activity
20232026
most citedSimulations of cluster ultra-diffuse galaxies in MOND

4 citations · 8 across the 8 of their papers we have counts for

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Showing astro-ph.GAShow all

10 papers · 1 filter

astro-ph.GA2026

The galactic HI-to-halo mass relation from isolated galaxies to cosmological hydrodynamic simulations

Marie Korsaga, Jonathan Freundlich, Benoit Famaey +15

The relation between HI and dark matter (DM) halo masses provides key insights into gas accretion and the regulation of galaxy formation. In a previous study based on SPARC and LIT…

astro-ph.GA2026

Mapping parameters of idealised hydrodynamic galaxy simulations to bar properties: a case study with the RAMSES code

Srikanth T. Nagesh, Benoit Famaey, Jonathan Freundlich +4

Cosmological simulations with high spatial resolution often struggle to reproduce the observed fraction of galactic bars across redshift and may produce bars that are too short. To…

astro-ph.GA2026★ 3 cited

MUSE-DARK III: The evolution of the radial acceleration relation at intermediate redshifts

B. I. Ciocan, N. F. Bouché, J. Fensch +5

The radial acceleration relation (RAR) is a tight empirical correlation between the observed radial acceleration (a_tot) and the baryonic radial acceleration (a_bar) measured acros…

astro-ph.GA2026★ 1 cited

MUSE-DARK-II: 3D morpho-kinematic modelling of lensed galaxies. Tully-Fisher relation of star-forming galaxies

Alexandre Jeanneau, Johan Richard, Nicolas F. Bouché +5

In a series of papers on lensed kinematics, we seek to combine the sensitivity of 3D forward modelling to low signal-to-noise ratio outskirts with the enhanced spatial resolution o…

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…