Multiband Gravitational-Wave Astronomy: Parameter Estimation and Tests of General Relativity with Space- and Ground-Based Detectors
With the discovery of the binary-black-hole (BBH) coalescence GW150914 the era of gravitational-wave (GW) astronomy has started. It has recently been shown that BBH with masses comparable to or higher than GW150914 would be visible in the Evolved Laser Interferometer Space Antenna (eLISA) band a few...
Main Author: | Vitale, Salvatore (Contributor) |
---|---|
Other Authors: | LIGO (Observatory : Massachusetts Institute of Technology) (Contributor) |
Format: | Article |
Language: | English |
Published: |
American Physical Society,
2017-07-06T17:55:25Z.
|
Subjects: | |
Online Access: | Get fulltext |
Similar Items
-
Gravitational wave astronomy using spaceborne detectors
by: Rubbo, Louis Joseph
Published: (2004) -
Parameter estimation for binary black holes with networks of third-generation gravitational-wave detectors
by: Vitale, Salvatore, et al.
Published: (2017) -
Sensitivity of the Advanced LIGO detectors at the beginning of gravitational wave astronomy
by: Martynov, D. V, et al.
Published: (2017) -
OBSERVATIONAL SELECTION EFFECTS WITH GROUND-BASED GRAVITATIONAL WAVE DETECTORS
by: Chen, Hsin-Yu, et al.
Published: (2017) -
Gravitational-Wave Tests of General Relativity with Ground-Based Detectors and Pulsar-Timing Arrays
by: Nicolás Yunes, et al.
Published: (2013-11-01)