activity
20002024
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations · 17.2k across the 76 of their papers we have counts for

collaborators

73 papers

astro-ph.EP2024★ 8 cited

HST astrometry of the closest Brown Dwarfs -- II. Improved parameters and constraints on a third body

L. R. Bedin, J. Dietrich, A. J. Burgasser +5

Located at less than 2pc away, Luhman16AB (WISE.J104915.57-531906.1) is the closest pair of brown dwarfs and third closest `stellar' system to Earth. An exoplanet candidate in the…

astro-ph.SR2023

Discovery of astrometric accelerations by dark companions in the globular cluster Centauri

Imants Platais, Johannes Sahlmann, Leo Girardi +6

We present results from the search for astrometric accelerations of stars in Centauri using 13 years of regularly-scheduled {\it Hubble Space Telescope} WFC3/UVIS calibration o…

astro-ph.SR2023

An update of SB9 orbits using HERMES/Mercator radial velocities

Thibault Merle, Dimitri Pourbaix, Alain Jorissen +3

The Gaia mission is delivering a large number of astrometric orbits for binary stars. By combining these with spectroscopic orbits for systems with two observable spectra (SB2), it…

astro-ph.IM2022★ 54 cited

Gaia Data Release 3: Gaia scan-angle dependent signals and spurious periods

B. Holl, C. Fabricius, J. Portell +23

Context: Gaia DR3 time series data may contain spurious signals related to the time-dependent scan angle. Aims: We aim to explain the origin of scan-angle dependent signals and how…

astro-ph.GA2022★ 14 cited

Gaia Data Release 3: Surface brightness profiles of galaxies and host galaxies of quasars

C. Ducourant, A. Krone-Martins, L. Galluccio +13

Since July 2014, the Gaia space mission has been continuously scanning the sky and observing the extragalactic Universe with unprecedented spatial resolution in the optical domain…

astro-ph.SR2022★ 144 cited

Gaia Data Release 3. Astrometric binary star processing

Jean-Louis Halbwachs, Dimitri Pourbaix, Frédéric Arenou +6

Context.The Gaia Early Data Release 3 contained the positions, parallaxes and proper motions of 1.5 billion sources, among which some did not fit well the "single star" model. Bina…