! Started logfile: /scr/pima/gb073_uvs/J2109+8021_X_uvs.log on Sat Dec 26 09:44:56 2015 obs /scr/pima/gb073_uvs/J2109+8021_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J2109+8021_X_uva.fits ! AN table 1: 29 integrations on 36 of 36 possible baselines. ! AN table 2: 29 integrations on 45 of 45 possible baselines. ! AN table 3: 29 integrations on 3 of 3 possible baselines. ! AN table 4: 58 integrations on 55 of 55 possible baselines. ! AN table 5: 58 integrations on 66 of 66 possible baselines. ! AN table 6: 29 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.809927 visibilities/baseline/integration-bin. ! Found source: J2109+8021 ! ! 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 69712 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/J2109+8021_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 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 116 telescope corrections were flagged in sub-array 4. ! A total of 116 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 116 telescope corrections were flagged in sub-array 4. ! A total of 116 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 116 telescope corrections were flagged in sub-array 4. ! A total of 116 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 116 telescope corrections were flagged in sub-array 4. ! A total of 116 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 5. ! A total of 58 telescope corrections were flagged in sub-array 1. ! A total of 87 telescope corrections were flagged in sub-array 2. ! A total of 87 telescope corrections were flagged in sub-array 3. ! A total of 174 telescope corrections were flagged in sub-array 4. ! A total of 174 telescope corrections were flagged in sub-array 5. ! A total of 58 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 6. ! A total of 58 telescope corrections were flagged in sub-array 1. ! A total of 87 telescope corrections were flagged in sub-array 2. ! A total of 87 telescope corrections were flagged in sub-array 3. ! A total of 174 telescope corrections were flagged in sub-array 4. ! A total of 174 telescope corrections were flagged in sub-array 5. ! A total of 58 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 7. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 116 telescope corrections were flagged in sub-array 4. ! A total of 116 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 8. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 116 telescope corrections were flagged in sub-array 4. ! A total of 116 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.004746Jy sigma=10.349070 ! Fit after self-cal, rms=0.947163Jy sigma=9.821965 ! 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 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 milli-arcsec ! Estimated beam: bmin=0.681 mas, bmaj=0.701 mas, bpa=-41.13 degrees ! Estimated noise=0.712296 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 = 0.0403997 Jy ! Component: 100 - total flux cleaned = 0.0497795 Jy ! Total flux subtracted in 100 components = 0.0497795 Jy ! Clean residual min=-0.002307 max=0.003794 Jy/beam ! Clean residual mean=0.000001 rms=0.000545 Jy/beam ! Combined flux in latest and established models = 0.0497795 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 0.0497795 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=0.071779Jy sigma=0.667659 ! Fit after self-cal, rms=0.070512Jy sigma=0.653818 ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00495266 Jy ! Component: 100 - total flux cleaned = 0.00717926 Jy ! Total flux subtracted in 100 components = 0.00717926 Jy ! Clean residual min=-0.002191 max=0.002388 Jy/beam ! Clean residual mean=0.000001 rms=0.000513 Jy/beam ! Combined flux in latest and established models = 0.0569587 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 9 components and 0.0569587 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=0.069994Jy sigma=0.648644 ! Fit after self-cal, rms=0.069981Jy sigma=0.648502 ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 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 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 milli-arcsec ! Estimated beam: bmin=0.9698 mas, bmaj=1.207 mas, bpa=76.14 degrees ! Estimated noise=0.316552 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 = 0.00241087 