! Started logfile: /scr/pima/gb073_uvs/J0133+2427_X_uvs.log on Sat Dec 26 09:31:27 2015 obs /scr/pima/gb073_uvs/J0133+2427_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J0133+2427_X_uva.fits ! AN table 1: 29 integrations on 55 of 55 possible baselines. ! AN table 2: 21 integrations on 45 of 45 possible baselines. ! AN table 3: 29 integrations on 10 of 10 possible baselines. ! AN table 4: 58 integrations on 28 of 28 possible baselines. ! AN table 5: 21 integrations on 55 of 55 possible baselines. ! AN table 6: 29 integrations on 55 of 55 possible baselines. ! Apparent sampling: 0.941421 visibilities/baseline/integration-bin. ! Found source: J0133+2427 ! ! 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 54256 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/J0133+2427_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 1 telescope corrections were flagged in sub-array 1. ! A total of 21 telescope corrections were flagged in sub-array 2. ! A total of 21 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 1 telescope corrections were flagged in sub-array 1. ! A total of 21 telescope corrections were flagged in sub-array 2. ! A total of 21 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 1 telescope corrections were flagged in sub-array 1. ! A total of 21 telescope corrections were flagged in sub-array 2. ! A total of 21 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 1 telescope corrections were flagged in sub-array 1. ! A total of 21 telescope corrections were flagged in sub-array 2. ! A total of 21 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 5. ! A total of 30 telescope corrections were flagged in sub-array 1. ! A total of 42 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 42 telescope corrections were flagged in sub-array 5. ! A total of 58 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 6. ! A total of 30 telescope corrections were flagged in sub-array 1. ! A total of 42 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 42 telescope corrections were flagged in sub-array 5. ! A total of 58 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 7. ! A total of 1 telescope corrections were flagged in sub-array 1. ! A total of 21 telescope corrections were flagged in sub-array 2. ! A total of 21 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 8. ! A total of 1 telescope corrections were flagged in sub-array 1. ! A total of 21 telescope corrections were flagged in sub-array 2. ! A total of 21 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.007099Jy sigma=9.869355 ! Fit after self-cal, rms=0.929000Jy sigma=9.074524 ! 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 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! Estimated beam: bmin=0.4946 mas, bmaj=1.216 mas, bpa=-10.83 degrees ! Estimated noise=0.775046 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 = 0.0548983 Jy ! Component: 100 - total flux cleaned = 0.0688013 Jy ! Total flux subtracted in 100 components = 0.0688013 Jy ! Clean residual min=-0.003022 max=0.006124 Jy/beam ! Clean residual mean=-0.000001 rms=0.000631 Jy/beam ! Combined flux in latest and established models = 0.0688013 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.0688013 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=0.081472Jy sigma=0.680186 ! Fit after self-cal, rms=0.080643Jy sigma=0.673739 ! Inverting map ! Your choice of large map pixels excluded 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0073433 Jy ! Component: 100 - total flux cleaned = 0.0113272 Jy ! Total flux subtracted in 100 components = 0.0113272 Jy ! Clean residual min=-0.002323 max=0.002493 Jy/beam ! Clean residual mean=-0.000000 rms=0.000547 Jy/beam ! Combined flux in latest and established models = 0.0801285 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 11 components and 0.0801285 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=0.079779Jy sigma=0.661970 ! Fit after self-cal, rms=0.079729Jy sigma=0.661769 ! Inverting map ! Your choice of large map pixels excluded 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 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 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! Estimated beam: bmin=0.6522 mas, bmaj=1.494 mas, bpa=-8.753 degrees ! Estimated noise=0.34705 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 = 0.00386797 Jy ! Component: 100 - total flux cleaned = 0.00560863 Jy ! Component: 150 - total flux cleaned = 0.00653886 Jy ! Component: 200 - total flux cleaned = 0.00705456 Jy ! Total flux subtracted in 200 components = 0.00705456 Jy ! Clean residual min=-0.001188 max=0.001915 Jy/beam ! Clean residual mean=-0.000000 rms=0.000289 Jy/beam ! Combined flux in latest and established models = 0.087183 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 29 components and 0.087183 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=0.079578Jy sigma=0.659931 ! Fit after self-cal, rms=0.079552Jy sigma=0.659843 ! Inverting map ! Your choice of large map pixels excluded 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! Added new window around map position (3.2, 0.