! Started logfile: 1800+440_X.log on Mon Sep 10 19:53:45 2007 observe 1800+440_X.edt ! Reading UV FITS file: 1800+440_X.edt ! AN table 1: 33 integrations on 171 of 171 possible baselines. ! AN table 2: 17 integrations on 171 of 171 possible baselines. ! AN table 3: 33 integrations on 171 of 171 possible baselines. ! AN table 4: 13 integrations on 171 of 171 possible baselines. ! Apparent sampling: 0.0853436 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 1800+440 ! 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 2132 lines of history. ! ! Reading 5604 visibilities. ![@gonzo7-0.1 1800+440_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 617 telescope corrections were flagged in sub-array 1. ! A total of 293 telescope corrections were flagged in sub-array 2. ! A total of 439 telescope corrections were flagged in sub-array 3. ! A total of 247 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 2. ! A total of 613 telescope corrections were flagged in sub-array 1. ! A total of 287 telescope corrections were flagged in sub-array 2. ! A total of 436 telescope corrections were flagged in sub-array 3. ! A total of 247 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 3. ! A total of 619 telescope corrections were flagged in sub-array 1. ! A total of 291 telescope corrections were flagged in sub-array 2. ! A total of 456 telescope corrections were flagged in sub-array 3. ! A total of 247 telescope corrections were flagged in sub-array 4. ! ! Correcting IF 4. ! A total of 627 telescope corrections were flagged in sub-array 1. ! A total of 290 telescope corrections were flagged in sub-array 2. ! A total of 451 telescope corrections were flagged in sub-array 3. ! A total of 247 telescope corrections were flagged in sub-array 4. ! ! Fit before self-cal, rms=0.290410Jy sigma=0.003248 ! Fit after self-cal, rms=0.289298Jy sigma=0.003246 ! 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=0.6287 mas, bmaj=0.8687 mas, bpa=19.73 degrees ! Estimated noise=2530.15 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 = 0.559246 Jy ! Total flux subtracted in 50 components = 0.559246 Jy ! Clean residual min=-0.034831 max=0.155968 Jy/beam ! Clean residual mean=0.000400 rms=0.010494 Jy/beam ! Combined flux in latest and established models = 0.559246 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 1 model components to the UV plane model. ! The established model now contains 1 components and 0.559246 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.180258Jy sigma=0.002099 ! Fit after self-cal, rms=0.180258Jy sigma=0.002099 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.122013 Jy ! Total flux subtracted in 50 components = 0.122013 Jy ! Clean residual min=-0.012758 max=0.034543 Jy/beam ! Clean residual mean=0.000182 rms=0.003735 Jy/beam ! Combined flux in latest and established models = 0.681259 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 3 model components to the UV plane model. ! The established model now contains 3 components and 0.681259 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.088221Jy sigma=0.001021 ! Fit after self-cal, rms=0.088224Jy sigma=0.001020 ! Inverting map ! clean: niter=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0353504 Jy ! Total flux subtracted in 50 components = 0.0353504 Jy ! Clean residual min=-0.009182 max=0.016813 Jy/beam ! Clean residual mean=0.000117 rms=0.002542 Jy/beam ! Combined flux in latest and established models = 0.716609 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 8 components and 0.716609 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.075668Jy sigma=0.000858 ! Fit after self-cal, rms=0.075641Jy sigma=0.000857 ! 