Gravitational-wave parameter estimation with gaps in LISA: a Bayesian data augmentation method

10 Jul 2019Quentin BaghiIra ThorpeJacob SlutskyJohn BakerTito Dal CantonNatalia KorsakovaNikos Karnesis

By listening to gravity in the low frequency band, between 0.1 mHz and 1 Hz, the future space-based gravitational-wave observatory LISA will be able to detect tens of thousands of astrophysical sources from cosmic dawn to the present. The detection and characterization of all resolvable sources is a challenge in itself, but LISA data analysis will be further complicated by interruptions occurring in the interferometric measurements... (read more)

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