activity
19972026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations · 25.1k across the 145 of their papers we have counts for

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Showing 2013Show all

9 papers · 1 filter

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…

astro-ph.SR2013★ 24 cited

A new procedure for defining a homogenous line-list for solar-type stars

S. G. Sousa, N. C. Santos, V. Adibekyan +9

Context. The homogenization of the stellar parameters is an important goal for large observational spectroscopic surveys, but it is very difficult to achieve it because of the dive…

astro-ph.SR2013★ 7 cited

iSpec: An integrated software framework for the analysis of stellar spectra

S. Blanco-Cuaresma, C. Soubiran, P. Jofré +1

iSpec is an integrated spectroscopic software framework suitable for the creation of spectral libraries such as the Benchmark Stars library and the determination of atmospheric par…

astro-ph.GA2013★ 1 cited

Gaia FGK Benchmark Stars and their reference parameters

Paula Jofre, Ulrike Heiter, Sergi Blanco-Cuaresma +1

In this article we summarise on-going work on the so-called Gaia FGK Benchmark Stars. This work consists of the determination of their atmospheric parameters and of the constructio…

astro-ph.GA2013★ 115 cited

On the metallicity of open clusters II. Spectroscopy

U. Heiter, C. Soubiran, M. Netopil +1

In a series of three papers, we investigate the current status of published metallicities for open clusters that were derived from a variety of photometric and spectroscopic method…

astro-ph.IM2013★ 149 cited

The Gaia astrophysical parameters inference system (Apsis). Pre-launch description

C. A. L. Bailer-Jones, R. Andrae, B. Arcay +46

The Gaia satellite will survey the entire celestial sphere down to 20th magnitude, obtaining astrometry, photometry, and low resolution spectrophotometry on one billion astronomica…