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00144176 Jy ! Component: 100 - total flux cleaned = 0.00174278 Jy ! Component: 150 - total flux cleaned = 0.00184901 Jy ! Component: 200 - total flux cleaned = 0.00191559 Jy ! Total flux subtracted in 200 components = 0.00191559 Jy ! Clean residual min=-0.001131 max=0.001350 Jy/beam ! Clean residual mean=0.000001 rms=0.000278 Jy/beam ! Combined flux in latest and established models = 0.0890986 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 42 components and 0.0890986 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=0.079519Jy sigma=0.659460 ! Fit after self-cal, rms=0.079510Jy sigma=0.659391 ! Inverting map ! Your choice of large map pixels excluded 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6522 x 1.494 at -8.753 degrees (North through East) ! Clean map min=-0.0010329 max=0.075839 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 0.94 FD 0.99 KP 0.98 LA 1.06 ! MC 0.90 MK 1.01 NL 0.94 ON 0.86 ! OV 1.02 PT 0.96 SC 1.02 ! ! 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* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! FD 1.00* KP 1.00* MC 1.00* ON 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 FD 0.94 KP 0.98 LA 1.04 ! MK 0.97 NL 0.99 PT 0.95 SC 0.96 ! ! Telescope amplitude corrections in sub-array 5: ! 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* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.93 EF 1.00* FD 1.07 KP 0.96 ! LA 1.03 MC 0.97 NL 0.99 ON 0.97 ! OV 1.01 PT 0.99 SC 0.92 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.05 FD 1.00 KP 1.03 LA 1.09 ! MC 0.97 MK 1.12 NL 1.00 ON 0.91 ! OV 1.03 PT 1.06 SC 0.95 ! ! 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* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! FD 1.00* KP 1.00* MC 1.00* ON 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.06 FD 1.04 KP 1.00 LA 1.07 ! MK 1.00 NL 1.03 PT 1.00 SC 1.00 ! ! Telescope amplitude corrections in sub-array 5: ! 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* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.99 EF 1.00* FD 1.08 KP 0.96 ! LA 1.03 MC 1.08 NL 1.01 ON 0.97 ! OV 1.08 PT 1.03 SC 1.00 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 1.01 KP 1.01 LA 0.98 ! MC 0.96 MK 0.97 NL 1.01 ON 0.96 ! OV 0.97 PT 0.99 SC 1.05 ! ! 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* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! FD 1.00* KP 1.00* MC 1.00* ON 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.04 FD 1.02 KP 0.94 LA 0.97 ! MK 0.96 NL 1.02 PT 1.02 SC 0.97 ! ! Telescope amplitude corrections in sub-array 5: ! 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* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.01 EF 1.00* FD 1.00 KP 0.95 ! LA 0.96 MC 1.11 NL 0.94 ON 0.95 ! OV 1.00 PT 1.02 SC 1.02 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.95 FD 1.07 KP 0.98 LA 1.01 ! MC 0.93 MK 0.96 NL 0.96 ON 0.93 ! OV 1.01 PT 1.06 SC 0.98 ! ! 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* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! FD 1.00 KP 0.96 MC 0.92 ON 0.97 ! SC 0.91 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 FD 0.96 KP 0.95 LA 0.98 ! MK 0.98 NL 1.09 PT 1.03 SC 1.01 ! ! Telescope amplitude corrections in sub-array 5: ! 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* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.98 EF 1.00* FD 0.99 KP 1.02 ! LA 0.99 MC 1.14 NL 0.98 ON 0.89 ! OV 0.98 PT 1.06 SC 1.03 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.03 KP 0.90 LA 0.99 ! MC 1.14 MK 0.99 NL 1.02 ON 1.06 ! OV 1.03 PT 0.96 SC 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* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! FD 0.91 KP 0.96 MC 1.10 ON 1.05 ! SC 0.94 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 0.99 KP 0.95 LA 0.99 ! MK 0.97 NL 1.04 PT 0.94 SC 1.00 ! ! Telescope amplitude corrections in sub-array 5: ! 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* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 0.97 KP 0.93 ! LA 0.98 MC 1.14 NL 0.99 ON 1.02 ! OV 1.15 PT 0.97 SC 1.05 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.98 KP 0.94 LA 1.01 ! MC 1.09 MK 0.95 NL 0.97 ON 1.10 ! OV 0.99 PT 0.93 SC 0.98 ! ! 