! Started logfile: /scr/pima/rv118_uvs/J0013+4051_X_dfm.log on Sun Dec 10 00:06:09 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/rv118_uvs/J0013+4051_X_uva.fits ! Reading UV FITS file: /scr/pima/rv118_uvs/J0013+4051_X_uva.fits ! AN table 1: 3 integrations on 36 of 36 possible baselines. ! AN table 2: 17 integrations on 6 of 6 possible baselines. ! AN table 3: 40 integrations on 28 of 28 possible baselines. ! AN table 4: 8 integrations on 45 of 45 possible baselines. ! AN table 5: 12 integrations on 55 of 55 possible baselines. ! Apparent sampling: 0.403404 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0013+4051 ! ! 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 3792 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 J0013+4051_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 9 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! A total of 200 telescope corrections were flagged in sub-array 3. ! A total of 26 telescope corrections were flagged in sub-array 4. ! A total of 104 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 9 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! A total of 200 telescope corrections were flagged in sub-array 3. ! A total of 26 telescope corrections were flagged in sub-array 4. ! A total of 104 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 9 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! A total of 200 telescope corrections were flagged in sub-array 3. ! A total of 26 telescope corrections were flagged in sub-array 4. ! A total of 104 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 9 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! A total of 200 telescope corrections were flagged in sub-array 3. ! A total of 26 telescope corrections were flagged in sub-array 4. ! A total of 104 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=1.123838Jy sigma=15.703703 ! Fit after self-cal, rms=0.535635Jy sigma=6.996228 ! clrmod: Cleared the established, tentative and continuum models. ! Redundant starting model cleared. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.51% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec ! Estimated beam: bmin=0.6366 mas, bmaj=0.9199 mas, bpa=32.49 degrees ! Estimated noise=1.29832 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 = 0.384787 Jy ! Component: 100 - total flux cleaned = 0.504855 Jy ! Total flux subtracted in 100 components = 0.504855 Jy ! Clean residual min=-0.015364 max=0.054494 Jy/beam ! Clean residual mean=0.000145 rms=0.003953 Jy/beam ! Combined flux in latest and established models = 0.504855 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.504855 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.136204Jy sigma=1.840414 ! Fit after self-cal, rms=0.135488Jy sigma=1.832410 ! Inverting map ! Your choice of large map pixels excluded 5.51% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0604575 Jy ! Component: 100 - total flux cleaned = 0.0924013 Jy ! Total flux subtracted in 100 components = 0.0924013 Jy ! Clean residual min=-0.010752 max=0.021400 Jy/beam ! Clean residual mean=0.000052 rms=0.002498 Jy/beam ! Combined flux in latest and established models = 0.597256 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 10 components and 0.597256 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.103174Jy sigma=1.272583 ! Fit after self-cal, rms=0.102469Jy sigma=1.265488 ! Inverting map ! Your choice of large map pixels excluded 5.51% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec ! Added new window around map position (-0.4, 0.8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0225999 Jy ! Component: 100 - total flux cleaned = 0.0345199 Jy ! Total flux subtracted in 100 components = 0.0345199 Jy ! Clean residual min=-0.009232 max=0.013381 Jy/beam ! Clean residual mean=0.000016 rms=0.002198 Jy/beam ! Combined flux in latest and established models = 0.631776 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 17 components and 0.631776 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.096283Jy sigma=1.155865 ! Fit after self-cal, rms=0.095881Jy sigma=1.150174 ! Inverting map ! Your choice of large map pixels excluded 5.51% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec ! Added new window around map position (1.6, 1.8). