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Abstract: Wavelength space binary spectral disentangling is discussed with a data-driven, steepest-descent chi-square minimizing, global fitting procedure that applies stacked synthetic spectra to render composites. With additional constraints such as Gaia distance, mass ratio, orbital period, and separation of the binary members the stellar parameter precision can be improved even for non-eclipsing systems. We follow the orbits of 36 systems of which we discuss JL 277 here.
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Last update: April 29, 2025