! Started logfile: /scr/pima/gb073_uvs/J1245+5709_X_uvs.log on Sat Dec 26 09:38:51 2015 obs /scr/pima/gb073_uvs/J1245+5709_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1245+5709_X_uva.fits ! AN table 1: 58 integrations on 55 of 55 possible baselines. ! AN table 2: 29 integrations on 45 of 45 possible baselines. ! AN table 3: 29 integrations on 78 of 78 possible baselines. ! AN table 4: 29 integrations on 3 of 3 possible baselines. ! AN table 5: 29 integrations on 36 of 36 possible baselines. ! AN table 6: 29 integrations on 55 of 55 possible baselines. ! AN table 7: 29 integrations on 6 of 6 possible baselines. ! AN table 8: 28 integrations on 3 of 3 possible baselines. ! Apparent sampling: 0.839955 visibilities/baseline/integration-bin. ! Found source: J1245+5709 ! ! 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 65456 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/J1245+5709_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 67 telescope corrections were flagged in sub-array 1. ! A total of 32 telescope corrections were flagged in sub-array 2. ! A total of 34 telescope corrections were flagged in sub-array 3. ! A total of 32 telescope corrections were flagged in sub-array 5. ! A total of 36 telescope corrections were flagged in sub-array 6. ! A total of 84 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 2. ! A total of 67 telescope corrections were flagged in sub-array 1. ! A total of 32 telescope corrections were flagged in sub-array 2. ! A total of 34 telescope corrections were flagged in sub-array 3. ! A total of 32 telescope corrections were flagged in sub-array 5. ! A total of 36 telescope corrections were flagged in sub-array 6. ! A total of 84 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 3. ! A total of 67 telescope corrections were flagged in sub-array 1. ! A total of 32 telescope corrections were flagged in sub-array 2. ! A total of 34 telescope corrections were flagged in sub-array 3. ! A total of 32 telescope corrections were flagged in sub-array 5. ! A total of 36 telescope corrections were flagged in sub-array 6. ! A total of 84 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 4. ! A total of 67 telescope corrections were flagged in sub-array 1. ! A total of 32 telescope corrections were flagged in sub-array 2. ! A total of 34 telescope corrections were flagged in sub-array 3. ! A total of 32 telescope corrections were flagged in sub-array 5. ! A total of 36 telescope corrections were flagged in sub-array 6. ! A total of 84 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 5. ! A total of 125 telescope corrections were flagged in sub-array 1. ! A total of 61 telescope corrections were flagged in sub-array 2. ! A total of 63 telescope corrections were flagged in sub-array 3. ! A total of 87 telescope corrections were flagged in sub-array 4. ! A total of 61 telescope corrections were flagged in sub-array 5. ! A total of 65 telescope corrections were flagged in sub-array 6. ! A total of 29 telescope corrections were flagged in sub-array 7. ! A total of 84 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 6. ! A total of 125 telescope corrections were flagged in sub-array 1. ! A total of 61 telescope corrections were flagged in sub-array 2. ! A total of 63 telescope corrections were flagged in sub-array 3. ! A total of 87 telescope corrections were flagged in sub-array 4. ! A total of 61 telescope corrections were flagged in sub-array 5. ! A total of 65 telescope corrections were flagged in sub-array 6. ! A total of 29 telescope corrections were flagged in sub-array 7. ! A total of 84 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 7. ! A total of 67 telescope corrections were flagged in sub-array 1. ! A total of 32 telescope corrections were flagged in sub-array 2. ! A total of 34 telescope corrections were flagged in sub-array 3. ! A total of 32 telescope corrections were flagged in sub-array 5. ! A total of 36 telescope corrections were flagged in sub-array 6. ! A total of 84 telescope corrections were flagged in sub-array 8. ! ! Correcting IF 8. ! A total of 67 telescope corrections were flagged in sub-array 1. ! A total of 32 telescope corrections were flagged in sub-array 2. ! A total of 34 telescope corrections were flagged in sub-array 3. ! A total of 32 telescope corrections were flagged in sub-array 5. ! A total of 36 telescope corrections were flagged in sub-array 6. ! A total of 84 telescope corrections were flagged in sub-array 8. ! ! Fit before self-cal, rms=1.007503Jy sigma=9.261737 ! Fit after self-cal, rms=0.921509Jy sigma=8.458397 ! 