S. Belli

activity

20192026

most citedThe Evolution and Origin of Ionized Gas Velocity Dispersion from

z \sim 2.6

z \sim 0.6

with KMOS

^{3D}

174 citations · 174 across the 3 of their papers we have counts for

collaborators

Showing astro-ph.GAShow all

3 papers · 1 filter

astro-ph.GA2026

Resolved Maps of Gas and Dust in a Massive Quiescent Galaxy at z=2 from INQUEST-JWST: Evidence of Accretion and Rejuvenation

Sai Gangula, Andrew B. Newman, Meng Gu +10

Quiescent galaxies in the distant universe exhibit a range of gas content that may indicate a variety of quenching processes are at play. Mapping the distribution and kinematics of…

astro-ph.GA2025

Impact of stochastic star-formation histories and dust on selecting quiescent galaxies with JWST photometry

K. Lisiecki, D. Donevski, A. W. S. Man +16

While the James Webb Space Telescope (JWST) now allows identifying quiescent galaxies (QGs) out to early epochs, the photometric selection of quiescent galaxy candidates (QGCs) and…

astro-ph.GA2019★ 174 cited

The Evolution and Origin of Ionized Gas Velocity Dispersion from $z \sim 2.6$ to $z \sim 0.6$ with KMOS $^{3D}$

Hannah D. N. Übler, Reinhard Genzel, Emily Wisnioski +27

We present the $0.6 < z < 2.6$ evolution of the ionized gas velocity dispersion in 175 star-forming disk galaxies based on data from the full KMOS $^{3D}$ integral field spectroscop…

Resolved Maps of Gas and Dust in a Massive Quiescent Galaxy at z=2 from INQUEST-JWST: Evidence of Accretion and Rejuvenation

Impact of stochastic star-formation histories and dust on selecting quiescent galaxies with JWST photometry

The Evolution and Origin of Ionized Gas Velocity Dispersion from z∼2.6 to z∼0.6 with KMOS3D

The Evolution and Origin of Ionized Gas Velocity Dispersion from $z \sim 2.6$ to $z \sim 0.6$ with KMOS $^{3D}$