! Started logfile: /scr/pima/gb073_uvs/J1838+5735_X_uvs.log on Sat Dec 26 09:44:24 2015 obs /scr/pima/gb073_uvs/J1838+5735_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1838+5735_X_uva.fits ! AN table 1: 29 integrations on 45 of 45 possible baselines. ! AN table 2: 29 integrations on 66 of 66 possible baselines. ! AN table 3: 58 integrations on 66 of 66 possible baselines. ! AN table 4: 29 integrations on 36 of 36 possible baselines. ! Apparent sampling: 0.895934 visibilities/baseline/integration-bin. ! Found source: J1838+5735 ! ! 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 57992 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/J1838+5735_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 58 telescope corrections were flagged in sub-array 3. ! A total of 29 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 58 telescope corrections were flagged in sub-array 3. ! A total of 29 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 58 telescope corrections were flagged in sub-array 3. ! A total of 29 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 58 telescope corrections were flagged in sub-array 3. ! A total of 29 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 116 telescope corrections were flagged in sub-array 3. ! A total of 58 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 116 telescope corrections were flagged in sub-array 3. ! A total of 58 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 58 telescope corrections were flagged in sub-array 3. ! A total of 29 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 58 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=1.006101Jy sigma=10.298490 ! Fit after self-cal, rms=0.932813Jy sigma=9.545936 ! 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 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 milli-arcsec ! Estimated beam: bmin=0.4109 mas, bmaj=0.7434 mas, bpa=-40.93 degrees ! Estimated noise=0.718688 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 = 0.0534017 Jy ! Component: 100 - total flux cleaned = 0.066396 Jy ! Total flux subtracted in 100 components = 0.066396 Jy ! Clean residual min=-0.004307 max=0.005942 Jy/beam ! Clean residual mean=-0.000000 rms=0.000598 Jy/beam ! Combined flux in latest and established models = 0.066396 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 0.066396 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=0.080983Jy sigma=0.685762 ! Fit after self-cal, rms=0.080215Jy sigma=0.678890 ! Inverting map ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00597961 Jy ! Component: 100 - total flux cleaned = 0.00666653 Jy ! Total flux subtracted in 100 components = 0.00666653 Jy ! Clean residual min=-0.003876 max=0.004253 Jy/beam ! Clean residual mean=-0.000000 rms=0.000566 Jy/beam ! Combined flux in latest and established models = 0.0730626 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 9 components and 0.0730626 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=0.079713Jy sigma=0.673445 ! Fit after self-cal, rms=0.079705Jy sigma=0.673376 ! Inverting map ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 milli-arcsec ! Added new window around map position (0.2, 0.8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00080834 Jy ! Component: 100 - total flux cleaned = 0.000911234 Jy ! Total flux subtracted in 100 components = 0.000911234 Jy ! Clean residual min=-0.002917 max=0.003579 Jy/beam ! Clean residual mean=-0.000000 rms=0.000553 Jy/beam ! Combined flux in latest and established models = 0.0739738 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 14 components and 0.0739738 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=0.079548Jy sigma=0.672124 ! Fit after self-cal, rms=0.079525Jy sigma=0.671965 ! Inverting map ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 milli-arcsec ! Added new window around map position (1, -1). