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Statistical analysis of galaxy surveys ― I. Robust error estimation for two-point clustering statistics

Author
NORBERG, P1 ; BAUGH, C. M2 ; GAZTANAGA, E3 ; CROTON, D. J4 5
[1] SUPA†, Institute for Astronomy, University of Edinburgh, Royal Observatory, Blackford Hill, Edinburgh EH93HJ, United Kingdom
[2] Institute for Computational Cosmology, Department of Physics, University of Durham, South Road, Durham DH1 3LE, United Kingdom
[3] Instituto de Ciencias del Espacio (IEEC/CSIC), F. de Ciencias UAB, Torre C5- Par-2a, Bellaterra, 08193 Barcelona, Spain
[4] Department of Astronomy, University of California, Berkeley, CA, 94720, United States
[5] Centre for Astrophysics and Supercomputing, Swinburne University of Technology, Mail H39, PO Box 218, Hawthorn, Victoria, 3122, Australia
Source

Monthly notices of the Royal Astronomical Society (Print). 2009, Vol 396, Num 1, pp 19-38, 20 p ; ref : 1/2 p

CODEN
MNRAA4
ISSN
0035-8711
Scientific domain
Astronomy earth cosmic environment
Publisher
Wiley-Blackwell, Malden, MA
Publication country
United States
Document type
Article
Language
English
Author keyword
cosmology: theory galaxies: statistics large-scale structure of Universe
Keyword (fr)
Agencement galaxies Analyse statistique Bootstrap Cosmologie Déplacement vers le rouge Estimateur Fonction corrélation Galaxies Matière sombre Matrice covariance Modèle Simulation numérique Structure grande échelle Système n corps Vecteur propre
Keyword (en)
Galaxies clustering Statistical analysis Bootstrap Cosmology Red shift Estimator Correlation functions Galaxies Dark matter Covariance matrices Models Digital simulation Large-scale structure N body system Eigenvectors
Keyword (es)
Disposición galaxias Bootstrap Estimador Modelo Sistema n cuerpos
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
21534191

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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