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Fig. 7.

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Mass-mass diagram for PSR J1946+2052. The regions consistent with the measured P ˙ b , ω ˙ , γ , h 3 , ς $ \dot{P}_{\mathrm{b}},\ \dot{\omega},\ \gamma,\ h_3,\ \varsigma $, and their 1-σ uncertainties are displayed in red, green, blue, purple, and orange. Note that b in this diagram has been corrected by removing the external contributions. The grey area is excluded by the mass function and sin i ≤ 1. The inset is an expanded view, showing in more detail the intersection of all PK parameters and the self-consistency of GR. The ω ˙ $ \dot\omega $-line is based on the leading-order Equation (4). The (small) modifications related to the next-to-leading order contributions to the periastron advance are discussed in detail in Sect. 4.4.

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