! Started logfile: J0854+2006_X_2010_10_13_pus_uvs.log on Mon Feb 28 17:16:06 2011 obs J0854+2006_X_2010_10_13_pus_uva.fits ! Reading UV FITS file: J0854+2006_X_2010_10_13_pus_uva.fits ! AN table 1: 264 integrations on 105 of 105 possible baselines. ! AN table 2: 28 integrations on 105 of 105 possible baselines. ! AN table 3: 15 integrations on 105 of 105 possible baselines. ! Apparent sampling: 0.106096 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J0854+2006 ! ! There are 4 IFs, and a total of 4 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 8.40996e+09 8e+06 1 8e+06 ! 02 2 8.47996e+09 8e+06 1 8e+06 ! 03 3 8.79496e+09 8e+06 1 8e+06 ! 04 4 8.89996e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 5978 lines of history. ! ! Reading 13680 visibilities. select I ! Polarization I is unavailable. ! Selecting polarization: RR, channels: 1..4 ! Reading IF 1 channels: 1..1 ! Reading IF 2 channels: 2..2 ! Reading IF 3 channels: 3..3 ! Reading IF 4 channels: 4..4 print "field_size =",field_size ! field_size = 256 print "field_cell =",field_cell ! field_cell = 0.2 print "taper_size =",taper_size ! taper_size = 70 ![@muppet J0854+2006_X_2010_10_13_pus] 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 = 256x256 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 3064 telescope corrections were flagged in sub-array 1. ! A total of 327 telescope corrections were flagged in sub-array 2. ! A total of 159 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 2. ! A total of 3064 telescope corrections were flagged in sub-array 1. ! A total of 327 telescope corrections were flagged in sub-array 2. ! A total of 159 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 3. ! A total of 3064 telescope corrections were flagged in sub-array 1. ! A total of 327 telescope corrections were flagged in sub-array 2. ! A total of 159 telescope corrections were flagged in sub-array 3. ! ! Correcting IF 4. ! A total of 3064 telescope corrections were flagged in sub-array 1. ! A total of 327 telescope corrections were flagged in sub-array 2. ! A total of 159 telescope corrections were flagged in sub-array 3. ! ! Fit before self-cal, rms=2.511538Jy sigma=0.030231 ! Fit after self-cal, rms=2.502239Jy sigma=0.030187 ! 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 7.23% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec ! Estimated beam: bmin=0.5306 mas, bmaj=0.8498 mas, bpa=-3.348 degrees ! Estimated noise=960.273 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 = 2.49789 Jy ! Component: 100 - total flux cleaned = 3.11441 Jy ! Total flux subtracted in 100 components = 3.11441 Jy ! Clean residual min=-0.162358 max=0.241600 Jy/beam ! Clean residual mean=0.005380 rms=0.049081 Jy/beam ! Combined flux in latest and established models = 3.11441 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 3.11441 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.982380Jy sigma=0.011848 ! Fit after self-cal, rms=0.982395Jy sigma=0.011848 ! Inverting map ! Your choice of large map pixels excluded 7.23% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 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 7.23% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec ! Estimated beam: bmin=0.6833 mas, bmaj=1.163 mas, bpa=-3.279 degrees ! Estimated noise=587.072 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 = 0.427372 Jy ! Component: 100 - total flux cleaned = 0.619909 Jy ! Component: 150 - total flux cleaned = 0.709964 Jy ! Component: 200 - total flux cleaned = 0.754238 Jy ! Total flux subtracted in 200 components = 0.754238 Jy ! Clean residual min=-0.080268 max=0.171850 Jy/beam ! Clean residual mean=0.016714 rms=0.042293 Jy/beam ! Combined flux in latest and established models = 3.86865 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 21 components and 3.86865 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.858561Jy sigma=0.009675 ! Fit after self-cal, rms=0.858166Jy sigma=0.009673 ! Inverting map ! Your choice of large map pixels excluded 7.23% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 105 