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Volumn 297, Issue 1-4, 2005, Pages 245-255

Status and first results of the magic telescope

Author keywords

Cherenkov telescope; MAGIC; Very high energy gamma ray

Indexed keywords


EID: 17744391819     PISSN: 0004640X     EISSN: None     Source Type: Journal    
DOI: 10.1007/s10509-005-7627-5     Document Type: Conference Paper
Times cited : (24)

References (9)
  • 5
    • 0002063652 scopus 로고
    • The MAGIC telescope project based on a 17 m diameter parabolic solar concentrator
    • M. Cresti (eds.), Padova, Italy
    • Lorenz, E., et al.: 1995, in: M. Cresti (eds.), The MAGIC Telescope Project Based on a 17 m Diameter Parabolic Solar Concentrator, Proceedings of the Workshop: Towards a Major Atmospheric Cherenkov Detector IV, Padova, Italy, p. 277.
    • (1995) Proceedings of the Workshop: Towards aMajor Atmospheric Cherenkov Detector IV , pp. 277
    • Lorenz, E.1
  • 6
    • 17744374248 scopus 로고    scopus 로고
    • Extending The Cherenkov Technique Down To An Energy Threshold of A Few GeV: The Ultimate Instrument For Ground-Based Gamma-Ray Astronomy, Tokyo
    • Merck, M., et al.: 2003, in: Extending The Cherenkov Technique Down To An Energy Threshold of A Few GeV: The Ultimate Instrument For Ground-Based Gamma-Ray Astronomy, Proceedings of the International Cosmic Ray Conference, Tokyo.
    • (2003) Proceedings of the International Cosmic Ray Conference
    • Merck, M.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.