! Started logfile: /scr/pima/gb073_uvs/J0050-0929_X_uvs.log on Sat Dec 26 09:30:51 2015 obs /scr/pima/gb073_uvs/J0050-0929_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J0050-0929_X_uva.fits ! AN table 1: 24 integrations on 10 of 10 possible baselines. ! AN table 2: 10 integrations on 55 of 55 possible baselines. ! AN table 3: 6 integrations on 6 of 6 possible baselines. ! AN table 4: 12 integrations on 36 of 36 possible baselines. ! AN table 5: 6 integrations on 6 of 6 possible baselines. ! AN table 6: 7 integrations on 6 of 6 possible baselines. ! AN table 7: 12 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.740938 visibilities/baseline/integration-bin. ! Found source: J0050-0929 ! ! 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 11120 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/J0050-0929_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 24 telescope corrections were flagged in sub-array 1. ! A total of 24 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 3. ! A total of 37 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 10 telescope corrections were flagged in sub-array 6. ! A total of 34 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 2. ! A total of 24 telescope corrections were flagged in sub-array 1. ! A total of 24 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 3. ! A total of 37 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 10 telescope corrections were flagged in sub-array 6. ! A total of 34 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 3. ! A total of 24 telescope corrections were flagged in sub-array 1. ! A total of 24 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 3. ! A total of 37 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 10 telescope corrections were flagged in sub-array 6. ! A total of 34 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 4. ! A total of 24 telescope corrections were flagged in sub-array 1. ! A total of 24 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 3. ! A total of 37 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 10 telescope corrections were flagged in sub-array 6. ! A total of 34 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 5. ! A total of 24 telescope corrections were flagged in sub-array 1. ! A total of 24 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 3. ! A total of 48 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 10 telescope corrections were flagged in sub-array 6. ! A total of 46 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 6. ! A total of 24 telescope corrections were flagged in sub-array 1. ! A total of 24 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 3. ! A total of 48 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 10 telescope corrections were flagged in sub-array 6. ! A total of 46 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 7. ! A total of 24 telescope corrections were flagged in sub-array 1. ! A total of 24 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 3. ! A total of 37 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 10 telescope corrections were flagged in sub-array 6. ! A total of 34 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 8. ! A total of 24 telescope corrections were flagged in sub-array 1. ! A total of 24 telescope corrections were flagged in sub-array 2. ! A total of 6 telescope corrections were flagged in sub-array 3. ! A total of 37 telescope corrections were flagged in sub-array 4. ! A total of 6 telescope corrections were flagged in sub-array 5. ! A total of 10 telescope corrections were flagged in sub-array 6. ! A total of 34 telescope corrections were flagged in sub-array 7. ! ! Fit before self-cal, rms=1.371610Jy sigma=10.396701 ! Fit after self-cal, rms=0.253823Jy sigma=1.401885 ! 