Reproduction repository for "Diagnosing the interstellar medium of galaxies with far-infrared emission lines III. Physical parameters of observed galaxies"
This repository contains data and code to reproduce the results of the research "Diagnosing the interstellar medium of galaxies with far-infrared emission lines III. Physical parameters of observed galaxies". Each step of the work is described in a step-by-step file with their respective Jupyter notebooks.
The most important software packages to work with the files in this repository are in environment.yml. This file is also used to launch a Binder to open the Jupyter notebooks interactively. We print all the packages in a given notebook using the IPython magic extension watermark. We also use autotpep8 to format the code to the PEP 8 style guide.
The following is the organization of the repository with a simple description of the files or folder contents
.
├── CITATION.cff <- Metadata for citation
├── LICENSE <- License file
├── environment.yml <- File containing the required software
├── README.md <- This file
├── StepByStep.md <- File describing the steps taken in this work
├── data
│ ├── interim <- Intermediate data that has been transformed
│ ├── processed <- Results from DiagISM and final data
│ └── raw <- Original data from Paper II
├── notebooks <- Jupyter notebooks
└── figures <- Figures created from the Jupyter notebooks
The file containing the estimated physical parameters from the observational sample can be found in the predictions_DiagISM_obsSample.csv file.
Unfortunately not all the raw data is available in the repository. Data from the SIDES lightcone catalog is ~2Gb, then we decided not to included in this repository, but if you want to use it you can check the webpage to obtain the catalogue.
Beside this, the mock_sample.csv file is not stored in Github (~100Mb) and need to be stored locally by running the notebook AppA_Predictions_newlinreg.