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19972026
most citedAn Upper Limit on the Reflected Light from the Planet Orbiting the Star tau Bootis

193 citations · 1.3k across the 31 of their papers we have counts for

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Showing 2008Show all

6 papers · 1 filter

astro-ph2008

Impact of low-frequency p modes on the inversions of the internal rotation of the Sun

D. Salabert, A. Eff-Darwich, R. Howe +1

We used the m-averaged spectrum technique ("collapsogram") to extract the low-frequency solar p-mode parameters of low- and intermediate-angular degrees (l \leq 35) in long time se…

astro-ph2008

What can we learn on the structure and the dynamics of the solar core with g modes?

S. Mathur, J. Ballot, A Eff-Darwich +4

The detection of the signature of dipole gravity modes has opened the path to study the solar inner radiative zone. Indeed, g modes should be the best probes to infer the propertie…

astro-ph2008★ 103 cited

A New Spectroscopic and Photometric Analysis of the Transiting Planet Systems TrES-3 and TrES-4

A. Sozzetti, G. Torres, D. Charbonneau +17

We report new spectroscopic and photometric observations of the parent stars of the recently discovered transiting planets TrES-3 and TrES-4. A detailed abundance analysis based on…

astro-ph2008★ 25 cited

Analysis of MDI High-Degree Mode Frequencies and their Rotational Splittings

M. C. Rabello-Soares, S. G. Korzennik, J. Schou

Here we present a detailed analysis of solar acoustic mode frequencies and their rotational splittings for modes with degree up to 900. They were obtained by applying spherical har…

astro-ph2008★ 39 cited

Sensitivity analysis of the solar rotation to helioseismic data from GONG, GOLF and MDI observations

A. Eff-Darwich, S. G. Korzennik, S. J. Jimenez-Reyes +1

Accurate determination of the rotation rate in the radiative zone of the sun from helioseismic observations requires rotational frequency splittings of exceptional quality as well…

astro-ph2008★ 39 cited

Influence of Low-Degree High-Order p-Mode Splittings on the Solar Rotation Profile

R. A. Garcia, S. Mathur, J. Ballot +3

The solar rotation profile is well constrained down to about 0.25 R thanks to the study of acoustic modes. Since the radius of the inner turning point of a resonant acoustic mode i…