activity
19942024
most citedA continuum from clear to cloudy hot-Jupiter exoplanets without primordial water depletion

979 citations · 14.5k across the 149 of their papers we have counts for

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91 papers · 1 filter

astro-ph2008★ 229 cited

Stellar activity of planetary host star HD 189733

I. Boisse, C. Moutou, A. Vidal-Madjar +20

Extra-solar planet search programs require high-precision velocity measurements. They need to study how to disentangle radial-velocity variations due to Doppler motion from the noi…

astro-ph2008★ 1 cited

NUV radii of the extrasolar planet HD 209458b

J. M. Desert, A. Vidal-Madjar, A. Lecavelier des Etangs +2

Extrasolar planetary transits are powerful tools to probe their atmosphere and to extract key physical properties of planets, like their mean densities, chemical compositions, or a…

astro-ph2008★ 146 cited

TiO and VO broad band absorption features in the optical spectrum of the atmosphere of the hot-Jupiter HD209458b

J. -M. Desert, A. Vidal-Madjar, A. Lecavelier des Etangs +4

The presence of titanium oxide (TiO) and vanadium oxide (VO) gas phase species is searched for in the atmosphere of the hot Jupiter HD209458b. We compared a model for the planets t…

astro-ph2008★ 4 cited

Atmospheric composition and structure of HD209458b

J. -M. Désert, A. Vidal-Madjar, A. Lecavelier des Etangs +4

Transiting planets like HD209458b offer a unique opportunity to scrutinize their atmospheric composition and structure. Transit spectroscopy probes the transition region between th…

astro-ph2008★ 220 cited

Misaligned spin-orbit in the XO-3 planetary system?

G. Hebrard, F. Bouchy, F. Pont +20

The transiting extrasolar planet XO-3b is remarkable, with a high mass and eccentric orbit. The unusual characteristics make it interesting to test whether its orbital plane is par…

astro-ph2008★ 1 cited

Discovery of a peculiar Cepheid-like star towards the northern edge of the Small Magellanic Cloud

J. B. Marquette, P. Tisserand, P. Francois +37

For seven years, the EROS-2 project obtained a mass of photometric data on variable stars. We present a peculiar Cepheid-like star, in the direction of the Small Magellanic Cloud,…

astro-ph2008★ 19 cited

ELODIE metallicity-biased search for transiting Hot Jupiters V. An intermediate-period Jovian planet orbiting HD45652

N. C. Santos, S. Udry, F. Bouchy +20

We present the detection of a 0.47 Jupiter mass planet in a 44-day period eccentric trajectory (e=0.39) orbiting the metal-rich star HD45652. This planet, the seventh giant planet…

astro-ph2008★ 121 cited

Rayleigh scattering by H2 in the extrasolar planet HD209458b

A. Lecavelier des Etangs, A. Vidal-Madjar, J. -M. Desert +1

Transiting planets, such as HD209458b, offer a unique opportunity to scrutinize the planetary atmospheric content. Although molecular hydrogen is expected to be the main atmospheri…

astro-ph2008★ 39 cited

Molecular hydrogen in the circumstellar environments of Herbig Ae/Be stars probed by FUSE

C. Martin-Zaidi, M. Deleuil, J. Le Bourlot +7

We observed molecular hydrogen around a sample of pre-main sequence stars in order to better characterize their gaseous CS environments. We analyzed the FUSE (Far Ultraviolet Spect…

astro-ph2008★ 140 cited

New observations of the extended hydrogen exosphere of the extrasolar planet HD209458b

David Ehrenreich, Alain Lecavelier des Etangs, Guillaume Hébrard +5

Atomic hydrogen escaping from the planet HD209458b provides the largest observational signature ever detected for an extrasolar planet atmosphere. However, the Space Telescope Imag…

astro-ph2008★ 121 cited

Determining atmospheric conditions at the terminator of the hot-Jupiter HD209458b

