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Volumn 47, Issue 8, 2003, Pages 741-745

The shape of the CMB power spectrum

Author keywords

Cosmic microwave background anisotropies; Observations; Phenomenology

Indexed keywords


EID: 0242319617     PISSN: 13876473     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.newar.2003.07.027     Document Type: Short Survey
Times cited : (1)

References (12)
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    • Bridle, S.L.1
  • 3
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    • Grainge, K. et al., 2002. Available from (arXiv:astro-ph/0212495) (preprint)
    • (2002)
    • Grainge, K.1
  • 5
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    • Available from (arXiv:astro-ph/0212289) (preprint)
    • Kuo, T.T.S. et al., 2002. Available from (arXiv:astro-ph/0212289) (preprint)
    • (2002)
    • Kuo, T.T.S.1
  • 9
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    • Pearson, T.J. et al., 2002. Available from (arXiv:astro-ph/0205388) (preprint)
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  • 10
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    • Available from (arXiv:stro-ph/0212229) (preprint)
    • Ruhl, J.E. et al., 2002. Available from (arXiv:stro-ph/0212229) (preprint)
    • (2002)
    • Ruhl, J.E.1
  • 11
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    • Available from (arXiv:astro-ph/0302209) (preprint)
    • Spergel, D.N. et al., 2003. Available from (arXiv:astro-ph/0302209) (preprint)
    • (2003)
    • Spergel, D.N.1
  • 12
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    • Available from (arXiv:astro-ph/0302218) (preprint)
    • Verde, L. et al., 2003. Available from (arXiv:astro-ph/0302218) (preprint)
    • (2003)
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.