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Analysis of Gaia measurement timeseries that led to the discovery of the black hole Gaia BH3
A jupyter notebook for fitting the orbit of Gaia BH3 and determining the black hole's mass.
To execute it online, please click on the binder
badge above or navigate to https://mybinder.org/v2/gh/esa/gaia-bhthree/1.0.0?labpath=Gaia_BH3_fit_astrometric_orbit.ipynb
link
Content of this repository
The notebook demonstrates the following steps:
- Load the timeseries data of the Gaia astrometric instrument. The data are identical to the ones published with the paper and available at the CDS (https://cdsarc.cds.unistra.fr/ftp/J/A+A/686/L2/tableb1.dat).
- Fit an orbit to the astrometric data and determine the black hole's mass.
- Load the timeseries data of the Gaia radial-velocity instrument. The data are identical to the ones published with the paper and available at the CDS (https://cdsarc.cds.unistra.fr/ftp/J/A+A/686/L2/tableb2.dat).
- Fit an orbit to the combination of astrometric and radial-velocity data and determine the black hole's mass.
Environment installation
- This notebook is most easily executed within the associated
binder
environment in a web browser, where no software installation is needed.
- For local execution, one can use the environment.yml file included in this repository to create a python environment using conda with the necessary dependencies for code execution:
conda env create --file gaia-bhthree/environment.yml