! Started logfile: /scr/pima/gb073_uvs/J1203+4510_X_uvs.log on Sat Dec 26 09:37:41 2015 obs /scr/pima/gb073_uvs/J1203+4510_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1203+4510_X_uva.fits ! AN table 1: 29 integrations on 66 of 66 possible baselines. ! AN table 2: 29 integrations on 66 of 66 possible baselines. ! AN table 3: 29 integrations on 66 of 66 possible baselines. ! AN table 4: 29 integrations on 55 of 55 possible baselines. ! AN table 5: 29 integrations on 36 of 36 possible baselines. ! Apparent sampling: 0.952989 visibilities/baseline/integration-bin. ! Found source: J1203+4510 ! ! 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 63896 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/J1203+4510_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 30 telescope corrections were flagged in sub-array 2. ! A total of 30 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 30 telescope corrections were flagged in sub-array 2. ! A total of 30 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 30 telescope corrections were flagged in sub-array 2. ! A total of 30 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 30 telescope corrections were flagged in sub-array 2. ! A total of 30 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 59 telescope corrections were flagged in sub-array 2. ! A total of 59 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 6. ! A total of 58 telescope corrections were flagged in sub-array 1. ! A total of 59 telescope corrections were flagged in sub-array 2. ! A total of 59 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 7. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 30 telescope corrections were flagged in sub-array 2. ! A total of 30 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 30 telescope corrections were flagged in sub-array 2. ! A total of 30 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=1.008055Jy sigma=9.695546 ! Fit after self-cal, rms=0.927428Jy sigma=8.897117 ! 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 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Estimated beam: bmin=0.485 mas, bmaj=0.7601 mas, bpa=-21.46 degrees ! Estimated noise=0.759698 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 = 0.0575038 Jy ! Component: 100 - total flux cleaned = 0.0713136 Jy ! Total flux subtracted in 100 components = 0.0713136 Jy ! Clean residual min=-0.003161 max=0.005731 Jy/beam ! Clean residual mean=-0.000001 rms=0.000616 Jy/beam ! Combined flux in latest and established models = 0.0713136 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 0.0713136 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=0.088715Jy sigma=0.682430 ! Fit after self-cal, rms=0.088240Jy sigma=0.678803 ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00659605 Jy ! Component: 100 - total flux cleaned = 0.0100761 Jy ! Total flux subtracted in 100 components = 0.0100761 Jy ! Clean residual min=-0.003286 max=0.002921 Jy/beam ! Clean residual mean=-0.000000 rms=0.000567 Jy/beam ! Combined flux in latest and established models = 0.0813897 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 9 components and 0.0813897 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=0.087683Jy sigma=0.671491 ! Fit after self-cal, rms=0.087694Jy sigma=0.671414 ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 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 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Estimated beam: bmin=0.6692 mas, bmaj=1 mas, bpa=-16.4 degrees ! Estimated noise=0.334149 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 = 0.00247271 Jy ! Component: 100 - total flux cleaned = 0.00357847 Jy ! Component: 150 - total flux cleaned = 0.00393966 Jy ! Component: 200 - total flux cleaned = 0.00401114 Jy ! Total flux subtracted in 200 components = 0.00401114 Jy ! Clean residual min=-0.001458 max=0.001387 Jy/beam ! Clean residual mean=0.000002 rms=0.000273 Jy/beam ! Combined flux in latest and established models = 0.0854008 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 15 components and 0.0854008 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=0.087640Jy sigma=0.670860 ! Fit after self-cal, rms=0.087643Jy sigma=0.670834 ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6692 x 1 at -16.4 degrees (North through East) ! Clean map min=-0.0011029 max=0.076289 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 0.98 KP 1.04 ! LA 1.06 MC 1.04 MK 0.98 NL 0.96 ! OV 0.99 PT 0.99 SC 0.80 ZC 0.81 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.95 EF 1.00* FD 0.93 KP 1.03 ! LA 1.06 MC 0.88 NL 0.92 ON 0.94 ! OV 1.09 PT 0.94 SC 0.95 ZC 0.81 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 EF 1.00* FD 0.98 KP 1.02 ! LA 1.04 MC 0.96 MK 0.98 NL 0.95 ! ON 1.04 OV 0.97 PT 0.96 SC 0.94 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.91 EF 1.00* FD 0.97 KP 1.01 ! LA 1.04 MC 1.03 MK 1.06 NL 0.90 ! ON 0.92 PT 0.98 SC 0.96 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.95 FD 1.01 KP 0.99 LA 1.01 ! MK 0.93 NL 0.95 ON 0.89 OV 1.01 ! PT 0.93 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 EF 1.00* FD 1.00 KP 1.03 ! LA 1.03 MC 0.99 MK 1.02 NL 1.07 ! OV 1.01 PT 1.03 SC 0.85 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 EF 1.00* FD 0.94 KP 0.97 ! LA 1.12 MC 0.96 NL 1.00 ON 1.02 ! OV 1.08 PT 1.12 SC 0.95 ZC 0.83 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 EF 1.00* FD 1.12 KP 0.97 ! LA 1.08 MC 1.18 MK 1.07 NL 0.96 ! ON 0.99 OV 1.04 PT 1.05 SC 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 EF 1.00* FD 1.04 KP 1.01 ! LA 1.12 MC 1.01 MK 0.97 NL 0.96 ! ON 1.00 PT 1.08 SC 0.91 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 FD 1.03 KP 1.02 LA 1.04 ! MK 0.97 NL 0.99 ON 1.01 OV 1.03 ! PT 1.04 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 EF 1.00* FD 1.06 KP 0.94 ! LA 0.99 MC 1.00 MK 0.96 NL 1.00 ! OV 0.99 PT 1.02 SC 0.81 ZC 0.76 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 EF 1.00* FD 1.00 KP 0.97 ! LA 0.97 MC 1.04 NL 0.95 ON 1.06 ! OV 0.97 PT 1.03 SC 0.91 ZC 0.79 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 EF 1.00* FD 0.96 KP 0.99 ! LA 0.96 MC 1.02 MK 0.99 NL 0.94 ! ON 1.03 OV 1.00 PT 0.98 SC 1.06 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.93 EF 1.00* FD 1.02 KP 1.03 ! LA 0.96 MC 0.96 MK 0.96 NL 0.95 ! ON 0.97 PT 1.02 SC 0.99 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.06 FD 1.07 KP 0.95 LA 0.96 ! MK 0.90 NL 0.97 ON 0.86 OV 1.01 ! PT 1.00 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 EF 1.00* FD 1.05 KP 1.05 ! LA 0.99 MC 1.04 MK 1.04 NL 1.01 ! OV 0.95 PT 1.04 SC 0.76 ZC 0.75 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.09 EF 1.00* FD 0.98 KP 1.10 ! LA 1.01 MC 1.01 NL 0.93 ON 1.04 ! OV 0.93 PT 1.09 SC 0.92 ZC 0.75 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.11 EF 1.00* FD 1.05 KP 1.01 ! LA 1.01 MC 1.07 MK 0.93 NL 0.98 ! ON 1.04 OV 1.07 PT 1.06 SC 1.02 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 EF 1.00* FD 1.01 KP 1.03 ! LA 0.99 MC 0.99 MK 1.00 NL 0.93 ! ON 0.92 PT 1.00 SC 1.02 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.09 FD 1.05 KP 0.94 LA 0.98 ! MK 0.88 NL 0.92 ON 0.91 OV 1.04 ! PT 1.07 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.97 KP 0.90 ! LA 0.99 MC 1.22 MK 0.99 NL 1.01 ! OV 1.08 PT 0.93 SC 0.87 ZC 0.77 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.07 KP 0.91 ! LA 0.96 MC 1.13 NL 1.04 ON 1.16 ! OV 1.05 PT 1.02 SC 0.99 ZC 0.78 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00 KP 0.87 ! LA 1.05 MC 1.20 MK 1.03 NL 1.06 ! ON 1.28 OV 1.01 PT 0.91 SC 1.03 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 0.97 KP 0.89 ! LA 1.00 MC 1.19 MK 0.94 NL 0.99 ! ON 1.08 PT 0.98 SC 0.99 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 1.04 KP 0.88 LA 0.98 ! MK 0.97 NL 0.98 