! Started logfile: /scr/pima/bg219b_uvs/J1046+5354_S_dfm.log on Thu May 19 20:13:58 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/J1046+5354_S_uva.fits ! Reading UV FITS file: /scr/pima/bg219b_uvs/J1046+5354_S_uva.fits ! AN table 1: 48 integrations on 36 of 36 possible baselines. ! Apparent sampling: 0.807292 visibilities/baseline/integration-bin. ! Found source: J1046+5354 ! ! 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 5580 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 J1046+5354_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 25 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 25 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 25 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 25 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=1.032819Jy sigma=23.647267 ! Fit after self-cal, rms=0.796247Jy sigma=18.227120 ! 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=3.789 mas, bmaj=5.164 mas, bpa=30.31 degrees ! Estimated noise=0.688787 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 = 0.159573 Jy ! Component: 100 - total flux cleaned = 0.194389 Jy ! Total flux subtracted in 100 components = 0.194389 Jy ! Clean residual min=-0.005964 max=0.009885 Jy/beam ! Clean residual mean=0.000042 rms=0.001814 Jy/beam ! Combined flux in latest and established models = 0.194389 Jy ! Performing phase self-cal ! Adding 2 model components to the UV plane model. ! The established model now contains 2 components and 0.194389 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.063662Jy sigma=1.401837 ! Fit after self-cal, rms=0.063653Jy sigma=1.401697 ! 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=4.604 mas, bmaj=6.126 mas, bpa=25.07 degrees ! Estimated noise=0.424528 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 = 0.011967 Jy ! Component: 100 - total flux cleaned = 0.0169481 Jy ! Component: 150 - total flux cleaned = 0.0178583 Jy ! Component: 200 - total flux cleaned = 0.0178642 Jy ! Total flux subtracted in 200 components = 0.0178642 Jy ! Clean residual min=-0.005134 max=0.008043 Jy/beam ! Clean residual mean=0.000063 rms=0.001684 Jy/beam ! Combined flux in latest and established models = 0.212253 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 19 components and 0.212253 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.061653Jy sigma=1.354340 ! Fit after self-cal, rms=0.061575Jy sigma=1.352760 ! Inverting map print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 4.604 x 6.126 at 25.07 degrees (North through East) ! Clean map min=-0.0049422 max=0.20551 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=0.061575Jy sigma=1.352760 ! Fit after self-cal, rms=0.061575Jy sigma=1.352760 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=4.604 mas, bmaj=6.126 mas, bpa=25.07 degrees ! Estimated noise=0.424528 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 = 0.000537063 Jy ! Component: 100 - total flux cleaned = 0.000336616 Jy ! Component: 150 - total flux cleaned = 0.000253416 Jy ! Component: 200 - total flux cleaned = 0.000147518 Jy ! Total flux subtracted in 200 components = 0.000147518 Jy ! Clean residual min=-0.005082 max=0.007893 Jy/beam ! Clean residual mean=0.000063 rms=0.001664 Jy/beam ! Combined flux in latest and established models = 0.2124 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 27 components and 0.2124 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.061491Jy sigma=1.350790 ! Fit after self-cal, rms=0.061477Jy sigma=1.350558 ! 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=0.061477Jy sigma=1.350558 ! Fit after self-cal, rms=0.060508Jy sigma=1.340481 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=4.619 mas, bmaj=6.126 mas, bpa=24.5 degrees ! Estimated noise=0.419465 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00238277 Jy ! Component: 100 - total flux cleaned = -0.0033655 Jy ! Component: 150 - total flux cleaned = -0.00363315 Jy ! Component: 200 - total flux cleaned = -0.00384158 Jy ! Total flux subtracted in 200 components = -0.00384158 Jy ! Clean residual min=-0.004787 max=0.007579 Jy/beam ! Clean residual mean=0.000063 rms=0.001560 Jy/beam ! Combined flux in latest and established models = 0.208559 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 38 components and 0.208559 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.060422Jy sigma=1.338126 ! Fit after self-cal, rms=0.060418Jy sigma=1.337995 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 (-65.5, -66.5). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00636451 Jy ! Component: 100 - total flux cleaned = 0.00906756 Jy ! Component: 150 - total flux cleaned = 0.0102788 Jy ! Component: 200 - total flux cleaned = 0.0110367 Jy ! Total flux subtracted in 200 components = 0.0110367 Jy ! Clean residual min=-0.004941 max=0.005529 Jy/beam ! Clean residual mean=0.000050 rms=0.001391 Jy/beam ! Combined flux in latest and established models = 0.219595 Jy ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 67 components and 0.219595 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.059732Jy sigma=1.321884 ! Fit after self-cal, rms=0.059636Jy sigma=1.320120 ! 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=0.059636Jy sigma=1.320120 ! Fit after self-cal, rms=0.059426Jy sigma=1.318552 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=4.625 mas, bmaj=6.126 mas, bpa=24.24 degrees ! Estimated noise=0.41711 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000618074 Jy ! Component: 100 - total flux cleaned = 0.000812929 Jy ! Component: 150 - total flux cleaned = 0.00109034 Jy ! Component: 200 - total flux cleaned = 0.00143974 Jy ! Total flux subtracted in 200 components = 0.00143974 Jy ! Clean residual min=-0.004907 max=0.005098 Jy/beam ! Clean residual mean=0.000046 rms=0.001300 Jy/beam ! Combined flux in latest and established models = 0.221035 Jy selfcal ! Performing phase self-cal ! Adding 27 model components to the UV plane model. ! The established model now contains 80 components and 0.221035 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.059268Jy sigma=1.314711 ! Fit after self-cal, rms=0.059256Jy sigma=1.314453 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 = 0.00073818 Jy ! Component: 100 - total flux cleaned = 0.00100493 Jy ! Component: 150 - total flux cleaned = 0.00128135 Jy ! Component: 200 - total flux cleaned = 0.00145478 Jy ! Total flux subtracted in 200 components = 0.00145478 Jy ! Clean residual min=-0.004992 max=0.005041 Jy/beam ! Clean residual mean=0.000044 rms=0.001282 Jy/beam ! Combined flux in latest and established models = 0.22249 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 86 components and 0.22249 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.059201Jy sigma=1.313254 ! Fit after self-cal, rms=0.059196Jy sigma=1.313173 ! 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=0.059196Jy sigma=1.313173 ! Fit after self-cal, rms=0.058509Jy sigma=1.303291 clean clean_niter,clean_gain ! Inverting map and beam ! Estimated beam: bmin=7.926 mas, bmaj=9.01 mas, bpa=11.33 degrees ! Estimated noise=0.485435 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0010774 Jy ! Component: 100 - total flux cleaned = -0.00117079 Jy ! Component: 150 - total flux cleaned = -0.00113514 Jy ! Component: 200 - total flux cleaned = -0.00103802 Jy ! Total flux subtracted in 200 components = -0.00103802 Jy ! Clean residual min=-0.005789 max=0.006853 Jy/beam ! Clean residual mean=0.000058 rms=0.001716 Jy/beam ! Combined flux in latest and established models = 0.221452 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 100 components and 0.221452 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.058466Jy sigma=1.302294 ! Fit after self-cal, rms=0.058460Jy sigma=1.302094 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 = -0.000193287 Jy ! Component: 100 - total flux cleaned = -0.000134481 Jy ! Component: 150 - total flux cleaned = -5.22737e-05 Jy ! Component: 200 - total flux cleaned = -1.58531e-06 Jy ! Total flux subtracted in 200 components = -1.58531e-06 Jy ! Clean residual min=-0.005832 max=0.006740 Jy/beam ! Clean residual mean=0.000058 rms=0.001715 Jy/beam ! Combined flux in latest and established models = 0.22145 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 109 components and 0.22145 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.058444Jy sigma=1.301711 ! Fit after self-cal, rms=0.058441Jy sigma=1.301647 ! 