! Started logfile: /scr/pima/gb073_uvs/J2218+0052_X_uvs.log on Sat Dec 26 09:45:31 2015 obs /scr/pima/gb073_uvs/J2218+0052_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J2218+0052_X_uva.fits ! AN table 1: 80 integrations on 6 of 6 possible baselines. ! AN table 2: 29 integrations on 36 of 36 possible baselines. ! AN table 3: 56 integrations on 28 of 28 possible baselines. ! AN table 4: 116 integrations on 10 of 10 possible baselines. ! AN table 5: 29 integrations on 66 of 66 possible baselines. ! AN table 6: 29 integrations on 55 of 55 possible baselines. ! AN table 7: 20 integrations on 10 of 10 possible baselines. ! Apparent sampling: 0.851149 visibilities/baseline/integration-bin. ! Found source: J2218+0052 ! ! 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 54208 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/J2218+0052_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 188 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 3 telescope corrections were flagged in sub-array 3. ! A total of 165 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 188 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 3 telescope corrections were flagged in sub-array 3. ! A total of 165 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 188 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 3 telescope corrections were flagged in sub-array 3. ! A total of 165 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 188 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 3 telescope corrections were flagged in sub-array 3. ! A total of 165 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 5. ! A total of 188 telescope corrections were flagged in sub-array 1. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 59 telescope corrections were flagged in sub-array 3. ! A total of 165 telescope corrections were flagged in sub-array 4. ! A total of 58 telescope corrections were flagged in sub-array 5. ! A total of 58 telescope corrections were flagged in sub-array 6. ! A total of 20 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 6. ! A total of 188 telescope corrections were flagged in sub-array 1. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 59 telescope corrections were flagged in sub-array 3. ! A total of 165 telescope corrections were flagged in sub-array 4. ! A total of 58 telescope corrections were flagged in sub-array 5. ! A total of 58 telescope corrections were flagged in sub-array 6. ! A total of 20 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 7. ! A total of 188 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 3 telescope corrections were flagged in sub-array 3. ! A total of 165 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 8. ! A total of 188 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 3 telescope corrections were flagged in sub-array 3. ! A total of 165 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.004407Jy sigma=8.931918 ! Fit after self-cal, rms=0.935279Jy sigma=8.367324 ! 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 6.66% of the data. ! The x-axis pixel size should ideally be below 0.1648 milli-arcsec ! Estimated beam: bmin=0.6706 mas, bmaj=0.827 mas, bpa=4.355 degrees ! Estimated noise=0.83533 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 = 0.0529136 Jy ! Component: 100 - total flux cleaned = 0.0651447 Jy ! Total flux subtracted in 100 components = 0.0651447 Jy ! Clean residual min=-0.003284 max=0.007036 Jy/beam ! Clean residual mean=-0.000001 rms=0.000685 Jy/beam ! Combined flux in latest and established models = 0.0651447 Jy ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 4 components and 0.0651447 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=0.089880Jy sigma=0.660089 ! Fit after self-cal, rms=0.088979Jy sigma=0.650928 ! Inverting map ! Your choice of large map pixels excluded 6.66% of the data. ! The x-axis pixel size should ideally be below 0.1648 milli-arcsec ! Added new window around map position (-0.2, -2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00717645 Jy ! Component: 100 - total flux cleaned = 0.00824873 Jy ! Total flux subtracted in 100 components = 0.00824873 Jy ! Clean residual min=-0.002832 max=0.003591 Jy/beam ! Clean residual