This repository contains the data that was presented in the paper by Baron & Ménard (2019; https://arxiv.org/abs/1903.01996). The repository consists of a jupyter notebook that loads the data and explores it. In addition, the repository contains a python code to estimate the black hole mass of type II AGN, using the narrow Halpha, Hbeta, and [OIII] emission line fluxes.
- Dalya Baron (TAU)
- Brice Ménard (JHU)
The jupyter notebook and the code in the repository require the following packages:
- Python 3.7.1
- numpy 1.15.4
- scipy 1.1.0
- matplotlib 3.0.2
- astropy 3.1