! Started logfile: /scr/pima/gb073_uvs/J0114+1325_X_uvs.log on Sat Dec 26 09:31:21 2015 obs /scr/pima/gb073_uvs/J0114+1325_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J0114+1325_X_uva.fits ! AN table 1: 29 integrations on 55 of 55 possible baselines. ! AN table 2: 29 integrations on 28 of 28 possible baselines. ! AN table 3: 29 integrations on 36 of 36 possible baselines. ! AN table 4: 29 integrations on 28 of 28 possible baselines. ! AN table 5: 29 integrations on 28 of 28 possible baselines. ! AN table 6: 29 integrations on 15 of 15 possible baselines. ! AN table 7: 29 integrations on 28 of 28 possible baselines. ! Apparent sampling: 0.841822 visibilities/baseline/integration-bin. ! Found source: J0114+1325 ! ! 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 42576 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/J0114+1325_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 29 telescope corrections were flagged in sub-array 3. ! A total of 33 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 87 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 33 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 87 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 33 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 87 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 33 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 5. ! A total of 87 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! A total of 33 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 6. ! A total of 87 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! A total of 33 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 7. ! A total of 87 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 33 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 8. ! A total of 87 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 33 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=1.003762Jy sigma=10.816575 ! Fit after self-cal, rms=0.957279Jy sigma=10.363016 ! 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 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 milli-arcsec ! Estimated beam: bmin=0.7633 mas, bmaj=1.508 mas, bpa=-0.4539 degrees ! Estimated noise=0.80893 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 = 0.0343622 Jy ! Component: 100 - total flux cleaned = 0.0418554 Jy ! Total flux subtracted in 100 components = 0.0418554 Jy ! Clean residual min=-0.002641 max=0.002718 Jy/beam ! Clean residual mean=0.000000 rms=0.000573 Jy/beam ! Combined flux in latest and established models = 0.0418554 Jy ! Performing phase self-cal ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 0.0418554 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=0.064970Jy sigma=0.653403 ! Fit after self-cal, rms=0.063254Jy sigma=0.633547 ! Inverting map ! Your choice of large map pixels excluded 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00325986 Jy ! Component: 100 - total flux cleaned = 0.00367103 Jy ! Total flux subtracted in 100 components = 0.00367103 Jy ! Clean residual min=-0.002493 max=0.002239 Jy/beam ! Clean residual mean=0.000000 rms=0.000558 Jy/beam ! Combined flux in latest and established models = 0.0455265 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.0455265 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=0.063007Jy sigma=0.632009 ! Fit after self-cal, rms=0.062995Jy sigma=0.631923 ! Inverting map ! Your choice of large map pixels excluded 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 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 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 milli-arcsec ! Estimated beam: bmin=1.056 mas, bmaj=1.993 mas, bpa=1.906 degrees ! Estimated noise=0.358861 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 (-0.8, -4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00221118 Jy ! Component: 100 - total flux cleaned = 0.00329156 Jy ! Component: 150 - total flux cleaned = 0.00377873 Jy ! Component: 200 - total flux cleaned = 0.00403178 Jy ! Total flux subtracted in 200 components = 0.00403178 Jy ! Clean residual min=-0.001309 max=0.001187 Jy/beam ! Clean residual mean=0.000001 rms=0.000290 Jy/beam ! Combined flux in latest and established models = 0.0495582 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 21 components and 0.0495582 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=0.062923Jy sigma=0.631206 ! Fit after