! Started logfile: /scr/pima/gb073_uvs/J0945+5757_X_uvs.log on Sat Dec 26 09:35:24 2015 obs /scr/pima/gb073_uvs/J0945+5757_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J0945+5757_X_uva.fits ! AN table 1: 29 integrations on 45 of 45 possible baselines. ! AN table 2: 29 integrations on 21 of 21 possible baselines. ! AN table 3: 29 integrations on 45 of 45 possible baselines. ! AN table 4: 29 integrations on 55 of 55 possible baselines. ! Apparent sampling: 0.928126 visibilities/baseline/integration-bin. ! Found source: J0945+5757 ! ! 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 35744 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/J0945+5757_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 29 telescope corrections were flagged in sub-array 4. ! ! 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 29 telescope corrections were flagged in sub-array 4. ! ! 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 29 telescope corrections were flagged in sub-array 4. ! ! 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 29 telescope corrections were flagged in sub-array 4. ! ! 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 58 telescope corrections were flagged in sub-array 4. ! ! 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 58 telescope corrections were flagged in sub-array 4. ! ! 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 29 telescope corrections were flagged in sub-array 4. ! ! 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 29 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=1.003687Jy sigma=10.229440 ! Fit after self-cal, rms=0.952376Jy sigma=9.720070 ! 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 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 milli-arcsec ! Estimated beam: bmin=0.4572 mas, bmaj=0.8442 mas, bpa=-20.49 degrees ! Estimated noise=0.97984 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 = 0.0387613 Jy ! Component: 100 - total flux cleaned = 0.0472298 Jy ! Total flux subtracted in 100 components = 0.0472298 Jy ! Clean residual min=-0.003120 max=0.003303 Jy/beam ! Clean residual mean=-0.000001 rms=0.000695 Jy/beam ! Combined flux in latest and established models = 0.0472298 Jy ! Performing phase self-cal ! Adding 3 model components to the UV plane model. ! The established model now contains 3 components and 0.0472298 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=0.073542Jy sigma=0.661657 ! Fit after self-cal, rms=0.072245Jy sigma=0.647601 ! Inverting map ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00255175 Jy ! Component: 100 - total flux cleaned = 0.00275395 Jy ! Total flux subtracted in 100 components = 0.00275395 Jy ! Clean residual min=-0.003171 max=0.002988 Jy/beam ! Clean residual mean=-0.000001 rms=0.000672 Jy/beam ! Combined flux in latest and established models = 0.0499838 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.0499838 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=0.072027Jy sigma=0.646130 ! Fit after self-cal, rms=0.072002Jy sigma=0.646050 ! Inverting map ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 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 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 milli-arcsec ! Estimated beam: bmin=0.665 mas, bmaj=1.118 mas, bpa=-13.49 degrees ! Estimated noise=0.439107 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 = 0.000814373 Jy ! Component: 100 - total flux cleaned = 0.000845401 Jy ! Component: 150 - total flux cleaned = 0.000846464 Jy ! Component: 200 - total flux cleaned = 0.000846878 Jy ! Total flux subtracted in 200 components = 0.000846878 Jy ! Clean residual min=-0.001299 max=0.001458 Jy/beam ! Clean residual mean=-0.000004 rms=0.000331 Jy/beam ! Combined flux in latest and established models = 0.0508307 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 8 components and 0.0508307 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=0.071952Jy sigma=0.645892 ! Fit after self-cal, rms=0.071945Jy sigma=0.645877 ! Inverting map ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.665 x 1.118 at -13.49 degrees (North through East) ! Clean map min=-0.0011411 max=0.051529 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 0.90 EF 1.00* FD 0.99 KP 1.01 ! LA 1.03 MK 1.10 NL 0.93 OV 1.09 ! PT 1.02 ZC 1.08 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* LA 1.00* ! MC 1.00* NL 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 EF 1.00* FD 0.97 KP 0.94 ! LA 1.01 MC 0.89 NL 0.91 ON 0.98 ! OV 1.06 PT 0.97 SC 1.08 