! Started logfile: /scr/pima/gb073_uvs/J0136+3905_X_uvs.log on Sat Dec 26 09:31:34 2015 obs /scr/pima/gb073_uvs/J0136+3905_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J0136+3905_X_uva.fits ! AN table 1: 58 integrations on 55 of 55 possible baselines. ! AN table 2: 29 integrations on 66 of 66 possible baselines. ! AN table 3: 29 integrations on 45 of 45 possible baselines. ! AN table 4: 17 integrations on 36 of 36 possible baselines. ! AN table 5: 29 integrations on 55 of 55 possible baselines. ! AN table 6: 29 integrations on 28 of 28 possible baselines. ! Apparent sampling: 0.767077 visibilities/baseline/integration-bin. ! Found source: J0136+3905 ! ! 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 57856 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/J0136+3905_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 58 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 34 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 58 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 34 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 58 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 34 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 58 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 34 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 5. ! A total of 116 telescope corrections were flagged in sub-array 1. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 34 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 6. ! A total of 116 telescope corrections were flagged in sub-array 1. ! A total of 58 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 34 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 7. ! A total of 58 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 34 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 8. ! A total of 58 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 34 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=1.003856Jy sigma=10.355097 ! Fit after self-cal, rms=0.956110Jy sigma=9.885532 ! 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 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! Estimated beam: bmin=0.4436 mas, bmaj=1.173 mas, bpa=-15.59 degrees ! Estimated noise=0.784569 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 = 0.0369392 Jy ! Component: 100 - total flux cleaned = 0.0450027 Jy ! Total flux subtracted in 100 components = 0.0450027 Jy ! Clean residual min=-0.002303 max=0.002944 Jy/beam ! Clean residual mean=0.000000 rms=0.000536 Jy/beam ! Combined flux in latest and established models = 0.0450027 Jy ! Performing phase self-cal ! Adding 2 model components to the UV plane model. ! The established model now contains 2 components and 0.0450027 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=0.089994Jy sigma=0.659776 ! Fit after self-cal, rms=0.088621Jy sigma=0.640709 ! Inverting map ! Your choice of large map pixels excluded 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00324814 Jy ! Component: 100 - total flux cleaned = 0.00332931 Jy ! Total flux subtracted in 100 components = 0.00332931 Jy ! Clean residual min=-0.002210 max=0.002378 Jy/beam ! Clean residual mean=0.000000 rms=0.000518 Jy/beam ! Combined flux in latest and established models = 0.048332 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 6 components and 0.048332 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=0.088437Jy sigma=0.639591 ! Fit after self-cal, rms=0.088421Jy sigma=0.639466 ! Inverting map ! Your choice of large map pixels excluded 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 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 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! Estimated beam: bmin=0.654 mas, bmaj=1.42 mas, bpa=-12.3 degrees ! Estimated noise=0.326088 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 = 0.000616344 Jy ! Component: 100 - total flux cleaned = 0.000657485 Jy ! Component: 150 - total flux cleaned = 0.000674317 Jy ! Component: 200 - total flux cleaned = 0.000687304 Jy ! Total flux subtracted in 200 components = 0.000687304 Jy ! Clean residual min=-0.001179 max=0.001056 Jy/beam ! Clean residual mean=0.000002 rms=0.000249 Jy/beam ! Combined