! Started logfile: /scr/pima/gb073_uvs/J0214+5144_X_uvs.log on Sat Dec 26 09:32:01 2015 obs /scr/pima/gb073_uvs/J0214+5144_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J0214+5144_X_uva.fits ! AN table 1: 29 integrations on 36 of 36 possible baselines. ! AN table 2: 29 integrations on 78 of 78 possible baselines. ! AN table 3: 29 integrations on 55 of 55 possible baselines. ! AN table 4: 29 integrations on 66 of 66 possible baselines. ! Apparent sampling: 0.790169 visibilities/baseline/integration-bin. ! Found source: J0214+5144 ! ! 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 43080 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/J0214+5144_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 40 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 68 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 40 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 68 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 40 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 68 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 40 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 68 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 5. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 69 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 97 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 6. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 69 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 97 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 7. ! A total of 40 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 68 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 8. ! A total of 40 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 68 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=1.006750Jy sigma=9.684432 ! Fit after self-cal, rms=0.929076Jy sigma=8.915664 ! 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 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec ! Estimated beam: bmin=0.5198 mas, bmaj=0.6452 mas, bpa=-13 degrees ! Estimated noise=0.908982 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 = 0.049707 Jy ! Component: 100 - total flux cleaned = 0.0641502 Jy ! Total flux subtracted in 100 components = 0.0641502 Jy ! Clean residual min=-0.003954 max=0.008604 Jy/beam ! Clean residual mean=-0.000004 rms=0.000813 Jy/beam ! Combined flux in latest and established models = 0.0641502 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.0641502 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=0.086798Jy sigma=0.727635 ! Fit after self-cal, rms=0.086017Jy sigma=0.721705 ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec ! Added new window around map position (0.8, 0.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00966008 Jy ! Component: 100 - total flux cleaned = 0.0157031 Jy ! Total flux subtracted in 100 components = 0.0157031 Jy ! Clean residual min=-0.003377 max=0.006020 Jy/beam ! Clean residual mean=-0.000003 rms=0.000714 Jy/beam ! Combined flux in latest and established models = 0.0798533 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 15 components and 0.0798533 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=0.083749Jy sigma=0.690242 ! Fit after self-cal, rms=0.083631Jy sigma=0.689383 ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00532269 Jy ! Component: 100 - total flux cleaned = 0.00892632 Jy ! Total flux subtracted in 100 components = 0.00892632 Jy ! Clean residual min=-0.003023 max=0.003832 Jy/beam ! Clean residual mean=-0.000002 rms=0.000669 Jy/beam ! Combined flux in latest and established models = 0.0887796 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 20 components and 0.0887796 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=0.082848Jy sigma=0.678291 ! Fit after self-cal, rms=0.082785Jy sigma=0.677850 ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 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 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec ! Estimated beam: bmin=0.7396 mas, bmaj=0.8767 mas, bpa=-14.13 degrees ! Estimated noise=0.385208 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 = 0.00762539 Jy ! Component: 100 - total flux cleaned = 0.0115379 Jy ! Component: 150 - total flux cleaned = 0.0136623 Jy ! Component: 200 - total flux cleaned = 0.0148222 Jy ! Total flux subtracted in 200 components = 0.0148222 Jy ! Clean residual min=-0.002102 max=0.004649 Jy/beam ! Clean residual mean=-0.000009 rms=0.000546 Jy/beam ! Combined flux in latest and established models = 0.103602 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 28 components and 0.103602 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=0.082208Jy sigma=0.669826 ! Fit after self-cal, rms=0.082133Jy sigma=0.669253 ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec ! Added new window around map position (2.6, 1.