! Started logfile: /scr/pima/gb073_uvs/J1539+4735_X_uvs.log on Sat Dec 26 09:41:49 2015 obs /scr/pima/gb073_uvs/J1539+4735_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1539+4735_X_uva.fits ! AN table 1: 29 integrations on 55 of 55 possible baselines. ! AN table 2: 29 integrations on 55 of 55 possible baselines. ! AN table 3: 54 integrations on 55 of 55 possible baselines. ! AN table 4: 29 integrations on 36 of 36 possible baselines. ! AN table 5: 29 integrations on 45 of 45 possible baselines. ! AN table 6: 29 integrations on 36 of 36 possible baselines. ! Apparent sampling: 0.962734 visibilities/baseline/integration-bin. ! Found source: J1539+4735 ! ! 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 73576 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/J1539+4735_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 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 54 telescope corrections were flagged in sub-array 3. ! A total of 29 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 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 54 telescope corrections were flagged in sub-array 3. ! A total of 29 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 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 54 telescope corrections were flagged in sub-array 3. ! A total of 29 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 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 54 telescope corrections were flagged in sub-array 3. ! A total of 29 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 58 telescope corrections were flagged in sub-array 1. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 108 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! A total of 58 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 6. ! A total of 58 telescope corrections were flagged in sub-array 1. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 108 telescope corrections were flagged in sub-array 3. ! A total of 29 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! A total of 58 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 7. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 54 telescope corrections were flagged in sub-array 3. ! A total of 29 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 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 54 telescope corrections were flagged in sub-array 3. ! A total of 29 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=1.005160Jy sigma=10.847171 ! Fit after self-cal, rms=0.937016Jy sigma=10.109467 ! 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 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 milli-arcsec ! Estimated beam: bmin=0.5071 mas, bmaj=0.9414 mas, bpa=-34.8 degrees ! Estimated noise=0.657797 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 = 0.0503309 Jy ! Component: 100 - total flux cleaned = 0.0613327 Jy ! Total flux subtracted in 100 components = 0.0613327 Jy ! Clean residual min=-0.002605 max=0.003471 Jy/beam ! Clean residual mean=0.000001 rms=0.000474 Jy/beam ! Combined flux in latest and established models = 0.0613327 Jy ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 4 components and 0.0613327 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=0.073313Jy sigma=0.675056 ! Fit after self-cal, rms=0.072503Jy sigma=0.667027 ! Inverting map ! Your choice of large map pixels excluded 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00405026 Jy ! Component: 100 - total flux cleaned = 0.00588428 Jy ! Total flux subtracted in 100 components = 0.00588428 Jy ! Clean residual min=-0.002177 max=0.002102 Jy/beam ! Clean residual mean=0.000000 rms=0.000455 Jy/beam ! Combined flux in latest and established models = 0.0672169 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 8 components and 0.0672169 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=0.072249Jy sigma=0.663885 ! Fit after self-cal, rms=0.072273Jy sigma=0.663837 ! Inverting map ! Your choice of large map pixels excluded 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 