! Started logfile: /scr/pima/rv119_uvs/J2145+1115_X_dfm.log on Sun Dec 17 11:38:14 2017 float field_size field_size = 1024 float field_cell field_cell = 0.2000 float taper_size taper_size = 70.0 float freq freq = 8.36575 obs /scr/pima/rv119_uvs/J2145+1115_X_uva.fits ! Reading UV FITS file: /scr/pima/rv119_uvs/J2145+1115_X_uva.fits ! AN table 1: 172 integrations on 55 of 55 possible baselines. ! AN table 2: 15 integrations on 28 of 28 possible baselines. ! Apparent sampling: 0.216397 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J2145+1115 ! ! 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 8552 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 J2145+1115_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 1288 telescope corrections were flagged in sub-array 1. ! A total of 60 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 2. ! A total of 1288 telescope corrections were flagged in sub-array 1. ! A total of 60 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 3. ! A total of 1288 telescope corrections were flagged in sub-array 1. ! A total of 60 telescope corrections were flagged in sub-array 2. ! ! Correcting IF 4. ! A total of 1288 telescope corrections were flagged in sub-array 1. ! A total of 60 telescope corrections were flagged in sub-array 2. ! ! Fit before self-cal, rms=1.032725Jy sigma=14.493337 ! Fit after self-cal, rms=0.763184Jy sigma=10.575499 ! 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 13% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1767 milli-arcsec ! Estimated beam: bmin=0.5388 mas, bmaj=0.9079 mas, bpa=-3.053 degrees ! Estimated noise=0.909916 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 = 0.199063 Jy ! Component: 100 - total flux cleaned = 0.246189 Jy ! Total flux subtracted in 100 components = 0.246189 Jy ! Clean residual min=-0.006933 max=0.016956 Jy/beam ! Clean residual mean=0.000012 rms=0.001481 Jy/beam ! Combined flux in latest and established models = 0.246188 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 0.246188 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.093445Jy sigma=1.031108 ! Fit after self-cal, rms=0.093545Jy sigma=1.030643 ! Inverting map ! Your choice of large map pixels excluded 13% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1767 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0163436 Jy ! Component: 100 - total flux cleaned = 0.0235627 Jy ! Total flux subtracted in 100 components = 0.0235627 Jy ! Clean residual min=-0.005748 max=0.010745 Jy/beam ! Clean residual mean=0.000005 rms=0.001183 Jy/beam ! Combined flux in latest and established models = 0.269751 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 12 components and 0.269751 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.090281Jy sigma=0.971192 ! Fit after self-cal, rms=0.090305Jy sigma=0.970593 ! Inverting map ! Your choice of large map pixels excluded 13% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1767 milli-arcsec ! Added new window around map position (0.4, -1.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00773719 Jy ! Component: 100 - total flux cleaned = 0.00859714 Jy ! Total flux subtracted in 100 components = 0.00859714 Jy ! Clean residual min=-0.004829 max=0.006521 Jy/beam ! Clean residual mean=0.000002 rms=0.001076 Jy/beam ! Combined flux in latest and established models = 0.278348 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 19 components and 0.278348 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.089270Jy sigma=0.956334 ! Fit after self-cal, rms=0.089072Jy sigma=0.955074 ! Inverting map ! Your choice of large map pixels excluded 13% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1767 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 13% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1767 milli-arcsec ! Estimated beam: bmin=0.5961 mas, bmaj=0.9508 mas, bpa=-3.935 degrees ! Estimated noise=0.604262 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 (0.4, -3). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0072498 Jy ! Component: 100 - total flux cleaned = 0.010588 Jy ! Component: 150 - total flux cleaned = 0.011017 Jy ! Component: 200 - total flux cleaned = 0.0113042 Jy ! Total flux subtracted in 200 components = 0.0113042 Jy ! Clean residual min=-0.003215 max=0.004499 Jy/beam ! Clean residual mean=-0.000001 rms=0.000789 Jy/beam ! Combined flux in latest and established models = 0.289653 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 29 components and 0.289653 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.088424Jy sigma=0.944200 ! Fit after self-cal, rms=0.088323Jy sigma=0.942756 ! Inverting map ! Your choice of large map pixels excluded 13% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1767 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5961 x 0.9508 at -3.935 degrees (North through East) ! Clean map min=-0.0026632 max=0.24875 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 141 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 1.00 HH 1.00 HN 1.00 ! KP 0.95 LA 1.02 NL 0.99 NY 1.02 ! PT 1.02 SC 0.99 WZ 1.01 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.07 FD 1.10 KP 1.07 LA 1.00 ! MK 1.03 NL 0.98 OV 0.99 PT 0.97 ! ! ! Correcting IF 2. ! A total of 141 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 0.99 HH 0.98 HN 1.01 ! KP 0.98 LA 1.00 NL 1.00 NY 1.01 ! PT 1.01 SC 0.97 WZ 0.98 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 1.08 KP 1.01 LA 0.93 ! MK 1.06 NL 1.02 OV 1.03 PT 1.00 ! ! ! Correcting IF 3. ! A total of 141 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.05 FD 0.99 HH 1.07 HN 1.04 ! KP 0.97 LA 0.99 NL 0.97 NY 1.02 ! PT 1.02 SC 0.96 WZ 0.96 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 1.09 KP 1.03 LA 0.98 ! MK 1.04 NL 1.00 OV 1.01 PT 1.00 ! ! ! Correcting IF 4. ! A total of 141 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 0.96 HH 1.25 HN 1.02 ! KP 0.95 LA 0.98 NL 0.99 NY 1.01 ! PT 1.03 SC 0.94 WZ 0.97 ! ! A total of 12 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 1.01 KP 0.98 LA 0.97 ! MK 0.98 NL 1.09 OV 1.04 PT 0.99 ! ! ! Fit before self-cal, rms=0.088323Jy sigma=0.942756 ! Fit after self-cal, rms=0.088793Jy sigma=0.927710 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 11.5% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1775 milli-arcsec ! Estimated beam: bmin=0.576 mas, bmaj=1.055 mas, bpa=-5 degrees ! Estimated noise=0.62218 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 = 0.00129229 Jy ! Component: 100 - total flux cleaned = 0.00177755 Jy ! Component: 150 - total flux cleaned = 0.00211962 Jy ! Component: 200 - total flux cleaned = 0.00218161 Jy ! Total flux subtracted in 200 components = 0.00218161 Jy ! Clean residual min=-0.003128 max=0.003039 Jy/beam ! Clean residual mean=-0.000004 rms=0.000656 Jy/beam ! Combined flux in latest and established models = 0.291834 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 38 components and 0.291834 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.088563Jy sigma=0.925212 ! Fit after self-cal, rms=0.088617Jy sigma=0.924972 ! Inverting map ! Your choice of large map pixels excluded 11.5% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1775 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=0.088617Jy sigma=0.924972 ! Fit after self-cal, rms=0.089986Jy sigma=0.918460 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 11.5% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1775 milli-arcsec ! Estimated beam: bmin=0.5757 mas, bmaj=1.055 mas, bpa=-5.11 degrees ! Estimated noise=0.622683 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000404765 Jy ! Component: 100 - total flux cleaned = 0.000554007 Jy ! Component: 150 - total flux cleaned = 0.00064031 Jy ! Component: 200 - total flux cleaned = 0.000718921 Jy ! Total flux subtracted in 200 components = 0.000718921 Jy ! Clean residual min=-0.002840 max=0.002588 Jy/beam ! Clean residual mean=-0.000001 rms=0.000573 Jy/beam ! Combined flux in latest and established models = 0.292553 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 