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Christophe Pichon

Researcher at Institut d'Astrophysique de Paris

Publications -  137
Citations -  12194

Christophe Pichon is an academic researcher from Institut d'Astrophysique de Paris. The author has contributed to research in topics: Galaxy & Star formation. The author has an hindex of 35, co-authored 123 publications receiving 10812 citations. Previous affiliations of Christophe Pichon include Centre national de la recherche scientifique & Korea Institute for Advanced Study.

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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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SDSS-III: Massive Spectroscopic Surveys of the Distant Universe, the Milky Way Galaxy, and Extra-Solar Planetary Systems

Daniel J. Eisenstein, +239 more
TL;DR: SDSS-III as discussed by the authors 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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The Eighth Data Release of the Sloan Digital Sky Survey: First Data from SDSS-III

Hiroaki Aihara, +194 more
TL;DR: The first data release of SDSS-III is described in this article, which includes five-band imaging of roughly 5200 deg2 in the southern Galactic cap, bringing the total footprint of the Sloan Digital Sky Survey imaging to 14,555 deg2, or over a third of the Celestial Sphere.
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The Eighth Data Release of the Sloan Digital Sky Survey: First Data from SDSS-III

Hiroaki Aihara, +179 more
TL;DR: The first data release of SDSS-III (and the eighth counting from the beginning of the Sloan Digital Sky Survey (SDSS) is described in this paper, which includes five-band imaging of roughly 5200 deg^2 in the Southern Galactic Cap.
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The Horizon-AGN Simulation: Morphological Diversity of Galaxies ,Promoted by AGN Feedback

TL;DR: In this paper, the critical role of active galactic nuclei (AGN) in setting up the correct galaxy morphology for the massive end of the population was identified by comparing the state-of-the-art hydrodynamical cosmological simulations Horizon-AGN and Horizon-noAGN.