: bmin=0.5807 mas, bmaj=0.8531 mas, bpa=-20.8 degrees ! Estimated noise=0.304703 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5807 x 0.8531 at -20.8 degrees (North through East) ! Clean map min=-0.0008648 max=0.12466 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 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 milli-arcsec ! Estimated beam: bmin=0.4301 mas, bmaj=0.6315 mas, bpa=-23.58 degrees ! Estimated noise=0.650255 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0966545 Jy ! Component: 100 - total flux cleaned = 0.117856 Jy ! Component: 150 - total flux cleaned = 0.125471 Jy ! Component: 200 - total flux cleaned = 0.130086 Jy ! Total flux subtracted in 200 components = 0.130086 Jy ! Clean residual min=-0.001993 max=0.002426 Jy/beam ! Clean residual mean=0.000001 rms=0.000453 Jy/beam ! Combined flux in latest and established models = 0.130086 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 0.130086 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 milli-arcsec ! Estimated beam: bmin=0.5807 mas, bmaj=0.8531 mas, bpa=-20.8 degrees ! Estimated noise=0.304703 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 = 0.00510032 Jy ! Component: 100 - total flux cleaned = 0.00770049 Jy ! Component: 150 - total flux cleaned = 0.00934787 Jy ! Component: 200 - total flux cleaned = 0.0105018 Jy ! Total flux subtracted in 200 components = 0.0105018 Jy ! Clean residual min=-0.001042 max=0.000857 Jy/beam ! Clean residual mean=-0.000001 rms=0.000213 Jy/beam ! Combined flux in latest and established models = 0.140588 Jy ! Adding 22 model components to the UV plane model. ! The established model now contains 28 components and 0.140588 Jy ! Inverting map ! Your choice of large map pixels excluded 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 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 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 milli-arcsec ! Estimated beam: bmin=2.683 mas, bmaj=2.912 mas, bpa=45.92 degrees ! Estimated noise=0.41042 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00102212 Jy ! Component: 100 - total flux cleaned = 0.00139632 Jy ! Component: 150 - total flux cleaned = 0.00146509 Jy ! Component: 200 - total flux cleaned = 0.00149368 Jy ! Total flux subtracted in 200 components = 0.00149368 Jy ! Clean residual min=-0.001212 max=0.001008 Jy/beam ! Clean residual mean=-0.000005 rms=0.000273 Jy/beam ! Combined flux in latest and established models = 0.142082 Jy flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 8.09129e-06 Jy ! Component: 100 - total flux cleaned = 8.42096e-06 Jy ! Component: 150 - total flux cleaned = 8.55346e-06 Jy ! Component: 200 - total flux cleaned = 8.5191e-06 Jy ! Total flux subtracted in 200 components = 8.5191e-06 Jy ! Clean residual min=-0.001219 max=0.001007 Jy/beam ! Clean residual mean=-0.000005 rms=0.000273 Jy/beam ! Combined flux in latest and established models = 0.14209 Jy ! Adding 23 model components to the UV plane model. ! The established model now contains 48 components and 0.14209 Jy ! Inverting map ! Your choice of large map pixels excluded 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 milli-arcsec ! Estimated beam: bmin=0.5807 mas, bmaj=0.8531 mas, bpa=-20.8 degrees ! Estimated noise=0.304703 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000126589 Jy ! Component: 100 - total flux cleaned = 0.000128972 Jy ! Component: 150 - total flux cleaned = 0.000111496 Jy ! Component: 200 - total flux cleaned = 0.00012745 Jy ! Total flux subtracted in 200 components = 0.00012745 Jy ! Clean residual min=-0.000999 max=0.000851 Jy/beam ! Clean residual mean=-0.000002 rms=0.000208 Jy/beam ! Combined flux in latest and established models = 0.142218 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 58 components and 0.142218 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=0.086801Jy sigma=0.665934 ! Fit after self-cal, rms=0.086787Jy sigma=0.665881 wmodel /scr/pima/gb073_uvs/J1819+5511_X_map.mod ! Writing 58 model components to file: /scr/pima/gb073_uvs/J1819+5511_X_map.mod wobs /scr/pima/gb073_uvs/J1819+5511_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1819+5511_X_uvs.fits wwins /scr/pima/gb073_uvs/J1819+5511_X_map.win ! wwins: Wrote 4 windows to /scr/pima/gb073_uvs/J1819+5511_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 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000339013 Jy ! Component: 100 - total flux cleaned = -0.000405557 Jy ! Component: 150 - total flux cleaned = -0.00035843 Jy ! Component: 200 - total flux cleaned = -0.000296384 Jy ! Component: 250 - total flux cleaned = -0.000266081 Jy ! Component: 300 - total flux cleaned = -0.000310608 Jy ! Component: 350 - total flux cleaned = -0.000251687 Jy ! Component: 400 - total flux cleaned = -0.000222829 Jy ! Component: 450 - total flux cleaned = -0.00020869 Jy ! Component: 500 - total flux cleaned = -0.000180468 Jy ! Component: 550 - total flux cleaned = -0.000138467 Jy ! Component: 600 - total flux cleaned = -9.69714e-05 Jy ! Component: 650 - total flux cleaned = -4.22287e-05 Jy ! Component: 700 - total flux