@Article{HAWCCollaborationAlbert+SalesaGreus2022,
author="HAWC Collaboration (Albert, A. et al
and Salesa Greus, F.",
title="HAWC Study of the Ultra-high-energy Spectrum of MGRO J1908+06",
journal="Astrophysical Journal",
year="2022",
publisher="IOP Publishing Ltd",
volume="928",
number="2",
pages="116--13pp",
abstract="We report TeV gamma-ray observations of the ultra-high-energy source MGRO J1908+06 using data from the High Altitude Water Cherenkov Observatory. This source is one of the highest-energy known gamma-ray sources, with emission extending past 200 TeV. Modeling suggests that the bulk of the TeV gamma-ray emission is leptonic in nature, driven by the energetic radio-faint pulsar PSR J1907+0602. Depending on what assumptions are included in the model, a hadronic component may also be allowed. Using the results of the modeling, we discuss implications for detection prospects by multi-messenger campaigns.",
optnote="WOS:000776453700001",
optnote="exported from refbase (https://references.ific.uv.es/refbase/show.php?record=5187), last updated on Sat, 16 Apr 2022 19:21:00 +0000",
issn="0004-637x",
doi="10.3847/1538-4357/ac56e5",
opturl="https://arxiv.org/abs/2112.00674",
opturl="https://doi.org/10.3847/1538-4357/ac56e5",
language="English"
}