- Timestamp:
- Dec 16, 2016, 8:29:21 AM (10 years ago)
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trunk/doc/release.2015/ps1.analysis/analysis.tex (modified) (6 diffs)
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trunk/doc/release.2015/ps1.analysis/analysis.tex
r39873 r39876 3 3 % \pdfoutput=1 4 4 5 % bounding box is not read correctly without 'graphicx' 6 \RequirePackage{graphicx} 5 7 \RequirePackage{color} 6 8 \RequirePackage{code} … … 12 14 13 15 %\def\plotext{pdf} 16 %\def\plottype{pdf} 17 14 18 \def\plotext{ps} 15 19 \def\plottype{eps} … … 574 578 \begin{figure}[htbp] 575 579 \begin{center} 576 \includegraphics[type=\plottype,ext=.\plotext,width=\hsize,height=0.5\hsize,viewport=60 60 560 310,clip]{peaks} 580 \includegraphics[type=\plottype,ext=.\plotext,width=\hsize,clip]{peaks} 581 % \includegraphics[type=\plottype,ext=.\plotext,width=3.5in,clip]{peaks} 582 % \includegraphics[type=\plottype,ext=.\plotext,width=\hsize,height=0.5\hsize,viewport=60 60 560 310,clip]{peaks} 577 583 \caption{\label{fig:peaks} Illustration of peak finding and culling peaks within a 578 584 footprint. Insignificant peaks within the footprint of a brighter … … 616 622 \begin{figure}[htbp] 617 623 \begin{center} 618 \includegraphics[type=\plottype,ext=.\plotext,width=\hsize,height=2.0\hsize,viewport=60 60 413 760]{FWHM.smooth.trend.ps1} 624 % \includegraphics[type=\plottype,ext=.\plotext,width=\hsize,height=2.0\hsize,viewport=60 60 413 760]{FWHM.smooth.trend.ps1} 625 \includegraphics[type=\plottype,ext=.\plotext,width=\hsize]{FWHM.smooth.trend.ps1} 619 626 \caption{\label{fig:moments.window} Example of the biases encountered when measuring the second 620 627 moments. A simulated image was generated using the PS1 PSF … … 903 910 \begin{figure}[htbp] 904 911 \begin{center} 905 \includegraphics[type=\plottype,ext=.\plotext,width=\hsize,height=\hsize,viewport=60 60 560 560]{moment.class} 912 % \includegraphics[type=\plottype,ext=.\plotext,width=\hsize,height=\hsize,viewport=60 60 560 560]{moment.class} 913 \includegraphics[type=\plottype,ext=.\plotext,width=\hsize]{moment.class} 906 914 \caption{\label{fig:moment.class} Illustration of PSF star selection using the FWHM derived 907 915 from the second moments in $X_{\rm ccd}$ and $Y_{\rm ccd}$ … … 1310 1318 \begin{figure}[htbp] 1311 1319 \begin{center} 1312 \includegraphics[type=\plottype,ext=.\plotext,width=\hsize,height=\hsize,viewport=60 60 560 560]{radial.profiles} 1320 % \includegraphics[type=\plottype,ext=.\plotext,width=\hsize,height=\hsize,viewport=60 60 560 560]{radial.profiles} 1321 \includegraphics[type=\plottype,ext=.\plotext,width=\hsize]{radial.profiles} 1313 1322 \caption{\label{fig:radial.profiles} Radial profiles of stellar images from PS1. These two 1314 1323 profiles illustrate the radial trend of the PS1 PSFs for a star
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