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Pulsars in a Bubble? Following Electron Diffusion in the Galaxy with TeV Gamma Rays
Free accessArXiv | 2019| -
Dark Matter Limits From Dwarf Spheroidal Galaxies with The HAWC Gamma-Ray Observatory
Free accessArXiv | 2017| -
Sensitivity of the High Altitude Water Cherenkov Detector to Sources of Multi-TeV Gamma Rays
Free accessArXiv | 2013| -
Daily monitoring of TeV gamma-ray emission from Mrk 421, Mrk 501, and the Crab Nebula with HAWC
Free accessArXiv | 2017| -
Extended gamma-ray sources around pulsars constrain the origin of the positron flux at Earth
Free accessArXiv | 2017| -
Search for Very High Energy Gamma Rays from the Northern $\textit{Fermi}$ Bubble Region with HAWC
Free accessArXiv | 2017| -
Data Acquisition Architecture and Online Processing System for the HAWC gamma-ray observatory
Free accessArXiv | 2017| -
Milagro Limits and HAWC Sensitivity for the Rate-Density of Evaporating Primordial Black Holes
Free accessArXiv | 2014|
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