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 13% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec ! Estimated beam: bmin=0.5165 mas, bmaj=0.7388 mas, bpa=21.3 degrees ! Estimated noise=1.83938 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 = 0.694958 Jy ! Component: 100 - total flux cleaned = 0.860105 Jy ! Total flux subtracted in 100 components = 0.860105 Jy ! Clean residual min=-0.052927 max=0.068835 Jy/beam ! Clean residual mean=-0.000096 rms=0.007552 Jy/beam ! Combined flux in latest and established models = 0.860105 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 11 components and 0.860105 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=0.223356Jy sigma=1.401392 ! Fit after self-cal, rms=0.223319Jy sigma=1.401179 ! Inverting map ! Your choice of large map pixels excluded 13% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0781133 Jy ! Component: 100 - total flux cleaned = 0.121494 Jy ! Total flux subtracted in 100 components = 0.121494 Jy ! Clean residual min=-0.042451 max=0.031107 Jy/beam ! Clean residual mean=-0.000015 rms=0.005852 Jy/beam ! Combined flux in latest and established models = 0.981599 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 15 components and 0.981599 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=0.200065Jy sigma=1.117486 ! Fit after self-cal, rms=0.199912Jy sigma=1.116849 ! Inverting map ! Your choice of large map pixels excluded 13% of the data. ! The x-axis pixel size should ideally be below 0.1649 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 13% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec ! Estimated beam: bmin=0.6657 mas, bmaj=0.9599 mas, bpa=15.14 degrees ! Estimated noise=1.12182 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 = 0.0156975 Jy ! Component: 100 - total flux cleaned = 0.016173 Jy ! Component: 150 - total flux cleaned = 0.0161801 Jy ! Component: 200 - total flux cleaned = 0.0166017 Jy ! Total flux subtracted in 200 components = 0.0166017 Jy ! Clean residual min=-0.032540 max=0.021639 Jy/beam ! Clean residual mean=-0.000021 rms=0.004861 Jy/beam ! Combined flux in latest and established models = 0.998201 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 18 components and 0.998201 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=0.197767Jy sigma=1.099585 ! Fit after self-cal, rms=0.197736Jy sigma=1.099517 ! Inverting map ! Your choice of large map pixels excluded 13% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6657 x 0.9599 at 15.14 degrees (North through East) ! Clean map min=-0.02722 max=0.90969 Jy/beam if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! EF 1.00* HH 1.04 MC 0.99 ON 1.07 ! ZC 0.72 ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* FD 1.00 HH 0.97 KP 1.01 ! LA 1.10 MC 0.89 NL 0.97 ON 0.94 ! OV 1.03 PT 0.98 SC 0.97 ! ! A total of 18 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 FD 0.99 HH 0.98 KP 0.99 ! LA 1.04 MC 0.87 NL 0.94 PT 0.99 ! SC 0.92 ! ! A total of 18 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 0.00* HH 0.00* ON 0.00* ZC 0.00* ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 0.00* HH 0.00* MC 0.00* SC 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 0.97 FD 0.96 HH 0.96 KP 0.97 ! LA 1.04 MC 0.88 NL 0.91 OV 0.99 ! PT 0.96 SC 0.93 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! EF 1.00* HH 1.07 MC 1.01 ON 1.05 ! ZC 0.75 ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* FD 1.04 HH 0.99 KP 1.03 ! LA 1.08 MC 0.93 NL 1.00 ON 0.95 ! OV 1.08 PT 1.01 SC 1.00 ! ! A total of 18 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.06 FD 1.05 HH 0.96 KP 1.02 ! LA 1.07 MC 0.90 NL 0.97 PT 1.04 ! SC 0.97 ! ! A total of 18 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 0.00* HH 0.00* ON 0.00* ZC 0.00* ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 0.00* HH 0.00* MC 0.00* SC 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.03 FD 1.02 HH 0.96 KP 0.98 ! LA 1.04 MC 0.89 NL 0.94 OV 1.01 ! PT 1.01 SC 0.96 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! EF 1.00* HH 1.03 MC 1.04 ON 1.03 ! ZC 0.69 ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* FD 1.02 HH 0.96 KP 0.95 ! LA 1.03 MC 0.91 NL 0.99 ON 0.91 ! OV 1.04 PT 1.03 SC 1.02 ! ! A total of 18 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.06 FD 1.01 HH 0.96 KP 0.95 ! LA 1.00 MC 0.87 