A Transiting “51 Peg-like” Planet

By G. Henry, G. Marcy, R. P. Butler, S. Vogt. Astrophysical Journal, 2000

771 citations recorded by the source corpus.

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In Astronomy and Astrophysics

Citations in the corpus

A time-dependent radiative model of HD 209458b (2004, background): “The discovery of HD 209458b (Charbonneau et al. 2000; Henry et al. 2000) allows us for the first time to directly probe the structure of a planet outside our Solar System.”
Rejecting Astrophysical False Positives from the TrES Transiting Planet Survey: The Example of GSC 03885–00829 (2006, methodology): “We now have estimates for the radii and masses of 9 planets from transit observations similar to those first successfully performed by Charbonneau et al. (2000) and Henry et al. (2000).”
OBSERVATIONS OF MASS LOSS FROM THE TRANSITING EXOPLANET HD 209458b (2010, methodology): “Very shortly thereafter, accurate measurements of the mass and radius of HD 209458b were extracted from radial velocity and photometric transit observations by Henry et al. (2000) and Charbonneau et al. (2000).”
Detection of an Extrasolar Planet Atmosphere (2001, background): “Since the discovery of planetary transits in the light curve of HD 209458 (Charbonneau et al. 2000; Henry et al. 2000; Mazeh et al. 2000), this star has been the subject of intensive study.”
The Rossiter-McLaughlin Effect and Analytic Radial Velocity Curves for Transiting Extrasolar Planetary Systems (2004, background): “One of them, HD 209458b, was first discovered spectroscopically and was soon later found to exhibit a transit signature in front of the stellar disk for a duration of 2 hr in its orbital period of 3.5 days (Henry et al. 2000; Charbonneau et al. 2000).”
Two Classes of Hot Jupiters (2007, background): “This interest has only intensified with the discovery of transiting planets (Charbonneau et al. 2000; Henry et al. 2000), allowing the measurement of planetary radii and more accurate planetary masses.”
Detection of atmospheric haze on an extrasolar planet: the 0.55–1.05 μm transmission spectrum of HD 189733b with the Hubble Space Telescope (2007, background): “HD 209458 (Charbonneau et al. 2000; Henry et al. 2000) and HD 189733 (Bouchy et al. 2005) are the most scrutinized systems because their bright host star (V ∼ 7.7 mag) and large radius allow precise enough spectroscopic measurements.”
Stellar Abundance and Galactic Chemical Evolution through LAMOST Spectroscopic Survey (2006, background): “The first observation of a transit of host stars confirmed the existence of planets (Henry et al. 2000).”
RETIRED A STARS AND THEIR COMPANIONS. III. COMPARING THE MASS–PERIOD DISTRIBUTIONS OF PLANETS AROUND A-TYPE STARS AND SUN-LIKE STARS (2009, background): “The APT observations are also useful to search for possible transits of the planetary companions (e.g., Henry et al. 2000b; Sato et al. 2005a; Winn et al. 2009a).”
On the Star-Magnetosphere Interaction of Close-in Exoplanets (2004, background): “The light curves obtained during planetary transits of its host star have provided unique information on the orbital parameters, size, and average density of this hot Jupiter or closein extrasolar giant planet (CEGP; Charbonneau et al. 2000; Henry et al. 2000).”
Atmospheric circulation and tides of ``51 Pegasus b-like'' planets (2002, background): “They are also more easily characterized by the transit method than are other planets, as indicated by the discovery of the transiting gas giant HD209458b (Charbonneau et al. 2000; Henry et al. 2000).”
On the Radii of Extrasolar Giant Planets (2003, background): “Indeed, the celebrated occultations of HD 209458 (V ¼ 7:65) (Charbonneau et al. 2000; Henry et al. 2000) have provided a scientific bonanza.”
Dynamical Instabilities in Extrasolar Planetary Systems Containing Two Giant Planets (2000, background): “Some of the most exciting recent developments include the detections of planetary transits in HD 209458 (Charbonneau et al. 2000; Henry et al. 2000) and two sub-Saturn-mass candidates around HD 16141 and HD 46375 (Marcy et al. 2000).”
ATMOSPHERIC ESCAPE FROM HOT JUPITERS (2008, background): “Observations of HD 209458b, the first hot Jupiter observed to transit its host star (Henry et al. 2000; Charbonneau et al. 2000), suggest that the planet may indeed be losing atomic hydrogen.”
Transits and Occultations (2010, background): “This was the path to discovery for 6 of the 64 known systems, including the first example, HD 209458b (Charbonneau et al. 2000, Henry et al. 2000, Mazeh et al. 2000).”