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=0.7224 mas, bmaj=0.9169 mas, bpa=15.68 degrees ! Estimated noise=1410.32 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 = 0.0238475 Jy ! Component: 100 - total flux cleaned = 0.0371883 Jy ! Total flux subtracted in 100 components = 0.0371883 Jy ! Clean residual min=-0.006974 max=0.010615 Jy/beam ! Clean residual mean=0.000287 rms=0.001961 Jy/beam ! Combined flux in latest and established models = 0.753797 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 13 model components to the UV plane model. ! The established model now contains 17 components and 0.753797 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.069419Jy sigma=0.000767 ! Fit after self-cal, rms=0.069349Jy sigma=0.000767 ! Inverting map print "****************************************" ! **************************************** print "*** Finished Natural Weighting CLEAN ***" ! *** Finished Natural Weighting CLEAN *** print "****************************************" ! **************************************** gscale true ! Performing overall amplitude self-cal ! ! Correcting IF 1. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* GC 0.99 GG 1.00* ! HN 1.00* KP 1.00* LA 1.00* MA 1.19 ! MK 1.00* NL 1.00* NY 1.01 ON 1.00* ! OV 1.00* PT 1.00* SC 1.00* TC 1.00* ! TS 0.96 WF 1.00* WZ 1.00* ! ! A total of 6 telescope corrections were flagged in sub-array 2. ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 FD 1.00* GC 1.00* GG 1.00* ! HN 0.97 KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 0.97 NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 0.99 TC 1.00* ! TS 1.00* WF 1.00* WZ 1.01 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.00 GC 1.04 GG 1.00* ! HN 0.98 KP 1.00* LA 0.99 MA 1.02 ! MK 1.00* NL 0.99 NY 1.01 ON 1.00 ! OV 1.00* PT 0.99 SC 0.99 TC 1.00* ! TS 1.00* WF 1.00* WZ 1.00 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! ! Correcting IF 2. ! A total of 6 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* GC 1.01 GG 1.00* ! HN 1.00* KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 1.00* NY 1.02 ON 1.07 ! OV 1.00* PT 1.00* SC 1.00* TC 1.00* ! TS 0.98 WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 1.00* GC 1.00* GG 1.00* ! HN 0.97 KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 0.98 NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 1.02 TC 1.00* ! TS 1.00* WF 1.00* WZ 1.02 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 FD 0.99 GC 1.04 GG 1.00* ! HN 0.97 KP 1.00* LA 0.99 MA 1.02 ! MK 1.00* NL 0.99 NY 1.00 ON 1.02 ! OV 1.00* PT 1.00 SC 1.00 TC 1.00* ! TS 1.00* WF 1.00* WZ 0.99 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! ! Correcting IF 3. ! A total of 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* GC 1.07 GG 1.00* ! HN 1.00* KP 1.00* LA 1.00* MA 1.02 ! MK 1.00* NL 1.00* NY 0.97 ON 1.07 ! OV 1.00* PT 1.00* SC 1.00* TC 1.00* ! TS 1.00 WF 1.00* WZ 1.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.01 FD 1.00* GC 1.00* GG 1.00* ! HN 0.97 KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 0.99 NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 0.99 TC 1.00* ! TS 1.00* WF 1.00* WZ 1.00 ! ! Telescope amplitude corrections in sub-array 3: ! BR 0.99 FD 1.00 GC 1.04 GG 1.00* ! HN 0.98 KP 1.00* LA 0.99 MA 1.02 ! MK 1.00* NL 0.99 NY 1.00 ON 1.00 ! OV 1.00* PT 1.00 SC 1.00 TC 1.00* ! TS 1.00* WF 1.00* WZ 1.00 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! ! Correcting IF 4. ! Telescope amplitude corrections in sub-array 1: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! Telescope amplitude corrections in sub-array 2: ! BR 1.04 FD 1.00* GC 1.00* GG 1.00* ! HN 0.97 KP 1.00* LA 1.00* MA 1.00* ! MK 1.00* NL 0.97 NY 1.00* ON 1.00* ! OV 1.00* PT 1.00* SC 0.99 TC 1.00* ! TS 1.00* WF 1.00* WZ 1.00 ! ! Telescope amplitude corrections in sub-array 3: ! BR 1.00 FD 1.00 GC 1.04 GG 1.00* ! HN 