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00247853 Jy ! Component: 100 - total flux cleaned = 0.00317882 Jy ! Total flux subtracted in 100 components = 0.00317882 Jy ! Clean residual min=-0.002559 max=0.002812 Jy/beam ! Clean residual mean=-0.000000 rms=0.000544 Jy/beam ! Combined flux in latest and established models = 0.0771526 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 20 components and 0.0771526 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=0.079388Jy sigma=0.670595 ! Fit after self-cal, rms=0.079371Jy sigma=0.670416 ! Inverting map ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 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 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 milli-arcsec ! Estimated beam: bmin=0.5844 mas, bmaj=0.9855 mas, bpa=-38.11 degrees ! Estimated noise=0.320165 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 = 0.00209091 Jy ! Component: 100 - total flux cleaned = 0.00258931 Jy ! Component: 150 - total flux cleaned = 0.00269267 Jy ! Component: 200 - total flux cleaned = 0.00275345 Jy ! Total flux subtracted in 200 components = 0.00275345 Jy ! Clean residual min=-0.001151 max=0.001534 Jy/beam ! Clean residual mean=-0.000002 rms=0.000253 Jy/beam ! Combined flux in latest and established models = 0.0799061 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 22 components and 0.0799061 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=0.079300Jy sigma=0.669753 ! Fit after self-cal, rms=0.079288Jy sigma=0.669637 ! Inverting map ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 milli-arcsec ! Added new window around map position (3, -1.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00140835 Jy ! Component: 100 - total flux cleaned = 0.00176225 Jy ! Component: 150 - total flux cleaned = 0.00185121 Jy ! Component: 200 - total flux cleaned = 0.00190511 Jy ! Total flux subtracted in 200 components = 0.00190511 Jy ! Clean residual min=-0.001193 max=0.001102 Jy/beam ! Clean residual mean=-0.000002 rms=0.000243 Jy/beam ! Combined flux in latest and established models = 0.0818112 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 31 components and 0.0818112 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=0.079248Jy sigma=0.669279 ! Fit after self-cal, rms=0.079242Jy sigma=0.669239 ! Inverting map ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5844 x 0.9855 at -38.11 degrees (North through East) ! Clean map min=-0.0025051 max=0.067431 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 0.99 EF 1.00* FD 0.97 KP 0.96 ! LA 1.03 MK 0.97 NL 1.02 OV 0.97 ! PT 0.93 ZC 0.97 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 EF 1.00* FD 0.99 KP 1.01 ! LA 1.08 MK 0.99 NL 0.94 ON 1.03 ! OV 1.00 PT 0.94 SC 0.92 ZC 0.86 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.96 EF 1.00* FD 0.97 KP 1.06 ! LA 1.09 MC 0.94 NL 0.95 ON 0.95 ! OV 0.98 PT 0.92 SC 0.91 ZC 0.91 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.92 EF 1.00* KP 1.01 LA 1.07 ! MK 0.80 NL 0.93 OV 0.92 PT 1.02 ! ZC 1.06 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 EF 1.00* FD 1.02 KP 1.05 ! LA 1.10 MK 1.04 NL 0.99 OV 1.08 ! PT 0.96 ZC 0.90 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 EF 1.00* FD 0.99 KP 0.99 ! LA 1.10 MK 1.00 NL 0.97 ON 1.09 ! OV 1.03 PT 1.03 SC 0.95 ZC 1.01 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 EF 1.00* FD 1.06 KP 1.09 ! LA 1.06 MC 1.01 NL 1.00 ON 1.03 ! OV 1.05 PT 1.08 SC 1.00 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 EF 1.00* KP 1.03 LA 1.05 ! MK 1.01 NL 0.97 OV 1.01 PT 0.96 ! ZC 1.02 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 EF 1.00* FD 1.02 KP 1.03 ! LA 0.93 MK 0.99 NL 0.96 OV 1.00 ! PT 1.02 ZC 0.97 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 EF 1.00* FD 1.00 KP 0.93 ! LA 0.95 MK 1.00 NL 0.98 ON 1.08 ! OV 0.94 PT 0.99 SC 0.88 ZC 0.92 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 EF 1.00* FD 1.01 KP 1.03 ! LA 1.03 MC 1.00 NL 0.95 ON 0.87 ! OV 1.00 PT 1.01 SC 1.03 ZC 0.88 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.95 EF 1.00* KP 0.99 LA 0.95 ! MK 0.92 NL 0.99 OV 0.97 PT 1.02 ! ZC 1.08 