! Started logfile: /scr/pima/rv124_uvs/J1751+0939_X_dfm.log on Mon Dec 24 00:20:33 2018 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/rv124_uvs/J1751+0939_X_uva.fits ! Reading UV FITS file: /scr/pima/rv124_uvs/J1751+0939_X_uva.fits ! AN table 1: 71 integrations on 10 of 10 possible baselines. ! AN table 2: 41 integrations on 78 of 78 possible baselines. ! AN table 3: 40 integrations on 21 of 21 possible baselines. ! AN table 4: 13 integrations on 3 of 3 possible baselines. ! Apparent sampling: 0.307291 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1751+0939 ! ! 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 5884 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 J1751+0939_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 print "===============================================================" ! =============================================================== ! print "=== Difmap script: pima_mupet_01.dvm version of 2016.05.19 === " ! === Difmap script: pima_mupet_01.dvm version of 2016.05.19 === ! 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 165 telescope corrections were flagged in sub-array 1. ! A total of 423 telescope corrections were flagged in sub-array 2. ! A total of 126 telescope corrections were flagged in sub-array 3. ! A total of 3 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 165 telescope corrections were flagged in sub-array 1. ! A total of 423 telescope corrections were flagged in sub-array 2. ! A total of 126 telescope corrections were flagged in sub-array 3. ! A total of 3 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 253 telescope corrections were flagged in sub-array 1. ! A total of 435 telescope corrections were flagged in sub-array 2. ! A total of 126 telescope corrections were flagged in sub-array 3. ! A total of 39 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 253 telescope corrections were flagged in sub-array 1. ! A total of 435 telescope corrections were flagged in sub-array 2. ! A total of 126 telescope corrections were flagged in sub-array 3. ! A total of 39 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=2.053635Jy sigma=64.897666 ! Fit after self-cal, rms=1.046145Jy sigma=57.747783 ! 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 8.3% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1784 milli-arcsec ! Estimated beam: bmin=0.364 mas, bmaj=0.403 mas, bpa=-35.21 degrees ! Estimated noise=0.594006 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 = 0.639778 Jy ! Component: 100 - total flux cleaned = 1.04851 Jy ! Total flux subtracted in 100 components = 1.04851 Jy ! Clean residual min=-0.116197 max=0.344001 Jy/beam ! Clean residual mean=-0.000002 rms=0.023096 Jy/beam ! Combined flux in latest and established models = 1.04851 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 1.04851 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.975187Jy sigma=16.854274 ! Fit after self-cal, rms=0.975668Jy sigma=16.845848 ! Inverting map ! Your choice of large map pixels excluded 8.3% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1784 milli-arcsec ! Added new window around map position (0, 0.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.34052 Jy ! Component: 100 - total flux cleaned = 0.568921 Jy ! Total flux subtracted in 100 components = 0.568921 Jy ! Clean residual min=-0.095375 max=0.198628 Jy/beam ! Clean residual mean=-0.000116 rms=0.015985 Jy/beam ! Combined flux in latest and established models = 1.61743 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 12 components and 1.61743 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.619416Jy sigma=11.426032 ! Fit after self-cal, rms=0.656014Jy sigma=10.841170 ! Inverting map ! Your choice of large map pixels excluded 8.3% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1784 milli-arcsec ! Added new window around map position (0, -0.6). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.19266 Jy ! Component: 100 - total flux cleaned = 0.329087 Jy ! Total flux subtracted in 100 components = 0.329087 Jy ! Clean residual min=-0.072915 max=0.078126 Jy/beam ! Clean residual mean=-0.000182 rms=0.010300 Jy/beam ! Combined flux in latest and established models = 1.94652 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 15 components and 1.94652 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.522305Jy sigma=8.169413 ! Fit after self-cal, rms=0.496111Jy sigma=7.822825 ! Inverting map ! Your choice of large map pixels excluded 8.3% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1784 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.111175 Jy ! Component: 100 - total flux cleaned = 0.188535 Jy ! Total flux subtracted in 100 components = 0.188535 Jy ! Clean residual min=-0.072106 max=0.059970 Jy/beam ! Clean residual mean=-0.000220 rms=0.008882 Jy/beam ! Combined flux in latest and established models = 2.13505 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 17 components and 2.13505 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.451362Jy sigma=7.172527 ! Fit after self-cal, rms=0.448427Jy sigma=6.956243 ! Inverting map ! Your choice of large map pixels excluded 8.3% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1784 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0690092 Jy ! Component: 100 - total flux cleaned = 0.113844 Jy ! Total flux subtracted in 100 components = 0.113844 Jy ! Clean residual min=-0.071445 max=0.051105 Jy/beam ! Clean residual mean=-0.000242 rms=0.008221 Jy/beam ! Combined flux in latest and established models = 2.2489 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 17 components and 2.2489 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.439360Jy sigma=6.570215 ! Fit after self-cal, rms=0.433832Jy sigma=6.476379 ! Inverting map ! Your choice of large map pixels excluded 8.3% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1784 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 8.3% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1784 milli-arcsec ! Estimated beam: bmin=0.3551 mas, bmaj=0.4236 mas, bpa=43.53 degrees ! Estimated noise=0.428488 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 = -0.00254419 Jy ! Component: 100 - total flux cleaned = -0.00831607 Jy ! Component: 150 - total flux cleaned = -0.0126108 Jy ! Component: 200 - total flux cleaned = -0.0152414 Jy ! Total flux subtracted in 200 components = -0.0152414 Jy ! Clean residual min=-0.065781 max=0.034276 Jy/beam ! Clean residual mean=-0.010907 rms=0.007429 Jy/beam ! Combined flux in latest and established models = 2.23366 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 21 components and 2.23366 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.427849Jy sigma=6.604939 ! Fit after self-cal, rms=0.432495Jy sigma=6.553688 ! Inverting map ! Your choice of large map pixels excluded 8.3% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1784 milli-arcsec print "============== Finished natural weighting clean ==============" ! ============== Finished natural weighting clean ============== ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.3551 x 0.4236 at 43.53 degrees (North through East) ! Clean map min=-0.039494 max=0.7519 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 54 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 1.00* NY 1.04 WN 1.71 WZ 0.85 ! YG 1.94 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 FD 0.88 HH 1.00* HN 1.05 ! KP 1.19 LA 1.03 NL 1.07 NY 0.56 ! OV 0.99 PT 0.90 SC 0.81 WN 1.40 ! WZ 0.84 ! ! A total of 48 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 0.96 KP 1.09 MK 0.94 ! OV 0.97 PT 0.92 YG 6.67 ! ! A total of 36 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! MK 0.00* NY 0.00* YG 0.00* ! ! ! Correcting IF 2. ! A total of 54 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 1.00* NY 1.21 WN 1.78 WZ 0.74 ! YG 1.61 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 0.88 HH 1.00* HN 1.06 ! KP 1.16 LA 1.01 NL 1.07 NY 0.71 ! OV 0.98 PT 0.88 SC 0.82 WN 1.47 ! WZ 0.84 ! ! A total of 48 