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* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! FD 0.91 KP 0.86 MC 1.06 ON 1.05 ! SC 0.91 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 0.94 KP 0.95 LA 0.98 ! MK 0.95 NL 1.04 PT 0.93 SC 1.02 ! ! Telescope amplitude corrections in sub-array 5: ! 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* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! 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 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MC 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 2: ! BR 1.00* EF 1.00* FD 1.00* LA 1.00* ! MC 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! FD 1.00* KP 1.00* MC 1.00* ON 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.06 FD 1.02 KP 0.95 LA 1.00 ! MK 1.01 NL 1.07 PT 1.01 SC 1.06 ! ! Telescope amplitude corrections in sub-array 5: ! 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* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.97 EF 1.00* FD 1.07 KP 0.90 ! LA 1.04 MC 1.15 NL 0.98 ON 1.14 ! OV 1.14 PT 0.99 SC 1.06 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MC 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 2: ! BR 1.00* EF 1.00* FD 1.00* LA 1.00* ! MC 1.00* NL 1.00* ON 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! FD 1.00* KP 1.00* MC 1.00* ON 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 FD 0.98 KP 0.91 LA 1.03 ! MK 1.07 NL 1.11 PT 1.02 SC 0.96 ! ! Telescope amplitude corrections in sub-array 5: ! 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* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! 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* ! ! ! Fit before self-cal, rms=0.079510Jy sigma=0.659391 ! Fit after self-cal, rms=0.079492Jy sigma=0.657927 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! Estimated beam: bmin=0.6536 mas, bmaj=1.494 mas, bpa=-8.763 degrees ! Estimated noise=0.346555 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 (16.8, 14). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00115694 Jy ! Component: 100 - total flux cleaned = 0.0013935 Jy ! Component: 150 - total flux cleaned = 0.00146653 Jy ! Component: 200 - total flux cleaned = 0.00150707 Jy ! Total flux subtracted in 200 components = 0.00150707 Jy ! Clean residual min=-0.001187 max=0.001039 Jy/beam ! Clean residual mean=0.000000 rms=0.000249 Jy/beam ! Combined flux in latest and established models = 0.0906057 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 55 components and 0.0906057 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=0.079465Jy sigma=0.657736 ! Fit after self-cal, rms=0.079479Jy sigma=0.657655 ! Inverting map ! Your choice of large map pixels excluded 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 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=0.079479Jy sigma=0.657655 ! Fit after self-cal, rms=0.079233Jy sigma=0.657267 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! Estimated beam: bmin=0.6525 mas, bmaj=1.49 mas, bpa=-8.84 degrees ! Estimated noise=0.346488 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00052809 Jy ! Component: 100 - total flux cleaned = 0.00059029 Jy ! Component: 150 - total flux cleaned = 0.000627226 Jy ! Component: 200 - total flux cleaned = 0.000678761 Jy ! Total flux subtracted in 200 components = 0.000678761 Jy ! Clean residual min=-0.001092 max=0.001049 Jy/beam ! Clean residual mean=0.000000 rms=0.000239 Jy/beam ! Combined flux in latest and established models = 0.0912844 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 63 components and 0.0912844 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=0.079222Jy sigma=0.657205 ! Fit after self-cal, rms=0.079224Jy sigma=0.657183 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 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 = 0.000208108 Jy ! Component: 100 - total flux cleaned = 0.000257479 Jy ! Component: 150 - total flux cleaned = 0.000288362 Jy ! Component: 200 - total flux cleaned = 0.000317561 Jy ! Total flux subtracted in 200 components = 0.000317561 Jy ! Clean residual min=-0.001078 max=0.001056 Jy/beam ! Clean residual mean=0.000000 rms=0.000239 Jy/beam ! Combined flux in latest and established models = 0.091602 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 69 components and 0.091602 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=0.079217Jy sigma=0.657145 ! Fit after self-cal, rms=0.079219Jy sigma=0.657132 ! Inverting map ! Your choice of large map pixels excluded 