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0138898 Jy ! Component: 100 - total flux cleaned = 0.0226067 Jy ! Total flux subtracted in 100 components = 0.0226067 Jy ! Clean residual min=-0.009311 max=0.012037 Jy/beam ! Clean residual mean=-0.000007 rms=0.002048 Jy/beam ! Combined flux in latest and established models = 0.654383 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 26 components and 0.654383 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.094557Jy sigma=1.121399 ! Fit after self-cal, rms=0.094193Jy sigma=1.115600 ! Inverting map ! Your choice of large map pixels excluded 5.51% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec print "************** FINISHED UNIFORM WEIGHTING CLEAN **************" ! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** ! uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. win_mult = win_mult * 1.6 clean_niter = clean_niter * 2 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.51% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec ! Estimated beam: bmin=0.7014 mas, bmaj=1.001 mas, bpa=36.65 degrees ! Estimated noise=1.03164 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 = 0.00931087 Jy ! Component: 100 - total flux cleaned = 0.0139436 Jy ! Component: 150 - total flux cleaned = 0.0155104 Jy ! Component: 200 - total flux cleaned = 0.0157298 Jy ! Total flux subtracted in 200 components = 0.0157298 Jy ! Clean residual min=-0.010355 max=0.007815 Jy/beam ! Clean residual mean=-0.000034 rms=0.001972 Jy/beam ! Combined flux in latest and established models = 0.670113 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 34 components and 0.670113 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.093342Jy sigma=1.100293 ! Fit after self-cal, rms=0.093195Jy sigma=1.098725 ! Inverting map ! Your choice of large map pixels excluded 5.51% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7014 x 1.001 at 36.65 degrees (North through East) ! Clean map min=-0.0087665 max=0.4961 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.98 KP 0.97 LA 1.01 ! MK 1.02 NL 1.01 NY 1.15 OV 1.00 ! PT 1.01 ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! KK 1.11 NY 1.02 ON 0.98 WZ 0.96 ! ! A total of 78 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 HH 1.12 HN 1.00 LA 0.98 ! NL 1.05 ON 0.99 SC 1.02 WZ 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 FD 0.97 HN 1.00 KP 1.16 ! LA 0.99 NL 0.99 ON 1.00 PT 1.02 ! SC 1.01 WZ 0.99 ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.06 FD 0.95 HN 1.01 KK 0.96 ! KP 1.00 LA 0.97 NL 1.31 NY 0.98 ! OV 0.99 PT 0.99 SC 0.95 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 1.01 KP 0.99 LA 0.99 ! MK 0.99 NL 1.00 NY 1.10 OV 1.02 ! PT 1.02 ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! KK 1.03 NY 0.99 ON 0.98 WZ 1.03 ! ! A total of 78 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.05 HH 1.28 HN 1.02 LA 0.98 ! NL 1.03 ON 0.99 SC 0.95 WZ 1.00 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 FD 0.96 HN 1.03 KP 1.19 ! LA 0.96 NL 0.97 ON 1.02 PT 1.04 ! SC 1.00 WZ 0.99 ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 FD 0.95 HN 1.00 KK 0.98 ! KP 1.00 LA 0.96 NL 1.31 NY 1.09 ! OV 0.98 PT 0.96 SC 1.00 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.98 KP 0.96 LA 1.00 ! MK 1.00 NL 0.98 NY 1.16 OV 0.97 ! PT 1.02 ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! KK 1.34 NY 0.95 ON 1.02 WZ 0.94 ! ! A total of 78 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 HH 1.20 HN 0.98 LA 0.99 ! NL 1.10 ON 0.97 SC 0.97 WZ 0.98 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 FD 0.95 HN 0.99 KP 1.15 ! LA 1.00 NL 0.98 ON 0.98 PT 1.01 ! SC 0.98 WZ 0.97 ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 FD 0.91 HN 0.95 KK 0.99 ! KP 1.01 LA 0.98 NL 1.48 NY 1.01 ! OV 0.96 PT 0.95 SC 0.94 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 