! Started logfile: /scr/pima/gb073_uvs/J0834+4403_X_uvs.log on Sat Dec 26 09:34:37 2015 obs /scr/pima/gb073_uvs/J0834+4403_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J0834+4403_X_uva.fits ! AN table 1: 58 integrations on 66 of 66 possible baselines. ! AN table 2: 29 integrations on 55 of 55 possible baselines. ! AN table 3: 29 integrations on 55 of 55 possible baselines. ! AN table 4: 29 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.833834 visibilities/baseline/integration-bin. ! Found source: J0834+4403 ! ! 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 55520 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/J0834+4403_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 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 87 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 87 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 87 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 145 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 145 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 58 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 58 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=1.004822Jy sigma=9.961816 ! Fit after self-cal, rms=0.939904Jy sigma=9.317836 ! 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 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! Estimated beam: bmin=0.435 mas, bmaj=1.004 mas, bpa=-20.99 degrees ! Estimated noise=0.753739 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 = 0.0479496 Jy ! Component: 100 - total flux cleaned = 0.0584112 Jy ! Total flux subtracted in 100 components = 0.0584112 Jy ! Clean residual min=-0.002765 max=0.007439 Jy/beam ! Clean residual mean=0.000010 rms=0.000633 Jy/beam ! Combined flux in latest and established models = 0.0584112 Jy ! Performing phase self-cal ! Adding 3 model components to the UV plane model. ! The established model now contains 3 components and 0.0584112 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=0.092152Jy sigma=0.695996 ! Fit after self-cal, rms=0.091109Jy sigma=0.685765 ! Inverting map ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! Added new window around map position (1.4, 5). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00690064 Jy ! Component: 100 - total flux cleaned = 0.0108772 Jy ! Total flux subtracted in 100 components = 0.0108772 Jy ! Clean residual min=-0.002599 max=0.002883 Jy/beam ! Clean residual mean=0.000008 rms=0.000574 Jy/beam ! Combined flux in latest and established models = 0.0692884 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 9 components and 0.0692884 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=0.090427Jy sigma=0.675766 ! Fit after self-cal, rms=0.090332Jy sigma=0.674844 ! Inverting map ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00382929 Jy ! Component: 100 - total flux cleaned = 0.00643094 Jy ! Total flux subtracted in 100 components = 0.00643094 Jy ! Clean residual min=-0.002403 max=0.002730 Jy/beam ! Clean residual mean=0.000006 rms=0.000556 Jy/beam ! Combined flux in latest and established models = 0.0757193 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 15 components and 0.0757193 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=0.090103Jy sigma=0.671250 ! Fit after self-cal, rms=0.090090Jy sigma=0.671003 ! Inverting map ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 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 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! Estimated beam: bmin=0.5849 mas, bmaj=1.261 mas, bpa=-16.8 degrees ! Estimated noise=0.336846 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 = 0.00411817 Jy ! Component: 100 - total flux cleaned = 0.00633829 Jy ! Component: 150 - total flux cleaned = 0.00780589 Jy ! Component: 200 - total flux cleaned = 0.00882126 Jy ! Total flux subtracted in 200 components = 0.00882126 Jy ! Clean residual min=-0.001439 max=0.001766 Jy/beam ! Clean residual mean=0.000008 rms=0.000313 Jy/beam ! Combined flux in latest and established models = 0.0845406 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 30 components and 0.0845406 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=0.089936Jy sigma=0.668390 ! Fit after self-cal, rms=0.089901Jy sigma=0.667869 ! Inverting map ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! Added new window around map position (1.2, -7.