! Started logfile: /scr/pima/rv119_uvs/J1043+2408_X_dfm.log on Sun Dec 17 11:35:14 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/J1043+2408_X_uva.fits ! Reading UV FITS file: /scr/pima/rv119_uvs/J1043+2408_X_uva.fits ! AN table 1: 2 integrations on 45 of 45 possible baselines. ! AN table 2: 16 integrations on 36 of 36 possible baselines. ! AN table 3: 82 integrations on 78 of 78 possible baselines. ! Apparent sampling: 0.127867 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1043+2408 ! ! 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 3612 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 J1043+2408_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 86 telescope corrections were flagged in sub-array 2. ! A total of 830 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 86 telescope corrections were flagged in sub-array 2. ! A total of 830 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 86 telescope corrections were flagged in sub-array 2. ! A total of 830 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 86 telescope corrections were flagged in sub-array 2. ! A total of 830 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=1.176194Jy sigma=16.297995 ! Fit after self-cal, rms=0.468287Jy sigma=6.926518 ! 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 9.78% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec ! Estimated beam: bmin=0.6875 mas, bmaj=0.9933 mas, bpa=-6.04 degrees ! Estimated noise=1.15269 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 = 0.403493 Jy ! Component: 100 - total flux cleaned = 0.502073 Jy ! Total flux subtracted in 100 components = 0.502073 Jy ! Clean residual min=-0.009836 max=0.037804 Jy/beam ! Clean residual mean=0.000011 rms=0.002190 Jy/beam ! Combined flux in latest and established models = 0.502073 Jy ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 4 components and 0.502073 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.158171Jy sigma=1.408584 ! Fit after self-cal, rms=0.157755Jy sigma=1.404345 ! Inverting map ! Your choice of large map pixels excluded 9.78% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0375768 Jy ! Component: 100 - total flux cleaned = 0.0546911 Jy ! Total flux subtracted in 100 components = 0.0546911 Jy ! Clean residual min=-0.008646 max=0.008474 Jy/beam ! Clean residual mean=0.000005 rms=0.001578 Jy/beam ! Combined flux in latest and established models = 0.556764 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 10 components and 0.556764 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.140206Jy sigma=1.165609 ! Fit after self-cal, rms=0.139968Jy sigma=1.162078 ! Inverting map ! Your choice of large map pixels excluded 9.78% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00859761 Jy ! Component: 100 - total flux cleaned = 0.00927858 Jy ! Total flux subtracted in 100 components = 0.00927858 Jy ! Clean residual min=-0.008105 max=0.007466 Jy/beam ! Clean residual mean=0.000004 rms=0.001522 Jy/beam ! Combined flux in latest and established models = 0.566042 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 12 components and 0.566042 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.135393Jy sigma=1.135913 ! Fit after self-cal, rms=0.135351Jy sigma=1.135003 ! Inverting map ! Your choice of large map pixels excluded 9.78% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 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 9.78% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec ! Estimated beam: bmin=0.7698 mas, bmaj=1.051 mas, bpa=-6.353 degrees ! Estimated noise=0.971621 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 = 0.00122901 Jy ! Component: 100 - total flux cleaned = 0.00123109 Jy ! Component: 150 - total flux cleaned = 0.00124541 Jy ! Component: 200 - total flux cleaned = 0.00165632 Jy ! Total flux subtracted in 200 components = 0.00165632 Jy ! Clean residual min=-0.006991 max=0.008084 Jy/beam ! Clean residual mean=0.000008 rms=0.001519 Jy/beam ! Combined