Revisiting Marked Galaxy Clustering from a Joint Point Process Perspective
Tsutomu T. Takeuchi (Nagoya University, Institute of Statistical Mathematics)

TL;DR
This paper introduces a joint point process framework for galaxy clustering that captures mark-dependent interactions, providing a more detailed analysis than traditional summary statistics.
Contribution
It formulates galaxies as points with marks in a product space and defines a joint correlation function and diagnostics to analyze mark-dependent clustering.
Findings
The joint pair correlation function $g(r;m_1,m_2)$ describes mark-dependent clustering.
The diagnostic $ riangle_{ind}(r;m_1,m_2)$ quantifies deviations from independence.
Common diagnostics are shown as averaged projections of the joint structure.
Abstract
Marked correlation functions, in which galaxy properties such as luminosity or stellar mass are treated as marks, are widely used to test models of galaxy formation. In astronomy, however, these statistics are typically implemented as summary measures that do not preserve the joint structure of mark pairs conditioned on separation. In this work, we formulate galaxies as points on the product space , where denotes position and a mark, and introduce the joint pair correlation function as the fundamental quantity describing mark-dependent clustering. We further define a diagnostic quantity that locally quantifies deviations from the independence hypothesis relative to spatial clustering alone, thereby providing a projection-free description of which mark pairs are over- or underrepresented at a…
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