! Started logfile: /scr/pima/rv119_uvs/J1130+3815_X_dfm.log on Sun Dec 17 11:35:40 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/rv119_uvs/J1130+3815_X_uva.fits ! Reading UV FITS file: /scr/pima/rv119_uvs/J1130+3815_X_uva.fits ! AN table 1: 32 integrations on 6 of 6 possible baselines. ! AN table 2: 5 integrations on 6 of 6 possible baselines. ! AN table 3: 42 integrations on 78 of 78 possible baselines. ! Apparent sampling: 0.282447 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1130+3815 ! ! 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 3952 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 J1130+3815_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 30 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! A total of 340 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 30 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! A total of 340 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 30 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! A total of 340 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 30 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! A total of 340 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=1.328814Jy sigma=18.596865 ! Fit after self-cal, rms=0.315129Jy sigma=3.912093 ! 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 5.23% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! Estimated beam: bmin=0.6657 mas, bmaj=0.8365 mas, bpa=-36.73 degrees ! Estimated noise=1.09587 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 = 0.629934 Jy ! Component: 100 - total flux cleaned = 0.837745 Jy ! Total flux subtracted in 100 components = 0.837745 Jy ! Clean residual min=-0.019867 max=0.092090 Jy/beam ! Clean residual mean=-0.000035 rms=0.004724 Jy/beam ! Combined flux in latest and established models = 0.837745 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.837745 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.215245Jy sigma=2.953091 ! Fit after self-cal, rms=0.210149Jy sigma=2.932461 ! Inverting map ! Your choice of large map pixels excluded 5.23% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.105736 Jy ! Component: 100 - total flux cleaned = 0.168531 Jy ! Total flux subtracted in 100 components = 0.168531 Jy ! Clean residual min=-0.010150 max=0.036193 Jy/beam ! Clean residual mean=-0.000016 rms=0.002539 Jy/beam ! Combined flux in latest and established models = 1.00628 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 19 components and 1.00628 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.133961Jy sigma=1.653826 ! Fit after self-cal, rms=0.131054Jy sigma=1.632127 ! Inverting map ! Your choice of large map pixels excluded 5.23% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! Added new window around map position (-0.2, -0.8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.045897 Jy ! Component: 100 - total flux cleaned = 0.0748891 Jy ! Total flux subtracted in 100 components = 0.0748891 Jy ! Clean residual min=-0.007196 max=0.018717 Jy/beam ! Clean residual mean=-0.000007 rms=0.001774 Jy/beam ! Combined flux in latest and established models = 1.08117 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 29 components and 1.08117 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.108940Jy sigma=1.234013 ! Fit after self-cal, rms=0.107552Jy sigma=1.218063 ! Inverting map ! Your choice of large map pixels excluded 5.23% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0230071 Jy ! Component: 100 - total flux cleaned = 0.0373129 Jy ! Total flux subtracted in 100 components = 0.0373129 Jy ! Clean residual min=-0.007007 max=0.010341 Jy/beam ! Clean residual mean=-0.000003 rms=0.001497 Jy/beam ! Combined flux in latest and established models = 1.11848 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 36 components and 1.11848 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.101254Jy sigma=1.093743 ! Fit after self-cal, rms=0.100611Jy sigma=1.086366 ! Inverting map ! Your choice of large map pixels excluded 5.23% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0121037 