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 EF 1.00* FD 0.88 KP 1.05 ! LA 1.13 MK 1.09 NL 1.10 OV 1.05 ! PT 1.01 ZC 1.10 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* LA 1.00* ! MC 1.00* NL 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.11 EF 1.00* FD 1.09 KP 1.01 ! LA 1.18 MC 1.14 NL 1.02 ON 0.93 ! OV 1.17 PT 0.93 SC 0.95 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.05 EF 1.00* FD 0.96 KP 1.00 ! LA 0.98 MK 1.02 NL 1.04 OV 1.01 ! PT 0.99 ZC 1.03 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* LA 1.00* ! MC 1.00* NL 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.11 EF 1.00* FD 1.11 KP 0.90 ! LA 0.94 MC 1.00 NL 0.85 ON 0.99 ! OV 1.01 PT 1.07 SC 1.14 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.15 EF 1.00* FD 1.03 KP 1.00 ! LA 1.00 MK 0.99 NL 0.99 OV 1.09 ! PT 1.07 ZC 1.00 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* LA 1.00* ! MC 1.00* NL 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! 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* ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.98 KP 0.87 ! LA 1.09 MK 0.93 NL 1.06 OV 1.17 ! PT 0.96 ZC 0.91 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* LA 1.00* ! MC 1.00* NL 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.06 KP 0.87 ! LA 0.98 MC 1.04 NL 1.06 ON 0.92 ! OV 1.01 PT 0.95 SC 1.11 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.03 KP 0.88 ! LA 1.00 MK 0.95 NL 1.13 OV 1.03 ! PT 0.98 ZC 0.93 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* LA 1.00* ! MC 1.00* NL 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 0.92 KP 0.87 ! LA 1.06 MC 1.12 NL 0.96 ON 0.87 ! PT 1.02 SC 0.90 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 0.99 KP 0.87 ! LA 1.03 MC 1.10 NL 1.06 ON 0.99 ! OV 0.97 PT 0.90 SC 1.02 ! ! ! 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* MK 1.00* NL 1.00* OV 1.00* ! PT 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* LA 1.00* ! MC 1.00* NL 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.11 EF 1.00* FD 1.03 KP 0.94 ! LA 0.98 MC 1.11 NL 1.10 ON 0.85 ! PT 0.89 SC 0.97 ! ! Telescope amplitude corrections in sub-array 4: ! 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* ! ! ! 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* MK 1.00* NL 1.00* OV 1.00* ! PT 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 EF 1.00* FD 0.98 LA 0.86 ! MC 0.94 NL 0.93 SC 0.98 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.15 EF 1.00* FD 1.12 KP 0.87 ! LA 1.04 MC 1.15 NL 0.93 ON 0.88 ! PT 0.99 SC 0.98 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.11 EF 1.00* FD 0.91 KP 0.95 ! LA 1.02 MC 1.19 NL 1.02 ON 1.06 ! OV 0.96 PT 0.99 SC 1.06 ! ! ! Fit before self-cal, rms=0.071945Jy sigma=0.645877 ! Fit after self-cal, rms=0.072691Jy sigma=0.644394 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 milli-arcsec ! Estimated beam: bmin=0.6664 mas, bmaj=1.119 mas, bpa=-13.41 degrees ! Estimated noise=0.442435 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 = 0.000262259 Jy ! Component: 100 - total flux cleaned = 0.000262053 Jy ! Component: 150 - total flux cleaned = 0.000242489 Jy ! Component: 200 - total flux cleaned = 0.00020862 Jy ! Total flux subtracted in 200 components = 0.00020862 Jy ! Clean residual min=-0.001204 max=0.001405 Jy/beam ! Clean residual mean=-0.000007 rms=0.000306 Jy/beam ! Combined flux in latest and established models = 0.0510393 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 9 components and 0.0510393 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=0.072667Jy sigma=0.644332 ! Fit after self-cal, rms=0.072712Jy sigma=0.644157 ! Inverting map ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 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=0.072712Jy sigma=0.644157 ! Fit after self-cal, rms=0.072915Jy sigma=0.643745 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 milli-arcsec ! Estimated beam: bmin=0.6672 mas, bmaj=1.121 mas, bpa=-12.93 degrees ! Estimated noise=0.441512 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -9.28846e-07 Jy ! Component: 100 - total flux cleaned = -2.93239e-06 Jy ! Component: 150 - total flux cleaned = -1.98564e-05 Jy ! Component: 200 - total flux cleaned = -6.34429e-06 Jy ! Total flux subtracted in 200 components = -6.34429e-06 Jy ! Clean residual min=-0.001185 max=0.001396 Jy/beam ! Clean residual mean=-0.000007 rms=0.000296 Jy/beam ! Combined flux in latest and established models = 0.0510329 Jy selfcal ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 9 components and 0.0510329 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=0.072902Jy sigma=0.643702 ! Fit after self-cal, rms=0.072919Jy sigma=0.643646 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 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 (-9.4, -5.