Optimising large galaxy surveys for ISW detection

Astronomy and Astrophysics

Volumn 485, Issue 2, 2008, Pages 395-401

  Douspis, M ^a   Castro, G ^b   Caprini, C ^c   Aghanim, N ^a  

^a UNIVERSITÉ PARIS SUD   (France)

^b INSTITUTO SUPERIOR TÉCNICO   (Portugal)

^c CEA SACLAY   (France)

Author keywords

Cosmology: cosmic microwave background; Cosmology: cosmological parameters; Surveys

Indexed keywords

ASTROPHYSICS; CORRELATION METHODS; COSMOLOGY; DIFFERENCE EQUATIONS; DIFFERENTIATION (CALCULUS); EQUATIONS OF STATE; GALAXIES; STANDARDS; SURVEYS;

(PL) PROPERTIES; COSMIC MICROWAVE BACKGROUND (CMG); COSMOLOGICAL PARAMETERS; CROSS CORRELATIONS; CROSS-CORRELATION CONSTRAINTS; DARK ENERGY; ENERGY MODELING; EQUATION OF STATE (EOS); GALAXY DISTRIBUTION; HIGH REDSHIFT; LARGE-SCALE STRUCTURES; MATRIX ANALYSIS; RED SHIFTING; SIGNAL TO NOISE ANALYSIS; STRENGTH (IGC: D5/D6);

POWER GENERATION;

EID: 46649103070     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200809499     Document Type: Article

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