! Started logfile: /scr/pima/gb073_uvs/J1651+4002_X_uvs.log on Sat Dec 26 09:42:35 2015 obs /scr/pima/gb073_uvs/J1651+4002_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1651+4002_X_uva.fits ! AN table 1: 29 integrations on 55 of 55 possible baselines. ! AN table 2: 29 integrations on 66 of 66 possible baselines. ! AN table 3: 29 integrations on 45 of 45 possible baselines. ! AN table 4: 29 integrations on 21 of 21 possible baselines. ! AN table 5: 29 integrations on 55 of 55 possible baselines. ! AN table 6: 29 integrations on 28 of 28 possible baselines. ! Apparent sampling: 0.837292 visibilities/baseline/integration-bin. ! Found source: J1651+4002 ! ! 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 52448 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/J1651+4002_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 29 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 5. ! ! 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 29 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 5. ! ! 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 29 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 5. ! ! 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 29 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 5. ! A total of 58 telescope corrections were flagged in sub-array 1. ! A total of 58 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 59 telescope corrections were flagged in sub-array 5. ! A total of 29 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 58 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 59 telescope corrections were flagged in sub-array 5. ! A total of 29 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 29 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 5. ! ! 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 29 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=1.003163Jy sigma=10.903483 ! Fit after self-cal, rms=0.956323Jy sigma=10.406888 ! 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 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 milli-arcsec ! Estimated beam: bmin=0.4697 mas, bmaj=1.227 mas, bpa=-20.69 degrees ! Estimated noise=0.755696 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 = 0.035587 Jy ! Component: 100 - total flux cleaned = 0.0434399 Jy ! Total flux subtracted in 100 components = 0.0434399 Jy ! Clean residual min=-0.002502 max=0.002548 Jy/beam ! Clean residual mean=-0.000000 rms=0.000530 Jy/beam ! Combined flux in latest and established models = 0.0434399 Jy ! Performing phase self-cal ! Adding 3 model components to the UV plane model. ! The established model now contains 3 components and 0.0434399 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=0.071085Jy sigma=0.670883 ! Fit after self-cal, rms=0.069359Jy sigma=0.651021 ! Inverting map ! Your choice of large map pixels excluded 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00443435 Jy ! Component: 100 - total flux cleaned = 0.00555188 Jy ! Total flux subtracted in 100 components = 0.00555188 Jy ! Clean residual min=-0.002391 max=0.002219 Jy/beam ! Clean residual mean=-0.000001 rms=0.000504 Jy/beam ! Combined flux in latest and established models = 0.0489917 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 12 components and 0.0489917 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=0.069095Jy sigma=0.648929 ! Fit after self-cal, rms=0.069086Jy sigma=0.648861 ! Inverting map ! Your choice of large map pixels excluded 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 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 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 milli-arcsec ! Estimated beam: bmin=0.6954 mas, bmaj=1.544 mas, bpa=-17.4 degrees ! Estimated noise=0.313036 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 = -0.000138273 Jy ! Component: 100 - total flux cleaned = -0.000138931 Jy ! Component: 150 - total flux cleaned = -0.000112127 Jy ! Component: 200 - total flux cleaned = -9.08881e-05 Jy ! Total flux subtracted in 200 components = -9.08881e-05 Jy ! Clean residual min=-0.000951 max=0.000894 Jy/beam ! Clean residual mean=0.000001 rms=0.000215 Jy/beam ! Combined flux in latest and established models = 0.0489008 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 13 components and 0.0489008 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=0.069053Jy sigma=0.648674 ! Fit after self-cal, rms=0.069042Jy sigma=0.648661 ! Inverting map ! Your choice of large map pixels excluded 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6954 x 1.544 at -17.4 degrees (North through East) ! Clean map min=-0.00078888 max=0.047737 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 0.96 KP 1.08 ! LA 1.03 MC 0.91 NL 0.88 OV 0.95 ! PT 1.00 SC 0.93 ZC 0.91 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 EF 1.00* FD 1.01 KP 0.99 ! LA 1.03 MC 1.05 NL 0.98 ON 0.84 ! OV 1.00 PT 1.00 SC 1.09 ZC 0.90 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* ON 1.00* OV 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* ! ! 