  The last six years have witnessed major revisions of our knowledge about the
Crab Pulsar. The consensus scenario for the origin of the high-energy pulsed
emission has been challenged with the discovery of a very-high-energy power law
tail extending up to 400 GeV, above the expected spectral cut off at a few GeV.
Now, new measurements obtained by the MAGIC collaboration extend the energy
spectrum of the Crab Pulsar even further, on the TeV regime. Above 400 GeV the
pulsed emission comes mainly from the inter-pulse, which becomes more prominent
with energy due to a harder spectral index. These findings require gamma-ray
production via inverse Compton scattering close to or beyond the light cylinder
radius by an underlying particle population with Lorentz factors greater than 5
times 106. We will present those new results and discuss the implications in
our current knowledge concerning pulsar environments.
