The role of distant pulsars in the detectability of continuous gravitational waves

Open Access

Fig. 4.

Corner plot of the CGW parameter posteriors (excluding log₁₀ℳ_c, Φ₀, ψ) created from the joint MCMC chain of 500 realisations of each dataset. The darker contours correspond to the PTA with pulsars at 1 kpc, and the lighter contours correspond to the PTA with pulsars at 4 kpc.

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