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Welcome to yt!
yt is an analysis and visualization system written in Python, designed for use with Astrophysical Simulation codes. yt can process data in a myraid of ways and make a variety of visualizations. It is designed to be portable across simulation codes, and it is developed by developers from a variety of instutions and backgrounds.
For more information, see the ApJS paper on yt.
Version 2.3
We are proud to announce the release of yt version 2.3, on December 15, 2011. This release includes several new features, bug fixes, and numerous improvements to the code base and documentation. There are a few major additions since yt-2.2 (Released September 1, 2011), including:
- Improved and expanded documentation located at http://yt-project.org/doc/.
- Boolean logic data containers (joins, intersections and nots) to select arbitrary data regions.
- Multi-level parallelism for subgroups of MPI tasks.
- Extensive answer tests.
- Isocontouring and flux-over-surface calculations, with WebGL interface.
- A reorganized field system.
- Adaptive resolution HEALpix-based all-sky volume rendering.
- Radial column density calculations.
- Memory usage, performance enhancements and bug fixes throughout the code.
Destinations
- Documentation (quick start and installation)
- How to cite YT in a paper
- Which astrophysical simulation codes are supported?
- A gallery of visualizations
Communication Channels
- yt-users mailing list (highly recommended!)
- IRC Channel (
#ytonchat.freenode.net) - RSS feed
- commit notification list
- yt-dev mailing list
HELP!
If you're having trouble with installation or usage, we actually have a page in the documentation with suggestions on how to ask for help.
Other Wiki Pages
This revision is from 2012-01-27 18:31