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 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 milli-arcsec ! Estimated beam: bmin=0.7313 mas, bmaj=1.231 mas, bpa=-28.31 degrees ! Estimated noise=0.279425 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 = 0.00129935 Jy ! Component: 100 - total flux cleaned = 0.00192484 Jy ! Component: 150 - total flux cleaned = 0.00204853 Jy ! Component: 200 - total flux cleaned = 0.00209903 Jy ! Total flux subtracted in 200 components = 0.00209903 Jy ! Clean residual min=-0.000996 max=0.000976 Jy/beam ! Clean residual mean=0.000000 rms=0.000212 Jy/beam ! Combined flux in latest and established models = 0.069316 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 9 components and 0.069316 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=0.072246Jy sigma=0.663630 ! Fit after self-cal, rms=0.072255Jy sigma=0.663623 ! Inverting map ! Your choice of large map pixels excluded 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7313 x 1.231 at -28.31 degrees (North through East) ! Clean map min=-0.00084361 max=0.06545 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 EF 1.00* FD 0.96 KP 1.06 ! LA 1.04 MK 0.96 NL 0.94 ON 0.92 ! OV 1.03 PT 0.98 ZC 0.80 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.87 EF 1.00* FD 0.99 KP 1.02 ! LA 1.11 MC 0.99 NL 0.98 ON 0.96 ! OV 1.06 PT 0.97 SC 0.93 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 EF 1.00* FD 1.01 KP 0.95 ! LA 1.07 MK 1.03 NL 0.98 ON 1.03 ! OV 1.03 PT 1.01 SC 0.95 ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* FD 0.89 KP 0.98 LA 1.24 ! NL 0.93 ON 0.83 OV 1.06 PT 0.95 ! SC 0.94 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 1.01 KP 1.07 LA 1.01 ! MK 0.92 NL 0.95 ON 0.89 OV 1.02 ! PT 0.96 SC 0.98 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.98 EF 1.00* FD 0.96 KP 0.96 ! LA 0.96 MK 1.00 NL 0.93 OV 1.05 ! PT 0.98 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.07 EF 1.00* FD 1.04 KP 1.03 ! LA 1.06 MK 1.09 NL 0.99 ON 1.08 ! OV 1.06 PT 1.05 ZC 0.76 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.02 EF 1.00* FD 1.03 KP 1.00 ! LA 1.09 MC 0.88 NL 1.03 ON 0.95 ! OV 1.11 PT 1.07 SC 1.00 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 EF 1.00* FD 1.04 KP 1.00 ! LA 1.11 MK 1.00 NL 1.01 ON 0.94 ! OV 1.03 PT 1.06 SC 1.01 ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* FD 1.01 KP 1.11 LA 1.03 ! NL 0.97 ON 0.92 OV 1.00 PT 1.04 ! SC 0.99 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 1.00 KP 1.00 LA 1.04 ! MK 1.11 NL 0.99 ON 1.06 OV 0.99 ! PT 1.06 SC 0.96 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.08 EF 1.00* FD 0.98 KP 1.02 ! LA 0.98 MK 0.99 NL 1.05 OV 1.10 ! PT 1.06 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.94 EF 1.00* FD 0.98 KP 1.00 ! LA 0.98 MK 1.08 NL 0.93 ON 0.96 ! OV 1.04 PT 0.94 ZC 0.74 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 EF 1.00* FD 0.98 KP 0.94 ! LA 1.05 MC 1.11 NL 0.92 ON 0.95 ! OV 0.99 PT 0.99 SC 0.97 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 EF 1.00* FD 0.99 KP 0.96 ! LA 1.00 MK 0.99 NL 0.98 ON 1.00 ! OV 1.00 PT 1.03 SC 1.08 ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* FD 1.01 KP 0.98 LA 0.94 ! NL 0.98 ON 0.88 OV 1.05 PT 0.99 ! SC 1.09 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 0.94 KP 1.01 LA 1.01 ! MK 0.96 NL 1.00 ON 0.84 OV 1.06 ! PT 1.03 SC 0.96 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.96 EF 1.00* FD 1.03 KP 1.03 ! LA 1.02 MK 1.00 NL 0.89 OV 1.07 ! PT 0.99 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 EF 1.00* FD 1.02 KP 0.99 ! LA 0.99 MK 1.08 NL 1.01 ON 0.97 ! OV 1.02 PT 1.04 ZC 0.76 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.96 EF 1.00* FD 1.02 KP 1.01 ! LA 1.01 MC 0.97 NL 1.00 ON 0.97 ! OV 1.00 PT 1.04 SC 0.96 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 EF 1.00* FD 1.04 KP 1.02 ! LA 0.98 MK 0.98 NL 1.00 ON 1.06 ! OV 1.05 PT 1.06 SC 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* FD 1.07 KP 0.99 LA 1.03 ! NL 1.00 ON 0.82 OV 0.96 PT 1.04 ! SC 1.00 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 