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00185306 Jy ! Component: 100 - total flux cleaned = 0.00298729 Jy ! Component: 150 - total flux cleaned = 0.00379733 Jy ! Component: 200 - total flux cleaned = 0.0041357 Jy ! Total flux subtracted in 200 components = 0.0041357 Jy ! Clean residual min=-0.001300 max=0.001244 Jy/beam ! Clean residual mean=0.000003 rms=0.000281 Jy/beam ! Combined flux in latest and established models = 0.0886763 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 40 components and 0.0886763 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=0.089856Jy sigma=0.667316 ! Fit after self-cal, rms=0.089848Jy sigma=0.667228 ! Inverting map ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5849 x 1.261 at -16.8 degrees (North through East) ! Clean map min=-0.001142 max=0.061091 Jy/beam if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.93 EF 1.00* FD 1.02 KP 0.99 ! LA 1.05 MC 0.86 NL 0.93 ON 0.94 ! OV 1.01 PT 0.97 SC 0.98 ZC 0.88 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 EF 1.00* FD 1.00 KP 1.00 ! LA 1.06 MK 1.07 NL 0.95 ON 1.13 ! OV 1.03 PT 0.94 SC 0.93 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.08 EF 1.00* FD 1.03 KP 1.01 ! LA 1.05 MC 0.89 NL 0.98 ON 0.92 ! PT 0.94 SC 0.96 ZC 0.85 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 EF 1.00* FD 1.04 KP 0.97 ! LA 1.03 MK 1.01 NL 0.90 ON 1.15 ! PT 0.96 SC 0.93 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 EF 1.00* FD 1.08 KP 1.00 ! LA 1.08 MC 0.99 NL 0.94 ON 0.87 ! OV 1.08 PT 1.02 SC 1.04 ZC 0.87 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.06 EF 1.00* FD 1.00 KP 1.00 ! LA 1.07 MK 1.03 NL 1.04 ON 0.91 ! OV 1.11 PT 1.01 SC 1.01 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 EF 1.00* FD 1.08 KP 1.16 ! LA 1.08 MC 0.95 NL 0.94 ON 0.95 ! PT 0.91 SC 1.11 ZC 0.87 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.12 EF 1.00* FD 1.09 KP 0.99 ! LA 1.10 MK 0.99 NL 1.02 ON 1.13 ! PT 1.00 SC 1.02 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.05 EF 1.00* FD 1.02 KP 0.94 ! LA 0.96 MC 1.01 NL 0.96 ON 0.90 ! OV 1.01 PT 1.01 SC 1.09 ZC 0.94 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 EF 1.00* FD 1.04 KP 1.02 ! LA 1.02 MK 1.01 NL 0.98 ON 0.84 ! OV 0.98 PT 0.97 SC 0.95 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.96 EF 1.00* FD 1.00 KP 0.99 ! LA 1.01 MC 0.93 NL 0.95 ON 0.97 ! PT 0.97 SC 1.11 ZC 0.86 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 EF 1.00* FD 1.01 KP 0.94 ! LA 1.02 MK 1.01 NL 1.00 ON 0.89 ! PT 0.98 SC 0.98 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 EF 1.00* FD 1.01 KP 0.97 ! LA 0.98 MC 1.00 NL 1.02 ON 1.06 ! OV 1.02 PT 1.04 SC 1.00 ZC 0.96 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 EF 1.00* FD 1.05 KP 1.06 ! LA 1.06 MK 1.04 NL 1.00 ON 0.88 ! OV 1.04 PT 1.02 SC 0.99 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 EF 1.00* FD 1.03 KP 0.99 ! LA 0.95 MC 1.03 NL 1.09 ON 0.93 ! PT 1.06 SC 1.00 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 EF 1.00* FD 1.02 KP 0.99 ! LA 0.98 MK 0.96 NL 1.06 ON 0.96 ! PT 1.02 SC 0.99 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.05 KP 0.94 ! LA 0.95 MC 1.19 NL 1.05 ON 1.22 ! OV 0.99 PT 0.95 SC 1.02 ZC 1.03 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 0.95 KP 0.90 ! LA 1.05 MK 0.99 NL 1.02 ON 1.22 ! OV 0.99 PT 1.00 SC 1.09 