! Started logfile: /scr/pima/gb073_uvs/J2250+3824_X_uvs.log on Sat Dec 26 09:45:58 2015 obs /scr/pima/gb073_uvs/J2250+3824_X_uva.fits ! Reading UV FITS file: /scr/pima/gb073_uvs/J2250+3824_X_uva.fits ! AN table 1: 29 integrations on 21 of 21 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: 29 integrations on 28 of 28 possible baselines. ! AN table 5: 29 integrations on 36 of 36 possible baselines. ! AN table 6: 58 integrations on 55 of 55 possible baselines. ! Apparent sampling: 0.841334 visibilities/baseline/integration-bin. ! Found source: J2250+3824 ! ! 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 59728 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/J2250+3824_X] float lim_self lim_self = 120.0 float lim_val lim_va = 1.2 integer clean_niter clean_niter = 100 float clean_gain clean_gain = 0.03 float dynam dynam = 6.0 float soltime1 soltime1 = 120 float soltime2 soltime2 = 20 float thresh thresh = 0.5 float win_mult win_mult = 1.8 float time_av time_av = 16 float old_peak float new_peak float flux_cutoff mapsize field_size, field_cell ! Map grid = 1024x1024 pixels with 0.200x0.200 milli-arcsec cellsize. startmod ! Applying default point source starting model. ! Performing phase self-cal ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 1 Jy ! ! Correcting IF 1. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 5. ! A total of 29 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 29 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! A total of 116 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 6. ! A total of 29 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 29 telescope corrections were flagged in sub-array 4. ! A total of 29 telescope corrections were flagged in sub-array 5. ! A total of 116 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 7. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 8. ! A total of 29 telescope corrections were flagged in sub-array 1. ! A total of 29 telescope corrections were flagged in sub-array 2. ! A total of 29 telescope corrections were flagged in sub-array 3. ! A total of 58 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=1.005345Jy sigma=10.831581 ! Fit after self-cal, rms=0.949337Jy sigma=10.230976 ! 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 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 milli-arcsec ! Estimated beam: bmin=0.54 mas, bmaj=1.079 mas, bpa=-9.818 degrees ! Estimated noise=0.676108 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 = 0.0400846 Jy ! Component: 100 - total flux cleaned = 0.0488257 Jy ! Total flux subtracted in 100 components = 0.0488257 Jy ! Clean residual min=-0.002175 max=0.002949 Jy/beam ! Clean residual mean=0.000000 rms=0.000480 Jy/beam ! Combined flux in latest and established models = 0.0488257 Jy ! Performing phase self-cal ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 0.0488257 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=0.071894Jy sigma=0.674980 ! Fit after self-cal, rms=0.070458Jy sigma=0.658412 ! Inverting map ! Your choice of large map pixels excluded 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00357103 Jy ! Component: 100 - total flux cleaned = 0.00523693 Jy ! Total flux subtracted in 100 components = 0.00523693 Jy ! Clean residual min=-0.002171 max=0.002446 Jy/beam ! Clean residual mean=-0.000000 rms=0.000473 Jy/beam ! Combined flux in latest and established models = 0.0540626 Jy ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 7 components and 0.0540626 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=0.070150Jy sigma=0.655071 ! Fit after self-cal, rms=0.070151Jy sigma=0.654976 ! Inverting map ! Your choice of large map pixels excluded 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 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 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 milli-arcsec ! Estimated beam: bmin=0.7315 mas, bmaj=1.452 mas, bpa=-5.04 degrees ! Estimated noise=0.302274 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 (-0.8, -0.