1.04 KP 1.01 LA 0.97 ! MK 0.98 NL 1.01 ON 0.87 OV 0.96 ! PT 1.03 SC 0.97 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00 EF 1.00* FD 1.05 KP 0.93 ! LA 1.00 MK 0.96 NL 1.00 OV 1.03 ! PT 1.07 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.99 KP 0.90 ! LA 1.12 MK 1.00 NL 0.95 ON 2.03 ! OV 1.08 PT 0.96 ZC 0.84 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 0.98 KP 0.93 ! LA 1.03 MC 1.34 NL 1.03 ON 1.10 ! OV 0.99 PT 1.01 SC 0.93 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.01 KP 0.87 ! LA 1.00 MK 1.00 NL 1.01 ON 1.17 ! OV 1.04 PT 1.02 SC 0.95 ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* FD 0.94 KP 0.94 LA 1.03 ! NL 1.01 ON 0.98 OV 1.12 PT 1.00 ! SC 0.95 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 1.09 KP 0.92 LA 0.97 ! MK 0.98 NL 1.02 ON 1.17 OV 1.03 ! PT 0.97 SC 1.07 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 0.93 KP 0.88 ! LA 1.07 MK 0.89 NL 0.98 OV 1.09 ! PT 0.99 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.97 KP 0.81 ! LA 1.07 MK 0.98 NL 1.00 ON 2.22 ! OV 0.95 PT 0.99 ZC 0.82 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.02 KP 0.88 ! LA 1.04 MC 1.21 NL 0.98 ON 1.31 ! OV 1.17 PT 0.96 SC 0.92 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.03 KP 0.87 ! LA 0.96 MK 1.02 NL 1.00 ON 1.18 ! OV 1.07 PT 0.92 SC 1.00 ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* FD 1.05 KP 0.82 LA 0.99 ! NL 0.99 ON 1.12 OV 1.16 PT 0.99 ! SC 0.99 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 0.90 KP 0.92 LA 0.99 ! MK 0.99 NL 0.95 ON 1.06 OV 1.02 ! PT 1.00 SC 0.94 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.02 KP 0.90 ! LA 1.00 MK 0.89 NL 0.94 OV 1.01 ! PT 0.89 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.05 EF 1.00* FD 1.00 KP 0.91 ! LA 1.02 MK 0.95 NL 1.06 ON 1.71 ! OV 1.00 PT 1.01 ZC 0.61 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.96 EF 1.00* FD 1.10 KP 0.91 ! LA 1.01 MC 1.10 NL 0.96 ON 1.32 ! OV 1.00 PT 1.07 SC 1.02 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 EF 1.00* FD 1.02 KP 0.94 ! LA 1.05 MK 0.98 NL 1.04 ON 1.25 ! OV 0.95 PT 0.96 SC 0.96 ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* FD 0.96 KP 1.00 LA 0.99 ! NL 0.99 ON 1.21 OV 1.06 PT 0.94 ! SC 1.06 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 1.08 KP 0.87 LA 1.03 ! MK 0.97 NL 1.02 ON 1.05 OV 0.96 ! PT 0.94 SC 1.10 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.95 EF 1.00* FD 1.02 KP 0.85 ! LA 1.09 MK 0.96 NL 1.06 OV 1.03 ! PT 1.02 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 0.98 EF 1.00* FD 0.97 KP 0.99 ! LA 1.02 MK 1.02 NL 1.03 ON 1.99 ! OV 0.93 PT 0.91 ZC 0.62 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.97 EF 1.00* FD 1.08 KP 0.93 ! LA 0.98 MC 1.24 NL 0.96 ON 1.16 ! OV 1.01 PT 0.98 SC 0.99 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 EF 1.00* FD 1.00 KP 0.90 ! LA 1.04 MK 0.99 NL 1.00 ON 1.23 ! OV 0.93 PT 1.04 SC 1.01 ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* FD 1.01 KP 0.94 LA 1.05 ! NL 1.05 ON 1.14 OV 1.02 PT 0.95 ! SC 1.03 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 1.07 KP 0.94 LA 1.11 ! MK 1.00 NL 0.92 ON 1.31 OV 1.00 ! PT 0.98 SC 0.91 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.01 EF 1.00* FD 1.00 KP 0.96 ! LA 1.00 MK 0.97 NL 0.94 OV 1.00 ! PT 1.02 ! ! ! Fit before self-cal, rms=0.072255Jy sigma=0.663623 ! Fit after self-cal, rms=0.073610Jy sigma=0.659752 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 milli-arcsec ! Estimated beam: bmin=0.7322 mas, bmaj=1.232 mas, bpa=-28.29 degrees ! Estimated noise=0.279271 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 = 4.1428e-05 Jy ! Component: 100 - total flux cleaned = 3.5015e-05 Jy ! Component: 150 - total flux cleaned = 3.49426e-05 Jy ! Component: 200 - total flux cleaned = 2.9965e-05 Jy ! Total flux subtracted in 200 components = 2.9965e-05 Jy ! Clean residual min=-0.000745 max=0.000794 Jy/beam ! Clean residual mean=0.000000 rms=0.000180 Jy/beam ! Combined flux in latest and established models = 0.0693459 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 13 components and 0.0693459 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=0.073609Jy sigma=0.659748 ! Fit after self-cal, rms=0.073675Jy sigma=0.659519 ! Inverting map ! Your choice of large map pixels excluded 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 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=0.073675Jy sigma=0.659519 ! Fit after self-cal, rms=0.074260Jy sigma=0.659316 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 milli-arcsec ! Estimated beam: bmin=0.7326 mas, bmaj=1.232 mas, bpa=-28.32 degrees ! Estimated noise=0.279825 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000134849 Jy ! Component: 100 - total flux cleaned = 0.000134671 Jy ! Component: 150 - total flux cleaned = 0.000126185 Jy ! Component: 200 - total flux cleaned = 0.000122564 Jy ! Total flux subtracted in 200 components = 0.000122564 Jy ! Clean residual min=-0.000758 max=0.000742 Jy/beam ! Clean residual mean=0.000000 rms=0.000180 Jy/beam ! Combined flux in latest and established models = 0.0694685 Jy selfcal ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 14 components and 0.0694685 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=0.074259Jy sigma=0.659314 ! Fit after self-cal, rms=0.074270Jy sigma=0.659303 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 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 = -3.93772e-06 Jy ! Component: 100 - total flux cleaned = -2.20162e-07 Jy ! Component: 150 - total flux cleaned = 3.15451e-06 Jy ! Component: 200 - total flux cleaned = 3.152e-06 Jy ! Total flux subtracted in 200 components = 3.152e-06 Jy ! Clean residual min=-0.000752 max=0.000741 Jy/beam ! Clean residual mean=0.000000 rms=0.000180 Jy/beam ! Combined flux in latest and established models = 0.0694716 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 16 components and 0.0694716 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=0.074269Jy sigma=0.659300 ! Fit after self-cal, rms=0.074269Jy sigma=0.659301 ! Inverting map ! Your choice of large map pixels excluded 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 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=0.074269Jy sigma=0.659301 ! Fit after self-cal, rms=0.074514Jy sigma=0.659287 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 milli-arcsec ! Estimated beam: bmin=0.7329 mas, bmaj=1.23 mas, bpa=-28.36 degrees ! Estimated noise=0.28049 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000169284 Jy ! Component: 100 - total flux cleaned = 0.000169252 Jy ! Component: 150 - total flux cleaned = 0.000165214 Jy ! Component: 200 - total flux cleaned = 0.000168775 Jy ! Total flux subtracted in 200 components = 0.000168775 Jy ! Clean residual min=-0.000758 max=0.000743 Jy/beam ! Clean residual mean=0.000000 rms=0.000180 Jy/beam ! Combined flux in latest and established models = 0.0696404 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 17 components and 0.0696404 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=0.074513Jy sigma=0.659284 ! Fit after self-cal, rms=0.074514Jy sigma=0.659285 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 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 = -3.73763e-07 Jy ! Component: 100 - total flux cleaned = -6.13921e-07 Jy ! Component: 150 - total flux cleaned = -8.86972e-07 Jy ! Component: 200 - total flux cleaned = -8.95881e-07 Jy ! Total flux subtracted in 200 components = -8.95881e-07 Jy ! Clean residual min=-0.000756 max=0.000743 Jy/beam ! Clean residual mean=0.000000 rms=0.000180 Jy/beam ! Combined flux in latest and established models = 0.0696395 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 18 components and 0.0696395 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=0.074513Jy sigma=0.659283 ! Fit after self-cal, rms=0.074512Jy sigma=0.659283 ! Inverting map ! Your choice of large map pixels excluded 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 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=0.074512Jy sigma=0.659283 ! Fit after self-cal, rms=0.074697Jy sigma=0.659272 