An optimally weighted estimator of the linear power spectrum disentangling the growth of density perturbations across galaxy surveys

DOI10.1088/1475-7516/2017/04/029OpenAlexW3104342517MaRDI QIDQ5024246

D. Sorini

Publication date: 28 January 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1612.00725

zbMATH Keywords

power spectrumcosmological perturbation theorygalaxy clusteringcosmological parameters from LSS

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Uses Software

• CAMB

Cites Work

• Halo models of large scale structure
• Large-scale structure of the universe and cosmological perturbation theory
• A microscopic, non-equilibrium, statistical field theory for cosmic structure formation

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