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 0.98 KP 0.90 ! LA 1.03 MC 1.26 NL 0.97 ON 1.15 ! PT 0.98 SC 1.03 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.05 KP 0.95 ! LA 1.16 MK 1.02 NL 0.96 ON 1.03 ! PT 0.93 SC 0.93 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.03 KP 0.94 ! LA 0.94 MC 1.13 NL 1.03 ON 1.17 ! OV 1.04 PT 0.96 SC 0.98 ZC 0.83 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.01 KP 0.90 ! LA 1.01 MK 1.00 NL 1.02 ON 1.21 ! OV 1.06 PT 0.89 SC 0.98 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.09 KP 0.91 ! LA 1.02 MC 1.19 NL 1.00 ON 1.44 ! PT 0.91 SC 0.89 ZC 0.85 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.08 KP 0.93 ! LA 0.99 MK 0.99 NL 1.13 ON 0.92 ! PT 0.98 SC 0.90 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 EF 1.00* FD 1.02 KP 0.92 ! LA 1.01 MC 1.12 NL 1.06 ON 1.27 ! OV 0.97 PT 1.05 SC 1.02 ZC 0.65 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.93 EF 1.00* FD 1.05 KP 0.98 ! LA 1.07 MK 1.02 NL 0.99 ON 1.19 ! OV 0.93 PT 1.06 SC 0.96 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.06 EF 1.00* FD 1.00 KP 0.89 ! LA 1.04 MC 1.30 NL 1.06 ON 1.21 ! PT 0.94 SC 1.04 ZC 0.71 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 EF 1.00* FD 1.01 KP 0.86 ! LA 1.08 MK 1.08 NL 0.98 ON 1.17 ! PT 0.95 SC 0.93 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 EF 1.00* FD 1.04 KP 0.92 ! LA 1.04 MC 1.16 NL 1.03 ON 1.26 ! OV 0.99 PT 0.98 SC 1.04 ZC 0.63 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 EF 1.00* FD 1.03 KP 0.91 ! LA 1.09 MK 1.13 NL 1.08 ON 1.08 ! OV 0.98 PT 1.02 SC 0.95 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 EF 1.00* FD 1.08 KP 0.90 ! LA 1.01 MC 1.25 NL 0.96 ON 1.10 ! PT 1.02 SC 1.12 ZC 0.73 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.04 EF 1.00* FD 1.03 KP 0.96 ! LA 1.08 MK 0.99 NL 0.99 ON 1.25 ! PT 0.97 SC 0.99 ! ! ! Fit before self-cal, rms=0.089848Jy sigma=0.667228 ! Fit after self-cal, rms=0.084468Jy sigma=0.664098 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! Estimated beam: bmin=0.5817 mas, bmaj=1.265 mas, bpa=-17.15 degrees ! Estimated noise=0.337849 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 = 0.000579423 Jy ! Component: 100 - total flux cleaned = 0.000778345 Jy ! Component: 150 - total flux cleaned = 0.000819579 Jy ! Component: 200 - total flux cleaned = 0.000802925 Jy ! Total flux subtracted in 200 components = 0.000802925 Jy ! Clean residual min=-0.001081 max=0.000996 Jy/beam ! Clean residual mean=-0.000000 rms=0.000240 Jy/beam ! Combined flux in latest and established models = 0.0894792 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 51 components and 0.0894792 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=0.084454Jy sigma=0.663976 ! Fit after self-cal, rms=0.084496Jy sigma=0.663699 ! Inverting map ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 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=0.084496Jy sigma=0.663699 ! Fit after self-cal, rms=0.080929Jy sigma=0.662208 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! Estimated beam: bmin=0.5812 mas, bmaj=1.265 mas, bpa=-17.2 degrees ! Estimated noise=0.338651 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000571502 Jy ! Component: 100 - total flux cleaned = 0.000595994 Jy ! Component: 150 - total flux cleaned = 0.000579661 Jy ! Component: 200 - total flux cleaned = 0.000536326 Jy ! Total flux subtracted in 200 components = 0.000536326 Jy ! Clean residual min=-0.000999 max=0.001003 Jy/beam ! Clean residual mean=-0.000000 rms=0.000233 Jy/beam ! Combined flux in latest and established models = 0.0900155 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 58 components and 0.0900155 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=0.080919Jy sigma=0.662134 ! Fit after self-cal, rms=0.080930Jy sigma=0.661959 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 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 (0.6, 2.