How to detect gamma-rays from ground: an introduction to the detection concepts
arXiv:2401.04460 · doi:10.1007/978-981-16-4544-0_61-1
Abstract
Indirect detection of gamma rays with ground-based observatories is currently the most sensitive experimental approach to characterize the gamma-ray sky at energies \,TeV. Ground-based detection of gamma-rays relies on the electromagnetic showers that gamma rays initiate in the Earth's atmosphere. In this chapter we will review the properties of electromagnetic air showers as well as the differences with respect to cosmic-ray showers that enable the rejection of the cosmic ray background. The experimental techniques that have been developed for ground-based detection of gamma rays will be introduced. These fall onto three main categories: air shower particle detectors, sampling Cherenkov arrays, and imaging atmospheric Cherenkov telescopes. Hybrid concepts as well as other experimental approaches are also discussed.
arXiv comment24 pages, 11 figures, invited chapter in Handbook of X-ray and Gamma-ray Astrophysics (eds. Cosimo Bambi and Andrea Santangelo)
References in corpus (34)
- Observations of the Crab Nebula with H.E.S.S
- Observation of the Crab Nebula with the HAWC Gamma-Ray Observatory
- Teraelectronvolt Astronomy
- The major upgrade of the MAGIC telescopes, Part I: The hardware improvements and the commissioning of the system
- Monte Carlo design studies for the Cherenkov Telescope Array
- Sensitivity of the High Altitude Water Cherenkov Detector to Sources of Multi-TeV Gamma Rays
- Discovery of TeV Gamma-Ray Emission from the Cygnus Region of the Galaxy
- Observation of TeV Gamma Rays from the Crab Nebula with Milagro Using a New Background Rejection Technique
- On the sensitivity of the HAWC observatory to gamma-ray bursts
- Impact of atmospheric parameters on the atmospheric Cherenkov technique
- Multi-Tev Gamma-Ray Observation from the Crab Nebula Using the Tibet-III Air Shower Array Finely Tuned by the Cosmic-Ray Moon's Shadow
- Impact of aerosols and adverse atmospheric conditions on the data quality for spectral analysis of the H.E.S.S. telescopes
- 5@5 - a 5 GeV energy threshold array of imaging atmospheric Cherenkov telescopes at 5 km altitude
- Detection of the Geminga pulsar with MAGIC hints at a power-law tail emission beyond 15 GeV
- First detection of the Crab Nebula at TeV energies with a Cherenkov telescope in a dual-mirror Schwarzschild-Couder configuration: the ASTRI-Horn telescope
- First Ground-based Measurement of Sub-20 GeV to 100 GeV -rays from the Vela Pulsar with H.E.S.S. II
- Gamma-ray blazar spectra with H.E.S.S. II mono analysis: the case of PKS 2155-304 and PG 1553+113
- Detection of the Crab Nebula with the 9.7 m Prototype Schwarzschild-Couder Telescope
- High Energy Gamma-Ray Observations of the Crab Nebula and Pulsar with the Solar Tower Atmospheric Cherenkov Effect Experiment
- FACT - Monitoring Blazars at Very High Energies
- The STACEE-32 Ground Based Gamma-ray Detector
- A luminous and isolated gamma-ray flare from the blazar B2 1215+30
- Monte Carlo Studies of Geomagnetic Field Effects on the Imaging Air Cherenkov Technique for the MAGIC Telescope Site
- A method to correct IACT data for atmospheric absorption due to the Saharan Air Layer
- Detection of Atmospheric Cherenkov Radiation Using Solar Heliostat Mirrors
- Design and Performance of the Prototype Schwarzschild-Couder Telescope Camera
- Gamma/Hadron Separation with the HAWC Observatory
- Influence of the Geomagnetic Field on the IACT detection technique for possible sites of CTA observatories
- An elastic lidar system for the H.E.S.S. Experiment
- Improving Time and Position Resolution of RPC detectors using Time Over Threshold Information
- Panoramic SETI: Program Update and High-Energy Astrophysics Applications
- Very high-energy observations of the two high-frequency peaked BL Lac objects 1ES 1218+304 and H 1426+428
- Optimization of large homogeneous air Cherenkov arrays and application to the design of a 1TeV-100TeV gamma-ray observatory
- Panoramic SETI: on-sky results from prototype telescopes and instrumental design