! Started logfile: /scr/pima/gb073_uvs/J1055+0205_X_uvs.log on Sat Dec 26 09:36:39 2015 obs /scr/pima/gb073_uvs/J1055+0205_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1055+0205_X_uva.fits ! AN table 1: 25 integrations on 28 of 28 possible baselines. ! AN table 2: 145 integrations on 10 of 10 possible baselines. ! AN table 3: 29 integrations on 55 of 55 possible baselines. ! AN table 4: 29 integrations on 55 of 55 possible baselines. ! AN table 5: 29 integrations on 15 of 15 possible baselines. ! AN table 6: 21 integrations on 28 of 28 possible baselines. ! AN table 7: 29 integrations on 66 of 66 possible baselines. ! Apparent sampling: 0.841851 visibilities/baseline/integration-bin. ! Found source: J1055+0205 ! ! 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 55744 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/J1055+0205_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 2 telescope corrections were flagged in sub-array 1. ! A total of 180 telescope corrections were flagged in sub-array 2. ! A total of 36 telescope corrections were flagged in sub-array 3. ! A total of 46 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 30 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 2. ! A total of 2 telescope corrections were flagged in sub-array 1. ! A total of 180 telescope corrections were flagged in sub-array 2. ! A total of 36 telescope corrections were flagged in sub-array 3. ! A total of 46 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 30 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 3. ! A total of 2 telescope corrections were flagged in sub-array 1. ! A total of 180 telescope corrections were flagged in sub-array 2. ! A total of 36 telescope corrections were flagged in sub-array 3. ! A total of 46 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 30 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 4. ! A total of 2 telescope corrections were flagged in sub-array 1. ! A total of 180 telescope corrections were flagged in sub-array 2. ! A total of 36 telescope corrections were flagged in sub-array 3. ! A total of 46 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 30 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 5. ! A total of 27 telescope corrections were flagged in sub-array 1. ! A total of 180 telescope corrections were flagged in sub-array 2. ! A total of 36 telescope corrections were flagged in sub-array 3. ! A total of 75 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 21 telescope corrections were flagged in sub-array 6. ! A total of 59 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 6. ! A total of 27 telescope corrections were flagged in sub-array 1. ! A total of 180 telescope corrections were flagged in sub-array 2. ! A total of 36 telescope corrections were flagged in sub-array 3. ! A total of 75 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 21 telescope corrections were flagged in sub-array 6. ! A total of 59 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 7. ! A total of 2 telescope corrections were flagged in sub-array 1. ! A total of 180 telescope corrections were flagged in sub-array 2. ! A total of 36 telescope corrections were flagged in sub-array 3. ! A total of 46 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 30 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 8. ! A total of 2 telescope corrections were flagged in sub-array 1. ! A total of 180 telescope corrections were flagged in sub-array 2. ! A total of 36 telescope corrections were flagged in sub-array 3. ! A total of 46 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 30 telescope corrections were flagged in sub-array 7. ! ! Fit before self-cal, rms=1.009879Jy sigma=8.386814 ! Fit after self-cal, rms=0.917638Jy sigma=7.626472 ! 