Amanote Research

Amanote Research

    RegisterSign In

LISA Observations of Supermassive Black Holes: Parameter Estimation Using Full Post-Newtonian Inspiral Waveforms

Physical Review D
doi 10.1103/physrevd.77.024030
Full Text
Open PDF
Abstract

Available in full text

Date

January 17, 2008

Authors
Miquel TriasAlicia M. Sintes
Publisher

American Physical Society (APS)


Related search

Parameter Estimation for Coalescing Massive Binary Black Holes With LISA Using the Full 2-Post-Newtonian Gravitational Waveform and Spin-Orbit Precession

Physical Review D
2009English

Post-Newtonian Dynamical Modeling of Supermassive Black Holes in Galactic-Scale Simulations

Astrophysical Journal
AstrophysicsAstronomyPlanetary ScienceSpace
2017English

Observational Evidence for Supermassive Black Holes

Symposium - International Astronomical Union
1989English

Supermassive Black Holes Then and Now

1998English

Disks Around Merging Binary Black Holes: From GW150914 to Supermassive Black Holes

Physical Review D
AstronomyPhysics
2018English

Formation of the First Supermassive Black Holes

English

Using Electromagnetic Observations to Aid Gravitational-Wave Parameter Estimation of Compact Binaries Observed With LISA

Astronomy and Astrophysics
AstrophysicsAstronomyPlanetary ScienceSpace
2012English

Gravitational Wave Background From Supermassive Black Holes

2011English

Searching for Low-Mass Supermassive Black Holes

Symposium - International Astronomical Union
1999English

Amanote Research

Note-taking for researchers

Follow Amanote

© 2025 Amaplex Software S.P.R.L. All rights reserved.

Privacy PolicyRefund Policy