! Started logfile: /scr/pima/gb073_uvs/J0841+2319_X_uvs.log on Sat Dec 26 09:34:44 2015 obs /scr/pima/gb073_uvs/J0841+2319_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J0841+2319_X_uva.fits ! AN table 1: 20 integrations on 36 of 36 possible baselines. ! AN table 2: 145 integrations on 10 of 10 possible baselines. ! AN table 3: 23 integrations on 55 of 55 possible baselines. ! AN table 4: 10 integrations on 66 of 66 possible baselines. ! AN table 5: 29 integrations on 55 of 55 possible baselines. ! AN table 6: 29 integrations on 6 of 6 possible baselines. ! AN table 7: 23 integrations on 66 of 66 possible baselines. ! Apparent sampling: 0.680981 visibilities/baseline/integration-bin. ! Found source: J0841+2319 ! ! 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 40216 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/J0841+2319_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 181 telescope corrections were flagged in sub-array 2. ! A total of 69 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 50 telescope corrections were flagged in sub-array 6. ! A total of 29 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 2. ! A total of 181 telescope corrections were flagged in sub-array 2. ! A total of 69 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 50 telescope corrections were flagged in sub-array 6. ! A total of 29 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 3. ! A total of 181 telescope corrections were flagged in sub-array 2. ! A total of 69 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 50 telescope corrections were flagged in sub-array 6. ! A total of 29 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 4. ! A total of 181 telescope corrections were flagged in sub-array 2. ! A total of 69 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 50 telescope corrections were flagged in sub-array 6. ! A total of 29 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 5. ! A total of 20 telescope corrections were flagged in sub-array 1. ! A total of 181 telescope corrections were flagged in sub-array 2. ! A total of 92 telescope corrections were flagged in sub-array 3. ! A total of 40 telescope corrections were flagged in sub-array 4. ! A total of 65 telescope corrections were flagged in sub-array 5. ! A total of 50 telescope corrections were flagged in sub-array 6. ! A total of 52 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 6. ! A total of 20 telescope corrections were flagged in sub-array 1. ! A total of 181 telescope corrections were flagged in sub-array 2. ! A total of 92 telescope corrections were flagged in sub-array 3. ! A total of 40 telescope corrections were flagged in sub-array 4. ! A total of 65 telescope corrections were flagged in sub-array 5. ! A total of 50 telescope corrections were flagged in sub-array 6. ! A total of 52 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 7. ! A total of 181 telescope corrections were flagged in sub-array 2. ! A total of 69 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 50 telescope corrections were flagged in sub-array 6. ! A total of 29 telescope corrections were flagged in sub-array 7. ! ! Correcting IF 8. ! A total of 181 telescope corrections were flagged in sub-array 2. ! A total of 69 telescope corrections were flagged in sub-array 3. ! A total of 30 telescope corrections were flagged in sub-array 4. ! A total of 36 telescope corrections were flagged in sub-array 5. ! A total of 50 telescope corrections were flagged in sub-array 6. ! A total of 29 telescope corrections were flagged in sub-array 7. ! ! Fit before self-cal, rms=1.008589Jy sigma=9.206641 ! Fit after self-cal, rms=0.925127Jy sigma=8.495682 ! 