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 7.09% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=0.5451 mas, bmaj=0.8435 mas, bpa=-5.424 degrees ! Estimated noise=0.762357 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 = 0.0672009 Jy ! Component: 100 - total flux cleaned = 0.0831811 Jy ! Total flux subtracted in 100 components = 0.0831811 Jy ! Clean residual min=-0.003693 max=0.006439 Jy/beam ! Clean residual mean=-0.000001 rms=0.000703 Jy/beam ! Combined flux in latest and established models = 0.0831811 Jy ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 4 components and 0.0831811 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=0.106156Jy sigma=0.667179 ! Fit after self-cal, rms=0.105527Jy sigma=0.662344 ! Inverting map ! Your choice of large map pixels excluded 7.09% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00683058 Jy ! Component: 100 - total flux cleaned = 0.00966131 Jy ! Total flux subtracted in 100 components = 0.00966131 Jy ! Clean residual min=-0.003308 max=0.003567 Jy/beam ! Clean residual mean=-0.000000 rms=0.000657 Jy/beam ! Combined flux in latest and established models = 0.0928424 Jy ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 6 components and 0.0928424 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=0.104980Jy sigma=0.659053 ! Fit after self-cal, rms=0.104943Jy sigma=0.658873 ! Inverting map ! Your choice of large map pixels excluded 7.09% of the data. ! The x-axis pixel size should ideally be below 0.165 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 7.09% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=0.6601 mas, bmaj=1.017 mas, bpa=-4.848 degrees ! Estimated noise=0.414274 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 (-6.2, -1.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00370665 Jy ! Component: 100 - total flux cleaned = 0.00519893 Jy ! Component: 150 - total flux cleaned = 0.00566219 Jy ! Component: 200 - total flux cleaned = 0.00599847 Jy ! Total flux subtracted in 200 components = 0.00599847 Jy ! Clean residual min=-0.002257 max=0.002469 Jy/beam ! Clean residual mean=-0.000002 rms=0.000429 Jy/beam ! Combined flux in latest and established models = 0.0988409 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 23 components and 0.0988409 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=0.104793Jy sigma=0.657565 ! Fit after self-cal, rms=0.104765Jy sigma=0.657345 ! Inverting map ! Your choice of large map pixels excluded 7.09% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! Added new window around map position (0.2, -7). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00243327 Jy ! Component: 100 - total flux cleaned = 0.00299655 Jy ! Component: 150 - total flux cleaned = 0.00336643 Jy ! Component: 200 - total flux cleaned = 0.00355399 Jy ! Total flux subtracted in 200 components = 0.00355399 Jy ! Clean residual min=-0.002098 max=0.002229 Jy/beam ! Clean residual mean=-0.000002 rms=0.000410 Jy/beam ! Combined flux in latest and established models = 0.102395 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 35 components and 0.102395 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=0.104655Jy sigma=0.656806 ! Fit after self-cal, rms=0.104643Jy sigma=0.656738 ! Inverting map ! Your choice of large map pixels excluded 7.09% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! Added new window around map position (-3.6, -0.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00223791 Jy ! Component: 100 - total flux cleaned = 0.00261763 Jy ! Component: 150 - total flux cleaned = 0.00271017 Jy ! Component: 200 - total flux cleaned = 0.00275305 Jy ! Total flux subtracted in 200 components = 0.00275305 Jy ! Clean residual min=-0.002023 max=0.001911 Jy/beam ! Clean residual mean=-0.000001 rms=0.000400 Jy/beam ! Combined flux in latest and established models = 0.105148 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 50 components and 0.105148 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=0.104567Jy sigma=0.656197 ! Fit after self-cal, rms=0.104561Jy sigma=0.656057 ! Inverting map ! Your choice of large map pixels excluded 