scispace - formally typeset
N

N. Meunier

Researcher at Centre national de la recherche scientifique

Publications -  51
Citations -  1343

N. Meunier is an academic researcher from Centre national de la recherche scientifique. The author has contributed to research in topics: Radial velocity & Stars. The author has an hindex of 20, co-authored 42 publications receiving 1105 citations. Previous affiliations of N. Meunier include Joseph Fourier University & University of Grenoble.

Papers
More filters
Journal ArticleDOI

Using the Sun to estimate Earth-like planets detection capabilities - I. Impact of cold spots

TL;DR: In this paper, the photometric contribution of spots and plages to the radial velocity (RV) signal partially balance each other out, so that the residual signal is comparable to the spot signal.
Journal ArticleDOI

Astrometric and photometric accuracies in high contrast imaging : The SPHERE speckle calibration tool (SpeCal)

TL;DR: The SPHERE consortium developed a dedicated piece of software to process the data as mentioned in this paper, which corrects for instrumental artifacts and uses the speckle calibration tool to minimize the stellar light halo that prevents us from detecting faint sources like exoplanets or circumstellar disks.
Journal ArticleDOI

Reconstructing the solar integrated radial velocity using MDI/SOHO

TL;DR: In this paper, the authors used Dopplergrams and magnetograms obtained by MDI/SOHO over one solar cycle to reconstruct the solar integrated radial velocity in the Ni line 6768 A.
Journal ArticleDOI

High precision astrometry mission for the detection and characterization of nearby habitable planetary systems with the Nearby Earth Astrometric Telescope (NEAT)

Fabien Malbet, +54 more
TL;DR: The Nearby Earth Astrometric Telescope (NEAT) as discussed by the authors is designed to carry out space-borne extremely high-precision measurements at the 0.05 mu as (1 sigma) accuracy level, sufficient to detect dynamical effects due to orbiting planets of mass even lower than Earth's around the nearest stars.
Journal ArticleDOI

Using the Sun to estimate Earth-like planets detection capabilities IV. Correcting for the convective component

TL;DR: In this paper, the authors investigated the impact of stellar activity on the detectability of an Earth-mass planet in the habitable zone of the Sun as seen edge-on from a neighbour star in several typical cases.