self-cal, rms=0.062886Jy sigma=0.630813 ! Inverting map ! Your choice of large map pixels excluded 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.056 x 1.993 at 1.906 degrees (North through East) ! Clean map min=-0.0012997 max=0.045516 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: ! EF 1.00* FD 1.00* HH 1.00* KP 1.00* ! LA 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 2: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 1.00* HH 1.00* LA 1.00* ! NL 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! FD 1.02 KP 0.95 LA 1.05 MK 1.04 ! OV 0.96 PT 0.97 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.07 FD 1.02 KP 1.03 LA 1.01 ! NL 0.91 OV 1.01 PT 1.00 SC 0.97 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! EF 1.00* FD 1.00* HH 1.00* KP 1.00* ! LA 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 2: ! BR 1.07 FD 1.08 KP 1.04 LA 0.99 ! MK 1.11 NL 1.03 OV 1.00 PT 1.01 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.95 FD 1.15 KP 0.91 LA 1.12 ! MK 1.06 NL 1.17 PT 1.09 SC 1.20 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 1.00* HH 1.00* LA 1.00* ! NL 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! FD 1.16 KP 0.92 LA 1.06 MK 1.12 ! OV 1.01 PT 1.01 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.13 FD 1.05 KP 1.09 LA 1.19 ! NL 1.11 OV 0.97 PT 0.99 SC 1.20 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! EF 1.00* FD 1.00* HH 1.00* KP 1.00* ! LA 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 2: ! BR 1.13 FD 1.00 KP 1.00 LA 1.09 ! MK 1.04 NL 1.08 OV 0.94 PT 0.98 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 FD 1.02 KP 1.05 LA 1.08 ! MK 1.03 NL 0.94 PT 1.00 SC 1.15 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 1.00* HH 1.00* LA 1.00* ! NL 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! FD 0.93 KP 0.94 LA 1.07 MK 1.00 ! OV 1.02 PT 1.03 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.06 FD 0.96 KP 1.05 LA 0.97 ! NL 0.99 OV 0.92 PT 0.98 SC 1.13 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! EF 1.00* FD 1.00* HH 1.00* KP 1.00* ! LA 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 2: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.07 FD 1.03 KP 1.04 LA 1.05 ! MK 1.01 NL 1.07 PT 0.89 SC 0.98 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 1.00* HH 1.00* LA 1.00* ! NL 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! FD 1.05 KP 0.90 LA 0.95 MK 1.12 ! OV 0.96 PT 1.14 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.13 FD 1.05 KP 1.13 LA 0.94 ! NL 0.96 OV 1.00 PT 0.98 SC 1.19 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! EF 1.00* FD 1.00* HH 1.00* KP 1.00* ! LA 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 2: ! BR 1.00* FD 1.01 KP 0.94 LA 0.94 ! MK 1.13 NL 1.04 OV 1.01 PT 0.84 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 0.96 KP 1.00 LA 0.99 ! MK 0.95 NL 0.99 PT 1.01 SC 0.99 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 1.00* HH 1.00* LA 1.00* ! NL 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! FD 0.84 KP 0.90 LA 1.10 MK 1.01 ! OV 1.04 PT 0.91 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* FD 0.99 KP 0.86 LA 1.04 ! NL 1.06 OV 0.89 PT 1.04 SC 1.07 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! EF 1.00* FD 1.00* HH 1.00* KP 1.00* ! LA 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 2: ! BR 1.00* FD 1.01 KP 0.86 LA 1.14 ! MK 1.05 NL 1.02 OV 0.95 PT 0.97 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 0.92 KP 0.95 LA 1.07 ! MK 0.97 NL 1.06 PT 0.90 SC 1.12 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 1.00* HH 1.00* LA 1.00* ! NL 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! FD 0.87 KP 0.88 LA 0.94 MK 0.89 ! OV 1.02 PT 0.91 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* FD 1.13 KP 0.84 LA 1.05 ! NL 1.10 OV 1.02 PT 0.87 SC 0.88 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! EF 1.00* FD 1.00* HH 1.00* KP 1.00* ! LA 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 2: ! BR 0.98 FD 1.04 KP 1.09 LA 0.95 ! MK 0.94 NL 0.97 OV 1.06 PT 0.98 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.03 FD 0.95 KP 1.01 LA 1.08 ! MK 0.93 NL 1.03 PT 1.02 SC 1.04 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 1.00* HH 1.00* LA 1.00* ! NL 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! FD 1.00* KP 1.00* LA 1.00* MK 1.00* ! OV 1.00* PT 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.01 FD 0.94 KP 0.90 