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00312384 Jy ! Component: 100 - total flux cleaned = 0.00478417 Jy ! Component: 150 - total flux cleaned = 0.00582041 Jy ! Component: 200 - total flux cleaned = 0.00618102 Jy ! Total flux subtracted in 200 components = 0.00618102 Jy ! Clean residual min=-0.001162 max=0.001792 Jy/beam ! Clean residual mean=0.000000 rms=0.000266 Jy/beam ! Combined flux in latest and established models = 0.0602436 Jy ! Performing phase self-cal ! Adding 16 model components to the UV plane model. ! The established model now contains 20 components and 0.0602436 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=0.070005Jy sigma=0.653362 ! Fit after self-cal, rms=0.069992Jy sigma=0.653007 ! Inverting map ! Your choice of large map pixels excluded 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 milli-arcsec ! Added new window around map position (-2.4, 1.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00187703 Jy ! Component: 100 - total flux cleaned = 0.00284296 Jy ! Component: 150 - total flux cleaned = 0.00322545 Jy ! Component: 200 - total flux cleaned = 0.0033125 Jy ! Total flux subtracted in 200 components = 0.0033125 Jy ! Clean residual min=-0.001081 max=0.001126 Jy/beam ! Clean residual mean=-0.000000 rms=0.000232 Jy/beam ! Combined flux in latest and established models = 0.0635561 Jy ! Performing phase self-cal ! Adding 20 model components to the UV plane model. ! The established model now contains 37 components and 0.0635561 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=0.069941Jy sigma=0.652374 ! Fit after self-cal, rms=0.069930Jy sigma=0.652240 ! Inverting map ! Your choice of large map pixels excluded 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! restore ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7315 x 1.452 at -5.04 degrees (North through East) ! Clean map min=-0.00093257 max=0.053337 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: ! EF 1.00* FD 1.00* LA 1.00* MC 1.00* ! NL 1.00* SC 1.00* ZC 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.91 EF 1.00* FD 1.03 KP 1.06 ! LA 1.11 MC 0.85 NL 1.03 ON 0.91 ! OV 0.96 PT 1.07 SC 0.88 ZC 1.03 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.04 EF 1.00* FD 0.96 KP 1.01 ! LA 1.11 MK 1.01 NL 0.92 ON 0.92 ! PT 1.02 SC 0.97 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.91 FD 1.02 KP 1.01 LA 1.06 ! MK 1.17 NL 0.96 PT 0.89 SC 0.91 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.98 FD 1.04 KP 0.98 LA 1.09 ! MK 0.95 NL 1.01 ON 0.96 PT 0.87 ! SC 0.87 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.90 EF 1.00* FD 0.99 KP 1.03 ! LA 1.01 MK 1.02 NL 0.97 ON 0.86 ! OV 1.06 PT 0.92 SC 0.95 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! EF 1.00* FD 1.00* LA 1.00* MC 1.00* ! NL 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 1.05 EF 1.00* FD 1.02 KP 0.98 ! LA 0.97 MK 1.02 NL 1.14 ON 0.98 ! PT 1.06 SC 0.94 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 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 6: ! BR 1.05 EF 1.00* FD 1.06 KP 1.04 ! LA 1.04 MK 1.02 NL 1.00 ON 0.97 ! OV 1.01 PT 0.99 SC 0.91 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! EF 1.00* FD 1.06 LA 0.91 MC 0.90 ! NL 0.90 SC 1.13 ZC 0.94 ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 