A new pulsar timing model for scalar-tensor gravity with applications to PSR J2222-0137 and pulsar-black hole binaries

Open Access

Fig. D.1

Mass-mass diagram in DEF gravity corresponding to a point near the ‘horn’ with α₀ = −10⁻¹, β₀ = −1.9. The performed test is the same as for Fig. 1. The shadowed area is the allowed region at 68% CL limit for a corresponding PK parameter. The solid green line corresponds to the observed value of ${\dot{P}}_{b}^{G W}$ $\dot P_{\rm{b}}^{GW}$ .

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