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 milli-arcsec ! Estimated beam: bmin=2.44 mas, bmaj=3.122 mas, bpa=-1.026 degrees ! Estimated noise=0.354703 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000240271 Jy ! Component: 100 - total flux cleaned = 0.000321447 Jy ! Component: 150 - total flux cleaned = 0.000337261 Jy ! Component: 200 - total flux cleaned = 0.000339552 Jy ! Total flux subtracted in 200 components = 0.000339552 Jy ! Clean residual min=-0.000803 max=0.000743 Jy/beam ! Clean residual mean=-0.000000 rms=0.000212 Jy/beam ! Combined flux in latest and established models = 0.0699791 Jy selfcal ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 19 components and 0.0699791 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=0.074696Jy sigma=0.659274 ! Fit after self-cal, rms=0.074697Jy sigma=0.659272 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 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 = 1.27269e-05 Jy ! Component: 100 - total flux cleaned = 1.39502e-05 Jy ! Component: 150 - total flux cleaned = 1.72068e-05 Jy ! Component: 200 - total flux cleaned = 1.93057e-05 Jy ! Total flux subtracted in 200 components = 1.93057e-05 Jy ! Clean residual min=-0.000804 max=0.000745 Jy/beam ! Clean residual mean=-0.000000 rms=0.000212 Jy/beam ! Combined flux in latest and established models = 0.0699984 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 19 components and 0.0699984 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=0.074697Jy sigma=0.659274 ! Fit after self-cal, rms=0.074698Jy sigma=0.659274 ! Inverting map ! Your choice of large map pixels excluded 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 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 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 milli-arcsec ! Estimated beam: bmin=0.7333 mas, bmaj=1.229 mas, bpa=-28.39 degrees ! Estimated noise=0.281168 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7333 x 1.229 at -28.39 degrees (North through East) ! Clean map min=-0.00065964 max=0.06576 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 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 milli-arcsec ! Estimated beam: bmin=0.5074 mas, bmaj=0.9423 mas, bpa=-35.05 degrees ! Estimated noise=0.662964 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0512398 Jy ! Component: 100 - total flux cleaned = 0.0624738 Jy ! Component: 150 - total flux cleaned = 0.0658362 Jy ! Component: 200 - total flux cleaned = 0.0669644 Jy ! Total flux subtracted in 200 components = 0.0669644 Jy ! Clean residual min=-0.001876 max=0.001914 Jy/beam ! Clean residual mean=0.000000 rms=0.000417 Jy/beam ! Combined flux in latest and established models = 0.0669644 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 11 model components to the UV plane model. ! The established model now contains 11 components and 0.0669644 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 milli-arcsec ! Estimated beam: bmin=0.7333 mas, bmaj=1.229 mas, bpa=-28.39 degrees ! Estimated noise=0.281168 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 = 0.00149673 Jy ! Component: 100 - total flux cleaned = 0.00215234 Jy ! Component: 150 - total flux cleaned = 0.0024729 Jy ! Component: 200 - total flux cleaned = 0.00263364 Jy ! Total flux subtracted in 200 components = 0.00263364 Jy ! Clean residual min=-0.000767 max=0.000740 Jy/beam ! Clean residual mean=0.000000 rms=0.000181 Jy/beam ! Combined flux in latest and established models = 0.0695981 Jy ! Adding 13 model components to the UV plane model. ! The established model now contains 21 components and 0.0695981 Jy ! Inverting map ! Your choice of large map pixels excluded 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 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 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 milli-arcsec ! Estimated beam: bmin=2.44 mas, bmaj=3.122 mas, bpa=-1.026 degrees ! Estimated noise=0.354703 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000200041 Jy ! Component: 100 - total flux cleaned = 