46 components and 0.292553 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.089888Jy sigma=0.917684 ! Fit after self-cal, rms=0.089949Jy sigma=0.917562 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 11.5% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1775 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 = -0.000232282 Jy ! Component: 100 - total flux cleaned = -0.000119205 Jy ! Component: 150 - total flux cleaned = -8.33848e-05 Jy ! Component: 200 - total flux cleaned = -5.10867e-05 Jy ! Total flux subtracted in 200 components = -5.10867e-05 Jy ! Clean residual min=-0.002831 max=0.002492 Jy/beam ! Clean residual mean=-0.000001 rms=0.000569 Jy/beam ! Combined flux in latest and established models = 0.292502 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 52 components and 0.292502 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.089893Jy sigma=0.917184 ! Fit after self-cal, rms=0.089884Jy sigma=0.917141 ! Inverting map ! Your choice of large map pixels excluded 11.5% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1775 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=0.089884Jy sigma=0.917141 ! Fit after self-cal, rms=0.090253Jy sigma=0.915423 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 11.5% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1775 milli-arcsec ! Estimated beam: bmin=0.5754 mas, bmaj=1.054 mas, bpa=-5.102 degrees ! Estimated noise=0.622627 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000310591 Jy ! Component: 100 - total flux cleaned = 0.000308417 Jy ! Component: 150 - total flux cleaned = 0.000308642 Jy ! Component: 200 - total flux cleaned = 0.000336964 Jy ! Total flux subtracted in 200 components = 0.000336964 Jy ! Clean residual min=-0.002792 max=0.002363 Jy/beam ! Clean residual mean=0.000001 rms=0.000552 Jy/beam ! Combined flux in latest and established models = 0.292839 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 53 components and 0.292839 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.090201Jy sigma=0.915101 ! Fit after self-cal, rms=0.090203Jy sigma=0.915064 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 11.5% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1775 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 = -0.000122348 Jy ! Component: 100 - total flux cleaned = -0.000123576 Jy ! Component: 150 - total flux cleaned = -0.000123892 Jy ! Component: 200 - total flux cleaned = -9.69384e-05 Jy ! Total flux subtracted in 200 components = -9.69384e-05 Jy ! Clean residual min=-0.002788 max=0.002293 Jy/beam ! Clean residual mean=0.000001 rms=0.000550 Jy/beam ! Combined flux in latest and established models = 0.292742 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 55 components and 0.292742 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.090176Jy sigma=0.914882 ! Fit after self-cal, rms=0.090169Jy sigma=0.914864 ! Inverting map ! Your choice of large map pixels excluded 11.5% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1775 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=0.090169Jy sigma=0.914864 ! Fit after self-cal, rms=0.090147Jy sigma=0.914802 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 11.5% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1775 milli-arcsec ! Estimated beam: bmin=2.549 mas, bmaj=2.637 mas, bpa=-62.16 degrees ! Estimated noise=0.886884 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000544676 Jy ! Component: 100 - total flux cleaned = 0.000681019 Jy ! Component: 150 - total flux cleaned = 0.000766367 Jy ! Component: 200 - total flux cleaned = 0.000817569 Jy ! Total flux subtracted in 200 components = 0.000817569 Jy ! Clean residual min=-0.002985 max=0.003376 Jy/beam ! Clean residual mean=0.000002 rms=0.000799 Jy/beam ! Combined flux in latest and established models = 0.29356 Jy selfcal ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 61 components and 0.29356 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.090144Jy sigma=0.914946 ! Fit after self-cal, rms=0.090144Jy