Comparison of GAIA and RAVE Spectroscopic Atmospheric Analysis with Orbital Solution of Eclipsing Binaries

Details Comparison of GAIA and RAVE Spectroscopic Atmospheric Analysis with Orbital Solution of Eclipsing Binaries Comparison of GAIA and RAVE Spectroscopic Atmospheric Analysis with Orbital Solution of Eclipsing Binaries

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..374..201s&link_type=abstract

From Stars to Galaxies: Building the Pieces to Build Up the Universe. ASP Conference Series, Vol. 374, proceedings of the confer

Computer Science

Scientific paper

χ^2 atmospheric analysis on the spectra of five eclipsing binaries
obtained at quadratures is compared with results from orbital solutions
obtained in a GAIA-like fashion. The analyzed Asiago spectra cover the
8450-8750 Å range common to the GAIA and RAVE spectroscopic
surveys. Excellent agreement for parameters in common is found.

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