Jy ! Component: 100 - total flux cleaned = 0.00310433 Jy ! Component: 150 - total flux cleaned = 0.0031017 Jy ! Component: 200 - total flux cleaned = 0.00309923 Jy ! Total flux subtracted in 200 components = 0.00309923 Jy ! Clean residual min=-0.001021 max=0.000988 Jy/beam ! Clean residual mean=0.000002 rms=0.000230 Jy/beam ! Combined flux in latest and established models = 0.0600579 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 14 components and 0.0600579 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=0.069890Jy sigma=0.647821 ! Fit after self-cal, rms=0.069892Jy sigma=0.647721 ! Inverting map ! Your choice of large map pixels excluded 5.97% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.9698 x 1.207 at 76.14 degrees (North through East) ! Clean map min=-0.00091145 max=0.056746 Jy/beam if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val ! Selfcal amplitude corrections will be limited to 0.833333 -> 1.2. ! Selfcal phase corrections will not be limited. gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* OV 1.00* PT 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 EF 1.00* FD 0.96 KP 1.03 ! LA 0.96 NL 0.94 OV 0.99 PT 1.01 ! SC 0.95 ZC 0.91 ! ! A total of 87 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* MK 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! PT 1.00* ZC 1.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 EF 1.00* FD 1.14 KP 1.03 ! LA 1.10 NL 0.93 OV 1.04 PT 0.99 ! ZC 0.95 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.93 EF 1.00* FD 1.06 KP 1.13 ! LA 1.18 NL 0.98 OV 1.06 PT 1.04 ! SC 0.94 ZC 1.09 ! ! A total of 87 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* MK 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! PT 1.00* ZC 1.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 EF 1.00* FD 1.01 KP 0.98 ! LA 1.03 NL 0.94 OV 1.12 PT 0.96 ! ZC 0.97 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.98 EF 1.00* FD 0.92 KP 0.97 ! LA 1.05 NL 1.07 OV 1.01 PT 1.03 ! SC 0.95 ZC 0.95 ! ! A total of 87 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* MK 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! PT 1.00* ZC 1.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 EF 1.00* FD 1.11 KP 0.92 ! LA 1.01 NL 0.95 OV 1.05 PT 0.98 ! ZC 1.00 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.11 EF 1.00* FD 1.04 KP 1.03 ! LA 1.04 NL 0.99 OV 1.03 PT 1.06 ! SC 0.99 ZC 1.13 ! ! A total of 87 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* MK 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! PT 1.00* ZC 1.00* ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.90 KP 0.85 ! LA 1.06 NL 0.99 OV 1.16 PT 0.92 ! ZC 0.84 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 0.94 KP 0.99 ! LA 0.94 NL 1.07 OV 1.03 PT 0.96 ! SC 0.98 ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* MK 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! PT 1.00* ZC 1.00* ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* OV 1.00* PT 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* MK 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 0.95 KP 0.99 ! LA 0.94 MK 1.00 NL 0.99 ON 0.86 ! OV 1.02 PT 1.06 SC 1.04 ZC 1.16 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! PT 1.00* ZC 1.00* ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* OV 1.00* PT 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! A total of 87 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* MK 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 EF 1.00* FD 1.08 KP 0.98 ! LA 1.04 MK 0.96 NL 0.99 ON 0.86 ! OV 0.99 PT 0.99 SC 1.03 ZC 0.91 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! PT 1.00* ZC 1.00* ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* OV 1.00* PT 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! A total of 87 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 0.00* MK 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! PT 1.00* ZC 1.00* ! ! ! Fit before self-cal, rms=0.069892Jy sigma=0.647721 ! Fit after self-cal, rms=0.070071Jy sigma=0.648264 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 6.03% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 milli-arcsec ! Estimated beam: bmin=0.9683 mas, bmaj=1.202 mas, bpa=75.23 degrees ! Estimated noise=0.319014 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 = 0.000377727 Jy ! Component: 100 - total flux cleaned = 0.000380905 Jy ! Component: 150 - total flux cleaned = 0.000380987 Jy ! Component: 200 - total flux cleaned = 0.000380483 Jy ! Total flux subtracted in 200 components = 0.000380483 Jy ! Clean residual min=-0.000948 max=0.000954 Jy/beam ! Clean residual mean=0.000001 rms=0.000222 Jy/beam ! Combined flux in latest and established models = 0.0604384 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 17 components and 0.0604384 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=0.070052Jy sigma=0.648131 ! Fit after self-cal, rms=0.070057Jy sigma=0.648084 ! Inverting map ! Your choice of large map pixels excluded 6.03% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 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=0.070057Jy sigma=0.648084 ! Fit after self-cal, rms=0.070536Jy sigma=0.647436 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.03% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 milli-arcsec ! Estimated beam: bmin=0.9693 mas, bmaj=1.199 mas, bpa=75.43 degrees ! Estimated noise=0.321097 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000389534 Jy ! Component: 100 - total flux cleaned = 0.000387658 Jy ! Component: 150 - total flux cleaned = 0.000386173 Jy ! Component: 200 - total flux cleaned = 0.000368442 Jy ! Total flux subtracted in 200 components = 0.000368442 Jy ! Clean residual min=-0.000908 max=0.000937 Jy/beam ! Clean residual mean=0.000001 rms=0.000216 Jy/beam ! Combined flux in latest and established models = 0.0608069 Jy selfcal ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 17 components and 0.0608069 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=0.070515Jy sigma=0.647366 ! Fit after self-cal, rms=0.070528Jy sigma=0.647314 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.03% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 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 (34, -50). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000566115 Jy ! Component: 100 - total flux cleaned = 0.000547365 Jy ! Component: 150 - total flux cleaned = 0.000547586 Jy ! Component: 200 - total flux cleaned = 0.000530983 Jy ! Total flux subtracted in 200 components = 0.000530983 Jy ! Clean residual min=-0.000916 max=0.000867 Jy/beam ! Clean residual mean=0.000001 rms=0.000214 Jy/beam ! Combined flux in latest and established models = 0.0613378 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 26 components and 0.0613378 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=0.070514Jy sigma=0.647194 ! Fit after self-cal, rms=0.070511Jy sigma=0.647177 ! Inverting map ! Your choice of large map pixels excluded 6.03% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 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=0.070511Jy sigma=0.647177 ! Fit after self-cal, rms=0.070870Jy sigma=0.647125 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.03% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 milli-arcsec ! Estimated beam: bmin=0.9699 mas, bmaj=1.197 mas, bpa=75.38 degrees ! Estimated noise=0.32257 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000453067 Jy ! Component: 100 - total flux cleaned = 0.000434748 Jy ! Component: 150 - total flux cleaned = 0.000416974 Jy ! Component: 200 - total flux cleaned = 0.000416953 Jy ! Total flux subtracted in 200 components = 0.000416953 Jy ! Clean residual min=-0.000898 max=0.000838 Jy/beam ! Clean residual mean=0.000001 rms=0.000213 Jy/beam ! Combined flux in latest and established models = 0.0617548 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 27 components and 0.0617548 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=0.070855Jy sigma=0.647061 ! Fit after self-cal, rms=0.070856Jy sigma=0.647053 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.03% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 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 = 5.86148e-05 Jy ! Component: 100 - total flux cleaned = 4.27499e-05 Jy ! Component: 150 - total flux cleaned = 1.24833e-05 Jy ! Component: 200 - total flux cleaned = 1.22103e-05 Jy ! Total flux subtracted in 200 components = 1.22103e-05 Jy ! Clean residual min=-0.000891 max=0.000841 Jy/beam ! Clean residual mean=0.000001 rms=0.000212 Jy/beam ! Combined flux in latest and