activity
20112026
most citedFast, Slow, Early, Late: Quenching Massive Galaxies at z~0.8

170 citations · 1.4k across the 56 of their papers we have counts for

collaborators

56 papers

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

A systematic study of AGN feedback in a disk galaxy using MACER. III. High Gas Fractions in AGN Hosts

Yuxuan Zou, Feng Yuan, Suoqing Ji +4

We use high-resolution hydrodynamic simulations in the MACER framework to explain why low-redshift PG quasar hosts can retain substantial cold-gas reservoirs, with gas fractions an…

astro-ph.GA2026

When Galaxies Refuel: Evolution of the Perturbed Spiral Galaxy NGC1385

Xiaoyu Kang, Eva Sextl, Rolf-Peter Kudritzki +5

The spiral galaxy NGC 1385 is characterized by a vigorous and protracted history of star formation, particularly in its central regions, leading to a current star formation rate th…

astro-ph.GA2026

The Narrow-Line Seyfert 1 Phenomenon: Accretion State Versus Host Galaxy Properties

Kaizheng Guo, Hassen M. Yesuf, Lei Hao +3

The physical origin of the narrow-line Seyfert 1 (NLS1) and broad-line Seyfert 1 (BLS1) dichotomy remains debated, with competing scenarios invoking host-galaxy evolution or intrin…

astro-ph.GA2026

DESI as sparse Integral Field Spectrograph I: Spatially resolved chemical enrichment in star-forming galaxies at

Vibhore Negi, Ravi Joshi, B. Vishnupriya +8

We present a spatially resolved chemical abundance analysis of 2291 star-forming galaxies at , spanning nearly four orders of magnitude in stellar mass ($8 \le \rm log…

astro-ph.GA2026

The Importance of Galaxy-Wide Star Formation in Driving Winds at z~1

Weichen Wang, Susan A. Kassin, S. M. Faber +11

In this work, we study winds for a representative sample of 86 star-forming galaxies (SFGs) at z~1 with , by measuring the Mg II line profiles…

astro-ph.GA2026

Beyond Mass and Multiscale Environments: What Shapes Low Surface Brightness Galaxies? Evidence from MaNGA

Mengting Shen, Hassen M. Yesuf, Lei Hao +4

The origin of low surface brightness (LSB) galaxies remains a key open question in galaxy formation, reflecting the balance internal mechanisms and environmental influence. Using M…

astro-ph.HE2026

Electromagnetic Flares from Compact-Object Mergers in AGN Disks: Signatures and Predictions

Hiromichi Tagawa, Zoltán Haiman, Shigeo S. Kimura +2

Accretion disks in active galactic nuclei (AGN) are promising sites for mergers of stellar-mass black holes (BHs) detectable via gravitational waves (GWs). These environments facil…

astro-ph.GA2026

SDSS-IV MaNGA: Distinct Structural Growth and Star Formation in Low and High Surface Brightness Disks

Mengting Shen, Jun Yin, Hassen M. Yesuf +7

We analyze a clean sample of 1,118 late-type, face-on galaxies without AGN contamination from the MaNGA survey. Their photometric structures are quantified via two-component (bulge…

astro-ph.GA2026

Galaxy and black hole coevolution in dark matter haloes not captured by cosmological simulations

Hassen M. Yesuf, Connor Bottrell

Star formation in galaxies is governed by internal and environmental processes, yet their relative roles are not well understood. In particular, uncertainties in measurements of ac…

astro-ph.GA2025

HST Confirms Sub-5 kpc Dual Quasar Pairs at Cosmic Noon

Qian Wang, Xuheng Ding, John Silverman +12

During cosmic noon (), when both star formation and black hole growth peaked, galaxy mergers are predicted to trigger dual active galactic nuclei (AGN) that eventually co…

astro-ph.GA2025

Extended Components of Little Red Dots in the Rest-Frame Optical

Yiyang Zhang, Xuheng Ding, Lilan Yang +26

Recent JWST observations have revealed a population of red, compact, high-redshift objects called Little Red Dots (LRDs), whose host components have remained largely unconstrained,…

astro-ph.GA2025

The Size Evolution and the Size-Mass Relation of Lyman-Alpha Emitters across as Observed by JWST