NL 0.94 PT 1.02 ! SC 0.99 ! ! A total of 18 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 0.00* HH 0.00* ON 0.00* ZC 0.00* ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 0.00* HH 0.00* MC 0.00* SC 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.02 FD 0.99 HH 0.95 KP 0.93 ! LA 0.98 MC 0.88 NL 0.91 OV 0.98 ! PT 1.00 SC 0.97 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! EF 1.00* HH 1.06 MC 1.02 ON 1.04 ! ZC 0.71 ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* FD 1.04 HH 1.01 KP 0.97 ! LA 1.03 MC 0.94 NL 1.02 ON 0.90 ! OV 1.05 PT 1.07 SC 1.04 ! ! A total of 18 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.04 FD 1.03 HH 0.95 KP 0.98 ! LA 1.02 MC 0.89 NL 0.97 PT 1.05 ! SC 0.99 ! ! A total of 18 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 0.00* HH 0.00* ON 0.00* ZC 0.00* ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 0.00* HH 0.00* MC 0.00* SC 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.02 FD 1.02 HH 1.00 KP 0.95 ! LA 1.00 MC 0.90 NL 0.93 OV 0.98 ! PT 1.00 SC 0.99 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! EF 1.00* HH 1.08 MC 1.36 ON 1.46 ! ZC 0.73 ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* FD 1.04 HH 0.96 KP 0.90 ! LA 1.03 MC 1.24 NL 1.03 ON 1.18 ! OV 1.08 PT 1.00 SC 1.05 ! ! A total of 18 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.02 HH 0.97 KP 0.89 ! LA 1.02 MC 1.12 NL 0.99 PT 1.00 ! SC 0.99 ! ! A total of 18 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 0.00* HH 0.00* ON 0.00* ZC 0.00* ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 0.00* HH 0.00* MC 0.00* SC 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* FD 1.01 HH 0.97 KP 0.87 ! LA 0.98 MC 1.12 NL 0.97 OV 1.03 ! PT 0.99 SC 0.98 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! EF 1.00* HH 1.15 MC 1.35 ON 1.51 ! ZC 0.71 ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* FD 1.01 HH 1.03 KP 0.88 ! LA 1.03 MC 1.18 NL 1.04 ON 1.20 ! OV 1.10 PT 0.96 SC 0.99 ! ! A total of 18 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.03 HH 0.99 KP 0.87 ! LA 1.01 MC 1.13 NL 0.98 PT 0.94 ! SC 0.98 ! ! A total of 18 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 0.00* HH 0.00* ON 0.00* ZC 0.00* ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 0.00* HH 0.00* MC 0.00* SC 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* FD 1.02 HH 1.00 KP 0.85 ! LA 0.98 MC 1.14 NL 0.96 OV 1.04 ! PT 0.94 SC 0.96 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! EF 1.00* HH 1.34 MC 1.51 ON 1.49 ! ZC 0.56 ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* FD 1.08 HH 1.18 KP 0.92 ! LA 1.10 MC 1.26 NL 1.06 ON 1.29 ! OV 1.05 PT 1.02 SC 1.04 ! ! A total of 18 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.04 FD 1.06 HH 1.18 KP 0.91 ! LA 1.04 MC 1.21 NL 1.02 PT 1.03 ! SC 1.00 ! ! A total of 18 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 0.00* HH 0.00* ON 0.00* ZC 0.00* ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 0.00* HH 0.00* MC 0.00* SC 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.02 FD 1.03 HH 1.24 KP 0.90 ! LA 1.02 MC 1.23 NL 0.99 OV 0.99 ! PT 1.00 SC 0.98 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! EF 1.00* HH 1.32 MC 1.51 ON 1.51 ! ZC 0.54 ! ! A total of 3 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* FD 1.05 HH 1.15 KP 0.91 ! LA 1.08 MC 1.28 NL 1.05 ON 1.31 ! OV 1.05 PT 1.03 SC 1.04 ! ! A total of 18 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.06 FD 1.03 HH 1.15 KP 0.92 ! LA 1.05 MC 1.27 NL 0.99 PT 1.02 ! SC 1.00 ! ! A total of 18 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! EF 0.00* HH 0.00* ON 0.00* ZC 0.00* ! ! A total of 18 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 0.00* HH 0.00* MC 0.00* SC 0.00* ! ! A total of 3 telescope corrections were flagged in sub-array 7. ! Telescope amplitude corrections in sub-array 7: ! BR 1.02 FD 1.02 HH 1.20 KP 0.89 ! LA 1.03 MC 1.28 NL 0.97 OV 0.98 ! PT 1.01 SC 0.99 ! ! ! Fit before self-cal, rms=0.197736Jy sigma=1.099517 ! Fit after self-cal, rms=0.156110Jy sigma=0.721028 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec ! Estimated beam: bmin=0.6794 mas, bmaj=1.054 mas, bpa=10.83 degrees ! Estimated noise=1.14282 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 = -0.00360862 Jy ! Component: 100 - total flux cleaned = -0.00392511 Jy ! Component: 150 - total flux cleaned = -0.00418259 Jy ! Component: 200 - total flux cleaned = -0.00428261 Jy ! Total flux subtracted in 200 components = -0.00428261 Jy ! Clean residual min=-0.006970 max=0.006914 Jy/beam ! Clean residual mean=0.000000 rms=0.001650 Jy/beam ! Combined flux in latest and established models = 0.993918 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 21 components and 0.993918 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=0.155813Jy sigma=0.719161 ! Fit after self-cal, rms=0.156955Jy sigma=0.718237 ! Inverting map ! Your choice of large map pixels excluded 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 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=0.156955Jy sigma=0.718237 ! Fit after self-cal, rms=0.184072Jy sigma=0.656289 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec ! Estimated beam: bmin=0.6825 mas, bmaj=1.053 mas, bpa=11.18 degrees ! Estimated noise=1.14209 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00293653 Jy ! Component: 100 - total flux cleaned = -0.00307048 Jy ! Component: 150 - total flux cleaned = -0.00326081 Jy ! Component: 200 - total flux cleaned = -0.00332926 Jy ! Total flux subtracted in 200 components = -0.00332926 Jy ! Clean residual min=-0.005005 max=0.004365 Jy/beam ! Clean residual mean=0.000005 rms=0.000882 Jy/beam ! Combined flux in latest and established models = 0.990589 Jy selfcal ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 23 components and 0.990589 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=0.183961Jy sigma=0.655245 ! Fit after self-cal, rms=0.180808Jy sigma=0.655038 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 7.70919e-05 Jy ! Component: 100 - total flux cleaned = 7.57196e-05 Jy ! Component: 150 - total flux cleaned = 7.82037e-05 Jy ! Component: 200 - total flux cleaned = 8.19837e-05 Jy ! Total flux subtracted in 200 components = 8.19837e-05 Jy ! Clean residual min=-0.004818 max=0.004259 Jy/beam ! Clean residual mean=0.000005 rms=0.000876 Jy/beam ! Combined flux in latest and established models = 0.990671 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 24 components and 0.990671 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=0.180833Jy sigma=0.655179 ! Fit after self-cal, rms=0.180765Jy sigma=0.655122 ! Inverting map ! Your choice of large map pixels excluded 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 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=0.180765Jy sigma=0.655122 ! Fit after self-cal, rms=0.180042Jy sigma=0.653935 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec ! Estimated beam: bmin=0.6855 mas, bmaj=1.054 mas, bpa=11.2 degrees ! Estimated noise=1.14253 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00242054 Jy ! Component: 100 - total flux cleaned = -0.0026271 Jy ! Component: 150 - total flux cleaned = -0.00270772 Jy ! Component: 200 - total flux cleaned = -0.00284102 Jy ! Total flux subtracted in 200 components = -0.00284102 Jy ! Clean residual min=-0.004631 max=0.004204 Jy/beam ! Clean residual mean=0.000005 rms=0.000844 Jy/beam ! Combined flux in latest and established models = 0.98783 Jy selfcal ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 24 components and 0.98783 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=0.179986Jy sigma=0.653414 ! Fit after self-cal, rms=0.180012Jy sigma=0.653343 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 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 = 1.92813e-06 Jy ! Component: 100 - total flux cleaned = -1.47932e-06 Jy ! Component: 150 - total flux cleaned = -5.87522e-05 Jy ! Component: 200 - total flux cleaned = -5.6323e-05 Jy ! Total flux subtracted in 200 components = -5.6323e-05 Jy ! Clean residual min=-0.004371 max=0.004130 Jy/beam ! Clean residual mean=0.000005 rms=0.000839 Jy/beam ! Combined flux in