! Started logfile: /scr/pima/rv117_uvs/J0702-1951_X_dfm.log on Sat Dec 9 23:42:08 2017 float field_size field_size = 1024 float field_cell field_cell = 0.2000 float taper_size taper_size = 70.0 float freq freq = 8.36575 obs /scr/pima/rv117_uvs/J0702-1951_X_uva.fits ! Reading UV FITS file: /scr/pima/rv117_uvs/J0702-1951_X_uva.fits ! AN table 1: 5 integrations on 6 of 6 possible baselines. ! AN table 2: 2 integrations on 15 of 15 possible baselines. ! AN table 3: 2 integrations on 28 of 28 possible baselines. ! AN table 4: 2 integrations on 10 of 10 possible baselines. ! AN table 5: 4 integrations on 28 of 28 possible baselines. ! AN table 6: 15 integrations on 3 of 3 possible baselines. ! Apparent sampling: 0.979522 visibilities/baseline/integration-bin. ! Found source: J0702-1951 ! ! There are 4 IFs, and a total of 4 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 8.36575e+09 8e+06 1 8e+06 ! 02 2 8.44575e+09 8e+06 1 8e+06 ! 03 3 8.80575e+09 8e+06 1 8e+06 ! 04 4 8.92575e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 74 lines of history. ! ! Reading 1148 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 J0702-1951_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 6 telescope corrections were flagged in sub-array 1. ! A total of 3 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 3 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 3 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 3 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.426703Jy sigma=18.598669 ! Fit after self-cal, rms=0.245042Jy sigma=2.657531 ! 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 4.68% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! Estimated beam: bmin=0.7013 mas, bmaj=0.8945 mas, bpa=20.25 degrees ! Estimated noise=2.16257 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 = 0.762705 Jy ! Component: 100 - total flux cleaned = 0.968443 Jy ! Total flux subtracted in 100 components = 0.968443 Jy ! Clean residual min=-0.030915 max=0.091024 Jy/beam ! Clean residual mean=0.000152 rms=0.007936 Jy/beam ! Combined flux in latest and established models = 0.968444 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 0.968444 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.206356Jy sigma=2.481857 ! Fit after self-cal, rms=0.205785Jy sigma=2.475695 ! Inverting map ! Your choice of large map pixels excluded 4.68% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! Added new window around map position (0.6, -1). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0969037 Jy ! Component: 100 - total flux cleaned = 0.149771 Jy ! Total flux subtracted in 100 components = 0.149771 Jy ! Clean residual min=-0.024141 max=0.042884 Jy/beam ! Clean residual mean=0.000033 rms=0.005041 Jy/beam ! Combined flux in latest and established models = 1.11821 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 11 components and 1.11821 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.144133Jy sigma=1.576897 ! Fit after self-cal, rms=0.140166Jy sigma=1.522468 ! Inverting map ! Your choice of large map pixels excluded 4.68% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! Added new window around map position (-0.4, -2.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0420592 Jy ! Component: 100 - total flux cleaned = 0.0557838 Jy ! Total flux subtracted in 100 components = 0.0557838 Jy ! Clean residual min=-0.020147 max=0.024864 Jy/beam ! Clean residual mean=-0.000011 rms=0.004043 Jy/beam ! Combined flux in latest and established models = 1.174 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 15 components and 1.174 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.127033Jy sigma=1.324928 ! Fit after self-cal, rms=0.125272Jy sigma=1.297691 ! Inverting map ! Your choice of large map pixels excluded 4.68% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! Added new window around map position (1.6, -0.8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0192842 Jy ! Component: 100 - total flux cleaned = 0.0225934 Jy ! Total flux subtracted in 100 components = 0.0225934 Jy ! Clean residual min=-0.016960 max=0.019086 Jy/beam ! Clean residual mean=-0.000029 rms=0.003633 Jy/beam ! Combined flux in latest and established models = 1.19659 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 20 components and 1.19659 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.120208Jy