Bayesian sensitivity of binary pulsars to ultra-light dark matter

Open Access

Fig. 1.

Description of Keplerian orbits in terms of the orbital elements viewed in the fundamental reference frame (X,Y,Z). The Cartesian orbital frame (x,y,z) and the polar one $(r, θ, z)$ $(r, \theta , z)$ are also shown (centred on M₂ for convenience)

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