! Started logfile: /scr/pima/gb073_uvs/J1725+5851_X_uvs.log on Sat Dec 26 09:42:49 2015 obs /scr/pima/gb073_uvs/J1725+5851_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1725+5851_X_uva.fits ! AN table 1: 58 integrations on 55 of 55 possible baselines. ! AN table 2: 58 integrations on 55 of 55 possible baselines. ! AN table 3: 29 integrations on 66 of 66 possible baselines. ! AN table 4: 29 integrations on 10 of 10 possible baselines. ! Apparent sampling: 0.913444 visibilities/baseline/integration-bin. ! Found source: J1725+5851 ! ! 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 62728 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/J1725+5851_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 87 telescope corrections were flagged in sub-array 1. ! A total of 87 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 87 telescope corrections were flagged in sub-array 1. ! A total of 87 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 87 telescope corrections were flagged in sub-array 1. ! A total of 87 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 87 telescope corrections were flagged in sub-array 1. ! A total of 87 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 5. ! A total of 145 telescope corrections were flagged in sub-array 1. ! A total of 145 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 6. ! A total of 145 telescope corrections were flagged in sub-array 1. ! A total of 145 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 7. ! A total of 87 telescope corrections were flagged in sub-array 1. ! A total of 87 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 8. ! A total of 87 telescope corrections were flagged in sub-array 1. ! A total of 87 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=1.004429Jy sigma=10.585064 ! Fit after self-cal, rms=0.950949Jy sigma=10.035512 ! 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 2.65% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 milli-arcsec ! Estimated beam: bmin=0.5007 mas, bmaj=0.6952 mas, bpa=-70.55 degrees ! Estimated noise=0.697448 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 = 0.0402268 Jy ! Component: 100 - total flux cleaned = 0.049456 Jy ! Total flux subtracted in 100 components = 0.049456 Jy ! Clean residual min=-0.002132 max=0.003450 Jy/beam ! Clean residual mean=0.000004 rms=0.000500 Jy/beam ! Combined flux in latest and established models = 0.0494561 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 0.0494561 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=0.075886Jy sigma=0.676916 ! Fit after self-cal, rms=0.074438Jy sigma=0.659764 ! Inverting map ! Your choice of large map pixels excluded 2.65% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00439046 Jy ! Component: 100 - total flux cleaned = 0.00507771 Jy ! Total flux subtracted in 100 components = 0.00507771 Jy ! Clean residual min=-0.002021 max=0.002267 Jy/beam ! Clean residual mean=0.000003 rms=0.000478 Jy/beam ! Combined flux in latest and established models = 0.0545338 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 8 components and 0.0545338 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=0.074178Jy sigma=0.657289 ! Fit after self-cal, rms=0.074167Jy sigma=0.657224 ! Inverting map ! Your choice of large map pixels excluded 2.65% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 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 2.65% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 milli-arcsec ! Estimated beam: bmin=0.7281 mas, bmaj=0.918 mas, bpa=-60.97 degrees ! Estimated noise=0.316998 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 (1.6, -1.