sigma=1.233449 ! Fit after self-cal, rms=0.119655Jy sigma=1.226099 ! Inverting map ! Your choice of large map pixels excluded 4.68% of the data. ! The x-axis pixel size should ideally be below 0.1646 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 4.68% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! Estimated beam: bmin=0.8766 mas, bmaj=1.079 mas, bpa=20.9 degrees ! Estimated noise=1.79312 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 = 0.0112863 Jy ! Component: 100 - total flux cleaned = 0.0127371 Jy ! Component: 150 - total flux cleaned = 0.013036 Jy ! Component: 200 - total flux cleaned = 0.0132907 Jy ! Total flux subtracted in 200 components = 0.0132907 Jy ! Clean residual min=-0.012685 max=0.014871 Jy/beam ! Clean residual mean=-0.000041 rms=0.003347 Jy/beam ! Combined flux in latest and established models = 1.20988 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 23 components and 1.20988 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.117243Jy sigma=1.195870 ! Fit after self-cal, rms=0.116950Jy sigma=1.192104 ! Inverting map ! Your choice of large map pixels excluded 4.68% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8766 x 1.079 at 20.9 degrees (North through East) ! Clean map min=-0.01439 max=0.94792 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.89 HN 1.35 ON 1.07 SC 0.99 ! ! Telescope amplitude corrections in sub-array 2: ! FD 1.00 HH 1.02 HN 1.04 LA 1.21 ! SC 1.00 WZ 0.90 ! ! Telescope amplitude corrections in sub-array 3: ! FD 0.99 HH 0.93 HN 1.04 KP 0.98 ! LA 0.96 NL 1.00 PT 1.01 SC 1.00 ! ! Telescope amplitude corrections in sub-array 4: ! HN 0.98 LA 1.03 NL 1.02 OV 1.01 ! PT 0.98 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 FD 1.01 KP 0.97 LA 1.02 ! MK 1.00 NL 1.04 OV 0.97 PT 1.00 ! ! A total of 42 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! HH 0.00* ON 0.00* WZ 0.00* ! ! ! Correcting IF 2. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 0.95 HN 1.28 ON 1.08 SC 0.98 ! ! Telescope amplitude corrections in sub-array 2: ! FD 0.99 HH 1.04 HN 1.08 LA 1.23 ! SC 0.95 WZ 0.97 ! ! Telescope amplitude corrections in sub-array 3: ! FD 0.99 HH 0.83 HN 1.05 KP 0.99 ! LA 0.93 NL 1.00 PT 1.05 SC 1.00 ! ! Telescope amplitude corrections in sub-array 4: ! HN 0.96 LA 1.00 NL 0.99 OV 0.99 ! PT 1.00 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 FD 0.99 KP 0.97 LA 0.99 ! MK 1.00 NL 1.05 OV 0.97 PT 0.99 ! ! A total of 42 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! HH 0.00* ON 0.00* WZ 0.00* ! ! ! Correcting IF 3. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 1.00 HN 1.22 ON 1.06 SC 0.96 ! ! Telescope amplitude corrections in sub-array 2: ! FD 0.94 HH 1.02 HN 1.04 LA 1.35 ! SC 0.96 WZ 0.94 ! ! Telescope amplitude corrections in sub-array 3: ! FD 1.01 HH 0.96 HN 1.05 KP 0.98 ! LA 0.99 NL 0.99 PT 1.04 SC 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! HN 0.98 LA 0.98 NL 0.99 OV 1.01 ! PT 1.00 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.03 FD 0.98 KP 0.99 LA 1.02 ! MK 0.98 NL 1.05 OV 0.96 PT 0.99 ! ! A total of 42 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! HH 0.00* ON 0.00* WZ 0.00* ! ! ! Correcting IF 4. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! HH 1.16 HN 1.43 ON 1.05 SC 0.89 ! ! Telescope amplitude corrections in sub-array 2: ! FD 0.96 HH 1.14 HN 1.07 LA 1.28 ! SC 0.94 WZ 0.93 ! ! Telescope amplitude corrections in sub-array 3: ! FD 0.99 HH 1.09 HN 1.07 KP 0.97 ! LA 0.95 NL 0.98 PT 1.06 SC 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! HN 0.92 LA 1.07 NL 0.99 OV 0.97 ! PT 1.00 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 FD 1.00 KP 0.98 LA 1.00 ! MK 0.99 NL 1.05 OV 0.96 PT 0.99 ! ! A total of 42 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! HH 0.00* ON 0.00* WZ 0.00* ! ! ! Fit before self-cal, rms=0.116950Jy sigma=1.192104 ! Fit after self-cal, rms=0.095465Jy sigma=0.994652 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! Estimated beam: bmin=0.8725 mas, bmaj=1.525 mas, bpa=3.846 degrees ! Estimated noise=1.87055 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 = -0.00715455 Jy ! Component: 100 - total flux cleaned = -0.00916954 Jy ! Component: 150 - total flux cleaned = -0.0100354 Jy ! Component: 200 - total flux cleaned = -0.0107375 Jy ! Total flux subtracted in 200 components = -0.0107375 Jy ! Clean residual min=-0.010762 max=0.010876 Jy/beam ! Clean residual mean=0.000033 rms=0.002437 Jy/beam ! Combined flux in latest and established models = 1.19915 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 31 components and 1.19915 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.093482Jy sigma=0.969425 ! Fit after self-cal, rms=0.093671Jy sigma=0.965783 ! Inverting map ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 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=0.093671Jy sigma=0.965783 ! Fit after self-cal, rms=0.088289Jy sigma=0.877432 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! Estimated beam: bmin=0.8727 mas, bmaj=1.523 mas, bpa=3.803 degrees ! Estimated noise=1.87047 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000197283 Jy ! Component: 100 - total flux cleaned = -0.000830771 Jy ! Component: 150 - total flux cleaned = -0.00137739 Jy ! Component: 200 - total flux cleaned = -0.00149858 Jy ! Total flux subtracted in 200 components = -0.00149858 Jy ! Clean residual min=-0.006741 max=0.007194 Jy/beam ! Clean residual mean=-0.000002 rms=0.001627 Jy/beam ! Combined flux in latest and established models = 1.19765 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 36 components and 1.19765 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.087437Jy sigma=0.866322 ! Fit after self-cal, rms=0.087333Jy sigma=0.864468 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 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 (19.8, 19.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00340518 Jy ! Component: 100 - total flux cleaned = 0.00339234 Jy ! Component: 150 - total flux cleaned = 0.00286193 Jy ! Component: 200 - total flux cleaned = 0.002228 Jy ! Total flux subtracted in 200 components = 0.002228 Jy ! Clean residual min=-0.006849 max=0.006883 Jy/beam ! Clean residual mean=0.000003 rms=0.001553 Jy/beam ! Combined flux in latest and established models = 1.19987 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 45 components and 1.19987 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.086339Jy sigma=0.852539 ! Fit after self-cal, rms=0.086228Jy sigma=0.851893 ! Inverting map ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! Added new window around map position (-26.2, 6.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00496229 Jy ! Component: 100 - total flux cleaned = 0.00581783 Jy ! Component: 150 - total flux cleaned = 0.00597252 Jy ! Component: 200 - total flux cleaned = 0.00611311 Jy ! Total flux subtracted in 200 components = 0.00611311 Jy ! Clean residual min=-0.006457 max=0.006734 Jy/beam ! Clean residual mean=-0.000001 rms=0.001494 Jy/beam ! Combined flux in latest and established models = 1.20599 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 53 components and 1.20599 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.085373Jy sigma=0.842971 ! Fit after self-cal, rms=0.085331Jy sigma=0.842497 ! Inverting map ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! Added new window around map position (-1.8, 20.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00262307 Jy ! Component: 100 - total flux cleaned = 0.00279623 Jy ! Component: 150 - total flux cleaned = 0.00353775 Jy ! Component: 200 - total flux cleaned = 0.0039522 Jy ! Total flux subtracted in 200 components = 0.0039522 Jy ! Clean residual min=-0.006153 max=0.006388 Jy/beam ! Clean residual mean=0.000002 rms=0.001426 Jy/beam ! Combined flux in latest and established models = 1.20994 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 64 components and 1.20994 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.084348Jy sigma=0.831265 ! Fit after self-cal, rms=0.084306Jy sigma=0.830772 ! Inverting map ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! Added new window around map position (-9.6, 21). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00627765 Jy ! Component: 100 - total flux cleaned = 0.00924374 Jy ! Component: 150 - total flux cleaned = 0.010457 Jy ! Component: 200 - total flux cleaned = 0.0113453 Jy ! Total flux subtracted in 200 components = 0.0113453 Jy ! Clean residual min=-0.005558 max=0.005656 Jy/beam ! Clean residual mean=0.000014 rms=0.001346 Jy/beam ! Combined flux in latest and established models = 1.22129 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 72 components and 1.22128 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.083516Jy sigma=0.821454 ! Fit after self-cal, rms=0.083489Jy sigma=0.821015 ! Inverting map ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 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=0.083489Jy sigma=0.821015 ! Fit after self-cal, rms=0.083011Jy sigma=0.817070 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! Estimated beam: bmin=0.8723 mas, bmaj=1.521 mas, bpa=3.848 degrees ! Estimated noise=1.8674 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00152641 Jy ! Component: 100 - total flux cleaned = 0.00294254 Jy ! Component: 150 - total flux cleaned = 0.00319981 Jy ! Component: 200 - total flux cleaned = 0.00368589 Jy ! Total flux subtracted in 200 components = 0.00368589 Jy ! Clean residual min=-0.005066 max=0.005354 Jy/beam ! Clean residual mean=0.000009 rms=0.001281 Jy/beam ! Combined flux in latest and established models = 1.22497 Jy selfcal ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 76 components and 1.22497 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.082490Jy sigma=0.810763 ! Fit after self-cal, rms=0.082490Jy sigma=0.810489 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 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 = 1.65035e-06 Jy ! Component: 100 - total flux cleaned = 0.000230386 Jy ! Component: 150 - total flux cleaned = 0.000448287 Jy ! Component: 200 - total flux cleaned = 0.000660426 Jy ! Total flux subtracted in 200 components = 0.000660426 Jy ! Clean residual min=-0.005009 max=0.005280 Jy/beam ! Clean residual mean=0.000010 rms=0.001260 Jy/beam ! Combined flux in latest and established models = 1.22563 Jy ! Performing phase self-cal ! Adding 32 model components to the UV plane model. ! The established model now contains 81 components and 1.22563 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.082106Jy sigma=0.806670 ! Fit after self-cal, rms=0.082086Jy sigma=0.806540 ! Inverting map ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 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=0.082086Jy sigma=0.806540 ! Fit after self-cal, rms=0.082057Jy sigma=0.805956 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! Estimated beam: bmin=2.344 mas, bmaj=4.221 mas, bpa=-3.464 degrees ! Estimated noise=2.20557 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00172537 Jy ! Component: 100 - total flux cleaned = 0.00240739 Jy ! Component: 150 - total flux cleaned = 0.00284983 Jy ! Component: 200 - total flux cleaned = 0.00315294 Jy ! Total flux subtracted in 200 components = 0.00315294 Jy ! Clean residual min=-0.004107 max=0.004829 Jy/beam ! Clean residual mean=0.000014 rms=0.001263 Jy/beam ! Combined flux in latest and established models = 1.22878 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 100 components and 1.22878 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.082067Jy sigma=0.805309 ! Fit after self-cal, rms=0.082075Jy sigma=0.805237 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 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 = 0.000386144 Jy ! Component: 100 - total flux cleaned = 0.000672488 Jy ! Component: 150 - total flux cleaned = 0.000893541 Jy ! Component: 200 - total flux cleaned = 0.00106218 Jy ! Total flux subtracted in 200 components = 0.00106218 Jy ! Clean residual min=-0.004131 max=0.004861 Jy/beam ! Clean residual mean=0.000015 rms=0.001259 Jy/beam ! Combined flux in latest and established models = 1.22985 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 109 components and 1.22985 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.082077Jy sigma=0.804795 ! Fit after self-cal, rms=0.082074Jy sigma=0.804734 ! Inverting map ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 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 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! Estimated beam: bmin=0.8725 mas, bmaj=1.521 mas, bpa=3.825 degrees ! Estimated noise=1.86597 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8725 x 1.521 at 3.825 degrees (North through East) ! Clean map min=-0.018128 max=0.94683 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=0.082074Jy sigma=0.804734 ! Fit after self-cal, rms=0.075174Jy sigma=0.698366 ! Inverting map and beam ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! Estimated beam: bmin=0.8723 mas, bmaj=1.521 mas, bpa=3.835 degrees ! Estimated noise=1.86542 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000544849 Jy ! Component: 100 - total