activity
20112025
most citedSub-millimeter galaxies as progenitors of compact quiescent galaxies

304 citations · 2k across the 34 of their papers we have counts for

collaborators

34 papers

astro-ph.GA2025★ 17 cited

A merging pair of massive quiescent galaxies at in the Cosmic Vine

K. Ito, F. Valentino, M. Farcy +26

We report the spectroscopic confirmation of a merging pair of massive quiescent galaxies at . Using JWST observations, we confirm that the two galaxies lie at a projected s…

astro-ph.GA2025★ 28 cited

Gas outflows in two recently quenched galaxies at z = 4 and 7

F. Valentino, K. E. Heintz, G. Brammer +33

Outflows are a key element in the baryon cycle of galaxies, and their properties provide a fundamental test for our models of how star formation quenches in galaxies. Here we repor…

astro-ph.GA2023★ 16 cited

SUPER VII. Morphology and kinematics of H emission in AGN host galaxies at Cosmic noon using SINFONI

D. Kakkad, V. Mainieri, G. Vietri +19

We present spatially resolved H properties of 21 type 1 AGN host galaxies at z2 derived from the SUPER survey. These targets were observed with the adaptive optics capabil…

astro-ph.GA2021★ 21 cited

A Multiwavelength Study of ELAN Environments (AMUSE). Mass budget, satellites spin alignment and gas infall in a massive quasar host halo

Fabrizio Arrigoni Battaia, Chian-Chou Chen, Hau-Yu Baobab Liu +14

The systematic targeting of extended Ly emission around high-redshift quasars resulted in the discovery of rare and bright Enormous Ly Nebulae (ELANe) associated with multipl…

astro-ph.GA2021★ 52 cited

Characterization of Two 2mm-detected Optically-Obscured Dusty Star-Forming Galaxies

Sinclaire M. Manning, Caitlin M. Casey, Jorge A. Zavala +22

The 2mm Mapping Obscuration to Reionization with ALMA (MORA) Survey was designed to detect high redshift (), massive, dusty star-forming galaxies (DSFGs). Here we presen…

astro-ph.GA2021★ 76 cited

Mapping Obscuration to Reionization with ALMA (MORA): 2mm Efficiently Selects the Highest-Redshift Obscured Galaxies

Caitlin M. Casey, Jorge A. Zavala, Sinclaire M. Manning +24

We present the characteristics of 2mm-selected sources from the largest Atacama Large Millimeter and submillimeter Array (ALMA) blank-field contiguous survey conducted to-date, the…

astro-ph.GA2021★ 64 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.GA2021★ 26 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.GA2021★ 5 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.GA2021★ 127 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.GA2020★ 25 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★ 17 cited

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…

astro-ph.GA2020★ 23 cited

REQUIEM-2D: Spatially Resolved Stellar Populations from HST 2D Grism Spectroscopy

Mohammad Akhshik, Katherine E. Whitaker, Gabriel Brammer +13

We present a novel Bayesian methodology to jointly model photometry and deep Hubble Space Telescope (HST) 2d grism spectroscopy of high-redshift galaxies. Our requiem2d code measur…

astro-ph.GA2019★ 44 cited

X-shooter Spectroscopy and HST Imaging of 15 Ultra Massive Quiescent Galaxies at

Mikkel Stockmann, Sune Toft, Anna Gallazzi +23

We present a detailed analysis of a large sample of spectroscopically confirmed ultra-massive quiescent galaxies () at . This sam…

astro-ph.GA2019★ 82 cited

Physical Characterization of an Unlensed Dusty Star-Forming Galaxy at

Caitlin M. Casey, Jorge A. Zavala, Manuel Aravena +23

We present a physical characterization of MMJ100026.36+021527.9 (a.k.a. ``MAMBO-9''), a dusty star-forming galaxy (DSFG) at . This is the highest redshift unlensed…

astro-ph.GA2019★ 26 cited

Compact Star-Forming Galaxies as Old Starbursts Becoming Quiescent

C. Gómez-Guijarro, G. E. Magdis, F. Valentino +8

Optically-compact star-forming galaxies (SFGs) have been proposed as immediate progenitors of quiescent galaxies, although their origin and nature are debated. Were they formed in…

astro-ph.GA2019★ 16 cited

MUSE unravels the ionisation and origin of metal enriched absorbers in the gas halo of a z = 2.92 radio galaxy

S. Kolwa, J. Vernet, C. De Breuck +9

We have used the Multi-Unit Spectroscopic Explorer (MUSE) to study the circumgalactic medium (CGM) of a z = 2.92 radio galaxy, MRC 0943-242 by parametrising its emitting and absorb…

astro-ph.GA2019★ 22 cited

Quenching by gas compression and consumption: A case study of a massive radio galaxy at z = 2.57

Allison W. S. Man, Matthew D. Lehnert, Joël D. R. Vernet +2

The objective of this work is to study how active galactic nuclei (AGN) influence star formation in host galaxies. We present a detailed investigation of the star-formation history…

astro-ph.GA2018★ 138 cited

Star formation quenching in massive galaxies

Allison Man, Sirio Belli

Understanding how and why star formation turns off in massive galaxies is a major challenge for studies of galaxy evolution. Many theoretical explanations have been proposed, but a…

astro-ph.GA2018★ 33 cited

Neutral versus ionized gas kinematics at z~2.6: The AGN-host starburst galaxy PKS 0529-549

Federico Lelli, Carlos De Breuck, Theresa Falkendal +4

We present a multiwavelength study of the AGN-host starburst galaxy PKS 0529-549 at z~2.6. We use (1) new ALMA observations of the dust continuum and of the [CI] 370 um line, traci…

astro-ph.GA2018★ 22 cited

Thirty-fold: Extreme gravitational lensing of a quiescent galaxy at

H. Ebeling, M. Stockmann, J. Richard +4

We report the discovery of eMACSJ1341-QG-1, a quiescent galaxy at located behind the massive galaxy cluster eMACSJ1341.92442 (). The system was identified as…

astro-ph.GA2017★ 120 cited

A massive, dead disk galaxy in the early Universe

Sune Toft, Johannes Zabl, Johan Richard +10

At redshift z = 2, when the Universe was just three billion years old, half of the most massive galaxies were extremely compact and had already exhausted their fuel for star format…

astro-ph.GA2017★ 82 cited

ALMA reveals starburst-like interstellar medium conditions in a compact star-forming galaxy at z ~ 2 using [CI] and CO

Gergö Popping, Roberto Decarli, Allison W. S. Man +9

We present ALMA detections of the [CI] 1-0, CO J=3-2, and CO J=4-3 emission lines, as well as the ALMA band 4 continuum for a compact star-forming galaxy (cSFG) at z=2.225, 3D-HST…

astro-ph.GA2017★ 43 cited

The Bright and Dark Sides of High-Redshift starburst galaxies from {\it Herschel} and {\it Subaru} observations

A. Puglisi, E. Daddi, A. Renzini +15

We present rest-frame optical spectra from the FMOS-COSMOS survey of twelve \textit{Herschel} starburst galaxies, with Star Formation Rate (SFR) elevated by 8,…