Missing baryons, bulk flows, and the E-mode polarization of the cosmic microwave background

Astronomy and Astrophysics

Volumn 490, Issue 1, 2008, Pages 25-29

  Hernandez Monteagudo C ^a   Sunyaev, R A ^a,b  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^b Russian Academy of Sciences   (Russian Federation)

Author keywords

Cosmology: cosmic microwave background; Cosmology: large scale structure of Universe

Indexed keywords

CORRELATION METHODS; COSMOLOGY; PERTURBATION TECHNIQUES; POLARIZATION;

ALL-SKY; CMB EXPERIMENTS; COSMIC MICROWAVE BACKGROUND; COSMOLOGICAL PERTURBATIONS; COSMOLOGY: COSMIC MICROWAVE BACKGROUND; COSMOLOGY: LARGE-SCALE STRUCTURE OF UNIVERSE; CROSS CORRELATIONS; GALAXY GROUPS; GRAVITATIONAL ATTRACTIONS; LINEAR POTENTIALS; POISSONIAN; POLARIZATION FIELD; RED-SHIFTS; REIONIZATION; SUPERCLUSTERS; THOMSON SCATTERING;

FERMIONS;

EID: 53849099675     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810204     Document Type: Article

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