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@@ -33,14 +33,14 @@
<a href="humour.html">Other Carpets</a></p>
<p><b>Mailing Lists</b><br />
-<a href="http://lists.carpetcode.org/listinfo/developers/">Subscribe</a><br />
-<a href="http://lists.carpetcode.org/archives/developers/">List&nbsp;Archive</a><br />
-<a href="http://lists.carpetcode.org/listinfo/carpet-cvs/">CVS&nbsp;messages</a><br />
-<a href="http://lists.carpetcode.org/listinfo/carpet-darcs/">darcs/git&nbsp;messages</a></p>
+<a href="http://cactuscode.org/community/mailinglists/">List&nbsp;Management</a><br />
+<a href="http://cactuscode.org/mailman/listinfo/developers">Subscribe</a><br />
+<a href="http://cactuscode.org/pipermail/developers/">List&nbsp;Archive</a><br />
+</p>
<p><b>Development</b><br />
<a href="get-carpet.html">Download</a><br />
-<a href="http://bugs.carpetcode.org/">Bug&nbsp;Reports</a><br />
+<a href="http://trac.einsteintoolkit.org/">Bug&nbsp;Reports</a><br />
<a href="contributors.html">Contributors</a></p>
<!-- These are outdated
<a href="feature-requests.html">Missing&nbsp;features</a><br />
@@ -121,127 +121,35 @@ Barcelona<br />
<h2>News</h2>
- <table><tr><td valign="top">
- <p><b>March 30, 2009:</b> We have ported Carpet to
- the <a href="http://www-03.ibm.com/systems/deepcomputing/bluegene/">BlueGene/P</a>
- architecture, using
- the <a href="http://www.alcf.anl.gov/resources/storage.php">Surveyor</a>
- system at the <a href="http://www.alcf.anl.gov/">ALCF</a>. The
- graph to the right shows preliminary performance and scaling
- results, comparing different compilers and options
- (<a href="http://gcc.gnu.org/">gcc</a>, <a href="http://www.ibm.com/software/awdtools/xlcpp/">IBM's
- XL compilers</a> without OpenMP, and IBM's XL compilers
- with <a href="http://www.openmp.org/">OpenMP</a>, which required
- reducing the optimisation level). For these benchmarks, the
- problem size was reduced to about one eighth of the standard
- size, using 13<sup>3</sup> grid points per core. The results
- show that Carpet scales fine up to the size of the total machine
- (4k cores), but further work on compiler options is
- required.</p>
- </td><td valign="top">
- <p><a href="scaling-surveyor/results-surveyor.pdf"><img
- src="scaling-surveyor/results-surveyor.png"
- width="180" alt="AMR benchmark results" /></a></p>
- </td></tr></table>
-
- <table><tr><td valign="top">
- <p><b>March 20, 2009:</b> Carpet can now perform <i>performance
- experiments</i> by artificially increasing the size or the
- number of MPI messages exchanged between processes. This can
- help determine whether either the communication bandwidth or the
- communication latency are a bottleneck of a particular
- simulation. The figure to the right shows results for the
- standard <a href="http://www.cct.lsu.edu/~eschnett/McLachlan/">McLachlan</a>
- AMR benchmark run on
- the <a href="http://en.wikipedia.org/wiki/Cray_XT4">Cray XT4</a>
- <a href="http://www.nics.tennessee.edu/computing-resources/kraken">Kraken</a>, using 25<sup>3</sup> grid points per core. These
- results indicate that the additional latency from increasing the
- number of messages has no significant effect, and hence the
- benchmark is bandwidth limited for this problem size.</p>
- </td><td valign="top">
- <p><a href="scaling-whatif/results-whatif.pdf"><img
- src="scaling-whatif/results-whatif.png"
- width="180" alt="AMR benchmark results" /></a></p>
- </td></tr></table>
-
- <table><tr><td valign="top">
- <p><b>March 16, 2009:</b> Erik Schnetter and Steve Brandt
- published a white
- paper <a href="http://www.cct.lsu.edu/CCT-TR/CCT-TR-2009-4"><i>Relativistic
- Astrophysics on the SiCortex Architecture</i></a>. This paper
- expands on a
- <a href="http://www.sicortex.com/news_events/campaigns/lsu_webinar">webinar</a>
- by Erik and Steve that was hosted
- by <a href="http://www.sicortex.com/">SiCortex</a>.</p>
- <p>The graph at the right shows Carpet's parallel scalability
- using
- the <a href="http://www.cct.lsu.edu/~eschnett/McLachlan/">McLachlan</a>
- code with nine levels of AMR for a set of current HPC systems.
- The results have been rescaled to the architectures' theoretical
- single-core peak performance. This makes it possible to compare
- Carpet's scalability on different architectures. (It is not
- possible to compare the systems' absolute performance in this
- figure.)</p>
- </td><td valign="top">
- <p><a href="sicortex/results-scaled.pdf"><img
- src="sicortex/results-scaled.png"
- width="180" alt="AMR benchmark results" /></a></p>
- </td></tr></table>
-
- <table><tr><td valign="top">
- <p><b>November 9, 2008:</b> In the context of
- the <a href="http://www.cct.lsu.edu/xirel/">XiRel project</a>,
- we re-designed Carpet's communication layer to avoid many
- operations that had a cost of O(<var>N</var>), growing linearly
- with the number of MPI processes. Such costs are generally not
- acceptable when running on several thousand cores, and have to
- be reduced e.g. to O(log <var>N</var>). Carpet now stores the
- communication schedule (mostly) in a distributed manner,
- increasing performance and reducing its memory requirement.
