Is there a need and another way to measure the cosmic microwave background temperature more accurately?

Astronomy and Astrophysics

Volumn 478, Issue 2, 2008, Pages

  Chluba, J ^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: cosmological parameters; Cosmology: theory

Indexed keywords

ABSOLUTE MEASUREMENTS; ANGULAR SCALE; COSMIC MICROWAVE BACKGROUNDS; COSMOLOGICAL PARAMETERS; COSMOLOGY: COSMIC MICROWAVE BACKGROUND; COSMOLOGY: COSMOLOGICAL PARAMETERS; COSMOLOGY: THEORY; FREE ELECTRON; FREQUENCY-DEPENDENT; LOW FREQUENCY; POWER-SPECTRA; QUASI-PERIODIC; RED-SHIFTED; SPECIFIC ENTROPY;

COSMIC RAY MEASUREMENT; MICROWAVES;

COSMOLOGY;

EID: 43049106612     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20078200     Document Type: Article

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