! Started logfile: /scr/pima/gb073_uvs/J1838+4802_X_uvs.log on Sat Dec 26 09:44:17 2015 obs /scr/pima/gb073_uvs/J1838+4802_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J1838+4802_X_uva.fits ! AN table 1: 29 integrations on 28 of 28 possible baselines. ! AN table 2: 29 integrations on 45 of 45 possible baselines. ! AN table 3: 29 integrations on 66 of 66 possible baselines. ! AN table 4: 29 integrations on 55 of 55 possible baselines. ! AN table 5: 29 integrations on 36 of 36 possible baselines. ! AN table 6: 29 integrations on 36 of 36 possible baselines. ! Apparent sampling: 0.821623 visibilities/baseline/integration-bin. ! Found source: J1838+4802 ! ! 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 50704 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/J1838+4802_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 58 telescope corrections were flagged in sub-array 2. ! A total of 58 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 58 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 58 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 58 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 58 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 58 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 58 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 5. ! A total of 87 telescope corrections were flagged in sub-array 1. ! A total of 87 telescope corrections were flagged in sub-array 2. ! A total of 87 telescope corrections were flagged in sub-array 3. ! A total of 87 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! A total of 58 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 6. ! A total of 87 telescope corrections were flagged in sub-array 1. ! A total of 87 telescope corrections were flagged in sub-array 2. ! A total of 87 telescope corrections were flagged in sub-array 3. ! A total of 87 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! A total of 58 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 7. ! A total of 58 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 58 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 8. ! A total of 58 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 58 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! A total of 29 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.002308Jy sigma=11.350591 ! Fit after self-cal, rms=0.964812Jy sigma=10.997880 ! clrmod: Cleared the established, tentative and continuum models. ! Redundant starting model cleared. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 milli-arcsec ! Estimated beam: bmin=0.5169 mas, bmaj=1.061 mas, bpa=-21.87 degrees ! Estimated noise=0.744691 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 = 0.0297348 Jy ! Component: 100 - total flux cleaned = 0.0362189 Jy ! Total flux subtracted in 100 components = 0.0362189 Jy ! Clean residual min=-0.002228 max=0.002659 Jy/beam ! Clean residual mean=0.000000 rms=0.000543 Jy/beam ! Combined flux in latest and established models = 0.0362189 Jy ! Performing phase self-cal ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 0.0362189 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=0.062769Jy sigma=0.660901 ! Fit after self-cal, rms=0.060913Jy sigma=0.638786 ! Inverting map ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00364707 Jy ! Component: 100 - total flux cleaned = 0.00349903 Jy ! Total flux subtracted in 100 components = 0.00349903 Jy ! Clean residual min=-0.002502 max=0.002392 Jy/beam ! Clean residual mean=0.000000 rms=0.000514 Jy/beam ! Combined flux in latest and established models = 0.0397179 Jy ! Performing phase self-cal ! Adding 3 model components to the UV plane model. ! The established model now contains 3 components and 0.0397179 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=0.060758Jy sigma=0.638041 ! Fit after self-cal, rms=0.060728Jy sigma=0.637888 ! Inverting map ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 milli-arcsec print "************** FINISHED UNIFORM WEIGHTING CLEAN **************" ! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** ! uvw 0,-1 ! Uniform weighting is not currently selected. ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. win_mult = win_mult * 1.6 clean_niter = clean_niter * 2 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 milli-arcsec ! Estimated beam: bmin=0.783 mas, bmaj=1.49 mas, bpa=-15.08 degrees ! Estimated noise=0.320958 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 = -0.000712142 Jy ! Component: 100 - total flux cleaned = -0.000768829 Jy ! Component: 150 - total flux cleaned = -0.000791365 Jy ! Component: 200 - total flux cleaned = -0.000781785 Jy ! Total flux subtracted in 200 components = -0.000781785 Jy ! Clean residual min=-0.001069 max=0.001247 Jy/beam ! Clean residual mean=0.000002 rms=0.000239 Jy/beam ! Combined flux in latest and established models = 0.0389361 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 13 components and 0.0389361 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=0.060721Jy sigma=0.637750 ! Fit after self-cal, rms=0.060707Jy sigma=0.637732 ! Inverting map ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.783 x 1.49 at -15.08 degrees (North through East) ! Clean map min=-0.00092926 max=0.039634 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* LA 1.00* ! MC 1.00* NL 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.05 EF 1.00* FD 1.03 KP 0.97 ! LA 1.12 NL 0.90 OV 1.01 PT 1.05 ! SC 1.00* ZC 0.96 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.95 EF 1.00* FD 1.00 KP 1.05 ! LA 1.18 MK 1.10 NL 0.96 ON 1.00* ! OV 1.18 PT 0.93 SC 1.08 ZC 0.90 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 EF 1.00* FD 1.00 KP 0.94 ! LA 1.07 MK 0.98 NL 1.01 ON 1.00* ! OV 1.11 PT 0.96 SC 1.02 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 0.93 KP 1.00 LA 0.98 ! MK 1.05 NL 0.99 OV 1.10 PT 1.02 ! SC 0.85 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.90 FD 0.96 KP 1.01 LA 1.03 ! MK 1.03 NL 1.04 ON 1.00* OV 1.02 ! PT 0.96 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.89 EF 1.00* FD 1.01 LA 0.98 ! MC 0.84 NL 0.91 PT 1.04 SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 1.00* OV 1.00* PT 1.00* ! SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.13 EF 1.00* FD 1.10 KP 1.04 ! LA 1.11 MK 1.07 NL 1.19 ON 1.00* ! OV 1.11 PT 1.09 SC 1.00 ZC 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 EF 1.00* FD 1.05 KP 0.89 ! LA 0.97 MK 1.06 NL 1.18 ON 1.00* ! OV 1.01 PT 1.12 SC 1.03 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 1.06 KP 0.91 LA 1.07 ! MK 1.12 NL 1.01 OV 1.13 PT 1.09 ! SC 1.09 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.99 FD 0.95 KP 1.04 LA 1.10 ! MK 1.12 NL 1.13 ON 1.00* OV 1.10 ! PT 1.15 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* LA 1.00* ! MC 1.00* NL 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.05 EF 1.00* FD 1.00 KP 0.95 ! LA 1.02 NL 1.08 OV 0.94 PT 1.09 ! SC 1.00* ZC 1.00 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.17 EF 1.00* FD 1.05 KP 0.99 ! LA 1.03 MK 1.06 NL 1.11 ON 1.00* ! OV 1.04 PT 1.01 SC 1.05 ZC 0.97 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.96 EF 1.00* FD 0.93 KP 1.10 ! LA 1.07 MK 1.07 NL 0.97 ON 1.00* ! OV 0.98 PT 0.88 SC 1.06 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 0.99 KP 0.99 LA 1.02 ! MK 1.03 NL 1.07 OV 0.92 PT 0.95 ! SC 1.07 ! ! 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* ON 1.00* OV 1.00* ! PT 1.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* LA 1.00* ! MC 1.00* NL 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 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* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.01 EF 1.00* FD 1.02 KP 1.13 ! LA 1.14 MK 1.14 NL 0.96 ON 1.00* ! OV 0.93 PT 1.02 SC 1.19 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 1.05 KP 1.03 LA 1.06 ! MK 1.11 NL 1.10 OV 0.95 PT 1.09 ! SC 1.03 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.99 FD 1.05 KP 1.04 LA 1.16 ! MK 1.09 NL 1.04 ON 1.00* OV 1.09 ! PT 1.04 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* LA 1.00* ! MC 1.00* NL 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.02 KP 0.83 ! LA 0.99 NL 0.94 OV 0.95 PT 0.95 ! SC 1.00* ZC 1.06 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 1.16 KP 0.85 ! LA 1.05 MK 0.95 NL 1.18 ON 1.00* ! OV 0.96 PT 1.03 SC 1.10 ZC 0.94 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 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: ! EF 1.00* FD 0.91 KP 1.02 LA 1.16 ! MK 1.08 NL 1.04 OV 0.96 PT 0.87 ! SC 1.05 ! ! 