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

Open Access

Table 1

Parameters of telescopes used in simulations.

Telescope	Ø_eff (m)	Bandwidth (MHz)	σ_TOA (µs)
Effelsberg	100	200/400	2.67
Nançay	94	512	2.02
Lovell	76	400	3.66
MeerKAT	108	856	0.84
FAST	300	500	0.12

Notes. Effective diameter of telescopes, observing bandwidth, and TOA uncertainties of PSR J2222–0137 used in the simulations. All information is based on the L-band data from real observations, and is scaled to 15-min integration over the full bandwidth.

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