TeV gamma rays probe the non-thermal Universe in ways that are not possible at other wavelengths. The HAWC observatory, under construction in Mexico, will be able to analyze and survey the TeV sky more completely than any competing detectors that use air Cherenkov techniques, and perhaps yield new insight onto the nature of cosmic accelerators responsible for gamma ray bursts, active galactic nuclei flares, and other cataclysmic astrophysical events. Before it's deployment, one of HAWC's electronic data acquisition systems, the scaler system, will be tested using a pulse generator. The pulse generator's capabilities are assessed and documented.Committee Member/Second Reader: Andreas Tepe; Committee Member/Second Reader: Brian Kennedy; Fa...
The HAWC (High Altitude Water Cherenkov) observatory, located on the slopes of the Sierra Negra volc...
Ground-based gamma-ray astronomy is a powerful tool to study cosmic-ray physics, providing a diagnos...
With the successful realization of the current-generation of ground-based detectors, TeV Astronomy h...
AbstractThe High Altitude Water Cherenkov (HAWC) Observatory is a TeV gamma-ray detector located at ...
We present the sensitivity of HAWC to gamma ray bursts (GRBs). HAWC is a very high-energy gamma-ray ...
Abstract: Gamma-ray bursts (GRBs) are among the most energetic phenomena in the known universe and a...
The High-Altitude Water Cherenkov Observatory (HAWC) is a TeV gamma-ray detector located at an altit...
© Owned by the authors, published by EDP Sciences, 2015. The High-Altitude Water Cherenkov (HAWC) Te...
The high altitude water cherenkov gamma-ray observatory (HAWC) has been fully operational since Marc...
AbstractThe High-Altitude Water Cherenkov (HAWC) Observatory is designed to observe extensive air sh...
Ground-based gamma-ray astronomy has historically implemented two dramatically different techniques....
The Gamma Ray Observatory (GRO), the second in NASA\u27s series of Great Observatories, is the next ...
Presented on September 21, 2015 in the Klaus Advanced Computing Building, room 1116W at 3:00 p.m.Ste...
International audienceObservations of high energy gamma rays are an essential probe of the cosmic-ra...
The Atmospheric Cherenkov Imaging Technique has opened up the gamma-ray spectrum from 100 GeV to 50 ...
The HAWC (High Altitude Water Cherenkov) observatory, located on the slopes of the Sierra Negra volc...
Ground-based gamma-ray astronomy is a powerful tool to study cosmic-ray physics, providing a diagnos...
With the successful realization of the current-generation of ground-based detectors, TeV Astronomy h...
AbstractThe High Altitude Water Cherenkov (HAWC) Observatory is a TeV gamma-ray detector located at ...
We present the sensitivity of HAWC to gamma ray bursts (GRBs). HAWC is a very high-energy gamma-ray ...
Abstract: Gamma-ray bursts (GRBs) are among the most energetic phenomena in the known universe and a...
The High-Altitude Water Cherenkov Observatory (HAWC) is a TeV gamma-ray detector located at an altit...
© Owned by the authors, published by EDP Sciences, 2015. The High-Altitude Water Cherenkov (HAWC) Te...
The high altitude water cherenkov gamma-ray observatory (HAWC) has been fully operational since Marc...
AbstractThe High-Altitude Water Cherenkov (HAWC) Observatory is designed to observe extensive air sh...
Ground-based gamma-ray astronomy has historically implemented two dramatically different techniques....
The Gamma Ray Observatory (GRO), the second in NASA\u27s series of Great Observatories, is the next ...
Presented on September 21, 2015 in the Klaus Advanced Computing Building, room 1116W at 3:00 p.m.Ste...
International audienceObservations of high energy gamma rays are an essential probe of the cosmic-ra...
The Atmospheric Cherenkov Imaging Technique has opened up the gamma-ray spectrum from 100 GeV to 50 ...
The HAWC (High Altitude Water Cherenkov) observatory, located on the slopes of the Sierra Negra volc...
Ground-based gamma-ray astronomy is a powerful tool to study cosmic-ray physics, providing a diagnos...
With the successful realization of the current-generation of ground-based detectors, TeV Astronomy h...