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20172021
most citedA massive stellar bulge in a regularly rotating galaxy 1.2 billion years after the Big Bang

127 citations · 531 across the 10 of their papers we have counts for

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Showing astro-ph.GAShow all

14 papers · 1 filter

astro-ph.GA202164 cited

Quenching of star formation from a lack of inflowing gas to galaxies

Katherine E. Whitaker, Christina C. Williams, Lamiya Mowla +16

Star formation in half of massive galaxies was quenched by the time the Universe was three billion years old. Very low amounts of molecular gas appear responsible for this, at leas…

astro-ph.GA202126 cited

An exquisitely deep view of quenching galaxies through the gravitational lens: Stellar population, morphology, and ionized gas

Allison W. S. Man, Johannes Zabl, Gabriel B. Brammer +6

This work presents an in-depth analysis of four gravitationally lensed red galaxies at z = 1.6-3.2. The sources are magnified by factors of 2.7-30 by foreground clusters, enabling…

astro-ph.GA20215 cited

Molecular gas in a gravitationally lensed galaxy group at

Jeff Shen, Allison W. S. Man, Johannes Zabl +5

Most molecular gas studies of galaxies are of intrinsically bright objects, despite the galaxy population being primarily "normal" galaxies with less extreme star formati…

astro-ph.GA2021127 cited

A massive stellar bulge in a regularly rotating galaxy 1.2 billion years after the Big Bang

Federico Lelli, Enrico M. Di Teodoro, Filippo Fraternali +5

Cosmological models predict that galaxies forming in the early Universe experience a chaotic phase of gas accretion and star formation, followed by gas ejection due to feedback pro…

astro-ph.GA202025 cited

Recent Star-formation in a Massive Slowly-Quenched Lensed Quiescent Galaxy at z=1.88

Mohammad Akhshik, Katherine E. Whitaker, Joel Leja +10

In this letter, we reconstruct the formation pathway of MRG-S0851, a massive, , strongly lensed, red, galaxy at . While the global p…

astro-ph.GA2020

The interacting nature of dwarf galaxies hosting superluminous supernovae

Simon Vanggaard Ørum, David Lykke Ivens, Patrick Strandberg +3

(Abridged) Type I superluminous supernovae (SLSNe I) are rare, powerful explosions whose mechanism and progenitors remain elusive. SLSNe I show a preference for low-metallicity, ac…