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.
Figure 2 shows the associated SP metric for each analysis
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Angular Resolution of a Bayesian Search for Anisotropic Stochastic Gravitational Wave Backgrounds with LISA
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.