activity
19972026
most citedThe PLATO 2.0 Mission

1.3k citations · 3.4k across the 63 of their papers we have counts for

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Showing 2008Show all

8 papers · 1 filter

astro-ph2008★ 14 cited

Excitation and damping of p-mode oscillations of alpha Cen B

W. J. Chaplin, G. Houdek, Y. Elsworth +3

This paper presents an analysis of observational data on the p-mode spectrum of the star alpha Cen B and a comparison with theoretical computations of the stochastic excitation and…

astro-ph2008★ 9 cited

SMEI observations of previously unseen pulsation frequencies in gamma Doradus

N. J. Tarrant, W. J. Chaplin, Y. P. Elsworth +2

Aims: As g-mode pulsators, gamma-Doradus-class stars may naively be expected to show a large number of modes. Taking advantage of the long photometric time-series generated by the…

astro-ph2008

Reliability of P mode event classification using contemporaneous BiSON and GOLF observations

R. Simoniello, W. J. Chaplin, Y. P. Elsworth +1

We carried out a comparison of the signals seen in contemporaneous BiSON and GOLF data sets. Both instruments perform Doppler shift velocity measurements in integrated sunlight, al…

astro-ph2008★ 18 cited

solarFLAG hare and hounds: estimation of p-mode frequencies from Sun-as-star helioseismology data

S. J. Jimenez-Reyes, W. J. Chaplin, R. A. Garcia +14

We report on the results of the latest solarFLAG hare-and-hounds exercise, which was concerned with testing methods for extraction of frequencies of low-degree solar p modes from d…

astro-ph2008★ 76 cited

Challenges for asteroseismic analysis of Sun-like stars

W. J. Chaplin, G. Houdek, T. Appourchaux +3

Asteroseismology of Sun-like stars is undergoing rapid expansion with, for example, new data from the CoRoT mission and continuation of ground-based campaigns. There is also the ex…

astro-ph2008★ 4 cited

A framework for describing correlated excitation of solar p modes

W. J. Chaplin, Y. Elsworth, T. Toutain

In a previous paper we suggested that, for a given p mode, the excitation function is the same as the component of the solar background noise that has an identical surface spherica…