  The Crab pulsar is the only astronomical pulsed source detected above 100
GeV. The emission mechanism of very high energy gamma-ray pulsation is not yet
fully understood, although several theoretical models have been proposed. In
order to test the new models, we measured the light curve and the spectra of
the Crab pulsar with high precision by means of deep observations. We analyzed
135 hours of selected MAGIC data taken between 2009 and 2013 in stereoscopic
mode. In order to discuss the spectral shape in connection with lower energies,
4.6 years of Fermi-LAT data were also analyzed. The known two pulses per period
were detected with a significance of 8.0 sigma and 12.6 sigma. In addition,
significant bridge emission was found between the two pulses with 6.2 sigma.
This emission can not be explained with the existing theories. These data can
be used for testing new theoretical models.

High Energy Astrophysical Phenomena