flux in latest and established models = 0.567699 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 14 components and 0.567699 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.124804Jy sigma=1.087554 ! Fit after self-cal, rms=0.124731Jy sigma=1.087011 ! Inverting map ! Your choice of large map pixels excluded 9.78% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7698 x 1.051 at -6.353 degrees (North through East) ! Clean map min=-0.0054657 max=0.51302 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 FD 0.94 HN 1.02 KP 0.99 ! LA 0.99 MK 1.00 NL 1.01 OV 0.98 ! PT 1.00 SC 0.96 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 FD 1.00 KP 0.99 LA 1.01 ! MK 1.02 NL 1.05 NY 1.06 OV 1.01 ! PT 1.01 ! ! A total of 138 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 0.94 HH 0.74 HN 1.02 ! KP 1.01 LA 1.01 NL 1.02 NY 1.02 ! ON 1.00 OV 1.02 PT 1.02 SC 0.96 ! WZ 1.00 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 0.96 HN 0.99 KP 0.98 ! LA 0.97 MK 1.01 NL 1.02 OV 0.99 ! PT 0.99 SC 0.98 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 0.99 KP 1.00 LA 1.02 ! MK 0.99 NL 1.07 NY 1.06 OV 1.01 ! PT 1.00 ! ! A total of 138 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 FD 0.94 HH 0.73 HN 1.04 ! KP 1.02 LA 1.01 NL 1.00 NY 0.99 ! ON 0.96 OV 1.02 PT 1.01 SC 0.97 ! WZ 0.99 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 0.90 HN 0.98 KP 0.99 ! LA 0.99 MK 1.03 NL 1.02 OV 0.96 ! PT 1.01 SC 1.00 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 0.97 KP 0.98 LA 1.01 ! MK 1.03 NL 1.10 NY 1.10 OV 1.02 ! PT 0.99 ! ! A total of 138 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 0.93 HH 0.82 HN 1.01 ! KP 1.00 LA 1.01 NL 1.02 NY 1.03 ! ON 1.02 OV 0.98 PT 1.01 SC 0.97 ! WZ 0.95 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.95 HN 0.99 KP 0.95 ! LA 0.95 MK 1.00 NL 1.04 OV 0.95 ! PT 0.99 SC 0.91 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 0.95 KP 0.97 LA 1.03 ! MK 1.02 NL 1.08 NY 1.09 OV 1.01 ! PT 1.00 ! ! A total of 138 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.04 FD 0.95 HH 0.93 HN 1.02 ! KP 1.01 LA 1.00 NL 1.00 NY 0.99 ! ON 0.99 OV 0.98 PT 1.00 SC 0.92 ! WZ 0.97 ! ! ! Fit before self-cal, rms=0.124731Jy sigma=1.087011 ! Fit after self-cal, rms=0.080191Jy sigma=0.949020 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec ! Estimated beam: bmin=0.7384 mas, bmaj=1.212 mas, bpa=-3.947 degrees ! Estimated noise=0.977038 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 (1.4, 1.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00408729 Jy ! Component: 100 - total flux cleaned = 0.00386834 Jy ! Component: 150 - total flux cleaned = 0.00359898 Jy ! Component: 200 - total flux cleaned = 0.00337779 Jy ! Total flux subtracted in 200 components = 0.00337779 Jy ! Clean residual min=-0.005084 max=0.004262 Jy/beam ! Clean residual mean=0.000013 rms=0.001040 Jy/beam ! Combined flux in latest and established models = 0.571077 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 25 components and 0.571076 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.079803Jy sigma=0.942442 ! Fit after self-cal, rms=0.079714Jy sigma=0.941571 ! Inverting map ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 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=0.079714Jy sigma=0.941571 ! Fit after self-cal, rms=0.078486Jy sigma=0.905312 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec ! Estimated beam: bmin=0.7381 mas, bmaj=1.212 mas, bpa=-4.02 degrees ! Estimated noise=0.977943 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00195077 Jy ! Component: 100 - total flux cleaned = 0.00220479 Jy ! Component: 150 - total flux cleaned = 0.00206263 Jy ! Component: 200 - total flux cleaned = 0.00206252 Jy ! Total flux subtracted in 200 components = 0.00206252 Jy ! Clean residual min=-0.004138 max=0.004036 Jy/beam ! Clean residual mean=0.000005 rms=0.000902 Jy/beam ! Combined flux in latest and established models = 0.573139 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 35 