Revisiting the WMAP-NVSS angular cross correlation. A skeptic's view

Astronomy and Astrophysics

Volumn 520, Issue 14, 2010, Pages

  Hernandez Monteagudo C ^a  

^a MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

Author keywords

cosmic microwave background; large scale structure of Universe

Indexed keywords

ANGULAR CORRELATIONS; ANGULAR SCALE; COSMIC MICROWAVE BACKGROUNDS; CROSS CORRELATIONS; FOURIER SPACE; GRAVITATIONAL POTENTIAL; HIGH-REDSHIFT; LARGE SCALE STRUCTURE OF UNIVERSE; MODEL PREDICTION; MULTIPOLES; PIXEL SIZE; POINT SOURCES; RADIO GALAXIES; RADIO SOURCES; SOURCE POPULATION; VERY LARGE ARRAYS;

COMPUTER SIMULATION; CORRELATION METHODS; GALAXIES; LIBRARIES; RADIO ASTRONOMY; SIGNAL TO NOISE RATIO; SURVEYS;

COSMOLOGY;

EID: 77957950494     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913344     Document Type: Article

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