Effect of data gaps on the detectability and parameter estimation of massive black hole binaries with LISA
Kallol Dey, Nikolaos Karnesis, Alexandre Toubiana, Enrico Barausse,, Natalia Korsakova, Quentin Baghi, Soumen Basak

TL;DR
This study evaluates how data gaps in LISA's observations affect the detection and parameter estimation of massive black hole binaries, finding scheduled gaps are mostly negligible while unscheduled gaps can be more impactful.
Contribution
It provides a comprehensive analysis of the impact of both scheduled and unscheduled data gaps on LISA's ability to detect and characterize massive black hole binaries.
Findings
Scheduled gaps have negligible impact unless they coincide with coalescence.
Unscheduled gaps are likely to have a more significant effect on detection and parameter estimation.
Data gaps generally do not severely hinder the detection of long-lived black hole binary signals.
Abstract
Massive black hole binaries are expected to provide the strongest gravitational wave signals for the Laser Interferometer Space Antenna (LISA), a space mission targeting mHz frequencies. As a result of the technological challenges inherent in the mission's design, implementation and long duration (4 yr nominal), the LISA data stream is expected to be affected by relatively long gaps where no data is collected (either because of hardware failures, or because of scheduled maintenance operations, such as re-pointing of the antennas toward the Earth). Depending on their mass, massive black hole binary signals may range from quasi-transient to very long lived, and it is unclear how data gaps will impact detection and parameter estimation of these sources. Here, we will explore this question by using state-of-the-art astrophysical models for the population of massive black hole…
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