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00488035 Jy ! Component: 100 - total flux cleaned = 0.00751529 Jy ! Component: 150 - total flux cleaned = 0.00911711 Jy ! Component: 200 - total flux cleaned = 0.00994716 Jy ! Total flux subtracted in 200 components = 0.00994716 Jy ! Clean residual min=-0.001818 max=0.002419 Jy/beam ! Clean residual mean=-0.000003 rms=0.000425 Jy/beam ! Combined flux in latest and established models = 0.113549 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 53 components and 0.113549 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=0.081890Jy sigma=0.665818 ! Fit after self-cal, rms=0.081837Jy sigma=0.665164 ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec ! Added new window around map position (4.8, 2.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00258141 Jy ! Component: 100 - total flux cleaned = 0.00415746 Jy ! Component: 150 - total flux cleaned = 0.00517488 Jy ! Component: 200 - total flux cleaned = 0.00553704 Jy ! Total flux subtracted in 200 components = 0.00553704 Jy ! Clean residual min=-0.001799 max=0.001947 Jy/beam ! Clean residual mean=0.000001 rms=0.000371 Jy/beam ! Combined flux in latest and established models = 0.119086 Jy ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 76 components and 0.119086 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=0.081753Jy sigma=0.664113 ! Fit after self-cal, rms=0.081746Jy sigma=0.663955 ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7396 x 0.8767 at -14.13 degrees (North through East) ! Clean map min=-0.0014813 max=0.067552 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 0.97 FD 1.03 KP 1.04 LA 1.04 ! MC 0.86 MK 1.01 NL 1.00 OV 1.00 ! PT 0.95 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* MK 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 EF 1.00* FD 0.98 KP 0.94 ! LA 1.05 MC 1.02 MK 1.03 NL 0.99 ! ON 0.85 PT 1.00 SC 0.97 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.12 EF 1.00* FD 1.14 KP 0.99 ! LA 0.98 MC 0.96 NL 0.94 ON 1.00* ! OV 1.09 PT 0.89 SC 0.92 ZC 0.89 ! ! ! Correcting IF 2. ! 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* OV 1.00* ! PT 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00 EF 1.00* FD 0.99 KP 1.01 ! LA 1.13 MC 0.94 MK 0.93 NL 1.03 ! ON 0.91 OV 1.08 PT 1.00 SC 1.03 ! ZC 0.92 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.94 EF 1.00* FD 1.01 KP 1.02 ! LA 1.09 MC 0.93 MK 0.97 NL 0.90 ! ON 1.08 PT 1.12 SC 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.12 EF 1.00* FD 1.08 KP 1.03 ! LA 1.00 MC 0.95 NL 0.96 ON 1.00* ! OV 1.07 PT 0.98 SC 0.95 ZC 1.02 ! ! ! Correcting IF 3. ! 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* OV 1.00* ! PT 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 EF 1.00* FD 1.02 KP 0.95 ! LA 0.96 MC 0.95 MK 0.99 NL 1.00 ! ON 0.94 OV 1.02 PT 1.00 SC 1.05 ! ZC 0.84 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.08 EF 1.00* FD 1.04 KP 0.91 ! LA 1.01 MC 0.85 MK 1.03 NL 1.00 ! ON 0.93 PT 0.99 SC 1.06 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! ! Correcting IF 4. ! 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* OV 1.00* ! PT 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 EF 1.00* FD 0.97 KP 1.01 ! LA 1.05 MC 0.91 MK 1.02 NL 1.04 ! ON 0.87 OV 0.95 PT 1.00 SC 0.99 ! ZC 0.87 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 EF 1.00* FD 0.98 KP 0.98 ! LA 1.00 MC 0.94 MK 1.02 NL 0.98 ! ON 0.95 PT 1.03 SC 0.94 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.08 EF 1.00* FD 1.12 KP 0.97 ! LA 0.96 MC 1.13 NL 0.92 ON 1.00* ! OV 1.05 PT 0.96 SC 1.06 ZC 0.84 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.03 KP 0.94 LA 0.99 ! MC 1.01 MK 1.04 NL 1.03 OV 1.02 ! PT 1.02 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* MK 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.01 