! Started logfile: /scr/pima/gb073_uvs/J1314+2348_X_uvs.log on Sat Dec 26 09:39:33 2015 obs /scr/pima/gb073_uvs/J1314+2348_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1314+2348_X_uva.fits ! AN table 1: 29 integrations on 55 of 55 possible baselines. ! AN table 2: 29 integrations on 78 of 78 possible baselines. ! AN table 3: 29 integrations on 36 of 36 possible baselines. ! AN table 4: 29 integrations on 55 of 55 possible baselines. ! AN table 5: 29 integrations on 45 of 45 possible baselines. ! Apparent sampling: 0.858223 visibilities/baseline/integration-bin. ! Found source: J1314+2348 ! ! 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 53560 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/J1314+2348_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 39 telescope corrections were flagged in sub-array 1. ! A total of 30 telescope corrections were flagged in sub-array 2. ! A total of 38 telescope corrections were flagged in sub-array 4. ! A total of 42 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 2. ! A total of 39 telescope corrections were flagged in sub-array 1. ! A total of 30 telescope corrections were flagged in sub-array 2. ! A total of 38 telescope corrections were flagged in sub-array 4. ! A total of 42 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 3. ! A total of 39 telescope corrections were flagged in sub-array 1. ! A total of 30 telescope corrections were flagged in sub-array 2. ! A total of 38 telescope corrections were flagged in sub-array 4. ! A total of 42 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 4. ! A total of 39 telescope corrections were flagged in sub-array 1. ! A total of 30 telescope corrections were flagged in sub-array 2. ! A total of 38 telescope corrections were flagged in sub-array 4. ! A total of 42 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 5. ! A total of 68 telescope corrections were flagged in sub-array 1. ! A total of 59 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 67 telescope corrections were flagged in sub-array 4. ! A total of 71 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 6. ! A total of 68 telescope corrections were flagged in sub-array 1. ! A total of 59 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 67 telescope corrections were flagged in sub-array 4. ! A total of 71 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 7. ! A total of 39 telescope corrections were flagged in sub-array 1. ! A total of 30 telescope corrections were flagged in sub-array 2. ! A total of 38 telescope corrections were flagged in sub-array 4. ! A total of 42 telescope corrections were flagged in sub-array 5. ! ! Correcting IF 8. ! A total of 39 telescope corrections were flagged in sub-array 1. ! A total of 30 telescope corrections were flagged in sub-array 2. ! A total of 38 telescope corrections were flagged in sub-array 4. ! A total of 42 telescope corrections were flagged in sub-array 5. ! ! Fit before self-cal, rms=1.007781Jy sigma=9.168373 ! Fit after self-cal, rms=0.912338Jy sigma=8.268885 ! 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 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 milli-arcsec ! Estimated beam: bmin=0.465 mas, bmaj=1.164 mas, bpa=-6.305 degrees ! Estimated noise=0.879276 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 = 0.0657464 Jy ! Component: 100 - total flux cleaned = 0.0811743 Jy ! Total flux subtracted in 100 components = 0.0811743 Jy ! Clean residual min=-0.003487 max=0.006347 Jy/beam ! Clean residual mean=0.000001 rms=0.000783 Jy/beam ! Combined flux in latest and established models = 0.0811743 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 0.0811743 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=0.090853Jy sigma=0.701844 ! Fit after self-cal, rms=0.090427Jy sigma=0.699329 ! Inverting map ! Your choice of large map pixels excluded 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00768693 Jy ! Component: 100 - total flux cleaned = 0.0124337 Jy ! Total flux subtracted in 100 components = 0.0124337 Jy ! Clean residual min=-0.003074 max=0.005202 Jy/beam ! Clean residual mean=0.000001 rms=0.000716 Jy/beam ! Combined flux in latest and established models = 0.093608 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 11 components and 0.093608 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=0.089160Jy sigma=0.681604 ! Fit after self-cal, rms=0.089134Jy sigma=0.681444 ! Inverting map ! Your choice of large map pixels excluded 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 milli-arcsec ! Added new window around map position (-0.8, 0.2). