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20202026
most citedKnocking on giants' doors: I. The evolution of the dust-to-stellar mass ratio in distant dusty galaxies

65 citations · 71 across the 13 of their papers we have counts for

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Showing 2026Show all

6 papers · 1 filter

astro-ph.GA2026

Probing the molecular gas content of galaxies in an over-dense group at z~0.7: A test case for environmental quenching

Jonathan Freundlich, Benoît Epinat, Thierry Contini +14

We investigated the impact of group environment on molecular gas reservoirs at an intermediate redshift by observing the CO(2-1) emission from the galaxy group COSMOS-Gr30 at $z \s…

astro-ph.GA2026

IllustrisTNG50 angular momentum maps: tracing the morpho-kinematic evolution of galaxies

Juan Manuel Pacheco-Arias, Benoît Epinat, Philippe Amram +2

Following the first observational study of the two-dimensional spatial distribution of stellar specific angular momentum (sAM) in late-type galaxies, we quantify the morpho-kinemat…

astro-ph.GA2026

Euclid preparation. Probing galaxy evolution within cosmic voids in Euclid-like simulations

Euclid Collaboration, G. Papini, O. Cucciati +294

The evolution of galaxies is profoundly influenced by the environment in which they reside. Cosmic voids serve as pristine laboratories for studying galaxy evolution in the relativ…

astro-ph.GA2026

Cosmic evolution of the [CII]-to-dense neutral gas relation

Cédric Accard, Florent Renaud, Katarina Kraljic +3

The [CII] 158 m line is widely used to trace star formation and the gas contents of high-redshift galaxies. However, it remains unclear under which physical conditions it reliab…

astro-ph.GA2026

Starbursts hiding in the main sequence: a pathway toward quenching?

Florent Renaud, Katarina Kraljic, Jonathan Freundlich +10

Star-forming galaxies spend most of their lifetimes on the star-forming main sequence, which establishes a tight empirical and statistical relation between stellar mass and star-fo…

astro-ph.GA2026

Evaluating star formation rates at z = 5

D. Ismail, K. Kraljic, M. Béthermin +11

Inferring the star formation rates (SFR) in high redshift galaxies remains challenging, owing to observational limitations or uncertainties in calibration methods that link luminos…