Published May 28, 2026 | Version 1.0
Dataset Open

Dataset corresponding to "On the effective spin-mass ratio relation of binary black hole mergers that evolved in isolation" (arXiv:2411.15112)

  • 1. Rheinische Friedrich-Wilhelms-Universität Bonn Argelander-Institut für Astronomie
  • 2. Helmholtz-Instituts für Strahlen- und Kernphysik, Universität Bonn

Contributors

Project member:

  • 1. ROR icon Max Planck Institute for Astrophysics

Description

The dataset corresponds to the 11 binary-evolution calculations presented in the paper "On the effective spin-mass ratio relation of binary black hole mergers that evolved in isolation" by Sambaran Banerjee and Aleksandra Olejak (arXiv:2411.15112). Each model is run with six different metallicities, so there are 66 folders in total. In each folder, the file 'mergerlist0.dat' contains the list of compact-binary GW mergers for the corresponding metallicity and binary-evolution model. See the Jupyter Notebook inside the parent directory for the details. The dict in the beginning of the notebook serves as a guide to which folder contains which model(s).

 

To obtain the dataset, simply download the tarball and unpack it. The unpacked root folder is 'BSE_share_zenodo', which contains the entire folder hierarchy (~7 GB).

Files

Files (3.3 GB)

Name Size Download all
md5:a529fa84b453645c4cc4ac9647abdd5d
3.3 GB Download

Additional details

Funding

Deutsche Forschungsgemeinschaft
Die Dynamik der stellaren schwarzen Löcher in dichten stellaren Systemen und ihre Rolle bei der Gravitationswellenerzeugung 405620641

Software

Programming language
Python