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Annie C. Robin

Researcher at Centre national de la recherche scientifique

Publications -  332
Citations -  66192

Annie C. Robin is an academic researcher from Centre national de la recherche scientifique. The author has contributed to research in topics: Galaxy & Stars. The author has an hindex of 83, co-authored 318 publications receiving 57251 citations. Previous affiliations of Annie C. Robin include University of Barcelona & National University of Distance Education.

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Gaia Data Release 2. Summary of the contents and survey properties

Anthony G. A. Brown, +452 more
TL;DR: The second Gaia data release, Gaia DR2 as mentioned in this paper, is a major advance with respect to Gaia DR1 in terms of completeness, performance, and richness of the data products.
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The Gaia mission

T. Prusti, +624 more
TL;DR: Gaia as discussed by the authors 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 interferometric concept was changed to a direct-imaging approach.
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The eleventh and twelfth data releases of the Sloan Digital Sky Survey: final data from SDSS-III

Shadab Alam, +363 more
TL;DR: The third generation of the Sloan Digital Sky Survey (SDSS-III) took data from 2008 to 2014 using the original SDSS wide-field imager, the original and an upgraded multi-object fiber-fed optical spectrograph, a new near-infrared high-resolution spectrogram, and a novel optical interferometer.
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Sdss-iii: massive spectroscopic surveys of the distant universe, the milky way, and extra-solar planetary systems

Daniel J. Eisenstein, +263 more
TL;DR: SDSS-III as mentioned in this paper is a program of four spectroscopic surveys on three scientific themes: dark energy and cosmological parameters, the history and structure of the Milky Way, and the population of giant planets around other stars.
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A synthetic view on structure and evolution of the Milky Way

TL;DR: In this article, new constraints on evolution parameters obtained from the Besancon model of population synthesis and analysis of optical and near-infrared star counts are presented, in agreement with Hipparcos results and the observed rotation curve.