The Galaxy Count Correlation Function in Redshift Space Revisited

In the near future, cosmology will enter the wide and deep galaxy survey era, enabling high-precision studies of the large-scale structure of the universe in three dimensions. To test cosmological models and determine their parameters accurately, it is necessary to use data with exact theoretical ex...

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Veröffentlicht in:	The Astrophysical journal 2017-08, Vol.845 (1), p.28, Article 28
Hauptverfasser:	Campagne, J.-E., Plaszczynski, S., Neveu, J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Addition theorem Astronomical models Astrophysics ASTROPHYSICS, COSMOLOGY AND ASTRONOMY Closed form solutions Correlation CORRELATION FUNCTIONS CORRELATIONS COSMOLOGICAL MODELS COSMOLOGY cosmology: theory DISTANCE Exact solutions Expansion FLUCTUATIONS GALAXIES GRAVITATIONAL LENSES Large scale structure of the universe large-scale structure of universe LEGENDRE POLYNOMIALS LIMBS methods: numerical MULTIPOLES Parameters Physics Polynomials RED SHIFT Relativistic effects RELATIVISTIC RANGE Software SPACE SPECTRA SPHERICAL CONFIGURATION Spherical harmonics Stars & galaxies Three dimensional models UNIVERSE Variation
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