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 FD 0.96 KP 1.08 MK 0.91 ! OV 0.97 PT 0.92 YG 6.59 ! ! A total of 36 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! MK 0.00* NY 0.00* YG 0.00* ! ! ! Correcting IF 3. ! A total of 102 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.00* NY 0.00* WN 0.00* WZ 0.00* ! YG 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 0.89 HH 1.00* HN 1.07 ! KP 1.18 LA 1.01 NL 1.08 NY 1.00* ! OV 0.98 PT 0.89 SC 0.79 WN 1.43 ! WZ 0.79 ! ! A total of 48 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 FD 0.95 KP 1.06 MK 0.91 ! OV 0.96 PT 0.94 YG 3.22 ! ! Telescope amplitude corrections in sub-array 4: ! MK 0.00* NY 0.00* YG 0.00* ! ! ! Correcting IF 4. ! A total of 102 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.00* NY 0.00* WN 0.00* WZ 0.00* ! YG 0.00* ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 0.89 HH 1.00* HN 1.05 ! KP 1.17 LA 1.02 NL 1.08 NY 1.00* ! OV 0.97 PT 0.89 SC 0.82 WN 1.23 ! WZ 0.80 ! ! A total of 48 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 0.95 KP 1.07 MK 0.89 ! OV 0.97 PT 0.92 YG 3.47 ! ! Telescope amplitude corrections in sub-array 4: ! MK 0.00* NY 0.00* YG 0.00* ! ! ! Fit before self-cal, rms=0.432495Jy sigma=6.553688 ! Fit after self-cal, rms=0.272653Jy sigma=3.429942 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 milli-arcsec ! Estimated beam: bmin=0.4461 mas, bmaj=0.677 mas, bpa=36.2 degrees ! Estimated noise=0.937805 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 = -0.0209759 Jy ! Component: 100 - total flux cleaned = -0.0278594 Jy ! Component: 150 - total flux cleaned = -0.0343377 Jy ! Component: 200 - total flux cleaned = -0.0393476 Jy ! Total flux subtracted in 200 components = -0.0393476 Jy ! Clean residual min=-0.067558 max=0.041166 Jy/beam ! Clean residual mean=-0.006177 rms=0.007994 Jy/beam ! Combined flux in latest and established models = 2.19431 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 22 components and 2.19431 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.249961Jy sigma=3.195259 ! Fit after self-cal, rms=0.229296Jy sigma=3.026697 ! Inverting map ! Your choice of large map pixels excluded 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 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=0.229296Jy sigma=3.026697 ! Fit after self-cal, rms=0.207133Jy sigma=2.812867 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 milli-arcsec ! Estimated beam: bmin=0.4901 mas, bmaj=0.7129 mas, bpa=30.26 degrees ! Estimated noise=1.03411 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0160762 Jy ! Component: 100 - total flux cleaned = -0.0210562 Jy ! Component: 150 - total flux cleaned = -0.0258834 Jy ! Component: 200 - total flux cleaned = -0.0292069 Jy ! Total flux subtracted in 200 components = -0.0292069 Jy ! Clean residual min=-0.053791 max=0.036231 Jy/beam ! Clean residual mean=-0.005860 rms=0.007079 Jy/beam ! Combined flux in latest and established models = 2.1651 Jy selfcal ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 22 components and 2.1651 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.194376Jy sigma=2.705244 ! Fit after self-cal, rms=0.195794Jy sigma=2.661353 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 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 = 0.000905212 Jy ! Component: 100 - total flux cleaned = -0.00209253 Jy ! Component: 150 - total flux cleaned = -0.005342 Jy ! Component: 200 - total flux cleaned = -0.00592956 Jy ! Total flux subtracted in 200 components = -0.00592956 Jy ! Clean residual min=-0.053100 max=0.036052 Jy/beam ! Clean residual mean=-0.005769 rms=0.007000 Jy/beam ! Combined flux in latest and established models = 2.15917 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 22 components and 2.15917 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.193411Jy sigma=2.658907 ! Fit after self-cal, rms=0.193760Jy sigma=2.615802 ! Inverting map ! Your choice of large map pixels excluded 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 