activity
20242026
most citedModeling the inner part of the jet in M87: Confronting jet morphology with theory

41 citations · 78 across the 22 of their papers we have counts for

collaborators

24 papers

cs.DB2026

JetStream: Generating Verified Query Accelerators for Existing Database Systems

Akhilesh Balasingam, Amadou Ngom, Geoffrey X. Yu +1

Recent work has shown that LLMs can synthesize highly specialized database systems for fixed workloads, but these systems replace the DBMS's native storage and assume static data:…

astro-ph.GA2026

Ubiquitous nuclear disks and bars embedded in massive galaxies in the cosmic morning

Jianyuan Luo, Fangzhou Jiang, Jinning Liang +8

The morphology of the central regions of high-redshift galaxies remains relatively unexplored, while recent case studies suggest that giant disks can emerge without first developin…

astro-ph.GA2026

Reconstructing the Projected Dark Matter Field across 0.1-100 Mpc Scales from the SDSS Survey

Kunyao Zhao, Yingjie Peng, Dingyi Zhao +16

Dark matter sets the gravitational environment in which galaxies form and evolve, but cannot be observed directly. We present a conditional diffusion model that reconstructs the pr…

astro-ph.GA2026

No Detectable One-halo Galactic Conformity Signal with Halo-mass Estimates Consistent with Weak-lensing Constraints

Dingyi Zhao, Yingjie Peng, Luis C. Ho +17

One-halo galactic conformity is the tendency for satellites in halos with quenched centrals to have lower star-formation activity than those in halos with star-forming centrals at…

astro-ph.GA2026

Widespread Inflows Reveal Baryonic Cycling in Star-forming and Quiescent Galaxies

Hassen M. Yesuf, Ravi Joshi, Yuxuan Zou +8

Cool-gas inflows, required to sustain star formation, have been fundamental in simulations yet remained observationally elusive. Using DESI spectroscopy of ~30,000 galaxies, we ide…

astro-ph.GA2026

The Structural Abundance Crisis of Massive Galaxies in Current Cosmological Simulations

Hassen M. Yesuf, Connor Bottrell, Luis C. Ho +5

The internal structure of galaxies encodes the complex baryon cycle driven by gas accretion, star formation, and feedback, together with secular evolution and environmentally drive…

astro-ph.GA2026

The VariableTNG project: mass-dependent regulation of galaxy morphology by baryonic feedback

Yikai Liu, Hong Guo, Volker Springel +3

Galaxy morphology is shaped by both assembly history and baryonic processes, but their relative roles remain uncertain. We use the VariableTNG (VTNG) simulation suite to investigat…

astro-ph.GA2026

The VariableTNG project: how baryonic mechanisms shape galaxy properties

Kexin Liu, Hong Guo, Luis C. Ho +3

We use 50 Sobol-sampled VariableTNG simulations, varying eight subgrid parameters at fixed cosmology and initial conditions, to determine which baryonic processes regulate galaxies…

astro-ph.GA2026

The VariableTNG project: Unveiling the physical drivers of galaxy quenching

Ignacio G. Alfaro, Antonio D. Montero-Dorta, Hong Guo +4

Understanding the physical processes that regulate galaxy quenching is a key challenge in galaxy formation and evolution. The VariableTNG (VTNG) project provides a laboratory to in…

astro-ph.GA2026

Star formation powers optical line emission from the CGM

Huanian Zhang, Lizhi Xie, Zhijie Qu +9

Using integral field spectroscopy, we explore the disk-halo interface, or the inner circumgalactic medium (CGM), of individual galaxies by constructing and analyzing emission-line…

astro-ph.GA2026

Insights into the Physical Nature of Polar Ring Galaxies from H I Observations

Niankun Yu, Han Zheng, Chao-Wei Tsai +10

Polar ring galaxies (PRGs) host an outer ring of gas and stars oriented nearly perpendicular to the main stellar body. They represent extreme examples of misaligned systems and pro…

astro-ph.GA2025

The impact of external gas accretion on the distribution of HI gas in galaxies

Qianhan Zhang, Min Bao, Yanmei Chen +3

Using the data from Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) and HI-MaNGA surveys, we build a sample of 37 gas-star misaligned galaxies with robust HI detections…

astro-ph.GA2025★ 3 cited

Symmetry in Fundamental Parameters of Galaxies on the Star-forming Main Sequence

Zhicheng He, Enci Wang, Luis C. Ho +4

The Star-Forming Main Sequence (SFMS) serves as a critical framework for understanding galaxy evolution, highlighting the relationship between star formation rates (SFR) and stella…

astro-ph.GA2025★ 1 cited

A Potential Link between Nuclear Winds and Cold Gas Outflows on Kiloparsec Scales in Reionization-Era Quasars