components and 0.573139 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.078299Jy sigma=0.902773 ! Fit after self-cal, rms=0.078307Jy sigma=0.902378 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000304613 Jy ! Component: 100 - total flux cleaned = 0.000246142 Jy ! Component: 150 - total flux cleaned = 0.000248791 Jy ! Component: 200 - total flux cleaned = 0.000251257 Jy ! Total flux subtracted in 200 components = 0.000251257 Jy ! Clean residual min=-0.004057 max=0.003972 Jy/beam ! Clean residual mean=0.000005 rms=0.000896 Jy/beam ! Combined flux in latest and established models = 0.57339 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 39 components and 0.57339 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.078203Jy sigma=0.901203 ! Fit after self-cal, rms=0.078188Jy sigma=0.901081 ! Inverting map ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 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=0.078188Jy sigma=0.901081 ! Fit after self-cal, rms=0.077637Jy sigma=0.890296 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec ! Estimated beam: bmin=0.7376 mas, bmaj=1.213 mas, bpa=-4.06 degrees ! Estimated noise=0.97788 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00128977 Jy ! Component: 100 - total flux cleaned = 0.00159128 Jy ! Component: 150 - total flux cleaned = 0.00180677 Jy ! Component: 200 - total flux cleaned = 0.00200049 Jy ! Total flux subtracted in 200 components = 0.00200049 Jy ! Clean residual min=-0.003712 max=0.003851 Jy/beam ! Clean residual mean=-0.000001 rms=0.000857 Jy/beam ! Combined flux in latest and established models = 0.575391 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 46 components and 0.575391 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.077546Jy sigma=0.889362 ! Fit after self-cal, rms=0.077536Jy sigma=0.889190 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 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 (13.8, -25.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00344243 Jy ! Component: 100 - total flux cleaned = 0.00445295 Jy ! Component: 150 - total flux cleaned = 0.00451642 Jy ! Component: 200 - total flux cleaned = 0.00457198 Jy ! Total flux subtracted in 200 components = 0.00457198 Jy ! Clean residual min=-0.003657 max=0.003684 Jy/beam ! Clean residual mean=0.000000 rms=0.000831 Jy/beam ! Combined flux in latest and established models = 0.579963 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 63 components and 0.579963 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.077357Jy sigma=0.886378 ! Fit after self-cal, rms=0.077332Jy sigma=0.886150 ! Inverting map ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec ! Added new window around map position (-11.2, -42.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00332152 Jy ! Component: 100 - total flux cleaned = 0.00396745 Jy ! Component: 150 - total flux cleaned = 0.00415026 Jy ! Component: 200 - total flux cleaned = 0.00415042 Jy ! Total flux subtracted in 200 components = 0.00415042 Jy ! Clean residual min=-0.003558 max=0.003572 Jy/beam ! Clean residual mean=0.000001 rms=0.000816 Jy/beam ! Combined flux in latest and established models = 0.584113 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 77 components and 0.584113 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.077108Jy sigma=0.883329 ! Fit after self-cal, rms=0.077107Jy sigma=0.883156 ! Inverting map ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec ! Added new window around map position (37.4, -22.