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00531828 Jy ! Component: 100 - total flux cleaned = 0.00865299 Jy ! Total flux subtracted in 100 components = 0.00865299 Jy ! Clean residual min=-0.002994 max=0.003743 Jy/beam ! Clean residual mean=0.000000 rms=0.000681 Jy/beam ! Combined flux in latest and established models = 0.102261 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 18 components and 0.102261 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=0.088556Jy sigma=0.673916 ! Fit after self-cal, rms=0.088512Jy sigma=0.673430 ! Inverting map ! Your choice of large map pixels excluded 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 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 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 milli-arcsec ! Estimated beam: bmin=0.6304 mas, bmaj=1.408 mas, bpa=-5.598 degrees ! Estimated noise=0.375439 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 = 0.00612767 Jy ! Component: 100 - total flux cleaned = 0.00916842 Jy ! Component: 150 - total flux cleaned = 0.0108251 Jy ! Component: 200 - total flux cleaned = 0.0117513 Jy ! Total flux subtracted in 200 components = 0.0117513 Jy ! Clean residual min=-0.001635 max=0.002322 Jy/beam ! Clean residual mean=-0.000002 rms=0.000396 Jy/beam ! Combined flux in latest and established models = 0.114012 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 31 components and 0.114012 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=0.088221Jy sigma=0.669574 ! Fit after self-cal, rms=0.088199Jy sigma=0.669272 ! Inverting map ! Your choice of large map pixels excluded 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 milli-arcsec ! Added new window around map position (-1.6, 1). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0017693 Jy ! Component: 100 - total flux cleaned = 0.00211731 Jy ! Component: 150 - total flux cleaned = 0.0021981 Jy ! Component: 200 - total flux cleaned = 0.00219656 Jy ! Total flux subtracted in 200 components = 0.00219656 Jy ! Clean residual min=-0.001603 max=0.001909 Jy/beam ! Clean residual mean=-0.000002 rms=0.000369 Jy/beam ! Combined flux in latest and established models = 0.116209 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 48 components and 0.116209 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=0.088121Jy sigma=0.668650 ! Fit after self-cal, rms=0.088117Jy sigma=0.668550 ! Inverting map ! Your choice of large map pixels excluded 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6304 x 1.408 at -5.598 degrees (North through East) ! Clean map min=-0.0014623 max=0.087018 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. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! 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* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.00 KP 0.94 LA 1.04 ! MK 1.03 NL 0.94 OV 1.02 PT 0.93 ! SC 1.02 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.91 EF 1.00* FD 1.09 KP 1.03 ! LA 1.01 MC 1.00 NL 0.94 ON 0.96 ! PT 0.94 SC 0.95 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! 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* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.05 KP 0.99 LA 1.05 ! MK 1.06 NL 0.99 OV 1.00 PT 1.03 ! SC 1.12 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.05 EF 1.00* FD 1.02 KP 1.01 ! LA 1.01 MC 0.94 NL 1.02 ON 0.89 ! PT 1.06 SC 0.99 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! 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* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.10 FD 0.99 KP 0.93 LA 1.01 ! MK 0.93 NL 0.88 OV 0.99 PT 1.02 ! SC 1.08 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.05 EF 1.00* FD 1.03 KP 0.96 ! LA 0.96 MC 0.89 NL 0.95 ON 1.11 ! PT 1.05 SC 0.99 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! 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* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 1.03 KP 1.00 LA 1.01 ! MK 0.95 NL 1.00 OV 1.06 PT 1.07 ! SC 1.13 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00 EF 1.00* FD 1.05 KP 0.95 ! LA 0.97 MC 1.03 NL 1.02 ON 0.92 ! PT 1.06 SC 0.94 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! 