EF 1.00* FD 0.97 KP 0.95 ! LA 1.04 MC 1.05 NL 0.98 ON 0.91 ! OV 1.03 PT 0.99 SC 1.07 ZC 0.98 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.03 EF 1.00* FD 0.92 KP 0.95 ! LA 1.01 MK 1.05 NL 1.04 ON 0.90 ! PT 1.02 SC 1.13 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 FD 1.00 KP 0.94 LA 0.99 ! MK 1.06 NL 1.04 PT 0.97 SC 1.05 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.96 FD 0.95 KP 0.99 LA 0.90 ! MK 1.07 NL 0.96 ON 0.88 PT 0.95 ! SC 1.06 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.07 EF 1.00* FD 1.01 KP 0.98 ! LA 0.93 MK 0.99 NL 0.98 ON 0.91 ! OV 1.00 PT 0.96 SC 1.02 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! EF 1.00* FD 0.94 LA 1.09 MC 0.85 ! NL 1.02 SC 0.90 ZC 1.01 ! ! 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 1.11 KP 0.97 ! LA 0.97 MK 1.00 NL 0.98 ON 0.89 ! PT 1.01 SC 1.14 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.00* KP 1.00* LA 1.00* ! MK 1.00* NL 1.00* PT 1.00* SC 1.00* ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.04 FD 0.96 KP 0.92 LA 1.10 ! MK 1.18 NL 0.93 ON 0.88 PT 1.05 ! SC 1.16 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.97 EF 1.00* FD 1.03 KP 1.01 ! LA 1.00 MK 0.98 NL 1.05 ON 0.88 ! OV 0.98 PT 0.99 SC 1.08 ! ! ! Correcting IF 5. ! Telescope amplitude corrections in sub-array 1: ! EF 1.00* FD 0.89 LA 0.99 MC 0.86 ! NL 0.94 SC 0.86 ZC 0.94 ! ! 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 1.04 KP 0.88 ! LA 1.01 MK 1.04 NL 1.11 ON 0.93 ! PT 0.95 SC 0.95 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.01 KP 0.90 LA 1.06 ! MK 1.02 NL 1.02 PT 0.90 SC 0.97 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.00* FD 0.93 KP 0.99 LA 1.02 ! MK 1.02 NL 1.03 ON 1.00 PT 0.96 ! SC 1.11 ! ! Telescope amplitude corrections in sub-array 6: ! BR 1.00* EF 1.00* FD 1.00 KP 0.94 ! LA 0.93 MK 0.98 NL 1.04 ON 1.17 ! OV 1.05 PT 0.98 SC 0.99 ! ! ! Correcting IF 6. ! Telescope amplitude corrections in sub-array 1: ! EF 1.00* FD 1.00* LA 1.00* MC 1.00* ! NL 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 1.02 KP 0.88 ! LA 1.05 MK 1.02 NL 1.10 ON 0.86 ! PT 0.98 SC 0.93 ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 0.94 KP 0.91 LA 0.95 ! MK 1.05 NL 1.14 PT 0.94 SC 1.03 ! ! Telescope amplitude corrections in sub-array 5: ! BR 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 6: ! BR 1.00* EF 1.00* FD 0.99 KP 0.99 ! LA 0.96 MK 1.06 NL 0.97 ON 0.95 ! OV 1.05 PT 1.00 SC 0.99 ! ! ! Correcting IF 7. ! Telescope amplitude corrections in sub-array 1: ! EF 1.00* FD 1.00* LA 1.00* MC 1.00* ! NL 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 0.95 EF 1.00* FD 1.00 KP 0.98 ! LA 1.12 MK 0.99 NL 1.03 ON 1.02 ! PT 1.00 SC 0.98 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.94 FD 1.12 KP 0.92 LA 0.96 ! MK 1.14 NL 1.07 PT 1.01 SC 0.99 ! ! Telescope amplitude corrections in sub-array 5: ! BR 1.11 FD 0.90 KP 0.89 LA 1.09 ! MK 0.99 NL 1.08 ON 0.91 PT 1.03 ! SC 0.95 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.97 EF 1.00* FD 1.00 KP 0.94 ! LA 1.10 MK 1.12 NL 1.15 ON 1.02 ! OV 0.96 PT 1.01 SC 1.01 ! ! ! Correcting IF 8. ! Telescope amplitude corrections in sub-array 1: ! EF 1.00* FD 1.00* LA 1.00* MC 1.00* ! NL 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 1.08 EF 1.00* FD 0.84 KP 0.93 ! LA 1.15 MK 0.97 NL 1.02 ON 1.01 ! PT 0.95 SC 1.08 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.92 FD 0.93 KP 0.99 LA 0.95 ! MK 1.14 NL 1.16 PT 0.97 SC 1.05 ! ! Telescope amplitude corrections in sub-array 5: ! BR 0.95 FD 1.02 KP 0.93 LA 1.02 ! MK 1.10 NL 1.09 ON 1.13 PT 0.90 ! SC 0.87 ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.96 EF 1.00* FD 1.00 KP 0.89 ! LA 0.99 MK 1.00 NL 1.06 ON 1.05 ! OV 0.97 PT 1.03 SC 1.05 ! ! ! Fit before self-cal, rms=0.069930Jy sigma=0.652240 ! Fit after self-cal, rms=0.069412Jy sigma=0.650820 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 milli-arcsec ! Estimated beam: bmin=0.7333 mas, bmaj=1.441 mas, bpa=-5.221 degrees ! Estimated noise=0.30146 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 = 0.000388705 Jy ! Component: 100 - total flux cleaned = 0.000369137 Jy ! Component: 150 - total flux cleaned = 0.000402091 Jy ! Component: 200 - total flux cleaned = 0.000416117 Jy ! Total flux subtracted in 200 components = 0.000416117 Jy ! Clean residual min=-0.000962 max=0.000896 Jy/beam ! Clean residual mean=0.000000 rms=0.000208 Jy/beam ! Combined flux in latest and established models = 0.0639722 Jy ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 50 components and 0.0639722 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=0.069402Jy sigma=0.650700 ! Fit after self-cal, rms=0.069406Jy sigma=0.650481 ! Inverting map ! Your choice of large map pixels excluded 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 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=0.069406Jy sigma=0.650481 ! Fit after self-cal, rms=0.069511Jy sigma=0.650305 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 milli-arcsec ! Estimated beam: bmin=0.7336 mas, bmaj=1.442 mas, bpa=-5.211 degrees ! Estimated noise=0.301373 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 7.79074e-05 Jy ! Component: 100 - total flux cleaned = 0.000109701 Jy ! Component: 150 - total flux cleaned = 0.000137357 Jy ! Component: 200 - total flux cleaned = 0.000186373 Jy ! Total flux subtracted in 200 components = 0.000186373 Jy ! Clean residual min=-0.000958 max=0.000902 Jy/beam ! Clean residual mean=0.000000 rms=0.000204 Jy/beam ! Combined flux in latest and established models = 0.0641586 Jy selfcal ! Performing phase self-cal ! Adding 23 model components to the UV plane model. ! The established model now contains 57 components and 0.0641586 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=0.069505Jy sigma=0.650243 ! Fit after self-cal, rms=0.069510Jy sigma=0.650206 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 milli-arcsec repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000106573 Jy ! Component: 100 - total flux cleaned = 0.000143033 Jy ! Component: 150 - total flux cleaned = 0.000142991 Jy ! Component: 200 - total flux cleaned = 0.000143124 Jy ! Total flux subtracted in 200 components = 0.000143124 Jy ! Clean residual min=-0.000964 max=0.000898 Jy/beam ! Clean residual mean=0.000000 rms=0.000203 Jy/beam ! Combined flux in latest and established models = 0.0643018 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 63 components and 0.0643018 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=0.069506Jy sigma=0.650174 ! Fit after self-cal, rms=0.069503Jy sigma=0.650170 ! Inverting map ! Your choice of large map pixels excluded 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 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=0.069503Jy sigma=0.650170 ! Fit after self-cal, rms=0.069590Jy sigma=0.650055 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 milli-arcsec ! Estimated beam: bmin=0.7334 mas, bmaj=1.442 mas, bpa=-5.223 degrees ! Estimated noise=0.301021 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 3.04415e-07 Jy ! Component: 100 - total flux cleaned = 3.52153e-05 Jy ! Component: 150 - total flux cleaned = 4.61648e-05 Jy ! Component: 200 - total flux cleaned = 5.62704e-05 Jy ! Total flux subtracted in 200 components = 5.62704e-05 Jy ! Clean residual min=-0.000958 max=0.000895 Jy/beam ! Clean residual mean=-0.000000 rms=0.000200 Jy/beam ! Combined flux in latest and established models = 0.064358 Jy selfcal ! Performing phase self-cal ! Adding 21 model components to the UV plane model. ! The established model now contains 66 components and 0.0643581 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=0.069587Jy sigma=0.650024 ! Fit after self-cal, rms=0.069593Jy sigma=0.650003 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 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 = 4.62291e-05 Jy ! Component: 100 - total flux cleaned = 5.67949e-05 Jy ! Component: 150 - total flux cleaned = 4.75214e-05 Jy ! Component: 200 - total flux cleaned = 3.86863e-05 Jy ! Total flux subtracted in 200 components = 3.86863e-05 Jy ! Clean residual min=-0.000962 max=0.000896 Jy/beam ! Clean residual mean=0.000000 rms=0.000200 Jy/beam ! Combined flux in latest and established models = 0.0643967 Jy ! Performing phase self-cal ! Adding 25 model components to the UV plane model. ! The established model now contains 70 components and 0.0643968 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=0.069590Jy sigma=0.649982 ! Fit after self-cal, rms=0.069588Jy sigma=0.649978 ! Inverting map ! Your choice of large map pixels excluded 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 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=0.069588Jy sigma=0.649978 ! Fit after self-cal, rms=0.069569Jy sigma=0.649976 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 milli-arcsec ! Estimated beam: bmin=2.41 mas, bmaj=2.963 mas, bpa=4.792 degrees ! Estimated noise=0.38597 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -9.09972e-05 Jy ! Component: 100 - total flux cleaned = -3.81703e-05 Jy ! Component: 150 - total flux cleaned = 1.2895e-06 Jy ! Component: 200 - total flux cleaned = 1.43726e-06 Jy ! Total flux subtracted in 200 components = 1.43726e-06 Jy ! Clean residual min=-0.001035 max=0.001050 Jy/beam ! Clean residual mean=0.000000 rms=0.000268 Jy/beam ! Combined flux in latest and established models = 0.0643982 Jy selfcal ! Performing phase self-cal ! Adding 9 model components to the UV plane model. ! The established model now contains 76 components and 0.0643982 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=0.069571Jy sigma=0.649984 ! Fit after self-cal, rms=0.069567Jy sigma=0.649968 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 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 = -7.96169e-06 Jy ! Component: 100 - total flux cleaned = 4.13978e-05 Jy ! Component: 150 - total flux cleaned = 6.07967e-05 Jy ! Component: 200 - total flux cleaned = 6.06818e-05 Jy ! Total flux subtracted in 200 components = 6.06818e-05 Jy ! Clean residual min=-0.001043 max=0.001053 Jy/beam ! Clean residual mean=0.000000 rms=0.000267 Jy/beam ! Combined flux in latest and established models = 0.0644589 Jy ! Performing phase self-cal ! Adding 14 model components to the UV plane model. ! The established model now contains 80 components and 0.0644589 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=0.069568Jy sigma=0.649982 ! Fit after self-cal, rms=0.069566Jy sigma=0.649977 ! Inverting map ! Your choice of large map pixels excluded 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 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 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 milli-arcsec ! Estimated beam: bmin=0.733 mas, bmaj=1.443 mas, bpa=-5.235 degrees ! Estimated noise=0.300747 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.733 x 1.443 at -5.235 degrees (North through East) ! Clean map min=-0.0010002 max=0.053103 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 