activity
20092026
most citedThe Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III

2.5k citations · 14.3k across the 73 of their papers we have counts for

collaborators

73 papers

astro-ph.GA2026

Weak Evolution of Cosmic Atomic Hydrogen over the Past 4.5 Billion Years

Chuan-Peng Zhang, Hong Guo, Yizhou Gu +49

The cosmic star formation rate density (CSFRD) has declined sharply toward the present day, but the roles of the atomic and molecular gas reservoirs remain uncertain. We measure th…

astro-ph.GA2023★ 1 cited

NeutralUniverseMachine: An Empirical Model for the Evolution of HI and H Gas in the Universe

Hong Guo, Jing Wang, Michael G. Jones +1

Accurately modeling the cold gas content in the universe is challenging for current theoretical models. We propose a new empirical model NeutralUniverseMachine for the evolution of…

astro-ph.CO2023★ 6 cited

Small scale clustering of BOSS galaxies: dependence on luminosity, color, age, stellar mass, specific star formation rate and other properties

Zhongxu Zhai, Will J. Percival, Hong Guo

We measure and analyze galaxy clustering and the dependence on luminosity, color, age, stellar mass and specific star formation rate using Baryon Oscillation Spectroscopic Survey (…

astro-ph.CO2023

Abundance matching analysis of the emission line galaxy sample in the extended Baryon Oscillation Spectroscopic Survey

Sicheng Lin, Jeremy L. Tinker, Michael R. Blanton +4

We present the measurements of the small-scale clustering for the emission line galaxy (ELG) sample from the extended Baryon Oscillation Spectroscopic Survey (eBOSS) in the Sloan D…

astro-ph.CO2023★ 11 cited

Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing

Juliana Kwan, Shun Saito, Alexie Leauthaud +7

We construct accurate emulators for the projected and redshift space galaxy correlation functions and excess surface density as measured by galaxy-galaxy lensing, based on Halo Occ…

astro-ph.CO2023★ 37 cited

Constraints on from a full-scale and full-shape analysis of redshift-space clustering and galaxy-galaxy lensing in BOSS

Johannes U. Lange, Andrew P. Hearin, Alexie Leauthaud +5

We present a novel simulation-based cosmological analysis of galaxy-galaxy lensing and galaxy redshift-space clustering. Compared to analysis methods based on perturbation theory,…

astro-ph.GA2022★ 27 cited

Effects of Active Galactic Nucleus Feedback on Cold Gas Depletion and Quenching of Central Galaxies

Wenlin Ma, Kexin Liu, Hong Guo +5

We investigate the influence of active galactic nucleus (AGN) feedback on the galaxy cold gas content and its connection to galaxy quenching in three hydrodynamical simulations of…

astro-ph.GA2022★ 7 cited

Galaxy-halo size relation from Sloan Digital Sky Survey Data Release 7 and the ELUCID simulation

Youcai Zhang, Xiaohu Yang, Hong Guo

Based on galaxies in the Sloan Digital Sky Survey Data Release 7 (SDSS DR7) and dark matter haloes in the dark matter only, cosmological and constrained ELUCID simulation, we inves…

astro-ph.GA2022★ 2 cited

Theoretical Models of the Atomic Hydrogen Content in Dark Matter Halos

Zhixing Li, Hong Guo, Yi Mao

Atomic hydrogen (H I) gas, mostly residing in dark matter halos after cosmic reionization, is the fuel for star formation. Its relation with properties of host halo is the key to u…

astro-ph.GA2022★ 24 cited

SDSS-IV MaNGA: Global Properties of Kinematically Misaligned Galaxies

Yuren Zhou, Yanmei Chen, Yong Shi +6

We select 456 gas-star kinematically misaligned galaxies from the internal Product Launch-10 of MaNGA survey, including 74 star-forming (SF), 136 green-valley (GV) and 206 quiescen…

astro-ph.GA2022★ 13 cited

Cold Gas Reservoirs of Low- and High-mass Central Galaxies Differ in Response to Active Galactic Nucleus Feedback

Hong Guo, Michael G. Jones, Jing Wang

The growth of supermassive black holes, especially the associated state of active galactic nuclei (AGNs), is generally believed to be the key step in regulating star formation in m…

astro-ph.GA2022★ 25 cited

Evidence of Galaxy Assembly Bias in SDSS DR7 Galaxy Samples from Count Statistics

