activity
19962026
most citedCANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey

2.2k citations · 6.7k across the 74 of their papers we have counts for

collaborators

75 papers

astro-ph.GA2026

COSMOS-3D: Diverse Environments and Hot-dust Signatures among Dusty Star-forming Galaxies at = 4.9-7.2

Siwei Zou, Manuel Aravena, Shaoze Geng +20

Dusty star-forming galaxies (DSFGs) are expected to trace early massive-halo assembly, but the connection between dust-obscured star formation, morphology, hot dust, and environmen…

astro-ph.CO2026

Halo Mass of ULIRGs at Cosmic Noon

Jun Pan, Ming Li, Cheng Cheng +1

We present a clustering analysis of ultraluminous infrared galaxies (ULIRGs) at , uniformly selected by flux and IRAC colors in the COSMOS and BOO…

astro-ph.GA2026

Ly Escape in JWST/NIRCam F430M-Selected H Emitters at

Cheng Cheng, Zhen-Ya Zheng, Chunyan Jiang +8

We study the Ly escape fraction () in an H-selected sample of star-forming galaxies at , identified via JWST/NIRCam F430M excess and covered by archi…

astro-ph.GA2026

HI Depletion Begins Well Beyond the Virial Radius: A FAST Stacking Study of 36 Galaxy Clusters to 5R200

Cheng Cheng, Chuan-Peng Zhang, Edo Ibar +10

We present a stacking study of the neutral atomic hydrogen (HI) content in and around 36 local galaxy clusters at , using a combination of the FAST all sky HI survey (FASHI…

astro-ph.GA2026★ 2 cited

ULTIMATE-deblending I. A 50-band Ultraviolet to Mid-infrared Photometric Catalog Combining Space- and Ground-based Data in the JWST/PRIMER survey

Hanwen Sun, Tao Wang, Ke Xu +16

Our understanding of the early Universe has long been limited by biased galaxy samples selected through various color criteria. With deep JWST infrared imaging, mass-complete galax…

astro-ph.GA2025

HI-detected Dwarf Galaxies in the FASHI Survey: Insights from Single- and Double-Peaked Emission-Line Samples

Cheng Cheng, Jia-Sheng Huang, Wei Du +4

We present a sample of low HI mass dwarf galaxies () detected by The FAST All Sky HI Survey (FASHI) project. Due to the faint and irregular morphology of…

astro-ph.GA2025

COSMOS-3D: Dense Circumnuclear Gas across Black Hole Growth Phases at z ~ 3

Zi-Jian Li, Siwei Zou, Jianwei Lyu +25

We report the discovery of two broad-line X-ray AGNs (cid_414 and cid_947) at z ~ 3 identified in the JWST Cycle 3 COSMOS-3D program using NIRCam F444W grism spectroscopy. Both exh…

astro-ph.GA2025

An H Cloud in the HI Tail: Recent Star Formation in the Outskirts of NGC 4258 Revealed by Nanshan 1-m Telescope

Cheng Cheng, Jia-Sheng Huang, Peng Wei +12

We present first-light deep H imaging taken with the Nanshan 1-meter wide-field telescope on the local galaxy NGC 4258, alongside archival data from Hubble Space telescope (HST)…

astro-ph.GA2025

Probing Obscured Star Formation in Galaxy Clusters Using JWST Medium Band Images: 3.3 PAH Emitter Sample in Abell 2744

Cheng Cheng, Xin Wang, Piaoran Liang +7

Star-forming galaxies in galaxy clusters play a crucial role in understanding the advanced stages of galaxy evolution within dense environments. We present a sample of 3.3m PAH-…

astro-ph.GA2025

PEARLS: 21 Transients Found in the Three-Epoch NIRCam Observations in the Continuous Viewing Zone of the James Webb Space Telescope

Haojing Yan, Bangzheng Sun, Zhiyuan Ma +39

We present 21 transients from our three-epoch, four-band NIRCam observations covering 14.16 arcmin^2 in the Spitzer IRAC Dark Field (IDF), taken by the JWST Prime Extragalactic Are…

astro-ph.GA2025

Starburst Galaxies in Their Last Billion Years: An H Absorption Line Selected Sample

Shumei Wu, Jia-Sheng Huang, Cheng Cheng +1

In this paper, we focus on the study of starburst galaxies in their final billion years. Our galaxy selection is based solely on the presence of the H absorption line, which per…

astro-ph.GA2025

Comparison of Global HI and H Line Profiles in MaNGA Galaxy Pairs with FAST

Gaoxiang Jin, Y. Sophia Dai, Cheng Cheng +3

We present case studies comparing the global HI and H emission line profiles of six galaxy pairs. The six pairs are selected to have different nuclear activities, with two hosti…

astro-ph.GA2024★ 17 cited

NOEMA formIng Cluster survEy (NICE): Characterizing eight massive galaxy groups at in the COSMOS field

