! Started logfile: J1743-0350_X_2001_07_05_pus_uvs.log on Wed Jul 4 21:34:15 2007 obs J1743-0350_X_2001_07_05_pus_uva.fits ! Reading UV FITS file: J1743-0350_X_2001_07_05_pus_uva.fits ! AN table 1: 153 integrations on 171 of 171 possible baselines. ! AN table 2: 10 integrations on 171 of 171 possible baselines. ! AN table 3: 66 integrations on 171 of 171 possible baselines. ! AN table 4: 177 integrations on 171 of 171 possible baselines. ! AN table 5: 128 integrations on 171 of 171 possible baselines. ! AN table 6: 17 integrations on 171 of 171 possible baselines. ! Apparent sampling: 0.140022 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: J1743-0350 ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! Warning: Unknown AN-table MNTSTA value (3). ! Will assume that it is ground-based. ! ! There are 4 IFs, and a total of 4 channels: ! ! IF Channel Frequency Freq offset Number of Overall IF ! origin at origin per channel channels bandwidth ! ------------------------------------------------------------- (Hz) ! 01 1 8.40997e+09 8e+06 1 8e+06 ! 02 2 8.47997e+09 8e+06 1 8e+06 ! 03 3 8.79497e+09 8e+06 1 8e+06 ! 04 4 8.89997e+09 8e+06 1 8e+06 ! ! Polarization(s): RR ! ! Read 2370 lines of history. ! ! Reading 52772 visibilities. select I ! Polarization I is unavailable. ! Selecting polarization: RR, channels: 1..4 ! Reading IF 1 channels: 1..1 ! Reading IF 2 channels: 2..2 ! Reading IF 3 channels: 3..3 ! Reading IF 4 channels: 4..4 print "field_size =",field_size ! field_size = 256 print "field_cell =",field_cell ! field_cell = 0.2 print "taper_size =",taper_size ! taper_size = 70 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 = 256x256 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 1595 telescope corrections were flagged in sub-array 1. ! A total of 190 telescope corrections were flagged in sub-array 2. ! A total of 581 telescope corrections were flagged in sub-array 3. ! A total of 2609 telescope corrections were flagged in sub-array 4. ! A total of 1879 telescope corrections were flagged in sub-array 5. ! A total of 323 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 2. ! A total of 1595 telescope corrections were flagged in sub-array 1. ! A total of 190 telescope corrections were flagged in sub-array 2. ! A total of 581 telescope corrections were flagged in sub-array 3. ! A total of 2609 telescope corrections were flagged in sub-array 4. ! A total of 1879 telescope corrections were flagged in sub-array 5. ! A total of 323 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 3. ! A total of 1595 telescope corrections were flagged in sub-array 1. ! A total of 190 telescope corrections were flagged in sub-array 2. ! A total of 581 telescope corrections were flagged in sub-array 3. ! A total of 2609 telescope corrections were flagged in sub-array 4. ! A total of 1879 telescope corrections were flagged in sub-array 5. ! A total of 323 telescope corrections were flagged in sub-array 6. ! ! Correcting IF 4. ! A total of 1595 telescope corrections were flagged in sub-array 1. ! A total of 190 telescope corrections were flagged in sub-array 2. ! A total of 581 telescope corrections were flagged in sub-array 3. ! A total of 2609 telescope corrections were flagged in sub-array 4. ! A total of 1879 telescope corrections were flagged in sub-array 5. ! A total of 323 telescope corrections were flagged in sub-array 6. ! ! Fit before self-cal, rms=3.187840Jy sigma=0.030043 ! Fit after self-cal, rms=2.771112Jy sigma=0.025963 ! 