Results 1 to 10 of about 208,249 (317)

TAIGA - An advanced hybrid detector complex for astroparticle physics and high energy gamma-ray astronomy [PDF]

SciPost Physics Proceedings, 2023
The physical motivations, present status, main results in study of cosmic rays and in the field of gamma-ray astronomy as well future plans of the TAIGA-1 (Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy) project are presented.
N. M. Budnev, I. Astapov, P. Bezyazeekov, E. Bonvech, A. Borodin, A. Bulan, D. Chernov, A. Chiavassa, A. Dyachok, A. Gafarov, A. Garmash, V. Grebenyuk, E. Gress, O. Gress, T. Gress, A. Grinyuk, O. Grishin, A. D. Ivanova, A. L. Ivanova, N. Kalmykov, V. Kindin, S. Kiryuhin, R. Kokoulin, K. Kompaniets, E. Korosteleva, V. Kozhin, E. Kravchenko, A. Kryukov, L. Kuzmichev, A. Lagutin, M. Lavrova, Y. Lemeshev, B. Lubsandorzhiev, N. Lubsandorzhiev, A. Lukanov, D. Lukyantsev, S. Malakhov, R. Mirgazov, R. Monkhoev, E. Osipova, A. Pakhorukov, L. Pankov, A. Pan, A. Panov, A. Petrukhin, I. Poddubnyi, D. Podgrudkov, V. Ponomareva, E. Popova, E. Postnikov, V. Prosin, V. Ptuskin, A. Pushnin, R. Raikin, A. Razumov, G. Rubtsov, E. Ryabov, V. Samoliga, A. Satyshev, A. Silaev, A. Silaev, A. Sidorenkov, A. Skurikhin, A. Sokolov, L. Sveshnikova, V. Tabolenko, L. Tkachev, A. Tanaev, M. Ternovoy, R. Togoo, N. Ushakov, A. Vaidyanathan, P. Volchugov, N. Volkov, D. Voronin, A. Zagorodnikov, D. Zhurov, I. Yashin
doaj   +2 more sources

Gamma ray astronomy [PDF]

Surveys in High Energy Physics, 2001
Abstract The energy domain between 10 MeV and hundreds of GeV is an essential one for the multifrequency study of extreme astrophysical sources. The understanding of spectra of detected gamma rays is necessary for developing models for acceleration, emission, absorption and propagation of very high-energy particles at their sources and in space.
A. Morselli
  +9 more sources

35 Years of Ground-Based Gamma-ray Astronomy

Universe, 2021
This paper provides a brief, personal account of the development of ground-based gamma-ray astronomy, primarily over the last 35 years, with some digressions into the earlier history of the field.
Paula Chadwick
doaj   +2 more sources

CubeSats for Gamma-Ray Astronomy

, 2022
After many years of flying in space primarily for educational purposes, CubeSats - tiny satellites with form factors corresponding to arrangements of "1U" units, or cubes, each 10 cm on a side - have come into their own as valuable platforms for technology advancement and scientific investigations. CubeSats offer comparatively rapid, low-cost access to
Bloser, Peter F., Murphy, David, Fiore, Fabrizio, Perkins, Jeremy   +3 more
openaire   +3 more sources

The future of gamma-ray astronomy [PDF]

Comptes Rendus. Physique, 2016
To be published in Comptes Rendus Physique (2016)
J. Knodlseder
semanticscholar   +7 more sources

The AGILE gamma-ray astronomy mission [PDF]

AIP Conference Proceedings, 2000
We describe the AGILE gamma-ray astronomy satellite which has recently been selected as the first Small Scientific Mission of the Italian Space Agency. With a launch in 2002, AGILE will provide a unique tool for high-energy astrophysics in the 30 MeV - 50 GeV range before GLAST.
S. Mereghetti
openalex   +5 more sources

Nucleosynthesis and gamma ray-line astronomy [PDF]

Nuclear Physics B - Proceedings Supplements, 2000
4 ...
E. Vangioni–Flam, R. Ramaty, Michel Cassé   +2 more
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TeV gamma-ray astronomy [PDF]

Research in Astronomy and Astrophysics, 2009
Invited review, published in Research in Astronomy and Astrophysics (see http://www.raa-journal.org/raa/index.php/raa/article/view/251)
Wei Cui
openalex   +4 more sources

H.E.S.S.-II - Gamma ray astronomy from 20 GeV to hundreds of TeV’s

EPJ Web of Conferences, 2017
Since the commissioning of the fifth, largest telescope (28 m diameter) in December 2012, H.E.S.S. II is the only hybrid array of Imaging Atmospheric Cherenkov Telescopes operating in the energy range ~ 20 GeV to ~ 100 TeV.
de Naurois Mathieu
doaj   +2 more sources

Gamma Ray Astronomy with LHAASO

Journal of Physics: Conference Series, 2016
The aim of LHAASO is the development of an air shower experiment able to monitor with unprecedented sensitivity the gamma ray sky at energies from ~200 GeV to 1 PeV, and at the same time be an instrument able to measure the cosmic ray spectrum, composition and anisotropy in a wide energy range (~1 TeV to 1 EeV). LHAASO, thanks to the large area and the
VERNETTO, Silvia Teresa, LHAASO Collaboration   +1 more
openaire   +4 more sources