! Started logfile: /scr/pima/gb073_uvs/J1202+4444_X_uvs.log on Sat Dec 26 09:37:35 2015 obs /scr/pima/gb073_uvs/J1202+4444_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1202+4444_X_uva.fits ! AN table 1: 29 integrations on 36 of 36 possible baselines. ! AN table 2: 29 integrations on 66 of 66 possible baselines. ! AN table 3: 29 integrations on 55 of 55 possible baselines. ! AN table 4: 29 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.730113 visibilities/baseline/integration-bin. ! Found source: J1202+4444 ! ! 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 34216 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/J1202+4444_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 58 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 5. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 87 telescope corrections were flagged in sub-array 2. ! A total of 87 telescope corrections were flagged in sub-array 3. ! A total of 87 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 87 telescope corrections were flagged in sub-array 2. ! A total of 87 telescope corrections were flagged in sub-array 3. ! A total of 87 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 7. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 8. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=1.002546Jy sigma=10.889906 ! Fit after self-cal, rms=0.962939Jy sigma=10.535908 ! 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 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 milli-arcsec ! Estimated beam: bmin=0.541 mas, bmaj=1.173 mas, bpa=-14.32 degrees ! Estimated noise=0.93495 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 = 0.0303305 Jy ! Component: 100 - total flux cleaned = 0.0369445 Jy ! Total flux subtracted in 100 components = 0.0369445 Jy ! Clean residual min=-0.002905 max=0.003913 Jy/beam ! Clean residual mean=0.000001 rms=0.000634 Jy/beam ! Combined flux in latest and established models = 0.0369445 Jy ! Performing phase self-cal ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 0.0369445 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=0.066265Jy sigma=0.657116 ! Fit after self-cal, rms=0.064333Jy sigma=0.634150 ! Inverting map ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00421514 Jy ! Component: 100 - total flux cleaned = 0.00444763 Jy ! Total flux subtracted in 100 components = 0.00444763 Jy ! Clean residual min=-0.002477 max=0.003201 Jy/beam ! Clean residual mean=-0.000001 rms=0.000605 Jy/beam ! Combined flux in latest and established models = 0.0413921 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 8 components and 0.0413922 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=0.064070Jy sigma=0.632945 ! Fit after self-cal, rms=0.064037Jy sigma=0.632618 ! Inverting map ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 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 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 milli-arcsec ! Estimated beam: bmin=0.8251 mas, bmaj=1.481 mas, bpa=-7.822 degrees ! Estimated noise=0.404781 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 (-2.4, 1.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00128595 Jy ! Component: 100 - total flux cleaned = 0.00111937 Jy ! Component: 150 - total flux cleaned = 0.000984318 Jy ! Component: 200 - total flux cleaned = 0.000867952 Jy ! Total flux subtracted in 200 components = 0.000867952 Jy ! Clean residual min=-0.001420 max=0.001376 Jy/beam ! Clean residual mean=0.000002 rms=0.000312 Jy/beam ! Combined flux in latest and established models = 0.0422601 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 27 components and 0.0422601 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=0.063978Jy sigma=0.632132 ! Fit after self-cal, rms=0.063943Jy sigma=0.631945 ! Inverting map ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8251 x 1.481 at -7.822 degrees (North through East) ! Clean map min=-0.0012334 max=0.041099 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 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.85 EF 1.00* FD 0.93 KP 1.05 ! LA 0.95 MC 0.90 NL 1.02 ON 1.00* ! OV 1.05 PT 1.08 SC 1.00 ZC 0.97 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 EF 1.00* FD 0.96 KP 1.03 ! LA 1.00 MK 1.04 NL 1.02 ON 1.00* ! PT 1.04 SC 0.95 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* 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* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* 