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.94 FD 0.81 HH 1.22 HN 1.06 ! KB 1.00 KK 0.96 KP 0.95 LA 0.98 ! MK 1.02 NL 1.16 NY 0.99 OV 0.97 ! PT 0.94 SC 0.96 TS 1.00 ! ! A total of 36 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.90 FD 1.00* HH 1.00* HN 1.00* ! KB 0.99 KK 1.00* KP 1.00* LA 1.00* ! MK 1.05 NL 1.00* NY 1.00* OV 0.96 ! PT 1.00* SC 1.00* TS 0.99 ! ! A total of 9 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00* HH 0.98 HN 1.07 ! KB 1.00* KK 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.40 NY 0.97 OV 1.00* ! PT 1.00* SC 1.03 TS 1.00* ! ! ! Correcting IF 2. ! A total of 105 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 FD 0.95 HH 1.21 HN 1.08 ! KB 1.01 KK 0.99 KP 0.95 LA 0.95 ! MK 0.96 NL 1.19 NY 0.99 OV 1.00 ! PT 0.95 SC 0.97 TS 1.02 ! ! A total of 36 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.93 FD 1.00* HH 1.00* HN 1.00* ! KB 0.99 KK 1.00* KP 1.00* LA 1.00* ! MK 1.00 NL 1.00* NY 1.00* OV 0.99 ! PT 1.00* SC 1.00* TS 1.00 ! ! A total of 9 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00* HH 0.98 HN 1.09 ! KB 1.00* KK 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.45 NY 0.96 OV 1.00* ! PT 1.00* SC 1.05 TS 1.00* ! ! ! Correcting IF 3. ! A total of 105 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.96 FD 0.95 HH 1.21 HN 1.09 ! KB 0.99 KK 0.95 KP 0.94 LA 0.93 ! MK 1.00 NL 1.14 NY 1.03 OV 0.97 ! PT 0.98 SC 0.99 TS 1.00 ! ! A total of 36 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.90 FD 1.00* HH 1.00* HN 1.00* ! KB 0.98 KK 1.00* KP 1.00* LA 1.00* ! MK 1.04 NL 1.00* NY 1.00* OV 0.97 ! PT 1.00* SC 1.00* TS 0.97 ! ! A total of 9 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00* HH 0.94 HN 1.10 ! KB 1.00* KK 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.35 NY 1.02 OV 1.00* ! PT 1.00* SC 1.08 TS 1.00* ! ! ! Correcting IF 4. ! A total of 105 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.96 HH 1.22 HN 1.06 ! KB 0.98 KK 0.98 KP 0.94 LA 1.00 ! MK 0.98 NL 1.17 NY 1.00 OV 1.02 ! PT 0.94 SC 0.98 TS 0.91 ! ! A total of 36 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 0.95 FD 1.00* HH 1.00* HN 1.00* ! KB 0.97 KK 1.00* KP 1.00* LA 1.00* ! MK 1.03 NL 1.00* NY 1.00* OV 1.00 ! PT 1.00* SC 1.00* TS 0.88 ! ! A total of 9 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00* HH 0.93 HN 1.08 ! KB 1.00* KK 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.40 NY 1.00 OV 1.00* ! PT 1.00* SC 1.04 TS 1.00* ! ! ! Fit before self-cal, rms=0.858166Jy sigma=0.009673 ! Fit after self-cal, rms=0.811657Jy sigma=0.008445 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec ! Estimated beam: bmin=0.6923 mas, bmaj=1.22 mas, bpa=-4.574 degrees ! Estimated noise=593.599 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 = -0.0236333 Jy ! Component: 100 - total flux cleaned = -0.0227664 Jy ! Component: 150 - total flux cleaned = -0.0227627 Jy ! Component: 200 - total flux cleaned = -0.0227362 Jy ! Total flux subtracted in 200 components = -0.0227362 Jy ! Clean residual min=-0.127077 max=0.128608 Jy/beam ! Clean residual mean=0.006921 rms=0.035651 Jy/beam ! Combined flux in latest and established models = 3.84592 Jy ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 23 components and 3.84592 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.809546Jy sigma=0.008437 ! Fit after self-cal, rms=0.809706Jy sigma=0.008436 ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 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. ! ! Fit before self-cal, rms=0.809706Jy sigma=0.008436 ! Fit after self-cal, rms=0.645171Jy sigma=0.002349 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec ! Estimated beam: bmin=0.6962 mas, bmaj=1.238 mas, bpa=-5.041 degrees ! Estimated noise=595.385 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00479347 Jy ! Component: 100 - total flux cleaned = 0.00351894 Jy ! Component: 150 - total flux cleaned = 0.00176419 Jy ! Component: 200 - total flux cleaned = 0.00072565 Jy ! Total flux subtracted in 200 components = 0.00072565 Jy ! Clean residual min=-0.019176 max=0.075668 Jy/beam ! Clean residual mean=0.001588 rms=0.008434 Jy/beam ! Combined flux in latest and established models = 3.84664 Jy selfcal ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 23 components and 3.84664 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.644067Jy sigma=0.002317 ! Fit after self-cal, rms=0.645524Jy sigma=0.002313 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (-0.8, -1). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.071892 Jy ! Component: 100 - total flux cleaned = 0.0775161 Jy ! Component: 150 - total flux cleaned = 0.0745377 Jy ! Component: 200 - total flux cleaned = 0.0720305 Jy ! Total flux subtracted in 200 components = 0.0720305 Jy ! Clean residual min=-0.020003 max=0.032896 Jy/beam ! Clean residual mean=-0.000221 rms=0.005369 Jy/beam ! Combined flux in latest and established models = 3.91867 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 37 components and 3.91867 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.636060Jy sigma=0.002034 ! Fit after self-cal, rms=0.634196Jy sigma=0.001983 ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.013499 Jy ! Component: 100 - total flux cleaned = 0.0119617 Jy ! Component: 150 - total flux cleaned = 0.0100905 Jy ! Component: 200 - total flux cleaned = 0.0106269 Jy ! Total flux subtracted in 200 components = 0.0106269 Jy ! Clean residual min=-0.020797 max=0.024002 Jy/beam ! Clean residual mean=-0.000487 rms=0.004714 Jy/beam ! Combined flux in latest and established models = 3.9293 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 43 components and 3.9293 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.631588Jy sigma=0.001921 ! Fit after self-cal, rms=0.631095Jy sigma=0.001908 ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 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. ! ! Fit before self-cal, rms=0.631095Jy sigma=0.001908 ! Fit after self-cal, rms=0.697232Jy sigma=0.001759 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec ! Estimated beam: bmin=0.6972 mas, bmaj=1.239 mas, bpa=-5.018 degrees ! Estimated noise=595.868 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0250262 Jy ! Component: 100 - total flux cleaned = 0.0257218 Jy ! Component: 150 - total flux cleaned = 0.0268291 Jy ! Component: 200 - total flux cleaned = 0.0287412 Jy ! Total flux subtracted in 200 components = 0.0287412 Jy ! Clean residual min=-0.011795 max=0.020559 Jy/beam ! Clean residual mean=0.000210 rms=0.003496 Jy/beam ! Combined flux in latest and established models = 3.95804 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 52 components and 3.95804 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.695361Jy sigma=0.001685 ! Fit after self-cal, rms=0.694193Jy sigma=0.001669 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 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 (-5.2, -3). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.014139 Jy ! Component: 100 - total flux cleaned = 0.0152626 Jy ! Component: 150 - total flux cleaned = 0.015704 Jy ! Component: 200 - total flux cleaned = 0.0168711 Jy ! Total flux subtracted in 200 components = 0.0168711 Jy ! Clean residual min=-0.012068 max=0.014927 Jy/beam ! Clean residual mean=-0.000173 rms=0.002962 Jy/beam ! Combined flux in latest and established models = 3.97491 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 59 components and 3.97491 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.693246Jy sigma=0.001634 ! Fit after self-cal, rms=0.693071Jy sigma=0.001628 ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec ! Added new window around map position (-2.6, 1.