activity
20202025
most citedEffects of close binary evolution on the main-sequence morphology of young star clusters

75 citations · 106 across the 5 of their papers we have counts for

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Showing astro-ph.GAShow all

5 papers · 1 filter

astro-ph.GA2025

The observed total star formation rate function up to z \sim 6: complementary UV and IR contributions and comparison with state-of-the-art galaxy formation models

A. Traina, C. Gruppioni, I. Delvecchio +21

We investigate how the obscured IR-derived and the dust-corrected UV star formation rate functions (SFRFs) compare with each other, and with predictions from state-of-the-art theor…

astro-ph.GA20254 cited

ACOSMOS: The dust content of massive quiescent galaxies and its evolution with cosmic time

Sylvia Adscheid, Benjamin Magnelli, Laure Ciesla +3

We study the dust content of massive () quiescent galaxies (QGs) at redshifts to place constraints on the evolution of their cold interstella…

astro-ph.GA2024

Dust emission from the bulk of galaxies at the Epoch of Reionization

L. Ciesla, S. Adscheid, B. Magnelli +6

[Abridged] Our view of dust in primordial galaxies is limited towards a few tens of z~7 galaxies, pre-selected from UV-optical observations, and are thus not necessarily representa…

astro-ph.GA202427 cited

ACOSMOS and AGOODSS: Continuum Source Catalogues and Multi-band Number Counts

Sylvia Adscheid, Benjamin Magnelli, Daizhong Liu +7

Galaxy submillimetre number counts are a fundamental measurement in our understanding of galaxy evolution models. Most early measurements are obtained via single-dish telescopes wi…

astro-ph.GA2023

ACOSMOS: Dissecting the gas content of star-forming galaxies across the main sequence at 1.2 < 1.6

Tsan-Ming Wang, Benjamin Magnelli, Eva Schinnerer +5

We aim to understand the physical mechanisms that drive star formation in a sample of mass-complete (>10) star-forming galaxies (SFGs) at 1.2 < 1.6. We se…