From fe6e54a4ecdc335179f69e0c53740a70b4def8ff Mon Sep 17 00:00:00 2001 From: Phil Bull Date: Sun, 30 Jun 2024 21:27:13 +0100 Subject: [PATCH] Make useful links appear earlier in readme --- README.md | 14 +++++++------- 1 file changed, 7 insertions(+), 7 deletions(-) diff --git a/README.md b/README.md index cdb63bc..8a2e594 100644 --- a/README.md +++ b/README.md @@ -14,6 +14,13 @@ Hydra uses a technique called **Gibbs sampling** to efficiently draw samples fro distribution of *all* the parameters. It is implemented in Python and is compatible with the data formats used by the HERA pipeline, such as _UVData_ and _UVBeam_. +## Learn about the code and different 'heads' of Hydra + +* See the [API documentation](https://hydraradio.github.io/Hydra/api/) +* Run the example script, [example.py](https://hydraradio.github.io/Hydra/example.html) +* Read the [frequently-asked questions](https://hydraradio.github.io/Hydra/faq.html) about the code and maths +* Learn about the different ["heads"](https://hydraradio.github.io/Hydra/heads.html) (conditional distribution samplers) of Hydra. + ## What is Gibbs sampling? Gibbs sampling is a way of breaking up the joint posterior distribution for a set of parameters into a @@ -71,13 +78,6 @@ At present, Hydra is parallelised in a basic way, meaning that it can only run o a single HPC node). There are plans to make a distributed version that can scale to much larger problem sizes, but for now the main limitation is the amount of RAM available on each node. -## Learn about the code and different 'heads' of Hydra - -* See the [API documentation](https://hydraradio.github.io/Hydra/api/) -* Run the example script, [example.py](https://hydraradio.github.io/Hydra/example.html) -* Read the [frequently-asked questions](https://hydraradio.github.io/Hydra/faq.html) about the code and maths -* Learn about the different ["heads"](https://hydraradio.github.io/Hydra/heads.html) (conditional distribution samplers) of Hydra. - ## Who is behind Hydra? Hydra is a project based out of Phil Bull's research group at the Jodrell Bank Centre for Astrophysics