activity
20142024
most citedThe Gaia mission

7.1k citations · 12.1k across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.GA20248 cited

Limitations and rotation of the two-armed phase spiral in the Milky Way stellar disc

Simon Alinder, Paul McMillan, Thomas Bensby

Context: The Milky Way's history of recent disturbances is vividly demonstrated by a structure in the vertical phase-space distribution known as the Gaia phase spiral. A one-armed…

astro-ph.GA2024129 cited

Discovery of a dormant 33 solar-mass black hole in pre-release Gaia astrometry

Gaia Collaboration, P. Panuzzo, T. Mazeh +412

Gravitational waves from black-hole merging events have revealed a population of extra-galactic BHs residing in short-period binaries with masses that are higher than expected base…

astro-ph.GA2024

KRATOS: A large suite of N-body simulations to interpret the stellar kinematics of LMC-like discs

Ó. Jiménez-Arranz, S. Roca-Fàbrega, M. Romero-Gómez +4

We present KRATOS, a comprehensive suite of 28 open access pure N-body simulations of isolated and interacting LMC-like galaxies, to study the formation of substructures in their d…

astro-ph.GA20241 cited

Orbital analysis of stars in the nuclear stellar disc of the Milky Way

N. Nieuwmunster, M. Schultheis, M. Sormani +4

While orbital analysis studies were so far mainly focused on the Galactic halo, it is possible now to do these studies in the heavily obscured region close to the Galactic Centre.…

astro-ph.SR2023

Gaia Focused Product Release: Radial velocity time series of long-period variables

Gaia Collaboration, M. Trabucchi, N. Mowlavi +403

The third Gaia Data Release (DR3) provided photometric time series of more than 2 million long-period variable (LPV) candidates. Anticipating the publication of full radial-velocit…

astro-ph.GA20236 cited

Finding the dispersing siblings of young open clusters. Dynamical traceback simulations using Gaia DR3

Eero Vaher, David Hobbs, Paul McMillan +1

Context. Stars tend to form in clusters, but many escape their birth clusters very early. Identifying the escaped members of clusters can inform us about the dissolution of star cl…