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* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! 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* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! 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* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.13 KP 0.86 LA 1.04 ! MK 1.02 NL 1.06 OV 1.08 PT 1.00 ! SC 1.02 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* OV 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! 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* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.05 FD 1.05 KP 0.95 LA 1.07 ! MK 1.01 NL 0.95 OV 0.99 PT 1.02 ! SC 1.00 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ! ! ! Fit before self-cal, rms=0.088117Jy sigma=0.668550 ! Fit after self-cal, rms=0.088087Jy sigma=0.667595 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 milli-arcsec ! Estimated beam: bmin=0.6292 mas, bmaj=1.405 mas, bpa=-5.646 degrees ! Estimated noise=0.376128 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 = 0.000901208 Jy ! Component: 100 - total flux cleaned = 0.00101449 Jy ! Component: 150 - total flux cleaned = 0.00108466 Jy ! Component: 200 - total flux cleaned = 0.00110584 Jy ! Total flux subtracted in 200 components = 0.00110584 Jy ! Clean residual min=-0.001584 max=0.001629 Jy/beam ! Clean residual mean=-0.000001 rms=0.000347 Jy/beam ! Combined flux in latest and established models = 0.117315 Jy ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 52 components and 0.117315 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=0.088068Jy sigma=0.667461 ! Fit after self-cal, rms=0.088070Jy sigma=0.667419 ! Inverting map ! Your choice of large map pixels excluded 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 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=0.088070Jy sigma=0.667419 ! Fit after self-cal, rms=0.088024Jy sigma=0.667414 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 milli-arcsec ! Estimated beam: bmin=0.6291 mas, bmaj=1.405 mas, bpa=-5.656 degrees ! Estimated noise=0.375972 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00032939 Jy ! Component: 100 - total flux cleaned = 0.000373571 Jy ! Component: 150 - total flux cleaned = 0.000373669 Jy ! Component: 200 - total flux cleaned = 0.000373539 Jy ! Total flux subtracted in 200 components = 0.000373539 Jy ! Clean residual min=-0.001583 max=0.001542 Jy/beam ! Clean residual mean=-0.000001 rms=0.000345 Jy/beam ! Combined flux in latest and established models = 0.117688 Jy selfcal ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 55 components and 0.117688 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=0.088013Jy sigma=0.667332 ! Fit after self-cal, rms=0.088013Jy sigma=0.667320 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000132995 Jy ! Component: 100 - total flux cleaned = 0.000132855 Jy ! Component: 150 - total flux cleaned = 0.000133691 Jy ! Component: 200 - total flux cleaned = 0.000150333 Jy ! Total flux subtracted in 200 components = 0.000150333 Jy ! Clean residual min=-0.001584 max=0.001547 Jy/beam ! Clean residual mean=-0.000001 rms=0.000344 Jy/beam ! Combined flux in latest and established models = 0.117839 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 56 components and 0.117839 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=0.088008Jy sigma=0.667281 ! Fit after self-cal, rms=0.088008Jy sigma=0.667274 ! Inverting map ! Your choice of large map pixels excluded 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 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=0.088008Jy sigma=0.667274 ! Fit after self-cal, rms=0.087920Jy sigma=0.667269 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 milli-arcsec ! Estimated beam: bmin=0.629 mas, bmaj=1.405 mas, bpa=-5.668 degrees ! Estimated noise=0.375558 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 4.89084e-05 Jy ! Component: 100 - total flux cleaned = 6.68742e-05 Jy ! Component: 150 - total flux cleaned = 6.68316e-05 Jy ! Component: 200 - total flux cleaned = 6.66868e-05 Jy ! Total flux subtracted in 200 components = 6.66868e-05 Jy ! Clean residual min=-0.001573 max=0.001561 Jy/beam ! Clean residual mean=-0.000001 rms=0.000344 Jy/beam ! Combined flux in latest and established models = 0.117905 Jy selfcal ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 59 components and 0.117905 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=0.087915Jy sigma=0.667226 ! Fit after self-cal, rms=0.087915Jy sigma=0.667218 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 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 = 5.09367e-05 Jy ! Component: 100 - total flux cleaned = 6.67972e-05 Jy ! Component: 150 - total flux cleaned = 6.69807e-05 Jy ! Component: 200 - total flux cleaned = 8.13629e-05 Jy ! Total flux subtracted in 200 components = 8.13629e-05 Jy ! Clean residual min=-0.001571 max=0.001565 Jy/beam ! Clean residual mean=-0.000001 rms=0.000343 Jy/beam ! Combined flux in latest and established models = 0.117987 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 63 components and 0.117987 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=0.087909Jy sigma=0.667189 ! Fit after self-cal, rms=0.087909Jy sigma=0.667180 ! Inverting map ! Your choice of large map pixels excluded 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 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=0.087909Jy sigma=0.667180 ! Fit after self-cal, rms=0.087747Jy sigma=0.666918 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 milli-arcsec ! Estimated beam: bmin=2.865 mas, bmaj=3.018 mas, bpa=-51.47 degrees ! Estimated noise=0.473422 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000183385 Jy ! Component: 100 - total flux cleaned = 0.000243589 Jy ! Component: 150 - total flux cleaned = 0.000244217 Jy ! Component: 200 - total flux cleaned = 0.000235288 Jy ! Total flux subtracted in 200 components = 0.000235288 Jy ! Clean residual min=-0.001856 max=0.001732 Jy/beam ! Clean residual mean=-0.000002 rms=0.000479 Jy/beam ! Combined flux in latest and established models = 0.118222 Jy selfcal ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 68 components and 0.118222 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=0.087734Jy sigma=0.666847 ! Fit after self-cal, rms=0.087737Jy sigma=0.666825 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000121051 Jy ! Component: 100 - total flux cleaned = 0.000158981 Jy ! Component: 150 - total flux cleaned = 0.000159377 Jy ! Component: 200 - total flux cleaned = 0.000159404 Jy ! Total flux subtracted in 200 components = 0.000159404 Jy ! Clean residual min=-0.001855 max=0.001712 Jy/beam ! Clean residual mean=-0.000002 rms=0.000477 Jy/beam ! Combined flux in latest and established models = 0.118381 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 70 components and 0.118381 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=0.087729Jy sigma=0.666789 ! Fit after self-cal, rms=0.087731Jy sigma=0.666787 ! Inverting map ! Your choice of large map pixels excluded 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 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 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 milli-arcsec ! Estimated beam: bmin=0.629 mas, bmaj=1.404 mas, bpa=-5.653 degrees ! Estimated noise=0.375286 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.629 x 1.404 at -5.653 degrees (North through East) ! Clean map min=-0.001483 max=0.08623 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 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 milli-arcsec ! Estimated beam: bmin=0.4643 mas, bmaj=1.162 mas, bpa=-6.356 degrees ! Estimated noise=0.876957 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0655796 Jy ! Component: 100 - total flux cleaned = 0.0816374 Jy ! Component: 150 - total flux cleaned = 0.0905649 Jy ! Component: 200 - total flux cleaned = 0.0969067 Jy ! Total flux subtracted in 200 components = 0.0969067 Jy ! Clean residual min=-0.003015 max=0.003780 Jy/beam ! Clean residual mean=0.000001 rms=0.000692 Jy/beam ! Combined flux in latest and established models = 0.0969067 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 0.0969067 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 milli-arcsec ! Estimated beam: bmin=0.629 mas, bmaj=1.404 mas, bpa=-5.653 degrees ! Estimated noise=0.375286 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 = 0.00938751 Jy ! Component: 100 - total flux cleaned = 0.0142145 Jy ! Component: 150 - total flux cleaned = 0.0170958 Jy ! Component: 200 - total flux cleaned = 0.0189394 Jy ! Total flux subtracted in 200 components = 0.0189394 Jy ! Clean residual min=-0.001654 