1.00 KP 1.00 LA 1.02 ! MK 1.02 NL 0.98 NY 1.09 OV 1.00 ! PT 0.97 ! ! A total of 24 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! KK 1.00 NY 0.97 ON 1.01 WZ 0.99 ! ! A total of 78 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 HH 1.16 HN 1.03 LA 0.98 ! NL 0.99 ON 0.99 SC 0.97 WZ 0.94 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 FD 0.97 HN 0.99 KP 1.17 ! LA 0.96 NL 0.93 ON 1.01 PT 1.03 ! SC 1.01 WZ 0.96 ! ! A total of 6 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 FD 0.94 HN 0.97 KK 1.03 ! KP 0.98 LA 0.97 NL 1.45 NY 1.05 ! OV 0.97 PT 0.92 SC 0.92 ! ! ! Fit before self-cal, rms=0.093195Jy sigma=1.098725 ! Fit after self-cal, rms=0.085020Jy sigma=0.953474 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec ! Estimated beam: bmin=0.7035 mas, bmaj=1.168 mas, bpa=26.98 degrees ! Estimated noise=1.07306 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 = -0.00133651 Jy ! Component: 100 - total flux cleaned = -0.0014463 Jy ! Component: 150 - total flux cleaned = -0.00176204 Jy ! Component: 200 - total flux cleaned = -0.00185605 Jy ! Total flux subtracted in 200 components = -0.00185605 Jy ! Clean residual min=-0.004801 max=0.004664 Jy/beam ! Clean residual mean=-0.000043 rms=0.001065 Jy/beam ! Combined flux in latest and established models = 0.668257 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 42 components and 0.668257 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.084559Jy sigma=0.947697 ! Fit after self-cal, rms=0.084584Jy sigma=0.947032 ! Inverting map ! Your choice of large map pixels excluded 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 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=0.084584Jy sigma=0.947032 ! Fit after self-cal, rms=0.084632Jy sigma=0.946384 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec ! Estimated beam: bmin=0.7039 mas, bmaj=1.167 mas, bpa=26.96 degrees ! Estimated noise=1.07387 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000287048 Jy ! Component: 100 - total flux cleaned = -0.00047757 Jy ! Component: 150 - total flux cleaned = -0.000561799 Jy ! Component: 200 - total flux cleaned = -0.000640667 Jy ! Total flux subtracted in 200 components = -0.000640667 Jy ! Clean residual min=-0.004545 max=0.004633 Jy/beam ! Clean residual mean=-0.000036 rms=0.001047 Jy/beam ! Combined flux in latest and established models = 0.667616 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 44 components and 0.667616 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.084392Jy sigma=0.943801 ! Fit after self-cal, rms=0.084346Jy sigma=0.943501 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 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 (-8.4, 0.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00260015 Jy ! Component: 100 - total flux cleaned = 0.0027083 Jy ! Component: 150 - total flux cleaned = 0.0025334 Jy ! Component: 200 - total flux cleaned = 0.00253458 Jy ! Total flux subtracted in 200 components = 0.00253458 Jy ! Clean residual min=-0.004567 max=0.004131 Jy/beam ! Clean residual mean=-0.000049 rms=0.001014 Jy/beam ! Combined flux in latest and established models = 0.670151 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 60 components and 0.670151 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.084010Jy sigma=0.939743 ! Fit after self-cal, rms=0.083985Jy sigma=0.939465 ! Inverting map ! Your choice of large map pixels excluded 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 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=0.083985Jy sigma=0.939465 ! Fit after self-cal, rms=0.084210Jy sigma=0.939101 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec ! Estimated beam: bmin=0.7041 mas, bmaj=1.168 mas, bpa=26.9 degrees ! Estimated noise=1.07462 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000995143 Jy ! Component: 100 - total flux cleaned = 0.00116547 Jy ! Component: 150 - total flux cleaned = 0.00108531 Jy ! Component: 200 - total flux cleaned = 0.00108708 Jy ! Total flux subtracted in 200 components = 0.00108708 