flux in latest and established models = 0.0490193 Jy ! Performing phase self-cal ! Adding 13 model components to the UV plane model. ! The established model now contains 17 components and 0.0490193 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=0.088401Jy sigma=0.639422 ! Fit after self-cal, rms=0.088401Jy sigma=0.639409 ! Inverting map ! Your choice of large map pixels excluded 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.654 x 1.42 at -12.3 degrees (North through East) ! Clean map min=-0.0010471 max=0.049759 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* ON 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* 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* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* FD 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* FD 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 6: ! BR 0.99 FD 0.96 KP 1.03 LA 1.03 ! MK 1.03 NL 0.98 OV 1.03 PT 1.00 ! ! ! 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* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.07 EF 1.00* FD 1.03 KP 1.08 ! LA 1.03 MC 0.84 NL 1.08 ON 0.86 ! OV 1.00 PT 1.10 SC 0.94 ZC 1.09 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* FD 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* FD 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 6: ! BR 1.13 FD 1.01 KP 1.08 LA 0.97 ! MK 1.15 NL 1.03 OV 1.07 PT 1.04 ! ! ! 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* ON 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* 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* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* FD 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* FD 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 6: ! BR 1.00 FD 1.03 KP 0.99 LA 1.01 ! MK 1.08 NL 1.07 OV 1.00 PT 0.96 ! ! ! 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* ON 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* 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* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* FD 0.97 LA 0.95 MC 0.94 ! NL 1.05 ON 1.00* PT 0.94 SC 1.17 ! ZC 1.00 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 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 6: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.95 KP 0.95 ! LA 1.03 MC 1.03 NL 1.02 ON 0.87 ! PT 0.95 SC 0.96 ZC 0.98 ! ! 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* 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* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* FD 0.90 LA 1.03 MC 0.97 ! NL 1.05 ON 1.00* PT 1.06 SC 1.06 ! ZC 0.90 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 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 6: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 1.00* ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 0.96 KP 0.89 ! LA 1.00 MC 1.02 NL 1.00 ON 1.10 ! PT 0.87 SC 0.97 ZC 0.98 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 0.91 KP 0.95 ! LA 1.04 MC 0.88 NL 1.07 ON 0.92 ! OV 1.13 PT 1.02 SC 0.86 ZC 1.00 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* FD 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* FD 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 6: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* OV 1.00* PT 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* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.20 EF 1.00* FD 0.85 KP 0.92 ! LA 0.96 MC 0.92 NL 0.97 ON 0.89 ! OV 1.12 PT 0.90 SC 1.00 ZC 1.03 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* FD 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* FD 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 6: ! BR 0.98 FD 0.95 KP 0.94 LA 1.10 ! MK 0.98 NL 1.04 OV 1.07 PT 0.94 ! ! ! 