activity
20082024
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations · 17.3k across the 59 of their papers we have counts for

collaborators

59 papers

astro-ph.GA2024★ 129 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.GA2023★ 47 cited

The Pristine survey -- XXIII. Data Release 1 and an all-sky metallicity catalogue based on Gaia DR3 BP/RP spectro-photometry

Nicolas F. Martin, Else Starkenburg, Zhen Yuan +38

We used the spectro-photometric information of ~219 million stars from Gaia's DR3 to calculate synthetic, narrow-band, metallicity-sensitive CaHK magnitudes that mimic the observat…

astro-ph.CO2023★ 29 cited

Constraints on the cosmological coupling of black holes from Gaia

Rene Andrae, Kareem El-Badry

Recent work has suggested that black holes (BHs) could be cosmologically coupled to the accelerated expansion of the universe, potentially becoming a candidate for dark energy. Thi…

astro-ph.SR2023★ 143 cited

Robust Data-driven Metallicities for 175 Million Stars from Gaia XP Spectra

Rene Andrae, Hans-Walter Rix, Vedant Chandra

We derive and publish data-driven estimates of stellar metallicities [M/H] for 175 million stars with low-resolution XP spectra published in Gaia DR3. The [M/H] values, along with…

astro-ph.SR2022★ 19 cited

Ultracool dwarfs in Gaia DR3

L. M. Sarro, A. Berihuete, R. L. Smart +36

Aims. In this work we use the Gaia DR3 set of ultracool dwarf candidates and complement the Gaia spectrophotometry with additional photometry in order to characterise its global pr…

astro-ph.GA2022★ 123 cited

The Poor Old Heart of the Milky Way

Hans-Walter Rix, Vedant Chandra, René Andrae +9

Massive disk galaxies like our Milky Way should host an ancient, metal-poor, and centrally concentrated stellar population. This population reflects the star formation and enrichme…