7.09% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6601 x 1.017 at -4.848 degrees (North through East) ! Clean map min=-0.0016547 max=0.086787 Jy/beam if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 1.07 KP 1.04 LA 1.01 ! MK 1.03 NL 0.92 OV 0.99 PT 0.95 ! ! A total of 105 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.00 MC 0.92 ON 0.84 ! ZC 0.83 ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* FD 0.95 HH 0.99 KP 1.01 ! LA 1.03 MC 0.97 NL 0.95 ON 0.94 ! PT 0.96 SC 0.90 ZC 0.78 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 EF 1.00* FD 0.91 KP 0.99 ! LA 1.13 MC 0.86 NL 0.94 ON 1.02 ! OV 1.03 PT 0.98 SC 0.96 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 0.96 MC 0.90 ON 0.93 ! SC 0.97 ZC 0.93 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.02 FD 0.95 KP 1.02 LA 1.08 ! MK 0.98 NL 0.94 PT 0.93 SC 1.00 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00 EF 1.00* FD 1.03 HH 1.04 ! KP 0.97 LA 1.18 MC 0.99 NL 0.93 ! ON 0.83 OV 0.99 PT 0.96 SC 0.98 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.97 FD 1.03 KP 1.02 LA 1.07 ! MK 1.12 NL 1.02 OV 1.04 PT 0.98 ! ! A total of 105 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.01 MC 0.94 ON 0.79 ! ZC 0.88 ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* FD 0.93 HH 0.95 KP 1.11 ! LA 1.14 MC 1.00 NL 1.06 ON 1.12 ! PT 1.04 SC 0.84 ZC 0.85 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.07 EF 1.00* FD 1.02 KP 1.01 ! LA 1.05 MC 0.87 NL 1.03 ON 0.97 ! OV 0.98 PT 1.10 SC 1.04 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 1.08 MC 1.09 ON 0.97 ! SC 0.83 ZC 0.83 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.08 FD 1.01 KP 1.05 LA 1.00 ! MK 1.00 NL 1.03 PT 1.03 SC 1.00 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.08 EF 1.00* FD 1.02 HH 0.84 ! KP 1.02 LA 1.16 MC 1.07 NL 1.01 ! ON 0.87 OV 1.08 PT 1.01 SC 1.07 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.92 FD 0.98 KP 0.98 LA 0.94 ! MK 1.05 NL 1.00 OV 1.05 PT 1.01 ! ! A total of 105 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 0.96 MC 0.87 ON 0.87 ! ZC 0.81 ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* FD 1.11 HH 0.87 KP 0.87 ! LA 1.08 MC 1.07 NL 1.04 ON 0.97 ! PT 1.01 SC 0.87 ZC 0.89 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.14 EF 1.00* FD 1.03 KP 1.00 ! LA 0.97 MC 1.05 NL 0.96 ON 0.95 ! OV 0.95 PT 1.01 SC 1.05 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 0.98 MC 0.95 ON 0.85 ! SC 0.88 ZC 0.85 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.01 FD 1.02 KP 0.98 LA 1.00 ! MK 0.92 NL 0.98 PT 1.02 SC 1.04 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.13 EF 1.00* FD 0.95 HH 0.85 ! KP 0.99 LA 1.04 MC 1.08 NL 0.91 ! ON 1.02 OV 1.03 PT 1.06 SC 1.07 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 1.04 KP 1.02 LA 1.03 ! MK 0.94 NL 0.95 OV 1.09 PT 1.05 ! ! A total of 105 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.05 MC 0.91 ON 0.85 ! ZC 0.80 ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* FD 1.01 HH 1.04 KP 0.97 ! LA 1.07 MC 0.94 NL 1.01 ON 0.95 ! PT 1.12 SC 1.02 ZC 0.77 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.09 EF 1.00* FD 1.04 KP 0.99 ! LA 1.05 MC 0.96 NL 0.94 ON 0.87 ! OV 0.91 PT 1.05 SC 1.03 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 0.94 MC 0.98 ON 0.94 ! SC 0.89 ZC 0.88 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00 FD 1.05 KP 1.07 LA 0.99 ! MK 1.02 NL 1.00 PT 0.99 SC 0.94 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.03 EF 1.00* FD 1.03 HH 0.88 ! KP 1.04 LA 1.05 MC 0.90 NL 1.02 ! ON 0.96 OV 1.02 PT 1.02 SC 1.12 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.05 KP 0.91 LA 0.90 ! MK 1.05 NL 1.02 OV 1.14 PT 1.00 ! ! A total of 105 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.02 MC 1.12 ON 1.08 ! ZC 0.77 ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* FD 0.99 HH 1.02 KP 0.87 ! LA 1.06 MC 1.41 NL 1.10 ON 1.19 ! PT 0.97 SC 0.98 ZC 0.72 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 0.99 