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00175941 Jy ! Component: 100 - total flux cleaned = 0.00265767 Jy ! Component: 150 - total flux cleaned = 0.00304903 Jy ! Component: 200 - total flux cleaned = 0.00317731 Jy ! Total flux subtracted in 200 components = 0.00317731 Jy ! Clean residual min=-0.001064 max=0.001124 Jy/beam ! Clean residual mean=0.000000 rms=0.000242 Jy/beam ! Combined flux in latest and established models = 0.0577111 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 28 components and 0.0577111 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=0.074119Jy sigma=0.656710 ! Fit after self-cal, rms=0.074114Jy sigma=0.656613 ! Inverting map ! Your choice of large map pixels excluded 2.65% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7281 x 0.918 at -60.97 degrees (North through East) ! Clean map min=-0.00090295 max=0.052812 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 1.05 EF 1.00* FD 1.00 KP 1.01 ! LA 0.98 MC 1.03 NL 0.96 ON 0.85 ! OV 1.09 PT 0.95 SC 0.88 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.94 EF 1.00* FD 0.99 KP 0.98 ! LA 1.03 MK 1.04 NL 0.98 ON 0.99 ! OV 1.08 PT 0.92 ZC 0.90 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.08 EF 1.00* FD 1.09 KP 1.00 ! LA 1.03 MK 1.11 NL 0.92 ON 0.99 ! OV 1.04 PT 0.94 SC 0.99 ZC 0.95 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 EF 1.00* LA 0.91 MK 0.93 ! OV 0.98 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 EF 1.00* FD 0.96 KP 1.09 ! LA 1.12 MC 0.89 NL 0.94 ON 0.89 ! OV 1.03 PT 1.02 SC 1.10 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 EF 1.00* FD 1.06 KP 1.05 ! LA 1.12 MK 1.03 NL 0.99 ON 0.98 ! OV 1.04 PT 1.01 ZC 0.97 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.13 EF 1.00* FD 1.04 KP 0.99 ! LA 1.04 MK 1.06 NL 0.98 ON 0.94 ! OV 1.03 PT 1.05 SC 1.03 ZC 0.92 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.94 EF 1.00* LA 0.95 MK 0.98 ! OV 1.10 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 EF 1.00* FD 1.00 KP 1.01 ! LA 1.00 MC 0.87 NL 1.02 ON 0.84 ! OV 1.00 PT 1.07 SC 1.08 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 EF 1.00* FD 0.97 KP 0.95 ! LA 1.00 MK 0.99 NL 0.93 ON 1.01 ! OV 1.03 PT 1.03 ZC 0.93 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.05 EF 1.00* FD 1.04 KP 0.92 ! LA 0.98 MK 0.93 NL 0.93 ON 1.12 ! OV 1.11 PT 0.96 SC 1.04 ZC 0.94 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.92 EF 1.00* LA 0.92 MK 0.93 ! OV 1.12 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 EF 1.00* FD 1.00 KP 1.02 ! LA 1.03 MC 0.97 NL 1.08 ON 0.87 ! OV 1.02 PT 1.05 SC 1.08 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 EF 1.00* FD 1.04 KP 0.99 ! LA 1.00 MK 0.98 NL 0.98 ON 1.07 ! OV 1.00 PT 1.03 ZC 1.02 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.07 EF 1.00* FD 1.02 KP 0.93 ! LA 1.00 MK 0.88 NL 0.98 ON 0.96 ! OV 0.98 PT 1.09 SC 1.12 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.91 EF 1.00* LA 0.98 MK 0.87 ! OV 1.06 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.98 KP 0.98 ! LA 0.98 MC 1.05 NL 1.05 ON 0.96 ! OV 1.05 PT 1.00 SC 0.97 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.09 KP 0.90 ! LA 0.99 MK 1.00 NL 1.08 ON 1.04 ! OV 1.15 PT 0.96 ZC 0.96 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.02 KP 0.88 ! LA 1.02 MK 1.14 NL 0.93 ON 1.16 ! OV 1.02 PT 0.95 SC 1.10 ZC 0.96 ! ! A total of 87 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* EF 0.00* LA 0.00* MK 0.00* ! OV 0.00* ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.91 KP 0.96 ! LA 1.02 MC 1.05 NL 1.07 ON 1.00 ! OV 1.06 PT 0.98 SC 0.98 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00 KP 0.87 ! LA 0.99 MK 1.04 NL 0.97 ON 1.21 ! OV 1.05 PT 0.93 ZC 0.91 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.01 KP 0.90 ! LA 1.04 MK 1.07 NL 0.96 ON 1.46 ! OV 1.03 PT 0.92 SC 1.05 ZC 0.86 ! ! A total of 87 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* EF 0.00* LA 0.00* MK 0.00* ! OV 0.00* ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.07 EF 1.00* FD 1.05 KP 0.91 ! LA 0.98 MC 1.07 NL 0.99 ON 1.17 ! OV 0.93 PT 1.00 SC 1.09 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 EF 1.00* FD 1.05 KP 0.91 ! LA 0.99 MK 1.00 NL 1.04 ON 1.20 ! OV 1.04 PT 0.90 ZC 0.79 