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000976041 Jy ! Component: 100 - total flux cleaned = 0.000983036 Jy ! Component: 150 - total flux cleaned = 0.00093349 Jy ! Component: 200 - total flux cleaned = 0.000889297 Jy ! Total flux subtracted in 200 components = 0.000889297 Jy ! Clean residual min=-0.000975 max=0.000961 Jy/beam ! Clean residual mean=-0.000001 rms=0.000226 Jy/beam ! Combined flux in latest and established models = 0.0909048 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 76 components and 0.0909048 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=0.080917Jy sigma=0.661796 ! Fit after self-cal, rms=0.080918Jy sigma=0.661776 ! Inverting map ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 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=0.080918Jy sigma=0.661776 ! Fit after self-cal, rms=0.080986Jy sigma=0.661727 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! Estimated beam: bmin=0.5801 mas, bmaj=1.263 mas, bpa=-17.29 degrees ! Estimated noise=0.339427 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000670491 Jy ! Component: 100 - total flux cleaned = 0.000834458 Jy ! Component: 150 - total flux cleaned = 0.000834081 Jy ! Component: 200 - total flux cleaned = 0.000820285 Jy ! Total flux subtracted in 200 components = 0.000820285 Jy ! Clean residual min=-0.000982 max=0.000950 Jy/beam ! Clean residual mean=-0.000001 rms=0.000224 Jy/beam ! Combined flux in latest and established models = 0.0917251 Jy selfcal ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 84 components and 0.0917251 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=0.080978Jy sigma=0.661646 ! Fit after self-cal, rms=0.080980Jy sigma=0.661633 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 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 = 9.88658e-05 Jy ! Component: 100 - total flux cleaned = 8.60193e-05 Jy ! Component: 150 - total flux cleaned = 8.65152e-05 Jy ! Component: 200 - total flux cleaned = 8.64428e-05 Jy ! Total flux subtracted in 200 components = 8.64428e-05 Jy ! Clean residual min=-0.000993 max=0.000946 Jy/beam ! Clean residual mean=-0.000001 rms=0.000223 Jy/beam ! Combined flux in latest and established models = 0.0918115 Jy ! Performing phase self-cal ! Adding 33 model components to the UV plane model. ! The established model now contains 88 components and 0.0918115 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=0.080976Jy sigma=0.661600 ! Fit after self-cal, rms=0.080975Jy sigma=0.661596 ! Inverting map ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 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=0.080975Jy sigma=0.661596 ! Fit after self-cal, rms=0.080993Jy sigma=0.661575 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! Estimated beam: bmin=2.639 mas, bmaj=2.871 mas, bpa=14.37 degrees ! Estimated noise=0.453547 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000545782 Jy ! Component: 100 - total flux cleaned = 0.00056273 Jy ! Component: 150 - total flux cleaned = 0.000587684 Jy ! Component: 200 - total flux cleaned = 0.000637912 Jy ! Total flux subtracted in 200 components = 0.000637912 Jy ! Clean residual min=-0.000956 max=0.001091 Jy/beam ! Clean residual mean=-0.000001 rms=0.000290 Jy/beam ! Combined flux in latest and established models = 0.0924494 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 95 components and 0.0924494 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=0.080992Jy sigma=0.661553 ! Fit after self-cal, rms=0.080992Jy sigma=0.661542 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 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 = 0.000153559 Jy ! Component: 100 - total flux cleaned = 0.000154094 Jy ! Component: 150 - total flux cleaned = 0.000137475 Jy ! Component: 200 - total