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20212026
most citedSpatial variations in aromatic hydrocarbon emission in a dust-rich galaxy

66 citations · 210 across the 21 of their papers we have counts for

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Showing 2023Show all

6 papers · 1 filter

astro-ph.GA2023★ 1 cited

Protoclusters as Drivers of Stellar Mass Growth in the Early Universe, a Case Study: Taralay -- a Massive Protocluster at z ~ 4.57

Priti Staab, Brian C. Lemaux, Ben Forrest +26

Simulations predict that the galaxy populations inhabiting protoclusters may contribute considerably to the total amount of stellar mass growth of galaxies in the early universe. I…

astro-ph.GA2023

The ALMA-ALPINE [CII] survey: Kennicutt-Schmidt relation in four massive main-sequence galaxies at z~4.5

M. Béthermin, C. Accard, C. Guillaume +40

The Kennicutt-Schmidt (KS) relation between the gas and the star formation rate (SFR) surface density (-) is essential to understand star formation proces…

astro-ph.GA2023★ 2 cited

JWST's TEMPLATES for Star Formation: The First Resolved Gas-Phase Metallicity Maps of Dust-Obscured Star-Forming Galaxies at 4

Jack E. Birkin, Taylor A. Hutchison, Brian Welch +23

We present the first spatially resolved maps of gas-phase metallicity for two dust-obscured star-forming galaxies (DSFGs) at 4, from the JWST TEMPLATES Early Release Scienc…

astro-ph.GA2023★ 27 cited

Elentári: A Proto-Supercluster in COSMOS

Ben Forrest, Brian C. Lemaux, Ekta Shah +25

Motivated by spectroscopic confirmation of three overdense regions in the COSMOS field at , we analyze the uniquely deep multi-wavelength photometry and extensive spectr…

astro-ph.GA2023★ 19 cited

Observations of neutral carbon in 29 high-z lensed dusty star forming galaxies and the comparison of gas mass tracers

G. Gururajan, M. Béthermin, N. Sulzenauer +10

The nature and evolution of high-redshift dusty star-forming galaxies (high-z DSFGs) remain an open question. Their massive gas reservoirs play an important role in driving the int…

astro-ph.GA2023★ 66 cited

Spatial variations in aromatic hydrocarbon emission in a dust-rich galaxy

Justin S. Spilker, Kedar A. Phadke, Manuel Aravena +35

Dust grains absorb half of the radiation emitted by stars throughout the history of the universe, re-emitting this energy at infrared wavelengths. Polycyclic aromatic hydrocarbons…