Construct the emission line galaxy-host halo connection through auto and cross correlations. Gao, H., Jing, Y. P., Zheng, Y., & Xu, K. Technical Report November, 2021. Publication Title: arXiv e-prints ADS Bibcode: 2021arXiv211111657G Type: articlePaper abstract bibtex We investigate the [O\textbackslash,II] emission line galaxy (ELG)-host halo connection via auto and cross correlations, and propose a concise and effective method to populate ELGs in dark matter halos without assuming a parameterized halo occupation distribution (HOD) model. Using the observational data from VIMOS Public Extragalactic Redshift Survey (VIPERS), we measure the auto and cross correlation functions between ELGs selected by [O\textbackslash,II] luminosity and normal galaxies selected by stellar mass. Combining the stellar-halo mass relation (SHMR) derived for the normal galaxies and the fraction of ELGs observed in the normal galaxy population, we demonstrate that we can establish an accurate ELG-halo connection. With the ELG-halo connection, we can accurately reproduce the auto and cross correlation functions of ELGs and normal galaxies both in real-space and in redshift-space, once the satellite fraction is properly reduced. Our method provides a novel strategy to generate ELG mock catalogs for ongoing and upcoming galaxy redshift surveys. We also provide a simple description for the HOD of ELGs.
@techreport{gao_construct_2021,
title = {Construct the emission line galaxy-host halo connection through auto and cross correlations},
url = {https://ui.adsabs.harvard.edu/abs/2021arXiv211111657G},
abstract = {We investigate the [O{\textbackslash},II] emission line galaxy (ELG)-host halo connection via auto and cross correlations, and propose a concise and effective method to populate ELGs in dark matter halos without assuming a parameterized halo occupation distribution (HOD) model. Using the observational data from VIMOS Public Extragalactic Redshift Survey (VIPERS), we measure the auto and cross correlation functions between ELGs selected by [O{\textbackslash},II] luminosity and normal galaxies selected by stellar mass. Combining the stellar-halo mass relation (SHMR) derived for the normal galaxies and the fraction of ELGs observed in the normal galaxy population, we demonstrate that we can establish an accurate ELG-halo connection. With the ELG-halo connection, we can accurately reproduce the auto and cross correlation functions of ELGs and normal galaxies both in real-space and in redshift-space, once the satellite fraction is properly reduced. Our method provides a novel strategy to generate ELG mock catalogs for ongoing and upcoming galaxy redshift surveys. We also provide a simple description for the HOD of ELGs.},
urldate = {2021-12-17},
author = {Gao, Hongyu and Jing, Y. P. and Zheng, Yun and Xu, Kun},
month = nov,
year = {2021},
note = {Publication Title: arXiv e-prints
ADS Bibcode: 2021arXiv211111657G
Type: article},
keywords = {Astrophysics - Astrophysics of Galaxies, Astrophysics - Cosmology and Nongalactic Astrophysics},
}
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