activity
20102019
most citedThe [CII] 158 micron line emission in high-redshift galaxies

198 citations · 659 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2019★ 11 cited

G.A.S. I: A prescription for turbulence-regulated star formation and its impact on galaxy properties

M. Cousin, P. Guillard, M. D. Lehnert

Star formation in galaxies is inefficient, and understanding how star formation is regulated in galaxies is one of the most fundamental challenges of contemporary astrophysics. Rad…

astro-ph.GA2019★ 18 cited

G.A.S. II: Dust extinction in galaxies; Luminosity functions and InfraRed eXcess

M. Cousin, V. Buat, G. Lagache +1

Dust is a crucial component of the interstellar medium of galaxies. The presence of dust strongly affects the light produced by stars within a galaxy. As these photons are our main…

astro-ph.GA2017★ 198 cited

The [CII] 158 micron line emission in high-redshift galaxies

G. Lagache, M. Cousin, M. Chatzikos

The [CII] fine structure transition at 158 microns is the dominant cooling line of cool interstellar gas, and is the brightest of emission lines from star forming galaxies from FIR…

astro-ph.GA2017★ 186 cited

The impact of clustering and angular resolution on far-infrared and millimeter continuum observations

Matthieu Bethermin, Hao-Yi Wu, Guilaine Lagache +7

Follow-up observations at high-angular resolution of submillimeter galaxies showed that the single-dish sources are comprised of a blend of several galaxies. Consequently, number c…

astro-ph.GA2016★ 18 cited

Metal enrichment in a semi-analytical model, fundamental scaling relations, and the case of Milky Way galaxies

Morgane Cousin, Véronique Buat, Samuel Boissier +3

Gas flows play a fundamental role in galaxy formation and evolution, providing the fuel for the star formation process. These mechanisms leave an imprint in the amount of heavy ele…

astro-ph.GA2014★ 19 cited

Towards a new modelling of gas flows in a semi-analytical model of galaxy formation and evolution

Morgane Cousin, Guilaine Lagache, Matthieu Bethermin +1

We present an extended version of the semi-analytical model, GalICS. Like its predecessor, eGalICS applies a post-treatment of the baryonic physics on pre-computed dark-matter merg…

astro-ph.GA2014★ 21 cited

Galaxy stellar mass assembly: the difficulty matching observations and semi-analytical predictions

Morgane Cousin, Guilaine Lagache, Matthieu Bethermin +2

Semi-analytical models (SAMs) are currently the best way to understand the formation of galaxies within the cosmic dark-matter structures. While they fairly well reproduce the loca…

astro-ph.CO2013★ 108 cited

The redshift-evolution of the distribution of star formation among dark matter halos as seen in the infrared

Matthieu Béthermin, Lingyu Wang, Olivier Doré +5

[Abridged] Recent studies revealed a strong correlation between the star formation rate (SFR) and stellar mass of star-forming galaxies, the so-called star-forming main sequence. A…

astro-ph.CO2010★ 80 cited

Submillimeter Number Counts at 250, 350 and 500 microns in BLAST data

M. Béthermin, H. Dole, M. Cousin +1

BLAST (Balloon-borne Large-Aperture Submillimeter Telescope) performed the first deep and wide extragalactic survey at 250, 350 and 500 um. The extragalactic number counts at these…