! Started logfile: /scr/pima/rv117_uvs/J1419+5423_X_dfm.log on Sat Dec 9 23:44:21 2017 float field_size field_size = 1024 float field_cell field_cell = 0.2000 float taper_size taper_size = 70.0 float freq freq = 8.36575 obs /scr/pima/rv117_uvs/J1419+5423_X_uva.fits ! Reading UV FITS file: /scr/pima/rv117_uvs/J1419+5423_X_uva.fits ! AN table 1: 2 integrations on 28 of 28 possible baselines. ! AN table 2: 2 integrations on 45 of 45 possible baselines. ! AN table 3: 2 integrations on 3 of 3 possible baselines. ! AN table 4: 10 integrations on 45 of 45 possible baselines. ! AN table 5: 14 integrations on 45 of 45 possible baselines. ! AN table 6: 12 integrations on 15 of 15 possible baselines. ! AN table 7: 2 integrations on 6 of 6 possible baselines. ! Apparent sampling: 0.484551 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1419+5423 ! ! There are 4 IFs, and a total of 4 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 8.36575e+09 8e+06 1 8e+06 ! 02 2 8.44575e+09 8e+06 1 8e+06 ! 03 3 8.80575e+09 8e+06 1 8e+06 ! 04 4 8.92575e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 74 lines of history. ! ! Reading 2760 visibilities. select rr, 1,2,3,4,5,6,7,8,9,10,11,12,13,14,15,16 ! Restricting channel ranges to the available 4 channels. ! Selecting polarization: RR, channels: 1..4 ! Reading IF 1 channels: 1..1 ! Reading IF 2 channels: 2..2 ! Reading IF 3 channels: 3..3 ! Reading IF 4 channels: 4..4 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 ![@/opt64/bin/pima_mupet_01.dfm J1419+5423_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 32 telescope corrections were flagged in sub-array 4. ! A total of 56 telescope corrections were flagged in sub-array 5. ! A total of 36 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 32 telescope corrections were flagged in sub-array 4. ! A total of 56 telescope corrections were flagged in sub-array 5. ! A total of 36 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 32 telescope corrections were flagged in sub-array 4. ! A total of 56 telescope corrections were flagged in sub-array 5. ! A total of 36 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 32 telescope corrections were flagged in sub-array 4. ! A total of 56 telescope corrections were flagged in sub-array 5. ! A total of 36 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=2.449190Jy sigma=25.741463 ! Fit after self-cal, rms=1.266365Jy sigma=13.349726 ! 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 0.291% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! Estimated beam: bmin=0.678 mas, bmaj=0.9833 mas, bpa=12.13 degrees ! Estimated noise=1.53072 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 = 1.62034 Jy ! Component: 100 - total flux cleaned = 2.05838 Jy ! Total flux subtracted in 100 components = 2.05838 Jy ! Clean residual min=-0.031956 max=0.184606 Jy/beam ! Clean residual mean=-0.000073 rms=0.008426 Jy/beam ! Combined flux in latest and established models = 2.05838 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 2.05838 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.374016Jy sigma=3.848952 ! Fit after self-cal, rms=0.372382Jy sigma=3.835408 ! Inverting map ! Your choice of large map pixels excluded 0.291% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.194294 Jy ! Component: 100 - total flux cleaned = 0.292868 Jy ! Total flux subtracted in 100 components = 0.292868 Jy ! Clean residual min=-0.018500 max=0.079236 Jy/beam ! Clean residual mean=-0.000029 rms=0.004724 Jy/beam ! Combined flux in latest and established models = 2.35125 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 12 components and 2.35125 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.202781Jy sigma=2.029412 ! Fit after self-cal, rms=0.200042Jy sigma=2.003772 ! Inverting map ! Your choice of large map pixels excluded 0.291% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! Added new window around map position (1, -0.6). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0768863 Jy ! Component: 100 - total flux cleaned = 0.119209 Jy ! Total flux subtracted in 100 components = 0.119209 Jy ! Clean residual min=-0.016705 max=0.037748 Jy/beam ! Clean residual mean=-0.000012 rms=0.003678 Jy/beam ! Combined flux in latest and established models = 2.47046 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 22 components and 2.47046 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.154861Jy sigma=1.526465 ! Fit after self-cal, rms=0.150432Jy sigma=1.479624 ! Inverting map ! Your choice of large map pixels excluded 0.291% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0370905 Jy ! Component: 100 - total flux cleaned = 0.0596041 Jy ! Total flux subtracted in 100 components = 0.0596041 Jy ! Clean residual min=-0.015008 max=0.019418 Jy/beam ! Clean residual mean=-0.000003 rms=0.003259 Jy/beam ! Combined flux in latest and established models = 2.53006 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 33 components and 2.53006 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.137355Jy sigma=1.345280 ! Fit after self-cal, rms=0.135973Jy sigma=1.330302 ! Inverting map ! Your choice of large map pixels excluded 0.291% of the data. ! The x-axis pixel size should ideally be below 0.1847 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 0.291% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! Estimated beam: bmin=0.7998 mas, bmaj=1.114 mas, bpa=13.01 degrees ! Estimated noise=1.36336 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 = 0.0236967 Jy ! Component: 100 - total flux cleaned = 0.0366204 Jy ! Component: 150 - total flux cleaned = 0.0414174 Jy ! Component: 200 - total flux cleaned = 0.0424993 Jy ! Total flux subtracted in 200 components = 0.0424993 Jy ! Clean residual min=-0.013102 max=0.014676 Jy/beam ! Clean residual mean=-0.000005 rms=0.002961 Jy/beam ! Combined flux in latest and established models = 2.57256 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 41 components and 2.57256 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.131194Jy sigma=1.284388 ! Fit after self-cal, rms=0.130635Jy sigma=1.277565 ! Inverting map ! Your choice of large map pixels excluded 0.291% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7998 x 1.114 at 13.01 degrees (North through East) ! Clean map min=-0.011888 max=2.0966 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! FD 1.03 HN 1.01 LA 0.98 NL 1.00 ! NY 1.00 PT 1.02 SC 0.98 WZ 0.97 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 1.01 HN 0.98 KP 1.01 ! LA 0.99 NL 1.00 NY 1.00 ON 0.96 ! OV 1.01 PT 1.01 ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* HN 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 0.99 HN 1.00 KP 1.00 ! LA 0.99 MK 0.98 NL 1.00 OV 0.99 ! PT 1.01 SC 0.99 ! ! A total of 12 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 FD 1.02 HN 1.05 KP 1.01 ! LA 0.97 MK 1.00 NL 0.98 NY 0.99 ! OV 0.98 PT 1.01 ! ! A total of 24 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.00 MK 1.00 NY 0.99 ON 1.00 ! OV 1.02 WZ 1.02 ! ! Telescope amplitude corrections in sub-array 7: ! KP 1.01 MK 1.02 ON 1.00 OV 1.02 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! FD 1.03 HN 0.99 LA 0.98 NL 0.99 ! NY 1.00 PT 1.01 SC 0.99 WZ 0.98 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 1.00 HN 0.99 KP 1.02 ! LA 0.98 NL 0.99 NY 1.02 ON 0.99 ! OV 1.02 PT 1.00 ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* HN 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 1.02 HN 1.00 KP 1.00 ! LA 0.99 MK 0.99 NL 0.99 OV 0.99 ! PT 1.02 SC 0.99 ! ! A total of 12 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 FD 1.00 HN 1.03 KP 1.01 ! LA 0.96 MK 1.01 NL 0.98 NY 0.98 ! OV 0.99 PT 1.00 ! ! A total of 24 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.01 MK 1.02 NY 1.00 ON 0.99 ! OV 1.00 WZ 1.02 ! ! Telescope amplitude corrections in sub-array 7: ! KP 1.00 MK 1.03 ON 1.04 OV 1.02 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! FD 1.04 HN 0.98 LA 0.99 NL 0.99 ! NY 1.01 PT 1.03 SC 0.99 WZ 0.97 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 