Author pages are created from data sourced from our academic publisher partnerships and public sources.
- Publications
- Influence
Share This Author
Laser Interferometer Space Antenna
- P. Amaro-Seoane, H. Audley, +81 authors P. Zweifel
- Physics
- 13 April 2012
Following the selection of The Gravitational Universe by ESA, and the successful flight of LISA Pathfinder, the LISA Consortium now proposes a 4 year mission in response to ESA's call for missions… Expand
Stellar Remnants in Galactic Nuclei: Mass Segregation
- M. Freitag, P. Amaro-Seoane, V. Kalogera
- Physics
- 11 March 2006
The study of how stars distribute themselves around a massive black hole (MBH) in the center of a galaxy is an important prerequisite for the understanding of many galactic-center processes. These… Expand
Surface brightness profile of the Milky Way’s nuclear star cluster
- R. Schodel, A. Feldmeier, +4 authors S. Nishiyama
- Physics
- 26 March 2014
Context. Although the Milky Way nuclear star cluster (MWNSC) was discovered more than four decades ago, several of its key properties have not been determined unambiguously up to now because of the… Expand
The PLATO 2.0 mission
PLATO 2.0 has recently been selected for ESA’s M3 launch opportunity (2022/24). Providing accurate key planet parameters (radius, mass, density and age) in statistical numbers, it addresses… Expand
Low-frequency gravitational-wave science with eLISA/NGO
- P. Amaro-Seoane, S. Aoudia, +27 authors H. Ward
- Physics
- 3 February 2012
We review the expected science performance of the New Gravitational-Wave Observatory (NGO, a.k.a. eLISA), a mission under study by the European Space Agency for launch in the early 2020s. eLISA will… Expand
Post-Newtonian Dynamics in Dense Star Clusters: Highly Eccentric, Highly Spinning, and Repeated Binary Black Hole Mergers.
- C. Rodríguez, P. Amaro-Seoane, S. Chatterjee, F. Rasio
- Physics, Medicine
- Physical review letters
- 10 April 2018
We present models of realistic globular clusters with post-Newtonian dynamics for black holes. By modeling the relativistic accelerations and gravitational-wave emission in isolated binaries and… Expand
Sensitivity studies for third-generation gravitational wave observatories
- S. Hild, M. Abernathy, +136 authors K. Yamamoto
- Physics
- 4 December 2010
Advanced gravitational wave detectors, currently under construction, are expected to directly observe gravitational wave signals of astrophysical origin. The Einstein Telescope (ET), a… Expand
The distribution of stars around the Milky Way's central black hole II: Diffuse light from sub-giants and dwarfs
- R. Schodel, E. Gallego-Cano, +4 authors H. Baumgardt
- Physics
- 13 January 2017
This is the second of three papers that search for the predicted stellar cusp around the Milky Way's central black hole, Sagittarius A*, with new data and methods. We aim to infer the distribution of… Expand
Doing Science with eLISA: Astrophysics and Cosmology in the Millihertz Regime
- P. Amaro-Seoane, S. Aoudia, +27 authors H. Ward
- Physics
- 17 January 2012
This document introduces the exciting and fundamentally new science and astronomy that the European New Gravitational Wave Observatory (NGO) mission (derived from the previous LISA proposal) will… Expand
Scientific objectives of Einstein Telescope
- B. Sathyaprakash, M. Abernathy, +222 authors K. Yamamoto
- Physics
- 2 June 2012
The advanced interferometer network will herald a new era in observational astronomy. There is a very strong science case to go beyond the advanced detector network and build detectors that operate… Expand
...
1
2
3
4
5
...