latest and established models = 0.987774 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 24 components and 0.987773 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=0.180038Jy sigma=0.653500 ! Fit after self-cal, rms=0.179993Jy sigma=0.653447 ! Inverting map ! Your choice of large map pixels excluded 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 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=0.179993Jy sigma=0.653447 ! Fit after self-cal, rms=0.180332Jy sigma=0.652632 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec ! Estimated beam: bmin=2.587 mas, bmaj=4.153 mas, bpa=-11.19 degrees ! Estimated noise=1.33685 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00204941 Jy ! Component: 100 - total flux cleaned = -0.00222444 Jy ! Component: 150 - total flux cleaned = -0.00224696 Jy ! Component: 200 - total flux cleaned = -0.0022681 Jy ! Total flux subtracted in 200 components = -0.0022681 Jy ! Clean residual min=-0.003289 max=0.003613 Jy/beam ! Clean residual mean=0.000010 rms=0.000876 Jy/beam ! Combined flux in latest and established models = 0.985505 Jy selfcal ! Performing phase self-cal ! Adding 3 model components to the UV plane model. ! The established model now contains 25 components and 0.985505 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=0.180345Jy sigma=0.652585 ! Fit after self-cal, rms=0.180357Jy sigma=0.652527 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 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 = -0.00017645 Jy ! Component: 100 - total flux cleaned = -0.000178864 Jy ! Component: 150 - total flux cleaned = -0.000180223 Jy ! Component: 200 - total flux cleaned = -0.000181179 Jy ! Total flux subtracted in 200 components = -0.000181179 Jy ! Clean residual min=-0.003340 max=0.003615 Jy/beam ! Clean residual mean=0.000009 rms=0.000877 Jy/beam ! Combined flux in latest and established models = 0.985324 Jy ! Performing phase self-cal ! Adding 3 model components to the UV plane model. ! The established model now contains 25 components and 0.985324 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=0.180381Jy sigma=0.652521 ! Fit after self-cal, rms=0.180376Jy sigma=0.652480 ! Inverting map ! Your choice of large map pixels excluded 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 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 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec ! Estimated beam: bmin=0.688 mas, bmaj=1.056 mas, bpa=11.18 degrees ! Estimated noise=1.14303 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.688 x 1.056 at 11.18 degrees (North through East) ! Clean map min=-0.003261 max=0.91277 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. ! ! Correcting IF 5. ! ! Correcting IF 6. ! ! Correcting IF 7. ! ! Correcting IF 8. ! ! Fit before self-cal, rms=0.180376Jy sigma=0.652480 ! Fit after self-cal, rms=0.674182Jy sigma=0.599236 ! Inverting map and beam ! Your choice of large map pixels excluded 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec ! Estimated beam: bmin=0.689 mas, bmaj=1.057 mas, bpa=11.29 degrees ! Estimated noise=1.14215 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0019632 Jy ! Component: 100 - total flux cleaned = -0.00212826 Jy ! Component: 150 - total flux cleaned = -0.00227051 Jy ! Component: 200 - total flux cleaned = -0.00239815 Jy ! Total flux subtracted in 200 components = -0.00239815 Jy ! Clean residual min=-0.003996 max=0.003966 Jy/beam ! Clean residual mean=0.000005 rms=0.000800 Jy/beam ! Combined flux in latest and established models = 0.982926 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 26 components and 0.982926 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=0.674167Jy sigma=0.598934 ! Fit after self-cal, rms=0.674576Jy sigma=0.598872 ! Inverting map ! Your choice of large map pixels excluded 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 2.7454e-07 Jy ! Component: 100 - total flux cleaned = -6.02099e-05 Jy ! Component: 150 - total flux cleaned = -0.000115833 Jy ! Component: 200 - total flux cleaned = -0.000111018 Jy ! Total flux subtracted in 200 components = -0.000111018 Jy ! Clean residual min=-0.003855 max=0.003978 Jy/beam ! Clean residual mean=0.000005 rms=0.000796 Jy/beam ! Combined flux in latest and established models = 0.982815 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 26 components and 0.982815 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=0.674591Jy sigma=0.598956 ! Fit after self-cal, rms=0.674736Jy sigma=0.598925 ! Inverting map ! Your choice of large map pixels excluded 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec ! Added new window around map position (-2, -14.