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* ON 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 1.00* LA 1.00* ! MC 1.00* NL 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 0.94 KP 0.90 ! LA 1.01 NL 0.97 OV 1.16 PT 0.90 ! SC 1.00* ZC 0.91 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* EF 1.00* FD 0.94 KP 0.84 ! LA 0.98 MK 1.10 NL 1.08 ON 1.00* ! OV 0.99 PT 1.08 SC 0.92 ZC 0.92 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* EF 1.00* FD 0.90 KP 0.92 ! LA 0.93 MK 1.01 NL 1.09 ON 1.00* ! OV 1.11 PT 0.97 SC 0.97 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 0.86 KP 0.92 LA 0.91 ! MK 1.00 NL 1.08 OV 1.05 PT 0.91 ! SC 1.01 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* FD 0.92 KP 0.89 LA 1.04 ! MK 0.91 NL 0.98 ON 1.00* OV 0.92 ! PT 0.89 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* LA 1.00* ! MC 1.00* NL 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.95 EF 1.00* FD 1.02 KP 0.96 ! LA 1.03 NL 0.94 OV 1.02 PT 0.88 ! SC 1.00* ZC 0.94 ! ! 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* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.12 EF 1.00* FD 0.95 KP 0.87 ! LA 0.96 MK 1.01 NL 1.12 ON 1.00* ! OV 1.02 PT 0.95 SC 1.00 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 0.99 KP 0.96 LA 0.94 ! MK 0.98 NL 0.93 OV 0.91 PT 1.02 ! SC 0.96 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.89 FD 0.95 KP 0.91 LA 1.09 ! MK 1.00 NL 1.03 ON 1.00* OV 1.04 ! PT 1.09 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* EF 1.00* FD 1.00* LA 1.00* ! MC 1.00* NL 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.00* EF 1.00* FD 1.00* KP 1.00* ! LA 1.00* NL 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* ! OV 1.00* PT 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.94 EF 1.00* FD 0.96 KP 0.92 ! LA 1.13 MK 1.01 NL 0.97 ON 1.00* ! OV 1.07 PT 1.00 SC 0.87 ! ! Telescope amplitude corrections in sub-array 5: ! EF 1.00* FD 1.13 KP 0.95 LA 1.06 ! MK 1.12 NL 0.97 OV 0.97 PT 0.84 ! SC 0.95 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.93 FD 0.89 KP 0.86 LA 0.87 ! MK 1.08 NL 1.05 ON 1.00* OV 1.12 ! PT 0.84 ! ! ! Fit before self-cal, rms=0.060707Jy sigma=0.637732 ! Fit after self-cal, rms=0.061158Jy sigma=0.636102 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 milli-arcsec ! Estimated beam: bmin=0.7822 mas, bmaj=1.489 mas, bpa=-15.52 degrees ! Estimated noise=0.324714 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 = 0.000259526 Jy ! Component: 100 - total flux cleaned = 0.000234705 Jy ! Component: 150 - total flux cleaned = 0.000215003 Jy ! Component: 200 - total flux cleaned = 0.000214634 Jy ! Total flux subtracted in 200 components = 0.000214634 Jy ! Clean residual min=-0.000883 max=0.000998 Jy/beam ! Clean residual mean=0.000001 rms=0.000221 Jy/beam ! Combined flux in latest and established models = 0.0391508 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 16 components and 0.0391508 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=0.061149Jy sigma=0.636073 ! Fit after self-cal, rms=0.061158Jy sigma=0.635592 ! Inverting map ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 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=0.061158Jy sigma=0.635592 ! Fit after self-cal, rms=0.061478Jy sigma=0.635472 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 milli-arcsec ! Estimated beam: bmin=0.7812 mas, bmaj=1.48 mas, bpa=-15.9 degrees ! Estimated noise=0.326143 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000209467 