! Started logfile: /scr/pima/rv124_uvs/J1130+3815_X_dfm.log on Mon Dec 24 00:18:31 2018 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/rv124_uvs/J1130+3815_X_uva.fits ! Reading UV FITS file: /scr/pima/rv124_uvs/J1130+3815_X_uva.fits ! AN table 1: 71 integrations on 55 of 55 possible baselines. ! AN table 2: 68 integrations on 45 of 45 possible baselines. ! AN table 3: 8 integrations on 6 of 6 possible baselines. ! AN table 4: 47 integrations on 10 of 10 possible baselines. ! AN table 5: 6 integrations on 28 of 28 possible baselines. ! Apparent sampling: 0.29421 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1130+3815 ! ! 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 9004 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 J1130+3815_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 print "===============================================================" ! =============================================================== ! print "=== Difmap script: pima_mupet_01.dvm version of 2016.05.19 === " ! === Difmap script: pima_mupet_01.dvm version of 2016.05.19 === ! 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 517 telescope corrections were flagged in sub-array 1. ! A total of 420 telescope corrections were flagged in sub-array 2. ! A total of 9 telescope corrections were flagged in sub-array 3. ! A total of 117 telescope corrections were flagged in sub-array 4. ! A total of 21 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 517 telescope corrections were flagged in sub-array 1. ! A total of 420 telescope corrections were flagged in sub-array 2. ! A total of 9 telescope corrections were flagged in sub-array 3. ! A total of 117 telescope corrections were flagged in sub-array 4. ! A total of 21 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 575 telescope corrections were flagged in sub-array 1. ! A total of 420 telescope corrections were flagged in sub-array 2. ! A total of 20 telescope corrections were flagged in sub-array 3. ! A total of 157 telescope corrections were flagged in sub-array 4. ! A total of 25 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 575 telescope corrections were flagged in sub-array 1. ! A total of 420 telescope corrections were flagged in sub-array 2. ! A total of 20 telescope corrections were flagged in sub-array 3. ! A total of 157 telescope corrections were flagged in sub-array 4. ! A total of 25 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=1.509131Jy sigma=31.134111 ! Fit after self-cal, rms=0.383679Jy sigma=23.853856 ! 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 0.603% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec ! Estimated beam: bmin=0.5123 mas, bmaj=0.9601 mas, bpa=41.88 degrees ! Estimated noise=0.920146 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 = 0.759896 Jy ! Component: 100 - total flux cleaned = 1.0363 Jy ! Total flux subtracted in 100 components = 1.0363 Jy ! Clean residual min=-0.027194 max=0.111397 Jy/beam ! Clean residual mean=-0.000296 rms=0.006386 Jy/beam ! Combined flux in latest and established models = 1.0363 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 1.0363 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.295395Jy sigma=4.304678 ! Fit after self-cal, rms=0.286940Jy sigma=4.227872 ! Inverting map ! Your choice of large map pixels excluded 0.603% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.117382 Jy ! Component: 100 - total flux cleaned = 0.181942 Jy ! Total flux subtracted in 100 components = 0.181942 Jy ! Clean residual min=-0.018492 max=0.043769 Jy/beam ! Clean residual mean=-0.000272 rms=0.004231 Jy/beam ! Combined flux in latest and established models = 1.21825 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 17 components and 1.21825 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.226990Jy sigma=2.912024 ! Fit after self-cal, rms=0.226598Jy sigma=2.893718 ! Inverting map ! Your choice of large map pixels excluded 0.603% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec ! Added new window around map position (0.8, 1.