activity
20052023
most citedThe orbital motion, absolute mass, and high-altitude winds of exoplanet HD209458b

851 citations · 9.7k across the 108 of their papers we have counts for

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Showing 2010Show all

7 papers · 1 filter

astro-ph.EP2010★ 7 cited

Exoplanet-atmospheres at high spectral resolution: A CRIRES survey of hot-Jupiters

Ignas Snellen, Remco de Kok, Ernst de Mooij +3

Recently, we presented the detection of carbon monoxide in the transmission spectrum of extrasolar planet HD209458b, using CRIRES, the Cryogenic high-resolution Infrared Echelle Sp…

astro-ph.SR2010★ 75 cited

The Banana Project. III. Spin-orbit Alignment in the Long-period Eclipsing Binary NY Cephei

Simon Albrecht, Joshua Winn, Joshua Carter +2

Binaries are not always neatly aligned. Previous observations of the DI Her system showed that the spin axes of both stars are highly inclined with respect to one another and the o…

astro-ph.EP2010★ 84 cited

Orbital Orientations of Exoplanets: HAT-P-4b is Prograde and HAT-P-14b is Retrograde

Joshua N. Winn, Andrew W. Howard, John Asher Johnson +9

We present observations of the Rossiter-McLaughlin effect for two exoplanetary systems, revealing the orientations of their orbits relative to the rotation axes of their parent sta…

astro-ph.EP2010★ 173 cited

The Oblique Orbit of the Super-Neptune HAT-P-11b

Joshua N. Winn, John Asher Johnson, Andrew W. Howard +6

We find the orbit of the Neptune-sized exoplanet HAT-P-11b to be highly inclined relative to the equatorial plane of its host star. This conclusion is based on spectroscopic observ…

astro-ph.EP2010★ 738 cited

Hot Stars with Hot Jupiters Have High Obliquities

Joshua N. Winn, Daniel Fabrycky, Simon Albrecht +1

We show that stars with transiting planets for which the stellar obliquity is large are preferentially hot (T_eff > 6250 K). This could explain why small obliquities were observed…

astro-ph.EP2010★ 851 cited

The orbital motion, absolute mass, and high-altitude winds of exoplanet HD209458b

Ignas A. G. Snellen, Remco J. de Kok, Ernst J. W. de Mooij +1

For extrasolar planets discovered using the radial velocity method, the spectral characterization of the host star leads to a mass-estimate of the star and subsequently of the orbi…

astro-ph.EP2010★ 117 cited

The HAT-P-13 Exoplanetary System: Evidence for Spin-Orbit Alignment and a Third Companion

Joshua N. Winn, John Asher Johnson, Andrew W. Howard +6

We present new radial-velocity measurements of HAT-P-13, a star with two previously known companions: a transiting giant planet "b" with an orbital period of 3 days, and a more mas…