mean=0.000001 rms=0.000611 Jy/beam ! Combined flux in latest and established models = 0.0733935 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 10 components and 0.0733935 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=0.088453Jy sigma=0.647594 ! Fit after self-cal, rms=0.088392Jy sigma=0.647124 ! Inverting map ! Your choice of large map pixels excluded 6.66% of the data. ! The x-axis pixel size should ideally be below 0.1648 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0020508 Jy ! Component: 100 - total flux cleaned = 0.00204853 Jy ! Total flux subtracted in 100 components = 0.00204853 Jy ! Clean residual min=-0.002624 max=0.003220 Jy/beam ! Clean residual mean=0.000001 rms=0.000583 Jy/beam ! Combined flux in latest and established models = 0.075442 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 13 components and 0.075442 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=0.088245Jy sigma=0.646479 ! Fit after self-cal, rms=0.088210Jy sigma=0.646375 ! Inverting map ! Your choice of large map pixels excluded 6.66% of the data. ! The x-axis pixel size should ideally be below 0.1648 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 6.66% of the data. ! The x-axis pixel size should ideally be below 0.1648 milli-arcsec ! Estimated beam: bmin=0.8029 mas, bmaj=1.154 mas, bpa=-2.387 degrees ! Estimated noise=0.389802 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 (-0.6, -16.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00111512 Jy ! Component: 100 - total flux cleaned = 0.000984155 Jy ! Component: 150 - total flux cleaned = 0.000876068 Jy ! Component: 200 - total flux cleaned = 0.000782046 Jy ! Total flux subtracted in 200 components = 0.000782046 Jy ! Clean residual min=-0.001698 max=0.001966 Jy/beam ! Clean residual mean=0.000001 rms=0.000369 Jy/beam ! Combined flux in latest and established models = 0.076224 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 25 components and 0.076224 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=0.088103Jy sigma=0.645777 ! Fit after self-cal, rms=0.088078Jy sigma=0.645676 ! Inverting map ! Your choice of large map pixels excluded 6.66% of the data. ! The x-axis pixel size should ideally be below 0.1648 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8029 x 1.154 at -2.387 degrees (North through East) ! Clean map min=-0.0016473 max=0.068172 Jy/beam if ( peak(flux,max)/imstat(rms) < lim_self ) selflim lim_val ! Selfcal amplitude corrections will be limited to 0.833333 -> 1.2. ! Selfcal phase corrections will not be limited. gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 132 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 0.97 KP 1.02 LA 1.05 ! MK 1.05 NL 0.95 OV 1.05 PT 1.04 ! ! A total of 63 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 EF 1.00* FD 1.04 HH 1.04 ! KP 1.07 LA 1.11 MC 0.85 NL 0.88 ! ON 0.86 OV 1.01 PT 0.99 SC 1.13 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00 EF 1.00* FD 0.96 HH 1.08 ! KP 1.05 LA 1.09 NL 0.97 ON 0.90 ! OV 1.04 PT 0.96 SC 1.00 ! ! Telescope amplitude corrections in sub-array 7: ! BR 0.99 KP 1.11 LA 1.02 MK 0.90 ! OV 0.99 ! ! ! Correcting IF 2. ! A total of 132 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.07 EF 1.00* FD 1.12 KP 1.03 ! LA 1.12 MC 0.84 NL 1.06 PT 0.98 ! SC 0.97 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.04 FD 1.03 KP 1.03 LA 1.09 ! MK 1.07 NL 1.07 OV 1.02 PT 1.07 ! ! A total of 63 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.06 EF 1.00* FD 1.04 HH 0.95 ! KP 1.13 LA 1.08 MC 1.04 NL 1.01 ! ON 0.92 OV 1.05 PT 1.04 SC 0.99 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.06 EF 1.00* FD 1.13 HH 1.09 ! KP 0.94 LA 1.08 NL 0.93 ON 0.94 ! OV 0.98 PT 1.11 SC 1.04 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* KP 1.00* LA 1.00* MK 1.00* ! OV 1.00* ! ! ! Correcting IF 3. ! A total of 132 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.05 FD 0.99 KP 0.95 LA 1.01 ! MK 0.96 NL 1.07 OV 1.05 PT 0.97 ! ! A total of 63 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.06 EF 1.00* FD 0.98 HH 0.96 ! KP 0.95 LA 1.01 MC 1.04 NL 1.00 ! ON 0.90 OV 1.00 PT 1.09 SC 0.97 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! KP 1.00* LA 1.00* NL 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* KP 