PIMMS: Pulsation-Informed Magnetic Mapping of Stars with Zeeman-Doppler imaging - I. Formalism and numerical tests

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Table 1

Pulsation mode parameters used to test PIMMS.

ID	$f (d^{- 1})$ $Mathematical equation: ${f \over {({d^{ - 1}})}}$$	ℓ	m
f₁	7.14846	0	0
f₂	7.75603	4	3
f₃	6.82308	4	2

Notes. The pulsation modes used are taken from Briquet et al. (2012) for the magnetic β Cep star V2052 Oph.

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