! Started logfile: /scr/pima/gb073_uvs/J1357+7643_X_uvs.log on Sat Dec 26 09:40:13 2015 obs /scr/pima/gb073_uvs/J1357+7643_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1357+7643_X_uva.fits ! AN table 1: 6 integrations on 55 of 55 possible baselines. ! AN table 2: 6 integrations on 78 of 78 possible baselines. ! AN table 3: 6 integrations on 66 of 66 possible baselines. ! Apparent sampling: 1 visibilities/baseline/integration-bin. ! Found source: J1357+7643 ! ! There are 8 IFs, and a total of 8 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 8.39799e+09 8e+06 1 8e+06 ! 02 2 8.40599e+09 8e+06 1 8e+06 ! 03 3 8.46799e+09 8e+06 1 8e+06 ! 04 4 8.47599e+09 8e+06 1 8e+06 ! 05 5 8.78299e+09 8e+06 1 8e+06 ! 06 6 8.79099e+09 8e+06 1 8e+06 ! 07 7 8.88799e+09 8e+06 1 8e+06 ! 08 8 8.89599e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 0 lines of history. ! ! Reading 9552 visibilities. select RR ! Selecting polarization: RR, channels: 1..8 ! Reading IF 1 channels: 1..1 ! Reading IF 2 channels: 2..2 ! Reading IF 3 channels: 3..3 ! Reading IF 4 channels: 4..4 ! Reading IF 5 channels: 5..5 ! Reading IF 6 channels: 6..6 ! Reading IF 7 channels: 7..7 ! Reading IF 8 channels: 8..8 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 ![@/home/lpetrov/bin/01_muppet /scr/pima/gb073_uvs/J1357+7643_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 6 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 5. ! A total of 12 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! A total of 12 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 6. ! A total of 12 telescope corrections were flagged in sub-array 1. ! A total of 12 telescope corrections were flagged in sub-array 2. ! A total of 12 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 7. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 8. ! A total of 6 telescope corrections were flagged in sub-array 1. ! A total of 6 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=1.176825Jy sigma=10.918904 ! Fit after self-cal, rms=0.379999Jy sigma=3.384239 ! 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 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 milli-arcsec ! Estimated beam: bmin=0.5022 mas, bmaj=0.6817 mas, bpa=-20.26 degrees ! Estimated noise=1.49752 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 = 0.492026 Jy ! Component: 100 - total flux cleaned = 0.601639 Jy ! Total flux subtracted in 100 components = 0.601639 Jy ! Clean residual min=-0.020767 max=0.037607 Jy/beam ! Clean residual mean=-0.000001 rms=0.004362 Jy/beam ! Combined flux in latest and established models = 0.601638 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 0.601638 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.163886Jy sigma=1.249952 ! Fit after self-cal, rms=0.163879Jy sigma=1.249874 ! Inverting map ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0412696 Jy ! Component: 100 - total flux cleaned = 0.0652605 Jy ! Total flux subtracted in 100 components = 0.0652605 Jy ! Clean residual min=-0.023734 max=0.022583 Jy/beam ! Clean residual mean=-0.000002 rms=0.003765 Jy/beam ! Combined flux in latest and established models = 0.666899 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 7 components and 0.666899 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.152747Jy sigma=1.084176 ! Fit after self-cal, rms=0.152751Jy sigma=1.084100 ! Inverting map ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 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 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 milli-arcsec ! Estimated beam: bmin=0.6369 mas, bmaj=0.8315 mas, bpa=-21.56 degrees ! Estimated noise=0.923013 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 (-1.2, -1). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.01251 Jy ! Component: 100 - total flux cleaned = 0.0166084 Jy ! Component: 150 - total flux cleaned = 0.0195576 Jy ! Component: 200 - total flux cleaned = 0.0212736 Jy ! Total flux subtracted in 200 components = 0.0212736 Jy ! Clean residual min=-0.014838 max=0.010807 Jy/beam ! Clean residual mean=-0.000004 rms=0.002279 Jy/beam ! Combined flux in latest and established models = 0.688173 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 18 components and 0.688173 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.147531Jy sigma=1.031091 ! Fit after self-cal, rms=0.147333Jy sigma=1.029372 ! Inverting map ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6369 x 0.8315 at -21.56 degrees (North through East) ! Clean map min=-0.012423 max=0.63777 Jy/beam if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.94 EF 1.00* FD 0.96 KP 0.97 ! LA 1.02 MC 0.94 MK 0.97 NL 0.95 ! OV 1.00 PT 0.95 ZC 0.75 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.93 EF 1.00* FD 1.00 KP 1.01 ! LA 1.05 MC 0.98 MK 0.97 NL 0.93 ! ON 1.03 OV 1.01 PT 0.96 SC 0.92 ! ZC 0.79 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 EF 1.00* FD 0.97 KP 1.00 ! LA 1.04 MC 0.91 MK 1.01 NL 0.94 ! ON 0.97 OV 1.01 PT 0.96 SC 0.95 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 EF 1.00* FD 0.99 KP 1.00 ! LA 1.08 MC 0.94 MK 1.00 NL 0.97 ! OV 1.01 PT 1.00 ZC 0.76 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 EF 1.00* FD 1.02 KP 1.02 ! LA 1.07 MC 0.99 MK 1.01 NL 0.97 ! ON 1.04 OV 1.03 PT 1.00 SC 0.97 ! ZC 0.83 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 EF 1.00* FD 1.00 KP 1.03 ! LA 1.06 MC 0.94 MK 1.02 NL 0.98 ! ON 0.98 OV 1.04 PT 1.01 SC 0.97 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 EF 1.00* FD 1.01 KP 0.93 ! LA 0.98 MC 0.93 MK 0.95 NL 0.94 ! OV 0.97 PT 0.99 ZC 0.73 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 EF 1.00* FD 1.00 KP 0.96 ! LA 1.00 MC 1.00 MK 0.97 NL 0.94 ! ON 1.02 OV 1.00 PT 1.00 SC 0.99 ! ZC 0.80 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 EF 1.00* FD 0.99 KP 0.94 ! LA 1.00 MC 0.92 MK 0.97 NL 0.95 ! ON 0.91 OV 1.00 PT 1.01 SC 1.02 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 EF 1.00* FD 1.01 KP 0.96 ! LA 0.99 MC 0.92 MK 0.98 NL 0.98 ! OV 0.97 PT 1.00 ZC 0.75 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 EF 1.00* FD 1.03 KP 0.98 ! LA 1.01 MC 1.01 MK 0.98 NL 0.95 ! ON 1.04 OV 1.01 PT 1.04 SC 1.00 ! ZC 0.82 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 EF 1.00* FD 1.02 KP 0.99 ! LA 1.03 MC 0.95 MK 1.00 NL 0.98 ! ON 0.96 OV 1.01 PT 1.01 SC 1.02 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.02 KP 0.89 ! LA 1.00 MC 1.21 MK 0.98 NL 1.00 ! OV 1.05 PT 0.96 ZC 0.76 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.04 KP 0.90 ! LA 1.01 MC 1.28 MK 0.97 NL 0.99 ! ON 1.25 OV 1.06 PT 0.98 SC 1.02 ! ZC 0.84 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 0.98 KP 0.93 ! LA 0.99 MC 1.18 MK 0.97 NL 1.01 ! ON 1.17 OV 1.07 PT 0.97 SC 1.03 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.01 KP 0.86 ! LA 0.98 MC 1.21 MK 0.99 NL 1.00 ! OV 1.04 PT 0.93 ZC 0.72 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.04 KP 0.88 ! LA 1.00 MC 1.27 MK 0.98 NL 0.99 ! ON 1.30 OV 1.07 PT 0.94 SC 0.96 ! ZC 0.83 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 0.99 KP 0.88 ! LA 1.01 MC 1.20 MK 0.99 NL 0.99 ! ON 1.19 OV 1.06 PT 0.96 SC 0.99 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 EF 1.00* FD 1.01 KP 0.92 ! LA 1.03 MC 1.26 MK 1.08 NL 1.05 ! OV 1.00 PT 0.99 ZC 0.55 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 EF 1.00* FD 1.07 KP 0.93 ! LA 1.05 MC 1.32 MK 1.04 NL 1.03 ! ON 1.36 OV 1.01 PT 1.01 SC 1.01 ! ZC 0.63 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 EF 1.00* FD 1.04 KP 0.88 ! LA 1.07 MC 1.29 MK 1.10 NL 1.01 ! ON 1.29 OV 1.01 PT 0.98 SC 1.01 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 