0.98 KP 1.00* LA 0.98 MA 1.03 ! MK 1.00* NL 0.98 NY 1.00 ON 0.99 ! OV 1.00* PT 0.99 SC 1.00 TC 1.00* ! TS 1.00* WF 1.00* WZ 1.00 ! ! Telescope amplitude corrections in sub-array 4: ! BR 0.00* FD 0.00* GC 0.00* GG 0.00* ! HN 0.00* KP 0.00* LA 0.00* MA 0.00* ! MK 0.00* NL 0.00* NY 0.00* ON 0.00* ! OV 0.00* PT 0.00* SC 0.00* TC 0.00* ! TS 0.00* WF 0.00* WZ 0.00* ! ! ! Fit before self-cal, rms=0.069349Jy sigma=0.000767 ! Fit after self-cal, rms=0.068420Jy sigma=0.000745 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=0.7271 mas, bmaj=0.9212 mas, bpa=15.6 degrees ! Estimated noise=1406.75 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 = 0.00420449 Jy ! Component: 100 - total flux cleaned = 0.00538463 Jy ! Total flux subtracted in 100 components = 0.00538463 Jy ! Clean residual min=-0.004900 max=0.006547 Jy/beam ! Clean residual mean=0.000081 rms=0.001357 Jy/beam ! Combined flux in latest and established models = 0.759182 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 9 model components to the UV plane model. ! The established model now contains 23 components and 0.759182 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.068165Jy sigma=0.000742 ! Fit after self-cal, rms=0.068139Jy sigma=0.000742 ! 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 = 0.000751104 Jy ! Component: 100 - total flux cleaned = 0.00104314 Jy ! Total flux subtracted in 100 components = 0.00104314 Jy ! Clean residual min=-0.004898 max=0.006461 Jy/beam ! Clean residual mean=0.000069 rms=0.001329 Jy/beam ! Combined flux in latest and established models = 0.760225 Jy ! Performing amp+phase self-cal over 1 minute time intervals ! Adding 8 model components to the UV plane model. ! The established model now contains 25 components and 0.760225 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.068050Jy sigma=0.000741 ! Fit after self-cal, rms=0.067243Jy sigma=0.000733 ! Inverting map and beam ! Estimated beam: bmin=0.7263 mas, bmaj=0.9204 mas, bpa=15.66 degrees ! Estimated noise=1407.91 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 = 0.00266785 Jy ! Component: 100 - total flux cleaned = 0.00411319 Jy ! Total flux subtracted in 100 components = 0.00411319 Jy ! Clean residual min=-0.004945 max=0.006130 Jy/beam ! Clean residual mean=0.000046 rms=0.001277 Jy/beam ! Combined flux in latest and established models = 0.764338 Jy ! Performing phase self-cal over 0.6 minute time intervals ! Adding 9 model components to the UV plane model. ! The established model now contains 26 components and 0.764338 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.067134Jy sigma=0.000732 ! Fit after self-cal, rms=0.067123Jy sigma=0.000732 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 1800+440_X ! Writing UV FITS file: 1800+440_X.uvf ! Writing 26 model components to file: 1800+440_X.mod ! wwins: Wrote 1 windows to 1800+440_X.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7263 x 0.9204 at 15.66 degrees (North through East) ! Clean map min=-0.0047591 max=0.71937 Jy/beam ! Writing clean map to FITS file: 1800+440_X.fits ! Writing difmap environment to: 1800+440_X.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 1800+440_X] device 1800+440_Xuv.ps/vps,1,2 ! Attempting to open device: '1800+440_Xuv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 1800+440_Xim.ps/vps ! Attempting to open device: '1800+440_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=0.7263 mas, bmaj=0.9204 mas, bpa=15.66 degrees ! Estimated noise=1407.91 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.7263 x 0.9204 at 15.66 degrees (North through East) ! Clean map min=-0.0047591 max=0.71937 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo7-0.1] quit ! Quitting program ! Log file 1800+440_X.log closed on Mon Sep 10 19:53:51 2007