cleaned = 1.19541e-05 Jy ! Component: 750 - total flux cleaned = 5.23718e-05 Jy ! Component: 800 - total flux cleaned = 0.000106046 Jy ! Component: 850 - total flux cleaned = 0.000172277 Jy ! Component: 900 - total flux cleaned = 0.00026425 Jy ! Component: 950 - total flux cleaned = 0.000225137 Jy ! Component: 1000 - total flux cleaned = 0.000303127 Jy ! Component: 1050 - total flux cleaned = 0.000316094 Jy ! Component: 1100 - total flux cleaned = 0.000354481 Jy ! Component: 1150 - total flux cleaned = 0.00036733 Jy ! Component: 1200 - total flux cleaned = 0.000405265 Jy ! Component: 1250 - total flux cleaned = 0.000392597 Jy ! Component: 1300 - total flux cleaned = 0.000455248 Jy ! Component: 1350 - total flux cleaned = 0.000430287 Jy ! Component: 1400 - total flux cleaned = 0.000442663 Jy ! Component: 1450 - total flux cleaned = 0.000491993 Jy ! Component: 1500 - total flux cleaned = 0.000479822 Jy ! Component: 1550 - total flux cleaned = 0.000504237 Jy ! Component: 1600 - total flux cleaned = 0.000528548 Jy ! Component: 1650 - total flux cleaned = 0.000576982 Jy ! Component: 1700 - total flux cleaned = 0.000649308 Jy ! Component: 1750 - total flux cleaned = 0.000625239 Jy ! Component: 1800 - total flux cleaned = 0.000613368 Jy ! Component: 1850 - total flux cleaned = 0.000672933 Jy ! Component: 1900 - total flux cleaned = 0.000732365 Jy ! Component: 1950 - total flux cleaned = 0.000815094 Jy ! Component: 2000 - total flux cleaned = 0.000767888 Jy ! Component: 2050 - total flux cleaned = 0.000779689 Jy ! Component: 2100 - total flux cleaned = 0.000838144 Jy ! Component: 2150 - total flux cleaned = 0.000896459 Jy ! Component: 2200 - total flux cleaned = 0.000907978 Jy ! Component: 2250 - total flux cleaned = 0.000919481 Jy ! Component: 2300 - total flux cleaned = 0.000977112 Jy ! Component: 2350 - total flux cleaned = 0.000988629 Jy ! Component: 2400 - total flux cleaned = 0.00100012 Jy ! Component: 2450 - total flux cleaned = 0.00100009 Jy ! Component: 2500 - total flux cleaned = 0.00106836 Jy ! Component: 2550 - total flux cleaned = 0.00111374 Jy ! Component: 2600 - total flux cleaned = 0.00115893 Jy ! Component: 2650 - total flux cleaned = 0.00114763 Jy ! Component: 2700 - total flux cleaned = 0.00114757 Jy ! Component: 2750 - total flux cleaned = 0.0012372 Jy ! Component: 2800 - total flux cleaned = 0.00124834 Jy ! Component: 2850 - total flux cleaned = 0.00131514 Jy ! Component: 2900 - total flux cleaned = 0.00130411 Jy ! Component: 2950 - total flux cleaned = 0.00138157 Jy ! Component: 3000 - total flux cleaned = 0.00141466 Jy ! Component: 3050 - total flux cleaned = 0.00146969 Jy ! Component: 3100 - total flux cleaned = 0.00153555 Jy ! Component: 3150 - total flux cleaned = 0.00153555 Jy ! Component: 3200 - total flux cleaned = 0.00152465 Jy ! Component: 3250 - total flux cleaned = 0.00148114 Jy ! Component: 3300 - total flux cleaned = 0.00164392 Jy ! Component: 3350 - total flux cleaned = 0.00168719 Jy ! Component: 3400 - total flux cleaned = 0.00177348 Jy ! Component: 3450 - total flux cleaned = 0.00175202 Jy ! Component: 3500 - total flux cleaned = 0.00180563 Jy ! Component: 3550 - total flux cleaned = 0.00188059 Jy ! Component: 3600 - total flux cleaned = 0.00189127 Jy ! Component: 3650 - total flux cleaned = 0.00191255 Jy ! Component: 3700 - total flux cleaned = 0.00194441 Jy ! Component: 3750 - total flux cleaned = 0.00198675 Jy ! Component: 3800 - total flux cleaned = 0.00198675 Jy ! Component: 3850 - total flux cleaned = 0.00204996 Jy ! Component: 3900 - total flux cleaned = 0.00207098 Jy ! Component: 3950 - total flux cleaned = 0.0021234 Jy ! Component: 4000 - total flux cleaned = 0.00214433 Jy ! Component: 4050 - total flux cleaned = 0.0021756 Jy ! Total flux subtracted in 4096 components = 0.00220678 Jy ! Clean residual min=-0.000631 max=0.000590 Jy/beam ! Clean residual mean=-0.000001 rms=0.000170 Jy/beam ! Combined flux in latest and established models = 0.144424 Jy keep ! Adding 387 model components to the UV plane model. ! The established model now contains 445 components and 0.144424 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1819+5511_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5807 x 0.8531 at -20.8 degrees (North through East) ! Clean map min=-0.00073497 max=0.12501 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1819+5511_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.125011 invert ! Inverting map ! Your choice of large map pixels excluded 3.03% of the data. ! The x-axis pixel size should ideally be below 0.177 milli-arcsec ! The y-axis pixel size should ideally be below 0.1805 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00016966 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.407146 0.407146 0.814292 1.62858 3.25717 6.51434 13.0287 26.0574 52.1147 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0005 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.125 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 736.836 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1819+5511_X_uvs.log closed on Sat Dec 26 09:44:02 2015