Non-linear corrections to the cosmological matter power spectrum and scale-dependent galaxy bias: Implications for parameter estimation

Journal of Cosmology and Astroparticle Physics

Volumn 2008, Issue 7, 2008, Pages

  Hamann, Jan ^a   Hannestad, Steen ^b   Melchiorri, Alessandro ^c   Wong, Yvonne Y Y ^d  

^a UNIVERSITÉ DE SAVOIE   (France)

^b AARHUS UNIVERSITY   (Denmark)

^c SAPIENZA UNIVERSITY OF ROME   (Italy)

^d MAX PLANCK INSTITUT FÜR PHYSIK   (Germany)

Author keywords

Dark matter; Power spectrum; Semi analytic modelling; Surveys of galaxies

Indexed keywords

EID: 49749141967     PISSN: 14757516     EISSN: 14757516     Source Type: Journal    
DOI: 10.1088/1475-7516/2008/07/017     Document Type: Article

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