Since its launch, in late 2004, Swift has been locating Gamma-Ray Bursts (GRBs) at a rate of ∼ 100 per year. Very high energy (VHE) emission (> 100 GeV) is predicted by several models. Here, we present the results of a search for VHE emission from the most recent GRBs to fall within the Milagro field of view. © Società Italiana di Fisica.link_to_subscribed_fulltex
Gamma-ray bursts (GRBs), thought to be produced by the core-collapse of massive stars or merging com...
Milagrito, a detector sensitive to very high energy gamma rays, monitored the northern sky from 1997...
Recent rapid localizations of short, hard gamma-ray bursts (GRBs) by the Swift andHETE satellites ha...
Abstract: Gamma-ray bursts (GRBs) have been detected up to GeV energies and are predicted by many mo...
The Milagro gamma-ray observatory employs a water Cherenkov detector to observe extensive air shower...
Milagro is a wide field (2 sr) high duty cycle (>90%) ground-based water Cherenkov detector designed...
Milagro is a water-Cherenkov detector that observes the extended air showers produced by cosmic gamm...
Abstract. The Milagro detector surveyed the sky almost continuously in the very high energy regime f...
The Milagro Gamma-Ray Observatory employs a water Cerenkov detector to observe extensive air showers...
The Milagro gamma-ray observatory employs a water Cherenkov detector to observe extensive air shower...
Recent rapid localizations of short, hard gamma-ray bursts (GRBs) by the Swift and HETE satellites h...
Recent rapid localizations of short, hard gamma-ray bursts (GRBs) by the Swift and HETE satellites h...
discovered one of the brightest gamma-ray bursts ever recorded. With a peak visual magnitude of 5.3,...
Recent rapid localizations of short, hard gamma-ray bursts (GRBs) by the Swift and HETE satellites h...
The Milagro telescope monitors the northern sky for 100 GeV - 100 TeV transient emission through con...
Gamma-ray bursts (GRBs), thought to be produced by the core-collapse of massive stars or merging com...
Milagrito, a detector sensitive to very high energy gamma rays, monitored the northern sky from 1997...
Recent rapid localizations of short, hard gamma-ray bursts (GRBs) by the Swift andHETE satellites ha...
Abstract: Gamma-ray bursts (GRBs) have been detected up to GeV energies and are predicted by many mo...
The Milagro gamma-ray observatory employs a water Cherenkov detector to observe extensive air shower...
Milagro is a wide field (2 sr) high duty cycle (>90%) ground-based water Cherenkov detector designed...
Milagro is a water-Cherenkov detector that observes the extended air showers produced by cosmic gamm...
Abstract. The Milagro detector surveyed the sky almost continuously in the very high energy regime f...
The Milagro Gamma-Ray Observatory employs a water Cerenkov detector to observe extensive air showers...
The Milagro gamma-ray observatory employs a water Cherenkov detector to observe extensive air shower...
Recent rapid localizations of short, hard gamma-ray bursts (GRBs) by the Swift and HETE satellites h...
Recent rapid localizations of short, hard gamma-ray bursts (GRBs) by the Swift and HETE satellites h...
discovered one of the brightest gamma-ray bursts ever recorded. With a peak visual magnitude of 5.3,...
Recent rapid localizations of short, hard gamma-ray bursts (GRBs) by the Swift and HETE satellites h...
The Milagro telescope monitors the northern sky for 100 GeV - 100 TeV transient emission through con...
Gamma-ray bursts (GRBs), thought to be produced by the core-collapse of massive stars or merging com...
Milagrito, a detector sensitive to very high energy gamma rays, monitored the northern sky from 1997...
Recent rapid localizations of short, hard gamma-ray bursts (GRBs) by the Swift andHETE satellites ha...
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