sigma=0.914905 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 11.5% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1775 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 = 0.00014387 Jy ! Component: 100 - total flux cleaned = 0.000212958 Jy ! Component: 150 - total flux cleaned = 0.000241984 Jy ! Component: 200 - total flux cleaned = 0.000255076 Jy ! Total flux subtracted in 200 components = 0.000255076 Jy ! Clean residual min=-0.002972 max=0.003384 Jy/beam ! Clean residual mean=0.000002 rms=0.000794 Jy/beam ! Combined flux in latest and established models = 0.293815 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 64 components and 0.293815 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.090145Jy sigma=0.915071 ! Fit after self-cal, rms=0.090146Jy sigma=0.915062 ! Inverting map ! Your choice of large map pixels excluded 11.5% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1775 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 11.5% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1775 milli-arcsec ! Estimated beam: bmin=0.5752 mas, bmaj=1.053 mas, bpa=-5.08 degrees ! Estimated noise=0.622545 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5752 x 1.053 at -5.08 degrees (North through East) ! Clean map min=-0.0023455 max=0.24985 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 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 11.5% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1775 milli-arcsec ! Estimated beam: bmin=0.5221 mas, bmaj=0.9538 mas, bpa=-3.828 degrees ! Estimated noise=0.937795 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.198898 Jy ! Component: 100 - total flux cleaned = 0.246799 Jy ! Component: 150 - total flux cleaned = 0.266102 Jy ! Component: 200 - total flux cleaned = 0.276488 Jy ! Total flux subtracted in 200 components = 0.276488 Jy ! Clean residual min=-0.004512 max=0.005303 Jy/beam ! Clean residual mean=0.000003 rms=0.000951 Jy/beam ! Combined flux in latest and established models = 0.276488 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 0.276488 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 11.5% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1775 milli-arcsec ! Estimated beam: bmin=0.5752 mas, bmaj=1.053 mas, bpa=-5.08 degrees ! Estimated noise=0.622545 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 = 0.00726607 Jy ! Component: 100 - total flux cleaned = 0.0117443 Jy ! Component: 150 - total flux cleaned = 0.0134961 Jy ! Component: 200 - total flux cleaned = 0.0144575 Jy ! Total flux subtracted in 200 components = 0.0144575 Jy ! Clean residual min=-0.002993 max=0.002521 Jy/beam ! Clean residual mean=0.000003 rms=0.000582 Jy/beam ! Combined flux in latest and established models = 0.290945 Jy ! Adding 15 model components to the UV plane model. ! The established model now contains 20 components and 0.290945 Jy ! Inverting map ! Your choice of large map pixels excluded 11.5% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1775 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 11.5% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1775 milli-arcsec ! Estimated beam: bmin=2.549 mas, bmaj=2.637 mas, bpa=-62.16 degrees ! Estimated noise=0.886884 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00213948 Jy ! Component: 100 - total flux cleaned = 0.00289399 Jy ! Component: 150 - total flux cleaned = 0.00304311 Jy ! Component: 200 - total flux cleaned = 0.00316338 Jy ! Total flux subtracted in 200 components = 0.00316338 Jy ! Clean residual min=-0.002988 max=0.003393 Jy/beam ! Clean residual mean=0.000001 rms=0.000792 Jy/beam ! Combined flux in latest and established models = 0.294109 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) ! Added new window around map position (-34.8, -49.