Add to ORKGAbstract: The LAGO project aims at the detection of high energy photons from GRBs using the single particle technique in ground based water Cherenkov detectors. To reach a reasonable sensitivity, high altitude mountain sites have been selected and detectors are in operation in Mexico (Sierra Negra, 4650m a.s.l.) and Bolivia (Chacaltaya, 5300m a.s.l.). We report on detector calibration and operation at high altitude, search for bursts in 4 months of preliminary data, as well as search for signal when satellites report a burst
Observing gamma ray bursts (GRBs) in the TeV energy range can be extremely valuable in providing ins...
AbstractThe LAGO project is a recent collaboration that comes from the association of latin american...
The Milagro gamma-ray observatory employs a water Cherenkov detector to observe extensive air shower...
The Large Aperture GRB Observatory (LAGO) project aims at the detection of high energy photons from ...
The Large Aperture GRB Observatory (LAGO) is aiming at the detection of the high energy (around 100G...
Abstract: The LAGO project is an international effort of many groups in different countries to opera...
The Large Aperture GRB Observatory (LAGO) project aims at the detection of high energy photons from ...
In order to characterise the behaviour of Water Cherenkov Detectors (WCD) under a sudden increase of...
© 2017. The American Astronomical Society. All rights reserved.. The High Altitude Water Cherenkov (...
The ARGO-YBJ experiment is designed for very high energy gamma-astronomy and cosmic ray researches. ...
Milagro is a wide field (2 sr) high duty cycle (>90%) ground-based water Cherenkov detector designed...
The High Altitude Water Cherenkov (HAWC) observatory is an array of large water Cherenkov detectors ...
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...
ARGO-YBJ is a "full coverage" air shower detector consisting of a 6700 m2 carpet of Resistive Plate ...
Observing gamma ray bursts (GRBs) in the TeV energy range can be extremely valuable in providing ins...
AbstractThe LAGO project is a recent collaboration that comes from the association of latin american...
The Milagro gamma-ray observatory employs a water Cherenkov detector to observe extensive air shower...
The Large Aperture GRB Observatory (LAGO) project aims at the detection of high energy photons from ...
The Large Aperture GRB Observatory (LAGO) is aiming at the detection of the high energy (around 100G...
Abstract: The LAGO project is an international effort of many groups in different countries to opera...
The Large Aperture GRB Observatory (LAGO) project aims at the detection of high energy photons from ...
In order to characterise the behaviour of Water Cherenkov Detectors (WCD) under a sudden increase of...
© 2017. The American Astronomical Society. All rights reserved.. The High Altitude Water Cherenkov (...
The ARGO-YBJ experiment is designed for very high energy gamma-astronomy and cosmic ray researches. ...
Milagro is a wide field (2 sr) high duty cycle (>90%) ground-based water Cherenkov detector designed...
The High Altitude Water Cherenkov (HAWC) observatory is an array of large water Cherenkov detectors ...
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...
ARGO-YBJ is a "full coverage" air shower detector consisting of a 6700 m2 carpet of Resistive Plate ...
Observing gamma ray bursts (GRBs) in the TeV energy range can be extremely valuable in providing ins...
AbstractThe LAGO project is a recent collaboration that comes from the association of latin american...
The Milagro gamma-ray observatory employs a water Cherenkov detector to observe extensive air shower...