established models = 0.061767 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 28 components and 0.061767 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=0.070847Jy sigma=0.647004 ! Fit after self-cal, rms=0.070845Jy sigma=0.647001 ! Inverting map ! Your choice of large map pixels excluded 6.03% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 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=0.070845Jy sigma=0.647001 ! Fit after self-cal, rms=0.070904Jy sigma=0.646842 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.03% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 milli-arcsec ! Estimated beam: bmin=2.607 mas, bmaj=3.638 mas, bpa=71.69 degrees ! Estimated noise=0.3839 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000100965 Jy ! Component: 100 - total flux cleaned = 0.000120477 Jy ! Component: 150 - total flux cleaned = 0.000129502 Jy ! Component: 200 - total flux cleaned = 0.000145921 Jy ! Total flux subtracted in 200 components = 0.000145921 Jy ! Clean residual min=-0.000829 max=0.000804 Jy/beam ! Clean residual mean=0.000001 rms=0.000213 Jy/beam ! Combined flux in latest and established models = 0.0619129 Jy selfcal ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 32 components and 0.0619129 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=0.070903Jy sigma=0.646814 ! Fit after self-cal, rms=0.070900Jy sigma=0.646784 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.03% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 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 = 6.93625e-06 Jy ! Component: 100 - total flux cleaned = 1.50753e-05 Jy ! Component: 150 - total flux cleaned = 2.30936e-05 Jy ! Component: 200 - total flux cleaned = 3.67066e-05 Jy ! Total flux subtracted in 200 components = 3.67066e-05 Jy ! Clean residual min=-0.000823 max=0.000804 Jy/beam ! Clean residual mean=0.000001 rms=0.000213 Jy/beam ! Combined flux in latest and established models = 0.0619496 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 34 components and 0.0619496 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=0.070899Jy sigma=0.646768 ! Fit after self-cal, rms=0.070898Jy sigma=0.646763 ! Inverting map ! Your choice of large map pixels excluded 6.03% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 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 6.03% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 milli-arcsec ! Estimated beam: bmin=0.971 mas, bmaj=1.194 mas, bpa=75.39 degrees ! Estimated noise=0.323006 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.971 x 1.194 at 75.39 degrees (North through East) ! Clean map min=-0.00082552 max=0.058614 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 6.03% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 milli-arcsec ! Estimated beam: bmin=0.6728 mas, bmaj=0.6987 mas, bpa=-31.86 degrees ! Estimated noise=0.725225 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0420791 Jy ! Component: 100 - total flux cleaned = 0.0521814 Jy ! Component: 150 - total flux cleaned = 0.0565242 Jy ! Component: 200 - total flux cleaned = 0.0589257 Jy ! Total flux subtracted in 200 components = 0.0589257 Jy ! Clean residual min=-0.002306 max=0.002417 Jy/beam ! Clean residual mean=0.000001 rms=0.000518 Jy/beam ! Combined flux in latest and established models = 0.0589257 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 0.0589257 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 6.03% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 milli-arcsec ! Estimated beam: bmin=0.971 mas, bmaj=1.194 mas, bpa=75.39 degrees ! Estimated noise=0.323006 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 = 0.00228399 Jy ! Component: 100 - total flux cleaned = 0.00278888 Jy ! Component: 150 - total flux cleaned = 0.00297193 Jy ! Component: 200 - total flux cleaned = 0.00296986 Jy ! Total flux subtracted in 200 components = 0.00296986 Jy ! Clean residual min=-0.000985 max=0.000906 Jy/beam ! Clean residual mean=0.000001 rms=0.000217 Jy/beam ! Combined flux in latest and established models = 0.0618955 Jy ! Adding 14 model components to the UV plane model. ! The established model now contains 21 components and 0.0618955 Jy ! Inverting map ! Your choice of large map pixels excluded 6.03% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 