Gould / Prsa / USA 11 Jet Propulsion Laboratory / USA 21 Orbital Sciences Corp. / /
Currency
pence / / /
Facility
Lowell Observatory / Palomar Observatory / Space Telescope Science Institute / University of Arizona / Technology Research Institute / Steward Observatory / Lawrence Hall of Science / University Affiliated Research Center / SETI Institute / University of Texas / Aarhus University / Southern Connecticut State University / Villanova University / McDonald Observatory / University of California / San Jose State University / Institute of Technology / /
IndustryTerm
exoplanet search / High resolution imaging / speckle imaging / post-processing examination / hierarchical systems / triple-star systems / spectroscopic and imaging follow-up observation / search techniques / data-processing pipeline / hierarchical multiple systems / triple star systems / star systems / multi-candidate systems / binary systems / /
MusicGroup
Kepler / Neptune / /
Organization
Science Operations Center / Aarhus University / Research Center / Univ. of Calif. / University of California / Santa Cruz / University of Texas at Austin / Carnegie Institution of Washington / Villanova University / NASA Ames Research Center / MIT / Harvard / Institute of Technology / SETI Institute / Centre for Astrophysics Research / University of California / Berkeley / Univ. of Florida / Astrophysics Research / Science & Technology Research Institute / Space Telescope Science Institute / Smithsonian Center for Astrophysics / Southern Connecticut State University / University of Arizona / San Jose State University / San Jose / Exoplanet Science Institute / San Diego State Univ. / /
Person
Elisa V / Thomas N. Gautier / William Borucki / Jeffrey Van / /
Characteristics of planetary candidates observed by Kepler, II: Analysis of the first four months of data William J. Borucki0,1, David G. Koch1, Gibor Basri2, Natalie Batalha3, Timothy M. Brown5, Stephen T. Bryson1, Doug