Kuan Wang, Yao-Yuan Mao, Andrew R. Zentner +4

We present observational constraints on the galaxy-halo connection, focusing particularly on galaxy assembly bias, from a novel combination of counts-in-cylinders statistics, $P(N_…

astro-ph.CO2022★ 59 cited

The Aemulus Project V: Cosmological constraint from small-scale clustering of BOSS galaxies

Zhongxu Zhai, Jeremy L. Tinker, Arka Banerjee +6

We analyze clustering measurements of BOSS galaxies using a simulation-based emulator of two-point statistics. We focus on the monopole and quadrupole of the redshift-space correla…

astro-ph.CO2022★ 6 cited

A Pair of Early- and Late-Forming Galaxy Cluster Samples: a Novel Way of Studying Halo Assembly Bias Assisted by a Constrained Simulation

Yen-Ting Lin, Hironao Miyatake, Hong Guo +4

The halo assembly bias, a phenomenon referring to dependencies of the large-scale bias of a dark matter halo other than its mass, is a fundamental property of the standard cosmolog…

astro-ph.GA2022★ 5 cited

The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar and APOGEE-2 Data

Abdurro'uf, Katherine Accetta, Conny Aerts +337

This paper documents the seventeenth data release (DR17) from the Sloan Digital Sky Surveys; the fifth and final release from the fourth phase (SDSS-IV). DR17 contains the complete…

astro-ph.GA2021★ 16 cited

Connections between galaxy properties and halo formation time in the cosmic web

Youcai Zhang, Xiaohu Yang, Hong Guo

By linking galaxies in Sloan Digital Sky Survey (SDSS) to subhaloes in the ELUCID simulation, we investigate the relation between subhalo formation time and the galaxy properties,…

astro-ph.GA2021

The clustering of galaxies in the DESI imaging legacy surveys DR8: I. the luminosity and color dependent intrinsic clustering

Zhaoyu Wang, Haojie Xu, Xiaohu Yang +5

In a recent study, we developed a method to model the impact of photometric redshift uncertainty on the two-point correlation function (2PCF). In this method, we can obtain both th…

astro-ph.GA2021★ 38 cited

Star Formation and Quenching of Central Galaxies from Stacked HI Measurements

Hong Guo, Michael G. Jones, Jing Wang +1

We quantitatively investigate the dependence of central galaxy HI mass () on the stellar mass (), halo mass (), star formation rate (SFR), and centra…

astro-ph.CO2021★ 5 cited

On the Constraints of Galaxy Assembly Bias in Velocity Space

Kevin S. McCarthy, Zheng Zheng, Hong Guo +2

If the formation of central galaxies in dark matter haloes traces the assembly history of their host haloes, in haloes of fixed mass, central galaxy clustering may show dependence…

astro-ph.CO2021★ 68 cited

Five-percent measurements of the growth rate from simulation-based modelling of redshift-space clustering in BOSS LOWZ

Johannes U. Lange, Andrew P. Hearin, Alexie Leauthaud +3

We use a simulation-based modelling approach to analyse the anisotropic clustering of the BOSS LOWZ sample over the radial range to $63 \, h^{-1} \,…

astro-ph.GA2020★ 96 cited

An Extended Halo-based Group/Cluster finder: application to the DESI legacy imaging surveys DR8

Xiaohu Yang, Haojie Xu, Min He +20

We extend the halo-based group finder developed by \citet[][]{Yang2005a} to use data {\it simultaneously} with either photometric or spectroscopic redshifts. A mock galaxy redshift…

astro-ph.CO2020★ 40 cited

On the halo-mass and radial scale dependence of the lensing is low effect

Johannes U. Lange, Alexie Leauthaud, Sukhdeep Singh +4

The canonical CDM cosmological model makes precise predictions for the clustering and lensing properties of galaxies. It has been shown that the lensing amplitude of galaxies in…

astro-ph.CO2020★ 67 cited

Evidence for galaxy assembly bias in BOSS CMASS redshift-space galaxy correlation function

Sihan Yuan, Boryana Hadzhiyska, Sownak Bose +2

Building accurate and flexible galaxy-halo connection models is crucial in modeling galaxy clustering on non-linear scales. Recent studies have found that halo concentration by its…

astro-ph.GA2020★ 4 cited

Populating HI gas in dark matter halos: I. method

Yi Lu, Xiaohu Yang, Chengze Liu +4

We combine data from the Sloan Digital Sky Survey (SDSS) and the Arecibo Legacy Fast ALFA Survey (ALFALFA) to establish an empirical model for the HI gas content within dark matter…