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Volumn 315, Issue 5820, 2007, Pages 1822-1824

Early optical polarization of a gamma-ray burst afterglow

Author keywords

[No Author keywords available]

Indexed keywords

ELECTROMAGNETIC FIELD; GAMMA RAY RADIATION; MAGNETIC FIELD; OPTICAL PROPERTY; POLARIZATION;

EID: 34147200078     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1138484     Document Type: Article
Times cited : (89)

References (32)
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    • 0344873760 scopus 로고    scopus 로고
    • J. Greiner et al., Nature 426, 157 (2003).
    • (2003) Nature , vol.426 , pp. 157
    • Greiner, J.1
  • 21
    • 34147201176 scopus 로고    scopus 로고
    • Materials and methods are available as supporting material on Science Online.
    • Materials and methods are available as supporting material on Science Online.
  • 22
    • 34147210576 scopus 로고    scopus 로고
    • E. Molinari et al., http://arxiv.org/abs/astro-ph/0612607 (2006).
    • (2006)
    • Molinari, E.1
  • 32
    • 34147193109 scopus 로고    scopus 로고
    • We thank S. Covino for useful discussions during the initial stages of the RINGO project. RINGO is a Liverpool Telescope fast-track instrument internally funded by the Astrophysics Research Institute of Liverpool John Moores University. The Liverpool Telescope is operated on the island of La Palma, the Canary Islands, by Liverpool John Moores University at the Observatorio del Roque de los Muchachos of the Institute de Astrofisica de Canarias. C.G.M. thanks the Royal Society for financial support
    • We thank S. Covino for useful discussions during the initial stages of the RINGO project. RINGO is a Liverpool Telescope fast-track instrument internally funded by the Astrophysics Research Institute of Liverpool John Moores University. The Liverpool Telescope is operated on the island of La Palma, the Canary Islands, by Liverpool John Moores University at the Observatorio del Roque de los Muchachos of the Institute de Astrofisica de Canarias. C.G.M. thanks the Royal Society for financial support.


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.