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UVES NGSL Project: RV correction
We have corrected all NGSL spectra for barycentric and heliocentric shifts. Then we measured the stellar radial velocity, whenever possible, by correlating the target spectrum in the 8700 A region with a reference spectrum of known radial velocity. In those cases when this was impossible (e.g. for early-type stars with few, highly rotationally broadened lines), we have adopted the values listed in SIMBAD. The derived radial velocities are listed here. Send comments to <Reinhard.Hanuschik@eso.org> Last update: 2009-10-05 17:52:42 |