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

Open Access

Table A.1

Properties of the pre-calculated grids of NSs.

Axis	Type	# of points	Range
α₀	Log	101	[−10⁻¹, −10⁻⁵]
β₀	Lin	21	[−6.0, −5.0]
		51	[−5.0, −4.0]
		281	[−4.0, +10.0]
Pc (dyn/cm²)	Log	21	[10³⁴, 5 × 10³⁴]
		81	[5 × 10³⁴, 5 × 10³⁵]
		21	[5 × 10³⁵, 10³⁶]

Notes. The grids are 3D and depend on {α₀,β₀, p_c}. Each axis of a grid can be divided into several intervals and be either linearly or logarithmically separated.

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