Jy ! Component: 100 - total flux cleaned = 0.0196063 Jy ! Total flux subtracted in 100 components = 0.0196063 Jy ! Clean residual min=-0.007017 max=0.008301 Jy/beam ! Clean residual mean=-0.000001 rms=0.001403 Jy/beam ! Combined flux in latest and established models = 1.13808 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 38 components and 1.13808 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.098682Jy sigma=1.047966 ! Fit after self-cal, rms=0.098445Jy sigma=1.045185 ! Inverting map ! Your choice of large map pixels excluded 5.23% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! Added new window around map position (1.4, -1.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00733968 Jy ! Component: 100 - total flux cleaned = 0.0102634 Jy ! Total flux subtracted in 100 components = 0.0102634 Jy ! Clean residual min=-0.006891 max=0.007571 Jy/beam ! Clean residual mean=0.000000 rms=0.001359 Jy/beam ! Combined flux in latest and established models = 1.14835 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 41 components and 1.14835 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.097542Jy sigma=1.030931 ! Fit after self-cal, rms=0.097468Jy sigma=1.030171 ! Inverting map ! Your choice of large map pixels excluded 5.23% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 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 5.23% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! Estimated beam: bmin=0.7397 mas, bmaj=0.9572 mas, bpa=-39.96 degrees ! Estimated noise=0.916364 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 (0.6, 2.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0076323 Jy ! Component: 100 - total flux cleaned = 0.0111924 Jy ! Component: 150 - total flux cleaned = 0.0128338 Jy ! Component: 200 - total flux cleaned = 0.0142531 Jy ! Total flux subtracted in 200 components = 0.0142531 Jy ! Clean residual min=-0.006068 max=0.006804 Jy/beam ! Clean residual mean=0.000007 rms=0.001314 Jy/beam ! Combined flux in latest and established models = 1.1626 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 56 components and 1.1626 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.096071Jy sigma=1.013628 ! Fit after self-cal, rms=0.095948Jy sigma=1.012074 ! Inverting map ! Your choice of large map pixels excluded 5.23% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7397 x 0.9572 at -39.96 degrees (North through East) ! Clean map min=-0.0055241 max=0.81836 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 66 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.89 HN 1.07 NY 1.00 ON 0.93 ! ! Telescope amplitude corrections in sub-array 2: ! FD 1.08 HH 0.83 HN 0.97 SC 1.00 ! ! A total of 24 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 0.98 HN 1.00 KP 0.98 ! LA 1.00 MK 1.01 NL 1.00 NY 0.99 ! ON 0.98 OV 0.99 PT 1.00 SC 0.98 ! WZ 1.00 ! ! ! Correcting IF 2. ! A total of 66 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.91 HN 1.15 NY 0.93 ON 0.93 ! ! Telescope amplitude corrections in sub-array 2: ! FD 1.10 HH 0.73 HN 0.96 SC 0.98 ! ! A total of 24 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 0.99 HN 1.00 KP 0.99 ! LA 0.99 MK 1.01 NL 1.00 NY 0.98 ! ON 1.01 OV 0.99 PT 1.00 SC 0.96 ! WZ 0.99 ! ! ! Correcting IF 3. ! A total of 66 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 1.08 HN 1.07 NY 1.01 ON 0.97 ! ! Telescope amplitude corrections in sub-array 2: ! FD 1.09 HH 0.86 HN 1.00 SC 1.02 ! ! A total of 24 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 0.98 HN 1.00 KP 0.99 ! LA 1.01 MK 1.01 NL 1.01 NY 1.00 ! ON 1.05 OV 0.99 PT 1.00 SC 0.97 ! WZ 0.97 ! ! ! Correcting IF 4. ! A total of 66 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 1.23 HN 1.17 NY 0.99 ON 0.95 ! ! Telescope amplitude corrections in sub-array 2: ! FD 1.12 HH 0.87 HN 1.02 SC 0.90 ! ! A total of 24 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 0.97 HN 1.01 KP 0.98 ! LA 1.01 MK 1.00 NL 1.03 NY 0.99 ! ON 1.02 OV 0.99 PT 1.01 SC 0.94 ! WZ 0.98 ! ! ! Fit before self-cal, rms=0.095948Jy sigma=1.012074 ! Fit after self-cal, rms=0.082524Jy sigma=0.972691 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! Estimated beam: bmin=0.7429 mas, bmaj=0.9571 mas, bpa=-34.76 degrees ! Estimated noise=0.924139 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 (-30.2, -19). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00194078 Jy ! Component: 100 - total flux cleaned = 0.00212046 Jy ! Component: 150 - total flux cleaned = 0.00180516 Jy ! Component: 200 - total flux cleaned = 0.00180437 Jy ! Total flux subtracted in 200 components = 0.00180437 Jy ! Clean residual min=-0.005169 max=0.004798 Jy/beam ! Clean residual mean=-0.000003 rms=0.001125 Jy/beam ! Combined flux in latest and established models = 1.1644 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 73 components and 1.16441 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081774Jy sigma=0.961704 ! Fit after self-cal, rms=0.081751Jy sigma=0.960643 ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 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=0.081751Jy sigma=0.960643 ! Fit after self-cal, rms=0.076429Jy sigma=0.883897 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! Estimated beam: bmin=0.7412 mas, bmaj=0.9607 mas, bpa=-34.98 degrees ! Estimated noise=0.925224 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00116963 Jy ! Component: 100 - total flux cleaned = 0.000389924 Jy ! Component: 150 - total flux cleaned = -0.000269334 Jy ! Component: 200 - total flux cleaned = -0.000520806 Jy ! Total flux subtracted in 200 components = -0.000520806 Jy ! Clean residual min=-0.003822 max=0.003719 Jy/beam ! Clean residual mean=-0.000008 rms=0.000844 Jy/beam ! Combined flux in latest and established models = 1.16388 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 87 components and 1.16388 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.076092Jy sigma=0.878882 ! Fit after self-cal, rms=0.076029Jy sigma=0.878132 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 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 = 2.74181e-05 Jy ! Component: 100 - total flux cleaned = -0.000304659 Jy ! Component: 150 - total flux cleaned = -0.000304989 Jy ! Component: 200 - total flux cleaned = -0.000376017 Jy ! Total flux subtracted in 200 components = -0.000376017 Jy ! Clean residual min=-0.003811 max=0.003696 Jy/beam ! Clean residual mean=-0.000008 rms=0.000836 Jy/beam ! Combined flux in latest and established models = 1.16351 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 92 components and 1.16351 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.075852Jy sigma=0.875607 ! Fit after self-cal, rms=0.075811Jy sigma=0.875144 ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 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=0.075811Jy sigma=0.875144 ! Fit after self-cal, rms=0.074839Jy sigma=0.855544 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! Estimated beam: bmin=0.7404 mas, bmaj=0.9616 mas, bpa=-34.98 degrees ! Estimated noise=0.925876 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000627163 Jy ! Component: 100 - total flux cleaned = -7.22947e-05 Jy ! Component: 150 - total flux cleaned = -0.000455425 Jy ! Component: 200 - total flux cleaned = -0.000808477 Jy ! Total flux subtracted in 200 components = -0.000808477 Jy ! Clean residual min=-0.003470 max=0.003415 Jy/beam ! Clean residual mean=-0.000005 rms=0.000770 Jy/beam ! Combined flux in latest and established models = 1.1627 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 99 components and 1.1627 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.074651Jy sigma=0.852618 ! Fit after self-cal, rms=0.074621Jy sigma=0.852236 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 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 = -3.85232e-05 Jy ! Component: 100 - total flux cleaned = -0.000316327 Jy ! Component: 150 - total flux cleaned = -0.00044368 Jy ! Component: 200 - total flux cleaned = -0.000441441 Jy ! Total flux subtracted in 200 components = -0.000441441 Jy ! Clean residual min=-0.003436 max=0.003324 Jy/beam ! Clean residual mean=-0.000005 rms=0.000764 