Jy ! Clean residual min=-0.004342 max=0.004060 Jy/beam ! Clean residual mean=-0.000051 rms=0.001006 Jy/beam ! Combined flux in latest and established models = 0.671238 Jy selfcal ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 62 components and 0.671237 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.084012Jy sigma=0.937343 ! Fit after self-cal, rms=0.083983Jy sigma=0.937215 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 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 = 0.000323615 Jy ! Component: 100 - total flux cleaned = 0.000323627 Jy ! Component: 150 - total flux cleaned = 0.000322523 Jy ! Component: 200 - total flux cleaned = 0.000322874 Jy ! Total flux subtracted in 200 components = 0.000322874 Jy ! Clean residual min=-0.004312 max=0.004024 Jy/beam ! Clean residual mean=-0.000053 rms=0.000999 Jy/beam ! Combined flux in latest and established models = 0.67156 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 62 components and 0.67156 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.083827Jy sigma=0.935980 ! Fit after self-cal, rms=0.083802Jy sigma=0.935900 ! Inverting map ! Your choice of large map pixels excluded 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 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=0.083802Jy sigma=0.935900 ! Fit after self-cal, rms=0.083923Jy sigma=0.935757 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec ! Estimated beam: bmin=2.486 mas, bmaj=3.074 mas, bpa=-63.48 degrees ! Estimated noise=1.53847 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00165607 Jy ! Component: 100 - total flux cleaned = 0.00139777 Jy ! Component: 150 - total flux cleaned = 0.00114811 Jy ! Component: 200 - total flux cleaned = 0.00102265 Jy ! Total flux subtracted in 200 components = 0.00102265 Jy ! Clean residual min=-0.005262 max=0.005198 Jy/beam ! Clean residual mean=-0.000144 rms=0.001455 Jy/beam ! Combined flux in latest and established models = 0.672583 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 69 components and 0.672583 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.084002Jy sigma=0.935875 ! Fit after self-cal, rms=0.083983Jy sigma=0.935672 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 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 = 7.39374e-05 Jy ! Component: 100 - total flux cleaned = -2.70501e-05 Jy ! Component: 150 - total flux cleaned = -0.000209104 Jy ! Component: 200 - total flux cleaned = -0.000261296 Jy ! Total flux subtracted in 200 components = -0.000261296 Jy ! Clean residual min=-0.005247 max=0.005152 Jy/beam ! Clean residual mean=-0.000140 rms=0.001455 Jy/beam ! Combined flux in latest and established models = 0.672322 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 72 components and 0.672322 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.084048Jy sigma=0.935990 ! Fit after self-cal, rms=0.084049Jy sigma=0.935875 ! Inverting map ! Your choice of large map pixels excluded 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 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 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec ! Estimated beam: bmin=0.7041 mas, bmaj=1.168 mas, bpa=26.85 degrees ! Estimated noise=1.07509 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7041 x 1.168 at 26.85 degrees (North through East) ! Clean map min=-0.0037732 max=0.50385 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=0.084049Jy sigma=0.935875 ! Fit after self-cal, rms=0.079988Jy sigma=0.864910 ! Inverting map and beam ! Your choice of large map pixels excluded 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec ! Estimated beam: bmin=0.7037 mas, bmaj=1.167 mas, bpa=26.83 degrees ! Estimated noise=1.07569 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00051792 Jy ! Component: 100 - total flux cleaned = 0.000834929 Jy ! Component: 150 - total flux cleaned = 0.0007658 Jy ! Component: 200 - total flux cleaned = 0.000835542 Jy ! Total flux subtracted in 200 components = 0.000835542 Jy ! Clean residual min=-0.004178 max=0.004014 Jy/beam ! Clean