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* ON 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* 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* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* MK 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! EF 1.00* FD 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* FD 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 6: ! BR 1.01 FD 0.88 KP 0.89 LA 0.96 ! MK 0.96 NL 1.11 OV 1.05 PT 0.98 ! ! ! Fit before self-cal, rms=0.088401Jy sigma=0.639409 ! Fit after self-cal, rms=0.084099Jy sigma=0.638960 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! Estimated beam: bmin=0.6537 mas, bmaj=1.418 mas, bpa=-12.21 degrees ! Estimated noise=0.325945 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 = 3.16269e-05 Jy ! Component: 100 - total flux cleaned = 3.185e-05 Jy ! Component: 150 - total flux cleaned = 3.21316e-05 Jy ! Component: 200 - total flux cleaned = 3.22437e-05 Jy ! Total flux subtracted in 200 components = 3.22437e-05 Jy ! Clean residual min=-0.001119 max=0.001036 Jy/beam ! Clean residual mean=0.000002 rms=0.000244 Jy/beam ! Combined flux in latest and established models = 0.0490515 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 20 components and 0.0490515 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=0.084094Jy sigma=0.638932 ! Fit after self-cal, rms=0.084096Jy sigma=0.638876 ! Inverting map ! Your choice of large map pixels excluded 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 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=0.084096Jy sigma=0.638876 ! Fit after self-cal, rms=0.084765Jy sigma=0.638781 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! Estimated beam: bmin=0.6535 mas, bmaj=1.417 mas, bpa=-12.19 degrees ! Estimated noise=0.326041 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 6.03332e-05 Jy ! Component: 100 - total flux cleaned = 6.9008e-05 Jy ! Component: 150 - total flux cleaned = 6.82981e-05 Jy ! Component: 200 - total flux cleaned = 6.8384e-05 Jy ! Total flux subtracted in 200 components = 6.8384e-05 Jy ! Clean residual min=-0.001086 max=0.001021 Jy/beam ! Clean residual mean=0.000002 rms=0.000242 Jy/beam ! Combined flux in latest and established models = 0.0491199 Jy selfcal ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 20 components and 0.0491199 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=0.084763Jy sigma=0.638775 ! Fit after self-cal, rms=0.084758Jy sigma=0.638758 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 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 = -4.52957e-06 Jy ! Component: 100 - total flux cleaned = 7.95165e-06 Jy ! Component: 150 - total flux cleaned = 8.01394e-06 Jy ! Component: 200 - total flux cleaned = 7.88647e-06 Jy ! Total flux subtracted in 200 components = 7.88647e-06 Jy ! Clean residual min=-0.001089 max=0.001020 Jy/beam ! Clean residual mean=0.000002 rms=0.000242 Jy/beam ! Combined flux in latest and established models = 0.0491278 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 23 components and 0.0491278 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=0.084756Jy sigma=0.638755 ! Fit after self-cal, rms=0.084755Jy sigma=0.638755 ! Inverting map ! Your choice of large map pixels excluded 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 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=0.084755Jy sigma=0.638755 ! Fit after self-cal, rms=0.084690Jy sigma=0.638726 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! Estimated beam: bmin=0.6535 mas, bmaj=1.416 mas, bpa=-12.19 degrees ! Estimated noise=0.326384 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 5.64988e-05 Jy ! Component: 100 - total flux cleaned = 6.67899e-05 Jy ! Component: 150 - total flux cleaned = 6.65791e-05 Jy ! Component: 200 - total flux cleaned = 6.65055e-05 Jy ! Total flux subtracted in 200 components = 6.65055e-05 Jy ! Clean residual min=-0.001076 max=0.001007 Jy/beam ! Clean residual mean=0.000002 rms=0.000241 Jy/beam ! Combined flux in latest and established models = 0.0491943 Jy selfcal ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 25 components and 0.0491943 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=0.084688Jy sigma=0.638729 ! Fit after self-cal, rms=0.084686Jy sigma=0.638712 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -6.80785e-06 Jy ! Component: 100 - total flux cleaned = -2.14356e-06 Jy ! Component: 150 - total flux cleaned = -2.10256e-06 Jy ! Component: 200 - total flux cleaned = -1.97336e-06 Jy ! Total flux subtracted in 200 components = -1.97336e-06 Jy ! Clean residual min=-0.001078 max=0.001001 Jy/beam ! Clean residual mean=0.000002 rms=0.000241 