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 6.73% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.4653 mas, bmaj=0.6787 mas, bpa=0.8255 degrees ! Estimated noise=0.745208 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 = 0.057077 Jy ! Component: 100 - total flux cleaned = 0.0714801 Jy ! Total flux subtracted in 100 components = 0.0714801 Jy ! Clean residual min=-0.003169 max=0.007211 Jy/beam ! Clean residual mean=-0.000002 rms=0.000678 Jy/beam ! Combined flux in latest and established models = 0.0714801 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 0.0714801 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=0.088116Jy sigma=0.710428 ! Fit after self-cal, rms=0.087566Jy sigma=0.706357 ! Inverting map ! Your choice of large map pixels excluded 6.73% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Added new window around map position (0, 1). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00903653 Jy ! Component: 100 - total flux cleaned = 0.0146011 Jy ! Total flux subtracted in 100 components = 0.0146011 Jy ! Clean residual min=-0.002920 max=0.004381 Jy/beam ! Clean residual mean=-0.000001 rms=0.000611 Jy/beam ! Combined flux in latest and established models = 0.0860812 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 11 components and 0.0860812 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=0.085760Jy sigma=0.684232 ! Fit after self-cal, rms=0.085675Jy sigma=0.683570 ! Inverting map ! Your choice of large map pixels excluded 6.73% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00485876 Jy ! Component: 100 - total flux cleaned = 0.00817505 Jy ! Total flux subtracted in 100 components = 0.00817505 Jy ! Clean residual min=-0.002749 max=0.004066 Jy/beam ! Clean residual mean=-0.000001 rms=0.000590 Jy/beam ! Combined flux in latest and established models = 0.0942562 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 16 components and 0.0942562 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=0.085091Jy sigma=0.676172 ! Fit after self-cal, rms=0.085061Jy sigma=0.675912 ! Inverting map ! Your choice of large map pixels excluded 6.73% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Added new window around map position (0.2, 2.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00424378 Jy ! Component: 100 - total flux cleaned = 0.00715824 Jy ! Total flux subtracted in 100 components = 0.00715824 Jy ! Clean residual min=-0.002693 max=0.002925 Jy/beam ! Clean residual mean=-0.000001 rms=0.000572 Jy/beam ! Combined flux in latest and established models = 0.101414 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 24 components and 0.101414 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=0.084686Jy sigma=0.670787 ! Fit after self-cal, rms=0.084657Jy sigma=0.670498 ! Inverting map ! Your choice of large map pixels excluded 6.73% of the data. ! The x-axis pixel size should ideally be below 0.1643 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 6.73% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.6288 mas, bmaj=0.8873 mas, bpa=5.408 degrees ! Estimated noise=0.337586 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 = 0.00535899 Jy ! Component: 100 - total flux cleaned = 0.00854299 Jy ! Component: 150 - total flux cleaned = 0.010647 Jy ! Component: 200 - total flux cleaned = 0.0120493 Jy ! Total flux subtracted in 200 components = 0.0120493 Jy ! Clean residual min=-0.001754 max=0.002245 Jy/beam ! Clean residual mean=-0.000002 rms=0.000346 Jy/beam ! Combined flux in latest and established models = 0.113464 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 37 components and 0.113464 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=0.084326Jy sigma=0.666250 ! Fit after self-cal, rms=0.084297Jy sigma=0.665838 ! Inverting map ! Your choice of large map pixels excluded 6.73% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Added new window around map position (-0.6, 3.