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00282151 Jy ! Component: 100 - total flux cleaned = 0.00331361 Jy ! Component: 150 - total flux cleaned = 0.00393521 Jy ! Component: 200 - total flux cleaned = 0.00429518 Jy ! Total flux subtracted in 200 components = 0.00429518 Jy ! Clean residual min=-0.003422 max=0.003252 Jy/beam ! Clean residual mean=0.000001 rms=0.000792 Jy/beam ! Combined flux in latest and established models = 0.588408 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 87 components and 0.588408 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.076888Jy sigma=0.879930 ! Fit after self-cal, rms=0.076884Jy sigma=0.879756 ! Inverting map ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 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=0.076884Jy sigma=0.879756 ! Fit after self-cal, rms=0.076875Jy sigma=0.878787 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec ! Estimated beam: bmin=2.751 mas, bmaj=2.78 mas, bpa=9.724 degrees ! Estimated noise=1.2422 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00201492 Jy ! Component: 100 - total flux cleaned = 0.00273397 Jy ! Component: 150 - total flux cleaned = 0.00324389 Jy ! Component: 200 - total flux cleaned = 0.00371566 Jy ! Total flux subtracted in 200 components = 0.00371566 Jy ! Clean residual min=-0.003367 max=0.003860 Jy/beam ! Clean residual mean=0.000001 rms=0.000948 Jy/beam ! Combined flux in latest and established models = 0.592124 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 101 components and 0.592124 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.076835Jy sigma=0.878147 ! Fit after self-cal, rms=0.076830Jy sigma=0.878061 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000542235 Jy ! Component: 100 - total flux cleaned = 0.000725492 Jy ! Component: 150 - total flux cleaned = 0.000887924 Jy ! Component: 200 - total flux cleaned = 0.00095187 Jy ! Total flux subtracted in 200 components = 0.00095187 Jy ! Clean residual min=-0.003352 max=0.003776 Jy/beam ! Clean residual mean=0.000001 rms=0.000940 Jy/beam ! Combined flux in latest and established models = 0.593075 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 110 components and 0.593075 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.076826Jy sigma=0.877994 ! Fit after self-cal, rms=0.076825Jy sigma=0.877982 ! Inverting map ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 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 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec ! Estimated beam: bmin=0.7374 mas, bmaj=1.213 mas, bpa=-4.061 degrees ! Estimated noise=0.977599 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7374 x 1.213 at -4.061 degrees (North through East) ! Clean map min=-0.0028395 max=0.50503 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=0.076825Jy sigma=0.877982 ! Fit after self-cal, rms=0.072988Jy sigma=0.817976 ! Inverting map and beam ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec ! Estimated beam: bmin=0.737 mas, bmaj=1.213 mas, bpa=-4.086 degrees ! Estimated noise=0.977964 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000982788 Jy ! Component: 100 - total flux cleaned = 0.00159246 Jy ! Component: 150 - total flux cleaned = 0.00170534 Jy ! Component: 200 - total flux cleaned = 0.00176051 Jy ! Total flux subtracted in 200 components = 0.00176051 Jy ! Clean residual min=-0.003340 max=0.003319 Jy/beam ! Clean residual mean=-0.000000 rms=0.000774 Jy/beam ! Combined flux in latest and established models = 0.594836 Jy ! Performing phase self-cal ! Adding 35 model components to the UV plane model. ! The established model now contains 116 components and 0.594836 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.072854Jy sigma=0.816758 ! Fit after self-cal, rms=0.072850Jy sigma=0.816728 ! Inverting map ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000272848 Jy ! Component: 100 - total flux cleaned = 0.000324709 Jy ! Component: 150 - total flux cleaned = 0.000326031 Jy ! Component: 200 - total flux cleaned = 0.000375355 Jy ! Total flux subtracted in 200 components = 0.000375355 Jy ! Clean residual min=-0.003294 max=0.003299 Jy/beam ! Clean residual mean=-0.000000 rms=0.000771 Jy/beam ! Combined flux in latest and established models = 0.595211 Jy ! Performing phase self-cal ! Adding 44 model components to the UV plane model. ! The established model now contains 124 components and 0.595211 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.072752Jy sigma=0.815902 ! Fit after self-cal, rms=0.072749Jy sigma=0.815892 ! Inverting map ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec ! Added new window around map position (30, 16). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00220673 Jy ! Component: 100 - total flux cleaned = 0.0024319 Jy ! Component: 150 - total flux cleaned = 0.00264102 Jy ! Component: 200 - total flux cleaned = 0.00264196 Jy ! Total flux subtracted in 200 components = 0.00264196 Jy ! Clean residual min=-0.003261 max=0.003178 Jy/beam ! Clean residual mean=0.000001 rms=0.000758 Jy/beam ! Combined flux in latest and established models = 0.597853 Jy ! Performing phase self-cal ! Adding 37 model components to the UV plane model. ! The established model now contains 139 components and 0.597853 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.072610Jy sigma=0.814018 ! Fit after self-cal, rms=0.072598Jy sigma=0.813898 ! Inverting map ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.072598Jy sigma=0.813898 ! Fit after self-cal, rms=0.072611Jy sigma=0.813687 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 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec ! Estimated beam: bmin=0.6682 mas, bmaj=1.042 mas, bpa=-4.696 degrees ! Estimated noise=1.17968 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.39727 Jy ! Component: 100 - total flux cleaned = 0.497792 Jy ! Component: 150 - total flux cleaned = 0.537036 Jy ! Component: 200 - total flux cleaned = 0.553557 Jy ! Total flux subtracted in 200 components = 0.553557 Jy ! Clean residual min=-0.004951 max=0.007394 Jy/beam ! Clean residual mean=0.000000 rms=0.001141 Jy/beam ! Combined flux in latest and established models = 0.553557 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 10 model components to the UV plane model. ! The established model now contains 10 components and 0.553557 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec ! Estimated beam: bmin=0.7369 mas, bmaj=1.213 mas, bpa=-4.091 degrees ! Estimated noise=0.978108 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 = 0.0114852 Jy ! Component: 100 - total flux cleaned = 0.0183131 Jy ! Component: 150 - total flux cleaned = 0.0237191 Jy ! Component: 200 - total flux cleaned = 0.028232 Jy ! Total flux subtracted in 200 components = 0.028232 Jy ! Clean residual min=-0.003672 max=0.003842 Jy/beam ! Clean residual mean=-0.000001 rms=0.000884 Jy/beam ! Combined flux in latest and established models = 0.581789 Jy ! Adding 29 model components to the UV plane model. ! The established model now contains 32 components and 0.581789 Jy ! Inverting map ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec ! Added new window around map position (-30.6, -20.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00413069 Jy ! Component: 100 - total flux cleaned = 0.00758793 Jy ! Component: 150 - total flux cleaned = 0.0102846 Jy ! Component: 200 - total flux cleaned = 0.0116285 Jy ! Total flux subtracted in 200 components = 0.0116285 Jy ! Clean residual min=-0.003509 max=0.003361 Jy/beam ! Clean residual mean=0.000001 rms=0.000826 Jy/beam ! Combined flux in latest and established models = 0.593417 Jy ! Adding 36 model components to the UV plane model. ! The established model now contains 48 components and 0.593417 Jy ! Inverting map ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 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 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec ! Estimated beam: bmin=2.75 mas, bmaj=2.779 mas, bpa=8.556 degrees ! Estimated noise=1.24395 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0029577 Jy ! Component: 100 - total flux cleaned = 0.00384786 Jy ! Component: 150 - total flux cleaned = 0.00457988 Jy ! Component: 200 - total flux cleaned = 0.00526444 Jy ! Total flux subtracted in 200 components = 0.00526444 Jy ! Clean residual min=-0.003523 max=0.003596 Jy/beam ! Clean residual mean=0.000005 rms=0.000902 Jy/beam ! Combined flux in latest and established models = 0.598682 