! Started logfile: 1821+107_X.log on Wed May 14 15:59:04 2008 observe 1821+107_X.edt ! Reading UV FITS file: 1821+107_X.edt ! AN table 1: 48 integrations on 153 of 153 possible baselines. ! Apparent sampling: 0.0269608 visibilities/baseline/integration-bin. ! *** This seems a bit low - see "help observe" on the binwid argument. ! Found source: 1821+107 ! ! 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 946 lines of history. ! ! Reading 792 visibilities. ![@gonzo7-0.1-pw 1821+107_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 857 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 2. ! A total of 852 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 3. ! A total of 855 telescope corrections were flagged in sub-array 1. ! ! Correcting IF 4. ! A total of 850 telescope corrections were flagged in sub-array 1. ! ! Fit before self-cal, rms=0.716851Jy sigma=0.008694 ! Fit after self-cal, rms=0.720587Jy sigma=0.008677 ! 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 peakw win_mult ! Inverting map and beam ! Estimated beam: bmin=0.5262 mas, bmaj=1.469 mas, bpa=-8.111 degrees ! Estimated noise=10665.4 mJy/beam. ! Added new window around map position (0, 0). 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=50 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.20378 Jy ! Total flux subtracted in 50 components = 0.20378 Jy ! Clean residual min=-0.043313 max=0.056830 Jy/beam ! Clean residual mean=0.000096 rms=0.015268 Jy/beam ! Combined flux in latest and established models = 0.20378 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 0.20378 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.128082Jy sigma=0.001562 ! Fit after self-cal, rms=0.128078Jy sigma=0.001562 ! 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=0.5615 mas, bmaj=1.595 mas, bpa=-7.369 degrees ! Estimated noise=8905.61 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 = 0.0844494 Jy ! Component: 100 - total flux cleaned = 0.132013 Jy ! Total flux subtracted in 100 components = 0.132013 Jy ! Clean residual min=-0.034677 max=0.032183 Jy/beam ! Clean residual mean=0.000107 rms=0.012228 Jy/beam ! Combined flux in latest and established models = 0.335794 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 17 components and 0.335794 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.065149Jy sigma=0.000792 ! Fit after self-cal, rms=0.064992Jy sigma=0.000790 ! 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 3 telescope corrections were flagged in sub-array 1. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* GC 1.00* HH 1.00* ! HN 0.92 KK 1.00* KP 1.00* LA 1.00* ! MC 1.00* MK 1.00* NL 0.91 NY 0.93 ! ON 1.00* OV 1.00* PT 1.00* SC 1.00* ! WF 1.00* WZ 0.94 ! ! ! 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 1.00* HH 1.00* ! HN 1.08 KK 1.00* KP 1.00* LA 1.00* ! MC 0.90 MK 1.00* NL 0.76 NY 1.22 ! ON 1.00* OV 1.00* PT 1.00* SC 1.17 ! WF 1.00* WZ 0.73 ! ! ! Correcting IF 3. ! Telescope amplitude corrections in sub-array 1: ! BR 1.00* FD 1.00* GC 1.00* HH 1.00* ! HN 1.01 KK 1.00* KP 1.00* LA 1.00* ! MC 0.99 MK 1.00* NL 0.91 NY 1.06 ! ON 1.00* OV 1.00* PT 1.00* SC 0.95 ! WF 0.96 WZ 1.00* ! ! ! Correcting IF 4. ! 