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frontends.yaml
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frontends:
- citations: []
comments: Halo finding format
index_type:
- particle
name: adaptahop
usage_citations: []
- citations: []
comments: Halo finding format
index_type:
- particle
name: ahf
usage_citations: []
- citations:
- '@amrvac-paper'
- '@doi:10.1088/0067-0049/214/1/4'
- '@doi:10.3847/1538-4365/aaa6c8'
comments: 'MPI-AMRVAC is a parallel adaptive mesh refinement framework aimed at
solving (primarily hyperbolic) partial differential equations by a number of different
numerical schemes.
The emphasis is on (near) conservation laws and on shock-dominated problems in
particular.
'
index_type:
- grid
name: amrvac
usage_citations:
- '@doi:10.1051/0004-6361/202037616'
- '@doi:10.1051/0004-6361/202039630'
- '@doi:10.1051/0004-6361/201937414'
- citations: []
comments: 'While listed as a "particle" dataset, AREPO data is properly described
as a moving mesh.
For visualization purposes, yt treats it similarly to an SPH dataset; some efforts
have been made to properly apply nearest-neighbor interpolation, but these have
not been mainlined in the yt visualization routines as of yet.
'
index_type:
- particle
name: arepo
usage_citations:
- '@doi:10.3847/1538-4357/aa6dff'
- '@doi:10.1093/mnras/stab2553'
- citations: []
comments: 'ART, or ''NMSU-ART'' as it is occasionally referred to internally, is
an octree-based code that is often used for cosmology simulations and galaxy formation
simulations.
yt supports two sets of data formats in the NMSU-ART family.
The first is a particle-only format, where the particles are stored independently
of any gas structure.
The second is the hydro data format, wherein gas values are stored organized into
an octree.
Each of these constitutes a different indexing system, sharing similar datatypes,
units, and so forth.
'
index_type:
- octree
- particle
name: art
usage_citations:
- '@doi:10.3847/1538-4357/aa6dff'
- '@doi:10.1093/mnras/staa3972'
- citations: []
comments: 'The ARTIO frontend, which shares some ancestry with the `art` or ''NMSU-ART''
frontend, utilizes a special purpose library for input/output operations called
`libartio`, which is bundled with yt.
Utilizing `libartio` is interesting from a historical perspective, as it provided
an opportunity to reorganize the way that yt understood indexing of octree datasets.
Whereas previously yt required a full understanding of data distribution, the
`artio` frontend outsourced much of that to the internal library, which it regarded
as essentially an opaque API.
Reducing the amount of internal bookkeepping that yt had to do provided a lighter-weight
interface to the data, which in turn has enabled other frontends to be created
using opaque APIs.
'
index_type:
- octree
name: artio
usage_citations:
- '@doi:10.1093/mnras/stac1164'
- citations: []
comments: null
index_type:
- grid
name: athena
usage_citations:
- '@doi:10.3847/1538-4357/aa9b80'
- citations: []
comments: null
index_type:
- grid
name: athena_pp
usage_citations:
- '@doi:10.3847/2041-8213/abbffd'
- citations:
- '@doi:10.21105/joss.01370'
- '@doi:10.1088/1742-6596/1031/1/012024'
- '@doi:10.21105/joss.02513'
- '@doi:10.21105/joss.01757'
comments: 'BoxLib is the predecessor to the AMReX adaptive mesh refinement library [@doi:10.21105/joss.01370] and supports all BoxLib and AMReX codes that use the native BoxLib binary output. AMReX implements patch-based AMR following Berger and Colella [@berger-collela-paper] with typical refinement jumps of 2 or 4 between levels (this factor can vary in the level hierarchy).'
index_type:
- grid
name: boxlib
usage_citations:
- '@doi:10.1093/mnras/stac439'
- '@doi:10.1007/s00162-020-00548-6'
- '@doi:10.1103/PhysRevD.100.063528'
- '@doi:10.1103/PhysRevD.103.063525'
- '@doi:10.1103/PhysRevD.105.023516'
- '@doi:10.1016/j.cpc.2022.108457'
- citations:
- '@doi:10.1088/0067-0049/217/2/24'
comments: 'CHOLLA is a uniform-resolution grid code operating almost entirely on GPUs.'
index_type:
- grid
name: cholla
usage_citations: []
- citations: []
comments: null
index_type:
- grid
name: chombo
usage_citations:
- '@doi:10.3847/1538-3881/ab9abf'
- '@doi:10.3847/1538-4357/ab54c6'
- '@doi:10.1093/mnras/stw2153'
- citations: []
comments: null
index_type:
- particle
name: eagle
usage_citations:
- '@doi:10.1093/mnras/stab1057'
- '@doi:10.1093/mnras/stab651'
- '@doi:10.1093/mnras/staa3590'
- '@doi:10.1093/mnras/stab1057'
- citations:
- '@doi:10.1088/0067-0049/211/2/19'
comments: 'Enzo was the very first code supported by yt, and while many remnants
of that have been removed, many still remain.
During the development of yt 3.0 in particular, many "enzo-isms" were removed;
however, as Enzo uses a patch-based grid data format, much of the naming conventions
for grid objects still mirror those in use in Enzo.
These include names such as `GridLeftEdge` and `ActiveDimensions` (which refers
to the dimensions not including ghost zones).
There are several ''sub-frontends'' within the Enzo frontend; these include dedicated
1D and 2D readers, as well as historical frontends (of varying functionality)
for reading HDF4, ''unpacked'' HDF5 and other sub-dialects of Enzo.