EF 1.00* FD 1.03 KP 0.90 ! LA 1.02 MC 1.33 MK 1.02 NL 1.02 ! OV 0.99 PT 1.00 ZC 0.52 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 EF 1.00* FD 1.05 KP 0.92 ! LA 1.06 MC 1.38 MK 1.05 NL 1.02 ! ON 1.37 OV 1.03 PT 1.01 SC 0.98 ! ZC 0.60 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 EF 1.00* FD 1.03 KP 0.91 ! LA 1.07 MC 1.29 MK 1.07 NL 1.00 ! ON 1.24 OV 1.01 PT 1.00 SC 1.04 ! ! ! Fit before self-cal, rms=0.147333Jy sigma=1.029372 ! Fit after self-cal, rms=0.094452Jy sigma=0.670182 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 milli-arcsec ! Estimated beam: bmin=0.6338 mas, bmaj=0.8419 mas, bpa=-20.79 degrees ! Estimated noise=0.916115 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 (-2.4, -1.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00286178 Jy ! Component: 100 - total flux cleaned = 0.00331103 Jy ! Component: 150 - total flux cleaned = 0.00353933 Jy ! Component: 200 - total flux cleaned = 0.0036305 Jy ! Total flux subtracted in 200 components = 0.0036305 Jy ! Clean residual min=-0.003585 max=0.003015 Jy/beam ! Clean residual mean=0.000003 rms=0.000708 Jy/beam ! Combined flux in latest and established models = 0.691803 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 28 components and 0.691803 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.094033Jy sigma=0.665434 ! Fit after self-cal, rms=0.094080Jy sigma=0.664955 ! Inverting map ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 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. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.094080Jy sigma=0.664955 ! Fit after self-cal, rms=0.094225Jy sigma=0.664300 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 milli-arcsec ! Estimated beam: bmin=0.6337 mas, bmaj=0.8429 mas, bpa=-20.83 degrees ! Estimated noise=0.915989 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00116867 Jy ! Component: 100 - total flux cleaned = 0.00126504 Jy ! Component: 150 - total flux cleaned = 0.00126098 Jy ! Component: 200 - total flux cleaned = 0.00125993 Jy ! Total flux subtracted in 200 components = 0.00125993 Jy ! Clean residual min=-0.003403 max=0.002862 Jy/beam ! Clean residual mean=0.000003 rms=0.000677 Jy/beam ! Combined flux in latest and established models = 0.693063 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 34 components and 0.693063 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.094018Jy sigma=0.661951 ! Fit after self-cal, rms=0.094011Jy sigma=0.661885 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 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 = 0.000454846 Jy ! Component: 100 - total flux cleaned = 0.000518418 Jy ! Component: 150 - total flux cleaned = 0.000520977 Jy ! Component: 200 - total flux cleaned = 0.000574806 Jy ! Total flux subtracted in 200 components = 0.000574806 Jy ! Clean residual min=-0.003353 max=0.002827 Jy/beam ! Clean residual mean=0.000003 rms=0.000669 Jy/beam ! Combined flux in latest and established models = 0.693638 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 41 components and 0.693638 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.093938Jy sigma=0.661228 ! Fit after self-cal, rms=0.093934Jy sigma=0.661201 ! Inverting map ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 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. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.093934Jy sigma=0.661201 ! Fit after self-cal, rms=0.094125Jy sigma=0.660622 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 milli-arcsec ! Estimated beam: bmin=0.6336 mas, bmaj=0.8442 mas, bpa=-20.82 degrees ! Estimated noise=0.915879 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00010672 Jy ! Component: 100 - total flux cleaned = 4.13157e-05 Jy ! Component: 150 - total flux cleaned = 3.98713e-05 Jy ! Component: 200 - total flux cleaned = 9.3002e-05 Jy ! Total flux subtracted in 200 components = 9.3002e-05 Jy ! Clean residual min=-0.003156 max=0.002675 Jy/beam ! Clean residual mean=0.000003 rms=0.000651 Jy/beam ! Combined flux in latest and established models = 0.693731 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 43 components and 0.693731 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.094016Jy sigma=0.659522 ! Fit after self-cal, rms=0.094015Jy sigma=0.659498 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 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 = 0.000230153 Jy ! Component: 100 - total flux cleaned = 0.000279098 Jy ! Component: 150 - total flux cleaned = 0.000279088 Jy ! Component: 200 - total flux cleaned = 0.000323312 Jy ! Total flux subtracted in 200 components = 0.000323312 Jy ! Clean residual min=-0.003118 max=0.002689 Jy/beam ! Clean residual mean=0.000002 rms=0.000646 Jy/beam ! Combined flux in latest and established models = 0.694054 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 44 components and 0.694054 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.093973Jy sigma=0.659131 ! Fit after self-cal, rms=0.093971Jy sigma=0.659117 ! Inverting map ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 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. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.093971Jy sigma=0.659117 ! Fit after self-cal, rms=0.094105Jy sigma=0.658794 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 milli-arcsec ! Estimated beam: bmin=2.594 mas, bmaj=2.881 mas, bpa=72.32 degrees ! Estimated noise=1.2286 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000199023 Jy ! Component: 100 - total flux cleaned = 0.000394904 Jy ! Component: 150 - total flux cleaned = 0.000482625 Jy ! Component: 200 - total flux cleaned = 0.000548062 Jy ! Total flux subtracted in 200 components = 0.000548062 Jy ! Clean residual min=-0.003348 max=0.002801 Jy/beam ! Clean residual mean=0.000006 rms=0.000864 Jy/beam ! Combined flux in latest and established models = 0.694602 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 54 components and 0.694602 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.094102Jy sigma=0.658646 ! Fit after self-cal, rms=0.094107Jy sigma=0.658608 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 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 = 0.000158065 Jy ! Component: 100 - total flux cleaned = 0.000213253 Jy ! Component: 150 - total flux cleaned = 0.000241868 Jy ! Component: 200 - total flux cleaned = 0.00025525 Jy ! Total flux subtracted in 200 components = 0.00025525 Jy ! Clean residual min=-0.003322 max=0.002820 Jy/beam ! Clean residual mean=0.000005 rms=0.000863 Jy/beam ! Combined flux in latest and established models = 0.694857 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 57 components and 0.694857 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.094104Jy sigma=0.658559 ! Fit after self-cal, rms=0.094104Jy sigma=0.658549 ! Inverting map ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 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 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 milli-arcsec ! Estimated beam: bmin=0.6334 mas, bmaj=0.8455 mas, bpa=-20.79 degrees ! Estimated noise=0.915581 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6334 x 0.8455 at -20.79 degrees (North through East) ! Clean map min=-0.0048984 max=0.6322 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. