Measuring Galaxy Abundance and Clustering at High Redshift from Incomplete Spectroscopic Data: Tests on Mock Catalogs

Measuring Galaxy Abundance and Clustering at High Redshift from Incomplete Spectroscopic Data: Tests on Mock Catalogs

The number density and correlation function of galaxies are two key quantities to characterize the distribution of the observed galaxy population. High- z spectroscopic surveys, which usually involve complex target selection and are incomplete in redshift sampling, present both opport...

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Bibliographic Details
Main Authors:	Jiacheng Meng, Cheng Li, H. J. Mo, Yangyao Chen, Kai Wang
Format:	Article
Language:	English
Published:	IOP Publishing 2024-01-01
Series:	The Astrophysical Journal
Subjects:	Galaxy abundances Two-point correlation function Redshift surveys High-redshift galaxies
Online Access:	https://doi.org/10.3847/1538-4357/ad2931

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