! Started logfile: /scr/pima/rv120_uvs/J1308+3546_X_dfm.log on Fri Dec 22 22:42:32 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/rv120_uvs/J1308+3546_X_uva.fits ! Reading UV FITS file: /scr/pima/rv120_uvs/J1308+3546_X_uva.fits ! AN table 1: 26 integrations on 45 of 45 possible baselines. ! AN table 2: 58 integrations on 21 of 21 possible baselines. ! AN table 3: 87 integrations on 55 of 55 possible baselines. ! AN table 4: 29 integrations on 1 of 1 possible baselines. ! Apparent sampling: 0.546515 visibilities/baseline/integration-bin. ! Found source: J1308+3546 ! ! 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 79 lines of history. ! ! Reading 15744 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 J1308+3546_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 26 telescope corrections were flagged in sub-array 1. ! A total of 46 telescope corrections were flagged in sub-array 2. ! A total of 551 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 26 telescope corrections were flagged in sub-array 1. ! A total of 46 telescope corrections were flagged in sub-array 2. ! A total of 551 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 26 telescope corrections were flagged in sub-array 1. ! A total of 46 telescope corrections were flagged in sub-array 2. ! A total of 551 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 26 telescope corrections were flagged in sub-array 1. ! A total of 46 telescope corrections were flagged in sub-array 2. ! A total of 551 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=1.085773Jy sigma=19.738407 ! Fit after self-cal, rms=0.609054Jy sigma=10.876615 ! 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 3.59% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! Estimated beam: bmin=0.7164 mas, bmaj=0.874 mas, bpa=26.16 degrees ! Estimated noise=0.597852 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 = 0.308988 Jy ! Component: 100 - total flux cleaned = 0.376685 Jy ! Total flux subtracted in 100 components = 0.376685 Jy ! Clean residual min=-0.009513 max=0.021176 Jy/beam ! Clean residual mean=-0.000017 rms=0.001758 Jy/beam ! Combined flux in latest and established models = 0.376685 Jy ! Performing phase self-cal ! Adding 3 model components to the UV plane model. ! The established model now contains 3 components and 0.376685 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.091418Jy sigma=1.334043 ! Fit after self-cal, rms=0.091398Jy sigma=1.333926 ! Inverting map ! Your choice of large map pixels excluded 3.59% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0220146 Jy ! Component: 100 - total flux cleaned = 0.0261591 Jy ! Total flux subtracted in 100 components = 0.0261591 Jy ! Clean residual min=-0.008963 max=0.010293 Jy/beam ! Clean residual mean=-0.000007 rms=0.001449 Jy/beam ! Combined flux in latest and established models = 0.402844 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 10 components and 0.402844 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.087186Jy sigma=1.177209 ! Fit after self-cal, rms=0.087128Jy sigma=1.177002 ! Inverting map ! Your choice of large map pixels excluded 3.59% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! Added new window around map position (1, -1). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00495529 Jy ! Component: 100 - total flux cleaned = 0.00635559 Jy ! Total flux subtracted in 100 components = 0.00635559 Jy ! Clean residual min=-0.008747 max=0.009450 Jy/beam ! Clean residual mean=-0.000005 rms=0.001372 Jy/beam ! Combined flux in latest and established models = 0.4092 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 17 components and 0.4092 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.086303Jy sigma=1.152033 ! Fit after self-cal, rms=0.086276Jy sigma=1.150880 ! Inverting map ! Your choice of large map pixels excluded 3.59% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! Added new window around map position (-1.8, -0.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00526115 Jy ! Component: 100 - total flux cleaned = 0.00661251 Jy ! Total flux subtracted in 100 components = 0.00661251 Jy ! Clean residual min=-0.008484 max=0.007427 Jy/beam ! Clean residual mean=-0.000003 rms=0.001334 Jy/beam ! Combined flux in latest and established models = 0.415812 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 21 components and 0.415812 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.085646Jy sigma=1.139804 ! Fit after self-cal, rms=0.085583Jy sigma=1.138774 ! Inverting map ! Your choice of large map pixels excluded 3.59% of the data. ! The y-axis pixel size should ideally be below 0.1609 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 3.59% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! Estimated beam: bmin=0.8923 mas, bmaj=1.036 mas, bpa=24.33 degrees ! Estimated noise=0.350333 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 (1.8, 0.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00372652 Jy ! Component: 100 - total flux cleaned = 0.00461366 Jy ! Component: 150 - total flux cleaned = 0.00443627 Jy ! Component: 200 - total flux cleaned = 0.00443589 Jy ! Total flux subtracted in 200 components = 0.00443589 Jy ! Clean residual min=-0.005907 max=0.006733 Jy/beam ! Clean residual mean=-0.000003 rms=0.001047 Jy/beam ! Combined flux in latest and established models = 0.420248 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 37 components and 0.420248 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.084525Jy sigma=1.117405 ! Fit after self-cal, rms=0.084492Jy sigma=1.116823 ! Inverting map ! Your choice of large map pixels excluded 3.59% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! Added new window around map position (4.4, -1). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00160244 Jy ! Component: 100 - total flux cleaned = 0.00178721 Jy ! Component: 150 - total flux cleaned = 0.00195119 Jy ! Component: 200 - total flux cleaned = 0.00210208 Jy ! Total flux subtracted in 200 components = 0.00210208 Jy ! Clean residual min=-0.005711 max=0.005443 Jy/beam ! Clean residual mean=-0.000002 rms=0.001006 Jy/beam ! Combined flux in latest and established models = 0.42235 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 50 components and 0.42235 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.083537Jy sigma=1.103440 ! Fit after self-cal, rms=0.083529Jy sigma=1.102748 ! Inverting map ! Your choice of large map pixels excluded 3.59% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8923 x 1.036 at 24.33 degrees (North through East) ! Clean map min=-0.0077323 max=0.39314 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.98 HN 1.03 KP 0.99 ! LA 0.98 MK 0.96 NL 0.99 NY 0.98 ! OV 0.98 PT 1.01 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.07 HH 0.93 HN 1.13 NL 1.01 ! NY 0.97 SC 1.11 WZ 0.94 ! ! A total of 24 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 1.01 HN 0.94 KK 1.12 ! KP 1.00 LA 1.01 MK 0.98 NL 0.99 ! OV 1.01 PT 1.01 SC 0.97 ! ! Telescope amplitude corrections in sub-array 4: ! KK 0.00* NY 0.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.99 HN 1.03 KP 0.99 ! LA 0.99 MK 0.96 NL 1.00 NY 1.02 ! OV 0.99 PT 1.00 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.06 HH 0.93 HN 1.15 NL 1.02 ! NY 0.99 SC 1.11 WZ 0.92 ! ! A total of 24 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.01 HN 0.91 KK 1.10 ! KP 1.00 LA 1.01 MK 1.01 NL 0.99 ! OV 1.00 PT 1.00 SC 0.98 ! ! Telescope amplitude corrections in sub-array 4: ! KK 0.00* NY 0.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 0.97 HN 1.00 KP 0.98 ! LA 0.98 MK 0.96 NL 0.97 NY 1.01 ! OV 0.98 PT 0.99 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.07 HH 0.95 HN 1.15 NL 0.99 ! NY 0.99 SC 1.12 WZ 0.91 ! ! A total of 24 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 FD 1.01 HN 0.92 KK 1.07 ! KP 1.00 LA 1.00 MK 0.99 NL 0.97 ! OV 0.99 PT 0.99 SC 0.94 ! ! Telescope amplitude corrections in sub-array 4: ! KK 0.00* NY 0.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 0.96 HN 1.04 KP 0.97 ! LA 0.96 MK 0.97 NL 0.97 NY 0.99 ! OV 0.97 PT 0.98 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.08 HH 0.96 HN 1.14 NL 0.99 ! NY 0.99 SC 1.09 WZ 0.92 ! ! A total of 24 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 1.00 HN 0.92 KK 1.10 ! KP 0.99 LA 0.98 MK 1.02 NL 0.98 ! OV 0.98 PT 0.98 SC 0.96 ! ! Telescope amplitude corrections in sub-array 4: ! KK 0.00* NY 0.00* ! ! ! Fit before self-cal, rms=0.083529Jy sigma=1.102748 ! Fit after self-cal, rms=0.082002Jy sigma=1.035869 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! Estimated beam: bmin=0.89 mas, bmaj=1.044 mas, bpa=25.71 degrees ! Estimated noise=0.349388 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 = -0.00284423 