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0443421 Jy ! Component: 100 - total flux cleaned = 0.0726404 Jy ! Total flux subtracted in 100 components = 0.0726404 Jy ! Clean residual min=-0.017164 max=0.033675 Jy/beam ! Clean residual mean=-0.000267 rms=0.003720 Jy/beam ! Combined flux in latest and established models = 1.29089 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 19 components and 1.29089 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.218340Jy sigma=2.629761 ! Fit after self-cal, rms=0.218090Jy sigma=2.617577 ! Inverting map ! Your choice of large map pixels excluded 0.603% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec ! Added new window around map position (0.2, -1.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0287264 Jy ! Component: 100 - total flux cleaned = 0.0455385 Jy ! Total flux subtracted in 100 components = 0.0455385 Jy ! Clean residual min=-0.016223 max=0.021457 Jy/beam ! Clean residual mean=-0.000264 rms=0.003449 Jy/beam ! Combined flux in latest and established models = 1.33642 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 25 components and 1.33642 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.215474Jy sigma=2.482693 ! Fit after self-cal, rms=0.215248Jy sigma=2.464893 ! Inverting map ! Your choice of large map pixels excluded 0.603% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec ! Added new window around map position (-1.8, -2.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.019925 Jy ! Component: 100 - total flux cleaned = 0.0316729 Jy ! Total flux subtracted in 100 components = 0.0316729 Jy ! Clean residual min=-0.015318 max=0.019014 Jy/beam ! Clean residual mean=-0.000263 rms=0.003322 Jy/beam ! Combined flux in latest and established models = 1.3681 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 37 components and 1.3681 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.216159Jy sigma=2.450899 ! Fit after self-cal, rms=0.215895Jy sigma=2.440308 ! Inverting map ! Your choice of large map pixels excluded 0.603% of the data. ! The y-axis pixel size should ideally be below 0.1828 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 0.603% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec ! Estimated beam: bmin=0.4469 mas, bmaj=1.172 mas, bpa=43.25 degrees ! Estimated noise=0.554553 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 = -0.0210645 Jy ! Component: 100 - total flux cleaned = -0.0327003 Jy ! Component: 150 - total flux cleaned = -0.0365359 Jy ! Component: 200 - total flux cleaned = -0.0380197 Jy ! Total flux subtracted in 200 components = -0.0380197 Jy ! Clean residual min=-0.034498 max=0.010270 Jy/beam ! Clean residual mean=-0.016086 rms=0.005042 Jy/beam ! Combined flux in latest and established models = 1.33008 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 49 components and 1.33008 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.211273Jy sigma=2.400538 ! Fit after self-cal, rms=0.211137Jy sigma=2.398030 ! Inverting map ! Your choice of large map pixels excluded 0.603% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec print "============== Finished natural weighting clean ==============" ! ============== Finished natural weighting clean ============== ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.4469 x 1.172 at 43.25 degrees (North through East) ! Clean map min=-0.032729 max=0.75293 Jy/beam gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 66 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! FD 0.92 HH 1.00* HN 1.05 KP 1.05 ! LA 1.02 NL 1.06 NY 0.81 PT 0.84 ! SC 1.04 WN 1.64 WZ 0.97 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 FD 0.92 HN 1.07 KP 1.09 ! LA 1.03 MK 1.03 NL 1.06 OV 0.96 ! PT 0.87 SC 0.90 ! ! A total of 15 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 MK 1.01 NY 0.63 OV 0.95 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HH 1.00* NY 0.73 WN 1.65 WZ 1.02 ! YG 3.76 ! ! A total of 3 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.98 FD 0.91 HN 1.03 KP 1.11 ! NL 1.17 NY 0.73 PT 0.86 SC 0.95 ! ! ! Correcting IF 2. ! A total of 66 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! FD 0.90 HH 1.00* HN 1.06 KP 1.04 ! LA 1.01 NL 1.05 NY 0.91 PT 0.86 ! SC 1.04 WN 1.66 WZ 0.93 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 0.92 HN 1.08 KP 1.09 ! LA 1.02 MK 1.03 NL 1.05 OV 0.96 ! PT 0.87 SC 0.89 ! ! A total of 15 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 MK 1.01 NY 