Jy ! Component: 100 - total flux cleaned = 0.000199033 Jy ! Component: 150 - total flux cleaned = 0.000190012 Jy ! Component: 200 - total flux cleaned = 0.00019026 Jy ! Total flux subtracted in 200 components = 0.00019026 Jy ! Clean residual min=-0.000893 max=0.000926 Jy/beam ! Clean residual mean=0.000001 rms=0.000221 Jy/beam ! Combined flux in latest and established models = 0.039341 Jy selfcal ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 17 components and 0.039341 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=0.061472Jy sigma=0.635448 ! Fit after self-cal, rms=0.061481Jy sigma=0.635331 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -3.51342e-05 Jy ! Component: 100 - total flux cleaned = -5.87913e-05 Jy ! Component: 150 - total flux cleaned = -7.02521e-05 Jy ! Component: 200 - total flux cleaned = -7.01854e-05 Jy ! Total flux subtracted in 200 components = -7.01854e-05 Jy ! Clean residual min=-0.000890 max=0.000937 Jy/beam ! Clean residual mean=0.000001 rms=0.000220 Jy/beam ! Combined flux in latest and established models = 0.0392708 Jy ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 17 components and 0.0392708 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=0.061478Jy sigma=0.635315 ! Fit after self-cal, rms=0.061474Jy sigma=0.635302 ! Inverting map ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 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=0.061474Jy sigma=0.635302 ! Fit after self-cal, rms=0.061934Jy sigma=0.635288 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 milli-arcsec ! Estimated beam: bmin=0.7819 mas, bmaj=1.481 mas, bpa=-16.08 degrees ! Estimated noise=0.327959 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000164501 Jy ! Component: 100 - total flux cleaned = 0.000146699 Jy ! Component: 150 - total flux cleaned = 0.000132485 Jy ! Component: 200 - total flux cleaned = 0.000132495 Jy ! Total flux subtracted in 200 components = 0.000132495 Jy ! Clean residual min=-0.000900 max=0.000928 Jy/beam ! Clean residual mean=0.000001 rms=0.000221 Jy/beam ! Combined flux in latest and established models = 0.0394033 Jy selfcal ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 17 components and 0.0394033 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=0.061929Jy sigma=0.635276 ! Fit after self-cal, rms=0.061935Jy sigma=0.635240 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 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 = -1.8601e-05 Jy ! Component: 100 - total flux cleaned = -3.90884e-05 Jy ! Component: 150 - total flux cleaned = -4.45243e-05 Jy ! Component: 200 - total flux cleaned = -4.45386e-05 Jy ! Total flux subtracted in 200 components = -4.45386e-05 Jy ! Clean residual min=-0.000925 max=0.000930 Jy/beam ! Clean residual mean=0.000001 rms=0.000221 Jy/beam ! Combined flux in latest and established models = 0.0393588 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 18 components and 0.0393588 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=0.061933Jy sigma=0.635230 ! Fit after self-cal, rms=0.061926Jy sigma=0.635193 ! Inverting map ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 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=0.061926Jy sigma=0.635193 ! Fit after self-cal, rms=0.062317Jy sigma=0.635187 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 milli-arcsec ! Estimated beam: bmin=2.602 mas, bmaj=3.04 mas, bpa=2.17 degrees ! Estimated noise=0.402233 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000383534 Jy ! Component: 100 - total flux cleaned = 0.000421025 Jy ! Component: 150 - total flux cleaned = 0.000421283 Jy ! Component: 200 - total flux cleaned = 0.00042404 Jy ! Total flux subtracted in 200 components = 0.00042404 Jy ! Clean residual min=-0.001020 max=0.000967 Jy/beam ! Clean residual mean=0.000001 rms=0.000282 Jy/beam ! Combined flux in latest and established models = 0.0397828 Jy selfcal ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 20 components and 0.0397828 