! Started logfile: 1124-186_X.log on Sun Apr 12 14:26:27 2009 observe 1124-186_X.edt ! Reading UV FITS file: 1124-186_X.edt ! AN table 1: 9 integrations on 190 of 190 possible baselines. ! AN table 2: 20 integrations on 190 of 190 possible baselines. ! AN table 3: 15 integrations on 190 of 190 possible baselines. ! AN table 4: 24 integrations on 190 of 190 possible baselines. ! Apparent sampling: 0.0609133 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 1124-186 ! ! 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 1491 lines of history. ! ! Reading 3148 visibilities. ![@gonzo7-0.1 1124-186_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 = 7.0 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 180 telescope corrections were flagged in sub-array 1. ! A total of 328 telescope corrections were flagged in sub-array 2. ! A total of 281 telescope corrections were flagged in sub-array 3. ! A total of 436 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 180 telescope corrections were flagged in sub-array 1. ! A total of 332 telescope corrections were flagged in sub-array 2. ! A total of 281 telescope corrections were flagged in sub-array 3. ! A total of 434 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 180 telescope corrections were flagged in sub-array 1. ! A total of 329 telescope corrections were flagged in sub-array 2. ! A total of 281 telescope corrections were flagged in sub-array 3. ! A total of 437 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 180 telescope corrections were flagged in sub-array 1. ! A total of 329 telescope corrections were flagged in sub-array 2. ! A total of 281 telescope corrections were flagged in sub-array 3. ! A total of 433 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=0.297897Jy sigma=3.510987 ! Fit after self-cal, rms=0.288953Jy sigma=3.507936 ! 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=0.4815 mas, bmaj=1.172 mas, bpa=5.332 degrees ! Estimated noise=1.91275 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 = 0.597529 Jy ! Total flux subtracted in 50 components = 0.597529 Jy ! Clean residual min=-0.041794 max=0.166902 Jy/beam ! Clean residual mean=-0.000182 rms=0.015234 Jy/beam ! Combined flux in latest and established models = 0.597529 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 2 model components to the UV plane model. ! The established model now contains 2 components and 0.597529 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.274053Jy sigma=4.337414 ! Fit after self-cal, rms=0.274060Jy sigma=4.337360 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.151032 Jy ! Total flux subtracted in 50 components = 0.151032 Jy ! Clean residual min=-0.030637 max=0.062064 Jy/beam ! Clean residual mean=-0.000131 rms=0.009077 Jy/beam ! Combined flux in latest and established models = 0.748561 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 12 model components to the UV plane model. ! The established model now contains 14 components and 0.748561 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.191658Jy sigma=2.706481 ! Fit after self-cal, rms=0.191611Jy sigma=2.706009 ! 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=0.646 mas, bmaj=1.527 mas, bpa=0.3573 degrees ! Estimated noise=1.30125 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 = 0.0835333 Jy ! Component: 100 - total flux cleaned = 0.117819 Jy ! Total flux subtracted in 100 components = 0.117819 Jy ! Clean residual min=-0.021413 max=0.031075 Jy/beam ! Clean residual mean=-0.000309 rms=0.006915 Jy/beam ! Combined flux in latest and established models = 0.86638 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 17 model components to the UV plane model. ! The established model now contains 27 components and 0.86638 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.167866Jy sigma=2.026722 ! Fit after self-cal, rms=0.167710Jy sigma=2.024284 ! 