activity
19982026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations · 17.2k across the 102 of their papers we have counts for

collaborators

102 papers

astro-ph.SR2026

The PLATO Science Calibration and Validation Plan: Targets for the First Long-pointing Field

Konstanze Zwintz, Conny Aerts, Andrew Tkachenko +56

In order to meet the science goals of the PLATO space mission, an extensive science calibration and validation plan has been designed. This paper describes this plan, as well as th…

astro-ph.SR2026

Gaia FGK Benchmark Stars: Selecting Infrared Lines for Abundance Determination

Scarlet Elgueta, Paula Jofré, Claudia Aguilera-Gómez +7

The advent of new and more powerful infrared spectrographs has significantly motivated the advancement of the study of atomic and molecular line lists and stellar atmosphere models…

astro-ph.SR2025★ 3 cited

Gaia FGK Benchmark Stars: spectral library, metallicities and abundances of and Fe-peak elements of the third version

L. Casamiquela, C. Soubiran, P. Jofré +14

The accurate determination of chemical abundances in stars plays a pivotal role in understanding stellar structure and evolution, nucleosynthesis, and the chemical enrichment histo…

astro-ph.GA2023

Gaia Focused Product Release: Spatial distribution of two diffuse interstellar bands

Gaia Collaboration, M. Schultheis, H. Zhao +15

Diffuse interstellar bands (DIBs) are absorption features seen in optical and infrared spectra of stars that are probably caused by large and complex molecules in the ISM. Here we…

astro-ph.SR2023

Gaia FGK Benchmark Stars: fundamental Teff and log g of the third version

Caroline Soubiran, Orlagh Creevey, Nadege Lagarde +8

Context. Large spectroscopic surveys devoted to the study of the Milky Way, including Gaia, use automated pipelines to massively determine the atmospheric parameters of millions of…

astro-ph.EP2023★ 28 cited

Retrieval of the dayside atmosphere of WASP-43b with CRIRES+

F. Lesjak, L. Nortmann, F. Yan +15

Accurately estimating the C/O ratio of hot Jupiter atmospheres is a promising pathway towards understanding planet formation and migration, as well as the formation of clouds and t…