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 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=0.079219Jy sigma=0.657132 ! Fit after self-cal, rms=0.079305Jy sigma=0.656746 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! Estimated beam: bmin=0.6525 mas, bmaj=1.491 mas, bpa=-8.843 degrees ! Estimated noise=0.346377 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -3.14078e-05 Jy ! Component: 100 - total flux cleaned = -4.65771e-05 Jy ! Component: 150 - total flux cleaned = -3.22063e-05 Jy ! Component: 200 - total flux cleaned = 7.73521e-06 Jy ! Total flux subtracted in 200 components = 7.73521e-06 Jy ! Clean residual min=-0.001056 max=0.000947 Jy/beam ! Clean residual mean=0.000000 rms=0.000228 Jy/beam ! Combined flux in latest and established models = 0.0916097 Jy selfcal ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 79 components and 0.0916097 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=0.079300Jy sigma=0.656704 ! Fit after self-cal, rms=0.079314Jy sigma=0.656666 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 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 = -2.93539e-05 Jy ! Component: 100 - total flux cleaned = -3.38943e-06 Jy ! Component: 150 - total flux cleaned = 9.25567e-06 Jy ! Component: 200 - total flux cleaned = 8.93425e-06 Jy ! Total flux subtracted in 200 components = 8.93425e-06 Jy ! Clean residual min=-0.001052 max=0.000949 Jy/beam ! Clean residual mean=0.000000 rms=0.000228 Jy/beam ! Combined flux in latest and established models = 0.0916187 Jy ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 83 components and 0.0916187 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=0.079310Jy sigma=0.656639 ! Fit after self-cal, rms=0.079310Jy sigma=0.656639 ! Inverting map ! Your choice of large map pixels excluded 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 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=0.079310Jy sigma=0.656639 ! Fit after self-cal, rms=0.079290Jy sigma=0.656646 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! Estimated beam: bmin=2.582 mas, bmaj=2.932 mas, bpa=0.9151 degrees ! Estimated noise=0.453971 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00030039 Jy ! Component: 100 - total flux cleaned = -0.00037962 Jy ! Component: 150 - total flux cleaned = -0.00040252 Jy ! Component: 200 - total flux cleaned = -0.000424238 Jy ! Total flux subtracted in 200 components = -0.000424238 Jy ! Clean residual min=-0.001163 max=0.001035 Jy/beam ! Clean residual mean=0.000001 rms=0.000278 Jy/beam ! Combined flux in latest and established models = 0.0911945 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 90 components and 0.0911945 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=0.079289Jy sigma=0.656628 ! Fit after self-cal, rms=0.079291Jy sigma=0.656625 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 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 = -6.66879e-05 Jy ! Component: 100 - total flux cleaned = -8.117e-05 Jy ! Component: 150 - total flux cleaned = -8.7919e-05 Jy ! Component: 200 - total flux cleaned = -9.43065e-05 Jy ! Total flux subtracted in 200 components = -9.43065e-05 Jy ! Clean residual min=-0.001140 max=0.001027 Jy/beam ! Clean residual mean=0.000001 rms=0.000277 Jy/beam ! Combined flux in latest and established models = 0.0911002 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 90 components and 0.0911002 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=0.079290Jy sigma=0.656622 ! Fit after self-cal, rms=0.079289Jy sigma=0.656619 ! Inverting map ! Your choice of large map pixels excluded 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 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 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! Estimated beam: bmin=0.6523 mas, bmaj=1.491 mas, bpa=-8.857 degrees ! Estimated noise=0.346267 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6523 x 1.491 at -8.857 degrees (North through East) ! Clean map min=-0.00088047 max=0.075791 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 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! Estimated beam: bmin=0.4954 mas, bmaj=1.215 mas, bpa=-10.93 degrees ! Estimated noise=0.771874 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0551525 Jy ! Component: 100 - total flux cleaned = 0.0695554 Jy ! Component: 150 - total flux cleaned = 0.076644 Jy ! Component: 200 - total flux cleaned = 0.080549 Jy ! Total flux subtracted in 200 components = 0.080549 Jy ! Clean residual min=-0.002379 max=0.002338 Jy/beam ! Clean residual mean=-0.000000 rms=0.000536 Jy/beam ! Combined flux in latest and established models = 