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 3.17% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=0.5619 mas, bmaj=1.402 mas, bpa=-2.797 degrees ! Estimated noise=821.229 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 = 2.63125 Jy ! Component: 100 - total flux cleaned = 3.36147 Jy ! Total flux subtracted in 100 components = 3.36147 Jy ! Clean residual min=-0.081747 max=0.338111 Jy/beam ! Clean residual mean=0.002980 rms=0.033957 Jy/beam ! Combined flux in latest and established models = 3.36147 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 10 components and 3.36147 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.736717Jy sigma=0.007136 ! Fit after self-cal, rms=0.736503Jy sigma=0.007134 ! Inverting map ! Your choice of large map pixels excluded 3.17% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.393019 Jy ! Component: 100 - total flux cleaned = 0.631633 Jy ! Total flux subtracted in 100 components = 0.631634 Jy ! Clean residual min=-0.046664 max=0.124857 Jy/beam ! Clean residual mean=0.000968 rms=0.016520 Jy/beam ! Combined flux in latest and established models = 3.99311 Jy ! Performing phase self-cal ! Adding 15 model components to the UV plane model. ! The established model now contains 20 components and 3.99311 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.378657Jy sigma=0.003428 ! Fit after self-cal, rms=0.377850Jy sigma=0.003420 ! Inverting map ! Your choice of large map pixels excluded 3.17% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.158698 Jy ! Component: 100 - total flux cleaned = 0.267876 Jy ! Total flux subtracted in 100 components = 0.267876 Jy ! Clean residual min=-0.040246 max=0.066236 Jy/beam ! Clean residual mean=0.000124 rms=0.011012 Jy/beam ! Combined flux in latest and established models = 4.26098 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 26 components and 4.26098 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.306009Jy sigma=0.002444 ! Fit after self-cal, rms=0.304979Jy sigma=0.002435 ! Inverting map ! Your choice of large map pixels excluded 3.17% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec ! Added new window around map position (0.2, -1.4). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0809663 Jy ! Component: 100 - total flux cleaned = 0.137515 Jy ! Total flux subtracted in 100 components = 0.137515 Jy ! Clean residual min=-0.036813 max=0.037369 Jy/beam ! Clean residual mean=-0.000309 rms=0.008986 Jy/beam ! Combined flux in latest and established models = 4.3985 Jy ! Performing phase self-cal ! Adding 12 model components to the UV plane model. ! The established model now contains 32 components and 4.3985 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.299850Jy sigma=0.002247 ! Fit after self-cal, rms=0.299361Jy sigma=0.002242 ! Inverting map ! Your choice of large map pixels excluded 3.17% of the data. ! The x-axis pixel size should ideally be below 0.1608 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 3.17% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=0.7431 mas, bmaj=2.133 mas, bpa=-6.221 degrees ! Estimated noise=353.043 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 = -0.0072803 Jy ! Component: 100 - total flux cleaned = -0.00975401 Jy ! Component: 150 - total flux cleaned = -0.00978734 Jy ! Component: 200 - total flux cleaned = -0.00936486 Jy ! Total flux subtracted in 200 components = -0.00936486 Jy ! Clean residual min=-0.035631 max=0.039913 Jy/beam ! Clean residual mean=-0.001806 rms=0.009968 Jy/beam ! Combined flux in latest and established models = 4.38913 Jy ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 41 components and 4.38913 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.295675Jy sigma=0.002223 ! Fit after self-cal, rms=0.295623Jy sigma=0.002222 ! Inverting map ! Your choice of large map pixels excluded 3.17% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec print "************** FINISHED NATURAL WEIGHTING CLEAN **************" ! ************** FINISHED NATURAL WEIGHTING CLEAN ************** ! gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.02 GC 1.00* GG 1.00* ! HH 1.27 HN 0.98 KK 1.00* KP 1.10 ! LA 1.02 MC 1.07 MK 1.00* NL 1.01 ! NY 1.00* OV 1.00* PT 1.01 SC 1.00 ! TS 1.00* WF 1.01 WZ 0.97 