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=0.193760Jy sigma=2.615802 ! Fit after self-cal, rms=0.192545Jy sigma=2.398914 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 milli-arcsec ! Estimated beam: bmin=0.5236 mas, bmaj=0.7524 mas, bpa=25.85 degrees ! Estimated noise=1.09624 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00743908 Jy ! Component: 100 - total flux cleaned = -0.0123716 Jy ! Component: 150 - total flux cleaned = -0.0165247 Jy ! Component: 200 - total flux cleaned = -0.0200521 Jy ! Total flux subtracted in 200 components = -0.0200521 Jy ! Clean residual min=-0.050777 max=0.034178 Jy/beam ! Clean residual mean=-0.005525 rms=0.006598 Jy/beam ! Combined flux in latest and established models = 2.13912 Jy selfcal ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 22 components and 2.13912 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.186001Jy sigma=2.315480 ! Fit after self-cal, rms=0.186780Jy sigma=2.285270 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 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 = 0.00212629 Jy ! Component: 100 - total flux cleaned = 0.000811836 Jy ! Component: 150 - total flux cleaned = -0.000833704 Jy ! Component: 200 - total flux cleaned = -0.00134573 Jy ! Total flux subtracted in 200 components = -0.00134573 Jy ! Clean residual min=-0.051450 max=0.034242 Jy/beam ! Clean residual mean=-0.005504 rms=0.006454 Jy/beam ! Combined flux in latest and established models = 2.13777 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 22 components and 2.13777 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.185114Jy sigma=2.265057 ! Fit after self-cal, rms=0.184322Jy sigma=2.234331 ! Inverting map ! Your choice of large map pixels excluded 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 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=0.184322Jy sigma=2.234331 ! Fit after self-cal, rms=0.183296Jy sigma=2.131617 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 milli-arcsec ! Estimated beam: bmin=2.53 mas, bmaj=2.696 mas, bpa=-9.419 degrees ! Estimated noise=1.74586 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0149954 Jy ! Component: 100 - total flux cleaned = -0.0182799 Jy ! Component: 150 - total flux cleaned = -0.0182758 Jy ! Component: 200 - total flux cleaned = -0.0182652 Jy ! Total flux subtracted in 200 components = -0.0182652 Jy ! Clean residual min=-0.027066 max=0.023972 Jy/beam ! Clean residual mean=-0.013635 rms=0.003842 Jy/beam ! Combined flux in latest and established models = 2.11951 Jy selfcal ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 22 components and 2.11951 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.182252Jy sigma=2.110139 ! Fit after self-cal, rms=0.182095Jy sigma=2.109461 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 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 = 3.42981e-05 Jy ! Component: 100 - total flux cleaned = 4.05478e-05 Jy ! Component: 150 - total flux cleaned = 4.06282e-05 Jy ! Component: 200 - total flux cleaned = 0.000139307 Jy ! Total flux subtracted in 200 components = 0.000139307 Jy ! Clean residual min=-0.027027 max=0.024126 Jy/beam ! Clean residual mean=-0.013641 rms=0.003836 Jy/beam ! Combined flux in latest and established models = 2.11965 Jy ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 22 components and 2.11965 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.181966Jy sigma=2.107253 ! Fit after self-cal, rms=0.181936Jy sigma=2.106398 ! Inverting map ! Your choice of large map pixels excluded 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 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 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 milli-arcsec ! Estimated beam: bmin=0.5492 mas, bmaj=0.7865 mas, bpa=21.86 degrees ! Estimated noise=1.13637 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5492 x 0.7865 at 21.86 degrees (North through East) ! Clean map min=-0.034771 max=1.3591 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=0.181936Jy