! Started logfile: /scr/pima/gb073_uvs/J1419+3821_X_uvs.log on Sat Dec 26 09:40:26 2015 obs /scr/pima/gb073_uvs/J1419+3821_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1419+3821_X_uva.fits ! AN table 1: 5 integrations on 21 of 21 possible baselines. ! AN table 2: 5 integrations on 36 of 36 possible baselines. ! AN table 3: 12 integrations on 66 of 66 possible baselines. ! Apparent sampling: 1 visibilities/baseline/integration-bin. ! Found source: J1419+3821 ! ! 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 8616 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/J1419+3821_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 12 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 12 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 12 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 12 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 5. ! A total of 5 telescope corrections were flagged in sub-array 1. ! A total of 5 telescope corrections were flagged in sub-array 2. ! A total of 24 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 6. ! A total of 5 telescope corrections were flagged in sub-array 1. ! A total of 5 telescope corrections were flagged in sub-array 2. ! A total of 24 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 7. ! A total of 12 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 8. ! A total of 12 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=1.486561Jy sigma=13.450899 ! Fit after self-cal, rms=0.232048Jy sigma=1.964731 ! clrmod: Cleared the established, tentative and continuum models. ! Redundant starting model cleared. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=0.4826 mas, bmaj=0.9524 mas, bpa=21.55 degrees ! Estimated noise=1.6363 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 = 0.854283 Jy ! Component: 100 - total flux cleaned = 1.04888 Jy ! Total flux subtracted in 100 components = 1.04888 Jy ! Clean residual min=-0.049116 max=0.069710 Jy/beam ! Clean residual mean=-0.000027 rms=0.007722 Jy/beam ! Combined flux in latest and established models = 1.04888 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 1.04888 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=0.213303Jy sigma=1.721401 ! Fit after self-cal, rms=0.213309Jy sigma=1.721375 ! Inverting map ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0717127 Jy ! Component: 100 - total flux cleaned = 0.110284 Jy ! Total flux subtracted in 100 components = 0.110284 Jy ! Clean residual min=-0.046678 max=0.050698 Jy/beam ! Clean residual mean=-0.000141 rms=0.006217 Jy/beam ! Combined flux in latest and established models = 1.15917 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 11 components and 1.15917 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=0.194411Jy sigma=1.398058 ! Fit after self-cal, rms=0.194415Jy sigma=1.397986 ! Inverting map ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Added new window around map position (-1.6, 0.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00758403 Jy ! Component: 100 - total flux cleaned = 0.0046124 Jy ! Total flux subtracted in 100 components = 0.0046124 Jy ! Clean residual min=-0.039216 max=0.041824 Jy/beam ! Clean residual mean=-0.000147 rms=0.005599 Jy/beam ! Combined flux in latest and established models = 1.16378 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 17 components and 1.16378 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=0.182320Jy sigma=1.320605 ! Fit after self-cal, rms=0.181844Jy sigma=1.315905 ! Inverting map ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec print "************** FINISHED UNIFORM WEIGHTING CLEAN **************" ! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** ! uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. win_mult = win_mult * 1.6 clean_niter = clean_niter * 2 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=0.575 mas, bmaj=1.099 mas, bpa=21.71 degrees ! Estimated noise=1.00926 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 = 0.000800511 Jy ! Component: 100 - total flux cleaned = 0.00223012 Jy ! Component: 150 - total flux cleaned = 0.00464112 Jy ! Component: 200 - total flux cleaned = 0.00517304 Jy ! Total flux subtracted in 200 components = 0.00517304 Jy ! Clean residual min=-0.032686 max=0.021825 Jy/beam ! Clean residual mean=-0.000714 rms=0.005061 Jy/beam ! Combined flux in latest and established models = 1.16895 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 27 components and 1.16895 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=0.176440Jy sigma=1.270901 ! Fit after self-cal, rms=0.176360Jy sigma=1.268676 ! Inverting map ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.575 x 1.099 at 21.71 degrees (North through East) ! Clean map min=-0.028514 max=1.0952 Jy/beam if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.92 FD 0.93 KP 0.96 LA 1.01 ! MK 1.04 OV 0.96 PT 0.92 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.93 FD 0.96 KP 0.96 LA 1.01 ! MK 1.02 NL 0.90 OV 0.97 PT 0.94 ! SC 0.97 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 EF 1.00* FD 0.97 HH 0.96 ! KP 1.07 LA 1.12 MC 0.92 NL 0.92 ! ON 1.01 PT 1.00 SC 0.94 ZC 0.87 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.98 KP 0.98 LA 1.02 ! MK 1.06 OV 0.99 PT 0.99 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 0.99 KP 0.99 LA 1.04 ! MK 1.05 NL 0.95 OV 1.00 PT 0.99 ! SC 1.00 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 EF 1.00* FD 1.03 HH 0.98 ! KP 1.08 LA 1.15 MC 0.94 NL 0.94 ! ON 1.01 PT 1.06 SC 0.96 ZC 0.89 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 0.97 KP 0.93 LA 0.96 ! MK 1.01 OV 0.97 PT 0.97 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 0.98 KP 0.92 LA 0.96 ! MK 1.00 NL 0.92 OV 0.97 PT 0.98 ! SC 1.05 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 EF 1.00* FD 1.01 HH 0.94 ! KP 1.03 LA 1.06 MC 0.93 NL 0.93 ! ON 0.99 PT 1.05 SC 0.99 ZC 0.86 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 0.98 KP 0.95 LA 0.97 ! MK 1.03 OV 0.96 PT 1.00 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 0.99 KP 0.95 LA 0.98 ! MK 1.02 NL 0.94 OV 0.96 PT 1.00 ! SC 1.05 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 EF 1.00* FD 1.02 HH 0.96 ! KP 1.06 LA 1.08 MC 0.95 NL 0.96 ! ON 1.01 PT 1.07 SC 1.00 ZC 0.89 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.98 KP 0.87 LA 0.96 ! MK 1.03 OV 1.03 PT 0.97 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 0.98 KP 0.88 LA 0.96 ! MK 1.04 NL 0.96 OV 1.03 PT 0.96 ! SC 1.06 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.02 HH 0.94 ! KP 0.98 LA 1.10 MC 1.19 NL 0.98 ! ON 1.23 PT 1.03 SC 1.02 ZC 0.92 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.98 KP 0.86 LA 0.96 ! MK 1.05 OV 1.02 PT 0.92 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* FD 0.98 KP 0.86 LA 0.98 ! MK 1.05 NL 0.96 OV 1.03 PT 0.92 ! SC 1.01 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.02 HH 0.98 ! KP 0.95 LA 1.09 MC 1.21 NL 0.97 ! ON 1.27 PT 1.00 SC 0.99 ZC 0.89 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 1.01 KP 0.89 LA 1.02 ! MK 1.10 OV 0.97 PT 0.99 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 1.02 KP 0.87 LA 1.03 ! MK 1.10 NL 1.00 OV 0.98 PT 0.98 ! SC 1.04 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 EF 1.00* FD 1.06 HH 1.17 ! KP 1.00 LA 1.16 MC 1.25 NL 1.01 ! ON 1.32 PT 1.05 SC 1.01 ZC 0.75 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 1.00 KP 0.91 LA 0.99 ! MK 1.10 OV 0.98 PT 1.00 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 1.01 KP 0.89 LA 1.02 ! MK 1.10 NL 0.99 OV 0.98 PT 0.99 ! SC 1.06 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 EF 1.00* FD 1.05 HH 1.11 ! KP 1.00 LA 1.16 MC 1.30 NL 1.00 ! ON 1.32 PT 1.06 SC 1.01 ZC 0.71 ! ! ! Fit before self-cal, rms=0.176360Jy sigma=1.268676 ! Fit after self-cal, rms=0.114253Jy sigma=0.740376 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=0.5757 mas, bmaj=1.101 mas, bpa=21.28 degrees ! Estimated noise=1.00536 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (-2.4, -0.