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00271349 Jy ! Component: 100 - total flux cleaned = 0.00417893 Jy ! Component: 150 - total flux cleaned = 0.00514314 Jy ! Component: 200 - total flux cleaned = 0.00578738 Jy ! Total flux subtracted in 200 components = 0.00578738 Jy ! Clean residual min=-0.001732 max=0.001615 Jy/beam ! Clean residual mean=0.000001 rms=0.000302 Jy/beam ! Combined flux in latest and established models = 0.119251 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 55 components and 0.119251 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=0.084233Jy sigma=0.665018 ! Fit after self-cal, rms=0.084217Jy sigma=0.664813 ! Inverting map ! Your choice of large map pixels excluded 6.73% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6288 x 0.8873 at 5.408 degrees (North through East) ! Clean map min=-0.0012718 max=0.07834 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 1.02 EF 1.00* FD 1.00 KP 1.01 ! LA 1.05 MC 0.93 NL 0.94 OV 1.05 ! PT 0.92 SC 0.92 ZC 0.80 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.96 EF 1.00* KP 1.02 LA 1.13 ! MC 0.95 MK 1.00 NL 1.10 OV 0.95 ! PT 0.97 ZC 0.84 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 EF 1.00* FD 0.99 KP 0.97 ! LA 1.08 MC 1.21 MK 0.93 NL 0.96 ! ON 0.98 OV 1.01 PT 0.96 SC 1.07 ! ZC 0.93 ! ! A total of 87 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.95 EF 1.00* LA 1.14 MC 1.05 ! NL 0.93 ON 0.98 PT 0.95 SC 0.99 ! ZC 0.81 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.94 EF 1.00* FD 0.99 KP 0.97 ! LA 1.05 MC 0.94 NL 0.94 ON 0.88 ! PT 0.94 SC 1.03 ZC 0.74 ! ! Telescope amplitude corrections in sub-array 7: ! BR 0.93 KP 0.91 MK 0.89 OV 0.98 ! ! Telescope amplitude corrections in sub-array 8: ! EF 0.00* MC 0.00* ZC 0.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.05 EF 1.00* FD 1.01 KP 1.03 ! LA 1.06 MC 1.00 NL 1.01 OV 1.06 ! PT 0.97 SC 0.96 ZC 0.82 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 EF 1.00* KP 1.01 LA 0.99 ! MC 0.99 MK 1.06 NL 1.13 OV 1.07 ! PT 1.10 ZC 0.87 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 EF 1.00* FD 1.12 KP 1.01 ! LA 1.01 MC 1.08 MK 1.04 NL 0.97 ! ON 0.89 OV 1.06 PT 1.03 SC 0.95 ! ZC 1.00 ! ! A total of 87 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.06 EF 1.00* LA 1.15 MC 0.97 ! NL 1.05 ON 0.93 PT 1.08 SC 1.06 ! ZC 0.94 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.98 EF 1.00* FD 0.98 KP 1.02 ! LA 1.02 MC 1.02 NL 0.92 ON 0.95 ! PT 1.00 SC 1.00 ZC 0.87 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00 KP 0.98 MK 0.97 OV 1.13 ! ! Telescope amplitude corrections in sub-array 8: ! EF 0.00* MC 0.00* ZC 0.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 EF 1.00* FD 1.08 KP 0.94 ! LA 1.01 MC 0.93 NL 0.95 OV 1.04 ! PT 0.99 SC 0.97 ZC 0.79 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 EF 1.00* KP 0.94 LA 0.96 ! MC 0.85 MK 0.94 NL 0.99 OV 1.05 ! PT 1.05 ZC 0.82 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.96 EF 1.00* FD 1.03 KP 0.97 ! LA 0.94 MC 1.11 MK 1.01 NL 1.02 ! ON 0.99 OV 1.02 PT 1.01 SC 1.01 ! ZC 0.87 ! ! A total of 87 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.04 EF 1.00* LA 1.00 MC 1.02 ! NL 1.04 ON 0.90 PT 0.94 SC 1.09 ! ZC 0.75 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.01 EF 1.00* FD 0.96 KP 0.93 ! LA 0.98 MC 0.99 NL 0.95 ON 0.93 ! PT 1.03 SC 1.11 ZC 0.83 ! ! Telescope amplitude corrections in sub-array 7: ! BR 0.97 KP 0.95 MK 0.95 OV 0.97 ! ! Telescope amplitude corrections in sub-array 8: ! EF 0.00* MC 0.00* ZC 0.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 EF 1.00* FD 1.02 KP 0.97 ! LA 1.05 MC 1.02 NL 1.06 OV 1.08 ! PT 1.01 SC 0.92 ZC 0.81 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.99 EF 1.00* KP 0.93 LA 1.08 ! MC 0.93 MK 1.01 NL 1.10 OV 0.99 ! PT 1.04 ZC 0.80 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.01 EF 1.00* FD 1.04 KP 0.99 ! LA 0.97 MC 1.03 MK 1.03 NL 1.00 ! ON 1.00 OV 1.07 PT 1.00 SC 1.07 ! ZC 0.92 ! ! A total of 87 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.97 EF 1.00* LA 1.00 MC 1.03 ! NL 1.04 ON 0.90 PT 1.00 SC 1.03 ! ZC 0.81 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.95 EF 1.00* FD 1.06 KP 0.96 ! LA 0.95 MC 1.08 NL 0.95 ON 0.95 ! PT 0.99 SC 1.03 ZC 0.90 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00 KP 0.98 MK 0.94 OV 1.03 ! ! Telescope amplitude