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Pierre Royer

Researcher at Katholieke Universiteit Leuven

Publications -  146
Citations -  10750

Pierre Royer is an academic researcher from Katholieke Universiteit Leuven. The author has contributed to research in topics: Stars & Asymptotic giant branch. The author has an hindex of 40, co-authored 144 publications receiving 9873 citations. Previous affiliations of Pierre Royer include University of Liège.

Papers
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Journal ArticleDOI

Apsidal motion in the massive binary HD 152248

TL;DR: In this article, a large set of optical spectra was used to reconstruct the spectra of the individual binary components and establish their radial velocities using a disentangling code.
Journal ArticleDOI

The ESO Diffuse Interstellar Bands Large Exploration Survey: EDIBLES I. Project description, survey sample and quality assessment

TL;DR: The ESO Diffuse Interstellar Bands Large Exploration Survey (EDIBLES) as mentioned in this paper was designed to provide an observationally unbiased view of the presence and behaviour of the DIBs towards early-spectral-type stars whose lines-of-sight probe the diffuse-to-translucent ISM.
Journal ArticleDOI

Herschel observations of the nebula M1-67 around the Wolf-Rayet star WR 124

TL;DR: In this article, infrared images of the Wolf-Rayet star M1-67 around the star WR 124 have been obtained along with optical imaging observations along with infrared spectroscopic analysis, revealing a clumpy dusty nebula that extends up to 1 pc.
Journal ArticleDOI

Apsidal motion in the massive binary HD152248

TL;DR: In this article, a large set of optical spectra was used to reconstruct the spectra of the individual binary components and establish their radial velocities using a disentangling code.
Proceedings ArticleDOI

On the optical alignment of the PLATO cameras

TL;DR: In this article, the authors present an error budget for the optical measurements to be performed during the alignment, i.e. the definition of the best image plane at the operational temperature and the optical alignment itself, at room temperature.