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 EF 1.00* FD 1.01 KP 0.95 ! LA 1.00 MK 1.05 NL 1.04 ON 1.13 ! OV 0.97 PT 0.98 SC 0.95 ZC 0.82 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.84 EF 1.00* LA 0.96 MK 0.97 ! OV 0.90 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 0.94 EF 1.00* FD 0.98 KP 1.01 ! LA 0.97 MC 1.11 NL 1.04 ON 1.23 ! OV 0.99 PT 0.94 SC 1.05 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.90 EF 1.00* FD 1.02 KP 1.00 ! LA 0.98 MK 1.05 NL 1.02 ON 1.29 ! OV 1.01 PT 1.02 ZC 0.68 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.05 EF 1.00* FD 1.01 KP 0.94 ! LA 1.09 MK 1.07 NL 1.06 ON 1.26 ! OV 1.08 PT 0.95 SC 0.99 ZC 0.77 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.86 EF 1.00* LA 1.01 MK 0.94 ! OV 0.79 ! ! ! Fit before self-cal, rms=0.074114Jy sigma=0.656613 ! Fit after self-cal, rms=0.073736Jy sigma=0.654986 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.66% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 milli-arcsec ! Estimated beam: bmin=0.7221 mas, bmaj=0.9116 mas, bpa=-63.67 degrees ! Estimated noise=0.317702 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 = 0.000482162 Jy ! Component: 100 - total flux cleaned = 0.000585136 Jy ! Component: 150 - total flux cleaned = 0.000640777 Jy ! Component: 200 - total flux cleaned = 0.000681039 Jy ! Total flux subtracted in 200 components = 0.000681039 Jy ! Clean residual min=-0.000951 max=0.000968 Jy/beam ! Clean residual mean=0.000000 rms=0.000217 Jy/beam ! Combined flux in latest and established models = 0.0583921 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 41 components and 0.0583921 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=0.073732Jy sigma=0.654935 ! Fit after self-cal, rms=0.073751Jy sigma=0.654703 ! Inverting map ! Your choice of large map pixels excluded 2.66% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 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=0.073751Jy sigma=0.654703 ! Fit after self-cal, rms=0.074080Jy sigma=0.654160 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.66% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 milli-arcsec ! Estimated beam: bmin=0.7201 mas, bmaj=0.9113 mas, bpa=-63.81 degrees ! Estimated noise=0.318622 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000353824 Jy ! Component: 100 - total flux cleaned = 0.000427441 Jy ! Component: 150 - total flux cleaned = 0.000474302 Jy ! Component: 200 - total flux cleaned = 0.00049158 Jy ! Total flux subtracted in 200 components = 0.00049158 Jy ! Clean residual min=-0.000907 max=0.000931 Jy/beam ! Clean residual mean=0.000002 rms=0.000215 Jy/beam ! Combined flux in latest and established models = 0.0588837 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 47 components and 0.0588837 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=0.074077Jy sigma=0.654137 ! Fit after self-cal, rms=0.074090Jy sigma=0.654052 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.66% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 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) ! Added new window around map position (-40.2, 42.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000743056 Jy ! Component: 100 - total flux cleaned = 0.000827887 Jy ! Component: 150 - total flux cleaned = 0.00085318 Jy ! Component: 200 - total flux cleaned = 0.000900761 Jy ! Total flux subtracted in 200 components = 0.000900761 Jy ! Clean residual min=-0.000916 max=0.000916 Jy/beam ! Clean residual mean=0.000001 rms=0.000215 Jy/beam ! Combined flux in latest and established models = 0.0597845 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 60 components and 0.0597845 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=0.074079Jy sigma=0.653952 ! Fit after self-cal, rms=0.074077Jy sigma=0.653934 ! Inverting map ! Your choice of large map pixels excluded 2.66% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 milli-arcsec ! Added new window around map position (-23, -29.