activity
20032024
most citedThe Gaia mission

7.1k citations · 9.9k across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2024

Stellar Population Astrophysics (SPA) with TNG, Fluorine abundances in seven open clusters

Shilpa Bijavara Seshashayana, Henrik Jönsson, Valentina D'Orazi +9

The age, evolution, and chemical properties of the Galactic disk can be effectively ascertained using open clusters. Within the large program Stellar Populations Astrophysics at th…

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.IM2017★ 395 cited

Gaia Data Release 1: Catalogue validation

F. Arenou, X. Luri, C. Babusiaux +42

Before the publication of the Gaia Catalogue, the contents of the first data release have undergone multiple dedicated validation tests. These tests aim at analysing in-depth the C…

astro-ph.IM2016★ 2.1k cited

Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties

Gaia Collaboration, A. G. A. Brown, A. Vallenari +5

At about 1000 days after the launch of Gaia we present the first Gaia data release, Gaia DR1, consisting of astrometry and photometry for over 1 billion sources brighter than magni…

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.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…