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 1.00* HH 1.00* ! HN 0.91 KK 1.00* KP 1.00* LA 1.00* ! MC 0.96 MK 1.00* NL 0.92 NY 1.08 ! ON 1.00* OV 1.00* PT 1.00* SC 0.99 ! WF 1.00* WZ 0.87 ! ! ! Fit before self-cal, rms=0.064992Jy sigma=0.000790 ! Fit after self-cal, rms=0.057480Jy sigma=0.000543 dynam = dynam - 0.5 doamp = false flux_cutoff = imstat(rms) * dynam ! Inverting map and beam ! Estimated beam: bmin=0.5567 mas, bmaj=1.633 mas, bpa=-7.7 degrees ! Estimated noise=9087.79 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) ! clean: niter=100 gain=0.03 cutoff=0 ! Component: 050 - total flux cleaned = 0.0158046 Jy ! Component: 100 - total flux cleaned = 0.0227562 Jy ! Total flux subtracted in 100 components = 0.0227562 Jy ! Clean residual min=-0.017102 max=0.014124 Jy/beam ! Clean residual mean=0.000006 rms=0.004079 Jy/beam ! Combined flux in latest and established models = 0.35855 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 19 components and 0.35855 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.051984Jy sigma=0.000475 ! Fit after self-cal, rms=0.051989Jy sigma=0.000474 ! 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 = 0.00146864 Jy ! Component: 100 - total flux cleaned = 0.0014663 Jy ! Total flux subtracted in 100 components = 0.0014663 Jy ! Clean residual min=-0.017570 max=0.013560 Jy/beam ! Clean residual mean=0.000003 rms=0.004011 Jy/beam ! Combined flux in latest and established models = 0.360016 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 22 components and 0.360016 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.051463Jy sigma=0.000470 ! Fit after self-cal, rms=0.046587Jy sigma=0.000442 ! Inverting map and beam ! Estimated beam: bmin=0.5537 mas, bmaj=1.628 mas, bpa=-7.715 degrees ! Estimated noise=9034.62 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 = 0.0039952 Jy ! Component: 100 - total flux cleaned = 0.00508841 Jy ! Total flux subtracted in 100 components = 0.00508841 Jy ! Clean residual min=-0.014048 max=0.013402 Jy/beam ! Clean residual mean=0.000005 rms=0.003641 Jy/beam ! Combined flux in latest and established models = 0.365105 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 29 components and 0.365105 Jy ! ! Correcting IF 1. ! ! Correcting IF 2. ! ! Correcting IF 3. ! ! Correcting IF 4. ! ! Fit before self-cal, rms=0.045975Jy sigma=0.000436 ! Fit after self-cal, rms=0.045994Jy sigma=0.000436 ! Inverting map print "***********************************" ! *********************************** print "*** Finished Amplitude Self-Cal ***" ! *** Finished Amplitude Self-Cal *** print "***********************************" ! *********************************** save 1821+107_X ! Writing UV FITS file: 1821+107_X.uvf ! Writing 29 model components to file: 1821+107_X.mod ! wwins: Wrote 1 windows to 1821+107_X.win ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5537 x 1.628 at -7.715 degrees (North through East) ! Clean map min=-0.013441 max=0.26201 Jy/beam ! Writing clean map to FITS file: 1821+107_X.fits ! Writing difmap environment to: 1821+107_X.par print "****************************" ! **************************** print "*** Now, make some plots ***" ! *** Now, make some plots *** print "****************************" ! **************************** ![@gonzo_plot 1821+107_X] device 1821+107_Xuv.ps/vps,1,2 ! Attempting to open device: '1821+107_Xuv.ps/vps' radplot ! Using default options string "m1" uvplot ! Using default options string "" device 1821+107_Xim.ps/vps ! Attempting to open device: '1821+107_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=0.5537 mas, bmaj=1.628 mas, bpa=-7.715 degrees ! Estimated noise=9034.62 mJy/beam. mappl cln ! restore: Substituting estimate of restoring beam from last 'invert'. ! Restoring with beam: 0.5537 x 1.628 at -7.715 degrees (North through East) ! Clean map min=-0.013441 max=0.26201 Jy/beam ![Exited script file: gonzo_plot] ![Exited script file: gonzo7-0.1-pw] quit ! Quitting program ! Log file 1821+107_X.log closed on Wed May 14 15:59:11 2008