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 milli-arcsec ! Estimated beam: bmin=0.5408 mas, bmaj=1.07 mas, bpa=-10.09 degrees ! Estimated noise=0.672885 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0410937 Jy ! Component: 100 - total flux cleaned = 0.0501892 Jy ! Component: 150 - total flux cleaned = 0.053689 Jy ! Component: 200 - total flux cleaned = 0.0560964 Jy ! Total flux subtracted in 200 components = 0.0560964 Jy ! Clean residual min=-0.002032 max=0.001961 Jy/beam ! Clean residual mean=0.000000 rms=0.000456 Jy/beam ! Combined flux in latest and established models = 0.0560964 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 13 model components to the UV plane model. ! The established model now contains 13 components and 0.0560964 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 milli-arcsec ! Estimated beam: bmin=0.733 mas, bmaj=1.443 mas, bpa=-5.235 degrees ! Estimated noise=0.300747 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 = 0.0032149 Jy ! Component: 100 - total flux cleaned = 0.00525549 Jy ! Component: 150 - total flux cleaned = 0.00661878 Jy ! Component: 200 - total flux cleaned = 0.00717342 Jy ! Total flux subtracted in 200 components = 0.00717342 Jy ! Clean residual min=-0.000963 max=0.001040 Jy/beam ! Clean residual mean=-0.000000 rms=0.000212 Jy/beam ! Combined flux in latest and established models = 0.0632699 Jy ! Adding 27 model components to the UV plane model. ! The established model now contains 35 components and 0.0632699 Jy ! Inverting map ! Your choice of large map pixels excluded 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 milli-arcsec ! Added new window around map position (-11.2, 8.8). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000623469 Jy ! Component: 100 - total flux cleaned = 0.0008019 Jy ! Component: 150 - total flux cleaned = 0.000937449 Jy ! Component: 200 - total flux cleaned = 0.00106201 Jy ! Total flux subtracted in 200 components = 0.00106201 Jy ! Clean residual min=-0.000933 max=0.000836 Jy/beam ! Clean residual mean=0.000000 rms=0.000201 Jy/beam ! Combined flux in latest and established models = 0.0643319 Jy ! Adding 29 model components to the UV plane model. ! The established model now contains 49 components and 0.0643319 Jy ! Inverting map ! Your choice of large map pixels excluded 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 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 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 milli-arcsec ! Estimated beam: bmin=2.41 mas, bmaj=2.963 mas, bpa=4.792 degrees ! Estimated noise=0.38597 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000367894 Jy ! Component: 100 - total flux cleaned = 0.000541897 Jy ! Component: 150 - total flux cleaned = 0.000673454 Jy ! Component: 200 - total flux cleaned = 0.000744631 Jy ! Total flux subtracted in 200 components = 0.000744631 Jy ! Clean residual min=-0.001002 max=0.001000 Jy/beam ! Clean residual mean=0.000000 rms=0.000257 Jy/beam ! Combined flux in latest and established models = 0.0650765 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 = 5.06992e-05 Jy ! Component: 100 - total flux cleaned = 9.47632e-05 Jy ! Component: 150 - total flux cleaned = 0.000126171 Jy ! Component: 200 - total flux cleaned = 0.00014716 Jy ! Total flux subtracted in 200 components = 0.00014716 Jy ! Clean residual min=-0.000994 max=0.000980 Jy/beam ! Clean residual mean=0.000000 rms=0.000255 Jy/beam ! Combined flux in latest and established models = 0.0652237 Jy ! Adding 27 model components to the UV plane model. ! The established model now contains 70 components and 0.0652237 Jy ! Inverting