Cosmic string gravitational wave backgrounds at LISA: II. Reconstruction of conventional signals over astrophysical foregrounds
Androniki Dimitriou, Daniel G. Figueroa, Peera Simakachorn, Isak Stomberg, Bryan Zaldivar
astro-ph.CO, gr-qc, hep-ph
Submitted: 2026-07-16
Comments: 18 pages + 7 figures
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Cosmic string gravitational wave backgrounds at LISA: I. Signal survey, template reconstruction, and model comparison
- Observation of Gravitational Waves from a Binary Black Hole Merger
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
- GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run
- GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
- The population of merging compact binaries inferred using gravitational waves through GWTC-3
- The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background
- The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals
- Search for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array
- Searching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I
- Sensitivity Studies for Third-Generation Gravitational Wave Observatories
- The Science of the Einstein Telescope
- Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
- Cosmic Explorer: The U.S. Contribution to Gravitational-Wave Astronomy beyond LIGO
- Cosmology with the Laser Interferometer Space Antenna
- Observationally driven Galactic double white dwarf population for LISA
- Stochastic gravitational wave background from stellar origin binary black holes in LISA
- Computation of stochastic background from extreme mass ratio inspiral populations for LISA
- The Astrophysical Gravitational Wave Background in the mHz band is likely dominated by White Dwarf binaries
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