corrections in sub-array 8: ! EF 0.00* MC 0.00* ZC 0.00* ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.08 KP 0.87 ! LA 1.02 MC 1.29 NL 0.97 OV 1.09 ! PT 0.97 SC 1.00 ZC 0.85 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* KP 0.88 LA 0.96 ! MC 1.23 MK 1.02 NL 1.12 OV 1.09 ! PT 0.92 ZC 0.86 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.05 KP 0.88 ! LA 1.02 MC 1.32 MK 1.05 NL 1.00 ! ON 1.28 OV 1.05 PT 1.03 SC 1.09 ! ZC 0.97 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* LA 1.02 MC 1.09 ! NL 1.12 ON 1.06 PT 0.98 SC 1.12 ! ZC 0.96 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.07 KP 0.92 ! LA 0.96 MC 1.32 NL 1.01 ON 1.22 ! PT 0.94 SC 1.02 ZC 0.87 ! ! A total of 87 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 0.00* KP 0.00* MK 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! EF 0.00* MC 0.00* ZC 0.00* ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.05 KP 0.87 ! LA 1.01 MC 1.28 NL 1.04 OV 1.09 ! PT 0.91 SC 0.99 ZC 0.84 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* KP 0.84 LA 1.06 ! MC 1.18 MK 1.03 NL 1.07 OV 1.04 ! PT 1.00 ZC 0.76 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 0.99 KP 0.86 ! LA 0.97 MC 1.34 MK 1.05 NL 1.05 ! ON 1.25 OV 1.07 PT 0.96 SC 1.06 ! ZC 0.98 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* LA 1.16 MC 1.22 ! NL 0.98 ON 1.06 PT 0.81 SC 0.98 ! ZC 0.86 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 0.99 KP 0.83 ! LA 0.99 MC 1.21 NL 0.94 ON 1.22 ! PT 0.96 SC 1.09 ZC 0.80 ! ! A total of 87 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 0.00* KP 0.00* MK 0.00* OV 0.00* ! ! Telescope amplitude corrections in sub-array 8: ! EF 0.00* MC 0.00* ZC 0.00* ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 EF 1.00* FD 1.07 KP 0.94 ! LA 1.06 MC 1.37 NL 1.03 OV 1.00 ! PT 1.01 SC 0.89 ZC 0.68 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 EF 1.00* KP 0.95 LA 1.03 ! MC 1.37 MK 0.94 NL 1.13 OV 1.03 ! PT 0.96 ZC 0.67 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.14 EF 1.00* FD 1.00 KP 0.94 ! LA 1.03 MC 1.38 MK 1.03 NL 1.08 ! ON 1.36 OV 0.98 PT 1.00 SC 1.05 ! ZC 0.83 ! ! A total of 87 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.88 EF 1.00* LA 1.22 MC 1.30 ! NL 1.04 ON 1.21 PT 0.96 SC 0.98 ! ZC 0.74 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.95 EF 1.00* FD 1.05 KP 0.98 ! LA 0.98 MC 1.26 NL 1.04 ON 1.22 ! PT 0.97 SC 0.98 ZC 0.67 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.03 KP 1.00 MK 0.90 OV 0.85 ! ! Telescope amplitude corrections in sub-array 8: ! EF 0.00* MC 0.00* ZC 0.00* ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 0.94 EF 1.00* FD 1.06 KP 0.89 ! LA 1.04 MC 1.50 NL 1.03 OV 1.04 ! PT 0.93 SC 0.94 ZC 0.64 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 EF 1.00* KP 0.90 LA 1.06 ! MC 1.22 MK 0.94 NL 1.10 OV 0.97 ! PT 1.02 ZC 0.58 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 EF 1.00* FD 1.01 KP 0.91 ! LA 0.97 MC 1.32 MK 1.09 NL 1.03 ! ON 1.39 OV 1.03 PT 1.02 SC 1.08 ! ZC 0.75 ! ! A total of 87 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.90 EF 1.00* LA 1.00 MC 1.28 ! NL 1.00 ON 1.16 PT 1.00 SC 0.93 ! ZC 0.73 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.03 EF 1.00* FD 0.99 KP 0.98 ! LA 1.07 MC 1.30 NL 1.04 ON 1.23 ! PT 0.96 SC 1.11 ZC 0.62 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.06 KP 0.89 MK 1.01 OV 0.99 ! ! Telescope amplitude corrections in sub-array 8: ! EF 0.00* MC 0.00* ZC 0.00* ! ! ! Fit before self-cal, rms=0.084217Jy sigma=0.664813 ! Fit after self-cal, rms=0.084443Jy sigma=0.658409 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 6.82% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.6268 mas, bmaj=0.8907 mas, bpa=7.725 degrees ! Estimated noise=0.340372 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 = 0.000561471 Jy ! Component: 100 - total flux cleaned = 0.000658179 Jy ! Component: 150 - total flux cleaned = 0.000712873 Jy ! Component: 200 - total flux cleaned = 0.000735452 Jy ! Total flux subtracted in 200 components = 0.000735452 Jy ! Clean residual min=-0.001065 max=0.001071 Jy/beam ! Clean residual mean=-0.000004 rms=0.000228 Jy/beam ! Combined flux in latest and established models = 0.119987 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 65 components and 0.119987 