Yongda Zhu, Marcia J. Rieke, Luis C. Ho +23

Feedback from accreting supermassive black holes may regulate galaxy evolution, but statistical evidence linking nuclear winds to kiloparsec-scale cold gas outflows remains limited…

astro-ph.GA2025★ 1 cited

Formation and Environmental Context of Giant Bulgeless Disk Galaxies in the Early Universe: Insights from Cosmological Simulations

Fangzhou Jiang, Jinning Liang, Bingcheng Jin +7

Giant bulgeless disk galaxies, theoretically expected to be rare in the early Universe, have been confirmed by the James Webb Space Telescope (JWST) to exist as early as 2 billion…

astro-ph.GA2025★ 1 cited

The Origin of the Gas and Its Low Star Formation Efficiency in Quiescent Galaxies

Yang A. Li, Luis C. Ho, Jinyi Shangguan +2

Quiescent galaxies (QGs) typically have little cold gas to form stars. The discovery of gas-rich QGs challenges our conventional understanding of the evolutionary paths of galaxies…

astro-ph.GA2025

The critical role of dark matter halos in driving star formation

Jing Dou, Yingjie Peng, Qiusheng Gu +13

Understanding the physical mechanisms that drive star formation is crucial for advancing our knowledge of galaxy evolution. We explore the interrelationships between key galaxy pro…

astro-ph.GA2025★ 16 cited

Formation of the Little Red Dots from the Core-collapse of Self-interacting Dark Matter Halos

Fangzhou Jiang, Zixiang Jia, Haonan Zheng +5

We present a statistical study of black hole (BH) formation and growth seeded by gravothermal core collapse of self-interacting dark matter (SIDM) halos at high redshift, using a c…

astro-ph.GA2024

The HI reservoir in central spiral galaxies and the implied star formation process

Jing Dou, Yingjie Peng, Qiusheng Gu +14

The cold interstellar medium (ISM) as the raw material for star formation is critical to understanding galaxy evolution. It is generally understood that galaxies stop making stars…

astro-ph.GA2024★ 4 cited

The Transition from Galaxy-wide Gas Inflow to Outflow in Quasar Host Galaxies

Zhicheng He, Zhifu Chen, Guilin Liu +8

Galactic-wide outflows driven by active galactic nuclei (AGNs) is a routinely invoked feedback mechanism in galaxy evolution models. Hitherto, the interplay among the interstellar…

astro-ph.GA2024★ 9 cited

From Halos to Galaxies. VI. Improved halo mass estimation for SDSS groups and measurement of the halo mass function

Dingyi Zhao, Yingjie Peng, Yipeng Jing +18

In CDM cosmology, galaxies form and evolve in their host dark matter (DM) halos. Halo mass is crucial for understanding the halo-galaxy connection. The abundance matching (AM) t…

astro-ph.GA2024★ 2 cited

From Halos to Galaxies. X: Decoding Galaxy SEDs with Physical Priors and Accurate Star Formation History Reconstruction

Zeyu Gao, Yingjie Peng, Kai Wang +18

The spectral energy distribution (SED) of galaxies is essential for deriving fundamental properties like stellar mass and star formation history (SFH). However, conventional method…

astro-ph.GA2024

From Halos to Galaxies. IX. Estimate of Halo Assembly History for SDSS Galaxy Groups

Cheqiu Lyu, Yingjie Peng, Yipeng Jing +15

The properties of the galaxies are tightly connected to their host halo mass and halo assembly history. Accurate measurement of the halo assembly history in observation is challeng…

astro-ph.HE2024★ 41 cited

Modeling the inner part of the jet in M87: Confronting jet morphology with theory

Hai Yang, Feng Yuan, Hui Li +7

The formation of jets in black hole accretion systems is a long-standing problem. It has been proposed that a jet can be formed by extracting the rotation energy of the black hole…