  We report the results of a 60-hr photometric campaign of a rapidly
oscillating Ap star, J0855 (TYC 2488-1241-1). We have utilised the multi-site
Las Cumbres Observatory's (LCO) 0.4-m telescopes to obtain short cadence B-band
observations of an roAp star previously lacking detailed study. Our
observations confirm the rotation period presented in the discovery paper of
this star ($P_{\rm rot}=3.0918$ d), and reveal the star to be pulsating in a
distorted mode. The B data show this star to be among the highest amplitude
roAp stars, with a peak-to-peak amplitude of 24 mmag. Modelling of the
pulsation frequency at 197.2714 d$^{-1}$ (2283 $\mu$Hz; P=7.30 min) shows that
this star belongs to the subgroup of super-critical pulsators, where the
observed frequencies are above the theoretical acoustic cutoff frequency. From
the modelling, we deduce that the star's rotation axis is inclination angle of
about $30^\circ$ to the line-of-sight, with an angle of obliquity of the
magnetic axis to the rotation axis of either $40^\circ$ or $24^\circ$ depending
on whether the pulsation mode is dipole or quadrupole, respectively.