Jy ! Component: 100 - total flux cleaned = -0.00298113 Jy ! Component: 150 - total flux cleaned = -0.00275744 Jy ! Component: 200 - total flux cleaned = -0.00265575 Jy ! Total flux subtracted in 200 components = -0.00265575 Jy ! Clean residual min=-0.003704 max=0.004076 Jy/beam ! Clean residual mean=0.000001 rms=0.000746 Jy/beam ! Combined flux in latest and established models = 0.419694 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 63 components and 0.419694 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081577Jy sigma=1.029111 ! Fit after self-cal, rms=0.081666Jy sigma=1.028811 ! Inverting map ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! Added new window around map position (-0.6, 1.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00259111 Jy ! Component: 100 - total flux cleaned = 0.00258787 Jy ! Component: 150 - total flux cleaned = 0.00268757 Jy ! Component: 200 - total flux cleaned = 0.00268684 Jy ! Total flux subtracted in 200 components = 0.00268684 Jy ! Clean residual min=-0.003473 max=0.003184 Jy/beam ! Clean residual mean=0.000004 rms=0.000735 Jy/beam ! Combined flux in latest and established models = 0.422381 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 74 components and 0.422381 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081329Jy sigma=1.024181 ! Fit after self-cal, rms=0.081301Jy sigma=1.023846 ! Inverting map ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 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=0.081301Jy sigma=1.023846 ! Fit after self-cal, rms=0.081805Jy sigma=0.960341 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! Estimated beam: bmin=0.8948 mas, bmaj=1.038 mas, bpa=24.97 degrees ! Estimated noise=0.350441 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00108692 Jy ! Component: 100 - total flux cleaned = 0.00131018 Jy ! Component: 150 - total flux cleaned = 0.001415 Jy ! Component: 200 - total flux cleaned = 0.00150519 Jy ! Total flux subtracted in 200 components = 0.00150519 Jy ! Clean residual min=-0.002122 max=0.002771 Jy/beam ! Clean residual mean=0.000002 rms=0.000508 Jy/beam ! Combined flux in latest and established models = 0.423886 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 93 components and 0.423886 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081482Jy sigma=0.954396 ! Fit after self-cal, rms=0.081517Jy sigma=0.954025 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 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 (-3.8, -6.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00188738 Jy ! Component: 100 - total flux cleaned = 0.00197357 Jy ! Component: 150 - total flux cleaned = 0.00189986 Jy ! Component: 200 - total flux cleaned = 0.00197154 Jy ! Total flux subtracted in 200 components = 0.00197154 Jy ! Clean residual min=-0.002126 max=0.002575 Jy/beam ! Clean residual mean=0.000003 rms=0.000490 Jy/beam ! Combined flux in latest and established models = 0.425858 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 103 components and 0.425858 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081305Jy sigma=0.950702 ! Fit after self-cal, rms=0.081295Jy sigma=0.950521 ! Inverting map ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! Added new window around map position (4, 7.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00191652 Jy ! Component: 100 - total flux cleaned = 0.00225354 Jy ! Component: 150 - total flux cleaned = 0.00238251 Jy ! Component: 200 - total flux cleaned = 0.00244418 Jy ! Total flux subtracted in 200 components = 0.00244418 Jy ! Clean residual min=-0.002155 max=0.002315 Jy/beam ! Clean residual mean=0.000004 rms=0.000477 Jy/beam ! Combined flux in latest and established models = 0.428302 Jy ! Performing phase self-cal ! Adding 38 model components to the UV plane model. ! The established model now contains 117 components and 0.428302 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081133Jy sigma=0.948073 ! Fit after self-cal, rms=0.081124Jy sigma=0.947974 ! Inverting map ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! Added new window around map position (-0.8, -1.