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=0.084417Jy sigma=0.658172 ! Fit after self-cal, rms=0.084558Jy sigma=0.657739 ! Inverting map ! Your choice of large map pixels excluded 6.82% of the data. ! The x-axis pixel size should ideally be below 0.1643 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=0.084558Jy sigma=0.657739 ! Fit after self-cal, rms=0.085059Jy sigma=0.657248 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.82% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.6274 mas, bmaj=0.8888 mas, bpa=7.335 degrees ! Estimated noise=0.341581 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000714099 Jy ! Component: 100 - total flux cleaned = 0.000759842 Jy ! Component: 150 - total flux cleaned = 0.000760055 Jy ! Component: 200 - total flux cleaned = 0.00079731 Jy ! Total flux subtracted in 200 components = 0.00079731 Jy ! Clean residual min=-0.001048 max=0.001012 Jy/beam ! Clean residual mean=-0.000007 rms=0.000222 Jy/beam ! Combined flux in latest and established models = 0.120784 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 73 components and 0.120784 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=0.085047Jy sigma=0.657149 ! Fit after self-cal, rms=0.085066Jy sigma=0.657113 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.82% of the data. ! The x-axis pixel size should ideally be below 0.1643 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 = 0.000105716 Jy ! Component: 100 - total flux cleaned = 0.000123846 Jy ! Component: 150 - total flux cleaned = 0.000140939 Jy ! Component: 200 - total flux cleaned = 0.000155715 Jy ! Total flux subtracted in 200 components = 0.000155715 Jy ! Clean residual min=-0.001047 max=0.000999 Jy/beam ! Clean residual mean=-0.000007 rms=0.000221 Jy/beam ! Combined flux in latest and established models = 0.12094 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 75 components and 0.12094 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=0.085060Jy sigma=0.657056 ! Fit after self-cal, rms=0.085060Jy sigma=0.657052 ! Inverting map ! Your choice of large map pixels excluded 6.82% of the data. ! The x-axis pixel size should ideally be below 0.1643 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=0.085060Jy sigma=0.657052 ! Fit after self-cal, rms=0.085446Jy sigma=0.657023 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.82% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.6272 mas, bmaj=0.8863 mas, bpa=7.204 degrees ! Estimated noise=0.342505 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000564635 Jy ! Component: 100 - total flux cleaned = 0.000633385 Jy ! Component: 150 - total flux cleaned = 0.000648535 Jy ! Component: 200 - total flux cleaned = 0.00064841 Jy ! Total flux subtracted in 200 components = 0.00064841 Jy ! Clean residual min=-0.001045 max=0.000991 Jy/beam ! Clean residual mean=-0.000007 rms=0.000220 Jy/beam ! Combined flux in latest and established models = 0.121588 Jy selfcal ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 78 components and 0.121588 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=0.085439Jy sigma=0.656964 ! Fit after self-cal, rms=0.085435Jy sigma=0.656918 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.82% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 8.56954e-05 Jy ! Component: 100 - total flux cleaned = 0.000113787 Jy ! Component: 150 - total flux cleaned = 0.000113966 Jy ! Component: 200 - total flux cleaned = 0.00012661 Jy ! Total flux subtracted in 200 components = 0.00012661 Jy ! Clean residual min=-0.001045 max=0.000986 Jy/beam ! Clean residual mean=-0.000007 rms=0.000220 Jy/beam ! Combined flux in latest and established models = 0.121715 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 80 components and 0.121715 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=0.085431Jy sigma=0.656883 ! Fit after self-cal, rms=0.085431Jy sigma=0.656879 ! Inverting map ! Your choice of large map pixels excluded 6.82% of the data. ! The x-axis pixel size should ideally be below 0.1643 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=0.085431Jy sigma=0.656879 ! Fit after self-cal, rms=0.085679Jy sigma=0.656857 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.82% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=2.724 mas, bmaj=3.139 