map ! Your choice of large map pixels excluded 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 milli-arcsec ! Estimated beam: bmin=0.733 mas, bmaj=1.443 mas, bpa=-5.235 degrees ! Estimated noise=0.300747 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -1.76502e-05 Jy ! Component: 100 - total flux cleaned = -1.81062e-05 Jy ! Component: 150 - total flux cleaned = -1.84128e-05 Jy ! Component: 200 - total flux cleaned = -4.79365e-06 Jy ! Total flux subtracted in 200 components = -4.79365e-06 Jy ! Clean residual min=-0.000911 max=0.000852 Jy/beam ! Clean residual mean=0.000000 rms=0.000195 Jy/beam ! Combined flux in latest and established models = 0.0652189 Jy selfcal ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 79 components and 0.0652189 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=0.069574Jy sigma=0.649964 ! Fit after self-cal, rms=0.069577Jy sigma=0.649916 wmodel /scr/pima/gb073_uvs/J2250+3824_X_map.mod ! Writing 79 model components to file: /scr/pima/gb073_uvs/J2250+3824_X_map.mod wobs /scr/pima/gb073_uvs/J2250+3824_X_uvs.fits ! Writing UV FITS file: /scr/pima/gb073_uvs/J2250+3824_X_uvs.fits wwins /scr/pima/gb073_uvs/J2250+3824_X_map.win ! wwins: Wrote 4 windows to /scr/pima/gb073_uvs/J2250+3824_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 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 milli-arcsec ! clean: niter=4096 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -0.000202352 Jy ! Component: 100 - total flux cleaned = -0.000352374 Jy ! Component: 150 - total flux cleaned = -0.000467271 Jy ! Component: 200 - total flux cleaned = -0.000564978 Jy ! Component: 250 - total flux cleaned = -0.000660393 Jy ! Component: 300 - total flux cleaned = -0.000753861 Jy ! Component: 350 - total flux cleaned = -0.000845691 Jy ! Component: 400 - total flux cleaned = -0.000936076 Jy ! Component: 450 - total flux cleaned = -0.00101256 Jy ! Component: 500 - total flux cleaned = -0.00105055 Jy ! Component: 550 - total flux cleaned = -0.00105069 Jy ! Component: 600 - total flux cleaned = -0.00106299 Jy ! Component: 650 - total flux cleaned = -0.0011114 Jy ! Component: 700 - total flux cleaned = -0.00108746 Jy ! Component: 750 - total flux cleaned = -0.00111121 Jy ! Component: 800 - total flux cleaned = -0.00109939 Jy ! Component: 850 - total flux cleaned = -0.00109962 Jy ! Component: 900 - total flux cleaned = -0.00113436 Jy ! Component: 950 - total flux cleaned = -0.00115719 Jy ! Component: 1000 - total flux cleaned = -0.00112293 Jy ! Component: 1050 - total flux cleaned = -0.00116808 Jy ! Component: 1100 - total flux cleaned = -0.00113444 Jy ! Component: 1150 - total flux cleaned = -0.00115675 Jy ! Component: 1200 - total flux cleaned = -0.00116776 Jy ! Component: 1250 - total flux cleaned = -0.0011568 Jy ! Component: 1300 - total flux cleaned = -0.0012003 Jy ! Component: 1350 - total flux cleaned = -0.00116777 Jy ! Component: 1400 - total flux cleaned = -0.0011677 Jy ! Component: 1450 - total flux cleaned = -0.00117838 Jy ! Component: 1500 - total flux cleaned = -0.00119954 Jy ! Component: 1550 - total flux cleaned = -0.00118893 Jy ! Component: 1600 - total flux cleaned = -0.00118896 Jy ! Component: 1650 - total flux cleaned = -0.0011786 Jy ! Component: 1700 - total flux cleaned = -0.00114735 Jy ! Component: 1750 - total flux cleaned = -0.00109577 Jy ! Component: 1800 - total flux cleaned = -0.001106 Jy ! Component: 1850 - total flux cleaned = -0.00107546 Jy ! Component: 1900 - total flux cleaned = -0.00106537 Jy ! Component: 1950 - total flux cleaned = -0.00103505 Jy ! Component: 2000 - total flux cleaned = -0.0010452 Jy ! Component: 2050 - total flux