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 4.98% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! Estimated beam: bmin=0.6494 mas, bmaj=0.8834 mas, bpa=23.28 degrees ! Estimated noise=0.854682 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 = 0.0568066 Jy ! Component: 100 - total flux cleaned = 0.0730609 Jy ! Total flux subtracted in 100 components = 0.0730609 Jy ! Clean residual min=-0.003304 max=0.007090 Jy/beam ! Clean residual mean=0.000000 rms=0.000709 Jy/beam ! Combined flux in latest and established models = 0.0730609 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.0730609 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=0.089773Jy sigma=0.645178 ! Fit after self-cal, rms=0.088889Jy sigma=0.638568 ! Inverting map ! Your choice of large map pixels excluded 4.98% 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 = 0.00829831 Jy ! Component: 100 - total flux cleaned = 0.0105496 Jy ! Total flux subtracted in 100 components = 0.0105496 Jy ! Clean residual min=-0.003117 max=0.003537 Jy/beam ! Clean residual mean=0.000000 rms=0.000641 Jy/beam ! Combined flux in latest and established models = 0.0836105 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 10 components and 0.0836105 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=0.087885Jy sigma=0.631490 ! Fit after self-cal, rms=0.087829Jy sigma=0.631213 ! Inverting map ! Your choice of large map pixels excluded 4.98% 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 4.98% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! Estimated beam: bmin=0.8411 mas, bmaj=1.057 mas, bpa=40.73 degrees ! Estimated noise=0.455297 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 = 0.00212573 Jy ! Component: 100 - total flux cleaned = 0.00212747 Jy ! Component: 150 - total flux cleaned = 0.00211797 Jy ! Component: 200 - total flux cleaned = 0.00204074 Jy ! Total flux subtracted in 200 components = 0.00204074 Jy ! Clean residual min=-0.002124 max=0.002181 Jy/beam ! Clean residual mean=0.000004 rms=0.000400 Jy/beam ! Combined flux in latest and established models = 0.0856512 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 15 components and 0.0856512 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=0.087531Jy sigma=0.630224 ! Fit after self-cal, rms=0.087490Jy sigma=0.630132 ! Inverting map ! Your choice of large map pixels excluded 4.98% 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: 0.8411 x 1.057 at 40.73 degrees (North through East) ! Clean map min=-0.0018108 max=0.073608 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 0.99 FD 0.91 KP 1.05 LA 0.97 ! MK 1.13 NL 0.92 OV 1.01 PT 0.96 ! SC 1.01 ! ! A total of 108 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.05 EF 1.00* FD 0.91 KP 1.01 ! LA 1.00 MC 1.00* NL 0.97 ON 1.00* ! OV 1.02 PT 0.99 SC 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 EF 1.00* FD 0.91 KP 1.10 ! LA 1.00 MC 1.00* MK 1.18 NL 0.92 ! ON 1.00* OV 1.02 PT 0.87 SC 0.99 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! A total of 66 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.01 EF 1.00* FD 1.03 KP 0.99 ! LA 1.01 MC 0.88 NL 0.94 ON 0.85 ! OV 1.07 PT 0.97 SC 1.03 ZC 0.94 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.05 FD 1.03 KP 1.00 LA 1.10 ! MK 1.12 NL 0.97 OV 1.04 PT 1.04 ! SC 1.12 ! ! A total of 108 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.05 EF 1.00* FD 1.04 KP 1.02 ! LA 1.04 MC 1.00* NL 1.00 ON 1.00* ! OV 1.06 PT 1.03 SC 1.08 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.03 EF 1.00* FD 1.08 KP 1.15 ! LA 1.04 MC 1.00* MK 1.04 NL 1.04 ! ON 1.00* OV 1.04 PT 1.03 SC 0.92 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! A total of 66 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! 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* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.05 FD 1.06 KP 0.99 LA 0.90 ! MK 1.05 NL 1.05 OV 0.99 PT 1.01 ! SC 1.18 ! ! A total of 108 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 EF 1.00* FD 0.99 KP 0.92 ! LA 0.95 MC 1.00* NL 1.05 ON 1.00* ! OV 0.97 PT 0.97 SC 1.04 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.10 EF 1.00* FD 0.91 KP 0.94 ! LA 1.03 MC 1.00* MK 1.12 NL 1.09 ! ON 1.00* OV 1.03 PT 1.16 SC 0.95 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! A total of 66 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! 