1971 20160701171656.0 ASTROimport-128 Wright, D. J. 2008 Rotation and pulsation in g-mode main sequence pulsators The lack of well-identified modes is one of the major problems preventing an in-depth as- teroseismic study of gravity-mode (g-mode) main sequence pulsators. Since several of the currently available spectroscopic mode identification techniques have been developed for, or only extensively tested on pressure-mode pulsations, we started an investigation to improve them for the high radial order g-modes observed for slowly pulsating B (SPB) and γ Doradus (γ Dor) stars. A few high quality spectroscopic timeseries are being obtained for a selection of the most promising members of these groups with a large spread in projected rotational velocity that will serve as testbeds. These data will also enable us to study any observational relationship between the observed g-modes (degree l, azimuthal number m and/or pulsation amplitude) and the rotation of these non-radially pulsating stars. De Cat, P. Pollard, K. R. Zima, W. Communications in Asteroseismology 157 2008 383-384 http://esoads.eso.org/abs/2008CoAst.157..383W published in REFERD