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content/50.halo_finding_and_catalogs.md

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Furthermore, convergence studies and cross-simulation comparisons requires a consistent method for identifying dark matter halos, as well as the ability to track their growth over time.
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In past versions of `yt`, several specific halo finders were bundled and made available to work on any class of data `yt` was able to read.
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These included the HOP halo finder, the classic Friends-of-Friends (FOF) halo finder **CITE**, a scalable and Parallel HOP **CITE**, and a wrapping of the ORIGAMI **CITE** code for filament identification.
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These included the HOP halo finder, the classic Friends-of-Friends (FOF) halo finder [@doi:10.1086/191003], a scalable and Parallel HOP [@doi: 10.1086/305535], and a wrapping of the ORIGAMI code [@doi:10.1142/9789814623995_0378] for filament identification.
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To do so, `yt` would utilize direct in-memory connectors with these implementations; whereas typically data connectors are written for each individual dataset format for individual halo finding methods, this enabled a single connector to be written from `yt` to the halo finder.
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In addition to these bundled halo finders, a direct in-memory interface with Rockstar **CITE** was developed that sidestepped Rockstar's built in load-balancing to minimize data duplication and transfer.
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In addition to these bundled halo finders, a direct in-memory interface with Rockstar [@doi:10.1088/0004-637X/762/2/109] was developed that sidestepped Rockstar's built in load-balancing to minimize data duplication and transfer.
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`yt` provides a unique set of functionality for accessing halo catalogs, as it provides the ability to query their values both *as* catalogs and as the original, underlying datasets.
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This means that the same selection and analysis operations that can be conducted on a "primary" dataset can also be conducted on the halo catalog; furthermore, the halo catalog can be used as input to data selection operations.
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This enables, for instance, querying original dark matter particle values in a halo (as defined by any characteristic radius of that halo) simultaneously with querying baryonic cells or particles included within.
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As discussed in **CITE YTREE**, this can be used as input into other tools to provide sophisticated, graph-based queries of datasets and halo merger trees over cosmological time.
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As discussed in [@doi:10.5281/zenodo.8349044], this can be used as input into other tools to provide sophisticated, graph-based queries of datasets and halo merger trees over cosmological time, such as with the `ytree` package.
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`yt` also includes an internal halo finding tool that is not widely exposed, built on its implementation of a union-find data structure for identifying topologically connected sets.
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This implementation, a "particle contour tree," uses this union-find data structure to connect (via percolation) particles into simple Friends-of-Friends collections.
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These can then be used as input into more sophisticated phase-space finders, such as Rockstar, and as done in **CITE DARK SKY**.
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These can then be used as input into more sophisticated phase-space finders, such as Rockstar, and as done in [@doi:10.48550/arXiv.1407.2600].
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content/60.analysis_modules.md

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For much of its development history, `yt` took the approach of bundling as many analysis modules as possible in the primary repository.
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This provided the advantage of having all work be centralized, and ensuring that each download or installation of `yt` was a fully-featured system for analyzing a large swath of data, but it brought with it the development overhead of the entire `yt` package for what in many cases were isolated pieces of functionality with separable responsibilities.
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As a result of the slowing in speed of development as a result of review requirements (and limited personnel to conduct those reviews), some of the analysis modules that were bundled with `yt` have been "spun out" into their own repository, `yt_astro_analysis`.
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This repository, which is developed, released and installed separately from `yt`, includes modules for cosmological observation (upon which Triden, which is discussed in @sec:trident, is based), dark matter halo finding and analysis, tools for interacting with position-position-velocity cubes, and a system for exporting from `yt` to RADMC-3D [@ascl:1202.015].
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As a result of the slowing in speed of development as a result of review requirements (and limited personnel to conduct those reviews), some of the analysis modules that were bundled with `yt` have been "spun out" into their own repository, `yt_astro_analysis` [@doi:10.5281/zenodo.8431185].
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This repository, which is developed, released and installed separately from `yt`, includes modules for cosmological observation (upon which Triden, which is discussed in @sec:trident, is based), dark matter halo finding and analysis, tools for interacting with position-position-velocity cubes, light cone generation [@doi:10.1088/0004-637X/698/2/1795] and a system for exporting from `yt` to RADMC-3D [@ascl:1202.015].

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