activity
20232025
most citedIntroduction to the Chinese Space Station Survey Telescope (CSST)

59 citations · 85 across the 6 of their papers we have counts for

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Showing astro-ph.GAShow all

6 papers · 1 filter

astro-ph.GA20251 cited

Influence of Barlens on the Bulge Parameters in the 2D Image Decomposition

Xinyang Li, Zhao-Yu Li, Yang A. Li +2

Recent observations and simulations have shown that a buckled bar in the face-on view can be considered as a combination of a long flat bar and a short round barlens (corresponding…

astro-ph.GA2025

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.GA2024

Accuracy of Stellar Mass-to-light Ratios of Nearby Galaxies in the Near-Infrared

Taehyun Kim, Minjin Kim, Luis C. Ho +12

Future satellite missions are expected to perform all-sky surveys, thus providing the entire sky near-infrared spectral data and consequently opening a new window to investigate th…

astro-ph.GA202311 cited

The Subtle Effects of Mergers on Star Formation in Nearby Galaxies

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

Interactions and mergers play an important role in regulating the physical properties of galaxies, such as their morphology, gas content, and star formation rate (SFR). Controversy…

astro-ph.GA202313 cited

Panchromatic Photometry of Low-redshift, Massive Galaxies Selected from SDSS Stripe 82

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

The broadband spectral energy distribution of a galaxy encodes valuable information on its stellar mass, star formation rate (SFR), dust content, and possible fractional energy con…

astro-ph.GA2023

Redshifting galaxies from DESI to JWST CEERS: Correction of biases and uncertainties in quantifying morphology

Si-Yue Yu, Cheng Cheng, Yue Pan +2

Observations of high-redshift galaxies with unprecedented detail have now been rendered possible with JWST. However, accurately quantifying their morphology remains uncertain due t…