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 0.00* FD 0.00* GC 0.00* HH 0.00* ! HN 0.00* KK 0.00* KP 0.00* LA 0.00* ! MA 0.00* MC 0.00* MK 0.00* NL 0.00* ! NY 0.00* ON 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 2: ! BR 1.00 FD 0.92 GC 1.00* HH 1.00* ! HN 1.00* KK 0.85 KP 0.95 LA 1.13 ! MA 1.00* MC 1.00* MK 1.03 NL 0.96 ! NY 1.00* ON 1.00* OV 0.96 PT 0.96 ! SC 0.89 TS 1.00* WF 1.38 WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.10 FD 1.00* GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 1.00* LA 1.00* ! MA 1.00* MC 1.00* MK 0.95 NL 1.00* ! NY 1.00* ON 1.00* OV 1.03 PT 1.12 ! SC 1.00* TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.05 GC 1.00* HH 0.95 ! HN 1.00* KK 1.00* KP 1.00* LA 1.23 ! MA 0.95 MC 1.18 MK 1.00* NL 1.00 ! NY 1.00* ON 1.00* OV 1.00* PT 1.05 ! SC 0.81 TS 1.00* WF 1.00* WZ 1.00 ! ! ! Correcting IF 2. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* GC 0.00* HH 0.00* ! HN 0.00* KK 0.00* KP 0.00* LA 0.00* ! MA 0.00* MC 0.00* MK 0.00* NL 0.00* ! NY 0.00* ON 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 2: ! BR 0.99 FD 0.93 GC 1.00* HH 1.00* ! HN 1.00* KK 0.80 KP 0.95 LA 1.18 ! MA 1.00* MC 1.00* MK 1.02 NL 0.92 ! NY 1.00* ON 1.00* OV 0.96 PT 0.97 ! SC 1.00* TS 1.00* WF 1.36 WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.07 FD 1.00* GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 1.00* LA 1.00* ! MA 1.00* MC 1.00* MK 0.93 NL 1.00* ! NY 1.00* ON 1.00* OV 1.07 PT 1.15 ! SC 1.00* TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 9 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.01 GC 1.00* HH 1.00 ! HN 1.00* KK 1.00* KP 1.00* LA 1.27 ! MA 1.03 MC 1.14 MK 1.00* NL 0.93 ! NY 1.00* ON 1.00* OV 1.00* PT 1.08 ! SC 0.96 TS 1.00* WF 1.00* WZ 1.09 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* GC 0.00* HH 0.00* ! HN 0.00* KK 0.00* KP 0.00* LA 0.00* ! MA 0.00* MC 0.00* MK 0.00* NL 0.00* ! NY 0.00* ON 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 2: ! BR 0.98 FD 0.94 GC 1.00* HH 1.00* ! HN 1.00* KK 0.82 KP 0.93 LA 1.16 ! MA 1.00* MC 1.00* MK 1.02 NL 0.93 ! NY 1.00* ON 1.00* OV 0.97 PT 0.94 ! SC 0.99 TS 1.00* WF 1.33 WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.08 FD 1.00* GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 1.00* LA 1.00* ! MA 1.00* MC 1.00* MK 1.04 NL 1.00* ! NY 1.00* ON 1.00* OV 0.95 PT 1.09 ! SC 1.00* TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.02 GC 1.00* HH 1.04 ! HN 1.00* KK 1.00* KP 1.00* LA 1.17 ! MA 0.97 MC 1.16 MK 1.00* NL 0.96 ! NY 1.00* ON 1.00* OV 1.00* PT 1.03 ! SC 0.90 TS 1.00* WF 1.00* WZ 0.95 ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* GC 0.00* HH 0.00* ! HN 0.00* KK 0.00* KP 0.00* LA 0.00* ! MA 0.00* MC 0.00* MK 0.00* NL 0.00* ! NY 0.00* ON 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 2: ! BR 1.01 FD 0.94 GC 1.00* HH 1.00* ! HN 1.00* KK 0.84 KP 0.92 LA 1.17 ! MA 1.00* MC 1.00* MK 1.00 NL 0.94 ! NY 1.00* ON 1.00* OV 0.95 PT 0.95 ! SC 0.95 TS 1.00* WF 1.33 WZ 1.00* ! ! A total of 3 telescope corrections were flagged in sub-array 3. ! Telescope amplitude corrections in sub-array 3: ! BR 1.20 FD 1.00* GC 1.00* HH 1.00* ! HN 1.00* KK 1.00* KP 1.00* LA 1.00* ! MA 1.00* MC 1.00* MK 1.00 NL 1.00* ! NY 1.00* ON 1.00* OV 0.97 PT 1.23 ! SC 1.00* TS 1.00* WF 1.00* WZ 1.00* ! ! A total of 9 telescope corrections were flagged in sub-array 4. ! Telescope amplitude corrections