HM
Houjun Mo
astro-ph.GAastro-phastro-ph.COastro-ph.SRcond-mat.str-el
On Valency
published · living versionsW_nh624gpf·v1 · currentpublished
An Extended Halo-based Group/Cluster finder: application to the DESI legacy imaging surveys DR8
with Xiaohu Yang, Haojie Xu, Min He, Yizhou Gu +18
1 version
W_2xexpnbc·v1published
Preprints & journals
211 papers in the corpus · 1993–2026Fountain pattern of baryon cycle revealed in galaxy ecosystems2609.21374v1 · Chengyu Ma, Yangyao Chen, Enci Wang et al.2026 · 0 citationsarXiv
ELUCID. IX. Recovering the Substructures and History of the Coma Cluster2609.20442v2 · Xiong Luo, Huiyuan Wang, Weiguang Cui et al.2026 · 0 citationsarXiv
Massive Galaxy Halos Contain Less Inner Dark Matter Than Predicted2609.19132v1 · Yu-Chen Wang, Yingjie Peng, Xiaohu Yang et al.2026 · 0 citationsarXiv
Reconstructing the Projected Dark Matter Field across 0.1-100 Mpc Scales from the SDSS Survey2609.19295v1 · Kunyao Zhao, Yingjie Peng, Dingyi Zhao et al.2026 · 0 citationsarXiv
No Detectable One-halo Galactic Conformity Signal with Halo-mass Estimates Consistent with Weak-lensing Constraints2609.11313v1 · Dingyi Zhao, Yingjie Peng, Luis C. Ho et al.2026 · 0 citationsarXiv
ELUCID-DESI II. Revealing dark matter mass, tidal, and velocity (MTV) fields using galaxy group phase information2608.26668v1 · Qingyang Li, Xiaohu Yang, Wensheng Hong et al.2026 · 0 citationsarXiv
Evidence for the transformation from lenticular to spiral galaxies2608.25673v1 · Mengkui Zhou, Huiyuan Wang, Ran Li et al.2026 · 0 citationsarXiv
An emerging baryon cycle in a galaxy 500 million years after the Big Bang2608.09813v1 · Shengzhe Wang, Xin Wang, Hang Zhou et al.2026 · 0 citationsarXiv
Satellite quenching by radio jets of central galaxies in galaxy groups2607.02801v1 · Yijun Wang, Tao Wang, Dingyi Zhao et al.2026 · 0 citationsarXiv
Super-Eddington accretion of black holes in early nuclear bursts gives birth to Little Red Dots2605.31077v3 · Yangyao Chen, Houjun Mo2026 · 1 citationApJL 1007 (2026) L28
Galaxy populations in groups and clusters-II. Conditional luminosity functions at redshifts from z~1 to z~02604.04794v2 · Ce Gao, Cheng Li, Houjun Mo et al.2026 · 0 citationsMon Not R Astron Soc (2026)
A Bending in the Size-mass Relation of Star-forming Galaxies across at a Critical Stellar Mass of Revealed by JWST2603.22239v3 · Longyue Chen, Tao Wang, Hanwen Sun et al.2026 · 2 citationsarXiv
Interpreting the strong clustering of ultra-diffuse galaxies by halo spin bias2512.17742v2 · Qinglin Ma, Cheng Li, Yangyao Chen et al.2025 · 0 citationsarXiv
Connection between galaxy morphology and dark-matter halo structure II: predicting disk structure from dark-matter halo properties2512.13822v2 · Jinning Liang, Fangzhou Jiang, Houjun Mo et al.2025 · 1 citationarXiv
Radio AGN feedback sustains quiescence only in a minority of massive galaxies2511.06037v2 · Huiling Liu, Yan Lu, Hui Hong et al.2025 · 0 citationsarXiv
What is the True HI Gas Content in Massive Quiescent Galaxies in the Local Universe?2510.15145v2 · Xiao Li, Cheng Li, Cheng Cheng et al.2025 · 0 citationsarXiv
Galaxy Metallicity Gradients in the Reionization Epoch from the FIRE-2 Simulations2510.08997v2 · Xunda Sun, Xin Wang, Fangzhou Jiang et al.2025 · 1 citationarXiv
Two-phase formation of galaxies: the coevolution between galaxies and dark matter halos2509.16138v3 · Qinglin Ma, Yangyao Chen, Houjun Mo2025 · 1 citationMon Not R Astron Soc (2026)
A two-phase model of galaxy formation: IV. Seeding and growing supermassive black holes in dark matter halos2509.03283v3 · Yangyao Chen, Houjun Mo, Huiyuan Wang2025 · 1 citationarXiv
The Bigfoot: A footprint of a Coma cluster progenitor at z=3.982508.21356v2 · Hanwen Sun, Tao Wang, Emanuele Daddi et al.2025 · 6 citationsarXiv
Unexpected clustering pattern in dwarf galaxies challenges formation models.40399680 · Zhang, Ziwen, Chen, Yangyao, Rong, Yu et al.2025 · 6 citationsNature. 2025;642(8066):47-52
Testing a New Star Formation History Model from Principal Component Analysis to Facilitate Spectral Synthesis Modeling2502.18561v2 · Yanzhe Zhang, H.J. Mo, Katherine E. Whitaker et al.2025 · 0 citationsarXiv
Discovery of Ancient Globular Cluster Candidates in the Relic, a Quiescent Galaxy at 2501.07627v3 · Katherine E. Whitaker, Sam E. Cutler, Rupali Chandar et al.2025 · 5 citationsarXiv
What drives the HI content of central galaxies -- A comparison between hydrodynamic simulations and observations using Random Forest2411.07977v1 · Xiao Li, Cheng Li, Houjun Mo2024 · 4 citationsarXiv
Physical Processes Behind the Co-Evolution of Halos, Galaxies and Supermassive Black Holes in the IllustrisTNG Simulation2409.06208v3 · Hao Li, Yangyao Chen, Huiyuan Wang et al.2024 · 5 citationsarXiv