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 EF 1.00* FD 0.97 KP 1.01 ! LA 0.98 MK 1.01 NL 0.98 OV 1.00 ! PT 1.09 ZC 0.92 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 EF 1.00* FD 1.02 KP 1.05 ! LA 1.00 MK 1.02 NL 1.01 ON 1.05 ! OV 0.98 PT 1.05 SC 1.02 ZC 0.98 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 EF 1.00* FD 1.00 KP 1.04 ! LA 1.04 MC 1.00 NL 1.02 ON 0.89 ! OV 1.01 PT 1.04 SC 1.06 ZC 0.90 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 EF 1.00* KP 1.01 LA 1.01 ! MK 1.01 NL 0.97 OV 0.99 PT 1.02 ! ZC 0.99 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.94 KP 0.91 ! LA 0.96 MK 1.00 NL 1.02 OV 0.98 ! PT 0.97 ZC 1.03 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.07 KP 0.95 ! LA 1.00 MK 0.93 NL 0.96 ON 1.27 ! OV 1.11 PT 1.04 SC 0.88 ZC 0.94 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.01 KP 0.95 ! LA 1.07 MC 1.32 NL 1.01 ON 1.19 ! OV 1.09 PT 0.98 SC 1.03 ZC 0.90 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* KP 0.87 LA 1.05 ! MK 0.95 NL 0.92 OV 1.12 PT 1.07 ! ZC 0.96 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.99 KP 0.87 ! LA 0.96 MK 0.97 NL 1.03 OV 1.07 ! PT 0.88 ZC 0.98 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.02 KP 0.87 ! LA 0.95 MK 0.99 NL 0.97 ON 1.22 ! OV 1.10 PT 0.98 SC 1.02 ZC 0.88 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.04 KP 0.91 ! LA 1.04 MC 1.26 NL 1.02 ON 1.15 ! OV 1.05 PT 0.97 SC 1.01 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* KP 0.85 LA 1.10 ! MK 1.05 NL 0.94 OV 1.01 PT 0.92 ! ZC 0.99 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 EF 1.00* FD 1.13 KP 0.87 ! LA 1.08 MK 0.96 NL 1.06 OV 0.98 ! PT 0.98 ZC 0.71 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 EF 1.00* FD 1.05 KP 0.93 ! LA 1.03 MK 1.03 NL 1.00 ON 1.47 ! OV 0.97 PT 0.95 SC 0.97 ZC 0.75 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.05 EF 1.00* FD 1.06 KP 0.94 ! LA 1.05 MC 1.21 NL 1.06 ON 1.31 ! OV 1.00 PT 1.01 SC 1.04 ZC 0.74 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 EF 1.00* KP 0.94 LA 1.02 ! MK 1.02 NL 1.11 OV 1.03 PT 0.99 ! ZC 0.75 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 EF 1.00* FD 1.05 KP 0.99 ! LA 0.94 MK 1.05 NL 1.07 OV 1.05 ! PT 0.93 ZC 0.73 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 EF 1.00* FD 1.03 KP 0.98 ! LA 0.96 MK 1.15 NL 0.98 ON 1.51 ! OV 0.97 PT 1.03 SC 1.01 ZC 0.73 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 EF 1.00* FD 1.04 KP 0.97 ! LA 1.10 MC 1.34 NL 1.00 ON 1.23 ! OV 0.96 PT 1.00 SC 1.02 ZC 0.72 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.05 EF 1.00* KP 0.92 LA 1.11 ! MK 1.07 NL 0.91 OV 0.95 PT 1.04 ! ZC 0.73 ! ! ! Fit before self-cal, rms=0.079242Jy sigma=0.669239 ! Fit after self-cal, rms=0.078890Jy sigma=0.664759 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 milli-arcsec ! Estimated beam: bmin=0.5801 mas, bmaj=0.9716 mas, bpa=-39 degrees ! Estimated noise=0.319909 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 = 0.000833889 Jy ! Component: 100 - total flux cleaned = 0.000982731 Jy ! Component: 150 - total flux cleaned = 0.00106459 Jy ! Component: 200 - total flux cleaned = 0.00117635 Jy ! Total flux subtracted in 200 components = 0.00117635 Jy ! Clean residual min=-0.000919 max=0.000895 Jy/beam ! Clean residual mean=-0.000001 rms=0.000205 Jy/beam ! Combined flux in latest and established models = 0.0829875 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 41 components and 0.0829876 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=0.078872Jy sigma=0.664618 ! Fit after self-cal, rms=0.078898Jy sigma=0.664377 ! Inverting map ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 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=0.078898Jy sigma=0.664377 ! Fit after self-cal, rms=0.079234Jy sigma=0.664034 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 milli-arcsec ! Estimated beam: bmin=0.5781 mas, bmaj=0.9701 mas, bpa=-39.24 degrees ! Estimated noise=0.3211 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000714093 Jy ! Component: 100 - total flux cleaned = 0.000755199 Jy ! Component: 150 - total flux cleaned = 0.000843069 Jy ! Component: 200 - total flux cleaned = 0.000890937 Jy ! Total flux subtracted in 200 components = 0.000890937 Jy ! Clean residual min=-0.000925 max=0.000889 Jy/beam ! Clean residual mean=-0.000001 rms=0.000204 Jy/beam ! Combined flux in latest and established models = 0.0838785 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 46 components and 0.0838785 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=0.079221Jy sigma=0.663945 ! Fit after self-cal, rms=0.079226Jy sigma=0.663920 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 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 = 0.000140232 Jy ! Component: 100 - total flux cleaned = 0.000183118 Jy ! Component: 150 - total flux cleaned = 0.00020985 Jy ! Component: 200 - total flux cleaned = 0.000235259 Jy ! Total flux subtracted in 200 components = 0.000235259 Jy ! Clean residual min=-0.000934 max=0.000913 Jy/beam ! Clean residual mean=-0.000001 rms=0.000203 Jy/beam ! Combined flux in latest and established models = 0.0841138 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 50 components and 0.0841138 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=0.079220Jy sigma=0.663881 ! Fit after self-cal, rms=0.079221Jy sigma=0.663880 ! Inverting map ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 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=0.079221Jy sigma=0.663880 ! Fit after self-cal, rms=0.080066Jy sigma=0.663860 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 milli-arcsec ! Estimated beam: bmin=0.5766 mas, bmaj=0.9689 mas, bpa=-39.49 degrees ! Estimated noise=0.323715 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000747057 Jy ! Component: 100 - total flux cleaned = 0.000910636 Jy ! Component: 150 - total flux cleaned = 0.000939009 Jy ! Component: 200 - total flux cleaned = 0.000965186 Jy ! Total flux subtracted in 200 components = 0.000965186 Jy ! Clean residual min=-0.000933 max=0.000887 Jy/beam ! Clean residual mean=-0.000001 rms=0.000204 Jy/beam ! Combined flux in latest and established models = 0.0850789 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 51 components and 0.0850789 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=0.080055Jy sigma=0.663790 ! Fit after self-cal, rms=0.080058Jy sigma=0.663780 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 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 = 0.000115611 Jy ! Component: 100 - total flux cleaned = 0.000127032 Jy ! Component: 150 - total flux cleaned = 0.000137762 Jy ! Component: 200 - total flux cleaned = 0.000158179 Jy ! Total flux subtracted in 200 components = 0.000158179 Jy ! Clean residual min=-0.000939 max=0.000909 Jy/beam ! Clean residual mean=-0.000001 rms=0.000204 Jy/beam ! Combined flux in latest and established models = 0.0852371 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 55 components and 0.0852371 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=0.080054Jy sigma=0.663759 ! Fit after self-cal, rms=0.080054Jy sigma=0.663755 ! Inverting map ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 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=0.080054Jy sigma=0.663755 ! Fit after self-cal, rms=0.080371Jy sigma=0.663722 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 milli-arcsec ! Estimated beam: bmin=2.527 mas, bmaj=2.981 mas, bpa=30.26 degrees ! Estimated noise=0.432585 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000684116 Jy ! Component: 100 - total flux cleaned = 0.000990817 Jy ! Component: 150 - total flux cleaned = 0.00105025 Jy ! Component: 200 - total flux cleaned = 0.00106144 Jy ! Total flux subtracted in 200 components = 0.00106144 Jy ! Clean residual min=-0.000999 max=0.000932 Jy/beam ! Clean residual mean=-0.000002 rms=0.000251 Jy/beam ! Combined flux in latest and established models = 0.0862985 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 64 components and 0.0862985 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=0.080365Jy