residual mean=-0.000056 rms=0.000979 Jy/beam ! Combined flux in latest and established models = 0.673157 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 76 components and 0.673157 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.079790Jy sigma=0.863502 ! Fit after self-cal, rms=0.079766Jy sigma=0.863415 ! Inverting map ! Your choice of large map pixels excluded 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 6.83001e-05 Jy ! Component: 100 - total flux cleaned = 2.80512e-06 Jy ! Component: 150 - total flux cleaned = -6.27883e-05 Jy ! Component: 200 - total flux cleaned = -6.36912e-05 Jy ! Total flux subtracted in 200 components = -6.36912e-05 Jy ! Clean residual min=-0.004198 max=0.004031 Jy/beam ! Clean residual mean=-0.000055 rms=0.000975 Jy/beam ! Combined flux in latest and established models = 0.673093 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 76 components and 0.673093 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.079624Jy sigma=0.862427 ! Fit after self-cal, rms=0.079598Jy sigma=0.862366 ! Inverting map ! Your choice of large map pixels excluded 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.079598Jy sigma=0.862366 ! Fit after self-cal, rms=0.079568Jy sigma=0.862223 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 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec ! Estimated beam: bmin=0.636 mas, bmaj=1.007 mas, bpa=26.7 degrees ! Estimated noise=1.35857 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.390601 Jy ! Component: 100 - total flux cleaned = 0.512408 Jy ! Component: 150 - total flux cleaned = 0.574699 Jy ! Component: 200 - total flux cleaned = 0.609572 Jy ! Total flux subtracted in 200 components = 0.609572 Jy ! Clean residual min=-0.007639 max=0.017554 Jy/beam ! Clean residual mean=0.000044 rms=0.001821 Jy/beam ! Combined flux in latest and established models = 0.609572 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 0.609572 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec ! Estimated beam: bmin=0.7033 mas, bmaj=1.168 mas, bpa=26.78 degrees ! Estimated noise=1.07593 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 = 0.0263317 Jy ! Component: 100 - total flux cleaned = 0.0406689 Jy ! Component: 150 - total flux cleaned = 0.0494628 Jy ! Component: 200 - total flux cleaned = 0.0555313 Jy ! Total flux subtracted in 200 components = 0.0555313 Jy ! Clean residual min=-0.004669 max=0.005818 Jy/beam ! Clean residual mean=-0.000009 rms=0.001061 Jy/beam ! Combined flux in latest and established models = 0.665103 Jy ! Adding 18 model components to the UV plane model. ! The established model now contains 22 components and 0.665103 Jy ! Inverting map ! Your choice of large map pixels excluded 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec ! Added new window around map position (-1.2, -0.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00436895 Jy ! Component: 100 - total flux cleaned = 0.00496395 Jy ! Component: 150 - total flux cleaned = 0.00561771 Jy ! Component: 200 - total flux cleaned = 0.00607423 Jy ! Total flux subtracted in 200 components = 0.00607423 Jy ! Clean residual min=-0.004329 max=0.004128 Jy/beam ! Clean residual mean=-0.000041 rms=0.001007 Jy/beam ! Combined flux in latest and established models = 0.671177 Jy ! Adding 18 model components to the UV plane model. ! The established model now contains 35 components and 0.671177 Jy ! Inverting map ! Your choice of large map pixels excluded 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 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 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec ! Estimated beam: bmin=2.486 mas, bmaj=3.072 mas, bpa=-63.43 degrees ! Estimated noise=1.54174 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000813023 Jy ! Component: 100 - total flux cleaned = 0.000533375 Jy ! Component: 150 - total flux cleaned = 0.000425032 Jy ! Component: 200 - total flux cleaned = 0.000550902 Jy ! Total flux subtracted in 200 components = 0.000550902 Jy ! Clean residual min=-0.005367 max=0.005097 