KP 0.99 ! LA 0.94 MC 1.12 NL 1.08 ON 1.14 ! OV 0.99 PT 0.96 SC 1.01 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 0.99 MC 1.33 ON 1.15 ! SC 0.85 ZC 0.81 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* FD 1.00 KP 0.89 LA 0.98 ! MK 1.07 NL 1.03 PT 1.00 SC 1.00 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* EF 1.00* FD 0.97 HH 0.89 ! KP 0.94 LA 1.05 MC 1.29 NL 0.99 ! ON 1.17 OV 1.06 PT 0.99 SC 1.10 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.94 KP 0.84 LA 1.04 ! MK 0.95 NL 1.02 OV 1.14 PT 0.86 ! ! A total of 105 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 0.92 MC 1.17 ON 0.99 ! ZC 0.89 ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* FD 0.96 HH 0.97 KP 0.86 ! LA 1.04 MC 1.13 NL 1.08 ON 1.10 ! PT 1.03 SC 1.00 ZC 0.79 ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 0.96 KP 0.86 ! LA 1.08 MC 1.10 NL 1.04 ON 1.30 ! OV 1.00 PT 0.93 SC 1.01 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 1.00 MC 1.25 ON 1.04 ! SC 0.92 ZC 0.82 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* FD 0.99 KP 0.94 LA 0.96 ! MK 0.99 NL 0.91 PT 0.91 SC 0.94 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* EF 1.00* FD 1.03 HH 1.02 ! KP 0.95 LA 1.16 MC 1.25 NL 0.95 ! ON 1.06 OV 0.94 PT 1.01 SC 0.97 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 1.06 KP 0.87 LA 1.05 ! MK 1.09 NL 1.00 OV 1.04 PT 1.00 ! ! A total of 105 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.04 MC 1.08 ON 1.02 ! ZC 0.72 ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* FD 1.11 HH 1.11 KP 0.94 ! LA 1.09 MC 1.22 NL 1.03 ON 1.34 ! PT 0.99 SC 1.02 ZC 0.61 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.03 EF 1.00* FD 1.02 KP 0.94 ! LA 0.97 MC 1.25 NL 0.96 ON 1.21 ! OV 1.05 PT 0.95 SC 0.96 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 1.14 MC 1.01 ON 0.94 ! SC 0.90 ZC 0.80 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.04 FD 1.06 KP 0.85 LA 1.09 ! MK 1.09 NL 1.00 PT 1.03 SC 0.96 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.01 EF 1.00* FD 1.08 HH 1.09 ! KP 0.88 LA 1.17 MC 1.19 NL 0.94 ! ON 1.18 OV 1.06 PT 0.97 SC 1.07 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 1.14 FD 1.05 KP 0.87 LA 0.95 ! MK 1.09 NL 0.99 OV 1.01 PT 1.08 ! ! A total of 105 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.01 MC 1.04 ON 0.99 ! ZC 0.74 ! ! Telescope amplitude corrections in sub-array 3: ! EF 1.00* FD 0.99 HH 0.96 KP 0.92 ! LA 1.11 MC 1.50 NL 1.09 ON 1.21 ! PT 0.95 SC 0.91 ZC 0.58 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 EF 1.00* FD 1.00 KP 0.92 ! LA 1.01 MC 1.19 NL 1.08 ON 1.05 ! OV 0.96 PT 0.99 SC 1.02 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* HH 0.94 MC 1.07 ON 1.31 ! SC 0.91 ZC 0.79 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.95 FD 1.16 KP 1.01 LA 1.09 ! MK 0.97 NL 1.01 PT 0.95 SC 0.99 ! ! Telescope amplitude corrections in sub-array 7: ! BR 0.99 EF 1.00* FD 1.03 HH 1.03 ! KP 0.90 LA 1.08 MC 1.10 NL 1.10 ! ON 1.21 OV 1.01 PT 1.11 SC 1.05 ! ! ! Fit before self-cal, rms=0.104561Jy sigma=0.656057 ! Fit after self-cal, rms=0.100954Jy sigma=0.652321 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 0.165 milli-arcsec ! Estimated beam: bmin=0.6641 mas, bmaj=1.033 mas, bpa=-4.868 degrees ! Estimated noise=0.41675 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 = 0.000411511 Jy ! Component: 100 - total flux cleaned = 0.000374605 Jy ! Component: 150 - total flux cleaned = 0.000452992 Jy ! Component: 200 - total flux cleaned = 0.0005217 Jy ! Total flux subtracted in 200 components = 0.0005217 Jy ! Clean residual min=-0.001149 max=0.001287 Jy/beam ! Clean residual mean=-0.000000 rms=0.000281 Jy/beam ! Combined flux in latest and established models = 0.10567 Jy ! Performing phase self-cal ! Adding 24 model components to the UV plane model. ! The established model now contains 70 components and 0.10567 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=0.100939Jy sigma=0.652092 ! Fit after self-cal, rms=0.101090Jy