Note that the data point for ℓa max = 10 at ∆ϕ = 4π/5 is marked with a †; analysis of the original simulation recovered a significant bimodal- ity in the two-point metric

Dependence on ℓa max Consistent with the results in §III A, the choice of a higher ℓa max increases LISA’s ability to resolve two AS- GWB sources as measured by the TP metric, with

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Angular Resolution of a Bayesian Search for Anisotropic Stochastic Gravitational Wave Backgrounds with LISA

gr-qc · 2024-12-20 · conditional · novelty 6.0

For loud anisotropic gravitational wave backgrounds in LISA, Bayesian spherical harmonic searches reach their best angular resolution at ℓmax=16, limited by computation rather than by signal properties.

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Angular Resolution of a Bayesian Search for Anisotropic Stochastic Gravitational Wave Backgrounds with LISA gr-qc · 2024-12-20 · conditional · none · ref 3
For loud anisotropic gravitational wave backgrounds in LISA, Bayesian spherical harmonic searches reach their best angular resolution at ℓmax=16, limited by computation rather than by signal properties.

Note that the data point for ℓa max = 10 at ∆ϕ = 4π/5 is marked with a †; analysis of the original simulation recovered a significant bimodal- ity in the two-point metric

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