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* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.03 FD 1.10 KP 1.05 LA 1.02 ! MK 1.10 NL 1.00 OV 1.07 PT 0.99 ! SC 1.06 ! ! A total of 108 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.05 EF 1.00* FD 0.98 KP 1.02 ! LA 1.00 MC 1.00* NL 1.06 ON 1.00* ! OV 0.95 PT 1.02 SC 1.05 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.03 EF 1.00* FD 1.12 KP 0.98 ! LA 1.01 MC 1.00* MK 1.14 NL 1.04 ! ON 1.00* OV 1.10 PT 1.02 SC 1.02 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! A total of 66 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! 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* ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.02 KP 1.01 LA 0.97 ! MK 1.02 NL 0.99 OV 1.06 PT 1.14 ! SC 1.01 ! ! A total of 108 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.00 MC 1.10 ON 0.91 ! ZC 0.88 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.01 KP 0.95 ! LA 0.96 MC 1.00* NL 1.06 ON 1.00* ! OV 1.07 PT 0.99 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* MK 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.05 HH 0.86 ! LA 1.10 MC 1.07 NL 0.94 ON 1.07 ! PT 0.94 SC 1.05 ZC 0.86 ! ! A total of 66 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* EF 1.00* FD 1.07 KP 0.84 ! LA 1.10 MC 0.96 NL 0.94 ON 1.03 ! OV 1.17 PT 0.93 SC 1.02 ZC 1.04 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.10 KP 0.84 LA 1.01 ! MK 1.13 NL 1.04 OV 1.06 PT 0.93 ! SC 1.01 ! ! A total of 108 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 0.93 MC 1.03 ON 1.01 ! ZC 0.87 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 0.98 KP 0.89 ! LA 0.99 MC 1.00* NL 1.13 ON 1.00* ! OV 1.10 PT 1.04 SC 0.87 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 0.94 KP 0.89 ! LA 0.93 MC 1.00* MK 1.20 NL 1.12 ! ON 1.00* OV 1.00 PT 1.13 SC 0.95 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.04 HH 0.92 ! LA 0.99 MC 1.07 NL 1.02 ON 1.01 ! PT 1.09 SC 0.96 ZC 0.99 ! ! A total of 66 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! BR 1.00* EF 1.00* FD 0.98 KP 0.87 ! LA 1.00 MC 1.07 NL 0.98 ON 1.06 ! OV 1.09 PT 0.94 SC 1.00 ZC 0.92 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! 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* ! ! A total of 108 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.96 EF 1.00* FD 0.97 KP 1.02 ! LA 1.06 MC 1.00* NL 1.01 ON 1.00* ! OV 1.07 PT 0.92 SC 1.13 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.04 EF 1.00* FD 1.02 KP 0.97 ! LA 1.04 MC 1.00* MK 1.16 NL 1.08 ! ON 1.00* OV 0.95 PT 0.98 SC 1.17 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! A total of 66 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! 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* ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! 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* ! ! A total of 108 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! EF 1.00* HH 1.00* MC 1.00* ON 1.00* ! ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.10 EF 1.00* FD 1.03 KP 0.92 ! LA 1.04 MC 1.00* NL 1.04 ON 1.00* ! OV 0.99 PT 0.96 SC 1.03 ! ! 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* MK 1.00* NL 1.00* ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* EF 1.00* FD 1.00* HH 1.00* ! LA 1.00* MC 1.00* NL 1.00* ON 1.00* ! PT 1.00* SC 1.00* ZC 1.00* ! ! A total of 66 telescope corrections were flagged in sub-array 6. ! Telescope amplitude corrections in sub-array 6: ! EF 0.00* HH 0.00* MC 0.00* ZC 0.00* ! ! Telescope amplitude corrections in sub-array 7: ! 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* ! ! ! Fit before self-cal, rms=0.087490Jy sigma=0.630132 ! Fit after self-cal, rms=0.087127Jy sigma=0.633167 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! Estimated beam: bmin=0.8492 mas, bmaj=1.092 mas, bpa=33.02 degrees ! Estimated noise=0.462473 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 = 0.000215609 Jy ! Component: 100 - total flux cleaned = 0.000172793 Jy ! Component: 150 - total flux cleaned = 0.000133392 Jy ! Component: 200 - total flux cleaned = 6.32443e-05 Jy ! Total flux subtracted in 200 components = 6.32443e-05 Jy ! Clean residual min=-0.001798 max=0.001776 