Jy/beam ! Combined flux in latest and established models = 1.16226 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 100 components and 1.16226 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.074510Jy sigma=0.850530 ! Fit after self-cal, rms=0.074487Jy sigma=0.850268 ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 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=0.074487Jy sigma=0.850268 ! Fit after self-cal, rms=0.074555Jy sigma=0.849950 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! Estimated beam: bmin=2.4 mas, bmaj=2.504 mas, bpa=29.96 degrees ! Estimated noise=1.37425 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000153343 Jy ! Component: 100 - total flux cleaned = -0.000497593 Jy ! Component: 150 - total flux cleaned = -0.000700464 Jy ! Component: 200 - total flux cleaned = -0.000806623 Jy ! Total flux subtracted in 200 components = -0.000806623 Jy ! Clean residual min=-0.004501 max=0.004036 Jy/beam ! Clean residual mean=-0.000014 rms=0.001090 Jy/beam ! Combined flux in latest and established models = 1.16145 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 113 components and 1.16145 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.074519Jy sigma=0.849303 ! Fit after self-cal, rms=0.074507Jy sigma=0.849159 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 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 = 1.60976e-05 Jy ! Component: 100 - total flux cleaned = -0.000172487 Jy ! Component: 150 - total flux cleaned = -0.000238483 Jy ! Component: 200 - total flux cleaned = -0.000327783 Jy ! Total flux subtracted in 200 components = -0.000327783 Jy ! Clean residual min=-0.004503 max=0.004022 Jy/beam ! Clean residual mean=-0.000013 rms=0.001084 Jy/beam ! Combined flux in latest and established models = 1.16112 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 115 components and 1.16112 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.074516Jy sigma=0.849096 ! Fit after self-cal, rms=0.074504Jy sigma=0.848989 ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 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 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! Estimated beam: bmin=0.7399 mas, bmaj=0.9619 mas, bpa=-34.96 degrees ! Estimated noise=0.926152 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7399 x 0.9619 at -34.96 degrees (North through East) ! Clean map min=-0.0046988 max=0.82187 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=0.074504Jy sigma=0.848989 ! Fit after self-cal, rms=0.069000Jy sigma=0.772614 ! Inverting map and beam ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! Estimated beam: bmin=0.7401 mas, bmaj=0.9616 mas, bpa=-34.87 degrees ! Estimated noise=0.926467 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00053066 Jy ! Component: 100 - total flux cleaned = 0.000332595 Jy ! Component: 150 - total flux cleaned = 0.000214786 Jy ! Component: 200 - total flux cleaned = 0.000215886 Jy ! Total flux subtracted in 200 components = 0.000215886 Jy ! Clean residual min=-0.003440 max=0.003300 Jy/beam ! Clean residual mean=-0.000005 rms=0.000753 Jy/beam ! Combined flux in latest and established models = 1.16134 Jy ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 122 components and 1.16134 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.068892Jy sigma=0.770986 ! Fit after self-cal, rms=0.068881Jy sigma=0.770848 ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -4.88223e-05 Jy ! Component: 100 - total flux cleaned = -4.85088e-05 Jy ! Component: 150 - total flux cleaned = -4.90269e-05 Jy ! Component: 200 - total flux cleaned = -5.07483e-05 Jy ! Total flux subtracted in 200 components = -5.07483e-05 Jy ! Clean residual min=-0.003399 max=0.003251 Jy/beam ! Clean residual mean=-0.000005 rms=0.000750 Jy/beam ! Combined flux in latest and established models = 1.16129 Jy ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 125 components and 1.16129 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.068799Jy sigma=0.769802 ! Fit after self-cal, rms=0.068792Jy sigma=0.769709 ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.068792Jy sigma=0.769709 ! Fit after self-cal, rms=0.068819Jy sigma=0.769590 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 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! Estimated beam: bmin=0.6644 mas, bmaj=0.8363 mas, bpa=-33.1 degrees ! Estimated noise=1.11627 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.630346 Jy ! Component: 100 - total flux cleaned = 0.845554 Jy ! Component: 150 - total flux cleaned = 0.954083 Jy ! Component: 200 - total flux cleaned = 1.01852 Jy ! Total flux subtracted in 200 components = 1.01852 Jy ! Clean residual min=-0.008508 max=0.033689 Jy/beam ! Clean residual mean=-0.000024 rms=0.002072 Jy/beam ! Combined flux in latest and established models = 1.01852 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 22 model components to the UV plane model. ! The established model now contains 22 components and 1.01852 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! Estimated beam: bmin=0.7398 mas, bmaj=0.9619 mas, bpa=-34.88 degrees ! Estimated noise=0.926649 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 = 0.0564782 Jy ! Component: 100 - total flux cleaned = 0.0888714 Jy ! Component: 150 - total flux cleaned = 0.108154 Jy ! Component: 200 - total flux cleaned = 0.119927 Jy ! Total flux subtracted in 200 components = 0.119927 Jy ! Clean residual min=-0.003710 max=0.006074 Jy/beam ! Clean residual mean=-0.000015 rms=0.000918 Jy/beam ! Combined flux in latest and established models = 1.13845 Jy ! Adding 25 model components to the UV plane model. ! The established model now contains 39 components and 1.13845 Jy ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00734702 Jy ! Component: 100 - total flux cleaned = 0.0124702 Jy ! Component: 150 - total flux cleaned = 0.0148153 Jy ! Component: 200 - total flux cleaned = 0.016299 Jy ! Total flux subtracted in 200 components = 0.016299 Jy ! Clean residual min=-0.003336 max=0.003665 Jy/beam ! Clean residual mean=-0.000008 rms=0.000811 Jy/beam ! Combined flux in latest and established models = 1.15474 Jy ! Adding 28 model components to the UV plane model. ! The established model now contains 57 components and 1.15474 Jy ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! Added new window around map position (-1.2, 0.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00196807 Jy ! Component: 100 - total flux cleaned = 0.00310106 Jy ! Component: 150 - total flux cleaned = 0.00368436 Jy ! Component: 200 - total flux cleaned = 0.00412554 Jy ! Total flux subtracted in 200 components = 0.00412554 Jy ! Clean residual min=-0.003300 max=0.003382 Jy/beam ! Clean residual mean=-0.000006 rms=0.000785 Jy/beam ! Combined flux in latest and established models = 1.15887 Jy ! Adding 29 model components to the UV plane model. ! The established model now contains 71 components and 1.15887 Jy ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! Added new window around map position (28.4, 17.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00178001 Jy ! Component: 100 - total flux cleaned = 0.00208682 Jy ! Component: 150 - total flux cleaned = 0.00228384 Jy ! Component: 200 - total flux cleaned = 0.0026659 Jy ! Total flux subtracted in 200 components = 0.0026659 Jy ! Clean residual min=-0.003407 max=0.003250 Jy/beam ! Clean residual mean=-0.000006 rms=0.000770 Jy/beam ! Combined flux in latest and established models = 1.16154 Jy ! Adding 30 model components to the UV plane model. ! The established model now contains 76 components and 1.16154 Jy ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 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 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! Estimated beam: bmin=2.4 mas, bmaj=2.503 mas, bpa=29.81 degrees ! Estimated noise=1.37502 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00244013 Jy ! Component: 100 - total flux cleaned = 0.00319642 Jy ! Component: 150 - total flux cleaned = 0.00333778 Jy ! Component: 200 - total flux cleaned = 0.00342153 Jy ! Total flux subtracted in 200 components = 0.00342153 Jy ! Clean residual min=-0.004710 max=0.003739 Jy/beam ! Clean residual mean=-0.000016 rms=0.001043 Jy/beam ! Combined flux in latest and established models = 1.16496 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 = 0.000149953 Jy ! Component: 100 - total flux cleaned = 0.000253001 Jy ! Component: 150 - total flux cleaned = 0.000283989 Jy ! Component: 200 - total flux cleaned = 0.000284388 Jy ! Total flux subtracted in 200 components = 0.000284388 Jy ! Clean residual min=-0.004668 max=0.003695 Jy/beam ! Clean residual mean=-0.000016 rms=0.001035 Jy/beam ! Combined flux in latest and established models = 1.16524 Jy ! Adding 20 model components to the UV plane model. ! The established model now contains 94 components and 1.16524 Jy ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! Estimated beam: bmin=0.7398 mas, bmaj=0.9619 mas, bpa=-34.88 degrees ! Estimated noise=0.926649 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00177275 Jy ! Component: 100 - total flux cleaned = -0.00186548 Jy ! Component: 150 - total flux cleaned = -0.00186746 Jy ! Component: 200 - total flux cleaned = -0.00178465 Jy ! Total flux subtracted in 200 components = -0.00178465 Jy ! Clean residual min=-0.003470 max=0.003285 Jy/beam ! Clean residual mean=-0.000006 rms=0.000758 Jy/beam ! Combined flux in latest and established models = 1.16346 Jy selfcal ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 99 components and 1.16346 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.070143Jy sigma=0.772417 ! Fit after self-cal, rms=0.069278Jy sigma=0.768293 wmodel J1130+3815_X_map.mod ! Writing 99 model components to file: J1130+3815_X_map.mod wobs J1130+3815_X_uvs.fits ! Writing UV FITS file: J1130+3815_X_uvs.fits wwins J1130+3815_X_map.win ! wwins: Wrote 7 windows to J1130+3815_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 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000378026 Jy ! Component: 100 - total flux cleaned = -0.000320088 Jy ! Component: 150 - total flux cleaned = -0.000377846 Jy ! Component: 200 - total flux cleaned = -0.000268171 Jy ! Component: 250 - total flux cleaned = -0.000214499 Jy ! Component: 300 - total flux cleaned = -0.000161382 Jy ! Component: 350 - total flux cleaned = -0.000161004 Jy ! Component: 400 - total flux cleaned = -0.00016086 Jy ! Component: 450 - total flux cleaned = -0.000160512 Jy ! Component: 500 - total flux cleaned = -9.53228e-06 Jy ! Component: 550 - total flux cleaned = 8.93164e-05 Jy ! Component: 600 - total flux cleaned = 0.000137986 Jy ! Component: 650 - total flux cleaned = 8.94273e-05 Jy ! Component: 700 - total flux cleaned = 0.000233034 Jy ! Component: 750 - total flux cleaned = 0.000280397 Jy ! Component: 800 - total flux cleaned = 0.000467187 Jy ! Component: 850 - total flux cleaned = 0.000421127 Jy ! Component: 900 - total flux cleaned = 0.000558938 Jy ! Component: 950 - total flux cleaned = 0.000559159 Jy ! Component: 1000 - total flux cleaned = 0.000741232 Jy ! Component: 1050 - total flux cleaned = 0.000696263 Jy ! Component: 1100 - total flux cleaned = 0.000830353 Jy ! Component: 1150 - total flux cleaned = 0.000830399 Jy ! Component: 1200 - total flux cleaned = 0.000918569 Jy ! Component: 1250 - total flux cleaned = 0.000874435 Jy ! Component: 1300 - total flux cleaned = 0.000961986 Jy ! Component: 1350 - total flux cleaned = 0.000918501 Jy ! Component: 1400 - total flux cleaned = 0.000961747 Jy ! Component: 1450 - total flux cleaned = 0.000962109 Jy ! Component: 1500 - total flux cleaned = 0.000961906 Jy ! Component: 1550 - total flux cleaned = 0.00113124 Jy ! Component: 1600 - total flux cleaned = 0.00104674 Jy ! Component: 1650 - total flux cleaned = 0.000963189 Jy ! Component: 1700 - total flux cleaned = 0.00100491 Jy ! Component: 1750 - total flux cleaned = 0.000922235 Jy ! Component: 1800 - total flux cleaned = 0.000881268 Jy ! Component: 1850 - total flux cleaned = 0.000881236 Jy ! Component: 1900 - total flux cleaned = 0.000881496 Jy ! Component: 1950 - total flux cleaned = 0.000638031 Jy ! Component: 2000 - total flux cleaned = 0.000718644 