KP 0.93 ! LA 1.06 MC 1.16 MK 0.98 NL 1.00 ! ON 1.12 PT 0.92 SC 0.95 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.01 KP 0.88 LA 1.00 ! MC 0.97 MK 0.99 NL 1.04 OV 1.03 ! PT 0.93 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* MK 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.10 KP 0.85 ! LA 0.98 MC 1.03 MK 1.02 NL 0.93 ! ON 1.16 PT 0.99 SC 0.97 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.17 KP 0.90 ! LA 0.92 MC 1.17 NL 0.98 ON 1.00* ! OV 1.10 PT 1.01 SC 0.93 ZC 0.89 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 1.03 KP 0.97 LA 1.10 ! MC 0.96 MK 1.10 NL 1.04 OV 0.96 ! PT 0.98 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* MK 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* MK 1.00* NL 1.00* ! ON 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 1.06 FD 1.03 KP 0.95 LA 1.05 ! MC 1.00 MK 1.10 NL 1.06 OV 1.01 ! PT 0.93 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* MK 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* MK 1.00* NL 1.00* ! ON 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! ! Fit before self-cal, rms=0.081746Jy sigma=0.663955 ! Fit after self-cal, rms=0.080961Jy sigma=0.662116 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec ! Estimated beam: bmin=0.7333 mas, bmaj=0.874 mas, bpa=-14.73 degrees ! Estimated noise=0.384076 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 = 0.000653974 Jy ! Component: 100 - total flux cleaned = 0.000891272 Jy ! Component: 150 - total flux cleaned = 0.000997789 Jy ! Component: 200 - total flux cleaned = 0.0010908 Jy ! Total flux subtracted in 200 components = 0.0010908 Jy ! Clean residual min=-0.001396 max=0.001538 Jy/beam ! Clean residual mean=0.000001 rms=0.000322 Jy/beam ! Combined flux in latest and established models = 0.120177 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 85 components and 0.120177 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=0.080949Jy sigma=0.661986 ! Fit after self-cal, rms=0.080963Jy sigma=0.661887 ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 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=0.080963Jy sigma=0.661887 ! Fit after self-cal, rms=0.080888Jy sigma=0.661876 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec ! Estimated beam: bmin=0.7334 mas, bmaj=0.8739 mas, bpa=-14.77 degrees ! Estimated noise=0.383616 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000224211 Jy ! Component: 100 - total flux cleaned = 0.000344858 Jy ! Component: 150 - total flux cleaned = 0.000416167 Jy ! Component: 200 - total flux cleaned = 0.000481618 Jy ! Total flux subtracted in 200 components = 0.000481618 Jy ! Clean residual min=-0.001375 max=0.001531 Jy/beam ! Clean residual mean=0.000001 rms=0.000320 Jy/beam ! Combined flux in latest and established models = 0.120659 Jy selfcal ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 89 components and 0.120659 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=0.080881Jy sigma=0.661810 ! Fit after self-cal, rms=0.080881Jy sigma=0.661798 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 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 (18.2, 8.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00141157 Jy ! Component: 100 - total flux cleaned = 0.0019635 Jy ! Component: 150 - total flux cleaned = 0.00212552 Jy ! Component: 200 - total flux cleaned = 0.0022145 Jy ! Total flux subtracted in 200 components = 0.0022145 Jy ! Clean residual min=-0.001322 max=0.001565 Jy/beam ! Clean residual mean=0.000001 rms=0.000307 Jy/beam ! Combined flux in latest and established models = 0.122873 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 103 components and 0.122873 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=0.080855Jy sigma=0.661530 ! Fit after self-cal, rms=0.080843Jy sigma=0.661492 ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec ! Added new window around map position (10.4, 5.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00162833 Jy ! Component: 100 - total flux cleaned = 0.00257059 Jy ! Component: 150 - total flux cleaned = 0.0032226 Jy ! Component: 200 - total flux cleaned = 0.00357479 Jy ! Total flux subtracted in 200 components = 0.00357479 Jy ! Clean residual min=-0.001202 max=0.001400 Jy/beam ! Clean residual mean=0.000001 rms=0.000284 Jy/beam ! Combined flux in latest and established models = 0.126448 Jy ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 115 components and 0.126448 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=0.080811Jy sigma=0.661084 ! Fit after self-cal, rms=0.080806Jy sigma=0.661042 ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec ! Added new window around map position (-5.8, -18.