Jy/beam ! Clean residual mean=0.000003 rms=0.000367 Jy/beam ! Combined flux in latest and established models = 0.0857145 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 17 components and 0.0857145 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=0.087059Jy sigma=0.633029 ! Fit after self-cal, rms=0.087075Jy sigma=0.632866 ! Inverting map ! Your choice of large map pixels excluded 5.2% 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=0.087075Jy sigma=0.632866 ! Fit after self-cal, rms=0.087286Jy sigma=0.632473 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! Estimated beam: bmin=0.8488 mas, bmaj=1.09 mas, bpa=32.84 degrees ! Estimated noise=0.463321 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 4.76883e-05 Jy ! Component: 100 - total flux cleaned = 1.28939e-05 Jy ! Component: 150 - total flux cleaned = -1.67749e-05 Jy ! Component: 200 - total flux cleaned = -4.29343e-05 Jy ! Total flux subtracted in 200 components = -4.29343e-05 Jy ! Clean residual min=-0.001794 max=0.001736 Jy/beam ! Clean residual mean=0.000003 rms=0.000356 Jy/beam ! Combined flux in latest and established models = 0.0856715 Jy selfcal ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 17 components and 0.0856715 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=0.087249Jy sigma=0.632411 ! Fit after self-cal, rms=0.087266Jy sigma=0.632342 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.2% 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 = -5.88395e-05 Jy ! Component: 100 - total flux cleaned = -5.92591e-05 Jy ! Component: 150 - total flux cleaned = -8.12595e-05 Jy ! Component: 200 - total flux cleaned = -9.99806e-05 Jy ! Total flux subtracted in 200 components = -9.99806e-05 Jy ! Clean residual min=-0.001817 max=0.001699 Jy/beam ! Clean residual mean=0.000003 rms=0.000355 Jy/beam ! Combined flux in latest and established models = 0.0855715 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 17 components and 0.0855715 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=0.087246Jy sigma=0.632311 ! Fit after self-cal, rms=0.087239Jy sigma=0.632297 ! Inverting map ! Your choice of large map pixels excluded 5.2% 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=0.087239Jy sigma=0.632297 ! Fit after self-cal, rms=0.087555Jy sigma=0.632281 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! Estimated beam: bmin=0.8509 mas, bmaj=1.093 mas, bpa=32.44 degrees ! Estimated noise=0.464061 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -5.55525e-05 Jy ! Component: 100 - total flux cleaned = -7.91519e-05 Jy ! Component: 150 - total flux cleaned = -9.97898e-05 Jy ! Component: 200 - total flux cleaned = -0.000119578 Jy ! Total flux subtracted in 200 components = -0.000119578 Jy ! Clean residual min=-0.001834 max=0.001687 Jy/beam ! Clean residual mean=0.000003 rms=0.000353 Jy/beam ! Combined flux in latest and established models = 0.085452 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 20 components and 0.085452 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=0.087537Jy sigma=0.632266 ! Fit after self-cal, rms=0.087543Jy sigma=0.632238 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.2% 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 = -1.80112e-05 Jy ! Component: 100 - total flux cleaned = -1.73014e-05 Jy ! Component: 150 - total flux cleaned = 1.72228e-07 Jy ! Component: 200 - total flux cleaned = 7.6434e-07 Jy ! Total flux subtracted in 200 components = 7.6434e-07 Jy ! Clean residual min=-0.001822 max=0.001672 Jy/beam ! Clean residual mean=0.000003 rms=0.000352 Jy/beam ! Combined flux in latest and established models = 0.0854527 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 20 components and 0.0854527 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=0.087532Jy sigma=0.632218 ! Fit after self-cal, rms=0.087526Jy sigma=0.632209 ! Inverting map ! Your choice of large map pixels excluded 5.2% 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=0.087526Jy sigma=0.632209 ! Fit after self-cal, rms=0.087592Jy sigma=0.632040 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! Estimated