Jy/beam ! Combined flux in latest and established models = 0.0491923 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 26 components and 0.0491923 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=0.084686Jy sigma=0.638709 ! Fit after self-cal, rms=0.084685Jy sigma=0.638706 ! Inverting map ! Your choice of large map pixels excluded 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 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=0.084685Jy sigma=0.638706 ! Fit after self-cal, rms=0.084645Jy sigma=0.638704 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! Estimated beam: bmin=2.805 mas, bmaj=2.977 mas, bpa=10.04 degrees ! Estimated noise=0.404464 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000283278 Jy ! Component: 100 - total flux cleaned = 0.000299012 Jy ! Component: 150 - total flux cleaned = 0.000305644 Jy ! Component: 200 - total flux cleaned = 0.000305844 Jy ! Total flux subtracted in 200 components = 0.000305844 Jy ! Clean residual min=-0.001205 max=0.001145 Jy/beam ! Clean residual mean=0.000004 rms=0.000306 Jy/beam ! Combined flux in latest and established models = 0.0494982 Jy selfcal ! Performing phase self-cal ! Adding 4 model components to the UV plane model. ! The established model now contains 29 components and 0.0494982 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=0.084645Jy sigma=0.638730 ! Fit after self-cal, rms=0.084648Jy sigma=0.638724 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 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 = 2.33225e-05 Jy ! Component: 100 - total flux cleaned = 2.34947e-05 Jy ! Component: 150 - total flux cleaned = 2.43368e-05 Jy ! Component: 200 - total flux cleaned = 2.52706e-05 Jy ! Total flux subtracted in 200 components = 2.52706e-05 Jy ! Clean residual min=-0.001204 max=0.001143 Jy/beam ! Clean residual mean=0.000004 rms=0.000305 Jy/beam ! Combined flux in latest and established models = 0.0495235 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 29 components and 0.0495235 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=0.084649Jy sigma=0.638741 ! Fit after self-cal, rms=0.084648Jy sigma=0.638729 ! Inverting map ! Your choice of large map pixels excluded 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 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 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! Estimated beam: bmin=0.6535 mas, bmaj=1.416 mas, bpa=-12.18 degrees ! Estimated noise=0.32651 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6535 x 1.416 at -12.18 degrees (North through East) ! Clean map min=-0.00097325 max=0.050216 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 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! Estimated beam: bmin=0.4433 mas, bmaj=1.169 mas, bpa=-15.52 degrees ! Estimated noise=0.785973 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0390903 Jy ! Component: 100 - total flux cleaned = 0.0476474 Jy ! Component: 150 - total flux cleaned = 0.0482841 Jy ! Component: 200 - total flux cleaned = 0.0482994 Jy ! Total flux subtracted in 200 components = 0.0482994 Jy ! Clean residual min=-0.002178 max=0.002343 Jy/beam ! Clean residual mean=0.000000 rms=0.000514 Jy/beam ! Combined flux in latest and established models = 0.0482994 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 7 model components to the UV plane model. ! The established model now contains 7 components and 0.0482994 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! Estimated beam: bmin=0.6535 mas, bmaj=1.416 mas, bpa=-12.18 degrees ! Estimated noise=0.32651 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 = 0.000707006 Jy ! Component: 100 - total flux cleaned = 0.000730242 Jy ! Component: 150 - total flux cleaned = 0.000786576 Jy ! Component: 200 - total flux cleaned = 0.000830166 Jy ! Total flux subtracted in 200 components = 0.000830166 Jy ! Clean residual min=-0.001080 max=0.000999 Jy/beam ! Clean residual mean=0.000002 rms=0.000241 Jy/beam ! Combined flux in latest and established models = 0.0491295 Jy ! Adding 10 model components to the UV plane model. ! The established model now contains 15 components and 0.0491295 Jy ! Inverting map ! Your choice of