0.080549 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 0.080549 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! Estimated beam: bmin=0.6523 mas, bmaj=1.491 mas, bpa=-8.857 degrees ! Estimated noise=0.346267 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 = 0.00399245 Jy ! Component: 100 - total flux cleaned = 0.00636461 Jy ! Component: 150 - total flux cleaned = 0.00803999 Jy ! Component: 200 - total flux cleaned = 0.00925257 Jy ! Total flux subtracted in 200 components = 0.00925257 Jy ! Clean residual min=-0.001111 max=0.000996 Jy/beam ! Clean residual mean=-0.000000 rms=0.000238 Jy/beam ! Combined flux in latest and established models = 0.0898016 Jy ! Adding 25 model components to the UV plane model. ! The established model now contains 36 components and 0.0898016 Jy ! Inverting map ! Your choice of large map pixels excluded 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 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 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! Estimated beam: bmin=2.582 mas, bmaj=2.932 mas, bpa=0.9151 degrees ! Estimated noise=0.453971 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00110274 Jy ! Component: 100 - total flux cleaned = 0.00137212 Jy ! Component: 150 - total flux cleaned = 0.00141189 Jy ! Component: 200 - total flux cleaned = 0.0014591 Jy ! Total flux subtracted in 200 components = 0.0014591 Jy ! Clean residual min=-0.001089 max=0.001047 Jy/beam ! Clean residual mean=0.000000 rms=0.000278 Jy/beam ! Combined flux in latest and established models = 0.0912607 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 = 1.32911e-05 Jy ! Component: 100 - total flux cleaned = 1.21602e-06 Jy ! Component: 150 - total flux cleaned = -9.31191e-06 Jy ! Component: 200 - total flux cleaned = -1.91832e-05 Jy ! Total flux subtracted in 200 components = -1.91832e-05 Jy ! Clean residual min=-0.001096 max=0.001046 Jy/beam ! Clean residual mean=0.000000 rms=0.000277 Jy/beam ! Combined flux in latest and established models = 0.0912415 Jy ! Adding 21 model components to the UV plane model. ! The established model now contains 54 components and 0.0912415 Jy ! Inverting map ! Your choice of large map pixels excluded 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! Estimated beam: bmin=0.6523 mas, bmaj=1.491 mas, bpa=-8.857 degrees ! Estimated noise=0.346267 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000124637 Jy ! Component: 100 - total flux cleaned = -0.000208028 Jy ! Component: 150 - total flux cleaned = -0.000232467 Jy ! Component: 200 - total flux cleaned = -0.000209016 Jy ! Total flux subtracted in 200 components = -0.000209016 Jy ! Clean residual min=-0.001086 max=0.000928 Jy/beam ! Clean residual mean=0.000000 rms=0.000230 Jy/beam ! Combined flux in latest and established models = 0.0910325 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 65 components and 0.0910325 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=0.079311Jy sigma=0.656785 ! Fit after self-cal, rms=0.079301Jy sigma=0.656729 wmodel /scr/pima/gb073_uvs/J0133+2427_X_map.mod ! Writing 65 model components to file: /scr/pima/gb073_uvs/J0133+2427_X_map.mod wobs /scr/pima/gb073_uvs/J0133+2427_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J0133+2427_X_uvs.fits wwins /scr/pima/gb073_uvs/J0133+2427_X_map.win ! wwins: Wrote 3 windows to /scr/pima/gb073_uvs/J0133+2427_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 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000404467 Jy ! Component: 100 - total flux cleaned = -0.000596561 Jy ! Component: 150 - total flux cleaned = -0.00078201 Jy ! Component: 200 - total flux cleaned = -0.000897389 Jy ! Component: 250 - total flux cleaned = -0.00104307 Jy ! Component: 300 - total flux cleaned = -0.00120154 Jy ! Component: 350 - total flux cleaned = -0.00129492 Jy ! Component: 400 - total flux cleaned = -0.00134074 Jy ! Component: 450 - total flux cleaned = -0.00140137 Jy ! Component: 500 - total flux cleaned = -0.00149115 Jy ! Component: 550 - total flux cleaned = -0.00155013 Jy ! Component: 600 - total flux cleaned = -0.00156475 Jy ! Component: 650 - total flux cleaned = -0.00162286 Jy ! Component: 700 - total flux cleaned = -0.00163735 Jy ! Component: 750 - total flux cleaned = -0.00176549 Jy ! Component: 800 - total flux cleaned = -0.00172306 Jy ! Component: 850 - total flux cleaned = -0.00173724 Jy ! Component: 900 - total flux cleaned = -0.00180704 Jy ! Component: 950 - total flux cleaned = -0.00183477 Jy ! Component: 1000 - total flux cleaned = -0.00187592 Jy ! Component: 1050 - total flux cleaned = -0.00188978 Jy ! Component: 1100 - total