Changeset 41398 for trunk

Timestamp:

Aug 10, 2020, 8:38:13 PM (6 years ago)

Author:

eugene

Message:

mods for referee

Location:

trunk/doc/release.2015/ps1.dataproducts

Files:

• dataproducts.tex (modified) (4 diffs)
• referee.v0.pdf (added)
• report.v0.txt (added)

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

@@ -1 @@
-\documentclass[preprint2]{emulateapj}
+% \documentclass[preprint2]{emulateapj}
+\documentclass[iop,floatfix]{emulateapj}
 
 %% EAM 2019.08.26 : I am starting edits based on the comments I sent to HAF last month
@@ -241 +242 @@
 \section{Background}
 \label{sec:background}
-The Pan-STARRS Project teamed with Alex Szalay's database development group at The Johns Hopkins University (JHU) to undertake the task of providing a publicly accessible hierarchical database for \PS\ \citep{Heasley2008}. The JHU team was the major developer of the Sloan Digital Sky Survey (SDSS) public database \citep{Thakar2003}, and it was an early goal of the Pan-STARRS team to reuse as much of the existing software as possible. However, for a number of reasons including the much larger size of the \PS\ dataset, the wide variety of image and measurement types and the importance of temporal information, major changes to the code base were required.  Like the SDSS database, the database implementation for \PS\ is based on the Microsoft SQL Server product line, with supporting code forked from the SDSS Catalog Archive Server Jobs System (CasJobs).  Staying with SQL Server allows the use of a wealth of software developed for SDSS, including the  Hierarchical Triangular Mesh tools \citep{Szalay2007}.  The system developed for \PS\ is called the {\em Published Science Products Subsystem}, or PSPS \citep{Heasley2006}.
+
+The Pan-STARRS Project teamed with Alex Szalay's database development
+group at The Johns Hopkins University (JHU) to undertake the task of
+providing a publicly accessible hierarchical database for
+\PS\ \citep{Heasley2008}. The JHU team was the major developer of the
+Sloan Digital Sky Survey (SDSS) public database \citep{Thakar2003},
+and it was an early goal of the Pan-STARRS team to reuse as much of
+the existing software as possible. However, for a number of reasons
+including the much larger size of the \PS\ dataset, the wide variety
+of image and measurement types and the importance of temporal
+information, major changes to the code base were required.  Like the
+SDSS database, the database implementation for \PS\ is based on the
+Microsoft SQL Server product line, with supporting code forked from
+the SDSS Catalog Archive Server Jobs System (CasJobs).  Staying with
+SQL Server allows the use of a wealth of software developed for SDSS,
+including the Hierarchical Triangular Mesh tools \citep{Szalay2007}.
+The system developed for \PS\ is called the {\em Published Science
+  Products Subsystem}, or PSPS \citep{Heasley2006}.
+\note{define hierarchical, note relational}
+
 
 %(SDSS) public database \citep{Thakar2003}, and it is useful to reuse as much of the software developed for the SDSS as possible. However, due
@@ -266 +286 @@
 
 This paper covers multiple data releases.  The first \PS\ data release
-(DR1, Dec 2016) covers the 3$\pi$ \ippstage{stack} images and the static
-sky catalog.  The DR1 image products are deep stacked images
-along with ancillary data including signal, masks, variance, and
-number maps.  The DR1 catalog data products available from the PSPS
-include the PS1 static sky 3$\pi$ catalog. Source properties are
-organized into several tables, as described in
-Table~\ref{table:pspstables}; only tables referring to the static
-results, without time domain information, are included in DR1.
-
-Data Release 2 (DR2, Jan 2019), adds more of the PS1 image products
+(DR1, \textadd{database opened to public in} Dec 2016) covers the 3$\pi$
+\ippstage{stack} images and the static sky catalog.  The DR1 image
+products are deep stacked images along with ancillary data including
+signal, masks, variance, and number maps.  The DR1 catalog data
+products available from the PSPS include the PS1 static sky 3$\pi$
+catalog. Source properties are organized into several tables, as
+described in Table~\ref{table:pspstables}; only tables referring to
+the static results, without time domain information, are included in
+DR1.
+
+Data Release 2 (DR2, \textadd{database opened to public in} Jan 2019), adds more of the PS1 image products
 from the 3$\pi$ survey, including the single epoch \ippstage{warp} images
 and their ancillary data, such as signal, masks, and variance
 maps. DR2 provides the \ippdbtable{Detection} tables and \ippdbtable{Forced*}
+\footnote{\textadd{In this article, we refer to groups of tables with the same
+  base name using the file ``glob'' convention where, e.g., \ippdbtable{Forced*} refers
+  to a collection of tables starting with \ippdbtable{Forced}.}}
 tables, containing the single epoch source detections and the forced
 photometry.  DR2 also contains numerous improvements to the data
@@ -1609 +1633 @@
 
 \bibliographystyle{apj}
-%\bibliography{dataproducts}{}
-\input{dataproducts.bbl}
+\bibliography{dataproducts}{}
+%\input{dataproducts.bbl}
 
 \appendix