Relativistic effects in ultra-large-scale galaxy clustering
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Updated
Aug 15, 2023 - Python
Relativistic effects in ultra-large-scale galaxy clustering
Main tools and results from arxiv:
The codes for computing the scale-dependent peak height function and the scale-dependent valley depth function of the cosmic-log density field.
Various codes centered around problems in Bayesian inference, Bayesian Linear Regression, and Bayesian Non-Linear Parameter Estimation using the application of various Markov Chain Monte Carlo Algorithms
The Effects of Galaxy Assembly Bias on the Inference of Growth Rate from Redshift-Space Distortions (2019MNRAS.487.2424M)
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