0.81 OV 0.99 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HH 1.00* NY 0.85 WN 1.65 WZ 0.99 ! YG 3.67 ! ! A total of 3 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 FD 0.94 HN 1.04 KP 1.09 ! NL 1.15 NY 0.87 PT 0.86 SC 0.92 ! ! ! Correcting IF 3. ! A total of 90 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! FD 0.91 HH 1.00* HN 1.06 KP 1.02 ! LA 1.02 NL 1.06 NY 1.00* PT 0.85 ! SC 1.03 WN 1.66 WZ 0.97 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 FD 0.93 HN 1.09 KP 1.08 ! LA 1.02 MK 1.01 NL 1.05 OV 0.96 ! PT 0.87 SC 0.88 ! ! A total of 12 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* MK 0.00* NY 0.00* OV 0.00* ! ! A total of 78 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HH 0.00* NY 0.00* WN 0.00* WZ 0.00* ! YG 0.00* ! ! A total of 9 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.99 FD 0.95 HN 1.01 KP 1.05 ! NL 1.07 NY 1.00* PT 0.91 SC 0.91 ! ! ! Correcting IF 4. ! A total of 90 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! FD 0.95 HH 1.00* HN 1.04 KP 1.04 ! LA 1.05 NL 1.03 NY 1.00* PT 0.84 ! SC 1.05 WN 1.51 WZ 0.98 ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 0.93 HN 1.07 KP 1.08 ! LA 1.03 MK 0.99 NL 1.06 OV 0.97 ! PT 0.86 SC 0.90 ! ! A total of 12 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* MK 0.00* NY 0.00* OV 0.00* ! ! A total of 78 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! HH 0.00* NY 0.00* WN 0.00* WZ 0.00* ! YG 0.00* ! ! A total of 9 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.02 FD 0.96 HN 1.00 KP 1.12 ! NL 1.04 NY 1.00* PT 0.90 SC 0.93 ! ! ! Fit before self-cal, rms=0.211137Jy sigma=2.398030 ! Fit after self-cal, rms=0.099386Jy sigma=1.069782 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec ! Estimated beam: bmin=0.8345 mas, bmaj=1.08 mas, bpa=28.1 degrees ! Estimated noise=0.735075 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 = -0.0027795 Jy ! Component: 100 - total flux cleaned = -0.00247225 Jy ! Component: 150 - total flux cleaned = -0.00275561 Jy ! Component: 200 - total flux cleaned = -0.0029939 Jy ! Total flux subtracted in 200 components = -0.0029939 Jy ! Clean residual min=-0.009023 max=0.007702 Jy/beam ! Clean residual mean=-0.000863 rms=0.001486 Jy/beam ! Combined flux in latest and established models = 1.32708 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 68 components and 1.32708 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.097520Jy sigma=1.042141 ! Fit after self-cal, rms=0.097565Jy sigma=1.039912 ! Inverting map ! Your choice of large map pixels excluded 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 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=0.097565Jy sigma=1.039912 ! Fit after self-cal, rms=0.086710Jy sigma=0.896524 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec ! Estimated beam: bmin=0.8418 mas, bmaj=1.081 mas, bpa=26.78 degrees ! Estimated noise=0.734627 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00259177 Jy ! Component: 100 - total flux cleaned = -0.00300394 Jy ! Component: 150 - total flux cleaned = -0.00317716 Jy ! Component: 200 - total flux cleaned = -0.00333618 Jy ! Total flux subtracted in 200 components = -0.00333618 Jy ! Clean residual min=-0.005745 max=0.004554 Jy/beam ! Clean residual mean=-0.000620 rms=0.001021 Jy/beam ! Combined flux in latest and established models = 1.32375 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 75 components and 1.32375 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.085690Jy sigma=0.882959 ! Fit after self-cal, rms=0.085597Jy sigma=0.881305 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 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 = -0.000367167 Jy ! Component: 100 - total flux cleaned = 8.00349e-05 Jy ! Component: 150 - total flux cleaned = 8.01898e-05 Jy ! Component: 200 - total flux cleaned = 7.93982e-05 Jy ! Total flux subtracted in 200 components = 7.93982e-05 Jy ! Clean residual min=-0.005554 max=0.004195 Jy/beam ! Clean residual mean=-0.000621 rms=0.000988 Jy/beam ! Combined flux in latest and established models = 1.32383 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 77 components and 1.32383 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.085058Jy sigma=0.874579 ! Fit after self-cal, rms=0.085011Jy