flux cleaned = 0.000129924 Jy ! Total flux subtracted in 200 components = 0.000129924 Jy ! Clean residual min=-0.000932 max=0.001098 Jy/beam ! Clean residual mean=-0.000002 rms=0.000289 Jy/beam ! Combined flux in latest and established models = 0.0925793 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 98 components and 0.0925794 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=0.080993Jy sigma=0.661548 ! Fit after self-cal, rms=0.080993Jy sigma=0.661544 ! Inverting map ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 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 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! Estimated beam: bmin=0.579 mas, bmaj=1.26 mas, bpa=-17.38 degrees ! Estimated noise=0.340134 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.579 x 1.26 at -17.38 degrees (North through East) ! Clean map min=-0.00090727 max=0.061493 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 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! Estimated beam: bmin=0.4307 mas, bmaj=1.008 mas, bpa=-21.59 degrees ! Estimated noise=0.754256 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0487887 Jy ! Component: 100 - total flux cleaned = 0.0624526 Jy ! Component: 150 - total flux cleaned = 0.0693249 Jy ! Component: 200 - total flux cleaned = 0.0738172 Jy ! Total flux subtracted in 200 components = 0.0738172 Jy ! Clean residual min=-0.002293 max=0.002472 Jy/beam ! Clean residual mean=0.000007 rms=0.000537 Jy/beam ! Combined flux in latest and established models = 0.0738172 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 11 model components to the UV plane model. ! The established model now contains 11 components and 0.0738172 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! Estimated beam: bmin=0.579 mas, bmaj=1.26 mas, bpa=-17.38 degrees ! Estimated noise=0.340134 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 = 0.00557932 Jy ! Component: 100 - total flux cleaned = 0.00893722 Jy ! Component: 150 - total flux cleaned = 0.011291 Jy ! Component: 200 - total flux cleaned = 0.0130212 Jy ! Total flux subtracted in 200 components = 0.0130212 Jy ! Clean residual min=-0.001121 max=0.001366 Jy/beam ! Clean residual mean=0.000007 rms=0.000258 Jy/beam ! Combined flux in latest and established models = 0.0868384 Jy ! Adding 38 model components to the UV plane model. ! The established model now contains 42 components and 0.0868384 Jy ! Inverting map ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! Added new window around map position (2.2, 4.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00145491 Jy ! Component: 100 - total flux cleaned = 0.00255842 Jy ! Component: 150 - total flux cleaned = 0.00342838 Jy ! Component: 200 - total flux cleaned = 0.00394542 Jy ! Total flux subtracted in 200 components = 0.00394542 Jy ! Clean residual min=-0.000997 max=0.000942 Jy/beam ! Clean residual mean=0.000002 rms=0.000227 Jy/beam ! Combined flux in latest and established models = 0.0907838 Jy ! Adding 34 model components to the UV plane model. ! The established model now contains 64 components and 0.0907838 Jy ! Inverting map ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 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 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! Estimated beam: bmin=2.639 mas, bmaj=2.871 mas, bpa=14.37 degrees ! Estimated noise=0.453547 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000882671 Jy ! Component: 100 - total flux cleaned = 0.00115007 Jy ! Component: 150 - total flux cleaned = 0.00133498 Jy ! Component: 200 - total flux cleaned = 0.00149281 Jy ! Total flux subtracted in 200 components = 0.00149281 Jy ! Clean residual min=-0.000960 max=0.001090 Jy/beam ! Clean residual mean=-0.000000 rms=0.000287 Jy/beam ! Combined flux in latest and established models = 0.0922766 