Jy/beam ! Clean residual mean=-0.000126 rms=0.001404 Jy/beam ! Combined flux in latest and established models = 0.671728 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 = 0.000154418 Jy ! Component: 100 - total flux cleaned = 0.000262813 Jy ! Component: 150 - total flux cleaned = 0.000365744 Jy ! Component: 200 - total flux cleaned = 0.000495263 Jy ! Total flux subtracted in 200 components = 0.000495263 Jy ! Clean residual min=-0.005328 max=0.005114 Jy/beam ! Clean residual mean=-0.000133 rms=0.001400 Jy/beam ! Combined flux in latest and established models = 0.672224 Jy ! Adding 15 model components to the UV plane model. ! The established model now contains 50 components and 0.672224 Jy ! Inverting map ! Your choice of large map pixels excluded 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec ! Estimated beam: bmin=0.7033 mas, bmaj=1.168 mas, bpa=26.78 degrees ! Estimated noise=1.07593 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000253553 Jy ! Component: 100 - total flux cleaned = -0.000253609 Jy ! Component: 150 - total flux cleaned = -0.000159691 Jy ! Component: 200 - total flux cleaned = -6.90905e-05 Jy ! Total flux subtracted in 200 components = -6.90905e-05 Jy ! Clean residual min=-0.004253 max=0.003989 Jy/beam ! Clean residual mean=-0.000047 rms=0.000991 Jy/beam ! Combined flux in latest and established models = 0.672154 Jy selfcal ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 60 components and 0.672155 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.080186Jy sigma=0.867785 ! Fit after self-cal, rms=0.079915Jy sigma=0.866266 wmodel J0013+4051_X_map.mod ! Writing 60 model components to file: J0013+4051_X_map.mod wobs J0013+4051_X_uvs.fits ! Writing UV FITS file: J0013+4051_X_uvs.fits wwins J0013+4051_X_map.win ! wwins: Wrote 5 windows to J0013+4051_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 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000957693 Jy ! Component: 100 - total flux cleaned = -0.00118372 Jy ! Component: 150 - total flux cleaned = -0.00176971 Jy ! Component: 200 - total flux cleaned = -0.00212708 Jy ! Component: 250 - total flux cleaned = -0.00261864 Jy ! Component: 300 - total flux cleaned = -0.00310007 Jy ! Component: 350 - total flux cleaned = -0.00357426 Jy ! Component: 400 - total flux cleaned = -0.00384112 Jy ! Component: 450 - total flux cleaned = -0.00436441 Jy ! Component: 500 - total flux cleaned = -0.00468674 Jy ! Component: 550 - total flux cleaned = -0.0050676 Jy ! Component: 600 - total flux cleaned = -0.00556709 Jy ! Component: 650 - total flux cleaned = -0.00587461 Jy ! Component: 700 - total flux cleaned = -0.00630017 Jy ! Component: 750 - total flux cleaned = -0.00666036 Jy ! Component: 800 - total flux cleaned = -0.00683885 Jy ! Component: 850 - total flux cleaned = -0.00719133 Jy ! Component: 900 - total flux cleaned = -0.00724953 Jy ! Component: 950 - total flux cleaned = -0.00759492 Jy ! Component: 1000 - total flux cleaned = -0.00782317 Jy ! Component: 1050 - total flux cleaned = -0.00771029 Jy ! Component: 1100 - total flux cleaned = -0.00827014 Jy ! Component: 1150 - total flux cleaned = -0.00821448 Jy ! Component: 1200 - total flux cleaned = -0.00843483 Jy ! Component: 1250 - total flux cleaned = -0.00859882 Jy ! Component: 1300 - total flux cleaned = -0.00870678 Jy ! Component: 1350 - total flux cleaned = -0.00870657 Jy ! Component: 1400 - total flux cleaned = -0.00881338 Jy ! Component: 1450 - total flux cleaned = -0.0089721 Jy ! Component: 1500 - total flux cleaned = -0.00912954 Jy ! Component: 1550 - total flux cleaned = -0.00918165 Jy ! Component: 1600 - total flux cleaned = -0.00944013 Jy ! Component: 1650 - total flux cleaned = -0.00959308 Jy ! Component: 1700 - total flux cleaned = -0.00969438 Jy ! Component: 1750 - total flux cleaned = -0.00959381 Jy ! Component: 1800 - total flux cleaned = -0.00989441 Jy ! Component: 1850 - total flux cleaned = -0.00994395 Jy ! Component: 1900 - total flux cleaned = -0.00989449 Jy ! Component: 1950 - total flux cleaned = -0.0101398 Jy ! Component: 