sigma=0.873766 ! Inverting map ! Your choice of large map pixels excluded 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 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=0.085011Jy sigma=0.873766 ! Fit after self-cal, rms=0.080874Jy sigma=0.825817 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec ! Estimated beam: bmin=0.8302 mas, bmaj=1.079 mas, bpa=28.13 degrees ! Estimated noise=0.73219 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0023265 Jy ! Component: 100 - total flux cleaned = -0.00263366 Jy ! Component: 150 - total flux cleaned = -0.00276459 Jy ! Component: 200 - total flux cleaned = -0.00300305 Jy ! Total flux subtracted in 200 components = -0.00300305 Jy ! Clean residual min=-0.004525 max=0.003483 Jy/beam ! Clean residual mean=-0.000477 rms=0.000784 Jy/beam ! Combined flux in latest and established models = 1.32082 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 80 components and 1.32082 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.080186Jy sigma=0.818108 ! Fit after self-cal, rms=0.080146Jy sigma=0.817544 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 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 = -0.00014955 Jy ! Component: 100 - total flux cleaned = -0.000151069 Jy ! Component: 150 - total flux cleaned = -0.000149736 Jy ! Component: 200 - total flux cleaned = -0.000147433 Jy ! Total flux subtracted in 200 components = -0.000147433 Jy ! Clean residual min=-0.004298 max=0.003449 Jy/beam ! Clean residual mean=-0.000475 rms=0.000762 Jy/beam ! Combined flux in latest and established models = 1.32068 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 82 components and 1.32068 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.079819Jy sigma=0.813682 ! Fit after self-cal, rms=0.079799Jy sigma=0.813301 ! Inverting map ! Your choice of large map pixels excluded 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 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=0.079799Jy sigma=0.813301 ! Fit after self-cal, rms=0.079628Jy sigma=0.811339 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec ! Estimated beam: bmin=2.845 mas, bmaj=3.053 mas, bpa=49.99 degrees ! Estimated noise=0.978304 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000514703 Jy ! Component: 100 - total flux cleaned = -0.000759065 Jy ! Component: 150 - total flux cleaned = -0.000862814 Jy ! Component: 200 - total flux cleaned = -0.000995043 Jy ! Total flux subtracted in 200 components = -0.000995043 Jy ! Clean residual min=-0.003686 max=0.002428 Jy/beam ! Clean residual mean=-0.000873 rms=0.000903 Jy/beam ! Combined flux in latest and established models = 1.31968 Jy selfcal ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 85 components and 1.31968 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.079586Jy sigma=0.810717 ! Fit after self-cal, rms=0.079568Jy sigma=0.810450 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 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 = 0.000152497 Jy ! Component: 100 - total flux cleaned = 0.000200332 Jy ! Component: 150 - total flux cleaned = 0.000125616 Jy ! Component: 200 - total flux cleaned = 5.92238e-05 Jy ! Total flux subtracted in 200 components = 5.92238e-05 Jy ! Clean residual min=-0.003672 max=0.002375 Jy/beam ! Clean residual mean=-0.000875 rms=0.000894 Jy/beam ! Combined flux in latest and established models = 1.31974 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 86 components and 1.31974 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.079578Jy sigma=0.810822 ! Fit after self-cal, rms=0.079571Jy sigma=0.810662 ! Inverting map ! Your choice of large map pixels excluded 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 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 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec ! Estimated beam: bmin=0.8326 mas, bmaj=1.078 mas, bpa=28.05 degrees ! Estimated noise=0.732031 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8326 x 1.078 at 28.05 degrees (North through East) ! Clean map min=-0.0062353 max=1.0132 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=0.079571Jy sigma=0.810662 ! Fit after self-cal, rms=0.068459Jy sigma=0.708002 ! Inverting map and beam ! Your choice of large map pixels