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000855659 Jy ! Component: 100 - total flux cleaned = 0.00119807 Jy ! Component: 150 - total flux cleaned = 0.00122625 Jy ! Component: 200 - total flux cleaned = 0.00126503 Jy ! Total flux subtracted in 200 components = 0.00126503 Jy ! Clean residual min=-0.000933 max=0.000881 Jy/beam ! Clean residual mean=0.000002 rms=0.000211 Jy/beam ! Combined flux in latest and established models = 0.0610495 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 70 components and 0.0610495 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=0.074063Jy sigma=0.653825 ! Fit after self-cal, rms=0.074059Jy sigma=0.653807 ! Inverting map ! Your choice of large map pixels excluded 2.66% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 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=0.074059Jy sigma=0.653807 ! Fit after self-cal, rms=0.074182Jy sigma=0.653777 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.66% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 milli-arcsec ! Estimated beam: bmin=0.7189 mas, bmaj=0.9096 mas, bpa=-63.7 degrees ! Estimated noise=0.319703 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00050952 Jy ! Component: 100 - total flux cleaned = 0.000793905 Jy ! Component: 150 - total flux cleaned = 0.000884379 Jy ! Component: 200 - total flux cleaned = 0.000932324 Jy ! Total flux subtracted in 200 components = 0.000932324 Jy ! Clean residual min=-0.000938 max=0.000896 Jy/beam ! Clean residual mean=0.000002 rms=0.000212 Jy/beam ! Combined flux in latest and established models = 0.0619818 Jy selfcal ! Performing phase self-cal ! Adding 29 model components to the UV plane model. ! The established model now contains 74 components and 0.0619818 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=0.074175Jy sigma=0.653730 ! Fit after self-cal, rms=0.074174Jy sigma=0.653719 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.66% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 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 = 0.000235126 Jy ! Component: 100 - total flux cleaned = 0.00027036 Jy ! Component: 150 - total flux cleaned = 0.000281799 Jy ! Component: 200 - total flux cleaned = 0.000314306 Jy ! Total flux subtracted in 200 components = 0.000314306 Jy ! Clean residual min=-0.000934 max=0.000899 Jy/beam ! Clean residual mean=0.000002 rms=0.000212 Jy/beam ! Combined flux in latest and established models = 0.0622961 Jy ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 79 components and 0.0622961 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=0.074169Jy sigma=0.653690 ! Fit after self-cal, rms=0.074169Jy sigma=0.653687 ! Inverting map ! Your choice of large map pixels excluded 2.66% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 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=0.074169Jy sigma=0.653687 ! Fit after self-cal, rms=0.074205Jy sigma=0.653667 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.66% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 milli-arcsec ! Estimated beam: bmin=2.648 mas, bmaj=2.97 mas, bpa=2.105 degrees ! Estimated noise=0.409904 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000579086 Jy ! Component: 100 - total flux cleaned = 0.000877875 Jy ! Component: 150 - total flux cleaned = 0.00101495 Jy ! Component: 200 - total flux cleaned = 0.00112404 Jy ! Total flux subtracted in 200 components = 0.00112404 Jy ! Clean residual min=-0.001211 max=0.001086 Jy/beam ! Clean residual mean=0.000004 rms=0.000293 Jy/beam ! Combined flux in latest and established models = 0.0634201 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 88 components and 0.0634202 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=0.074206Jy sigma=0.653674 ! Fit after self-cal, rms=0.074205Jy sigma=0.653654 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.66% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 