• Corpus ID: 11454306

The First Kepler Mission Planet Confirmed With The Hobby-Eberly Telescope: Kepler-15b, a Hot Jupiter Enriched In Heavy Elements

@article{Endl2011TheFK,
  title={The First Kepler Mission Planet Confirmed With The Hobby-Eberly Telescope: Kepler-15b, a Hot Jupiter Enriched In Heavy Elements},
  author={Michael Endl and Phillip J. MacQueen and William D. Cochran and Erik J. Brugamyer and Lars A. Buchhave and Jason F. Rowe and Phillip W. Lucas and Howard Issacson and Stephen T. Bryson and Steve B. Howell and Jonathan J. Fortney and Terese T. Hansen and William J. Borucki and Douglas A. Caldwell and Jessie L. Christiansen and David R. Ciardi and B-O. Demory and Mark E. Everett and Eric B. Ford and Michael R. Haas and Matthew J. Holman and Elliott P. Horch and Jon M. Jenkins and David J. Koch and Jack J. Lissauer and Pavel Mach{\'a}lek and Martin D. Still and William F. Welsh and Dwight T. Sanderfer and Shawn E. Seader and Jeffrey C. Smith and Susan E. Thompson and Joseph D. Twicken},
  journal={arXiv: Earth and Planetary Astrophysics},
  year={2011}
}
We report the discovery of Kepler-15b, a new transiting exoplanet detected by NASA's Kepler mission. The transit signal with a period of 4.94 days was detected in the quarter 1 (Q1) Kepler photometry. For the first time, we have used the High-Resolution-Spectrograph (HRS) at the Hobby-Eberly Telescope (HET) to determine the mass of a Kepler planet via precise radial velocity (RV) measurements. The 24 HET/HRS radial velocities (RV) and 6 additional measurements from the FIES spectrograph at the… 

THE HOT-JUPITER KEPLER-17b: DISCOVERY, OBLIQUITY FROM STROBOSCOPIC STARSPOTS, AND ATMOSPHERIC CHARACTERIZATION

This paper reports the discovery and characterization of the transiting hot giant exoplanet Kepler-17b. The planet has an orbital period of 1.486 days, and radial velocity measurements from the

Transiting circumbinary planets Kepler-34 b and Kepler-35 b

The observed rate of circumbinary planets in this sample implies that more than ∼1% of close binary stars have giant planets in nearly coplanar orbits, yielding a Galactic population of at least several million.

The transiting circumbinary planets Kepler-34 b and Kepler-35 b Citation Welsh

Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. The MIT Faculty has made this

1 Alternate designations and summary of parameters

  • Physics
  • 2011
Blends of target stars with nearby stars on the sky can be a serious problem with Kepler targets since the contamination reduces the observed eclipse and transit depths, which might possibly lead to

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