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00079466 Jy ! Component: 100 - total flux cleaned = 0.000789087 Jy ! Component: 150 - total flux cleaned = 0.000789172 Jy ! Component: 200 - total flux cleaned = 0.000730212 Jy ! Total flux subtracted in 200 components = 0.000730212 Jy ! Clean residual min=-0.002082 max=0.002080 Jy/beam ! Clean residual mean=0.000005 rms=0.000466 Jy/beam ! Combined flux in latest and established models = 0.429032 Jy ! Performing phase self-cal ! Adding 41 model components to the UV plane model. ! The established model now contains 134 components and 0.429032 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081005Jy sigma=0.945580 ! Fit after self-cal, rms=0.080996Jy sigma=0.945489 ! Inverting map ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! Added new window around map position (-1.2, 4.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000341401 Jy ! Component: 100 - total flux cleaned = 0.000342791 Jy ! Component: 150 - total flux cleaned = 0.000282827 Jy ! Component: 200 - total flux cleaned = 0.000225338 Jy ! Total flux subtracted in 200 components = 0.000225338 Jy ! Clean residual min=-0.001988 max=0.001974 Jy/beam ! Clean residual mean=0.000005 rms=0.000452 Jy/beam ! Combined flux in latest and established models = 0.429258 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 143 components and 0.429258 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.080830Jy sigma=0.942789 ! Fit after self-cal, rms=0.080828Jy sigma=0.942677 ! Inverting map ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 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=0.080828Jy sigma=0.942677 ! Fit after self-cal, rms=0.081177Jy sigma=0.932049 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! Estimated beam: bmin=0.8945 mas, bmaj=1.035 mas, bpa=25.43 degrees ! Estimated noise=0.350749 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000515699 Jy ! Component: 100 - total flux cleaned = 0.000319495 Jy ! Component: 150 - total flux cleaned = 0.000138987 Jy ! Component: 200 - total flux cleaned = 8.28865e-05 Jy ! Total flux subtracted in 200 components = 8.28865e-05 Jy ! Clean residual min=-0.001613 max=0.001657 Jy/beam ! Clean residual mean=0.000002 rms=0.000375 Jy/beam ! Combined flux in latest and established models = 0.429341 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 154 components and 0.429341 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081054Jy sigma=0.930029 ! Fit after self-cal, rms=0.081063Jy sigma=0.929935 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 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 (1.2, -25). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000838593 Jy ! Component: 100 - total flux cleaned = 0.000785643 Jy ! Component: 150 - total flux cleaned = 0.000786299 Jy ! Component: 200 - total flux cleaned = 0.000835133 Jy ! Total flux subtracted in 200 components = 0.000835133 Jy ! Clean residual min=-0.001619 max=0.001502 Jy/beam ! Clean residual mean=0.000003 rms=0.000367 Jy/beam ! Combined flux in latest and established models = 0.430176 Jy ! Performing phase self-cal ! Adding 35 model components to the UV plane model. ! The established model now contains 168 components and 0.430176 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.080972Jy sigma=0.928511 ! Fit after self-cal, rms=0.080970Jy sigma=0.928458 ! Inverting map ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 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=0.080970Jy sigma=0.928458 ! Fit after self-cal, rms=0.081201Jy sigma=0.927979 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! Estimated beam: bmin=2.426 mas, bmaj=2.6 mas, bpa=-74.74 degrees ! Estimated noise=0.445508 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000369739 Jy ! Component: 100 - total flux cleaned = -0.000554767 Jy ! Component: 150 - total flux cleaned = -0.000555153 Jy ! Component: 200 - total flux cleaned = -0.000554971 Jy ! Total flux subtracted in 200 components = -0.000554971 Jy ! Clean residual min=-0.001746 max=0.001706 Jy/beam ! Clean residual mean=0.000006 rms=0.000416 Jy/beam ! Combined flux in latest and established models = 0.429621 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 184 components and 0.429621 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081173Jy sigma=0.927380 ! Fit after self-cal, rms=0.081171Jy sigma=0.927358 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -1.22647e-05 Jy ! Component: 100 - total flux cleaned = 1.21569e-05 Jy ! Component: 150 - total flux cleaned = 1.21103e-05 Jy ! Component: 200 - total flux cleaned = 5.75068e-05 