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HH 0.00* HN 0.00* KK 0.00* KP 0.00* ! LA 0.00* MC 0.00* MK 0.00* NL 0.00* ! NY 0.00* OV 0.00* PT 0.00* SC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.97 FD 1.00 GC 0.99 GG 1.00* ! HH 1.00* HN 0.99 KK 0.99 KP 0.99 ! LA 0.97 MC 1.00* MK 0.97 NL 1.00 ! NY 1.00* OV 0.98 PT 1.00 SC 1.05 ! TS 1.00* WF 1.02 WZ 1.00* ! ! A total of 36 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.97 FD 1.02 GC 1.01 GG 1.00* ! HH 1.00* HN 1.00* KK 1.02 KP 1.01 ! LA 1.00 MC 1.00* MK 0.98 NL 1.02 ! NY 1.00* OV 0.99 PT 1.01 SC 1.00* ! TS 0.99 WF 1.00* WZ 1.00* ! ! A total of 282 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.96 FD 0.96 GC 1.00* GG 1.00* ! HH 1.00* HN 0.96 KK 1.20 KP 0.94 ! LA 0.98 MC 1.00* MK 1.01 NL 0.98 ! NY 1.00* OV 0.98 PT 0.98 SC 1.03 ! TS 1.00* WF 0.99 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HH 0.00* HN 0.00* KK 0.00* KP 0.00* ! LA 0.00* MC 0.00* MK 0.00* NL 0.00* ! NY 0.00* OV 0.00* PT 0.00* SC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.01 GC 1.00* GG 1.00* ! HH 1.27 HN 0.97 KK 1.00* KP 1.12 ! LA 1.01 MC 1.07 MK 1.00* NL 0.97 ! NY 1.00* OV 1.00* PT 0.98 SC 0.96 ! TS 1.00* WF 1.00 WZ 0.98 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HH 0.00* HN 0.00* KK 0.00* KP 0.00* ! LA 0.00* MC 0.00* MK 0.00* NL 0.00* ! NY 0.00* OV 0.00* PT 0.00* SC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.98 FD 0.99 GC 0.96 GG 1.00* ! HH 1.00* HN 0.99 KK 0.98 KP 0.99 ! LA 0.97 MC 1.00* MK 0.97 NL 0.96 ! NY 1.00* OV 0.98 PT 0.97 SC 1.01 ! TS 1.00* WF 1.00 WZ 1.00* ! ! A total of 36 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 FD 1.01 GC 0.97 GG 1.00* ! HH 1.00* HN 1.00* KK 1.02 KP 1.02 ! LA 0.99 MC 1.00* MK 0.97 NL 0.99 ! NY 1.00* OV 0.99 PT 0.98 SC 1.00* ! TS 0.99 WF 1.00* WZ 1.00* ! ! A total of 282 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.97 FD 0.96 GC 1.00* GG 1.00* ! HH 1.00* HN 0.96 KK 1.20 KP 0.94 ! LA 0.97 MC 1.00* MK 1.01 NL 0.94 ! NY 1.00* OV 0.97 PT 0.95 SC 0.98 ! TS 1.00* WF 0.99 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HH 0.00* HN 0.00* KK 0.00* KP 0.00* ! LA 0.00* MC 0.00* MK 0.00* NL 0.00* ! NY 0.00* OV 0.00* PT 0.00* SC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.99 GC 1.00* GG 1.00* ! HH 1.36 HN 0.98 KK 1.00* KP 1.16 ! LA 1.03 MC 1.07 MK 1.00* NL 1.00 ! NY 1.00* OV 1.00* PT 1.00 SC 0.98 ! TS 1.00* WF 1.00 WZ 0.96 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HH 0.00* HN 0.00* KK 0.00* KP 0.00* ! LA 0.00* MC 0.00* MK 0.00* NL 0.00* ! NY 0.00* OV 0.00* PT 0.00* SC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.02 FD 0.97 GC 1.00 GG 1.00* ! HH 1.00* HN 0.99 KK 0.96 KP 1.03 ! LA 0.98 MC 1.00* MK 0.98 NL 0.98 ! NY 1.00* OV 1.02 PT 0.99 SC 1.03 ! TS 1.00* WF 1.00 WZ 1.00* ! ! A total of 36 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.02 FD 0.99 GC 1.02 GG 1.00* ! HH 1.00* HN 1.00* KK 0.99 KP 1.05 ! LA 1.01 MC 1.00* MK 0.99 NL 1.02 ! NY 1.00* OV 1.03 PT 1.00 SC 1.00* ! TS 0.97 WF 1.00* WZ 1.00* ! ! A total of 282 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 1.01 FD 0.94 GC 1.00* GG 1.00* ! HH 1.00* HN 0.97 KK 1.18 KP 0.98 ! LA 0.98 MC 1.00* MK 1.02 NL 0.97 ! NY 1.00* OV 1.01 PT 0.97 SC 0.99 ! TS 1.00* WF 0.99 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HH 0.00* HN 0.00* KK 0.00* KP 0.00* ! LA 0.00* MC 0.00* MK 0.00* NL 0.00* ! NY 0.00* OV 0.00* PT 0.00* SC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 0.98 GC 1.00* GG 1.00* ! HH 1.59 HN 1.00 KK 1.00* KP 1.13 ! LA 1.01 MC 1.06 MK 1.00* NL 1.01 ! NY 1.00* OV 1.00* PT 1.00 SC 1.03 ! TS 1.00* WF 1.00 WZ 0.96 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HH 0.00* HN 0.00* KK 0.00* KP 0.00* ! LA 0.00* MC 0.00* MK 0.00* NL 0.00* ! NY 0.00* OV 0.00* PT 0.00* SC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 FD 0.95 GC 1.00 GG 1.00* ! HH 1.00* HN 1.01 KK 0.98 KP 0.99 ! LA 0.96 MC 1.00* MK 1.02 NL 1.00 ! NY 1.00* OV 0.99 PT 0.99 SC 1.08 ! TS 1.00* WF 1.00 WZ 1.00* ! ! A total of 36 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 FD 0.98 GC 1.02 GG 1.00* ! HH 1.00* HN 1.00* KK 1.01 KP 1.02 ! LA 0.99 MC 1.00* MK 1.02 NL 1.04 ! NY 1.00* OV 1.00 PT 1.00 SC 1.00* ! TS 0.96 WF 1.00* WZ 1.00* ! ! A total of 282 telescope corrections were flagged in sub-array 5. ! Telescope amplitude corrections in sub-array 5: ! BR 0.98 FD 0.93 GC 1.00* GG 1.00* ! HH 1.00* HN 0.99 KK 1.20 KP 0.95 ! LA 0.97 MC 1.00* MK 1.05 NL 0.99 ! NY 1.00* OV 0.99 PT 0.97 SC 1.05 ! TS 1.00* WF 1.00 WZ 1.00* ! ! Telescope amplitude corrections in sub-array 6: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HH 0.00* HN 0.00* KK 0.00* KP 0.00* ! LA 0.00* MC 0.00* MK 0.00* NL 0.00* ! NY 0.00* OV 0.00* PT 0.00* SC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! ! Fit before self-cal, rms=0.295623Jy sigma=0.002222 ! Fit after self-cal, rms=0.193295Jy sigma=0.001359 dynam = dynam - 0.5 flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=0.7476 mas, bmaj=2.154 mas, bpa=-6.091 degrees ! Estimated noise=356.561 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 = 0.000192933 Jy ! Component: 100 - total flux cleaned = -0.00134558 Jy ! Component: 150 - total flux cleaned = -0.00212996 Jy ! Component: 200 - total flux cleaned = -0.0028261 Jy ! Total flux subtracted in 200 components = -0.0028261 Jy ! Clean residual min=-0.017498 max=0.007351 Jy/beam ! Clean residual mean=-0.000009 rms=0.001987 Jy/beam ! Combined flux in latest and established models = 4.38631 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 46 components and 4.38631 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.192414Jy sigma=0.001350 ! Fit after self-cal, rms=0.192415Jy sigma=0.001350 ! Inverting map ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 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. ! ! Fit before self-cal, rms=0.192415Jy sigma=0.001350 ! Fit after self-cal, rms=0.192413Jy sigma=0.001348 dynam = dynam - 0.75 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=0.7485 mas, bmaj=2.153 mas, bpa=-6.074 degrees ! Estimated noise=356.844 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000905424 Jy ! Component: 100 - total flux cleaned = 0.000423912 Jy ! Component: 150 - total flux cleaned = -0.000234097 Jy ! Component: 200 - total flux cleaned = -0.000815953 Jy ! Total flux subtracted in 200 components = -0.000815953 Jy ! Clean residual min=-0.016300 max=0.006993 Jy/beam ! Clean residual mean=0.000030 rms=0.001866 Jy/beam ! Combined flux in latest and established models = 4.38549 Jy selfcal ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 48 components and 4.38549 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.191813Jy sigma=0.001342 ! Fit after self-cal, rms=0.191739Jy sigma=0.001342 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 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 = -0.000140672 Jy ! Component: 100 - total flux cleaned = -0.000504166 Jy ! Component: 150 - total flux cleaned = -0.000827787 Jy ! Component: 200 - total flux cleaned = -0.000979162 Jy ! Total flux subtracted in 200 components = -0.000979162 Jy ! Clean residual min=-0.015827 max=0.006962 Jy/beam ! Clean residual mean=0.000056 rms=0.001825 Jy/beam ! Combined flux in latest and established models = 4.38451 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 49 components and 4.38451 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.191397Jy sigma=0.001339 ! Fit after self-cal, rms=0.191337Jy sigma=0.001339 ! Inverting map ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 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. ! ! Fit before self-cal, rms=0.191337Jy sigma=0.001339 ! Fit after self-cal, rms=0.191330Jy sigma=0.001337 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=0.7495 mas, bmaj=2.152 mas, bpa=-6.057 degrees ! Estimated noise=357.093 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00138646 Jy ! Component: 100 - total flux cleaned = 0.000796801 Jy ! Component: 150 - total flux cleaned = 0.000457178 Jy ! Component: 200 - total flux cleaned = 0.000135331 Jy ! Total flux subtracted in 200 components = 0.000135331 Jy ! Clean residual min=-0.014894 max=0.006806 Jy/beam ! Clean residual mean=0.000069 rms=0.001727 Jy/beam ! Combined flux in latest and established models = 4.38465 Jy selfcal ! Performing phase self-cal ! Adding 11 model components to the UV plane model. ! The established model now contains 49 components and 4.38465 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.190941Jy sigma=0.001333 ! Fit after self-cal, rms=0.190879Jy sigma=0.001333 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 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 = -0.00011389 Jy ! Component: 100 - total flux cleaned = -0.000409938 Jy ! Component: 150 - total flux cleaned = -0.000549969 Jy ! Component: 200 - total flux cleaned = -0.0006814 Jy ! Total flux subtracted in 200 components = -0.0006814 Jy ! Clean residual min=-0.014611 max=0.006758 Jy/beam ! Clean residual mean=0.000087 rms=0.001698 Jy/beam ! Combined flux in latest and established models = 4.38397 Jy ! Performing phase self-cal ! Adding 10 model components to the UV plane model. ! The established model now contains 49 components and 4.38397 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.190631Jy sigma=0.001330 ! Fit after self-cal, rms=0.190583Jy sigma=0.001330 ! Inverting map ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 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. ! ! Fit before self-cal, rms=0.190583Jy sigma=0.001330 ! Fit after self-cal, rms=0.190601Jy sigma=0.001329 clean clean_niter,clean_gain ! Inverting map and beam ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=2.17 mas, bmaj=3.299 mas, bpa=-0.8098 degrees ! Estimated noise=456.388 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.0011623 Jy ! Component: 100 - total flux cleaned = -0.00105051 Jy ! Component: 150 - total flux cleaned = -0.000977762 Jy ! Component: 200 - total flux cleaned = -0.000978077 Jy ! Total flux subtracted in 200 components = -0.000978077 Jy ! Clean residual min=-0.003890 max=0.005471 Jy/beam ! Clean residual mean=0.000319 rms=0.001269 Jy/beam ! Combined flux in latest and established models = 4.38299 Jy selfcal ! Performing phase self-cal ! Adding 7 model components to the UV plane model. ! The established model now contains 53 components and 4.38299 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.190637Jy sigma=0.001330 ! Fit after self-cal, rms=0.190521Jy sigma=0.001329 flux_cutoff = imstat(rms) * dynam ! Inverting map ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 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 = -4.94531e-05 Jy ! Component: 100 - total flux cleaned = -6.99953e-05 Jy ! Component: 150 - total flux cleaned = -7.81476e-05 Jy ! Component: 200 - total flux cleaned = -2.96568e-05 Jy ! Total flux subtracted in 200 components = -2.96568e-05 Jy ! Clean residual min=-0.003660 max=0.005540 Jy/beam ! Clean residual mean=0.000321 rms=0.001244 Jy/beam ! Combined flux in latest and established models = 4.38296 Jy ! Performing phase self-cal ! Adding 8 model components to the UV plane model. ! The established model now contains 54 components and 4.38296 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.190510Jy sigma=0.001329 ! Fit after self-cal, rms=0.190384Jy sigma=0.001328 ! Inverting map ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec ! Added new window around map position (0.4, -7.