max=0.001634 Jy/beam ! Clean residual mean=-0.000001 rms=0.000353 Jy/beam ! Combined flux in latest and established models = 0.115846 Jy ! Adding 36 model components to the UV plane model. ! The established model now contains 42 components and 0.115846 Jy ! Inverting map ! Your choice of large map pixels excluded 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 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 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 milli-arcsec ! Estimated beam: bmin=2.865 mas, bmaj=3.018 mas, bpa=-51.47 degrees ! Estimated noise=0.473422 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00166979 Jy ! Component: 100 - total flux cleaned = 0.00200794 Jy ! Component: 150 - total flux cleaned = 0.00218685 Jy ! Component: 200 - total flux cleaned = 0.00231727 Jy ! Total flux subtracted in 200 components = 0.00231727 Jy ! Clean residual min=-0.001904 max=0.001839 Jy/beam ! Clean residual mean=-0.000002 rms=0.000479 Jy/beam ! Combined flux in latest and established models = 0.118163 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 = 8.35837e-05 Jy ! Component: 100 - total flux cleaned = 0.000147902 Jy ! Component: 150 - total flux cleaned = 0.000148259 Jy ! Component: 200 - total flux cleaned = 0.000156474 Jy ! Total flux subtracted in 200 components = 0.000156474 Jy ! Clean residual min=-0.001867 max=0.001763 Jy/beam ! Clean residual mean=-0.000002 rms=0.000478 Jy/beam ! Combined flux in latest and established models = 0.11832 Jy ! Adding 24 model components to the UV plane model. ! The established model now contains 58 components and 0.11832 Jy ! Inverting map ! Your choice of large map pixels excluded 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 milli-arcsec ! Estimated beam: bmin=0.629 mas, bmaj=1.404 mas, bpa=-5.653 degrees ! Estimated noise=0.375286 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000308611 Jy ! Component: 100 - total flux cleaned = -0.000309341 Jy ! Component: 150 - total flux cleaned = -0.000309689 Jy ! Component: 200 - total flux cleaned = -0.000310278 Jy ! Total flux subtracted in 200 components = -0.000310278 Jy ! Clean residual min=-0.001515 max=0.001453 Jy/beam ! Clean residual mean=-0.000001 rms=0.000337 Jy/beam ! Combined flux in latest and established models = 0.11801 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 64 components and 0.11801 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=0.087727Jy sigma=0.666792 ! Fit after self-cal, rms=0.087711Jy sigma=0.666701 wmodel /scr/pima/gb073_uvs/J1314+2348_X_map.mod ! Writing 64 model components to file: /scr/pima/gb073_uvs/J1314+2348_X_map.mod wobs /scr/pima/gb073_uvs/J1314+2348_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1314+2348_X_uvs.fits wwins /scr/pima/gb073_uvs/J1314+2348_X_map.win ! wwins: Wrote 3 windows to /scr/pima/gb073_uvs/J1314+2348_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 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000192494 Jy ! Component: 100 - total flux cleaned = -0.000371077 Jy ! Component: 150 - total flux cleaned = -0.000274979 Jy ! Component: 200 - total flux cleaned = -0.000228798 Jy ! Component: 250 - total flux cleaned = -0.000251268 Jy ! Component: 300 - total flux cleaned = -0.000228269 Jy ! Component: 350 - total flux cleaned = -0.000205892 Jy ! Component: 400 - total flux cleaned = -0.000162606 Jy ! Component: 450 - total flux cleaned = -0.00014146 Jy ! Component: 500 - total flux cleaned = -0.0001626 Jy ! Component: 550 - total flux cleaned = -0.000265294 Jy ! Component: 600 - total flux cleaned = -0.000345944 Jy ! Component: 650 - total flux cleaned = -0.000365694 Jy ! Component: 700 - total flux cleaned = -0.000444708 Jy ! Component: 750 - total flux cleaned = -0.000464194 Jy ! Component: 800 - total flux cleaned = -0.000444918 Jy ! Component: 850 - total flux cleaned = -0.000559861 Jy ! Component: 900 - total flux cleaned = -0.000654489 Jy ! Component: 950 - total flux cleaned = -0.000766829 Jy ! Component: 1000 - total flux cleaned = -0.00076679 Jy ! Component: 1050 - total flux cleaned = -0.000914176 Jy ! Component: 1100 - total flux cleaned = -0.000950823 Jy ! Component: 1150 - total flux cleaned = -0.00104142 Jy ! Component: 1200 - total flux cleaned = -0.00114909 Jy ! Component: 1250 - total flux cleaned = -0.00122033 Jy ! Component: 1300 - total flux cleaned = -0.0012735 