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 = 0.000122118 Jy ! Component: 100 - total flux cleaned = 0.000167714 Jy ! Component: 150 - total flux cleaned = 0.000175217 Jy ! Component: 200 - total flux cleaned = 0.000182114 Jy ! Total flux subtracted in 200 components = 0.000182114 Jy ! Clean residual min=-0.000956 max=0.001095 Jy/beam ! Clean residual mean=-0.000001 rms=0.000286 Jy/beam ! Combined flux in latest and established models = 0.0924587 Jy ! Adding 32 model components to the UV plane model. ! The established model now contains 92 components and 0.0924587 Jy ! Inverting map ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! Estimated beam: bmin=0.579 mas, bmaj=1.26 mas, bpa=-17.38 degrees ! Estimated noise=0.340134 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000273405 Jy ! Component: 100 - total flux cleaned = -0.000274301 Jy ! Component: 150 - total flux cleaned = -0.000256973 Jy ! Component: 200 - total flux cleaned = -0.000224761 Jy ! Total flux subtracted in 200 components = -0.000224761 Jy ! Clean residual min=-0.000961 max=0.000961 Jy/beam ! Clean residual mean=-0.000000 rms=0.000219 Jy/beam ! Combined flux in latest and established models = 0.0922339 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 102 components and 0.092234 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=0.080981Jy sigma=0.661474 ! Fit after self-cal, rms=0.080971Jy sigma=0.661427 wmodel /scr/pima/gb073_uvs/J0834+4403_X_map.mod ! Writing 102 model components to file: /scr/pima/gb073_uvs/J0834+4403_X_map.mod wobs /scr/pima/gb073_uvs/J0834+4403_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J0834+4403_X_uvs.fits wwins /scr/pima/gb073_uvs/J0834+4403_X_map.win ! wwins: Wrote 5 windows to /scr/pima/gb073_uvs/J0834+4403_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 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -8.78406e-05 Jy ! Component: 100 - total flux cleaned = -0.00021959 Jy ! Component: 150 - total flux cleaned = -0.000267217 Jy ! Component: 200 - total flux cleaned = -0.000298332 Jy ! Component: 250 - total flux cleaned = -0.000344316 Jy ! Component: 300 - total flux cleaned = -0.000344147 Jy ! Component: 350 - total flux cleaned = -0.000389156 Jy ! Component: 400 - total flux cleaned = -0.000389269 Jy ! Component: 450 - total flux cleaned = -0.000404124 Jy ! Component: 500 - total flux cleaned = -0.000462118 Jy ! Component: 550 - total flux cleaned = -0.000462063 Jy ! Component: 600 - total flux cleaned = -0.000447766 Jy ! Component: 650 - total flux cleaned = -0.000503796 Jy ! Component: 700 - total flux cleaned = -0.000503596 Jy ! Component: 750 - total flux cleaned = -0.000531022 Jy ! Component: 800 - total flux cleaned = -0.000449048 Jy ! Component: 850 - total flux cleaned = -0.000503515 Jy ! Component: 900 - total flux cleaned = -0.000543928 Jy ! Component: 950 - total flux cleaned = -0.000530544 Jy ! Component: 1000 - total flux cleaned = -0.000543886 Jy ! Component: 1050 - total flux cleaned = -0.000530758 Jy ! Component: 1100 - total flux cleaned = -0.000543766 Jy ! Component: 1150 - total flux cleaned = -0.000556768 Jy ! Component: 1200 - total flux cleaned = -0.000569644 Jy ! Component: 1250 - total flux cleaned = -0.000569616 Jy ! Component: 1300 - total flux cleaned = -0.000531355 Jy ! Component: 1350 - total flux cleaned = -0.000531432 Jy ! Component: 1400 - total flux cleaned = -0.000468547 Jy ! Component: 1450 - total flux cleaned = -0.00053097 Jy ! Component: 1500 - total flux cleaned = -0.000506094 Jy ! Component: 1550 - total flux cleaned = -0.000506097 Jy ! Component: 1600 - total flux cleaned = -0.000505971 Jy ! Component: 1650 - total flux cleaned = -0.000579261 Jy ! Component: 1700 - total flux cleaned = -0.00051846 Jy ! Component: 1750 - total flux cleaned = -0.000542648 Jy ! Component: 1800 - total flux cleaned = -0.000590788 Jy ! Component: 1850 - total flux cleaned = -0.000530899 Jy ! Component: 1900 - total flux cleaned = -0.00060253 Jy ! Component: 1950 - total flux cleaned = -0.000566969 Jy ! Component: 2000 - total flux cleaned = -0.000602441 Jy ! Component: 2050 - total flux cleaned = -0.000625953 Jy ! Component: 2100 - total flux cleaned = -0.000614169 Jy ! Component: 2150 - total flux cleaned = -0.000637303 Jy ! Component: 2200 - total flux cleaned = -0.000590877 Jy ! Component: 2250 - total flux cleaned = -0.000613958 Jy ! Component: 2300 - total flux cleaned = -0.000613944 Jy ! Component: 2350 - total flux cleaned = -0.000613925 Jy ! Component: 2400 - total flux cleaned = -0.000511347 Jy ! Component: 2450 - total flux cleaned = -0.000545334 Jy ! Component: 2500 - total flux cleaned = -0.000624565 Jy ! Component: 2550 - total flux cleaned = -0.000568182 Jy ! Component: 2600 - total flux cleaned = -0.000590576 Jy ! Component: 2650 - total flux cleaned = -0.000545805 Jy ! Component: 2700 - total flux cleaned = -0.000534679 Jy ! Component: 2750 - total flux cleaned = -0.000490334 Jy ! Component: 2800 - total flux cleaned = -0.000490353 Jy ! Component: 2850 - total flux cleaned = -0.000523503 Jy ! Component: 2900 - total flux cleaned = -0.000490635 Jy ! Component: 2950 - total flux cleaned = -0.000490602 Jy ! Component: 3000 - total flux cleaned = -0.000479728 Jy ! Component: 3050 - total flux cleaned = -0.000468928 Jy ! Component: 3100 - total flux cleaned = -0.000522994 Jy ! Component: 3150 - total flux cleaned = -0.000523048 Jy ! Component: 3200 - total flux cleaned = -0.000469378 Jy ! Component: 3250 - total flux cleaned = -0.000501491 Jy ! Component: 3300 - total flux cleaned = -0.000490808 Jy ! Component: 3350 - total flux cleaned = -0.000480202 Jy ! Component: 3400 - total flux cleaned = -0.0005014 Jy ! Component: 3450 - total flux cleaned = -0.000575368 Jy ! Component: 3500 - total flux cleaned = -0.000491032 Jy ! Component: 3550 - total flux cleaned = -0.000533121 Jy ! Component: 3600 - total flux cleaned = -0.000554096 Jy ! Component: 3650 - total flux cleaned = -0.000522768 Jy ! Component: 3700 - total flux cleaned = -0.000533235 Jy ! Component: 3750 - total flux cleaned = -0.000595602 Jy ! Component: 3800 - total flux cleaned = -0.000647352 Jy ! Component: 3850 - total flux cleaned = -0.00061635 Jy ! Component: 3900 - total flux cleaned = -0.000647271 Jy ! Component: 3950 - total flux cleaned = -0.000647216 Jy ! Component: 4000 - total flux cleaned = -0.000667718 Jy ! Component: 4050 - total flux cleaned = -0.000698367 Jy ! Total flux subtracted in 4096 components = -0.000688145 Jy ! Clean residual min=-0.000692 max=0.000650 Jy/beam ! Clean residual mean=-0.000000 rms=0.000169 Jy/beam ! Combined flux in latest and established models = 0.0915458 Jy keep ! Adding 358 model components to the UV plane model. ! The established model now contains 460 components and 0.0915459 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J0834+4403_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.579 x 1.26 at -17.38 degrees (North through East) ! Clean map min=-0.0007768 max=0.062059 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J0834+4403_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0620586 invert ! Inverting map ! Your choice of large map pixels excluded 1.89% of the data. ! The x-axis pixel size should ideally be below 0.1821 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000168917 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.816566 0.816566 1.63313 3.26627 6.53253 13.0651 26.1301 52.2602 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0005 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.062 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 367.392 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J0834+4403_X_uvs.log closed on Sat Dec 26 09:34:44 2015