beam: bmin=2.609 mas, bmaj=2.959 mas, bpa=0.3869 degrees ! Estimated noise=0.546995 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000220755 Jy ! Component: 100 - total flux cleaned = -0.000221001 Jy ! Component: 150 - total flux cleaned = -0.000221486 Jy ! Component: 200 - total flux cleaned = -0.000235711 Jy ! Total flux subtracted in 200 components = -0.000235711 Jy ! Clean residual min=-0.002092 max=0.001859 Jy/beam ! Clean residual mean=0.000007 rms=0.000404 Jy/beam ! Combined flux in latest and established models = 0.085217 Jy selfcal ! Performing phase self-cal ! Adding 6 model components to the UV plane model. ! The established model now contains 24 components and 0.085217 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=0.087594Jy sigma=0.632049 ! Fit after self-cal, rms=0.087601Jy sigma=0.631992 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 5.2% 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 = -2.76672e-05 Jy ! Component: 100 - total flux cleaned = -2.80805e-05 Jy ! Component: 150 - total flux cleaned = -2.78196e-05 Jy ! Component: 200 - total flux cleaned = -2.74775e-05 Jy ! Total flux subtracted in 200 components = -2.74775e-05 Jy ! Clean residual min=-0.002077 max=0.001851 Jy/beam ! Clean residual mean=0.000007 rms=0.000403 Jy/beam ! Combined flux in latest and established models = 0.0851896 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 24 components and 0.0851896 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=0.087606Jy sigma=0.632040 ! Fit after self-cal, rms=0.087594Jy sigma=0.631949 ! Inverting map ! Your choice of large map pixels excluded 5.2% 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 5.2% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! Estimated beam: bmin=0.8518 mas, bmaj=1.094 mas, bpa=32.14 degrees ! Estimated noise=0.46455 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8518 x 1.094 at 32.14 degrees (North through East) ! Clean map min=-0.001629 max=0.07421 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 5.2% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! Estimated beam: bmin=0.6421 mas, bmaj=0.9111 mas, bpa=20.85 degrees ! Estimated noise=0.882777 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0577602 Jy ! Component: 100 - total flux cleaned = 0.0746692 Jy ! Component: 150 - total flux cleaned = 0.0820431 Jy ! Component: 200 - total flux cleaned = 0.0836503 Jy ! Total flux subtracted in 200 components = 0.0836503 Jy ! Clean residual min=-0.003152 max=0.003283 Jy/beam ! Clean residual mean=0.000000 rms=0.000640 Jy/beam ! Combined flux in latest and established models = 0.0836503 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 8 model components to the UV plane model. ! The established model now contains 8 components and 0.0836503 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 5.2% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! Estimated beam: bmin=0.8518 mas, bmaj=1.094 mas, bpa=32.14 degrees ! Estimated noise=0.46455 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) ! Added new window around map position (-0.8, -0.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00234645 Jy ! Component: 100 - total flux cleaned = 0.00234637 Jy ! Component: 150 - total flux cleaned = 0.00234516 Jy ! Component: 200 - total flux cleaned = 0.0022726 Jy ! Total flux subtracted in 200 components = 0.0022726 Jy ! Clean residual min=-0.001950 max=0.001886 Jy/beam ! Clean residual mean=0.000004 rms=0.000356 Jy/beam ! Combined flux in latest and established models = 0.0859229 Jy ! Adding 14 model components to the UV plane model. ! The established model now contains 19 components and 0.0859229 Jy ! Inverting map ! Your choice of large map pixels excluded 5.2% 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 5.2% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! Estimated beam: bmin=2.609 mas, bmaj=2.959 mas, bpa=0.3869 degrees ! Estimated noise=0.546995 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000738659 Jy ! Component: 100 - total flux cleaned = -0.000833322 