sigma=0.651587 ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.165 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=0.101090Jy sigma=0.651587 ! Fit after self-cal, rms=0.100401Jy sigma=0.650992 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 0.165 milli-arcsec ! Estimated beam: bmin=0.6648 mas, bmaj=1.038 mas, bpa=-4.906 degrees ! Estimated noise=0.417396 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000438816 Jy ! Component: 100 - total flux cleaned = 0.000536114 Jy ! Component: 150 - total flux cleaned = 0.000578202 Jy ! Component: 200 - total flux cleaned = 0.000596717 Jy ! Total flux subtracted in 200 components = 0.000596717 Jy ! Clean residual min=-0.001186 max=0.001270 Jy/beam ! Clean residual mean=-0.000000 rms=0.000272 Jy/beam ! Combined flux in latest and established models = 0.106266 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 72 components and 0.106266 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=0.100391Jy sigma=0.650876 ! Fit after self-cal, rms=0.100473Jy sigma=0.650768 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 0.165 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 (-24.8, 24.6). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000706372 Jy ! Component: 100 - total flux cleaned = 0.000632529 Jy ! Component: 150 - total flux cleaned = 0.000652768 Jy ! Component: 200 - total flux cleaned = 0.000671519 Jy ! Total flux subtracted in 200 components = 0.000671519 Jy ! Clean residual min=-0.001158 max=0.001157 Jy/beam ! Clean residual mean=-0.000000 rms=0.000269 Jy/beam ! Combined flux in latest and established models = 0.106938 Jy ! Performing phase self-cal ! Adding 18 model components to the UV plane model. ! The established model now contains 79 components and 0.106938 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=0.100456Jy sigma=0.650680 ! Fit after self-cal, rms=0.100457Jy sigma=0.650665 ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.165 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=0.100457Jy sigma=0.650665 ! Fit after self-cal, rms=0.099023Jy sigma=0.650285 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 0.165 milli-arcsec ! Estimated beam: bmin=0.6664 mas, bmaj=1.037 mas, bpa=-4.952 degrees ! Estimated noise=0.416956 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 6.62604e-05 Jy ! Component: 100 - total flux cleaned = 6.60785e-05 Jy ! Component: 150 - total flux cleaned = 2.39204e-05 Jy ! Component: 200 - total flux cleaned = 5.35422e-06 Jy ! Total flux subtracted in 200 components = 5.35422e-06 Jy ! Clean residual min=-0.001171 max=0.001052 Jy/beam ! Clean residual mean=-0.000000 rms=0.000258 Jy/beam ! Combined flux in latest and established models = 0.106943 Jy selfcal ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 86 components and 0.106943 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=0.099014Jy sigma=0.650207 ! Fit after self-cal, rms=0.099062Jy sigma=0.650146 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 0.165 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 = 6.83825e-05 Jy ! Component: 100 - total flux cleaned = 8.67861e-05 Jy ! Component: 150 - total flux cleaned = 0.000103083 Jy ! Component: 200 - total flux cleaned = 0.000102945 Jy ! Total flux subtracted in 200 components = 0.000102945 Jy ! Clean residual min=-0.001195 max=0.001078 Jy/beam ! Clean residual mean=-0.000000 rms=0.000257 Jy/beam ! Combined flux in latest and established models = 0.107046 Jy ! Performing phase self-cal ! Adding 26 model components to the UV plane model. ! The established model now contains 89 components and 0.107046 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=0.099055Jy sigma=0.650101 ! Fit after self-cal, rms=0.099056Jy sigma=0.650100 ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.165 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=0.099056Jy sigma=0.650100 ! Fit after self-cal, rms=0.099413Jy sigma=0.650070 