large map pixels excluded 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 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 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! Estimated beam: bmin=2.805 mas, bmaj=2.977 mas, bpa=10.04 degrees ! Estimated noise=0.404464 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000404359 Jy ! Component: 100 - total flux cleaned = 0.000436726 Jy ! Component: 150 - total flux cleaned = 0.000430234 Jy ! Component: 200 - total flux cleaned = 0.000429957 Jy ! Total flux subtracted in 200 components = 0.000429957 Jy ! Clean residual min=-0.001201 max=0.001129 Jy/beam ! Clean residual mean=0.000004 rms=0.000305 Jy/beam ! Combined flux in latest and established models = 0.0495595 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 = -6.70922e-07 Jy ! Component: 100 - total flux cleaned = -1.00098e-06 Jy ! Component: 150 - total flux cleaned = -1.90842e-06 Jy ! Component: 200 - total flux cleaned = -2.14384e-06 Jy ! Total flux subtracted in 200 components = -2.14384e-06 Jy ! Clean residual min=-0.001198 max=0.001138 Jy/beam ! Clean residual mean=0.000004 rms=0.000305 Jy/beam ! Combined flux in latest and established models = 0.0495573 Jy ! Adding 5 model components to the UV plane model. ! The established model now contains 20 components and 0.0495573 Jy ! Inverting map ! Your choice of large map pixels excluded 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! Estimated beam: bmin=0.6535 mas, bmaj=1.416 mas, bpa=-12.18 degrees ! Estimated noise=0.32651 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000287488 Jy ! Component: 100 - total flux cleaned = -0.00030694 Jy ! Component: 150 - total flux cleaned = -0.000315227 Jy ! Component: 200 - total flux cleaned = -0.000315227 Jy ! Total flux subtracted in 200 components = -0.000315227 Jy ! Clean residual min=-0.001086 max=0.001006 Jy/beam ! Clean residual mean=0.000002 rms=0.000241 Jy/beam ! Combined flux in latest and established models = 0.0492421 Jy selfcal ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 23 components and 0.0492421 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=0.084652Jy sigma=0.638713 ! Fit after self-cal, rms=0.084651Jy sigma=0.638710 wmodel /scr/pima/gb073_uvs/J0136+3905_X_map.mod ! Writing 23 model components to file: /scr/pima/gb073_uvs/J0136+3905_X_map.mod wobs /scr/pima/gb073_uvs/J0136+3905_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J0136+3905_X_uvs.fits wwins /scr/pima/gb073_uvs/J0136+3905_X_map.win ! wwins: Wrote 1 windows to /scr/pima/gb073_uvs/J0136+3905_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 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000324818 Jy ! Component: 100 - total flux cleaned = -0.000550366 Jy ! Component: 150 - total flux cleaned = -0.000604732 Jy ! Component: 200 - total flux cleaned = -0.000674226 Jy ! Component: 250 - total flux cleaned = -0.000725122 Jy ! Component: 300 - total flux cleaned = -0.000791753 Jy ! Component: 350 - total flux cleaned = -0.000840607 Jy ! Component: 400 - total flux cleaned = -0.000920631 Jy ! Component: 450 - total flux cleaned = -0.000983737 Jy ! Component: 500 - total flux cleaned = -0.000984083 Jy ! Component: 550 - total flux cleaned = -0.00107548 Jy ! Component: 600 - total flux cleaned = -0.00106032 Jy ! Component: 650 - total flux cleaned = -0.00106032 Jy ! Component: 700 - total flux cleaned = -0.00103105 Jy ! Component: 750 - total flux cleaned = -0.00106015 Jy ! Component: 800 - total flux cleaned = -0.001031 Jy ! Component: 850 - total flux cleaned = -0.00104531 Jy ! Component: 900 - total flux cleaned = -0.00104525 Jy ! Component: 950 - total flux cleaned = -0.00105911 Jy ! Component: 1000 - total flux cleaned = -0.00101755 Jy ! Component: 1050 - total flux cleaned = -0.0010311 Jy ! Component: 1100 - total flux cleaned = -0.00101755 Jy ! Component: 1150 - total flux cleaned = -0.000977223 Jy ! Component: 1200 - total flux cleaned = -0.000990719 Jy ! Component: 1250 - total flux cleaned = -0.000923952 Jy ! Component: 1300 - total flux cleaned = -0.000897584 Jy ! Component: 1350 - total flux cleaned = -0.00088437 Jy ! Component: 1400 - total flux cleaned = -0.000845221 Jy ! Component: 1450 - total flux cleaned = -0.000767539 Jy ! Component: 1500 - total flux cleaned = -0.000806047 Jy ! Component: 1550 - total flux cleaned = -0.000729306 Jy ! Component: 1600 - total flux cleaned = -0.00071679 Jy ! Component: 1650 - total flux cleaned = -0.000653586 Jy ! Component: 1700 - total flux cleaned = -0.000590877 Jy ! Component: 1750 - total flux cleaned = -0.000590863 Jy ! Component: 1800 - total flux cleaned = -0.000566083 Jy ! Component: 1850 - total flux cleaned = -0.000516843 Jy ! Component: 1900 - total flux cleaned = -0.000516745 Jy ! Component: 1950 - total flux cleaned = -0.000382956 Jy ! Component: 2000 - total flux cleaned = -0.000419336 Jy ! Component: 2050 - total flux cleaned = -0.000298948 Jy ! Component: 2100 - total flux cleaned = -0.00031103 Jy ! Component: 2150 - total flux cleaned = -0.000251633 Jy ! Component: 2200 - total flux cleaned = -0.000239796 Jy ! Component: 2250 - total flux cleaned = -0.000145579 Jy ! Component: 2300 - total flux cleaned = -0.00021589 Jy ! Component: 2350 - total flux cleaned = -0.000122582 Jy ! Component: 2400 - total flux cleaned = -5.30472e-05 Jy ! Component: 2450 - total flux cleaned = 1.62754e-05 Jy ! Component: 2500 - total flux cleaned = 9.65856e-05 Jy ! Component: 2550 - total flux cleaned = 0.000130769 Jy ! Component: 2600 - total flux cleaned = 0.000164967 Jy ! Component: 2650 - total flux cleaned = 0.000278157 Jy ! Component: 2700 - total flux cleaned = 0.000278085 Jy ! Component: 2750 - total flux cleaned = 0.000379091 Jy ! Component: 2800 - total flux cleaned = 0.000479558 Jy ! Component: 2850 - total flux cleaned = 0.000468383 Jy ! Component: 2900 - total flux cleaned = 0.000534782 Jy ! Component: 2950 - total flux cleaned = 0.000545695 Jy ! Component: 3000 - total flux cleaned = 0.000644536 Jy ! Component: 3050 - total flux cleaned = 0.000633575 Jy ! Component: 3100 - total flux cleaned = 0.000720458 Jy ! Component: 3150 - total flux cleaned = 0.000807015 Jy ! Component: 3200 - total flux cleaned = 0.000839371 Jy ! Component: 3250 - total flux cleaned = 0.000849984 Jy ! Component: 3300 - total flux cleaned = 0.000871342 Jy ! Component: 3350 - total flux cleaned = 0.000903404 Jy ! Component: 3400 - total flux cleaned = 0.000924638 Jy ! Component: 3450 - total flux cleaned = 0.000987993 Jy ! Component: 3500 - total flux cleaned = 0.000966965 Jy ! Component: 3550 - total flux cleaned = 0.00105077 Jy ! Component: 3600 - total flux cleaned = 0.00101945 Jy ! Component: 3650 - total flux cleaned = 0.00111301 Jy ! Component: 3700 - total flux cleaned = 0.00112329 Jy ! Component: 3750 - total flux cleaned = 0.00115427 Jy ! Component: 3800 - total flux cleaned = 0.0011748 Jy ! Component: 3850 - total flux cleaned = 0.00124651 Jy ! Component: 3900 - total flux cleaned = 0.0012363 Jy ! Component: 3950 - total flux cleaned = 0.00122613 Jy ! Component: 4000 - total flux cleaned = 0.001216 Jy ! Component: 4050 - total flux cleaned = 0.00123624 Jy ! Total flux subtracted in 4096 components = 0.00123622 Jy ! Clean residual min=-0.000625 max=0.000527 Jy/beam ! Clean residual mean=0.000002 rms=0.000168 Jy/beam ! Combined flux in latest and established models = 0.0504783 Jy keep ! Adding 333 model components to the UV plane model. ! The established model now contains 356 components and 0.0504783 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J0136+3905_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6535 x 1.416 at -12.18 degrees (North through East) ! Clean map min=-0.00090329 max=0.050261 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J0136+3905_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0502606 invert ! Inverting map ! Your choice of large map pixels excluded 4.81% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000167904 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -1.0022 1.0022 2.00441 4.00881 8.01762 16.0352 32.0705 64.141 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0005 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.05 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 299.34 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J0136+3905_X_uvs.log closed on Sat Dec 26 09:31:41 2015