Energy spectrum of cosmic-ray electrons at TeV energies.

F, Aharonian; AG, Akhperjanian; de Almeida U, Barres; AR, Bazer-Bachi; Y, Becherini; B, Behera; W, Benbow; K, Bernlöhr; C, Boisson; A, Bochow; V, Borrel; I, Braun; E, Brion; J, Brucker; P, Brun; R, Brucker; T, Bulik; I, Büsching; T, Boutelier; S, Carrigan; PM, Chadwick; A, Charbonnier; RC, Chaves; A, Cheesebrough; LM, Chounet; AC, Clapson; G, Coignet; L, Costamante; M, Dalton; B, Degrange; C, Deil; HJ, Dickinson; A, Djannati-Ataï; W, Domainko; LO, Drury; F, Dubois; G, Dubus; J, Dyks; M, Dyrda; K, Egberts; D, Emmanoulopoulos; P, Espigat; C, Farnier; F, Feinstein; A, Fiasson; G, Fontaine; M, Füsling; S, Gabici; YA, Gallant; L, Gérard; B, Giebels; JF, Glicenstein; B, Glück; P, Goret; C, Hadjichristidis; D, Hauser; M, Hauser; S, Heinz; G, Heinzelmann; G, Henri; G, Hermann; JA, Hinton; A, Hoffmann; W, Hofmann; M, Holleran; S, Hoppe; D, Horns; A, Jacholkowska; Jager OC, de; I, Jung; K, Katarzyński; S, Kaufmann; E, Kendziorra; M, Kerschhaggl; D, Khangulyan; B, Khélifi; D, Keogh; N, Komin; K, Kosack; G, Lamanna; JP, Lenain; T, Lohse; V, Marandon; JM, Martin; O, Martineau-Huynh; A, Marcowith; D, Maurin; TJ, McComb; C, Medina; R, Moderski; E, Moulin; M, Naumann-Godo; Naurois M, de; D, Nedbal; D, Nekrassov; J, Niemiec; SJ, Nolan; S, Ohm; JF, Olive; Oña Wilhelmi E, de; KJ, Orford; JL, Osborne; M, Ostrowski; M, Panter; G, Pedaletti; G, Pelletier; PO, Petrucci; S, Pita; G, Pühlhofer; M, Punch; A, Quirrenbach; BC, Raubenheimer; M, Raue; SM, Rayner; M, Renaud; F, Rieger; J, Ripken; L, Rob; S, Rosier-Lees; G, Rowell; B, Rudak; CB, Rulten; J, Ruppel; V, Sahakian; A, Santangelo; R, Schlickeiser; FM, Schöck; R, Schröder; U, Schwanke; S, Schwarzburg; S, Schwemmer; A, Shalchi; JL, Skilton; H, Sol; D, Spangler; Ł, Stawarz; R, Steenkamp; C, Stegmann; G, Superina; PH, Tam; JP, Tavernet; R, Terrier; O, Tibolla; Eldik C, van; G, Vasileiadis; C, Venter; JP, Vialle; P, Vincent; M, Vivier; HJ, Völk; F, Volpe; SJ, Wagner; M, Ward; AA, Zdziarski; A, Zech

doi:10.1103/physrevlett.101.261104

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Energy spectrum of cosmic-ray electrons at TeV energies.

Shared by NobleBlocks on Dec 1, 2008 • 12:00 AM UTC

Authors:

Aharonian F

Akhperjanian AG

Barres de Almeida U

Abstract

The very large collection area of ground-based gamma-ray telescopes gives them a substantial advantage over balloon or satellite based instruments in the detection of very-high-energy (>600 GeV) cosmic-ray electrons. Here we present the electron spectrum derived from data taken with the High Energy ...

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