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 0.165 milli-arcsec ! Estimated beam: bmin=2.581 mas, bmaj=3.359 mas, bpa=-0.7725 degrees ! Estimated noise=0.518929 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 6.95222e-05 Jy ! Component: 100 - total flux cleaned = -4.52751e-05 Jy ! Component: 150 - total flux cleaned = -0.000118927 Jy ! Component: 200 - total flux cleaned = -0.000162021 Jy ! Total flux subtracted in 200 components = -0.000162021 Jy ! Clean residual min=-0.001284 max=0.001003 Jy/beam ! Clean residual mean=-0.000001 rms=0.000305 Jy/beam ! Combined flux in latest and established models = 0.106884 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 97 components and 0.106884 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=0.099413Jy sigma=0.650056 ! Fit after self-cal, rms=0.099445Jy sigma=0.650016 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 0.165 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 = 3.23277e-06 Jy ! Component: 100 - total flux cleaned = -6.77071e-05 Jy ! Component: 150 - total flux cleaned = -0.000121604 Jy ! Component: 200 - total flux cleaned = -0.000170529 Jy ! Total flux subtracted in 200 components = -0.000170529 Jy ! Clean residual min=-0.001270 max=0.001015 Jy/beam ! Clean residual mean=-0.000001 rms=0.000302 Jy/beam ! Combined flux in latest and established models = 0.106714 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 100 components and 0.106714 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=0.099446Jy sigma=0.650012 ! Fit after self-cal, rms=0.099445Jy sigma=0.650010 ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.165 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 0.165 milli-arcsec ! Estimated beam: bmin=0.6676 mas, bmaj=1.037 mas, bpa=-4.943 degrees ! Estimated noise=0.416934 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6676 x 1.037 at -4.943 degrees (North through East) ! Clean map min=-0.00099029 max=0.08628 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 7.21% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! Estimated beam: bmin=0.5522 mas, bmaj=0.8273 mas, bpa=-5.655 degrees ! Estimated noise=0.773491 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0674304 Jy ! Component: 100 - total flux cleaned = 0.083052 Jy ! Component: 150 - total flux cleaned = 0.0893283 Jy ! Component: 200 - total flux cleaned = 0.0934156 Jy ! Total flux subtracted in 200 components = 0.0934156 Jy ! Clean residual min=-0.002520 max=0.002856 Jy/beam ! Clean residual mean=-0.000001 rms=0.000546 Jy/beam ! Combined flux in latest and established models = 0.0934156 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 0.0934156 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 0.165 milli-arcsec ! Estimated beam: bmin=0.6676 mas, bmaj=1.037 mas, bpa=-4.943 degrees ! Estimated noise=0.416934 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 = 0.00443146 Jy ! Component: 100 - total flux cleaned = 0.00720966 Jy ! Component: 150 - total flux cleaned = 0.00917001 Jy ! Component: 200 - total flux cleaned = 0.0106543 Jy ! Total flux subtracted in 200 components = 0.0106543 Jy ! Clean residual min=-0.001269 max=0.001248 Jy/beam ! Clean residual mean=-0.000001 rms=0.000274 Jy/beam ! Combined flux in latest and established models = 0.10407 Jy ! Adding 30 model components to the UV plane model. ! The established model now contains 35 components and 0.10407 Jy ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.165 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 0.165 milli-arcsec ! Estimated beam: bmin=2.581 mas, bmaj=3.359 mas, bpa=-0.7725 degrees ! Estimated noise=0.518929 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00154259 Jy ! Component: 100 - total flux cleaned = 0.00209189 Jy ! Component: 150 - total flux cleaned = 0.00235129 Jy ! Component: 200 - total flux cleaned = 0.00254796 Jy ! Total flux subtracted in 200 components = 0.00254796 Jy ! Clean residual min=-0.001284 max=0.001060 Jy/beam ! Clean