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00898422 Jy ! Component: 100 - total flux cleaned = 0.0110544 Jy ! Component: 150 - total flux cleaned = 0.0113857 Jy ! Component: 200 - total flux cleaned = 0.0117052 Jy ! Total flux subtracted in 200 components = 0.0117052 Jy ! Clean residual min=-0.011268 max=0.012795 Jy/beam ! Clean residual mean=-0.000444 rms=0.002667 Jy/beam ! Combined flux in latest and established models = 3.98662 Jy ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 68 components and 3.98662 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.692570Jy sigma=0.001609 ! Fit after self-cal, rms=0.692454Jy sigma=0.001606 ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 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. ! ! Fit before self-cal, rms=0.692454Jy sigma=0.001606 ! Fit after self-cal, rms=0.692531Jy sigma=0.001577 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec ! Estimated beam: bmin=2.586 mas, bmaj=2.767 mas, bpa=1.283 degrees ! Estimated noise=778.837 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0154343 Jy ! Component: 100 - total flux cleaned = 0.0219256 Jy ! Component: 150 - total flux cleaned = 0.0236848 Jy ! Component: 200 - total flux cleaned = 0.0248082 Jy ! Total flux subtracted in 200 components = 0.0248082 Jy ! Clean residual min=-0.008092 max=0.007408 Jy/beam ! Clean residual mean=-0.000379 rms=0.002368 Jy/beam ! Combined flux in latest and established models = 4.01142 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 77 components and 4.01143 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.692538Jy sigma=0.001571 ! Fit after self-cal, rms=0.692331Jy sigma=0.001568 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 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 = 0.00191122 Jy ! Component: 100 - total flux cleaned = 0.00289214 Jy ! Component: 150 - total flux cleaned = 0.00391891 Jy ! Component: 200 - total flux cleaned = 0.00476441 Jy ! Total flux subtracted in 200 components = 0.00476441 Jy ! Clean residual min=-0.007809 max=0.006472 Jy/beam ! Clean residual mean=-0.000655 rms=0.002285 Jy/beam ! Combined flux in latest and established models = 4.01619 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 82 components and 4.01619 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.692348Jy sigma=0.001566 ! Fit after self-cal, rms=0.692261Jy sigma=0.001565 ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 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 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec ! Estimated beam: bmin=0.6976 mas, bmaj=1.239 mas, bpa=-4.958 degrees ! Estimated noise=595.79 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6976 x 1.239 at -4.958 degrees (North through East) ! Clean map min=-0.011756 max=3.353 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 ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.692261Jy sigma=0.001565 ! Fit after self-cal, rms=0.813637Jy sigma=0.001370 ! Inverting map and beam ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec ! Estimated beam: bmin=0.6972 mas, bmaj=1.24 mas, bpa=-5.005 degrees ! Estimated noise=595.88 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00404738 Jy ! Component: 100 - total flux cleaned = 0.00405353 Jy ! Component: 150 - total flux cleaned = 0.00438181 Jy ! Component: 200 - total flux cleaned = 0.00360801 Jy ! Total flux subtracted in 200 components = 0.00360801 Jy ! Clean residual min=-0.007785 max=0.013140 Jy/beam ! Clean residual mean=-0.000047 rms=0.002123 Jy/beam ! Combined flux in latest and established models = 4.0198 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 86 components and 4.0198 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.813159Jy sigma=0.001347 ! Fit after self-cal, rms=0.813109Jy sigma=0.001344 ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec ! Added new window around map position (0.4, -4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00710086 Jy ! Component: 100 - total flux cleaned = 0.00740394 Jy ! Component: 150 - total flux cleaned = 0.00690836 Jy ! Component: 200 - total flux cleaned = 0.00668754 Jy ! Total flux subtracted in 200 components = 0.00668754 Jy ! Clean residual min=-0.006889 max=0.007653 Jy/beam ! Clean residual mean=-0.000221 rms=0.001859 Jy/beam ! Combined flux in latest and established models = 4.02649 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 98 components and 4.02649 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.812900Jy sigma=0.001330 ! Fit after self-cal, rms=0.812888Jy sigma=0.001330 ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.812888Jy sigma=0.001330 ! Fit after self-cal, rms=0.813559Jy sigma=0.001323 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 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec ! Estimated beam: bmin=0.5566 mas, bmaj=0.9181 mas, bpa=-3.241 degrees ! Estimated noise=996.562 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 2.54496 Jy ! Component: 100 - total flux cleaned = 3.12482 Jy ! Component: 150 - total flux cleaned = 3.37527 Jy ! Component: 200 - total flux cleaned = 3.5365 Jy ! Total flux subtracted in 200 components = 3.5365 Jy ! Clean residual min=-0.025708 max=0.088759 Jy/beam ! Clean residual mean=0.002135 rms=0.010701 Jy/beam ! Combined flux in latest and established models = 3.5365 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 18 model components to the UV plane model. ! The established model now contains 18 components and 3.5365 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec ! Estimated beam: bmin=0.6976 mas, bmaj=1.24 mas, bpa=-4.949 degrees ! Estimated noise=595.917 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 = 0.195081 Jy ! Component: 100 - total flux cleaned = 0.298596 Jy ! Component: 150 - total flux cleaned = 0.361024 Jy ! Component: 200 - total flux cleaned = 0.400617 Jy ! Total flux subtracted in 200 components = 0.400617 Jy ! Clean residual min=-0.006998 max=0.024078 Jy/beam ! Clean residual mean=0.002235 rms=0.004139 Jy/beam ! Combined flux in latest and established models = 3.93712 Jy ! Adding 38 model components to the UV plane model. ! The established model now contains 42 components and 3.93712 Jy ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec ! Added new window around map position (0.6, 1.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0276404 Jy ! Component: 100 - total flux cleaned = 0.0475624 Jy ! Component: 150 - total flux cleaned = 0.0628135 Jy ! Component: 200 - total flux cleaned = 0.0747749 Jy ! Total flux subtracted in 200 components = 0.0747749 Jy ! Clean residual min=-0.006748 max=0.009876 Jy/beam ! Clean residual mean=0.000437 rms=0.002204 Jy/beam ! Combined flux in latest and established models = 4.01189 Jy ! Adding 31 model components to the UV plane model. ! The established model now contains 64 components and 4.01189 Jy ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec ! Added new window around map position (-5, -0.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00816563 Jy ! Component: 100 - total flux cleaned = 0.0112954 Jy ! Component: 150 - total flux cleaned = 0.0141193 Jy ! Component: 200 - total flux cleaned = 0.0166883 Jy ! Total flux subtracted in 200 components = 0.0166883 Jy ! Clean residual min=-0.006520 max=0.006865 Jy/beam ! Clean residual mean=0.000065 rms=0.001833 Jy/beam ! Combined flux in latest and established models = 4.02858 Jy ! Adding 35 model components to the UV plane model. ! The established model now contains 81 components and 4.02858 Jy ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 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 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec ! Estimated beam: bmin=2.581 mas, bmaj=2.765 mas, bpa=0.815 degrees ! Estimated noise=779.805 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00758893 Jy ! Component: 100 - total flux cleaned = 0.0112566 Jy ! Component: 150 - total flux cleaned = 0.0122907 Jy ! Component: 200 - total flux cleaned = 0.0131758 Jy ! Total flux subtracted in 200 components = 0.0131758 Jy ! Clean residual min=-0.005916 max=0.005375 Jy/beam ! Clean residual mean=-0.000613 rms=0.001938 Jy/beam ! Combined flux in latest and established models = 4.04176 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 = 0.000478529 Jy ! Component: 100 - total flux cleaned = 0.000740277 Jy ! Component: 150 - total flux cleaned = 0.000821752 Jy ! Component: 200 - total flux cleaned = 0.000898658 Jy ! Total flux subtracted in 200 components = 0.000898658 Jy ! Clean residual min=-0.005697 max=0.005278 Jy/beam ! Clean residual mean=-0.000665 rms=0.001889 Jy/beam ! Combined flux in