TL;DR
This paper develops a methodology to measure baryon acoustic oscillations (BAO) from galaxy voids, identifying optimal void populations and demonstrating the first BAO detection from voids in observational data.
Contribution
It introduces a new approach to measure BAO signals from voids, including void classification by size and a cleaning procedure, validated on mock catalogues and applied to real data.
Findings
First robust detection of BAOs in void correlation functions
Void populations with zero large-scale bias yield the strongest BAO signal
Methodology effectively accounts for survey geometry and selection effects
Abstract
We investigate the necessary methodology to optimally measure the baryon acoustic oscillation (BAO) signal, from voids based on galaxy redshift catalogues. To this end, we study the dependency of the BAO signal on the population of voids classified by their sizes. We find for the first time the characteristic features of the correlation function of voids including the first robust detection of BAOs in mock galaxy catalogues. These show an anti-correlation around the scale corresponding to the smallest size of voids in the sample (the void exclusion effect), and dips at both sides of the BAO peak, which can be used to determine the significance of the BAO signal without any priori model. Furthermore, our analysis demonstrates that there is a scale dependent bias for different populations of voids depending on the radius, with the peculiar property that the void population with the…
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