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20022026
most citedThe reversal of the star formation-density relation in the distant universe

1.6k citations · 6.8k across the 35 of their papers we have counts for

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17 papers · 1 filter

astro-ph.CO2013★ 46 cited

Spatially-resolved dust properties of the GRB 980425 host galaxy

Michał J. Michałowski, L. K. Hunt, E. Palazzi +30

Gamma-ray bursts (GRBs) have been proposed as a tool for studying star formation in the Universe, so it is crucial to investigate whether their host galaxies and immediate environm…

astro-ph.CO2013★ 81 cited

Ultraviolet to infrared emission of z>1 galaxies: Can we derive reliable star formation rates and stellar masses?

V. Buat, S. Heinis, M. Boquien +6

We seek to derive star formation rates (SFR) and stellar masses (M_star) in distant galaxies and to quantify the main uncertainties affecting their measurement. We explore the impa…

astro-ph.CO2013★ 142 cited

Swirling around filaments: are large-scale structure vortices spinning up dark halos?

Clotilde Laigle, Christophe Pichon, Sandrine Codis +9

The kinematic analysis of dark matter and hydrodynamical simulations suggests that the vorticity in large-scale structure is mostly confined to, and predominantly aligned with thei…

astro-ph.CO2012★ 234 cited

A unified empirical model for infrared galaxy counts based on observed physical evolution of distant galaxies

Matthieu Béthermin, Emanuele Daddi, Georgios Magdis +10

We reproduce the mid-infrared to radio galaxy counts with a new empirical model based on our current understanding of the evolution of main-sequence (MS) and starburst (SB) galaxie…

astro-ph.CO2012★ 103 cited

Dissecting the stellar mass-SFR correlation in z=1 star-forming disk galaxies

F. Salmi, E. Daddi, D. Elbaz +5

Using a mass-limited sample of 24um-detected, star-forming galaxies at 0.5<z<1.3, we study the mass-star formation rate (SFR) correlation and its tightness. The correlation is well…

astro-ph.CO2012★ 5 cited

The spin of late-type galaxies at redshifts z < 1.2

Bernardo Cervantes-Sodi, X. Hernandez, Ho Seong Hwang +2

We study the evolution of the galactic spin using data of high redshift galaxies in the fields of the Great Observatories Origins Deep Survey (GOODS). Through simple dynamical cons…

astro-ph.CO2012★ 32 cited

Constraining the nature of the most distant Gamma-Ray Burst host galaxies

S. Basa, J. G. Cuby, S. Savaglio +5

Long duration gamma-ray bursts (GRBs) allow us to explore the distant Universe, and are potentially the most effective tracer of the most distant objects. Our current knowledge of…

astro-ph.CO2011★ 52 cited

GOODS-Herschel: the impact of galaxy-galaxy interactions on the far-infrared properties of galaxies

H. S. Hwang, D. Elbaz, M. Dickinson +15

We study the impact of galaxy-galaxy interactions on the FIR properties of galaxies and its evolution at 0<z<1.2. Using the high-z galaxies in the fields of GOODS observed by Hersc…

astro-ph.CO2011★ 164 cited

Red Nuggets at High Redshift: Structural Evolution of Quiescent Galaxies Over 10 Gyr of Cosmic History

Ivana Damjanov, Roberto G. Abraham, Karl Glazebrook +15

We present an analysis of the size growth seen in early-type galaxies over 10 Gyr of cosmic time. Our analysis is based on a homogeneous synthesis of published data from 17 spectro…

astro-ph.CO2011★ 1.1k cited

GOODS-Herschel: an infrared main sequence for star-forming galaxies

D. Elbaz, M. Dickinson, H. S. Hwang +52

We present the deepest far-IR observations obtained with Herschel and examine the 3-500um SEDs of galaxies at 0<z<2.5, supplemented by a local reference sample from IRAS, ISO, Spit…

astro-ph.CO2011★ 342 cited

Evolution of the dusty infrared luminosity function from z=0 to z=2.3 using observations from Spitzer

B. Magnelli, D. Elbaz, R. R. Chary +4

We derive the evolution of the infrared (IR) luminosity function (LF) over the last 4/5ths of cosmic time, using deep 24um and 70um imaging of the GOODS North and South fields. We…

astro-ph.CO2010★ 161 cited

Modeling the evolution of infrared galaxies: A Parametric backwards evolution model

Matthieu Béthermin, Hervé Dole, Guilaine Lagache +2

We aim at modeling the infrared galaxy evolution in an as simple as possible way and reproduce statistical properties among which the number counts between 15 microns and 1.1 mm, t…

astro-ph.CO2010★ 166 cited

Evolution of Dust Temperature of Galaxies through Cosmic Time as seen by Herschel

H. S. Hwang, D. Elbaz, G. E. Magdis +112

We study the dust properties of galaxies in the redshift range 0.1<z<2.8 observed by the Herschel Space Observatory in the field of the Great Observatories Origins Deep Survey-Nort…

astro-ph.CO2010★ 201 cited

Herschel unveils a puzzling uniformity of distant dusty galaxies

D. Elbaz, H. S. Hwang, B. Magnelli +106

The Herschel Space Observatory enables us to accurately measure the bolometric output of starburst galaxies and active galactic nuclei (AGN) by directly sampling the peak of their…

astro-ph.CO2009★ 56 cited

Quasar induced galaxy formation: a new paradigm ?

D. Elbaz, K. Jahnke, E. Pantin +2

We discuss observational evidence that quasars play a key role in the formation of galaxies starting from the detailed study of the quasar HE0450-2958 and extending the discussion…

astro-ph.CO2009★ 36 cited

A near-infrared excess in the continuum of high-redshift galaxies: a tracer of star formation and circumstellar disks?

E. Mentuch, R. G. Abraham, K. Glazebrook +13

A broad continuum excess in the near-infrared, peaking in the rest-frame at 2-5 micron, is detected in a spectroscopic sample of 88 galaxies at 0.5<z<2.0 taken from the Gemini Deep…

astro-ph.CO2009★ 95 cited

Cosmic star-formation history from a non-parametric inversion of infrared galaxy counts

Damien Le Borgne, David Elbaz, Pierre Ocvirk +1

[Abridged] This paper aims at providing new conservative constraints to the cosmic star-formation history from the empirical modeling of mid- and far-infrared data. We perform a no…