ON 1.23 OV 1.02 ! PT 0.97 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.99 KP 0.89 ! LA 1.01 MC 1.27 MK 1.01 NL 0.98 ! OV 1.08 PT 1.02 SC 0.90 ZC 0.80 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 0.98 KP 0.85 ! LA 1.04 MC 1.33 NL 1.10 ON 1.32 ! OV 1.11 PT 0.91 SC 1.00 ZC 0.72 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 0.99 KP 0.89 ! LA 0.97 MC 1.26 MK 0.99 NL 1.04 ! ON 1.20 OV 1.10 PT 0.99 SC 1.01 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.02 KP 0.85 ! LA 1.12 MC 1.13 MK 1.06 NL 1.01 ! ON 1.04 PT 0.90 SC 0.95 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 1.02 KP 0.87 LA 0.96 ! MK 1.02 NL 0.96 ON 1.13 OV 1.03 ! PT 0.97 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 0.95 EF 1.00* FD 0.99 KP 0.88 ! LA 1.13 MC 1.36 MK 1.14 NL 1.00 ! OV 0.99 PT 1.04 SC 0.87 ZC 0.62 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 EF 1.00* FD 1.03 KP 0.90 ! LA 1.06 MC 1.20 NL 1.06 ON 1.22 ! OV 1.05 PT 1.01 SC 1.04 ZC 0.58 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.16 EF 1.00* FD 1.06 KP 0.92 ! LA 1.00 MC 1.26 MK 1.12 NL 1.06 ! ON 1.22 OV 1.02 PT 1.04 SC 1.06 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 EF 1.00* FD 1.01 KP 0.93 ! LA 1.10 MC 1.11 MK 1.09 NL 1.03 ! ON 1.10 PT 1.01 SC 1.04 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.14 FD 0.95 KP 0.95 LA 1.10 ! MK 0.98 NL 1.05 ON 1.09 OV 0.97 ! PT 0.97 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 1.05 EF 1.00* FD 1.00 KP 0.93 ! LA 0.98 MC 1.29 MK 1.10 NL 1.02 ! OV 1.05 PT 1.03 SC 0.89 ZC 0.54 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 EF 1.00* FD 1.09 KP 1.02 ! LA 0.93 MC 1.40 NL 1.07 ON 1.20 ! OV 0.98 PT 0.94 SC 0.96 ZC 0.61 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 EF 1.00* FD 1.10 KP 0.92 ! LA 1.07 MC 1.33 MK 1.04 NL 1.05 ! ON 1.45 OV 1.02 PT 1.05 SC 0.92 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.05 EF 1.00* FD 0.99 KP 0.97 ! LA 1.06 MC 1.27 MK 1.05 NL 0.97 ! ON 1.28 PT 1.03 SC 0.97 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.95 FD 0.97 KP 0.96 LA 1.11 ! MK 1.02 NL 1.03 ON 1.01 OV 0.97 ! PT 1.03 ! ! ! Fit before self-cal, rms=0.087643Jy sigma=0.670834 ! Fit after self-cal, rms=0.087210Jy sigma=0.664630 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Estimated beam: bmin=0.664 mas, bmaj=1.005 mas, bpa=-16.16 degrees ! Estimated noise=0.334211 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 = 0.000213602 Jy ! Component: 100 - total flux cleaned = 0.000230787 Jy ! Component: 150 - total flux cleaned = 0.000230985 Jy ! Component: 200 - total flux cleaned = 0.000235424 Jy ! Total flux subtracted in 200 components = 0.000235424 Jy ! Clean residual min=-0.000897 max=0.000977 Jy/beam ! Clean residual mean=0.000001 rms=0.000215 Jy/beam ! Combined flux in latest and established models = 0.0856362 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 21 components and 0.0856363 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=0.087209Jy sigma=0.664626 ! Fit after self-cal, rms=0.087320Jy sigma=0.664300 ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 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=0.087320Jy sigma=0.664300 ! Fit after self-cal, rms=0.087757Jy sigma=0.664274 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Estimated beam: bmin=0.6634 mas, bmaj=1.006 mas, bpa=-16.18 degrees ! Estimated noise=0.334988 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00022256 Jy ! Component: 100 - total flux cleaned = 0.000234215 Jy ! Component: 150 - total flux cleaned = 0.000238683 Jy ! Component: 200 - total flux cleaned = 0.000242614 Jy ! Total flux subtracted in 200 components = 0.000242614 Jy ! Clean residual min=-0.000896 max=0.000973 Jy/beam ! Clean residual mean=0.000001 rms=0.000215 Jy/beam ! Combined flux in latest and established models = 0.0858789 Jy selfcal ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 22 components and 0.0858789 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=0.087756Jy sigma=0.664268 ! Fit after self-cal, rms=0.087767Jy sigma=0.664264 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 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 (-33.4, -20.