mas, bpa=85 degrees ! Estimated noise=0.466378 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00069334 Jy ! Component: 100 - total flux cleaned = 0.000980089 Jy ! Component: 150 - total flux cleaned = 0.00102503 Jy ! Component: 200 - total flux cleaned = 0.00103963 Jy ! Total flux subtracted in 200 components = 0.00103963 Jy ! Clean residual min=-0.000990 max=0.001107 Jy/beam ! Clean residual mean=-0.000017 rms=0.000286 Jy/beam ! Combined flux in latest and established models = 0.122754 Jy selfcal ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 84 components and 0.122754 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=0.085678Jy sigma=0.656858 ! Fit after self-cal, rms=0.085680Jy sigma=0.656843 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.82% of the data. ! The x-axis pixel size should ideally be below 0.1643 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 = 7.08027e-05 Jy ! Component: 100 - total flux cleaned = 0.000131446 Jy ! Component: 150 - total flux cleaned = 0.000162329 Jy ! Component: 200 - total flux cleaned = 0.000174875 Jy ! Total flux subtracted in 200 components = 0.000174875 Jy ! Clean residual min=-0.000996 max=0.001114 Jy/beam ! Clean residual mean=-0.000017 rms=0.000286 Jy/beam ! Combined flux in latest and established models = 0.122929 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 88 components and 0.122929 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=0.085680Jy sigma=0.656858 ! Fit after self-cal, rms=0.085680Jy sigma=0.656851 ! Inverting map ! Your choice of large map pixels excluded 6.82% of the data. ! The x-axis pixel size should ideally be below 0.1643 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 6.82% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.6272 mas, bmaj=0.8842 mas, bpa=7.093 degrees ! Estimated noise=0.343274 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6272 x 0.8842 at 7.093 degrees (North through East) ! Clean map min=-0.00086198 max=0.078465 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 6.82% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.4639 mas, bmaj=0.6723 mas, bpa=2.273 degrees ! Estimated noise=0.754944 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0574054 Jy ! Component: 100 - total flux cleaned = 0.0745648 Jy ! Component: 150 - total flux cleaned = 0.083967 Jy ! Component: 200 - total flux cleaned = 0.0902757 Jy ! Total flux subtracted in 200 components = 0.0902757 Jy ! Clean residual min=-0.002465 max=0.003820 Jy/beam ! Clean residual mean=-0.000003 rms=0.000569 Jy/beam ! Combined flux in latest and established models = 0.0902758 Jy uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Adding 12 model components to the UV plane model. ! The established model now contains 12 components and 0.0902758 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 6.82% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.6272 mas, bmaj=0.8842 mas, bpa=7.093 degrees ! Estimated noise=0.343274 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 = 0.0110844 Jy ! Component: 100 - total flux cleaned = 0.0175318 Jy ! Component: 150 - total flux cleaned = 0.021785 Jy ! Component: 200 - total flux cleaned = 0.0247163 Jy ! Total flux subtracted in 200 components = 0.0247163 Jy ! Clean residual min=-0.001181 max=0.001761 Jy/beam ! Clean residual mean=-0.000012 rms=0.000271 Jy/beam ! Combined flux in latest and established models = 0.114992 Jy ! Adding 52 model components to the UV plane model. ! The established model now contains 55 components and 0.114992 Jy ! Inverting map ! Your choice of large map pixels excluded 6.82% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Added new window around map position (0.6, 1.