Jy ! Total flux subtracted in 200 components = 5.75068e-05 Jy ! Clean residual min=-0.001729 max=0.001680 Jy/beam ! Clean residual mean=0.000006 rms=0.000414 Jy/beam ! Combined flux in latest and established models = 0.429678 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 191 components and 0.429678 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081154Jy sigma=0.926986 ! Fit after self-cal, rms=0.081153Jy sigma=0.926978 ! Inverting map ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 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 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! Estimated beam: bmin=0.8943 mas, bmaj=1.034 mas, bpa=25.41 degrees ! Estimated noise=0.350915 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8943 x 1.034 at 25.41 degrees (North through East) ! Clean map min=-0.0019086 max=0.39274 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 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! Estimated beam: bmin=0.7172 mas, bmaj=0.8668 mas, bpa=26.54 degrees ! Estimated noise=0.600281 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.309621 Jy ! Component: 100 - total flux cleaned = 0.37788 Jy ! Component: 150 - total flux cleaned = 0.39959 Jy ! Component: 200 - total flux cleaned = 0.409666 Jy ! Total flux subtracted in 200 components = 0.409666 Jy ! Clean residual min=-0.004494 max=0.004901 Jy/beam ! Clean residual mean=-0.000006 rms=0.000787 Jy/beam ! Combined flux in latest and established models = 0.409666 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 0.409666 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! Estimated beam: bmin=0.8943 mas, bmaj=1.034 mas, bpa=25.41 degrees ! Estimated noise=0.350915 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 = 0.00670826 Jy ! Component: 100 - total flux cleaned = 0.00878459 Jy ! Component: 150 - total flux cleaned = 0.0104053 Jy ! Component: 200 - total flux cleaned = 0.011972 Jy ! Total flux subtracted in 200 components = 0.011972 Jy ! Clean residual min=-0.002242 max=0.002756 Jy/beam ! Clean residual mean=-0.000003 rms=0.000469 Jy/beam ! Combined flux in latest and established models = 0.421638 Jy ! Adding 24 model components to the UV plane model. ! The established model now contains 30 components and 0.421638 Jy ! Inverting map ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! Added new window around map position (-2.4, 0.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00123003 Jy ! Component: 100 - total flux cleaned = 0.00217767 Jy ! Component: 150 - total flux cleaned = 0.00316458 Jy ! Component: 200 - total flux cleaned = 0.00367848 Jy ! Total flux subtracted in 200 components = 0.00367848 Jy ! Clean residual min=-0.001826 max=0.002396 Jy/beam ! Clean residual mean=-0.000000 rms=0.000429 Jy/beam ! Combined flux in latest and established models = 0.425316 Jy ! Adding 38 model components to the UV plane model. ! The established model now contains 49 components and 0.425316 Jy ! Inverting map ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! Added new window around map position (-2.2, -7). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00132518 Jy ! Component: 100 - total flux cleaned = 0.00160186 Jy ! Component: 150 - total flux cleaned = 0.00186457 Jy ! Component: 200 - total flux cleaned = 0.00203265 Jy ! Total flux subtracted in 200 components = 0.00203265 Jy ! Clean residual min=-0.001774 max=0.001985 Jy/beam ! Clean residual mean=0.000001 rms=0.000406 Jy/beam ! Combined flux in latest and established models = 0.427349 Jy ! Adding 39 model components to the UV plane model. ! The established model now contains 58 components and 0.427349 Jy ! Inverting map ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! Added new window around map position (1, 3.