Jy ! Component: 150 - total flux cleaned = -0.000918948 Jy ! Component: 200 - total flux cleaned = -0.00098199 Jy ! Total flux subtracted in 200 components = -0.00098199 Jy ! Clean residual min=-0.002072 max=0.001875 Jy/beam ! Clean residual mean=0.000007 rms=0.000400 Jy/beam ! Combined flux in latest and established models = 0.0849409 Jy flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam keep new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -4.41246e-05 Jy ! Component: 100 - total flux cleaned = -8.51723e-05 Jy ! Component: 150 - total flux cleaned = -0.000123699 Jy ! Component: 200 - total flux cleaned = -0.000160192 Jy ! Total flux subtracted in 200 components = -0.000160192 Jy ! Clean residual min=-0.002060 max=0.001842 Jy/beam ! Clean residual mean=0.000007 rms=0.000398 Jy/beam ! Combined flux in latest and established models = 0.0847807 Jy ! Adding 11 model components to the UV plane model. ! The established model now contains 30 components and 0.0847807 Jy ! Inverting map ! Your choice of large map pixels excluded 5.2% 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 5.2% of the data. ! The x-axis pixel size should ideally be below 0.18 milli-arcsec ! Estimated beam: bmin=0.8518 mas, bmaj=1.094 mas, bpa=32.14 degrees ! Estimated noise=0.46455 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000554336 Jy ! Component: 100 - total flux cleaned = 0.00061589 Jy ! Component: 150 - total flux cleaned = 0.000674279 Jy ! Component: 200 - total flux cleaned = 0.00072506 Jy ! Total flux subtracted in 200 components = 0.00072506 Jy ! Clean residual min=-0.001757 max=0.001821 Jy/beam ! Clean residual mean=0.000003 rms=0.000346 Jy/beam ! Combined flux in latest and established models = 0.0855058 Jy selfcal ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 33 components and 0.0855058 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=0.087686Jy sigma=0.632180 ! Fit after self-cal, rms=0.087699Jy sigma=0.631977 wmodel /scr/pima/gb073_uvs/J0841+2319_X_map.mod ! Writing 33 model components to file: /scr/pima/gb073_uvs/J0841+2319_X_map.mod wobs /scr/pima/gb073_uvs/J0841+2319_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J0841+2319_X_uvs.fits wwins /scr/pima/gb073_uvs/J0841+2319_X_map.win ! wwins: Wrote 2 windows to /scr/pima/gb073_uvs/J0841+2319_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 5.2% 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 = 0.000265449 Jy ! Component: 100 - total flux cleaned = 0.000409536 Jy ! Component: 150 - total flux cleaned = 0.000463907 Jy ! Component: 200 - total flux cleaned = 0.000489605 Jy ! Component: 250 - total flux cleaned = 0.000440134 Jy ! Component: 300 - total flux cleaned = 0.000464372 Jy ! Component: 350 - total flux cleaned = 0.000488037 Jy ! Component: 400 - total flux cleaned = 0.000534385 Jy ! Component: 450 - total flux cleaned = 0.000487819 Jy ! Component: 500 - total flux cleaned = 0.000487613 Jy ! Component: 550 - total flux cleaned = 0.000398782 Jy ! Component: 600 - total flux cleaned = 0.000377133 Jy ! Component: 650 - total flux cleaned = 0.000311998 Jy ! Component: 700 - total flux cleaned = 0.000205282 Jy ! Component: 750 - total flux cleaned = 0.00014214 Jy ! Component: 800 - total flux cleaned = 7.95301e-05 Jy ! Component: 850 - total flux cleaned = 3.80701e-05 Jy ! Component: 900 - total flux cleaned = 5.84703e-05 Jy ! Component: 950 - total flux cleaned = -2.25399e-05 Jy ! Component: 1000 - total flux cleaned = 5.72794e-05 Jy ! Component: 1050 - total flux cleaned = -2.51809e-06 Jy ! Component: 1100 - total flux cleaned = -2.22425e-05 Jy ! Component: 1150 - total flux cleaned = -4.16781e-05 Jy ! Component: 1200 - total flux cleaned = -6.09034e-05 Jy ! Component: 1250 - total flux cleaned = -4.17929e-05 Jy ! Component: 1300 - total flux cleaned = -3.95128e-06 Jy ! Component: 1350 - total flux cleaned = -4.15429e-05 Jy ! Component: 1400 - total flux cleaned = -4.26922e-06 Jy ! Component: 1450 - total flux cleaned = -4.10503e-05 Jy ! Component: 1500 - total flux cleaned = 5.07923e-05 Jy ! Component: 1550 - total flux