! Started logfile: 0003-066_X.log on Wed Jul 5 17:06:26 2006 observe 0003-066_X.edt ! Reading UV FITS file: 0003-066_X.edt ! AN table 1: 23 integrations on 190 of 190 possible baselines. ! AN table 2: 14 integrations on 190 of 190 possible baselines. ! AN table 3: 26 integrations on 190 of 190 possible baselines. ! AN table 4: 11 integrations on 190 of 190 possible baselines. ! Apparent sampling: 0.0810811 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 0003-066 ! ! 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 1409 lines of history. ! ! Reading 4560 visibilities. ![@gonzo8-0.1 0003-066_X] print "***********************************" ! *********************************** print "*** Using gonzo instruction set ***" ! *** Using gonzo instruction set *** print "***********************************" ! *********************************** float field_size field_size = 1024 float field_cell field_cell = 0.1 integer clean_niter clean_niter = 50 float clean_gain clean_gain = 0.03 float dynam dynam = 8.0 float win_mult win_mult = 1.8 float solint solint = 3.6/6.0 logical doflt doflt = true logical doamp float new_peak float flux_cutoff mapsize field_size,field_cell ! Map grid = 1024x1024 pixels with 0.100x0.100 milli-arcsec cellsize. select ! 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 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 334 telescope corrections were flagged in sub-array 1. ! A total of 280 telescope corrections were flagged in sub-array 2. ! A total of 444 telescope corrections were flagged in sub-array 3. ! A total of 196 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 338 telescope corrections were flagged in sub-array 1. ! A total of 280 telescope corrections were flagged in sub-array 2. ! A total of 449 telescope corrections were flagged in sub-array 3. ! A total of 196 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 334 telescope corrections were flagged in sub-array 1. ! A total of 280 telescope corrections were flagged in sub-array 2. ! A total of 445 telescope corrections were flagged in sub-array 3. ! A total of 196 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 334 telescope corrections were flagged in sub-array 1. ! A total of 280 telescope corrections were flagged in sub-array 2. ! A total of 445 telescope corrections were flagged in sub-array 3. ! A total of 196 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=0.670111Jy sigma=0.009926 ! Fit after self-cal, rms=0.671483Jy sigma=0.009968 ! clrmod: Cleared the established, tentative and continuum models. ! Redundant starting model cleared. uvweight 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. doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=0.6712 mas, bmaj=1.379 mas, bpa=0.7674 degrees ! Estimated noise=1540.79 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal doamp, doflt, solint new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (0, 0). ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 1.16632 Jy ! Total flux subtracted in 50 components = 1.16632 Jy ! Clean residual min=-0.084419 max=0.329137 Jy/beam ! Clean residual mean=0.001673 rms=0.026188 Jy/beam ! Combined flux in latest and established models = 1.16632 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 5 model components to the UV plane model. ! The established model now contains 5 components and 1.16632 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.541354Jy sigma=0.008084 ! Fit after self-cal, rms=0.541356Jy sigma=0.008084 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.299577 Jy ! Total flux subtracted in 50 components = 0.299577 Jy ! Clean residual min=-0.051908 max=0.119515 Jy/beam ! Clean residual mean=0.001174 rms=0.016173 Jy/beam ! Combined flux in latest and established models = 1.46589 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 11 model components to the UV plane model. ! The established model now contains 15 components and 1.46589 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.370836Jy sigma=0.005318 ! Fit after self-cal, rms=0.370902Jy sigma=0.005317 ! Inverting map print "****************************************" ! **************************************** print "*** Finished Uniform Weighting CLEAN ***" ! *** Finished Uniform Weighting CLEAN *** print "****************************************" ! **************************************** uvweight 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 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=0.8936 mas, bmaj=1.893 mas, bpa=-1.294 degrees ! Estimated noise=1020.23 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal doamp, doflt, solint