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.001111 Jy ! Component: 100 - total flux cleaned = 0.00109129 Jy ! Component: 150 - total flux cleaned = 0.00107586 Jy ! Component: 200 - total flux cleaned = 0.00107789 Jy ! Total flux subtracted in 200 components = 0.00107789 Jy ! Clean residual min=-0.007958 max=0.006943 Jy/beam ! Clean residual mean=-0.000100 rms=0.001474 Jy/beam ! Combined flux in latest and established models = 1.17003 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 40 components and 1.17003 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=0.111475Jy sigma=0.720381 ! Fit after self-cal, rms=0.111514Jy sigma=0.719240 ! Inverting map ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 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=0.111514Jy sigma=0.719240 ! Fit after self-cal, rms=0.106391Jy sigma=0.674026 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=0.5754 mas, bmaj=1.099 mas, bpa=21.2 degrees ! Estimated noise=1.00458 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00010414 Jy ! Component: 100 - total flux cleaned = 0.000350329 Jy ! Component: 150 - total flux cleaned = 0.000551494 Jy ! Component: 200 - total flux cleaned = 0.000542955 Jy ! Total flux subtracted in 200 components = 0.000542955 Jy ! Clean residual min=-0.005011 max=0.004485 Jy/beam ! Clean residual mean=0.000053 rms=0.000952 Jy/beam ! Combined flux in latest and established models = 1.17057 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 47 components and 1.17057 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=0.105082Jy sigma=0.664868 ! Fit after self-cal, rms=0.104985Jy sigma=0.664448 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 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 = -2.17143e-05 Jy ! Component: 100 - total flux cleaned = -0.000160633 Jy ! Component: 150 - total flux cleaned = -3.58351e-05 Jy ! Component: 200 - total flux cleaned = -3.7219e-05 Jy ! Total flux subtracted in 200 components = -3.7219e-05 Jy ! Clean residual min=-0.004935 max=0.004507 Jy/beam ! Clean residual mean=0.000053 rms=0.000918 Jy/beam ! Combined flux in latest and established models = 1.17054 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 51 components and 1.17054 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=0.104583Jy sigma=0.661930 ! Fit after self-cal, rms=0.104564Jy sigma=0.661844 ! Inverting map ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 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=0.104564Jy sigma=0.661844 ! Fit after self-cal, rms=0.104430Jy sigma=0.658941 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=0.5749 mas, bmaj=1.098 mas, bpa=21.17 degrees ! Estimated noise=1.00366 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000361544 Jy ! Component: 100 - total flux cleaned = -0.000330188 Jy ! Component: 150 - total flux cleaned = -0.000474193 Jy ! Component: 200 - total flux cleaned = -0.000369125 Jy ! Total flux subtracted in 200 components = -0.000369125 Jy ! Clean residual min=-0.003764 max=0.004001 Jy/beam ! Clean residual mean=0.000056 rms=0.000834 Jy/beam ! Combined flux in latest and established models = 1.17017 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 52 components and 1.17017 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=0.103878Jy sigma=0.655020 ! Fit after self-cal, rms=0.103843Jy sigma=0.654846 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 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 (-12.2, -35.