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00219892 Jy ! Component: 100 - total flux cleaned = 0.00238364 Jy ! Component: 150 - total flux cleaned = 0.00224208 Jy ! Component: 200 - total flux cleaned = 0.00230349 Jy ! Total flux subtracted in 200 components = 0.00230349 Jy ! Clean residual min=-0.003483 max=0.003357 Jy/beam ! Clean residual mean=0.000006 rms=0.000785 Jy/beam ! Combined flux in latest and established models = 0.985119 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 36 components and 0.985119 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=0.674707Jy sigma=0.598024 ! Fit after self-cal, rms=0.674464Jy sigma=0.597914 ! Inverting map ! Your choice of large map pixels excluded 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec ! Performing amp+phase self-cal ! ! 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=0.674464Jy sigma=0.597914 ! Fit after self-cal, rms=0.688416Jy sigma=0.597205 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 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec ! Estimated beam: bmin=0.5307 mas, bmaj=0.7807 mas, bpa=18.29 degrees ! Estimated noise=1.91326 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.698187 Jy ! Component: 100 - total flux cleaned = 0.857506 Jy ! Component: 150 - total flux cleaned = 0.918769 Jy ! Component: 200 - total flux cleaned = 0.949421 Jy ! Total flux subtracted in 200 components = 0.949421 Jy ! Clean residual min=-0.008328 max=0.015113 Jy/beam ! Clean residual mean=-0.000022 rms=0.001641 Jy/beam ! Combined flux in latest and established models = 0.949421 Jy uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Adding 12 model components to the UV plane model. ! The established model now contains 12 components and 0.949421 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec ! Estimated beam: bmin=0.6908 mas, bmaj=1.059 mas, bpa=11.22 degrees ! Estimated noise=1.14249 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 = 0.0204753 Jy ! Component: 100 - total flux cleaned = 0.0287834 Jy ! Component: 150 - total flux cleaned = 0.0325754 Jy ! Component: 200 - total flux cleaned = 0.033753 Jy ! Total flux subtracted in 200 components = 0.033753 Jy ! Clean residual min=-0.003787 max=0.003914 Jy/beam ! Clean residual mean=0.000004 rms=0.000792 Jy/beam ! Combined flux in latest and established models = 0.983174 Jy ! Adding 16 model components to the UV plane model. ! The established model now contains 20 components and 0.983174 Jy ! Inverting map ! Your choice of large map pixels excluded 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec ! Added new window around map position (-1.2, 4.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00257759 Jy ! Component: 100 - total flux cleaned = 0.00291241 Jy ! Component: 150 - total flux cleaned = 0.00320258 Jy ! Component: 200 - total flux cleaned = 0.00326973 Jy ! Total flux subtracted in 200 components = 0.00326973 Jy ! Clean residual min=-0.003709 max=0.003225 Jy/beam ! Clean residual mean=0.000009 rms=0.000743 Jy/beam ! Combined flux in latest and established models = 0.986443 Jy ! Adding 21 model components to the UV plane model. ! The established model now contains 37 components and 0.986444 Jy ! Inverting map ! Your choice of large map pixels excluded 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 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 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec ! Estimated beam: bmin=2.588 mas, bmaj=4.153 