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* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 EF 1.00* FD 1.04 KP 1.00 ! LA 1.12 MK 1.01 NL 0.99 ON 1.00* ! PT 1.11 SC 1.16 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* 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* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.03 KP 0.88 ! LA 0.96 MC 0.86 NL 1.10 ON 1.00* ! OV 1.20 PT 0.88 SC 0.98 ZC 0.93 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 0.97 KP 0.92 ! LA 1.00 MK 0.96 NL 1.14 ON 1.00* ! PT 1.00 SC 0.99 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* 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* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 0.97 KP 0.93 ! LA 0.91 MK 1.15 NL 1.14 ON 1.00* ! PT 0.94 SC 0.97 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* 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* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.94 EF 1.00* FD 0.85 KP 1.11 ! LA 1.01 MK 0.94 NL 1.19 ON 1.00* ! PT 0.91 SC 0.94 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* 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* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.85 EF 1.00* FD 0.93 KP 1.04 ! LA 1.14 MK 1.16 NL 0.99 ON 1.00* ! PT 0.86 SC 0.95 ! ! ! Fit before self-cal, rms=0.063943Jy sigma=0.631945 ! Fit after self-cal, rms=0.063754Jy sigma=0.631499 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 milli-arcsec ! Estimated beam: bmin=0.8243 mas, bmaj=1.479 mas, bpa=-7.967 degrees ! Estimated noise=0.404582 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 = 0.000363011 Jy ! Component: 100 - total flux cleaned = 0.000332912 Jy ! Component: 150 - total flux cleaned = 0.000282513 Jy ! Component: 200 - total flux cleaned = 0.000282326 Jy ! Total flux subtracted in 200 components = 0.000282326 Jy ! Clean residual min=-0.001240 max=0.001297 Jy/beam ! Clean residual mean=0.000000 rms=0.000300 Jy/beam ! Combined flux in latest and established models = 0.0425424 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 31 components and 0.0425424 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=0.063729Jy sigma=0.631350 ! Fit after self-cal, rms=0.063727Jy sigma=0.631137 ! Inverting map ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 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=0.063727Jy sigma=0.631137 ! Fit after self-cal, rms=0.063871Jy sigma=0.630930 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 milli-arcsec ! Estimated beam: bmin=0.8236 mas, bmaj=1.474 mas, bpa=-7.943 degrees ! Estimated noise=0.405291 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000226713 Jy ! Component: 100 - total flux cleaned = 0.000249399 Jy ! Component: 150 - total flux cleaned = 0.000289127 Jy ! Component: 200 - total flux cleaned = 0.000307874 Jy ! Total flux subtracted in 200 components = 0.000307874 Jy ! Clean residual min=-0.001150 max=0.001294 Jy/beam ! Clean residual mean=0.000000 rms=0.000293 Jy/beam ! Combined flux in latest and established models = 0.0428503 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 38 components and 0.0428503 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=0.063858Jy sigma=0.630868 ! Fit after self-cal, rms=0.063844Jy sigma=0.630587 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 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 (-25.2, -0.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00117392 Jy ! Component: 100 - total flux cleaned = 0.00128114 Jy ! Component: 150 - total flux cleaned = 0.00132329 Jy ! Component: 200 - total flux cleaned = 0.00132326 Jy ! Total flux subtracted in 200 components = 0.00132326 Jy ! Clean residual min=-0.001099 max=0.001217 Jy/beam ! Clean residual mean=0.000001 rms=0.000284 Jy/beam ! Combined flux in latest and established models = 0.0441736 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 47 components and 0.0441736 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=0.063815Jy sigma=0.630357 ! Fit after self-cal, rms=0.063797Jy sigma=0.630246 ! Inverting map ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 milli-arcsec ! Added new window around map position (15.4, 12.