activity
20142025
most citedThe Gaia mission

7.1k citations · 9.9k across the 16 of their papers we have counts for

collaborators

15 papers

astro-ph.GA20249 cited

WEAVE First Light Observations: Origin and Dynamics of the Shock Front in Stephan's Quintet

M. I. Arnaudova, S. Das, D. J. B. Smith +62

We present a detailed study of the large-scale shock front in Stephan's Quintet, a byproduct of past and ongoing interactions. Using integral-field spectroscopy from the new Willia…

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.GA2024

Structure, kinematics and time evolution of the Galactic Warp from Classical Cepheids

Mauro Cabrera-Gadea, Cecilia Mateu, Pau Ramos +11

The warp is a well-known undulation of the Milky Way disc. Its structure has been widely studied, but only since Gaia DR2 has it been possible to reveal its kinematic signature bey…

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.GA202311 cited

Exploring the structure and kinematics of the Milky Way through A stars

J. Ardèvol, M. Monguió, F. Figueras +2

Despite their relatively high intrinsic brightness and the fact that they are more numerous than younger OB stars and kinematically colder than older red giants, A-type stars have…