York / Tucson / Baltimore / Saumon et / Los Alamos / Honolulu / /
Company
NH3 and CO / Hp / / /
Facility
IRS pipeline / Spitzer Science Center / Mauna Kea Observatory / X. Fan Steward Observatory / Washington University / AZ J. T. Rayner Institute / R. S. Freedman SETI Institute / Saumon Los Alamos National Laboratory / T. R. Geballe Gemini Observatory / University of Hawaii / Johns Hopkins University / /
IndustryTerm
identical solutions / spectral energy distributions / metal-rich composition / chemical equilibrium / median rejection algorithm / Online material / possible solutions / chemical equilibrium calculations / metal-rich model spectra / strict chemical equilibrium / likely solutions / computing / chemical equilibrium value / chemical / mean clipping algorithm / /
MusicGroup
the IRS / CH4 / CO / H2O / NH3 / /
NaturalFeature
IRAC channel / Mauna Kea / /
Organization
DWARFS D. Saumon Los Alamos National Laboratory / Washington University / St. Louis / Spitzer Science Center / R. S. Freedman SETI Institute / Internal Revenue Service / T. R. Geballe Gemini Observatory / Hilo / HI D. Stephens and D. A. Golimowski Department of Physics and Astronomy / Johns Hopkins University / M. S. Marley NASA Ames Research Center / AZ J. T. Rayner Institute for Astronomy / University of Hawaii / NASA Ames Research Center / HI K. Lodders Department of Earth and Planetary Science / American Astronomical Society / /
Person
Gl / Yelle / / /
Position
General / representative / /
ProvinceOrState
Alabama / Hawaii / Missouri / New Mexico / Colorado / /
PublishedMedium
The Astrophysical Journal / /
Technology
S/N / X-ray / ESA / median rejection algorithm / S/ N / spectroscopy / mean clipping algorithm / combined using a mean clipping algorithm / /
A The Astrophysical Journal, 656:1136 – 1149, 2007 February 20 # 2007. The American Astronomical Society. All rights reserved. Printed in U.S.A. PHYSICAL PARAMETERS OF TWO VERY COOL T DWARFS