2000 - total flux cleaned = -0.0101875 Jy ! Component: 2050 - total flux cleaned = -0.0100907 Jy ! Component: 2100 - total flux cleaned = -0.0103309 Jy ! Component: 2150 - total flux cleaned = -0.010331 Jy ! Component: 2200 - total flux cleaned = -0.0103305 Jy ! Component: 2250 - total flux cleaned = -0.0102836 Jy ! Component: 2300 - total flux cleaned = -0.0105179 Jy ! Component: 2350 - total flux cleaned = -0.0106109 Jy ! Component: 2400 - total flux cleaned = -0.0104259 Jy ! Component: 2450 - total flux cleaned = -0.0106565 Jy ! Component: 2500 - total flux cleaned = -0.0107936 Jy ! Component: 2550 - total flux cleaned = -0.0108389 Jy ! Component: 2600 - total flux cleaned = -0.0109289 Jy ! Component: 2650 - total flux cleaned = -0.0109739 Jy ! Component: 2700 - total flux cleaned = -0.0109291 Jy ! Component: 2750 - total flux cleaned = -0.0109734 Jy ! Component: 2800 - total flux cleaned = -0.0111945 Jy ! Component: 2850 - total flux cleaned = -0.0110628 Jy ! Component: 2900 - total flux cleaned = -0.0111504 Jy ! Component: 2950 - total flux cleaned = -0.011281 Jy ! Component: 3000 - total flux cleaned = -0.0113241 Jy ! Component: 3050 - total flux cleaned = -0.0113237 Jy ! Component: 3100 - total flux cleaned = -0.0114524 Jy ! Component: 3150 - total flux cleaned = -0.0114095 Jy ! Component: 3200 - total flux cleaned = -0.0114519 Jy ! Component: 3250 - total flux cleaned = -0.0114943 Jy ! Component: 3300 - total flux cleaned = -0.0115781 Jy ! Component: 3350 - total flux cleaned = -0.0118285 Jy ! Component: 3400 - total flux cleaned = -0.0117867 Jy ! Component: 3450 - total flux cleaned = -0.0117867 Jy ! Component: 3500 - total flux cleaned = -0.0119102 Jy ! Component: 3550 - total flux cleaned = -0.0117467 Jy ! Component: 3600 - total flux cleaned = -0.0119909 Jy ! Component: 3650 - total flux cleaned = -0.0119501 Jy ! Component: 3700 - total flux cleaned = -0.0120307 Jy ! Component: 3750 - total flux cleaned = -0.0118302 Jy ! Component: 3800 - total flux cleaned = -0.0119102 Jy ! Component: 3850 - total flux cleaned = -0.0120296 Jy ! Component: 3900 - total flux cleaned = -0.0120691 Jy ! Component: 3950 - total flux cleaned = -0.0122265 Jy ! Component: 4000 - total flux cleaned = -0.0120697 Jy ! Component: 4050 - total flux cleaned = -0.0121476 Jy ! Total flux subtracted in 4096 components = -0.0122252 Jy ! Clean residual min=-0.002409 max=0.002067 Jy/beam ! Clean residual mean=-0.000016 rms=0.000632 Jy/beam ! Combined flux in latest and established models = 0.659929 Jy keep ! Adding 327 model components to the UV plane model. ! The established model now contains 387 components and 0.659929 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv118_uvs/J0013+4051_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7033 x 1.168 at 26.78 degrees (North through East) ! Clean map min=-0.0033123 max=0.50362 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv118_uvs/J0013+4051_X_map.fits wmodel /scr/pima/rv118_uvs/J0013+4051_X_map.mod ! Writing 387 model components to file: /scr/pima/rv118_uvs/J0013+4051_X_map.mod wobs /scr/pima/rv118_uvs/J0013+4051_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv118_uvs/J0013+4051_X_uvs.fits wwins /scr/pima/rv118_uvs/J0013+4051_X_map.win ! wwins: Wrote 6 windows to /scr/pima/rv118_uvs/J0013+4051_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.503622 invert ! Inverting map ! Your choice of large map pixels excluded 5.33% of the data. ! The x-axis pixel size should ideally be below 0.1747 milli-arcsec ! The y-axis pixel size should ideally be below 0.1574 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000630955 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.375851 0.375851 0.751701 1.5034 3.0068 6.01361 12.0272 24.0544 48.1089 96.2177 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0018 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.503 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 798.189 quit ! Quitting program ! Log file /scr/pima/rv118_uvs/J0013+4051_X_dfm.log closed on Sun Dec 10 00:06:14 2017