Published April 18, 2021
| Version 0.0.1
Dataset
Open
Dataset from: Gravitational wave sources in our Galactic backyard - Predictions for BHBH, BHNS and NSNS binaries in LISA
Creators
- 1. Center for Astrophysics | Harvard & Smithsonian, Max Planck Institute for Astrophysics (Munich)
- 2. Center for Astrophysics | Harvard & Smithsonian
- 3. Max Planck Institute for Astrophysics (Munich), Anton Pannekoek Institute for Astronomy & Grappa University of Amsterdam, Center for Astrophysics | Harvard & Smithsonian
- 4. Max Planck Institute for Astronomy (Heidelberg)
- 5. Center for Astrophysics | Harvard & Smithsonian, Anton Pannekoek Institute for Astronomy & Grappa University of Amsterdam, Max Planck Institute for Astrophysics (Munich)
- 6. School of Astronomy & Space Science, University of the Chinese Academy of Sciences, Anton Pannekoek Institute for Astronomy & Grappa University of Amsterdam, Max Planck Institute for Astrophysics (Munich)
Description
The data from all simulations used in "Gravitational wave sources in our Galactic backyard: Predictions for BHBH, BHNS and NSNS binaries in LISA"
Contents:
- detections_and_totals.zip
- simulations_4yr.zip
- Contains 60 .h5 files that contain the main simulations for a 4-year LISA mission. Each file contains the results for a single DCO type (BHBH, BHNS or NSNS) and model variation (20 variations) are labeled as {DCO_type}_{variation}_all.h5.
- simulations_10yr.zip
- As simulations_4yr.zip but for a 10-year LISA mission
- simple_mw_simulations.zip
- As simulations_4yr.zip but using a simple model for the Milky Way (discussed in Appendix D) and only for models A and F (hence only contains 6 .h5 files)
For a description of how to use these files to reproduce figures and results see the README.md in the associated GitHub repository: https://github.com/TomWagg/detecting-DCOs-in-LISA
Version 0.0.1 - Changes model E to E' as discussed in paper (now we allow HeHG donors to survive common-envelopes)