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=0.062316Jy sigma=0.635206 ! Fit after self-cal, rms=0.062325Jy sigma=0.635189 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 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 = 6.98478e-05 Jy ! Component: 100 - total flux cleaned = 7.02942e-05 Jy ! Component: 150 - total flux cleaned = 7.05844e-05 Jy ! Component: 200 - total flux cleaned = 7.07845e-05 Jy ! Total flux subtracted in 200 components = 7.07845e-05 Jy ! Clean residual min=-0.001025 max=0.000961 Jy/beam ! Clean residual mean=0.000001 rms=0.000282 Jy/beam ! Combined flux in latest and established models = 0.0398536 Jy ! Performing phase self-cal ! Adding 5 model components to the UV plane model. ! The established model now contains 20 components and 0.0398536 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=0.062324Jy sigma=0.635199 ! Fit after self-cal, rms=0.062323Jy sigma=0.635183 ! Inverting map ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. win_mult = win_mult / 1.2 print "************** FINISHED AMPLITUDE SELF-CAL **************" ! ************** FINISHED AMPLITUDE SELF-CAL ************** restore ! Inverting map and beam ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 milli-arcsec ! Estimated beam: bmin=0.7828 mas, bmaj=1.483 mas, bpa=-16.17 degrees ! Estimated noise=0.329519 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7828 x 1.483 at -16.17 degrees (North through East) ! Clean map min=-0.00081173 max=0.040126 Jy/beam if(peak(flux) > thresh) selfcal true, true clean clean_niter,clean_gain selfcal flux_cutoff = imstat(rms) * dynam repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) selfcal true, true end if print "************** CLEARING MODEL AND STARTING OVER **********" ! ************** CLEARING MODEL AND STARTING OVER ********** clrmod true ! clrmod: Cleared the established and tentative models. uvw 2,-1 ! Uniform weighting binwidth: 2 (pixels). ! Gridding weights will be scaled by errors raised to the power -1. ! Radial weighting is not currently selected. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 milli-arcsec ! Estimated beam: bmin=0.5114 mas, bmaj=1.055 mas, bpa=-23.05 degrees ! Estimated noise=0.763158 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0333345 Jy ! Component: 100 - total flux cleaned = 0.0402095 Jy ! Component: 150 - total flux cleaned = 0.0405358 Jy ! Component: 200 - total flux cleaned = 0.040615 Jy ! Total flux subtracted in 200 components = 0.040615 Jy ! Clean residual min=-0.002376 max=0.002221 Jy/beam ! Clean residual mean=-0.000000 rms=0.000512 Jy/beam ! Combined flux in latest and established models = 0.040615 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 6 model components to the UV plane model. ! The established model now contains 6 components and 0.040615 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 milli-arcsec ! Estimated beam: bmin=0.7828 mas, bmaj=1.483 mas, bpa=-16.17 degrees ! Estimated noise=0.329519 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 = -0.00103257 Jy ! Component: 100 - total flux cleaned = -0.00109025 Jy ! Component: 150 - total flux cleaned = -0.00113185 Jy ! Component: 200 - total flux cleaned = -0.00116158 Jy ! Total flux subtracted in 200 components = -0.00116158 Jy ! Clean residual min=-0.000943 max=0.000931 Jy/beam ! Clean residual mean=0.000001 rms=0.000222 Jy/beam ! Combined flux in latest and established models = 0.0394534 Jy ! Adding 6 model components to the UV plane model. ! The established model now contains 8 components and 0.0394534 Jy ! Inverting map ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 milli-arcsec uvtaper 0.3,taper_size ! Gaussian taper: value 0.3 at UV radius = 70 mega-wavelengths. clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 milli-arcsec ! Estimated beam: bmin=2.602 mas, bmaj=3.04 mas, bpa=2.17 degrees ! Estimated noise=0.402233 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000308803 Jy ! Component: 100 - total flux cleaned = 0.000309202 Jy ! Component: 150 - total flux cleaned = 0.00031316 Jy ! Component: 200 - total flux cleaned = 0.000320491 Jy ! Total flux subtracted in 200 components = 0.000320491 Jy ! Clean residual min=-0.001030 max=0.000960 Jy/beam ! Clean residual mean=0.000001 rms=0.000283 Jy/beam ! Combined flux in latest and established models = 0.0397739 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 = 6.93189e-06 Jy ! Component: 100 - total flux cleaned = 1.37134e-05 Jy ! Component: 150 - total flux cleaned = 2.03867e-05 Jy ! Component: 200 - total flux cleaned = 2.68197e-05 Jy ! Total flux subtracted in 200 components = 2.68197e-05 Jy ! Clean residual min=-0.001028 max=0.000961 Jy/beam ! Clean residual mean=0.000001 rms=0.000282 Jy/beam ! Combined flux in latest and established models = 0.0398007 Jy ! Adding 6 model components to the UV plane model. ! The established model now contains 12 components and 0.0398007 Jy ! Inverting map ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 milli-arcsec ! Estimated beam: bmin=0.7828 mas, bmaj=1.483 mas, bpa=-16.17 degrees ! Estimated noise=0.329519 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.000246576 Jy ! Component: 100 - total flux cleaned = -0.000238672 Jy ! Component: 150 - total flux cleaned = -0.000251942 Jy ! Component: 200 - total flux cleaned = -0.000252063 Jy ! Total flux subtracted in 200 components = -0.000252063 Jy ! Clean residual min=-0.000948 max=0.000934 Jy/beam ! Clean residual mean=0.000001 rms=0.000222 Jy/beam ! Combined flux in latest and established models = 0.0395486 Jy selfcal ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 17 components and 0.0395486 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=0.062321Jy sigma=0.635159 ! Fit after self-cal, rms=0.062318Jy sigma=0.635152 wmodel /scr/pima/gb073_uvs/J1838+4802_X_map.mod ! Writing 17 model components to file: /scr/pima/gb073_uvs/J1838+4802_X_map.mod wobs /scr/pima/gb073_uvs/J1838+4802_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J1838+4802_X_uvs.fits wwins /scr/pima/gb073_uvs/J1838+4802_X_map.win ! wwins: Wrote 1 windows to /scr/pima/gb073_uvs/J1838+4802_X_map.win x = (field_size-8) * field_cell / 4 addwin -x,x,-x,x clean (field_size*4),0.01 ! Inverting map ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = 0.000140871 Jy ! Component: 100 - total flux cleaned = 0.00027508 Jy ! Component: 150 - total flux cleaned = 0.000355899 Jy ! Component: 200 - total flux cleaned = 0.000434356 Jy ! Component: 250 - total flux cleaned = 0.000480451 Jy ! Component: 300 - total flux cleaned = 0.000555806 Jy ! Component: 350 - total flux cleaned = 0.000556089 Jy ! Component: 400 - total flux cleaned = 0.000585344 Jy ! Component: 450 - total flux cleaned = 0.000571235 Jy ! Component: 500 - total flux cleaned = 0.000627802 Jy ! Component: 550 - total flux cleaned = 0.000683016 Jy ! Component: 600 - total flux cleaned = 0.00071022 Jy ! Component: 650 - total flux cleaned = 0.000710291 Jy ! Component: 700 - total flux cleaned = 0.000803875 Jy ! Component: 750 - total flux cleaned = 0.000803751 Jy ! Component: 800 - total flux cleaned = 0.00084295 Jy ! Component: 850 - total flux cleaned = 0.000881521 Jy ! Component: 900 - total flux cleaned = 0.000868545 Jy ! Component: 950 - total flux cleaned = 0.000893841 Jy ! Component: 1000 - total flux cleaned = 0.000893872 Jy ! Component: 1050 - total flux cleaned = 0.000918731 Jy ! Component: 1100 - total flux cleaned = 0.000869489 Jy ! Component: 1150 - total flux cleaned = 0.000955045 Jy ! Component: 1200 - total flux cleaned = 0.000979213 Jy ! Component: 1250 - total flux cleaned = 0.00101528 Jy ! Component: 1300 - total flux cleaned = 0.00102724 Jy ! Component: 1350 - total flux cleaned = 0.00110985 Jy ! Component: 1400 - total flux cleaned = 0.00119186 Jy ! Component: 1450 - total flux cleaned = 0.00120349 Jy ! Component: 1500 - total flux cleaned = 0.00124949 Jy ! Component: 1550 - total flux cleaned = 0.00127237 Jy ! Component: 1600 - total flux