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.001184 Jy ! Component: 100 - total flux cleaned = 0.00133495 Jy ! Component: 150 - total flux cleaned = 0.00128585 Jy ! Component: 200 - total flux cleaned = 0.00121883 Jy ! Total flux subtracted in 200 components = 0.00121883 Jy ! Clean residual min=-0.001070 max=0.001212 Jy/beam ! Clean residual mean=0.000002 rms=0.000274 Jy/beam ! Combined flux in latest and established models = 0.0453924 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 61 components and 0.0453924 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=0.063763Jy sigma=0.629996 ! Fit after self-cal, rms=0.063744Jy sigma=0.629916 ! Inverting map ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 milli-arcsec ! Added new window around map position (5, -32.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000836104 Jy ! Component: 100 - total flux cleaned = 0.00108015 Jy ! Component: 150 - total flux cleaned = 0.00110837 Jy ! Component: 200 - total flux cleaned = 0.00106134 Jy ! Total flux subtracted in 200 components = 0.00106134 Jy ! Clean residual min=-0.001019 max=0.001169 Jy/beam ! Clean residual mean=0.000001 rms=0.000266 Jy/beam ! Combined flux in latest and established models = 0.0464537 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 70 components and 0.0464537 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=0.063711Jy sigma=0.629661 ! Fit after self-cal, rms=0.063699Jy sigma=0.629593 ! Inverting map ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 milli-arcsec ! Added new window around map position (-16, -31.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000830568 Jy ! Component: 100 - total flux cleaned = 0.000973831 Jy ! Component: 150 - total flux cleaned = 0.00102555 Jy ! Component: 200 - total flux cleaned = 0.000978984 Jy ! Total flux subtracted in 200 components = 0.000978984 Jy ! Clean residual min=-0.001011 max=0.001052 Jy/beam ! Clean residual mean=0.000002 rms=0.000258 Jy/beam ! Combined flux in latest and established models = 0.0474327 Jy ! Performing phase self-cal ! Adding 32 model components to the UV plane model. ! The established model now contains 80 components and 0.0474327 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=0.063670Jy sigma=0.629347 ! Fit after self-cal, rms=0.063655Jy sigma=0.629265 ! Inverting map ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 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=0.063655Jy sigma=0.629265 ! Fit after self-cal, rms=0.063522Jy sigma=0.629107 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 milli-arcsec ! Estimated beam: bmin=0.8235 mas, bmaj=1.474 mas, bpa=-8.023 degrees ! Estimated noise=0.405136 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00049494 Jy ! Component: 100 - total flux cleaned = 0.000520629 Jy ! Component: 150 - total flux cleaned = 0.000497361 Jy ! Component: 200 - total flux cleaned = 0.000497683 Jy ! Total flux subtracted in 200 components = 0.000497683 Jy ! Clean residual min=-0.000983 max=0.001043 Jy/beam ! Clean residual mean=0.000001 rms=0.000254 Jy/beam ! Combined flux in latest and established models = 0.0479304 Jy selfcal ! Performing phase self-cal ! Adding 35 model components to the UV plane model. ! The established model now contains 85 components and 0.0479304 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=0.063502Jy sigma=0.628955 ! Fit after self-cal, rms=0.063503Jy sigma=0.628848 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 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 = 0.000280774 Jy ! Component: 100 - total flux cleaned = 0.000280378 Jy ! Component: 150 - total flux cleaned = 0.000259555 Jy ! Component: 200 - total flux cleaned = 0.000259523 Jy ! Total flux subtracted in 200 components = 0.000259523 Jy ! Clean residual min=-0.000970 max=0.001021 Jy/beam ! Clean residual mean=0.000001 rms=0.000252 Jy/beam ! Combined flux in latest and established models = 0.0481899 Jy ! Performing phase self-cal ! Adding 33 model components to the UV plane model. ! The established model now contains 88 components and 0.0481899 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=0.063487Jy sigma=0.628738 ! Fit after self-cal, rms=0.063484Jy sigma=0.628720 ! Inverting map ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 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=0.063484Jy sigma=0.628720 ! Fit after self-cal, rms=0.063468Jy sigma=0.628729 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 milli-arcsec ! Estimated beam: bmin=2.665 mas, bmaj=2.852 mas, bpa=13.27 degrees ! Estimated noise=0.498535 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000373594 