Index: trunk/doc/design/ippSRS.tex
===================================================================
--- trunk/doc/design/ippSRS.tex	(revision 2169)
+++ trunk/doc/design/ippSRS.tex	(revision 2186)
@@ -1,3 +1,3 @@
- %%% $Id: ippSRS.tex,v 1.9 2004-10-18 22:06:13 eugene Exp $
+ %%% $Id: ippSRS.tex,v 1.10 2004-10-21 03:55:59 eugene Exp $
 \documentclass[panstarrs,spec]{panstarrs}
 
@@ -23,4 +23,5 @@
 \newcommand\VER[2]{\\ {\scriptsize QUALIFICATION METHOD: #1, TRACE: #2}}
 \newcommand\TASK{\\ {\scriptsize TASK}}
+\newcommand\grizy{$grizy$}
 
 % allow paragraphs to be listed in TOC for now 
@@ -40,10 +41,8 @@
 \RevisionsEnd
 
-\TBDsStart
-Section & Page & Number & Description \\ \hline
-        &      &        & choice of scripting language \\ \hline
-        &      &        & coding standards for scripting language \\ \hline
-        &      &        & low-spatial frequency sky model details \\ \hline
-\TBDsEnd
+\inserttbd
+
+\inserttbr
+\pagebreak 
 
 \tableofcontents
@@ -216,6 +215,6 @@
 \item In photometric weather, produce reduced science images for each
   full camera exposure which have background deviations from the
-  static sky in the same filter of less than \tbd{1\%} for the median
-  in large ($> 30$ pixels diameter) regions.\VER{ANALYSIS}{SCD:3.5.12}
+  static sky in the same filter of less than 1\% for the median in
+  large ($> 30$ pixels diameter) regions.\VER{ANALYSIS}{SCD:3.5.12}
   \label{TLR:5a}
 
@@ -255,5 +254,5 @@
 
 \item Degrade the stacked image by no more than \tbr{10
-  milliarcseconds} (FWHM added in quadrature) over the theoretical
+  milliarcseconds (FWHM added in quadrature)} over the theoretical
   limit for the stack under infinite
   sampling.\VER{ANALYSIS}{SCD:3.5.2}
@@ -262,10 +261,10 @@
 \item Perform the processing of science images to the level of
   transient detection and static sky inclusion at a rate such that
-  exposures taken at an average cadence of \tbr{40} seconds do not
+  exposures taken at an \tbr{average cadence of 40 seconds} do not
   accumulate in the processing buffer (average throughput
   requirement).\VER{TEST}{SCD:3.2.2.3}
   \label{TLR:17}
 
-\item Limit the false alarm rate (FAR) to less than \tbr{5\%} for
+\item Limit the \tbr{false alarm rate (FAR) to less than 5\%} for
   transient detections $> 5\sigma$ sent to the preferred client
   science pipelines.\footnote{note difference with PS-4: 1\%}
@@ -273,5 +272,5 @@
  \label{TLR:18}
 
-\item Perform transient detection to a completeness of \tbr{99\%} at
+\item Perform \tbr{transient detection to a completeness of 99\%} at
   the completeness for transient detections with a significant $>
   5\sigma$.\VER{ANALYSIS}{SCD:xxx}
@@ -287,5 +286,6 @@
 
 \item Send the IPP metadata and received OTIS metadata to the
-  Pan-STARRS Published Science Products Subsystem (PSPS) weekly.\VER{TASK}{SCD:3.2.2.18}
+  Pan-STARRS Published Science Products Subsystem (PSPS)
+  weekly.\VER{TASK}{SCD:3.2.2.18}
   \label{TLR:21}
 
@@ -294,17 +294,17 @@
   \label{TLR:22}
 
-\item Provide sufficent storage volume for \tbr{1 year} of raw images
-  from the AP and IVP Surveys.\footnote{note difference with PS-4: 1
-  month of raw images} \VER{INSPECT}{allocated}
+\item Provide sufficent storage volume for raw images from the AP and
+  IVP Surveys and the \grizy\ Static Sky.\footnote{note difference with
+  PS-4: 1 month of raw images} \VER{INSPECT}{allocated}
   \label{TLR:23}
 
 \item Provide sufficient storage volume for all detections from the
-  AP, IVP, and MVP Surveys.\footnote{note difference with PS-4: 1
-  year of detections}\VER{INSPECT}{allocated}
+  AP, IVP, and MVP Surveys.\footnote{note difference with PS-4: 1 year
+  of detections}\VER{INSPECT}{allocated}
   \label{TLR:24}
 
-\item Provide sufficient storage volume for \tbr{2 year} of
- metadata.\footnote{note difference with PS-4: 10
-  years of metadata}\VER{INSPECT}{allocated}
+\item Provide sufficient storage volume for 2 years of
+ metadata.\footnote{note difference with PS-4: 10 years of
+ metadata}\VER{INSPECT}{allocated}
   \label{TLR:25}
 \end{enumerate}
@@ -366,5 +366,5 @@
 \item Source code files shall use the UNIX line-break convention (line-feed only).  \VER{INSPECT}{allocated}
 \item C coding style shall adhere to the standard defined in the document `Pan-STARRS C-coding standard' (PSDC-430-004).  \VER{INSPECT}{allocated}
-\item Perl coding shall follow the standard defined in the document `Pan-STARRS Perl-coding standard' \tbd{(PSDC-430-0XX)}.\VER{INSPECT}{allocated}
+\item Perl coding shall follow the standard defined in the document \tbd{`Pan-STARRS Perl-coding standard' (PSDC-430-0XX)}.\VER{INSPECT}{allocated}
 \end{enumerate}
 
@@ -630,7 +630,11 @@
   reference to the specified image.\VER{TEST}{allocated}
 
-\item \tbd{total volume}
-
-\item \tbd{total number of entries}
+\item The IPP Image Server shall provide a total data capacity of 300
+  TB after the first year of PS-1 operations and 900 TB after the
+  second year of operations.\VER{INSPECT}{}
+
+\item The IPP Image Server shall provide storage for a total of $2
+  \times 10^8$ data objects by the end of the second year of PS-1
+  operations.
 
 \end{enumerate}
@@ -1206,5 +1210,5 @@
 \item The background residuals shall have a scatter of less than
   \tbr{1\%} of the input background amplitude for apertures of less
-  than \tbr{10~arcsec}.\VER{ANALYSIS}{TLR:1}
+  than \tbr{10 arcsec}.\VER{ANALYSIS}{TLR:1}
 
 \item The Phase 2 analysis shall detect cosmic rays with flux $> 5\sigma$ by