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 6.03% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 milli-arcsec ! Estimated beam: bmin=2.607 mas, bmaj=3.638 mas, bpa=71.69 degrees ! Estimated noise=0.3839 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000244722 Jy ! Component: 100 - total flux cleaned = 0.000258038 Jy ! Component: 150 - total flux cleaned = 0.000271186 Jy ! Component: 200 - total flux cleaned = 0.000294882 Jy ! Total flux subtracted in 200 components = 0.000294882 Jy ! Clean residual min=-0.000824 max=0.000794 Jy/beam ! Clean residual mean=0.000002 rms=0.000213 Jy/beam ! Combined flux in latest and established models = 0.0621904 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 = 2.11906e-05 Jy ! Component: 100 - total flux cleaned = 2.17872e-05 Jy ! Component: 150 - total flux cleaned = 2.21825e-05 Jy ! Component: 200 - total flux cleaned = 2.2952e-05 Jy ! Total flux subtracted in 200 components = 2.2952e-05 Jy ! Clean residual min=-0.000824 max=0.000797 Jy/beam ! Clean residual mean=0.000002 rms=0.000213 Jy/beam ! Combined flux in latest and established models = 0.0622134 Jy ! Adding 10 model components to the UV plane model. ! The established model now contains 28 components and 0.0622133 Jy ! Inverting map ! Your choice of large map pixels excluded 6.03% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 6.03% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 milli-arcsec ! Estimated beam: bmin=0.971 mas, bmaj=1.194 mas, bpa=75.39 degrees ! Estimated noise=0.323006 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 4.90477e-06 Jy ! Component: 100 - total flux cleaned = -4.84229e-05 Jy ! Component: 150 - total flux cleaned = -0.000147021 Jy ! Component: 200 - total flux cleaned = -0.000192695 Jy ! Total flux subtracted in 200 components = -0.000192695 Jy ! Clean residual min=-0.000937 max=0.000879 Jy/beam ! Clean residual mean=0.000001 rms=0.000211 Jy/beam ! Combined flux in latest and established models = 0.0620207 Jy selfcal ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 30 components and 0.0620207 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=0.070928Jy sigma=0.646943 ! Fit after self-cal, rms=0.070930Jy sigma=0.646931 wmodel /scr/pima/gb073_uvs/J2109+8021_X_map.mod ! Writing 30 model components to file: /scr/pima/gb073_uvs/J2109+8021_X_map.mod wobs /scr/pima/gb073_uvs/J2109+8021_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J2109+8021_X_uvs.fits wwins /scr/pima/gb073_uvs/J2109+8021_X_map.win ! wwins: Wrote 2 windows to /scr/pima/gb073_uvs/J2109+8021_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 6.03% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000137533 Jy ! Component: 100 - total flux cleaned = -0.000294714 Jy ! Component: 150 - total flux cleaned = -0.000371015 Jy ! Component: 200 - total flux cleaned = -0.000445003 Jy ! Component: 250 - total flux cleaned = -0.000575345 Jy ! Component: 300 - total flux cleaned = -0.000603536 Jy ! Component: 350 - total flux cleaned = -0.000645826 Jy ! Component: 400 - total flux cleaned = -0.000701171 Jy ! Component: 450 - total flux cleaned = -0.000673896 Jy ! Component: 500 - total flux cleaned = -0.000741782 Jy ! Component: 550 - total flux cleaned = -0.000755101 Jy ! Component: 600 - total flux cleaned = -0.000768407 Jy ! Component: 650 - total flux cleaned = -0.000781578 Jy ! Component: 700 - total flux cleaned = -0.000820842 Jy ! Component: 750 - total flux cleaned = -0.000859544 Jy ! Component: 800 - total flux cleaned = -0.000885191 Jy ! Component: 850 - total flux cleaned = -0.000885183 Jy ! Component: 900 - total flux cleaned = -0.000935791 Jy ! Component: 950 - total flux cleaned = -0.000898169 Jy ! Component: 1000 - total flux cleaned = -0.000998 Jy ! Component: 1050 - total flux cleaned = -0.00103517 Jy ! Component: 1100 - total flux cleaned = -0.00103519 Jy ! Component: 1150 - total flux cleaned = -0.00107191 Jy ! Component: 1200 - total flux cleaned = -0.00115696 Jy ! Component: 1250 - total flux cleaned = -0.0011811 Jy ! Component: 1300 - total flux cleaned = -0.00120513 Jy ! Component: 1350 - total flux cleaned = -0.00126489 Jy ! Component: 1400 - total flux cleaned = -0.00128853 Jy ! Component: 1450 - total flux cleaned = -0.00134751 Jy ! Component: 1500 - total