! Started logfile: /scr/pima/gb073_uvs/J1159+0112_X_uvs.log on Sat Dec 26 09:37:29 2015 obs /scr/pima/gb073_uvs/J1159+0112_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1159+0112_X_uva.fits ! AN table 1: 20 integrations on 55 of 55 possible baselines. ! AN table 2: 17 integrations on 6 of 6 possible baselines. ! AN table 3: 18 integrations on 15 of 15 possible baselines. ! AN table 4: 23 integrations on 66 of 66 possible baselines. ! AN table 5: 69 integrations on 10 of 10 possible baselines. ! AN table 6: 38 integrations on 15 of 15 possible baselines. ! AN table 7: 9 integrations on 28 of 28 possible baselines. ! Apparent sampling: 0.633718 visibilities/baseline/integration-bin. ! Found source: J1159+0112 ! ! 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 22824 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/J1159+0112_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 38 telescope corrections were flagged in sub-array 1. ! A total of 26 telescope corrections were flagged in sub-array 2. ! A total of 52 telescope corrections were flagged in sub-array 3. ! A total of 66 telescope corrections were flagged in sub-array 4. ! A total of 83 telescope corrections were flagged in sub-array 5. ! A total of 56 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 38 telescope corrections were flagged in sub-array 1. ! A total of 26 telescope corrections were flagged in sub-array 2. ! A total of 52 telescope corrections were flagged in sub-array 3. ! A total of 66 telescope corrections were flagged in sub-array 4. ! A total of 83 telescope corrections were flagged in sub-array 5. ! A total of 56 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 38 telescope corrections were flagged in sub-array 1. ! A total of 26 telescope corrections were flagged in sub-array 2. ! A total of 52 telescope corrections were flagged in sub-array 3. ! A total of 66 telescope corrections were flagged in sub-array 4. ! A total of 83 telescope corrections were flagged in sub-array 5. ! A total of 56 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 38 telescope corrections were flagged in sub-array 1. ! A total of 26 telescope corrections were flagged in sub-array 2. ! A total of 52 telescope corrections were flagged in sub-array 3. ! A total of 66 telescope corrections were flagged in sub-array 4. ! A total of 83 telescope corrections were flagged in sub-array 5. ! A total of 56 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 5. ! A total of 57 telescope corrections were flagged in sub-array 1. ! A total of 26 telescope corrections were flagged in sub-array 2. ! A total of 52 telescope corrections were flagged in sub-array 3. ! A total of 86 telescope corrections were flagged in sub-array 4. ! A total of 83 telescope corrections were flagged in sub-array 5. ! A total of 56 telescope corrections were flagged in sub-array 6. ! A total of 9 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 6. ! A total of 57 telescope corrections were flagged in sub-array 1. ! A total of 26 telescope corrections were flagged in sub-array 2. ! A total of 52 telescope corrections were flagged in sub-array 3. ! A total of 86 telescope corrections were flagged in sub-array 4. ! A total of 83 telescope corrections were flagged in sub-array 5. ! A total of 56 telescope corrections were flagged in sub-array 6. ! A total of 9 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 7. ! A total of 38 telescope corrections were flagged in sub-array 1. ! A total of 26 telescope corrections were flagged in sub-array 2. ! A total of 52 telescope corrections were flagged in sub-array 3. ! A total of 66 telescope corrections were flagged in sub-array 4. ! A total of 83 telescope corrections were flagged in sub-array 5. ! A total of 56 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 8. ! A total of 38 telescope corrections were flagged in sub-array 1. ! A total of 26 telescope corrections were flagged in sub-array 2. ! A total of 52 telescope corrections were flagged in sub-array 3. ! A total of 66 telescope corrections were flagged in sub-array 4. ! A total of 83 telescope corrections were flagged in sub-array 5. ! A total of 56 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.009904Jy sigma=8.031136 ! Fit after self-cal, rms=0.877265Jy sigma=7.007791 ! 