In:
Classical and Quantum Gravity, IOP Publishing, Vol. 34, No. 4 ( 2017-02-23), p. 044001-
Abstract:
The second-generation of gravitational-wave detectors are just starting
operation, and have already yielding their first detections. Research is now concentrated on how to maximize the scientific potential of gravitational-wave
astronomy. To support this eff ort, we present here design targets for a new
generation of detectors, which will be capable of observing compact binary sources with high signal-to-noise ratio throughout the Universe.
Type of Medium:
Online Resource
ISSN:
0264-9381
,
1361-6382
DOI:
10.1088/1361-6382/aa51f4
Language:
Unknown
Publisher:
IOP Publishing
Publication Date:
2017
detail.hit.zdb_id:
1473117-4
SSG:
16,12
Permalink