0.000259334 Jy ! Component: 150 - total flux cleaned = 0.000263036 Jy ! Component: 200 - total flux cleaned = 0.000268358 Jy ! Total flux subtracted in 200 components = 0.000268358 Jy ! Clean residual min=-0.000801 max=0.000744 Jy/beam ! Clean residual mean=-0.000000 rms=0.000212 Jy/beam ! Combined flux in latest and established models = 0.0698664 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 = 3.44048e-06 Jy ! Component: 100 - total flux cleaned = 6.89011e-06 Jy ! Component: 150 - total flux cleaned = 1.03276e-05 Jy ! Component: 200 - total flux cleaned = 1.52478e-05 Jy ! Total flux subtracted in 200 components = 1.52478e-05 Jy ! Clean residual min=-0.000802 max=0.000743 Jy/beam ! Clean residual mean=-0.000000 rms=0.000212 Jy/beam ! Combined flux in latest and established models = 0.0698817 Jy ! Adding 5 model components to the UV plane model. ! The established model now contains 23 components and 0.0698817 Jy ! Inverting map ! Your choice of large map pixels excluded 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 milli-arcsec ! Estimated beam: bmin=0.7333 mas, bmaj=1.229 mas, bpa=-28.39 degrees ! Estimated noise=0.281168 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000126881 Jy ! Component: 100 - total flux cleaned = -0.000142437 Jy ! Component: 150 - total flux cleaned = -0.000148831 Jy ! Component: 200 - total flux cleaned = -0.000148876 Jy ! Total flux subtracted in 200 components = -0.000148876 Jy ! Clean residual min=-0.000761 max=0.000739 Jy/beam ! Clean residual mean=0.000000 rms=0.000180 Jy/beam ! Combined flux in latest and established models = 0.0697328 Jy selfcal ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 25 components and 0.0697328 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=0.074696Jy sigma=0.659279 ! Fit after self-cal, rms=0.074695Jy sigma=0.659274 wmodel /scr/pima/gb073_uvs/J1539+4735_X_map.mod ! Writing 25 model components to file: /scr/pima/gb073_uvs/J1539+4735_X_map.mod wobs /scr/pima/gb073_uvs/J1539+4735_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1539+4735_X_uvs.fits wwins /scr/pima/gb073_uvs/J1539+4735_X_map.win ! wwins: Wrote 1 windows to /scr/pima/gb073_uvs/J1539+4735_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 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 8.36433e-05 Jy ! Component: 100 - total flux cleaned = 0.000138519 Jy ! Component: 150 - total flux cleaned = 0.000138141 Jy ! Component: 200 - total flux cleaned = 0.000164058 Jy ! Component: 250 - total flux cleaned = 0.00015155 Jy ! Component: 300 - total flux cleaned = 0.00013956 Jy ! Component: 350 - total flux cleaned = 0.000201137 Jy ! Component: 400 - total flux cleaned = 0.000249502 Jy ! Component: 450 - total flux cleaned = 0.000249564 Jy ! Component: 500 - total flux cleaned = 0.000296757 Jy ! Component: 550 - total flux cleaned = 0.000273355 Jy ! Component: 600 - total flux cleaned = 0.000261847 Jy ! Component: 650 - total flux cleaned = 0.000238902 Jy ! Component: 700 - total flux cleaned = 0.000272921 Jy ! Component: 750 - total flux cleaned = 0.000205406 Jy ! Component: 800 - total flux cleaned = 0.000227846 Jy ! Component: 850 - total flux cleaned = 0.000216697 Jy ! Component: 900 - total flux cleaned = 0.000205786 Jy ! Component: 950 - total flux cleaned = 0.000194796 Jy ! Component: 1000 - total flux cleaned = 0.000216576 Jy ! Component: 1050 - total flux cleaned = 0.000184279 Jy ! Component: 1100 - total flux cleaned = 0.000216558 Jy ! Component: 1150 - total flux cleaned = 0.000205825 Jy ! Component: 1200 - total flux cleaned = 0.000195156 Jy ! Component: 1250 - total flux cleaned = 0.000163522 Jy ! Component: 1300 - total flux cleaned = 0.000163467 Jy ! Component: 1350 - total flux cleaned = 0.000173968 Jy ! Component: 1400 - total flux cleaned = 0.000184338 Jy ! Component: 1450 - total flux cleaned = 0.00015327 Jy ! Component: 1500 - total flux cleaned = 0.000122415 Jy ! Component: 1550 - total flux cleaned = 0.000112205 Jy ! Component: 1600 - total flux cleaned = 6.1341e-05 Jy ! Component: 1650 - total flux