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000664326 Jy ! Component: 100 - total flux cleaned = 0.000718224 Jy ! Component: 150 - total flux cleaned = 0.000679537 Jy ! Component: 200 - total flux cleaned = 0.000630905 Jy ! Total flux subtracted in 200 components = 0.000630905 Jy ! Clean residual min=-0.000882 max=0.000944 Jy/beam ! Clean residual mean=0.000000 rms=0.000212 Jy/beam ! Combined flux in latest and established models = 0.0865098 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 35 components and 0.0865098 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=0.087753Jy sigma=0.664128 ! Fit after self-cal, rms=0.087752Jy sigma=0.664112 ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Added new window around map position (-33.6, -39.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000798601 Jy ! Component: 100 - total flux cleaned = 0.000970161 Jy ! Component: 150 - total flux cleaned = 0.00100282 Jy ! Component: 200 - total flux cleaned = 0.00100294 Jy ! Total flux subtracted in 200 components = 0.00100294 Jy ! Clean residual min=-0.000919 max=0.000905 Jy/beam ! Clean residual mean=0.000000 rms=0.000210 Jy/beam ! Combined flux in latest and established models = 0.0875127 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 47 components and 0.0875127 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=0.087740Jy sigma=0.664034 ! Fit after self-cal, rms=0.087739Jy sigma=0.664025 ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 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=0.087739Jy sigma=0.664025 ! Fit after self-cal, rms=0.087796Jy sigma=0.664007 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Estimated beam: bmin=0.6629 mas, bmaj=1.005 mas, bpa=-16.16 degrees ! Estimated noise=0.335461 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000389147 Jy ! Component: 100 - total flux cleaned = 0.000404879 Jy ! Component: 150 - total flux cleaned = 0.000418996 Jy ! Component: 200 - total flux cleaned = 0.000431923 Jy ! Total flux subtracted in 200 components = 0.000431923 Jy ! Clean residual min=-0.000898 max=0.000906 Jy/beam ! Clean residual mean=0.000000 rms=0.000210 Jy/beam ! Combined flux in latest and established models = 0.0879446 Jy selfcal ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 48 components and 0.0879446 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=0.087790Jy sigma=0.663971 ! Fit after self-cal, rms=0.087789Jy sigma=0.663969 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 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 (25.6, 14.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000796326 Jy ! Component: 100 - total flux cleaned = 0.00086538 Jy ! Component: 150 - total flux cleaned = 0.000925149 Jy ! Component: 200 - total flux cleaned = 0.00101371 Jy ! Total flux subtracted in 200 components = 0.00101371 Jy ! Clean residual min=-0.000902 max=0.000894 Jy/beam ! Clean residual mean=-0.000000 rms=0.000207 Jy/beam ! Combined flux in latest and established models = 0.0889583 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 60 components and 0.0889583 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=0.087774Jy sigma=0.663872 ! Fit after self-cal, rms=0.087770Jy sigma=0.663861 ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 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=0.087770Jy sigma=0.663861 ! Fit after self-cal, rms=0.087677Jy sigma=0.663856 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Estimated beam: bmin=2.668 mas, bmaj=2.888 mas, bpa=28.39 degrees ! Estimated noise=0.436478 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000437802 