in sub-array 4: ! BR 1.00* FD 1.00 GC 1.00* HH 1.15 ! HN 1.00* KK 1.00* KP 1.00* LA 1.16 ! MA 0.81 MC 1.15 MK 1.00* NL 0.93 ! NY 1.00* ON 1.00* OV 1.00* PT 1.02 ! SC 0.92 TS 1.00* WF 1.00* WZ 1.07 ! ! ! Fit before self-cal, rms=0.167710Jy sigma=2.024284 ! Fit after self-cal, rms=0.135329Jy sigma=1.235200 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=0.6467 mas, bmaj=1.555 mas, bpa=0.08491 degrees ! Estimated noise=1.29432 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 = 0.00758645 Jy ! Component: 100 - total flux cleaned = 0.00812197 Jy ! Total flux subtracted in 100 components = 0.00812197 Jy ! Clean residual min=-0.007810 max=0.009215 Jy/beam ! Clean residual mean=-0.000077 rms=0.002016 Jy/beam ! Combined flux in latest and established models = 0.874502 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 6 model components to the UV plane model. ! The established model now contains 32 components and 0.874502 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.134589Jy sigma=1.226134 ! Fit after self-cal, rms=0.134629Jy sigma=1.225606 ! 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 = 0.000733154 Jy ! Component: 100 - total flux cleaned = 0.000966706 Jy ! Total flux subtracted in 100 components = 0.000966706 Jy ! Clean residual min=-0.008083 max=0.009116 Jy/beam ! Clean residual mean=-0.000077 rms=0.002001 Jy/beam ! Combined flux in latest and established models = 0.875469 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 6 model components to the UV plane model. ! The established model now contains 35 components and 0.875469 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.134449Jy sigma=1.224194 ! Fit after self-cal, rms=0.134196Jy sigma=1.207016 ! Inverting map and beam ! Estimated beam: bmin=0.6447 mas, bmaj=1.556 mas, bpa=-0.04182 degrees ! Estimated noise=1.29476 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) ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.00443992 Jy ! Component: 100 - total flux cleaned = 0.00456087 Jy ! Total flux subtracted in 100 components = 0.00456087 Jy ! Clean residual min=-0.007256 max=0.008508 Jy/beam ! Clean residual mean=-0.000061 rms=0.001797 Jy/beam ! Combined flux in latest and established models = 0.88003 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 6 model components to the UV plane model. ! The established model now contains 36 components and 0.88003 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.133898Jy sigma=1.203177 ! Fit after self-cal, rms=0.133888Jy sigma=1.203012 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 1124-186_X ! Writing UV FITS file: 1124-186_X.uvf ! Writing 36 model components to file: 1124-186_X.mod ! wwins: Wrote 1 windows to 1124-186_X.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6447 x 1.556 at -0.04182 degrees (North through East) ! Clean map min=-0.00694 max=0.77652 Jy/beam ! Writing clean map to FITS file: 1124-186_X.fits ! Writing difmap environment to: 1124-186_X.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 1124-186_X] device 1124-186_Xuv.ps/vps,1,2 ! Attempting to open device: '1124-186_Xuv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 1124-186_Xim.ps/vps ! Attempting to open device: '1124-186_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=0.6447 mas, bmaj=1.556 mas, bpa=-0.04182 degrees ! Estimated noise=1.29476 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.6447 x 1.556 at -0.04182 degrees (North through East) ! Clean map min=-0.00694 max=0.77652 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo7-0.1] quit ! Quitting program ! Log file 1124-186_X.log closed on Sun Apr 12 14:26:33 2009