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19932026
most citedThe velocity function in the local environment from LCDM and LWDM constrained simulations

190 citations · 1.6k across the 37 of their papers we have counts for

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Showing astro-ph.GAShow all

9 papers · 1 filter

astro-ph.GA20241 cited

Variable gravitational potential of Milky Way analogues in HESTIA suite

Naira R. Arakelyan, Sergey V. Pilipenko, Stefan Gottlöber +3

Investigations of trajectories of various objects orbiting the Milky Way (MW) halo with modern precision, achievable in observations by Gaia, requires sophisticated, non-stationary…

astro-ph.GA20235 cited

Exploring the centre of mass properties of LG-like galaxies

Jean-Baptiste Salomon, Noam Libeskind, Yehuda Hoffman

From high resolution cosmological simulations of the Local Group in realistic environment, namely HESTIA simulations, we study the position and kinematic deviations that may arise…

astro-ph.GA2020

The proper motion of Andromeda from Gaia eDR3: confirming a nearly radial orbit

J. -B. Salomon, R. Ibata, C. Reylé +4

We present an analysis of the proper motion of the Andromeda galaxy (M31), based on the Early Third Data Release of the Gaia mission. We use the Gaia photometry to select young blu…

astro-ph.GA2020

The sum of the masses of the Milky Way and M31: a likelihood-free inference approach

Pablo Lemos, Niall Jeffrey, Lorne Whiteway +3

We use Density Estimation Likelihood-Free Inference, Cold Dark Matter simulations of galaxy pairs, and data from Gaia and the Hubble Space Telescope to infer the sum…

astro-ph.GA2020126 cited

The Hestia project: simulations of the Local Group

Noam I. Libeskind, Edoardo Carlesi, Rob J. J. Grand +19

We present the Hestia simulation suite: High-resolutions Environmental Simulations of The Immediate Area, a set of cosmological simulations of the Local Group. Initial conditions c…

astro-ph.GA201914 cited

On the Mass Assembly History of the Local Group

Edoardo Carlesi, Yehuda Hoffman, Stefan Gottlöber +4

In this work an ensemble of simulated Local Group analogues is used to constrain the properties of the mass assembly history of the Milky Way (MW) and Andromeda (M31) galaxies. The…