! Started logfile: /scr/pima/bg219b_uvs/J1041+523A_S_dfm.log on Thu May 19 20:13:36 2016 float field_size field_size = 1024 float field_cell field_cell = 0.5000 float taper_size taper_size = 20.0 float freq freq = 2.22000 obs /scr/pima/bg219b_uvs/J1041+523A_S_uva.fits ! Reading UV FITS file: /scr/pima/bg219b_uvs/J1041+523A_S_uva.fits ! AN table 1: 26 integrations on 36 of 36 possible baselines. ! Apparent sampling: 0.653846 visibilities/baseline/integration-bin. ! Found source: J1041+523A ! ! 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 2.22e+09 3.2e+07 1 3.2e+07 ! 02 2 2.252e+09 3.2e+07 1 3.2e+07 ! 03 3 2.284e+09 3.2e+07 1 3.2e+07 ! 04 4 2.348e+09 3.2e+07 1 3.2e+07 ! ! Polarization(s): RR ! ! Read 54 lines of history. ! ! Reading 2448 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 = 0.5 print "taper_size =", taper_size ! taper_size = 20 ![@/opt64/bin/pima_mupet_01.dfm J1041+523A_S] 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 0.500x0.500 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 60 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 60 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 60 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 60 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=1.114851Jy sigma=23.147790 ! Fit after self-cal, rms=0.536251Jy sigma=11.084976 ! 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 ! Estimated beam: bmin=3.821 mas, bmaj=5.454 mas, bpa=27.54 degrees ! Estimated noise=1.03666 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 = 0.366135 Jy ! Component: 100 - total flux cleaned = 0.445986 Jy ! Total flux subtracted in 100 components = 0.445986 Jy ! Clean residual min=-0.012880 max=0.022335 Jy/beam ! Clean residual mean=0.000093 rms=0.003853 Jy/beam ! Combined flux in latest and established models = 0.445986 Jy ! Performing phase self-cal ! Adding 2 model components to the UV plane model. ! The established model now contains 2 components and 0.445986 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.081022Jy sigma=1.651057 ! Fit after self-cal, rms=0.081016Jy sigma=1.650974 ! Inverting map 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 ! Estimated beam: bmin=4.902 mas, bmaj=6.392 mas, bpa=32.65 degrees ! Estimated noise=0.745227 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 = 0.0210421 Jy ! Component: 100 - total flux cleaned = 0.0283589 Jy ! Component: 150 - total flux cleaned = 0.0296946 Jy ! Component: 200 - total flux cleaned = 0.0303364 Jy ! Total flux subtracted in 200 components = 0.0303364 Jy ! Clean residual min=-0.012136 max=0.019202 Jy/beam ! Clean residual mean=0.000354 rms=0.004283 Jy/beam ! Combined flux in latest and established models = 0.476322 Jy ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 27 components and 0.476322 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.075990Jy sigma=1.538626 ! Fit after self-cal, rms=0.075958Jy sigma=1.537878 ! Inverting map print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 4.902 x 6.392 at 32.65 degrees (North through East) ! Clean map min=-0.011537 max=0.46937 Jy/beam if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val ! Selfcal amplitude corrections will be limited to 0.833333 -> 1.2. ! Selfcal phase corrections will not be limited. gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* HN 1.00* KP 1.00* ! LA 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* HN 1.00* KP 1.00* ! LA 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* HN 1.00* KP 1.00* ! LA 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* HN 1.00* KP 1.00* ! LA 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ! ! ! Fit before self-cal, rms=0.075958Jy sigma=1.537878 ! Fit after self-cal, rms=0.075958Jy sigma=1.537878 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=4.902 mas, bmaj=6.392 mas, bpa=32.65 degrees ! Estimated noise=0.745227 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 = 0.000108507 Jy ! Component: 100 - total flux cleaned = 0.000218226 Jy ! Component: 150 - total flux cleaned = 0.000215518 Jy ! Component: 200 - total flux cleaned = 0.00013842 Jy ! Total flux subtracted in 200 components = 0.00013842 Jy ! Clean residual min=-0.011906 max=0.019138 Jy/beam ! Clean residual mean=0.000353 rms=0.004256 Jy/beam ! Combined flux in latest and established models = 0.476461 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 35 components and 0.476461 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.075707Jy sigma=1.532555 ! Fit after self-cal, rms=0.075697Jy sigma=1.532320 ! Inverting map 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=0.075697Jy sigma=1.532320 ! Fit after self-cal, rms=0.073116Jy sigma=1.487810 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=4.928 mas, bmaj=6.382 mas, bpa=32.02 degrees ! Estimated noise=0.732351 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00612275 Jy ! Component: 100 - total flux cleaned = -0.0077031 Jy ! Component: 150 - total flux cleaned = -0.00832785 Jy ! Component: 200 - total flux cleaned = -0.0088576 Jy ! Total flux subtracted in 200 components = -0.0088576 Jy ! Clean residual min=-0.010967 max=0.018951 Jy/beam ! Clean residual mean=0.000323 rms=0.003971 Jy/beam ! Combined flux in latest and established models = 0.467603 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 50 components and 0.467603 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.072632Jy sigma=1.477383 ! Fit after self-cal, rms=0.072629Jy sigma=1.477212 flux_cutoff = imstat(rms) * dynam ! Inverting map 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 (51, 25). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0165339 Jy ! Component: 100 - total flux cleaned = 0.0246732 Jy ! Component: 150 - total flux cleaned = 0.027887 Jy ! Component: 200 - total flux cleaned = 0.0287146 Jy ! Total flux subtracted in 200 components = 0.0287146 Jy ! Clean residual min=-0.010997 max=0.014156 Jy/beam ! Clean residual mean=0.000273 rms=0.003196 Jy/beam ! Combined flux in latest and established models = 0.496318 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 75 components and 0.496318 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.068140Jy sigma=1.392218 ! Fit after self-cal, rms=0.067463Jy sigma=1.377267 ! Inverting map 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=0.067463Jy sigma=1.377267 ! Fit after self-cal, rms=0.064096Jy sigma=1.309539 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=4.928 mas, bmaj=6.368 mas, bpa=31.59 degrees ! Estimated noise=0.730832 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0032092 Jy ! Component: 100 - total flux cleaned = -0.00392715 Jy ! Component: 150 - total flux cleaned = -0.00403186 Jy ! Component: 200 - total flux cleaned = -0.00403058 Jy ! Total flux subtracted in 200 components = -0.00403058 Jy ! Clean residual min=-0.007777 max=0.007684 Jy/beam ! Clean residual mean=0.000163 rms=0.002128 Jy/beam ! Combined flux in latest and established models = 0.492287 Jy selfcal ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 98 components and 0.492287 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.063639Jy sigma=1.300850 ! Fit after self-cal, rms=0.063621Jy sigma=1.300155 flux_cutoff = imstat(rms) * dynam ! Inverting map 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 = 0.000235005 Jy ! Component: 100 - total flux cleaned = 8.89074e-05 Jy ! Component: 150 - total flux cleaned = 8.88741e-05 Jy ! Component: 200 - total flux cleaned = 2.64696e-05 Jy ! Total flux subtracted in 200 components = 2.64696e-05 Jy ! Clean residual min=-0.007755 max=0.007385 Jy/beam ! Clean residual mean=0.000160 rms=0.002077 Jy/beam ! Combined flux in latest and established models = 0.492314 Jy ! Performing phase self-cal ! Adding 38 model components to the UV plane model. ! The established model now contains 118 components and 0.492314 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.063474Jy sigma=1.297180 ! Fit after self-cal, rms=0.063473Jy sigma=1.296926 ! Inverting map uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 20 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=0.063473Jy sigma=1.296926 ! Fit after self-cal, rms=0.061540Jy sigma=1.256674 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=8.734 mas, bmaj=8.948 mas, bpa=19.88 degrees ! Estimated noise=0.855486 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000958175 Jy ! Component: 100 - total flux cleaned = -0.00137625 Jy ! Component: 150 - total flux cleaned = -0.00137848 Jy ! Component: 200 - total flux cleaned = -0.00137898 Jy ! Total flux subtracted in 200 components = -0.00137898 Jy ! Clean residual min=-0.008898 max=0.008425 Jy/beam ! Clean residual mean=0.000206 rms=0.002488 Jy/beam ! Combined flux in latest and established models = 0.490935 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 131 components and 0.490935 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.061416Jy sigma=1.254145 ! Fit after self-cal, rms=0.061408Jy sigma=1.253892 flux_cutoff = imstat(rms) * dynam ! Inverting map 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 = -0.000153946 Jy ! Component: 100 - total flux cleaned = -0.000289862 Jy ! Component: 150 - total flux cleaned = -0.000413052 Jy ! Component: 200 - total flux cleaned = -0.000487817 Jy ! Total flux subtracted in 200 components = -0.000487817 Jy ! Clean residual min=-0.008804 max=0.008298 Jy/beam ! Clean residual mean=0.000210 rms=0.002463 Jy/beam ! Combined flux in latest and established models = 0.490447 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 141 components and 0.490447 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.061388Jy sigma=1.253545 ! Fit after self-cal, rms=0.061384Jy sigma=1.253473 ! Inverting map 