1.00* LA 1.00* MK 1.00* ! OV 1.00* ! ! ! Correcting IF 4. ! A total of 132 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.18 EF 1.00* FD 1.09 KP 0.99 ! LA 1.02 MC 0.85 NL 1.08 PT 1.01 ! SC 1.13 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.06 FD 1.07 KP 1.02 LA 1.04 ! MK 1.01 NL 1.03 OV 1.00 PT 1.04 ! ! A total of 63 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.98 EF 1.00* FD 1.09 HH 0.94 ! KP 1.04 LA 1.03 MC 1.10 NL 1.04 ! ON 0.91 OV 1.02 PT 1.09 SC 1.02 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.05 EF 1.00* FD 0.99 HH 0.99 ! KP 1.02 LA 1.13 NL 1.03 ON 0.90 ! OV 0.99 PT 0.98 SC 1.17 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.05 KP 0.88 LA 1.02 MK 1.09 ! OV 1.06 ! ! ! Correcting IF 5. ! A total of 132 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.01 KP 0.83 ! LA 1.12 MC 1.14 NL 1.00 PT 0.96 ! SC 0.87 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 0.95 KP 0.92 LA 0.99 ! MK 1.00 NL 1.01 OV 1.12 PT 0.98 ! ! A total of 63 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 1.02 MC 1.03 ON 0.90 ! ZC 0.86 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.09 HH 0.88 ! KP 0.91 LA 0.99 MC 1.01 NL 1.07 ! ON 1.16 OV 0.99 PT 0.99 SC 1.12 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 0.92 HH 0.97 ! KP 0.98 LA 1.00 NL 0.97 ON 1.04 ! OV 1.01 PT 0.99 SC 1.02 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* KP 1.00* LA 1.00* MK 1.00* ! OV 1.00* ! ! ! Correcting IF 6. ! A total of 132 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 0.97 KP 0.90 LA 0.97 ! MK 1.00 NL 0.96 OV 1.00 PT 1.08 ! ! A total of 63 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 0.94 MC 0.94 ON 0.96 ! ZC 0.88 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 0.98 HH 1.11 ! KP 0.84 LA 1.12 MC 1.17 NL 0.98 ! ON 1.13 OV 1.07 PT 0.92 SC 0.96 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.10 HH 0.88 ! KP 0.96 LA 0.95 NL 1.00 ON 1.03 ! OV 1.08 PT 1.02 SC 0.99 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* KP 1.05 LA 0.93 MK 0.94 ! OV 0.93 ! ! ! Correcting IF 7. ! A total of 132 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.03 EF 1.00* FD 1.02 KP 0.89 ! LA 1.10 MC 1.11 NL 1.09 PT 0.88 ! SC 0.96 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.07 KP 0.85 LA 1.05 ! MK 1.11 NL 1.11 OV 1.00 PT 0.97 ! ! A total of 63 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! KP 1.00* LA 1.00* MC 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.04 EF 1.00* FD 0.95 HH 1.01 ! KP 0.86 LA 1.05 NL 1.05 ON 0.95 ! OV 1.09 PT 0.94 SC 1.03 ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* KP 1.00* LA 1.00* MK 1.00* ! OV 1.00* ! ! ! Correcting IF 8. ! A total of 132 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.94 EF 1.00* FD 1.09 KP 0.92 ! LA 0.97 MC 1.00 NL 1.14 PT 1.03 ! SC 0.84 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 0.96 KP 0.97 LA 0.99 ! MK 0.99 NL 1.08 OV 1.07 PT 0.97 ! ! A total of 63 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.13 EF 1.00* FD 0.97 HH 1.05 ! KP 0.93 LA 1.11 MC 1.11 NL 0.98 ! ON 1.17 OV 1.16 PT 1.04 SC 0.99 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.97 EF 1.00* FD 0.98 HH 1.02 ! KP 0.92 LA 1.00 NL 1.01 ON 1.11 ! OV 1.02 PT 1.01 SC 0.99 ! ! Telescope amplitude corrections in sub-array 7: ! BR 0.95 KP 0.85 LA 0.99 MK 0.88 ! OV 1.00 ! ! ! Fit before self-cal, rms=0.088078Jy sigma=0.645676 ! Fit after self-cal, rms=0.088789Jy sigma=0.647872 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 6.9% of the data. ! The x-axis pixel size should ideally be below 0.1648 milli-arcsec ! Estimated beam: bmin=0.7944 mas, bmaj=1.249 mas, bpa=-2.919 degrees ! Estimated noise=0.399199 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 = 0.00123287 Jy ! Component: 100 - total flux cleaned = 0.00123543 Jy ! Component: 150 - total flux cleaned = 0.00120938 Jy ! Component: 200 - total flux cleaned = 0.00113772 Jy ! Total flux subtracted in 200 components = 0.00113772 Jy ! Clean residual min=-0.001298 max=0.001403 Jy/beam ! Clean residual mean=0.000002 rms=0.000307 Jy/beam ! Combined flux in latest and established models = 0.0773618 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 30 components and 0.0773618 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=0.088749Jy