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 5.2% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=0.7009 mas, bmaj=0.8112 mas, bpa=-80.63 degrees ! Estimated noise=1.24616 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 = 0.0986117 Jy ! Component: 100 - total flux cleaned = 0.124239 Jy ! Total flux subtracted in 100 components = 0.124239 Jy ! Clean residual min=-0.005966 max=0.010540 Jy/beam ! Clean residual mean=-0.000001 rms=0.001171 Jy/beam ! Combined flux in latest and established models = 0.124239 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.124239 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=0.103012Jy sigma=0.654800 ! Fit after self-cal, rms=0.102486Jy sigma=0.652890 ! Inverting map ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0118081 Jy ! Component: 100 - total flux cleaned = 0.0179871 Jy ! Total flux subtracted in 100 components = 0.0179871 Jy ! Clean residual min=-0.004913 max=0.004513 Jy/beam ! Clean residual mean=0.000002 rms=0.000956 Jy/beam ! Combined flux in latest and established models = 0.142226 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 9 components and 0.142226 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=0.100989Jy sigma=0.638420 ! Fit after self-cal, rms=0.100915Jy sigma=0.638205 ! Inverting map ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.165 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 5.2% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=0.8237 mas, bmaj=0.9737 mas, bpa=-83.02 degrees ! Estimated noise=0.706177 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 = 0.00361339 Jy ! Component: 100 - total flux cleaned = 0.00370724 Jy ! Component: 150 - total flux cleaned = 0.0037122 Jy ! Component: 200 - total flux cleaned = 0.00363 Jy ! Total flux subtracted in 200 components = 0.00363 Jy ! Clean residual min=-0.004959 max=0.003886 Jy/beam ! Clean residual mean=0.000002 rms=0.000815 Jy/beam ! Combined flux in latest and established models = 0.145856 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 14 components and 0.145856 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=0.100720Jy sigma=0.637260 ! Fit after self-cal, rms=0.100751Jy sigma=0.637198 ! Inverting map ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8237 x 0.9737 at -83.02 degrees (North through East) ! Clean map min=-0.0043399 max=0.12987 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* HH 1.00* ! KP 1.00* LA 1.00* MC 1.00* NL 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! A total of 42 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 0.94 MC 0.85 NL 1.00* ! SC 1.10 ZC 0.93 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! KP 1.00* LA 1.00* MC 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! A total of 42 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 0.97 MC 0.92 ON 0.89 ! SC 1.06 ZC 0.83 ! ! Telescope amplitude corrections in sub-array 7: ! BR 0.99 FD 1.01 KP 0.94 LA 1.00 ! MK 1.03 NL 0.92 PT 0.96 SC 1.05 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 EF 1.00* FD 1.05 HH 1.03 ! KP 1.06 LA 1.02 MC 0.90 NL 0.95 ! OV 1.04 PT 1.03 SC 1.02 ! ! A total of 42 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 1.00* MC 1.00* NL 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! KP 1.00* LA 1.00* MC 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! A total of 42 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 0.91 MC 1.00 ON 0.90 ! SC 0.90 ZC 0.92 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.06 FD 1.06 KP 1.08 LA 1.01 ! MK 1.03 NL 0.97 PT 1.08 SC 0.94 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! KP 1.00* LA 1.00* MC 1.00* NL 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! A total of 42 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 1.00* MC 1.00* NL 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! KP 1.00* LA 1.00* MC 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! A total of 42 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 0.99 FD 1.03 KP 0.93 LA 0.97 ! MK 1.02 NL 0.93 PT 1.01 SC 1.08 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! KP 1.00* LA 1.00* MC 1.00* NL 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! A total of 42 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 1.00* MC 1.00* NL 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! KP 1.00* LA 1.00* MC 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! A total of 42 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 0.98 MC 0.93 ON 0.90 ! SC 1.13 ZC 0.86 ! ! Telescope amplitude corrections in sub-array 7: ! BR 0.97 FD 1.05 KP 1.01 LA 0.98 ! MK 1.12 NL 0.94 PT 1.04 SC 1.12 ! ! ! Correcting IF 5. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! KP 1.00* LA 1.00* MC 1.00* NL 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! A total of 42 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 1.00* MC 1.00* NL 1.00* ! SC 1.00* ZC 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! KP 1.00* LA 1.00* MC 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! A total of 42 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* FD 0.94 KP 0.95 LA 0.98 ! MK 1.02 NL 0.98 PT 0.96 SC 1.01 ! ! ! Correcting IF 6. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! KP 1.00* LA 1.00* MC 1.00* NL 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! A total of 42 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 1.00* MC 1.00* NL 1.00* ! SC 1.00* ZC 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! KP 1.00* LA 1.00* MC 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! A total of 42 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* FD 1.01 KP 0.92 LA 1.01 ! MK 1.07 NL 0.99 PT 1.01 SC 1.02 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! KP 1.00* LA 1.00* MC 1.00* NL 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! A total of 42 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 1.00* MC 1.00* NL 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! KP 1.00* LA 1.00* MC 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! A total of 42 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.02 FD 0.99 KP 0.94 LA 1.04 ! MK 1.18 NL 1.12 PT 0.99 SC 1.01 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! KP 1.00* LA 1.00* MC 1.00* NL 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! A total of 42 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* HH 1.00* MC 1.00* NL 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! KP 1.00* LA 1.00* MC 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! A total of 42 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.02 FD 1.07 KP 0.83 LA 1.07 ! MK 1.15 NL 1.04 PT 1.01 SC 1.02 ! ! ! Fit before self-cal, rms=0.100751Jy sigma=0.637198 ! Fit after self-cal, rms=0.099435Jy sigma=0.637760 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=0.8595 mas, bmaj=0.964 mas, bpa=-78.97 degrees ! Estimated noise=0.711256 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 = -0.000533355 Jy ! Component: 100 - total flux cleaned = -0.000606218 Jy ! Component: 150 - total flux cleaned = -0.000666201 Jy ! Component: 200 - total flux cleaned = -0.000665929 Jy ! Total flux subtracted in 200 components = -0.000665929 Jy ! Clean residual min=-0.004211 max=0.003276 Jy/beam ! Clean residual mean=0.000003 rms=0.000738 Jy/beam ! Combined flux in latest and established models = 0.14519 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 14 components and 0.14519 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=0.099382Jy sigma=0.637433 ! Fit after self-cal, rms=0.099449Jy sigma=0.637355 ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.165 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=0.099449Jy sigma=0.637355 ! Fit after self-cal, rms=0.099598Jy sigma=0.636562 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=0.86 mas, bmaj=0.9651 mas, bpa=-79.24 degrees ! Estimated noise=0.711042 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00012482 Jy ! Component: 100 - total flux cleaned = -0.00023947 Jy ! Component: 150 - total flux cleaned = -0.000239209 Jy ! Component: 200 - total flux cleaned = -0.00028919 Jy ! Total flux subtracted in 200 components = -0.00028919 Jy ! Clean residual min=-0.003892 max=0.003170 Jy/beam ! Clean residual mean=0.000003 rms=0.000704 Jy/beam ! Combined flux in latest and established models = 0.144901 Jy selfcal ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 14 components and 0.144901 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=0.099566Jy sigma=0.636411 ! Fit after self-cal, rms=0.099663Jy sigma=0.636299 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.165 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 = 3.34263e-05 Jy ! Component: 100 - total flux cleaned = -6.08258e-05 Jy ! Component: 150 - total flux cleaned = -0.000104034 Jy ! Component: 200 - total flux cleaned = -0.000105338 Jy ! Total flux subtracted in 200 components = -0.000105338 Jy ! Clean residual min=-0.003926 max=0.003106 Jy/beam ! Clean residual mean=0.000003 rms=0.000702 Jy/beam ! Combined flux in latest and established models = 0.144796 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 14 components and 0.144796 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=0.099650Jy sigma=0.636285 ! Fit after self-cal, rms=0.099676Jy sigma=0.636260 ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.165 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=0.099676Jy sigma=0.636260 ! Fit after self-cal, rms=0.099561Jy sigma=0.636160 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=0.8601 mas, bmaj=0.9645 mas, bpa=-79.05 degrees ! Estimated noise=0.710715 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -9.58277e-05 Jy ! Component: 100 - total flux cleaned = -0.000267514 Jy ! Component: 150 - total flux cleaned = -0.000305046 Jy ! Component: 200 - total flux cleaned = -0.000341315 Jy ! Total flux subtracted in 200 components = -0.000341315 Jy ! Clean residual min=-0.003857 max=0.003123 Jy/beam ! Clean residual mean=0.000003 rms=0.000693 Jy/beam ! Combined flux in latest and established models = 0.144454 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 15 components and 0.144454 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=0.099560Jy sigma=0.636187 ! Fit after self-cal, rms=0.099579Jy sigma=0.636147 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.165 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 = 7.31306e-05 Jy ! Component: 100 - total flux cleaned = -3.60485e-05 Jy ! Component: 150 - total flux cleaned = -6.90915e-05 Jy ! Component: 200 - total flux cleaned = -0.000102146 Jy ! Total flux subtracted in 200 components = -0.000102146 Jy ! Clean residual min=-0.003854 max=0.003082 Jy/beam ! Clean residual mean=0.000003 rms=0.000689 Jy/beam ! Combined flux in latest and established models = 0.144352 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 15 components and 0.144352 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=0.099584Jy sigma=0.636219 ! Fit after self-cal, rms=0.099603Jy sigma=0.636203 ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.165 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=0.099603Jy sigma=0.636203 ! Fit after self-cal, rms=0.099501Jy sigma=0.636050 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=2.655 mas, bmaj=3.375 mas, bpa=-3.245 degrees ! Estimated noise=0.8466 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000634499 Jy ! Component: 100 - total flux cleaned = -0.000657417 Jy ! Component: 150 - total flux cleaned = -0.000678641 Jy ! Component: 200 - total flux cleaned = -0.00068248 Jy ! Total flux subtracted in 200 components = -0.00068248 Jy ! Clean residual min=-0.003913 max=0.003149 Jy/beam ! Clean residual mean=0.000004 rms=0.000896 Jy/beam ! Combined flux in latest and established models = 0.14367 Jy selfcal ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 19 components and 0.14367 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=0.099471Jy sigma=0.635880 ! Fit after self-cal, rms=0.099473Jy sigma=0.635851 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.165 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 = 3.34395e-06 Jy ! Component: 100 - total flux cleaned = -1.73635e-05 Jy ! Component: 150 - total flux cleaned = -1.73828e-05 Jy ! Component: 200 - total flux cleaned = -2.14576e-05 Jy ! Total flux subtracted in 200 components = -2.14576e-05 Jy ! Clean residual min=-0.003904 max=0.003138 Jy/beam ! Clean residual mean=0.000004 rms=0.000895 Jy/beam ! Combined flux in latest and established models = 0.143648 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 19 components and 0.143648 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=0.099447Jy sigma=0.635746 ! Fit after self-cal, rms=0.099450Jy sigma=0.635731 ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.165 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 5.36% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=0.8594 mas, bmaj=0.9643 mas, bpa=-79.26 degrees ! Estimated noise=0.710405 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8594 x 0.9643 at -79.26 degrees (North through East) ! Clean map min=-0.0034725 max=0.13118 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 5.36% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=0.7181 mas, bmaj=0.8077 mas, bpa=-78.85 degrees ! Estimated noise=1.30848 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0992276 Jy ! Component: 100 - total flux cleaned = 0.12509 Jy ! Component: 150 - total flux cleaned = 0.137123 Jy ! Component: 200 - total flux cleaned = 0.143226 Jy ! Total flux subtracted in 200 components = 0.143226 Jy ! Clean residual min=-0.004301 max=0.004005 Jy/beam ! Clean residual mean=0.000003 rms=0.000944 Jy/beam ! Combined flux in latest and established models = 0.143226 