Jy ! Component: 100 - total flux cleaned = 0.000626708 Jy ! Component: 150 - total flux cleaned = 0.000778157 Jy ! Component: 200 - total flux cleaned = 0.000862211 Jy ! Total flux subtracted in 200 components = 0.000862211 Jy ! Clean residual min=-0.001025 max=0.000944 Jy/beam ! Clean residual mean=0.000000 rms=0.000248 Jy/beam ! Combined flux in latest and established models = 0.0898205 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 72 components and 0.0898205 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=0.087677Jy sigma=0.663850 ! Fit after self-cal, rms=0.087675Jy sigma=0.663845 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 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 = 0.000165566 Jy ! Component: 100 - total flux cleaned = 0.000239186 Jy ! Component: 150 - total flux cleaned = 0.00029736 Jy ! Component: 200 - total flux cleaned = 0.000332609 Jy ! Total flux subtracted in 200 components = 0.000332609 Jy ! Clean residual min=-0.001012 max=0.000940 Jy/beam ! Clean residual mean=0.000000 rms=0.000247 Jy/beam ! Combined flux in latest and established models = 0.0901531 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 80 components and 0.0901532 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=0.087676Jy sigma=0.663845 ! Fit after self-cal, rms=0.087676Jy sigma=0.663843 ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 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 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Estimated beam: bmin=0.6627 mas, bmaj=1.005 mas, bpa=-16.17 degrees ! Estimated noise=0.335395 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6627 x 1.005 at -16.17 degrees (North through East) ! Clean map min=-0.00080273 max=0.076545 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 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Estimated beam: bmin=0.4794 mas, bmaj=0.7652 mas, bpa=-20.97 degrees ! Estimated noise=0.761427 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0578782 Jy ! Component: 100 - total flux cleaned = 0.0718139 Jy ! Component: 150 - total flux cleaned = 0.0778759 Jy ! Component: 200 - total flux cleaned = 0.0811262 Jy ! Total flux subtracted in 200 components = 0.0811262 Jy ! Clean residual min=-0.002252 max=0.002328 Jy/beam ! Clean residual mean=-0.000001 rms=0.000513 Jy/beam ! Combined flux in latest and established models = 0.0811262 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 12 model components to the UV plane model. ! The established model now contains 12 components and 0.0811262 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Estimated beam: bmin=0.6627 mas, bmaj=1.005 mas, bpa=-16.17 degrees ! Estimated noise=0.335395 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 = 0.00290798 Jy ! Component: 100 - total flux cleaned = 0.00446201 Jy ! Component: 150 - total flux cleaned = 0.0056566 Jy ! Component: 200 - total flux cleaned = 0.00643864 Jy ! Total flux subtracted in 200 components = 0.00643864 Jy ! Clean residual min=-0.000932 max=0.000862 Jy/beam ! Clean residual mean=-0.000001 rms=0.000214 Jy/beam ! Combined flux in latest and established models = 0.0875649 Jy ! Adding 21 model components to the UV plane model. ! The established model now contains 29 components and 0.0875649 Jy ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 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 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Estimated beam: bmin=2.668 mas, bmaj=2.888 mas, bpa=28.39 degrees ! Estimated noise=0.436478 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000927913 Jy ! Component: 100 - total flux cleaned = 0.00143689 Jy ! Component: 150 - total flux cleaned = 0.00169483 Jy ! Component: 200 - total flux cleaned = 0.00191121 Jy ! Total flux subtracted in 200 components = 0.00191121 Jy ! Clean residual min=-0.001029 max=0.000928 Jy/beam ! Clean