collaborators

9 papers

astro-ph.GA2026

An emerging baryon cycle in a galaxy 500 million years after the Big Bang

Shengzhe Wang, Xin Wang, Hang Zhou +17

The emergence of stellar feedback as a regulator of galaxy growth marks a fundamental transition in cosmic history. At early times, rapid gas accretion and collapse may induce inte…

astro-ph.GA2026

Confirmation and Refutation of Lyman Continuum Leakers at with JWST NIRSpec/IFU

Shengzhe Wang, Xin Wang, Hang Zhou +10

Our understanding of the physical mechanisms and environments conducive to the escape of Lyman-continuum (LyC) radiation within the first 2 Gyr of cosmic history remains limited. H…

astro-ph.GA2026

A Spatially Resolved HI Survey of Seyfert Galaxies: the Role of AGN Feedback in Shaping Atomic Gas Reservoirs

Ruitian Li, Xin Wang, Daizhong Liu +19

Active galactic nucleus (AGN) feedback is a key ingredient in galaxy evolution, yet its impact on the cold atomic gas reservoir -- the neutral hydrogen (HI) phase -- remains poorly…

astro-ph.GA2026

The Structure and Evolution of LRDs: Insights from JWST NIRSpec Medium and High Resolution Spectroscopy at

Yuxuan Pang, Xin Wang, Cheng Cheng +5

We present an analysis of medium/high-resolution JWST/NIRSpec spectra for 11 LRDs at . By decomposing the broad and narrow components of the Balmer emission lines, we inv…

astro-ph.GA2026

The GLASS-JWST Early Release Science Program. V. H luminosity functions at and

Yuxuan Pang, Xin Wang, Tommaso Treu +11

We present H luminosity function (LF) measurements at redshifts and using JWST NIRISS grism data from the GLASS-JWST survey. Based on emission lines spect…

astro-ph.GA2026

The faint end of the UV luminosity function at from the Hubble Frontier Fields

Lei Sun, Xiao-Lei Meng, Xin Wang +7

By extending the Hubble Frontier Fields (HFF) observations to the F225W band using HST WFC3/UVIS, we measure the rest-frame UV luminosity function (LF) of galaxies at $0.4 < z < 0.…