mas, bpa=-11.18 degrees ! Estimated noise=1.33204 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 5.75559e-05 Jy ! Component: 100 - total flux cleaned = 0.00011657 Jy ! Component: 150 - total flux cleaned = 0.000195375 Jy ! Component: 200 - total flux cleaned = 0.000218604 Jy ! Total flux subtracted in 200 components = 0.000218604 Jy ! Clean residual min=-0.002795 max=0.002966 Jy/beam ! Clean residual mean=0.000019 rms=0.000781 Jy/beam ! Combined flux in latest and established models = 0.986662 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 = -2.05606e-05 Jy ! Component: 100 - total flux cleaned = -2.04599e-05 Jy ! Component: 150 - total flux cleaned = -2.0165e-05 Jy ! Component: 200 - total flux cleaned = -2.37858e-06 Jy ! Total flux subtracted in 200 components = -2.37858e-06 Jy ! Clean residual min=-0.002834 max=0.002906 Jy/beam ! Clean residual mean=0.000019 rms=0.000777 Jy/beam ! Combined flux in latest and established models = 0.98666 Jy ! Adding 14 model components to the UV plane model. ! The established model now contains 50 components and 0.98666 Jy ! Inverting map ! Your choice of large map pixels excluded 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec ! Estimated beam: bmin=0.6908 mas, bmaj=1.059 mas, bpa=11.22 degrees ! Estimated noise=1.14249 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000461266 Jy ! Component: 100 - total flux cleaned = 0.000397963 Jy ! Component: 150 - total flux cleaned = 0.00039674 Jy ! Component: 200 - total flux cleaned = 0.000397112 Jy ! Total flux subtracted in 200 components = 0.000397112 Jy ! Clean residual min=-0.003537 max=0.003248 Jy/beam ! Clean residual mean=0.000010 rms=0.000737 Jy/beam ! Combined flux in latest and established models = 0.987057 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 58 components and 0.987057 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=0.688422Jy sigma=0.597732 ! Fit after self-cal, rms=0.691035Jy sigma=0.596383 wmodel /scr/pima/gb073_uvs/J0050-0929_X_map.mod ! Writing 58 model components to file: /scr/pima/gb073_uvs/J0050-0929_X_map.mod wobs /scr/pima/gb073_uvs/J0050-0929_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J0050-0929_X_uvs.fits wwins /scr/pima/gb073_uvs/J0050-0929_X_map.win ! wwins: Wrote 3 windows to /scr/pima/gb073_uvs/J0050-0929_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 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.00156731 Jy ! Component: 100 - total flux cleaned = -0.00227434 Jy ! Component: 150 - total flux cleaned = -0.00271682 Jy ! Component: 200 - total flux cleaned = -0.00308479 Jy ! Component: 250 - total flux cleaned = -0.00344216 Jy ! Component: 300 - total flux cleaned = -0.00364296 Jy ! Component: 350 - total flux cleaned = -0.00422737 Jy ! Component: 400 - total flux cleaned = -0.00465686 Jy ! Component: 450 - total flux cleaned = -0.00498363 Jy ! Component: 500 - total flux cleaned = -0.00512131 Jy ! Component: 550 - total flux cleaned = -0.00516712 Jy ! Component: 600 - total flux cleaned = -0.0053011 Jy ! Component: 650 - total flux cleaned = -0.00547777 Jy ! Component: 700 - total flux cleaned = -0.00552112 Jy ! Component: 750 - total flux cleaned = -0.00565067 Jy ! Component: 800 - total flux cleaned = -0.00590606 Jy ! Component: 850 - total flux cleaned = -0.00603216 Jy ! Component: 900 - total flux cleaned = -0.00615665 Jy ! Component: 950 - total flux cleaned = -0.00628076 Jy ! Component: 1000 - total flux cleaned = -0.00640355 Jy ! Component: 1050 - total flux cleaned = -0.00668654 Jy ! Component: 1100 - total flux cleaned = -0.00688656 Jy ! Component: 1150 - total flux cleaned = -0.00704572 Jy ! Component: 1200 - total flux cleaned = -0.00716372 Jy ! Component: 1250 - total flux cleaned = -0.00728146 Jy ! Component: 1300 - total flux cleaned = -0.00751403 Jy ! Component: 1350 - total flux cleaned = -0.00778301 Jy ! Component: 1400 - total flux cleaned = -0.00770663 Jy ! Component: 1450 - total flux cleaned = -0.00797208 Jy ! Component: 1500 - total flux cleaned = -0.0082359 Jy ! Component: 1550 - total flux cleaned = -0.00819866 