sigma=0.647771 ! Fit after self-cal, rms=0.088764Jy sigma=0.647468 ! Inverting map ! Your choice of large map pixels excluded 6.9% of the data. ! The x-axis pixel size should ideally be below 0.1648 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=0.088764Jy sigma=0.647468 ! Fit after self-cal, rms=0.089943Jy sigma=0.647186 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.9% of the data. ! The x-axis pixel size should ideally be below 0.1648 milli-arcsec ! Estimated beam: bmin=0.7946 mas, bmaj=1.25 mas, bpa=-2.896 degrees ! Estimated noise=0.403166 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000931398 Jy ! Component: 100 - total flux cleaned = 0.000960819 Jy ! Component: 150 - total flux cleaned = 0.000914776 Jy ! Component: 200 - total flux cleaned = 0.000851501 Jy ! Total flux subtracted in 200 components = 0.000851501 Jy ! Clean residual min=-0.001297 max=0.001285 Jy/beam ! Clean residual mean=0.000001 rms=0.000305 Jy/beam ! Combined flux in latest and established models = 0.0782133 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 30 components and 0.0782133 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=0.089912Jy sigma=0.647129 ! Fit after self-cal, rms=0.089943Jy sigma=0.647084 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.9% of the data. ! The x-axis pixel size should ideally be below 0.1648 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 = 5.94117e-05 Jy ! Component: 100 - total flux cleaned = -2.00092e-05 Jy ! Component: 150 - total flux cleaned = -5.64648e-05 Jy ! Component: 200 - total flux cleaned = -0.000127002 Jy ! Total flux subtracted in 200 components = -0.000127002 Jy ! Clean residual min=-0.001292 max=0.001280 Jy/beam ! Clean residual mean=0.000001 rms=0.000303 Jy/beam ! Combined flux in latest and established models = 0.0780863 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 37 components and 0.0780863 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=0.089930Jy sigma=0.647044 ! Fit after self-cal, rms=0.089927Jy sigma=0.647032 ! Inverting map ! Your choice of large map pixels excluded 6.9% of the data. ! The x-axis pixel size should ideally be below 0.1648 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=0.089927Jy sigma=0.647032 ! Fit after self-cal, rms=0.090787Jy sigma=0.646976 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.9% of the data. ! The x-axis pixel size should ideally be below 0.1648 milli-arcsec ! Estimated beam: bmin=0.7935 mas, bmaj=1.249 mas, bpa=-2.911 degrees ! Estimated noise=0.406967 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000815285 Jy ! Component: 100 - total flux cleaned = 0.000857005 Jy ! Component: 150 - total flux cleaned = 0.000822534 Jy ! Component: 200 - total flux cleaned = 0.000773726 Jy ! Total flux subtracted in 200 components = 0.000773726 Jy ! Clean residual min=-0.001269 max=0.001304 Jy/beam ! Clean residual mean=0.000001 rms=0.000302 Jy/beam ! Combined flux in latest and established models = 0.07886 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 38 components and 0.07886 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=0.090765Jy sigma=0.646950 ! Fit after self-cal, rms=0.090767Jy sigma=0.646913 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.9% of the data. ! The x-axis pixel size should ideally be below 0.1648 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 (28.4, -9). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00114472 Jy ! Component: 100 - total flux cleaned = 0.00112787 Jy ! Component: 150 - total flux cleaned = 0.00110903 Jy ! Component: 200 - total flux cleaned = 0.001092 Jy ! Total flux subtracted in 200 components = 0.001092 Jy ! Clean residual min=-0.001265 max=0.001222 Jy/beam ! Clean residual mean=0.000001 rms=0.000295 Jy/beam ! Combined flux in latest and established models = 0.079952 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 48 components and 0.079952 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=0.090747Jy sigma=0.646793 ! Fit after self-cal, rms=0.090746Jy sigma=0.646771 ! Inverting map ! Your choice of large map pixels excluded 6.9% of the data. ! The x-axis pixel size should ideally be below 0.1648 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=0.090746Jy