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.094104Jy sigma=0.658549 ! Fit after self-cal, rms=0.089731Jy sigma=0.623891 ! Inverting map and beam ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 milli-arcsec ! Estimated beam: bmin=0.6338 mas, bmaj=0.8453 mas, bpa=-20.79 degrees ! Estimated noise=0.915045 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000423058 Jy ! Component: 100 - total flux cleaned = -0.000480092 Jy ! Component: 150 - total flux cleaned = -0.000528184 Jy ! Component: 200 - total flux cleaned = -0.000529751 Jy ! Total flux subtracted in 200 components = -0.000529751 Jy ! Clean residual min=-0.003053 max=0.002602 Jy/beam ! Clean residual mean=0.000002 rms=0.000630 Jy/beam ! Combined flux in latest and established models = 0.694328 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 59 components and 0.694328 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.089671Jy sigma=0.623228 ! Fit after self-cal, rms=0.089666Jy sigma=0.623217 ! Inverting map ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -9.08883e-05 Jy ! Component: 100 - total flux cleaned = -4.99071e-05 Jy ! Component: 150 - total flux cleaned = -1.21982e-05 Jy ! Component: 200 - total flux cleaned = -1.20319e-05 Jy ! Total flux subtracted in 200 components = -1.20319e-05 Jy ! Clean residual min=-0.003031 max=0.002583 Jy/beam ! Clean residual mean=0.000002 rms=0.000627 Jy/beam ! Combined flux in latest and established models = 0.694316 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 61 components and 0.694316 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.089642Jy sigma=0.623013 ! Fit after self-cal, rms=0.089638Jy sigma=0.623000 ! Inverting map ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.089638Jy sigma=0.623000 ! Fit after self-cal, rms=0.089716Jy sigma=0.622776 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 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 milli-arcsec ! Estimated beam: bmin=0.4982 mas, bmaj=0.6929 mas, bpa=-19.83 degrees ! Estimated noise=1.4876 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.488704 Jy ! Component: 100 - total flux cleaned = 0.595936 Jy ! Component: 150 - total flux cleaned = 0.629817 Jy ! Component: 200 - total flux cleaned = 0.647908 Jy ! Total flux subtracted in 200 components = 0.647908 Jy ! Clean residual min=-0.005099 max=0.009217 Jy/beam ! Clean residual mean=0.000001 rms=0.001209 Jy/beam ! Combined flux in latest and established models = 0.647908 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 12 model components to the UV plane model. ! The established model now contains 12 components and 0.647908 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 milli-arcsec ! Estimated beam: bmin=0.6334 mas, bmaj=0.8463 mas, bpa=-20.78 degrees ! Estimated noise=0.914791 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 = 0.0171002 Jy ! Component: 100 - total flux cleaned = 0.0265901 Jy ! Component: 150 - total flux cleaned = 0.0324639 Jy ! Component: 200 - total flux cleaned = 0.0364683 Jy ! Total flux subtracted in 200 components = 0.0364683 Jy ! Clean residual min=-0.003418 max=0.002917 Jy/beam ! Clean residual mean=0.000007 rms=0.000684 Jy/beam ! Combined flux in latest and established models = 0.684376 Jy ! Adding 31 model components to the UV plane model. ! The established model now contains 35 components and 0.684376 Jy ! Inverting map ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 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 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 milli-arcsec ! Estimated beam: bmin=2.594 mas, bmaj=2.88 mas, bpa=72.24 degrees ! Estimated noise=1.22691 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00457881 Jy ! Component: 100 - total flux cleaned = 0.00681341 Jy ! Component: 150 - total flux cleaned = 0.00807359 Jy ! Component: 200 - total flux cleaned = 0.00879022 Jy ! Total flux subtracted in 200 components = 0.00879022 Jy ! Clean residual min=-0.003474 max=0.002751 Jy/beam ! Clean residual mean=0.000008 rms=0.000847 Jy/beam ! Combined flux in latest and established models = 0.693166 