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=4.613 mas, bmaj=6.112 mas, bpa=24.23 degrees ! Estimated noise=0.415377 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 4.613 x 6.112 at 24.23 degrees (North through East) ! Clean map min=-0.0038264 max=0.20057 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=3.796 mas, bmaj=5.138 mas, bpa=29.49 degrees ! Estimated noise=0.67427 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.156143 Jy ! Component: 100 - total flux cleaned = 0.190209 Jy ! Component: 150 - total flux cleaned = 0.201598 Jy ! Component: 200 - total flux cleaned = 0.208555 Jy ! Total flux subtracted in 200 components = 0.208555 Jy ! Clean residual min=-0.004497 max=0.005504 Jy/beam ! Clean residual mean=0.000032 rms=0.001242 Jy/beam ! Combined flux in latest and established models = 0.208555 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 16 model components to the UV plane model. ! The established model now contains 16 components and 0.208555 Jy ! Inverting map and beam ! Estimated beam: bmin=4.613 mas, bmaj=6.112 mas, bpa=24.23 degrees ! Estimated noise=0.415377 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 (123.5, -71.5). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00640894 Jy ! Component: 100 - total flux cleaned = 0.0103824 Jy ! Component: 150 - total flux cleaned = 0.0121895 Jy ! Component: 200 - total flux cleaned = 0.01339 Jy ! Total flux subtracted in 200 components = 0.01339 Jy ! Clean residual min=-0.004078 max=0.004046 Jy/beam ! Clean residual mean=0.000036 rms=0.001088 Jy/beam ! Combined flux in latest and established models = 0.221945 Jy ! Adding 39 model components to the UV plane model. ! The established model now contains 53 components and 0.221945 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=7.926 mas, bmaj=9.01 mas, bpa=11.33 degrees ! Estimated noise=0.485435 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00329951 Jy ! Component: 100 - total flux cleaned = 0.00511953 Jy ! Component: 150 - total flux cleaned = 0.00575969 Jy ! Component: 200 - total flux cleaned = 0.00624845 Jy ! Total flux subtracted in 200 components = 0.00624845 Jy ! Clean residual min=-0.005756 max=0.005185 Jy/beam ! Clean residual mean=0.000070 rms=0.001549 Jy/beam ! Combined flux in latest and established models = 0.228194 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 = 0.000318417 Jy ! Component: 100 - total flux cleaned = 0.000509206 Jy ! Component: 150 - total flux cleaned = 0.000682466 Jy ! Component: 200 - total flux cleaned = 0.000841705 Jy ! Total flux subtracted in 200 components = 0.000841705 Jy ! Clean residual min=-0.005801 max=0.004912 Jy/beam ! Clean residual mean=0.000070 rms=0.001529 Jy/beam ! Combined flux in latest and established models = 0.229035 Jy ! Adding 60 model components to the UV plane model. ! The established model now contains 99 components and 0.229035 Jy ! Inverting map uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Estimated beam: bmin=4.613 mas, bmaj=6.112 mas, bpa=24.23 degrees ! Estimated noise=0.415377 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000649623 Jy ! Component: 100 - total flux cleaned = 0.000785257 Jy ! Component: 150 - total flux cleaned = 0.000788667 Jy ! Component: 200 - total flux cleaned = 0.000789859 Jy ! Total flux subtracted in 200 components = 0.000789859 Jy ! Clean residual min=-0.004073 max=0.003546 Jy/beam ! Clean residual mean=0.000033 rms=0.000993 Jy/beam ! Combined flux in latest and established models = 0.229825 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 117 components and 0.229825 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.058255Jy sigma=1.296353 ! Fit after self-cal, rms=0.058201Jy sigma=1.295119 wmodel /J1046+5354_S_map.mod ! wmodel: Unable to open new model file: /J1046+5354_S_map.mod ! Error occured in command: wmodel ![Exited script file: /opt64/bin/pima_mupet_01.dfm] ! wmap /scr/pima/bg219b_uvs/J1046+5354_S_map.fits ! Inverting map ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 4.613 x 6.112 at 24.23 degrees (North through East) ! Clean map min=-0.0039056 max=0.19907 Jy/beam ! Writing clean map to FITS file: /scr/pima/bg219b_uvs/J1046+5354_S_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 0.199067 invert ! Inverting map float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000980614 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -1.47781 1.47781 2.95562 5.91124 11.8225 23.645 47.29 94.5799 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0029 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.199 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 203.002 quit ! Quitting program ! Log file /scr/pima/bg219b_uvs/J1046+5354_S_dfm.log closed on Thu May 19 20:14:01 2016