This is a repository containing the code for figures in the paper with the correpsonding title, also included in the repo. It also contains notebooks with more elaborate examples.
Examples use common, non-astronomical data sets, for the following reasons:
- It makes the examples more general.
- It makes the examples simpler.
- It doesnt't bias towards any sub-field of astronomy, and reduces the chances of "naming and shaming" interpretations of the current paper.
In order to eb able to run all example code it should suffice to create a conda environment using the requirements file in this repo:
$ conda env create -n ds4s -f environment.yml
$ conda activate ds4s
It is all based on Python 3.9.