Jy ! Component: 2050 - total flux cleaned = 0.000718947 Jy ! Component: 2100 - total flux cleaned = 0.000799206 Jy ! Component: 2150 - total flux cleaned = 0.000759317 Jy ! Component: 2200 - total flux cleaned = 0.000680341 Jy ! Component: 2250 - total flux cleaned = 0.000641033 Jy ! Component: 2300 - total flux cleaned = 0.000758511 Jy ! Component: 2350 - total flux cleaned = 0.000797281 Jy ! Component: 2400 - total flux cleaned = 0.000603562 Jy ! Component: 2450 - total flux cleaned = 0.000603445 Jy ! Component: 2500 - total flux cleaned = 0.000680528 Jy ! Component: 2550 - total flux cleaned = 0.000603778 Jy ! Component: 2600 - total flux cleaned = 0.000755882 Jy ! Component: 2650 - total flux cleaned = 0.000603939 Jy ! Component: 2700 - total flux cleaned = 0.000414829 Jy ! Component: 2750 - total flux cleaned = 0.000527904 Jy ! Component: 2800 - total flux cleaned = 0.000490707 Jy ! Component: 2850 - total flux cleaned = 0.000565437 Jy ! Component: 2900 - total flux cleaned = 0.000379655 Jy ! Component: 2950 - total flux cleaned = 0.000453355 Jy ! Component: 3000 - total flux cleaned = 0.00030547 Jy ! Component: 3050 - total flux cleaned = 0.000195063 Jy ! Component: 3100 - total flux cleaned = 0.000268317 Jy ! Component: 3150 - total flux cleaned = 0.000268401 Jy ! Component: 3200 - total flux cleaned = 8.68558e-05 Jy ! Component: 3250 - total flux cleaned = 8.6964e-05 Jy ! Component: 3300 - total flux cleaned = -2.11963e-05 Jy ! Component: 3350 - total flux cleaned = -0.00016466 Jy ! Component: 3400 - total flux cleaned = -0.00016455 Jy ! Component: 3450 - total flux cleaned = -0.000129171 Jy ! Component: 3500 - total flux cleaned = -0.00012928 Jy ! Component: 3550 - total flux cleaned = -0.000235408 Jy ! Component: 3600 - total flux cleaned = -0.000200009 Jy ! Component: 3650 - total flux cleaned = -0.000235153 Jy ! Component: 3700 - total flux cleaned = -0.000409961 Jy ! Component: 3750 - total flux cleaned = -0.000444825 Jy ! Component: 3800 - total flux cleaned = -0.000410179 Jy ! Component: 3850 - total flux cleaned = -0.000514159 Jy ! Component: 3900 - total flux cleaned = -0.000548432 Jy ! Component: 3950 - total flux cleaned = -0.0005142 Jy ! Component: 4000 - total flux cleaned = -0.000719612 Jy ! Component: 4050 - total flux cleaned = -0.000685574 Jy ! Total flux subtracted in 4096 components = -0.000583549 Jy ! Clean residual min=-0.001875 max=0.002072 Jy/beam ! Clean residual mean=-0.000001 rms=0.000562 Jy/beam ! Combined flux in latest and established models = 1.16287 Jy keep ! Adding 352 model components to the UV plane model. ! The established model now contains 451 components and 1.16287 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv119_uvs/J1130+3815_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7398 x 0.9619 at -34.88 degrees (North through East) ! Clean map min=-0.0040037 max=0.82332 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv119_uvs/J1130+3815_X_map.fits wmodel /scr/pima/rv119_uvs/J1130+3815_X_map.mod ! Writing 451 model components to file: /scr/pima/rv119_uvs/J1130+3815_X_map.mod wobs /scr/pima/rv119_uvs/J1130+3815_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv119_uvs/J1130+3815_X_uvs.fits wwins /scr/pima/rv119_uvs/J1130+3815_X_map.win ! wwins: Wrote 8 windows to /scr/pima/rv119_uvs/J1130+3815_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.823317 invert ! Inverting map ! Your choice of large map pixels excluded 2.88% of the data. ! The x-axis pixel size should ideally be below 0.1824 milli-arcsec ! The y-axis pixel size should ideally be below 0.1698 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000561566 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.204623 0.204623 0.409246 0.818493 1.63699 3.27397 6.54794 13.0959 26.1918 52.3835 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0016 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.823 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 1466.11 quit ! Quitting program ! Log file /scr/pima/rv119_uvs/J1130+3815_X_dfm.log closed on Sun Dec 17 11:35:45 2017