flux cleaned = -0.00195753 Jy ! Component: 1150 - total flux cleaned = -0.00203837 Jy ! Component: 1200 - total flux cleaned = -0.002065 Jy ! Component: 1250 - total flux cleaned = -0.0020916 Jy ! Component: 1300 - total flux cleaned = -0.00213125 Jy ! Component: 1350 - total flux cleaned = -0.00218368 Jy ! Component: 1400 - total flux cleaned = -0.00224896 Jy ! Component: 1450 - total flux cleaned = -0.00231384 Jy ! Component: 1500 - total flux cleaned = -0.00232684 Jy ! Component: 1550 - total flux cleaned = -0.00237832 Jy ! Component: 1600 - total flux cleaned = -0.00244229 Jy ! Component: 1650 - total flux cleaned = -0.002404 Jy ! Component: 1700 - total flux cleaned = -0.00247989 Jy ! Component: 1750 - total flux cleaned = -0.0025303 Jy ! Component: 1800 - total flux cleaned = -0.00256797 Jy ! Component: 1850 - total flux cleaned = -0.00263036 Jy ! Component: 1900 - total flux cleaned = -0.00259307 Jy ! Component: 1950 - total flux cleaned = -0.00261774 Jy ! Component: 2000 - total flux cleaned = -0.00267935 Jy ! Component: 2050 - total flux cleaned = -0.00260578 Jy ! Component: 2100 - total flux cleaned = -0.00266686 Jy ! Component: 2150 - total flux cleaned = -0.00265473 Jy ! Component: 2200 - total flux cleaned = -0.00265476 Jy ! Component: 2250 - total flux cleaned = -0.00267898 Jy ! Component: 2300 - total flux cleaned = -0.00270307 Jy ! Component: 2350 - total flux cleaned = -0.00277493 Jy ! Component: 2400 - total flux cleaned = -0.00270334 Jy ! Component: 2450 - total flux cleaned = -0.00275081 Jy ! Component: 2500 - total flux cleaned = -0.00278638 Jy ! Component: 2550 - total flux cleaned = -0.00278634 Jy ! Component: 2600 - total flux cleaned = -0.00278637 Jy ! Component: 2650 - total flux cleaned = -0.00279818 Jy ! Component: 2700 - total flux cleaned = -0.00282147 Jy ! Component: 2750 - total flux cleaned = -0.00284469 Jy ! Component: 2800 - total flux cleaned = -0.00290253 Jy ! Component: 2850 - total flux cleaned = -0.00282176 Jy ! Component: 2900 - total flux cleaned = -0.00284479 Jy ! Component: 2950 - total flux cleaned = -0.00287912 Jy ! Component: 3000 - total flux cleaned = -0.00287904 Jy ! Component: 3050 - total flux cleaned = -0.00292464 Jy ! Component: 3100 - total flux cleaned = -0.00289056 Jy ! Component: 3150 - total flux cleaned = -0.00283399 Jy ! Component: 3200 - total flux cleaned = -0.00290169 Jy ! Component: 3250 - total flux cleaned = -0.00292412 Jy ! Component: 3300 - total flux cleaned = -0.00295775 Jy ! Component: 3350 - total flux cleaned = -0.0029131 Jy ! Component: 3400 - total flux cleaned = -0.00289094 Jy ! Component: 3450 - total flux cleaned = -0.00297971 Jy ! Component: 3500 - total flux cleaned = -0.00301293 Jy ! Component: 3550 - total flux cleaned = -0.00295773 Jy ! Component: 3600 - total flux cleaned = -0.00295768 Jy ! Component: 3650 - total flux cleaned = -0.00300154 Jy ! Component: 3700 - total flux cleaned = -0.00300157 Jy ! Component: 3750 - total flux cleaned = -0.00305611 Jy ! Component: 3800 - total flux cleaned = -0.00303433 Jy ! Component: 3850 - total flux cleaned = -0.00302348 Jy ! Component: 3900 - total flux cleaned = -0.00300182 Jy ! Component: 3950 - total flux cleaned = -0.00296952 Jy ! Component: 4000 - total flux cleaned = -0.00300178 Jy ! Component: 4050 - total flux cleaned = -0.00300176 Jy ! Total flux subtracted in 4096 components = -0.00301241 Jy ! Clean residual min=-0.000706 max=0.000657 Jy/beam ! Clean residual mean=-0.000000 rms=0.000180 Jy/beam ! Combined flux in latest and established models = 0.0880201 Jy keep ! Adding 334 model components to the UV plane model. ! The established model now contains 399 components and 0.0880201 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J0133+2427_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6523 x 1.491 at -8.857 degrees (North through East) ! Clean map min=-0.00081261 max=0.075658 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J0133+2427_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0756584 invert ! Inverting map ! Your choice of large map pixels excluded 2.62% of the data. ! The x-axis pixel size should ideally be below 0.1788 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.0001797 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.712543 0.712543 1.42509 2.85017 5.70035 11.4007 22.8014 45.6028 91.2055 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0005 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.075 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 421.027 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J0133+2427_X_uvs.log closed on Sat Dec 26 09:31:33 2015