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00067416 Jy ! Component: 100 - total flux cleaned = 0.000545475 Jy ! Component: 150 - total flux cleaned = 0.000524999 Jy ! Component: 200 - total flux cleaned = 0.000525565 Jy ! Total flux subtracted in 200 components = 0.000525565 Jy ! Clean residual min=-0.001213 max=0.001314 Jy/beam ! Clean residual mean=-0.000007 rms=0.000290 Jy/beam ! Combined flux in latest and established models = 0.0515585 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 19 components and 0.0515585 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=0.072893Jy sigma=0.643445 ! Fit after self-cal, rms=0.072892Jy sigma=0.643387 ! Inverting map ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 milli-arcsec ! Added new window around map position (14.4, 50). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00112581 Jy ! Component: 100 - total flux cleaned = 0.00120425 Jy ! Component: 150 - total flux cleaned = 0.00120369 Jy ! Component: 200 - total flux cleaned = 0.0011851 Jy ! Total flux subtracted in 200 components = 0.0011851 Jy ! Clean residual min=-0.001166 max=0.001263 Jy/beam ! Clean residual mean=-0.000005 rms=0.000286 Jy/beam ! Combined flux in latest and established models = 0.0527436 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 32 components and 0.0527436 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=0.072869Jy sigma=0.643179 ! Fit after self-cal, rms=0.072867Jy sigma=0.643116 ! Inverting map ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 milli-arcsec ! Added new window around map position (-35.6, -36.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000753099 Jy ! Component: 100 - total flux cleaned = 0.000955349 Jy ! Component: 150 - total flux cleaned = 0.00110005 Jy ! Component: 200 - total flux cleaned = 0.00105978 Jy ! Total flux subtracted in 200 components = 0.00105978 Jy ! Clean residual min=-0.001166 max=0.001179 Jy/beam ! Clean residual mean=-0.000006 rms=0.000281 Jy/beam ! Combined flux in latest and established models = 0.0538034 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 41 components and 0.0538034 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=0.072842Jy sigma=0.642881 ! Fit after self-cal, rms=0.072837Jy sigma=0.642829 ! Inverting map ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 milli-arcsec ! Added new window around map position (-44.2, 50.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000772973 Jy ! Component: 100 - total flux cleaned = 0.000946722 Jy ! Component: 150 - total flux cleaned = 0.00101728 Jy ! Component: 200 - total flux cleaned = 0.00103874 Jy ! Total flux subtracted in 200 components = 0.00103874 Jy ! Clean residual min=-0.001180 max=0.001103 Jy/beam ! Clean residual mean=-0.000008 rms=0.000278 Jy/beam ! Combined flux in latest and established models = 0.0548421 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 54 components and 0.0548421 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=0.072811Jy sigma=0.642625 ! Fit after self-cal, rms=0.072806Jy sigma=0.642587 ! Inverting map ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 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=0.072806Jy sigma=0.642587 ! Fit after self-cal, rms=0.072897Jy sigma=0.642556 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 milli-arcsec ! Estimated beam: bmin=0.6671 mas, bmaj=1.122 mas, bpa=-12.74 degrees ! Estimated noise=0.441247 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000523843 Jy ! Component: 100 - total flux cleaned = 0.000662758 Jy ! Component: 150 - total flux cleaned = 0.000663248 Jy ! Component: 200 - total flux cleaned = 0.000663082 Jy ! Total flux subtracted in 200 components = 0.000663082 Jy ! Clean residual min=-0.001178 max=0.001114 Jy/beam ! Clean residual mean=-0.000008 rms=0.000275 Jy/beam ! Combined flux in latest and established models = 0.0555052 Jy selfcal ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 55 components and 0.0555052 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=0.072881Jy sigma=0.642446 ! Fit after self-cal, rms=0.072892Jy sigma=0.642420 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 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 = 0.000211395 Jy ! Component: 100 - total