Nikolaj B. Sillassen, Shuowen Jin, Georgios E. Magdis +41

The NOEMA formIng Cluster survEy (NICE) is a large program targeting 69 massive galaxy group candidates at in six deep fields. We report spectroscopic confirmation of eight g…

astro-ph.GA2024

A Complete 16 m selected Galaxy Sample at . II: Morphological Analysis

Piaoran Liang, Y. Sophia Dai, Jia-Sheng Huang +2

We present morphological analysis of the 16m flux-density-limited galaxy sample at 0.81.3 from arXiv:2103.04585. At the targeted redshift, the 16m emission corresponds t…

astro-ph.GA2024

Close Major-merger Pairs at : Star-forming Galaxies with Pseudobulges

Chuan He, Cong Kevin Xu, Ute Lisenfeld +5

We present a study of star-forming galaxies (SFGs) with pseudobulges (bulges with Sérsic index ) in a local close major-merger galaxy pair sample (H-KPAIR). With data fr…

astro-ph.GA2024

Dust and Cold Gas Properties of Starburst HyLIRG-Quasars at

Feng-Yuan Liu, Y. Sophia Dai, Alain Omont +7

Some high-z active galactic nuclei (AGNs) are found to reside in extreme star-forming galaxies, such as hyper-luminous infrared galaxies (HyLIRGs), with AGN-removed o…

astro-ph.GA2024★ 5 cited

Understanding the Universal Dust Attenuation Scaling Relation of Star-Forming Galaxies

J. Qin, X. Z. Zheng, S. Wuyts +17

Star-forming galaxies (SFGs) adhere to a surprisingly tight scaling relation of dust attenuation parameterized by the infrared excess (IRX=), being jointly d…

astro-ph.GA2024

Active Galactic Nuclei in a Mid-Infrared Selected Galaxy Sample at z>0.13: [Ne V]3426 Line Emission as a Benchmark

Zi-Jian Li, Y. Sophia Dai, Jia-Sheng Huang +2

We present a 24 um-selected spectroscopic sample z > 0.13 (median z = 0.41) in the Lockman Hole field, consisting of 4035 spectra. Our aim is to identify AGNs and determine their f…

astro-ph.GA2023★ 17 cited

Noema formIng Cluster survEy (NICE): Discovery of a starbursting galaxy group with a radio-luminous core at z=3.95

Luwenjia Zhou, Tao Wang, Emanuele Daddi +34

The study of distant galaxy groups and clusters at the peak epoch of star formation is limited by the lack of a statistically and homogeneously selected and spectroscopically confi…

astro-ph.GA2023★ 1 cited

A Close Look at Ly Emitters with JWST/NIRCam at

Yixiao Liu, Y. Sophia Dai, Stijn Wuyts +2

We study 10 spectroscopically confirmed Ly emitters (LAEs) at in the UDS field, covered by JWST/NIRCam in the PRIMER program. All LAEs are detected in all NIRCam b…

astro-ph.GA2023

Infall Motions in the Hot Core Associated with Hypercompact HII Region G345.0061+01.794 B

Toktarkhan Komesh, Guido Garay, Christian Henkel +13

We report high angular resolution observations, made with the Atacama Large Millimeter Array in band 6, of high excitation molecular lines of and and of the…

astro-ph.EP2023★ 14 cited

Detection of TiO and VO in the atmosphere of WASP-121b and Evidence for its temporal variation

Qinglin Ouyang, Wei Wang, Meng Zhai +6

We report the transit observations of the ultra hot Jupiter WASP-121b using the Goodman High Throughput Spectrograph (GHTS) at the 4-meter ground-based telescope Southern Astrophys…

astro-ph.EP2023★ 10 cited

Tentative detection of titanium oxide in the atmosphere of WASP-69 b with a 4m ground-based telescope

Qinglin Ouyang, Wei Wang, Meng Zhai +6

Transiting planets provide unique opportunities for the atmospheric characterization of exoplanets as they can reveal composition and the temperature structures at the day-night te…

astro-ph.GA2022★ 37 cited

JWST's PEARLS: A JWST/NIRCam view of ALMA sources

Cheng Cheng, Jia-Sheng Huang, Ian Smail +33

We report the results of James Webb Space Telescope/NIRCam observations of 19 (sub)millimeter (submm/mm) sources detected by the Atacama Large Millimeter Array (ALMA). The accurate…