residual mean=-0.000000 rms=0.000251 Jy/beam ! Combined flux in latest and established models = 0.0894761 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 = 0.000118222 Jy ! Component: 100 - total flux cleaned = 0.000221042 Jy ! Component: 150 - total flux cleaned = 0.000312121 Jy ! Component: 200 - total flux cleaned = 0.000384149 Jy ! Total flux subtracted in 200 components = 0.000384149 Jy ! Clean residual min=-0.001028 max=0.000924 Jy/beam ! Clean residual mean=-0.000000 rms=0.000248 Jy/beam ! Combined flux in latest and established models = 0.0898602 Jy ! Adding 36 model components to the UV plane model. ! The established model now contains 61 components and 0.0898602 Jy ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! Estimated beam: bmin=0.6627 mas, bmaj=1.005 mas, bpa=-16.17 degrees ! Estimated noise=0.335395 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000176641 Jy ! Component: 100 - total flux cleaned = 0.00030657 Jy ! Component: 150 - total flux cleaned = 0.000425348 Jy ! Component: 200 - total flux cleaned = 0.000469311 Jy ! Total flux subtracted in 200 components = 0.000469311 Jy ! Clean residual min=-0.000917 max=0.000906 Jy/beam ! Clean residual mean=-0.000000 rms=0.000207 Jy/beam ! Combined flux in latest and established models = 0.0903296 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 72 components and 0.0903296 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=0.087687Jy sigma=0.663947 ! Fit after self-cal, rms=0.087687Jy sigma=0.663936 wmodel /scr/pima/gb073_uvs/J1203+4510_X_map.mod ! Writing 72 model components to file: /scr/pima/gb073_uvs/J1203+4510_X_map.mod wobs /scr/pima/gb073_uvs/J1203+4510_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1203+4510_X_uvs.fits wwins /scr/pima/gb073_uvs/J1203+4510_X_map.win ! wwins: Wrote 4 windows to /scr/pima/gb073_uvs/J1203+4510_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 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -5.25072e-05 Jy ! Component: 100 - total flux cleaned = -8.56778e-05 Jy ! Component: 150 - total flux cleaned = -0.000132276 Jy ! Component: 200 - total flux cleaned = -0.000177767 Jy ! Component: 250 - total flux cleaned = -0.000222184 Jy ! Component: 300 - total flux cleaned = -0.000236423 Jy ! Component: 350 - total flux cleaned = -0.000236276 Jy ! Component: 400 - total flux cleaned = -0.000236095 Jy ! Component: 450 - total flux cleaned = -0.000264267 Jy ! Component: 500 - total flux cleaned = -0.000292035 Jy ! Component: 550 - total flux cleaned = -0.000250399 Jy ! Component: 600 - total flux cleaned = -0.00029186 Jy ! Component: 650 - total flux cleaned = -0.000319133 Jy ! Component: 700 - total flux cleaned = -0.000305738 Jy ! Component: 750 - total flux cleaned = -0.000346084 Jy ! Component: 800 - total flux cleaned = -0.000346138 Jy ! Component: 850 - total flux cleaned = -0.000372653 Jy ! Component: 900 - total flux cleaned = -0.000385856 Jy ! Component: 950 - total flux cleaned = -0.000450974 Jy ! Component: 1000 - total flux cleaned = -0.000437887 Jy ! Component: 1050 - total flux cleaned = -0.000450731 Jy ! Component: 1100 - total flux cleaned = -0.000450756 Jy ! Component: 1150 - total flux cleaned = -0.000488922 Jy ! Component: 1200 - total flux cleaned = -0.000463619 Jy ! Component: 1250 - total flux cleaned = -0.000551527 Jy ! Component: 1300 - total flux cleaned = -0.000576513 Jy ! Component: 1350 - total flux cleaned = -0.000576468 Jy ! Component: 1400 - total flux cleaned = -0.000638017 Jy ! Component: 1450 - total flux cleaned = -0.000674821 Jy ! Component: 1500 - total flux cleaned = -0.000625981 Jy ! Component: 1550 - total flux cleaned = -0.000674575 Jy ! Component: 1600 - total flux cleaned = -0.000710878 Jy ! Component: 1650 - total flux cleaned = -0.000734958 Jy ! Component: 1700 - total flux cleaned = -0.00075882 Jy ! Component: 1750 - total flux cleaned = -0.000735065 