LA 1.05 ! NL 0.99 OV 1.07 PT 1.04 SC 1.02 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! EF 1.00* FD 1.00* HH 1.00* KP 1.00* ! LA 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 2: ! BR 0.96 FD 0.96 KP 0.88 LA 1.07 ! MK 1.01 NL 1.01 OV 1.04 PT 1.00 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.06 FD 0.92 KP 0.85 LA 1.16 ! MK 0.93 NL 1.00 PT 1.04 SC 1.19 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 1.00* HH 1.00* LA 1.00* ! NL 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! FD 1.00* KP 1.00* LA 1.00* MK 1.00* ! OV 1.00* PT 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.16 FD 0.94 KP 0.88 LA 1.14 ! NL 1.03 OV 0.89 PT 1.10 SC 1.00 ! ! ! Fit before self-cal, rms=0.062886Jy sigma=0.630813 ! Fit after self-cal, rms=0.063673Jy sigma=0.629529 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 milli-arcsec ! Estimated beam: bmin=1.064 mas, bmaj=2.004 mas, bpa=1.48 degrees ! Estimated noise=0.362952 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 = 0.00123805 Jy ! Component: 100 - total flux cleaned = 0.00147563 Jy ! Component: 150 - total flux cleaned = 0.00164049 Jy ! Component: 200 - total flux cleaned = 0.00168956 Jy ! Total flux subtracted in 200 components = 0.00168956 Jy ! Clean residual min=-0.001264 max=0.001144 Jy/beam ! Clean residual mean=0.000001 rms=0.000263 Jy/beam ! Combined flux in latest and established models = 0.0512478 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 26 components and 0.0512478 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=0.063630Jy sigma=0.629288 ! Fit after self-cal, rms=0.063657Jy sigma=0.628984 ! Inverting map ! Your choice of large map pixels excluded 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 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=0.063657Jy sigma=0.628984 ! Fit after self-cal, rms=0.064214Jy sigma=0.628846 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 milli-arcsec ! Estimated beam: bmin=1.067 mas, bmaj=2.007 mas, bpa=1.291 degrees ! Estimated noise=0.364812 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000769194 Jy ! Component: 100 - total flux cleaned = 0.000903106 Jy ! Component: 150 - total flux cleaned = 0.000902758 Jy ! Component: 200 - total flux cleaned = 0.000946081 Jy ! Total flux subtracted in 200 components = 0.000946081 Jy ! Clean residual min=-0.001266 max=0.001113 Jy/beam ! Clean residual mean=0.000001 rms=0.000260 Jy/beam ! Combined flux in latest and established models = 0.0521939 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 28 components and 0.0521939 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=0.064183Jy sigma=0.628693 ! Fit after self-cal, rms=0.064185Jy sigma=0.628549 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 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 = 0.000450432 Jy ! Component: 100 - total flux cleaned = 0.000471937 Jy ! Component: 150 - total flux cleaned = 0.000492811 Jy ! Component: 200 - total flux cleaned = 0.000532486 Jy ! Total flux subtracted in 200 components = 0.000532486 Jy ! Clean residual min=-0.001239 max=0.001120 Jy/beam ! Clean residual mean=0.000002 rms=0.000260 Jy/beam ! Combined flux in latest and established models = 0.0527264 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 29 components and 0.0527264 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=0.064164Jy sigma=0.628436 ! Fit after self-cal, rms=0.064154Jy sigma=0.628404 ! Inverting map ! Your choice of large map pixels excluded 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 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=0.064154Jy sigma=0.628404 ! Fit after self-cal, rms=0.064561Jy sigma=0.628387 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 milli-arcsec ! Estimated beam: bmin=1.069 mas, bmaj=2.006 mas, bpa=1.179 degrees ! Estimated noise=0.366372 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000468626 Jy ! Component: 100 - total flux cleaned = 0.000447691 Jy ! Component: 150 - total flux cleaned = 0.000487089 Jy ! Component: 200 - total flux cleaned = 0.00050591 Jy ! Total flux subtracted in 200 components = 0.00050591 Jy ! Clean residual min=-0.001239 max=0.001090 Jy/beam ! Clean residual mean=0.000002 rms=0.000259 Jy/beam ! Combined flux in latest and established models = 0.0532323 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 29 components and 0.0532323 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=0.064538Jy