activity
19962019
most citedThe PLATO 2.0 Mission

1.3k citations · 8.2k across the 98 of their papers we have counts for

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Showing 2010Show all

13 papers · 1 filter

astro-ph.EP2010★ 12 cited

Possible detection of phase changes from the non-transiting planet HD 46375b by CoRoT

P. Gaulme, M. Vannier, T. Guillot +19

The present work deals with the detection of phase changes in an exoplanetary system. HD 46375 is a solar analog known to host a non-transiting Saturn-mass exoplanet with a 3.0236…

astro-ph.SR2010★ 31 cited

HD 46375: seismic and spectropolarimetric analysis of a young Sun hosting a Saturn-like planet

P. Gaulme, S. Deheuvels, W. W. Weiss +13

HD 46375 is known to host a Saturn-like exoplanet orbiting at 0.04 AU from its host star. Stellar light reflected by the planet was tentatively identified in the 34-day CoRoT run a…

astro-ph.SR2010★ 182 cited

The universal red-giant oscillation pattern; an automated determination with CoRoT data

B. Mosser, K. Belkacem, M. J. Goupil +12

The CoRoT and Kepler satellites have provided thousands of red-giant oscillation spectra. The analysis of these spectra requires efficient methods for identifying all eigenmode par…

astro-ph.SR2010★ 42 cited

Plaskett's Star: Analysis of the CoRoT photometric data

L. Mahy, E. Gosset, F. Baudin +13

The SRa02 of the CoRoT space mission for Asteroseismology was partly devoted to stars belonging to the Mon OB2 association. An intense monitoring was performed on Plaskett's Star (…

astro-ph.SR2010

Exploring the magnetic topologies of cool stars

J. Morin, J. -F. Donati, P. Petit +19

Magnetic fields of cool stars can be directly investigated through the study of the Zeeman effect on photospheric spectral lines using several approaches. With spectroscopic measur…

astro-ph.SR2010★ 56 cited

Detection of frequency spacings in the young O-type binary HD 46149 from CoRoT photometry

P. Degroote, M. Briquet, M. Auvergne +15

Using the CoRoT space based photometry of the O-type binary HD46149, stellar atmospheric effects related to rotation can be separated from pulsations, because they leave distinct s…