Changeset 39883 for trunk/doc/release.2015/ps1.analysis/analysis.tex

Timestamp:

Dec 16, 2016, 5:11:22 PM (10 years ago)

Author:

eugene

Message:

moved ps figures to pics/ps

File:

• trunk/doc/release.2015/ps1.analysis/analysis.tex (modified) (5 diffs)

trunk/doc/release.2015/ps1.analysis/analysis.tex

@@ -26 +26 @@
 
 %\def\picdir{/home/eugene/chipresid.20140404}
-\def\picdir{/data/pikake.2/eugene/chipresid.20140404}
+\def\picdir{pics}
 
 % Pick a terse version of the title here;
@@ -584 +584 @@
 \begin{figure}[htbp]
   \begin{center}
- \includegraphics[width=\hsize,clip]{peaks}
+ \includegraphics[width=\hsize,clip]{pics/peaks}
   \caption{\label{fig:peaks} Illustration of peak finding and culling peaks within a
     footprint.  Insignificant peaks within the footprint of a brighter
@@ -626 +626 @@
 \begin{figure}[htbp]
   \begin{center}
-  \includegraphics[width=\hsize]{{FWHM.smooth.trend.ps1}.\plotext}
+  \includegraphics[width=\hsize]{{pics/FWHM.smooth.trend.ps1}.\plotext}
   \caption{\label{fig:moments.window} Example of the biases encountered when measuring the second
     moments.  A simulated image was generated using the PS1 PSF
@@ -913 +913 @@
 \begin{figure}[htbp]
   \begin{center}
-  \includegraphics[width=\hsize]{{moment.class}.\plotext}
+  \includegraphics[width=\hsize]{{pics/moment.class}.\plotext}
   \caption{\label{fig:moment.class} Illustration of PSF star selection using the FWHM derived
     from the second moments in $X_{\rm ccd}$ and $Y_{\rm ccd}$
@@ -1320 +1320 @@
 \begin{figure}[htbp]
   \begin{center}
-  \includegraphics[width=\hsize]{{radial.profiles}.\plotext}
+  \includegraphics[width=\hsize]{{pics/radial.profiles}.\plotext}
   \caption{\label{fig:radial.profiles} Radial profiles of stellar images from PS1.  These two
     profiles illustrate the radial trend of the PS1 PSFs for a star