sigma=2.106398 ! Fit after self-cal, rms=0.176166Jy sigma=2.062928 ! Inverting map and beam ! Your choice of large map pixels excluded 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 milli-arcsec ! Estimated beam: bmin=0.5587 mas, bmaj=0.7954 mas, bpa=19.92 degrees ! Estimated noise=1.1431 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00125096 Jy ! Component: 100 - total flux cleaned = -0.00429065 Jy ! Component: 150 - total flux cleaned = -0.00755326 Jy ! Component: 200 - total flux cleaned = -0.00925095 Jy ! Total flux subtracted in 200 components = -0.00925095 Jy ! Clean residual min=-0.046928 max=0.033560 Jy/beam ! Clean residual mean=-0.004721 rms=0.006133 Jy/beam ! Combined flux in latest and established models = 2.1104 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 22 components and 2.1104 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.172414Jy sigma=1.995019 ! Fit after self-cal, rms=0.171551Jy sigma=1.968067 ! Inverting map ! Your choice of large map pixels excluded 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00304144 Jy ! Component: 100 - total flux cleaned = 0.00242056 Jy ! Component: 150 - total flux cleaned = 0.000973742 Jy ! Component: 200 - total flux cleaned = 0.000114007 Jy ! Total flux subtracted in 200 components = 0.000114007 Jy ! Clean residual min=-0.047331 max=0.033180 Jy/beam ! Clean residual mean=-0.004723 rms=0.005988 Jy/beam ! Combined flux in latest and established models = 2.11051 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 22 components and 2.11051 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.170293Jy sigma=1.949285 ! Fit after self-cal, rms=0.169183Jy sigma=1.928333 ! Inverting map ! Your choice of large map pixels excluded 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.169183Jy sigma=1.928333 ! Fit after self-cal, rms=0.170492Jy sigma=1.872452 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 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 milli-arcsec ! Estimated beam: bmin=0.6082 mas, bmaj=0.8437 mas, bpa=-5.587 degrees ! Estimated noise=1.73594 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.36731 Jy ! Component: 100 - total flux cleaned = 1.82903 Jy ! Component: 150 - total flux cleaned = 2.00476 Jy ! Component: 200 - total flux cleaned = 2.07302 Jy ! Total flux subtracted in 200 components = 2.07302 Jy ! Clean residual min=-0.069591 max=0.060627 Jy/beam ! Clean residual mean=-0.000195 rms=0.009276 Jy/beam ! Combined flux in latest and established models = 2.07302 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 11 model components to the UV plane model. ! The established model now contains 11 components and 2.07302 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 milli-arcsec ! Estimated beam: bmin=0.5754 mas, bmaj=0.8226 mas, bpa=16.96 degrees ! Estimated noise=1.1649 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 = 0.0105468 Jy ! Component: 100 - total flux cleaned = 0.011717 Jy ! Component: 150 - total flux cleaned = 0.0146971 Jy ! Component: 200 - total flux cleaned = 0.0171889 Jy ! Total flux subtracted in 200 components = 0.0171889 Jy ! Clean residual min=-0.050557 max=0.046797 Jy/beam ! Clean residual mean=-0.004248 rms=0.007244 Jy/beam ! Combined flux in latest and established models = 2.09021 Jy ! Adding 7 model components to the UV plane model. ! The established model now contains 13 components and 2.09021 Jy ! Inverting map ! Your choice of large map pixels excluded 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 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 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 milli-arcsec ! Estimated beam: bmin=2.53 mas, bmaj=2.693 mas, bpa=-8.64 degrees ! Estimated noise=1.72869 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00952742 Jy ! Component: 100 - total flux cleaned = 0.00943746 Jy ! Component: 150 - total flux cleaned = 0.00939309 Jy ! Component: 200 - total flux cleaned = 0.00937252 Jy ! Total flux subtracted in 200 components = 0.00937252 Jy ! Clean residual min=-0.025346 max=0.024767 Jy/beam ! Clean residual mean=-0.011531 rms=0.003777 Jy/beam ! Combined flux in latest and established models = 2.09958 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 = -4.88308e-06 Jy ! Component: 100 - total flux cleaned = -7.46892e-06 Jy ! Component: 150 - total flux cleaned = -1.01537e-05 Jy ! Component: 200 - total flux cleaned = -1.27516e-05 Jy ! Total flux subtracted in 200 components = -1.27516e-05 Jy ! Clean residual min=-0.024970 max=0.024475 Jy/beam ! Clean residual mean=-0.011530 rms=0.003717 Jy/beam ! Combined flux in latest and established models = 2.09957 Jy ! Adding 4 model components to the UV plane model. ! The established model now contains 16 components and 2.09957 Jy ! Inverting map ! Your choice of large map pixels excluded 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 milli-arcsec ! Estimated beam: bmin=0.5754 mas, bmaj=0.8226 mas, bpa=16.96 degrees ! Estimated noise=1.1649 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00334865 Jy ! Component: 100 - total flux cleaned = -0.0033764 Jy ! Component: 150 - total flux cleaned = -0.00198381 Jy ! Component: 200 - total flux cleaned = -0.000206467 Jy ! Total flux subtracted in 200 components = -0.000206467 Jy ! Clean residual min=-0.048358 max=0.041748 Jy/beam ! Clean residual mean=-0.004404 rms=0.006880 Jy/beam ! Combined flux in latest and established models = 2.09936 Jy selfcal ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 18 components and 2.09936 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.186404Jy sigma=2.077649 ! Fit after self-cal, rms=0.181578Jy sigma=2.008457 wmodel J1751+0939_X_map.mod ! Writing 18 model components to file: J1751+0939_X_map.mod wobs J1751+0939_X_uvs.fits ! Writing UV FITS file: J1751+0939_X_uvs.fits wwins J1751+0939_X_map.win ! wwins: Wrote 3 windows to J1751+0939_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 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00928086 Jy ! Component: 100 - total flux cleaned = -0.0127393 Jy ! Component: 150 - total flux cleaned = -0.0184432 Jy ! Component: 200 - total flux cleaned = -0.0225835 Jy ! Component: 250 - total flux cleaned = -0.0287489 Jy ! Component: 300 - total flux cleaned = -0.0346631 Jy ! Component: 350 - total flux cleaned = -0.0418827 Jy ! Component: 400 - total flux cleaned = -0.048851 Jy ! Component: 450 - total flux cleaned = -0.055595 Jy ! Component: 500 - total flux cleaned = -0.063054 Jy ! Component: 550 - total flux cleaned = -0.0689299 Jy ! Component: 600 - total flux cleaned = -0.0750714 Jy ! Component: 650 - total flux cleaned = -0.0810412 Jy ! Component: 700 - total flux cleaned = -0.0864418 Jy ! Component: 750 - total flux cleaned = -0.0917098 Jy ! Component: 800 - total flux cleaned = -0.0976413 Jy ! Component: 850 - total flux cleaned = -0.102658 Jy ! Component: 900 - total flux cleaned = -0.107934 Jy ! Component: 950 - total flux cleaned = -0.113091 Jy ! Component: 1000 - total flux cleaned = -0.11849 Jy ! Component: 1050 - total flux cleaned = -0.123062 Jy ! Component: 1100 - total flux cleaned = -0.127201 Jy ! Component: 1150 - total flux cleaned = -0.131255 Jy ! Component: 1200 - total flux cleaned = -0.13556 Jy ! Component: 1250 - total flux cleaned = -0.139453 Jy ! Component: 1300 - total flux cleaned = -0.143589 Jy ! Component: 1350 - total flux cleaned = -0.147015 Jy ! Component: 1400 - total flux cleaned = -0.150378 Jy ! Component: 1450 - total flux cleaned = -0.153675 Jy ! Component: 1500 - total flux cleaned = -0.156621 Jy ! Component: 1550 - total flux cleaned = -0.159803 Jy ! Component: 1600 - total flux cleaned = -0.162643 Jy ! Component: 1650 - total flux cleaned = -0.165714 Jy ! Component: 1700 - total flux cleaned = -0.167637 Jy ! Component: 1750 - total flux cleaned = -0.169804 Jy ! Component: 1800 - total flux cleaned = -0.1722 Jy ! Component: 1850 - total flux cleaned = -0.174036 Jy ! Component: 1900 - total flux cleaned = -0.175587 Jy ! Component: 1950 - total flux cleaned = -0.177372 Jy ! Component: 2000 - total flux cleaned = -0.178878 Jy ! Component: 2050 - total flux cleaned = -0.180366 Jy ! Component: 2100 - total flux cleaned = -0.181347 Jy ! Component: 2150 - total flux cleaned = -0.183041 Jy ! Component: 2200 - total flux cleaned = -0.184947 Jy ! Component: 2250 - total flux cleaned = -0.18612 Jy ! Component: 2300 - total flux cleaned = -0.18705 Jy ! Component: 2350 - total flux cleaned = -0.188197 Jy ! Component: 2400 - total flux cleaned = -0.189553 Jy ! Component: 2450 - total flux cleaned = -0.190893 Jy ! Component: 2500 - total flux cleaned = -0.191777 Jy ! Component: 2550 - total flux cleaned = -0.192868 Jy ! Component: 2600 - total flux cleaned = -0.194161 Jy ! Component: 2650 - total flux cleaned = -0.195013 Jy ! Component: 2700 - total flux cleaned = -0.195856 Jy ! Component: 2750 - total flux cleaned = -0.196898 Jy ! Component: 2800 - total flux cleaned = -0.197722 Jy ! Component: 2850 - total flux cleaned = -0.198535 Jy ! Component: 2900 - total flux cleaned = -0.199338 Jy ! Component: 2950 - total flux cleaned = -0.200331 Jy ! Component: 3000 - total flux cleaned = -0.201312 Jy ! Component: 3050 - total flux cleaned = -0.201893 Jy ! Component: 3100 - total flux cleaned = -0.202661 Jy ! Component: 3150 - total flux cleaned = -0.203422 Jy ! Component: 3200 - total flux cleaned = -0.204359 Jy ! Component: 3250 - total flux cleaned = -0.204914 Jy ! Component: 3300 - total flux cleaned = -0.205466 Jy ! Component: 3350 - total flux cleaned = -0.206192 Jy ! Component: 3400 - total flux cleaned = -0.20709 Jy ! Component: 3450 - total flux cleaned = -0.2078 Jy ! Component: 3500 - total flux cleaned = -0.208501 Jy ! Component: 3550 - total flux cleaned = -0.209023 Jy ! Component: 3600 - total flux cleaned = -0.209538 Jy ! Component: 3650 - total flux cleaned = -0.210217 Jy ! Component: 3700 - total flux cleaned = -0.210891 Jy ! Component: 3750 - total flux cleaned = -0.211225 Jy ! Component: 3800 - total flux cleaned = -0.212051 Jy ! Component: 3850 - total flux cleaned = -0.21254 Jy ! Component: 3900 - total flux cleaned = -0.213026 Jy ! Component: 3950 - total flux cleaned = -0.213506 Jy ! Component: 4000 - total flux cleaned = -0.213982 Jy ! Component: 4050 - total flux cleaned = -0.214609 Jy ! Total flux subtracted in 4096 components = -0.215229 Jy ! Clean residual min=-0.008558 max=0.007715 Jy/beam ! Clean residual mean=-0.000570 rms=0.002359 Jy/beam ! Combined flux in latest and established models = 1.88414 Jy keep ! Adding 292 model components to the UV plane model. ! The established model now contains 310 components and 1.88414 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv124_uvs/J1751+0939_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5754 x 0.8226 at 16.96 degrees (North through East) ! Clean map min=-0.019709 max=1.4263 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv124_uvs/J1751+0939_X_map.fits wmodel /scr/pima/rv124_uvs/J1751+0939_X_map.mod ! Writing 310 model components to file: /scr/pima/rv124_uvs/J1751+0939_X_map.mod wobs /scr/pima/rv124_uvs/J1751+0939_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv124_uvs/J1751+0939_X_uvs.fits wwins /scr/pima/rv124_uvs/J1751+0939_X_map.win ! wwins: Wrote 4 windows to /scr/pima/rv124_uvs/J1751+0939_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 1.42629 invert ! Inverting map ! Your choice of large map pixels excluded 7.41% of the data. ! The x-axis pixel size should ideally be below 0.1692 milli-arcsec ! The y-axis pixel size should ideally be below 0.1806 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00234895 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.494066 0.494066 0.988132 1.97626 3.95253 7.90506 15.8101 31.6202 63.2405 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.007 print "peak= ", int(1000*peak_flux)/1000 ! peak= 1.426 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 607.206 quit ! Quitting program ! Log file /scr/pima/rv124_uvs/J1751+0939_X_dfm.log closed on Mon Dec 24 00:20:38 2018