Constraining the halo bispectrum in real and redshift space from perturbation theory and non-linear stochastic bias

Monthly Notices of the Royal Astronomical Society

Volumn 450, Issue 2, 2015, Pages 1836-1845

  Kitaura, Francisco Shu ^a   Gil Marín, Héctor ^b   Scóccola, Claudia G ^c,d,e   Chuang, Chia Hsun ^e   Müller, Volker ^a   Yepes, Gustavo ^e   Prada, Francisco ^e,f,g  

^a ASTROPHYSIKALISCHES INSTITUT POTSDAM   (Germany)

^b UNIVERSITY OF PORTSMOUTH   (United Kingdom)

^c INSTITUTO DE ASTROFÍSICA DE CANARIAS   (Spain)

^d UNIVERSIDAD DE LA LAGUNA   (Spain)

^e UNIVERSIDAD AUTÓNOMA DE MADRID   (Spain)

^f CAMPUS OF INTERNATIONAL EXCELLENCE UAM CSIC   (Spain)

^g INSTITUTO DE ASTROFÍSICA DE ANDALUCÍA CSIC   (Spain)

Author keywords

Catalogues; Galaxies: clusters: general; Galaxies: statistics; Large scale structure of Universe

Indexed keywords

GALAXIES; HIGHER ORDER STATISTICS; PERTURBATION TECHNIQUES; POWER SPECTRUM; PROBABILITY DENSITY FUNCTION; STOCHASTIC SYSTEMS; UNCERTAINTY ANALYSIS;

BISPECTRA; CATALOG; GALAXIES: CLUSTERS: GENERAL; GALAXIES: STATISTICS; LARGE SCALE STRUCTURE OF UNIVERSE; NUMBER DENSITY; PERTURBATION THEORY; POWER-SPECTRA; PROBABILITY DISTRIBUTION FUNCTIONS; RED SHIFT;

DISTRIBUTION FUNCTIONS;

EID: 84938099086     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1093/mnras/stv645     Document Type: Article

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