flux cleaned = -0.000653978 Jy ! Component: 150 - total flux cleaned = -0.000655363 Jy ! Component: 200 - total flux cleaned = -0.000752216 Jy ! Total flux subtracted in 200 components = -0.000752216 Jy ! Clean residual min=-0.004964 max=0.005254 Jy/beam ! Clean residual mean=0.000007 rms=0.001222 Jy/beam ! Combined flux in latest and established models = 1.22909 Jy ! Performing phase self-cal ! Adding 32 model components to the UV plane model. ! The established model now contains 113 components and 1.22909 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.074766Jy sigma=0.694307 ! Fit after self-cal, rms=0.074733Jy sigma=0.694141 ! Inverting map ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! Added new window around map position (-46.2, 38.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00290152 Jy ! Component: 100 - total flux cleaned = 0.00352964 Jy ! Component: 150 - total flux cleaned = 0.00352914 Jy ! Component: 200 - total flux cleaned = 0.00382532 Jy ! Total flux subtracted in 200 components = 0.00382532 Jy ! Clean residual min=-0.004622 max=0.005045 Jy/beam ! Clean residual mean=0.000001 rms=0.001173 Jy/beam ! Combined flux in latest and established models = 1.23292 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 126 components and 1.23292 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.074228Jy sigma=0.687232 ! Fit after self-cal, rms=0.074197Jy sigma=0.686860 ! Inverting map ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! Added new window around map position (-17.6, 7.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00425736 Jy ! Component: 100 - total flux cleaned = 0.00494538 Jy ! Component: 150 - total flux cleaned = 0.00525633 Jy ! Component: 200 - total flux cleaned = 0.00545368 Jy ! Total flux subtracted in 200 components = 0.00545368 Jy ! Clean residual min=-0.004929 max=0.004538 Jy/beam ! Clean residual mean=-0.000003 rms=0.001131 Jy/beam ! Combined flux in latest and established models = 1.23837 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 136 components and 1.23837 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.073687Jy sigma=0.681014 ! Fit after self-cal, rms=0.073657Jy sigma=0.680631 ! Inverting map ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.073657Jy sigma=0.680631 ! Fit after self-cal, rms=0.073663Jy sigma=0.679860 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 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! Estimated beam: bmin=0.695 mas, bmaj=1.23 mas, bpa=5.603 degrees ! Estimated noise=2.24051 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.746285 Jy ! Component: 100 - total flux cleaned = 0.953402 Jy ! Component: 150 - total flux cleaned = 1.05401 Jy ! Component: 200 - total flux cleaned = 1.11212 Jy ! Total flux subtracted in 200 components = 1.11212 Jy ! Clean residual min=-0.013138 max=0.029410 Jy/beam ! Clean residual mean=0.000081 rms=0.003557 Jy/beam ! Combined flux in latest and established models = 1.11212 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 19 model components to the UV plane model. ! The established model now contains 19 components and 1.11212 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! Estimated beam: bmin=0.8724 mas, bmaj=1.521 mas, bpa=3.847 degrees ! Estimated noise=1.86471 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 = 0.0445483 Jy ! Component: 100 - total flux cleaned = 0.0672997 Jy ! Component: 150 - total flux cleaned = 0.0794163 Jy ! Component: 200 - total flux cleaned = 0.085355 Jy ! Total flux subtracted in 200 components = 0.085355 Jy ! Clean residual min=-0.007620 max=0.009618 Jy/beam ! Clean residual mean=0.000006 rms=0.001674 Jy/beam ! Combined flux in latest and established models = 1.19747 Jy ! Adding 27 model components to the UV plane model. ! The established model now contains 36 components and 1.19747 Jy ! Inverting map ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! Added new window around map position (1.4, -3.