cleaned = 5.10888e-05 Jy ! Component: 1600 - total flux cleaned = 0.000123137 Jy ! Component: 1650 - total flux cleaned = 8.74508e-05 Jy ! Component: 1700 - total flux cleaned = 0.000158473 Jy ! Component: 1750 - total flux cleaned = 0.000176142 Jy ! Component: 1800 - total flux cleaned = 0.000263739 Jy ! Component: 1850 - total flux cleaned = 0.000176481 Jy ! Component: 1900 - total flux cleaned = 0.000245891 Jy ! Component: 1950 - total flux cleaned = 0.000314768 Jy ! Component: 2000 - total flux cleaned = 0.00034888 Jy ! Component: 2050 - total flux cleaned = 0.000365834 Jy ! Component: 2100 - total flux cleaned = 0.000433401 Jy ! Component: 2150 - total flux cleaned = 0.00036631 Jy ! Component: 2200 - total flux cleaned = 0.000449724 Jy ! Component: 2250 - total flux cleaned = 0.000499426 Jy ! Component: 2300 - total flux cleaned = 0.000515966 Jy ! Component: 2350 - total flux cleaned = 0.000597833 Jy ! Component: 2400 - total flux cleaned = 0.000630364 Jy ! Component: 2450 - total flux cleaned = 0.000711053 Jy ! Component: 2500 - total flux cleaned = 0.000711165 Jy ! Component: 2550 - total flux cleaned = 0.000695167 Jy ! Component: 2600 - total flux cleaned = 0.000758796 Jy ! Component: 2650 - total flux cleaned = 0.000711358 Jy ! Component: 2700 - total flux cleaned = 0.000821384 Jy ! Component: 2750 - total flux cleaned = 0.000837128 Jy ! Component: 2800 - total flux cleaned = 0.000852728 Jy ! Component: 2850 - total flux cleaned = 0.00091478 Jy ! Component: 2900 - total flux cleaned = 0.000914783 Jy ! Component: 2950 - total flux cleaned = 0.000960736 Jy ! Component: 3000 - total flux cleaned = 0.000960789 Jy ! Component: 3050 - total flux cleaned = 0.00105163 Jy ! Component: 3100 - total flux cleaned = 0.00108173 Jy ! Component: 3150 - total flux cleaned = 0.00106669 Jy ! Component: 3200 - total flux cleaned = 0.00111143 Jy ! Component: 3250 - total flux cleaned = 0.00114124 Jy ! Component: 3300 - total flux cleaned = 0.00124475 Jy ! Component: 3350 - total flux cleaned = 0.00118575 Jy ! Component: 3400 - total flux cleaned = 0.00121505 Jy ! Component: 3450 - total flux cleaned = 0.00122969 Jy ! Component: 3500 - total flux cleaned = 0.00124425 Jy ! Component: 3550 - total flux cleaned = 0.00131662 Jy ! Component: 3600 - total flux cleaned = 0.00127331 Jy ! Component: 3650 - total flux cleaned = 0.00137373 Jy ! Component: 3700 - total flux cleaned = 0.00137372 Jy ! Component: 3750 - total flux cleaned = 0.00141628 Jy ! Component: 3800 - total flux cleaned = 0.00141637 Jy ! Component: 3850 - total flux cleaned = 0.00140221 Jy ! Component: 3900 - total flux cleaned = 0.00145827 Jy ! Component: 3950 - total flux cleaned = 0.0015002 Jy ! Component: 4000 - total flux cleaned = 0.00155588 Jy ! Component: 4050 - total flux cleaned = 0.00150052 Jy ! Total flux subtracted in 4096 components = 0.00154198 Jy ! Clean residual min=-0.000913 max=0.000791 Jy/beam ! Clean residual mean=0.000001 rms=0.000230 Jy/beam ! Combined flux in latest and established models = 0.0870478 Jy keep ! Adding 328 model components to the UV plane model. ! The established model now contains 357 components and 0.0870477 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J0841+2319_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 5.2% 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: 0.8518 x 1.094 at 32.14 degrees (North through East) ! Clean map min=-0.0014228 max=0.073032 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J0841+2319_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0730323 invert ! Inverting map ! Your choice of large map pixels excluded 5.2% 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 0.000229064 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.940942 0.940942 1.88188 3.76377 7.52754 15.0551 30.1102 60.2203 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0006 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.073 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 318.829 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J0841+2319_X_uvs.log closed on Sat Dec 26 09:34:50 2015