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We present a search of very high energy gamma-ray emission from the Northern $textit{Fermi}$ Bubble region using data collected with the High Altitude Water Cherenkov (HAWC) gamma-ray observatory. The size of the data set is 290 days. No significant excess is observed in the Northern $textit{Fermi}$ Bubble region, hence upper limits above $1,text{TeV}$ are calculated. The upper limits are between $3times 10^{-7},text{GeV}, text{cm}^{-2}, text{s}^{-1},text{sr}^{-1}$ and $4times 10^{-8},text{GeV},text{cm}^{-2},text{s}^{-1},text{sr}^{-1}$. The upper limits disfavor a proton injection spectrum that extends beyond $100,text{TeV}$ without being suppressed. They also disfavor a hadronic injection spectrum derived from neutrino measurements.
A new ground-based wide-field extensive air shower array known as the High-Altitude Water Cherenkov (HAWC) Observatory promises a new window to monitoring the $sim$100 GeV gamma-ray sky with the potential for detecting a high energy spectral cutoff i
Gamma-ray bursts (GRBs) are among the most luminous sources in the universe. The nature of their emission at TeV energies is one of the most relevant open issues related to these events. The temporal and spectral features inferred from the early and
The bright gamma-ray quasar 4C +55.17 is a distant source ($z = 0.896$) with a hard spectrum at GeV energies as observed by the Large Area Telescope (LAT) on board the {{it Fermi}} satellite. This source is identified as a good source candidate for v
The binary millisecond radio pulsar PSR J1023+0038 exhibits many characteristics similar to the gamma-ray binary system PSR B1259--63/LS 2883, making it an ideal candidate for the study of high-energy non-thermal emission. It has been the subject of
The first limits on the prompt emission from the long gamma-ray burst (GRB) 130427A in the $>100 obreakspacerm{GeV}$ energy band are reported. GRB 130427A was the most powerful burst ever detected with a redshift $zlesssim0.5$ and featured the longes