Mauna Kea / Washington DC / Budapest / Boston / Cambridge / Pino Torinese / /
Company
A. M. & Sasselov D. D. / Marley / Ford / Sasselov D. D. / Research Corporation / /
Country
Hungary / Italy / United States / Israel / / /
Facility
Tel Aviv University / Wise Observatory / Lick Observatory / Konkoly Observatory / San Francisco State University / Fred Lawrence Whipple Observatory / Smithsonian Astrophysical Observatory / Clay Center / Keck Observatory / California Institute of Technology / Carnegie Institute of Washington DC / University of California / W. M. Keck Observatory / /
IndustryTerm
e-prints / gas giant planets / transit-search algorithm / planetary systems / irradiated gas giant planets / orbital solutions / insolation energy / /
MusicGroup
Sloan / /
NaturalFeature
Mauna Kea / /
Organization
California Institute of Technology / University of California / Hungarian Scientific Research Foundation / Israel Science Foundation / Harvard / University of California / Berkeley / Kepler Mission / W. M. Keck Foundation / San Francisco State University / San Francisco / Tel Aviv University / Tel Aviv / Department of Astronomy / Department of Physics & Astronomy / African Union / Hungarian Astronomical Association / National Aeronautics and Space Administration / Clay Center / Department of Terrestrial Magnetism / Smithsonian Center for Astrophysics / Smithsonian / Carnegie Institute of Washington DC / /
Person
Howard Isaacson / Gil Esquerdo / Amit Moran / Ron Dantowitz / Joel Hartman / Marek Kozubal / Saar / /
Position
Mayor / Mp / L115 Carpenter / Butler / Carpenter / minimum mass Mp / representative / /
Draft version May 1, 2007 – VERSION Submitted to ApJ Preprint typeset using LATEX style emulateapj v[removed]HAT-P-2b: A SUPER-MASSIVE PLANET IN AN ECCENTRIC ORBIT TRANSITING A BRIGHT STAR† ´ Bakos1,2 , G. Kova ´