sigma=0.646771 ! Fit after self-cal, rms=0.091463Jy sigma=0.646741 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 6.9% of the data. ! The x-axis pixel size should ideally be below 0.1648 milli-arcsec ! Estimated beam: bmin=2.766 mas, bmaj=3.473 mas, bpa=6.701 degrees ! Estimated noise=0.484946 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000160733 Jy ! Component: 100 - total flux cleaned = 0.000283414 Jy ! Component: 150 - total flux cleaned = 0.000297053 Jy ! Component: 200 - total flux cleaned = 0.000297752 Jy ! Total flux subtracted in 200 components = 0.000297752 Jy ! Clean residual min=-0.001142 max=0.001119 Jy/beam ! Clean residual mean=0.000001 rms=0.000328 Jy/beam ! Combined flux in latest and established models = 0.0802497 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 57 components and 0.0802497 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=0.091454Jy sigma=0.646725 ! Fit after self-cal, rms=0.091459Jy sigma=0.646716 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 6.9% of the data. ! The x-axis pixel size should ideally be below 0.1648 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 = 2.29742e-05 Jy ! Component: 100 - total flux cleaned = 2.35009e-05 Jy ! Component: 150 - total flux cleaned = 4.0015e-06 Jy ! Component: 200 - total flux cleaned = -5.02798e-06 Jy ! Total flux subtracted in 200 components = -5.02798e-06 Jy ! Clean residual min=-0.001131 max=0.001119 Jy/beam ! Clean residual mean=0.000001 rms=0.000326 Jy/beam ! Combined flux in latest and established models = 0.0802447 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 63 components and 0.0802447 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=0.091456Jy sigma=0.646716 ! Fit after self-cal, rms=0.091457Jy sigma=0.646715 ! Inverting map ! Your choice of large map pixels excluded 6.9% of the data. ! The x-axis pixel size should ideally be below 0.1648 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 6.9% of the data. ! The x-axis pixel size should ideally be below 0.1648 milli-arcsec ! Estimated beam: bmin=0.7934 mas, bmaj=1.247 mas, bpa=-2.909 degrees ! Estimated noise=0.410267 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7934 x 1.247 at -2.909 degrees (North through East) ! Clean map min=-0.0019008 max=0.070322 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 6.9% of the data. ! The x-axis pixel size should ideally be below 0.1648 milli-arcsec ! Estimated beam: bmin=0.6644 mas, bmaj=0.8603 mas, bpa=4.034 degrees ! Estimated noise=0.880626 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0548151 Jy ! Component: 100 - total flux cleaned = 0.0687971 Jy ! Component: 150 - total flux cleaned = 0.0760827 Jy ! Component: 200 - total flux cleaned = 0.0801618 Jy ! Total flux subtracted in 200 components = 0.0801618 Jy ! Clean residual min=-0.002560 max=0.003252 Jy/beam ! Clean residual mean=0.000001 rms=0.000583 Jy/beam ! Combined flux in latest and established models = 0.0801618 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 14 model components to the UV plane model. ! The established model now contains 14 components and 0.0801618 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 6.9% of the data. ! The x-axis pixel size should ideally be below 0.1648 milli-arcsec ! Estimated beam: bmin=0.7934 mas, bmaj=1.247 mas, bpa=-2.909 degrees ! Estimated noise=0.410267 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 = 0.00116372 Jy ! Component: 100 - total flux cleaned = 0.00144722 Jy ! Component: 150 - total flux cleaned = 0.00156382 Jy ! Component: 200 - total flux cleaned = 0.0017171 Jy ! Total flux subtracted in 200 components = 0.0017171 Jy ! Clean residual min=-0.001444 max=0.001370 Jy/beam ! Clean residual mean=0.000001 rms=0.000316 Jy/beam ! Combined flux in latest and established models = 0.0818789 Jy ! Adding 16 model components to the UV plane model. ! The established model now contains 25 components and 0.0818789 Jy ! Inverting map ! Your choice of large map pixels excluded 6.9% of the data. ! The x-axis pixel size should ideally be below 0.1648 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 6.9% of the data. ! The x-axis pixel size should ideally be below 0.1648 milli-arcsec ! Estimated beam: bmin=2.766 mas, bmaj=3.473 mas, bpa=6.701 degrees ! Estimated noise=0.484946 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000603167 Jy ! Component: 100 - total flux cleaned = -0.000845236 Jy ! Component: 150 - total flux cleaned = -0.000910331 Jy ! Component: 200 - total flux cleaned = -0.000967072 Jy ! Total flux subtracted in 200 components = -0.000967072 Jy ! Clean residual min=-0.001160 max=0.001185 Jy/beam ! Clean residual mean=0.000001 rms=0.000335 Jy/beam ! Combined flux in latest and established models = 0.0809118 Jy flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -4.97042e-05 Jy ! Component: 100 - total flux cleaned = -0.000108472 Jy ! Component: 150 - total flux cleaned = -0.000178125 Jy ! Component: 200 - total flux cleaned = -0.000218142 Jy ! Total flux subtracted in 200 components = -0.000218142 Jy ! Clean residual min=-0.001154 max=0.001159 Jy/beam ! Clean residual mean=0.000001 rms=0.000331 Jy/beam ! Combined flux in latest and established models = 0.0806937 Jy ! Adding 18 model components to the UV plane model. ! The established model now contains 40 components and 0.0806937 Jy ! Inverting map ! Your choice of large map pixels excluded 6.9% of the data. ! The x-axis pixel size should ideally be below 0.1648 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 6.9% of the data. ! The x-axis pixel size should ideally be below 0.1648 milli-arcsec ! Estimated beam: bmin=0.7934 mas, bmaj=1.247 mas, bpa=-2.909 degrees ! Estimated noise=0.410267 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000262926 Jy ! Component: 100 - total flux cleaned = 0.000383432 Jy ! Component: 150 - total flux cleaned = 0.000527306 Jy ! Component: 200 - total flux cleaned = 0.000659761 Jy ! Total flux subtracted in 200 components = 0.000659761 Jy ! Clean residual min=-0.001292 max=0.001286 Jy/beam ! Clean residual mean=0.000001 rms=0.000302 Jy/beam ! Combined flux in latest and established models = 0.0813534 Jy selfcal ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 43 components and 0.0813535 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=0.091509Jy sigma=0.646925 ! Fit after self-cal, rms=0.091522Jy sigma=0.646890 wmodel /scr/pima/gb073_uvs/J2218+0052_X_map.mod ! Writing 43 model components to file: /scr/pima/gb073_uvs/J2218+0052_X_map.mod wobs /scr/pima/gb073_uvs/J2218+0052_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J2218+0052_X_uvs.fits wwins /scr/pima/gb073_uvs/J2218+0052_X_map.win ! wwins: Wrote 4 windows to /scr/pima/gb073_uvs/J2218+0052_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 6.9% of the data. ! The x-axis pixel size should ideally be below 0.1648 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -5.65063e-05 Jy ! Component: 100 - total flux cleaned = 0.000121463 Jy ! Component: 150 - total flux cleaned = 0.000443685 Jy ! Component: 200 - total flux cleaned = 0.000673486 Jy ! Component: 250 - total flux cleaned = 0.000816681 Jy ! Component: 300 - total flux cleaned = 0.000957125 Jy ! Component: 350 - total flux cleaned = 0.000976923 Jy ! Component: 400 - total flux cleaned = 0.001055 Jy ! Component: 450 - total flux cleaned = 0.00109363 Jy ! Component: 500 - total flux cleaned = 0.00115089 Jy ! Component: 550 - total flux cleaned = 0.00122619 Jy ! Component: 600 - total flux cleaned = 0.00133716 Jy ! Component: 650 - total flux cleaned = 0.00133706 Jy ! Component: 700 - total flux cleaned = 0.00137332 Jy ! Component: 750 - total flux cleaned = 0.00144523 Jy ! Component: 800 - total flux cleaned = 0.00148036 Jy ! Component: 850 - total flux cleaned = 0.00151539 Jy ! Component: 900 - total flux cleaned = 0.0015849 Jy ! Component: 950 - total flux cleaned = 0.00158489 Jy ! Component: 1000 - total flux cleaned = 0.0015849 Jy ! Component: 1050 - total flux cleaned = 0.00161905 Jy ! Component: 1100 - total flux cleaned = 0.00160224 Jy ! Component: 1150 - total flux cleaned = 0.00158562 Jy ! Component: 1200 - total flux cleaned = 0.00158583 Jy ! Component: 1250 - total flux cleaned = 0.00158569 Jy ! Component: 1300 - total flux cleaned = 0.00161793 Jy ! Component: 1350 - total flux cleaned = 0.00160183 Jy ! Component: 1400 - total flux cleaned = 0.00161756 Jy ! Component: 1450 - total flux cleaned = 0.00168075 Jy ! Component: 1500 - total flux cleaned = 0.00166487 Jy ! Component: 1550 - total flux cleaned = 0.00169587 Jy ! Component: 1600 - total flux cleaned = 0.00169567 Jy ! Component: 1650 - total flux cleaned = 0.00171085 Jy ! Component: 1700 - total flux cleaned = 0.00172629 Jy ! Component: 1750 - total flux cleaned = 0.00180207 Jy ! Component: 1800 - total flux cleaned = 0.00187718 Jy ! Component: 1850 - total flux cleaned = 0.00189214 Jy ! Component: 1900 - total flux cleaned = 0.00193677 Jy ! Component: 1950 - total flux cleaned = 0.00199593 Jy ! Component: 2000 - total flux cleaned = 0.00204021 Jy ! Component: 2050 - total flux cleaned = 0.00220084 Jy ! Component: 2100 - total flux cleaned = 0.00227345 Jy ! Component: 2150 - total flux cleaned = 0.002259 Jy ! Component: 2200 - total flux cleaned = 0.00238811 Jy ! Component: 2250 - total flux cleaned = 0.00250224 Jy ! Component: 2300 - total flux cleaned = 0.00257322 Jy ! Component: 2350 - total flux cleaned = 0.00262969 Jy ! Component: 2400 - total flux cleaned = 0.00272783 Jy ! Component: 2450 - total flux cleaned = 0.00276953 Jy ! Component: 2500 - total flux cleaned = 0.00281106 Jy ! Component: 2550 - total flux cleaned = 0.00292138 Jy ! Component: 2600 - total flux cleaned = 0.00293504 Jy ! Component: 2650 - total flux cleaned = 0.00298963 Jy ! Component: 2700 - total flux cleaned = 0.00309827 Jy ! Component: 2750 - total flux cleaned = 0.0030982 Jy ! Component: 2800 - total flux cleaned = 0.00313854 Jy ! Component: 2850 - total flux cleaned = 0.00317863 Jy ! Component: 2900 - total flux cleaned = 0.00321864 Jy ! Component: 2950 - total flux cleaned = 0.00325819 Jy ! Component: 3000 - total flux cleaned = 0.00331082 Jy ! Component: 3050 - total flux cleaned = 0.00336302 Jy ! Component: 3100 - total flux cleaned = 0.00340216 Jy ! Component: 3150 - total flux cleaned = 0.00344104 Jy ! Component: 3200 - total flux cleaned = 0.00354431 Jy ! Component: 3250 - total flux cleaned = 0.00355718 Jy ! Component: 3300 - total flux cleaned = 0.00362101 Jy ! Component: 3350 - total flux cleaned = 0.00363378 Jy ! Component: 3400 - total flux cleaned = 0.00364638 Jy ! Component: 3450 - total flux cleaned = 0.00374721 Jy ! Component: 3500 - total flux cleaned = 0.00372221 Jy ! Component: 3550 - total flux cleaned = 0.00377216 Jy ! Component: 3600 - total flux cleaned = 0.00380954 Jy ! Component: 3650 - total flux cleaned = 0.00384653 Jy ! Component: 3700 - total flux cleaned = 0.00387114 Jy ! Component: 3750 - total flux cleaned = 0.00388344 Jy ! Component: 3800 - total flux cleaned = 0.00390791 Jy ! Component: 3850 - total flux cleaned = 0.0039445 Jy ! Component: 3900 - total flux cleaned = 0.00399294 Jy ! Component: 3950 - total flux cleaned = 0.00399285 Jy ! Component: 4000 - total flux cleaned = 0.00400478 Jy ! Component: 4050 - total flux cleaned = 0.00396881 Jy ! Total flux subtracted in 4096 components = 0.00396878 Jy ! Clean residual min=-0.000742 max=0.000833 Jy/beam ! Clean residual mean=0.000001 rms=0.000200 Jy/beam ! Combined flux in latest and established models = 0.0853222 Jy keep ! Adding 304 model components to the UV plane model. ! The established model now contains 347 components and 0.0853222 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J2218+0052_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 6.9% of the data. ! The x-axis pixel size should ideally be below 0.1648 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7934 x 1.247 at -2.909 degrees (North through East) ! Clean map min=-0.0016453 max=0.069637 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J2218+0052_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0696367 invert ! Inverting map ! Your choice of large map pixels excluded 6.9% of the data. ! The x-axis pixel size should ideally be below 0.1648 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000200176 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.862373 0.862373 1.72475 3.44949 6.89898 13.798 27.5959 55.1919 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0006 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.069 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 347.877 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J2218+0052_X_uvs.log closed on Sat Dec 26 09:45:36 2015