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 = 0.000656253 Jy ! Component: 100 - total flux cleaned = 0.00123414 Jy ! Component: 150 - total flux cleaned = 0.00157715 Jy ! Component: 200 - total flux cleaned = 0.00181241 Jy ! Total flux subtracted in 200 components = 0.00181241 Jy ! Clean residual min=-0.003320 max=0.003522 Jy/beam ! Clean residual mean=0.000006 rms=0.000878 Jy/beam ! Combined flux in latest and established models = 0.600494 Jy ! Adding 34 model components to the UV plane model. ! The established model now contains 82 components and 0.600494 Jy ! Inverting map ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec ! Estimated beam: bmin=0.7369 mas, bmaj=1.213 mas, bpa=-4.091 degrees ! Estimated noise=0.978108 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000607598 Jy ! Component: 100 - total flux cleaned = -0.000327381 Jy ! Component: 150 - total flux cleaned = -6.13436e-05 Jy ! Component: 200 - total flux cleaned = 0.000107033 Jy ! Total flux subtracted in 200 components = 0.000107033 Jy ! Clean residual min=-0.003391 max=0.003219 Jy/beam ! Clean residual mean=0.000002 rms=0.000788 Jy/beam ! Combined flux in latest and established models = 0.600601 Jy selfcal ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 95 components and 0.600601 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.074092Jy sigma=0.825136 ! Fit after self-cal, rms=0.074026Jy sigma=0.824160 wmodel J1043+2408_X_map.mod ! Writing 95 model components to file: J1043+2408_X_map.mod wobs J1043+2408_X_uvs.fits ! Writing UV FITS file: J1043+2408_X_uvs.fits wwins J1043+2408_X_map.win ! wwins: Wrote 7 windows to J1043+2408_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 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000960208 Jy ! Component: 100 - total flux cleaned = -0.00168027 Jy ! Component: 150 - total flux cleaned = -0.00237517 Jy ! Component: 200 - total flux cleaned = -0.00293907 Jy ! Component: 250 - total flux cleaned = -0.00316067 Jy ! Component: 300 - total flux cleaned = -0.00354229 Jy ! Component: 350 - total flux cleaned = -0.00370275 Jy ! Component: 400 - total flux cleaned = -0.00391405 Jy ! Component: 450 - total flux cleaned = -0.00417437 Jy ! Component: 500 - total flux cleaned = -0.00432872 Jy ! Component: 550 - total flux cleaned = -0.00458381 Jy ! Component: 600 - total flux cleaned = -0.00478505 Jy ! Component: 650 - total flux cleaned = -0.00503508 Jy ! Component: 700 - total flux cleaned = -0.00523267 Jy ! Component: 750 - total flux cleaned = -0.0055759 Jy ! Component: 800 - total flux cleaned = -0.00572187 Jy ! Component: 850 - total flux cleaned = -0.0058667 Jy ! Component: 900 - total flux cleaned = -0.00610536 Jy ! Component: 950 - total flux cleaned = -0.00620032 Jy ! Component: 1000 - total flux cleaned = -0.00662253 Jy ! Component: 1050 - total flux cleaned = -0.00648304 Jy ! Component: 1100 - total flux cleaned = -0.00676039 Jy ! Component: 1150 - total flux cleaned = -0.00671497 Jy ! Component: 1200 - total flux cleaned = -0.00676052 Jy ! Component: 1250 - total flux cleaned = -0.00689603 Jy ! Component: 1300 - total flux cleaned = -0.00689593 Jy ! Component: 1350 - total flux cleaned = -0.00716312 Jy ! Component: 1400 - total flux cleaned = -0.00703096 Jy ! Component: 1450 - total flux cleaned = -0.00725043 Jy ! Component: 1500 - total flux cleaned = -0.00729343 Jy ! Component: 1550 - total flux cleaned = -0.00729346 Jy ! Component: 1600 - total flux cleaned = -0.00725043 Jy ! Component: 1650 - total flux cleaned = -0.00725054 Jy ! Component: 1700 - total flux cleaned = -0.00708035 Jy ! Component: 1750 - total flux cleaned = -0.00720734 Jy ! Component: 1800 - total flux cleaned = -0.00724927 Jy ! Component: 1850 - total flux cleaned = -0.00720739 Jy ! Component: 1900 - total flux cleaned = -0.00708234 Jy ! Component: 1950 - total flux cleaned = -0.00700017 Jy ! Component: 2000 - total flux cleaned = -0.00716484 Jy ! Component: 2050 - total flux cleaned = -0.00696079 Jy ! Component: 2100 - total flux cleaned = -0.00704249 Jy ! Component: 2150 - total flux cleaned = -0.00696142 Jy ! Component: 2200 - total flux cleaned = -0.00712229 Jy ! Component: 2250 - total flux cleaned = -0.00704228 Jy ! Component: 2300 - total flux cleaned = -0.00720166 Jy ! Component: 2350 - total flux cleaned = -0.00735982 Jy ! Component: 2400 - total flux cleaned = -0.00708393 Jy ! Component: 2450 - total flux cleaned = -0.00724081 Jy ! Component: 2500 - total flux cleaned = -0.00727965 Jy ! Component: 2550 - total flux cleaned = -0.00739621 Jy ! Component: 2600 - total flux cleaned = -0.0073959 Jy ! Component: 2650 - total flux cleaned = -0.0075112 Jy ! Component: 2700 - total flux cleaned = -0.00747292 Jy ! Component: 2750 - total flux cleaned = -0.00766312 Jy ! Component: 2800 - total flux cleaned = -0.00762523 Jy ! Component: 2850 - total flux cleaned = -0.00773837 Jy ! Component: 2900 - total flux cleaned = -0.00796384 Jy ! Component: 2950 - total flux cleaned = -0.00811316 Jy ! Component: 3000 - total flux cleaned = -0.00815019 Jy ! Component: 3050 - total flux cleaned = -0.00837203 Jy ! Component: 3100 - total flux cleaned = -0.00829818 Jy ! Component: 3150 - total flux cleaned = -0.00848162 Jy ! Component: 3200 - total flux cleaned = -0.00855465 Jy ! Component: 3250 - total flux cleaned = -0.00855469 Jy ! Component: 3300 - total flux cleaned = -0.0084099 Jy ! Component: 3350 - total flux cleaned = -0.00848203 Jy ! Component: 3400 - total flux cleaned = -0.00869741 Jy ! Component: 3450 - total flux cleaned = -0.00887618 Jy ! Component: 3500 - total flux cleaned = -0.00869834 Jy ! Component: 3550 - total flux cleaned = -0.00873368 Jy ! Component: 3600 - total flux cleaned = -0.00880406 Jy ! Component: 3650 - total flux cleaned = -0.00887429 Jy ! Component: 3700 - total flux cleaned = -0.00883915 Jy ! Component: 3750 - total flux cleaned = -0.00866469 Jy ! Component: 3800 - total flux cleaned = -0.00876878 Jy ! Component: 3850 - total flux cleaned = -0.00894183 Jy ! Component: 3900 - total flux cleaned = -0.00901047 Jy ! Component: 3950 - total flux cleaned = -0.00904457 Jy ! Component: 4000 - total flux cleaned = -0.00911281 Jy ! Component: 4050 - total flux cleaned = -0.00921471 Jy ! Total flux subtracted in 4096 components = -0.00914682 Jy ! Clean residual min=-0.001878 max=0.002264 Jy/beam ! Clean residual mean=0.000001 rms=0.000556 Jy/beam ! Combined flux in latest and established models = 0.591454 Jy keep ! Adding 350 model components to the UV plane model. ! The established model now contains 445 components and 0.591454 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv119_uvs/J1043+2408_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7369 x 1.213 at -4.091 degrees (North through East) ! Clean map min=-0.002676 max=0.50525 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv119_uvs/J1043+2408_X_map.fits wmodel /scr/pima/rv119_uvs/J1043+2408_X_map.mod ! Writing 445 model components to file: /scr/pima/rv119_uvs/J1043+2408_X_map.mod wobs /scr/pima/rv119_uvs/J1043+2408_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv119_uvs/J1043+2408_X_uvs.fits wwins /scr/pima/rv119_uvs/J1043+2408_X_map.win ! wwins: Wrote 8 windows to /scr/pima/rv119_uvs/J1043+2408_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.505247 invert ! Inverting map ! Your choice of large map pixels excluded 5.77% of the data. ! The x-axis pixel size should ideally be below 0.167 milli-arcsec ! The y-axis pixel size should ideally be below 0.1705 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000555197 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.329659 0.329659 0.659318 1.31864 2.63727 5.27454 10.5491 21.0982 42.1963 84.3926 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0016 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.505 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 910.031 quit ! Quitting program ! Log file /scr/pima/rv119_uvs/J1043+2408_X_dfm.log closed on Sun Dec 17 11:35:19 2017