  We perform a Bayesian model selection analysis for interacting scenarios of
dark matter and modified holographic Ricci dark energy (MHRDE) with linear
interacting terms. We use a combination of some of the latest cosmological data
such as type Ia supernovae, cosmic chronometers, cosmic microwave background
and baryon acoustic oscillations measurements. We find strong evidence against
all the MHRDE interacting scenarios studied with respect to $\Lambda$CDM when
the full joint analysis is considered.