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0043429 Jy ! Component: 100 - total flux cleaned = 0.0057746 Jy ! Component: 150 - total flux cleaned = 0.00628805 Jy ! Component: 200 - total flux cleaned = 0.00662451 Jy ! Total flux subtracted in 200 components = 0.00662451 Jy ! Clean residual min=-0.003624 max=0.002392 Jy/beam ! Clean residual mean=-0.000003 rms=0.000928 Jy/beam ! Combined flux in latest and established models = 4.38958 Jy ! Performing phase self-cal ! Adding 19 model components to the UV plane model. ! The established model now contains 68 components and 4.38959 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.190217Jy sigma=0.001326 ! Fit after self-cal, rms=0.190160Jy sigma=0.001326 ! Inverting map ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 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 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=0.7504 mas, bmaj=2.15 mas, bpa=-6.044 degrees ! Estimated noise=357.281 mJy/beam. ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7504 x 2.15 at -6.044 degrees (North through East) ! Clean map min=-0.0058607 max=3.6837 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 ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.190160Jy sigma=0.001326 ! Fit after self-cal, rms=0.174799Jy sigma=0.001186 ! Inverting map and beam ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=0.7503 mas, bmaj=2.152 mas, bpa=-6.058 degrees ! Estimated noise=357.233 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00405849 Jy ! Component: 100 - total flux cleaned = 0.00448465 Jy ! Component: 150 - total flux cleaned = 0.00447898 Jy ! Component: 200 - total flux cleaned = 0.00429646 Jy ! Total flux subtracted in 200 components = 0.00429646 Jy ! Clean residual min=-0.011414 max=0.005006 Jy/beam ! Clean residual mean=-0.000142 rms=0.001331 Jy/beam ! Combined flux in latest and established models = 4.39388 Jy ! Performing phase self-cal ! Adding 28 model components to the UV plane model. ! The established model now contains 92 components and 4.39388 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.174309Jy sigma=0.001182 ! Fit after self-cal, rms=0.174273Jy sigma=0.001181 ! Inverting map ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.000594556 Jy ! Component: 100 - total flux cleaned = 0.000591672 Jy ! Component: 150 - total flux cleaned = 0.000256584 Jy ! Component: 200 - total flux cleaned = 9.33832e-05 Jy ! Total flux subtracted in 200 components = 9.33832e-05 Jy ! Clean residual min=-0.011045 max=0.004848 Jy/beam ! Clean residual mean=-0.000146 rms=0.001283 Jy/beam ! Combined flux in latest and established models = 4.39398 Jy ! Performing phase self-cal ! Adding 33 model components to the UV plane model. ! The established model now contains 103 components and 4.39397 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.173919Jy sigma=0.001178 ! Fit after self-cal, rms=0.173898Jy sigma=0.001178 ! Inverting map ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec ! Performing amp+phase self-cal ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.173898Jy sigma=0.001178 ! Fit after self-cal, rms=0.173969Jy sigma=0.001178 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 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=0.5698 mas, bmaj=1.478 mas, bpa=-3.818 degrees ! Estimated noise=831.353 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 2.65328 Jy ! Component: 100 - total flux cleaned = 3.35556 Jy ! Component: 150 - total flux cleaned = 3.72363 Jy ! Component: 200 - total flux cleaned = 3.94804 Jy ! Total flux subtracted in 200 components = 3.94804 Jy ! Clean residual min=-0.036750 max=0.118610 Jy/beam ! Clean residual mean=0.001322 rms=0.013551 Jy/beam ! Combined flux in latest and established models = 3.94804 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 21 model components to the UV plane model. ! The established model now contains 21 components and 3.94805 Jy ! Inverting map and beam ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=0.7506 mas, bmaj=2.151 mas, bpa=-6.054 degrees ! Estimated noise=357.356 