flux cleaned = 0.000211474 Jy ! Component: 150 - total flux cleaned = 0.000174346 Jy ! Component: 200 - total flux cleaned = 0.000174444 Jy ! Total flux subtracted in 200 components = 0.000174444 Jy ! Clean residual min=-0.001195 max=0.001118 Jy/beam ! Clean residual mean=-0.000008 rms=0.000274 Jy/beam ! Combined flux in latest and established models = 0.0556796 Jy ! Performing phase self-cal ! Adding 35 model components to the UV plane model. ! The established model now contains 59 components and 0.0556796 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=0.072880Jy sigma=0.642346 ! Fit after self-cal, rms=0.072880Jy sigma=0.642341 ! Inverting map ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 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=0.072880Jy sigma=0.642341 ! Fit after self-cal, rms=0.072820Jy sigma=0.642211 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 milli-arcsec ! Estimated beam: bmin=2.588 mas, bmaj=3.068 mas, bpa=43.65 degrees ! Estimated noise=0.548413 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -2.52624e-05 Jy ! Component: 100 - total flux cleaned = -4.50013e-05 Jy ! Component: 150 - total flux cleaned = -5.34824e-05 Jy ! Component: 200 - total flux cleaned = -6.1575e-05 Jy ! Total flux subtracted in 200 components = -6.1575e-05 Jy ! Clean residual min=-0.001324 max=0.001207 Jy/beam ! Clean residual mean=-0.000019 rms=0.000334 Jy/beam ! Combined flux in latest and established models = 0.055618 Jy selfcal ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 71 components and 0.055618 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=0.072821Jy sigma=0.642202 ! Fit after self-cal, rms=0.072834Jy sigma=0.642172 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 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 = -1.17548e-06 Jy ! Component: 100 - total flux cleaned = -1.27429e-06 Jy ! Component: 150 - total flux cleaned = -8.57895e-06 Jy ! Component: 200 - total flux cleaned = -8.56733e-06 Jy ! Total flux subtracted in 200 components = -8.56733e-06 Jy ! Clean residual min=-0.001318 max=0.001186 Jy/beam ! Clean residual mean=-0.000019 rms=0.000332 Jy/beam ! Combined flux in latest and established models = 0.0556095 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 75 components and 0.0556095 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=0.072834Jy sigma=0.642172 ! Fit after self-cal, rms=0.072835Jy sigma=0.642169 ! Inverting map ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 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 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 milli-arcsec ! Estimated beam: bmin=0.6676 mas, bmaj=1.121 mas, bpa=-12.69 degrees ! Estimated noise=0.440472 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6676 x 1.121 at -12.69 degrees (North through East) ! Clean map min=-0.00093617 max=0.051859 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 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 milli-arcsec ! Estimated beam: bmin=0.4596 mas, bmaj=0.8451 mas, bpa=-19.62 degrees ! Estimated noise=0.984618 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0403542 Jy ! Component: 100 - total flux cleaned = 0.0492097 Jy ! Component: 150 - total flux cleaned = 0.0512089 Jy ! Component: 200 - total flux cleaned = 0.0531362 Jy ! Total flux subtracted in 200 components = 0.0531362 Jy ! Clean residual min=-0.003001 max=0.003048 Jy/beam ! Clean residual mean=-0.000002 rms=0.000655 Jy/beam ! Combined flux in latest and established models = 0.0531362 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 9 model components to the UV plane model. ! The established model now contains 9 components and 0.0531362 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 milli-arcsec ! Estimated beam: bmin=0.6676 mas, bmaj=1.121 mas, bpa=-12.69 degrees ! Estimated noise=0.440472 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 = 0.00195168 Jy ! Component: 100 - total flux cleaned = 0.00264626 Jy ! Component: 150 - total flux cleaned = 0.00297803 Jy ! Component: 200 - total flux cleaned = 0.00318777 Jy ! Total flux subtracted in 200 components = 0.00318777 Jy ! Clean residual min=-0.001196 max=0.001258 Jy/beam ! Clean residual mean=-0.000008 rms=0.000286 Jy/beam ! Combined flux in latest and established models = 0.0563239 Jy ! Adding 21 model components to the UV plane model. ! The established model now contains 26 components and 0.0563239 Jy ! Inverting map ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 milli-arcsec ! Added new window around map position (-20.8, 17.