activity
20052024
most citedThe Gaia mission

7.1k citations · 7.5k across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.IM2024★ 13 cited

The PLATO Mission

Heike Rauer, Conny Aerts, Juan Cabrera +842

PLATO (PLAnetary Transits and Oscillations of stars) is ESA's M3 mission designed to detect and characterise extrasolar planets and perform asteroseismic monitoring of a large numb…

astro-ph.SR2022★ 91 cited

Gaia Data Release 3: The Galaxy in your preferred colours. Synthetic photometry from Gaia low-resolution spectra

Gaia Collaboration, P. Montegriffo, M. Bellazzini +27

Gaia Data Release 3 provides novel flux-calibrated low-resolution spectrophotometry for about 220 million sources in the wavelength range 330nm - 1050nm (XP spectra). Synthetic pho…

astro-ph.SR2022★ 34 cited

Gaia Data Release 3: Microlensing Events from All Over the Sky

Łukasz Wyrzykowski, K. Kruszyńska, K. A. Rybicki +12

Context: One of the rarest types of variability is the phenomenon of gravitational microlensing, a transient brightening of a background star due to an intervening lensing object.…

astro-ph.IM2016★ 7.1k cited

The Gaia mission

Gaia Collaboration

Gaia is a cornerstone mission in the science programme of the European Space Agency (ESA). The spacecraft construction was approved in 2006, following a study in which the original…

astro-ph.SR2016★ 34 cited

Vetting Galactic Leavitt Law Calibrators using Radial Velocities: On the Variability, Binarity, and Possible Parallax Error of 19 Long-period Cepheids

R. I. Anderson, S. Casertano, A. G. Riess +9

We investigate the radial velocity (RV) variability and spectroscopic binarity of 19 Galactic long-period ( d) classical Cepheid variable stars whose trig…

astro-ph.GA2013★ 47 cited

The Gaia-ESO Survey: Abundance ratios in the inner-disk open clusters Trumpler 20, NGC 4815, NGC 6705

L. Magrini, S. Randich, D. Romano +50

Open clusters are key tools to study the spatial distribution of abundances in the disk and their evolution with time. Using the first release of stellar parameters and abundances…