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DEV: Add gas properties to galaxy clusters / haloes #139
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Ideas
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Some references regarding intrinsic covariance of cluster properties (both theory and observations) |
design flow-through links to this question: #147 (comment) We might start with this issue and one on optical properties to decide which halo properties we need? |
Issue deprecated by more specific examples. Please see Discussion pages for general discussion of which gas components and models to implement. |
Description
We'll create a list of cluster gas properties -- intrinsic and observable --- based on halo properties.
Inputs
Outputs
References
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