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The first 10years of the HAWC Gamma-Ray Observatory: science results
Anna Lia Longinotti, HAWC Collaboration
The High-Altitude Water Cherenkov (HAWC) Observatory, located on the slopes of the Sierra Negra volcano in Mexico, began operations in March 2015. Over the past decade, HAWC has en…
HAWC Contributions to the 37th International Cosmic Ray Conference (ICRC2021)
HAWC Collaboration
Works submitted to the 37th International Cosmic Ray Conference. Contents: Operation, Calibration, and Analysis Galactic Gamma-Ray Physics Extra Galactic Gamma-Ray Physics Cosmic-R…
The Ultra-High-Energy Source MGRO J1908+06
Kelly Malone, HAWC Collaboration
The TeV gamma-ray source MGRO J1908+06 is one of the highest-energy sources known, with observed emission by the High Altitude Water Cherenkov (HAWC) Observatory extending well pas…
A search for spectral hardening in HAWC sources above 56 TeV
Kelly Malone, HAWC Collaboration
The High Altitude Water Cherenkov (HAWC) Observatory is a wide-field-of-view gamma-ray observatory that is optimized to detect gamma rays between ~300 GeV and several hundred TeV.…
Evidence that Ultra-High-Energy Gamma Rays are a Universal Feature Near Powerful Pulsars
HAWC Collaboration, A. Albert, R. Alfaro +97
The highest-energy known gamma-ray sources are all located within 0.5 degrees of extremely powerful pulsars. This raises the question of whether ultra-high-energy (UHE; 56 TeV)…
Multi-messenger Observations of a Binary Neutron Star Merger
LIGO Scientific Collaboration, Virgo Collaboration, Fermi GBM +66
On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIG…