Index: /trunk/doc/release.2015/systematics.20140411/diffusion.tex
===================================================================
--- /trunk/doc/release.2015/systematics.20140411/diffusion.tex	(revision 40310)
+++ /trunk/doc/release.2015/systematics.20140411/diffusion.tex	(revision 40311)
@@ -12,7 +12,7 @@
 \RequirePackage{graphicx}
 \RequirePackage{color}
-\RequirePackage{code}
+% \RequirePackage{code}
 % \RequirePackage{pbox}
-\input{astro.sty}
+\input{magnier.tex}
 
 %\newcommand\oldtext[1]{\color{red}#1}
@@ -32,10 +32,11 @@
 %\def\plotmode{bw}
 
-\def\plotext{pdf}
-%\def\plotext{ps}
+%\def\plotext{pdf}
+\def\plotext{eps}
 
 %\def\picdir{/home/eugene/chipresid.20140404}
 %\def\picdir{/data/kukui.2/eugene/chipresid.20140404}
-\def\picdir{pics}
+%\def\picdir{pics} %%% need to set this for local processing
+\def\picdir{.} %%% need to set this for the zip archive
 
 % Pick a terse version of the title here;
@@ -441,5 +442,5 @@
 high density of stars, but avoids the Galactic Plane where confusion
 may potentially contaminate the measurement.  We limit the analysis to
-good measurements (\ippmisc{PSF_QF} $>$ 0.85, see
+good measurements (\textsf{PSF\_QF} $>$ 0.85, see
 \citealt{magnier2017.analysis}) of likely stars ($|m_{psf} -
 m_{aper}| < 0.2$).  Only measurements with instrumental magnitude $<
@@ -1288,5 +1289,6 @@
 \bibliographystyle{apj}
 %\bibliography{lib}{}
-\input{diffusion.bbl}
+%\input{diffusion.bbl}
+\input{magnier_bib.tex}
 
 \end{document}