Po-Feng Wu

Physics and Astronomy · Physical Sciences

21h-index1.3kcitations95works6.22yr avg
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Research Topics

Galaxies: Formation, Evolution, Phenomena(68), Astronomy and Astrophysical Research(64), Stellar, planetary, and galactic studies(44), Astrophysics and Star Formation Studies(17), Gamma-ray bursts and supernovae(12)

Publications95 total

The ALMaQUEST Survey XVII: Unveiling Multiple Quenching Pathways in Green Valley Galaxies via Molecular Gas and Quenching Timescale Analyses
arXiv (Cornell University)·2026Open Access
The ALMaQUEST Survey XVII: Unveiling Multiple Quenching Pathways in Green Valley Galaxies via Molecular Gas and Quenching Timescale Analyses
ArXiv.org·2026Open Access
The LEGA-C galaxy survey: Multiple quenching channels for quiescent galaxies at <i>z</i> ∼ 1
Astronomy and Astrophysics·2025· 1 citedOpen Access
The LEGA-C galaxy survey: multiple quenching channels for quiescent galaxies at $z\sim1$
ArXiv.org·2025Open Access
LEGA-C stellar populations scaling relations. II: Dissecting mass-complete archaeological trends and their evolution since z~0.7 with LEGA-C and SDSS
arXiv (Cornell University)·2025Open Access
Unusually High Gas-to-dust Ratios Observed in High-redshift Quiescent Galaxies
The Astrophysical Journal Letters·2025· 1 citedOpen Access
A Multiwavelength Study of ELAN Environments (AMUSE <sup>2</sup> ): The Impact of Dense Environment on Massive Dusty Star-forming Galaxies at Cosmic Noon
The Astrophysical Journal·2025Open Access
A MUltiwavelength Study of ELAN Environments (AMUSE$^2$): The Impact of Dense Environment on Massive Dusty Star-Forming Galaxies at Cosmic Noon
arXiv (Cornell University)·2025Open Access
Unusually High Gas-to-Dust Ratios Observed in High-Redshift Quiescent Galaxies
arXiv (Cornell University)·2025Open Access
No Evidence of a Dichotomy in the Elliptical Galaxy Population
The Astrophysical Journal·2025Open Access
DeepDive: A deep dive into the physics of the first massive quiescent galaxies in the Universe
ArXiv.org·2025Open Access
Gas outflows in two recently quenched galaxies at <i>z</i> = 4 and 7
Astronomy and Astrophysics·2025· 15 citedOpen Access
More is better: Strong constraints on the stellar properties of LEGA-C <i>z</i>  ∼  1 galaxies with Prospector
Astronomy and Astrophysics·2025· 8 citedOpen Access
More is better: Strong constraints on the stellar properties of LEGA-C z ~ 1 galaxies with Prospector
arXiv (Cornell University)·2025Open Access
Ejective Feedback as a Quenching Mechanism in the First 1.5 Billion Years of the Universe: Detection of Neutral Gas Outflow in a z = 4 Recently Quenched Galaxy
The Astrophysical Journal·2025· 16 citedOpen Access
No Evidence of a Dichotomy in the Elliptical Galaxy Population
arXiv (Cornell University)·2024Open Access
Ejective feedback as a quenching mechanism in the 1.5 billion years of the universe: detection of neutral gas outflow in a $z=4$ recently quenched galaxy
arXiv (Cornell University)·2024Open Access
Age and metal gradients in massive quiescent galaxies at 0.6 ≲ <i>z</i> ≲ 1.0: implications for quenching and assembly histories
Monthly Notices of the Royal Astronomical Society·2024· 7 citedOpen Access
A Protocluster of Massive Quiescent Galaxies at z = 4
The Astrophysical Journal·2024· 26 citedOpen Access
The Gas-phase Mass–Metallicity Relation for Massive Galaxies at z ∼ 0.7 with the LEGA-C Survey
The Astrophysical Journal·2024· 6 citedOpen Access
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Frequent Co-authors

Arjen van der Wel(23), Rachel Bezanson(23), Eric F. Bell(21), Michael V. Maseda(19), Anna Gallazzi(18), David Sobral(18), Caroline M. S. Straatman(17), Adam Muzzin(17), Francesco D’Eugenio(16), Marijn Franx(16), B. C. Lemaux(14), R. R. Gal(14), Adam Tomczak(13), L. M. Lubin(13), G. Squires(13), Camilla Pacifici(12), Lu Shen(12), Josha van Houdt(11), Ivana Barišić(11), N. Rumbaugh(10)