FD 1.00 HN 0.98 KP 1.02 ! LA 0.99 NL 0.99 NY 1.01 ON 0.96 ! OV 1.02 PT 1.01 ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* HN 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 1.00 HN 1.00 KP 1.00 ! LA 0.99 MK 0.98 NL 0.99 OV 0.99 ! PT 1.01 SC 0.98 ! ! A total of 12 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 FD 0.99 HN 1.03 KP 1.02 ! LA 1.00 MK 1.00 NL 0.99 NY 0.97 ! OV 0.99 PT 0.99 ! ! A total of 24 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 1.00 MK 1.06 NY 0.99 ON 0.99 ! OV 1.00 WZ 1.02 ! ! Telescope amplitude corrections in sub-array 7: ! KP 0.97 MK 1.02 ON 1.06 OV 1.01 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! FD 1.05 HN 0.98 LA 1.00 NL 1.00 ! NY 0.98 PT 1.02 SC 0.98 WZ 0.98 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 1.00 HN 0.97 KP 1.01 ! LA 0.99 NL 0.98 NY 1.00 ON 0.99 ! OV 1.00 PT 1.01 ! ! A total of 6 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* HN 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 FD 1.01 HN 0.99 KP 1.00 ! LA 0.99 MK 0.97 NL 1.00 OV 0.98 ! PT 1.00 SC 0.98 ! ! A total of 12 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 FD 1.00 HN 1.04 KP 1.01 ! LA 0.99 MK 1.00 NL 0.97 NY 0.98 ! OV 1.00 PT 1.01 ! ! A total of 24 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! BR 0.99 MK 1.03 NY 0.95 ON 0.99 ! OV 1.05 WZ 1.01 ! ! Telescope amplitude corrections in sub-array 7: ! KP 0.97 MK 1.01 ON 0.99 OV 1.03 ! ! ! Fit before self-cal, rms=0.130635Jy sigma=1.277565 ! Fit after self-cal, rms=0.126696Jy sigma=1.214394 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! Estimated beam: bmin=0.7987 mas, bmaj=1.122 mas, bpa=15.49 degrees ! Estimated noise=1.39539 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 = 0.00235957 Jy ! Component: 100 - total flux cleaned = 0.00330093 Jy ! Component: 150 - total flux cleaned = 0.00379994 Jy ! Component: 200 - total flux cleaned = 0.00357792 Jy ! Total flux subtracted in 200 components = 0.00357792 Jy ! Clean residual min=-0.012081 max=0.013687 Jy/beam ! Clean residual mean=-0.000004 rms=0.002776 Jy/beam ! Combined flux in latest and established models = 2.57614 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 48 components and 2.57614 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.125260Jy sigma=1.202951 ! Fit after self-cal, rms=0.124984Jy sigma=1.199619 ! Inverting map ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 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. ! ! Fit before self-cal, rms=0.124984Jy sigma=1.199619 ! Fit after self-cal, rms=0.082558Jy sigma=0.789225 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! Estimated beam: bmin=0.7984 mas, bmaj=1.123 mas, bpa=15.33 degrees ! Estimated noise=1.39694 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00313728 Jy ! Component: 100 - total flux cleaned = 0.00313109 Jy ! Component: 150 - total flux cleaned = 0.00274103 Jy ! Component: 200 - total flux cleaned = 0.00241434 Jy ! Total flux subtracted in 200 components = 0.00241434 Jy ! Clean residual min=-0.005028 max=0.006140 Jy/beam ! Clean residual mean=0.000008 rms=0.001268 Jy/beam ! Combined flux in latest and established models = 2.57855 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 53 components and 2.57855 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081313Jy sigma=0.776475 ! Fit after self-cal, rms=0.081023Jy sigma=0.773602 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 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 (-3, -30.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00255632 Jy ! Component: 100 - total flux cleaned = 0.00472156 Jy ! Component: 150 - total flux cleaned = 0.0052162 Jy ! Component: 200 - total flux cleaned = 0.00536158 Jy ! Total flux subtracted in 200 components = 0.00536158 Jy ! Clean residual min=-0.005065 max=0.005694 Jy/beam ! Clean residual mean=0.000006 rms=0.001223 Jy/beam ! Combined flux in latest and established models = 2.58391 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 66 components and 2.58391 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.080161Jy sigma=0.764689 ! Fit after self-cal, rms=0.080002Jy sigma=0.763325 ! Inverting map ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! Added new window around map position (26.8, 22). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00322705 Jy ! Component: 100 - total flux cleaned = 0.00502367 Jy ! Component: 150 - total flux cleaned = 0.00615903 Jy ! Component: 200 - total flux cleaned = 0.00680716 Jy ! Total flux subtracted in 200 components = 0.00680716 Jy ! Clean residual min=-0.004915 max=0.005382 Jy/beam ! Clean residual mean=0.000005 rms=0.001187 Jy/beam ! Combined flux in latest and established models = 2.59072 Jy ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 75 components and 2.59072 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.079357Jy sigma=0.756174 ! Fit after self-cal, rms=0.079290Jy sigma=0.755380 ! Inverting map ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! Added new window around map position (1, 5.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00325061 Jy ! Component: 100 - total flux cleaned = 0.00413503 Jy ! Component: 150 - total flux cleaned = 0.00464963 Jy ! Component: 200 - total flux cleaned = 0.00501122 Jy ! Total flux subtracted in 200 components = 0.00501122 Jy ! Clean residual min=-0.004731 max=0.005461 Jy/beam ! Clean residual mean=0.000007 rms=0.001163 Jy/beam ! Combined flux in latest and established models = 2.59573 Jy ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 84 components and 2.59573 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.078742Jy sigma=0.749646 ! Fit after self-cal, rms=0.078691Jy sigma=0.749096 ! Inverting map ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! Added new window around map position (-19, 33.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00383892 Jy ! Component: 100 - total flux cleaned = 0.00588669 Jy ! Component: 150 - total flux cleaned = 0.00708752 Jy ! Component: 200 - total flux cleaned = 0.00763824 Jy ! Total flux subtracted in 200 components = 0.00763824 Jy ! Clean residual min=-0.004707 max=0.004871 Jy/beam ! Clean residual mean=0.000006 rms=0.001130 Jy/beam ! Combined flux in latest and established models = 2.60337 Jy ! Performing phase self-cal ! Adding 31 model components to the UV plane model. ! The established model now contains 94 components and 2.60337 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.078242Jy sigma=0.743676 ! Fit after self-cal, rms=0.078181Jy sigma=0.743175 ! Inverting map ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 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. ! ! Fit before self-cal, rms=0.078181Jy sigma=0.743175 ! Fit after self-cal, rms=0.073263Jy sigma=0.699449 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! Estimated beam: bmin=0.798 mas, bmaj=1.122 mas, bpa=15.36 degrees ! Estimated noise=1.39735 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000856072 Jy ! Component: 100 - total flux cleaned = 0.000105904 Jy ! Component: 150 - total flux cleaned = -0.000452756 Jy ! Component: 200 - total flux cleaned = -0.00116617 Jy ! Total flux subtracted in 200 components = -0.00116617 Jy ! Clean residual min=-0.003845 max=0.003912 Jy/beam ! Clean residual mean=0.000007 rms=0.000885 Jy/beam ! Combined flux in latest and established models = 2.6022 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 103 components and 2.6022 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.072881Jy sigma=0.695502 ! Fit after self-cal, rms=0.072835Jy sigma=0.695174 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 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 (10, -7.