sigma=0.628291 ! Fit after self-cal, rms=0.064542Jy sigma=0.628268 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 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 = 0.000162083 Jy ! Component: 100 - total flux cleaned = 0.000181297 Jy ! Component: 150 - total flux cleaned = 0.000199321 Jy ! Component: 200 - total flux cleaned = 0.000234345 Jy ! Total flux subtracted in 200 components = 0.000234345 Jy ! Clean residual min=-0.001235 max=0.001093 Jy/beam ! Clean residual mean=0.000002 rms=0.000258 Jy/beam ! Combined flux in latest and established models = 0.0534666 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 30 components and 0.0534666 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=0.064524Jy sigma=0.628183 ! Fit after self-cal, rms=0.064516Jy sigma=0.628170 ! Inverting map ! Your choice of large map pixels excluded 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 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=0.064516Jy sigma=0.628170 ! Fit after self-cal, rms=0.064719Jy sigma=0.628112 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 milli-arcsec ! Estimated beam: bmin=2.738 mas, bmaj=3.593 mas, bpa=0.06067 degrees ! Estimated noise=0.421231 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 8.19327e-05 Jy ! Component: 100 - total flux cleaned = 0.000112679 Jy ! Component: 150 - total flux cleaned = 0.00011857 Jy ! Component: 200 - total flux cleaned = 0.000118682 Jy ! Total flux subtracted in 200 components = 0.000118682 Jy ! Clean residual min=-0.001171 max=0.001173 Jy/beam ! Clean residual mean=0.000003 rms=0.000302 Jy/beam ! Combined flux in latest and established models = 0.0535853 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 40 components and 0.0535853 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=0.064721Jy sigma=0.628111 ! Fit after self-cal, rms=0.064727Jy sigma=0.628098 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 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 = 3.32517e-05 Jy ! Component: 100 - total flux cleaned = 6.6111e-05 Jy ! Component: 150 - total flux cleaned = 7.5982e-05 Jy ! Component: 200 - total flux cleaned = 7.14965e-05 Jy ! Total flux subtracted in 200 components = 7.14965e-05 Jy ! Clean residual min=-0.001169 max=0.001170 Jy/beam ! Clean residual mean=0.000003 rms=0.000302 Jy/beam ! Combined flux in latest and established models = 0.0536568 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 43 components and 0.0536568 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=0.064729Jy sigma=0.628102 ! Fit after self-cal, rms=0.064729Jy sigma=0.628096 ! Inverting map ! Your choice of large map pixels excluded 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 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 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 milli-arcsec ! Estimated beam: bmin=1.07 mas, bmaj=2.005 mas, bpa=1.122 degrees ! Estimated noise=0.366981 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.07 x 2.005 at 1.122 degrees (North through East) ! Clean map min=-0.0011633 max=0.04656 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 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 milli-arcsec ! Estimated beam: bmin=0.767 mas, bmaj=1.508 mas, bpa=-1.246 degrees ! Estimated noise=0.836396 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0374363 Jy ! Component: 100 - total flux cleaned = 0.0458223 Jy ! Component: 150 - total flux cleaned = 0.0490052 Jy ! Component: 200 - total flux cleaned = 0.0507106 Jy ! Total flux subtracted in 200 components = 0.0507106 Jy ! Clean residual min=-0.002355 max=0.002229 Jy/beam ! Clean residual mean=0.000001 rms=0.000546 Jy/beam ! Combined flux in latest and established models = 0.0507106 Jy uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Adding 12 model components to the UV plane model. ! The established model now contains 12 components and 0.0507106 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 milli-arcsec ! Estimated beam: bmin=1.07 mas, bmaj=2.005 mas, bpa=1.122 degrees ! Estimated noise=0.366981 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 = 0.00179275 Jy ! Component: 100 - total flux cleaned = 0.00238913 Jy ! Component: 150 - total flux cleaned = 0.0026531 Jy ! Component: 200 - total flux cleaned = 0.00271715 Jy ! Total flux subtracted in 200 components = 0.00271715 Jy ! Clean residual