latest and established models = 4.04266 Jy ! Adding 35 model components to the UV plane model. ! The established model now contains 105 components and 4.04266 Jy ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec ! Estimated beam: bmin=0.6976 mas, bmaj=1.24 mas, bpa=-4.949 degrees ! Estimated noise=595.917 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.005001 Jy ! Component: 100 - total flux cleaned = -0.00547173 Jy ! Component: 150 - total flux cleaned = -0.00546398 Jy ! Component: 200 - total flux cleaned = -0.00546442 Jy ! Total flux subtracted in 200 components = -0.00546442 Jy ! Clean residual min=-0.006442 max=0.005676 Jy/beam ! Clean residual mean=-0.000129 rms=0.001608 Jy/beam ! Combined flux in latest and established models = 4.03719 Jy selfcal ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 120 components and 4.03719 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.814309Jy sigma=0.001373 ! Fit after self-cal, rms=0.814434Jy sigma=0.001366 wmodel J0854+2006_X_2010_10_13_pus_map.mod ! Writing 120 model components to file: J0854+2006_X_2010_10_13_pus_map.mod wobs J0854+2006_X_2010_10_13_pus_uvs.fits ! Writing UV FITS file: J0854+2006_X_2010_10_13_pus_uvs.fits wwins J0854+2006_X_2010_10_13_pus_map.win ! wwins: Wrote 7 windows to J0854+2006_X_2010_10_13_pus_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 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec ! clean: niter=1024 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000619491 Jy ! Component: 100 - total flux cleaned = 0.000716115 Jy ! Component: 150 - total flux cleaned = 0.000717951 Jy ! Component: 200 - total flux cleaned = 0.000716969 Jy ! Component: 250 - total flux cleaned = 0.00106311 Jy ! Component: 300 - total flux cleaned = 0.00140121 Jy ! Component: 350 - total flux cleaned = 0.0017318 Jy ! Component: 400 - total flux cleaned = 0.00173229 Jy ! Component: 450 - total flux cleaned = 0.00189241 Jy ! Component: 500 - total flux cleaned = 0.00181369 Jy ! Component: 550 - total flux cleaned = 0.00181345 Jy ! Component: 600 - total flux cleaned = 0.00173676 Jy ! Component: 650 - total flux cleaned = 0.00166171 Jy ! Component: 700 - total flux cleaned = 0.00158704 Jy ! Component: 750 - total flux cleaned = 0.00144046 Jy ! Component: 800 - total flux cleaned = 0.00136772 Jy ! Component: 850 - total flux cleaned = 0.00122432 Jy ! Component: 900 - total flux cleaned = 0.0011537 Jy ! Component: 950 - total flux cleaned = 0.00108379 Jy ! Component: 1000 - total flux cleaned = 0.000945522 Jy ! Total flux subtracted in 1024 components = 0.000945409 Jy ! Clean residual min=-0.003810 max=0.003427 Jy/beam ! Clean residual mean=-0.000166 rms=0.001300 Jy/beam ! Combined flux in latest and established models = 4.03814 Jy keep ! Adding 74 model components to the UV plane model. ! The established model now contains 188 components and 4.03814 Jy ![Exited script file: muppet] wmap "J0854+2006_X_2010_10_13_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6976 x 1.24 at -4.949 degrees (North through East) ! Clean map min=-0.0086049 max=3.3465 Jy/beam ! Writing clean map to FITS file: J0854+2006_X_2010_10_13_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 3.34652 invert ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.1611 milli-arcsec ! The y-axis pixel size should ideally be below 0.1688 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.00130283 device "J0854+2006_X_2010_10_13_pus\_map.eps/VPS" ! Attempting to open device: 'J0854+2006_X_2010_10_13_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.116793 0.116793 0.233586 0.467171 0.934343 1.86869 3.73737 7.47474 14.9495 29.899 59.7979 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0039 print "peak=",int(1000*peak_flux)/1000 ! peak= 3.346 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6976 x 1.24 at -4.949 degrees (North through East) ! Clean map min=-0.0086049 max=3.3465 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J0854+2006_X_2010_10_13_pus\_map.gif/vgif" ! Attempting to open device: 'J0854+2006_X_2010_10_13_pus_map.gif/vgif' mapplot cln