activity
20162026
most citedMerging Galaxies with Tidal Tails in COSMOS to z=1

25 citations · 38 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2026

BayeSED-GALAXIES II. Bayesian full spectrum analysis of galaxies and application in the CSST wide-field slitless spectroscopy survey

Yunkun Han, Xian Zhong Zheng, Xiaohu Yang +21

The China Space Station Telescope (CSST) will conduct wide-field multiband photometric imaging and slitless spectroscopic surveys, advancing cosmology and galaxy evolution studies.…

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★ 7 cited

SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). V. Confusion-limited Submillimeter Galaxy Number Counts at 450 m and Data Release for the COSMOS Field

Zhen-Kai Gao, Chen-Fatt Lim, Wei-Hao Wang +19

We present confusion-limited SCUBA-2 450-m observations in the COSMOS-CANDELS region as part of the JCMT Large Program, SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). Our maps…

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

Revisiting Galaxy Evolution in Morphology in the COSMOS field (COSMOS-ReGEM):I. Merging Galaxies

Jian Ren, Nan Li, F. S. Liu +3

We revisit the evolution of galaxy morphology in the COSMOS field over the redshift range , using a large and complete sample of 33,605 galaxies with a stellar ma…

astro-ph.GA2016★ 5 cited

Measuring Structural Parameters Through Stacking Galaxy Images

Yubin Li, XianZhong Zheng, Qiu-Sheng Gu +4

It remains challenging to detect the low surface brightness structures of faint high-z galaxies, which is key to understanding the structural evolution of galaxies. The technique o…