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

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Table B.1

EOSs selected for the calculation of grids of NSs.

Name	M_max (M_⊙)	R_1,4 (km)	Name	M_max (M_⊙)	R_1,4 (km)
SLy	2.049	11.736	APR3	2.390	12.094
APR4	2.213	11.428	WFF1	2.133	10.414
WFF2	2.198	11.159	ENG	2.240	12.059
MPA1	2.461	12.473	MS1	2.767	14.918
MS1b	2.776	14.583	H4	2.032	13.759
ALF2	2.086	13.188

Notes. All EOSs have the maximum mass of a NS in $M_{NS, \max}^{GR} > 2 M_{⊙}$ $M_{{\rm{NS}},\max }^{{\rm{GR}}} > 2{M_ \odot }$ and taken in piece-wise polytropic approximation from Read et al. (2009). R_1,4 is the radius of a 1.4 M_⊙ NS.

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