residual mean=-0.000001 rms=0.000304 Jy/beam ! Combined flux in latest and established models = 0.106618 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 = 9.10873e-05 Jy ! Component: 100 - total flux cleaned = 0.000144842 Jy ! Component: 150 - total flux cleaned = 0.000190758 Jy ! Component: 200 - total flux cleaned = 0.000198806 Jy ! Total flux subtracted in 200 components = 0.000198806 Jy ! Clean residual min=-0.001300 max=0.001058 Jy/beam ! Clean residual mean=-0.000001 rms=0.000304 Jy/beam ! Combined flux in latest and established models = 0.106817 Jy ! Adding 36 model components to the UV plane model. ! The established model now contains 65 components and 0.106817 Jy ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.165 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 0.165 milli-arcsec ! Estimated beam: bmin=0.6676 mas, bmaj=1.037 mas, bpa=-4.943 degrees ! Estimated noise=0.416934 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000221399 Jy ! Component: 100 - total flux cleaned = 0.000286021 Jy ! Component: 150 - total flux cleaned = 0.000284859 Jy ! Component: 200 - total flux cleaned = 0.000310343 Jy ! Total flux subtracted in 200 components = 0.000310343 Jy ! Clean residual min=-0.001251 max=0.001053 Jy/beam ! Clean residual mean=-0.000000 rms=0.000260 Jy/beam ! Combined flux in latest and established models = 0.107127 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 77 components and 0.107127 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=0.099459Jy sigma=0.650149 ! Fit after self-cal, rms=0.099453Jy sigma=0.650096 wmodel /scr/pima/gb073_uvs/J1055+0205_X_map.mod ! Writing 77 model components to file: /scr/pima/gb073_uvs/J1055+0205_X_map.mod wobs /scr/pima/gb073_uvs/J1055+0205_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1055+0205_X_uvs.fits wwins /scr/pima/gb073_uvs/J1055+0205_X_map.win ! wwins: Wrote 5 windows to /scr/pima/gb073_uvs/J1055+0205_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 7.21% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000459101 Jy ! Component: 100 - total flux cleaned = -0.000559204 Jy ! Component: 150 - total flux cleaned = -0.000616038 Jy ! Component: 200 - total flux cleaned = -0.000597601 Jy ! Component: 250 - total flux cleaned = -0.00057951 Jy ! Component: 300 - total flux cleaned = -0.000561598 Jy ! Component: 350 - total flux cleaned = -0.000578903 Jy ! Component: 400 - total flux cleaned = -0.000647527 Jy ! Component: 450 - total flux cleaned = -0.000664587 Jy ! Component: 500 - total flux cleaned = -0.000731596 Jy ! Component: 550 - total flux cleaned = -0.000748226 Jy ! Component: 600 - total flux cleaned = -0.000797736 Jy ! Component: 650 - total flux cleaned = -0.000878931 Jy ! Component: 700 - total flux cleaned = -0.000830594 Jy ! Component: 750 - total flux cleaned = -0.000878407 Jy ! Component: 800 - total flux cleaned = -0.000941606 Jy ! Component: 850 - total flux cleaned = -0.00094177 Jy ! Component: 900 - total flux cleaned = -0.000988249 Jy ! Component: 950 - total flux cleaned = -0.000988154 Jy ! Component: 1000 - total flux cleaned = -0.000973031 Jy ! Component: 1050 - total flux cleaned = -0.00101868 Jy ! Component: 1100 - total flux cleaned = -0.0010336 Jy ! Component: 1150 - total flux cleaned = -0.00103344 Jy ! Component: 1200 - total flux cleaned = -0.00107796 Jy ! Component: 1250 - total flux cleaned = -0.00101897 Jy ! Component: 1300 - total flux cleaned = -0.00106282 Jy ! Component: 1350 - total flux cleaned = -0.00101911 Jy ! Component: 1400 - total flux cleaned = -0.00107687 Jy ! Component: 1450 - total flux cleaned = -0.00106237 Jy ! Component: 1500 - total flux cleaned = -0.00106232 Jy ! Component: 1550 - total flux cleaned = -0.000977158 Jy ! Component: 1600 - total flux cleaned = -0.00101962 Jy ! Component: 1650 - total flux cleaned = -0.00103369 Jy ! Component: 1700 - total flux cleaned = -0.00101955 Jy ! Component: 1750 - total flux cleaned = -0.0010334 Jy ! Component: 