The skewness and kurtosis of the projected density distribution function: Validity of perturbation theory

Astronomy and Astrophysics

Volumn 331, Issue 3, 1998, Pages 829-837

  Gaztanaga E ^a,b   Bernardeau, F ^c  

^a INSTITUT D ESTUDIS ESPACIALS DE CATALUNYA IEEC   (Spain)

^b NASA HEADQUARTERS   (United States)

^c CEA SACLAY   (France)

Author keywords

Cosmic microwave background; Dark matter; Gravitational lensing; Large scale structure of Universe

Indexed keywords

EID: 0039786735     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: None     Document Type: Article

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