cleaned = -0.00100527 Jy ! Component: 2100 - total flux cleaned = -0.000995339 Jy ! Component: 2150 - total flux cleaned = -0.000985504 Jy ! Component: 2200 - total flux cleaned = -0.00102486 Jy ! Component: 2250 - total flux cleaned = -0.000985692 Jy ! Component: 2300 - total flux cleaned = -0.000975947 Jy ! Component: 2350 - total flux cleaned = -0.000937064 Jy ! Component: 2400 - total flux cleaned = -0.000956425 Jy ! Component: 2450 - total flux cleaned = -0.00095645 Jy ! Component: 2500 - total flux cleaned = -0.000965979 Jy ! Component: 2550 - total flux cleaned = -0.0010042 Jy ! Component: 2600 - total flux cleaned = -0.000947087 Jy ! Component: 2650 - total flux cleaned = -0.000937625 Jy ! Component: 2700 - total flux cleaned = -0.000937613 Jy ! Component: 2750 - total flux cleaned = -0.000937682 Jy ! Component: 2800 - total flux cleaned = -0.000928316 Jy ! Component: 2850 - total flux cleaned = -0.000937594 Jy ! Component: 2900 - total flux cleaned = -0.000937603 Jy ! Component: 2950 - total flux cleaned = -0.000965276 Jy ! Component: 3000 - total flux cleaned = -0.000873199 Jy ! Component: 3050 - total flux cleaned = -0.000873168 Jy ! Component: 3100 - total flux cleaned = -0.000864001 Jy ! Component: 3150 - total flux cleaned = -0.000863973 Jy ! Component: 3200 - total flux cleaned = -0.000845853 Jy ! Component: 3250 - total flux cleaned = -0.000827787 Jy ! Component: 3300 - total flux cleaned = -0.000809732 Jy ! Component: 3350 - total flux cleaned = -0.000764803 Jy ! Component: 3400 - total flux cleaned = -0.000782657 Jy ! Component: 3450 - total flux cleaned = -0.000791561 Jy ! Component: 3500 - total flux cleaned = -0.000809284 Jy ! Component: 3550 - total flux cleaned = -0.000773868 Jy ! Component: 3600 - total flux cleaned = -0.000765081 Jy ! Component: 3650 - total flux cleaned = -0.000756292 Jy ! Component: 3700 - total flux cleaned = -0.000738787 Jy ! Component: 3750 - total flux cleaned = -0.000756264 Jy ! Component: 3800 - total flux cleaned = -0.000712738 Jy ! Component: 3850 - total flux cleaned = -0.000704067 Jy ! Component: 3900 - total flux cleaned = -0.000704066 Jy ! Component: 3950 - total flux cleaned = -0.000669588 Jy ! Component: 4000 - total flux cleaned = -0.000643818 Jy ! Component: 4050 - total flux cleaned = -0.000686619 Jy ! Total flux subtracted in 4096 components = -0.000678062 Jy ! Clean residual min=-0.000507 max=0.000656 Jy/beam ! Clean residual mean=0.000000 rms=0.000143 Jy/beam ! Combined flux in latest and established models = 0.0645408 Jy keep ! Adding 338 model components to the UV plane model. ! The established model now contains 417 components and 0.0645408 Jy ![Exited script file: /home/lpetrov/bin/01_muppet] wmap "/scr/pima/gb073_uvs/J2250+3824_X\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.733 x 1.443 at -5.235 degrees (North through East) ! Clean map min=-0.00097397 max=0.052897 Jy/beam ! Writing clean map to FITS file: /scr/pima/gb073_uvs/J2250+3824_X_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 0.0528973 invert ! Inverting map ! Your choice of large map pixels excluded 2.63% of the data. ! The x-axis pixel size should ideally be below 0.1797 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.000143335 loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.812908 0.812908 1.62582 3.25163 6.50326 13.0065 26.013 52.0261 print "clev= ", int(3*image_rms*10000)/10000 ! clev= 0.0004 print "peak= ", int(1000*peak_flux)/1000 ! peak= 0.052 print "dyn_range= ", int(1000*peak_flux/image_rms)/1000 ! dyn_range= 369.045 quit ! Quitting program ! Log file /scr/pima/gb073_uvs/J2250+3824_X_uvs.log closed on Sat Dec 26 09:46:05 2015