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 8 model components to the UV plane model. ! The established model now contains 8 components and 0.143226 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=0.8594 mas, bmaj=0.9643 mas, bpa=-79.26 degrees ! Estimated noise=0.710405 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 = 0.00152654 Jy ! Component: 100 - total flux cleaned = 0.00174081 Jy ! Component: 150 - total flux cleaned = 0.00174745 Jy ! Component: 200 - total flux cleaned = 0.00166601 Jy ! Total flux subtracted in 200 components = 0.00166601 Jy ! Clean residual min=-0.004140 max=0.003256 Jy/beam ! Clean residual mean=0.000003 rms=0.000722 Jy/beam ! Combined flux in latest and established models = 0.144892 Jy ! Adding 5 model components to the UV plane model. ! The established model now contains 12 components and 0.144892 Jy ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.165 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 5.36% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=2.655 mas, bmaj=3.375 mas, bpa=-3.245 degrees ! Estimated noise=0.8466 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000668894 Jy ! Component: 100 - total flux cleaned = -0.000699363 Jy ! Component: 150 - total flux cleaned = -0.000751419 Jy ! Component: 200 - total flux cleaned = -0.000776572 Jy ! Total flux subtracted in 200 components = -0.000776572 Jy ! Clean residual min=-0.003921 max=0.003161 Jy/beam ! Clean residual mean=0.000004 rms=0.000898 Jy/beam ! Combined flux in latest and established models = 0.144116 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 = -2.22606e-05 Jy ! Component: 100 - total flux cleaned = -2.30707e-05 Jy ! Component: 150 - total flux cleaned = -4.58182e-05 Jy ! Component: 200 - total flux cleaned = -4.77724e-05 Jy ! Total flux subtracted in 200 components = -4.77724e-05 Jy ! Clean residual min=-0.003911 max=0.003150 Jy/beam ! Clean residual mean=0.000004 rms=0.000896 Jy/beam ! Combined flux in latest and established models = 0.144068 Jy ! Adding 8 model components to the UV plane model. ! The established model now contains 18 components and 0.144068 Jy ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=0.8594 mas, bmaj=0.9643 mas, bpa=-79.26 degrees ! Estimated noise=0.710405 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000938146 Jy ! Component: 100 - total flux cleaned = 0.0009382 Jy ! Component: 150 - total flux cleaned = 0.000870643 Jy ! Component: 200 - total flux cleaned = 0.00080549 Jy ! Total flux subtracted in 200 components = 0.00080549 Jy ! Clean residual min=-0.003935 max=0.003190 Jy/beam ! Clean residual mean=0.000003 rms=0.000705 Jy/beam ! Combined flux in latest and established models = 0.144874 Jy selfcal ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 19 components and 0.144874 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=0.099565Jy sigma=0.636474 ! Fit after self-cal, rms=0.099515Jy sigma=0.636381 wmodel /scr/pima/gb073_uvs/J1159+0112_X_map.mod ! Writing 19 model components to file: /scr/pima/gb073_uvs/J1159+0112_X_map.mod wobs /scr/pima/gb073_uvs/J1159+0112_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1159+0112_X_uvs.fits wwins /scr/pima/gb073_uvs/J1159+0112_X_map.win ! wwins: Wrote 1 windows to /scr/pima/gb073_uvs/J1159+0112_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 5.36% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00162713 Jy ! Component: 100 - total flux cleaned = -0.00256057 Jy ! Component: 150 - total flux cleaned = -0.00357862 Jy ! Component: 200 - total flux cleaned = -0.00449143 Jy ! Component: 250 - total flux cleaned = -0.0051234 Jy ! Component: 300 - total flux cleaned = -0.00568722 Jy ! Component: 350 - total flux cleaned = -0.00605245 Jy ! Component: 400 - total flux cleaned = -0.00640916 Jy ! Component: 450 - total flux cleaned = -0.00684295 Jy ! Component: 500 - total flux cleaned = -0.00709656 Jy ! Component: 550 - total flux cleaned = -0.00730348 Jy ! Component: 600 - total flux cleaned = -0.00754713 Jy ! Component: 650 - total flux cleaned = -0.00782528 Jy ! Component: 700 - total flux cleaned = -0.00805824 Jy ! Component: 750 - total flux cleaned = -0.00813347 Jy ! Component: 800 - total flux cleaned = -0.00820747 Jy ! Component: 850 - total flux cleaned = -0.00828129 Jy ! Component: 900 - total flux cleaned = -0.00835366 Jy ! Component: 950 - total flux cleaned = -0.00849665 Jy ! Component: 1000 - total flux cleaned = -0.00863655 Jy ! Component: 1050 - total flux cleaned = -0.0086368 Jy ! Component: 