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 = 0.000235339 Jy ! Component: 100 - total flux cleaned = 0.000320691 Jy ! Component: 150 - total flux cleaned = 0.000339435 Jy ! Component: 200 - total flux cleaned = 0.000362831 Jy ! Total flux subtracted in 200 components = 0.000362831 Jy ! Clean residual min=-0.001207 max=0.001059 Jy/beam ! Clean residual mean=0.000004 rms=0.000292 Jy/beam ! Combined flux in latest and established models = 0.063783 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 91 components and 0.063783 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=0.074206Jy sigma=0.653671 ! Fit after self-cal, rms=0.074206Jy sigma=0.653667 ! Inverting map ! Your choice of large map pixels excluded 2.66% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 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 2.66% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 milli-arcsec ! Estimated beam: bmin=0.7178 mas, bmaj=0.9083 mas, bpa=-63.75 degrees ! Estimated noise=0.320502 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7178 x 0.9083 at -63.75 degrees (North through East) ! Clean map min=-0.00076734 max=0.053045 Jy/beam if(peak(flux) > thresh) selfcal true, true clean clean_niter,clean_gain selfcal flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) selfcal true, true end if print "************** CLEARING MODEL AND STARTING OVER **********" ! ************** CLEARING MODEL AND STARTING OVER ********** clrmod true ! clrmod: Cleared the established and tentative models. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.66% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 milli-arcsec ! Estimated beam: bmin=0.4938 mas, bmaj=0.6919 mas, bpa=-73.08 degrees ! Estimated noise=0.692393 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0411896 Jy ! Component: 100 - total flux cleaned = 0.0506602 Jy ! Component: 150 - total flux cleaned = 0.0542412 Jy ! Component: 200 - total flux cleaned = 0.0557152 Jy ! Total flux subtracted in 200 components = 0.0557152 Jy ! Clean residual min=-0.001850 max=0.002252 Jy/beam ! Clean residual mean=0.000003 rms=0.000452 Jy/beam ! Combined flux in latest and established models = 0.0557151 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 13 model components to the UV plane model. ! The established model now contains 13 components and 0.0557151 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.66% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 milli-arcsec ! Estimated beam: bmin=0.7178 mas, bmaj=0.9083 mas, bpa=-63.75 degrees ! Estimated noise=0.320502 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 = 0.00221889 Jy ! Component: 100 - total flux cleaned = 0.00357783 Jy ! Component: 150 - total flux cleaned = 0.0046342 Jy ! Component: 200 - total flux cleaned = 0.00549707 Jy ! Total flux subtracted in 200 components = 0.00549707 Jy ! Clean residual min=-0.000954 max=0.000928 Jy/beam ! Clean residual mean=0.000003 rms=0.000220 Jy/beam ! Combined flux in latest and established models = 0.0612122 Jy ! Adding 24 model components to the UV plane model. ! The established model now contains 32 components and 0.0612122 Jy ! Inverting map ! Your choice of large map pixels excluded 2.66% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 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 2.66% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 milli-arcsec ! Estimated beam: bmin=2.648 mas, bmaj=2.97 mas, bpa=2.105 degrees ! Estimated noise=0.409904 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00104503 Jy ! Component: 100 - total flux cleaned = 0.00163388 Jy ! Component: 150 - total flux cleaned = 0.00204995 Jy ! Component: 200 - total flux cleaned = 0.00232321 Jy ! Total flux subtracted in 200 components = 0.00232321 Jy ! Clean residual min=-0.001202 max=0.001051 Jy/beam ! Clean residual mean=0.000005 rms=0.000295 Jy/beam ! Combined flux in latest and established models = 0.0635354 