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Volumn 328, Issue 5974, 2010, Pages 73-75

Evidence for strong extragalactic magnetic fields from fermi observations of TeV blazars

Author keywords

[No Author keywords available]

Indexed keywords

AMPLIFICATION; COSMIC RAY; ELECTROMAGNETIC FIELD; GAMMA RAY RADIATION; GAUSSIAN METHOD; MAGNETIC FIELD;

EID: 77950486567     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1184192     Document Type: Article
Times cited : (1183)

References (51)
  • 13
    • 42749106516 scopus 로고    scopus 로고
    • A. Lewis, Phys. Rev. 70, 043011 (2004).
    • (2004) Phys. Rev. , vol.70 , pp. 043011
    • Lewis, A.1
  • 22
  • 26
    • 0000755047 scopus 로고
    • R. Plaga, Nature 374, 430 (1995).
    • (1995) Nature , vol.374 , pp. 430
    • Plaga, R.1
  • 34
    • 77950497048 scopus 로고    scopus 로고
    • www-glast.slac.stanford.edu/software/IS/ glast-lat-performance.htm
  • 38
    • 77950485148 scopus 로고    scopus 로고
    • When this paper was ready for publication, we became aware of analysis of the signal from TeV blazars reported by the Fermi collaboration (39 Our analysis is consistent with the one of 139) and extends the results obtained in 139
    • When this paper was ready for publication, we became aware of analysis of the signal from TeV blazars reported by the Fermi collaboration (39). Our analysis is consistent with the one of 139) and extends the results obtained in 139).
  • 40
    • 77950510422 scopus 로고    scopus 로고
    • The cut-off energies of intrinsic spectra of H 2356-309 and 1ES 1101-232 could be so low that the flux of the cascade emission could be below Fermi upper bounds on GeV source flux. This is illustrated in the bottom graph of Fig. 1 for the case of 1ES 1101-1232 See SOM for more details.
    • The cut-off energies of intrinsic spectra of H 2356-309 and 1ES 1101-232 could be so low that the flux of the cascade emission could be below Fermi upper bounds on GeV source flux. This is illustrated in the bottom graph of Fig. 1 for the case of 1ES 1101-1232 See SOM for more details.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.