-ART data enjoys
very preliminary support and is supported by Christopher Moody.
+ART data enjoys preliminary support and is supported by Christopher Moody.
Please contact the ``yt-dev`` mailing list if you are interested in using yt
for ART data, or if you are interested in assisting with development of yt to
+At the moment, the ART octree is 'regridded' at each level to make the native
+octree look more like a mesh-based code. As a result, the initial outlay
+is about ~60 seconds to grid octs onto a mesh. This will be improved in
+``yt-3.0``, where octs will be supported natively.
+To load an ART dataset you can use the ``load`` command provided by
+``yt.mods`` and passing the gas mesh file. It will search for and attempt
+to find the complementary dark matter and stellar particle header and data
+files. However, your simulations may not follow the same naming convention,
+but you can specify the individual files.
+So for example, a single snapshot might have a series of files looking like
+ 10MpcBox_csf512_a0.300.d #Gas mesh
+ PMcrda0.300.DAT #Particle header
+ PMcrs0a0.300.DAT #Particle data (positions,velocities)
+ stars_a0.300.dat #Stellar data (metallicities, ages, etc.)
+The ART frontend tries to find the associated files matching the above, but
+if that fails you can specify ``file_particle_data``,``file_particle_data``,
+``file_star_data`` in addition to the specifying the gas mesh. You also have
+the option of gridding these particles, and assigning them onto the meshes.
+This process is in beta, and for the time being it's best to leave
+``do_grid_particles=False`` as the deault.
+To speed up the loading of an ART file, you have a few options. You can turn
+off the particles entirely by setting ``discover_particles=False``. You can
+also only grid octs up to a certain level, ``limit_level=5``, which is useful
+when debugging by artificially creating a 'smaller' dataset to work with.
+Finally, when stellar ages are computed we 'spread' the ages evenly within a
+smoothing window. By default this is turned on and set to 10Myr. To turn this
+off you can set ``spread=False``, and you can tweak the age smoothing window
+by specifying the window in seconds, ``spread=1.0e7*265*24*3600``.
+ file = "/u/cmoody3/data/art_snapshots/SFG1/10MpcBox_csf512_a0.460.d"
+ pf = load(file,discover_particles=True,grid_particles=2,limit_level=3)
+ print na.sum(dd['particle_type']==0)
+In the above example code, the first line imports the standard yt functions,
+followed by defining the gas mesh file, and load it only through level 3,
+but gridding particles through on to meshes on level 2 and higher. Finally,
+we create a data container and ask it to gather the particle_type array. In
+this case type==0 is for the most highly-refined dark matter particle, and
+we print out how many high-resolution star particles we find in the simulation.
+Typically, however, you shouldn't have to specify any keyword arguments to load