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00318931 Jy ! Component: 100 - total flux cleaned = 0.00470525 Jy ! Component: 150 - total flux cleaned = 0.00515593 Jy ! Component: 200 - total flux cleaned = 0.00550993 Jy ! Total flux subtracted in 200 components = 0.00550993 Jy ! Clean residual min=-0.002812 max=0.002210 Jy/beam ! Clean residual mean=0.000006 rms=0.000658 Jy/beam ! Combined flux in latest and established models = 0.299619 Jy ! Adding 31 model components to the UV plane model. ! The established model now contains 50 components and 0.299619 Jy ! Inverting map ! Your choice of large map pixels excluded 11.5% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1775 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 11.5% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1775 milli-arcsec ! Estimated beam: bmin=0.5752 mas, bmaj=1.053 mas, bpa=-5.08 degrees ! Estimated noise=0.622545 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -2.74175e-05 Jy ! Component: 100 - total flux cleaned = 0.000369178 Jy ! Component: 150 - total flux cleaned = 0.000550133 Jy ! Component: 200 - total flux cleaned = 0.000719632 Jy ! Total flux subtracted in 200 components = 0.000719632 Jy ! Clean residual min=-0.002716 max=0.002363 Jy/beam ! Clean residual mean=0.000000 rms=0.000530 Jy/beam ! Combined flux in latest and established models = 0.300338 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 64 components and 0.300338 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.090305Jy sigma=0.914960 ! Fit after self-cal, rms=0.090197Jy sigma=0.914514 wmodel J2145+1115_X_map.mod ! Writing 64 model components to file: J2145+1115_X_map.mod wobs J2145+1115_X_uvs.fits ! Writing UV FITS file: J2145+1115_X_uvs.fits wwins J2145+1115_X_map.win ! wwins: Wrote 4 windows to J2145+1115_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 11.5% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1775 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000669672 Jy ! Component: 100 - total flux cleaned = -0.00121737 Jy ! Component: 150 - total flux cleaned = -0.00197263 Jy ! Component: 200 - total flux cleaned = -0.00235489 Jy ! Component: 250 - total flux cleaned = -0.0027245 Jy ! Component: 300 - total flux cleaned = -0.00312087 Jy ! Component: 350 - total flux cleaned = -0.00329751 Jy ! Component: 400 - total flux cleaned = -0.00354058 Jy ! Component: 450 - total flux cleaned = -0.00371095 Jy ! Component: 500 - total flux cleaned = -0.00367678 Jy ! Component: 550 - total flux cleaned = -0.0035772 Jy ! Component: 600 - total flux cleaned = -0.00357728 Jy ! Component: 650 - total flux cleaned = -0.0036099 Jy ! Component: 700 - total flux cleaned = -0.00360995 Jy ! Component: 750 - total flux cleaned = -0.00354725 Jy ! Component: 800 - total flux cleaned = -0.00354712 Jy ! Component: 850 - total flux cleaned = -0.00351595 Jy ! Component: 900 - total flux cleaned = -0.00339475 Jy ! Component: 950 - total flux cleaned = -0.00345473 Jy ! Component: 1000 - total flux cleaned = -0.00336594 Jy ! Component: 1050 - total flux cleaned = -0.00333678 Jy ! Component: 1100 - total flux cleaned = -0.00339438 Jy ! Component: 1150 - total flux cleaned = -0.00333643 Jy ! Component: 1200 - total flux cleaned = -0.00342238 Jy ! Component: 1250 - total flux cleaned = -0.00342197 Jy ! Component: 1300 - total flux cleaned = -0.00347826 Jy ! Component: 1350 - total flux cleaned = -0.00364562 Jy ! Component: 1400 - total flux cleaned = -0.00367339 Jy ! Component: 1450 - total flux cleaned = -0.00386467 Jy ! Component: 1500 - total flux cleaned = -0.0039192 Jy ! Component: 1550 - total flux cleaned = -0.004027 Jy ! Component: 1600 - total flux cleaned = -0.00424105 Jy ! Component: 1650 - total flux cleaned = -0.00434732 Jy ! Component: 1700 - total flux cleaned = -0.00434742 Jy ! Component: 1750 - total flux cleaned = -0.00458313 Jy ! Component: 1800 - total flux cleaned = -0.004531 Jy ! Component: 1850 - total flux cleaned = -0.00466041 Jy ! Component: 1900 - total flux cleaned = -0.00486577 Jy ! Component: 1950 - total flux cleaned = -0.00491678 Jy ! Component: 2000 - total flux cleaned = -0.00504346 Jy ! Component: 2050 - total flux cleaned = -0.00501849 Jy ! Component: 2100 - total flux cleaned = -0.00514335 Jy ! Component: 2150 - total flux cleaned = -0.00529225 Jy ! Component: 2200 - total flux cleaned = -0.00539112 Jy ! Component: 2250 - total flux cleaned = -0.0054645 Jy ! Component: 2300 - total flux cleaned = -0.00546447 Jy ! Component: 2350 - total flux cleaned = -0.00536765 Jy ! Component: 2400 - total flux cleaned = -0.00556001 Jy ! Component: 2450 - total flux cleaned = -0.00556007 Jy ! Component: 2500 - total flux cleaned = -0.0054889 Jy ! Component: 2550 - total flux cleaned = -0.0056073 Jy ! Component: 2600 - total flux cleaned = -0.00558355 Jy ! Component: 2650 - total flux cleaned = -0.00551347 Jy ! Component: 2700 - total flux cleaned = -0.00549012 Jy ! Component: 2750 - total flux cleaned = -0.00562902 Jy ! Component: 2800 - total flux cleaned = -0.00553699 Jy ! Component: 2850 - total flux cleaned = -0.00560565 Jy ! Component: 2900 - total flux cleaned = -0.00558299 Jy ! Component: 2950 - total flux cleaned = -0.00562805 Jy ! Component: 3000 - total flux cleaned = -0.00556036 Jy ! Component: 3050 - total flux cleaned = -0.00564999 Jy ! Component: 3100 - total flux cleaned = -0.00565 Jy ! Component: 3150 - total flux cleaned = -0.00569424 Jy ! Component: 3200 - total flux cleaned = -0.00567236 Jy ! Component: 3250 - total flux cleaned = -0.00562836 Jy ! Component: 3300 - total flux cleaned = -0.00569383 Jy ! Component: 3350 - total flux cleaned = -0.00567226 Jy ! Component: 3400 - total flux cleaned = -0.0057372 Jy ! Component: 3450 - total flux cleaned = -0.00569422 Jy ! Component: 3500 - total flux cleaned = -0.0056728 Jy ! Component: 3550 - total flux cleaned = -0.0057366 Jy ! Component: 3600 - total flux cleaned = -0.00573668 Jy ! Component: 3650 - total flux cleaned = -0.00573678 Jy ! Component: 3700 - total flux cleaned = -0.00582073 Jy ! Component: 3750 - total flux cleaned = -0.00588355 Jy ! Component: 3800 - total flux cleaned = -0.00584184 Jy ! Component: 3850 - total flux cleaned = -0.00588339 Jy ! Component: 3900 - total flux cleaned = -0.00588336 Jy ! Component: 3950 - total flux cleaned = -0.00594481 Jy ! Component: 4000 - total flux cleaned = -0.00602643 Jy ! Component: 4050 - total flux cleaned = -0.00596536 Jy ! Total flux subtracted in 4096 components = -0.00602629 Jy ! Clean residual min=-0.001085 max=0.001382 Jy/beam ! Clean residual mean=-0.000001 rms=0.000326 Jy/beam ! Combined flux in latest and established models = 0.294312 Jy keep ! Adding 334 model components to the UV plane model. ! The established model now contains 398 components and 0.294312 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv119_uvs/J2145+1115_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 11.5% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1775 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5752 x 1.053 at -5.08 degrees (North through East) ! Clean map min=-0.0019128 max=0.2496 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv119_uvs/J2145+1115_X_map.fits wmodel /scr/pima/rv119_uvs/J2145+1115_X_map.mod ! Writing 398 model components to file: /scr/pima/rv119_uvs/J2145+1115_X_map.mod wobs /scr/pima/rv119_uvs/J2145+1115_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv119_uvs/J2145+1115_X_uvs.fits wwins /scr/pima/rv119_uvs/J2145+1115_X_map.win ! wwins: Wrote 5 windows to /scr/pima/rv119_uvs/J2145+1115_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.249605 invert ! Inverting map ! Your choice of large map pixels excluded 11.5% of the data. ! The x-axis pixel size should ideally be below 0.1681 milli-arcsec ! The y-axis pixel size should ideally be below 0.1775 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000324744 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.39031 0.39031 0.780619 1.56124 3.12248 6.24495 12.4899 24.9798 49.9596 99.9193 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0009 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.249 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 768.62 quit ! Quitting program ! Log file /scr/pima/rv119_uvs/J2145+1115_X_dfm.log closed on Sun Dec 17 11:38:18 2017