Qi Song, F. S. Liu, Jian Ren +14

Understanding the morphological structures of Lyman-alpha emitters (LAEs) is crucial for unveiling their formation pathways and the physical origins of Ly emission. However, the…

astro-ph.GA2025

The JWST Unveils the Bimodal Nature of Lyman Alpha Emitters at 3 <z<7: Pristine versus Merger-Driven Populations

Jian Ren, F. S. Liu, Nan Li +8

We present a systematic study of merging galaxies among Lyman-alpha emitters (LAEs) using JWST/NIRCam high-resolution imaging data. From a large sample of 817 spectroscopically con…

astro-ph.GA2025

The connection between galaxy mergers, star formation and AGN activity in the HSC-SSP

Kiyoaki Christopher Omori, Connor Bottrell, Sabine Bellstedt +6

Internal gas inflows driven by galaxy mergers are considered to enhance star formation rates (SFR), fuel supermassive black hole growth and stimulate active galactic nuclei (AGN).…

astro-ph.GA2025

The Evolution of Size and Merger Fraction of Submillimeter Galaxies across as Observed by JWST

Jian Ren, F. S. Liu, Nan Li +9

Precise tracking of the growth in galaxy size and the evolution of merger fractions with redshift is vital for understanding the formation history of submillimeter galaxies (SMGs).…

astro-ph.GA2024★ 2 cited

Baryonic Ecosystem in Galaxies (BEINGMgII). Host Galaxies of Ultra-strong MgII Absorbers in Subaru Hyper Suprime-Cam Survey

Ravi Joshi, Sarbeswar Das, Michele Fumagalli +5

We study the galaxies hosting ultra-strong MgII (USMgII) absorbers at small impact parameters of 2" (5 - 20 kpc), spanning a redshift range of , using deep…

astro-ph.GA2024

Radial Profiles of , , Gas Metallicity and Their Correlations Across the Galactic Mass-Size Plane

Lin Lin, Shiyin Shen, Hassen M. Yesuf +2

We analyzed the global and resolved properties of approximately 1,240 nearby star-forming galaxies from the MaNGA survey, comparing compact and extended galaxies -- those with smal…

astro-ph.GA2024★ 4 cited

IllustrisTNG in the HSC-SSP: No Shortage of Thin Disk Galaxies in TNG50

Dewang Xu, Hua Gao, Connor Bottrell +2

We perform a thorough analysis of the projected shapes of nearby galaxies in both observations and cosmological simulations. We implement a forward-modeling approach to overcome th…

astro-ph.GA2024★ 1 cited

Calibrating non-parametric morphological indicators from {\it JWST} images for galaxies over

Jian Ren, F. S. Liu, Nan Li +6

The measurements of morphological indicators of galaxies are often influenced by a series of observational effects. In this study, we utilize a sample of over 800 TNG50 simulated g…

astro-ph.GA2023

Structure and Color Gradients of Ultra-diffuse Galaxies in Distant Massive Galaxy Clusters

Pinsong Zhao, Fengshan Liu, Qifan Cui +2

We have measured structural parameters and radial color profiles of 108 ultra-diffuse galaxies (UDGs), carefully selected from six distant massive galaxy clusters in the Hubble Fro…

astro-ph.GA2023

Galaxy mergers in Subaru HSC-SSP: a deep representation learning approach for identification and the role of environment on merger incidence

Kiyoaki Christopher Omori, Connor Bottrell, Mike Walmsley +7

We take a deep learning-based approach for galaxy merger identification in Subaru HSC-SSP, specifically through the use of deep representation learning and fine-tuning, with the ai…

astro-ph.GA2023★ 55 cited

IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation

Connor Bottrell, Hassen M. Yesuf, Gergö Popping +13

At fixed galaxy stellar mass, there is a clear observational connection between structural asymmetry and offset from the star forming main sequence, SFMS. Herein, we use the TNG…