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00292454 Jy ! Component: 100 - total flux cleaned = 0.0033388 Jy ! Component: 150 - total flux cleaned = 0.00342936 Jy ! Component: 200 - total flux cleaned = 0.00342638 Jy ! Total flux subtracted in 200 components = 0.00342638 Jy ! Clean residual min=-0.003710 max=0.003556 Jy/beam ! Clean residual mean=0.000045 rms=0.000801 Jy/beam ! Combined flux in latest and established models = 1.17359 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 59 components and 1.17359 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=0.103543Jy sigma=0.652803 ! Fit after self-cal, rms=0.103522Jy sigma=0.652608 ! Inverting map ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 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=0.103522Jy sigma=0.652608 ! Fit after self-cal, rms=0.103542Jy sigma=0.651422 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=2.803 mas, bmaj=3.081 mas, bpa=-27.05 degrees ! Estimated noise=1.33075 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000387611 Jy ! Component: 100 - total flux cleaned = 0.000340182 Jy ! Component: 150 - total flux cleaned = 0.000342505 Jy ! Component: 200 - total flux cleaned = 0.000342237 Jy ! Total flux subtracted in 200 components = 0.000342237 Jy ! Clean residual min=-0.003319 max=0.003187 Jy/beam ! Clean residual mean=0.000103 rms=0.000906 Jy/beam ! Combined flux in latest and established models = 1.17394 Jy selfcal ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 65 components and 1.17394 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=0.103552Jy sigma=0.651516 ! Fit after self-cal, rms=0.103558Jy sigma=0.651381 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 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 = 0.000149891 Jy ! Component: 100 - total flux cleaned = 0.000225674 Jy ! Component: 150 - total flux cleaned = 0.000224695 Jy ! Component: 200 - total flux cleaned = 0.000198711 Jy ! Total flux subtracted in 200 components = 0.000198711 Jy ! Clean residual min=-0.003277 max=0.003128 Jy/beam ! Clean residual mean=0.000102 rms=0.000899 Jy/beam ! Combined flux in latest and established models = 1.17414 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 68 components and 1.17414 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=0.103594Jy sigma=0.651701 ! Fit after self-cal, rms=0.103594Jy sigma=0.651612 ! Inverting map ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. win_mult = win_mult / 1.2 print "************** FINISHED AMPLITUDE SELF-CAL **************" ! ************** FINISHED AMPLITUDE SELF-CAL ************** restore ! Inverting map and beam ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=0.5746 mas, bmaj=1.097 mas, bpa=21.15 degrees ! Estimated noise=1.00304 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5746 x 1.097 at 21.15 degrees (North through East) ! Clean map min=-0.011771 max=1.0882 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 ! Performing amp+phase self-cal ! ! 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=0.103594Jy sigma=0.651612 ! Fit after self-cal, rms=0.098935Jy sigma=0.614410 ! Inverting map and beam ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=0.5746 mas, bmaj=1.096 mas, bpa=21.17 degrees ! Estimated noise=1.00259 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -9.87024e-05 Jy ! Component: 100 - total flux cleaned = 0.000121339 Jy ! Component: 150 - total flux cleaned = 0.000315441 Jy ! Component: 200 - total flux cleaned = 0.000579821 Jy ! Total flux subtracted in 200 components = 0.000579821 Jy ! Clean residual min=-0.003347 max=0.003356 Jy/beam ! Clean residual mean=0.000039 rms=0.000745 Jy/beam ! Combined flux in latest and established models = 1.17472 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 69 components and 1.17472 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=0.098665Jy sigma=0.612255 ! Fit after self-cal, rms=0.098640Jy sigma=0.612188 ! Inverting map ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000312749 Jy ! Component: 100 - total flux cleaned = 0.000386805 Jy ! Component: 150 - total flux cleaned = 0.000315576 Jy ! Component: 200 - total flux cleaned = 0.00024983 Jy ! Total flux subtracted in 200 components = 0.00024983 Jy ! Clean residual min=-0.003263 max=0.003208 Jy/beam ! Clean residual mean=0.000038 rms=0.000734 Jy/beam ! Combined flux in latest and established models = 1.17497 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 74 components and 1.17497 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=0.098512Jy sigma=0.611373 ! Fit after self-cal, rms=0.098504Jy sigma=0.611355 ! Inverting map ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Performing amp+phase self-cal ! ! 