'
index_type:
- grid
name: enzo
usage_citations:
- '@doi:10.3847/1538-4357/aa6dff'
- '@doi:10.1088/0004-637X/764/2/136'
- '@doi:10.3847/1538-4365/abfa17'
- '@doi:10.3847/1538-4357/ac6c87'
- '@doi:10.1093/mnras/stu979'
- '@doi:10.3847/1538-4357/ac5960'
- citations: []
comments: 'Enzo-E is a nearly full-rewrite of the Enzo infrastructure designed for
emerging and future architectures.
'
index_type:
- grid
name: enzo_e
usage_citations:
- '@doi:10.3847/1538-4357/ac3c48'
- citations: []
comments: 'Exodus II, and its output in NetCDF4 format, was the initial driver for
higher-order unstructured mesh support in yt.
The original driver for developing this format was for simulations of nuclear
reactors.
'
index_type:
- unstructured mesh
name: exodus_ii
usage_citations: []
- citations: []
comments: null
index_type:
- grid
name: fits
usage_citations: []
- citations: []
comments: 'FLASH is a block-refinement adaptive mesh refinement code used in
many different fields, including astrophysics and high-energy density
physics.
'
index_type:
- grid
name: flash
usage_citations:
- '@doi:10.1093/mnras/stac1275'
- '@doi:10.3847/1538-4357/aadcf7'
- '@doi:10.1093/mnras/staa3902'
- '@doi:10.3847/1538-4357/ab4db1'
- '@doi:10.3847/1538-4357/abc011'
- '@doi:10.3847/2041-8213/ababae'
- citations: []
comments: null
index_type:
- particle
name: gadget
usage_citations:
- '@doi:10.3847/1538-4357/ac088a'
- citations: []
comments: Halo finding
index_type:
- particle
name: gadget_fof
usage_citations: []
- citations:
- '@doi:10.1093/mnras/sty2586'
comments: null
index_type:
- grid
name: gamer
usage_citations: []
- citations: []
comments: Custom built for yt
index_type:
- grid
name: gdf
usage_citations: []
- citations: []
comments: null
index_type:
- particle
name: gizmo
usage_citations:
- '@doi:10.1093/mnras/stac1542'
- '@doi:10.3847/1538-4357/aa6dff'
- citations: []
comments: null
index_type:
- particle
name: halo_catalog
usage_citations: []
- citations: []
comments: null
index_type:
- particle
name: http_stream
usage_citations: []
- citations: []
comments: null
index_type:
- unstructured mesh
name: moab
usage_citations: []
- citations: []
comments: null
index_type:
- grid
name: nc4_cm1
usage_citations: []
- citations: []
comments: null
index_type:
- particle
name: open_pmd
usage_citations: []
- citations: []
comments: null
index_type:
- particle
name: owls
usage_citations: []
- citations: []
comments: null
index_type:
- particle
name: owls_subfind
usage_citations: []
- citations: []
comments: null
index_type:
- octree
name: ramses
usage_citations:
- '@doi:10.1051/0004-6361/202243170'
- '@doi:10.1051/0004-6361/202037698'
- '@doi:10.1051/0004-6361/201936188'
- '@doi:10.1051/0004-6361/201935504'
- '@doi:10.1093/mnras/sty2859'
- '@doi:10.1093/mnras/sty024'
- '@doi:10.3847/1538-4357/aa989a'
- '@doi:10.1093/mnras/stx1706'
- '@doi:10.3847/1538-4357/833/2/202'
- '@doi:10.3847/0004-637X/826/1/22'
- '@doi:10.1088/0004-637X/807/1/67'
- '@doi:10.1088/0067-0049/210/1/14'
- '@doi:10.1093/mnras/stt1789'
- '@doi:10.1088/0004-637X/765/1/39'
- '@doi:10.3847/1538-4357/aa6dff'
- '@doi:10.48550/arXiv.2206.11913'
- '@doi:10.1051/0004-6361/201834496'
- '@doi:10.1093/mnras/stac1663'
- '@doi:10.1051/0004-6361/201936188'
- '@doi:10.1093/mnras/stac2963'
- '@doi:10.1093/mnras/stx2316'
- '@doi:10.1093/mnras/stac2963'
- citations: []
comments: null
index_type:
- particle
name: rockstar
usage_citations: []
- citations: []
comments: null
index_type:
- particle
name: sdf
usage_citations:
- '@doi:10.1051/0004-6361/201937337'
- citations: []
comments: 'A base frontend from which other SPH-type frontends can be defined.'
index_type:
- particle
name: sph
usage_citations: []
- citations: []
comments: null
index_type:
- multi
name: stream
usage_citations:
- '@doi:10.1002/ESSOAR.10506118.2'
- '@doi:10.3847/1538-4357/ab290c'
- citations:
- '@doi:10.21105/joss.02430'
comments: null
index_type:
- particle
name: swift
usage_citations:
- '@doi:10.3847/1538-4357/ac20d4'
- '@doi:10.48550/arXiv.2203.13915'
- citations: []
comments: null
index_type:
- particle
name: tipsy
usage_citations:
- '@doi:10.1016/j.ascom.2016.02.002'
- '@doi:10.1093/mnras/stw1741'
- citations: []
comments: 'An internal frontend for re-loading saved data and derived data'
index_type:
- particle
name: ytdata
usage_citations:
- '@doi:10.1093/mnras/sty2103'
- citations:
- '@doi:10.1177/10943420221143775'
comments: 'Parthenon is a performance portable block-structured adaptive mesh
refinement framework and the basis for various downstream codes such as
AthenaPK, Phoebus, or KHARMA.
'
index_type:
- grid
name: parthenon
usage_citations: []