The construction and use of LISA sensitivity curves

The Laser Interferometer Space Antenna (LISA) will open the mHz band of the gravitational wave spectrum for exploration. Sensitivity curves are a useful tool for surveying the types of sources that can be detected by the LISA mission. Here we describe how the sensitivity curve is constructed, and ho...

Full description

Saved in:
Bibliographic Details
Published inClassical and quantum gravity Vol. 36; no. 10; pp. 105011 - 105026
Main Authors Robson, Travis, Cornish, Neil J, Liu, Chang
Format Journal Article
LanguageEnglish
Published IOP Publishing 23.05.2019
Subjects
data analysis
gravitational waves
LISA
Online AccessGet full text

Cover

More Information
Summary:The Laser Interferometer Space Antenna (LISA) will open the mHz band of the gravitational wave spectrum for exploration. Sensitivity curves are a useful tool for surveying the types of sources that can be detected by the LISA mission. Here we describe how the sensitivity curve is constructed, and how it can be used to compute the signal-to-noise ratio for a wide range of binary systems. We adopt the 2018 LISA mission performance requirement design parameters. We consider both sky-averaged sensitivities, and the sensitivity to sources at particular sky locations. The calculations are included in a publicly available Python notebook.
Bibliography:CQG-105360.R1
ISSN:0264-9381
1361-6382
DOI:10.1088/1361-6382/ab1101