Add to ORKGRecent rapid localizations of short, hard gamma-ray bursts (GRBs) by the Swift andHETE satellites have led to the observation of the first afterglows and the measurement of the first redshifts from this type of burst (Fox et al. 2005
Since the discovery of the first short-hard gamma-ray burst afterglows in 2005, the handful of obser...
Since its launch, in late 2004, Swift has been locating Gamma-Ray Bursts (GRBs) at a rate of ∼ 100 p...
We are in an exciting period of discovery for gamma-ray bursts. The Swift observatory is detecting 1...
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...
Recent rapid localizations of short, hard gamma-ray bursts (GRBs) by the Swift and HETE satellites h...
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...
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...
The study of the early high-energy emission from both long and short gamma-ray bursts (GRBs) has bee...
The AGILE gamma-ray burst GRB 080514B is the first detected to have emission above 30 MeV and an opt...
Gamma-ray bursts (GRBs) are bright flashes of gamma-ray energy that originate in distant galaxies an...
Abstract. GRBs remained a puzzle for many high-energy astrophysicists since their dis-covery in 1967...
We present the discovery of the first millimeter afterglow of a short-duration $\gamma$-ray burst (S...
Since the discovery of the first short-hard gamma-ray burst afterglows in 2005, the handful of obser...
Since its launch, in late 2004, Swift has been locating Gamma-Ray Bursts (GRBs) at a rate of ∼ 100 p...
We are in an exciting period of discovery for gamma-ray bursts. The Swift observatory is detecting 1...
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...
Recent rapid localizations of short, hard gamma-ray bursts (GRBs) by the Swift and HETE satellites h...
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...
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...
The study of the early high-energy emission from both long and short gamma-ray bursts (GRBs) has bee...
The AGILE gamma-ray burst GRB 080514B is the first detected to have emission above 30 MeV and an opt...
Gamma-ray bursts (GRBs) are bright flashes of gamma-ray energy that originate in distant galaxies an...
Abstract. GRBs remained a puzzle for many high-energy astrophysicists since their dis-covery in 1967...
We present the discovery of the first millimeter afterglow of a short-duration $\gamma$-ray burst (S...
Since the discovery of the first short-hard gamma-ray burst afterglows in 2005, the handful of obser...
Since its launch, in late 2004, Swift has been locating Gamma-Ray Bursts (GRBs) at a rate of ∼ 100 p...
We are in an exciting period of discovery for gamma-ray bursts. The Swift observatory is detecting 1...