Jy ! Component: 1600 - total flux cleaned = -0.00853274 Jy ! Component: 1650 - total flux cleaned = -0.00882686 Jy ! Component: 1700 - total flux cleaned = -0.0089728 Jy ! Component: 1750 - total flux cleaned = -0.00919107 Jy ! Component: 1800 - total flux cleaned = -0.00940749 Jy ! Component: 1850 - total flux cleaned = -0.00955057 Jy ! Component: 1900 - total flux cleaned = -0.00976374 Jy ! Component: 1950 - total flux cleaned = -0.00983485 Jy ! Component: 2000 - total flux cleaned = -0.0101167 Jy ! Component: 2050 - total flux cleaned = -0.0103265 Jy ! Component: 2100 - total flux cleaned = -0.0105696 Jy ! Component: 2150 - total flux cleaned = -0.0106733 Jy ! Component: 2200 - total flux cleaned = -0.0109134 Jy ! Component: 2250 - total flux cleaned = -0.0111519 Jy ! Component: 2300 - total flux cleaned = -0.0112877 Jy ! Component: 2350 - total flux cleaned = -0.0116582 Jy ! Component: 2400 - total flux cleaned = -0.0117921 Jy ! Component: 2450 - total flux cleaned = -0.0120585 Jy ! Component: 2500 - total flux cleaned = -0.0120582 Jy ! Component: 2550 - total flux cleaned = -0.0122559 Jy ! Component: 2600 - total flux cleaned = -0.0125505 Jy ! Component: 2650 - total flux cleaned = -0.0125832 Jy ! Component: 2700 - total flux cleaned = -0.0129391 Jy ! Component: 2750 - total flux cleaned = -0.0130999 Jy ! Component: 2800 - total flux cleaned = -0.0133241 Jy ! Component: 2850 - total flux cleaned = -0.0136106 Jy ! Component: 2900 - total flux cleaned = -0.0135787 Jy ! Component: 2950 - total flux cleaned = -0.013768 Jy ! Component: 3000 - total flux cleaned = -0.0140817 Jy ! Component: 3050 - total flux cleaned = -0.0141756 Jy ! Component: 3100 - total flux cleaned = -0.0143309 Jy ! Component: 3150 - total flux cleaned = -0.0145472 Jy ! Component: 3200 - total flux cleaned = -0.014793 Jy ! Component: 3250 - total flux cleaned = -0.0150071 Jy ! Component: 3300 - total flux cleaned = -0.0151896 Jy ! Component: 3350 - total flux cleaned = -0.0153109 Jy ! Component: 3400 - total flux cleaned = -0.0154315 Jy ! Component: 3450 - total flux cleaned = -0.0157012 Jy ! Component: 3500 - total flux cleaned = -0.0159098 Jy ! Component: 3550 - total flux cleaned = -0.0162065 Jy ! Component: 3600 - total flux cleaned = -0.0162952 Jy ! Component: 3650 - total flux cleaned = -0.0164715 Jy ! Component: 3700 - total flux cleaned = -0.0165596 Jy ! Component: 3750 - total flux cleaned = -0.0167049 Jy ! Component: 3800 - total flux cleaned = -0.0169076 Jy ! Component: 3850 - total flux cleaned = -0.0170228 Jy ! Component: 3900 - total flux cleaned = -0.0172526 Jy ! Component: 3950 - total flux cleaned = -0.017424 Jy ! Component: 4000 - total flux cleaned = -0.0174809 Jy ! Component: 4050 - total flux cleaned = -0.0177076 Jy ! Total flux subtracted in 4096 components = -0.0178487 Jy ! Clean residual min=-0.001540 max=0.001769 Jy/beam ! Clean residual mean=0.000001 rms=0.000461 Jy/beam ! Combined flux in latest and established models = 0.969208 Jy keep ! Adding 299 model components to the UV plane model. ! The established model now contains 357 components and 0.969208 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J0050-0929_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6908 x 1.059 at 11.22 degrees (North through East) ! Clean map min=-0.0028663 max=0.90913 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J0050-0929_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.909131 invert ! Inverting map ! Your choice of large map pixels excluded 13.4% of the data. ! The x-axis pixel size should ideally be below 0.1649 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000460005 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.151795 0.151795 0.30359 0.607179 1.21436 2.42872 4.85743 9.71487 19.4297 38.8595 77.7189 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0013 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.909 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 1976.35 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J0050-0929_X_uvs.log closed on Sat Dec 26 09:30:56 2015