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 = 0.21574 Jy ! Component: 100 - total flux cleaned = 0.322824 Jy ! Component: 150 - total flux cleaned = 0.379588 Jy ! Component: 200 - total flux cleaned = 0.410833 Jy ! Total flux subtracted in 200 components = 0.410833 Jy ! Clean residual min=-0.008841 max=0.017252 Jy/beam ! Clean residual mean=0.000744 rms=0.002727 Jy/beam ! Combined flux in latest and established models = 4.35888 Jy ! Adding 39 model components to the UV plane model. ! The established model now contains 47 components and 4.35888 Jy ! Inverting map ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec ! Added new window around map position (-0.6, -0.4). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0133203 Jy ! Component: 100 - total flux cleaned = 0.0168469 Jy ! Component: 150 - total flux cleaned = 0.0194798 Jy ! Component: 200 - total flux cleaned = 0.0213747 Jy ! Total flux subtracted in 200 components = 0.0213747 Jy ! Clean residual min=-0.008181 max=0.008494 Jy/beam ! Clean residual mean=0.000221 rms=0.001908 Jy/beam ! Combined flux in latest and established models = 4.38025 Jy ! Adding 15 model components to the UV plane model. ! The established model now contains 56 components and 4.38025 Jy ! Inverting map ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec ! Added new window around map position (0.6, 0.2). ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00185586 Jy ! Component: 100 - total flux cleaned = 0.00225844 Jy ! Component: 150 - total flux cleaned = 0.0026375 Jy ! Component: 200 - total flux cleaned = 0.00298916 Jy ! Total flux subtracted in 200 components = 0.00298916 Jy ! Clean residual min=-0.006620 max=0.006386 Jy/beam ! Clean residual mean=0.000157 rms=0.001631 Jy/beam ! Combined flux in latest and established models = 4.38324 Jy ! Adding 16 model components to the UV plane model. ! The established model now contains 64 components and 4.38324 Jy ! Inverting map ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 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 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=2.17 mas, bmaj=3.3 mas, bpa=-0.8335 degrees ! Estimated noise=456.447 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0048769 Jy ! Component: 100 - total flux cleaned = 0.00631334 Jy ! Component: 150 - total flux cleaned = 0.00727489 Jy ! Component: 200 - total flux cleaned = 0.00764354 Jy ! Total flux subtracted in 200 components = 0.00764354 Jy ! Clean residual min=-0.002006 max=0.002317 Jy/beam ! Clean residual mean=-0.000005 rms=0.000808 Jy/beam ! Combined flux in latest and established models = 4.39089 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 = -9.23294e-07 Jy ! Component: 100 - total flux cleaned = -7.4748e-05 Jy ! Component: 150 - total flux cleaned = -0.00020946 Jy ! Component: 200 - total flux cleaned = -0.000273977 Jy ! Total flux subtracted in 200 components = -0.000273977 Jy ! Clean residual min=-0.001876 max=0.002207 Jy/beam ! Clean residual mean=0.000007 rms=0.000739 Jy/beam ! Combined flux in latest and established models = 4.39061 Jy ! Adding 33 model components to the UV plane model. ! The established model now contains 91 components and 4.39061 Jy ! Inverting map ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec uvtaper 0,0 ! No UV-taper is currently set. clean ! Inverting map and beam ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec ! Estimated beam: bmin=0.7506 mas, bmaj=2.151 mas, bpa=-6.054 degrees ! Estimated noise=357.356 mJy/beam. ! clean: niter=200 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00179144 Jy ! Component: 100 - total flux cleaned = -0.00241063 Jy ! Component: 150 - total flux cleaned = -0.00268549 Jy ! Component: 200 - total flux cleaned = -0.00240622 Jy ! Total flux subtracted in 200 components = -0.00240622 Jy ! Clean residual min=-0.006424 max=0.005315 Jy/beam ! Clean residual