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00314672 Jy ! Component: 100 - total flux cleaned = 0.00372021 Jy ! Component: 150 - total flux cleaned = 0.00343482 Jy ! Component: 200 - total flux cleaned = 0.00316871 Jy ! Total flux subtracted in 200 components = 0.00316871 Jy ! Clean residual min=-0.003854 max=0.003710 Jy/beam ! Clean residual mean=0.000009 rms=0.000861 Jy/beam ! Combined flux in latest and established models = 2.60537 Jy ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 113 components and 2.60537 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.072518Jy sigma=0.691358 ! Fit after self-cal, rms=0.072461Jy sigma=0.691035 ! Inverting map ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 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. ! ! Fit before self-cal, rms=0.072461Jy sigma=0.691035 ! Fit after self-cal, rms=0.072352Jy sigma=0.690349 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! Estimated beam: bmin=2.429 mas, bmaj=2.721 mas, bpa=74.65 degrees ! Estimated noise=1.99939 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00259596 Jy ! Component: 100 - total flux cleaned = 0.00251528 Jy ! Component: 150 - total flux cleaned = 0.00243407 Jy ! Component: 200 - total flux cleaned = 0.00236668 Jy ! Total flux subtracted in 200 components = 0.00236668 Jy ! Clean residual min=-0.003855 max=0.005275 Jy/beam ! Clean residual mean=0.000020 rms=0.001097 Jy/beam ! Combined flux in latest and established models = 2.60774 Jy selfcal ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 135 components and 2.60774 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.072292Jy sigma=0.689683 ! Fit after self-cal, rms=0.072277Jy sigma=0.689521 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 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 (12.8, -11.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00478362 Jy ! Component: 100 - total flux cleaned = 0.00761121 Jy ! Component: 150 - total flux cleaned = 0.00927961 Jy ! Component: 200 - total flux cleaned = 0.00972603 Jy ! Total flux subtracted in 200 components = 0.00972603 Jy ! Clean residual min=-0.003803 max=0.003450 Jy/beam ! Clean residual mean=0.000029 rms=0.001033 Jy/beam ! Combined flux in latest and established models = 2.61747 Jy ! Performing phase self-cal ! Adding 38 model components to the UV plane model. ! The established model now contains 166 components and 2.61747 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.072047Jy sigma=0.687396 ! Fit after self-cal, rms=0.072021Jy sigma=0.687147 ! Inverting map ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 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 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! Estimated beam: bmin=0.7977 mas, bmaj=1.122 mas, bpa=15.36 degrees ! Estimated noise=1.39763 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7977 x 1.122 at 15.36 degrees (North through East) ! Clean map min=-0.0032473 max=2.0915 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. ! ! Fit before self-cal, rms=0.072021Jy sigma=0.687147 ! Fit after self-cal, rms=0.060762Jy sigma=0.532774 ! Inverting map and beam ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! Estimated beam: bmin=0.7976 mas, bmaj=1.122 mas, bpa=15.35 degrees ! Estimated noise=1.39775 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00302359 Jy ! Component: 100 - total flux cleaned = 0.00388644 Jy ! Component: 150 - total flux cleaned = 0.0043831 Jy ! Component: 200 - total flux cleaned = 0.00466209 Jy ! Total flux subtracted in 200 components = 0.00466209 Jy ! Clean residual min=-0.003516 max=0.003617 Jy/beam ! Clean residual mean=0.000011 rms=0.000817 Jy/beam ! Combined flux in latest and established models = 2.62213 Jy ! Performing phase self-cal ! Adding 35 model components to the UV plane model. ! The established model now contains 189 components and 2.62213 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.060423Jy sigma=0.528977 ! Fit after self-cal, rms=0.060401Jy sigma=0.528855 ! Inverting map ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! Added new window around map position (-11, 29.