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00129343 Jy ! Component: 100 - total flux cleaned = 0.00203364 Jy ! Component: 150 - total flux cleaned = 0.00260942 Jy ! Component: 200 - total flux cleaned = 0.00289086 Jy ! Total flux subtracted in 200 components = 0.00289086 Jy ! Clean residual min=-0.001127 max=0.001166 Jy/beam ! Clean residual mean=0.000001 rms=0.000271 Jy/beam ! Combined flux in latest and established models = 0.129339 Jy ! Performing phase self-cal ! Adding 30 model components to the UV plane model. ! The established model now contains 131 components and 0.129339 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=0.080782Jy sigma=0.660790 ! Fit after self-cal, rms=0.080777Jy sigma=0.660766 ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec ! Added new window around map position (-50, 32.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00104598 Jy ! Component: 100 - total flux cleaned = 0.00149835 Jy ! Component: 150 - total flux cleaned = 0.00171391 Jy ! Component: 200 - total flux cleaned = 0.00182475 Jy ! Total flux subtracted in 200 components = 0.00182475 Jy ! Clean residual min=-0.001102 max=0.001137 Jy/beam ! Clean residual mean=0.000001 rms=0.000264 Jy/beam ! Combined flux in latest and established models = 0.131163 Jy ! Performing phase self-cal ! Adding 37 model components to the UV plane model. ! The established model now contains 144 components and 0.131163 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=0.080759Jy sigma=0.660607 ! Fit after self-cal, rms=0.080755Jy sigma=0.660595 ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 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=0.080755Jy sigma=0.660595 ! Fit after self-cal, rms=0.080611Jy sigma=0.660500 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec ! Estimated beam: bmin=0.7345 mas, bmaj=0.8737 mas, bpa=-14.85 degrees ! Estimated noise=0.383205 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000551941 Jy ! Component: 100 - total flux cleaned = 0.000948558 Jy ! Component: 150 - total flux cleaned = 0.00119225 Jy ! Component: 200 - total flux cleaned = 0.0012982 Jy ! Total flux subtracted in 200 components = 0.0012982 Jy ! Clean residual min=-0.001078 max=0.001145 Jy/beam ! Clean residual mean=0.000001 rms=0.000262 Jy/beam ! Combined flux in latest and established models = 0.132462 Jy selfcal ! Performing phase self-cal ! Adding 42 model components to the UV plane model. ! The established model now contains 150 components and 0.132462 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=0.080602Jy sigma=0.660413 ! Fit after self-cal, rms=0.080600Jy sigma=0.660407 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 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 (33.4, -46.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00100185 Jy ! Component: 100 - total flux cleaned = 0.0014695 Jy ! Component: 150 - total flux cleaned = 0.00183609 Jy ! Component: 200 - total flux cleaned = 0.00210542 Jy ! Total flux subtracted in 200 components = 0.00210542 Jy ! Clean residual min=-0.001032 max=0.001099 Jy/beam ! Clean residual mean=0.000000 rms=0.000257 Jy/beam ! Combined flux in latest and established models = 0.134567 Jy ! Performing phase self-cal ! Adding 49 model components to the UV plane model. ! The established model now contains 161 components and 0.134567 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=0.080584Jy sigma=0.660260 ! Fit after self-cal, rms=0.080583Jy sigma=0.660245 ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 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=0.080583Jy sigma=0.660245 ! Fit after self-cal, rms=0.080561Jy sigma=0.660233 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec ! Estimated beam: bmin=2.711 mas, bmaj=2.979 mas, bpa=-68.99 degrees ! Estimated noise=0.499947 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000823457 Jy ! Component: 100 - total flux cleaned = 