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CoRoT photometric measurements of asteroseismic targets need complementaryground-based spectroscopic observations. We are using the planet-hunter HARPSspectrograph attached to the 3.6m-ESO telescope in the framework of twoconsecutive Large Programmes. We discuss its use to study line-profilevariations and we report on a specific result obtained for the Delta Sct starHD 170699.

The spectroscopic observations of CoRoT asteroseismic targets with HARPS