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The LISA Response Function

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arxiv gr-qc/0209011 v4 pith:QOJUVTUR submitted 2002-09-03 gr-qc

The LISA Response Function

Neil J. Cornish , Louis J. Rubbo This is my paper
classification gr-qc
keywords gravitationallisaresponsewavefoundfunctioninterferometermodulations
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The orbital motion of the Laser Interferometer Space Antenna (LISA) introduces modulations into the observed gravitational wave signal. These modulations can be used to determine the location and orientation of a gravitational wave source. The complete LISA response to an arbitary gravitational wave is derived using a coordinate free approach in the transverse-traceless gauge. The general response function reduces to that found by Cutler (PRD 57, 7089 1998) for low frequency, monochromatic plane waves. Estimates of the noise in the detector are found to be complicated by the time variation of the interferometer arm lengths.

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Impact of Spacecraft Orbit Uncertainties and Velocity Mismodeling on the LISA Gravitational-Wave Response

    gr-qc 2026-07 unverdicted novelty 6.0

    The work provides the first quantitative characterization of how spacecraft orbit uncertainties and velocity mismodeling propagate into LISA gravitational-wave response mismatches and parameter biases.

  2. Neural posterior estimation of Galactic Binary signals for the LISA mission

    astro-ph.IM 2026-06 unverdicted novelty 6.0

    Conditional normalizing flows perform likelihood-free parameter estimation for single and overlapping LISA galactic binaries, generating thousands of posterior samples per second after training on simulations.

  3. Construction of Sensitivity Curves for Dynamic LISA and Taiji

    gr-qc 2026-06 unverdicted novelty 5.0

    Dynamic LISA/Taiji sensitivity curves exhibit 20% low-frequency variation and 70% directional source-count variation relative to static models, with quadrant patterns at low frequencies.

  4. Global time-frequency search for stellar-mass binary black holes in LISA

    gr-qc 2025-10 unverdicted novelty 5.0

    A time-frequency semi-coherent search pipeline detects stellar-mass BBH inspirals in LISA data down to coherent SNR of approximately 11-14 on the Yorsh data challenge for aligned-spin, low-eccentricity systems.