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=0.098504Jy sigma=0.611355 ! Fit after self-cal, rms=0.098528Jy sigma=0.610709 print "************** CLEARING MODEL AND STARTING OVER **********" ! ************** CLEARING MODEL AND STARTING OVER ********** clrmod true ! clrmod: Cleared the established and tentative models. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=0.4811 mas, bmaj=0.9506 mas, bpa=20.8 degrees ! Estimated noise=1.61914 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.845248 Jy ! Component: 100 - total flux cleaned = 1.03645 Jy ! Component: 150 - total flux cleaned = 1.10498 Jy ! Component: 200 - total flux cleaned = 1.13398 Jy ! Total flux subtracted in 200 components = 1.13398 Jy ! Clean residual min=-0.010192 max=0.013498 Jy/beam ! Clean residual mean=0.000039 rms=0.001652 Jy/beam ! Combined flux in latest and established models = 1.13398 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 8 model components to the UV plane model. ! The established model now contains 8 components and 1.13398 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=0.5744 mas, bmaj=1.096 mas, bpa=21.14 degrees ! Estimated noise=1.00194 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 = 0.0172608 Jy ! Component: 100 - total flux cleaned = 0.0222126 Jy ! Component: 150 - total flux cleaned = 0.0250488 Jy ! Component: 200 - total flux cleaned = 0.0276049 Jy ! Total flux subtracted in 200 components = 0.0276049 Jy ! Clean residual min=-0.004198 max=0.007694 Jy/beam ! Clean residual mean=0.000086 rms=0.000910 Jy/beam ! Combined flux in latest and established models = 1.16158 Jy ! Adding 21 model components to the UV plane model. ! The established model now contains 23 components and 1.16158 Jy ! Inverting map ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Added new window around map position (1.8, -0.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0044496 Jy ! Component: 100 - total flux cleaned = 0.005608 Jy ! Component: 150 - total flux cleaned = 0.00665055 Jy ! Component: 200 - total flux cleaned = 0.00758805 Jy ! Total flux subtracted in 200 components = 0.00758805 Jy ! Clean residual min=-0.003585 max=0.003794 Jy/beam ! Clean residual mean=0.000057 rms=0.000772 Jy/beam ! Combined flux in latest and established models = 1.16917 Jy ! Adding 22 model components to the UV plane model. ! The established model now contains 38 components and 1.16917 Jy ! Inverting map ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Added new window around map position (0.2, -2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0012246 Jy ! Component: 100 - total flux cleaned = 0.00162551 Jy ! Component: 150 - total flux cleaned = 0.00211901 Jy ! Component: 200 - total flux cleaned = 0.00257274 Jy ! Total flux subtracted in 200 components = 0.00257274 Jy ! Clean residual min=-0.003199 max=0.003078 Jy/beam ! Clean residual mean=0.000047 rms=0.000719 Jy/beam ! Combined flux in latest and established models = 1.17174 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 50 components and 1.17175 Jy ! Inverting map ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=2.802 mas, bmaj=3.081 mas, bpa=-27.07 degrees ! Estimated noise=1.33015 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00180442 Jy ! Component: 100 - total flux cleaned = 0.0021816 Jy ! Component: 150 - total flux cleaned = 0.00228086 Jy ! Component: 200 - total flux cleaned = 0.0023216 Jy ! Total flux