sigma=0.663704 ! Fit after self-cal, rms=0.080360Jy sigma=0.663685 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 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 = 1.7473e-05 Jy ! Component: 100 - total flux cleaned = 4.88628e-05 Jy ! Component: 150 - total flux cleaned = 5.81931e-05 Jy ! Component: 200 - total flux cleaned = 6.23451e-05 Jy ! Total flux subtracted in 200 components = 6.23451e-05 Jy ! Clean residual min=-0.000999 max=0.000944 Jy/beam ! Clean residual mean=-0.000002 rms=0.000252 Jy/beam ! Combined flux in latest and established models = 0.0863609 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 66 components and 0.0863609 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=0.080360Jy sigma=0.663683 ! Fit after self-cal, rms=0.080358Jy sigma=0.663681 ! Inverting map ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 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 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 milli-arcsec ! Estimated beam: bmin=0.5745 mas, bmaj=0.9674 mas, bpa=-39.73 degrees ! Estimated noise=0.325474 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5745 x 0.9674 at -39.73 degrees (North through East) ! Clean map min=-0.0010498 max=0.067947 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 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 milli-arcsec ! Estimated beam: bmin=0.4051 mas, bmaj=0.7328 mas, bpa=-42.53 degrees ! Estimated noise=0.71402 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0537346 Jy ! Component: 100 - total flux cleaned = 0.0674554 Jy ! Component: 150 - total flux cleaned = 0.0736824 Jy ! Component: 200 - total flux cleaned = 0.0768925 Jy ! Total flux subtracted in 200 components = 0.0768925 Jy ! Clean residual min=-0.002090 max=0.002186 Jy/beam ! Clean residual mean=-0.000000 rms=0.000491 Jy/beam ! Combined flux in latest and established models = 0.0768925 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 14 model components to the UV plane model. ! The established model now contains 14 components and 0.0768925 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 milli-arcsec ! Estimated beam: bmin=0.5745 mas, bmaj=0.9674 mas, bpa=-39.73 degrees ! Estimated noise=0.325474 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 = 0.00405417 Jy ! Component: 100 - total flux cleaned = 0.00608541 Jy ! Component: 150 - total flux cleaned = 0.00708124 Jy ! Component: 200 - total flux cleaned = 0.00749814 Jy ! Total flux subtracted in 200 components = 0.00749814 Jy ! Clean residual min=-0.000952 max=0.001006 Jy/beam ! Clean residual mean=-0.000001 rms=0.000216 Jy/beam ! Combined flux in latest and established models = 0.0843906 Jy ! Adding 19 model components to the UV plane model. ! The established model now contains 24 components and 0.0843906 Jy ! Inverting map ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 milli-arcsec ! Added new window around map position (-7.4, 23.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000540917 Jy ! Component: 100 - total flux cleaned = 0.000883994 Jy ! Component: 150 - total flux cleaned = 0.00115496 Jy ! Component: 200 - total flux cleaned = 0.0013945 Jy ! Total flux subtracted in 200 components = 0.0013945 Jy ! Clean residual min=-0.000931 max=0.000910 Jy/beam ! Clean residual mean=-0.000001 rms=0.000207 Jy/beam ! Combined flux in latest and established models = 0.0857851 Jy ! Adding 23 model components to the UV plane model. ! The established model now contains 35 components and 0.0857851 Jy ! Inverting map ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 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 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 milli-arcsec ! Estimated beam: bmin=2.527 mas, bmaj=2.981 mas, bpa=30.26 degrees ! Estimated noise=0.432585 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00075943 Jy ! Component: 100 - total flux cleaned = 0.00118886 Jy ! Component: 150 - total flux cleaned = 0.00130283 Jy ! Component: 200 - total flux cleaned = 0.00131161 Jy ! Total flux subtracted in 200 components = 0.00131161 Jy ! Clean residual min=-0.000984 max=0.000935 Jy/beam ! Clean residual mean=-0.000002 rms=0.000247 Jy/beam ! Combined flux in latest and established models = 0.0870967 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 = 7.92356e-06 Jy ! Component: 100 - total flux cleaned = 1.50976e-05 Jy ! Component: 150 - total flux cleaned = 2.13031e-05 Jy ! Component: 200 - total flux cleaned = 2.10078e-05 Jy ! Total flux subtracted in 200 components = 2.10078e-05 Jy ! Clean residual min=-0.001001 max=0.000946 Jy/beam ! Clean residual mean=-0.000002 rms=0.000246 Jy/beam ! Combined flux in latest and established models = 0.0871178 Jy ! Adding 17 model components to the UV plane model. ! The established model now contains 49 components and 0.0871178 Jy ! Inverting map ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 milli-arcsec ! Estimated beam: bmin=0.5745 mas, bmaj=0.9674 mas, bpa=-39.73 degrees ! Estimated noise=0.325474 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000146038 Jy ! Component: 100 - total flux cleaned = -0.000146085 Jy ! Component: 150 - total flux cleaned = -0.000165158 Jy ! Component: 200 - total flux cleaned = -0.000182345 Jy ! Total flux subtracted in 200 components = -0.000182345 Jy ! Clean residual min=-0.000939 max=0.000873 Jy/beam ! Clean residual mean=-0.000001 rms=0.000202 Jy/beam ! Combined flux in latest and established models = 0.0869354 Jy selfcal ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 62 components and 0.0869354 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=0.080357Jy sigma=0.663714 ! Fit after self-cal, rms=0.080352Jy sigma=0.663674 wmodel /scr/pima/gb073_uvs/J1838+5735_X_map.mod ! Writing 62 model components to file: /scr/pima/gb073_uvs/J1838+5735_X_map.mod wobs /scr/pima/gb073_uvs/J1838+5735_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1838+5735_X_uvs.fits wwins /scr/pima/gb073_uvs/J1838+5735_X_map.win ! wwins: Wrote 5 windows to /scr/pima/gb073_uvs/J1838+5735_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 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -7.66031e-05 Jy ! Component: 100 - total flux cleaned = -2.97365e-05 Jy ! Component: 150 - total flux cleaned = -1.46272e-05 Jy ! Component: 200 - total flux cleaned = -2.95039e-05 Jy ! Component: 250 - total flux cleaned = -8.79148e-05 Jy ! Component: 300 - total flux cleaned = -0.000188398 Jy ! Component: 350 - total flux cleaned = -0.000188728 Jy ! Component: 400 - total flux cleaned = -0.000245003 Jy ! Component: 450 - total flux cleaned = -0.000300245 Jy ! Component: 500 - total flux cleaned = -0.000341145 Jy ! Component: 550 - total flux cleaned = -0.000381851 Jy ! Component: 600 - total flux cleaned = -0.000435389 Jy ! Component: 650 - total flux cleaned = -0.000461882 Jy ! Component: 700 - total flux cleaned = -0.000527814 Jy ! Component: 750 - total flux cleaned = -0.000554036 Jy ! Component: 800 - total flux cleaned = -0.000632009 Jy ! Component: 850 - total flux cleaned = -0.000696461 Jy ! Component: 900 - total flux cleaned = -0.000760401 Jy ! Component: 950 - total flux cleaned = -0.000798531 Jy ! Component: 1000 - total flux cleaned = -0.000849162 Jy ! Component: 1050 - total flux cleaned = -0.00084925 Jy ! Component: 1100 - total flux cleaned = -0.000911536 Jy ! Component: 1150 - total flux cleaned = -0.000973391 Jy ! Component: 1200 - total flux cleaned = -0.000936416 Jy ! Component: 1250 - total flux cleaned = -0.000997588 Jy ! Component: 1300 - total flux cleaned = -0.00100974 Jy ! Component: 1350 - total flux cleaned = -0.00107024 Jy ! Component: 1400 - total flux cleaned = -0.00110639 Jy ! Component: 1450 - total flux cleaned = -0.00114235 Jy ! Component: 1500 - total flux cleaned = -0.00121391 Jy ! Component: 1550 - total flux cleaned = -0.00122579 Jy ! Component: 1600 - total flux cleaned = -0.00124931 Jy ! Component: 1650 - total flux cleaned = -0.00127277 Jy ! Component: 1700 - total flux cleaned = -0.00128447 Jy ! Component: 1750 - total flux cleaned = -0.0013543 Jy ! Component: 1800 - total flux cleaned = -0.00134267 Jy ! Component: 1850 - total flux cleaned = -0.00140025 Jy ! Component: 1900 - total flux cleaned = -0.00137731 Jy ! Component: 1950 - total flux cleaned = -0.00141162 Jy ! Component: 2000 - total flux cleaned = -0.00145713 Jy ! Component: 2050 - total flux cleaned = -0.00143447 Jy ! Component: 2100 - total flux cleaned = -0.00147957 Jy ! Component: 2150 - total flux cleaned = -0.00145711 Jy ! Component: 2200 - total flux cleaned = -0.00153538 Jy ! Component: 2250 - total flux cleaned = -0.0015689 Jy ! Component: 2300 - total flux cleaned = -0.00154675 Jy ! Component: 2350 - total flux cleaned = -0.00160202 Jy ! Component: 2400 - total flux cleaned = -0.001646 Jy ! Component: 2450 - total flux cleaned = -0.00168987 Jy ! Component: 2500 - total flux cleaned = -0.0016899 Jy ! Component: 2550 - total flux cleaned = -0.00167906 Jy ! Component: 2600 - total flux cleaned = -0.00168984 Jy ! Component: 2650 - total flux cleaned = -0.00172233 Jy ! Component: 2700 - total flux cleaned = -0.00170077 Jy ! Component: 2750 - total flux cleaned = -0.0017974 Jy ! Component: 2800 - total flux cleaned = -0.00175457 Jy ! Component: 2850 - total flux cleaned = -0.00175451 Jy ! Component: 2900 - total flux cleaned = -0.00174389 Jy ! Component: 2950 - total flux cleaned = -0.00180746 Jy ! Component: 3000 - total flux cleaned = -0.00184972 Jy ! Component: 3050 - total flux cleaned = -0.00183922 Jy ! Component: 3100 - total flux cleaned = -0.00184968 Jy ! Component: 3150 - total flux cleaned = -0.00187058 Jy ! Component: 3200 - total flux cleaned = -0.00192271 Jy ! Component: 3250 - total flux cleaned = -0.00190187 Jy ! Component: 3300 - total flux cleaned = -0.00190182 Jy ! Component: 3350 - total flux cleaned = -0.00193293 Jy ! Component: 3400 - total flux cleaned = -0.00195349 Jy ! Component: 3450 - total flux cleaned = -0.00197407 Jy ! Component: 3500 - total flux cleaned = -0.0020355 Jy ! Component: 3550 - total flux cleaned = -0.00202535 Jy ! Component: 3600 - total flux cleaned = -0.00207629 Jy ! Component: 3650 - total flux cleaned = -0.00209656 Jy ! Component: 3700 - total flux cleaned = -0.0021573 Jy ! Component: 3750 - total flux cleaned = -0.00213709 Jy ! Component: 3800 - total flux cleaned = -0.00218749 Jy ! Component: 3850 - total flux cleaned = -0.00222766 Jy ! Component: 3900 - total flux cleaned = -0.00225768 Jy ! Component: 3950 - total flux cleaned = -0.00218774 Jy ! Component: 4000 - total flux cleaned = -0.00223755 Jy ! Component: 4050 - total flux cleaned = -0.0022773 Jy ! Total flux subtracted in 4096 components = -0.00226733 Jy ! Clean residual min=-0.000558 max=0.000541 Jy/beam ! Clean residual mean=-0.000000 rms=0.000162 Jy/beam ! Combined flux in latest and established models = 0.0846681 Jy keep ! Adding 345 model components to the UV plane model. ! The established model now contains 407 components and 0.0846681 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1838+5735_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5745 x 0.9674 at -39.73 degrees (North through East) ! Clean map min=-0.00081617 max=0.068205 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1838+5735_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0682052 invert ! Inverting map ! Your choice of large map pixels excluded 0.661% of the data. ! The x-axis pixel size should ideally be below 0.1862 milli-arcsec ! The y-axis pixel size should ideally be below 0.196 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000162109 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.713035 0.713035 1.42607 2.85214 5.70428 11.4086 22.8171 45.6342 91.2685 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0004 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.068 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 420.736 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1838+5735_X_uvs.log closed on Sat Dec 26 09:44:31 2015