0.00135877 Jy ! Component: 150 - total flux cleaned = 0.00170004 Jy ! Component: 200 - total flux cleaned = 0.00199728 Jy ! Total flux subtracted in 200 components = 0.00199728 Jy ! Clean residual min=-0.001198 max=0.001270 Jy/beam ! Clean residual mean=0.000001 rms=0.000332 Jy/beam ! Combined flux in latest and established models = 0.136564 Jy selfcal ! Performing phase self-cal ! Adding 22 model components to the UV plane model. ! The established model now contains 174 components and 0.136564 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=0.080558Jy sigma=0.660184 ! Fit after self-cal, rms=0.080556Jy sigma=0.660173 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 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 = 0.000178263 Jy ! Component: 100 - total flux cleaned = 0.000390815 Jy ! Component: 150 - total flux cleaned = 0.000553753 Jy ! Component: 200 - total flux cleaned = 0.000702248 Jy ! Total flux subtracted in 200 components = 0.000702248 Jy ! Clean residual min=-0.001182 max=0.001264 Jy/beam ! Clean residual mean=0.000001 rms=0.000327 Jy/beam ! Combined flux in latest and established models = 0.137267 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 186 components and 0.137267 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=0.080556Jy sigma=0.660160 ! Fit after self-cal, rms=0.080555Jy sigma=0.660155 ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 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 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec ! Estimated beam: bmin=0.735 mas, bmaj=0.8737 mas, bpa=-14.91 degrees ! Estimated noise=0.383118 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.735 x 0.8737 at -14.91 degrees (North through East) ! Clean map min=-0.00087377 max=0.066827 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 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec ! Estimated beam: bmin=0.5172 mas, bmaj=0.6448 mas, bpa=-13.89 degrees ! Estimated noise=0.900564 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0488771 Jy ! Component: 100 - total flux cleaned = 0.0658275 Jy ! Component: 150 - total flux cleaned = 0.0757484 Jy ! Component: 200 - total flux cleaned = 0.0823841 Jy ! Total flux subtracted in 200 components = 0.0823841 Jy ! Clean residual min=-0.003033 max=0.004217 Jy/beam ! Clean residual mean=-0.000003 rms=0.000680 Jy/beam ! Combined flux in latest and established models = 0.0823841 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 16 model components to the UV plane model. ! The established model now contains 16 components and 0.0823841 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec ! Estimated beam: bmin=0.735 mas, bmaj=0.8737 mas, bpa=-14.91 degrees ! Estimated noise=0.383118 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 = 0.0116325 Jy ! Component: 100 - total flux cleaned = 0.0185568 Jy ! Component: 150 - total flux cleaned = 0.023387 Jy ! Component: 200 - total flux cleaned = 0.0269343 Jy ! Total flux subtracted in 200 components = 0.0269343 Jy ! Clean residual min=-0.001684 max=0.002439 Jy/beam ! Clean residual mean=-0.000005 rms=0.000431 Jy/beam ! Combined flux in latest and established models = 0.109318 Jy ! Adding 49 model components to the UV plane model. ! The established model now contains 54 components and 0.109318 Jy ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec ! Added new window around map position (1.8, 0.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00287358 Jy ! Component: 100 - total flux cleaned = 0.00526498 Jy ! Component: 150 - total flux cleaned = 0.0073439 Jy ! Component: 200 - total flux cleaned = 0.0091839 Jy ! Total flux subtracted in 200 components = 0.0091839 Jy ! Clean residual min=-0.001376 max=0.001439 Jy/beam ! Clean residual mean=-0.000002 rms=0.000337 Jy/beam ! Combined flux in latest and established models = 0.118502 Jy ! Adding 45 model components to the UV plane model. ! The established model now contains 85 components and 0.118502 Jy ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec ! Added new window around map position (-25.2, -24.