flux cleaned = -0.00135928 Jy ! Component: 1550 - total flux cleaned = -0.0014408 Jy ! Component: 1600 - total flux cleaned = -0.00147556 Jy ! Component: 1650 - total flux cleaned = -0.00149862 Jy ! Component: 1700 - total flux cleaned = -0.00156764 Jy ! Component: 1750 - total flux cleaned = -0.00162481 Jy ! Component: 1800 - total flux cleaned = -0.00164761 Jy ! Component: 1850 - total flux cleaned = -0.00163628 Jy ! Component: 1900 - total flux cleaned = -0.00169259 Jy ! Component: 1950 - total flux cleaned = -0.00174866 Jy ! Component: 2000 - total flux cleaned = -0.00180445 Jy ! Component: 2050 - total flux cleaned = -0.00184891 Jy ! Component: 2100 - total flux cleaned = -0.00188208 Jy ! Component: 2150 - total flux cleaned = -0.00191508 Jy ! Component: 2200 - total flux cleaned = -0.00192605 Jy ! Component: 2250 - total flux cleaned = -0.00194784 Jy ! Component: 2300 - total flux cleaned = -0.00200221 Jy ! Component: 2350 - total flux cleaned = -0.00200222 Jy ! Component: 2400 - total flux cleaned = -0.00205603 Jy ! Component: 2450 - total flux cleaned = -0.00209901 Jy ! Component: 2500 - total flux cleaned = -0.00208843 Jy ! Component: 2550 - total flux cleaned = -0.00216287 Jy ! Component: 2600 - total flux cleaned = -0.00216293 Jy ! Component: 2650 - total flux cleaned = -0.00221569 Jy ! Component: 2700 - total flux cleaned = -0.00222624 Jy ! Component: 2750 - total flux cleaned = -0.00220526 Jy ! Component: 2800 - total flux cleaned = -0.00224693 Jy ! Component: 2850 - total flux cleaned = -0.00226774 Jy ! Component: 2900 - total flux cleaned = -0.00228839 Jy ! Component: 2950 - total flux cleaned = -0.00235023 Jy ! Component: 3000 - total flux cleaned = -0.00235025 Jy ! Component: 3050 - total flux cleaned = -0.00237067 Jy ! Component: 3100 - total flux cleaned = -0.0024114 Jy ! Component: 3150 - total flux cleaned = -0.00244184 Jy ! Component: 3200 - total flux cleaned = -0.0024216 Jy ! Component: 3250 - total flux cleaned = -0.00246193 Jy ! Component: 3300 - total flux cleaned = -0.00249209 Jy ! Component: 3350 - total flux cleaned = -0.00250213 Jy ! Component: 3400 - total flux cleaned = -0.002552 Jy ! Component: 3450 - total flux cleaned = -0.00257187 Jy ! Component: 3500 - total flux cleaned = -0.00257189 Jy ! Component: 3550 - total flux cleaned = -0.00259162 Jy ! Component: 3600 - total flux cleaned = -0.00262118 Jy ! Component: 3650 - total flux cleaned = -0.00268013 Jy ! Component: 3700 - total flux cleaned = -0.00270944 Jy ! Component: 3750 - total flux cleaned = -0.00275813 Jy ! Component: 3800 - total flux cleaned = -0.00273866 Jy ! Component: 3850 - total flux cleaned = -0.00277747 Jy ! Component: 3900 - total flux cleaned = -0.00280653 Jy ! Component: 3950 - total flux cleaned = -0.00285472 Jy ! Component: 4000 - total flux cleaned = -0.00287394 Jy ! Component: 4050 - total flux cleaned = -0.00289312 Jy ! Total flux subtracted in 4096 components = -0.00292178 Jy ! Clean residual min=-0.000532 max=0.000546 Jy/beam ! Clean residual mean=0.000001 rms=0.000163 Jy/beam ! Combined flux in latest and established models = 0.0590989 Jy keep ! Adding 330 model components to the UV plane model. ! The established model now contains 360 components and 0.0590989 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J2109+8021_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 6.03% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.971 x 1.194 at 75.39 degrees (North through East) ! Clean map min=-0.00077727 max=0.057783 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J2109+8021_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.057783 invert ! Inverting map ! Your choice of large map pixels excluded 6.03% of the data. ! The x-axis pixel size should ideally be below 0.1825 milli-arcsec ! The y-axis pixel size should ideally be below 0.1825 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000163227 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.847447 0.847447 1.69489 3.38979 6.77958 13.5592 27.1183 54.2366 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0004 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.057 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 354.004 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J2109+8021_X_uvs.log closed on Sat Dec 26 09:45:03 2015