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00226991 Jy ! Component: 100 - total flux cleaned = 0.00301562 Jy ! Component: 150 - total flux cleaned = 0.00310285 Jy ! Component: 200 - total flux cleaned = 0.00301659 Jy ! Total flux subtracted in 200 components = 0.00301659 Jy ! Clean residual min=-0.003416 max=0.003394 Jy/beam ! Clean residual mean=0.000011 rms=0.000803 Jy/beam ! Combined flux in latest and established models = 2.62514 Jy ! Performing phase self-cal ! Adding 43 model components to the UV plane model. ! The established model now contains 202 components and 2.62514 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.060104Jy sigma=0.525545 ! Fit after self-cal, rms=0.060079Jy sigma=0.525398 ! Inverting map ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.060079Jy sigma=0.525398 ! Fit after self-cal, rms=0.060018Jy sigma=0.525006 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 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! Estimated beam: bmin=0.6745 mas, bmaj=0.9897 mas, bpa=14.59 degrees ! Estimated noise=1.57251 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.61391 Jy ! Component: 100 - total flux cleaned = 2.06506 Jy ! Component: 150 - total flux cleaned = 2.27046 Jy ! Component: 200 - total flux cleaned = 2.38593 Jy ! Total flux subtracted in 200 components = 2.38593 Jy ! Clean residual min=-0.011915 max=0.058386 Jy/beam ! Clean residual mean=-0.000027 rms=0.003175 Jy/beam ! Combined flux in latest and established models = 2.38593 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 2.38593 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! Estimated beam: bmin=0.7974 mas, bmaj=1.122 mas, bpa=15.35 degrees ! Estimated noise=1.398 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 = 0.0907104 Jy ! Component: 100 - total flux cleaned = 0.138633 Jy ! Component: 150 - total flux cleaned = 0.16556 Jy ! Component: 200 - total flux cleaned = 0.181048 Jy ! Total flux subtracted in 200 components = 0.181048 Jy ! Clean residual min=-0.004758 max=0.007780 Jy/beam ! Clean residual mean=-0.000003 rms=0.001084 Jy/beam ! Combined flux in latest and established models = 2.56697 Jy ! Adding 28 model components to the UV plane model. ! The established model now contains 31 components and 2.56697 Jy ! Inverting map ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00933495 Jy ! Component: 100 - total flux cleaned = 0.0162119 Jy ! Component: 150 - total flux cleaned = 0.0213857 Jy ! Component: 200 - total flux cleaned = 0.025138 Jy ! Total flux subtracted in 200 components = 0.025138 Jy ! Clean residual min=-0.004076 max=0.004284 Jy/beam ! Clean residual mean=0.000005 rms=0.000939 Jy/beam ! Combined flux in latest and established models = 2.59211 Jy ! Adding 38 model components to the UV plane model. ! The established model now contains 57 components and 2.59211 Jy ! Inverting map ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! Added new window around map position (-1, -1.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00262442 Jy ! Component: 100 - total flux cleaned = 0.00497256 Jy ! Component: 150 - total flux cleaned = 0.00718531 Jy ! Component: 200 - total flux cleaned = 0.00958875 Jy ! Total flux subtracted in 200 components = 0.00958875 Jy ! Clean residual min=-0.003972 max=0.003860 Jy/beam ! Clean residual mean=0.000006 rms=0.000890 Jy/beam ! Combined flux in latest and established models = 2.6017 Jy ! Adding 53 model components to the UV plane model. ! The established model now contains 81 components and 2.6017 Jy ! Inverting map ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 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 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! Estimated beam: bmin=2.428 mas, bmaj=2.721 mas, bpa=74.62 degrees ! Estimated noise=2.00074 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00503318 Jy ! Component: 100 - total flux cleaned = 0.00879911 Jy ! Component: 150 - total flux cleaned = 0.0111524 Jy ! Component: 200 - total flux cleaned = 0.012869 Jy ! Total flux subtracted in 200 components = 0.012869 Jy ! Clean residual min=-0.003854 max=0.003300 Jy/beam ! Clean residual mean=0.000025 rms=0.001021 Jy/beam ! Combined flux in latest and established models = 2.61457 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 = 0.00160938 Jy ! Component: 100 - total flux cleaned = 0.00289306 Jy ! Component: 150 - total flux cleaned = 0.0038377 Jy ! Component: 200 - total flux cleaned = 0.00449972 Jy ! Total flux subtracted in 200 components = 0.00449972 Jy ! Clean residual min=-0.003652 max=0.003240 Jy/beam ! Clean residual mean=0.000027 rms=0.000995 Jy/beam ! Combined flux in latest and established models = 2.61907 Jy ! Adding 66 model components to the UV plane model. ! The established model now contains 143 components and 2.61907 Jy ! Inverting map ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! Estimated beam: bmin=0.7974 mas, bmaj=1.122 mas, bpa=15.35 degrees ! Estimated noise=1.398 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00124951 Jy ! Component: 100 - total flux cleaned = -0.00111362 Jy ! Component: 150 - total flux cleaned = -0.000860404 Jy ! Component: 200 - total flux cleaned = -0.00062333 Jy ! Total flux subtracted in 200 components = -0.00062333 Jy ! Clean residual min=-0.003931 max=0.003741 Jy/beam ! Clean residual mean=0.000010 rms=0.000838 Jy/beam ! Combined flux in latest and established models = 2.61845 Jy selfcal ! Performing phase self-cal ! Adding 36 model components to the UV plane model. ! The established model now contains 158 components and 2.61845 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.060837Jy sigma=0.539347 ! Fit after self-cal, rms=0.060206Jy sigma=0.529582 wmodel J1419+5423_X_map.mod ! Writing 158 model components to file: J1419+5423_X_map.mod wobs J1419+5423_X_uvs.fits ! Writing UV FITS file: J1419+5423_X_uvs.fits wwins J1419+5423_X_map.win ! wwins: Wrote 10 windows to J1419+5423_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 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00119863 Jy ! Component: 100 - total flux cleaned = -0.00184425 Jy ! Component: 150 - total flux cleaned = -0.00246162 Jy ! Component: 200 - total flux cleaned = -0.00300284 Jy ! Component: 250 - total flux cleaned = -0.00347545 Jy ! Component: 300 - total flux cleaned = -0.00394001 Jy ! Component: 350 - total flux cleaned = -0.00411265 Jy ! Component: 400 - total flux cleaned = -0.0045659 Jy ! Component: 450 - total flux cleaned = -0.00490114 Jy ! Component: 500 - total flux cleaned = -0.00490149 Jy ! Component: 550 - total flux cleaned = -0.0052307 Jy ! Component: 600 - total flux cleaned = -0.00533841 Jy ! Component: 650 - total flux cleaned = -0.00544581 Jy ! Component: 700 - total flux cleaned = -0.00549842 Jy ! Component: 750 - total flux cleaned = -0.00555118 Jy ! Component: 800 - total flux cleaned = -0.00555112 Jy ! Component: 850 - total flux cleaned = -0.00565436 Jy ! Component: 900 - total flux cleaned = -0.00560273 Jy ! Component: 950 - total flux cleaned = -0.00565408 Jy ! Component: 1000 - total flux cleaned = -0.00565463 Jy ! Component: 1050 - total flux cleaned = -0.00575531 Jy ! Component: 1100 - total flux cleaned = -0.00575486 Jy ! Component: 1150 - total flux cleaned = -0.00595249 Jy ! Component: 1200 - total flux cleaned = -0.00590334 Jy ! Component: 1250 - total flux cleaned = -0.00595209 Jy ! Component: 1300 - total flux cleaned = -0.00595219 Jy ! Component: 1350 - total flux cleaned = -0.00628791 Jy ! Component: 1400 - total flux cleaned = -0.00604887 Jy ! Component: 1450 - total flux cleaned = -0.00619158 Jy ! Component: 1500 - total flux cleaned = -0.00628604 Jy ! Component: 1550 - total flux cleaned = -0.00623936 Jy ! Component: 1600 - total flux cleaned = -0.00656531 Jy ! Component: 1650 - total flux cleaned = -0.0066579 Jy ! Component: 1700 - total flux cleaned = -0.00670442 Jy ! Component: 1750 - total flux cleaned = -0.00688742 Jy ! Component: 1800 - total flux cleaned = -0.00711513 Jy ! Component: 1850 - total flux cleaned = -0.00716035 Jy ! Component: 1900 - total flux cleaned = -0.00697998 Jy ! Component: 1950 - total flux cleaned = -0.00706983 Jy ! Component: 2000 - total flux