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00208633 Jy ! Component: 100 - total flux cleaned = 0.00359214 Jy ! Component: 150 - total flux cleaned = 0.00470276 Jy ! Component: 200 - total flux cleaned = 0.00553059 Jy ! Total flux subtracted in 200 components = 0.00553059 Jy ! Clean residual min=-0.001064 max=0.000922 Jy/beam ! Clean residual mean=-0.000008 rms=0.000224 Jy/beam ! Combined flux in latest and established models = 0.120523 Jy ! Adding 32 model components to the UV plane model. ! The established model now contains 67 components and 0.120523 Jy ! Inverting map ! Your choice of large map pixels excluded 6.82% of the data. ! The x-axis pixel size should ideally be below 0.1643 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 6.82% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=2.724 mas, bmaj=3.139 mas, bpa=85 degrees ! Estimated noise=0.466378 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00115415 Jy ! Component: 100 - total flux cleaned = 0.00173538 Jy ! Component: 150 - total flux cleaned = 0.0020612 Jy ! Component: 200 - total flux cleaned = 0.00224899 Jy ! Total flux subtracted in 200 components = 0.00224899 Jy ! Clean residual min=-0.000985 max=0.001092 Jy/beam ! Clean residual mean=-0.000018 rms=0.000286 Jy/beam ! Combined flux in latest and established models = 0.122772 Jy flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 6.04378e-05 Jy ! Component: 100 - total flux cleaned = 8.25883e-05 Jy ! Component: 150 - total flux cleaned = 9.53514e-05 Jy ! Component: 200 - total flux cleaned = 0.000107408 Jy ! Total flux subtracted in 200 components = 0.000107408 Jy ! Clean residual min=-0.000982 max=0.001096 Jy/beam ! Clean residual mean=-0.000017 rms=0.000286 Jy/beam ! Combined flux in latest and established models = 0.122879 Jy ! Adding 33 model components to the UV plane model. ! The established model now contains 92 components and 0.122879 Jy ! Inverting map ! Your choice of large map pixels excluded 6.82% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 6.82% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! Estimated beam: bmin=0.6272 mas, bmaj=0.8842 mas, bpa=7.093 degrees ! Estimated noise=0.343274 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00016946 Jy ! Component: 100 - total flux cleaned = -0.000209309 Jy ! Component: 150 - total flux cleaned = -0.000220534 Jy ! Component: 200 - total flux cleaned = -0.000219932 Jy ! Total flux subtracted in 200 components = -0.000219932 Jy ! Clean residual min=-0.001053 max=0.000962 Jy/beam ! Clean residual mean=-0.000007 rms=0.000218 Jy/beam ! Combined flux in latest and established models = 0.122659 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 103 components and 0.122659 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=0.085669Jy sigma=0.656785 ! Fit after self-cal, rms=0.085664Jy sigma=0.656743 wmodel /scr/pima/gb073_uvs/J1245+5709_X_map.mod ! Writing 103 model components to file: /scr/pima/gb073_uvs/J1245+5709_X_map.mod wobs /scr/pima/gb073_uvs/J1245+5709_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1245+5709_X_uvs.fits wwins /scr/pima/gb073_uvs/J1245+5709_X_map.win ! wwins: Wrote 5 windows to /scr/pima/gb073_uvs/J1245+5709_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 6.82% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000154287 Jy ! Component: 100 - total flux cleaned = -0.000239423 Jy ! Component: 150 - total flux cleaned = -0.00032154 Jy ! Component: 200 - total flux cleaned = -0.000402354 Jy ! Component: 250 - total flux cleaned = -0.000513031 Jy ! Component: 300 - total flux cleaned = -0.000575226 Jy ! Component: 350 - total flux cleaned = -0.000652172 Jy ! Component: 400 - total flux cleaned = -0.000682613 Jy ! Component: 450 - total flux cleaned = -0.000712902 Jy ! Component: 500 - total flux cleaned = -0.000786905 Jy ! Component: 550 - total flux cleaned = -0.0007722 Jy ! Component: 600 - total flux cleaned = -0.000801401 Jy ! Component: 650 - total flux cleaned = -0.00080136 Jy ! Component: 700 - total flux cleaned = -0.000801514 Jy ! Component: 750 - total flux cleaned = -0.000844097 Jy ! Component: 800 - total flux cleaned = -0.000886099 Jy ! Component: 850 - total flux cleaned = -0.000886253 Jy ! Component: 900 - total flux cleaned = -0.000982913 Jy ! Component: 950 - total flux cleaned = -0.000983016 Jy ! Component: 1000 - total flux cleaned = -0.000955613 Jy ! Component: 1050 - total flux cleaned = -0.000982882 Jy ! Component: 1100 - total flux cleaned = -0.00103678 Jy ! Component: 1150 - total flux cleaned = -0.00106346 Jy ! Component: 1200 - total flux cleaned = -0.00110328 Jy ! Component: 1250 - total flux cleaned = -0.00111651 Jy ! Component: 1300 - total flux cleaned = -0.00111641 Jy ! Component: 1350 - total flux cleaned = -0.00118163 Jy ! Component: 1400 - total flux cleaned = -0.00116868 Jy ! Component: 1450 - total