  One of the brightest regions of diffuse gamma-ray emission in the northern
sky is the Cygnus star-forming region, where one can assume the most energetic
processes are taking place. The Dragonfly Nebula (MGRO J2019+37) is one of the
brightest sources in the Cygnus region. First discovered by MILAGRO, it was
later resolved into two sources by VERITAS: the faint point-like source VER
J2016+371 and the bright extended source VER J2019+368. The latter accounts for
the bulk of the MGRO J2019+37 emission, with the spectrum among the hardest in
the TeV range. We report the results of a dedicated MAGIC observational
campaign of VER J2019+368. The data obtained with the Very Large Zenith Angle
observational technique provides an effective collection area of about one
square kilometer. We used $\sim$45 hours of data collected under Very Large
Zenith Angles for exploring the flux of the source at TeV energies.
