Quantifying Environmental Effects on Galaxy Properties using Non-spherical Voids Identified from SDSS DR7
Abstract
Cosmic voids provide a distinct low-density region for studying the environmental effects of galaxy properties. Using the SDSS DR7 catalog, we identify non-spherical voids via Voronoi tessellation and the watershed algorithm, and classify void galaxies based on their local volume. We compare and find that void galaxies classified by this method are systematically less massive, fainter, bluer, and have higher specific star formation rate (sSFR) than non-void galaxies and all galaxy samples. We then divide void and non-void galaxies into stellar mass bins to focus on the environmental dependence of g−r color and sSFR. By further classifying galaxies into blue/red and star-forming/quiescent populations, we calculate the ratio of blue to red and star-forming to quiescent for void and non-void galaxies separately. Comparing the ratio of the void value to the non-void value for both metrics presents an overall decreasing trend with stellar mass M* over the 9.4−10.4 range in log[M*/M⊙], indicating a stronger environmental effect in lower-mass systems. These results show that our classification of void galaxies in non-spherical voids based on local volume offers a robust approach for quantifying the influence of underdense environments on galaxy evolution.
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BibTeX
@misc{song2026quantifying,
title = {{Quantifying Environmental Effects on Galaxy Properties using Non-spherical Voids Identified from SDSS DR7}},
author = {Yingxiao Song and Xiaohu Yang and Yan Gong and Haitao Miao and Xingchen Zhou and Yizhou Gu and Yingjie Peng},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2607.07268},
eprint = {2607.07268},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2607.07268},
}
RIS
TY - UNPB
TI - Quantifying Environmental Effects on Galaxy Properties using Non-spherical Voids Identified from SDSS DR7
AU - Yingxiao Song
AU - Xiaohu Yang
AU - Yan Gong
AU - Haitao Miao
AU - Xingchen Zhou
AU - Yizhou Gu
AU - Yingjie Peng
PY - 2026
DA - 2026/09/16
PB - arXiv
DO - 10.48550/arxiv.2607.07268
UR - https://arxiv.org/abs/2607.07268
AB - Cosmic voids provide a distinct low-density region for studying the environmental effects of galaxy properties. Using the SDSS DR7 catalog, we identify non-spherical voids via Voronoi tessellation and the watershed algorithm, and classify void galaxies based on their local volume. We compare and find that void galaxies classified by this method are systematically less massive, fainter, bluer, and have higher specific star formation rate (sSFR) than non-void galaxies and all galaxy samples. We then divide void and non-void galaxies into stellar mass bins to focus on the environmental dependence of g−r color and sSFR. By further classifying galaxies into blue/red and star-forming/quiescent populations, we calculate the ratio of blue to red and star-forming to quiescent for void and non-void galaxies separately. Comparing the ratio of the void value to the non-void value for both metrics presents an overall decreasing trend with stellar mass M_* over the 9.4−10.4 range in log[M_*/M_⊙], indicating a stronger environmental effect in lower-mass systems. These results show that our classification of void galaxies in non-spherical voids based on local volume offers a robust approach for quantifying the influence of underdense environments on galaxy evolution.
ER -