1100 - total flux cleaned = -0.00873917 Jy ! Component: 1150 - total flux cleaned = -0.00873923 Jy ! Component: 1200 - total flux cleaned = -0.00883899 Jy ! Component: 1250 - total flux cleaned = -0.00887123 Jy ! Component: 1300 - total flux cleaned = -0.00900082 Jy ! Component: 1350 - total flux cleaned = -0.00900063 Jy ! Component: 1400 - total flux cleaned = -0.00912628 Jy ! Component: 1450 - total flux cleaned = -0.00918876 Jy ! Component: 1500 - total flux cleaned = -0.0091892 Jy ! Component: 1550 - total flux cleaned = -0.0093419 Jy ! Component: 1600 - total flux cleaned = -0.00949218 Jy ! Component: 1650 - total flux cleaned = -0.00952173 Jy ! Component: 1700 - total flux cleaned = -0.00949231 Jy ! Component: 1750 - total flux cleaned = -0.00949237 Jy ! Component: 1800 - total flux cleaned = -0.00960734 Jy ! Component: 1850 - total flux cleaned = -0.00980629 Jy ! Component: 1900 - total flux cleaned = -0.00975001 Jy ! Component: 1950 - total flux cleaned = -0.00991793 Jy ! Component: 2000 - total flux cleaned = -0.00997328 Jy ! Component: 2050 - total flux cleaned = -0.0101101 Jy ! Component: 2100 - total flux cleaned = -0.0100829 Jy ! Component: 2150 - total flux cleaned = -0.0101102 Jy ! Component: 2200 - total flux cleaned = -0.0102698 Jy ! Component: 2250 - total flux cleaned = -0.0103749 Jy ! Component: 2300 - total flux cleaned = -0.0102444 Jy ! Component: 2350 - total flux cleaned = -0.0102704 Jy ! Component: 2400 - total flux cleaned = -0.0104245 Jy ! Component: 2450 - total flux cleaned = -0.0103991 Jy ! Component: 2500 - total flux cleaned = -0.0104493 Jy ! Component: 2550 - total flux cleaned = -0.0104994 Jy ! Component: 2600 - total flux cleaned = -0.0105487 Jy ! Component: 2650 - total flux cleaned = -0.0104996 Jy ! Component: 2700 - total flux cleaned = -0.0104755 Jy ! Component: 2750 - total flux cleaned = -0.0104995 Jy ! Component: 2800 - total flux cleaned = -0.0104996 Jy ! Component: 2850 - total flux cleaned = -0.0105235 Jy ! Component: 2900 - total flux cleaned = -0.0104529 Jy ! Component: 2950 - total flux cleaned = -0.0104059 Jy ! Component: 3000 - total flux cleaned = -0.0104061 Jy ! Component: 3050 - total flux cleaned = -0.0103135 Jy ! Component: 3100 - total flux cleaned = -0.0103366 Jy ! Component: 3150 - total flux cleaned = -0.0102685 Jy ! Component: 3200 - total flux cleaned = -0.0102684 Jy ! Component: 3250 - total flux cleaned = -0.0102685 Jy ! Component: 3300 - total flux cleaned = -0.0102463 Jy ! Component: 3350 - total flux cleaned = -0.0103564 Jy ! Component: 3400 - total flux cleaned = -0.0102688 Jy ! Component: 3450 - total flux cleaned = -0.0102689 Jy ! Component: 3500 - total flux cleaned = -0.0102905 Jy ! Component: 3550 - total flux cleaned = -0.0103118 Jy ! Component: 3600 - total flux cleaned = -0.0102902 Jy ! Component: 3650 - total flux cleaned = -0.010248 Jy ! Component: 3700 - total flux cleaned = -0.0102478 Jy ! Component: 3750 - total flux cleaned = -0.0102478 Jy ! Component: 3800 - total flux cleaned = -0.0101436 Jy ! Component: 3850 - total flux cleaned = -0.0102054 Jy ! Component: 3900 - total flux cleaned = -0.010185 Jy ! Component: 3950 - total flux cleaned = -0.0101645 Jy ! Component: 4000 - total flux cleaned = -0.0101441 Jy ! Component: 4050 - total flux cleaned = -0.0100836 Jy ! Total flux subtracted in 4096 components = -0.0100834 Jy ! Clean residual min=-0.001204 max=0.001201 Jy/beam ! Clean residual mean=0.000002 rms=0.000335 Jy/beam ! Combined flux in latest and established models = 0.13479 Jy keep ! Adding 321 model components to the UV plane model. ! The established model now contains 340 components and 0.13479 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1159+0112_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8594 x 0.9643 at -79.26 degrees (North through East) ! Clean map min=-0.0021353 max=0.13014 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1159+0112_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.130137 invert ! Inverting map ! Your choice of large map pixels excluded 5.36% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000334039 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.770048 0.770048 1.5401 3.08019 6.16038 12.3208 24.6415 49.283 98.5661 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.001 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.13 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 389.586 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1159+0112_X_uvs.log closed on Sat Dec 26 09:37:34 2015