Gravitational-wave sensitivity curves

C. J. Moore, R. H. Cole, Christopher Philip Luke Berry

Research output: Contribution to journalArticlepeer-review

227 Scopus citations

Abstract

There are several common conventions in use by the gravitational-wave community to describe the amplitude of sources and the sensitivity of detectors. These are frequently confused. We outline the merits of and differences between the various quantities used for parameterizing noise curves and characterizing gravitational-wave amplitudes. We conclude by producing plots that consistently compare different detectors. Similar figures can be generated on-line for general use at http://rhcole.com/apps/GWplotter.

Original languageEnglish (US)
Article number015014
JournalClassical and Quantum Gravity
Volume32
Issue number1
DOIs
StatePublished - Jan 8 2015

Keywords

  • black holes
  • gravitational waves
  • pulsar timing
  • pulsar timing arrays

ASJC Scopus subject areas

  • Physics and Astronomy (miscellaneous)

Fingerprint Dive into the research topics of 'Gravitational-wave sensitivity curves'. Together they form a unique fingerprint.

Cite this