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20042026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations · 17.2k across the 40 of their papers we have counts for

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Showing astro-ph.SRShow all

12 papers · 1 filter

astro-ph.SR2022★ 2 cited

Yet another star in the Albireo system -- The discovery of Albireo Ad

D. Jack, K. -P. Schröder, M. Mittag +1

Context. Albireo is a well-known bright visual double star. It is still unclear if the components A and B form a gravitationally bound system. The component Albireo A is itself a b…

astro-ph.SR2021★ 11 cited

Prediction of Astrometric-Microlensing Events from Gaia eDR3 Proper Motions

Jonas Klüter, Ulrich Bastian, Markus Demleitner +1

Astrometric microlensing is a unique tool to measure stellar masses. It allows us to determine the mass of the lensing star with an accuracy of a few per cent. In this paper, we up…

astro-ph.SR2020★ 11 cited

A celestial matryoshka: Dynamical and spectroscopic analysis of the Albireo system

Ronald Drimmel, Alessandro Sozzetti, Klaus-Peter Schroeder +4

We present a spectroscopic characterisation and a new orbital solution for the binary system beta Cyg Aa/Ac (MCA 55), the primary component (beta Cyg A) of the well-known wide doub…

astro-ph.SR2020★ 340 cited

Gaia Early Data Release 3: The Gaia Catalogue of Nearby Stars

Gaia Collaboration, R. L. Smart, L. M. Sarro +420

We produce a clean and well-characterised catalogue of objects within 100\,pc of the Sun from the \G\ Early Data Release 3. We characterise the catalogue through comparisons to the…

astro-ph.SR2019★ 9 cited

Gaia 8: Discovery of a star cluster containing beta Lyrae -- and of a larger old (extinct) star formation complex surrounding it

U. Bastian

Aims: To try and clarify whether there are stars in the neighbourhood of Lyrae which are physically connected to the famous prototype eclipsing binary. Methods: Scrutinize the…

astro-ph.SR2018★ 5 cited

The mass of Albireo Aa and the nature of Albireo AB: New aspects from Gaia DR2

U. Bastian, R. Anton

Aims: We aim to clarify the nature of Albireo AB and specifically to decipher whether it is an optical or physical pair. We also try to determine the mass of Albireo Aa. Methods: W…

astro-ph.SR2018★ 22 cited

Prediction of astrometric microlensing events from Gaia DR2 proper motions

J. Klüter, U. Bastian, M. Demleitner +1

Context: Astrometric gravitational microlensing is an excellent tool to determine the mass of stellar objects. Using precise astrometric measurements of the lensed position of a ba…

astro-ph.SR2018★ 16 cited

Ongoing Astrometric Microlensing Events of Two Nearby Stars

J. Klüter, U. Bastian, M. Demleitner +1

Context. Astrometric microlensing is an excellent tool to determine the mass of a stellar object. By measuring the astrometric shift of a background source star in combination with…

astro-ph.SR2018★ 135 cited

Gaia Data Release 2: Variable stars in the colour-absolute magnitude diagram

Gaia Collaboration, L. Eyer, L. Rimoldini +14

The ESA Gaia mission provides a unique time-domain survey for more than 1.6 billion sources with G ~ 21 mag. We showcase stellar variability across the Galactic colour-absolute mag…

astro-ph.SR2018

Gaia Data Release 2: Observational Hertzsprung-Russell diagrams

Gaia Collaboration, C. Babusiaux, F. van Leeuwen +450

We highlight the power of the Gaia DR2 in studying many fine structures of the Hertzsprung-Russell diagram (HRD). Gaia allows us to present many different HRDs, depending in partic…

astro-ph.SR2017★ 101 cited

Gaia Data Release 1. Testing the parallaxes with local Cepheids and RR Lyrae stars

Gaia Collaboration, G. Clementini, L. Eyer +588

Parallaxes for 331 classical Cepheids, 31 Type II Cepheids and 364 RR Lyrae stars in common between Gaia and the Hipparcos and Tycho-2 catalogues are published in Gaia Data Release…

astro-ph.SR2010★ 55 cited

Constraints on the origin of the massive, hot, and rapidly rotating magnetic white dwarf RE J 0317-853 from an HST parallax measurement

Baybars Külebi, Stefan Jordan, Edmund Nelan +2

We use the parallax measurements of RE J 0317-853 to determine its mass, radius, and cooling age and thereby constrain its evolutionary origins. We observed RE J 0317-853 with the…