  Above $\sim$3 keV, the X-ray spectrum of the active galactic nuclei (AGN) is
characterized by the intrinsic continuum and compton reflection features. For
type-1 AGN, several regions could contribute to the reflection. In order to
investigate the nature of the reflecting medium, we perform a systematic
analysis of the reflector using XMM-Newton and NuSTAR observations of a sample
of 22 type-1 AGN. We create a baseline model which includes Galactic absorption
and an intrinsically absorbed power-law plus a reflection model. We test a set
of nine reflection models in a sub-sample of five objects. Based on these
results, we select three models to be tested on the entire sample, accounting
for distinct physical scenarios: neutral/distant reflection,
ionized/relativistic reflection, and neutral/distant+ionized/relativistic
reflection, namely hybrid model. We find that 18 sources require the reflection
component to fit their spectra. Among them, 67$\%$ prefer the hybrid model.
Neutral and ionized models are equally preferred by three sources. We conclude
that both the neutral/distant reflector most probably associated with the inner
edges of the torus and the ionized/relativistic reflector associated with the
accretion disk are required to describe the reflection in type-1 AGN.
