activity
20162026
most citedGOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies

89 citations · 519 across the 22 of their papers we have counts for

collaborators

22 papers

astro-ph.GA2026

How galaxies acquire their stellar mass at high redshift: High star formation efficiencies and the relative roles of dust and initial mass function

Hao Fu, Francesco Shankar, Fabio Fontanot +9

JWST has measured an unprecedented abundance of galaxies above , whose formation and evolution are still difficult to reconcile within traditional galaxy evolution mo…

astro-ph.GA2025

Ram-pressure stripping caught in action in a young cluster at

Ke Xu, Tao Wang, Emanuele Daddi +16

Galaxy clusters in the local Universe are dominated by massive quiescent galaxies with old ages, formed at high redshifts. Whether their quenching is driven by internal processes o…

astro-ph.GA2024★ 17 cited

NOEMA formIng Cluster survEy (NICE): Characterizing eight massive galaxy groups at in the COSMOS field

Nikolaj B. Sillassen, Shuowen Jin, Georgios E. Magdis +41

The NOEMA formIng Cluster survEy (NICE) is a large program targeting 69 massive galaxy group candidates at in six deep fields. We report spectroscopic confirmation of eight g…

astro-ph.GA2023★ 17 cited

Noema formIng Cluster survEy (NICE): Discovery of a starbursting galaxy group with a radio-luminous core at z=3.95

Luwenjia Zhou, Tao Wang, Emanuele Daddi +34

The study of distant galaxy groups and clusters at the peak epoch of star formation is limited by the lack of a statistically and homogeneously selected and spectroscopically confi…

astro-ph.GA2023★ 12 cited

Accelerated Formation of Ultra-Massive Galaxies in the First Billion Years

Mengyuan Xiao, Pascal Oesch, David Elbaz +35

Recent JWST observations have revealed an unexpected abundance of massive galaxy candidates in the early Universe, extending further in redshift and to lower luminosity than what h…

astro-ph.GA2023★ 8 cited

Accelerated structural evolution of galaxies in a starbursting cluster at z=2.51

Can Xu, Tao Wang, Qiusheng Gu +11

Structural properties of cluster galaxies during their peak formation epoch, provide key information on whether and how environment affects galaxy formation and evolut…

astro-ph.GA2023

The IR Compactness of Dusty Galaxies Set Star-formation and Dust Properties at z~0-2

Jed McKinney, Alexandra Pope, Allison Kirkpatrick +9

Surface densities of gas, dust and stars provide a window into the physics of star-formation that, until the advent of high-resolution far-infrared/sub-millimeter observations, has…

astro-ph.GA2023★ 38 cited

Little Red Dots: an abundant population of faint AGN at z~5 revealed by the EIGER and FRESCO JWST surveys

Jorryt Matthee, Rohan P. Naidu, Gabriel Brammer +25

Characterising the prevalence and properties of faint active galactic nuclei (AGN) in the early Universe is key for understanding the formation of supermassive black holes (SMBHs)…

astro-ph.GA2023★ 36 cited

JWST CEERS probes the role of stellar mass and morphology in obscuring galaxies

Carlos Gómez-Guijarro, Benjamin Magnelli, David Elbaz +38

In recent years, observations have uncovered a population of massive galaxies that are invisible or very faint in deep optical/near-infrared (near-IR) surveys but brighter at longe…

astro-ph.GA2023★ 12 cited

The Gas Mass Reservoir of Quiescent Galaxies at Cosmic Noon

David Blánquez-Sesé, C. Gómez-Guijarro, G. E. Magdis +14

We present a 1.1mm stacking analysis of moderately massive (log(/) = 10.7 0.2) quiescent galaxies (QGs) at , searching for cold du…

astro-ph.GA2022★ 41 cited

The hidden side of cosmic star formation at z > 3: Bridging optically-dark and Lyman break galaxies with GOODS-ALMA

Mengyuan Xiao, David Elbaz, Carlos Gómez-Guijarro +37

Our current understanding of the cosmic star formation history at z>3 is primarily based on UV-selected galaxies (i.e., LBGs). Recent studies of H-dropouts have revealed that we ma…

astro-ph.GA2022★ 13 cited

Starbursts with suppressed velocity dispersion revealed in a forming cluster at z=2.51

Mengyuan Xiao, Tao Wang, David Elbaz +19

One of the most prominent features of galaxy clusters is the presence of a dominant population of massive ellipticals in their cores. Stellar archaeology suggests that these gigant…

astro-ph.GA2022★ 43 cited

GOODS-ALMA 2.0: Starbursts in the main sequence reveal compact star formation regulating galaxy evolution prequenching

C. Gómez-Guijarro, D. Elbaz, M. Xiao +38

Compact star formation appears to be generally common in dusty star-forming galaxies (SFGs). However, its role in the framework set by the scaling relations in galaxy evolution rem…

astro-ph.GA2021★ 14 cited

Star-Forming S0 Galaxies in SDSS-IV MaNGA Survey

Ke Xu, Qiusheng Gu, Shiying Lu +3

To investigate star-forming activities in early-type galaxies, we select a sample of 52 star-forming S0 galaxies (SFS0s) from the SDSS-IV MaNGA survey. We find that SFS0s have smal…

astro-ph.GA2021★ 89 cited

GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies

C. Gómez-Guijarro, D. Elbaz, M. Xiao +36

Submillimeter/millimeter observations of dusty star-forming galaxies with the Atacama Large Millimeter/submillimeter Array (ALMA) have shown that dust continuum emission generally…

astro-ph.GA2021★ 5 cited

PGC 38025: A Star-forming Lenticular Galaxy With an Off-nuclear Star-forming Core

Zhengyi Chen, Qiu-Sheng Gu, Rubén García-Benito +4

Lenticular galaxies (S0s) were considered mainly as passive evolved spirals due to environmental effects for a long time; however, most S0s in the field cannot fit into this common…

astro-ph.GA2020★ 51 cited

GOODS-ALMA: The slow downfall of star-formation in = 2-3 massive galaxies

M. Franco, D. Elbaz, L. Zhou +34

We investigate the properties of a sample of 35 galaxies, detected with ALMA at 1.1 mm in the GOODS-ALMA field (area of 69 arcmin, resolution = 0.60", RMS 0.18 mJy bea…

astro-ph.GA2020★ 24 cited

GOODS-ALMA: Using IRAC and VLA to probe fainter millimeter galaxies

M. Franco, D. Elbaz, L. Zhou +33

In this paper, we extend the source detection in the GOODS-ALMA field (69 arcmin, rms sensitivity 0.18 mJy.beam), to deeper levels than presented in Franco…

astro-ph.GA2020★ 7 cited

The physical properties of S0 galaxy PGC 26218: the origin of starburst and star formation

Xue Ge, Qiu-Sheng Gu, Rubén García-Benito +2

We present 2D-spectroscopic observations from Centro Astronómico Hispano Alemán (CAHA) 3.5 m telescope and the millimetre observation from NOrthern Extended Millimeter Array (NOEMA…

astro-ph.GA2018★ 65 cited

Revealing environmental dependence of molecular gas content in a distant X-ray cluster at z=2.51

Tao Wang, David Elbaz, Emanuele Daddi +13

We present a census of the molecular gas properties of galaxies in the most distant known X-ray cluster, CLJ1001, at z=2.51, using deep observations of CO(1-0) with JVLA. In total…

astro-ph.GA2018★ 6 cited

The Physical Characteristics of Interstellar Medium in NGC 3665 with Herschel Observations

Meng-Yuan Xiao, Yinghe Zhao, Qiu-Sheng Gu +1

We present the analysis of the physical properties of the interstellar medium (ISM) in the nearby early-type galaxy NGC 3665, based on the far-infrared (FIR) photometric and spectr…

astro-ph.GA2016★ 21 cited

The Nuclear Activities of Nearby S0 Galaxies

Mengyuan Xiao, Qiusheng Gu, Yanmei Chen +1

We present a study of nuclear activities in nearby S0 galaxies. After cross-matching the Sloan Digital Sky Survey Data Release 7 (SDSS DR7) with the Third Reference Catalog of Brig…