1800 - total flux cleaned = -0.000992007 Jy ! Component: 1850 - total flux cleaned = -0.000964587 Jy ! Component: 1900 - total flux cleaned = -0.00100547 Jy ! Component: 1950 - total flux cleaned = -0.000924216 Jy ! Component: 2000 - total flux cleaned = -0.000978154 Jy ! Component: 2050 - total flux cleaned = -0.000937943 Jy ! Component: 2100 - total flux cleaned = -0.000857993 Jy ! Component: 2150 - total flux cleaned = -0.000858019 Jy ! Component: 2200 - total flux cleaned = -0.000910799 Jy ! Component: 2250 - total flux cleaned = -0.000897831 Jy ! Component: 2300 - total flux cleaned = -0.000871801 Jy ! Component: 2350 - total flux cleaned = -0.000871761 Jy ! Component: 2400 - total flux cleaned = -0.00087173 Jy ! Component: 2450 - total flux cleaned = -0.000923158 Jy ! Component: 2500 - total flux cleaned = -0.000871926 Jy ! Component: 2550 - total flux cleaned = -0.000846352 Jy ! Component: 2600 - total flux cleaned = -0.000858977 Jy ! Component: 2650 - total flux cleaned = -0.000846414 Jy ! Component: 2700 - total flux cleaned = -0.000858918 Jy ! Component: 2750 - total flux cleaned = -0.000833747 Jy ! Component: 2800 - total flux cleaned = -0.000771369 Jy ! Component: 2850 - total flux cleaned = -0.000796236 Jy ! Component: 2900 - total flux cleaned = -0.000808571 Jy ! Component: 2950 - total flux cleaned = -0.000759268 Jy ! Component: 3000 - total flux cleaned = -0.000722477 Jy ! Component: 3050 - total flux cleaned = -0.000759154 Jy ! Component: 3100 - total flux cleaned = -0.000771356 Jy ! Component: 3150 - total flux cleaned = -0.0007108 Jy ! Component: 3200 - total flux cleaned = -0.000698771 Jy ! Component: 3250 - total flux cleaned = -0.000734881 Jy ! Component: 3300 - total flux cleaned = -0.000746839 Jy ! Component: 3350 - total flux cleaned = -0.000782531 Jy ! Component: 3400 - total flux cleaned = -0.000758911 Jy ! Component: 3450 - total flux cleaned = -0.000723391 Jy ! Component: 3500 - total flux cleaned = -0.000782464 Jy ! Component: 3550 - total flux cleaned = -0.000735489 Jy ! Component: 3600 - total flux cleaned = -0.000747112 Jy ! Component: 3650 - total flux cleaned = -0.00077041 Jy ! Component: 3700 - total flux cleaned = -0.000758767 Jy ! Component: 3750 - total flux cleaned = -0.000758821 Jy ! Component: 3800 - total flux cleaned = -0.000712754 Jy ! Component: 3850 - total flux cleaned = -0.000724272 Jy ! Component: 3900 - total flux cleaned = -0.000735673 Jy ! Component: 3950 - total flux cleaned = -0.000769941 Jy ! Component: 4000 - total flux cleaned = -0.000735874 Jy ! Component: 4050 - total flux cleaned = -0.000701913 Jy ! Total flux subtracted in 4096 components = -0.000679348 Jy ! Clean residual min=-0.000711 max=0.000672 Jy/beam ! Clean residual mean=0.000000 rms=0.000187 Jy/beam ! Combined flux in latest and established models = 0.106448 Jy keep ! Adding 343 model components to the UV plane model. ! The established model now contains 420 components and 0.106448 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1055+0205_X\_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 0.165 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6676 x 1.037 at -4.943 degrees (North through East) ! Clean map min=-0.00081441 max=0.085814 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1055+0205_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0858138 invert ! Inverting map ! Your choice of large map pixels excluded 7.21% of the data. ! The x-axis pixel size should ideally be below 0.165 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000186472 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.651895 0.651895 1.30379 2.60758 5.21516 10.4303 20.8607 41.7213 83.4426 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0005 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.085 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 460.196 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1055+0205_X_uvs.log closed on Sat Dec 26 09:36:45 2015