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20122018
most citedThe long lives of giant clumps and the birth of outflows in gas-rich galaxies at high redshift

207 citations · 1.2k across the 19 of their papers we have counts for

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Showing astro-ph.COShow all

7 papers · 1 filter

astro-ph.CO2015★ 60 cited

nIFTy galaxy cluster simulations II: radiative models

Federico Sembolini, Pascal Jahan Elahi, Frazer R. Pearce +19

We have simulated the formation of a massive galaxy cluster (M = 1.110) in a CDM universe using 10 different codes (RAMSES, 2 in…

astro-ph.CO2013★ 207 cited

The long lives of giant clumps and the birth of outflows in gas-rich galaxies at high redshift

Frederic Bournaud, Valentin Perret, Florent Renaud +13

Star-forming disk galaxies at high redshift are often subject to violent disk instability, characterized by giant clumps whose fate is yet to be understood. The main question is wh…

astro-ph.CO2013★ 125 cited

Evolution of the mass, size, and star formation rate in high-redshift merging galaxies MIRAGE - A new sample of simulations with detailed stellar feedback

V. Perret, F. Renaud, B. Epinat +5

We aim at addressing the questions related to galaxy mass assembly through major and minor wet merging processes in the redshift range 1<z<2. A consequent fraction of Milky Way lik…

astro-ph.CO2012

The intriguing life of star-forming galaxies in the redshift range 1 < z < 2 using MASSIV

P. Amram, C. Lopez-Sanjuan, B. Epinat +13

MASSIV (Massiv Assembly Survey with SINFONI in VVDS) is an ESO large program which consists of 84 star-forming galaxies, spanning in a wide range of stellar masses, observed with t…

astro-ph.CO2012★ 1 cited

Mass Assembly of High-z Galaxies with MASSIV

V. Perret, B. Epinat, P. Amram +13

MASSIV (Mass Assembly Survey with SINFONI in VVDS) is a sample of 84 distant star-forming galaxies observed with the SINFONI Integral Field Unit (IFU) on the VLT. These galaxies ar…

astro-ph.CO2012★ 68 cited

MASSIV: Mass Assembly Survey with SINFONI in VVDS. V. The major merger rate of star-forming galaxies at 0.9 < z < 1.8 from IFS-based close pairs

C. López-Sanjuan, O. Le Fèvre, L. A. M. Tasca +12

We aim to measure the major merger rate of star-forming galaxies at 0.9 < z <1.8, using close pairs identified from integral field spectroscopy (IFS). We use the velocity field map…