min=-0.001289 max=0.001141 Jy/beam ! Clean residual mean=0.000002 rms=0.000267 Jy/beam ! Combined flux in latest and established models = 0.0534277 Jy ! Adding 12 model components to the UV plane model. ! The established model now contains 21 components and 0.0534277 Jy ! Inverting map ! Your choice of large map pixels excluded 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 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 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 milli-arcsec ! Estimated beam: bmin=2.738 mas, bmaj=3.593 mas, bpa=0.06067 degrees ! Estimated noise=0.421231 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000202181 Jy ! Component: 100 - total flux cleaned = 0.000235482 Jy ! Component: 150 - total flux cleaned = 0.000243048 Jy ! Component: 200 - total flux cleaned = 0.000248674 Jy ! Total flux subtracted in 200 components = 0.000248674 Jy ! Clean residual min=-0.001171 max=0.001176 Jy/beam ! Clean residual mean=0.000003 rms=0.000304 Jy/beam ! Combined flux in latest and established models = 0.0536764 Jy flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 6.69138e-08 Jy ! Component: 100 - total flux cleaned = 4.18016e-06 Jy ! Component: 150 - total flux cleaned = 4.19037e-06 Jy ! Component: 200 - total flux cleaned = 4.16272e-06 Jy ! Total flux subtracted in 200 components = 4.16272e-06 Jy ! Clean residual min=-0.001173 max=0.001173 Jy/beam ! Clean residual mean=0.000003 rms=0.000303 Jy/beam ! Combined flux in latest and established models = 0.0536805 Jy ! Adding 15 model components to the UV plane model. ! The established model now contains 35 components and 0.0536805 Jy ! Inverting map ! Your choice of large map pixels excluded 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 milli-arcsec ! Estimated beam: bmin=1.07 mas, bmaj=2.005 mas, bpa=1.122 degrees ! Estimated noise=0.366981 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 6.18753e-05 Jy ! Component: 100 - total flux cleaned = 6.32328e-05 Jy ! Component: 150 - total flux cleaned = 6.5057e-05 Jy ! Component: 200 - total flux cleaned = 6.60098e-05 Jy ! Total flux subtracted in 200 components = 6.60098e-05 Jy ! Clean residual min=-0.001270 max=0.001118 Jy/beam ! Clean residual mean=0.000002 rms=0.000263 Jy/beam ! Combined flux in latest and established models = 0.0537465 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 38 components and 0.0537465 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=0.064754Jy sigma=0.628211 ! Fit after self-cal, rms=0.064759Jy sigma=0.628164 wmodel /scr/pima/gb073_uvs/J0114+1325_X_map.mod ! Writing 38 model components to file: /scr/pima/gb073_uvs/J0114+1325_X_map.mod wobs /scr/pima/gb073_uvs/J0114+1325_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J0114+1325_X_uvs.fits wwins /scr/pima/gb073_uvs/J0114+1325_X_map.win ! wwins: Wrote 2 windows to /scr/pima/gb073_uvs/J0114+1325_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 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000161844 Jy ! Component: 100 - total flux cleaned = -0.000181695 Jy ! Component: 150 - total flux cleaned = -0.000200139 Jy ! Component: 200 - total flux cleaned = -7.89241e-05 Jy ! Component: 250 - total flux cleaned = -6.21826e-05 Jy ! Component: 300 - total flux cleaned = -1.2637e-05 Jy ! Component: 350 - total flux cleaned = 1.9495e-05 Jy ! Component: 400 - total flux cleaned = 8.21998e-05 Jy ! Component: 450 - total flux cleaned = 8.22457e-05 Jy ! Component: 500 - total flux cleaned = 0.000112932 Jy ! Component: 550 - total flux cleaned = 0.000113134 Jy ! Component: 600 - total flux cleaned = 0.000142884 Jy ! Component: 650 - total flux cleaned = 0.000142751 Jy ! Component: 700 - total flux cleaned = 0.000142634 Jy ! Component: 750 - total flux cleaned = 8.60104e-05 Jy ! Component: 800 - total flux cleaned = 7.219e-05 Jy ! Component: 850 - total flux cleaned = 1.68612e-05 Jy ! Component: 900 - total flux cleaned = -2.40453e-05 Jy ! Component: 950 - total flux cleaned = -6.43707e-05 Jy ! Component: 1000 - total flux cleaned = -0.000104209 Jy ! Component: 1050 - total flux cleaned = -0.000117377 Jy ! Component: 1100 - total flux cleaned = -0.000156476 Jy ! Component: 1150 - total flux cleaned = -0.00015669 Jy ! Component: 1200 - total flux cleaned = -0.000207878 Jy ! Component: 1250 - total flux cleaned = -0.000245742 Jy ! Component: 1300 - total flux cleaned = -0.000295918 Jy ! Component: 1350 - total flux cleaned = -0.000308296 Jy ! Component: 1400 - total flux cleaned = -0.000320415 Jy ! Component: 1450 - total flux cleaned = -0.000345069 Jy ! Component: 1500 - total flux cleaned = -0.000430067 Jy ! Component: 1550 - total flux cleaned = -0.000429977 Jy ! Component: 1600 - total flux cleaned = -0.000430209 Jy ! Component: 1650 - total flux cleaned = -0.000394728 Jy ! Component: 1700 - total flux cleaned = -0.000430073 Jy ! Component: 1750 - total flux cleaned = -0.000465148 Jy ! Component: 1800 - total flux cleaned = -0.000488244 Jy ! Component: 1850 - total flux cleaned = -0.000499594 Jy ! Component: 1900 - total flux cleaned = -0.000545185 Jy ! Component: 1950 - total flux cleaned = -0.000499838 Jy ! Component: 2000 - total flux cleaned = -0.000500008 Jy ! Component: 2050 - total flux cleaned = -0.000566874 Jy ! Component: 2100 - total flux cleaned = -0.000555877 Jy ! Component: 2150 - total flux cleaned = -0.000588824 Jy ! Component: 2200 - total flux cleaned = -0.000599837 Jy ! Component: 2250 - total flux cleaned = -0.00062148 Jy ! Component: 2300 - total flux cleaned = -0.000621421 Jy ! Component: 2350 - total flux cleaned = -0.00058926 Jy ! Component: 2400 - total flux cleaned = -0.000599906 Jy ! Component: 2450 - total flux cleaned = -0.000620919 Jy ! Component: 2500 - total flux cleaned = -0.000589534 Jy ! Component: 2550 - total flux cleaned = -0.000547718 Jy ! Component: 2600 - total flux cleaned = -0.000547878 Jy ! Component: 2650 - total flux cleaned = -0.000568497 Jy ! Component: 2700 - total flux cleaned = -0.000558136 Jy ! Component: 2750 - total flux cleaned = -0.000547861 Jy ! Component: 2800 - total flux cleaned = -0.000527698 Jy ! Component: 2850 - total flux cleaned = -0.000507626 Jy ! Component: 2900 - total flux cleaned = -0.000477554 Jy ! Component: 2950 - total flux cleaned = -0.000517289 Jy ! Component: 3000 - total flux cleaned = -0.000507436 Jy ! Component: 3050 - total flux cleaned = -0.000507322 Jy ! Component: 3100 - total flux cleaned = -0.000448632 Jy ! Component: 3150 - total flux cleaned = -0.000429137 Jy ! Component: 3200 - total flux cleaned = -0.000419498 Jy ! Component: 3250 - total flux cleaned = -0.000371336 Jy ! Component: 3300 - total flux cleaned = -0.000409689 Jy ! Component: 3350 - total flux cleaned = -0.000333387 Jy ! Component: 3400 - total flux cleaned = -0.000333297 Jy ! Component: 3450 - total flux cleaned = -0.000333408 Jy ! Component: 3500 - total flux cleaned = -0.000333397 Jy ! Component: 3550 - total flux cleaned = -0.000361373 Jy ! Component: 3600 - total flux cleaned = -0.000370638 Jy ! Component: 3650 - total flux cleaned = -0.000315159 Jy ! Component: 3700 - total flux cleaned = -0.000361239 Jy ! Component: 3750 - total flux cleaned = -0.000352162 Jy ! Component: 3800 - total flux cleaned = -0.000306677 Jy ! Component: 3850 - total flux cleaned = -0.000315739 Jy ! Component: 3900 - total flux cleaned = -0.000279667 Jy ! Component: 3950 - total flux cleaned = -0.000297622 Jy ! Component: 4000 - total flux cleaned = -0.000270828 Jy ! Component: 4050 - total flux cleaned = -0.000297467 Jy ! Total flux subtracted in 4096 components = -0.000279698 Jy ! Clean residual min=-0.000523 max=0.000446 Jy/beam ! Clean residual mean=0.000001 rms=0.000149 Jy/beam ! Combined flux in latest and established models = 0.0534668 Jy keep ! Adding 302 model components to the UV plane model. ! The established model now contains 340 components and 0.0534669 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J0114+1325_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 1.07 x 2.005 at 1.122 degrees (North through East) ! Clean map min=-0.00086743 max=0.046304 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J0114+1325_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0463041 invert ! Inverting map ! Your choice of large map pixels excluded 5.8% of the data. ! The x-axis pixel size should ideally be below 0.17 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000148829 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.964247 0.964247 1.92849 3.85699 7.71398 15.428 30.8559 61.7118 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0004 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.046 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 311.123 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J0114+1325_X_uvs.log closed on Sat Dec 26 09:31:26 2015