new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.189061 Jy ! Component: 100 - total flux cleaned = 0.277302 Jy ! Total flux subtracted in 100 components = 0.277302 Jy ! Clean residual min=-0.043751 max=0.099116 Jy/beam ! Clean residual mean=0.005306 rms=0.018346 Jy/beam ! Combined flux in latest and established models = 1.7432 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 40 model components to the UV plane model. ! The established model now contains 49 components and 1.7432 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.308436Jy sigma=0.003809 ! Fit after self-cal, rms=0.307591Jy sigma=0.003805 ! Inverting map print "****************************************" ! **************************************** print "*** Finished Natural Weighting CLEAN ***" ! *** Finished Natural Weighting CLEAN *** print "****************************************" ! **************************************** gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00 FD 0.96 GC 1.07 HN 1.07 ! LA 0.98 NL 0.95 OV 0.97 SC 0.94 ! WF 1.20 GG 1.00* HH 1.00* KK 1.00 ! KP 0.96 MA 1.00* MC 1.00* MK 1.04 ! NY 1.00* TS 1.00* WZ 1.00* PT 0.93 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* GC 0.00* HN 0.00* ! LA 0.00* NL 0.00* OV 0.00* SC 0.00* ! WF 0.00* GG 0.00* HH 0.00* KK 0.00* ! KP 0.00* MA 0.00* MC 0.00* MK 0.00* ! NY 0.00* TS 0.00* WZ 0.00* PT 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00* GC 1.00* HN 0.95 ! LA 1.00* NL 1.25 OV 1.00* SC 0.97 ! WF 0.80 GG 1.00* HH 1.53 KK 1.00* ! KP 1.00* MA 1.04 MC 0.94 MK 1.00* ! NY 1.00* TS 1.00* WZ 0.89 PT 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.98 FD 1.00* GC 1.11 HN 1.00* ! LA 1.00* NL 1.00* OV 1.05 SC 1.00* ! WF 1.00* GG 1.00* HH 1.00* KK 1.00 ! KP 1.28 MA 1.00* MC 1.00* MK 0.98 ! NY 1.00* TS 1.00* WZ 1.00* PT 1.00* ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 1.02 FD 0.94 GC 1.10 HN 1.09 ! LA 0.98 NL 0.92 OV 0.99 SC 2.16 ! WF 1.15 GG 1.00* HH 1.00* KK 1.00 ! KP 0.93 MA 1.00* MC 1.00* MK 1.03 ! NY 1.00* TS 1.00* WZ 1.00* PT 0.96 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* GC 0.00* HN 0.00* ! LA 0.00* NL 0.00* OV 0.00* SC 0.00* ! WF 0.00* GG 0.00* HH 0.00* KK 0.00* ! KP 0.00* MA 0.00* MC 0.00* MK 0.00* ! NY 0.00* TS 0.00* WZ 0.00* PT 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00* GC 1.00* HN 0.96 ! LA 1.00* NL 1.22 OV 1.00* SC 1.28 ! WF 0.81 GG 1.00* HH 1.00* KK 1.00* ! KP 1.00* MA 1.15 MC 0.92 MK 1.00* ! NY 1.00* TS 1.00* WZ 0.89 PT 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 FD 1.00* GC 1.13 HN 1.00* ! LA 1.00* NL 1.00* OV 1.04 SC 1.00* ! WF 1.00* GG 1.00* HH 1.00* KK 0.99 ! KP 1.19 MA 1.00* MC 1.00* MK 0.97 ! NY 1.00* TS 1.00* WZ 1.00* PT 1.00* ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.01 FD 0.94 GC 1.12 HN 1.10 ! LA 0.98 NL 0.91 OV 0.95 SC 0.97 ! WF 1.19 GG 1.00* HH 1.00* KK 1.02 ! KP 0.93 MA 1.00* MC 1.00* MK 1.05 ! NY 1.00* TS 1.00* WZ 1.00* PT 0.97 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* GC 0.00* HN 0.00* ! LA 0.00* NL 0.00* OV 0.00* SC 0.00* ! WF 0.00* GG 0.00* HH 0.00* KK 0.00* ! KP 0.00* MA 0.00* MC 0.00* MK 0.00* ! NY 0.00* TS 0.00* WZ 0.00* PT 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00* GC 1.00* HN 0.94 ! LA 1.00* NL 1.26 OV 1.00* SC 0.97 ! WF 0.84 GG 1.00* HH 1.35 KK 1.00* ! KP 1.00* MA 1.26 MC 0.97 MK 1.00* ! NY 1.00* TS 1.00* WZ 0.90 PT 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 1.00 FD 1.00* GC 1.16 HN 1.00* ! LA 1.00* NL 1.00* OV 1.00 SC 1.00* ! WF 1.00* GG 1.00* HH 1.00* KK 0.99 ! KP 1.18 MA 1.00* MC 1.00* MK 0.93 ! NY 1.00* TS 1.00* WZ 1.00* PT 1.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.99 FD 0.93 GC 1.18 HN 1.08 ! LA 0.98 NL 0.91 OV 0.95 SC 0.96 ! WF 1.15 GG 1.00* HH 1.00* KK 1.00 ! KP 0.94 MA 1.00* MC 1.00* MK 1.08 ! NY 1.00* TS 1.00* WZ 1.00* PT 0.97 ! ! Telescope amplitude corrections in sub-array 2: ! BR 0.00* FD 0.00* GC 0.00* HN 0.00* ! LA 0.00* NL 0.00* OV 0.00* SC 0.00* ! WF 0.00* GG 0.00* HH 0.00* KK 0.00* ! KP 0.00* MA 0.00* MC 0.00* MK 0.00* ! NY 0.00* TS 0.00* WZ 0.00* PT 0.00* ! ! A total of 24 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.00* FD 1.00* GC 1.00* HN 0.94 ! LA 1.00* NL 1.33 OV 1.00* SC 1.00 ! WF 0.80 GG 1.00* HH 1.50 KK 1.00* ! KP 1.00* MA 1.12 MC 0.97 MK 1.00* ! NY 1.00* TS 1.00* WZ 0.86 PT 1.00* ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.99 FD 1.00* GC 1.11 HN 1.00* ! LA 1.00* NL 1.00* OV 1.03 SC 1.00* ! WF 1.00* GG 1.00* HH 1.00* KK 0.95 ! KP 1.14 MA 1.00* MC 1.00* MK 0.95 ! NY 1.00* TS 1.00* WZ 1.00* PT 1.00* ! ! ! Fit before self-cal, rms=0.307591Jy sigma=0.003805 ! Fit after self-cal, rms=0.254083Jy sigma=0.003058 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=0.9006 