most citedGalaxy Metallicity Gradients in the Reionization Epoch from the FIRE-2 Simulations

1 citations · 1 across the 4 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2026

Pandora cluster Lensing, AGN, and Transient Exploration (PLATE) from JWST Multi-Epoch Imaging. I. Discovery of a type II supernova candidate in a spiral galaxy at

Yuxuan Pang, Xin Wang, Ping Chen +14

We report the discovery and multi-wavelength analysis of a transient PLATE-23a in the Abell 2744 field, as the first results of the Pandora Lensing, AGN, and Transient E…

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.GA20261 cited

Galaxy Metallicity Gradients in the Reionization Epoch from the FIRE-2 Simulations

Xunda Sun, Xin Wang, Fangzhou Jiang +10

We employ the high-redshift suite of FIRE-2 cosmological hydrodynamic zoom-in simulations to investigate the evolution of gas-phase metallicity radial gradients in galaxies in the…

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.…