Jy ! Component: 1800 - total flux cleaned = -0.000734991 Jy ! Component: 1850 - total flux cleaned = -0.000805857 Jy ! Component: 1900 - total flux cleaned = -0.000817661 Jy ! Component: 1950 - total flux cleaned = -0.000852859 Jy ! Component: 2000 - total flux cleaned = -0.000864589 Jy ! Component: 2050 - total flux cleaned = -0.000876225 Jy ! Component: 2100 - total flux cleaned = -0.000922485 Jy ! Component: 2150 - total flux cleaned = -0.00102631 Jy ! Component: 2200 - total flux cleaned = -0.00103785 Jy ! Component: 2250 - total flux cleaned = -0.00109507 Jy ! Component: 2300 - total flux cleaned = -0.00110655 Jy ! Component: 2350 - total flux cleaned = -0.00116339 Jy ! Component: 2400 - total flux cleaned = -0.00129927 Jy ! Component: 2450 - total flux cleaned = -0.00125411 Jy ! Component: 2500 - total flux cleaned = -0.00135532 Jy ! Component: 2550 - total flux cleaned = -0.00138897 Jy ! Component: 2600 - total flux cleaned = -0.00144488 Jy ! Component: 2650 - total flux cleaned = -0.00156741 Jy ! Component: 2700 - total flux cleaned = -0.00153414 Jy ! Component: 2750 - total flux cleaned = -0.00156734 Jy ! Component: 2800 - total flux cleaned = -0.00163361 Jy ! Component: 2850 - total flux cleaned = -0.00175472 Jy ! Component: 2900 - total flux cleaned = -0.00176568 Jy ! Component: 2950 - total flux cleaned = -0.00184231 Jy ! Component: 3000 - total flux cleaned = -0.00184236 Jy ! Component: 3050 - total flux cleaned = -0.00190757 Jy ! Component: 3100 - total flux cleaned = -0.0019834 Jy ! Component: 3150 - total flux cleaned = -0.00196174 Jy ! Component: 3200 - total flux cleaned = -0.00202648 Jy ! Component: 3250 - total flux cleaned = -0.00209103 Jy ! Component: 3300 - total flux cleaned = -0.00214462 Jy ! Component: 3350 - total flux cleaned = -0.00220875 Jy ! Component: 3400 - total flux cleaned = -0.0022408 Jy ! Component: 3450 - total flux cleaned = -0.00224077 Jy ! Component: 3500 - total flux cleaned = -0.0023044 Jy ! Component: 3550 - total flux cleaned = -0.00229376 Jy ! Component: 3600 - total flux cleaned = -0.00242037 Jy ! Component: 3650 - total flux cleaned = -0.00246245 Jy ! Component: 3700 - total flux cleaned = -0.00248345 Jy ! Component: 3750 - total flux cleaned = -0.00250436 Jy ! Component: 3800 - total flux cleaned = -0.00252519 Jy ! Component: 3850 - total flux cleaned = -0.00256687 Jy ! Component: 3900 - total flux cleaned = -0.00255651 Jy ! Component: 3950 - total flux cleaned = -0.00266009 Jy ! Component: 4000 - total flux cleaned = -0.00269113 Jy ! Component: 4050 - total flux cleaned = -0.00267049 Jy ! Total flux subtracted in 4096 components = -0.00269109 Jy ! Clean residual min=-0.000609 max=0.000675 Jy/beam ! Clean residual mean=-0.000000 rms=0.000168 Jy/beam ! Combined flux in latest and established models = 0.0876385 Jy keep ! Adding 364 model components to the UV plane model. ! The established model now contains 436 components and 0.0876385 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1203+4510_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6627 x 1.005 at -16.17 degrees (North through East) ! Clean map min=-0.00070027 max=0.076833 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1203+4510_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0768333 invert ! Inverting map ! Your choice of large map pixels excluded 3.25% of the data. ! The x-axis pixel size should ideally be below 0.1645 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000167606 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.654428 0.654428 1.30886 2.61771 5.23542 10.4708 20.9417 41.8834 83.7668 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0005 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.076 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 458.415 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1203+4510_X_uvs.log closed on Sat Dec 26 09:37:47 2015