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Copy file name to clipboardExpand all lines: src/plotting/convenience.jl
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@@ -4230,6 +4230,13 @@ Plot the atomic to molecular gas transition for a set of metallicity ranges.
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- `trans_mode::Union{Symbol,Tuple{TranslationType,RotationType,Dict{Symbol,Vector{String}}}}=:all_box`: How to translate and rotate the cells/particles, before filtering with `filter_mode`. For options see [`selectTransformation`](@ref).
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- `filter_mode::Union{Symbol,Tuple{Function,Dict{Symbol,Vector{String}}}}=:all`: Which cells/particles will be selected. For options see [`selectFilter`](@ref).
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- `theme::Attributes=Theme()`: Plot theme that will take precedence over [`DEFAULT_THEME`](@ref).
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# References
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C. Christensen et al. (2012). *Implementing molecular hydrogen in hydrodynamic simulations of galaxy formation*. Monthly Notices of the Royal Astronomical Society, **425(4)**, 3058–3076. [doi:10.1111/j.1365-2966.2012.21628.x](https://doi.org/10.1111/j.1365-2966.2012.21628.x)
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N. Y. Gnedin et al. (2011). *ENVIRONMENTAL DEPENDENCE OF THE KENNICUTT-SCHMIDT RELATION IN GALAXIES*. The Astrophysical Journal, **728(2)**, 88. [doi:10.1088/0004-637x/728/2/88](https://doi.org/10.1088/0004-637x/728/2/88)
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"""
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functionatomicMolecularTransition(
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simulation_paths::Vector{String},
@@ -4245,15 +4252,17 @@ function atomicMolecularTransition(
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