subtracted in 200 components = 0.0023216 Jy ! Clean residual min=-0.002862 max=0.002989 Jy/beam ! Clean residual mean=0.000099 rms=0.000846 Jy/beam ! Combined flux in latest and established models = 1.17407 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 = 1.33254e-06 Jy ! Component: 100 - total flux cleaned = 3.02691e-06 Jy ! Component: 150 - total flux cleaned = 4.2272e-06 Jy ! Component: 200 - total flux cleaned = 3.90968e-06 Jy ! Total flux subtracted in 200 components = 3.90968e-06 Jy ! Clean residual min=-0.002861 max=0.003019 Jy/beam ! Clean residual mean=0.000099 rms=0.000844 Jy/beam ! Combined flux in latest and established models = 1.17407 Jy ! Adding 25 model components to the UV plane model. ! The established model now contains 72 components and 1.17407 Jy ! Inverting map ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! Estimated beam: bmin=0.5744 mas, bmaj=1.096 mas, bpa=21.14 degrees ! Estimated noise=1.00194 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000902651 Jy ! Component: 100 - total flux cleaned = -0.000810695 Jy ! Component: 150 - total flux cleaned = -0.000641478 Jy ! Component: 200 - total flux cleaned = -0.000479933 Jy ! Total flux subtracted in 200 components = -0.000479933 Jy ! Clean residual min=-0.003164 max=0.002980 Jy/beam ! Clean residual mean=0.000040 rms=0.000693 Jy/beam ! Combined flux in latest and established models = 1.17359 Jy selfcal ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 81 components and 1.17359 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=0.098269Jy sigma=0.608572 ! Fit after self-cal, rms=0.098043Jy sigma=0.607287 wmodel /scr/pima/gb073_uvs/J1419+3821_X_map.mod ! Writing 81 model components to file: /scr/pima/gb073_uvs/J1419+3821_X_map.mod wobs /scr/pima/gb073_uvs/J1419+3821_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1419+3821_X_uvs.fits wwins /scr/pima/gb073_uvs/J1419+3821_X_map.win ! wwins: Wrote 6 windows to /scr/pima/gb073_uvs/J1419+3821_X_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00093923 Jy ! Component: 100 - total flux cleaned = -0.00157762 Jy ! Component: 150 - total flux cleaned = -0.00203665 Jy ! Component: 200 - total flux cleaned = -0.00233386 Jy ! Component: 250 - total flux cleaned = -0.00257422 Jy ! Component: 300 - total flux cleaned = -0.00276221 Jy ! Component: 350 - total flux cleaned = -0.00299342 Jy ! Component: 400 - total flux cleaned = -0.00299329 Jy ! Component: 450 - total flux cleaned = -0.003127 Jy ! Component: 500 - total flux cleaned = -0.00317075 Jy ! Component: 550 - total flux cleaned = -0.00321475 Jy ! Component: 600 - total flux cleaned = -0.00321523 Jy ! Component: 650 - total flux cleaned = -0.00338282 Jy ! Component: 700 - total flux cleaned = -0.0032575 Jy ! Component: 750 - total flux cleaned = -0.00321686 Jy ! Component: 800 - total flux cleaned = -0.00317641 Jy ! Component: 850 - total flux cleaned = -0.00313725 Jy ! Component: 900 - total flux cleaned = -0.003216 Jy ! Component: 950 - total flux cleaned = -0.00321538 Jy ! Component: 1000 - total flux cleaned = -0.00309885 Jy ! Component: 1050 - total flux cleaned = -0.00298413 Jy ! Component: 1100 - total flux cleaned = -0.00302277 Jy ! Component: 1150 - total flux cleaned = -0.00305975 Jy ! Component: 1200 - total flux cleaned = -0.00294846 Jy ! Component: 1250 - total flux cleaned = -0.00298484 Jy ! Component: 1300 - total flux cleaned = -0.00298504 Jy ! Component: 1350 - total flux cleaned = -0.002913 Jy ! Component: 1400 - total flux cleaned = -0.00284213 Jy ! Component: 1450 - total flux cleaned = -0.00280689 Jy ! Component: 1500 - total flux cleaned = -0.00270178 Jy ! Component: 1550 - total flux cleaned = -0.00266691 Jy ! Component: 1600 - total flux cleaned = -0.00249437 Jy ! Component: 1650 - total flux cleaned = -0.00252901 Jy ! Component: 1700 - total flux cleaned = -0.00246078 Jy ! Component: 1750 - total flux cleaned = -0.00235921 Jy ! Component: 