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= ENZO =

ENZO IS AN OPEN SOURCE CODE.  We encourage you to take it, inspect it, use it,
and contribute back any changes you have made.  We strive to make the the Enzo
community a community of *developers*.

== RESOURCES ==

Enzo's main webpage is:

 * http://enzo-project.org

Enzo is developed in the open on bitbucket.org:

 * Stable Version: https://bitbucket.org/enzo/enzo-stable
 * Development Version: https://bitbucket.org/enzo/enzo-dev

Documentation, including instructions for compilation, can be found at:

 * http://enzo-project.org/docs/2.2/

Please subscribe to the Enzo Users' mailing list at:

 * https://mailman.ucsd.edu/mailman/listinfo/enzo-users-l

You can also follow the Enzo Project on google+ at:

 * https://plus.google.com/115923030596894217717

If you have received this source code through an archive, rather than the
mercurial version control system, we highly encourage you to upgrade to the
version controlled source, as no support can be provided for archived
("tarball") sources.

== DEVELOPERS ==

Many people have contributed to the development of Enzo -- here's just a short
list of the people who have recently contributed, in alphabetical order:
   
   * Tom Abel               tabel@stanford.edu
   * James Bordner          jobordner@ucsd.edu
   * Greg Bryan             gbryan@astro.columbia.edu
   * Renyue Cen             cen@astro.princeton.edu
   * Dave Collins           dcollins@physics.ucsd.edu
   * Brian Crosby           crosby.bd@gmail.com
   * Nathan Goldbaum        goldbaum@ucolick.org
   * Oliver Hahn            hahn@phys.ethz.ch
   * Robert Harkness        harkness@sdsc.edu
   * Elizabeth Harper-Clark h-clark@astro.utoronto.ca
   * Cameron Hummels        chummels@gmail.com
   * Ji-hoon Kim            mornkr@ucolick.org
   * Daegene Koh            dkoh30@gatech.edu
   * Alexei Kritsuk         akritsuk@ucsd.edu
   * Michael Kuhlen         mqk@astro.berkeley.edu
   * Eve Lee                elee@cita.utoronto.ca
   * Yuan Li                yuan@astro.columbia.edu
   * Michael Norman         mlnorman@ucsd.edu
   * JS Oishi               jsoishi@gmail.com
   * Brian O'Shea           oshea@msu.edu
   * Pascal Paschos         ppaschos@minbari.ucsd.edu
   * Carolyn Peruta         perutaca@msu.edu
   * Alex Razoumov          razoumov@gmail.com
   * Dan Reynolds           reynolds@smu.edu
   * Munier Salem           msalem@astro.columbia.edu
   * Christine Simpson      csimpson@astro.columbia.edu
   * Samuel Skillman        samskillman@gmail.com 
   * Stephen Skory          s@skory.us
   * Britton Smith          brittonsmith@gmail.com
   * Geoffrey So            gsiisg@gmail.com
   * Elizabeth Tasker       tasker@astro1.sci.hokudai.ac.jp
   * Matthew Turk           matthewturk@gmail.com
   * Rick Wagner            rwagner@physics.ucsd.edu
   * Peng Wang              pengw@slac.stanford.edu
   * John Wise              jwise@physics.gatech.edu
   * Hao Xu                 haxu@ucsd.edu
   * Fen Zhao               fenzhao@stanford.edu


Recent activity

John Wise

John Wise pushed 36 commits to jwise77/clean-copy

4e0e026 - Fixing mixed precision issues.
5c0b49c - Adding OpenMP config flag for Kraken-gnu make file.
27df924 - Fixing functionality that stops a simulation after a certain number of
4e2bd86 - Undid a change I had made in the Linux Makefile.
f2047d4 - Removed stdlib import from hydro_rk/Grid_MHDRK2_1stStep.C
John Wise

John Wise pushed 37 commits to jwise77/clean-copy

5f20d61 - Merging from mainline and resolving a conflict.
1605f1d - This should now work for specifying which fields to use for refinement.
ffb3b0e - Adding quick note about referring to the method paper.
498d0cf - Add some docs to the source code, and setting the number of fields to 1 by default. If the user specifies additional fields, they will ...
08b1dec - Adding documentation for the second derivative refinement method.
John Wise

John Wise pushed 2 commits to jwise77/clean-copy

8f44901 - Ensure that the default creation time is slightly before the
3c6352e - The creation time of the source wasn't defined and defaults to zero,
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