excluded 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec ! Estimated beam: bmin=0.8357 mas, bmaj=1.078 mas, bpa=27.7 degrees ! Estimated noise=0.732172 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00158199 Jy ! Component: 100 - total flux cleaned = -0.0016989 Jy ! Component: 150 - total flux cleaned = -0.00170587 Jy ! Component: 200 - total flux cleaned = -0.00170984 Jy ! Total flux subtracted in 200 components = -0.00170984 Jy ! Clean residual min=-0.004120 max=0.003042 Jy/beam ! Clean residual mean=-0.000379 rms=0.000688 Jy/beam ! Combined flux in latest and established models = 1.31803 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 88 components and 1.31803 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.068063Jy sigma=0.703388 ! Fit after self-cal, rms=0.068054Jy sigma=0.703069 ! Inverting map ! Your choice of large map pixels excluded 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -3.00012e-05 Jy ! Component: 100 - total flux cleaned = -3.12473e-05 Jy ! Component: 150 - total flux cleaned = -3.0888e-05 Jy ! Component: 200 - total flux cleaned = -3.09023e-05 Jy ! Total flux subtracted in 200 components = -3.09023e-05 Jy ! Clean residual min=-0.003959 max=0.002946 Jy/beam ! Clean residual mean=-0.000378 rms=0.000674 Jy/beam ! Combined flux in latest and established models = 1.318 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 89 components and 1.318 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.067843Jy sigma=0.700609 ! Fit after self-cal, rms=0.067837Jy sigma=0.700373 ! Inverting map ! Your choice of large map pixels excluded 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.067837Jy sigma=0.700373 ! Fit after self-cal, rms=0.067729Jy sigma=0.698898 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 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec ! Estimated beam: bmin=0.7964 mas, bmaj=0.9572 mas, bpa=12.05 degrees ! Estimated noise=1.09342 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.817168 Jy ! Component: 100 - total flux cleaned = 1.06392 Jy ! Component: 150 - total flux cleaned = 1.17527 Jy ! Component: 200 - total flux cleaned = 1.23784 Jy ! Total flux subtracted in 200 components = 1.23784 Jy ! Clean residual min=-0.013861 max=0.031931 Jy/beam ! Clean residual mean=-0.000035 rms=0.002984 Jy/beam ! Combined flux in latest and established models = 1.23784 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 17 model components to the UV plane model. ! The established model now contains 17 components and 1.23784 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec ! Estimated beam: bmin=0.8392 mas, bmaj=1.078 mas, bpa=27.38 degrees ! Estimated noise=0.732337 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 = 0.0494319 Jy ! Component: 100 - total flux cleaned = 0.0694582 Jy ! Component: 150 - total flux cleaned = 0.0715627 Jy ! Component: 200 - total flux cleaned = 0.0728391 Jy ! Total flux subtracted in 200 components = 0.0728391 Jy ! Clean residual min=-0.011465 max=0.013358 Jy/beam ! Clean residual mean=-0.000244 rms=0.003062 Jy/beam ! Combined flux in latest and established models = 1.31068 Jy ! Adding 13 model components to the UV plane model. ! The established model now contains 23 components and 1.31068 Jy ! Inverting map ! Your choice of large map pixels excluded 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec ! Added new window around map position (-0.6, 1). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00366425 Jy ! Component: 100 - total flux cleaned = 0.00366535 Jy ! Component: 150 - total flux cleaned = 0.0041609 Jy ! Component: 200 - total flux cleaned = 0.00416903 Jy ! Total flux subtracted in 200 components = 0.00416903 Jy ! Clean residual min=-0.009190 max=0.009622 Jy/beam ! Clean residual mean=-0.000292 rms=0.002433 Jy/beam ! Combined flux in latest and established models = 1.31485 Jy ! Adding 18 model components to the UV plane model. ! The established model now contains 35 components and 1.31485 Jy ! Inverting map ! Your choice of large map pixels excluded 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 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 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec ! Estimated beam: bmin=2.846 mas, bmaj=3.052 