activity
20172026
most citedDusty Starbursts Masquerading as Ultra-high Redshift Galaxies in JWST CEERS Observations

139 citations · 394 across the 19 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

18 papers · 1 filter

astro-ph.GA2026

The Zero-Age Massive Stellar Population of W49A from VLA Observations

M. Juárez-Gama, R. Galván-Madrid, G. Suárez +14

We use all-configuration VLA data at 3.3 cm with a physical resolution of ~2000 AU to infer the embedded zero-age massive stellar population of the W49A protocluster, as traced by…

astro-ph.GA2025★ 3 cited

PASSAGES: The Discovery of a Strongly Lensed Protocluster Core Candidate at Cosmic Noon

Nicholas Foo, Kevin C. Harrington, Brenda Frye +22

Investigating the processes by which galaxies rapidly build up their stellar mass during the peak of their star formation () is crucial to advancing our understanding of the…

astro-ph.GA2025★ 1 cited

ngVLA Synthetic Observations of Ionized Gas in Massive Protostars

Jesús M. Jáquez-Domínguez, Roberto Galván-Madrid, Alfonso Trejo-Cruz +11

Massive star formation involves significant ionization in the innermost regions near the central object, such as gravitationally trapped H II regions, jets, ionized disks, or winds…

astro-ph.GA2024

A Census of the Deep Radio Sky with the VLA I: 10GHz Survey of the GOODS-N field

Eric F. Jiménez-Andrade, Eric J. Murphy, Emmanuel Momjian +4

We present the first high-resolution, high-frequency radio continuum survey that fully maps an extragalactic deep field: the 10GHz survey of the Great Observatories Origins Deep Su…

astro-ph.GA2024★ 11 cited

ACOSMOS: Measuring the cosmic dust-attenuated star formation rate density at

Benjamin Magnelli, Sylvia Adscheid, Tsan-Ming Wang +14

[Abridged] In recent years, conflicting results have provided an uncertain view of the dust-attenuated properties of star-forming galaxies (SFGs). To solve this, we used the…

astro-ph.GA2023

ACOSMOS: Dissecting the gas content of star-forming galaxies across the main sequence at 1.2 < 1.6

Tsan-Ming Wang, Benjamin Magnelli, Eva Schinnerer +5

We aim to understand the physical mechanisms that drive star formation in a sample of mass-complete (>10) star-forming galaxies (SFGs) at 1.2 < 1.6. We se…