1800 - total flux cleaned = -0.00225846 Jy ! Component: 1850 - total flux cleaned = -0.00209259 Jy ! Component: 1900 - total flux cleaned = -0.00212587 Jy ! Component: 1950 - total flux cleaned = -0.00209294 Jy ! Component: 2000 - total flux cleaned = -0.00189749 Jy ! Component: 2050 - total flux cleaned = -0.00186512 Jy ! Component: 2100 - total flux cleaned = -0.0019614 Jy ! Component: 2150 - total flux cleaned = -0.00180189 Jy ! Component: 2200 - total flux cleaned = -0.00167518 Jy ! Component: 2250 - total flux cleaned = -0.00186418 Jy ! Component: 2300 - total flux cleaned = -0.00173909 Jy ! Component: 2350 - total flux cleaned = -0.00161478 Jy ! Component: 2400 - total flux cleaned = -0.00173837 Jy ! Component: 2450 - total flux cleaned = -0.00167686 Jy ! Component: 2500 - total flux cleaned = -0.00167644 Jy ! Component: 2550 - total flux cleaned = -0.00158526 Jy ! Component: 2600 - total flux cleaned = -0.00149478 Jy ! Component: 2650 - total flux cleaned = -0.00149501 Jy ! Component: 2700 - total flux cleaned = -0.00149501 Jy ! Component: 2750 - total flux cleaned = -0.00152451 Jy ! Component: 2800 - total flux cleaned = -0.0014953 Jy ! Component: 2850 - total flux cleaned = -0.00137818 Jy ! Component: 2900 - total flux cleaned = -0.00140731 Jy ! Component: 2950 - total flux cleaned = -0.00129164 Jy ! Component: 3000 - total flux cleaned = -0.00137784 Jy ! Component: 3050 - total flux cleaned = -0.00137775 Jy ! Component: 3100 - total flux cleaned = -0.00129258 Jy ! Component: 3150 - total flux cleaned = -0.00123612 Jy ! Component: 3200 - total flux cleaned = -0.00132072 Jy ! Component: 3250 - total flux cleaned = -0.00129282 Jy ! Component: 3300 - total flux cleaned = -0.00137589 Jy ! Component: 3350 - total flux cleaned = -0.00134815 Jy ! Component: 3400 - total flux cleaned = -0.00132063 Jy ! Component: 3450 - total flux cleaned = -0.00140242 Jy ! Component: 3500 - total flux cleaned = -0.00137524 Jy ! Component: 3550 - total flux cleaned = -0.00137508 Jy ! Component: 3600 - total flux cleaned = -0.00137526 Jy ! Component: 3650 - total flux cleaned = -0.00132164 Jy ! Component: 3700 - total flux cleaned = -0.0013217 Jy ! Component: 3750 - total flux cleaned = -0.00142781 Jy ! Component: 3800 - total flux cleaned = -0.00137508 Jy ! Component: 3850 - total flux cleaned = -0.00134888 Jy ! Component: 3900 - total flux cleaned = -0.00142711 Jy ! Component: 3950 - total flux cleaned = -0.00134893 Jy ! Component: 4000 - total flux cleaned = -0.00142646 Jy ! Component: 4050 - total flux cleaned = -0.00134911 Jy ! Total flux subtracted in 4096 components = -0.00137466 Jy ! Clean residual min=-0.001579 max=0.001319 Jy/beam ! Clean residual mean=0.000023 rms=0.000416 Jy/beam ! Combined flux in latest and established models = 1.17222 Jy keep ! Adding 319 model components to the UV plane model. ! The established model now contains 399 components and 1.17222 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1419+3821_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5744 x 1.096 at 21.14 degrees (North through East) ! Clean map min=-0.0099246 max=1.0876 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1419+3821_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 1.0876 invert ! Inverting map ! Your choice of large map pixels excluded 2.99% of the data. ! The x-axis pixel size should ideally be below 0.1931 milli-arcsec ! The y-axis pixel size should ideally be below 0.169 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000414515 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.114339 0.114339 0.228677 0.457355 0.91471 1.82942 3.65884 7.31768 14.6354 29.2707 58.5414 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0012 print "peak= ", int(1000*peak_flux)/1000 ! peak= 1.087 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 2623.78 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1419+3821_X_uvs.log closed on Sat Dec 26 09:40:31 2015