- These improvements are currently being tested; preliminary
- scaling results are shown in the figure to the right.</p>
- </td><td valign="top">
- <p><a href="scaling-improved/results-best.pdf"><img
- src="scaling-improved/results-best.png"
- width="180" alt="AMR benchmark results" /></a></p>
- </td></tr></table>
-
- <p><b>June 25, 2008:</b> We are happy to announce
- the <a href="http://www.cct.lsu.edu/~eschnett/SimFactory"><i>Simulation
- Factory</i></a>, a tool to help access remote HPC systems,
- manage source trees, and submit and control simulations. The
- Simulation Factory contains a set of abstractions of the tasks
- which are necessary to set up and successfully finish numerical
- simulations using the Cactus framework. These abstractions hide
- tedious low-level management tasks, they capture "best
- practices" of experienced users, and they create a log trail
- ensuring repeatable and well-documented scientific results.
- Using these abstractions, many types of potentially disastrous
- user errors are avoided, and different supercomputers can be
- used in a uniform manner.</p>
-
- <table><tr><td valign="top">
- <p><b>March 29, 2008:</b> We have benchmarked McLachlan, a new
- BSSN-type vacuum Einstein code, using Carpet for unigrid and AMR
- calculations. We compare several current large machines:
- <a href="http://www.nersc.gov/nusers/systems/franklin/">Franklin</a>
- (NERSC), <a href="http://www.loni.org/systems/system.php?system=QueenBee">Queen
- Bee</a> (LONI),
- and <a href="http://www.tacc.utexas.edu/services/userguides/ranger/">Ranger</a>
- (TACC).
- <!-- These machines have different architectures and
- interconnects.--></p>
- </td><td valign="top">
- <p><a
- href="scaling-amr/results-carpet-1lev.pdf"><img
- src="scaling-amr/results-carpet-1lev.png" width="180"
- alt="Unigrid benchmark results" /></a></p>
- </td><td valign="top">
- <p><a
- href="scaling-amr/results-carpet-9lev.pdf"><img
- src="scaling-amr/results-carpet-9lev.png" width="180"
- alt="AMR benchmark results" /></a></p>
- </td></tr></table>
+ <p><b>February 15, 2011:</b>
+ The <a href="get-carpet.html">download instructions</a> for Carpet
+ now also point to <a href="http://code.google.com/">Google
+ Code</a>, where the current development version is availble for
+ download.</p>
+
+ <p><b>November 23, 2010:</b> We are pleased to announce the second
+ release (code name
+ "<a href="http://en.wikipedia.org/wiki/Subrahmanyan_Chandrasekhar">Chandrasekhar</a>")
+ of the Einstein Toolkit, an open, community developed software
+ infrastructure for relativistic astrophysics. This release is
+ mainly a maintenance release incorporating fixes accumulated since
+ the previous release in June 2010, as well as additional test
+ suites.</p>
+
+ <p><b>August 30, 2011:</b> Notes from our
+ <a href="http://ccrg.rit.edu/~carpet/wiki/Main_Page">Carpet
+ Developer Workshop</a> at RIT are now available.</p>
+
+ <p><b>June 17, 2010:</b> We are pleased to announce the first
+ release (code name
+ "<a href="http://en.wikipedia.org/wiki/Bohr-Einstein_debates">Bohr</a>")
+ of the Einstein Toolkit, an open, community developed software
+ infrastructure for relativistic astrophysics. The Einstein Toolkit
+ is a collection of over 130 software components and tools for
+ simulating and analyzing general relativistic astrophysical
+ systems that builds on numerous software efforts in the numerical
+ relativity community including CactusEinstein, the Whisky
+ hydrodynamics code, and the Carpet AMR infrastructure.</p>
<p><a href="olds.html"><b>Old News...</b></a></p>
@@ -291,6 +199,7 @@ Barcelona<br />
<h2>Interacting with the developers</h2>
+<!-- outdated
<p>Most discussions about Carpet, i.e. user questions, feature
requests, and bug reports, are held on the Carpet developers'
mailing list <a
@@ -300,7 +209,17 @@ Barcelona<br />
You will also find the mailing list archive there. We thank <a
href="http://www.tat.physik.uni-tuebingen.de/~kobras/">Daniel
Kobras</a> for managing the mailing list server.</p>
-
+-->
+ <p>Most discussions about Carpet, i.e. user questions, feature
+ requests, and bug reports, are held on the Cactus developers'
+ mailing
+ list <a href="mailto:developers@cactuscode.org">developers@cactuscode.org</a>.
+ You can subscribe and unsubscribe from
+ our <a href="http://cactuscode.org/community/mailinglists/">list
+ management web page</a>. You will also find the mailing list
+ archive there.</p>
+
+<!-- outdated
<p>We have started to use <a
href="http://www.bugzilla.org/">Bugzilla</a> to keep track of
requested features or reported bugs in Carpet. You can submit or
@@ -309,6 +228,12 @@ Barcelona<br />
have created an account there. The old <a
href="feature-requests.html">list of missing features</a> have not
yet been moved over to Bugzilla.</p>
+-->
+
+ <p>We use <a href="http://trac.edgewall.org/">TRAC</a> to keep
+ track of requested features or reported bugs in Carpet. You can
+ submit or comment on issues from
+ our <a href="http://trac.einsteintoolkit.org/">TRAC site</a>.</p>
<hr />
@@ -493,7 +418,7 @@ Barcelona<br />
<p>
<!-- Created: Tue Aug 12 12:12:08 CEST 2003 -->
<!-- hhmts start -->
-Last modified: Mon Mar 30 2009
+Last modified: Tue Feb 15 2011
<!-- hhmts end -->
</p>