Cargando…
Deep learning merger masses estimation from gravitational waves signals in the frequency domain
Detection of gravitational waves (GW) from compact binary mergers provide a new window into multi-messenger astrophysics. The standard technique to determine the merger parameters is matched filtering, consisting in comparing the signal to a template bank. This approach can be time consuming and com...
Autores principales: | Marulanda, Juan Pablo, Santa, Camilo, Romano, Antonio Enea |
---|---|
Lenguaje: | eng |
Publicado: |
2020
|
Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/j.physletb.2020.135790 http://cds.cern.ch/record/2715500 |
Ejemplares similares
-
Black hole mergers, gravitational waves and scaling relations
por: Arbey, Alexandre, et al.
Publicado: (2019) -
Constraining gravity theories with the gravitational stability mass
por: Santa Vélez, Camilo, et al.
Publicado: (2019) -
Mirage of Luminal Modified Gravitational-Wave Propagation
por: Romano, Antonio Enea, et al.
Publicado: (2023) -
Unveiling the gravitational universe at $\mu$-Hz frequencies
por: Sesana, Alberto, et al.
Publicado: (2019) -
Constraining the time evolution of the propagation speed of gravitational waves with multimessenger astronomy
por: Romano, Antonio Enea, et al.
Publicado: (2023)