Jy ! Component: 100 - total flux cleaned = 0.000389628 Jy ! Component: 150 - total flux cleaned = 0.000417833 Jy ! Component: 200 - total flux cleaned = 0.000405542 Jy ! Total flux subtracted in 200 components = 0.000405542 Jy ! Clean residual min=-0.001187 max=0.001292 Jy/beam ! Clean residual mean=-0.000001 rms=0.000305 Jy/beam ! Combined flux in latest and established models = 0.0485955 Jy selfcal ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 102 components and 0.0485955 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=0.063461Jy sigma=0.628687 ! Fit after self-cal, rms=0.063452Jy sigma=0.628597 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 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 = 0.000194152 Jy ! Component: 100 - total flux cleaned = 0.000193515 Jy ! Component: 150 - total flux cleaned = 0.000205411 Jy ! Component: 200 - total flux cleaned = 0.000228595 Jy ! Total flux subtracted in 200 components = 0.000228595 Jy ! Clean residual min=-0.001184 max=0.001266 Jy/beam ! Clean residual mean=-0.000001 rms=0.000303 Jy/beam ! Combined flux in latest and established models = 0.0488241 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 107 components and 0.0488241 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=0.063448Jy sigma=0.628574 ! Fit after self-cal, rms=0.063446Jy sigma=0.628567 ! Inverting map ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 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 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 milli-arcsec ! Estimated beam: bmin=0.824 mas, bmaj=1.474 mas, bpa=-7.997 degrees ! Estimated noise=0.404883 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.824 x 1.474 at -7.997 degrees (North through East) ! Clean map min=-0.0019673 max=0.041133 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 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 milli-arcsec ! Estimated beam: bmin=0.5394 mas, bmaj=1.167 mas, bpa=-14.55 degrees ! Estimated noise=0.935849 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0331274 Jy ! Component: 100 - total flux cleaned = 0.0409185 Jy ! Component: 150 - total flux cleaned = 0.0448555 Jy ! Component: 200 - total flux cleaned = 0.0473857 Jy ! Total flux subtracted in 200 components = 0.0473857 Jy ! Clean residual min=-0.002553 max=0.002805 Jy/beam ! Clean residual mean=-0.000003 rms=0.000602 Jy/beam ! Combined flux in latest and established models = 0.0473857 Jy uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Adding 13 model components to the UV plane model. ! The established model now contains 13 components and 0.0473857 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 milli-arcsec ! Estimated beam: bmin=0.824 mas, bmaj=1.474 mas, bpa=-7.997 degrees ! Estimated noise=0.404883 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 = 0.00120498 Jy ! Component: 100 - total flux cleaned = 0.00172837 Jy ! Component: 150 - total flux cleaned = 0.00189079 Jy ! Component: 200 - total flux cleaned = 0.0018896 Jy ! Total flux subtracted in 200 components = 0.0018896 Jy ! Clean residual min=-0.001227 max=0.001266 Jy/beam ! Clean residual mean=0.000001 rms=0.000285 Jy/beam ! Combined flux in latest and established models = 0.0492753 Jy ! Adding 24 model components to the UV plane model. ! The established model now contains 34 components and 0.0492753 Jy ! Inverting map ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 milli-arcsec ! Added new window around map position (0.6, 8.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000486134 Jy ! Component: 100 - total flux cleaned = 0.000398077 Jy ! Component: 150 - total flux cleaned = 0.000357925 Jy ! Component: 200 - total flux cleaned = 0.000320651 Jy ! Total flux subtracted in 200 components = 0.000320651 Jy ! Clean residual min=-0.001151 max=0.001169 Jy/beam ! Clean residual mean=0.000000 rms=0.000269 Jy/beam ! Combined flux in latest and established models = 0.049596 Jy ! Adding 35 model components to the UV plane model. ! The established model now contains 49 components and 0.049596 Jy ! Inverting map ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 milli-arcsec ! Added new window around map position (-22.8, -11.