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 ! Estimated beam: bmin=4.927 mas, bmaj=6.354 mas, bpa=31.16 degrees ! Estimated noise=0.731214 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 4.927 x 6.354 at 31.16 degrees (North through East) ! Clean map min=-0.0074807 max=0.45663 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 ! Estimated beam: bmin=3.843 mas, bmaj=5.433 mas, bpa=26.47 degrees ! Estimated noise=1.01046 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.356732 Jy ! Component: 100 - total flux cleaned = 0.43468 Jy ! Component: 150 - total flux cleaned = 0.45695 Jy ! Component: 200 - total flux cleaned = 0.468692 Jy ! Total flux subtracted in 200 components = 0.468692 Jy ! Clean residual min=-0.008622 max=0.009234 Jy/beam ! Clean residual mean=0.000041 rms=0.002071 Jy/beam ! Combined flux in latest and established models = 0.468693 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 18 model components to the UV plane model. ! The established model now contains 18 components and 0.468693 Jy ! Inverting map and beam ! Estimated beam: bmin=4.927 mas, bmaj=6.354 mas, bpa=31.16 degrees ! Estimated noise=0.731214 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) ! Added new window around map position (-72, -34). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0123906 Jy ! Component: 100 - total flux cleaned = 0.0173645 Jy ! Component: 150 - total flux cleaned = 0.0207197 Jy ! Component: 200 - total flux cleaned = 0.0230224 Jy ! Total flux subtracted in 200 components = 0.0230224 Jy ! Clean residual min=-0.008732 max=0.006987 Jy/beam ! Clean residual mean=0.000079 rms=0.001759 Jy/beam ! Combined flux in latest and established models = 0.491715 Jy ! Adding 43 model components to the UV plane model. ! The established model now contains 57 components and 0.491715 Jy ! Inverting map uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 20 mega-wavelengths. clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=8.734 mas, bmaj=8.948 mas, bpa=19.88 degrees ! Estimated noise=0.855486 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00183509 Jy ! Component: 100 - total flux cleaned = 0.00251362 Jy ! Component: 150 - total flux cleaned = 0.00304989 Jy ! Component: 200 - total flux cleaned = 0.00327802 Jy ! Total flux subtracted in 200 components = 0.00327802 Jy ! Clean residual min=-0.008419 max=0.007684 Jy/beam ! Clean residual mean=0.000095 rms=0.002197 Jy/beam ! Combined flux in latest and established models = 0.494993 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 = 0.000298741 Jy ! Component: 100 - total flux cleaned = 0.000382209 Jy ! Component: 150 - total flux cleaned = 0.000613147 Jy ! Component: 200 - total flux cleaned = 0.00095745 Jy ! Total flux subtracted in 200 components = 0.00095745 Jy ! Clean residual min=-0.008121 max=0.007542 Jy/beam ! Clean residual mean=0.000076 rms=0.002157 Jy/beam ! Combined flux in latest and established models = 0.49595 Jy ! Adding 75 model components to the UV plane model. ! The established model now contains 129 components and 0.49595 Jy ! Inverting map uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Estimated beam: bmin=4.927 mas, bmaj=6.354 mas, bpa=31.16 degrees ! Estimated noise=0.731214 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000103933 Jy ! Component: 100 - total flux cleaned = 0.000120862 Jy ! Component: 150 - total flux cleaned = 2.54047e-05 Jy ! Component: 200 - total flux cleaned = -0.000146614 Jy ! Total flux subtracted in 200 components = -0.000146614 Jy ! Clean residual min=-0.007102 max=0.005924 Jy/beam ! Clean residual mean=0.000034 rms=0.001534 Jy/beam ! Combined flux in latest and established models = 0.495804 Jy selfcal ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 151 components and 0.495804 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.060825Jy sigma=1.240823 ! Fit after self-cal, rms=0.060605Jy sigma=1.236257 wmodel /J1041+523A_S_map.mod ! wmodel: Unable to open new model file: /J1041+523A_S_map.mod ! Error occured in command: wmodel ![Exited script file: /opt64/bin/pima_mupet_01.dfm] ! wmap /scr/pima/bg219b_uvs/J1041+523A_S_map.fits ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 4.927 x 6.354 at 31.16 degrees (North through East) ! Clean map min=-0.0070499 max=0.45362 Jy/beam ! Writing clean map to FITS file: /scr/pima/bg219b_uvs/J1041+523A_S_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.453617 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00147261 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.973909 0.973909 1.94782 3.89564 7.79128 15.5826 31.1651 62.3302 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0044 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.453 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 308.036 quit ! Quitting program ! Log file /scr/pima/bg219b_uvs/J1041+523A_S_dfm.log closed on Thu May 19 20:13:38 2016