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2018

The construction and use of LISA sensitivity curves

Robson, Travis, Cornish, Neil, Liu, Chang

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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 Phase-0 reference design parameters.

The construction and use of LISA sensitivity curves · Around

Built on

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Larson S L, Hiscock W A and Hellings R W 2000 Phys. Rev
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Prince T A, Tinto M, Larson S L and Armstrong J W 2002 Phys. Rev
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Rubbo L J, Cornish N J and Poujade O 2004 Phys. Rev. D
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