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 = 0.000225604 Jy ! Component: 100 - total flux cleaned = 0.000320973 Jy ! Component: 150 - total flux cleaned = 0.00039324 Jy ! Component: 200 - total flux cleaned = 0.000459472 Jy ! Total flux subtracted in 200 components = 0.000459472 Jy ! Clean residual min=-0.003444 max=0.002695 Jy/beam ! Clean residual mean=0.000007 rms=0.000843 Jy/beam ! Combined flux in latest and established models = 0.693626 Jy ! Adding 26 model components to the UV plane model. ! The established model now contains 54 components and 0.693626 Jy ! Inverting map ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 milli-arcsec ! Estimated beam: bmin=0.6334 mas, bmaj=0.8463 mas, bpa=-20.78 degrees ! Estimated noise=0.914791 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000504887 Jy ! Component: 100 - total flux cleaned = -0.000325709 Jy ! Component: 150 - total flux cleaned = -0.00027751 Jy ! Component: 200 - total flux cleaned = -0.000324047 Jy ! Total flux subtracted in 200 components = -0.000324047 Jy ! Clean residual min=-0.003010 max=0.002682 Jy/beam ! Clean residual mean=0.000003 rms=0.000628 Jy/beam ! Combined flux in latest and established models = 0.693301 Jy selfcal ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 61 components and 0.693302 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.089629Jy sigma=0.622330 ! Fit after self-cal, rms=0.089593Jy sigma=0.621989 wmodel /scr/pima/gb073_uvs/J1357+7643_X_map.mod ! Writing 61 model components to file: /scr/pima/gb073_uvs/J1357+7643_X_map.mod wobs /scr/pima/gb073_uvs/J1357+7643_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1357+7643_X_uvs.fits wwins /scr/pima/gb073_uvs/J1357+7643_X_map.win ! wwins: Wrote 3 windows to /scr/pima/gb073_uvs/J1357+7643_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 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000837379 Jy ! Component: 100 - total flux cleaned = -0.00103511 Jy ! Component: 150 - total flux cleaned = -0.00103626 Jy ! Component: 200 - total flux cleaned = -0.000946453 Jy ! Component: 250 - total flux cleaned = -0.000902403 Jy ! Component: 300 - total flux cleaned = -0.000816822 Jy ! Component: 350 - total flux cleaned = -0.000774777 Jy ! Component: 400 - total flux cleaned = -0.000733718 Jy ! Component: 450 - total flux cleaned = -0.000733455 Jy ! Component: 500 - total flux cleaned = -0.000611841 Jy ! Component: 550 - total flux cleaned = -0.000571479 Jy ! Component: 600 - total flux cleaned = -0.000413281 Jy ! Component: 650 - total flux cleaned = -0.000374437 Jy ! Component: 700 - total flux cleaned = -0.000335275 Jy ! Component: 750 - total flux cleaned = -0.000220456 Jy ! Component: 800 - total flux cleaned = -3.17318e-05 Jy ! Component: 850 - total flux cleaned = -6.87442e-05 Jy ! Component: 900 - total flux cleaned = -6.81253e-05 Jy ! Component: 950 - total flux cleaned = 7.75944e-05 Jy ! Component: 1000 - total flux cleaned = 0.000222327 Jy ! Component: 1050 - total flux cleaned = 0.000436454 Jy ! Component: 1100 - total flux cleaned = 0.000436696 Jy ! Component: 1150 - total flux cleaned = 0.000682459 Jy ! Component: 1200 - total flux cleaned = 0.000820848 Jy ! Component: 1250 - total flux cleaned = 0.00089016 Jy ! Component: 1300 - total flux cleaned = 0.00102644 Jy ! Component: 1350 - total flux cleaned = 0.00126361 Jy ! Component: 1400 - total flux cleaned = 0.00139769 Jy ! Component: 1450 - total flux cleaned = 0.00136436 Jy ! Component: 1500 - total flux cleaned = 0.00139785 Jy ! Component: 1550 - total flux cleaned = 0.00143036 Jy ! Component: 1600 - total flux cleaned = 0.00149587 Jy ! Component: 1650 - total flux cleaned = 0.00175429 Jy ! Component: 1700 - total flux cleaned = 0.00152947 Jy ! Component: 1750 - total flux cleaned = 0.00162529 Jy ! Component: 1800 - total