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0017203 Jy ! Component: 100 - total flux cleaned = 0.00324303 Jy ! Component: 150 - total flux cleaned = 0.00463448 Jy ! Component: 200 - total flux cleaned = 0.00590718 Jy ! Total flux subtracted in 200 components = 0.00590718 Jy ! Clean residual min=-0.001236 max=0.001221 Jy/beam ! Clean residual mean=-0.000001 rms=0.000297 Jy/beam ! Combined flux in latest and established models = 0.124409 Jy ! Adding 60 model components to the UV plane model. ! The established model now contains 110 components and 0.124409 Jy ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 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 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec ! Estimated beam: bmin=2.711 mas, bmaj=2.979 mas, bpa=-68.99 degrees ! Estimated noise=0.499947 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0020986 Jy ! Component: 100 - total flux cleaned = 0.00368562 Jy ! Component: 150 - total flux cleaned = 0.00502462 Jy ! Component: 200 - total flux cleaned = 0.00617572 Jy ! Total flux subtracted in 200 components = 0.00617572 Jy ! Clean residual min=-0.001272 max=0.001168 Jy/beam ! Clean residual mean=-0.000001 rms=0.000380 Jy/beam ! Combined flux in latest and established models = 0.130585 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 = 0.00099259 Jy ! Component: 100 - total flux cleaned = 0.00185301 Jy ! Component: 150 - total flux cleaned = 0.00260523 Jy ! Component: 200 - total flux cleaned = 0.00326784 Jy ! Total flux subtracted in 200 components = 0.00326784 Jy ! Clean residual min=-0.001185 max=0.001196 Jy/beam ! Clean residual mean=-0.000000 rms=0.000346 Jy/beam ! Combined flux in latest and established models = 0.133853 Jy ! Adding 79 model components to the UV plane model. ! The established model now contains 170 components and 0.133853 Jy ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec ! Estimated beam: bmin=0.735 mas, bmaj=0.8737 mas, bpa=-14.91 degrees ! Estimated noise=0.383118 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000835503 Jy ! Component: 100 - total flux cleaned = 0.00138975 Jy ! Component: 150 - total flux cleaned = 0.00174222 Jy ! Component: 200 - total flux cleaned = 0.00192974 Jy ! Total flux subtracted in 200 components = 0.00192974 Jy ! Clean residual min=-0.001080 max=0.001139 Jy/beam ! Clean residual mean=-0.000000 rms=0.000254 Jy/beam ! Combined flux in latest and established models = 0.135783 Jy selfcal ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 184 components and 0.135783 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=0.080567Jy sigma=0.660211 ! Fit after self-cal, rms=0.080554Jy sigma=0.660090 wmodel /scr/pima/gb073_uvs/J0214+5144_X_map.mod ! Writing 184 model components to file: /scr/pima/gb073_uvs/J0214+5144_X_map.mod wobs /scr/pima/gb073_uvs/J0214+5144_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J0214+5144_X_uvs.fits wwins /scr/pima/gb073_uvs/J0214+5144_X_map.win ! wwins: Wrote 11 windows to /scr/pima/gb073_uvs/J0214+5144_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 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.00028613 Jy ! Component: 100 - total flux cleaned = 0.000478997 Jy ! Component: 150 - total flux cleaned = 0.000628446 Jy ! Component: 200 - total flux cleaned = 0.000756861 Jy ! Component: 250 - total flux cleaned = 0.00088304 Jy ! Component: 300 - total flux cleaned = 0.000989472 Jy ! Component: 350 - total flux cleaned = 0.00112866 Jy ! Component: 400 - total flux cleaned = 0.0012828 Jy ! Component: 450 - total flux cleaned = 0.00136704 Jy ! Component: 500 - total flux cleaned = 0.00143377 Jy ! Component: 550 - total flux cleaned = 0.00156557 Jy ! Component: 600 - total flux cleaned = 0.00163069 Jy ! Component: 650 - total flux cleaned = 0.00166298 Jy ! Component: 700 - total flux cleaned = 0.00171095 Jy ! Component: 750 - total flux cleaned = 0.00180545 Jy ! Component: 800 - total flux cleaned = 0.00183671 Jy ! Component: 850 - total flux cleaned = 0.00189893 Jy ! Component: 900 - total flux cleaned = 0.00192978 Jy ! Component: 950 - total flux cleaned = 0.00203648 Jy ! Component: 1000 - total flux cleaned = 0.00196046 Jy ! Component: 1050 - total flux cleaned = 0.00202062 Jy ! Component: 1100 - total flux cleaned = 0.00206539 Jy ! Component: 1150 - total flux cleaned = 0.00203566 Jy ! Component: 1200 - total flux cleaned = 0.00207983 Jy ! Component: 1250 - total flux cleaned = 0.0021237 Jy ! Component: 1300 - total flux cleaned = 0.00210915 Jy ! Component: 1350 - total flux