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* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.01 FD 0.97 KP 1.01 LA 1.13 ! MK 1.08 NL 0.89 OV 1.03 PT 1.00 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 EF 1.00* FD 1.02 KP 0.99 ! LA 0.99 MC 0.91 NL 0.99 OV 1.02 ! PT 1.03 SC 0.90 ZC 0.91 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.96 EF 1.00* FD 0.98 KP 1.07 ! LA 1.10 MC 0.96 NL 0.90 ON 0.86 ! OV 1.05 PT 1.09 SC 1.10 ZC 0.83 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.08 EF 1.00* FD 1.09 KP 1.01 ! LA 1.03 MK 1.04 ON 0.84 OV 0.96 ! PT 1.00 SC 1.15 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.06 FD 0.98 KP 1.00 LA 1.02 ! MK 1.13 NL 0.96 PT 0.91 ! ! 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* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.06 FD 1.12 KP 1.01 LA 1.11 ! MK 1.05 NL 0.96 OV 1.03 PT 1.11 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 EF 1.00* FD 0.97 KP 0.96 ! LA 1.00 MC 1.07 NL 0.98 ON 0.90 ! OV 1.01 PT 1.06 SC 1.08 ZC 0.94 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* ON 1.00* OV 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.06 FD 1.01 KP 0.99 LA 1.05 ! MK 1.08 NL 0.87 PT 0.95 ! ! 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* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.97 FD 0.90 KP 0.96 LA 0.98 ! MK 1.06 NL 1.06 OV 0.96 PT 0.97 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 EF 1.00* FD 1.00 KP 1.05 ! LA 1.09 MC 1.10 NL 0.94 OV 1.02 ! PT 1.02 SC 0.86 ZC 0.96 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 EF 1.00* FD 1.03 KP 1.11 ! LA 1.04 MC 1.03 NL 0.98 ON 0.91 ! OV 0.97 PT 1.04 SC 1.00 ZC 0.98 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* ON 1.00* OV 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 FD 1.03 KP 0.98 LA 1.08 ! MK 0.99 NL 0.92 PT 1.03 ! ! 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* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.93 FD 0.99 KP 1.07 LA 1.02 ! MK 1.19 NL 0.96 OV 0.88 PT 1.11 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.05 KP 1.00 ! LA 0.99 MC 1.12 NL 1.09 ON 0.95 ! OV 1.03 PT 0.99 SC 1.10 ZC 0.96 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* ON 1.00* OV 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 0.99 KP 0.88 LA 1.06 ! MK 1.07 NL 0.87 PT 1.10 ! ! 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* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* FD 1.05 KP 1.04 LA 1.04 ! MK 0.99 NL 0.97 OV 0.98 PT 1.07 ! ! ! 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* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00 KP 1.04 ! LA 1.06 MC 1.10 NL 1.09 ON 0.93 ! OV 1.07 PT 1.00 SC 1.02 ZC 0.83 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 0.95 KP 0.93 ! LA 0.95 MK 1.05 ON 0.98 OV 1.08 ! PT 0.95 SC 0.93 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 0.99 KP 0.94 LA 0.96 ! MK 0.91 NL 0.94 PT 0.93 ! ! 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* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* FD 0.98 KP 0.95 LA 1.01 ! MK 1.08 NL 1.01 OV 1.01 PT 0.91 ! ! ! 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* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 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* MC 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 3: ! BR 0.96 EF 1.00* FD 1.09 KP 0.94 ! LA 0.96 MK 0.92 ON 1.15 OV 1.02 ! PT 0.90 SC 0.98 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.94 FD 0.98 KP 0.86 LA 1.09 ! MK 1.08 NL 0.99 PT 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* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 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* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 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* MC 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 3: ! BR 1.01 EF 1.00* FD 0.86 KP 0.94 ! LA 1.13 MK 0.94 ON 1.08 OV 1.00 ! PT 1.04 SC 1.09 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.09 FD 0.99 KP 0.91 LA 1.11 ! MK 1.06 NL 