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000536486 Jy ! Component: 100 - total flux cleaned = 0.00053453 Jy ! Component: 150 - total flux cleaned = 0.000533092 Jy ! Component: 200 - total flux cleaned = 0.000466976 Jy ! Total flux subtracted in 200 components = 0.000466976 Jy ! Clean residual min=-0.001150 max=0.001169 Jy/beam ! Clean residual mean=-0.000008 rms=0.000278 Jy/beam ! Combined flux in latest and established models = 0.0567909 Jy ! Adding 29 model components to the UV plane model. ! The established model now contains 36 components and 0.0567909 Jy ! Inverting map ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 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 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 milli-arcsec ! Estimated beam: bmin=2.588 mas, bmaj=3.068 mas, bpa=43.65 degrees ! Estimated noise=0.548413 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -7.40258e-05 Jy ! Component: 100 - total flux cleaned = -7.20222e-05 Jy ! Component: 150 - total flux cleaned = -0.000117881 Jy ! Component: 200 - total flux cleaned = -0.000157527 Jy ! Total flux subtracted in 200 components = -0.000157527 Jy ! Clean residual min=-0.001420 max=0.001060 Jy/beam ! Clean residual mean=-0.000018 rms=0.000324 Jy/beam ! Combined flux in latest and established models = 0.0566334 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 = -1.07224e-05 Jy ! Component: 100 - total flux cleaned = -1.06292e-05 Jy ! Component: 150 - total flux cleaned = -2.14918e-05 Jy ! Component: 200 - total flux cleaned = -3.13715e-05 Jy ! Total flux subtracted in 200 components = -3.13715e-05 Jy ! Clean residual min=-0.001402 max=0.001067 Jy/beam ! Clean residual mean=-0.000018 rms=0.000322 Jy/beam ! Combined flux in latest and established models = 0.056602 Jy ! Adding 19 model components to the UV plane model. ! The established model now contains 53 components and 0.056602 Jy ! Inverting map ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 milli-arcsec ! Estimated beam: bmin=0.6676 mas, bmaj=1.121 mas, bpa=-12.69 degrees ! Estimated noise=0.440472 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000150712 Jy ! Component: 100 - total flux cleaned = -0.000151042 Jy ! Component: 150 - total flux cleaned = -0.000207056 Jy ! Component: 200 - total flux cleaned = -0.000233118 Jy ! Total flux subtracted in 200 components = -0.000233118 Jy ! Clean residual min=-0.001120 max=0.001142 Jy/beam ! Clean residual mean=-0.000007 rms=0.000272 Jy/beam ! Combined flux in latest and established models = 0.0563689 Jy selfcal ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 65 components and 0.0563689 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=0.072891Jy sigma=0.642355 ! Fit after self-cal, rms=0.072907Jy sigma=0.642294 wmodel /scr/pima/gb073_uvs/J0945+5757_X_map.mod ! Writing 65 model components to file: /scr/pima/gb073_uvs/J0945+5757_X_map.mod wobs /scr/pima/gb073_uvs/J0945+5757_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J0945+5757_X_uvs.fits wwins /scr/pima/gb073_uvs/J0945+5757_X_map.win ! wwins: Wrote 6 windows to /scr/pima/gb073_uvs/J0945+5757_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 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000127785 Jy ! Component: 100 - total flux cleaned = -8.71846e-05 Jy ! Component: 150 - total flux cleaned = -2.81641e-05 Jy ! Component: 200 - total flux cleaned = 9.89169e-06 Jy ! Component: 250 - total flux cleaned = -8.97125e-06 Jy ! Component: 300 - total flux cleaned = 8.95835e-06 Jy ! Component: 350 - total flux cleaned = -6.35376e-05 Jy ! Component: 400 - total flux cleaned = -6.40514e-05 Jy ! Component: 450 - total flux cleaned = -0.000133938 Jy ! Component: 500 - total flux cleaned = -0.000202408 Jy ! Component: 550 - total flux cleaned = -0.000202419 Jy ! Component: 600 - total flux cleaned = -0.000218984 Jy ! Component: 650 - total flux cleaned = -0.000301674 Jy ! Component: 700 - total flux cleaned = -0.000317995 Jy ! Component: 750 - total flux cleaned = -0.000382762 Jy ! Component: 800 - total flux cleaned = -0.000382714 Jy ! Component: 850 - total flux cleaned = -0.000446722 Jy ! Component: 900 - total flux cleaned = -0.000446602 Jy ! Component: 950 - total flux cleaned = -0.000478017 Jy ! Component: 1000 - total flux cleaned = -0.000524624 Jy ! Component: 1050 - total flux cleaned = -0.000540007 Jy ! Component: 1100 - total flux cleaned = -0.00061659 Jy ! Component: 1150 - total flux cleaned = -0.000647067 Jy ! Component: 