flux cleaned = 0.00162528 Jy ! Component: 1850 - total flux cleaned = 0.00168816 Jy ! Component: 1900 - total flux cleaned = 0.00178178 Jy ! Component: 1950 - total flux cleaned = 0.00171976 Jy ! Component: 2000 - total flux cleaned = 0.00171971 Jy ! Component: 2050 - total flux cleaned = 0.00181137 Jy ! Component: 2100 - total flux cleaned = 0.00184189 Jy ! Component: 2150 - total flux cleaned = 0.00181161 Jy ! Component: 2200 - total flux cleaned = 0.00172151 Jy ! Component: 2250 - total flux cleaned = 0.00184097 Jy ! Component: 2300 - total flux cleaned = 0.00175162 Jy ! Component: 2350 - total flux cleaned = 0.0017517 Jy ! Component: 2400 - total flux cleaned = 0.00169277 Jy ! Component: 2450 - total flux cleaned = 0.00183886 Jy ! Component: 2500 - total flux cleaned = 0.00157782 Jy ! Component: 2550 - total flux cleaned = 0.00172209 Jy ! Component: 2600 - total flux cleaned = 0.00160734 Jy ! Component: 2650 - total flux cleaned = 0.00152175 Jy ! Component: 2700 - total flux cleaned = 0.00163536 Jy ! Component: 2750 - total flux cleaned = 0.00166356 Jy ! Component: 2800 - total flux cleaned = 0.00155124 Jy ! Component: 2850 - total flux cleaned = 0.00163493 Jy ! Component: 2900 - total flux cleaned = 0.0016627 Jy ! Component: 2950 - total flux cleaned = 0.00169027 Jy ! Component: 3000 - total flux cleaned = 0.00160761 Jy ! Component: 3050 - total flux cleaned = 0.00168953 Jy ! Component: 3100 - total flux cleaned = 0.00171673 Jy ! Component: 3150 - total flux cleaned = 0.0016896 Jy ! Component: 3200 - total flux cleaned = 0.00177058 Jy ! Component: 3250 - total flux cleaned = 0.00160979 Jy ! Component: 3300 - total flux cleaned = 0.0014767 Jy ! Component: 3350 - total flux cleaned = 0.00158299 Jy ! Component: 3400 - total flux cleaned = 0.00163594 Jy ! Component: 3450 - total flux cleaned = 0.00158347 Jy ! Component: 3500 - total flux cleaned = 0.00160974 Jy ! Component: 3550 - total flux cleaned = 0.00163576 Jy ! Component: 3600 - total flux cleaned = 0.00173933 Jy ! Component: 3650 - total flux cleaned = 0.00161028 Jy ! Component: 3700 - total flux cleaned = 0.00168723 Jy ! Component: 3750 - total flux cleaned = 0.00163607 Jy ! Component: 3800 - total flux cleaned = 0.00171229 Jy ! Component: 3850 - total flux cleaned = 0.00163642 Jy ! Component: 3900 - total flux cleaned = 0.0016363 Jy ! Component: 3950 - total flux cleaned = 0.00168627 Jy ! Component: 4000 - total flux cleaned = 0.0016114 Jy ! Component: 4050 - total flux cleaned = 0.0016363 Jy ! Total flux subtracted in 4096 components = 0.00166111 Jy ! Clean residual min=-0.001494 max=0.001526 Jy/beam ! Clean residual mean=0.000001 rms=0.000399 Jy/beam ! Combined flux in latest and established models = 0.694963 Jy keep ! Adding 350 model components to the UV plane model. ! The established model now contains 411 components and 0.694963 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1357+7643_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6334 x 0.8463 at -20.78 degrees (North through East) ! Clean map min=-0.0023994 max=0.6313 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1357+7643_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.6313 invert ! Inverting map ! Your choice of large map pixels excluded 6.74% of the data. ! The x-axis pixel size should ideally be below 0.1642 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000398651 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.189443 0.189443 0.378886 0.757771 1.51554 3.03109 6.06217 12.1243 24.2487 48.4974 96.9947 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0011 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.631 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 1583.59 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1357+7643_X_uvs.log closed on Sat Dec 26 09:40:17 2015