San Francisco / Strasbourg / Tucson / Pasadena / Santiago / Cambridge / Nashville / London / /
Company
Dra AB / Kharchenko N. V. / Kraft / Breach Publishing Co. / Wilson / Ford / Piskunov A. E. / Space Sciences Laboratory / Astronomy Inc. / /
Country
Chile / Poland / France / United States / / /
Facility
Tennessee State University / Astronomical Observatory / Boswell Science Hall / A. Mickiewicz University / Analysis Center/California Institute of Technology / University of Massachusetts / Hall D. S. / California Institute of Technology / University of California / College of Arts / NASA Exoplanet Science Institute / /
IndustryTerm
wavelength solution / photocentric orbital solution / spectroscopic/astrometric orbital solution / close binary systems / improbable solution / orbital solution / young moving / spectroscopic orbital solution / primodial gas / photocentric circular orbital solution / astrometric solution / /
NaturalFeature
Mauna Kea / /
Organization
California Institute of Technology / University of California / University of Massachusetts / Association of Universities for Research / A. Mickiewicz University / Nicolaus Copernicus Astronomical Center / National Science Foundation / Tennessee State University / UC Berkeley / Cambridge Univ. / Yale / Department of Mathematics and Physics / Department of Mathematics / NASA Exoplanet Science Institute / European Social Fund / PTI V / UC Berkeley Astronomy Department / Ministry of Science and Higher Education / Foundation for Polish Science / Galactic Centre / Royal Astronomical Society / National Aeronautics and Space Administration / Department of Astrophysics / Division of Physics / College of Arts / College of Arts and Sciences / Center of Excellence / /
Person
Tsevi Mazeh / Prot / Kevin Rykoski / Arne Rau / / /
Position
Mayor / night assistant / Carpenter / author / Professor / calibrator / /
Product
RV / Keck I/HIRES / /
ProgrammingLanguage
K / /
ProvinceOrState
Tennessee / California / Arizona / Massachusetts / /
Mon. Not. R. Astron. Soc. 419, 1285–doi:j19785.x New high-precision orbital and physical parameters of the double-lined low-mass spectroscopic binary BY Draconis