mas, bpa=49.83 degrees ! Estimated noise=0.976832 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00364816 Jy ! Component: 100 - total flux cleaned = 0.00373623 Jy ! Component: 150 - total flux cleaned = 0.00373774 Jy ! Component: 200 - total flux cleaned = 0.00381124 Jy ! Total flux subtracted in 200 components = 0.00381124 Jy ! Clean residual min=-0.003420 max=0.002249 Jy/beam ! Clean residual mean=-0.000740 rms=0.000820 Jy/beam ! Combined flux in latest and established models = 1.31866 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 = -6.65216e-05 Jy ! Component: 100 - total flux cleaned = -6.86028e-05 Jy ! Component: 150 - total flux cleaned = -0.00012516 Jy ! Component: 200 - total flux cleaned = -0.000127135 Jy ! Total flux subtracted in 200 components = -0.000127135 Jy ! Clean residual min=-0.003382 max=0.002263 Jy/beam ! Clean residual mean=-0.000737 rms=0.000813 Jy/beam ! Combined flux in latest and established models = 1.31853 Jy ! Adding 9 model components to the UV plane model. ! The established model now contains 44 components and 1.31853 Jy ! Inverting map ! Your choice of large map pixels excluded 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec ! Estimated beam: bmin=0.8392 mas, bmaj=1.078 mas, bpa=27.38 degrees ! Estimated noise=0.732337 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00198145 Jy ! Component: 100 - total flux cleaned = -0.00198177 Jy ! Component: 150 - total flux cleaned = -0.00160722 Jy ! Component: 200 - total flux cleaned = -0.00162709 Jy ! Total flux subtracted in 200 components = -0.00162709 Jy ! Clean residual min=-0.007794 max=0.008131 Jy/beam ! Clean residual mean=-0.000317 rms=0.001971 Jy/beam ! Combined flux in latest and established models = 1.31691 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 46 components and 1.31691 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.074318Jy sigma=0.992252 ! Fit after self-cal, rms=0.070403Jy sigma=0.942876 wmodel J1130+3815_X_map.mod ! Writing 46 model components to file: J1130+3815_X_map.mod wobs J1130+3815_X_uvs.fits ! Writing UV FITS file: J1130+3815_X_uvs.fits wwins J1130+3815_X_map.win ! wwins: Wrote 5 windows to J1130+3815_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 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00181698 Jy ! Component: 100 - total flux cleaned = -0.00315634 Jy ! Component: 150 - total flux cleaned = -0.00420001 Jy ! Component: 200 - total flux cleaned = -0.00498456 Jy ! Component: 250 - total flux cleaned = -0.00552907 Jy ! Component: 300 - total flux cleaned = -0.00647782 Jy ! Component: 350 - total flux cleaned = -0.00709312 Jy ! Component: 400 - total flux cleaned = -0.00749461 Jy ! Component: 450 - total flux cleaned = -0.00818155 Jy ! Component: 500 - total flux cleaned = -0.00865867 Jy ! Component: 550 - total flux cleaned = -0.00903289 Jy ! Component: 600 - total flux cleaned = -0.00939905 Jy ! Component: 650 - total flux cleaned = -0.00957911 Jy ! Component: 700 - total flux cleaned = -0.0100201 Jy ! Component: 750 - total flux cleaned = -0.0102789 Jy ! Component: 800 - total flux cleaned = -0.0105334 Jy ! Component: 850 - total flux cleaned = -0.0108663 Jy ! Component: 900 - total flux cleaned = -0.0109485 Jy ! Component: 950 - total flux cleaned = -0.0112702 Jy ! Component: 1000 - total flux cleaned = -0.011349 Jy ! Component: 1050 - total flux cleaned = -0.0115816 Jy ! Component: 1100 - total flux cleaned = -0.011733 Jy ! Component: 1150 - total flux cleaned = -0.0118071 Jy ! Component: 1200 - total flux cleaned = -0.0119546 Jy ! Component: 1250 - total flux cleaned = -0.0121715 Jy ! Component: 1300 - total flux cleaned = -0.0123143 Jy ! Component: 1350 - total flux cleaned = -0.0123842 Jy ! Component: 1400 - total flux cleaned = -0.0125919 Jy ! Component: 1450 - total flux cleaned = -0.012728 Jy ! Component: 1500 - total flux cleaned = -0.0127943 Jy ! Component: 1550 - total flux cleaned = -0.0128604 Jy ! Component: 1600 - total flux cleaned = -0.0130543 Jy ! Component: 1650 - total flux cleaned = -0.0130552 Jy ! Component: 1700 - total flux cleaned = -0.0133681 Jy ! Component: 1750 - total flux cleaned = -0.0133681 Jy ! Component: 1800 - total flux cleaned = -0.0136105 Jy ! Component: 1850 - total flux cleaned = -0.0137885 Jy ! Component: 1900 - total flux cleaned = -0.0137881 Jy ! Component: 1950 - total flux cleaned = -0.0139614 Jy ! Component: 2000 - total flux cleaned = -0.0140751 Jy ! Component: 2050 - total flux cleaned = -0.0141869 Jy ! Component: 2100 - total flux cleaned = -0.0142422 Jy ! Component: 2150 - total flux cleaned = -0.0144061 Jy ! Component: 2200 - total flux cleaned = -0.0145133 Jy ! Component: 2250 - total flux cleaned = -0.0146187 Jy ! Component: 2300 - total flux cleaned = -0.014671 Jy ! Component: 2350 - total flux cleaned = -0.0147743 Jy ! Component: 2400 - total flux cleaned = -0.014927 Jy ! Component: 2450 - total flux cleaned = -0.0149766 Jy ! Component: 2500 - total flux cleaned = -0.0151248 Jy ! Component: 2550 - total flux cleaned = -0.0151735 Jy ! Component: 2600 - total flux cleaned = -0.0153655 Jy ! Component: 2650 - total flux cleaned = -0.015413 Jy ! Component: 2700 - total flux cleaned = -0.0156007 Jy ! Component: 2750 - total flux cleaned = -0.0156927 Jy ! Component: 2800 - total flux cleaned = -0.015738 Jy ! Component: 2850 - total flux cleaned = -0.0158283 Jy ! Component: 2900 - total flux cleaned = -0.0158734 Jy ! Component: 2950 - total flux cleaned = -0.0160494 Jy ! Component: 3000 - total flux cleaned = -0.0161367 Jy ! Component: 3050 - total flux cleaned = -0.0162228 Jy ! Component: 3100 - total flux cleaned = -0.0163078 Jy ! Component: 3150 - total flux cleaned = -0.016392 Jy ! Component: 3200 - total flux cleaned = -0.0164751 Jy ! Component: 3250 - total flux cleaned = -0.0165575 Jy ! Component: 3300 - total flux cleaned = -0.0166791 Jy ! Component: 3350 - total flux cleaned = -0.0166786 Jy ! Component: 3400 - total flux cleaned = -0.0167977 Jy ! Component: 3450 - total flux cleaned = -0.0167981 Jy ! Component: 3500 - total flux cleaned = -0.0168758 Jy ! Component: 3550 - total flux cleaned = -0.0169912 Jy ! Component: 3600 - total flux cleaned = -0.0170293 Jy ! Component: 3650 - total flux cleaned = -0.017142 Jy ! Component: 3700 - total flux cleaned = -0.0171786 Jy ! Component: 3750 - total flux cleaned = -0.0172154 Jy ! Component: 3800 - total flux cleaned = -0.0172883 Jy ! Component: 3850 - total flux cleaned = -0.0173604 Jy ! Component: 3900 - total flux cleaned = -0.0174316 Jy ! Component: 3950 - total flux cleaned = -0.0174314 Jy ! Component: 4000 - total flux cleaned = -0.0175016 Jy ! Component: 4050 - total flux cleaned = -0.0176057 Jy ! Total flux subtracted in 4096 components = -0.0175712 Jy ! Clean residual min=-0.001852 max=0.001714 Jy/beam ! Clean residual mean=-0.000060 rms=0.000574 Jy/beam ! Combined flux in latest and established models = 1.29933 Jy keep ! Adding 411 model components to the UV plane model. ! The established model now contains 454 components and 1.29934 Jy ![Exited script file: /opt64/bin/pima_mupet_01.dfm] wmap /scr/pima/rv124_uvs/J1130+3815_X_map.fits ! Inverting map ! Your choice of large map pixels excluded 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8392 x 1.078 at 27.38 degrees (North through East) ! Clean map min=-0.0026251 max=1.0266 Jy/beam ! Writing clean map to FITS file: /scr/pima/rv124_uvs/J1130+3815_X_map.fits wmodel /scr/pima/rv124_uvs/J1130+3815_X_map.mod ! Writing 454 model components to file: /scr/pima/rv124_uvs/J1130+3815_X_map.mod wobs /scr/pima/rv124_uvs/J1130+3815_X_uvs.fits ! Writing UV FITS file: /scr/pima/rv124_uvs/J1130+3815_X_uvs.fits wwins /scr/pima/rv124_uvs/J1130+3815_X_map.win ! wwins: Wrote 6 windows to /scr/pima/rv124_uvs/J1130+3815_X_map.win float peak_flux peak_flux = peak(flux,max) print "The peak flux is", peak_flux ! The peak flux is 1.02661 invert ! Inverting map ! Your choice of large map pixels excluded 0.594% of the data. ! The y-axis pixel size should ideally be below 0.1828 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000565773 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.165332 0.165332 0.330664 0.661328 1.32266 2.64531 5.29062 10.5812 21.1625 42.325 84.6499 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0016 print "peak= ", int(1000*peak_flux)/1000 ! peak= 1.026 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 1814.53 quit ! Quitting program ! Log file /scr/pima/rv124_uvs/J1130+3815_X_dfm.log closed on Mon Dec 24 00:18:36 2018