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 = 9.85365e-05 Jy ! Component: 100 - total flux cleaned = 0.000172869 Jy ! Component: 150 - total flux cleaned = 0.000236201 Jy ! Component: 200 - total flux cleaned = 0.00027914 Jy ! Total flux subtracted in 200 components = 0.00027914 Jy ! Clean residual min=-0.001206 max=0.001053 Jy/beam ! Clean residual mean=0.000004 rms=0.000293 Jy/beam ! Combined flux in latest and established models = 0.0638146 Jy ! Adding 27 model components to the UV plane model. ! The established model now contains 55 components and 0.0638146 Jy ! Inverting map ! Your choice of large map pixels excluded 2.66% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.66% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 milli-arcsec ! Estimated beam: bmin=0.7178 mas, bmaj=0.9083 mas, bpa=-63.75 degrees ! Estimated noise=0.320502 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000319296 Jy ! Component: 100 - total flux cleaned = -0.00029576 Jy ! Component: 150 - total flux cleaned = -0.000276149 Jy ! Component: 200 - total flux cleaned = -0.000241791 Jy ! Total flux subtracted in 200 components = -0.000241791 Jy ! Clean residual min=-0.000943 max=0.000932 Jy/beam ! Clean residual mean=0.000002 rms=0.000213 Jy/beam ! Combined flux in latest and established models = 0.0635728 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 66 components and 0.0635728 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=0.074220Jy sigma=0.653787 ! Fit after self-cal, rms=0.074223Jy sigma=0.653764 wmodel /scr/pima/gb073_uvs/J1725+5851_X_map.mod ! Writing 66 model components to file: /scr/pima/gb073_uvs/J1725+5851_X_map.mod wobs /scr/pima/gb073_uvs/J1725+5851_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1725+5851_X_uvs.fits wwins /scr/pima/gb073_uvs/J1725+5851_X_map.win ! wwins: Wrote 4 windows to /scr/pima/gb073_uvs/J1725+5851_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 2.66% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -8.6141e-05 Jy ! Component: 100 - total flux cleaned = -0.00028002 Jy ! Component: 150 - total flux cleaned = -0.000436037 Jy ! Component: 200 - total flux cleaned = -0.000557941 Jy ! Component: 250 - total flux cleaned = -0.000647371 Jy ! Component: 300 - total flux cleaned = -0.000691288 Jy ! Component: 350 - total flux cleaned = -0.000763133 Jy ! Component: 400 - total flux cleaned = -0.000848354 Jy ! Component: 450 - total flux cleaned = -0.000946256 Jy ! Component: 500 - total flux cleaned = -0.000987737 Jy ! Component: 550 - total flux cleaned = -0.00111039 Jy ! Component: 600 - total flux cleaned = -0.00116434 Jy ! Component: 650 - total flux cleaned = -0.00127098 Jy ! Component: 700 - total flux cleaned = -0.00133696 Jy ! Component: 750 - total flux cleaned = -0.00140208 Jy ! Component: 800 - total flux cleaned = -0.00146667 Jy ! Component: 850 - total flux cleaned = -0.00142808 Jy ! Component: 900 - total flux cleaned = -0.00145368 Jy ! Component: 950 - total flux cleaned = -0.0014915 Jy ! Component: 1000 - total flux cleaned = -0.00151636 Jy ! Component: 1050 - total flux cleaned = -0.00151615 Jy ! Component: 1100 - total flux cleaned = -0.00152839 Jy ! Component: 1150 - total flux cleaned = -0.00154074 Jy ! Component: 1200 - total flux cleaned = -0.00154076 Jy ! Component: 1250 - total flux cleaned = -0.00157684 Jy ! Component: 1300 - total flux cleaned = -0.00160087 Jy ! Component: 1350 - total flux cleaned = -0.00156516 Jy ! Component: 1400 - total flux cleaned = -0.00156526 Jy ! Component: 1450 - total flux cleaned = -0.0015888 Jy ! Component: 1500 - total flux cleaned = -0.00163552 Jy ! Component: 1550 - total flux cleaned = -0.0016703 Jy ! Component: 1600 - total flux cleaned = -0.00163571 Jy ! Component: 1650 - total flux cleaned = -0.00169306 Jy ! Component: 1700 - total flux cleaned = -0.00170457 Jy ! Component: 1750 - total flux cleaned = -0.00165915 Jy ! Component: 1800 - total flux cleaned = -0.00171568 