cleaned = 0.00130649 Jy ! Component: 1650 - total flux cleaned = 0.00132919 Jy ! Component: 1700 - total flux cleaned = 0.00139633 Jy ! Component: 1750 - total flux cleaned = 0.0014298 Jy ! Component: 1800 - total flux cleaned = 0.00147396 Jy ! Component: 1850 - total flux cleaned = 0.0015288 Jy ! Component: 1900 - total flux cleaned = 0.00153958 Jy ! Component: 1950 - total flux cleaned = 0.0016046 Jy ! Component: 2000 - total flux cleaned = 0.00163685 Jy ! Component: 2050 - total flux cleaned = 0.00166896 Jy ! Component: 2100 - total flux cleaned = 0.00169029 Jy ! Component: 2150 - total flux cleaned = 0.00171136 Jy ! Component: 2200 - total flux cleaned = 0.00179552 Jy ! Component: 2250 - total flux cleaned = 0.00177472 Jy ! Component: 2300 - total flux cleaned = 0.00186823 Jy ! Component: 2350 - total flux cleaned = 0.00188891 Jy ! Component: 2400 - total flux cleaned = 0.00196075 Jy ! Component: 2450 - total flux cleaned = 0.00198113 Jy ! Component: 2500 - total flux cleaned = 0.00200137 Jy ! Component: 2550 - total flux cleaned = 0.00203162 Jy ! Component: 2600 - total flux cleaned = 0.00205174 Jy ! Component: 2650 - total flux cleaned = 0.00207182 Jy ! Component: 2700 - total flux cleaned = 0.00213154 Jy ! Component: 2750 - total flux cleaned = 0.0021712 Jy ! Component: 2800 - total flux cleaned = 0.00217119 Jy ! Component: 2850 - total flux cleaned = 0.00226928 Jy ! Component: 2900 - total flux cleaned = 0.00231809 Jy ! Component: 2950 - total flux cleaned = 0.00235696 Jy ! Component: 3000 - total flux cleaned = 0.0023376 Jy ! Component: 3050 - total flux cleaned = 0.00242409 Jy ! Component: 3100 - total flux cleaned = 0.00246244 Jy ! Component: 3150 - total flux cleaned = 0.00245291 Jy ! Component: 3200 - total flux cleaned = 0.00247182 Jy ! Component: 3250 - total flux cleaned = 0.00250959 Jy ! Component: 3300 - total flux cleaned = 0.00251904 Jy ! Component: 3350 - total flux cleaned = 0.00255654 Jy ! Component: 3400 - total flux cleaned = 0.00258451 Jy ! Component: 3450 - total flux cleaned = 0.00259378 Jy ! Component: 3500 - total flux cleaned = 0.00263084 Jy ! Component: 3550 - total flux cleaned = 0.00269539 Jy ! Component: 3600 - total flux cleaned = 0.00268621 Jy ! Component: 3650 - total flux cleaned = 0.00274106 Jy ! Component: 3700 - total flux cleaned = 0.00277745 Jy ! Component: 3750 - total flux cleaned = 0.00277743 Jy ! Component: 3800 - total flux cleaned = 0.0027865 Jy ! Component: 3850 - total flux cleaned = 0.00281346 Jy ! Component: 3900 - total flux cleaned = 0.00285837 Jy ! Component: 3950 - total flux cleaned = 0.00283156 Jy ! Component: 4000 - total flux cleaned = 0.00286715 Jy ! Component: 4050 - total flux cleaned = 0.00287604 Jy ! Total flux subtracted in 4096 components = 0.00288494 Jy ! Clean residual min=-0.000500 max=0.000516 Jy/beam ! Clean residual mean=0.000001 rms=0.000147 Jy/beam ! Combined flux in latest and established models = 0.0424336 Jy keep ! Adding 328 model components to the UV plane model. ! The established model now contains 345 components and 0.0424336 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J1838+4802_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7828 x 1.483 at -16.17 degrees (North through East) ! Clean map min=-0.00068843 max=0.040135 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J1838+4802_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0401347 invert ! Inverting map ! Your choice of large map pixels excluded 0.917% of the data. ! The x-axis pixel size should ideally be below 0.1902 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000146735 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -1.09682 1.09682 2.19365 4.38729 8.77458 17.5492 35.0983 70.1967 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0004 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.04 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 273.517 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J1838+4802_X_uvs.log closed on Sat Dec 26 09:44:23 2015