Index: trunk/doc/release.2015/ps1.analysis/analysis.tex
===================================================================
--- trunk/doc/release.2015/ps1.analysis/analysis.tex	(revision 39960)
+++ trunk/doc/release.2015/ps1.analysis/analysis.tex	(revision 39974)
@@ -5,5 +5,8 @@
 \RequirePackage{color}
 \RequirePackage{code}
+\RequirePackage{url}
 \input{astro.sty}
+
+\DeclareUrlCommand\email{\urlstyle{rm}}
 
 % online version may use color, but print version needs b/w
@@ -111,9 +114,8 @@
   * find a brighter-fatter reference
 * define more tests and generate examples
-  * simulation example of background subtraction at different densities
+  * simulation example of background subtraction
+    at different densities
   * real example of oversubtracted galaxy
 * check all references
-* fix the \code macro to work with alternate concepts
-  * DONE : the use of \textbf style formats was a problem : expects \textbf{foobar}
 \end{verbatim}
 
@@ -124,4 +126,8 @@
 extended source model fitting, and the techniques for ``forced''
 photometry measurements.
+
+\url{http://eugene@ifa.hawaii.edu}
+
+\end{document}
 
 %Chambers et al. 2017 (Paper I)
@@ -178,6 +184,4 @@
     from early users of the data products are welcome during the
     submission and refereeing process.}}
-
-\end{document}
 
 \section{Background}
@@ -295,5 +299,5 @@
 supplied guess model.  
 
-\section{\code{psphot} Design Goals}
+\section{\nocode{psphot} Design Goals}
 
 \code{psphot} has a number of important requirements that it must meet, and a
@@ -369,5 +373,5 @@
 \end{itemize}
 
-\section{\code{psphot} Analysis Process}
+\section{\nocode{psphot} Analysis Process}
 
 \subsection{Overview}
@@ -447,5 +451,5 @@
 PV3).  3) Pixels which lie outside of a user-defined coordinate window
 are considered non-data pixels (eg, overscan) and are marked as
-invalid.  (psphot recipe keywords \code{XMIN}, \code{XMAX},
+invalid.  (\code{psphot} recipe keywords \code{XMIN}, \code{XMAX},
 \code{YMIN}, \code{YMAX}, all set to 0 for PS1 PV3 -- invalid pixels
 were specified for PS1 PV3 with a supplied mask image, see
@@ -465,5 +469,5 @@
 
 \begin{table*}
-\caption{\label{tab:mask_values} \code{psphot} / GPC1 Mask Image Pixel Values}\vspace{-0.5cm}
+\caption{\label{tab:mask_values} \nocode{psphot} / GPC1 Mask Image Pixel Values}\vspace{-0.5cm}
 \begin{center}
 \begin{tabular}{lcl}
@@ -524,5 +528,5 @@
 Before sources are detected in the image, a model of the background is
 subtracted.  The image is divided into a grid of background points
-with a spacing defined by the psphot recipe values
+with a spacing defined by the \code{psphot} recipe values
 \code{BACKGROUND.XBIN, BACKGROUND.YBIN}, set to 400 pixels for PS1
 PV3.  Superpixels of size \code{BACKGROUND.XSAMPLE,
@@ -1090,5 +1094,5 @@
   for a given order of the PSF 2D variations.}\vspace{-0.5cm}
 \begin{center}
-\begin{tabular}{lcl}
+\begin{tabular}{llll}
 \hline
 \hline
@@ -1209,5 +1213,5 @@
 because of the highly diagonal matrix with small off-diagonal terms:
 the dot product of source $i$ and source $j$ is 1 where $i = j$ and
-much less than 1 where $i \noteq j$.
+much less than 1 where $i \neq j$.
 
 Once a solution set for $A_i$ is found, all of the sources are
@@ -1229,5 +1233,5 @@
 subtracted as discussed above.
 
-\node{code review for the next bit}
+\note{code review for the next bit}
 
 Once a solution has been achieved for a source, \code{psphot} attempts to
@@ -1617,5 +1621,5 @@
 analysis, $b_0 = $20\degree, $r_b = $15\degree, $\sigma_b = $50\degree.
 
-%  \note{need a discussion of the detector saturation behavior
+% \note{need a discussion of the detector saturation behavior
 
 % \note{more detail below?}  
@@ -1956,6 +1960,6 @@
 
 \bibliographystyle{apj}
-% \bibliography{lib}{}
-\input{analysis.bbl}
+\bibliography{lib}{}
+%\input{analysis.bbl}
 
 \end{document}