Jy ! Component: 1850 - total flux cleaned = -0.00171568 Jy ! Component: 1900 - total flux cleaned = -0.00171587 Jy ! Component: 1950 - total flux cleaned = -0.0017492 Jy ! Component: 2000 - total flux cleaned = -0.00176032 Jy ! Component: 2050 - total flux cleaned = -0.00174935 Jy ! Component: 2100 - total flux cleaned = -0.00173842 Jy ! Component: 2150 - total flux cleaned = -0.00174934 Jy ! Component: 2200 - total flux cleaned = -0.00173845 Jy ! Component: 2250 - total flux cleaned = -0.00177098 Jy ! Component: 2300 - total flux cleaned = -0.00178176 Jy ! Component: 2350 - total flux cleaned = -0.00178182 Jy ! Component: 2400 - total flux cleaned = -0.00178184 Jy ! Component: 2450 - total flux cleaned = -0.00181375 Jy ! Component: 2500 - total flux cleaned = -0.00179252 Jy ! Component: 2550 - total flux cleaned = -0.00178203 Jy ! Component: 2600 - total flux cleaned = -0.0018345 Jy ! Component: 2650 - total flux cleaned = -0.00182403 Jy ! Component: 2700 - total flux cleaned = -0.00179267 Jy ! Component: 2750 - total flux cleaned = -0.00186552 Jy ! Component: 2800 - total flux cleaned = -0.00185522 Jy ! Component: 2850 - total flux cleaned = -0.00188622 Jy ! Component: 2900 - total flux cleaned = -0.00188617 Jy ! Component: 2950 - total flux cleaned = -0.00192712 Jy ! Component: 3000 - total flux cleaned = -0.00195782 Jy ! Component: 3050 - total flux cleaned = -0.00190687 Jy ! Component: 3100 - total flux cleaned = -0.00193737 Jy ! Component: 3150 - total flux cleaned = -0.00198794 Jy ! Component: 3200 - total flux cleaned = -0.00200811 Jy ! Component: 3250 - total flux cleaned = -0.00198801 Jy ! Component: 3300 - total flux cleaned = -0.00199805 Jy ! Component: 3350 - total flux cleaned = -0.00199808 Jy ! Component: 3400 - total flux cleaned = -0.00199802 Jy ! Component: 3450 - total flux cleaned = -0.00196823 Jy ! Component: 3500 - total flux cleaned = -0.00199789 Jy ! Component: 3550 - total flux cleaned = -0.00198806 Jy ! Component: 3600 - total flux cleaned = -0.00197815 Jy ! Component: 3650 - total flux cleaned = -0.00194876 Jy ! Component: 3700 - total flux cleaned = -0.00189011 Jy ! Component: 3750 - total flux cleaned = -0.00188034 Jy ! Component: 3800 - total flux cleaned = -0.00193867 Jy ! Component: 3850 - total flux cleaned = -0.00193867 Jy ! Component: 3900 - total flux cleaned = -0.001958 Jy ! Component: 3950 - total flux cleaned = -0.00194838 Jy ! Component: 4000 - total flux cleaned = -0.00194838 Jy ! Component: 4050 - total flux cleaned = -0.00195797 Jy ! Total flux subtracted in 4096 components = -0.00195794 Jy ! Clean residual min=-0.000556 max=0.000552 Jy/beam ! Clean residual mean=0.000001 rms=0.000158 Jy/beam ! Combined flux in latest and established models = 0.0616148 Jy keep ! Adding 389 model components to the UV plane model. ! The established model now contains 455 components and 0.0616148 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1725+5851_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 2.66% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7178 x 0.9083 at -63.75 degrees (North through East) ! Clean map min=-0.00062552 max=0.052978 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1725+5851_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0529776 invert ! Inverting map ! Your choice of large map pixels excluded 2.66% of the data. ! The x-axis pixel size should ideally be below 0.1963 milli-arcsec ! The y-axis pixel size should ideally be below 0.1724 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000157537 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.892098 0.892098 1.7842 3.56839 7.13678 14.2736 28.5471 57.0943 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0004 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.052 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 336.285 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1725+5851_X_uvs.log closed on Sat Dec 26 09:42:56 2015