메뉴 건너뛰기




Volumn 413, Issue 3, 2004, Pages 833-842

Using peak distribution of the cosmic microwave background for WMAP and Planck data analysis: Formalism and simulations

Author keywords

Cosmic microwave background; Cosmology; Methods: numerical

Indexed keywords

ACOUSTIC NOISE; ACOUSTIC WAVES; ALGORITHMS; ANISOTROPY; COMPUTATIONAL METHODS; COMPUTER SIMULATION; CORRELATION METHODS; COSMIC RAYS; DATA REDUCTION; FOURIER TRANSFORMS; ITERATIVE METHODS; NUMERICAL METHODS; PHOTONS; ROBUSTNESS (CONTROL SYSTEMS); STATISTICAL METHODS; THRESHOLD VOLTAGE;

EID: 10744226814     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20031583     Document Type: Article
Times cited : (10)

References (36)
  • 8
    • 0012226408 scopus 로고    scopus 로고
    • Germany, 31st July - 4th August 2000, ed. by A. J. Banday, S. Zaroubi, & M. Bartelmann (Heidelberg: Springer-Verlag)
    • Hinshaw, G. 2000, Proceedings of the MPA/ESO/MPE Workshop "Mining the Sky", held at Garching, Germany, 31st July - 4th August 2000, ed. by A. J. Banday, S. Zaroubi, & M. Bartelmann (Heidelberg: Springer-Verlag), 2001, 447
    • (2000) Proceedings of the MPA/ESO/MPE Workshop "Mining the Sky", Held at Garching , pp. 447
    • Hinshaw, G.1
  • 14
    • 0001815457 scopus 로고
    • Kaiser, N. 1984, ApJ, 282, L9
    • (1984) ApJ , vol.282
    • Kaiser, N.1
  • 26
    • 0742329527 scopus 로고    scopus 로고
    • 2003 [astro-ph/0304513]
    • Penn, U. 2003 [astro-ph/0304513]
    • Penn, U.1


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.