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19942022
most citedCFBDS J005910.90-011401.3: reaching the T-Y Brown Dwarf transition?

144 citations · 1.1k across the 21 of their papers we have counts for

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Showing 2020Show all

6 papers · 1 filter

astro-ph.SR2020

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.GA2020

Gaia Early Data Release 3: Acceleration of the solar system from Gaia astrometry

Gaia Collaboration, S. A. Klioner, F. Mignard +414

Context. Gaia Early Data Release 3 (Gaia EDR3) provides accurate astrometry for about 1.6 million compact (QSO-like) extragalactic sources, 1.2 million of which have the best-quali…

astro-ph.GA2020

Kinematics and dynamics of Gaia red clump stars

Jean-Baptiste Salomon, Olivier Bienaymé, Céline Reylé +2

We analyse the kinematics and dynamics of a homogeneous sample of red clump stars selected from the second Gaia data release catalogue in the direction of the Galactic poles. The l…

astro-ph.GA2020

The Blanco DECam Bulge Survey. I. The Survey Description and Early Results

R. Michael Rich, Christian I. Johnson, Michael Young +18

The Blanco Dark Energy Camera (DECam) Bulge survey is a Vera Rubin Observatory (LSST) pathfinder imaging survey, spanning sq. deg. of the Southern Galactic bulge, $-2^\c…

astro-ph.EP2020121 cited

Predictions of the Nancy Grace Roman Space Telescope Galactic Exoplanet Survey II: Free-Floating Planet Detection Rates

Samson A. Johnson, Matthew T. Penny, B. Scott Gaudi +5

The Nancy Grace Roman Space Telescope (Roman) will perform a Galactic Exoplanet Survey (RGES) to discover bound exoplanets with semi-major axes greater than 1 au using gravitationa…

astro-ph.EP202012 cited

MaBlS-2: high-precision microlensing modelling for the large-scale survey era

David Specht, Eamonn Kerins, Supachai Awiphan +1

Galactic microlensing datasets now comprise in excess of events, and with the advent of next generation microlensing surveys that may be undertaken with facilities such as t…