1200 - total flux cleaned = -0.000707222 Jy ! Component: 1250 - total flux cleaned = -0.000722096 Jy ! Component: 1300 - total flux cleaned = -0.000751711 Jy ! Component: 1350 - total flux cleaned = -0.000810757 Jy ! Component: 1400 - total flux cleaned = -0.000810688 Jy ! Component: 1450 - total flux cleaned = -0.00082548 Jy ! Component: 1500 - total flux cleaned = -0.000912382 Jy ! Component: 1550 - total flux cleaned = -0.000898141 Jy ! Component: 1600 - total flux cleaned = -0.000998155 Jy ! Component: 1650 - total flux cleaned = -0.00101251 Jy ! Component: 1700 - total flux cleaned = -0.00106891 Jy ! Component: 1750 - total flux cleaned = -0.00105489 Jy ! Component: 1800 - total flux cleaned = -0.0011108 Jy ! Component: 1850 - total flux cleaned = -0.00111079 Jy ! Component: 1900 - total flux cleaned = -0.00117981 Jy ! Component: 1950 - total flux cleaned = -0.00117988 Jy ! Component: 2000 - total flux cleaned = -0.00123452 Jy ! Component: 2050 - total flux cleaned = -0.0012482 Jy ! Component: 2100 - total flux cleaned = -0.00134269 Jy ! Component: 2150 - total flux cleaned = -0.00132927 Jy ! Component: 2200 - total flux cleaned = -0.00138267 Jy ! Component: 2250 - total flux cleaned = -0.00138266 Jy ! Component: 2300 - total flux cleaned = -0.00143547 Jy ! Component: 2350 - total flux cleaned = -0.00146187 Jy ! Component: 2400 - total flux cleaned = -0.00152737 Jy ! Component: 2450 - total flux cleaned = -0.00147521 Jy ! Component: 2500 - total flux cleaned = -0.00154003 Jy ! Component: 2550 - total flux cleaned = -0.0015918 Jy ! Component: 2600 - total flux cleaned = -0.00156607 Jy ! Component: 2650 - total flux cleaned = -0.00164298 Jy ! Component: 2700 - total flux cleaned = -0.0015919 Jy ! Component: 2750 - total flux cleaned = -0.00161725 Jy ! Component: 2800 - total flux cleaned = -0.00161734 Jy ! Component: 2850 - total flux cleaned = -0.00162997 Jy ! Component: 2900 - total flux cleaned = -0.00163004 Jy ! Component: 2950 - total flux cleaned = -0.00165503 Jy ! Component: 3000 - total flux cleaned = -0.00169241 Jy ! Component: 3050 - total flux cleaned = -0.00168007 Jy ! Component: 3100 - total flux cleaned = -0.00172942 Jy ! Component: 3150 - total flux cleaned = -0.001754 Jy ! Component: 3200 - total flux cleaned = -0.0017418 Jy ! Component: 3250 - total flux cleaned = -0.00176613 Jy ! Component: 3300 - total flux cleaned = -0.00175401 Jy ! Component: 3350 - total flux cleaned = -0.00183871 Jy ! Component: 3400 - total flux cleaned = -0.00182675 Jy ! Component: 3450 - total flux cleaned = -0.00183875 Jy ! Component: 3500 - total flux cleaned = -0.00187461 Jy ! Component: 3550 - total flux cleaned = -0.00188655 Jy ! Component: 3600 - total flux cleaned = -0.00191029 Jy ! Component: 3650 - total flux cleaned = -0.00191029 Jy ! Component: 3700 - total flux cleaned = -0.00189854 Jy ! Component: 3750 - total flux cleaned = -0.00198082 Jy ! Component: 3800 - total flux cleaned = -0.00194564 Jy ! Component: 3850 - total flux cleaned = -0.00193391 Jy ! Component: 3900 - total flux cleaned = -0.00194555 Jy ! Component: 3950 - total flux cleaned = -0.0019919 Jy ! Component: 4000 - total flux cleaned = -0.00198025 Jy ! Component: 4050 - total flux cleaned = -0.00199179 Jy ! Total flux subtracted in 4096 components = -0.00196888 Jy ! Clean residual min=-0.000626 max=0.000673 Jy/beam ! Clean residual mean=-0.000001 rms=0.000186 Jy/beam ! Combined flux in latest and established models = 0.0544 Jy keep ! Adding 344 model components to the UV plane model. ! The established model now contains 409 components and 0.0544 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J0945+5757_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6676 x 1.121 at -12.69 degrees (North through East) ! Clean map min=-0.00092721 max=0.051328 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J0945+5757_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0513281 invert ! Inverting map ! Your choice of large map pixels excluded 1.29% of the data. ! The x-axis pixel size should ideally be below 0.1952 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000186315 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -1.08896 1.08896 2.17792 4.35585 8.71169 17.4234 34.8468 69.6936 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0005 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.051 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 275.491 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J0945+5757_X_uvs.log closed on Sat Dec 26 09:35:30 2015