Add to ORKGImaging Atmospheric Cherenkov Telescopes (IACTs) have consolidated during the last years as the most viable instrument for the detection of -rays in the GeV-TeV energy band. A new generation of IACTs equipped with larger re ectors and improved technology is currently opening up the unexplored energy window between 30 and 300 GeV with an astounding number of source detections. There is a variety of new objects, from extragalactic sources like BL Lacs out to always further distances to galactic supernova remnants, plerions and X-ray binaries. Even more exciting news is that several sources remain to date unidentied.
Imaging Atmospheric Cherenkov Telescopes (IACTs) allow us to observe Active Galactic Nuclei (AGNs) i...
Ground-based gamma-ray astronomy is part of a new field of fundamental research of Astroparticle Ph...
H.E.S.S. is an array of five Imaging Atmospheric Cherenkov Telescopes (IACTs) located 1800 m above s...
With the successful realization of the current-generation of ground-based detectors, TeV Astronomy h...
Fermi-LAT observations have proven that GeV g-ray emission is a relatively common feature formany Ga...
This is an Open Access book published by World Scientific Publishing Company. It is distributed unde...
High energy gamma-ray astronomy has recently made significant progress through ground-based instrume...
Proceedings of the 30th ICRC, Merida, Mexico (2007). Rogelio Caballero, Juan Carlos D'Olivo, Gustavo...
VERITAS, an Imaging Atmospheric Cherenkov Telescope (IACT) system for gammma-ray astronomy in the Ge...
With the successful realization of the current-generation of ground-based detectors, TeV Astronomy h...
In the last two decades a new window for ground-based high energy astrophysics has been opened. This...
Between 1997 and the end of the detector operation in fall 2002, about 5500 hours of observational d...
High energy gamma-ray astronomy is a newly emerging and very successful branch of astronomy and astr...
Fermi-LAT observations have proven that GeV γ-ray emission is a relatively common feature for many ...
Very-high energy (VHE; E > 100 GeV) gamma-rays provide a powerful insight into the non-thermal unive...
Imaging Atmospheric Cherenkov Telescopes (IACTs) allow us to observe Active Galactic Nuclei (AGNs) i...
Ground-based gamma-ray astronomy is part of a new field of fundamental research of Astroparticle Ph...
H.E.S.S. is an array of five Imaging Atmospheric Cherenkov Telescopes (IACTs) located 1800 m above s...
With the successful realization of the current-generation of ground-based detectors, TeV Astronomy h...
Fermi-LAT observations have proven that GeV g-ray emission is a relatively common feature formany Ga...
This is an Open Access book published by World Scientific Publishing Company. It is distributed unde...
High energy gamma-ray astronomy has recently made significant progress through ground-based instrume...
Proceedings of the 30th ICRC, Merida, Mexico (2007). Rogelio Caballero, Juan Carlos D'Olivo, Gustavo...
VERITAS, an Imaging Atmospheric Cherenkov Telescope (IACT) system for gammma-ray astronomy in the Ge...
With the successful realization of the current-generation of ground-based detectors, TeV Astronomy h...
In the last two decades a new window for ground-based high energy astrophysics has been opened. This...
Between 1997 and the end of the detector operation in fall 2002, about 5500 hours of observational d...
High energy gamma-ray astronomy is a newly emerging and very successful branch of astronomy and astr...
Fermi-LAT observations have proven that GeV γ-ray emission is a relatively common feature for many ...
Very-high energy (VHE; E > 100 GeV) gamma-rays provide a powerful insight into the non-thermal unive...
Imaging Atmospheric Cherenkov Telescopes (IACTs) allow us to observe Active Galactic Nuclei (AGNs) i...
Ground-based gamma-ray astronomy is part of a new field of fundamental research of Astroparticle Ph...
H.E.S.S. is an array of five Imaging Atmospheric Cherenkov Telescopes (IACTs) located 1800 m above s...