1.05 PT 0.94 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.97 EF 1.00* FD 0.90 KP 0.93 ! LA 1.10 MK 1.02 NL 1.04 ON 0.92 ! OV 1.00 PT 1.07 SC 1.04 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.05 FD 0.99 KP 1.02 LA 1.06 ! MK 0.97 NL 0.98 OV 0.94 PT 0.91 ! ! ! Fit before self-cal, rms=0.069042Jy sigma=0.648661 ! Fit after self-cal, rms=0.068598Jy sigma=0.647649 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 milli-arcsec ! Estimated beam: bmin=0.6913 mas, bmaj=1.546 mas, bpa=-17.69 degrees ! Estimated noise=0.313071 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 = 6.3665e-05 Jy ! Component: 100 - total flux cleaned = 6.3575e-05 Jy ! Component: 150 - total flux cleaned = 6.42633e-05 Jy ! Component: 200 - total flux cleaned = 6.54981e-05 Jy ! Total flux subtracted in 200 components = 6.54981e-05 Jy ! Clean residual min=-0.000829 max=0.000890 Jy/beam ! Clean residual mean=0.000001 rms=0.000205 Jy/beam ! Combined flux in latest and established models = 0.0489663 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 15 components and 0.0489663 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=0.068588Jy sigma=0.647612 ! Fit after self-cal, rms=0.068593Jy sigma=0.647452 ! Inverting map ! Your choice of large map pixels excluded 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 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=0.068593Jy sigma=0.647452 ! Fit after self-cal, rms=0.068647Jy sigma=0.647385 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 milli-arcsec ! Estimated beam: bmin=0.6906 mas, bmaj=1.545 mas, bpa=-17.65 degrees ! Estimated noise=0.313355 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 9.01755e-05 Jy ! Component: 100 - total flux cleaned = 9.04152e-05 Jy ! Component: 150 - total flux cleaned = 8.98876e-05 Jy ! Component: 200 - total flux cleaned = 7.89877e-05 Jy ! Total flux subtracted in 200 components = 7.89877e-05 Jy ! Clean residual min=-0.000841 max=0.000873 Jy/beam ! Clean residual mean=0.000001 rms=0.000204 Jy/beam ! Combined flux in latest and established models = 0.0490453 Jy selfcal ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 15 components and 0.0490453 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=0.068640Jy sigma=0.647357 ! Fit after self-cal, rms=0.068642Jy sigma=0.647348 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 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 (-28.4, -7). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000435325 Jy ! Component: 100 - total flux cleaned = 0.000281243 Jy ! Component: 150 - total flux cleaned = 0.000238103 Jy ! Component: 200 - total flux cleaned = 0.000201451 Jy ! Total flux subtracted in 200 components = 0.000201451 Jy ! Clean residual min=-0.000835 max=0.000861 Jy/beam ! Clean residual mean=0.000001 rms=0.000202 Jy/beam ! Combined flux in latest and established models = 0.0492468 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 25 components and 0.0492468 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=0.068631Jy sigma=0.647238 ! Fit after self-cal, rms=0.068628Jy sigma=0.647220 ! Inverting map ! Your choice of large map pixels excluded 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 milli-arcsec ! Added new window around map position (28, 2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000279208 Jy ! Component: 100 - total flux cleaned = 0.000284057 Jy ! Component: 150 - total flux cleaned = 0.000271233 Jy ! Component: 200 - total flux cleaned = 0.000201436 Jy ! Total flux subtracted in 200 components = 0.000201436 Jy ! Clean residual min=-0.000850 max=0.000805 Jy/beam ! Clean residual mean=0.000001 rms=0.000199 Jy/beam ! Combined flux in latest and established models = 0.0494482 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 35 components and 0.0494482 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=0.068612Jy sigma=0.647103 ! Fit after self-cal, rms=0.068600Jy sigma=0.647046 ! Inverting map ! Your choice of large map pixels excluded 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 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=0.068600Jy sigma=0.647046 ! Fit after self-cal, rms=0.068701Jy sigma=0.647000 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 milli-arcsec ! Estimated beam: bmin=0.6906 mas, bmaj=1.545 mas, bpa=-17.58 degrees ! Estimated noise=0.313867 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000160172 Jy ! Component: 100 - total flux cleaned = 0.000177135 Jy ! Component: 150 - total flux cleaned = 0.000122947 Jy ! Component: 200 - total flux cleaned = 0.000110036 Jy ! Total flux subtracted in 200 components = 0.000110036 Jy ! Clean residual min=-0.000895 max=0.000805 Jy/beam ! Clean residual mean=0.000001 rms=0.000199 Jy/beam ! Combined flux in latest and established models = 0.0495583 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 37 components and 0.0495583 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=0.068692Jy sigma=0.646951 ! Fit after self-cal, rms=0.068693Jy sigma=0.646932 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 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 = 8.04885e-05 Jy ! Component: 100 - total flux cleaned = 5.58113e-05 Jy ! Component: 150 - total flux cleaned = 4.40513e-05 Jy ! Component: 200 - total flux cleaned = 4.44927e-05 Jy ! Total flux subtracted in 200 components = 4.44927e-05 Jy ! Clean residual min=-0.000896 max=0.000814 Jy/beam ! Clean residual mean=0.000001 rms=0.000198 Jy/beam ! Combined flux in latest and established models = 0.0496027 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 42 components and 0.0496028 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=0.068688Jy sigma=0.646902 ! Fit after self-cal, rms=0.068685Jy sigma=0.646882 ! Inverting map ! Your choice of large map pixels excluded 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 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=0.068685Jy sigma=0.646882 ! Fit after self-cal, rms=0.068761Jy sigma=0.646873 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 milli-arcsec ! Estimated beam: bmin=2.746 mas, bmaj=2.993 mas, bpa=33.4 degrees ! Estimated noise=0.391157 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -1.49123e-05 Jy ! Component: 100 - total flux cleaned = -2.44933e-05 Jy ! Component: 150 - total flux cleaned = -2.49953e-05 Jy ! Component: 200 - total flux cleaned = -2.49421e-05 Jy ! Total flux subtracted in 200 components = -2.49421e-05 Jy ! Clean residual min=-0.000845 max=0.000842 Jy/beam ! Clean residual mean=0.000001 rms=0.000245 Jy/beam ! Combined flux in latest and established models = 0.0495778 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 55 components and 0.0495778 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=0.068761Jy sigma=0.646866 ! Fit after self-cal, rms=0.068760Jy sigma=0.646861 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 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 = -1.18924e-05 Jy ! Component: 100 - total flux cleaned = 7.19328e-06 Jy ! Component: 150 - total flux cleaned = 1.30307e-05 Jy ! Component: 200 - total flux cleaned = 1.88428e-05 Jy ! Total flux subtracted in 200 components = 1.88428e-05 Jy ! Clean residual min=-0.000844 max=0.000833 Jy/beam ! Clean residual mean=0.000001 rms=0.000244 Jy/beam ! Combined flux in latest and established models = 0.0495967 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 55 components and 0.0495967 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=0.068760Jy sigma=0.646859 ! Fit after self-cal, rms=0.068760Jy sigma=0.646856 ! Inverting map ! Your choice of large map pixels excluded 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 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 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 milli-arcsec ! Estimated beam: bmin=0.6905 mas, bmaj=1.545 mas, bpa=-17.56 degrees ! Estimated noise=0.314193 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6905 x 1.545 at -17.56 degrees (North through East) ! Clean map min=-0.00080898 max=0.047986 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 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 milli-arcsec ! Estimated beam: bmin=0.466 mas, bmaj=1.23 mas, bpa=-20.84 degrees ! Estimated noise=0.754363 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0377069 Jy ! Component: 100 - total flux cleaned = 0.0461783 Jy ! Component: 150 - total flux cleaned = 0.0491893 Jy ! Component: 200 - total flux cleaned = 0.0505667 Jy ! Total flux subtracted in 200 components = 0.0505667 Jy ! Clean residual min=-0.002194 max=0.002106 Jy/beam ! Clean residual mean=-0.000001 rms=0.000487 Jy/beam ! Combined flux in latest and established models = 0.0505667 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 0.0505667 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 milli-arcsec ! Estimated beam: bmin=0.6905 mas, bmaj=1.545 mas, bpa=-17.56 degrees ! Estimated noise=0.314193 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 = -0.000112954 Jy ! Component: 100 - total flux cleaned = -7.58359e-05 Jy ! Component: 150 - total flux cleaned = -7.39894e-05 Jy ! Component: 200 - total flux cleaned = -0.000129704 Jy ! Total flux subtracted in 200 components = -0.000129704 Jy ! Clean residual min=-0.000936 max=0.000830 Jy/beam ! Clean residual mean=0.000001 rms=0.000202 Jy/beam ! Combined flux in latest and established models = 0.050437 Jy ! Adding 14 model components to the UV plane model. ! The established model now contains 21 components and 0.050437 Jy ! Inverting map ! Your choice of large map pixels excluded 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 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 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 milli-arcsec ! Estimated beam: bmin=2.746 mas, bmaj=2.993 mas, bpa=33.4 degrees ! Estimated noise=0.391157 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000260854 Jy ! Component: 100 - total flux cleaned = -0.000414814 Jy ! Component: 150 - total flux cleaned = -0.000523842 Jy ! Component: 200 - total flux cleaned = -0.000615102 Jy ! Total flux subtracted in 200 components = -0.000615102 Jy ! Clean residual min=-0.000856 max=0.000847 Jy/beam ! Clean residual mean=0.000001 rms=0.000244 Jy/beam ! Combined flux in latest and established models = 0.0498219 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 = -5.2024e-05 Jy ! Component: 100 - total flux cleaned = -8.29541e-05 Jy ! Component: 150 - total flux cleaned = -0.000124393 Jy ! Component: 200 - total flux cleaned = -0.000155153 Jy ! Total flux subtracted in 200 components = -0.000155153 Jy ! Clean residual min=-0.000854 max=0.000838 Jy/beam ! Clean residual mean=0.000001 rms=0.000244 Jy/beam ! Combined flux in latest and established models = 0.0496667 Jy ! Adding 15 model components to the UV plane model. ! The established model now contains 35 components and 0.0496667 Jy ! Inverting map ! Your choice of large map pixels excluded 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 milli-arcsec ! Estimated beam: bmin=0.6905 mas, bmaj=1.545 mas, bpa=-17.56 degrees ! Estimated noise=0.314193 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 5.33389e-05 Jy ! Component: 100 - total flux cleaned = 3.07275e-05 Jy ! Component: 150 - total flux cleaned = 1.0491e-05 Jy ! Component: 200 - total flux cleaned = -2.76748e-05 Jy ! Total flux subtracted in 200 components = -2.76748e-05 Jy ! Clean residual min=-0.000903 max=0.000811 Jy/beam ! Clean residual mean=0.000001 rms=0.000199 Jy/beam ! Combined flux in latest and established models = 0.0496391 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 40 components and 0.0496391 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=0.068790Jy sigma=0.646985 ! Fit after self-cal, rms=0.068795Jy sigma=0.646966 wmodel /scr/pima/gb073_uvs/J1651+4002_X_map.mod ! Writing 40 model components to file: /scr/pima/gb073_uvs/J1651+4002_X_map.mod wobs /scr/pima/gb073_uvs/J1651+4002_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1651+4002_X_uvs.fits wwins /scr/pima/gb073_uvs/J1651+4002_X_map.win ! wwins: Wrote 3 windows to /scr/pima/gb073_uvs/J1651+4002_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 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -4.06789e-05 Jy ! Component: 100 - total flux cleaned = 3.64151e-06 Jy ! Component: 150 - total flux cleaned = 3.35267e-06 Jy ! Component: 200 - total flux cleaned = -2.48474e-05 Jy ! Component: 250 - total flux cleaned = -6.57919e-05 Jy ! Component: 300 - total flux cleaned = -0.000119502 Jy ! Component: 350 - total flux cleaned = -0.000159234 Jy ! Component: 400 - total flux cleaned = -0.000224227 Jy ! Component: 450 - total flux cleaned = -0.000262816 Jy ! Component: 500 - total flux cleaned = -0.000313555 Jy ! Component: 550 - total flux cleaned = -0.000338721 Jy ! Component: 600 - total flux cleaned = -0.00040081 Jy ! Component: 650 - total flux cleaned = -0.000425327 Jy ! Component: 700 - total flux cleaned = -0.00047424 Jy ! Component: 750 - total flux cleaned = -0.000510428 Jy ! Component: 800 - total flux cleaned = -0.000522302 Jy ! Component: 850 - total flux cleaned = -0.000534329 Jy ! Component: 900 - total flux cleaned = -0.000593458 Jy ! Component: 950 - total flux cleaned = -0.000640568 Jy ! Component: 1000 - total flux cleaned = -0.000698981 Jy ! Component: 1050 - total flux cleaned = -0.000733688 Jy ! Component: 1100 - total flux cleaned = -0.000745213 Jy ! Component: 1150 - total flux cleaned = -0.000813665 Jy ! Component: 1200 - total flux cleaned = -0.000825133 Jy ! Component: 1250 - total flux cleaned = -0.000903858 Jy ! Component: 1300 - total flux cleaned = -0.000881491 Jy ! Component: 1350 - total flux cleaned = -0.000903637 Jy ! Component: 1400 - total flux cleaned = -0.000914695 Jy ! Component: 1450 - total flux cleaned = -0.000925603 Jy ! Component: 1500 - total flux cleaned = -0.00101298 Jy ! Component: 1550 - total flux cleaned = -0.000958723 Jy ! Component: 1600 - total flux cleaned = -0.00100188 Jy ! Component: 1650 - total flux cleaned = -0.000969703 Jy ! Component: 1700 - total flux cleaned = -0.00103382 Jy ! Component: 1750 - total flux cleaned = -0.00107628 Jy ! Component: 1800 - total flux cleaned = -0.00107632 Jy ! Component: 1850 - total flux cleaned = -0.0011078 Jy ! Component: 1900 - total flux cleaned = -0.00112867 Jy ! Component: 1950 - total flux cleaned = -0.00107663 Jy ! Component: 2000 - total flux cleaned = -0.00112824 Jy ! Component: 2050 - total flux cleaned = -0.00111794 Jy ! Component: 2100 - total flux cleaned = -0.00113843 Jy ! Component: 2150 - total flux cleaned = -0.00112827 Jy ! Component: 2200 - total flux cleaned = -0.00117901 Jy ! Component: 2250 - total flux cleaned = -0.00120934 Jy ! Component: 2300 - total flux cleaned = -0.00114901 Jy ! Component: 2350 - total flux cleaned = -0.00119904 Jy ! Component: 2400 - total flux cleaned = -0.00126881 Jy ! Component: 2450 - total flux cleaned = -0.00129848 Jy ! Component: 2500 - total flux cleaned = -0.00131822 Jy ! Component: 2550 - total flux cleaned = -0.00134765 Jy ! Component: 2600 - total flux cleaned = -0.0013477 Jy ! Component: 2650 - total flux cleaned = -0.00141591 Jy ! Component: 2700 - total flux cleaned = -0.00138674 Jy ! Component: 2750 - total flux cleaned = -0.00141578 Jy ! Component: 2800 - total flux cleaned = -0.00143504 Jy ! Component: 2850 - total flux cleaned = -0.00153097 Jy ! Component: 2900 - total flux cleaned = -0.00150224 Jy ! Component: 2950 - total flux cleaned = -0.00153073 Jy ! Component: 3000 - total flux cleaned = -0.00155917 Jy ! Component: 3050 - total flux cleaned = -0.00157807 Jy ! Component: 3100 - total flux cleaned = -0.00155926 Jy ! Component: 3150 - total flux cleaned = -0.00163422 Jy ! Component: 3200 - total flux cleaned = -0.00165282 Jy ! Component: 3250 - total flux cleaned = -0.00169934 Jy ! Component: 3300 - total flux cleaned = -0.00169933 Jy ! Component: 3350 - total flux cleaned = -0.00171774 Jy ! Component: 3400 - total flux cleaned = -0.00169934 Jy ! Component: 3450 - total flux cleaned = -0.00177276 Jy ! Component: 3500 - total flux cleaned = -0.00184586 Jy ! Component: 3550 - total flux cleaned = -0.0018458 Jy ! Component: 3600 - total flux cleaned = -0.00182765 Jy ! Component: 3650 - total flux cleaned = -0.00186389 Jy ! Component: 3700 - total flux cleaned = -0.00187296 Jy ! Component: 3750 - total flux cleaned = -0.00189998 Jy ! Component: 3800 - total flux cleaned = -0.00192678 Jy ! Component: 3850 - total flux cleaned = -0.00189107 Jy ! Component: 3900 - total flux cleaned = -0.00194446 Jy ! Component: 3950 - total flux cleaned = -0.00198882 Jy ! Component: 4000 - total flux cleaned = -0.00197999 Jy ! Component: 4050 - total flux cleaned = -0.00199762 Jy ! Total flux subtracted in 4096 components = -0.00201517 Jy ! Clean residual min=-0.000516 max=0.000564 Jy/beam ! Clean residual mean=0.000000 rms=0.000149 Jy/beam ! Combined flux in latest and established models = 0.0476239 Jy keep ! Adding 343 model components to the UV plane model. ! The established model now contains 383 components and 0.0476239 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1651+4002_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6905 x 1.545 at -17.56 degrees (North through East) ! Clean map min=-0.00072796 max=0.048046 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1651+4002_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0480462 invert ! Inverting map ! Your choice of large map pixels excluded 1.69% of the data. ! The x-axis pixel size should ideally be below 0.1884 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000149495 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.933445 0.933445 1.86689 3.73378 7.46756 14.9351 29.8703 59.7405 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0004 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.048 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 321.389 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1651+4002_X_uvs.log closed on Sat Dec 26 09:42:41 2015