MAGIC observations of Dragonfly Nebula at TeV Energies using the Very Large Zenith Angle Technique

Darko Zarić; Razmik Mirzoyan; Ievgen Vovk; Petar Temnikov; Michele Peresano; Nikola Godinović; Juliane van Scherpenberg; Jürgen Besenrieder

arXiv · 1909.05107

MAGIC observations of Dragonfly Nebula at TeV Energies using the Very Large Zenith Angle Technique

Darko Zarić·Razmik Mirzoyan·Ievgen Vovk·Petar Temnikov·Michele Peresano·Nikola Godinović·Juliane van Scherpenberg·Jürgen Besenrieder

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Abstract

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.

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Darko Zarić, Razmik Mirzoyan, Ievgen Vovk, Petar Temnikov, Michele Peresano, Nikola Godinović, Juliane van Scherpenberg, Jürgen Besenrieder. 2019-09-11. MAGIC observations of Dragonfly Nebula at TeV Energies using the Very Large Zenith Angle Technique. https://arxiv.org/abs/1909.05107

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