Possibility of Detection of Exomoons with Inclined Orbits Orbiting Pulsar Planets Using the Time-of-Arrival Analysis

Table 2

TOA produced by hypothetical exomoons orbiting the known pulsar planets.

Pulsar	Planet	𝑀𝐽	𝑎	𝑖	TOA1	TOA2
PSR B1620-26	b	2.5	23 AU	50^∘	7412.42 ns	21987.5 ns
PSR 1719-14	b	1.0	0.0044 AU	50^∘	1.42 ns	4.21 ns
PSR B1257+12	b	7×10^−5	0.19 AU	50^∘	61.23 ns	181.64 ns
PSR B1257+12	c	0.013	0.36 AU	53^∘	120.96 ns	337.94 ns
PSR B1257+12	d	0.012	0.46 AU	47^∘	141.54 ns	419.84 ns