  MAGIC is a stereoscopic system of two Imaging Atmospheric Cherenkov
Telescopes operating in the very high energy (VHE) range from about 50 GeV to
over 50 TeV. The VHE gamma-ray spectra measured at Earth carry an imprint of
the extragalactic background light (EBL) and can be used to study the EBL
density and its evolution in time. In the last few years, precision
measurements of several blazars in the redshift range from z=0.03 up to z=0.9
were performed with MAGIC obtaining strong limits on the EBL density from
single sources. In this paper, we present the results from a combined
likelihood analysis using this broad redshift range sample of blazars allowing
us to probe the EBL at different wavelengths. The implications on the EBL
models and perspectives for future observations with MAGIC are also discussed.