flux cleaned = -0.0012075 Jy ! Component: 1500 - total flux cleaned = -0.00119476 Jy ! Component: 1550 - total flux cleaned = -0.0012459 Jy ! Component: 1600 - total flux cleaned = -0.00122056 Jy ! Component: 1650 - total flux cleaned = -0.00125849 Jy ! Component: 1700 - total flux cleaned = -0.00129628 Jy ! Component: 1750 - total flux cleaned = -0.00130879 Jy ! Component: 1800 - total flux cleaned = -0.00132122 Jy ! Component: 1850 - total flux cleaned = -0.00132123 Jy ! Component: 1900 - total flux cleaned = -0.00137073 Jy ! Component: 1950 - total flux cleaned = -0.00128434 Jy ! Component: 2000 - total flux cleaned = -0.00135803 Jy ! Component: 2050 - total flux cleaned = -0.00139481 Jy ! Component: 2100 - total flux cleaned = -0.00138257 Jy ! Component: 2150 - total flux cleaned = -0.00138263 Jy ! Component: 2200 - total flux cleaned = -0.00141887 Jy ! Component: 2250 - total flux cleaned = -0.00140673 Jy ! Component: 2300 - total flux cleaned = -0.00143078 Jy ! Component: 2350 - total flux cleaned = -0.00147869 Jy ! Component: 2400 - total flux cleaned = -0.0015264 Jy ! Component: 2450 - total flux cleaned = -0.00157394 Jy ! Component: 2500 - total flux cleaned = -0.00155017 Jy ! Component: 2550 - total flux cleaned = -0.00158559 Jy ! Component: 2600 - total flux cleaned = -0.00165624 Jy ! Component: 2650 - total flux cleaned = -0.00166802 Jy ! Component: 2700 - total flux cleaned = -0.00173827 Jy ! Component: 2750 - total flux cleaned = -0.00184316 Jy ! Component: 2800 - total flux cleaned = -0.00184323 Jy ! Component: 2850 - total flux cleaned = -0.00183164 Jy ! Component: 2900 - total flux cleaned = -0.00186624 Jy ! Component: 2950 - total flux cleaned = -0.00194683 Jy ! Component: 3000 - total flux cleaned = -0.00201573 Jy ! Component: 3050 - total flux cleaned = -0.00201581 Jy ! Component: 3100 - total flux cleaned = -0.00202718 Jy ! Component: 3150 - total flux cleaned = -0.00203855 Jy ! Component: 3200 - total flux cleaned = -0.00208388 Jy ! Component: 3250 - total flux cleaned = -0.00212912 Jy ! Component: 3300 - total flux cleaned = -0.00219679 Jy ! Component: 3350 - total flux cleaned = -0.00223048 Jy ! Component: 3400 - total flux cleaned = -0.00225294 Jy ! Component: 3450 - total flux cleaned = -0.00227526 Jy ! Component: 3500 - total flux cleaned = -0.00235321 Jy ! Component: 3550 - total flux cleaned = -0.00235322 Jy ! Component: 3600 - total flux cleaned = -0.00239749 Jy ! Component: 3650 - total flux cleaned = -0.00247477 Jy ! Component: 3700 - total flux cleaned = -0.0024858 Jy ! Component: 3750 - total flux cleaned = -0.00251879 Jy ! Component: 3800 - total flux cleaned = -0.00257352 Jy ! Component: 3850 - total flux cleaned = -0.00264999 Jy ! Component: 3900 - total flux cleaned = -0.00263914 Jy ! Component: 3950 - total flux cleaned = -0.00265003 Jy ! Component: 4000 - total flux cleaned = -0.00267161 Jy ! Component: 4050 - total flux cleaned = -0.00273644 Jy ! Total flux subtracted in 4096 components = -0.00279031 Jy ! Clean residual min=-0.000634 max=0.000603 Jy/beam ! Clean residual mean=-0.000003 rms=0.000177 Jy/beam ! Combined flux in latest and established models = 0.119869 Jy keep ! Adding 342 model components to the UV plane model. ! The established model now contains 445 components and 0.119869 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1245+5709_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 6.82% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6272 x 0.8842 at 7.093 degrees (North through East) ! Clean map min=-0.00082208 max=0.078404 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1245+5709_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.078404 invert ! Inverting map ! Your choice of large map pixels excluded 6.82% of the data. ! The x-axis pixel size should ideally be below 0.1643 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000176327 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.674688 0.674688 1.34938 2.69875 5.3975 10.795 21.59 43.18 86.36 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0005 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.078 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 444.65 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1245+5709_X_uvs.log closed on Sat Dec 26 09:38:58 2015