Can cosmic shear shed light on low cosmic microwave background multipoles?

Physical Review Letters

Volumn 91, Issue 22, 2003, Pages

  Kesden, Michael ^a   Kamionkowski, Marc ^a   Cooray, Asantha ^a  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

COSMIC RAYS; FOURIER TRANSFORMS; GRAPH THEORY; GRAVITATIONAL EFFECTS; INTEGRAL EQUATIONS; MATHEMATICAL MODELS; MONTE CARLO METHODS; PERTURBATION TECHNIQUES; PROBABILITY DISTRIBUTIONS; RANDOM PROCESSES; SPECTRUM ANALYSIS; TEMPERATURE;

COSMIC MICROWAVE BACKGROUND; COSMIC SHEAR PATTERN; SACHS-WOLFE EFFECT; SCALE-INVARIANT POWER SPECTRUM; TEMPERATURE-POLARIZATION PATTERN;

ASTROPHYSICS;

EID: 0347949967     PISSN: 00319007     EISSN: 10797114     Source Type: Journal    
DOI: 10.1103/PhysRevLett.91.221302     Document Type: Article

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