David K. Sing, A. Vidal-Madjar, A. Lecavelier des Etangs +3

We present a theoretical model fit to the HST/STIS optical transit transmission spectrum of HD209458b. In our fit, we use the sodium absorption line profile along with the Rayleigh…

astro-ph2008★ 413 cited

Rayleigh scattering in the transit spectrum of HD 189733b

A. Lecavelier des Etangs, F. Pont, A. Vidal-Madjar +1

The transit spectrum of the exoplanet HD 189733b has recently been obtained between 0.55 and 1.05 microns. Here we present an analysis of this spectrum. We develop first-order equa…

astro-ph2008★ 153 cited

Exoplanet HD 209458b : Evaporation strengthened

A. Vidal-Madjar, A. Lecavelier des Etangs, J. -M. Desert +4

Following re-analysis of Hubble Space Telescope observations of primary transits of the extrasolar planet HD209458b at Lyman-alpha, Ben-Jaffel (2007, BJ007) claims that no sign of…

astro-ph2008★ 191 cited

HST/STIS Optical Transit Transmission Spectra of the hot-Jupiter HD209458b

David K. Sing, A. Vidal-Madjar, J. -M. Desert +2

We present the transmission spectra of the hot-Jupiter HD209458b taken with the Space Telescope Imaging Spectrograph aboard the Hubble Space Telescope. Our analysis combines data a…

astro-ph2008★ 37 cited

R Coronae Borealis stars in the Galactic Bulge discovered by EROS-2

P. Tisserand, J. B. Marquette, P. R. Wood +33

Rare types of variable star may give unique insight into short-lived stages of stellar evolution. The systematic monitoring of millions of stars and advanced light curve analysis t…

astro-ph2007★ 88 cited

A Spitzer Search for Water in the Transiting Exoplanet HD189733b

David Ehrenreich, Guillaume Hébrard, Alain Lecavelier Des Etangs +5

We present Spitzer Space Telescope observations of the extrasolar planet HD189733b primary transit, obtained simultaneously at 3.6 and 5.8 microns with the Infrared Array Camera. T…

astro-ph2007★ 379 cited

Water vapour in the atmosphere of a transiting extrasolar planet

Giovanna Tinetti, Alfred Vidal-Madjar, Mao-Chang Liang +10

Water is predicted to be among, if not the most abundant molecular species after hydrogen in the atmospheres of close-in extrasolar giant planets (hot-Jupiters) Several attempts ha…

astro-ph2007★ 107 cited

Spectropolarimetric observations of the transiting planetary system of the K dwarf HD 189733

C. Moutou, J. -F. Donati, R. Savalle +7

With a Jupiter-mass planet orbiting at a distance of only 0.031 AU, the active K2 dwarf HD 189733 is a potential candidate in which to study the magnetospheric interactions of a co…

astro-ph2007★ 31 cited

Elodie metallicity-biased search for transiting Hot Jupiters IV. Intermediate period planets orbiting the stars HD43691 and HD132406

R. Da Silva, S. Udry, F. Bouchy +21

We report here the discovery of two planet candidates as a result of our planet-search programme biased in favour of high-metallicity stars, using the ELODIE spectrograph at the Ob…

astro-ph2007★ 83 cited

Refined parameters and spectroscopic transit of the super-massive planet HD147506b

B. Loeillet, A. Shporer, F. Bouchy +26

In this paper, we report a refined determination of the orbital parameters and the detection of the Rossiter-McLaughlin effect of the recently discovered transiting exoplanet HD147…

astro-ph2006★ 82 cited

Infrared Transmission Spectra for Extrasolar Giant Planets

G. Tinetti, M. C. Liang, A. Vidal-Madjar +3

Among the hot Jupiters that transit their parent stars known to date, the two best candidates to be observed with transmission spectroscopy in the mid-infrared (MIR) are HD189733b…

astro-ph2006★ 20 cited

Interstellar abundances in the neutral and ionized gas of NGC604

V. Lebouteiller, D. Kunth, J. Lequeux +5

We present FUSE spectra of the giant HII region NGC604 in the spiral galaxy M33. Chemical abundances are derived from far-UV absorption lines and are compared to those derived from…

astro-ph2006★ 940 cited

Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds

P. Tisserand, L. Le Guillou, C. Afonso +35

The EROS-2 project was designed to test the hypothesis that massive compact halo objects (the so-called ``machos'') could be a major component of the dark matter halo of the Milky…

astro-ph2006★ 10 cited

Removing the Microlensing Blending-Parallax Degeneracy Using Source Variability

R. J. Assef, A. Gould, the EROS-2 +2

Microlensing event MACHO 97-SMC-1 is one of the rare microlensing events for which the source is a variable star, simply because most variable stars are systematically eliminated f…