cleaned = 0.0021236 Jy ! Component: 1400 - total flux cleaned = 0.00212366 Jy ! Component: 1450 - total flux cleaned = 0.00212374 Jy ! Component: 1500 - total flux cleaned = 0.00210948 Jy ! Component: 1550 - total flux cleaned = 0.00213777 Jy ! Component: 1600 - total flux cleaned = 0.00212362 Jy ! Component: 1650 - total flux cleaned = 0.00213758 Jy ! Component: 1700 - total flux cleaned = 0.00209574 Jy ! Component: 1750 - total flux cleaned = 0.00219296 Jy ! Component: 1800 - total flux cleaned = 0.00217914 Jy ! Component: 1850 - total flux cleaned = 0.00223405 Jy ! Component: 1900 - total flux cleaned = 0.00219302 Jy ! Component: 1950 - total flux cleaned = 0.0022475 Jy ! Component: 2000 - total flux cleaned = 0.00219333 Jy ! Component: 2050 - total flux cleaned = 0.00227405 Jy ! Component: 2100 - total flux cleaned = 0.00227396 Jy ! Component: 2150 - total flux cleaned = 0.00227402 Jy ! Component: 2200 - total flux cleaned = 0.00228739 Jy ! Component: 2250 - total flux cleaned = 0.00230062 Jy ! Component: 2300 - total flux cleaned = 0.00230063 Jy ! Component: 2350 - total flux cleaned = 0.00227438 Jy ! Component: 2400 - total flux cleaned = 0.00231363 Jy ! Component: 2450 - total flux cleaned = 0.00228761 Jy ! Component: 2500 - total flux cleaned = 0.00235249 Jy ! Component: 2550 - total flux cleaned = 0.00236535 Jy ! Component: 2600 - total flux cleaned = 0.00231378 Jy ! Component: 2650 - total flux cleaned = 0.00235228 Jy ! Component: 2700 - total flux cleaned = 0.00237787 Jy ! Component: 2750 - total flux cleaned = 0.00237786 Jy ! Component: 2800 - total flux cleaned = 0.00231454 Jy ! Component: 2850 - total flux cleaned = 0.00235253 Jy ! Component: 2900 - total flux cleaned = 0.00235257 Jy ! Component: 2950 - total flux cleaned = 0.00234005 Jy ! Component: 3000 - total flux cleaned = 0.00241504 Jy ! Component: 3050 - total flux cleaned = 0.00240255 Jy ! Component: 3100 - total flux cleaned = 0.00240251 Jy ! Component: 3150 - total flux cleaned = 0.0023655 Jy ! Component: 3200 - total flux cleaned = 0.00239009 Jy ! Component: 3250 - total flux cleaned = 0.00241462 Jy ! Component: 3300 - total flux cleaned = 0.0024024 Jy ! Component: 3350 - total flux cleaned = 0.00245119 Jy ! Component: 3400 - total flux cleaned = 0.00246331 Jy ! Component: 3450 - total flux cleaned = 0.00245119 Jy ! Component: 3500 - total flux cleaned = 0.00254782 Jy ! Component: 3550 - total flux cleaned = 0.0025478 Jy ! Component: 3600 - total flux cleaned = 0.00254774 Jy ! Component: 3650 - total flux cleaned = 0.00257165 Jy ! Component: 3700 - total flux cleaned = 0.0026075 Jy ! Component: 3750 - total flux cleaned = 0.00265509 Jy ! Component: 3800 - total flux cleaned = 0.00269064 Jy ! Component: 3850 - total flux cleaned = 0.00267885 Jy ! Component: 3900 - total flux cleaned = 0.0026789 Jy ! Component: 3950 - total flux cleaned = 0.00271412 Jy ! Component: 4000 - total flux cleaned = 0.00270237 Jy ! Component: 4050 - total flux cleaned = 0.00273745 Jy ! Total flux subtracted in 4096 components = 0.00277234 Jy ! Clean residual min=-0.000716 max=0.000678 Jy/beam ! Clean residual mean=0.000000 rms=0.000189 Jy/beam ! Combined flux in latest and established models = 0.138555 Jy keep ! Adding 357 model components to the UV plane model. ! The established model now contains 541 components and 0.138555 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J0214+5144_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.735 x 0.8737 at -14.91 degrees (North through East) ! Clean map min=-0.00079715 max=0.067205 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J0214+5144_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0672051 invert ! Inverting map ! Your choice of large map pixels excluded 2.68% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! The y-axis pixel size should ideally be below 0.1797 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000188873 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.843118 0.843118 1.68624 3.37247 6.74495 13.4899 26.9798 53.9596 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0005 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.067 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 355.822 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J0214+5144_X_uvs.log closed on Sat Dec 26 09:32:08 2015