  Recently, researches performed by two groups have revealed that the magnetar
spin-down energy injection model with full energy trapping can explain the
early-time light curves of SN 2010gx, SN 2013dg, LSQ12dlf, SSS120810 and
CSS121015, but fails to fit the late-time light curves of these Superluminous
Supernovae (SLSNe). These results imply that the original magnetar-powered
model is challenged in explaining these SLSNe. Our paper aims to simultaneously
explain both the early- and late-time data/upper limits by considering the
leakage of hard emissions. We incorporate quantitatively the leakage effect
into the original magnetar-powered model and derive a new semi-analytical
equation. Comparing the light curves reproduced by our revised magnetar-powered
model to the observed data and/or upper limits of these five SLSNe, we found
that the late-time light curves reproduced by our semi-analytical equation are
in good agreement with the late-time observed data and/or upper limits of SN
2010gx, CSS121015, SN 2013dg and LSQ12dlf and the late-time excess of
SSS120810, indicating that the magnetar-powered model might be responsible for
these SLSNe and that the gamma ray and X-ray leakage are unavoidable when the
hard photons were down-Comptonized to softer photons. To determine the details
of the leakage effect and unveil the nature of SLSNe, more high quality
bolometric light curves and spectra of SLSNe are required.