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000769744 Jy ! Component: 100 - total flux cleaned = 0.00107864 Jy ! Component: 150 - total flux cleaned = 0.00129778 Jy ! Component: 200 - total flux cleaned = 0.00157803 Jy ! Total flux subtracted in 200 components = 0.00157803 Jy ! Clean residual min=-0.001701 max=0.001644 Jy/beam ! Clean residual mean=0.000002 rms=0.000388 Jy/beam ! Combined flux in latest and established models = 0.428927 Jy ! Adding 42 model components to the UV plane model. ! The established model now contains 69 components and 0.428927 Jy ! Inverting map ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 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 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! Estimated beam: bmin=2.426 mas, bmaj=2.6 mas, bpa=-74.74 degrees ! Estimated noise=0.445508 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.001056 Jy ! Component: 100 - total flux cleaned = 0.00144918 Jy ! Component: 150 - total flux cleaned = 0.00158861 Jy ! Component: 200 - total flux cleaned = 0.00166465 Jy ! Total flux subtracted in 200 components = 0.00166465 Jy ! Clean residual min=-0.001762 max=0.001720 Jy/beam ! Clean residual mean=0.000007 rms=0.000416 Jy/beam ! Combined flux in latest and established models = 0.430591 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 = 4.68499e-05 Jy ! Component: 100 - total flux cleaned = 6.80032e-05 Jy ! Component: 150 - total flux cleaned = 6.77658e-05 Jy ! Component: 200 - total flux cleaned = 8.74054e-05 Jy ! Total flux subtracted in 200 components = 8.74054e-05 Jy ! Clean residual min=-0.001734 max=0.001696 Jy/beam ! Clean residual mean=0.000008 rms=0.000413 Jy/beam ! Combined flux in latest and established models = 0.430679 Jy ! Adding 38 model components to the UV plane model. ! The established model now contains 105 components and 0.430679 Jy ! Inverting map ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! Estimated beam: bmin=0.8943 mas, bmaj=1.034 mas, bpa=25.41 degrees ! Estimated noise=0.350915 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000156627 Jy ! Component: 100 - total flux cleaned = -9.3733e-05 Jy ! Component: 150 - total flux cleaned = 0.000147265 Jy ! Component: 200 - total flux cleaned = 0.000146246 Jy ! Total flux subtracted in 200 components = 0.000146246 Jy ! Clean residual min=-0.001665 max=0.001603 Jy/beam ! Clean residual mean=0.000003 rms=0.000370 Jy/beam ! Combined flux in latest and established models = 0.430825 Jy selfcal ! Performing phase self-cal ! Adding 36 model components to the UV plane model. ! The established model now contains 111 components and 0.430825 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081367Jy sigma=0.928876 ! Fit after self-cal, rms=0.081334Jy sigma=0.928146 wmodel J1308+3546_X_map.mod ! Writing 111 model components to file: J1308+3546_X_map.mod wobs J1308+3546_X_uvs.fits ! Writing UV FITS file: J1308+3546_X_uvs.fits wwins J1308+3546_X_map.win ! wwins: Wrote 14 windows to J1308+3546_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 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000621252 Jy ! Component: 100 - total flux cleaned = -0.000822618 Jy ! Component: 150 - total flux cleaned = -0.000906172 Jy ! Component: 200 - total flux cleaned = -0.000933094 Jy ! Component: 250 - total flux cleaned = -0.000854222 Jy ! Component: 300 - total flux cleaned = -0.000828901 Jy ! Component: 350 - total flux cleaned = -0.000803906 Jy ! Component: 400 - total flux cleaned = -0.000729262 Jy ! Component: 450 - total flux cleaned = -0.000655509 Jy ! Component: 500 - total flux cleaned = -0.000582713 Jy ! Component: 550 - total flux cleaned = -0.00046213 Jy ! Component: 600 - total flux cleaned = -0.000414725 Jy ! Component: 650 - total flux cleaned = -0.000320234 Jy ! Component: 700 - total flux cleaned = -0.000320441 Jy ! Component: 750 - total flux cleaned = -0.0002042 Jy ! Component: 800 - total flux cleaned = -0.00020405 Jy ! Component: 850 - total flux cleaned = -0.000181019 Jy ! Component: 900 - total flux cleaned = -0.000181072 Jy ! Component: 950 - total flux cleaned = -0.000180909 Jy ! Component: 1000 - total flux cleaned = -0.000203025 Jy ! Component: 1050 - total flux cleaned = -0.000180673 Jy ! Component: 1100 - total flux cleaned = -0.000224703 Jy ! Component: 1150 - total flux cleaned = -0.000246749 Jy ! Component: 1200 - total flux cleaned = -0.00029042 Jy ! Component: 1250 - total flux cleaned = -0.000311997 Jy ! Component: 1300 - total flux cleaned = -0.000290527 Jy ! Component: 1350 - total flux cleaned = -0.000375897 Jy ! Component: 1400 - total flux cleaned = -0.000269772 Jy ! Component: 1450 - total flux cleaned = -0.000311961 Jy ! Component: 1500 - total flux cleaned = -0.000354042 Jy ! Component: 1550 - total flux cleaned = -0.000333188 Jy ! Component: 1600 - total flux cleaned = -0.000333358 Jy ! Component: 1650 - total flux cleaned = -0.000395256 Jy ! Component: 1700 - total flux cleaned = -0.000313163 Jy ! Component: 1750 - total flux cleaned = -0.000374786 Jy ! Component: 1800 - total flux cleaned = -0.000476288 Jy ! Component: 1850 - total flux cleaned = -0.000415671 Jy ! Component: 1900 - total flux cleaned = -0.000435797 Jy ! Component: 1950 - total flux cleaned = -0.000516014 Jy ! Component: 2000 - total flux cleaned = -0.000515987 Jy ! Component: 2050 - total flux cleaned = -0.000476366 Jy ! Component: 2100 - total flux cleaned = -0.000496192 Jy ! Component: 2150 - total flux cleaned = -0.000555213 Jy ! Component: 2200 - total flux cleaned = -0.000633599 Jy ! Component: 2250 - total flux cleaned = -0.000633671 Jy ! Component: 2300 - total flux cleaned = -0.0006725 Jy ! Component: 2350 - total flux cleaned = -0.000691695 Jy ! Component: 2400 - total flux cleaned = -0.00076887 Jy ! Component: 2450 - total flux cleaned = -0.00069205 Jy ! Component: 2500 - total flux cleaned = -0.000691995 Jy ! Component: 2550 - total flux cleaned = -0.000711098 Jy ! Component: 2600 - total flux cleaned = -0.000749079 Jy ! Component: 2650 - total flux cleaned = -0.000692478 Jy ! Component: 2700 - total flux cleaned = -0.000748872 Jy ! Component: 2750 - total flux cleaned = -0.000842537 Jy ! Component: 2800 - total flux cleaned = -0.000823775 Jy ! Component: 2850 - total flux cleaned = -0.000842291 Jy ! Component: 2900 - total flux cleaned = -0.00087942 Jy ! Component: 2950 - total flux cleaned = -0.000805465 Jy ! Component: 3000 - total flux cleaned = -0.000860638 Jy ! Component: 3050 - total flux cleaned = -0.000879027 Jy ! Component: 3100 - total flux cleaned = -0.000933831 Jy ! Component: 3150 - total flux cleaned = -0.000970234 Jy ! Component: 3200 - total flux cleaned = -0.000897756 Jy ! Component: 3250 - total flux cleaned = -0.00087967 Jy ! Component: 3300 - total flux cleaned = -0.000897731 Jy ! Component: 3350 - total flux cleaned = -0.000987399 Jy ! Component: 3400 - total flux cleaned = -0.000951654 Jy ! Component: 3450 - total flux cleaned = -0.000987366 Jy ! Component: 3500 - total flux cleaned = -0.00091637 Jy ! Component: 3550 - total flux cleaned = -0.00100481 Jy ! Component: 3600 - total flux cleaned = -0.00104009 Jy ! Component: 3650 - total flux cleaned = -0.000969839 Jy ! Component: 3700 - total flux cleaned = -0.000917268 Jy ! Component: 3750 - total flux cleaned = -0.000969581 Jy ! Component: 3800 - total flux cleaned = -0.000969557 Jy ! Component: 3850 - total flux cleaned = -0.000986802 Jy ! Component: 3900 - total flux cleaned = -0.000969561 Jy ! Component: 3950 - total flux cleaned = -0.0008834 Jy ! Component: 4000 - total flux cleaned = -0.000883344 Jy ! Component: 4050 - total flux cleaned = -0.000900445 Jy ! Total flux subtracted in 4096 components = -0.000917527 Jy ! Clean residual min=-0.000853 max=0.001086 Jy/beam ! Clean residual mean=0.000002 rms=0.000282 Jy/beam ! Combined flux in latest and established models = 0.429908 Jy keep ! Adding 347 model components to the UV plane model. ! The established model now contains 454 components and 0.429908 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv120_uvs/J1308+3546_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8943 x 1.034 at 25.41 degrees (North through East) ! Clean map min=-0.0017084 max=0.39365 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv120_uvs/J1308+3546_X_map.fits wmodel /scr/pima/rv120_uvs/J1308+3546_X_map.mod ! Writing 454 model components to file: /scr/pima/rv120_uvs/J1308+3546_X_map.mod wobs /scr/pima/rv120_uvs/J1308+3546_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv120_uvs/J1308+3546_X_uvs.fits wwins /scr/pima/rv120_uvs/J1308+3546_X_map.win ! wwins: Wrote 15 windows to /scr/pima/rv120_uvs/J1308+3546_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.393654 invert ! Inverting map ! Your choice of large map pixels excluded 3.51% of the data. ! The y-axis pixel size should ideally be below 0.1609 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000281806 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.214761 0.214761 0.429522 0.859045 1.71809 3.43618 6.87236 13.7447 27.4894 54.9789 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0008 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.393 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 1396.9 quit ! Quitting program ! Log file /scr/pima/rv120_uvs/J1308+3546_X_dfm.log closed on Fri Dec 22 22:42:38 2017