Jy ! Component: 1350 - total flux cleaned = -0.00129085 Jy ! Component: 1400 - total flux cleaned = -0.0013781 Jy ! Component: 1450 - total flux cleaned = -0.00141272 Jy ! Component: 1500 - total flux cleaned = -0.00148165 Jy ! Component: 1550 - total flux cleaned = -0.0015841 Jy ! Component: 1600 - total flux cleaned = -0.0015669 Jy ! Component: 1650 - total flux cleaned = -0.00158386 Jy ! Component: 1700 - total flux cleaned = -0.00163435 Jy ! Component: 1750 - total flux cleaned = -0.00171749 Jy ! Component: 1800 - total flux cleaned = -0.00175063 Jy ! Component: 1850 - total flux cleaned = -0.00181636 Jy ! Component: 1900 - total flux cleaned = -0.00189799 Jy ! Component: 1950 - total flux cleaned = -0.00204424 Jy ! Component: 2000 - total flux cleaned = -0.00202802 Jy ! Component: 2050 - total flux cleaned = -0.0020923 Jy ! Component: 2100 - total flux cleaned = -0.0021721 Jy ! Component: 2150 - total flux cleaned = -0.00215618 Jy ! Component: 2200 - total flux cleaned = -0.00228251 Jy ! Component: 2250 - total flux cleaned = -0.00232952 Jy ! Component: 2300 - total flux cleaned = -0.00234509 Jy ! Component: 2350 - total flux cleaned = -0.0024539 Jy ! Component: 2400 - total flux cleaned = -0.00251592 Jy ! Component: 2450 - total flux cleaned = -0.00251596 Jy ! Component: 2500 - total flux cleaned = -0.00262325 Jy ! Component: 2550 - total flux cleaned = -0.00262318 Jy ! Component: 2600 - total flux cleaned = -0.00269913 Jy ! Component: 2650 - total flux cleaned = -0.00274449 Jy ! Component: 2700 - total flux cleaned = -0.00275952 Jy ! Component: 2750 - total flux cleaned = -0.00280443 Jy ! Component: 2800 - total flux cleaned = -0.00283424 Jy ! Component: 2850 - total flux cleaned = -0.00284906 Jy ! Component: 2900 - total flux cleaned = -0.00290803 Jy ! Component: 2950 - total flux cleaned = -0.00293737 Jy ! Component: 3000 - total flux cleaned = -0.00290807 Jy ! Component: 3050 - total flux cleaned = -0.00289337 Jy ! Component: 3100 - total flux cleaned = -0.00293697 Jy ! Component: 3150 - total flux cleaned = -0.00298036 Jy ! Component: 3200 - total flux cleaned = -0.00295154 Jy ! Component: 3250 - total flux cleaned = -0.00293727 Jy ! Component: 3300 - total flux cleaned = -0.00298013 Jy ! Component: 3350 - total flux cleaned = -0.00299442 Jy ! Component: 3400 - total flux cleaned = -0.0030511 Jy ! Component: 3450 - total flux cleaned = -0.00309353 Jy ! Component: 3500 - total flux cleaned = -0.00316385 Jy ! Component: 3550 - total flux cleaned = -0.00316386 Jy ! Component: 3600 - total flux cleaned = -0.00323362 Jy ! Component: 3650 - total flux cleaned = -0.00324742 Jy ! Component: 3700 - total flux cleaned = -0.00326127 Jy ! Component: 3750 - total flux cleaned = -0.00328886 Jy ! Component: 3800 - total flux cleaned = -0.00331649 Jy ! Component: 3850 - total flux cleaned = -0.00327547 Jy ! Component: 3900 - total flux cleaned = -0.00330292 Jy ! Component: 3950 - total flux cleaned = -0.00334388 Jy ! Component: 4000 - total flux cleaned = -0.00338462 Jy ! Component: 4050 - total flux cleaned = -0.00342517 Jy ! Total flux subtracted in 4096 components = -0.00349269 Jy ! Clean residual min=-0.000792 max=0.000792 Jy/beam ! Clean residual mean=-0.000000 rms=0.000229 Jy/beam ! Combined flux in latest and established models = 0.114517 Jy keep ! Adding 370 model components to the UV plane model. ! The established model now contains 434 components and 0.114517 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1314+2348_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.629 x 1.404 at -5.653 degrees (North through East) ! Clean map min=-0.001217 max=0.086165 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1314+2348_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0861652 invert ! Inverting map ! Your choice of large map pixels excluded 8.58% of the data. ! The x-axis pixel size should ideally be below 0.1657 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000229013 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.797349 0.797349 1.5947 3.1894 6.3788 12.7576 25.5152 51.0304 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0006 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.086 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 376.246 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1314+2348_X_uvs.log closed on Sat Dec 26 09:39:39 2015