cleaned = -0.00724873 Jy ! Component: 2050 - total flux cleaned = -0.00729284 Jy ! Component: 2100 - total flux cleaned = -0.00751392 Jy ! Component: 2150 - total flux cleaned = -0.007382 Jy ! Component: 2200 - total flux cleaned = -0.00729415 Jy ! Component: 2250 - total flux cleaned = -0.00746859 Jy ! Component: 2300 - total flux cleaned = -0.00755529 Jy ! Component: 2350 - total flux cleaned = -0.00746884 Jy ! Component: 2400 - total flux cleaned = -0.00764099 Jy ! Component: 2450 - total flux cleaned = -0.0075554 Jy ! Component: 2500 - total flux cleaned = -0.00755532 Jy ! Component: 2550 - total flux cleaned = -0.00772507 Jy ! Component: 2600 - total flux cleaned = -0.00759823 Jy ! Component: 2650 - total flux cleaned = -0.00768216 Jy ! Component: 2700 - total flux cleaned = -0.00768235 Jy ! Component: 2750 - total flux cleaned = -0.00768237 Jy ! Component: 2800 - total flux cleaned = -0.00759891 Jy ! Component: 2850 - total flux cleaned = -0.00764029 Jy ! Component: 2900 - total flux cleaned = -0.00768173 Jy ! Component: 2950 - total flux cleaned = -0.00755846 Jy ! Component: 3000 - total flux cleaned = -0.00764029 Jy ! Component: 3050 - total flux cleaned = -0.00764037 Jy ! Component: 3100 - total flux cleaned = -0.00747809 Jy ! Component: 3150 - total flux cleaned = -0.00768032 Jy ! Component: 3200 - total flux cleaned = -0.00751936 Jy ! Component: 3250 - total flux cleaned = -0.00751916 Jy ! Component: 3300 - total flux cleaned = -0.00759904 Jy ! Component: 3350 - total flux cleaned = -0.0077183 Jy ! Component: 3400 - total flux cleaned = -0.00755969 Jy ! Component: 3450 - total flux cleaned = -0.00763865 Jy ! Component: 3500 - total flux cleaned = -0.0079536 Jy ! Component: 3550 - total flux cleaned = -0.00787536 Jy ! Component: 3600 - total flux cleaned = -0.00752385 Jy ! Component: 3650 - total flux cleaned = -0.00771845 Jy ! Component: 3700 - total flux cleaned = -0.00779592 Jy ! Component: 3750 - total flux cleaned = -0.00764138 Jy ! Component: 3800 - total flux cleaned = -0.00783407 Jy ! Component: 3850 - total flux cleaned = -0.00775764 Jy ! Component: 3900 - total flux cleaned = -0.00775779 Jy ! Component: 3950 - total flux cleaned = -0.0077956 Jy ! Component: 4000 - total flux cleaned = -0.00790953 Jy ! Component: 4050 - total flux cleaned = -0.0078339 Jy ! Total flux subtracted in 4096 components = -0.00787182 Jy ! Clean residual min=-0.002705 max=0.002265 Jy/beam ! Clean residual mean=0.000004 rms=0.000625 Jy/beam ! Combined flux in latest and established models = 2.61058 Jy keep ! Adding 350 model components to the UV plane model. ! The established model now contains 507 components and 2.61058 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv117_uvs/J1419+5423_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7974 x 1.122 at 15.35 degrees (North through East) ! Clean map min=-0.0033233 max=2.089 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv117_uvs/J1419+5423_X_map.fits wmodel /scr/pima/rv117_uvs/J1419+5423_X_map.mod ! Writing 507 model components to file: /scr/pima/rv117_uvs/J1419+5423_X_map.mod wobs /scr/pima/rv117_uvs/J1419+5423_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv117_uvs/J1419+5423_X_uvs.fits wwins /scr/pima/rv117_uvs/J1419+5423_X_map.win ! wwins: Wrote 11 windows to /scr/pima/rv117_uvs/J1419+5423_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 2.08903 invert ! Inverting map ! Your choice of large map pixels excluded 0.31% of the data. ! The x-axis pixel size should ideally be below 0.1847 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000625028 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.0897587 0.0897587 0.179517 0.359035 0.71807 1.43614 2.87228 5.74456 11.4891 22.9782 45.9565 91.9129 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0018 print "peak= ", int(1000*peak_flux)/1000 ! peak= 2.089 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 3342.29 quit ! Quitting program ! Log file /scr/pima/rv117_uvs/J1419+5423_X_dfm.log closed on Sat Dec 9 23:44:26 2017