Data release for "Discovering neutron stars with LISA via measurements of orbital eccentricity in Galactic binaries"
Authors/Creators
- 1. University of Birmingham
- 2. California Institute of Technology
- 3. Max Planck Institute for Astrophysics
Description
Posterior samples and code to reproduce all figures associated with Discovering neutron stars with LISA via measurements of orbital eccentricity in Galactic binaries.
The parameter_estimation folder contains the following:
campaigns: Analyses of eccentric quasi-monochromatic binaries, gridding over gravitational-wave frequency, eccentricty, and SNR. See theREADMEinside for more information. The resulting posteriors are used in Figure 3, and the fitting formula Eq. 20.fiducial_source_checks: Analyses that vary parameters other than SNR and frequency to investigate the effect on the minimum eccentricity that can be recovered. Used in Figure A1. Posteriors used for Figure 4 are also found in thegolden_binaryfolder.nhat_runs: Various analyses used for Figures 5, 6, B1, and C1. See theREADMEinside for more information. Also see theREADMEineccentric_gb_scriptsand links therein.
The notebooks folder contains code to produce Figures 2, 3, 4, 6, and A1. Also included are notebooks to produce the fitting formula Eq. 20 (emin_grid.ipynb), and to inspect analyses in the campaigns and fiducial_source_checks folders.
The eccentric_gb_scripts folder contains code to produce Figures 1, 5, B1 and C1. See the README inside for more information.