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00712367 Jy ! Component: 100 - total flux cleaned = 0.0114583 Jy ! Component: 150 - total flux cleaned = 0.0153797 Jy ! Component: 200 - total flux cleaned = 0.0187433 Jy ! Total flux subtracted in 200 components = 0.0187433 Jy ! Clean residual min=-0.006376 max=0.006123 Jy/beam ! Clean residual mean=0.000001 rms=0.001437 Jy/beam ! Combined flux in latest and established models = 1.21622 Jy ! Adding 33 model components to the UV plane model. ! The established model now contains 60 components and 1.21622 Jy ! Inverting map ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 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 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! Estimated beam: bmin=2.343 mas, bmaj=4.221 mas, bpa=-3.448 degrees ! Estimated noise=2.2048 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00636676 Jy ! Component: 100 - total flux cleaned = 0.0110314 Jy ! Component: 150 - total flux cleaned = 0.0147771 Jy ! Component: 200 - total flux cleaned = 0.0171306 Jy ! Total flux subtracted in 200 components = 0.0171306 Jy ! Clean residual min=-0.004652 max=0.004609 Jy/beam ! Clean residual mean=-0.000012 rms=0.001265 Jy/beam ! Combined flux in latest and established models = 1.23335 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 = 0.00154585 Jy ! Component: 100 - total flux cleaned = 0.00307755 Jy ! Component: 150 - total flux cleaned = 0.00438798 Jy ! Component: 200 - total flux cleaned = 0.00532307 Jy ! Total flux subtracted in 200 components = 0.00532307 Jy ! Clean residual min=-0.004536 max=0.004332 Jy/beam ! Clean residual mean=-0.000010 rms=0.001198 Jy/beam ! Combined flux in latest and established models = 1.23867 Jy ! Adding 38 model components to the UV plane model. ! The established model now contains 95 components and 1.23867 Jy ! Inverting map ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! Estimated beam: bmin=0.8724 mas, bmaj=1.521 mas, bpa=3.847 degrees ! Estimated noise=1.86471 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00112857 Jy ! Component: 100 - total flux cleaned = 0.00170793 Jy ! Component: 150 - total flux cleaned = 0.00206203 Jy ! Component: 200 - total flux cleaned = 0.00255176 Jy ! Total flux subtracted in 200 components = 0.00255176 Jy ! Clean residual min=-0.005577 max=0.005227 Jy/beam ! Clean residual mean=-0.000003 rms=0.001243 Jy/beam ! Combined flux in latest and established models = 1.24122 Jy selfcal ! Performing phase self-cal ! Adding 33 model components to the UV plane model. ! The established model now contains 114 components and 1.24122 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.075066Jy sigma=0.697001 ! Fit after self-cal, rms=0.074135Jy sigma=0.685814 wmodel J0702-1951_X_map.mod ! Writing 114 model components to file: J0702-1951_X_map.mod wobs J0702-1951_X_uvs.fits ! Writing UV FITS file: J0702-1951_X_uvs.fits wwins J0702-1951_X_map.win ! wwins: Wrote 11 windows to J0702-1951_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 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000479039 Jy ! Component: 100 - total flux cleaned = -0.00056558 Jy ! Component: 150 - total flux cleaned = -0.000737607 Jy ! Component: 200 - total flux cleaned = -0.000987983 Jy ! Component: 250 - total flux cleaned = -0.00082585 Jy ! Component: 300 - total flux cleaned = -0.000588545 Jy ! Component: 350 - total flux cleaned = -0.000511844 Jy ! Component: 400 - total flux cleaned = -0.000208395 Jy ! Component: 450 - total flux cleaned = 0.000239981 Jy ! Component: 500 - total flux cleaned = 0.000679673 Jy ! Component: 550 - total flux cleaned = 0.00118364 Jy ! Component: 600 - total flux cleaned = 0.00146713 Jy ! Component: 650 - total flux cleaned = 0.00160855 Jy ! Component: 700 - total flux cleaned = 0.00202496 Jy ! Component: 750 - total flux cleaned = 0.00236712 Jy ! Component: 800 - total flux cleaned = 0.00256956 Jy ! Component: 850 - total flux cleaned = 0.00283593 Jy ! Component: 900 - total flux cleaned = 0.00296829 Jy ! Component: 950 - total flux cleaned = 0.0030344 Jy ! Component: 1000 - total flux cleaned = 0.00342032 Jy ! Component: 1050 - total flux cleaned = 0.00361112 Jy ! Component: 1100 - total flux cleaned = 0.00379991 Jy ! Component: 1150 - total flux cleaned = 0.00392411 Jy ! Component: 1200 - total flux cleaned = 0.00392495 Jy ! Component: 1250 - total flux cleaned = 0.00422866 Jy ! Component: 1300 - total flux cleaned = 0.00440936 Jy ! Component: 1350 - total flux cleaned = 0.00452785 Jy ! Component: 1400 - total flux cleaned = 0.00458738 Jy ! Component: 1450 - total flux cleaned = 0.0048784 Jy ! Component: 1500 - total flux cleaned = 0.00476227 Jy ! Component: 1550 - total flux cleaned = 0.00476321 Jy ! Component: 1600 - total flux cleaned = 0.00498894 