From Halos to Galaxies. VI. Improved halo mass estimation for SDSS groups and measurement of the halo mass function2408.12442v2 · Dingyi Zhao, Yingjie Peng, Yipeng Jing et al.2024 · 9 citationsApJ 979 42 (2025)
On the kinematic nature of apparent discs at high redshifts: Local counterparts are not dominated by ordered rotation but by tangentially anisotropic random motion2408.10735v2 · Bitao Wang, Yingjie Peng, Michele Cappellari et al.2024 · 5 citationsarXiv
From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction2408.07749v2 · Zeyu Gao, Yingjie Peng, Kai Wang et al.2024 · 2 citationsApJ 979 66 (2025)
From Halos to Galaxies. IX. Estimate of Halo Assembly History for SDSS Galaxy Groups2407.03409v1 · Cheqiu Lyu, Yingjie Peng, Yipeng Jing et al.2024 · 5 citationsarXiv
A two-phase model of galaxy formation: III. The formation of globular clusters2405.18735v3 · Yangyao Chen, Houjun Mo, Huiyuan Wang2024 · 9 citationsMNRAS 540 (2025) 1235-1271
Gas-rich Ultra-diffuse Galaxies Are Originated from High Specific Angular Momentum2404.00555v1 · Yu Rong, Huijie Hu, Min He et al.2024 · 3 citationsarXiv
Connection between galaxy morphology and dark-matter halo structure I: a running threshold for thin discs and size predictors from the dark sector2403.14749v2 · Jinning Liang (1, Fangzhou Jiang, Houjun Mo (3 et al.2024 · 10 citationsMon Not R Astron Soc (2025) 2304-2323
CSST large-scale structure analysis pipeline: I. constructing reference mock galaxy redshift surveys2403.10754v1 · Yizhou Gu, Xiaohu Yang, Jiaxin Han et al.2024 · 17 citationsarXiv
JWST/MIRI reveals the true number density of massive galaxies in the early Universe2403.02399v4 · Tao Wang, Hanwen Sun, Luwenjia Zhou et al.2024 · 27 citationsThe Astrophysical Journal Letters, 988:L35(14pp), 2025 July 20
ELUCID VIII: Simulating the Coma Galaxy Cluster to Calibrate Model and Understand Feedback2401.14730v2 · Xiong Luo, Huiyuan Wang, Weiguang Cui et al.2024 · 10 citationsarXiv
On the existence, rareness and uniqueness of quenched HI-rich galaxies in the local Universe2312.03601v3 · Xiao Li, Cheng Li, H. J. Mo et al.2023 · 13 citationsarXiv
Post-starburst galaxies in SDSS-IV MaNGA: Two broad categories of evolutionary pathways2312.03616v2 · Zhuo Cheng, Cheng Li, Niu Li et al.2023 · 11 citationsarXiv
A two-phase model of galaxy formation: II. The size-mass relation of dynamically hot galaxies2311.11713v2 · Yangyao Chen, Houjun Mo, Huiyuan Wang2023 · 6 citationsarXiv
A two-phase model of galaxy formation: I. The growth of galaxies and supermassive black holes2311.05030v3 · Houjun Mo, Yangyao Chen, Huiyuan Wang2023 · 23 citationsarXiv
An efficient and robust method to estimate halo concentration2310.00200v2 · Kai Wang, H.J. Mo, Yangyao Chen et al.2023 · 8 citationsarXiv
Characterizing the assembly of dark matter halos with protohalo size histories: I. Redshift evolution, relation to descendant halos, and halo assembly bias2309.01039v2 · Kai Wang, H.J. Mo, Yangyao Chen et al.2023 · 5 citationsMNRAS, Volume 528, Issue 2, February 2024, Pages 2046-2065
Halo mass-observable proxy scaling relations and their dependencies on galaxy and group properties2305.06803v2 · Ziwen Zhang, Huiyuan Wang, Wentao Luo et al.2023 · 12 citationsarXiv
Dynamical hotness, star formation quenching and growth of supermassive black holes2305.02910v2 · Hui Hong, Huiyuan Wang, H. J. Mo et al.2023 · 9 citationsarXiv
Massive Dark Matter Halos at High Redshift: Implications for Observations in the JWST Era2304.13890v2 · Yangyao Chen, H.J. Mo, Kai Wang2023 · 27 citationsarXiv
A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos2301.08972v2 · Yangyao Chen, H.J. Mo, Cheng Li et al.2023 · 2 citationsarXiv
Mapping dust attenuation and the 2175 Å bump at kpc scales in nearby galaxies2212.01918v2 · Shuang Zhou, Cheng Li, Niu Li et al.2022 · 1 citationarXiv
Relating galaxies across different redshift to study galaxy evolution2211.00485v2 · Kai Wang, Houjun Mo, Cheng Li et al.2022 · 11 citationsarXiv
Galaxy populations in groups and clusters: evidence for a characteristic stellar mass scale at 2210.17186v3 · Jiacheng Meng, Cheng Li, Houjun Mo et al.2022 · 11 citationsarXiv
Conditional HI mass functions and the HI-to-halo mass relation in the local Universe2209.07691v3 · Xiao Li, Cheng Li, H.J. Mo et al.2022 · 23 citationsarXiv
Anisotropy and characteristic scales in halo density gradient profiles2206.12163v2 · X. Wang, H. Wang, H. J. Mo2022 · 5 citationsA&A 667, A99 (2022)
Career total: at least 405 works. 211 are in this corpus.Showing the 50 most recent.
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