Stochastic gravitational wave background reconstruction for a nonequilateral and unequal-noise LISA constellation

We explore the impact of choosing different sets of time-delay interferometry (TDI) variables for detecting and reconstructing stochastic gravitational wave background (SGWB) signals and estimating the instrumental noise in LISA. Most works in the literature build their data analysis pipelines relyi...

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Detalles Bibliográficos
Autores principales: Hartwig, Olaf, Lilley, Marc, Muratore, Martina, Pieroni, Mauro
Lenguaje:eng
Publicado: 2023
Materias:
astro-ph.CO
Astrophysics and Astronomy
gr-qc
General Relativity and Cosmology
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.107.123531
http://cds.cern.ch/record/2855977

Internet

https://dx.doi.org/10.1103/PhysRevD.107.123531
http://cds.cern.ch/record/2855977

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