Jy ! Component: 1650 - total flux cleaned = 0.00482119 Jy ! Component: 1700 - total flux cleaned = 0.00482169 Jy ! Component: 1750 - total flux cleaned = 0.00509664 Jy ! Component: 1800 - total flux cleaned = 0.00520527 Jy ! Component: 1850 - total flux cleaned = 0.00520564 Jy ! Component: 1900 - total flux cleaned = 0.00525916 Jy ! Component: 1950 - total flux cleaned = 0.0052062 Jy ! Component: 2000 - total flux cleaned = 0.00520628 Jy ! Component: 2050 - total flux cleaned = 0.00515392 Jy ! Component: 2100 - total flux cleaned = 0.00510172 Jy ! Component: 2150 - total flux cleaned = 0.00499871 Jy ! Component: 2200 - total flux cleaned = 0.00504954 Jy ! Component: 2250 - total flux cleaned = 0.00484717 Jy ! Component: 2300 - total flux cleaned = 0.00489751 Jy ! Component: 2350 - total flux cleaned = 0.00479813 Jy ! Component: 2400 - total flux cleaned = 0.00499609 Jy ! Component: 2450 - total flux cleaned = 0.0047997 Jy ! Component: 2500 - total flux cleaned = 0.0046536 Jy ! Component: 2550 - total flux cleaned = 0.00455655 Jy ! Component: 2600 - total flux cleaned = 0.00460414 Jy ! Component: 2650 - total flux cleaned = 0.00455639 Jy ! Component: 2700 - total flux cleaned = 0.00436677 Jy ! Component: 2750 - total flux cleaned = 0.00431984 Jy ! Component: 2800 - total flux cleaned = 0.00427328 Jy ! Component: 2850 - total flux cleaned = 0.00413408 Jy ! Component: 2900 - total flux cleaned = 0.00413443 Jy ! Component: 2950 - total flux cleaned = 0.00413434 Jy ! Component: 3000 - total flux cleaned = 0.00417996 Jy ! Component: 3050 - total flux cleaned = 0.00422522 Jy ! Component: 3100 - total flux cleaned = 0.00422507 Jy ! Component: 3150 - total flux cleaned = 0.00426906 Jy ! Component: 3200 - total flux cleaned = 0.00426895 Jy ! Component: 3250 - total flux cleaned = 0.0040928 Jy ! Component: 3300 - total flux cleaned = 0.00422408 Jy ! Component: 3350 - total flux cleaned = 0.00444238 Jy ! Component: 3400 - total flux cleaned = 0.00457223 Jy ! Component: 3450 - total flux cleaned = 0.00474434 Jy ! Component: 3500 - total flux cleaned = 0.00465918 Jy ! Component: 3550 - total flux cleaned = 0.00487152 Jy ! Component: 3600 - total flux cleaned = 0.00491391 Jy ! Component: 3650 - total flux cleaned = 0.00529218 Jy ! Component: 3700 - total flux cleaned = 0.00537587 Jy ! Component: 3750 - total flux cleaned = 0.00550067 Jy ! Component: 3800 - total flux cleaned = 0.00574869 Jy ! Component: 3850 - total flux cleaned = 0.00595437 Jy ! Component: 3900 - total flux cleaned = 0.00611801 Jy ! Component: 3950 - total flux cleaned = 0.00619934 Jy ! Component: 4000 - total flux cleaned = 0.00636106 Jy ! Component: 4050 - total flux cleaned = 0.00656195 Jy ! Total flux subtracted in 4096 components = 0.00672172 Jy ! Clean residual min=-0.002817 max=0.002136 Jy/beam ! Clean residual mean=0.000006 rms=0.000662 Jy/beam ! Combined flux in latest and established models = 1.24794 Jy keep ! Adding 291 model components to the UV plane model. ! The established model now contains 404 components and 1.24794 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv117_uvs/J0702-1951_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8724 x 1.521 at 3.847 degrees (North through East) ! Clean map min=-0.0088425 max=0.93878 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv117_uvs/J0702-1951_X_map.fits wmodel /scr/pima/rv117_uvs/J0702-1951_X_map.mod ! Writing 404 model components to file: /scr/pima/rv117_uvs/J0702-1951_X_map.mod wobs /scr/pima/rv117_uvs/J0702-1951_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv117_uvs/J0702-1951_X_uvs.fits wwins /scr/pima/rv117_uvs/J0702-1951_X_map.win ! wwins: Wrote 12 windows to /scr/pima/rv117_uvs/J0702-1951_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.938783 invert ! Inverting map ! Your choice of large map pixels excluded 5.65% of the data. ! The x-axis pixel size should ideally be below 0.1646 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000658848 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.210543 0.210543 0.421086 0.842172 1.68434 3.36869 6.73738 13.4748 26.9495 53.899 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0019 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.938 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 1424.89 quit ! Quitting program ! Log file /scr/pima/rv117_uvs/J0702-1951_X_dfm.log closed on Sat Dec 9 23:42:12 2017