mean=0.000056 rms=0.001384 Jy/beam ! Combined flux in latest and established models = 4.38821 Jy selfcal ! Performing phase self-cal ! Adding 17 model components to the UV plane model. ! The established model now contains 97 components and 4.38821 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.176411Jy sigma=0.001205 ! Fit after self-cal, rms=0.176139Jy sigma=0.001203 wmodel J1743-0350_X_2001_07_05_pus_map.mod ! Writing 97 model components to file: J1743-0350_X_2001_07_05_pus_map.mod wobs J1743-0350_X_2001_07_05_pus_uvs.fits ! Writing UV FITS file: J1743-0350_X_2001_07_05_pus_uvs.fits wwins J1743-0350_X_2001_07_05_pus_map.win ! wwins: Wrote 5 windows to J1743-0350_X_2001_07_05_pus_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 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec ! clean: niter=1024 gain=0.01 cutoff=0 ! Component: 050 - total flux cleaned = -7.86072e-05 Jy ! Component: 100 - total flux cleaned = -0.000178031 Jy ! Component: 150 - total flux cleaned = -0.000180917 Jy ! Component: 200 - total flux cleaned = 9.21057e-05 Jy ! Component: 250 - total flux cleaned = 0.000620844 Jy ! Component: 300 - total flux cleaned = 0.00122188 Jy ! Component: 350 - total flux cleaned = 0.00164139 Jy ! Component: 400 - total flux cleaned = 0.00213534 Jy ! Component: 450 - total flux cleaned = 0.00245791 Jy ! Component: 500 - total flux cleaned = 0.00285571 Jy ! Component: 550 - total flux cleaned = 0.00316843 Jy ! Component: 600 - total flux cleaned = 0.00339899 Jy ! Component: 650 - total flux cleaned = 0.00370247 Jy ! Component: 700 - total flux cleaned = 0.00385169 Jy ! Component: 750 - total flux cleaned = 0.00392579 Jy ! Component: 800 - total flux cleaned = 0.00414366 Jy ! Component: 850 - total flux cleaned = 0.00414292 Jy ! Component: 900 - total flux cleaned = 0.00414337 Jy ! Component: 950 - total flux cleaned = 0.00421386 Jy ! Component: 1000 - total flux cleaned = 0.00428417 Jy ! Total flux subtracted in 1024 components = 0.00442169 Jy ! Clean residual min=-0.003447 max=0.003451 Jy/beam ! Clean residual mean=-0.000019 rms=0.001176 Jy/beam ! Combined flux in latest and established models = 4.39263 Jy keep ! Adding 53 model components to the UV plane model. ! The established model now contains 137 components and 4.39263 Jy wmap "J1743-0350_X_2001_07_05_pus\_map.fits" ! Inverting map ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7506 x 2.151 at -6.054 degrees (North through East) ! Clean map min=-0.0057627 max=3.6823 Jy/beam ! Writing clean map to FITS file: J1743-0350_X_2001_07_05_pus_map.fits float peak_flux peak_flux = peak(flux,max) print "The peak flux is",peak_flux ! The peak flux is 3.68234 invert ! Inverting map ! Your choice of large map pixels excluded 3.24% of the data. ! The x-axis pixel size should ideally be below 0.1608 milli-arcsec float image_rms image_rms = imstat(rms) print "The final image rms is",image_rms ! The final image rms is 0.0011756 device "J1743-0350_X_2001_07_05_pus\_map.eps/VPS" ! Attempting to open device: 'J1743-0350_X_2001_07_05_pus_map.eps/VPS' loglevs 100*3*image_rms/peak_flux ! The new contour levels are: ! -0.095776 0.095776 0.191552 0.383104 0.766208 1.53242 3.06483 6.12966 12.2593 24.5187 49.0373 98.0746 print "clev=",int(3*image_rms*10000)/10000 ! clev= 0.0035 print "peak=",int(1000*peak_flux)/1000 ! peak= 3.682 mapcolor none ! Mapplot colormap: none, contrast: 1 brightness: 0.5. mapplot cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7506 x 2.151 at -6.054 degrees (North through East) ! Clean map min=-0.0057627 max=3.6823 Jy/beam mapcolor color, 0.9 ! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5. device "J1743-0350_X_2001_07_05_pus\_map.gif/vgif" ! Attempting to open device: 'J1743-0350_X_2001_07_05_pus_map.gif/vgif' mapplot cln quit ! Quitting program ! Log file J1743-0350_X_2001_07_05_pus_uvs.log closed on Wed Jul 4 21:36:50 2007