activity
20172021
most citedOn the SFR-M main sequence archetypal star-formation history and analytical models

133 citations · 594 across the 13 of their papers we have counts for

collaborators

19 papers

astro-ph.GA202164 cited

Ultra diffuse galaxies in the MATLAS low-to-moderate density fields

Francine R. Marleau, Rebecca Habas, Melina Poulain +10

Recent advances in deep dedicated imaging surveys over the past decade have uncovered a surprisingly large number of extremely faint low surface brightness galaxies with large phys…

astro-ph.GA202112 cited

Stellar feedback in a clumpy galaxy at 3.4

E. Iani, A. Zanella, J. Vernet +18

Giant star-forming regions (clumps) are widespread features of galaxies at . Theory predicts that they can play a crucial role in galaxy evolution if they survive to…

astro-ph.GA202167 cited

Structure and morphology of the MATLAS dwarf galaxies and their central nuclei

Melina Poulain, Francine R. Marleau, Rebecca Habas +10

We present a photometric study of the dwarf galaxy population in the low to moderate density environments of the MATLAS (Mass Assembly of early-Type gaLAxies with their fine Struct…

astro-ph.GA202119 cited

Hierarchical fragmentation in high redshift galaxies revealed by hydrodynamical simulations

Baptiste Faure, Frédéric Bournaud, Jérémy Fensch +4

High-redshift star-forming galaxies have very different morphologies compared to nearby ones. Indeed, they are often dominated by bright star-forming structures of masses up to $10…

astro-ph.GA20218 cited

Low Surface Brightness Galaxies in z > 1 Galaxy Clusters: HST approaches the Progenitors of Local Ultra Diffuse Galaxies

Aisha Bachmann, Remco F. J. van der Burg, Jérémy Fensch +2

Ultra Diffuse Galaxies (UDGs), a type of large Low Surface Brightness (LSB) galaxies with particularly large effective radii (r_eff > 1.5 kpc), are now routinely studied in the loc…

astro-ph.GA202114 cited

A titanic interstellar medium ejection from a massive starburst galaxy at redshift 1.4

Annagrazia Puglisi, Emanuele Daddi, Marcella Brusa +12

Feedback-driven winds from star formation or active galactic nuclei might be a relevant channel for the abrupt quenching star formation in massive galaxies. However, both observati…