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000690889 Jy ! Component: 100 - total flux cleaned = 0.000796676 Jy ! Component: 150 - total flux cleaned = 0.000895836 Jy ! Component: 200 - total flux cleaned = 0.00089508 Jy ! Total flux subtracted in 200 components = 0.00089508 Jy ! Clean residual min=-0.001061 max=0.001072 Jy/beam ! Clean residual mean=0.000000 rms=0.000257 Jy/beam ! Combined flux in latest and established models = 0.0504911 Jy ! Adding 43 model components to the UV plane model. ! The established model now contains 63 components and 0.050491 Jy ! Inverting map ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 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 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 milli-arcsec ! Estimated beam: bmin=2.665 mas, bmaj=2.852 mas, bpa=13.27 degrees ! Estimated noise=0.498535 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000266005 Jy ! Component: 100 - total flux cleaned = 0.000311039 Jy ! Component: 150 - total flux cleaned = 0.000311791 Jy ! Component: 200 - total flux cleaned = 0.000259215 Jy ! Total flux subtracted in 200 components = 0.000259215 Jy ! Clean residual min=-0.001194 max=0.001221 Jy/beam ! Clean residual mean=-0.000001 rms=0.000292 Jy/beam ! Combined flux in latest and established models = 0.0507503 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 = -4.89291e-05 Jy ! Component: 100 - total flux cleaned = -6.37806e-05 Jy ! Component: 150 - total flux cleaned = -7.82802e-05 Jy ! Component: 200 - total flux cleaned = -0.000106126 Jy ! Total flux subtracted in 200 components = -0.000106126 Jy ! Clean residual min=-0.001173 max=0.001183 Jy/beam ! Clean residual mean=-0.000001 rms=0.000290 Jy/beam ! Combined flux in latest and established models = 0.0506441 Jy ! Adding 40 model components to the UV plane model. ! The established model now contains 96 components and 0.0506441 Jy ! Inverting map ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 milli-arcsec ! Estimated beam: bmin=0.824 mas, bmaj=1.474 mas, bpa=-7.997 degrees ! Estimated noise=0.404883 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -3.86575e-05 Jy ! Component: 100 - total flux cleaned = -9.14775e-05 Jy ! Component: 150 - total flux cleaned = -6.63761e-05 Jy ! Component: 200 - total flux cleaned = -9.00244e-05 Jy ! Total flux subtracted in 200 components = -9.00244e-05 Jy ! Clean residual min=-0.000991 max=0.001028 Jy/beam ! Clean residual mean=-0.000000 rms=0.000246 Jy/beam ! Combined flux in latest and established models = 0.0505541 Jy selfcal ! Performing phase self-cal ! Adding 36 model components to the UV plane model. ! The established model now contains 111 components and 0.0505541 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=0.063460Jy sigma=0.628618 ! Fit after self-cal, rms=0.063451Jy sigma=0.628512 wmodel /scr/pima/gb073_uvs/J1202+4444_X_map.mod ! Writing 111 model components to file: /scr/pima/gb073_uvs/J1202+4444_X_map.mod wobs /scr/pima/gb073_uvs/J1202+4444_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1202+4444_X_uvs.fits wwins /scr/pima/gb073_uvs/J1202+4444_X_map.win ! wwins: Wrote 8 windows to /scr/pima/gb073_uvs/J1202+4444_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 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.00014076 Jy ! Component: 100 - total flux cleaned = 0.000177495 Jy ! Component: 150 - total flux cleaned = 0.000211938 Jy ! Component: 200 - total flux cleaned = 0.000211589 Jy ! Component: 250 - total flux cleaned = 0.000162383 Jy ! Component: 300 - total flux cleaned = 0.000114307 Jy ! Component: 350 - total flux cleaned = 6.74749e-05 Jy ! Component: 400 - total flux cleaned = 0.000190914 Jy ! Component: 450 - total flux cleaned = 0.000190546 Jy ! Component: 500 - total flux cleaned = 0.000220237 Jy ! Component: 550 - total flux cleaned = 0.000249646 Jy ! Component: 600 - total flux cleaned = 0.000293082 Jy ! Component: 650 - total flux cleaned = 0.000293032 Jy ! Component: 700 - total flux cleaned = 0.000335532 Jy ! Component: 750 - total flux cleaned = 0.000377622 Jy ! Component: 800 - total flux cleaned = 0.000391219 Jy ! Component: 850 - total flux cleaned = 0.000377365 Jy ! Component: 900 - total flux cleaned = 0.000377482 Jy ! Component: 950 - total flux cleaned = 0.000431179 Jy ! Component: 1000 - total flux cleaned = 0.000431095 Jy ! Component: 1050 - total flux cleaned = 0.00045745 Jy ! Component: 1100 - total flux cleaned = 0.000470606 Jy ! Component: 1150 - total flux cleaned = 0.000522584 Jy ! Component: 1200 - total flux cleaned = 0.000522528 Jy ! Component: 1250 - total flux cleaned = 0.00052276 Jy ! Component: 1300 - total flux cleaned = 0.00057312 Jy ! Component: 1350 - total flux cleaned = 0.000560565 Jy ! Component: 1400 - total flux cleaned = 0.000572934 Jy ! Component: 1450 - total flux cleaned = 0.000609781 Jy ! Component: 1500 - total flux cleaned = 0.000597442 Jy ! Component: 1550 - total flux cleaned = 0.000548987 Jy ! Component: 1600 - total flux cleaned = 0.000549149 Jy ! Component: 1650 - total flux cleaned = 0.000549062 Jy ! Component: 1700 - total flux cleaned = 0.00053715 Jy ! Component: 1750 - total flux cleaned = 0.000478518 Jy ! Component: 1800 - total flux cleaned = 0.000536963 Jy ! Component: 1850 - total flux cleaned = 0.000513615 Jy ! Component: 1900 - total flux cleaned = 0.000559647 Jy ! Component: 1950 - total flux cleaned = 0.000548171 Jy ! Component: 2000 - total flux cleaned = 0.000570946 Jy ! Component: 2050 - total flux cleaned = 0.000559616 Jy ! Component: 2100 - total flux cleaned = 0.000581939 Jy ! Component: 2150 - total flux cleaned = 0.000581978 Jy ! Component: 2200 - total flux cleaned = 0.000626205 Jy ! Component: 2250 - total flux cleaned = 0.000626269 Jy ! Component: 2300 - total flux cleaned = 0.000637244 Jy ! Component: 2350 - total flux cleaned = 0.000626391 Jy ! Component: 2400 - total flux cleaned = 0.000669577 Jy ! Component: 2450 - total flux cleaned = 0.000637441 Jy ! Component: 2500 - total flux cleaned = 0.000594876 Jy ! Component: 2550 - total flux cleaned = 0.000637229 Jy ! Component: 2600 - total flux cleaned = 0.00065831 Jy ! Component: 2650 - total flux cleaned = 0.000574576 Jy ! Component: 2700 - total flux cleaned = 0.000595353 Jy ! Component: 2750 - total flux cleaned = 0.000564216 Jy ! Component: 2800 - total flux cleaned = 0.000512716 Jy ! Component: 2850 - total flux cleaned = 0.000512741 Jy ! Component: 2900 - total flux cleaned = 0.000471995 Jy ! Component: 2950 - total flux cleaned = 0.000441738 Jy ! Component: 3000 - total flux cleaned = 0.000482074 Jy ! Component: 3050 - total flux cleaned = 0.000451903 Jy ! Component: 3100 - total flux cleaned = 0.000431913 Jy ! Component: 3150 - total flux cleaned = 0.000402116 Jy ! Component: 3200 - total flux cleaned = 0.000362649 Jy ! Component: 3250 - total flux cleaned = 0.000352853 Jy ! Component: 3300 - total flux cleaned = 0.000362647 Jy ! Component: 3350 - total flux cleaned = 0.000372348 Jy ! Component: 3400 - total flux cleaned = 0.000314282 Jy ! Component: 3450 - total flux cleaned = 0.000314212 Jy ! Component: 3500 - total flux cleaned = 0.000333467 Jy ! Component: 3550 - total flux cleaned = 0.000276275 Jy ! Component: 3600 - total flux cleaned = 0.000276289 Jy ! Component: 3650 - total flux cleaned = 0.000266921 Jy ! Component: 3700 - total flux cleaned = 0.00022924 Jy ! Component: 3750 - total flux cleaned = 0.000210494 Jy ! Component: 3800 - total flux cleaned = 0.000182511 Jy ! Component: 3850 - total flux cleaned = 0.000145422 Jy ! Component: 3900 - total flux cleaned = 0.000200817 Jy ! Component: 3950 - total flux cleaned = 0.000136419 Jy ! Component: 4000 - total flux cleaned = 0.00010901 Jy ! Component: 4050 - total flux cleaned = 9.98969e-05 Jy ! Total flux subtracted in 4096 components = 9.08018e-05 Jy ! Clean residual min=-0.000555 max=0.000700 Jy/beam ! Clean residual mean=0.000000 rms=0.000153 Jy/beam ! Combined flux in latest and established models = 0.0506449 Jy keep ! Adding 313 model components to the UV plane model. ! The established model now contains 423 components and 0.0506449 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1202+4444_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.824 x 1.474 at -7.997 degrees (North through East) ! Clean map min=-0.0016171 max=0.041101 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1202+4444_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0411011 invert ! Inverting map ! Your choice of large map pixels excluded 5.37% of the data. ! The x-axis pixel size should ideally be below 0.1855 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000152735 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -1.11482 1.11482 2.22965 4.45929 8.91859 17.8372 35.6743 71.3487 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0004 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.041 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 269.1 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1202+4444_X_uvs.log closed on Sat Dec 26 09:37:40 2015