Understanding the relativistic overdensity of galaxy surveys
Didam Duniya (BIUST, Cape Town, AIMS, Western Cape)

TL;DR
This paper revisits the relativistic overdensity in galaxy surveys, providing a comprehensive and adaptable framework that incorporates both number-count and cosmic magnification effects, improving analysis accuracy for different sample types.
Contribution
It introduces a consistent approach to include relativistic effects in galaxy survey overdensity calculations, generalizing previous expressions and enabling application to various data sample types.
Findings
Unified expression for total observed overdensity incorporating relativistic effects.
Flexible framework applicable to flux-limited and volume-limited samples.
Enhanced accuracy in relativistic galaxy survey analyses.
Abstract
The main goal of galaxy surveys is to map the distribution of the galaxies, for the purpose of understanding the properties of this distribution and its implications for the content and the evolution of the universe. However, in order to realise the full potential of these surveys, we need to ensure that we are using the correct analysis: a relativistic analysis, which has been widely studied recently. In this work, the known relativistic overdensity of galaxy surveys is re-examined. Unlike in previous works, a consistent approach for incorporating both the relativistic number-count overdensity and the relativistic cosmic magnification overdensity in the total observed overdensity of a generic survey, is presented. Since in practice, analyses are often done for specific sample types (flux-limited or volume-limited) the approach in this work allows for the total observed overdensity to…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Cosmology and Gravitation Theories · Astrophysics and Cosmic Phenomena
