FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1935981978> ?p ?o ?g. }

• W1935981978 endingPage "627" @default.
• W1935981978 startingPage "610" @default.
• W1935981978 abstract "Following the discovery of the cosmic rays by Victor Hess in 1912, more than 70 years and numerous technological developments were needed before an unambiguous detection of the first very-high-energy gamma-ray source in 1989 was made. Since this discovery, the field on very-high-energy gamma-ray astronomy experienced a true revolution: a second, then a third generation of instruments were built, observing the atmospheric cascades from the ground, either through the atmospheric Cherenkov light they comprise, or via the direct detection of the charged particles they carry. Present arrays, 100 times more sensitive than the pioneering experiments, have detected a large number of astrophysical sources of various types, thus opening a new window on the non-thermal Universe. New, even more sensitive instruments are currently being built; these will allow us to explore further this fascinating domain. In this article we describe the detection techniques, the history of the field and the prospects for the future of ground-based very-high-energy gamma-ray astronomy. Depuis la découverte des rayons cosmiques en 1912 par Victor Hess, il aura fallu près de 70 ans et de nombreux développements pour aboutir à la première détection d'une source gamma de très haute énergie en 1989. Depuis cette découverte, le domaine de l'astronomie gamma de très haute énergie a vécu une véritable révolution : des détecteurs de deuxième, puis de troisième génération ont vu le jour, observant les cascades atmosphériques depuis le sol, soit à travers l'émission Tcherenkov atmosphérique qui les accompagne, soit en détectant directement les particules chargées qui les composent. Les réseaux récents, environ 100 fois plus sensibles que les plus anciens, ont détecté de très nombreuses sources astrophysiques de types variés et ont ainsi ouvert une nouvelle fenêtre sur l'Univers non thermique. De nouveaux réseaux de télescopes encore plus sensibles, en cours de construction, vont nous permettre de pousser encore plus loin l'exploration de ce domaine fascinant. Dans cet article, nous décrivons les techniques de détection, dressons un panorama historique du domaine et présentons les perspectives pour le futur de l'astronomie gamma de très haute énergie au sol." @default.
• W1935981978 created "2016-06-24" @default.
• W1935981978 creator A5025036902 @default.
• W1935981978 creator A5046893564 @default.
• W1935981978 date "2015-08-01" @default.
• W1935981978 modified "2023-10-16" @default.
• W1935981978 title "Ground-based detectors in very-high-energy gamma-ray astronomy" @default.
• W1935981978 cites W1914556314 @default.
• W1935981978 cites W1964548550 @default.
• W1935981978 cites W1965726692 @default.
• W1935981978 cites W1974281020 @default.
• W1935981978 cites W1977123713 @default.
• W1935981978 cites W1981094653 @default.
• W1935981978 cites W1983354252 @default.
• W1935981978 cites W1988993007 @default.
• W1935981978 cites W1994639828 @default.
• W1935981978 cites W2012825046 @default.
• W1935981978 cites W2021677098 @default.
• W1935981978 cites W2025100887 @default.
• W1935981978 cites W2031037636 @default.
• W1935981978 cites W2036805479 @default.
• W1935981978 cites W2056247568 @default.
• W1935981978 cites W2059743763 @default.
• W1935981978 cites W2063186026 @default.
• W1935981978 cites W2063935839 @default.
• W1935981978 cites W2069264289 @default.
• W1935981978 cites W2071922768 @default.
• W1935981978 cites W2082131976 @default.
• W1935981978 cites W2090687596 @default.
• W1935981978 cites W2094757406 @default.
• W1935981978 cites W2104721808 @default.
• W1935981978 cites W2116159083 @default.
• W1935981978 cites W2117634821 @default.
• W1935981978 cites W2146457982 @default.
• W1935981978 cites W2151018998 @default.
• W1935981978 cites W2153460074 @default.
• W1935981978 cites W2158354523 @default.
• W1935981978 cites W2165813309 @default.
• W1935981978 cites W2752966631 @default.
• W1935981978 cites W2761274035 @default.
• W1935981978 cites W2963906579 @default.
• W1935981978 cites W4298237502 @default.
• W1935981978 doi "https://doi.org/10.1016/j.crhy.2015.08.011" @default.
• W1935981978 hasPublicationYear "2015" @default.
• W1935981978 type Work @default.
• W1935981978 sameAs 1935981978 @default.
• W1935981978 citedByCount "48" @default.
• W1935981978 countsByYear W19359819782015 @default.
• W1935981978 countsByYear W19359819782016 @default.
• W1935981978 countsByYear W19359819782017 @default.
• W1935981978 countsByYear W19359819782018 @default.
• W1935981978 countsByYear W19359819782019 @default.
• W1935981978 countsByYear W19359819782020 @default.
• W1935981978 countsByYear W19359819782021 @default.
• W1935981978 countsByYear W19359819782022 @default.
• W1935981978 countsByYear W19359819782023 @default.
• W1935981978 crossrefType "journal-article" @default.
• W1935981978 hasAuthorship W1935981978A5025036902 @default.
• W1935981978 hasAuthorship W1935981978A5046893564 @default.
• W1935981978 hasBestOaLocation W19359819781 @default.
• W1935981978 hasConcept C111309251 @default.
• W1935981978 hasConcept C120665830 @default.
• W1935981978 hasConcept C121332964 @default.
• W1935981978 hasConcept C1276947 @default.
• W1935981978 hasConcept C163926583 @default.
• W1935981978 hasConcept C2985973956 @default.
• W1935981978 hasConcept C44870925 @default.
• W1935981978 hasConcept C522846370 @default.
• W1935981978 hasConcept C61696701 @default.
• W1935981978 hasConcept C72591435 @default.
• W1935981978 hasConcept C7910260 @default.
• W1935981978 hasConcept C94915269 @default.
• W1935981978 hasConceptScore W1935981978C111309251 @default.
• W1935981978 hasConceptScore W1935981978C120665830 @default.
• W1935981978 hasConceptScore W1935981978C121332964 @default.
• W1935981978 hasConceptScore W1935981978C1276947 @default.
• W1935981978 hasConceptScore W1935981978C163926583 @default.
• W1935981978 hasConceptScore W1935981978C2985973956 @default.
• W1935981978 hasConceptScore W1935981978C44870925 @default.
• W1935981978 hasConceptScore W1935981978C522846370 @default.
• W1935981978 hasConceptScore W1935981978C61696701 @default.
• W1935981978 hasConceptScore W1935981978C72591435 @default.
• W1935981978 hasConceptScore W1935981978C7910260 @default.
• W1935981978 hasConceptScore W1935981978C94915269 @default.
• W1935981978 hasIssue "6-7" @default.
• W1935981978 hasLocation W19359819781 @default.
• W1935981978 hasLocation W19359819782 @default.
• W1935981978 hasLocation W19359819783 @default.
• W1935981978 hasLocation W19359819784 @default.
• W1935981978 hasOpenAccess W1935981978 @default.
• W1935981978 hasPrimaryLocation W19359819781 @default.
• W1935981978 hasRelatedWork W1618956003 @default.
• W1935981978 hasRelatedWork W1657862823 @default.
• W1935981978 hasRelatedWork W1659720381 @default.
• W1935981978 hasRelatedWork W1911667320 @default.
• W1935981978 hasRelatedWork W2036264599 @default.
• W1935981978 hasRelatedWork W2792169186 @default.
• W1935981978 hasRelatedWork W2804866134 @default.

• next