activity
20232026
most citedMeasuring galaxy cluster mass profiles into the low acceleration regime with galaxy kinematics

24 citations · 68 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2026

The MUSE-Faint survey V. The binary fraction of Leo T

Daniel Vaz, Jarle Brinchmann, Sebastian Kamann +3

The Leo T dwarf galaxy, the faintest and least massive galaxy known to have recent star formation (), exhibits a high dynamical mass-to-light ratio based on its stellar…

astro-ph.GA2025★ 3 cited

The radial acceleration relation at the EDGE of galaxy formation: testing its universality in low-mass dwarf galaxies

Mariana P. Júlio, Justin I. Read, Marcel S. Pawlowski +6

A tight correlation between the baryonic and observed acceleration of galaxies has been reported over a wide range of mass () - the Radi…

astro-ph.GA2025★ 5 cited

GravSphere2: A higher-order Jeans method for mass-modeling spherical stellar systems

Andrés Bañares-Hernández, Justin I. Read, Mariana P. Júlio

Mass-modeling methods are used to infer the gravitational field of stellar systems, from globular clusters to giant elliptical galaxies. While many methods exist, most require assu…

astro-ph.GA2025

The effect of measurement uncertainties on the inferred stability of planes of satellite galaxies

Prem Kumar, Marcel S. Pawlowski, Kosuke Jamie Kanehisa +3

Observations have revealed that the MW, Andromeda, Centaurus A (and potentially other galaxies) host spatially thin and kinematically coherent planes of satellites. Such structures…

astro-ph.GA2024★ 1 cited

Testing a proposed "planarity" tool for studying satellite systems: On the alleged consistency of Milky Way satellite galaxy planes with CDM

Marcel S. Pawlowski, Mariana P. Júlio, Kosuke Jamie Kanehisa +1

The existence of planes of satellite galaxies has been identified as a long-standing challenge to CDM cosmology, due to the rarity of satellite systems in cosmological simulatio…

astro-ph.CO2024★ 1 cited

Gas thermodynamics meets galaxy kinematics: Joint mass measurements for eROSITA galaxy clusters

Pengfei Li, Ang Liu, Matthias Kluge +13

The mass of galaxy clusters is a critical quantity for probing cluster cosmology and testing theories of gravity, but its measurement could be biased given assumptions are inevitab…

astro-ph.GA2024★ 14 cited

The satellite galaxy plane of NGC 4490 in light of ΛCDM - Sparsity of similarly extreme analogs and a possible role of satellite pairs

Marcel S. Pawlowski, Oliver Müller, Salvatore Taibi +3

The galaxy system around NGC4490 was recently highlighted to display a flattened, kinematically correlated structure reminiscent of satellite galaxy planes around other hosts. Sinc…

astro-ph.GA2024★ 12 cited

Satellite group infall into the Milky Way: exploring the Crater-Leo case with new HST proper motions

Mariana P. Júlio, Marcel S. Pawlowski, Sangmo Tony Sohn +3

Context. Within Cold Dark Matter (CDM) simulations, Milky Way-like galaxies accrete some of their satellite galaxies in groups of 3-5 members rather than individually. It wa…

astro-ph.GA2023★ 8 cited

The MUSE-Faint survey. III. Constraining scalar field dark matter with Antlia B

Mariana P. Júlio, Jarle Brinchmann, Sebastiaan L. Zoutendijk +7

Aims. We use the stellar line-of-sight velocities of Antlia B (Ant B), a faint dwarf galaxy in the NGC 3109 association, to derive constraints on the fundamental properties of scal…

astro-ph.CO2023★ 24 cited

Measuring galaxy cluster mass profiles into the low acceleration regime with galaxy kinematics

Pengfei Li, Yong Tian, Mariana P. Júlio +7

We probe the dynamical mass profiles of 10 galaxy clusters from the HIghest X-ray FLUx Galaxy Cluster Sample (HIFLUGCS) using galaxy kinematics. We numerically solve the spherical…