cleaned = 3.0886e-05 Jy ! Component: 1700 - total flux cleaned = 4.10097e-05 Jy ! Component: 1750 - total flux cleaned = -9.18702e-06 Jy ! Component: 1800 - total flux cleaned = 8.16505e-07 Jy ! Component: 1850 - total flux cleaned = -6.88901e-05 Jy ! Component: 1900 - total flux cleaned = -5.89688e-05 Jy ! Component: 1950 - total flux cleaned = -0.000108397 Jy ! Component: 2000 - total flux cleaned = -0.000118142 Jy ! Component: 2050 - total flux cleaned = -7.89233e-05 Jy ! Component: 2100 - total flux cleaned = -0.000137543 Jy ! Component: 2150 - total flux cleaned = -0.000156955 Jy ! Component: 2200 - total flux cleaned = -0.000205376 Jy ! Component: 2250 - total flux cleaned = -0.000166785 Jy ! Component: 2300 - total flux cleaned = -0.000186001 Jy ! Component: 2350 - total flux cleaned = -0.000233954 Jy ! Component: 2400 - total flux cleaned = -0.000233952 Jy ! Component: 2450 - total flux cleaned = -0.000281533 Jy ! Component: 2500 - total flux cleaned = -0.000309945 Jy ! Component: 2550 - total flux cleaned = -0.000300532 Jy ! Component: 2600 - total flux cleaned = -0.000291134 Jy ! Component: 2650 - total flux cleaned = -0.000309877 Jy ! Component: 2700 - total flux cleaned = -0.000300555 Jy ! Component: 2750 - total flux cleaned = -0.000356423 Jy ! Component: 2800 - total flux cleaned = -0.000319236 Jy ! Component: 2850 - total flux cleaned = -0.000383979 Jy ! Component: 2900 - total flux cleaned = -0.000356335 Jy ! Component: 2950 - total flux cleaned = -0.000347125 Jy ! Component: 3000 - total flux cleaned = -0.000392911 Jy ! Component: 3050 - total flux cleaned = -0.000392885 Jy ! Component: 3100 - total flux cleaned = -0.000402085 Jy ! Component: 3150 - total flux cleaned = -0.000420208 Jy ! Component: 3200 - total flux cleaned = -0.000429256 Jy ! Component: 3250 - total flux cleaned = -0.000429261 Jy ! Component: 3300 - total flux cleaned = -0.000411269 Jy ! Component: 3350 - total flux cleaned = -0.0004113 Jy ! Component: 3400 - total flux cleaned = -0.00042027 Jy ! Component: 3450 - total flux cleaned = -0.000438097 Jy ! Component: 3500 - total flux cleaned = -0.000455949 Jy ! Component: 3550 - total flux cleaned = -0.000438231 Jy ! Component: 3600 - total flux cleaned = -0.00042939 Jy ! Component: 3650 - total flux cleaned = -0.000447076 Jy ! Component: 3700 - total flux cleaned = -0.000455867 Jy ! Component: 3750 - total flux cleaned = -0.000438286 Jy ! Component: 3800 - total flux cleaned = -0.000455801 Jy ! Component: 3850 - total flux cleaned = -0.000429593 Jy ! Component: 3900 - total flux cleaned = -0.000464474 Jy ! Component: 3950 - total flux cleaned = -0.000464474 Jy ! Component: 4000 - total flux cleaned = -0.000507844 Jy ! Component: 4050 - total flux cleaned = -0.000499167 Jy ! Total flux subtracted in 4096 components = -0.000473243 Jy ! Clean residual min=-0.000543 max=0.000554 Jy/beam ! Clean residual mean=0.000000 rms=0.000144 Jy/beam ! Combined flux in latest and established models = 0.0692595 Jy keep ! Adding 361 model components to the UV plane model. ! The established model now contains 386 components and 0.0692596 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1539+4735_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7333 x 1.229 at -28.39 degrees (North through East) ! Clean map min=-0.00064458 max=0.066135 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1539+4735_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0661355 invert ! Inverting map ! Your choice of large map pixels excluded 0.397% of the data. ! The x-axis pixel size should ideally be below 0.1781 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000144338 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.654739 0.654739 1.30948 2.61896 5.23791 10.4758 20.9516 41.9033 83.8066 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0004 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.066 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 458.197 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1539+4735_X_uvs.log closed on Sat Dec 26 09:41:56 2015