mas, bmaj=1.988 mas, bpa=-1.528 degrees ! Estimated noise=1005.88 mJy/beam. repeat if (peak(flux) > flux_cutoff) peakwin win_mult clean clean_niter,clean_gain flux_cutoff = imstat(rms) * dynam selfcal doamp, doflt, solint new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00892961 Jy ! Component: 100 - total flux cleaned = -0.0100344 Jy ! Total flux subtracted in 100 components = -0.0100344 Jy ! Clean residual min=-0.035153 max=0.069280 Jy/beam ! Clean residual mean=0.002598 rms=0.013438 Jy/beam ! Combined flux in latest and established models = 1.73316 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 10 model components to the UV plane model. ! The established model now contains 59 components and 1.73316 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.252930Jy sigma=0.003054 ! Fit after self-cal, rms=0.253150Jy sigma=0.003053 ! Inverting map dynam = dynam - 1.0 doamp = true solint = solint * (6.0/3.6) 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 doamp, doflt, solint new_peak = peak(flux) until(new_peak<=flux_cutoff) ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = -0.00149779 Jy ! Component: 100 - total flux cleaned = -0.00148673 Jy ! Total flux subtracted in 100 components = -0.00148673 Jy ! Clean residual min=-0.034751 max=0.069051 Jy/beam ! Clean residual mean=0.002617 rms=0.013421 Jy/beam ! Combined flux in latest and established models = 1.73167 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 9 model components to the UV plane model. ! The established model now contains 64 components and 1.73167 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.252742Jy sigma=0.003050 ! Fit after self-cal, rms=0.210709Jy sigma=0.002581 ! Inverting map and beam ! Estimated beam: bmin=0.8979 mas, bmaj=1.99 mas, bpa=-1.702 degrees ! Estimated noise=1006.73 mJy/beam. doamp = false solint = solint / (6.0/3.6) 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 doamp, doflt, solint new_peak = peak(flux) until(new_peak<=flux_cutoff) ! Added new window around map position (-5.7, 0.7). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0688031 Jy ! Component: 100 - total flux cleaned = 0.102499 Jy ! Total flux subtracted in 100 components = 0.102499 Jy ! Clean residual min=-0.023334 max=0.065600 Jy/beam ! Clean residual mean=0.001092 rms=0.008777 Jy/beam ! Combined flux in latest and established models = 1.83417 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 22 model components to the UV plane model. ! The established model now contains 86 components and 1.83417 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.192257Jy sigma=0.002199 ! Fit after self-cal, rms=0.191104Jy sigma=0.002185 ! Inverting map ! Added new window around map position (-2.7, 1). ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0625178 Jy ! Component: 100 - total flux cleaned = 0.0943439 Jy ! Total flux subtracted in 100 components = 0.0943438 Jy ! Clean residual min=-0.018382 max=0.030464 Jy/beam ! Clean residual mean=-0.000082 rms=0.006098 Jy/beam ! Combined flux in latest and established models = 1.92852 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 25 model components to the UV plane model. ! The established model now contains 111 components and 1.92852 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.173180Jy sigma=0.001838 ! Fit after self-cal, rms=0.170842Jy sigma=0.001812 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 0003-066_X ! Writing UV FITS file: 0003-066_X.uvf ! Writing 111 model components to file: 0003-066_X.mod ! wwins: Wrote 3 windows to 0003-066_X.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8979 x 1.99 at -1.702 degrees (North through East) ! Clean map min=-0.017661 max=1.5559 Jy/beam ! Writing clean map to FITS file: 0003-066_X.fits ! Writing difmap environment to: 0003-066_X.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 0003-066_X] device 0003-066_Xuv.ps/vps,1,2 ! Attempting to open device: '0003-066_Xuv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 0003-066_Xim.ps/vps ! Attempting to open device: '0003-066_Xim.ps/vps' uvweight 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. loglevs -1,2048,2 ! The new contour levels are: ! -1 1 2 4 8 16 32 64 128 256 512 1024 2048 cmul = imstat(rms)*3 ! Inverting map and beam ! Estimated beam: bmin=0.8979 mas, bmaj=1.99 mas, bpa=-1.702 degrees ! Estimated noise=1006.73 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.8979 x 1.99 at -1.702 degrees (North through East) ! Clean map min=-0.017661 max=1.5559 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo8-0.1] quit ! Quitting program ! Log file 0003-066_X.log closed on Wed Jul 5 17:06:43 2006