Systematic errors in weighted 2-point correlation functions: An application to interaction-induced star formation
Aday R. Robaina, Eric F. Bell

TL;DR
Weighted correlation functions are useful for galaxy property analysis but can dilute and smear true radial dependencies, requiring careful correction using mock catalogs to avoid misinterpretation of interaction effects.
Contribution
This paper demonstrates how weighted correlation functions can distort true radial dependencies in galaxy properties and provides a quantitative framework to correct for these effects.
Findings
Weighted correlation functions dilute the magnitude of radial property dependence.
Artificial enhancements can appear at larger radii due to pair matching effects.
Observed SFR enhancements match the simulated dilution effects.
Abstract
Weighted correlation functions are an increasingly important tool for understanding how galaxy properties depend on their separation from each other. We use a mock galaxy sample drawn from the Millenium simulation, assigning weights using a simple prescription to illustrate and explore how well a weighted correlation function recovers the true radial dependence of the input weights. We find that the use of a weighted correlation function results in a dilution of the magnitude of any radial dependence of properties and a smearing out of that radial dependence in radius, compared to the input behavior. We present a quantitative discussion of the dilution in the magnitude of radial dependence in properties in the special case of a constant enhancement at r < rc. In this particular case where there was a SFR enhancement at small radius r < rc = 35 kpc, the matching of one member of an…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Advanced Statistical Methods and Models · Astronomy and Astrophysical Research
